Sample records for electronic energy band

  1. Electron currents associated with an auroral band

    NASA Technical Reports Server (NTRS)

    Spiger, R. J.; Anderson, H. R.

    1975-01-01

    Measurements of electron pitch angle distributions and energy spectra over a broad auroral band were used to calculate net electric current carried by auroral electrons in the vicinity of the band. The particle energy spectrometers were carried by a Nike-Tomahawk rocket launched from Poker Flat, Alaska, at 0722 UT on February 25, 1972. Data are presented which indicate the existence of upward field-aligned currents of electrons in the energy range 0.5-20 keV. The spatial relationship of these currents to visual structure of the auroral arc and the characteristics of the electrons carrying the currents are discussed.

  2. Energies of rare-earth ion states relative to host bands in optical materials from electron photoemission spectroscopy

    NASA Astrophysics Data System (ADS)

    Thiel, Charles Warren

    There are a vast number of applications for rare-earth-activated materials and much of today's cutting-edge optical technology and emerging innovations are enabled by their unique properties. In many of these applications, interactions between the rare-earth ion and the host material's electronic states can enhance or inhibit performance and provide mechanisms for manipulating the optical properties. Continued advances in these technologies require knowledge of the relative energies of rare-earth and crystal band states so that properties of available materials may be fully understood and new materials may be logically developed. Conventional and resonant electron photoemission techniques were used to measure 4f electron and valence band binding energies in important optical materials, including YAG, YAlO3, and LiYF4. The photoemission spectra were theoretically modeled and analyzed to accurately determine relative energies. By combining these energies with ultraviolet spectroscopy, binding energies of excited 4fN-15d and 4fN+1 states were determined. While the 4fN ground-state energies vary considerably between different trivalent ions and lie near or below the top of the valence band in optical materials, the lowest 4f N-15d states have similar energies and are near the bottom of the conduction band. As an example for YAG, the Tb3+ 4f N ground state is in the band gap at 0.7 eV above the valence band while the Lu3+ ground state is 4.7 eV below the valence band maximum; however, the lowest 4fN-15d states are 2.2 eV below the conduction band for both ions. We found that a simple model accurately describes the binding energies of the 4fN, 4fN-1 5d, and 4fN+1 states. The model's success across the entire rare-earth series indicates that measurements on two different ions in a host are sufficient to predict the energies of all rare-earth ions in that host. This information provides new insight into electron transfer transitions, luminescence quenching, and valence

  3. Theoretical modeling of low-energy electronic absorption bands in reduced cobaloximes

    DOE PAGES

    Bhattacharjee, Anirban; Chavarot-Kerlidou, Murielle; Dempsey, Jillian L.; ...

    2014-08-11

    Here, we report that the reduced Co(I) states of cobaloximes are powerful nucleophiles that play an important role in the hydrogen-evolving catalytic activity of these species. In this work we have analyzed the low energy electronic absorption bands of two cobaloxime systems experimentally and using a variety of density functional theory and molecular orbital ab initio quantum chemical approaches. Overall we find a reasonable qualitative understanding of the electronic excitation spectra of these compounds but show that obtaining quantitative results remains a challenging task.

  4. Plasmon enhanced heterogeneous electron transfer with continuous band energy model

    NASA Astrophysics Data System (ADS)

    Zhao, Dandan; Niu, Lu; Wang, Luxia

    2017-08-01

    Photoinduced charge injection from a perylene dye molecule into the conduction band of a TiO2 system decorated by a metal nanoparticles (MNP) is studied theoretically. Utilizing the density matrix theory the charge transfer dynamics is analyzed. The continuous behavior of the TiO2 conduction band is accounted for by a Legendre polynomials expansion. The simulations consider optical excitation of the dye molecule coupled to the MNP and the subsequent electron injection into the TiO2 semiconductor. Due to the energy transfer coupling between the molecule and the MNP optical excitation and subsequent charge injection into semiconductor is strongly enhanced. The respective enhancement factor can reach values larger than 103. Effects of pulse duration, coupling strength and energetic resonances are also analyzed. The whole approach offers an efficient way to increase charge injection in dye-sensitized solar cells.

  5. Quasiparticle Energies and Band Gaps in Graphene Nanoribbons

    NASA Astrophysics Data System (ADS)

    Yang, Li; Park, Cheol-Hwan; Son, Young-Woo; Cohen, Marvin L.; Louie, Steven G.

    2007-11-01

    We present calculations of the quasiparticle energies and band gaps of graphene nanoribbons (GNRs) carried out using a first-principles many-electron Green’s function approach within the GW approximation. Because of the quasi-one-dimensional nature of a GNR, electron-electron interaction effects due to the enhanced screened Coulomb interaction and confinement geometry greatly influence the quasiparticle band gap. Compared with previous tight-binding and density functional theory studies, our calculated quasiparticle band gaps show significant self-energy corrections for both armchair and zigzag GNRs, in the range of 0.5 3.0 eV for ribbons of width 2.4 0.4 nm. The quasiparticle band gaps found here suggest that use of GNRs for electronic device components in ambient conditions may be viable.

  6. Laser-Induced Modification Of Energy Bands Of Transparent Solids

    NASA Astrophysics Data System (ADS)

    Gruzdev, Vitaly

    2010-10-01

    Laser-induced variations of electron energy bands of transparent solids significantly affect the initial stages of laser-induced ablation (LIA) influencing rates of ionization and light absorption by conduction-band electrons. We analyze fast variations with characteristic duration in femto-second time domain that include: 1) switching electron functions from bonding to anti-bonding configuration due to laser-induced ionization; 2) laser-driven oscillations of electrons in quasi-momentum space; and 3) direct distortion of the inter-atomic potential by electric field of laser radiation. Among those effects, the latter two have zero delay and reversibly modify band structure taking place from the beginning of laser action. They are of special interest due to their strong influence on the initial stage and threshold of laser ablation. The oscillations modify the electron-energy bands by adding pondermotive potential. The direct action of radiation's electric field leads to high-frequency Franz-Keldysh effect (FKE) spreading the allowed electron states into the forbidden-energy bands. FKE provides decrease of the effective band gap while the electron oscillations lead either to monotonous increase or oscillatory variations of the gap. We analyze the competition between those two opposite trends and their role in initiating LIA.

  7. Ultrafast laser-induced modifications of energy bands of non-metal crystals

    NASA Astrophysics Data System (ADS)

    Gruzdev, Vitaly

    2009-10-01

    Ultrafast laser-induced variations of electron energy bands of transparent solids significantly influence ionization and conduction-band electron absorption driving the initial stage of laser-induced damage (LID). The mechanisms of the variations are attributed to changing electron functions from bonding to anti-bonding configuration via laser-induced ionization; laser-driven electron oscillations in quasi-momentum space; and direct distortion of the inter-atomic potential by electric field of laser radiation. The ionization results in the band-structure modification via accumulation of broken chemical bonds between atoms and provides significant contribution to the overall modification only when enough excited electrons are accumulated in the conduction band. The oscillations are associated with modification of electron energy by pondermotive potential of the oscillations. The direct action of radiation's electric field leads to specific high-frequency Franz-Keldysh effect (FKE) spreading the allowed electron states into the bands of forbidden energy. Those processes determine the effective band gap that is a laser-driven energy gap between the modified electron energy bands. Among those mechanisms, the latter two provide reversible band-structure modification that takes place from the beginning of the ionization and are, therefore, of special interest due to their strong influence on the initial stage of the ionization. The pondermotive potential results either in monotonous increase or oscillatory variations of the effective band gap that has been taken into account in some ionization models. The classical FKE provides decrease of the band gap. We analyzing the competition between those two opposite trends of the effective-band-gap variations and discuss applications of those effects for considerations of the laser-induced damage and its threshold in transparent solids.

  8. The temperature-dependency of the optical band gap of ZnO measured by electron energy-loss spectroscopy in a scanning transmission electron microscope

    NASA Astrophysics Data System (ADS)

    Granerød, Cecilie S.; Galeckas, Augustinas; Johansen, Klaus Magnus; Vines, Lasse; Prytz, Øystein

    2018-04-01

    The optical band gap of ZnO has been measured as a function of temperature using Electron Energy-Loss Spectroscopy (EELS) in a (Scanning) Transmission Electron Microscope ((S)TEM) from approximately 100 K up towards 1000 K. The band gap narrowing shows a close to linear dependency for temperatures above 250 K and is accurately described by Varshni, Bose-Einstein, Pässler and Manoogian-Woolley models. Additionally, the measured band gap is compared with both optical absorption measurements and photoluminescence data. STEM-EELS is here shown to be a viable technique to measure optical band gaps at elevated temperatures, with an available temperature range up to 1500 K and the benefit of superior spatial resolution.

  9. Energy dependence of effective electron mass and laser-induced ionization of wide band-gap solids

    NASA Astrophysics Data System (ADS)

    Gruzdev, V. E.

    2008-10-01

    Most of the traditional theoretical models of laser-induced ionization were developed under the assumption of constant effective electron mass or weak dependence of the effective mass on electron energy. Those assumptions exclude from consideration all the effects resulting from significant increase of the effective mass with increasing of electron energy in real the conduction band. Promotion of electrons to the states with high effective mass can be done either via laserinduced electron oscillations or via electron-particle collisions. Increase of the effective mass during laser-material interactions can result in specific regimes of ionization. Performing a simple qualitative analysis by comparison of the constant-mass approximation vs realistic dependences of the effective mass on electron energy, we demonstrate that the traditional ionization models provide reliable estimation of the ionization rate in a very limited domain of laser intensity and wavelength. By taking into account increase of the effective mass with electron energy, we demonstrate that special regimes of high-intensity photo-ionization are possible depending on laser and material parameters. Qualitative analysis of the energy dependence of the effective mass also leads to conclusion that the avalanche ionization can be stopped by the effect of electron trapping in the states with large values of the effective mass.

  10. Role of Electronic Structure In Ion Band State Theory of Low Energy Nuclear Reactions

    NASA Astrophysics Data System (ADS)

    Chubb, Scott

    2004-03-01

    The Nuts and Bolts of our Ion Band State (IBS) theory of low energy nuclear reactions (LENR's) in palladium-deuteride (PdD) and palladium-hydride (PdH) are the electrons that hold together or tear apart the bonds (or lack of bonds) between deuterons (d's) or protons (p's) and the host material. In PdDx and PdH_x, this bonding is strongly correlated with loading: in ambient loading conditions (x< 0. 6), the bonding in hibits IBS occupation. As x arrow 1, slight increases and decreases in loading can lead to vibrations (which have conventionally been thought to occur from phonons) that can induce potential losses or increases of p/d. Naive assumptions about phonons fail to include these losses and increases. These effects can occur because neither H or D has core electrons and because in either PdD or PdH, the electrons near the Fermi Energy have negligible overlap with the nucleus of either D or H. I use these ideas to develop a formal justification, based on a generalization of conventional band theory (Scott Chubb, "Semi-Classical Conduction of Charged and Neutral Particles in Finite Lattices," 2004 March Meeting."), for the idea that occupation of IBS's can occur and that this can lead to nuclear reactions.

  11. Electronic Band Structure Tuning of Highly-Mismatched-Alloys for Energy Conversion Applications

    NASA Astrophysics Data System (ADS)

    Ting, Min

    Highly-mismatched alloys: ZnO1-xTe x and GaN1-xSb x are discussed within the context of finding the suitable material for a cost-effective Si-based tandem solar cell (SBTSC). SBTSC is an attractive concept for breaking through the energy conversion efficiency theoretical limit of a single junction solar cell. Combining with a material of 1.8 eV band gap, SBTSC can theoretically achieve energy conversion efficiency > 45%. ZnO and GaN are wide band gap semiconductors. Alloying Te in ZnO and alloying Sb in GaN result in large band gap reduction to < 2 eV from 3.3 eV and 3.4 eV respectively. The band gap reduction is majorly achieved by the upward shift of valence band (VB). Incorporating Te in ZnO modifies the VB of ZnO through the valence-band anticrossing (VBAC) interaction between localized Te states and ZnO VB delocalized states, which forms a Te-derived VB at 1 eV above the host VB. Similar band structure modification is resulted from alloying Sb in GaN. Zn1-xTex and GaN 1-xSbx thin films are synthesized across the whole composition range by pulsed laser deposition (PLD) and low temperature molecular beam epitaxy (LT-MBE) respectively. The electronic band edges of these alloys are measured by synchrotron X-ray absorption, emission, and the X-ray photoelectron spectroscopies. Modeling the optical absorption coefficient with the band anticrossing (BAC) model revealed that the Te and Sb defect levels to be at 0.99 eV and 1.2 eV above the VB of ZnO and GaN respectively. Electrically, Zn1-xTex is readily n-type conductive and GaN1-xSbx is strongly p-type conductive. A heterojunction device of p-type GaN 0.93Sb0.07 with n-type ZnO0.77Te0.93 upper cell (band gap at 1.8 eV) on Si bottom cell is proposed as a promising SBTSC device.

  12. Band-to-Band Tunneling-Dominated Thermo-Enhanced Field Electron Emission from p-Si/ZnO Nanoemitters.

    PubMed

    Huang, Zhizhen; Huang, Yifeng; Xu, Ningsheng; Chen, Jun; She, Juncong; Deng, Shaozhi

    2018-06-13

    Thermo-enhancement is an effective way to achieve high performance field electron emitters, and enables the individually tuning on the emission current by temperature and the electron energy by voltage. The field emission current from metal or n-doped semiconductor emitter at a relatively lower temperature (i.e., < 1000 K) is less temperature sensitive due to the weak dependence of free electron density on temperature, while that from p-doped semiconductor emitter is restricted by its limited free electron density. Here, we developed full array of uniform individual p-Si/ZnO nanoemitters and demonstrated the strong thermo-enhanced field emission. The mechanism of forming uniform nanoemitters with well Si/ZnO mechanical joint in the nanotemplates was elucidated. No current saturation was observed in the thermo-enhanced field emission measurements. The emission current density showed about ten-time enhancement (from 1.31 to 12.11 mA/cm 2 at 60.6 MV/m) by increasing the temperature from 323 to 623 K. The distinctive performance did not agree with the interband excitation mechanism but well-fit to the band-to-band tunneling model. The strong thermo-enhancement was proposed to be benefit from the increase of band-to-band tunneling probability at the surface portion of the p-Si/ZnO nanojunction. This work provides promising cathode for portable X-ray tubes/panel, ionization vacuum gauges and low energy electron beam lithography, in where electron-dose control at a fixed energy is needed.

  13. Positron and electron energy bands in several ionic crystals using restricted Hartree-Fock method

    NASA Astrophysics Data System (ADS)

    Kunz, A. B.; Waber, J. T.

    1981-08-01

    Using a restricted Hartree-Fock formalism and suitably localized and symmetrized wave functions, both the positron and electron energy bands were calculated for NaF, MgO and NiO. The lowest positron state at Γ 1 lies above the vacuum level and negative work functions are predicted. Positron annihilation rates were calculated and found to be in good agreement with measured lifetimes.

  14. Electron Phonon Coupling versus Photoelectron Energy Loss at the Origin of Replica Bands in Photoemission of FeSe on SrTiO3

    NASA Astrophysics Data System (ADS)

    Li, Fengmiao; Sawatzky, George A.

    2018-06-01

    The recent observation of replica bands in single-layer FeSe /SrTiO3 by angle-resolved photoemission spectroscopy (ARPES) has triggered intense discussions concerning the potential influence of the FeSe electrons coupling with substrate phonons on the superconducting transition temperature. Here we provide strong evidence that the replica bands observed in the single-layer FeSe /SrTiO3 system and several other cases are largely due to the energy loss processes of the escaping photoelectron, resulted from the well-known strong coupling of external propagating electrons to Fuchs-Kliewer surface phonons in ionic materials in general. The photoelectron energy loss in ARPES on single-layer FeSe /SrTiO3 is calculated using the demonstrated successful semiclassical dielectric theory in describing low energy electron energy loss spectroscopy of ionic insulators. Our result shows that the observed replica bands are mostly a result of extrinsic photoelectron energy loss and not a result of the electron phonon interaction of the Fe d electrons with the substrate phonons. The strong enhancement of the superconducting transition temperature in these monolayers remains an open question.

  15. Theoretical study of energy states of two-dimensional electron gas in pseudomorphically strained InAs HEMTs taking into account the non-parabolicity of the conduction band

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Nishio, Yui; Yamaguchi, Satoshi; Yamazaki, Youichi

    2013-12-04

    We determined rigorously the energy states of a two-dimensional electron gas (2DEG) in high electron mobility transistors (HEMTs) with a pseudomorphically strained InAs channel (InAs PHEMTs) taking into account the non-parabolicity of the conduction band for InAs. The sheet carrier concentration of 2DEG for the non-parabolic energy band was about 50% larger than that for the parabolic energy band and most of the electrons are confined strongly in the InAs layer. In addition, the threshold voltage for InAs PHEMTs was about 0.21 V lower than that for conventional InGaAs HEMTs.

  16. Band structure of an electron in a kind of periodic potentials with singularities

    NASA Astrophysics Data System (ADS)

    Hai, Kuo; Yu, Ning; Jia, Jiangping

    2018-06-01

    Noninteracting electrons in some crystals may experience periodic potentials with singularities and the governing Schrödinger equation cannot be defined at the singular points. The band structure of a single electron in such a one-dimensional crystal has been calculated by using an equivalent integral form of the Schrödinger equation. Both the perturbed and exact solutions are constructed respectively for the cases of a general singular weak-periodic system and its an exactly solvable version, Kronig-Penney model. Any one of them leads to a special band structure of the energy-dependent parameter, which results in an effective correction to the previous energy-band structure and gives a new explanation for forming the band structure. The used method and obtained results could be a valuable aid in the study of energy bands in solid-state physics, and the new explanation may trigger investigation to different physical mechanism of electron band structures.

  17. Design study of an S-band RF cavity of a dual-energy electron LINAC for the CIS

    NASA Astrophysics Data System (ADS)

    Lee, Byeong-No; Park, Hyungdal; Song, Ki-baek; Li, Yonggui; Lee, Byung Cheol; Cha, Sung-su; Lee, Jong-Chul; Shin, Seung-Wook; Chai, Jong-seo

    2014-01-01

    The design of a resonance frequency (RF) cavity for the dual-energy S-band electron linear accelerator (LINAC) has been carried out for the cargo inspection system (CIS). This Standing-wave-type RF cavity is operated at a frequency under the 2856-MHz resonance frequency and generates electron beams of 9 MeV (high mode) and 6 MeV (low mode). The electrons are accelerated from the initial energy of the electron gun to the target energy (9 or 6 MeV) inside the RF cavity by using the RF power transmitted from a 5.5-MW-class klystron. Then, electron beams with a 1-kW average power (both high mode and low mode) bombard an X-ray target a 2-mm spot size. The proposed accelerating gradient was 13 MV/m, and the designed Q value was about 7100. On going research on 15-MeV non-destructive inspections for military or other applications is presented.

  18. Band gap and electronic structure of MgSiN2

    NASA Astrophysics Data System (ADS)

    Quirk, J. B.; Râsander, M.; McGilvery, C. M.; Palgrave, R.; Moram, M. A.

    2014-09-01

    Density functional theory calculations and electron energy loss spectroscopy indicate that the electronic structure of ordered orthorhombic MgSiN2 is similar to that of wurtzite AlN. A band gap of 5.7 eV was calculated for both MgSiN2 (indirect) and AlN (direct) using the Heyd-Scuseria-Ernzerhof approximation. Correction with respect to the experimental room-temperature band gap of AlN indicates that the true band gap of MgSiN2 is 6.2 eV. MgSiN2 has an additional direct gap of 6.3 eV at the Γ point.

  19. Auger electron emission initiated by the creation of valence-band holes in graphene by positron annihilation.

    PubMed

    Chirayath, V A; Callewaert, V; Fairchild, A J; Chrysler, M D; Gladen, R W; Mcdonald, A D; Imam, S K; Shastry, K; Koymen, A R; Saniz, R; Barbiellini, B; Rajeshwar, K; Partoens, B; Weiss, A H

    2017-07-13

    Auger processes involving the filling of holes in the valence band are thought to make important contributions to the low-energy photoelectron and secondary electron spectrum from many solids. However, measurements of the energy spectrum and the efficiency with which electrons are emitted in this process remain elusive due to a large unrelated background resulting from primary beam-induced secondary electrons. Here, we report the direct measurement of the energy spectra of electrons emitted from single layer graphene as a result of the decay of deep holes in the valence band. These measurements were made possible by eliminating competing backgrounds by employing low-energy positrons (<1.25 eV) to create valence-band holes by annihilation. Our experimental results, supported by theoretical calculations, indicate that between 80 and 100% of the deep valence-band holes in graphene are filled via an Auger transition.

  20. Auger electron emission initiated by the creation of valence-band holes in graphene by positron annihilation

    PubMed Central

    Chirayath, V. A.; Callewaert, V.; Fairchild, A. J.; Chrysler, M. D.; Gladen, R. W.; Mcdonald, A. D.; Imam, S. K.; Shastry, K.; Koymen, A. R.; Saniz, R.; Barbiellini, B.; Rajeshwar, K.; Partoens, B.; Weiss, A. H.

    2017-01-01

    Auger processes involving the filling of holes in the valence band are thought to make important contributions to the low-energy photoelectron and secondary electron spectrum from many solids. However, measurements of the energy spectrum and the efficiency with which electrons are emitted in this process remain elusive due to a large unrelated background resulting from primary beam-induced secondary electrons. Here, we report the direct measurement of the energy spectra of electrons emitted from single layer graphene as a result of the decay of deep holes in the valence band. These measurements were made possible by eliminating competing backgrounds by employing low-energy positrons (<1.25 eV) to create valence-band holes by annihilation. Our experimental results, supported by theoretical calculations, indicate that between 80 and 100% of the deep valence-band holes in graphene are filled via an Auger transition. PMID:28703225

  1. Enhanced tunable narrow-band THz emission from laser-modulated electron beams

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Xiang, D.; Stupakov, G.; /SLAC

    2009-06-19

    We propose and analyze a scheme to generate enhanced narrow-band terahertz (THz) radiation through down-conversion of the frequency of optical lasers using laser-modulated electron beams. In the scheme the electron beam is first energy modulated by two lasers with wave numbers k{sub 1} and k2, respectively. After passing through a dispersion section, the energy modulation is converted to density modulation. Due to the nonlinear conversion process, the beam will have density modulation at wave number k = nk{sub 1} + mk{sub 2}, where n and m are positive or negative integers. By properly choosing the parameters for the lasers andmore » dispersion section, one can generate density modulation at THz frequency in the beam using optical lasers. This density-modulated beam can be used to generate powerful narrow-band THz radiation. Since the THz radiation is in tight synchronization with the lasers, it should provide a high temporal resolution for the optical-pump THz-probe experiments. The central frequency of the THz radiation can be easily tuned by varying the wavelength of the two lasers and the energy chirp of the electron beam. The proposed scheme is in principle able to generate intense narrow-band THz radiation covering the whole THz range and offers a promising way towards the tunable intense narrow-band THz sources.« less

  2. Reconstruction of Band Structure Induced by Electronic Nematicity in an FeSe Superconductor

    NASA Astrophysics Data System (ADS)

    Nakayama, K.; Miyata, Y.; Phan, G. N.; Sato, T.; Tanabe, Y.; Urata, T.; Tanigaki, K.; Takahashi, T.

    2014-12-01

    We have performed high-resolution angle-resolved photoemission spectroscopy on an FeSe superconductor (Tc˜8 K ), which exhibits a tetragonal-to-orthorhombic structural transition at Ts˜90 K . At low temperature, we found splitting of the energy bands as large as 50 meV at the M point in the Brillouin zone, likely caused by the formation of electronically driven nematic states. This band splitting persists up to T ˜110 K , slightly above Ts, suggesting that the structural transition is triggered by the electronic nematicity. We have also revealed that at low temperature the band splitting gives rise to a van Hove singularity within 5 meV of the Fermi energy. The present result strongly suggests that this unusual electronic state is responsible for the unconventional superconductivity in FeSe.

  3. Electron Elevator: Excitations across the Band Gap via a Dynamical Gap State.

    PubMed

    Lim, A; Foulkes, W M C; Horsfield, A P; Mason, D R; Schleife, A; Draeger, E W; Correa, A A

    2016-01-29

    We use time-dependent density functional theory to study self-irradiated Si. We calculate the electronic stopping power of Si in Si by evaluating the energy transferred to the electrons per unit path length by an ion of kinetic energy from 1 eV to 100 keV moving through the host. Electronic stopping is found to be significant below the threshold velocity normally identified with transitions across the band gap. A structured crossover at low velocity exists in place of a hard threshold. An analysis of the time dependence of the transition rates using coupled linear rate equations enables one of the excitation mechanisms to be clearly identified: a defect state induced in the gap by the moving ion acts like an elevator and carries electrons across the band gap.

  4. Energy band alignment and electronic states of amorphous carbon surfaces in vacuo and in aqueous environment

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Caro, Miguel A., E-mail: mcaroba@gmail.com; Department of Applied Physics, COMP Centre of Excellence in Computational Nanoscience, Aalto University, Espoo; Määttä, Jukka

    2015-01-21

    In this paper, we obtain the energy band positions of amorphous carbon (a–C) surfaces in vacuum and in aqueous environment. The calculations are performed using a combination of (i) classical molecular dynamics (MD), (ii) Kohn-Sham density functional theory with the Perdew-Burke-Ernzerhof (PBE) exchange-correlation functional, and (iii) the screened-exchange hybrid functional of Heyd, Scuseria, and Ernzerhof (HSE). PBE allows an accurate generation of a-C and the evaluation of the local electrostatic potential in the a-C/water system, HSE yields an improved description of energetic positions which is critical in this case, and classical MD enables a computationally affordable description of water. Ourmore » explicit calculation shows that, both in vacuo and in aqueous environment, the a-C electronic states available in the region comprised between the H{sub 2}/H{sub 2}O and O{sub 2}/H{sub 2}O levels of water correspond to both occupied and unoccupied states within the a-C pseudogap region. These are localized states associated to sp{sup 2} sites in a-C. The band realignment induces a shift of approximately 300 meV of the a-C energy band positions with respect to the redox levels of water.« less

  5. Electron elevator: Excitations across the band gap via a dynamical gap state

    DOE PAGES

    Lim, Anthony; Foulkes, W. M. C.; Horsfield, A. P.; ...

    2016-01-27

    We use time-dependent density functional theory to study self-irradiated Si. We calculate the electronic stopping power of Si in Si by evaluating the energy transferred to the electrons per unit path length by an ion of kinetic energy from 1 eV to 100 keV moving through the host. Electronic stopping is found to be significant below the threshold velocity normally identified with transitions across the band gap. A structured crossover at low velocity exists in place of a hard threshold. Lastly, an analysis of the time dependence of the transition rates using coupled linear rate equations enables one of themore » excitation mechanisms to be clearly identified: a defect state induced in the gap by the moving ion acts like an elevator and carries electrons across the band gap.« less

  6. Calculation of Energy Diagram of Asymmetric Graded-Band-Gap Semiconductor Superlattices.

    PubMed

    Monastyrskii, Liubomyr S; Sokolovskii, Bogdan S; Alekseichyk, Mariya P

    2017-12-01

    The paper theoretically investigates the peculiarities of energy diagram of asymmetric graded-band-gap superlattices with linear coordinate dependences of band gap and electron affinity. For calculating the energy diagram of asymmetric graded-band-gap superlattices, linearized Poisson's equation has been solved for the two layers forming a period of the superlattice. The obtained coordinate dependences of edges of the conduction and valence bands demonstrate substantial transformation of the shape of the energy diagram at changing the period of the lattice and the ratio of width of the adjacent layers. The most marked changes in the energy diagram take place when the period of lattice is comparable with the Debye screening length. In the case when the lattice period is much smaller that the Debye screening length, the energy diagram has the shape of a sawtooth-like pattern.

  7. Calculation of the Energy-Band Structure of the Kronig-Penney Model Using the Nearly-Free and Tightly-Bound-Electron Approximations

    ERIC Educational Resources Information Center

    Wetsel, Grover C., Jr.

    1978-01-01

    Calculates the energy-band structure of noninteracting electrons in a one-dimensional crystal using exact and approximate methods for a rectangular-well atomic potential. A comparison of the two solutions as a function of potential-well depth and ratio of lattice spacing to well width is presented. (Author/GA)

  8. Design and application of multimegawatt X -band deflectors for femtosecond electron beam diagnostics

    DOE PAGES

    Dolgashev, Valery A.; Bowden, Gordon; Ding, Yuantao; ...

    2014-10-02

    Performance of the x-ray free electron laser Linac Coherent Light Source (LCLS) and the Facility for Advanced Accelerator Experimental Tests (FACET) is determined by the properties of their extremely short electron bunches. Multi-GeV electron bunches in both LCLS and FACET are less than 100 fs long. Optimization of beam properties and understanding of free-electron laser operation require electron beam diagnostics with time resolution of about 10 fs. We designed, built and commissioned a set of high frequency X-band deflectors which can measure the beam longitudinal space charge distribution and slice energy spread to better than 10 fs resolution at fullmore » LCLS energy (14 GeV), and with 70 fs resolution at full FACET energy (20 GeV). Use of high frequency and high gradient in these devices allows them to reach unprecedented performance. We report on the physics motivation, design considerations, operational configuration, cold tests, and typical results of the X-band deflector systems currently in use at SLAC.« less

  9. Quantifying electronic band interactions in van der Waals materials using angle-resolved reflected-electron spectroscopy.

    PubMed

    Jobst, Johannes; van der Torren, Alexander J H; Krasovskii, Eugene E; Balgley, Jesse; Dean, Cory R; Tromp, Rudolf M; van der Molen, Sense Jan

    2016-11-29

    High electron mobility is one of graphene's key properties, exploited for applications and fundamental research alike. Highest mobility values are found in heterostructures of graphene and hexagonal boron nitride, which consequently are widely used. However, surprisingly little is known about the interaction between the electronic states of these layered systems. Rather pragmatically, it is assumed that these do not couple significantly. Here we study the unoccupied band structure of graphite, boron nitride and their heterostructures using angle-resolved reflected-electron spectroscopy. We demonstrate that graphene and boron nitride bands do not interact over a wide energy range, despite their very similar dispersions. The method we use can be generally applied to study interactions in van der Waals systems, that is, artificial stacks of layered materials. With this we can quantitatively understand the 'chemistry of layers' by which novel materials are created via electronic coupling between the layers they are composed of.

  10. Sub-band gap photo-enhanced secondary electron emission from high-purity single-crystal chemical-vapor-deposited diamond

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Yater, J. E., E-mail: joan.yater@nrl.navy.mil; Shaw, J. L.; Pate, B. B.

    2016-02-07

    Secondary-electron-emission (SEE) current measured from high-purity, single-crystal (100) chemical-vapor-deposited diamond is found to increase when sub-band gap (3.06 eV) photons are incident on the hydrogenated surface. Although the light does not produce photoemission directly, the SEE current increases by more than a factor of 2 before saturating with increasing laser power. In energy distribution curves (EDCs), the emission peak shows a corresponding increase in intensity with increasing laser power. However, the emission-onset energy in the EDCs remains constant, indicating that the bands are pinned at the surface. On the other hand, changes are observed on the high-energy side of the distributionmore » as the laser power increases, with a well-defined shoulder becoming more pronounced. From an analysis of this feature in the EDCs, it is deduced that upward band bending is present in the near-surface region during the SEE measurements and this band bending suppresses the SEE yield. However, sub-band gap photon illumination reduces the band bending and thereby increases the SEE current. Because the bands are pinned at the surface, we conclude that the changes in the band levels occur below the surface in the electron transport region. Sample heating produces similar effects as observed with sub-band gap photon illumination, namely, an increase in SEE current and a reduction in band bending. However, the upward band bending is not fully removed by either increasing laser power or temperature, and a minimum band bending of ∼0.8 eV is established in both cases. The sub-band gap photo-excitation mechanism is under further investigation, although it appears likely at present that defect or gap states play a role in the photo-enhanced SEE process. In the meantime, the study demonstrates the ability of visible light to modify the electronic properties of diamond and enhance the emission capabilities, which may have potential impact for diamond-based vacuum

  11. Surface-plasmon enhanced photodetection at communication band based on hot electrons

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Wu, Kai; Zhan, Yaohui, E-mail: yhzhan@suda.edu.cn, E-mail: xfli@suda.edu.cn; Wu, Shaolong

    2015-08-14

    Surface plasmons can squeeze light into a deep-subwavelength space and generate abundant hot electrons in the nearby metallic regions, enabling a new paradigm of photoconversion by the way of hot electron collection. Unlike the visible spectral range concerned in previous literatures, we focus on the communication band and design the infrared hot-electron photodetectors with plasmonic metal-insulator-metal configuration by using full-wave finite-element method. Titanium dioxide-silver Schottky interface is employed to boost the low-energy infrared photodetection. The photodetection sensitivity is strongly improved by enhancing the plasmonic excitation from a rationally engineered metallic grating, which enables a strong unidirectional photocurrent. With a five-stepmore » electrical simulation, the optimized device exhibits an unbiased responsivity of ∼0.1 mA/W and an ultra-narrow response band (FWHM = 4.66 meV), which promises to be a candidate as the compact photodetector operating in communication band.« less

  12. Kinks in the σ band of graphene induced by electron-phonon coupling.

    PubMed

    Mazzola, Federico; Wells, Justin W; Yakimova, Rositza; Ulstrup, Søren; Miwa, Jill A; Balog, Richard; Bianchi, Marco; Leandersson, Mats; Adell, Johan; Hofmann, Philip; Balasubramanian, T

    2013-11-22

    Angle-resolved photoemission spectroscopy reveals pronounced kinks in the dispersion of the σ band of graphene. Such kinks are usually caused by the combination of a strong electron-boson interaction and the cutoff in the Fermi-Dirac distribution. They are therefore not expected for the σ band of graphene that has a binding energy of more than ≈3.5 eV. We argue that the observed kinks are indeed caused by the electron-phonon interaction, but the role of the Fermi-Dirac distribution cutoff is assumed by a cutoff in the density of σ states. The existence of the effect suggests a very weak coupling of holes in the σ band not only to the π electrons of graphene but also to the substrate electronic states. This is confirmed by the presence of such kinks for graphene on several different substrates that all show a strong coupling constant of λ≈1.

  13. Correlation effects and electronic properties of Cr-substituted SZn with an intermediate band.

    PubMed

    Tablero, C

    2005-09-15

    A study using first principles of the electronic properties of S32Zn31Cr, a material derived from the SZn host semiconductor where a Cr atom has been substituted for each of the 32 Zn atoms, is presented. This material has an intermediate band sandwiched between the valence and conduction bands of the host semiconductor, which in a formal band-theoretic picture is metallic because the Fermi energy is located within the impurity band. The potential technological application of these materials is that when they are used to absorb photons in solar cells, the efficiency increases significantly with respect to the host semiconductor. An analysis of the gaps, bandwidths, density of states, total and orbital charges, and electronic density is carried out. The main effects of the local-density approximation with a Hubbard term corrections are an increase in the bandwidth, a modification of the relative composition of the five d and p transition-metal orbitals, and a splitting of the intermediate band. The results demonstrate that the main contribution to the intermediate band is the Cr atom. For values of U greater than 6 eV, where U is the empirical Hubbard term U parameter, this band is unfolded, thus creating two bands, a full one below the Fermi energy and an empty one above it, i.e., a metal-insulator transition.

  14. Quantifying electronic band interactions in van der Waals materials using angle-resolved reflected-electron spectroscopy

    PubMed Central

    Jobst, Johannes; van der Torren, Alexander J. H.; Krasovskii, Eugene E.; Balgley, Jesse; Dean, Cory R.; Tromp, Rudolf M.; van der Molen, Sense Jan

    2016-01-01

    High electron mobility is one of graphene's key properties, exploited for applications and fundamental research alike. Highest mobility values are found in heterostructures of graphene and hexagonal boron nitride, which consequently are widely used. However, surprisingly little is known about the interaction between the electronic states of these layered systems. Rather pragmatically, it is assumed that these do not couple significantly. Here we study the unoccupied band structure of graphite, boron nitride and their heterostructures using angle-resolved reflected-electron spectroscopy. We demonstrate that graphene and boron nitride bands do not interact over a wide energy range, despite their very similar dispersions. The method we use can be generally applied to study interactions in van der Waals systems, that is, artificial stacks of layered materials. With this we can quantitatively understand the ‘chemistry of layers' by which novel materials are created via electronic coupling between the layers they are composed of. PMID:27897180

  15. Electron momentum density and band structure calculations of α- and β-GeTe

    NASA Astrophysics Data System (ADS)

    Vadkhiya, Laxman; Arora, Gunjan; Rathor, Ashish; Ahuja, B. L.

    2011-12-01

    We have measured isotropic experimental Compton profile of α-GeTe by employing high energy (662 keV) γ-radiation from a 137Cs isotope. To compare our experiment, we have also computed energy bands, density of states, electron momentum densities and Compton profiles of α- and β-phases of GeTe using the linear combination of atomic orbitals method. The electron momentum density is found to play a major role in understanding the topology of bands in the vicinity of the Fermi level. It is seen that the density functional theory (DFT) with generalised gradient approximation is relatively in better agreement with the experiment than the local density approximation and hybrid Hartree-Fock/DFT.

  16. Multi-band Electronic Structure of Ferromagnetic CeRuPO

    NASA Astrophysics Data System (ADS)

    Takahashi, Masaya; Ootsuki, Daiki; Horio, Masafumi; Arita, Masashi; Namatame, Hirofumi; Taniguchi, Masaki; Saini, Naurang L.; Sugawara, Hitoshi; Mizokawa, Takashi

    2018-04-01

    We have studied the multi-band electronic structure of ferromagnetic CeRuPO (TC = 15 K) by means of angle-resolved photoemission spectroscopy (ARPES). The ARPES results show that three hole bands exist around the zone center and two of them cross the Fermi level (EF). Around the zone corner, two electron bands are observed and cross EF. These hole and electron bands, which can be assigned to the Ru 4d bands, are basically consistent with the band-structure calculation including their orbital characters. However, one of the electron bands with Ru 4d 3z2 - r2 character is strongly renormalized indicating correlation effect due to hybridization with the Ce 4f orbitals. The Ru 4d 3z2 - r2 band changes across TC suggesting that the out-of-plane 3z2 - r2 orbital channel plays essential roles in the ferromagnetism.

  17. Excitation of the Werner bands of H2 by electron impact

    NASA Technical Reports Server (NTRS)

    Stone, E. J.; Zipf, E. C.

    1972-01-01

    Absolute cross sections for the excitation of the H2 Werner band system were measured from energy threshold to 300 eV for electron impact on H2. The bands were observed in emission in the wavelength region 1100A to 1250A. The measured cross sections were compared with published transition probabilities, leading to the conclusion that the Werner bands are suitable as the basis for a relative spectral response calibration only when the bands are observed under sufficiently high resolution. The effect of the perturbation between the C 1Pi u and B 1 Sigma-u states of the hydrogen molecule was clearly observed in anomalies in the rotational intensity distribution in bands of the (3 v '') progression.

  18. Verification of band offsets and electron effective masses in GaAsN/GaAs quantum wells: Spectroscopic experiment versus 10-band k·p modeling

    NASA Astrophysics Data System (ADS)

    Ryczko, K.; Sek, G.; Sitarek, P.; Mika, A.; Misiewicz, J.; Langer, F.; Höfling, S.; Forchel, A.; Kamp, M.

    2013-06-01

    Optical transitions in GaAs1-xNx/GaAs quantum wells (QWs) have been probed by two complementary techniques, modulation spectroscopy in a form of photoreflectance and surface photovoltage spectroscopy. Transition energies in QWs of various widths and N contents have been compared with the results of band structure calculations based on the 10-band k.p Hamiltonian. Due to the observation of higher order transitions in the measured spectra, the band gap discontinuities at the GaAsN/GaAs interface and the electron effective masses could be determined, both treated as semi-free parameters to get the best matching between the theoretical and experimental energies. We have obtained the chemical conduction band offset values of 86% for x = 1.2% and 83% for x = 2.2%, respectively. For these determined band offsets, the electron effective masses equal to about 0.09 mo in QWs with 1.2% N and 0.15 mo for the case of larger N content of 2.2%.

  19. Asymmetry induces Q-band split in the electronic excitations of magnesium porphyrin

    NASA Astrophysics Data System (ADS)

    Jiang, Xiankai; Gao, Yi; Lal, Ratnesh; Hu, Jun; Song, Bo

    2018-07-01

    The electronic excitations of magnesium porphyrin (MgP), a molecular model for understanding the physics in light harvesting by biological systems, have been studied extensively. However, the theoretical underpinning of experimental measurements is still lacking, especially about the sub-bands in absorption spectrum. Here we propose that an asymmetry of MgP based on the uneven charge distribution of pyrrole rings and the linear structure of sp hybridised orbitals in Mg can largely influence the electronic excitations. Upon a very weak asymmetry of Mg-pyrrole bindings in MgP being introduced through the uneven distribution of charge, three different excitations are observed in the Q-band region of the experimental spectrum. Additionally, the predicted B-band excitations are highly correlated (10-2 eV level) with experimental measurements. In contrast, without this asymmetry, there are only two degenerate excitations in the Q-band region, and low agreement (10-1 eV level) of the B-band excitations with the experiment. The key physics of the unexpected and observable asymmetry in MgP is the ability of Mg to form sp hybridised orbitals on the third shell upon Mg binding to the nitrogen of pyrrole ring. Our findings provide new insight for high-energy efficiency of natural as well as artificial light-harvesting system for energy challenge.

  20. Energy level alignment and band bending at organic interfaces

    NASA Astrophysics Data System (ADS)

    Seki, Kazuhiko; Oji, Hiroshi; Ito, Eisuke; Hayashi, Naoki; Ouchi, Yukio; Ishii, Hisao

    1999-12-01

    Recent progress in the study of the energy level alignment and band bending at organic interfaces is reviewed, taking the examples mainly from the results of the group of the authors using ultraviolet photoelectron spectroscopy (UPS), metastable atom electron spectroscopy (MAES), and Kelvin probe method (KPM). As for the energy level alignment right at the interface, the formation of an electric dipole layer is observed for most of the organic/metal interfaces, even when no significant chemical interaction is observed. The origin of this dipole layer is examined by accumulating the data of various combinations of organics and metals, and the results indicate combined contribution from (1) charge transfer (CT) between the organic molecule and the metal, and (2) pushback of the electrons spilled out from metal surface, for the case of nonpolar organic molecule physisorbed on metals. Other factors such as chemical interaction and the orientation of polar molecules are also pointed out. As for the band bending, the careful examination of the existence/absence of band bending of purified TPD* molecule deposited on various metals in ultrahigh vacuum (UHV) revealed negligible band bending up to 100 nm thickness, and also the failure of the establishment of Fermi level alignment between organic layer and the metals. The implications of these findings are discussed, in relation to the future prospects of the studies in this field. (*:N,N'- diphenyl-N,N'-(3-methylphenyl)-1,1'-biphenyl-4,4'-diamine).

  1. Wave-function-based approach to quasiparticle bands: Insight into the electronic structure of c-ZnS

    NASA Astrophysics Data System (ADS)

    Stoyanova, A.; Hozoi, L.; Fulde, P.; Stoll, H.

    2011-05-01

    Ab initio wave-function-based methods are employed for the study of quasiparticle energy bands of zinc-blende ZnS, with focus on the Zn 3d “semicore” states. The relative energies of these states with respect to the top of the S 3p valence bands appear to be poorly described as compared to experimental values not only within the local density approximation (LDA), but also when many-body corrections within the GW approximation are applied to the LDA or LDA + U mean-field solutions [T. Miyake, P. Zhang, M. L. Cohen, and S. G. Louie, Phys. Rev. BPRBMDO1098-012110.1103/PhysRevB.74.245213 74, 245213 (2006)]. In the present study, we show that for the accurate description of the Zn 3d states a correlation treatment based on wave-function methods is needed. Our study rests on a local Hamiltonian approach which rigorously describes the short-range polarization and charge redistribution effects around an extra hole or electron placed into the valence respective conduction bands of semiconductors and insulators. The method also facilitates the computation of electron correlation effects beyond relaxation and polarization. The electron correlation treatment is performed on finite clusters cut off the infinite system. The formalism makes use of localized Wannier functions and embedding potentials derived explicitly from prior periodic Hartree-Fock calculations. The on-site and nearest-neighbor charge relaxation lead to corrections of several eV to the Hartree-Fock band energies and gap. Corrections due to long-range polarization are of the order of 1.0 eV. The dispersion of the Hartree-Fock bands is only slightly affected by electron correlations. We find the Zn 3d “semicore” states to lie ~9.0 eV below the top of the S 3p valence bands, in very good agreement with values from valence-band x-ray photoemission.

  2. Banded Structures in Electron Pitch Angle Diffusion Coefficients from Resonant Wave Particle Interactions

    NASA Technical Reports Server (NTRS)

    Tripathi, A. K.; Singhal, R. P.; Khazanov, G. V.; Avanov, L. A.

    2016-01-01

    Electron pitch angle (D (alpha)) and momentum (D(pp)) diffusion coefficients have been calculated due to resonant interactions with electrostatic electron cyclotron harmonic (ECH) and whistler mode chorus waves. Calculations have been performed at two spatial locations L = 4.6 and 6.8 for electron energies 10 keV. Landau (n = 0) resonance and cyclotron harmonic resonances n = +/-1, +/-2,...+/-5 have been included in the calculations. It is found that diffusion coefficient versus pitch angle (alpha) profiles show large dips and oscillations or banded structures. The structures are more pronounced for ECH and lower band chorus (LBC) and particularly at location 4.6. Calculations of diffusion coefficients have also been performed for individual resonances. It is noticed that the main contribution of ECH waves in pitch angle diffusion coefficient is due to resonances n = +1 and n = +2. A major contribution to momentum diffusion coefficients appears from n = +2. However, the banded structures in D alpha and Dpp coefficients appear only in the profile of diffusion coefficients for n = +2. The contribution of other resonances to diffusion coefficients is found to be, in general, quite small or even negligible. For LBC and upper band chorus waves, the banded structures appear only in Landau resonance. The Dpp diffusion coefficient for ECH waves is one to two orders smaller than D alpha coefficients. For chorus waves, Dpp coefficients are about an order of magnitude smaller than D alpha coefficients for the case n does not = 0. In case of Landau resonance, the values of Dpp coefficient are generally larger than the values of D alpha coefficients particularly at lower energies. As an aid to the interpretation of results, we have also determined the resonant frequencies. For ECH waves, resonant frequencies have been estimated for wave normal angle 89 deg and harmonic resonances n = +1, +2, and +3, whereas for whistler mode waves, the frequencies have been calculated for angle

  3. The dependence of the tunneling characteristic on the electronic energy bands and the carrier’s states of Graphene superlattice

    NASA Astrophysics Data System (ADS)

    Yang, C. H.; Shen, G. Z.; Ao, Z. M.; Xu, Y. W.

    2016-09-01

    Using the transfer matrix method, the carrier tunneling properties in graphene superlattice generated by the Thue-Morse sequence and Kolakoski sequence are investigated. The positions and strength of the transmission can be modulated by the barrier structures, the incident energy and angle, the height and width of the potential. These carriers tunneling characteristic can be understood from the energy band structures in the corresponding superlattice systems and the carrier’s states in well/barriers. The transmission peaks above the critical incident angle rely on the carrier’s resonance in the well regions. The structural diversity can modulate the electronic and transport properties, thus expanding its applications.

  4. Measurement of the low energy spectral contribution in coincidence with valence band (VB) energy levels of Ag(100) using VB-VB coincidence spectroscopy

    NASA Astrophysics Data System (ADS)

    Gladen, R. W.; Joglekar, P. V.; Lim, Z. H.; Shastry, K.; Hulbert, S. L.; Weiss, A. H.

    A set of coincidence measurements were obtained for the study and measurement of the electron contribution arising from the inter-valence band (VB) transitions along with the inelastically scattered VB electron contribution. These Auger-unrelated contributions arise in the Auger spectrum (Ag 4p NVV) obtained using Auger Photoelectron Coincidence Spectroscopy (APECS). The measured Auger-unrelated contribution can be eliminated from Auger spectrum to obtain the spectrum related to Auger. In our VB-VB coincidence measurement, a photon beam of energy 180eV was used to probe the Ag(100) sample. The coincidence spectrum was obtained using two Cylindrical Mirror Analyzers (CMA's). The scan CMA measured the low energy electron contribution in the energy range 0-70eV in coincidence with VB electrons measured by the fixed CMA. In this talk, we present the data obtained for VB-VB coincidence at the valence band energy of 171eV along with the coincidence measurements in the energy range of 4p core and valence band. NSF DMR 0907679, NSF Award Number: 1213727. Use of the National Synchrotron Light Source, Brookhaven National Laboratory, was supported by the U.S. DOE, Office of Science, Office of Basic Energy Sciences, under Contract No. DEAC02-98CH10886.

  5. Measurement of the low energy spectral contribution in coincidence with valence band (VB) energy levels of Ag(100) using VB-VB coincidence spectroscopy

    NASA Astrophysics Data System (ADS)

    Joglekar, P. V.; Gladen, R.; Lim, Z. H.; Shastry, K.; Hulbert, S. L.; Weiss, A. H.

    2015-03-01

    A set of coincidence measurements were obtained for the study and measurement of the electron contribution arising from the inter-valence band (VB) transitions along with the inelastically scattered VB electron contribution. These Auger-unrelated contributions arise in the Auger spectrum (Ag 4p NVV) obtained using Auger Photoelectron Coincidence Spectroscopy (APECS). The measured Auger-unrelated contribution can be eliminated from Auger spectrum to obtain the spectrum related to Auger. In our VB-VB coincidence measurement, a photon beam of energy 180eV was used to probe the Ag(100) sample. The coincidence spectrum was obtained using two Cylindrical Mirror Analyzers (CMA's). The scan CMA measured the low energy electron contribution in the energy range 0-70eV in coincidence with VB electrons measured by the fixed CMA. In this talk, we present the data obtained for VB-VB coincidence at the valence band energy of 171eV along with the coincidence measurements in the energy range of 4p core and valence band. NSF DMR 0907679, NSF Award Number: 1213727. Use of the National Synchrotron Light Source, Brookhaven National Laboratory, was supported by the U.S. DOE, Office of Science, Office of Basic Energy Sciences, under Contract No. DE-AC02-98CH10886.

  6. Electron affinities and ionization energies of Cu and Ag delafossite compounds: A hybrid functional study

    NASA Astrophysics Data System (ADS)

    Miao, Mao-Sheng; Yarbro, Sam; Barton, Phillip T.; Seshadri, Ram

    2014-01-01

    Using density functional theory with a hybrid functional, we calculate the ionization energies and electron affinities of a series of delafossite compounds (AMO2: A =Cu, Ag; M =B, Al, Ga, In, Sc). The alignments of the valence band maximum and the conduction band minimum, which directly relate to the ionization energies and electron affinities, were obtained by calculations of supercell slab models constructed in a nonpolar orientation. Our calculations reveal that the ionization energy decreases with an increasing atomic number of group-III elements, and thus suggest an improved p-type doping propensity for heavier compounds. For keeping both a low ionization energy and a band gap of sufficient size, CuScO2 is superior to the Cu-based group-III delafossites. By analyzing the electronic structures, we demonstrate that the compositional trend of the ionization energies and electron affinities is the result of a combined effect of d-band broadening due to Cu(Ag)-Cu(Ag) coupling and a repositioning of the d-band center.

  7. Wavefunction Properties and Electronic Band Structures of High-Mobility Semiconductor Nanosheet MoS2

    NASA Astrophysics Data System (ADS)

    Baik, Seung Su; Lee, Hee Sung; Im, Seongil; Choi, Hyoung Joon; Ccsaemp Team; Edl Team

    2014-03-01

    Molybdenum disulfide (MoS2) nanosheet is regarded as one of the most promising alternatives to the current semiconductors due to its significant band-gap and electron-mobility enhancement upon exfoliating. To elucidate such thickness-dependent properties, we have studied the electronic band structures of bulk and monolayer MoS2 by using the first-principles density-functional method as implemented in the SIESTA code. Based on the wavefunction analyses at the conduction band minimum (CBM) points, we have investigated possible origins of mobility difference between bulk and monolayer MoS2. We provide formation energies of substitutional impurities at the Mo and S sites, and discuss feasible electron sources which may induce a significant difference in the carrier lifetime. This work was supported by NRF of Korea (Grant Nos. 2009-0079462 and 2011-0018306), Nano-Material Technology Development Program (2012M3a7B4034985), and KISTI supercomputing center (Project No. KSC-2013-C3-008). Center for Computational Studies of Advanced Electronic Material Properties.

  8. High-perveance W-band Sheet-beam Electron Gun Design

    DTIC Science & Technology

    2008-04-01

    APR 2008 2. REPORT TYPE 3. DATES COVERED 00-00-2008 to 00-00-2008 4. TITLE AND SUBTITLE High -perveance W- band Sheet-beam Electron Gun Design 5a...8-98) Prescribed by ANSI Std Z39-18 10.1: High -perveance W- band Sheet-beam Electron Gun Design Khanh T. Nguyen1, John Pasour, Edward L. Wright1...effects due to cathode temperature are also included in the simulation. Keywords: Sheet beam; W- band ; electron gun; high perveance; amplifiers

  9. Discrete Electronic Bands in Semiconductors and Insulators: Potential High-Light-Yield Scintillators

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Shi, Hongliang; Du, Mao-Hua

    Bulk semiconductors and insulators typically have continuous valence and conduction bands. In this paper, we show that valence and conduction bands of a multinary semiconductor or insulator can be split to narrow discrete bands separated by large energy gaps. This unique electronic structure is demonstrated by first-principles calculations in several quaternary elpasolite compounds, i.e., Cs 2NaInBr 6, Cs 2NaBiCl 6, and Tl 2NaBiCl 6. The narrow discrete band structure in these quaternary elpasolites is due to the large electronegativity difference among cations and the large nearest-neighbor distances in cation sublattices. We further use Cs 2NaInBr 6 as an example tomore » show that the narrow bands can stabilize self-trapped and dopant-bound excitons (in which both the electron and the hole are strongly localized in static positions on adjacent sites) and promote strong exciton emission at room temperature. The discrete band structure should further suppress thermalization of hot carriers and may lead to enhanced impact ionization, which is usually considered inefficient in bulk semiconductors and insulators. Finally, these characteristics can enable efficient room-temperature light emission in low-gap scintillators and may overcome the light-yield bottleneck in current scintillator research.« less

  10. Discrete Electronic Bands in Semiconductors and Insulators: Potential High-Light-Yield Scintillators

    DOE PAGES

    Shi, Hongliang; Du, Mao-Hua

    2015-05-12

    Bulk semiconductors and insulators typically have continuous valence and conduction bands. In this paper, we show that valence and conduction bands of a multinary semiconductor or insulator can be split to narrow discrete bands separated by large energy gaps. This unique electronic structure is demonstrated by first-principles calculations in several quaternary elpasolite compounds, i.e., Cs 2NaInBr 6, Cs 2NaBiCl 6, and Tl 2NaBiCl 6. The narrow discrete band structure in these quaternary elpasolites is due to the large electronegativity difference among cations and the large nearest-neighbor distances in cation sublattices. We further use Cs 2NaInBr 6 as an example tomore » show that the narrow bands can stabilize self-trapped and dopant-bound excitons (in which both the electron and the hole are strongly localized in static positions on adjacent sites) and promote strong exciton emission at room temperature. The discrete band structure should further suppress thermalization of hot carriers and may lead to enhanced impact ionization, which is usually considered inefficient in bulk semiconductors and insulators. Finally, these characteristics can enable efficient room-temperature light emission in low-gap scintillators and may overcome the light-yield bottleneck in current scintillator research.« less

  11. Quasiparticle band gap of organic-inorganic hybrid perovskites: Crystal structure, spin-orbit coupling, and self-energy effects

    NASA Astrophysics Data System (ADS)

    Gao, Weiwei; Gao, Xiang; Abtew, Tesfaye A.; Sun, Yi-Yang; Zhang, Shengbai; Zhang, Peihong

    2016-02-01

    The quasiparticle band gap is one of the most important materials properties for photovoltaic applications. Often the band gap of a photovoltaic material is determined (and can be controlled) by various factors, complicating predictive materials optimization. An in-depth understanding of how these factors affect the size of the gap will provide valuable guidance for new materials discovery. Here we report a comprehensive investigation on the band gap formation mechanism in organic-inorganic hybrid perovskites by decoupling various contributing factors which ultimately determine their electronic structure and quasiparticle band gap. Major factors, namely, quasiparticle self-energy, spin-orbit coupling, and structural distortions due to the presence of organic molecules, and their influences on the quasiparticle band structure of organic-inorganic hybrid perovskites are illustrated. We find that although methylammonium cations do not contribute directly to the electronic states near band edges, they play an important role in defining the band gap by introducing structural distortions and controlling the overall lattice constants. The spin-orbit coupling effects drastically reduce the electron and hole effective masses in these systems, which is beneficial for high carrier mobilities and small exciton binding energies.

  12. Nanoscale charge distribution and energy band modification in defect-patterned graphene.

    PubMed

    Wang, Shengnan; Wang, Rui; Wang, Xiaowei; Zhang, Dongdong; Qiu, Xiaohui

    2012-04-21

    Defects were introduced precisely to exfoliated graphene (G) sheets on a SiO(2)/n(+) Si substrate to modulate the local energy band structure and the electron pathway using solution-phase oxidation followed by thermal reduction. The resulting nanoscale charge distribution and band gap modification were investigated by electrostatic force microscopy and spectroscopy. A transition phase with coexisting submicron-sized metallic and insulating regions in the moderately oxidized monolayer graphene were visualized and measured directly. It was determined that the delocalization of electrons/holes in a graphene "island" is confined by the surrounding defective C-O matrix, which acts as an energy barrier for mobile charge carriers. In contrast to the irreversible structural variations caused by the oxidation process, the electrical properties of graphene can be restored by annealing. The defect-patterned graphene and graphene oxide heterojunctions were further characterized by electrical transport measurement.

  13. Characteristic energy range of electron scattering due to plasmaspheric hiss

    DOE PAGES

    Ma, Q.; Li, W.; Thorne, R. M.; ...

    2016-11-15

    In this paper, we investigate the characteristic energy range of electron flux decay due to the interaction with plasmaspheric hiss in the Earth's inner magnetosphere. The Van Allen Probes have measured the energetic electron flux decay profiles in the Earth's outer radiation belt during a quiet period following the geomagnetic storm that occurred on 7 November 2015. The observed energy of significant electron decay increases with decreasing L shell and is well correlated with the energy band corresponding to the first adiabatic invariant μ = 4–200 MeV/G. The electron diffusion coefficients due to hiss scattering are calculated at L =more » 2–6, and the modeled energy band of effective pitch angle scattering is also well correlated with the constant μ lines and is consistent with the observed energy range of electron decay. Using the previously developed statistical plasmaspheric hiss model during modestly disturbed periods, we perform a 2-D Fokker-Planck simulation of the electron phase space density evolution at L = 3.5 and demonstrate that plasmaspheric hiss causes the significant decay of 100 keV–1 MeV electrons with the largest decay rate occurring at around 340 keV, forming anisotropic pitch angle distributions at lower energies and more flattened distributions at higher energies. Finally, our study provides reasonable estimates of the electron populations that can be most significantly affected by plasmaspheric hiss and the consequent electron decay profiles.« less

  14. Banded structures in electron pitch angle diffusion coefficients from resonant wave-particle interactions

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Tripathi, A. K., E-mail: aktrip2001@yahoo.co.in; Singhal, R. P., E-mail: rpsiitbhu@yahoo.com; Khazanov, G. V., E-mail: George.V.Khazanov@nasa.gov

    2016-04-15

    Electron pitch angle (D{sub αα}) and momentum (D{sub pp}) diffusion coefficients have been calculated due to resonant interactions with electrostatic electron cyclotron harmonic (ECH) and whistler mode chorus waves. Calculations have been performed at two spatial locations L = 4.6 and 6.8 for electron energies ≤10 keV. Landau (n = 0) resonance and cyclotron harmonic resonances n = ±1, ±2, … ±5 have been included in the calculations. It is found that diffusion coefficient versus pitch angle (α) profiles show large dips and oscillations or banded structures. The structures are more pronounced for ECH and lower band chorus (LBC) and particularly at location 4.6. Calculations of diffusionmore » coefficients have also been performed for individual resonances. It is noticed that the main contribution of ECH waves in pitch angle diffusion coefficient is due to resonances n = +1 and n = +2. A major contribution to momentum diffusion coefficients appears from n = +2. However, the banded structures in D{sub αα} and D{sub pp} coefficients appear only in the profile of diffusion coefficients for n = +2. The contribution of other resonances to diffusion coefficients is found to be, in general, quite small or even negligible. For LBC and upper band chorus waves, the banded structures appear only in Landau resonance. The D{sub pp} diffusion coefficient for ECH waves is one to two orders smaller than D{sub αα} coefficients. For chorus waves, D{sub pp} coefficients are about an order of magnitude smaller than D{sub αα} coefficients for the case n ≠ 0. In case of Landau resonance, the values of D{sub pp} coefficient are generally larger than the values of D{sub αα} coefficients particularly at lower energies. As an aid to the interpretation of results, we have also determined the resonant frequencies. For ECH waves, resonant frequencies have been estimated for wave normal angle 89° and harmonic resonances n = +1, +2, and

  15. Banded Structures in Electron Pitch Angle Diffusion Coefficients from Resonant Wave-Particle Interactions

    NASA Technical Reports Server (NTRS)

    Tripathi, A. K.; Singhal, R. P.; Khazanov, G. V.; Avanov, L. A.

    2016-01-01

    Electron pitch angle (D(sub (alpha alpha))) and momentum (D(sub pp)) diffusion coefficients have been calculated due to resonant interactions with electrostatic electron cyclotron harmonic (ECH) and whistler mode chorus waves. Calculations have been performed at two spatial locations L=4.6 and 6.8 for electron energies less than or equal to 10 keV. Landau (n=0) resonance and cyclotron harmonic resonances n= +/- 1, +/-2, ... +/-5 have been included in the calculations. It is found that diffusion coefficient versus pitch angle (alpha) profiles show large dips and oscillations or banded structures. The structures are more pronounced for ECH and lower band chorus (LBC) and particularly at location 4.6. Calculations of diffusion coefficients have also been performed for individual resonances. It is noticed that the main contribution of ECH waves in pitch angle diffusion coefficient is due to resonances n=+1 and n=+2. A major contribution to momentum diffusion coefficients appears from n=+2. However, the banded structures in D(sub alpha alpha) and D(sub pp) coefficients appear only in the profile of diffusion coefficients for n=+2. The contribution of other resonances to diffusion coefficients is found to be, in general, quite small or even negligible. For LBC and upper band chorus waves, the banded structures appear only in Landau resonance. The D(sub pp) diffusion coefficient for ECH waves is one to two orders smaller than D(sub alpha alpha) coefficients. For chorus waves, D(sub pp) coefficients are about an order of magnitude smaller than D(sub alpha alpha) coefficients for the case n does not equal 0. In case of Landau resonance, the values of D(sub pp) coefficient are generally larger than the values of D(sub alpha alpha) coefficients particularly at lower energies. As an aid to the interpretation of results, we have also determined the resonant frequencies. For ECH waves, resonant frequencies have been estimated for wave normal angle 89 deg and harmonic resonances

  16. Electron and hole photoemission detection for band offset determination of tunnel field-effect transistor heterojunctions

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Li, Wei; Key Laboratory for the Physics and Chemistry of Nanodevices and Department of Electronics, Peking University, Beijing 100871; Zhang, Qin

    2014-11-24

    We report experimental methods to ascertain a complete energy band alignment of a broken-gap tunnel field-effect transistor based on an InAs/GaSb hetero-junction. By using graphene as an optically transparent electrode, both the electron and hole barrier heights at the InAs/GaSb interface can be quantified. For a Al{sub 2}O{sub 3}/InAs/GaSb layer structure, the barrier height from the top of the InAs and GaSb valence bands to the bottom of the Al{sub 2}O{sub 3} conduction band is inferred from electron emission whereas hole emissions reveal the barrier height from the top of the Al{sub 2}O{sub 3} valence band to the bottom ofmore » the InAs and GaSb conduction bands. Subsequently, the offset parameter at the broken gap InAs/GaSb interface is extracted and thus can be used to facilitate the development of predicted models of electron quantum tunneling efficiency and transistor performance.« less

  17. 8-band and 14-band kp modeling of electronic band structure and material gain in Ga(In)AsBi quantum wells grown on GaAs and InP substrates

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Gladysiewicz, M.; Wartak, M. S.; Department of Physics and Computer Science, Wilfrid Laurier University, Waterloo, Ontario N2L 3C5

    The electronic band structure and material gain have been calculated for GaAsBi/GaAs quantum wells (QWs) with various bismuth concentrations (Bi ≤ 15%) within the 8-band and 14-band kp models. The 14-band kp model was obtained by extending the standard 8-band kp Hamiltonian by the valence band anticrossing (VBAC) Hamiltonian, which is widely used to describe Bi-related changes in the electronic band structure of dilute bismides. It has been shown that in the range of low carrier concentrations n < 5 × 10{sup 18 }cm{sup −3}, material gain spectra calculated within 8- and 14-band kp Hamiltonians are similar. It means that the 8-band kp model can be usedmore » to calculate material gain in dilute bismides QWs. Therefore, it can be applied to analyze QWs containing new dilute bismides for which the VBAC parameters are unknown. Thus, the energy gap and electron effective mass for Bi-containing materials are used instead of VBAC parameters. The electronic band structure and material gain have been calculated for 8 nm wide GaInAsBi QWs on GaAs and InP substrates with various compositions. In these QWs, Bi concentration was varied from 0% to 5% and indium concentration was tuned in order to keep the same compressive strain (ε = 2%) in QW region. For GaInAsBi/GaAs QW with 5% Bi, gain peak was determined to be at about 1.5 μm. It means that it can be possible to achieve emission at telecommunication windows (i.e., 1.3 μm and 1.55 μm) for GaAs-based lasers containing GaInAsBi/GaAs QWs. For GaInAsBi/Ga{sub 0.47}In{sub 0.53}As/InP QWs with 5% Bi, gain peak is predicted to be at about 4.0 μm, i.e., at the wavelengths that are not available in current InP-based lasers.« less

  18. Energy dependence of the spatial distribution of inelastically scattered electrons in backscatter electron diffraction

    NASA Astrophysics Data System (ADS)

    Ram, Farangis; De Graef, Marc

    2018-04-01

    In an electron backscatter diffraction pattern (EBSP), the angular distribution of backscattered electrons (BSEs) depends on their energy. Monte Carlo modeling of their depth and energy distributions suggests that the highest energy BSEs are more likely to hit the bottom of the detector than the top. In this paper, we examine experimental EBSPs to validate the modeled angular BSE distribution. To that end, the Kikuchi bandlet method is employed to measure the width of Kikuchi bands in both modeled and measured EBSPs. The results show that in an EBSP obtained with a 15 keV primary probe, the width of a Kikuchi band varies by about 0 .4∘ from the bottom of the EBSD detector to its top. The same is true for a simulated pattern that is composed of BSEs with 5 keV to 15 keV energies, which validates the Monte Carlo simulations.

  19. Theoretical study on electronic structure of bathocuproine: Renormalization of the band gap in the crystalline state and the large exciton binding energy

    NASA Astrophysics Data System (ADS)

    Yanagisawa, Susumu; Hatada, Shin-No-Suke; Morikawa, Yoshitada

    Bathocuproine (BCP) is a promising organic material of a hole blocking layer in organic light-emitting diodes or an electron buffer layer in organic photovoltaic cells. The nature of the unoccupied electronic states is a key characteristic of the material, which play vital roles in the electron transport. To elucidate the electronic properties of the molecular or crystalline BCP, we use the GW approximation for calculation of the fundamental gap, and the long-range corrected density functional theory for the molecular optical absorption. It is found that the band gap of the BCP single crystal is 4.39 eV, and it is in agreement with the recent low-energy inverse photoemission spectroscopy measurement. The polarization energy is estimated to be larger than 1 eV, demonstrating the large polarization effects induced by the electronic clouds surrounding the injected charge. The theoretical optical absorption energy is 3.68 eV, and the exciton binding energy is estimated to be 0.71 eV, implying the large binding in the eletron-hole pair distributed around the small part of the molecular region. This work was supported by the Grants-in-Aid for Young Scientists (B) (No. 26810009), and for Scientific Research on Innovative Areas ``3D Active-Site Science'' (No. 26105011) from Japan Society for the Promotion of Science.

  20. Energy band alignment of antiferroelectric (Pb,La)(Zr,Sn,Ti)O3

    NASA Astrophysics Data System (ADS)

    Klein, Andreas; Lohaus, Christian; Reiser, Patrick; Dimesso, Lucangelo; Wang, Xiucai; Yang, Tongqing

    2017-06-01

    The energy band alignment of antiferroelectric (Pb,La)(Zr,Sn,Ti)O3 is studied with photoelectron spectroscopy using interfaces with high work function RuO2 and low work function Sn-doped In2O3 (ITO). It is demonstrated how spectral deconvolution can be used to determine absolute Schottky barrier heights for insulating materials with a high accuracy. Using this approach it is found that the valence band maximum energy of (Pb,La)(Zr,Sn,Ti)O3 is found to be comparable to that of Pb- and Bi-containing ferroelectric materials, which is ∼1 eV higher than that of BaTiO3. The results provide additional evidence for the occupation of the 6s orbitals as origin of the higher valence band maximum, which is directly related to the electrical properties of such compounds. The results also verify that the energy band alignment determined by photoelectron spectroscopy of as-deposited electrodes is not influenced by polarisation. The electronic structure of (Pb,La)(Zr,Sn,Ti)O3 should enable doping of the material without strongly modifying its insulating properties, which is crucial for high energy density capacitors. Moreover, the position of the energy bands should result in a great freedom of selecting electrode materials in terms of avoiding charge injection.

  1. Transition-metal-substituted indium thiospinels as novel intermediate-band materials: prediction and understanding of their electronic properties.

    PubMed

    Palacios, P; Aguilera, I; Sánchez, K; Conesa, J C; Wahnón, P

    2008-07-25

    Results of density-functional calculations for indium thiospinel semiconductors substituted at octahedral sites with isolated transition metals (M=Ti,V) show an isolated partially filled narrow band containing three t2g-type states per M atom inside the usual semiconductor band gap. Thanks to this electronic structure feature, these materials will allow the absorption of photons with energy below the band gap, in addition to the normal light absorption of a semiconductor. To our knowledge, we demonstrate for the first time the formation of an isolated intermediate electronic band structure through M substitution at octahedral sites in a semiconductor, leading to an enhancement of the absorption coefficient in both infrared and visible ranges of the solar spectrum. This electronic structure feature could be applied for developing a new third-generation photovoltaic cell.

  2. Diamond /111/ studied by electron energy loss spectroscopy in the characteristic loss region

    NASA Technical Reports Server (NTRS)

    Pepper, S. V.

    1982-01-01

    Unoccupied surface states on diamond (111) annealed at greater than 900 C are studied by electron energy loss spectroscopy with valence band excitation. A feature found at 2.1 eV loss energy is attributed to an excitation from occupied surface states into unoccupied surface states of energy within the bulk band gap. A surface band gap of approximately 1 eV is estimated. This result supports a previous suggestion for unoccupied band gap states based on core level energy loss spectroscopy. Using the valence band excitation energy loss spectrosocpy, it is also suggested that hydrogen is removed from the as-polished diamond surface by a Menzel-Gomer-Redhead mechanism.

  3. Flat electronic bands in fractal-kagomé network and the effect of perturbation

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Nandy, Atanu, E-mail: atanunandy1989@gmail.com; Chakrabarti, Arunava, E-mail: arunava-chakrabarti@yahoo.co.in

    2016-05-06

    We demonstrate an analytical prescription of demonstrating the flat band [FB] states in a fractal incorporated kagomé type network that can give rise to a countable infinity of flat non-dispersive eigenstates with a multitude of localization area. The onset of localization can, in principle, be delayed in space by an appropriate choice of energy regime. The length scale, at which the onset of localization for each mode occurs, can be tuned at will following the formalism developed within the framework of real space renormalization group. This scheme leads to an exact determination of energy eigenvalue for which one can havemore » dispersionless flat electronic bands. Furthermore, we have shown the effect ofuniform magnetic field for the same non-translationally invariant network model that has ultimately led to an‘apparent invisibility’ of such staggered localized states and to generate absolutely continuous sub-bands in the energy spectrum and again an interesting re-entrant behavior of those FB states.« less

  4. Enhanced Spontaneous Emission of Bloch Oscillation Radiation from a Single Energy Band

    DTIC Science & Technology

    2006-06-30

    ignore interband tunneling , spon- taneous photon emission occurs as the Bloch electron inter- acts with the quantum radiation field; the emission occurs... interband coupling 17 and electron intraband scattering are ignored. Therefore, the quantum dynamics is described by the time-dependent Schrödinger...single band “n0” of a periodic crystal with energy n0K; the ef- fects of interband coupling15 and electron intraband scatter- ing are ignored

  5. Band Alignment and Controllable Electron Migration between Rutile and Anatase TiO2

    PubMed Central

    Mi, Yang; Weng, Yuxiang

    2015-01-01

    TiO2 is the most promising semiconductor for photocatalytic splitting of water for hydrogen and degradation of pollutants. The highly photocatalytic active form is its mixed phase of two polymorphs anatase and rutile rather than their pristine compositions. Such a synergetic effect is understood by the staggered band alignment favorable to spatial charge separation. However, electron migration in either direction between the two phases has been reported, the reason of which is still unknown. We determined the band alignment by a novel method, i.e., transient infrared absorption-excitation energy scanning spectra, showing their conduction bands being aligned, thus the electron migration direction is controlled by dynamical factors, such as varying the particle size of anatase, putting electron or hole scavengers on either the surface of anatase or rutile phases, or both. A quantitative criterion capable of predicting the migration direction under various conditions including particle size and surface chemical reactions is proposed, the predictions have been verified experimentally in several typical cases. This would give rise to a great potential in designing more effective titania photocatalysts. PMID:26169699

  6. HIGH-ENERGY ELECTRON IRRADIATION OF INTERSTELLAR CARBONACEOUS DUST ANALOGS: COSMIC-RAY EFFECTS ON THE CARRIERS OF THE 3.4 μ m ABSORPTION BAND

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Maté, Belén; Molpeceres, Germán; Jiménez-Redondo, Miguel

    2016-11-01

    The effects of cosmic rays on the carriers of the interstellar 3.4 μ m absorption band have been investigated in the laboratory. This band is attributed to stretching vibrations of CH{sub 3} and CH{sub 2} in carbonaceous dust. It is widely observed in the diffuse interstellar medium, but disappears in dense clouds. Destruction of CH{sub 3} and CH{sub 2} by cosmic rays could become relevant in dense clouds, shielded from the external ultraviolet field. For the simulations, samples of hydrogenated amorphous carbon (a-C:H) have been irradiated with 5 keV electrons. The decay of the band intensity versus electron fluence reflectsmore » a-C:H dehydrogenation, which is well described by a model assuming that H{sub 2} molecules, formed by the recombination of H atoms liberated through CH bond breaking, diffuse out of the sample. The CH bond destruction rates derived from the present experiments are in good accordance with those from previous ion irradiation experiments of HAC. The experimental simplicity of electron bombardment has allowed the use of higher-energy doses than in the ion experiments. The effects of cosmic rays on the aliphatic components of cosmic dust are found to be small. The estimated cosmic-ray destruction times for the 3.4 μ m band carriers lie in the 10{sup 8} yr range and cannot account for the disappearance of this band in dense clouds, which have characteristic lifetimes of 3 × 10{sup 7} yr. The results invite a more detailed investigation of the mechanisms of CH bond formation and breaking in the intermediate region between diffuse and dense clouds.« less

  7. Energy-banded ions in Saturn's magnetosphere

    NASA Astrophysics Data System (ADS)

    Thomsen, M. F.; Badman, S. V.; Jackman, C. M.; Jia, X.; Kivelson, M. G.; Kurth, W. S.

    2017-05-01

    Using data from the Cassini Plasma Spectrometer ion mass spectrometer, we report the first observation of energy-banded ions at Saturn. Observed near midnight at relatively high magnetic latitudes, the banded ions are dominantly H+, and they occupy the range of energies typically associated with the thermal pickup distribution in the inner magnetosphere (L < 10), but their energies decline monotonically with increasing radial distance (or time or decreasing latitude). Their pitch angle distribution suggests a source at low (or slightly southern) latitudes. The band energies, including their pitch angle dependence, are consistent with a bounce-resonant interaction between thermal H+ ions and the standing wave structure of a field line resonance. There is additional evidence in the pitch angle dependence of the band energies that the particles in each band may have a common time of flight from their most recent interaction with the wave, which may have been at slightly southern latitudes. Thus, while the particles are basically bounce resonant, their energization may be dominated by their most recent encounter with the standing wave.Plain Language SummaryDuring an outbound passage by the Cassini spacecraft through Saturn's inner magnetosphere, ion <span class="hlt">energy</span> distributions were observed that featured discrete flux peaks at regularly spaced <span class="hlt">energies</span>. The peaks persisted over several hours and several Saturn radii of distance away from the planet. We show that these "<span class="hlt">bands</span>" of ions are plausibly the result of an interaction between the Saturnian plasma and standing waves that form along the magnetospheric magnetic field lines. These observations are the first reported evidence that such standing waves may be present in the inner magnetosphere, where they could contribute to the radial transport of Saturn's radiation belt particles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JaJAP..54i1202S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JaJAP..54i1202S"><span>Interacting quasi-<span class="hlt">band</span> model for <span class="hlt">electronic</span> states in compound semiconductor alloys: Zincblende structure</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shinozuka, Yuzo; Oda, Masato</p> <p>2015-09-01</p> <p>The interacting quasi-<span class="hlt">band</span> model proposed for <span class="hlt">electronic</span> states in simple alloys is extended for compound semiconductor alloys with general lattice structures containing several atoms per unit cell. Using a tight-binding model, a variational <span class="hlt">electronic</span> wave function for quasi-Bloch states yields a non-Hermitian Hamiltonian matrix characterized by matrix elements of constituent crystals and concentration of constituents. Solving secular equations for each k-state yields the alloy’s <span class="hlt">energy</span> spectrum for any type of randomness and arbitrary concentration. The theory is used to address III-V (II-VI) alloys with a zincblende lattice with crystal <span class="hlt">band</span> structures well represented by the sp3s* model. Using the resulting 15 × 15 matrix, the concentration dependence of valence and conduction <span class="hlt">bands</span> is calculated in a unified scheme for typical alloys: Al1-xGaxAs, GaAs1-xPx, and GaSb1-xPx. Results agree well with experiments and are discussed with respect to the concentration dependence, direct-indirect gap transition, and <span class="hlt">band</span>-gap-bowing origin.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24576851','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24576851"><span>Superconductivity in an <span class="hlt">electron</span> <span class="hlt">band</span> just above the Fermi level: possible route to BCS-BEC superconductivity.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Okazaki, K; Ito, Y; Ota, Y; Kotani, Y; Shimojima, T; Kiss, T; Watanabe, S; Chen, C-T; Niitaka, S; Hanaguri, T; Takagi, H; Chainani, A; Shin, S</p> <p>2014-02-28</p> <p>Conventional superconductivity follows Bardeen-Cooper-Schrieffer(BCS) theory of <span class="hlt">electrons</span>-pairing in momentum-space, while superfluidity is the Bose-Einstein condensation(BEC) of atoms paired in real-space. These properties of solid metals and ultra-cold gases, respectively, are connected by the BCS-BEC crossover. Here we investigate the <span class="hlt">band</span> dispersions in FeTe(0.6)Se(0.4)(Tc = 14.5 K ~ 1.2 meV) in an accessible range below and above the Fermi level(EF) using ultra-high resolution laser angle-resolved photoemission spectroscopy. We uncover an <span class="hlt">electron</span> <span class="hlt">band</span> lying just 0.7 meV (~8 K) above EF at the Γ-point, which shows a sharp superconducting coherence peak with gap formation below Tc. The estimated superconducting gap Δ and Fermi <span class="hlt">energy</span> [Symbol: see text]F indicate composite superconductivity in an iron-based superconductor, consisting of strong-coupling BEC in the <span class="hlt">electron</span> <span class="hlt">band</span> and weak-coupling BCS-like superconductivity in the hole <span class="hlt">band</span>. The study identifies the possible route to BCS-BEC superconductivity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22305937-probing-optical-band-gaps-nanoscale-nifeo-cofeo-epitaxial-films-high-resolution-electron-energy-loss-spectroscopy','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22305937-probing-optical-band-gaps-nanoscale-nifeo-cofeo-epitaxial-films-high-resolution-electron-energy-loss-spectroscopy"><span>Probing optical <span class="hlt">band</span> gaps at the nanoscale in NiFe₂O₄ and CoFe₂O₄ epitaxial films by high resolution <span class="hlt">electron</span> <span class="hlt">energy</span> loss spectroscopy</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Dileep, K.; Loukya, B.; Datta, R., E-mail: ranjan@jncasr.ac.in</p> <p>2014-09-14</p> <p>Nanoscale optical <span class="hlt">band</span> gap variations in epitaxial thin films of two different spinel ferrites, i.e., NiFe₂O₄ (NFO) and CoFe₂O₄ (CFO), have been investigated by spatially resolved high resolution <span class="hlt">electron</span> <span class="hlt">energy</span> loss spectroscopy. Experimentally, both NFO and CFO show indirect/direct <span class="hlt">band</span> gaps around 1.52 eV/2.74 and 2.3 eV, and 1.3 eV/2.31 eV, respectively, for the ideal inverse spinel configuration with considerable standard deviation in the <span class="hlt">band</span> gap values for CFO due to various levels of deviation from the ideal inverse spinel structure. Direct probing of the regions in both the systems with tetrahedral A site cation vacancy, which is distinct frommore » the ideal inverse spinel configuration, shows significantly smaller <span class="hlt">band</span> gap values. The experimental results are supported by the density functional theory based modified Becke-Johnson exchange correlation potential calculated <span class="hlt">band</span> gap values for the different cation configurations.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JAP...121x4303Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JAP...121x4303Y"><span>Conductance modulation in Weyl semimetals with tilted <span class="hlt">energy</span> dispersion without a <span class="hlt">band</span> gap</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yesilyurt, Can; Siu, Zhuo Bin; Tan, Seng Ghee; Liang, Gengchiau; Jalil, Mansoor B. A.</p> <p>2017-06-01</p> <p>We investigate the tunneling conductance of Weyl semimetal with tilted <span class="hlt">energy</span> dispersion by considering <span class="hlt">electron</span> transmission through a p-n-p junction with one-dimensional electric and magnetic barriers. In the presence of both electric and magnetic barriers, we found that a large conductance gap can be produced with the aid of tilted <span class="hlt">energy</span> dispersion without a <span class="hlt">band</span> gap. The origin of this effect is the shift of the <span class="hlt">electron</span> wave-vector at barrier boundaries caused by (i) the pseudo-magnetic field induced by electrical potential, i.e., a newly discovered feature that is only possible in the materials possessing tilted <span class="hlt">energy</span> dispersion, (ii) the real magnetic field induced by a ferromagnetic layer deposited on the top of the system. We use a realistic barrier structure applicable in current nanotechnology and analyze the temperature dependence of the tunneling conductance. The new approach presented here may resolve a major problem of possible transistor applications in topological semimetals, i.e., the absence of normal backscattering and gapless <span class="hlt">band</span> structure.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014APS..MARW24008J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014APS..MARW24008J"><span>Measurement of the background in Auger-Photoemission Spectra (APECS) associated with multi-<span class="hlt">electron</span> and inelastic valence <span class="hlt">band</span> photoemission processes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Joglekar, Prasad; Shastry, Karthik; Hulbert, Steven; Weiss, Alex</p> <p>2014-03-01</p> <p>Auger Photoelectron Coincidence Spectroscopy (APECS), in which the Auger spectra is measured in coincidence with the core level photoelectron, is capable of pulling difficult to observe low <span class="hlt">energy</span> Auger peaks out of a large background due mostly to inelastically scattered valence <span class="hlt">band</span> photoelectrons. However the APECS method alone cannot eliminate the background due to valence <span class="hlt">band</span> VB photoemission processes in which the initial photon <span class="hlt">energy</span> is shared by 2 or more <span class="hlt">electrons</span> and one of the <span class="hlt">electrons</span> is in the <span class="hlt">energy</span> range of the core level photoemission peak. Here we describe an experimental method for estimating the contributions from these background processes in the case of an Ag N23VV Auger spectra obtained in coincidence with the 4p photoemission peak. A beam of 180eV photons was incident on a Ag sample and a series of coincidence measurements were made with one cylindrical mirror analyzer (CMA) set at a fixed <span class="hlt">energies</span> between the core and the valence <span class="hlt">band</span> and the other CMA scanned over a range corresponding to <span class="hlt">electrons</span> leaving the surface between 0eV and the 70eV. The spectra obtained were then used to obtain an estimate of the background in the APECS spectra due to multi-<span class="hlt">electron</span> and inelastic VB photoemission processes. NSF, Welch Foundation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20000058155','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20000058155"><span>High Resolution Emission Spectroscopy of the Alpha Pi-1 - Chi Sigma-1(+) Fourth Positive <span class="hlt">Band</span> System of CO from <span class="hlt">Electron</span> Impact</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Beegle, Luther W.; Ajello, Joseph M.; James, Geoffrey K.; Alvarez, Marcos; Dziczek, Dariusz</p> <p>2000-01-01</p> <p>We report <span class="hlt">electron</span>-impact induced fluorescence spectra [300 mA full width at half maximum (FWHM)] of CO for 20 and 100 eV impact <span class="hlt">energies</span> of the spectral region of 1300 to 2050 A and high resolution spectra (FWHM) of the v'=5 to v"=l and the v'=3 to v"=O <span class="hlt">bands</span> showing that the rotational structure of the <span class="hlt">band</span> system are modeled accurately. The excitation function of the (0,1) <span class="hlt">band</span> (1597 A) was measured from <span class="hlt">electron</span> impact in the <span class="hlt">energy</span> range from threshold to 750 eV and placed on an absolute scale from modem calibration standards.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012JPhCS.377a2093S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012JPhCS.377a2093S"><span><span class="hlt">Electron</span> <span class="hlt">band</span> structure of the high pressure cubic phase of AlH3</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shi, Hongliang; Zarifi, Niliffar; Yim, Wai-Leung; Tse, J. S.</p> <p>2012-07-01</p> <p>The <span class="hlt">electronic</span> <span class="hlt">band</span> structure of the cubic Pm3n phase of AlH3 stable above 100 GPa is examined with semi-local, Tran-Blaha modified Becke-Johnson local density approximation (TB-mBJLDA), screened hybrid density functionals and GW methods. The shift of the conduction <span class="hlt">band</span> to higher <span class="hlt">energy</span> with increasing pressure is predicted by all methods. However, there are significant differences in detail <span class="hlt">band</span> structure. In the pressure range from 90 to160 GPa, semi-local, hybrid functional and TB-mBJLDA calculations predicted that AlH3 is a poor metal. In comparison, GW calculations show a gap opening at 160 GPa and AlH3 becomes a small gap semi-conductor. From the trends of the calculated <span class="hlt">band</span> shifts, it can be concluded that the favourable conditions leading to the nesting of Fermi surfaces predicted by semi-local calculation have disappeared if the exchange term is included. The results highlight the importance of the correction to the exchange <span class="hlt">energy</span> on the <span class="hlt">band</span> structure of hydrogen dominant dense metal hydrides at high pressure hydrides and may help to rationalize the absence of superconductivity in AlH3 from experimental measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004PhRvB..70x5116D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004PhRvB..70x5116D"><span><span class="hlt">Electronic</span> structure and <span class="hlt">electron</span> <span class="hlt">energy</span>-loss spectroscopy of ZrO2 zirconia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dash, L. K.; Vast, Nathalie; Baranek, Philippe; Cheynet, Marie-Claude; Reining, Lucia</p> <p>2004-12-01</p> <p>The atomic and <span class="hlt">electronic</span> structures of zirconia are calculated within density functional theory, and their evolution is analyzed as the crystal-field symmetry changes from tetrahedral [cubic (c-ZrO2) and tetragonal (t-ZrO2) phases] to octahedral (hypothetical rutile ZrO2 ), to a mixing of these symmetries (monoclinic phase, m-ZrO2 ). We find that the theoretical bulk modulus in c-ZrO2 is 30% larger than the experimental value, showing that the introduction of yttria in zirconia has a significant effect. <span class="hlt">Electronic</span> structure fingerprints which characterize each phase from their <span class="hlt">electronic</span> spectra are identified. We have carried out <span class="hlt">electron</span> <span class="hlt">energy</span>-loss spectroscopy experiments at low momentum transfer and compared these results to the theoretical spectra calculated within the random phase approximation. We show a dependence of the valence and 4p ( N2,3 edge) plasmons on the crystal structure, the dependence of the latter being brought into the spectra by local-field effects. Last, we attribute low <span class="hlt">energy</span> excitations observed in EELS of m-ZrO2 to defect states 2eV above the top of the intrinsic valence <span class="hlt">band</span>, and the EELS fundamental <span class="hlt">band</span> gap value is reconciled with the 5.2 or 5.8eV gaps determined by vacuum ultraviolet spectroscopy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22399363-electron-transport-electron-energy-distributions-within-wurtzite-zinc-blende-phases-indium-nitride-response-application-constant-uniform-electric-field','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22399363-electron-transport-electron-energy-distributions-within-wurtzite-zinc-blende-phases-indium-nitride-response-application-constant-uniform-electric-field"><span><span class="hlt">Electron</span> transport and <span class="hlt">electron</span> <span class="hlt">energy</span> distributions within the wurtzite and zinc-blende phases of indium nitride: Response to the application of a constant and uniform electric field</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Siddiqua, Poppy; Hadi, Walid A.; Salhotra, Amith K.</p> <p>2015-03-28</p> <p>Within the framework of an ensemble semi-classical three-valley Monte Carlo <span class="hlt">electron</span> transport simulation approach, we critically contrast the nature of the <span class="hlt">electron</span> transport that occurs within the wurtzite and zinc-blende phases of indium nitride in response to the application of a constant and uniform electric field. We use the <span class="hlt">electron</span> <span class="hlt">energy</span> distribution and its relationship with the <span class="hlt">electron</span> transport characteristics in order to pursue this analysis. For the case of zinc-blende indium nitride, only a peak corresponding to the <span class="hlt">electrons</span> within the lowest <span class="hlt">energy</span> conduction <span class="hlt">band</span> valley is observed, this peak being seen to broaden and shift to higher energiesmore » in response to increases in the applied electric field strength, negligible amounts of upper <span class="hlt">energy</span> conduction <span class="hlt">band</span> valley occupancy being observed. In contrast, for the case of wurtzite indium nitride, in addition to the aforementioned lowest <span class="hlt">energy</span> conduction <span class="hlt">band</span> valley peak in the <span class="hlt">electron</span> <span class="hlt">energy</span> distribution, and its broadening and shifting to higher <span class="hlt">energies</span> in response to increases in the applied electric field strength, beyond a certain critical electric field strength, 30 kV/cm for the case of this particular material, upper <span class="hlt">energy</span> conduction <span class="hlt">band</span> valley occupancy is observed, this occupancy being further enhanced in response to further increases in the applied electric field strength. Reasons for these results are provided. The potential for device consequences is then commented upon.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28319838','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28319838"><span>Graphene oxide quantum dot-sensitized porous titanium dioxide microsphere: Visible-light-driven photocatalyst based on <span class="hlt">energy</span> <span class="hlt">band</span> engineering.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhang, Yu; Qi, Fuyuan; Li, Ying; Zhou, Xin; Sun, Hongfeng; Zhang, Wei; Liu, Daliang; Song, Xi-Ming</p> <p>2017-07-15</p> <p>We report a novel graphene oxide quantum dot (GOQD)-sensitized porous TiO 2 microsphere for efficient photoelectric conversion. Electro-chemical analysis along with the Mott-Schottky equation reveals conductivity type and <span class="hlt">energy</span> <span class="hlt">band</span> structure of the two semiconductors. Based on their <span class="hlt">energy</span> <span class="hlt">band</span> structures, visible light-induced <span class="hlt">electrons</span> can transfer from the p-type GOQD to the n-type TiO 2 . Enhanced photocurrent and photocatalytic activity in visible light further confirm the enhanced separation of <span class="hlt">electrons</span> and holes in the nanocomposite. Copyright © 2017 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhRvB..95w5105Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvB..95w5105Z"><span>Dynamical <span class="hlt">electron</span>-phonon coupling, G W self-consistency, and vertex effect on the <span class="hlt">electronic</span> <span class="hlt">band</span> gap of ice and liquid water</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ziaei, Vafa; Bredow, Thomas</p> <p>2017-06-01</p> <p>We study the impact of dynamical <span class="hlt">electron</span>-phonon (el-ph) effects on the <span class="hlt">electronic</span> <span class="hlt">band</span> gap of ice and liquid water by accounting for frequency-dependent Fan contributions in the el-ph mediated self-<span class="hlt">energy</span> within the many-body perturbation theory (MBPT). We find that the dynamical el-ph coupling effects greatly reduce the static el-ph <span class="hlt">band</span>-gap correction of the hydrogen-rich molecular ice crystal from-2.46 to -0.23 eV in great contrast to the result of Monserrat et al. [Phys. Rev. B 92, 140302 (2015), 10.1103/PhysRevB.92.140302]. This is of particular importance as otherwise the static el-ph gap correction would considerably reduce the <span class="hlt">electronic</span> <span class="hlt">band</span> gap, leading to considerable underestimation of the intense peaks of optical absorption spectra of ice which would be in great disagreement to experimental references. By contrast, the static el-ph gap correction of liquid water is very moderate (-0.32 eV), and inclusion of dynamical effects slightly reduces the gap correction to -0.19 eV. Further, we determine the diverse sensitivity of ice and liquid water to the G W self-consistency and show that the <span class="hlt">energy</span>-only self-consistent approach (GnWn ) exhibits large implicit vertex character in comparison to the quasiparticle self-consistent approach, for which an explicit calculation of vertex corrections is necessary for good agreement with experiment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JPCM...28B4003J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JPCM...28B4003J"><span>Correlation between morphology, <span class="hlt">electron</span> <span class="hlt">band</span> structure, and resistivity of Pb atomic chains on the Si(5 5 3)-Au surface</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jałochowski, M.; Kwapiński, T.; Łukasik, P.; Nita, P.; Kopciuszyński, M.</p> <p>2016-07-01</p> <p>Structural and <span class="hlt">electron</span> transport properties of multiple Pb atomic chains fabricated on the Si(5 5 3)-Au surface are investigated using scanning tunneling spectroscopy, reflection high <span class="hlt">electron</span> <span class="hlt">energy</span> diffraction, angular resolved photoemission <span class="hlt">electron</span> spectroscopy and in situ electrical resistance. The study shows that Pb atomic chains growth modulates the <span class="hlt">electron</span> <span class="hlt">band</span> structure of pristine Si(5 5 3)-Au surface and hence changes its sheet resistivity. Strong correlation between chains morphology, <span class="hlt">electron</span> <span class="hlt">band</span> structure and <span class="hlt">electron</span> transport properties is found. To explain experimental findings a theoretical tight-binding model of multiple atomic chains interacting on effective substrate is proposed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28738679','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28738679"><span>Probability of Two-Step Photoexcitation of <span class="hlt">Electron</span> from Valence <span class="hlt">Band</span> to Conduction <span class="hlt">Band</span> through Doping Level in TiO2.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Nishikawa, Masami; Shiroishi, Wataru; Honghao, Hou; Suizu, Hiroshi; Nagai, Hideyuki; Saito, Nobuo</p> <p>2017-08-17</p> <p>For an Ir-doped TiO 2 (Ir:TiO 2 ) photocatalyst, we examined the most dominant <span class="hlt">electron</span>-transfer path for the visible-light-driven photocatalytic performance. The Ir:TiO 2 photocatalyst showed a much higher photocatalytic activity under visible-light irradiation than nondoped TiO 2 after grafting with the cocatalyst of Fe 3+ . For the Ir:TiO 2 photocatalyst, the two-step photoexcitation of an <span class="hlt">electron</span> from the valence <span class="hlt">band</span> to the conduction <span class="hlt">band</span> through the Ir doping level occurred upon visible-light irradiation, as observed by <span class="hlt">electron</span> spin resonance spectroscopy. The two-step photoexcitation through the doping level was found to be a more stable process with a lower recombination rate of hole-<span class="hlt">electron</span> pairs than the two-step photoexcitation process through an oxygen vacancy. Once <span class="hlt">electrons</span> are photoexcited to the conduction <span class="hlt">band</span> by the two-step excitation, the <span class="hlt">electrons</span> can easily transfer to the surface because the conduction <span class="hlt">band</span> is a continuous <span class="hlt">electron</span> path, whereas the <span class="hlt">electrons</span> photoexcited at only the doping level could not easily transfer to the surface because of the discontinuity of this path. The observed two-step photoexcitation from the valence <span class="hlt">band</span> to the conduction <span class="hlt">band</span> through the doping level significantly contributes to the enhancement of the photocatalytic performance.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li class="active"><span>4</span></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_4 --> <div id="page_5" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li class="active"><span>5</span></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="81"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PhRvB..92l5441C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PhRvB..92l5441C"><span><span class="hlt">Energy</span> shift and conduction-to-valence <span class="hlt">band</span> transition mediated by a time-dependent potential barrier in graphene</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chaves, Andrey; da Costa, D. R.; de Sousa, G. O.; Pereira, J. M.; Farias, G. A.</p> <p>2015-09-01</p> <p>We investigate the scattering of a wave packet describing low-<span class="hlt">energy</span> <span class="hlt">electrons</span> in graphene by a time-dependent finite-step potential barrier. Our results demonstrate that, after Klein tunneling through the barrier, the <span class="hlt">electron</span> acquires an extra <span class="hlt">energy</span> which depends on the rate of change of the barrier height with time. If this rate is negative, the <span class="hlt">electron</span> loses <span class="hlt">energy</span> and ends up as a valence <span class="hlt">band</span> state after leaving the barrier, which effectively behaves as a positively charged quasiparticle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22606277-electronic-energy-loss-spectra-from-mono-layer-few-layers-phosphorene','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22606277-electronic-energy-loss-spectra-from-mono-layer-few-layers-phosphorene"><span><span class="hlt">Electronic</span> <span class="hlt">energy</span> loss spectra from mono-layer to few layers of phosphorene</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Mohan, Brij, E-mail: brijmohanhpu@yahoo.com; Thakur, Rajesh; Ahluwalia, P. K.</p> <p>2016-05-23</p> <p>Using first principles calculations, <span class="hlt">electronic</span> and optical properties of few-layers phosphorene has been investigated. <span class="hlt">Electronic</span> <span class="hlt">band</span> structure show a moderate <span class="hlt">band</span> gap of 0.9 eV in monolayer phosphorene which decreases with increasing number of layers. Optical properties of few-layers of phosphorene in infrared and visible region shows tunability with number of layers. <span class="hlt">Electron</span> <span class="hlt">energy</span> loss function has been plotted and huge red shift in plasmonic behaviours is found. These tunable <span class="hlt">electronic</span> and optical properties of few-layers of phosphorene can be useful for the applications of optoelectronic devices.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21828568','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21828568"><span>A simple <span class="hlt">energy</span> filter for low <span class="hlt">energy</span> <span class="hlt">electron</span> microscopy/photoelectron emission microscopy instruments.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tromp, R M; Fujikawa, Y; Hannon, J B; Ellis, A W; Berghaus, A; Schaff, O</p> <p>2009-08-05</p> <p>Addition of an <span class="hlt">electron</span> <span class="hlt">energy</span> filter to low <span class="hlt">energy</span> <span class="hlt">electron</span> microscopy (LEEM) and photoelectron emission microscopy (PEEM) instruments greatly improves their analytical capabilities. However, such filters tend to be quite complex, both <span class="hlt">electron</span> optically and mechanically. Here we describe a simple <span class="hlt">energy</span> filter for the existing IBM LEEM/PEEM instrument, which is realized by adding a single scanning aperture slit to the objective transfer optics, without any further modifications to the microscope. This <span class="hlt">energy</span> filter displays a very high <span class="hlt">energy</span> resolution ΔE/E = 2 × 10(-5), and a non-isochromaticity of ∼0.5 eV/10 µm. The setup is capable of recording selected area <span class="hlt">electron</span> <span class="hlt">energy</span> spectra and angular distributions at 0.15 eV <span class="hlt">energy</span> resolution, as well as <span class="hlt">energy</span> filtered images with a 1.5 eV <span class="hlt">energy</span> pass <span class="hlt">band</span> at an estimated spatial resolution of ∼10 nm. We demonstrate the use of this <span class="hlt">energy</span> filter in imaging and spectroscopy of surfaces using a laboratory-based He I (21.2 eV) light source, as well as imaging of Ag nanowires on Si(001) using the 4 eV <span class="hlt">energy</span> loss Ag plasmon.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20170008487&hterms=electronics&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Delectronics','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20170008487&hterms=electronics&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Delectronics"><span>Model Development for MODIS Thermal <span class="hlt">Band</span> <span class="hlt">Electronic</span> Crosstalk</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chang, Tiejun; Wu, Aisheng; Geng, Xu; Li, Yonghonh; Brinkman, Jake; Keller, Graziela; Xiong, Xiaoxiong</p> <p>2016-01-01</p> <p>MODerate-resolution Imaging Spectroradiometer (MODIS) has 36 <span class="hlt">bands</span>. Among them, 16 thermal emissive <span class="hlt">bands</span> covering a wavelength range from 3.8 to 14.4 m. After 16 years on-orbit operation, the <span class="hlt">electronic</span> crosstalk of a few Terra MODIS thermal emissive <span class="hlt">bands</span> developed substantial issues that cause biases in the EV brightness temperature measurements and surface feature contamination. The crosstalk effects on <span class="hlt">band</span> 27 with center wavelength at 6.7 m and <span class="hlt">band</span> 29 at 8.5 m increased significantly in recent years, affecting downstream products such as water vapor and cloud mask. The crosstalk effect is evident in the near-monthly scheduled lunar measurements, from which the crosstalk coefficients can be derived. The development of an alternative approach is very helpful for independent verification.In this work, a physical model was developed to assess the crosstalk impact on calibration as well as in Earth view brightness temperature retrieval. This model was applied to Terra MODIS <span class="hlt">band</span> 29 empirically to correct the Earth brightness temperature measurements. In the model development, the detectors nonlinear response is considered. The impact of the <span class="hlt">electronic</span> crosstalk is assessed in two steps. The first step consists of determining the impact on calibration using the on-board blackbody (BB). Due to the detectors nonlinear response and large background signal, both linear and nonlinear coefficients are affected by the crosstalk from sending <span class="hlt">bands</span>. The second step is to calculate the effects on the Earth view brightness temperature retrieval. The effects include those from affected calibration coefficients and the contamination of Earth view measurements. This model links the measurement bias with crosstalk coefficients, detector non-linearity, and the ratio of Earth measurements between the sending and receiving <span class="hlt">bands</span>. The correction of the <span class="hlt">electronic</span> cross talk can be implemented empirically from the processed bias at different brightness temperature. The implementation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22490729-edge-effects-band-gap-energy-bilayer-mos-sub-under-uniaxial-strain','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22490729-edge-effects-band-gap-energy-bilayer-mos-sub-under-uniaxial-strain"><span>Edge effects on <span class="hlt">band</span> gap <span class="hlt">energy</span> in bilayer 2H-MoS{sub 2} under uniaxial strain</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Dong, Liang; Wang, Jin; Dongare, Avinash M., E-mail: dongare@uconn.edu</p> <p>2015-06-28</p> <p>The potential of ultrathin MoS{sub 2} nanostructures for applications in <span class="hlt">electronic</span> and optoelectronic devices requires a fundamental understanding in their <span class="hlt">electronic</span> structure as a function of strain. Previous experimental and theoretical studies assume that an identical strain and/or stress state is always maintained in the top and bottom layers of a bilayer MoS{sub 2} film. In this study, a bilayer MoS{sub 2} supercell is constructed differently from the prototypical unit cell in order to investigate the layer-dependent <span class="hlt">electronic</span> <span class="hlt">band</span> gap <span class="hlt">energy</span> in a bilayer MoS{sub 2} film under uniaxial mechanical deformations. The supercell contains an MoS{sub 2} bottom layer andmore » a relatively narrower top layer (nanoribbon with free edges) as a simplified model to simulate the as-grown bilayer MoS{sub 2} flakes with free edges observed experimentally. Our results show that the two layers have different <span class="hlt">band</span> gap <span class="hlt">energies</span> under a tensile uniaxial strain, although they remain mutually interacting by van der Waals interactions. The deviation in their <span class="hlt">band</span> gap <span class="hlt">energies</span> grows from 0 to 0.42 eV as the uniaxial strain increases from 0% to 6% under both uniaxial strain and stress conditions. The deviation, however, disappears if a compressive uniaxial strain is applied. These results demonstrate that tensile uniaxial strains applied to bilayer MoS{sub 2} films can result in distinct <span class="hlt">band</span> gap <span class="hlt">energies</span> in the bilayer structures. Such variations need to be accounted for when analyzing strain effects on <span class="hlt">electronic</span> properties of bilayer or multilayered 2D materials using experimental methods or in continuum models.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19860026978&hterms=mobil&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dmobil','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19860026978&hterms=mobil&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dmobil"><span>Growth of the 889 per cm infrared <span class="hlt">band</span> in annealed <span class="hlt">electron</span>-irradiated silicon</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Svensson, B. G.; Lindstrom, J. L.; Corbett, J. W.</p> <p>1985-01-01</p> <p>Isothermal annealing of <span class="hlt">electron</span>-irradiated Czochralski silicon has been studied at four different temperatures ranging from 304 to 350 C using infrared spectroscopy. At annealing temperatures above 300 C the irradiation-induced <span class="hlt">band</span> at 830 per cm, usually attributed to a vacancy-oxygen complex (the A center), disappears and a new <span class="hlt">band</span> at 889 per cm grows up. Within the experimental accuracy, the activation <span class="hlt">energy</span> for the growth of this <span class="hlt">band</span> is found to be identical with the value given by Stavola et al. for 'anomalous' oxygen diffusion in silicon. Also the frequency factors for the two processes are in reasonable agreement. The results show that a vacancy-assisted process may provide an explanation for enhanced motion of oxygen in silicon.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004PhDT........31H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004PhDT........31H"><span>Spectroscopic study of hafnium silicate alloys prepared by RPECVD: Comparisons between conduction/valence <span class="hlt">band</span> offset <span class="hlt">energies</span> and optical <span class="hlt">band</span> gaps</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hong, Joon Goo</p> <p></p> <p>Aggressive scaling of devices has continued to improve MOSFET transistor performance. As lateral device dimensions continue to decrease, gate oxide thickness must be scaled down. As one of the promising high k alternative gate oxide materials, HfO2 and its silicates were investigated to understand their direct tunneling behavior by studying <span class="hlt">band</span> offset <span class="hlt">energies</span> with spectroscopy and electrical characterization. Local bonding change of remote plasma deposited (HfO2)x(SiO 2)1-x alloys were characterized by Fourier transform infrared (FTIR) spectroscopy, x-ray photoelectron spectroscopy (XPS), and Auger <span class="hlt">electron</span> spectroscopy (AES) as a function of alloy composition, x. Two different precursors with Hf Nitrato and Hf-tert-butoxide were tested to have amorphous deposition. Film composition was determined off-line by Rutherford backscattering spectroscopy (RBS) and these results were calibrated with on-line AES. As deposited Hf-silicate alloys were characterized by off-line XPS and AES for their chemical shifts interpreting with a partial charge transfer model as well as coordination changes. Sigmoidal dependence of valence <span class="hlt">band</span> offset <span class="hlt">energies</span> was observed. Hf 5d* state is fixed at the bottom of the conduction <span class="hlt">band</span> and located at 1.3 +/- 0.2 eV above the top of the Si conduction <span class="hlt">band</span> as a conduction <span class="hlt">band</span> offset by x-ray absorption spectroscopy (XAS). Optical <span class="hlt">band</span> gap <span class="hlt">energy</span> changes were observed with vacuum ultra violet spectroscopic ellipsometry (VUVSE) to verify compositional dependence of conduction and valence <span class="hlt">band</span> offset <span class="hlt">energy</span> changes. 1 nm EOT normalized tunneling current with Wentzel-Kramer-Brillouin (WKB) simulation based on the <span class="hlt">band</span> offset study and Franz two <span class="hlt">band</span> model showed the minimum at the intermediate composition matching with the experimental data. Non-linear trend in tunneling current was observed because the increases in physical thickness were mitigated by reductions in <span class="hlt">band</span> offset <span class="hlt">energies</span> and effective mass for tunneling. C-V curves were compared</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4792950','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4792950"><span>Stable topological insulators achieved using high <span class="hlt">energy</span> <span class="hlt">electron</span> beams</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Zhao, Lukas; Konczykowski, Marcin; Deng, Haiming; Korzhovska, Inna; Begliarbekov, Milan; Chen, Zhiyi; Papalazarou, Evangelos; Marsi, Marino; Perfetti, Luca; Hruban, Andrzej; Wołoś, Agnieszka; Krusin-Elbaum, Lia</p> <p>2016-01-01</p> <p>Topological insulators are potentially transformative quantum solids with metallic surface states which have Dirac <span class="hlt">band</span> structure and are immune to disorder. Ubiquitous charged bulk defects, however, pull the Fermi <span class="hlt">energy</span> into the bulk <span class="hlt">bands</span>, denying access to surface charge transport. Here we demonstrate that irradiation with swift (∼2.5 MeV <span class="hlt">energy</span>) <span class="hlt">electron</span> beams allows to compensate these defects, bring the Fermi level back into the bulk gap and reach the charge neutrality point (CNP). Controlling the beam fluence, we tune bulk conductivity from p- (hole-like) to n-type (<span class="hlt">electron</span>-like), crossing the Dirac point and back, while preserving the Dirac <span class="hlt">energy</span> dispersion. The CNP conductance has a two-dimensional character on the order of ten conductance quanta and reveals, both in Bi2Te3 and Bi2Se3, the presence of only two quantum channels corresponding to two topological surfaces. The intrinsic quantum transport of the topological states is accessible disregarding the bulk size. PMID:26961901</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011JAP...109k3724M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011JAP...109k3724M"><span>Branch-point <span class="hlt">energies</span> and the <span class="hlt">band</span>-structure lineup at Schottky contacts and heterostrucures</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mönch, Winfried</p> <p>2011-06-01</p> <p>Empirical branch-point <span class="hlt">energies</span> of Si, the group-III nitrides AlN, GaN, and InN, and the group-II and group-III oxides MgO, ZnO, Al2O3 and In2O3 are determined from experimental valance-<span class="hlt">band</span> offsets of their heterostructures. For Si, GaN, and MgO, these values agree with the branch-point <span class="hlt">energies</span> obtained from the barrier heights of their Schottky contacts. The empirical branch-point <span class="hlt">energies</span> of Si and the group-III nitrides are in very good agreement with results of previously published calculations using quite different approaches such as the empirical tight-binding approximation and modern <span class="hlt">electronic</span>-structure theory. In contrast, the empirical branch-point <span class="hlt">energies</span> of the group-II and group-III oxides do not confirm the respective theoretical results. As at Schottky contacts, the <span class="hlt">band</span>-structure lineup at heterostructures is also made up of a zero-charge-transfer term and an intrinsic electric-dipole contribution. Hence, valence-<span class="hlt">band</span> offsets are not equal to the difference of the branch-point <span class="hlt">energies</span> of the two semiconductors forming the heterostructure. The electric-dipole term may be described by the electronegativity difference of the two solids in contact. A detailed analysis of experimental Si Schottky barrier heights and heterostructure valence-<span class="hlt">band</span> offsets explains and proves these conclusions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1342054-electronic-band-structure-effects-stopping-protons-copper-electronic-band-structure-non-linear-effects-stopping-protons-copper','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1342054-electronic-band-structure-effects-stopping-protons-copper-electronic-band-structure-non-linear-effects-stopping-protons-copper"><span><span class="hlt">Electronic</span> <span class="hlt">band</span> structure effects in the stopping of protons in copper [<span class="hlt">Electronic</span> <span class="hlt">band</span> structure non-linear effects in the stopping of protons in copper</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Quashie, Edwin E.; Saha, Bidhan C.; Correa, Alfredo A.</p> <p>2016-10-05</p> <p>Here, we present an ab initio study of the <span class="hlt">electronic</span> stopping power of protons in copper over a wide range of proton velocities v = 0.02–10a.u. where we take into account nonlinear effects. Time-dependent density functional theory coupled with molecular dynamics is used to study <span class="hlt">electronic</span> excitations produced by energetic protons. A plane-wave pseudopotential scheme is employed to solve the time-dependent Kohn-Sham equations for a moving ion in a periodic crystal. The <span class="hlt">electronic</span> excitations and the <span class="hlt">band</span> structure determine the stopping power of the material and alter the interatomic forces for both channeling and off-channeling trajectories. Our off-channeling results aremore » in quantitative agreement with experiments, and at low velocity they unveil a crossover region of superlinear velocity dependence (with a power of ~1.5) in the velocity range v = 0.07–0.3a.u., which we associate to the copper crystalline <span class="hlt">electronic</span> <span class="hlt">band</span> structure. The results are rationalized by simple <span class="hlt">band</span> models connecting two separate regimes. We find that the limit of <span class="hlt">electronic</span> stopping v → 0 is not as simple as phenomenological models suggest and it is plagued by <span class="hlt">band</span>-structure effects.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26608712','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26608712"><span>Nanoscale measurements of unoccupied <span class="hlt">band</span> dispersion in few-layer graphene.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jobst, Johannes; Kautz, Jaap; Geelen, Daniël; Tromp, Rudolf M; van der Molen, Sense Jan</p> <p>2015-11-26</p> <p>The properties of any material are fundamentally determined by its <span class="hlt">electronic</span> <span class="hlt">band</span> structure. Each <span class="hlt">band</span> represents a series of allowed states inside a material, relating <span class="hlt">electron</span> <span class="hlt">energy</span> and momentum. The occupied <span class="hlt">bands</span>, that is, the filled <span class="hlt">electron</span> states below the Fermi level, can be routinely measured. However, it is remarkably difficult to characterize the empty part of the <span class="hlt">band</span> structure experimentally. Here, we present direct measurements of unoccupied <span class="hlt">bands</span> of monolayer, bilayer and trilayer graphene. To obtain these, we introduce a technique based on low-<span class="hlt">energy</span> <span class="hlt">electron</span> microscopy. It relies on the dependence of the <span class="hlt">electron</span> reflectivity on incidence angle and <span class="hlt">energy</span> and has a spatial resolution ∼10 nm. The method can be easily applied to other nanomaterials such as van der Waals structures that are available in small crystals only.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4674768','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4674768"><span>Nanoscale measurements of unoccupied <span class="hlt">band</span> dispersion in few-layer graphene</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Jobst, Johannes; Kautz, Jaap; Geelen, Daniël; Tromp, Rudolf M.; van der Molen, Sense Jan</p> <p>2015-01-01</p> <p>The properties of any material are fundamentally determined by its <span class="hlt">electronic</span> <span class="hlt">band</span> structure. Each <span class="hlt">band</span> represents a series of allowed states inside a material, relating <span class="hlt">electron</span> <span class="hlt">energy</span> and momentum. The occupied <span class="hlt">bands</span>, that is, the filled <span class="hlt">electron</span> states below the Fermi level, can be routinely measured. However, it is remarkably difficult to characterize the empty part of the <span class="hlt">band</span> structure experimentally. Here, we present direct measurements of unoccupied <span class="hlt">bands</span> of monolayer, bilayer and trilayer graphene. To obtain these, we introduce a technique based on low-<span class="hlt">energy</span> <span class="hlt">electron</span> microscopy. It relies on the dependence of the <span class="hlt">electron</span> reflectivity on incidence angle and <span class="hlt">energy</span> and has a spatial resolution ∼10 nm. The method can be easily applied to other nanomaterials such as van der Waals structures that are available in small crystals only. PMID:26608712</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26247853','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26247853"><span><span class="hlt">Energy</span> Impacts of Wide <span class="hlt">Band</span> Gap Semiconductors in U.S. Light-Duty Electric Vehicle Fleet.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Warren, Joshua A; Riddle, Matthew E; Graziano, Diane J; Das, Sujit; Upadhyayula, Venkata K K; Masanet, Eric; Cresko, Joe</p> <p>2015-09-01</p> <p>Silicon carbide and gallium nitride, two leading wide <span class="hlt">band</span> gap semiconductors with significant potential in electric vehicle power <span class="hlt">electronics</span>, are examined from a life cycle <span class="hlt">energy</span> perspective and compared with incumbent silicon in U.S. light-duty electric vehicle fleet. Cradle-to-gate, silicon carbide is estimated to require more than twice the <span class="hlt">energy</span> as silicon. However, the magnitude of vehicle use phase fuel savings potential is comparatively several orders of magnitude higher than the marginal increase in cradle-to-gate <span class="hlt">energy</span>. Gallium nitride cradle-to-gate <span class="hlt">energy</span> requirements are estimated to be similar to silicon, with use phase savings potential similar to or exceeding that of silicon carbide. Potential <span class="hlt">energy</span> reductions in the United States vehicle fleet are examined through several scenarios that consider the market adoption potential of electric vehicles themselves, as well as the market adoption potential of wide <span class="hlt">band</span> gap semiconductors in electric vehicles. For the 2015-2050 time frame, cumulative <span class="hlt">energy</span> savings associated with the deployment of wide <span class="hlt">band</span> gap semiconductors are estimated to range from 2-20 billion GJ depending on market adoption dynamics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JAP...123q5107U','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JAP...123q5107U"><span>Engineering the <span class="hlt">electronic</span> <span class="hlt">band</span> structures of novel cubic structured germanium monochalcogenides for thermoelectric applications</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ul Haq, Bakhtiar; AlFaify, S.; Ahmed, R.; Butt, Faheem K.; Laref, A.; Goumri-Said, Souraya; Tahir, S. A.</p> <p>2018-05-01</p> <p>Germanium mono-chalcogenides have received considerable attention for being a promising replacement for the relatively toxic and expensive chalcogenides in renewable and sustainable <span class="hlt">energy</span> applications. In this paper, we explore the potential of the recently discovered novel cubic structured (π-phase) GeS and GeSe for thermoelectric applications in the framework of density functional theory coupled with Boltzmann transport theory. To examine the modifications in their physical properties, the across composition alloying of π-GeS and π-GeSe (such as π-GeS1-xSex for x =0, 0.25, 0.50, 0.75, and 1) has been performed that has shown important effects on the <span class="hlt">electronic</span> <span class="hlt">band</span> structures and effective masses of charge carriers. An increase in Se composition in π-GeS1-xSex has induced a downward shift in their conduction <span class="hlt">bands</span>, resulting in the narrowing of their <span class="hlt">energy</span> <span class="hlt">band</span> gaps. The thermoelectric coefficients of π-GeS1-xSex have been accordingly influenced by the evolution of the <span class="hlt">electronic</span> <span class="hlt">band</span> structures and effective masses of charge carriers. π-GeS1-xSex features sufficiently larger values of Seebeck coefficients, power factors and figures of merit (ZTs), which experience further improvement with an increase in temperature, revealing their potential for high-temperature applications. The calculated results show that ZT values equivalent to unity can be achieved for π-GeS1-xSex at appropriate n-type doping levels. Our calculations for the formation enthalpies indicate that a π-GeS1-xSex alloying system is energetically stable and could be synthesized experimentally. These intriguing characteristics make π-GeS1-xSex a promising candidate for futuristic thermoelectric applications in <span class="hlt">energy</span> harvesting devices.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002PhRvB..65p5115W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002PhRvB..65p5115W"><span>Ab initio <span class="hlt">electronic</span> structure calculations for metallic intermediate <span class="hlt">band</span> formation in photovoltaic materials</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wahnón, P.; Tablero, C.</p> <p>2002-04-01</p> <p>A metallic isolated <span class="hlt">band</span> in the middle of the <span class="hlt">band</span> gap of several III-V semiconductors has been predicted as photovoltaic materials with the possibility of providing substantially enhanced efficiencies. We have investigated the <span class="hlt">electronic</span> <span class="hlt">band</span> structures and lattice constants of GanAsmM and GanPmM with M=Sc, Ti, V, and Cr, to identify whether this isolated <span class="hlt">band</span> is likely to exist by means of accurate calculations. For this task, we use the SIESTA program, an ab initio periodic density-functional method, fully self consistent in the local-density approximation. Norm-conserving, nonlocal pseudopotentials and confined linear combination of atomic orbitals have been used. We have carried out a case study of GanAsmTi and GanPmTi <span class="hlt">energy-band</span> structure including analyses of the effect of the basis set, fine k-point mesh to ensure numerical convergence, structural parameters, and generalized gradient approximation for exchange and correlation corrections. We find the isolated intermediate <span class="hlt">band</span> when one Ti atom replaces the position of one As (or P) atom in the crystal structure. For this kind of compound we show that the intermediate <span class="hlt">band</span> relative position inside the <span class="hlt">band</span> gap and width are sensitive to the dynamic relaxation of the crystal and the size of the basis set.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4174871','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4174871"><span><span class="hlt">Electronic</span> materials with a wide <span class="hlt">band</span> gap: recent developments</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Klimm, Detlef</p> <p>2014-01-01</p> <p>The development of semiconductor <span class="hlt">electronics</span> is reviewed briefly, beginning with the development of germanium devices (<span class="hlt">band</span> gap E g = 0.66 eV) after World War II. A tendency towards alternative materials with wider <span class="hlt">band</span> gaps quickly became apparent, starting with silicon (E g = 1.12 eV). This improved the signal-to-noise ratio for classical <span class="hlt">electronic</span> applications. Both semiconductors have a tetrahedral coordination, and by isoelectronic alternative replacement of Ge or Si with carbon or various anions and cations, other semiconductors with wider E g were obtained. These are transparent to visible light and belong to the group of wide <span class="hlt">band</span> gap semiconductors. Nowadays, some nitrides, especially GaN and AlN, are the most important materials for optical emission in the ultraviolet and blue regions. Oxide crystals, such as ZnO and β-Ga2O3, offer similarly good <span class="hlt">electronic</span> properties but still suffer from significant difficulties in obtaining stable and technologically adequate p-type conductivity. PMID:25295170</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvB..97t5113A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvB..97t5113A"><span><span class="hlt">Electronic</span> and spin structure of the wide-<span class="hlt">band</span>-gap topological insulator: Nearly stoichiometric Bi2Te2S</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Annese, E.; Okuda, T.; Schwier, E. F.; Iwasawa, H.; Shimada, K.; Natamane, M.; Taniguchi, M.; Rusinov, I. P.; Eremeev, S. V.; Kokh, K. A.; Golyashov, V. A.; Tereshchenko, O. E.; Chulkov, E. V.; Kimura, A.</p> <p>2018-05-01</p> <p>We have grown the phase-homogeneous ternary compound with composition Bi2Te1.85S1.15 very close to the stoichiometric Bi2Te2S . The measurements performed with spin- and angle-resolved photoelectron spectroscopy as well as density functional theory and G W calculations revealed a wide-<span class="hlt">band</span>-gap three-dimensional topological insulator phase. The surface <span class="hlt">electronic</span> spectrum is characterized by the topological surface state (TSS) with Dirac point located above the valence <span class="hlt">band</span> and Fermi level lying in the <span class="hlt">band</span> gap. TSS <span class="hlt">band</span> dispersion and constant <span class="hlt">energy</span> contour manifest a weak warping effect near the Fermi level along with in-plane and out-of-plane spin polarization along the Γ ¯-K ¯ line. We identified four additional states at deeper binding <span class="hlt">energies</span> with high in-plane spin polarization.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1982fegc.conf..867L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1982fegc.conf..867L"><span>Saturation of side-<span class="hlt">band</span> instabilities in a free-<span class="hlt">electron</span> laser</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lin, A. T.</p> <p></p> <p>The efficiency of a free <span class="hlt">electron</span> laser is intrinsically limited because the growth of the ponderomotive force produced by the interaction of the rippled magnetic field and the signal wave will eventually trap the <span class="hlt">electrons</span>. There are a number of approaches for enhancing the efficiency of a free <span class="hlt">electron</span> laser (FEL). One approach employs a dc field. Most of the efficiency enhancement calculations use a single-mode approximation which prohibits the side <span class="hlt">band</span> waves to grow. In the present investigation, a particle simulation procedure is employed to demonstrate that the enhancement process is ultimately terminated by the generation of side <span class="hlt">band</span> instabilities due to the interaction of the trapped <span class="hlt">electrons</span> and the signal wave. The side <span class="hlt">band</span> instability will play an important part in determining the maximum output power which can be obtained from a FEL. It is also shown that a considerable improvement in output power can still be achieved by carefully choosing the strength and the turn-on time of the dc electric field.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27168177','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27168177"><span>Hot-<span class="hlt">electron</span>-based solar <span class="hlt">energy</span> conversion with metal-semiconductor nanodiodes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lee, Young Keun; Lee, Hyosun; Lee, Changhwan; Hwang, Euyheon; Park, Jeong Young</p> <p>2016-06-29</p> <p><span class="hlt">Energy</span> dissipation at metal surfaces or interfaces between a metal and a dielectric generally results from elementary excitations, including phonons and <span class="hlt">electronic</span> excitation, once external <span class="hlt">energy</span> is deposited to the surface/interface during exothermic chemical processes or an electromagnetic wave incident. In this paper, we outline recent research activities to develop <span class="hlt">energy</span> conversion devices based on hot <span class="hlt">electrons</span>. We found that photon <span class="hlt">energy</span> can be directly converted to hot <span class="hlt">electrons</span> and that hot <span class="hlt">electrons</span> flow through the interface of metal-semiconductor nanodiodes where a Schottky barrier is formed and the <span class="hlt">energy</span> barrier is much lower than the work function of the metal. The detection of hot <span class="hlt">electron</span> flow can be successfully measured using the photocurrent; we measured the photoyield of photoemission with incident photons-to-current conversion efficiency (IPCE). We also show that surface plasmons (i.e. the collective oscillation of conduction <span class="hlt">band</span> <span class="hlt">electrons</span> induced by interaction with an electromagnetic field) are excited on a rough metal surface and subsequently decay into secondary <span class="hlt">electrons</span>, which gives rise to enhancement of the IPCE. Furthermore, the unique optical behavior of surface plasmons can be coupled with dye molecules, suggesting the possibility for producing additional channels for hot <span class="hlt">electron</span> generation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22596910-layer-specific-optical-band-gap-measurement-nanoscale-mos-sub-res-sub-van-der-waals-compounds-high-resolution-electron-energy-loss-spectroscopy','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22596910-layer-specific-optical-band-gap-measurement-nanoscale-mos-sub-res-sub-van-der-waals-compounds-high-resolution-electron-energy-loss-spectroscopy"><span>Layer specific optical <span class="hlt">band</span> gap measurement at nanoscale in MoS{sub 2} and ReS{sub 2} van der Waals compounds by high resolution <span class="hlt">electron</span> <span class="hlt">energy</span> loss spectroscopy</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Dileep, K., E-mail: dileep@jncasr.ac.in, E-mail: ranjan@jncasr.ac.in; Sahu, R.; Datta, R., E-mail: dileep@jncasr.ac.in, E-mail: ranjan@jncasr.ac.in</p> <p>2016-03-21</p> <p>Layer specific direct measurement of optical <span class="hlt">band</span> gaps of two important van der Waals compounds, MoS{sub 2} and ReS{sub 2}, is performed at nanoscale by high resolution <span class="hlt">electron</span> <span class="hlt">energy</span> loss spectroscopy. For monolayer MoS{sub 2}, the twin excitons (1.8 and 1.95 eV) originating at the K point of the Brillouin zone are observed. An indirect <span class="hlt">band</span> gap of 1.27 eV is obtained from the multilayer regions. Indirect to direct <span class="hlt">band</span> gap crossover is observed which is consistent with the previously reported strong photoluminescence from the monolayer MoS{sub 2}. For ReS{sub 2}, the <span class="hlt">band</span> gap is direct, and a value of 1.52 andmore » 1.42 eV is obtained for the monolayer and multilayer, respectively. The <span class="hlt">energy</span> loss function is dominated by features due to high density of states at both the valence and conduction <span class="hlt">band</span> edges, and the difference in analyzing <span class="hlt">band</span> gap with respect to ZnO is highlighted. Crystalline 1T ReS{sub 2} forms two dimensional chains like superstructure due to the clustering between four Re atoms. The results demonstrate the power of HREELS technique as a nanoscale optical absorption spectroscopy tool.« less</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li class="active"><span>5</span></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_5 --> <div id="page_6" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li class="active"><span>6</span></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="101"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23851673','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23851673"><span>Strain and curvature induced evolution of <span class="hlt">electronic</span> <span class="hlt">band</span> structures in twisted graphene bilayer.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yan, Wei; He, Wen-Yu; Chu, Zhao-Dong; Liu, Mengxi; Meng, Lan; Dou, Rui-Fen; Zhang, Yanfeng; Liu, Zhongfan; Nie, Jia-Cai; He, Lin</p> <p>2013-01-01</p> <p>It is well established that strain and geometry could affect the <span class="hlt">band</span> structure of graphene monolayer dramatically. Here we study the evolution of local <span class="hlt">electronic</span> properties of a twisted graphene bilayer induced by a strain and a high curvature, which are found to strongly affect the local <span class="hlt">band</span> structures of the twisted graphene bilayer. The <span class="hlt">energy</span> difference of the two low-<span class="hlt">energy</span> van Hove singularities decreases with increasing lattice deformation and the states condensed into well-defined pseudo-Landau levels, which mimic the quantization of massive chiral fermions in a magnetic field of about 100 T, along a graphene wrinkle. The joint effect of strain and out-of-plane distortion in the graphene wrinkle also results in a valley polarization with a significant gap. These results suggest that strained graphene bilayer could be an ideal platform to realize the high-temperature zero-field quantum valley Hall effect.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013JPCS...74...45S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013JPCS...74...45S"><span>A simplified approach to the <span class="hlt">band</span> gap correction of defect formation <span class="hlt">energies</span>: Al, Ga, and In-doped ZnO</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Saniz, R.; Xu, Y.; Matsubara, M.; Amini, M. N.; Dixit, H.; Lamoen, D.; Partoens, B.</p> <p>2013-01-01</p> <p>The calculation of defect levels in semiconductors within a density functional theory approach suffers greatly from the <span class="hlt">band</span> gap problem. We propose a <span class="hlt">band</span> gap correction scheme that is based on the separation of <span class="hlt">energy</span> differences in <span class="hlt">electron</span> addition and relaxation <span class="hlt">energies</span>. We show that it can predict defect levels with a reasonable accuracy, particularly in the case of defects with conduction <span class="hlt">band</span> character, and yet is simple and computationally economical. We apply this method to ZnO doped with group III elements (Al, Ga, In). As expected from experiment, the results indicate that Zn substitutional doping is preferred over interstitial doping in Al, Ga, and In-doped ZnO, under both zinc-rich and oxygen-rich conditions. Further, all three dopants act as shallow donors, with the +1 charge state having the most advantageous formation <span class="hlt">energy</span>. Also, doping effects on the <span class="hlt">electronic</span> structure of ZnO are sufficiently mild so as to affect little the fundamental <span class="hlt">band</span> gap and lowest conduction <span class="hlt">bands</span> dispersion, which secures their n-type transparent conducting behavior. A comparison with the extrapolation method based on LDA+U calculations and with the Heyd-Scuseria-Ernzerhof hybrid functional (HSE) shows the reliability of the proposed scheme in predicting the thermodynamic transition levels in shallow donor systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1414278-energy-impacts-wide-band-gap-semiconductors-light-duty-electric-vehicle-fleet','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1414278-energy-impacts-wide-band-gap-semiconductors-light-duty-electric-vehicle-fleet"><span><span class="hlt">Energy</span> Impacts of Wide <span class="hlt">Band</span> Gap Semiconductors in U.S. Light-Duty Electric Vehicle Fleet</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Warren, Joshua A.; Riddle, Matthew E.; Graziano, Diane J.</p> <p>2015-08-12</p> <p>Silicon carbide and gallium nitride, two leading wide <span class="hlt">band</span> gap semiconductors with significant potential in electric vehicle power <span class="hlt">electronics</span>, are examined from a life cycle <span class="hlt">energy</span> perspective and compared with incumbent silicon in U.S. light-duty electric vehicle fleet. Cradle-to-gate, silicon carbide is estimated to require more than twice the <span class="hlt">energy</span> as silicon. However, the magnitude of vehicle use phase fuel savings potential is comparatively several orders of magnitude higher than the marginal increase in cradle-to-gate <span class="hlt">energy</span>. Gallium nitride cradle-to-gate <span class="hlt">energy</span> requirements are estimated to be similar to silicon, with use phase savings potential similar to or exceeding that of siliconmore » carbide. Potential <span class="hlt">energy</span> reductions in the United States vehicle fleet are examined through several scenarios that consider the market adoption potential of electric vehicles themselves, as well as the market adoption potential of wide <span class="hlt">band</span> gap semiconductors in electric vehicles. For the 2015–2050 time frame, cumulative <span class="hlt">energy</span> savings associated with the deployment of wide <span class="hlt">band</span> gap semiconductors are estimated to range from 2–20 billion GJ depending on market adoption dynamics.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016SPIE10000E..1QC','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016SPIE10000E..1QC"><span>Model development for MODIS thermal <span class="hlt">band</span> <span class="hlt">electronic</span> cross-talk</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chang, Tiejun; Wu, Aisheng; Geng, Xu; Li, Yonghong; Brinkmann, Jake; Keller, Graziela; Xiong, Xiaoxiong (Jack)</p> <p>2016-10-01</p> <p>MODerate-resolution Imaging Spectroradiometer (MODIS) has 36 <span class="hlt">bands</span>. Among them, 16 thermal emissive <span class="hlt">bands</span> covering a wavelength range from 3.8 to 14.4 μm. After 16 years on-orbit operation, the <span class="hlt">electronic</span> crosstalk of a few Terra MODIS thermal emissive <span class="hlt">bands</span> develop substantial issues which cause biases in the EV brightness temperature measurements and surface feature contamination. The crosstalk effects on <span class="hlt">band</span> 27 with center wavelength at 6.7 μm and <span class="hlt">band</span> 29 at 8.5 μm increased significantly in recent years, affecting downstream products such as water vapor and cloud mask. The crosstalk issue can be observed from nearly monthly scheduled lunar measurements, from which the crosstalk coefficients can be derived. Most of MODIS thermal <span class="hlt">bands</span> are saturated at moon surface temperatures and the development of an alternative approach is very helpful for verification. In this work, a physical model was developed to assess the crosstalk impact on calibration as well as in Earth view brightness temperature retrieval. This model was applied to Terra MODIS <span class="hlt">band</span> 29 empirically for correction of Earth brightness temperature measurements. In the model development, the detector nonlinear response is considered. The impacts of the <span class="hlt">electronic</span> crosstalk are assessed in two steps. The first step consists of determining the impact on calibration using the on-board blackbody (BB). Due to the detector nonlinear response and large background signal, both linear and nonlinear coefficients are affected by the crosstalk from sending <span class="hlt">bands</span>. The crosstalk impact on calibration coefficients was calculated. The second step is to calculate the effects on the Earth view brightness temperature retrieval. The effects include those from affected calibration coefficients and the contamination of Earth view measurements. This model links the measurement bias with crosstalk coefficients, detector nonlinearity, and the ratio of Earth measurements between the sending and receiving <span class="hlt">bands</span>. The correction</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29428431','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29428431"><span><span class="hlt">Energy</span>-weighted dynamical scattering simulations of <span class="hlt">electron</span> diffraction modalities in the scanning <span class="hlt">electron</span> microscope.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pascal, Elena; Singh, Saransh; Callahan, Patrick G; Hourahine, Ben; Trager-Cowan, Carol; Graef, Marc De</p> <p>2018-04-01</p> <p>Transmission Kikuchi diffraction (TKD) has been gaining momentum as a high resolution alternative to <span class="hlt">electron</span> back-scattered diffraction (EBSD), adding to the existing <span class="hlt">electron</span> diffraction modalities in the scanning <span class="hlt">electron</span> microscope (SEM). The image simulation of any of these measurement techniques requires an <span class="hlt">energy</span> dependent diffraction model for which, in turn, knowledge of <span class="hlt">electron</span> <span class="hlt">energies</span> and diffraction distances distributions is required. We identify the sample-detector geometry and the effect of inelastic events on the diffracting <span class="hlt">electron</span> beam as the important factors to be considered when predicting these distributions. However, tractable models taking into account inelastic scattering explicitly are lacking. In this study, we expand the Monte Carlo (MC) <span class="hlt">energy</span>-weighting dynamical simulations models used for EBSD [1] and ECP [2] to the TKD case. We show that the foil thickness in TKD can be used as a means of <span class="hlt">energy</span> filtering and compare <span class="hlt">band</span> sharpness in the different modalities. The current model is shown to correctly predict TKD patterns and, through the dictionary indexing approach, to produce higher quality indexed TKD maps than conventional Hough transform approach, especially close to grain boundaries. Copyright © 2018 The Authors. Published by Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22493431-vibrational-renormalisation-electronic-band-gap-hexagonal-cubic-ice','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22493431-vibrational-renormalisation-electronic-band-gap-hexagonal-cubic-ice"><span>Vibrational renormalisation of the <span class="hlt">electronic</span> <span class="hlt">band</span> gap in hexagonal and cubic ice</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Engel, Edgar A., E-mail: eae32@cam.ac.uk; Needs, Richard J.; Monserrat, Bartomeu</p> <p>2015-12-28</p> <p><span class="hlt">Electron</span>-phonon coupling in hexagonal and cubic water ice is studied using first-principles quantum mechanical methods. We consider 29 distinct hexagonal and cubic ice proton-orderings with up to 192 molecules in the simulation cell to account for proton-disorder. We find quantum zero-point vibrational corrections to the minimum <span class="hlt">electronic</span> <span class="hlt">band</span> gaps ranging from −1.5 to −1.7 eV, which leads to improved agreement between calculated and experimental <span class="hlt">band</span> gaps. Anharmonic nuclear vibrations play a negligible role in determining the gaps. Deuterated ice has a smaller <span class="hlt">band</span>-gap correction at zero-temperature of −1.2 to −1.4 eV. Vibrations reduce the differences between the <span class="hlt">electronic</span> <span class="hlt">band</span> gapsmore » of different proton-orderings from around 0.17 eV to less than 0.05 eV, so that the <span class="hlt">electronic</span> <span class="hlt">band</span> gaps of hexagonal and cubic ice are almost independent of the proton-ordering when quantum nuclear vibrations are taken into account. The comparatively small reduction in the <span class="hlt">band</span> gap over the temperature range 0 − 240 K of around 0.1 eV does not depend on the proton ordering, or whether the ice is protiated or deuterated, or hexagonal, or cubic. We explain this in terms of the atomistic origin of the strong <span class="hlt">electron</span>-phonon coupling in ice.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JAP...122h5104W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JAP...122h5104W"><span><span class="hlt">Electronic</span> <span class="hlt">band</span> structures and excitonic properties of delafossites: A GW-BSE study</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Xiaoming; Meng, Weiwei; Yan, Yanfa</p> <p>2017-08-01</p> <p>We report the <span class="hlt">band</span> structures and excitonic properties of delafossites CuMO2 (M=Al, Ga, In, Sc, Y, Cr) calculated using the state-of-the-art GW-BSE approach. We evaluate different levels of self-consistency of the GW approximations, namely G0W0, GW0, GW, and QSGW, on the <span class="hlt">band</span> structures and find that GW0, in general, predicts the <span class="hlt">band</span> gaps in better agreement with experiments considering the <span class="hlt">electron</span>-hole effect. For CuCrO2, the HSE wave function is used as the starting point for the perturbative GW0 calculations, since it corrects the <span class="hlt">band</span> orders wrongly predicted by PBE. The discrepancy about the valence <span class="hlt">band</span> characters of CuCrO2 is classified based on both HSE and QSGW calculations. The PBE wave functions, already good, are used for other delafossites. All the delafossites are shown to be indirect <span class="hlt">band</span> gap semiconductors with large exciton binding <span class="hlt">energies</span>, varying from 0.24 to 0.44 eV, in consistent with experimental findings. The excitation mechanisms are explained by examining the exciton amplitude projections on the <span class="hlt">band</span> structures. Discrepancies compared with experiments are also addressed. The lowest and strongest exciton, mainly contributed from either Cu 3d → Cu 3p (Al, Ga, In) or Cu 3d → M 3d (M = Sc, Y, Cr) transitions, is always located at the L point of the rhombohedral Brillouin zone.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22907644','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22907644"><span>Spectroscopy of the simplest Criegee intermediate CH2OO: simulation of the first <span class="hlt">bands</span> in its <span class="hlt">electronic</span> and photoelectron spectra.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lee, Edmond P F; Mok, Daniel K W; Shallcross, Dudley E; Percival, Carl J; Osborn, David L; Taatjes, Craig A; Dyke, John M</p> <p>2012-09-24</p> <p>CH(2)OO, the simplest Criegee intermediate, and ozone are isoelectronic. They both play very important roles in atmospheric chemistry. Whilst extensive experimental studies have been made on ozone, there were no direct gas-phase studies on CH(2)OO until very recently when its photoionization spectrum was recorded and kinetics studies were made of some reactions of CH(2)OO with a number of molecules of atmospheric importance, using photoionization mass spectrometry to monitor CH(2)OO. In order to encourage more direct studies on CH(2)OO and other Criegee intermediates, the <span class="hlt">electronic</span> and photoelectron spectra of CH(2)OO have been simulated using high level <span class="hlt">electronic</span> structure calculations and Franck-Condon factor calculations, and the results are presented here. Adiabatic and vertical excitation <span class="hlt">energies</span> of CH(2)OO were calculated with TDDFT, EOM-CCSD, and CASSCF methods. Also, DFT, QCISD and CASSCF calculations were performed on neutral and low-lying ionic states, with single <span class="hlt">energy</span> calculations being carried out at higher levels to obtain more reliable ionization <span class="hlt">energies</span>. The results show that the most intense <span class="hlt">band</span> in the <span class="hlt">electronic</span> spectrum of CH(2) OO corresponds to the B(1)A' ← X(1)A' absorption. It is a broad <span class="hlt">band</span> in the region 250-450 nm showing extensive structure in vibrational modes involving O-O stretching and C-O-O bending. Evidence is presented to show that the <span class="hlt">electronic</span> absorption spectrum of CH(2)OO has probably been recorded in earlier work, albeit at low resolution. We suggest that CH(2)OO was prepared in this earlier work from the reaction of CH(2)I with O(2) and that the assignment of the observed spectrum solely to CH(2)IOO is incorrect. The low ionization <span class="hlt">energy</span> region of the photoelectron spectrum of CH(2)OO consists of two overlapping vibrationally structured <span class="hlt">bands</span> corresponding to one-<span class="hlt">electron</span> ionizations from the highest two occupied molecular orbitals of the neutral molecule. In each case, the adiabatic component is the most intense</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24783945','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24783945"><span>Direct imaging of <span class="hlt">band</span> profile in single layer MoS2 on graphite: quasiparticle <span class="hlt">energy</span> gap, metallic edge states, and edge <span class="hlt">band</span> bending.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhang, Chendong; Johnson, Amber; Hsu, Chang-Lung; Li, Lain-Jong; Shih, Chih-Kang</p> <p>2014-05-14</p> <p>Using scanning tunneling microscopy and spectroscopy, we probe the <span class="hlt">electronic</span> structures of single layer MoS2 on graphite. The apparent quasiparticle <span class="hlt">energy</span> gap of single layer MoS2 is measured to be 2.15 ± 0.06 eV at 77 K, albeit a higher second conduction <span class="hlt">band</span> threshold at 0.2 eV above the apparent conduction <span class="hlt">band</span> minimum is also observed. Combining it with photoluminescence studies, we deduce an exciton binding <span class="hlt">energy</span> of 0.22 ± 0.1 eV (or 0.42 eV if the second threshold is use), a value that is lower than current theoretical predictions. Consistent with theoretical predictions, we directly observe metallic edge states of single layer MoS2. In the bulk region of MoS2, the Fermi level is located at 1.8 eV above the valence <span class="hlt">band</span> maximum, possibly due to the formation of a graphite/MoS2 heterojunction. At the edge, however, we observe an upward <span class="hlt">band</span> bending of 0.6 eV within a short depletion length of about 5 nm, analogous to the phenomena of Fermi level pinning of a 3D semiconductor by metallic surface states.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JPCS..101...45S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JPCS..101...45S"><span>k - dependent Jeff=1/2 <span class="hlt">band</span> splitting and the <span class="hlt">electron</span>-hole asymmetry in SrIrO3</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Singh, Vijeta; Pulikkotil, J. J.</p> <p>2017-02-01</p> <p>The Ir ion in Srn+1 IrnO 3 n + 1 series of compounds is octahedrally coordinated. However, unlike Sr2IrO4 (n=1) and Sr3Ir2O7 (n=2) which are insulating due to spin-orbit induced Jeff splitting of the t2g <span class="hlt">bands</span>, SrIrO3 (n= ∞) is conducting. To explore whether such a splitting is relevant in SrIrO3, and if so to what extent, we investigate the <span class="hlt">electronic</span> structure of orthorhombic SrIrO3 using density functional theory. Calculations reveal that the crystal field split Ir t2 g <span class="hlt">bands</span> in SrIrO3 are indeed split into Jeff=3/2 and and Jeff=1/2 states. However, the splitting is found to be strongly k - dependent with its magnitude determined by the Ir - O orbital hybridization. Besides, we find that the spin-orbit induced pseudo-gap, into which the Fermi <span class="hlt">energy</span> is positioned, is composed of both light <span class="hlt">electron</span>-like and heavy hole-like <span class="hlt">bands</span>. These features in the <span class="hlt">band</span> structure of SrIrO3 suggest that variations in the carrier concentration control the <span class="hlt">electronic</span> transport properties in SrIrO3, which is consistent with the experiments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28682010','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28682010"><span>Organic High <span class="hlt">Electron</span> Mobility Transistors Realized by 2D <span class="hlt">Electron</span> Gas.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhang, Panlong; Wang, Haibo; Yan, Donghang</p> <p>2017-09-01</p> <p>A key breakthrough in inorganic modern <span class="hlt">electronics</span> is the <span class="hlt">energy-band</span> engineering that plays important role to improve device performance or develop novel functional devices. A typical application is high <span class="hlt">electron</span> mobility transistors (HEMTs), which utilizes 2D <span class="hlt">electron</span> gas (2DEG) as transport channel and exhibits very high <span class="hlt">electron</span> mobility over traditional field-effect transistors (FETs). Recently, organic <span class="hlt">electronics</span> have made very rapid progress and the <span class="hlt">band</span> transport model is demonstrated to be more suitable for explaining carrier behavior in high-mobility crystalline organic materials. Therefore, there emerges a chance for applying <span class="hlt">energy-band</span> engineering in organic semiconductors to tailor their optoelectronic properties. Here, the idea of <span class="hlt">energy-band</span> engineering is introduced and a novel device configuration is constructed, i.e., using quantum well structures as active layers in organic FETs, to realize organic 2DEG. Under the control of gate voltage, <span class="hlt">electron</span> carriers are accumulated and confined at quantized <span class="hlt">energy</span> levels, and show efficient 2D transport. The <span class="hlt">electron</span> mobility is up to 10 cm 2 V -1 s -1 , and the operation mechanisms of organic HEMTs are also argued. Our results demonstrate the validity of tailoring optoelectronic properties of organic semiconductors by <span class="hlt">energy-band</span> engineering, offering a promising way for the step forward of organic <span class="hlt">electronics</span>. © 2017 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhyB..522...66R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhyB..522...66R"><span><span class="hlt">Band</span> warping, <span class="hlt">band</span> non-parabolicity, and Dirac points in <span class="hlt">electronic</span> and lattice structures</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Resca, Lorenzo; Mecholsky, Nicholas A.; Pegg, Ian L.</p> <p>2017-10-01</p> <p>We illustrate at a fundamental level the physical and mathematical origins of <span class="hlt">band</span> warping and <span class="hlt">band</span> non-parabolicity in <span class="hlt">electronic</span> and vibrational structures. We point out a robust presence of pairs of topologically induced Dirac points in a primitive-rectangular lattice using a p-type tight-binding approximation. We analyze two-dimensional primitive-rectangular and square Bravais lattices with implications that are expected to generalize to more complex structures. <span class="hlt">Band</span> warping is shown to arise at the onset of a singular transition to a crystal lattice with a larger symmetry group, which allows the possibility of irreducible representations of higher dimensions, hence <span class="hlt">band</span> degeneracy, at special symmetry points in reciprocal space. <span class="hlt">Band</span> warping is incompatible with a multi-dimensional Taylor series expansion, whereas <span class="hlt">band</span> non-parabolicities are associated with multi-dimensional Taylor series expansions to all orders. Still <span class="hlt">band</span> non-parabolicities may merge into <span class="hlt">band</span> warping at the onset of a larger symmetry group. Remarkably, while still maintaining a clear connection with that merging, <span class="hlt">band</span> non-parabolicities may produce pairs of conical intersections at relatively low-symmetry points. Apparently, such conical intersections are robustly maintained by global topology requirements, rather than any local symmetry protection. For two p-type tight-binding <span class="hlt">bands</span>, we find such pairs of conical intersections drifting along the edges of restricted Brillouin zones of primitive-rectangular Bravais lattices as lattice constants vary relatively to each other, until these conical intersections merge into degenerate warped <span class="hlt">bands</span> at high-symmetry points at the onset of a square lattice. The conical intersections that we found appear to have similar topological characteristics as Dirac points extensively studied in graphene and other topological insulators, even though our conical intersections have none of the symmetry complexity and protection afforded by the latter more</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22419957-all-electron-gw-quasiparticle-band-structures-group-nitride-compounds','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22419957-all-electron-gw-quasiparticle-band-structures-group-nitride-compounds"><span>All-<span class="hlt">electron</span> GW quasiparticle <span class="hlt">band</span> structures of group 14 nitride compounds</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Chu, Iek-Heng; Cheng, Hai-Ping, E-mail: cheng@qtp.ufl.edu; Kozhevnikov, Anton</p> <p></p> <p>We have investigated the group 14 nitrides (M{sub 3}N{sub 4}) in the spinel phase (γ-M{sub 3}N{sub 4} with M = C, Si, Ge, and Sn) and β phase (β-M{sub 3}N{sub 4} with M = Si, Ge, and Sn) using density functional theory with the local density approximation and the GW approximation. The Kohn-Sham <span class="hlt">energies</span> of these systems have been first calculated within the framework of full-potential linearized augmented plane waves (LAPW) and then corrected using single-shot G{sub 0}W{sub 0} calculations, which we have implemented in the modified version of the Elk full-potential LAPW code. Direct <span class="hlt">band</span> gaps at the Γmore » point have been found for spinel-type nitrides γ-M{sub 3}N{sub 4} with M = Si, Ge, and Sn. The corresponding GW-corrected <span class="hlt">band</span> gaps agree with experiment. We have also found that the GW calculations with and without the plasmon-pole approximation give very similar results, even when the system contains semi-core d <span class="hlt">electrons</span>. These spinel-type nitrides are novel materials for potential optoelectronic applications because of their direct and tunable <span class="hlt">band</span> gaps.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PhRvB..93q4516C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhRvB..93q4516C"><span>Superconductivity versus bound-state formation in a two-<span class="hlt">band</span> superconductor with small Fermi <span class="hlt">energy</span>: Applications to Fe pnictides/chalcogenides and doped SrTiO3</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chubukov, Andrey V.; Eremin, Ilya; Efremov, Dmitri V.</p> <p>2016-05-01</p> <p>We analyze the interplay between superconductivity and the formation of bound pairs of fermions (BCS-BEC crossover) in a 2D model of interacting fermions with small Fermi <span class="hlt">energy</span> EF and weak attractive interaction, which extends to <span class="hlt">energies</span> well above EF. The 2D case is special because a two-particle bound state forms at arbitrary weak interaction, and already at weak coupling, one has to distinguish between the bound-state formation and superconductivity. We briefly review the situation in the one-<span class="hlt">band</span> model and then consider two different two-<span class="hlt">band</span> models: one with one hole <span class="hlt">band</span> and one <span class="hlt">electron</span> <span class="hlt">band</span> and another with two hole or two <span class="hlt">electron</span> <span class="hlt">bands</span>. In each case, we obtain the bound-state <span class="hlt">energy</span> 2 E0 for two fermions in a vacuum and solve the set of coupled equations for the pairing gaps and the chemical potentials to obtain the onset temperature of the pairing Tins and the quasiparticle dispersion at T =0 . We then compute the superfluid stiffness ρs(T =0 ) and obtain the actual Tc. For definiteness, we set EF in one <span class="hlt">band</span> to be near zero and consider different ratios of E0 and EF in the other <span class="hlt">band</span>. We show that at EF≫E0 , the behavior of both two-<span class="hlt">band</span> models is BCS-like in the sense that Tc≈Tins≪EF and Δ ˜Tc . At EF≪E0 , the two models behave differently: in the model with two hole/two <span class="hlt">electron</span> <span class="hlt">bands</span>, Tins˜E0/lnE/0EF , Δ ˜(E0EF) 1 /2 , and Tc˜EF , like in the one-<span class="hlt">band</span> model. In between Tins and Tc, the system displays a preformed pair behavior. In the model with one hole and one <span class="hlt">electron</span> <span class="hlt">bands</span>, Tc remains of order Tins, and both remain finite at EF=0 and of the order of E0. The preformed pair behavior still does exist in this model because Tc is numerically smaller than Tins. For both models, we reexpress Tins in terms of the fully renormalized two-particle scattering amplitude by extending to the two-<span class="hlt">band</span> case (the method pioneered by Gorkov and Melik-Barkhudarov back in 1961). We apply our results for the model with a hole and an <span class="hlt">electron</span> <span class="hlt">band</span> to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005ApPhL..87c2102K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005ApPhL..87c2102K"><span><span class="hlt">Band</span> gap and <span class="hlt">band</span> offset of (GaIn)(PSb) lattice matched to InP</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Köhler, F.; Böhm, G.; Meyer, R.; Amann, M.-C.</p> <p>2005-07-01</p> <p>Metastable (GaxIn1-x)(PySb1-y) layers were grown on (001) InP substrates by gas source molecular beam epitaxy. Low-temperature photoluminescence spectroscopy was applied to these heterostructures and revealed spatially indirect <span class="hlt">band-to-band</span> recombination of <span class="hlt">electrons</span> localized in the InP with holes in the (GaxIn1-x)(PySb1-y). In addition, samples with layer thicknesses larger than 100nm showed direct PL across the <span class="hlt">band</span> gap of (GaxIn1-x)(PySb1-y). <span class="hlt">Band</span>-gap <span class="hlt">energies</span> and <span class="hlt">band</span> offset <span class="hlt">energies</span> of (GaxIn1-x)(PySb1-y) relative to InP were derived from these PL data. A strong bowing parameter was observed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20481897','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20481897"><span>Effects of <span class="hlt">electronic</span> and lattice polarization on the <span class="hlt">band</span> structure of delafossite transparent conductive oxides.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Vidal, Julien; Trani, Fabio; Bruneval, Fabien; Marques, Miguel A L; Botti, Silvana</p> <p>2010-04-02</p> <p>We use hybrid functionals and restricted self-consistent GW, state-of-the-art theoretical approaches for quasiparticle <span class="hlt">band</span> structures, to study the <span class="hlt">electronic</span> states of delafossite Cu(Al,In)O2, the first p-type and bipolar transparent conductive oxides. We show that a self-consistent GW approximation gives remarkably wider <span class="hlt">band</span> gaps than all the other approaches used so far. Accounting for polaronic effects in the GW scheme we recover a very nice agreement with experiments. Furthermore, the modifications with respect to the Kohn-Sham <span class="hlt">bands</span> are strongly k dependent, which makes questionable the common practice of using a scissor operator. Finally, our results support the view that the low <span class="hlt">energy</span> structures found in optical experiments, and initially attributed to an indirect transition, are due to intrinsic defects in the samples.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120013672','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120013672"><span>Terra MODIS <span class="hlt">Band</span> 27 <span class="hlt">Electronic</span> Crosstalk Effect and Its Removal</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sun, Junqiang; Xiong, Xiaoxiong; Madhavan, Sriharsha; Wenny, Brian</p> <p>2012-01-01</p> <p>The MODerate-resolution Imaging Spectroradiometer (MODIS) is one of the primary instruments in the NASA Earth Observing System (EOS). The first MODIS instrument was launched in December, 1999 on-board the Terra spacecraft. MODIS has 36 <span class="hlt">bands</span>, covering a wavelength range from 0.4 micron to 14.4 micron. MODIS <span class="hlt">band</span> 27 (6.72 micron) is a water vapor <span class="hlt">band</span>, which is designed to be insensitive to Earth surface features. In recent Earth View (EV) images of Terra <span class="hlt">band</span> 27, surface feature contamination is clearly seen and striping has become very pronounced. In this paper, it is shown that <span class="hlt">band</span> 27 is impacted by <span class="hlt">electronic</span> crosstalk from <span class="hlt">bands</span> 28-30. An algorithm using a linear approximation is developed to correct the crosstalk effect. The crosstalk coefficients are derived from Terra MODIS lunar observations. They show that the crosstalk is strongly detector dependent and the crosstalk pattern has changed dramatically since launch. The crosstalk contributions are positive to the instrument response of <span class="hlt">band</span> 27 early in the mission but became negative and much larger in magnitude at later stages of the mission for most detectors of the <span class="hlt">band</span>. The algorithm is applied to both Black Body (BB) calibration and MODIS L1B products. With the crosstalk effect removed, the calibration coefficients of Terra MODIS <span class="hlt">band</span> 27 derived from the BB show that the detector differences become smaller. With the algorithm applied to MODIS L1B products, the Earth surface features are significantly removed and the striping is substantially reduced in the images of the <span class="hlt">band</span>. The approach developed in this report for removal of the <span class="hlt">electronic</span> crosstalk effect can be applied to other MODIS <span class="hlt">bands</span> if similar crosstalk behaviors occur.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22469724-binding-energy-excitons-formed-from-spatially-separated-electrons-holes-insulating-quantum-dots','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22469724-binding-energy-excitons-formed-from-spatially-separated-electrons-holes-insulating-quantum-dots"><span>Binding <span class="hlt">energy</span> of excitons formed from spatially separated <span class="hlt">electrons</span> and holes in insulating quantum dots</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Pokutnyi, S. I., E-mail: pokutnyi-sergey@inbox.ru; Kulchin, Yu. N.; Dzyuba, V. P.</p> <p></p> <p>It is found that the binding <span class="hlt">energy</span> of the ground state of an exciton formed from an <span class="hlt">electron</span> and a hole spatially separated from each other (the hole is moving within a quantum dot, and the <span class="hlt">electron</span> is localized above the spherical (quantum dot)–(insulating matrix) interface) in a nanosystem containing insulating Al{sub 2}O{sub 3} quantum dots is substantially increased (by nearly two orders of magnitude) compared to the exciton binding <span class="hlt">energy</span> in an Al{sub 2}O{sub 3} single crystal. It is established that, in the <span class="hlt">band</span> gap of an Al{sub 2}O{sub 3} nanoparticle, a <span class="hlt">band</span> of exciton states (formed from spatiallymore » separated <span class="hlt">electrons</span> and holes) appears. It is shown that there exists the possibility of experimentally detecting the ground and excited exciton states in the <span class="hlt">band</span> gap of Al{sub 2}O{sub 3} nanoparticles at room temperature from the absorption spectrum of the nanosystem.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JPhD...50X5106M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JPhD...50X5106M"><span>Influence of <span class="hlt">energy</span> <span class="hlt">band</span> alignment in mixed crystalline TiO2 nanotube arrays: good for photocatalysis, bad for <span class="hlt">electron</span> transfer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mohammadpour, Raheleh</p> <p>2017-12-01</p> <p>Despite the wide application ranges of TiO2, the precise explanation of the charge transport dynamic through a mixed crystal phase of this semiconductor has remained elusive. Here, in this research, mixed-phase TiO2 nanotube arrays (TNTAs) consisting of anatase and 0-15% rutile phases has been formed through various annealing processes and employed as a photoelectrode of a photovoltaic cell. Wide ranges of optoelectronic experiments have been employed to explore the <span class="hlt">band</span> alignment position, as well as the depth and density of trap states in TNTAs. Short circuit potential, as well as open circuit potential measurements specified that the <span class="hlt">band</span> alignment of more than 0.2 eV exists between the anatase and rutile phase Fermi levels, with a higher <span class="hlt">electron</span> affinity for anatase; this can result in a potential barrier in crystallite interfaces and the deterioration of <span class="hlt">electron</span> mobility through mixed phase structures. Moreover, a higher density of shallow localized trap states below the conduction <span class="hlt">band</span> with more depth (133 meV in anatase to 247 meV in 15% rutile phase) and also deep oxygen vacancy traps have been explored upon introducing the rutile phase. Based on our results, employing TiO2 nanotubes as just the <span class="hlt">electron</span> transport medium in mixed crystalline phases can deteriorate the charge transport mechanism, however, in photocatalytic applications when both <span class="hlt">electrons</span> and holes are present, a robust charge separation in crystalline anatase/rutile interphases will result in better performances.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1999JPhB...32.2729G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1999JPhB...32.2729G"><span>The <span class="hlt">electronic</span> states of cyclopropane studied by VUV absorption and <span class="hlt">electron</span> <span class="hlt">energy</span>-loss spectroscopies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gingell, M.; Mason, N. J.; Walker, I. C.; Marston, G.; Zhao, H.; Siggel, M. R. F.</p> <p>1999-06-01</p> <p>Absolute optical (VUV) absorption cross sections for cyclopropane have been measured from 5.0 to 11.2 and 20-40 eV using synchrotron radiation. Also, <span class="hlt">electron</span> <span class="hlt">energy</span>-loss (EEL) spectra have been obtained using incident <span class="hlt">electrons</span> of (a) 150 eV <span class="hlt">energy</span> scattered through small angles (<span class="hlt">energy</span> loss 5.0-15 eV) and (b) near-threshold <span class="hlt">energies</span> scattered through large angles (<span class="hlt">energy</span> loss 0-10.5 eV). Taken together these confirm that the low-lying excited <span class="hlt">electronic</span> states of cyclopropane are of Rydberg type and, although spectral <span class="hlt">bands</span> are diffuse, a known Rydberg series has been extended. Recent computations (Galasso V 1996 Chem. Phys. 206 289) appear to give a good account of the experimental spectrum from threshold to about 11 eV, but these must be extended if valence-excited states are to be characterized. Particular attention has been directed at the evaluation of absolute optical cross sections. These are now believed to be established over the <span class="hlt">energy</span> ranges 5-15 and 20-40 eV. In the gap region (15-20 eV) second-order radiation may affect the optical measurements. From consideration of second-order effects, and comparison of the present studies with earlier measurements, we propose a best-estimate cross section in this <span class="hlt">energy</span> region also.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li class="active"><span>6</span></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_6 --> <div id="page_7" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li class="active"><span>7</span></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="121"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ApPhL.112a1602M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ApPhL.112a1602M"><span><span class="hlt">Electronic</span> structure of indium-tungsten-oxide alloys and their <span class="hlt">energy</span> <span class="hlt">band</span> alignment at the heterojunction to crystalline silicon</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Menzel, Dorothee; Mews, Mathias; Rech, Bernd; Korte, Lars</p> <p>2018-01-01</p> <p>The <span class="hlt">electronic</span> structure of thermally co-evaporated indium-tungsten-oxide films is investigated. The stoichiometry is varied from pure tungsten oxide to pure indium oxide, and the <span class="hlt">band</span> alignment at the indium-tungsten-oxide/crystalline silicon heterointerface is monitored. Using in-system photoelectron spectroscopy, optical spectroscopy, and surface photovoltage measurements, we show that the work function of indium-tungsten-oxide continuously decreases from 6.3 eV for tungsten oxide to 4.3 eV for indium oxide, with a concomitant decrease in the <span class="hlt">band</span> bending at the hetero interface to crystalline silicon than indium oxide.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JPSJ...87a4003M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JPSJ...87a4003M"><span>Size Reduction of Hamiltonian Matrix for Large-Scale <span class="hlt">Energy</span> <span class="hlt">Band</span> Calculations Using Plane Wave Bases</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Morifuji, Masato</p> <p>2018-01-01</p> <p>We present a method of reducing the size of a Hamiltonian matrix used in calculations of <span class="hlt">electronic</span> states. In the <span class="hlt">electronic</span> states calculations using plane wave basis functions, a large number of plane waves are often required to obtain precise results. Even using state-of-the-art techniques, the Hamiltonian matrix often becomes very large. The large computational time and memory necessary for diagonalization limit the widespread use of <span class="hlt">band</span> calculations. We show a procedure of deriving a reduced Hamiltonian constructed using a small number of low-<span class="hlt">energy</span> bases by renormalizing high-<span class="hlt">energy</span> bases. We demonstrate numerically that the significant speedup of eigenstates evaluation is achieved without losing accuracy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMSM41F2559M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMSM41F2559M"><span>Observations of Multi-<span class="hlt">band</span> Structures in Double Star TC-1 PEACE <span class="hlt">Electron</span> and HIA Ion Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mohan Narasimhan, K.; Fazakerley, A. N.; Grimald, S.; Dandouras, I. S.; Mihaljcic, B.; Kistler, L. M.; Owen, C. J.</p> <p>2015-12-01</p> <p>Several authors have reported inner magnetosphere observations of proton distributions confined to narrow <span class="hlt">energy</span> <span class="hlt">bands</span> in the range 1 - 25 keV (Smith and Hoffman (1974), etc). These structures have been described as "nose structures", with reference to their appearance in <span class="hlt">energy</span>-time spectrograms and are also known as "<span class="hlt">bands</span>" if they occur for extended periods of time. Multi-nose structures have been observed if 2 or more noses appear at the same time (Vallat et al., 2007). Gaps between "noses" (or "<span class="hlt">bands</span>") have been explained in terms of the competing corotation, convection and magnetic gradient drifts. Charge exchange losses in slow drift paths for steady state scenarios and the role of substorm injections have also been considered (Li et al., 2000; Ebihara et al., 2004). We analyse observations of <span class="hlt">electron</span> and ion multi-<span class="hlt">band</span> structures frequently seen in Double-Star TC1 PEACE and HIA data. We present results from statistical surveys conducted using data from the duration of the mission. Furthermore, using a combination of both statistics and simulations, we test previous theories as to possible formation mechanisms and explore other possible explanations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22258790-feasibility-study-electron-transfer-quantum-well-infrared-photodetectors-spectral-tuning-long-wave-infrared-band','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22258790-feasibility-study-electron-transfer-quantum-well-infrared-photodetectors-spectral-tuning-long-wave-infrared-band"><span>Feasibility study of <span class="hlt">electron</span> transfer quantum well infrared photodetectors for spectral tuning in the long-wave infrared <span class="hlt">band</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Jolley, Greg; Dehdashti Akhavan, Nima; Umana-Membreno, Gilberto</p> <p></p> <p>An <span class="hlt">electron</span> transfer quantum well infrared photodetector (QWIP) consisting of repeating units of two coupled quantum wells (QWs) is capable of exhibiting a two color voltage dependent spectral response. However, significant <span class="hlt">electron</span> transfer between the coupled QWs is required for spectral tuning, which may require the application of relatively high electric fields. Also, the <span class="hlt">band</span> structure of coupled quantum wells is more complicated in comparison to a regular quantum well and, therefore, it is not always obvious if an <span class="hlt">electron</span> transfer QWIP can be designed such that it meets specific performance characteristics. This paper presents a feasibility study of themore » <span class="hlt">electron</span> transfer QWIP and its suitability for spectral tuning. Self consistent calculations have been performed of the bandstructure and the electric field that results from <span class="hlt">electron</span> population within the quantum wells, from which the optical characteristics have been obtained. The <span class="hlt">band</span> structure, spectral response, and the resonant final state <span class="hlt">energy</span> locations have been compared with standard QWIPs. It is shown that spectral tuning in the long-wave infrared <span class="hlt">band</span> can be achieved over a wide wavelength range of several microns while maintaining a relatively narrow spectral response FWHM. However, the total absorption strength is more limited in comparison to a standard QWIP, since the higher QW doping densities require much higher electric fields for <span class="hlt">electron</span> transfer.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27045790','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27045790"><span>Monoclinic Tungsten Oxide with {100} Facet Orientation and Tuned <span class="hlt">Electronic</span> <span class="hlt">Band</span> Structure for Enhanced Photocatalytic Oxidations.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhang, Ning; Chen, Chen; Mei, Zongwei; Liu, Xiaohe; Qu, Xiaolei; Li, Yunxiang; Li, Siqi; Qi, Weihong; Zhang, Yuanjian; Ye, Jinhua; Roy, Vellaisamy A L; Ma, Renzhi</p> <p>2016-04-27</p> <p>Exploring surface-exposed highly active crystal facets for photocatalytic oxidations is promising in utilizing monoclinic WO3 semiconductor. However, the previously reported highly active facets for monoclinic WO3 were mainly toward enhancing photocatalytic reductions. Here we report that the WO3 with {100} facet orientation and tuned surface <span class="hlt">electronic</span> <span class="hlt">band</span> structure can effectively enhance photocatalytic oxidation properties. The {100} faceted WO3 single crystals are synthesized via a facile hydrothermal method. The UV-visible diffuse reflectance, X-ray photoelectron spectroscopy valence <span class="hlt">band</span> spectra, and photoelectrochemical measurements suggest that the {100} faceted WO3 has a much higher <span class="hlt">energy</span> level of valence <span class="hlt">band</span> maximum compared with the normal WO3 crystals without preferred orientation of the crystal face. The density functional theory calculations reveal that the shift of O 2p and W 5d states in {100} face induce a unique <span class="hlt">band</span> structure. In comparison with the normal WO3, the {100} faceted WO3 exhibits an O2 evolution rate about 5.1 times in water splitting, and also shows an acetone evolution rate of 4.2 times as well as CO2 evolution rate of 3.8 times in gaseous degradation of 2-propanol. This study demonstrates an efficient crystal face engineering route to tune the surface <span class="hlt">electronic</span> <span class="hlt">band</span> structure for enhanced photocatalytic oxidations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvB..97o5154M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvB..97o5154M"><span>Effect of structural distortion on the <span class="hlt">electronic</span> <span class="hlt">band</span> structure of NaOsO3 studied within density functional theory and a three-orbital model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mohapatra, Shubhajyoti; Bhandari, Churna; Satpathy, Sashi; Singh, Avinash</p> <p>2018-04-01</p> <p>Effects of the structural distortion associated with the OsO6 octahedral rotation and tilting on the <span class="hlt">electronic</span> <span class="hlt">band</span> structure and magnetic anisotropy <span class="hlt">energy</span> for the 5 d3 compound NaOsO3 are investigated using the density functional theory (DFT) and within a three-orbital model. Comparison of the essential features of the DFT <span class="hlt">band</span> structures with the three-orbital model for both the undistorted and distorted structures provides insight into the orbital and directional asymmetry in the <span class="hlt">electron</span> hopping terms resulting from the structural distortion. The orbital mixing terms obtained in the transformed hopping Hamiltonian resulting from the octahedral rotations are shown to account for the fine features in the DFT <span class="hlt">band</span> structure. Staggered magnetization and the magnetic character of states near the Fermi <span class="hlt">energy</span> indicate weak coupling behavior.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/4729499-analysis-energy-losses-kev-electron-beam-fluoride-chloride-bromide-lithium','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/4729499-analysis-energy-losses-kev-electron-beam-fluoride-chloride-bromide-lithium"><span>ANALYSIS OF <span class="hlt">ENERGY</span> LOSSES OF A 30-kev <span class="hlt">ELECTRON</span> BEAM IN THE FLUORIDE, CHLORIDE, AND BROMIDE OF LITHIUM (in French)</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Pradal, F.; Gout, C.</p> <p>1963-02-01</p> <p>The <span class="hlt">energy</span> loss of a 30-kev <span class="hlt">electron</span> beam in films of LiF, LiCl, and LiBr were analyzed with a magnetic spectrograph. For LiF, the results are compared to the absorption curve in the ultraviolet. The rays observed seem due to the excitation of valence <span class="hlt">band</span> <span class="hlt">electrons</span> of the 2s <span class="hlt">band</span> of F/sup -/ and the 1s <span class="hlt">band</span> of Li/sup +/. In some cases, <span class="hlt">energy</span> losses less than 10 ev were observed, which seems connected to the presence of color centers. (tr-auth)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1997SSCom.101..417S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1997SSCom.101..417S"><span><span class="hlt">Electronic</span> <span class="hlt">band</span> structure study of colossal magnetoresistance in Tl 2Mn 2O 7</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Seo, D.-K.; Whangbo, M.-H.; Subramanian, M. A.</p> <p>1997-02-01</p> <p>The <span class="hlt">electronic</span> structure of Tl 2Mn 2O 7 was examined by performing tight binding <span class="hlt">band</span> calculations. The overlap between the Mn t 2g- and Tl 6 s-block <span class="hlt">bands</span> results in a partial filling of the Tl 6 s-block <span class="hlt">bands</span>. The associated Fermi surface consists of 12 cigar-shape <span class="hlt">electron</span> pockets with each <span class="hlt">electron</span> pocket about {1}/{1000} of the first Brillouin zone in size. The Tl 6 s-block <span class="hlt">bands</span> have orbital contributions from the Mn atoms, and the carrier density is very low. These are important for the occurrence of a colossal magnetoresistance in Tl 2Mn 2O 7.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28604864','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28604864"><span>From the Kohn-Sham <span class="hlt">band</span> gap to the fundamental gap in solids. An integer <span class="hlt">electron</span> approach.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Baerends, E J</p> <p>2017-06-21</p> <p>It is often stated that the Kohn-Sham occupied-unoccupied gap in both molecules and solids is "wrong". We argue that this is not a correct statement. The KS theory does not allow to interpret the exact KS HOMO-LUMO gap as the fundamental gap (difference (I - A) of <span class="hlt">electron</span> affinity (A) and ionization <span class="hlt">energy</span> (I), twice the chemical hardness), from which it indeed differs, strongly in molecules and moderately in solids. The exact Kohn-Sham HOMO-LUMO gap in molecules is much below the fundamental gap and very close to the much smaller optical gap (first excitation <span class="hlt">energy</span>), and LDA/GGA yield very similar gaps. In solids the situation is different: the excitation <span class="hlt">energy</span> to delocalized excited states and the fundamental gap (I - A) are very similar, not so disparate as in molecules. Again the Kohn-Sham and LDA/GGA <span class="hlt">band</span> gaps do not represent (I - A) but are significantly smaller. However, the special properties of an extended system like a solid make it very easy to calculate the fundamental gap from the ground state (neutral system) <span class="hlt">band</span> structure calculations entirely within a density functional framework. The correction Δ from the KS gap to the fundamental gap originates from the response part v resp of the exchange-correlation potential and can be calculated very simply using an approximation to v resp . This affords a calculation of the fundamental gap at the same level of accuracy as other properties of crystals at little extra cost beyond the ground state bandstructure calculation. The method is based on integer <span class="hlt">electron</span> systems, fractional <span class="hlt">electron</span> systems (an ensemble of N- and (N + 1)-<span class="hlt">electron</span> systems) and the derivative discontinuity are not invoked.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24806660','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24806660"><span>Pathways of <span class="hlt">energy</span> transfer in LHCII revealed by room-temperature 2D <span class="hlt">electronic</span> spectroscopy.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wells, Kym L; Lambrev, Petar H; Zhang, Zhengyang; Garab, Gyözö; Tan, Howe-Siang</p> <p>2014-06-21</p> <p>We present here the first room-temperature 2D <span class="hlt">electronic</span> spectroscopy study of <span class="hlt">energy</span> transfer in the plant light-harvesting complex II, LHCII. Two-dimensional <span class="hlt">electronic</span> spectroscopy has been used to study <span class="hlt">energy</span> transfer dynamics in LHCII trimers from the chlorophyll b Qy <span class="hlt">band</span> to the chlorophyll a Qy <span class="hlt">band</span>. Observing cross-peak regions corresponding to couplings between different excitonic states reveals partially resolved fine structure at the exciton level that cannot be isolated by pump-probe or linear spectroscopy measurements alone. Global analysis of the data has been performed to identify the pathways and time constants of <span class="hlt">energy</span> transfer. The measured waiting time (Tw) dependent 2D spectra are found to be composed of 2D decay-associated spectra with three timescales (0.3 ps, 2.3 ps and >20 ps). Direct and multistep cascading pathways from the high-<span class="hlt">energy</span> chlorophyll b states to the lowest-<span class="hlt">energy</span> chlorophyll a states have been resolved occurring on time scales of hundreds of femtoseconds to picoseconds.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015APS..MARG10001G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015APS..MARG10001G"><span>Influence of <span class="hlt">electronic</span> <span class="hlt">band</span> topology on phonon properties in Dirac materials</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Garate, Ion; Saha, Kush; Légaré, Katherine</p> <p>2015-03-01</p> <p>In Dirac materials, the interaction between <span class="hlt">electrons</span> and long-wavelength phonons has been shown to induce and stabilize topological insulation [1-2]. Here report on a theoretical study of the converse effect, namely the influence of <span class="hlt">band</span> topology on phonon properties. We calculate how <span class="hlt">electron</span>-phonon interactions change the bulk phonon dispersion as a function of pressure and temperature, in both trivial and topological phases. We find that (i) topological insulators are more prone to lattice instabilities than trivial insulators, and (ii) Raman and neutron scattering measurements can be used to determine the <span class="hlt">electronic</span> <span class="hlt">band</span> topology. Research funded by Canada's NSERC and Québec's RQMP.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26323493','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26323493"><span>Quantitative analysis on electric dipole <span class="hlt">energy</span> in Rashba <span class="hlt">band</span> splitting.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hong, Jisook; Rhim, Jun-Won; Kim, Changyoung; Ryong Park, Seung; Hoon Shim, Ji</p> <p>2015-09-01</p> <p>We report on quantitative comparison between the electric dipole <span class="hlt">energy</span> and the Rashba <span class="hlt">band</span> splitting in model systems of Bi and Sb triangular monolayers under a perpendicular electric field. We used both first-principles and tight binding calculations on p-orbitals with spin-orbit coupling. First-principles calculation shows Rashba <span class="hlt">band</span> splitting in both systems. It also shows asymmetric charge distributions in the Rashba split <span class="hlt">bands</span> which are induced by the orbital angular momentum. We calculated the electric dipole <span class="hlt">energies</span> from coupling of the asymmetric charge distribution and external electric field, and compared it to the Rashba splitting. Remarkably, the total split <span class="hlt">energy</span> is found to come mostly from the difference in the electric dipole <span class="hlt">energy</span> for both Bi and Sb systems. A perturbative approach for long wave length limit starting from tight binding calculation also supports that the Rashba <span class="hlt">band</span> splitting originates mostly from the electric dipole <span class="hlt">energy</span> difference in the strong atomic spin-orbit coupling regime.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4555038','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4555038"><span>Quantitative analysis on electric dipole <span class="hlt">energy</span> in Rashba <span class="hlt">band</span> splitting</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Hong, Jisook; Rhim, Jun-Won; Kim, Changyoung; Ryong Park, Seung; Hoon Shim, Ji</p> <p>2015-01-01</p> <p>We report on quantitative comparison between the electric dipole <span class="hlt">energy</span> and the Rashba <span class="hlt">band</span> splitting in model systems of Bi and Sb triangular monolayers under a perpendicular electric field. We used both first-principles and tight binding calculations on p-orbitals with spin-orbit coupling. First-principles calculation shows Rashba <span class="hlt">band</span> splitting in both systems. It also shows asymmetric charge distributions in the Rashba split <span class="hlt">bands</span> which are induced by the orbital angular momentum. We calculated the electric dipole <span class="hlt">energies</span> from coupling of the asymmetric charge distribution and external electric field, and compared it to the Rashba splitting. Remarkably, the total split <span class="hlt">energy</span> is found to come mostly from the difference in the electric dipole <span class="hlt">energy</span> for both Bi and Sb systems. A perturbative approach for long wave length limit starting from tight binding calculation also supports that the Rashba <span class="hlt">band</span> splitting originates mostly from the electric dipole <span class="hlt">energy</span> difference in the strong atomic spin-orbit coupling regime. PMID:26323493</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015MS%26E...73a2100V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015MS%26E...73a2100V"><span>Effect of Γ-X <span class="hlt">band</span> mixing on the donor binding <span class="hlt">energy</span> in a Quantum Wire</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vijaya Shanthi, R.; Jayakumar, K.; Nithiananthi, P.</p> <p>2015-02-01</p> <p>To invoke the technological applications of heterostructure semiconductors like Quantum Well (QW), Quantum Well Wire (QWW) and Quantum Dot (QD), it is important to understand the property of impurity <span class="hlt">energy</span> which is responsible for the peculiar <span class="hlt">electronic</span> & optical behavior of the Low Dimensional Semiconductor Systems (LDSS). Application of hydrostatic pressure P>35kbar drastically alters the <span class="hlt">band</span> offsets leading to the crossover of Γ <span class="hlt">band</span> of the well & X <span class="hlt">band</span> of the barrier resulting in an indirect transition of the carrier and this effect has been studied experimentally and theoretically in a QW structure. In this paper, we have investigated the effect of Γ-X <span class="hlt">band</span> mixing due to the application of hydrostatic pressure in a GaAs/AlxGa1-xAs QWW system. The results are presented and discussed for various widths of the wire.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JaJAP..57fKA05Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JaJAP..57fKA05Y"><span><span class="hlt">Energy</span> <span class="hlt">band</span> structure and electrical properties of Ga-oxide/GaN interface formed by remote oxygen plasma</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yamamoto, Taishi; Taoka, Noriyuki; Ohta, Akio; Truyen, Nguyen Xuan; Yamada, Hisashi; Takahashi, Tokio; Ikeda, Mitsuhisa; Makihara, Katsunori; Nakatsuka, Osamu; Shimizu, Mitsuaki; Miyazaki, Seiichi</p> <p>2018-06-01</p> <p>The <span class="hlt">energy</span> <span class="hlt">band</span> structure of a Ga-oxide/GaN structure formed by remote oxygen plasma exposure and the electrical interface properties of the GaN metal–oxide–semiconductor (MOS) capacitors with the SiO2/Ga-oxide/GaN structures with postdeposition annealing (PDA) at various temperatures have been investigated. Reflection high-<span class="hlt">energy</span> <span class="hlt">electron</span> diffraction and X-ray photoelectron spectroscopy clarified that the formed Ga-oxide layer is neither a single nor polycrystalline phase with high crystallinity. We found that the <span class="hlt">energy</span> <span class="hlt">band</span> offsets at the conduction <span class="hlt">band</span> minimum and at the valence <span class="hlt">band</span> maximum between the Ga-oxide layer and the GaN surface were 0.4 and 1.2 ± 0.2 eV, respectively. Furthermore, capacitance–voltage (C–V) characteristics revealed that the interface trap density (D it) is lower than the evaluation limit of Terman method without depending on the PDA temperatures, and that the SiO2/Ga-oxide stack can work as a protection layer to maintain the low D it, avoiding the significant decomposition of GaN at the high PDA temperature of 800 °C.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22596765-combined-analysis-energy-band-diagram-equivalent-circuit-nanocrystal-solid','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22596765-combined-analysis-energy-band-diagram-equivalent-circuit-nanocrystal-solid"><span>Combined analysis of <span class="hlt">energy</span> <span class="hlt">band</span> diagram and equivalent circuit on nanocrystal solid</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Kano, Shinya, E-mail: kano@eedept.kobe-u.ac.jp, E-mail: fujii@eedept.kobe-u.ac.jp; Sasaki, Masato; Fujii, Minoru, E-mail: kano@eedept.kobe-u.ac.jp, E-mail: fujii@eedept.kobe-u.ac.jp</p> <p></p> <p>We investigate a combined analysis of an <span class="hlt">energy</span> <span class="hlt">band</span> diagram and an equivalent circuit on nanocrystal (NC) solids. We prepared a flat silicon-NC solid in order to carry out the analysis. An <span class="hlt">energy</span> <span class="hlt">band</span> diagram of a NC solid is determined from DC transport properties. Current-voltage characteristics, photocurrent measurements, and conductive atomic force microscopy images indicate that a tunneling transport through a NC solid is dominant. Impedance spectroscopy gives an equivalent circuit: a series of parallel resistor-capacitors corresponding to NC/metal and NC/NC interfaces. The equivalent circuit also provides an evidence that the NC/NC interface mainly dominates the carrier transport throughmore » NC solids. Tunneling barriers inside a NC solid can be taken into account in a combined capacitance. Evaluated circuit parameters coincide with simple geometrical models of capacitances. As a result, impedance spectroscopy is also a useful technique to analyze semiconductor NC solids as well as usual DC transport. The analyses provide indispensable information to implement NC solids into actual <span class="hlt">electronic</span> devices.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22596886-electron-band-bending-polar-semipolar-non-polar-gan-surfaces','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22596886-electron-band-bending-polar-semipolar-non-polar-gan-surfaces"><span><span class="hlt">Electron</span> <span class="hlt">band</span> bending of polar, semipolar and non-polar GaN surfaces</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Bartoš, I.; Romanyuk, O., E-mail: romanyuk@fzu.cz; Houdkova, J.</p> <p>2016-03-14</p> <p>The magnitudes of the surface <span class="hlt">band</span> bending have been determined by X-ray photoelectron spectroscopy for polar, semipolar, and non-polar surfaces of wurtzite GaN crystals. All surfaces have been prepared from crystalline GaN samples grown by the hydride-vapour phase epitaxy and separated from sapphire substrates. The Ga 3d core level peak shifts have been used for <span class="hlt">band</span> bending determination. Small <span class="hlt">band</span> bending magnitudes and also relatively small difference between the <span class="hlt">band</span> bendings of the surfaces with opposite polarity have been found. These results point to the presence of <span class="hlt">electron</span> surface states of different amounts and types on surfaces of different polaritymore » and confirm the important role of the <span class="hlt">electron</span> surface states in compensation of the bound surface polarity charges in wurtzite GaN crystals.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22591665-modification-electronic-properties-graphene-using-low-energy-sup-ions','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22591665-modification-electronic-properties-graphene-using-low-energy-sup-ions"><span>Modification of <span class="hlt">electronic</span> properties of graphene by using low-<span class="hlt">energy</span> K{sup +} ions</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Kim, Jingul; Lee, Paengro; Ryu, Mintae</p> <p>2016-05-02</p> <p>Despite its superb <span class="hlt">electronic</span> properties, the semi-metallic nature of graphene with no <span class="hlt">band</span> gap (E{sub g}) at the Dirac point has been a stumbling block for its industrial application. We report an improved means of producing a tunable <span class="hlt">band</span> gap over other schemes by doping low <span class="hlt">energy</span> (10 eV) potassium ions (K{sup +}) on single layer graphene formed on 6H-SiC(0001) surface, where the noble Dirac nature of the π-<span class="hlt">band</span> remains almost unaltered. The changes in the π-<span class="hlt">band</span> induced by K{sup +} ions reveal that the <span class="hlt">band</span> gap increases gradually with increasing dose (θ) of the ions up to E{sub g} = 0.65 eV atmore » θ = 1.10 monolayers, demonstrating the tunable character of the <span class="hlt">band</span> gap. Our core level data for C 1s, Si 2p, and K 2p suggest that the K{sup +}-induced asymmetry in charge distribution among carbon atoms drives the opening of <span class="hlt">band</span> gap, which is in sharp contrast with no <span class="hlt">band</span> gap when neutral K atoms are adsorbed on graphene. This tunable K{sup +}-induced <span class="hlt">band</span> gap in graphene illustrates its potential application in graphene-based nano-<span class="hlt">electronics</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23556883','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23556883"><span>Feasibility of producing a short, high <span class="hlt">energy</span> s-<span class="hlt">band</span> linear accelerator using a klystron power source.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Baillie, Devin; St Aubin, J; Fallone, B G; Steciw, S</p> <p>2013-04-01</p> <p>To use a finite-element method (FEM) model to study the feasibility of producing a short s-<span class="hlt">band</span> (2.9985 GHz) waveguide capable of producing x-rays <span class="hlt">energies</span> up to 10 MV, for applications in a linac-MR, as well as conventional radiotherapy. An existing waveguide FEM model developed by the authors' group is used to simulate replacing the magnetron power source with a klystron. Peak fields within the waveguide are compared with a published experimental threshold for electric breakdown. The RF fields in the first accelerating cavity are scaled, approximating the effect of modifications to the first coupling cavity. <span class="hlt">Electron</span> trajectories are calculated within the RF fields, and the <span class="hlt">energy</span> spectrum, beam current, and focal spot of the <span class="hlt">electron</span> beam are analyzed. One <span class="hlt">electron</span> spectrum is selected for Monte Carlo simulations and the resulting PDD compared to measurement. When the first cavity fields are scaled by a factor of 0.475, the peak magnitude of the electric fields within the waveguide are calculated to be 223.1 MV∕m, 29% lower than the published threshold for breakdown at this operating frequency. Maximum <span class="hlt">electron</span> <span class="hlt">energy</span> increased from 6.2 to 10.4 MeV, and beam current increased from 134 to 170 mA. The focal spot FWHM is decreased slightly from 0.07 to 0.05 mm, and the width of the <span class="hlt">energy</span> spectrum increased slightly from 0.44 to 0.70 MeV. Monte Carlo results show dmax is at 2.15 cm for a 10 × 10 cm(2) field, compared with 2.3 cm for a Varian 10 MV linac, while the penumbral widths are 4.8 and 5.6 mm, respectively. The authors' simulation results show that a short, high-<span class="hlt">energy</span>, s-<span class="hlt">band</span> accelerator is feasible and electric breakdown is not expected to interfere with operation at these field strengths. With minor modifications to the first coupling cavity, all <span class="hlt">electron</span> beam parameters are improved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22598850-electron-phonon-relaxation-excited-electron-distribution-gallium-nitride','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22598850-electron-phonon-relaxation-excited-electron-distribution-gallium-nitride"><span><span class="hlt">Electron</span>-phonon relaxation and excited <span class="hlt">electron</span> distribution in gallium nitride</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Zhukov, V. P.; Donostia International Physics Center; Tyuterev, V. G., E-mail: valtyut00@mail.ru</p> <p>2016-08-28</p> <p>We develop a theory of <span class="hlt">energy</span> relaxation in semiconductors and insulators highly excited by the long-acting external irradiation. We derive the equation for the non-equilibrium distribution function of excited <span class="hlt">electrons</span>. The solution for this function breaks up into the sum of two contributions. The low-<span class="hlt">energy</span> contribution is concentrated in a narrow range near the bottom of the conduction <span class="hlt">band</span>. It has the typical form of a Fermi distribution with an effective temperature and chemical potential. The effective temperature and chemical potential in this low-<span class="hlt">energy</span> term are determined by the intensity of carriers' generation, the speed of <span class="hlt">electron</span>-phonon relaxation, rates ofmore » inter-<span class="hlt">band</span> recombination, and <span class="hlt">electron</span> capture on the defects. In addition, there is a substantial high-<span class="hlt">energy</span> correction. This high-<span class="hlt">energy</span> “tail” largely covers the conduction <span class="hlt">band</span>. The shape of the high-<span class="hlt">energy</span> “tail” strongly depends on the rate of <span class="hlt">electron</span>-phonon relaxation but does not depend on the rates of recombination and trapping. We apply the theory to the calculation of a non-equilibrium distribution of <span class="hlt">electrons</span> in an irradiated GaN. Probabilities of optical excitations from the valence to conduction <span class="hlt">band</span> and <span class="hlt">electron</span>-phonon coupling probabilities in GaN were calculated by the density functional perturbation theory. Our calculation of both parts of distribution function in gallium nitride shows that when the speed of the <span class="hlt">electron</span>-phonon scattering is comparable with the rate of recombination and trapping then the contribution of the non-Fermi “tail” is comparable with that of the low-<span class="hlt">energy</span> Fermi-like component. So the high-<span class="hlt">energy</span> contribution can essentially affect the charge transport in the irradiated and highly doped semiconductors.« less</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li class="active"><span>7</span></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_7 --> <div id="page_8" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="141"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JMMM..439..203H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JMMM..439..203H"><span>Spin- and valley-dependent <span class="hlt">electronic</span> <span class="hlt">band</span> structure and <span class="hlt">electronic</span> heat capacity of ferromagnetic silicene in the presence of strain, exchange field and Rashba spin-orbit coupling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hoi, Bui Dinh; Yarmohammadi, Mohsen; Kazzaz, Houshang Araghi</p> <p>2017-10-01</p> <p>We studied how the strain, induced exchange field and extrinsic Rashba spin-orbit coupling (RSOC) enhance the <span class="hlt">electronic</span> <span class="hlt">band</span> structure (EBS) and <span class="hlt">electronic</span> heat capacity (EHC) of ferromagnetic silicene in presence of external electric field (EF) by using the Kane-Mele Hamiltonian, Dirac cone approximation and the Green's function approach. Particular attention is paid to investigate the EHC of spin-up and spin-down <span class="hlt">bands</span> at Dirac K and K‧ points. We have varied the EF, strain, exchange field and RSOC to tune the <span class="hlt">energy</span> of inter-<span class="hlt">band</span> transitions and consequently EHC, leading to very promising features for future applications. Evaluation of EF exhibits three phases: Topological insulator (TI), valley-spin polarized metal (VSPM) and <span class="hlt">band</span> insulator (BI) at given aforementioned parameters. As a new finding, we have found a quantum anomalous Hall phase in BI regime at strong RSOCs. Interestingly, the effective mass of carriers changes with strain, resulting in EHC behaviors. Here, exchange field has the same behavior with EF. Finally, we have confirmed the reported and expected symmetry results for both Dirac points and spins with the study of valley-dependent EHC.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MS%26E..254g2002A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MS%26E..254g2002A"><span>Design of an <span class="hlt">Electronic</span> Chest-<span class="hlt">Band</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Atakan, R.; Acikgoz Tufan, H.; Baskan, H.; Eryuruk, S. H.; Akalin, N.; Kose, H.; Li, Y.; Kursun Bahadir, S.; Kalaoglu, F.</p> <p>2017-10-01</p> <p>In this study, an <span class="hlt">electronic</span> chest strap prototype was designed for measuring fitness level, performance optimization, mobility and fall detection. Knitting technology is used for production by using highly elastic nylon yarn. In order to evaluate comfort performance of the garment, yarn strength and elongation, air permeability, moisture management and FAST tests (Fabric Assurance Fabric Testing) were carried out, respectively. After testing of textile part of the chest <span class="hlt">band</span>, IMU sensors were integrated onto the garment by means of conductive yarns. Electrical conductivity of the circuit was also assessed at the end. Results indicated that the weight and the thickness of the product are relatively high for sports uses and it has a negative impact on comfort properties. However, it is highly stretchable and moisture management properties are still in acceptable values. From the perspective of possible application areas, developed smart chest <span class="hlt">band</span> in this research could be used in sports facilities as well as health care applications for elderly and disabled people.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PhRvP...4e4012Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PhRvP...4e4012Y"><span><span class="hlt">Band</span>-Gap and <span class="hlt">Band</span>-Edge Engineering of Multicomponent Garnet Scintillators from First Principles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yadav, Satyesh K.; Uberuaga, Blas P.; Nikl, Martin; Jiang, Chao; Stanek, Christopher R.</p> <p>2015-11-01</p> <p>Complex doping schemes in R3 Al5 O12 (where R is the rare-earth element) garnet compounds have recently led to pronounced improvements in scintillator performance. Specifically, by admixing lutetium and yttrium aluminate garnets with gallium and gadolinium, the <span class="hlt">band</span> gap is altered in a manner that facilitates the removal of deleterious <span class="hlt">electron</span> trapping associated with cation antisite defects. Here, we expand upon this initial work to systematically investigate the effect of substitutional admixing on the <span class="hlt">energy</span> levels of <span class="hlt">band</span> edges. Density-functional theory and hybrid density-functional theory (HDFT) are used to survey potential admixing candidates that modify either the conduction-<span class="hlt">band</span> minimum (CBM) or valence-<span class="hlt">band</span> maximum (VBM). We consider two sets of compositions based on Lu3 B5O12 where B is Al, Ga, In, As, and Sb, and R3Al5 O12 , where R is Lu, Gd, Dy, and Er. We find that admixing with various R cations does not appreciably affect the <span class="hlt">band</span> gap or <span class="hlt">band</span> edges. In contrast, substituting Al with cations of dissimilar ionic radii has a profound impact on the <span class="hlt">band</span> structure. We further show that certain dopants can be used to selectively modify only the CBM or the VBM. Specifically, Ga and In decrease the <span class="hlt">band</span> gap by lowering the CBM, while As and Sb decrease the <span class="hlt">band</span> gap by raising the VBM, the relative change in <span class="hlt">band</span> gap is quantitatively validated by HDFT. These results demonstrate a powerful approach to quickly screen the impact of dopants on the <span class="hlt">electronic</span> structure of scintillator compounds, identifying those dopants which alter the <span class="hlt">band</span> edges in very specific ways to eliminate both <span class="hlt">electron</span> and hole traps responsible for performance limitations. This approach should be broadly applicable for the optimization of <span class="hlt">electronic</span> and optical performance for a wide range of compounds by tuning the VBM and CBM.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29111653','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29111653"><span>Surface State Density Determines the <span class="hlt">Energy</span> Level Alignment at Hybrid Perovskite/<span class="hlt">Electron</span> Acceptors Interfaces.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zu, Fengshuo; Amsalem, Patrick; Ralaiarisoa, Maryline; Schultz, Thorsten; Schlesinger, Raphael; Koch, Norbert</p> <p>2017-11-29</p> <p>Substantial variations in the <span class="hlt">electronic</span> structure and thus possibly conflicting energetics at interfaces between hybrid perovskites and charge transport layers in solar cells have been reported by the research community. In an attempt to unravel the origin of these variations and enable reliable device design, we demonstrate that donor-like surface states stemming from reduced lead (Pb 0 ) directly impact the <span class="hlt">energy</span> level alignment at perovskite (CH 3 NH 3 PbI 3-x Cl x ) and molecular <span class="hlt">electron</span> acceptor layer interfaces using photoelectron spectroscopy. When forming the interfaces, it is found that <span class="hlt">electron</span> transfer from surface states to acceptor molecules occurs, leading to a strong decrease in the density of ionized surface states. As a consequence, for perovskite samples with low surface state density, the initial <span class="hlt">band</span> bending at the pristine perovskite surface can be flattened upon interface formation. In contrast, for perovskites with a high surface state density, the Fermi level is strongly pinned at the conduction <span class="hlt">band</span> edge, and only minor changes in surface <span class="hlt">band</span> bending are observed upon acceptor deposition. Consequently, depending on the initial perovskite surface state density, very different interface <span class="hlt">energy</span> level alignment situations (variations over 0.5 eV) are demonstrated and rationalized. Our findings help explain the rather dissimilar reported <span class="hlt">energy</span> levels at interfaces with perovskites, refining our understanding of the operating principles in devices comprising this material.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008PhRvB..78o5410G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008PhRvB..78o5410G"><span>Nonadiabatic dynamics of <span class="hlt">electron</span> scattering from adsorbates in surface <span class="hlt">bands</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gumhalter, Branko; Šiber, Antonio; Buljan, Hrvoje; Fauster, Thomas</p> <p>2008-10-01</p> <p>We present a comparative study of nonadiabatic dynamics of <span class="hlt">electron</span> scattering in quasi-two-dimensional surface <span class="hlt">band</span> which is induced by the long-range component of the interactions with a random array of adsorbates. Using three complementary model descriptions of intraband spatiotemporal propagation of quasiparticles that go beyond the single-adsorbate scattering approach we are able to identify distinct subsequent regimes of evolution of an <span class="hlt">electron</span> following its promotion into an unoccupied <span class="hlt">band</span> state: (i) early quadratic or ballistic decay of the initial-state survival probability within the Heisenberg uncertainty window, (ii) preasymptotic exponential decay governed by the self-consistent Fermi golden rule scattering rate, and (iii) asymptotic decay described by a combined inverse power-law and logarithmic behavior. The developed models are applied to discuss the dynamics of intraband adsorbate-induced scattering of hot <span class="hlt">electrons</span> excited into the n=1 image-potential <span class="hlt">band</span> on Cu(100) surface during the first stage of a two-photon photoemission process. Estimates of crossovers between the distinct evolution regimes enable assessments of the lifespan of a standard quasiparticle behavior and thereby of the range of applicability of the widely used Fermi golden rule and optical Bloch equations approach for description of adsorbate-induced quasiparticle decay and dephasing in ultrafast experiments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5812109','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5812109"><span>Bi-diketopyrrolopyrrole (Bi-DPP) as a novel <span class="hlt">electron</span> accepting compound in low <span class="hlt">band</span> gap π-conjugated donor–acceptor copolymers/oligomers</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ahner, Johannes; Nowotny, Jürgen; Schubert, Ulrich S.; Hager, Martin D.</p> <p>2017-01-01</p> <p>Abstract The synthesis and characterization of a novel 2,5-diketopyrrolo[3,4-c]pyrrole(DPP)-based accepting building block with the scheme DPP-neutral small linker-DPP (Bi-DPP) is presented, which was utilized as <span class="hlt">electron</span> accepting moiety for low <span class="hlt">band</span> gap π-conjugated donor–acceptor copolymers as well as for a donor–acceptor small molecule. The <span class="hlt">electron</span> accepting moiety Bi-DPP was prepared via a novel synthetic pathway by building up two DPP moieties step by step simultaneously starting from a neutral phenyl core unit. Characterization of the synthesized oligomeric and polymeric materials via cyclic voltammetry afford LUMO <span class="hlt">energy</span> levels from −3.49 to −3.59 eV as well as HOMO <span class="hlt">energy</span> levels from −5.07 to −5.34 eV resulting in low <span class="hlt">energy</span> <span class="hlt">band</span> gaps from 1.52 to 1.81 eV. Spin coating of the prepared donor–acceptor oligomers/polymers resulted in well-defined films. Moreover, UV–vis measurements of the investigated donor–acceptor systems showed a broad absorption over the whole visible region. It is demonstrated that Bi-DPP as an <span class="hlt">electron</span> accepting moiety in donor–acceptor systems offer potential properties for organic solar cell devices. PMID:29491794</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhRvS..20j4701J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvS..20j4701J"><span>Design of an X -<span class="hlt">band</span> <span class="hlt">electron</span> linear accelerator dedicated to decentralized 99Mo/99mTc supply: From beam <span class="hlt">energy</span> selection to yield estimation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jang, Jaewoong; Yamamoto, Masashi; Uesaka, Mitsuru</p> <p>2017-10-01</p> <p>The most frequently used radionuclide in diagnostic nuclear medicine, 99mTc, is generally obtained by the decay of its parent radionuclide, 99Mo. Recently, concerns have been raised over shortages of 99Mo/99mTc, owing to aging of the research reactors which have been supplying practically all of the global demand for 99Mo in a centralized fashion. In an effort to prevent such 99Mo/99mTc supply disruption and, furthermore, to ameliorate the underlying instability of the centralized 99Mo/99mTc supply chain, we designed an X -<span class="hlt">band</span> <span class="hlt">electron</span> linear accelerator which can be distributed over multiple regions, whereby 99Mo/99mTc can be supplied with improved accessibility. The <span class="hlt">electron</span> beam <span class="hlt">energy</span> was designed to be 35 MeV, at which an average beam power of 9.1 kW was calculated by the following beam dynamics analysis. Subsequent radioactivity modeling suggests that 11 of the designed <span class="hlt">electron</span> linear accelerators can realize self-sufficiency of 99Mo/99mTc in Japan.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ApPhL.112d2108Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ApPhL.112d2108Z"><span><span class="hlt">Band</span> offset and <span class="hlt">electron</span> affinity of MBE-grown SnSe2</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Qin; Li, Mingda Oscar; Lochocki, Edward B.; Vishwanath, Suresh; Liu, Xinyu; Yan, Rusen; Lien, Huai-Hsun; Dobrowolska, Malgorzata; Furdyna, Jacek; Shen, Kyle M.; Cheng, Guangjun; Hight Walker, Angela R.; Gundlach, David J.; Xing, Huili G.; Nguyen, N. V.</p> <p>2018-01-01</p> <p>SnSe2 is currently considered a potential two-dimensional material that can form a near-broken gap heterojunction in a tunnel field-effect transistor due to its large <span class="hlt">electron</span> affinity which is experimentally confirmed in this letter. With the results from internal photoemission and angle-resolved photoemission spectroscopy performed on Al/Al2O3/SnSe2/GaAs and SnSe2/GaAs test structures where SnSe2 is grown on GaAs by molecular beam epitaxy, we ascertain a (5.2 ± 0.1) eV <span class="hlt">electron</span> affinity of SnSe2. The <span class="hlt">band</span> offset from the SnSe2 Fermi level to the Al2O3 conduction <span class="hlt">band</span> minimum is found to be (3.3 ± 0.05) eV and SnSe2 is seen to have a high level of intrinsic <span class="hlt">electron</span> (n-type) doping with the Fermi level positioned at about 0.2 eV above its conduction <span class="hlt">band</span> minimum. It is concluded that the <span class="hlt">electron</span> affinity of SnSe2 is larger than that of most semiconductors and can be combined with other appropriate semiconductors to form near broken-gap heterojunctions for the tunnel field-effect transistor that can potentially achieve high on-currents.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28265085','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28265085"><span>Understanding <span class="hlt">band</span> gaps of solids in generalized Kohn-Sham theory.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Perdew, John P; Yang, Weitao; Burke, Kieron; Yang, Zenghui; Gross, Eberhard K U; Scheffler, Matthias; Scuseria, Gustavo E; Henderson, Thomas M; Zhang, Igor Ying; Ruzsinszky, Adrienn; Peng, Haowei; Sun, Jianwei; Trushin, Egor; Görling, Andreas</p> <p>2017-03-14</p> <p>The fundamental <span class="hlt">energy</span> gap of a periodic solid distinguishes insulators from metals and characterizes low-<span class="hlt">energy</span> single-<span class="hlt">electron</span> excitations. However, the gap in the <span class="hlt">band</span> structure of the exact multiplicative Kohn-Sham (KS) potential substantially underestimates the fundamental gap, a major limitation of KS density-functional theory. Here, we give a simple proof of a theorem: In generalized KS theory (GKS), the <span class="hlt">band</span> gap of an extended system equals the fundamental gap for the approximate functional if the GKS potential operator is continuous and the density change is delocalized when an <span class="hlt">electron</span> or hole is added. Our theorem explains how GKS <span class="hlt">band</span> gaps from metageneralized gradient approximations (meta-GGAs) and hybrid functionals can be more realistic than those from GGAs or even from the exact KS potential. The theorem also follows from earlier work. The <span class="hlt">band</span> edges in the GKS one-<span class="hlt">electron</span> spectrum are also related to measurable <span class="hlt">energies</span>. A linear chain of hydrogen molecules, solid aluminum arsenide, and solid argon provide numerical illustrations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5358356','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5358356"><span>Understanding <span class="hlt">band</span> gaps of solids in generalized Kohn–Sham theory</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Perdew, John P.; Yang, Weitao; Burke, Kieron; Yang, Zenghui; Gross, Eberhard K. U.; Scheffler, Matthias; Scuseria, Gustavo E.; Henderson, Thomas M.; Zhang, Igor Ying; Ruzsinszky, Adrienn; Peng, Haowei; Sun, Jianwei; Trushin, Egor; Görling, Andreas</p> <p>2017-01-01</p> <p>The fundamental <span class="hlt">energy</span> gap of a periodic solid distinguishes insulators from metals and characterizes low-<span class="hlt">energy</span> single-<span class="hlt">electron</span> excitations. However, the gap in the <span class="hlt">band</span> structure of the exact multiplicative Kohn–Sham (KS) potential substantially underestimates the fundamental gap, a major limitation of KS density-functional theory. Here, we give a simple proof of a theorem: In generalized KS theory (GKS), the <span class="hlt">band</span> gap of an extended system equals the fundamental gap for the approximate functional if the GKS potential operator is continuous and the density change is delocalized when an <span class="hlt">electron</span> or hole is added. Our theorem explains how GKS <span class="hlt">band</span> gaps from metageneralized gradient approximations (meta-GGAs) and hybrid functionals can be more realistic than those from GGAs or even from the exact KS potential. The theorem also follows from earlier work. The <span class="hlt">band</span> edges in the GKS one-<span class="hlt">electron</span> spectrum are also related to measurable <span class="hlt">energies</span>. A linear chain of hydrogen molecules, solid aluminum arsenide, and solid argon provide numerical illustrations. PMID:28265085</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhRvB..96o5439K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvB..96o5439K"><span>Quasiparticle <span class="hlt">energy</span> <span class="hlt">bands</span> and Fermi surfaces of monolayer NbSe2</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kim, Sejoong; Son, Young-Woo</p> <p>2017-10-01</p> <p>A quasiparticle <span class="hlt">band</span> structure of a single layer 2 H -NbSe2 is reported by using first-principles G W calculation. We show that a self-<span class="hlt">energy</span> correction increases the width of a partially occupied <span class="hlt">band</span> and alters its Fermi surface shape when comparing those using conventional mean-field calculation methods. Owing to a broken inversion symmetry in the trigonal prismatic single layer structure, the spin-orbit interaction is included and its impact on the Fermi surface and quasiparticle <span class="hlt">energy</span> <span class="hlt">bands</span> are discussed. We also calculate the doping dependent static susceptibilities from the <span class="hlt">band</span> structures obtained by the mean-field calculation as well as G W calculation with and without spin-orbit interactions. A complete tight-binding model is constructed within the three-<span class="hlt">band</span> third nearest neighbor hoppings and is shown to reproduce our G W quasiparticle <span class="hlt">energy</span> <span class="hlt">bands</span> and Fermi surface very well. Considering variations of the Fermi surface shapes depending on self-<span class="hlt">energy</span> corrections and spin-orbit interactions, we discuss the formations of charge density wave (CDW) with different dielectric environments and their implications on recent controversial experimental results on CDW transition temperatures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27364116','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27364116"><span><span class="hlt">Band</span>-like transport in highly crystalline graphene films from defective graphene oxides.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Negishi, R; Akabori, M; Ito, T; Watanabe, Y; Kobayashi, Y</p> <p>2016-07-01</p> <p>The electrical transport property of the reduced graphene oxide (rGO) thin-films synthesized from defective GO through thermal treatment in a reactive ethanol environment at high temperature above 1000 °C shows a <span class="hlt">band</span>-like transport with small thermal activation <span class="hlt">energy</span> (Ea~10 meV) that occurs during high carrier mobility (~210 cm(2)/Vs). Electrical and structural analysis using X-ray absorption fine structure, the valence <span class="hlt">band</span> photo-<span class="hlt">electron</span>, Raman spectra and transmission <span class="hlt">electron</span> microscopy indicate that a high temperature process above 1000 °C in the ethanol environment leads to an extraordinary expansion of the conjugated π-<span class="hlt">electron</span> system in rGO due to the efficient restoration of the graphitic structure. We reveal that Ea decreases with the increasing density of states near the Fermi level due to the expansion of the conjugated π-<span class="hlt">electron</span> system in the rGO. This means that Ea corresponds to the <span class="hlt">energy</span> gap between the top of the valence <span class="hlt">band</span> and the bottom of the conduction <span class="hlt">band</span>. The origin of the <span class="hlt">band</span>-like transport can be explained by the carriers, which are more easily excited into the conduction <span class="hlt">band</span> due to the decreasing <span class="hlt">energy</span> gap with the expansion of the conjugated π-<span class="hlt">electron</span> system in the rGO.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016NatSR...628936N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016NatSR...628936N"><span><span class="hlt">Band</span>-like transport in highly crystalline graphene films from defective graphene oxides</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Negishi, R.; Akabori, M.; Ito, T.; Watanabe, Y.; Kobayashi, Y.</p> <p>2016-07-01</p> <p>The electrical transport property of the reduced graphene oxide (rGO) thin-films synthesized from defective GO through thermal treatment in a reactive ethanol environment at high temperature above 1000 °C shows a <span class="hlt">band</span>-like transport with small thermal activation <span class="hlt">energy</span> (Ea~10 meV) that occurs during high carrier mobility (~210 cm2/Vs). Electrical and structural analysis using X-ray absorption fine structure, the valence <span class="hlt">band</span> photo-<span class="hlt">electron</span>, Raman spectra and transmission <span class="hlt">electron</span> microscopy indicate that a high temperature process above 1000 °C in the ethanol environment leads to an extraordinary expansion of the conjugated π-<span class="hlt">electron</span> system in rGO due to the efficient restoration of the graphitic structure. We reveal that Ea decreases with the increasing density of states near the Fermi level due to the expansion of the conjugated π-<span class="hlt">electron</span> system in the rGO. This means that Ea corresponds to the <span class="hlt">energy</span> gap between the top of the valence <span class="hlt">band</span> and the bottom of the conduction <span class="hlt">band</span>. The origin of the <span class="hlt">band</span>-like transport can be explained by the carriers, which are more easily excited into the conduction <span class="hlt">band</span> due to the decreasing <span class="hlt">energy</span> gap with the expansion of the conjugated π-<span class="hlt">electron</span> system in the rGO.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1999PhRvB..5910119X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1999PhRvB..5910119X"><span><span class="hlt">Energy</span> <span class="hlt">bands</span> and acceptor binding <span class="hlt">energies</span> of GaN</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xia, Jian-Bai; Cheah, K. W.; Wang, Xiao-Liang; Sun, Dian-Zhao; Kong, Mei-Ying</p> <p>1999-04-01</p> <p>The <span class="hlt">energy</span> <span class="hlt">bands</span> of zinc-blende and wurtzite GaN are calculated with the empirical pseudopotential method, and the pseudopotential parameters for Ga and N atoms are given. The calculated <span class="hlt">energy</span> <span class="hlt">bands</span> are in agreement with those obtained by the ab initio method. The effective-mass theory for the semiconductors of wurtzite structure is established, and the effective-mass parameters of GaN for both structures are given. The binding <span class="hlt">energies</span> of acceptor states are calculated by solving strictly the effective-mass equations. The binding <span class="hlt">energies</span> of donor and acceptor are 24 and 142 meV for the zinc-blende structure, 20 and 131, and 97 meV for the wurtzite structure, respectively, which are consistent with recent experimental results. It is proposed that there are two kinds of acceptor in wurtzite GaN. One kind is the general acceptor such as C, which substitutes N, which satisfies the effective-mass theory. The other kind of acceptor includes Mg, Zn, Cd, etc., the binding <span class="hlt">energy</span> of these acceptors is deviated from that given by the effective-mass theory. In this report, wurtzite GaN is grown by the molecular-beam epitaxy method, and the photoluminescence spectra were measured. Three main peaks are assigned to the donor-acceptor transitions from two kinds of acceptors. Some of the transitions were identified as coming from the cubic phase of GaN, which appears randomly within the predominantly hexagonal material.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JAP...122q5102W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JAP...122q5102W"><span>Thermoelectric <span class="hlt">band</span> engineering: The role of carrier scattering</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Witkoske, Evan; Wang, Xufeng; Lundstrom, Mark; Askarpour, Vahid; Maassen, Jesse</p> <p>2017-11-01</p> <p>Complex <span class="hlt">electronic</span> <span class="hlt">band</span> structures, with multiple valleys or <span class="hlt">bands</span> at the same or similar <span class="hlt">energies</span>, can be beneficial for thermoelectric performance, but the advantages can be offset by inter-valley and inter-<span class="hlt">band</span> scattering. In this paper, we demonstrate how first-principles <span class="hlt">band</span> structures coupled with recently developed techniques for rigorous simulation of <span class="hlt">electron</span>-phonon scattering provide the capabilities to realistically assess the benefits and trade-offs associated with these materials. We illustrate the approach using n-type silicon as a model material and show that intervalley scattering is strong. This example shows that the convergence of valleys and <span class="hlt">bands</span> can improve thermoelectric performance, but the magnitude of the improvement depends sensitively on the relative strengths of intra- and inter-valley <span class="hlt">electron</span> scattering. Because anisotropy of the <span class="hlt">band</span> structure also plays an important role, a measure of the benefit of <span class="hlt">band</span> anisotropy in the presence of strong intervalley scattering is presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018REDS..173....8L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018REDS..173....8L"><span>Modelling relativistic effects in momentum-resolved <span class="hlt">electron</span> <span class="hlt">energy</span> loss spectroscopy of graphene</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lyon, K.; Mowbray, D. J.; Miskovic, Z. L.</p> <p>2018-02-01</p> <p>We present an analytical model for the <span class="hlt">electron</span> <span class="hlt">energy</span> loss through a two-dimensional (2D) layer of graphene, fully taking into account relativistic effects. Using two different models for graphene's 2D conductivity, one a two-fluid hydrodynamic model with an added correction to account for the inter-<span class="hlt">band</span> <span class="hlt">electron</span> transitions near the Dirac point in undoped graphene, the other derived from ab initio plane-wave time-dependent density functional theory in the frequency domain (PW-TDDFT-ω) calculations applied on a graphene superlattice, we derive various different expressions for the probability density of <span class="hlt">energy</span> and momentum transfer from the incident <span class="hlt">electron</span> to graphene. To further compare with <span class="hlt">electron</span> <span class="hlt">energy</span> loss spectroscopy (EELS) experiments that use setups like scanning Transmission <span class="hlt">Electron</span> Microscopy, we integrated our <span class="hlt">energy</span> loss functions over a range of wavenumbers, and compared how the choice of range directly affects the shape, position, and relative heights of graphene's π → π* and σ → σ* transition peaks. Comparisons were made with experimental EELS data under different model inputs, revealing again the strong effect that the choice of wavenumber range has on the <span class="hlt">energy</span> loss.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2000JChPh.113.5413M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2000JChPh.113.5413M"><span>Modeling the free <span class="hlt">energy</span> surfaces of <span class="hlt">electron</span> transfer in condensed phases</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Matyushov, Dmitry V.; Voth, Gregory A.</p> <p>2000-10-01</p> <p>We develop a three-parameter model of <span class="hlt">electron</span> transfer (ET) in condensed phases based on the Hamiltonian of a two-state solute linearly coupled to a harmonic, classical solvent mode with different force constants in the initial and final states (a classical limit of the quantum Kubo-Toyozawa model). The exact analytical solution for the ET free <span class="hlt">energy</span> surfaces demonstrates the following features: (i) the range of ET reaction coordinates is limited by a one-sided fluctuation <span class="hlt">band</span>, (ii) the ET free <span class="hlt">energies</span> are infinite outside the <span class="hlt">band</span>, and (iii) the free <span class="hlt">energy</span> surfaces are parabolic close to their minima and linear far from the minima positions. The model provides an analytical framework to map physical phenomena conflicting with the Marcus-Hush two-parameter model of ET. Nonlinear solvation, ET in polarizable charge-transfer complexes, and configurational flexibility of donor-acceptor complexes are successfully mapped onto the model. The present theory leads to a significant modification of the <span class="hlt">energy</span> gap law for ET reactions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1995ZPhyD..34..283O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1995ZPhyD..34..283O"><span>High-resolution <span class="hlt">electron</span> microscopy and <span class="hlt">electron</span> <span class="hlt">energy</span>-loss spectroscopy of giant palladium clusters</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Oleshko, V.; Volkov, V.; Gijbels, R.; Jacob, W.; Vargaftik, M.; Moiseev, I.; van Tendeloo, G.</p> <p>1995-12-01</p> <p>Combined structural and chemical characterization of cationic polynuclear palladium coordination compounds Pd561L60(OAc)180, where L=1,10-phenantroline or 2,2'-bipyridine has been carried out by high-resolution <span class="hlt">electron</span> microscopy (HREM) and analytical <span class="hlt">electron</span> microscopy methods including <span class="hlt">electron</span> <span class="hlt">energy</span>-loss spectroscopy (EELS), zero-loss <span class="hlt">electron</span> spectroscopic imaging, and <span class="hlt">energy</span>-dispersive X-ray spectroscopy (EDX). The cell structure of the cluster matter with almost completely uniform metal core size distributions centered around 2.3 ±0.5 nm was observed. Zero-loss <span class="hlt">energy</span> filtering allowed to improve the image contrast and resolution. HREM images showed that most of the palladium clusters had a cubo-octahedral shape. Some of them had a distorted icosahedron structure exhibiting multiple twinning. The selected-area <span class="hlt">electron</span> diffraction patterns confirmed the face centered cubic structure with lattice parameter close to that of metallic palladium. The <span class="hlt">energy</span>-loss spectra of the populations of clusters contained several <span class="hlt">bands</span>, which could be assigned to the delayed Pd M4, 5-edge at 362 eV, the Pd M3-edge at 533 eV and the Pd M2-edge at 561 eV, the NK-edge at about 400 eV, the O K-edge at 532 eV overlapping with the Pd M3-edge and the carbon C K-edge at 284 eV. Background subtraction was applied to reveal the exact positions and fine structure of low intensity elemental peaks. EELS evaluations have been confirmed by EDX. The recorded series of the Pd M-edges and the N K-edge in the spectra of the giant palladium clusters obviously were related to Pd-Pd- and Pd-ligand bonding.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22594579-electronic-band-structure-optical-gain-gan-sub-bi-sub-sub-gaas-pyramidal-quantum-dots','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22594579-electronic-band-structure-optical-gain-gan-sub-bi-sub-sub-gaas-pyramidal-quantum-dots"><span><span class="hlt">Electronic</span> <span class="hlt">band</span> structure and optical gain of GaN{sub x}Bi{sub y}As{sub 1−x−y}/GaAs pyramidal quantum dots</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Song, Zhi-Gang; State Key Laboratory of Superlattices and Microstructures, Institute of Semiconductors, Chinese Academy of Sciences, P.O. Box 912, Beijing 100083; Bose, Sumanta</p> <p></p> <p>The <span class="hlt">electronic</span> <span class="hlt">band</span> structure and optical gain of GaN{sub x}Bi{sub y}As{sub 1−x−y}/GaAs pyramidal quantum dots (QDs) are investigated using the 16-<span class="hlt">band</span> k ⋅ p model with constant strain. The optical gain is calculated taking both homogeneous and inhomogeneous broadenings into consideration. The effective <span class="hlt">band</span> gap falls as we increase the composition of nitrogen (N) and bismuth (Bi) and with an appropriate choice of composition we can tune the emission wavelength to span within 1.3 μm–1.55 μm, for device application in fiber technology. The extent of this red shift is more profound in QDs compared with bulk material due to quantum confinement. Othermore » factors affecting the emission characteristics include virtual crystal, strain profile, <span class="hlt">band</span> anticrossing (BAC), and valence <span class="hlt">band</span> anticrossing (VBAC). The strain profile has a profound impact on the <span class="hlt">electronic</span> structure, specially the valence <span class="hlt">band</span> of QDs, which can be determined using the composition distribution of wave functions. All these factors eventually affect the optical gain spectrum. With an increase in QD size, we observe a red shift in the emission <span class="hlt">energy</span> and emergence of secondary peaks owing to transitions or greater <span class="hlt">energy</span> compared with the fundamental transition.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1415428-generation-highly-oblique-lower-band-chorus-via-nonlinear-three-wave-resonance','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1415428-generation-highly-oblique-lower-band-chorus-via-nonlinear-three-wave-resonance"><span>Generation of Highly Oblique Lower <span class="hlt">Band</span> Chorus Via Nonlinear Three-Wave Resonance</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Fu, Xiangrong; Gary, Stephen Peter; Reeves, Geoffrey D.; ...</p> <p>2017-09-05</p> <p>Chorus in the inner magnetosphere has been observed frequently at geomagnetically active times, typically exhibiting a two-<span class="hlt">band</span> structure with a quasi-parallel lower <span class="hlt">band</span> and an upper <span class="hlt">band</span> with a broad range of wave normal angles. But recent observations by Van Allen Probes confirm another type of lower <span class="hlt">band</span> chorus, which has a large wave normal angle close to the resonance cone angle. It has been proposed that these waves could be generated by a low-<span class="hlt">energy</span> beam-like <span class="hlt">electron</span> component or by temperature anisotropy of keV <span class="hlt">electrons</span> in the presence of a low-<span class="hlt">energy</span> plateau-like <span class="hlt">electron</span> component. This paper, however, presents an alternativemore » mechanism for generation of this highly oblique lower <span class="hlt">band</span> chorus. Through a nonlinear three-wave resonance, a quasi-parallel lower <span class="hlt">band</span> chorus wave can interact with a mildly oblique upper <span class="hlt">band</span> chorus wave, producing a highly oblique quasi-electrostatic lower <span class="hlt">band</span> chorus wave. This theoretical analysis is confirmed by 2-D electromagnetic particle-in-cell simulations. Furthermore, as the newly generated waves propagate away from the equator, their wave normal angle can further increase and they are able to scatter low-<span class="hlt">energy</span> <span class="hlt">electrons</span> to form a plateau-like structure in the parallel velocity distribution. As a result, the three-wave resonance mechanism may also explain the generation of quasi-parallel upper <span class="hlt">band</span> chorus which has also been observed in the magnetosphere.« less</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_8 --> <div id="page_9" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="161"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EL....11448001S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EL....11448001S"><span><span class="hlt">Energy</span> <span class="hlt">band</span> gaps in graphene nanoribbons with corners</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Szczȩśniak, Dominik; Durajski, Artur P.; Khater, Antoine; Ghader, Doried</p> <p>2016-05-01</p> <p>In the present paper, we study the relation between the <span class="hlt">band</span> gap size and the corner-corner length in representative chevron-shaped graphene nanoribbons (CGNRs) with 120° and 150° corner edges. The direct physical insight into the <span class="hlt">electronic</span> properties of CGNRs is provided within the tight-binding model with phenomenological edge parameters, developed against recent first-principle results. We show that the analyzed CGNRs exhibit inverse relation between their <span class="hlt">band</span> gaps and corner-corner lengths, and that they do not present a metal-insulator transition when the chemical edge modifications are introduced. Our results also suggest that the <span class="hlt">band</span> gap width for the CGNRs is predominantly governed by the armchair edge effects, and is tunable through edge modifications with foreign atoms dressing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19830042912&hterms=1084&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3D%2526%25231084','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19830042912&hterms=1084&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3D%2526%25231084"><span>EUV studies of N2 and O2 produced by low <span class="hlt">energy</span> <span class="hlt">electron</span> impact</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Morgan, H. D.; Mentall, J. E.</p> <p>1983-01-01</p> <p>The emission spectra resulting from <span class="hlt">electron</span> impact excitation on molecular nitrogen and oxygen in the 500-1200 A spectral region are investigated. <span class="hlt">Electron</span> <span class="hlt">energies</span> are from 0 to 300 eV. Numerous <span class="hlt">bands</span> of N2 are found between 800 and 1000 A. Excitation functions are measured for the NII 916 A, the OI 879 A, and the OII 834 multiplets, and nitrogen <span class="hlt">band</span> emission. Cross sections were measured at 200 eV for several of the <span class="hlt">band</span> emissions plus the NI 1135 A, NI 1164 A, NI 1177 A, NII 776 A, NII 1084 A, OI 1152 A, OI 1041 A, OI 999 A, OI 989 A, OI 879 A, OII 834 A, OII 616 A, OII 555 A, OII 539 A, and OII 718 A multiplets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ApPhL.111u3502K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ApPhL.111u3502K"><span>A tapered multi-gap multi-aperture pseudospark-sourced <span class="hlt">electron</span> gun based X-<span class="hlt">band</span> slow wave oscillator</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kumar, N.; Lamba, R. P.; Hossain, A. M.; Pal, U. N.; Phelps, A. D. R.; Prakash, R.</p> <p>2017-11-01</p> <p>The experimental study of a tapered, multi-gap, multi-aperture pseudospark-sourced <span class="hlt">electron</span> gun based X-<span class="hlt">band</span> plasma assisted slow wave oscillator is presented. The designed <span class="hlt">electron</span> gun is based on the pseudospark discharge concept and has been used to generate a high current density and high <span class="hlt">energy</span> <span class="hlt">electron</span> beam simultaneously. The distribution of apertures has been arranged such that the field penetration potency inside the backspace of the hollow-cathode is different while passing through the tapered gap region. This leads to non-concurrent ignition of the discharge through all the channels which is, in general, quite challenging in the case of multi-aperture plasma cathode <span class="hlt">electron</span> gun geometries. Multiple and successive hollow cathode phases are reported from this <span class="hlt">electron</span> gun geometry, which have been confirmed using simulations. This geometry also has led to the achievement of ˜71% fill factor inside the slow wave oscillator for an <span class="hlt">electron</span> beam of <span class="hlt">energy</span> of 20 keV and a beam current density in the range of 115-190 A/cm2 at a working argon gas pressure of 18 Pa. The oscillator has generated broadband microwave output in the frequency range of 10-11.7 GHz with a peak power of ˜10 kW for ˜50 ns.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22583270','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22583270"><span>Communication: <span class="hlt">electronic</span> <span class="hlt">band</span> gaps of semiconducting zig-zag carbon nanotubes from many-body perturbation theory calculations.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Umari, P; Petrenko, O; Taioli, S; De Souza, M M</p> <p>2012-05-14</p> <p><span class="hlt">Electronic</span> <span class="hlt">band</span> gaps for optically allowed transitions are calculated for a series of semiconducting single-walled zig-zag carbon nanotubes of increasing diameter within the many-body perturbation theory GW method. The dependence of the evaluated gaps with respect to tube diameters is then compared with those found from previous experimental data for optical gaps combined with theoretical estimations of exciton binding <span class="hlt">energies</span>. We find that our GW gaps confirm the behavior inferred from experiment. The relationship between the <span class="hlt">electronic</span> gap and the diameter extrapolated from the GW values is also in excellent agreement with a direct measurement recently performed through scanning tunneling spectroscopy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1402607-simulation-energy-dependent-electron-diffusion-processes-earth-outer-radiation-belt','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1402607-simulation-energy-dependent-electron-diffusion-processes-earth-outer-radiation-belt"><span>Simulation of <span class="hlt">energy</span>-dependent <span class="hlt">electron</span> diffusion processes in the Earth's outer radiation belt</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Ma, Q.; Li, W.; Thorne, R. M.; ...</p> <p>2016-04-28</p> <p>The radial and local diffusion processes induced by various plasma waves govern the highly energetic <span class="hlt">electron</span> dynamics in the Earth's radiation belts, causing distinct characteristics in <span class="hlt">electron</span> distributions at various <span class="hlt">energies</span>. In this study, we present our simulation results of the energetic <span class="hlt">electron</span> evolution during a geomagnetic storm using the University of California, Los Angeles 3-D diffusion code. Following the plasma sheet <span class="hlt">electron</span> injections, the <span class="hlt">electrons</span> at different <span class="hlt">energy</span> <span class="hlt">bands</span> detected by the Magnetic <span class="hlt">Electron</span> Ion Spectrometer (MagEIS) and Relativistic <span class="hlt">Electron</span> Proton Telescope (REPT) instruments on board the Van Allen Probes exhibit a rapid enhancement followed by a slow diffusivemore » movement in differential <span class="hlt">energy</span> fluxes, and the radial extent to which <span class="hlt">electrons</span> can penetrate into depends on <span class="hlt">energy</span> with closer penetration toward the Earth at lower <span class="hlt">energies</span> than higher <span class="hlt">energies</span>. We incorporate radial diffusion, local acceleration, and loss processes due to whistler mode wave observations to perform a 3-D diffusion simulation. Here, our simulation results demonstrate that chorus waves cause <span class="hlt">electron</span> flux increase by more than 1 order of magnitude during the first 18 h, and the subsequent radial extents of the energetic <span class="hlt">electrons</span> during the storm recovery phase are determined by the coupled radial diffusion and the pitch angle scattering by EMIC waves and plasmaspheric hiss. The radial diffusion caused by ULF waves and local plasma wave scattering are <span class="hlt">energy</span> dependent, which lead to the observed <span class="hlt">electron</span> flux variations with <span class="hlt">energy</span> dependences. Lastly, this study suggests that plasma wave distributions in the inner magnetosphere are crucial for the <span class="hlt">energy</span>-dependent intrusions of several hundred keV to several MeV <span class="hlt">electrons</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22483112-direct-band-gap-measurement-cu-ga-se-sub-thin-films-using-high-resolution-reflection-electron-energy-loss-spectroscopy','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22483112-direct-band-gap-measurement-cu-ga-se-sub-thin-films-using-high-resolution-reflection-electron-energy-loss-spectroscopy"><span>Direct <span class="hlt">band</span> gap measurement of Cu(In,Ga)(Se,S){sub 2} thin films using high-resolution reflection <span class="hlt">electron</span> <span class="hlt">energy</span> loss spectroscopy</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Heo, Sung; College of Information and Communication Engineering, Sungkyunkwan University, Cheoncheon-dong 300, Jangan-gu, Suwon 440-746; Lee, Hyung-Ik</p> <p>2015-06-29</p> <p>To investigate the <span class="hlt">band</span> gap profile of Cu(In{sub 1−x},Ga{sub x})(Se{sub 1−y}S{sub y}){sub 2} of various compositions, we measured the <span class="hlt">band</span> gap profile directly as a function of in-depth using high-resolution reflection <span class="hlt">energy</span> loss spectroscopy (HR-REELS), which was compared with the <span class="hlt">band</span> gap profile calculated based on the auger depth profile. The <span class="hlt">band</span> gap profile is a double-graded <span class="hlt">band</span> gap as a function of in-depth. The calculated <span class="hlt">band</span> gap obtained from the auger depth profile seems to be larger than that by HR-REELS. Calculated <span class="hlt">band</span> gaps are to measure the average <span class="hlt">band</span> gap of the spatially different varying compositions with respectmore » to considering its void fraction. But, the results obtained using HR-REELS are to be affected by the low <span class="hlt">band</span> gap (i.e., out of void) rather than large one (i.e., near void). Our findings suggest an analytical method to directly determine the <span class="hlt">band</span> gap profile as function of in-depth.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19830013719','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19830013719"><span>Ground state <span class="hlt">energy</span> of <span class="hlt">electrons</span> in a static point-ion lattice</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Styer, D. F.; Ashcroft, N. W.</p> <p>1983-01-01</p> <p>The ground state <span class="hlt">energy</span> of a neutral collection of protons and <span class="hlt">electrons</span> was investigated under the assumption that in the ground state configuration, static protons occupy the sites of a rigid Bravais lattice. The Wigner-Seitz method was used in conjunction with three postulated potentials: bare Coulomb, Thomas-Fermi screening, and screening by a uniform bare background charge. Within these approximations, the exact <span class="hlt">band</span>-minimum <span class="hlt">energy</span> and wave functions are derived. For each of the three potentials, the approximate minimum ground state <span class="hlt">energy</span> per proton (relative to isolated <span class="hlt">electrons</span> and protons) is, respectively, -1.078 Ry, -1.038 Ry, and -1.052 Ry. These three minima all fall at a density of about 0.60 gm/cu cm, which is thus an approximate lower bound on the density of metallic hydrogen at its transition pressure.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1248741-band-gap-band-edge-engineering-multicomponent-garnet-scintillators-from-first-principles','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1248741-band-gap-band-edge-engineering-multicomponent-garnet-scintillators-from-first-principles"><span><span class="hlt">Band</span>-gap and <span class="hlt">band</span>-edge engineering of multicomponent garnet scintillators from first principles</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Yadav, Satyesh K.; Uberuaga, Blas P.; Nikl, Martin; ...</p> <p>2015-11-24</p> <p>Complex doping schemes in R 3Al 5O 12 (where R is the rare-earth element) garnet compounds have recently led to pronounced improvements in scintillator performance. Specifically, by admixing lutetium and yttrium aluminate garnets with gallium and gadolinium, the <span class="hlt">band</span> gap is altered in a manner that facilitates the removal of deleterious <span class="hlt">electron</span> trapping associated with cation antisite defects. Here, we expand upon this initial work to systematically investigate the effect of substitutional admixing on the <span class="hlt">energy</span> levels of <span class="hlt">band</span> edges. Density-functional theory and hybrid density-functional theory (HDFT) are used to survey potential admixing candidates that modify either the conduction-<span class="hlt">band</span> minimummore » (CBM) or valence-<span class="hlt">band</span> maximum (VBM). We consider two sets of compositions based on Lu 3B 5O 12 where B is Al, Ga, In, As, and Sb, and R 3Al 5O 12, where R is Lu, Gd, Dy, and Er. We find that admixing with various R cations does not appreciably affect the <span class="hlt">band</span> gap or <span class="hlt">band</span> edges. In contrast, substituting Al with cations of dissimilar ionic radii has a profound impact on the <span class="hlt">band</span> structure. We further show that certain dopants can be used to selectively modify only the CBM or the VBM. Specifically, Ga and In decrease the <span class="hlt">band</span> gap by lowering the CBM, while As and Sb decrease the <span class="hlt">band</span> gap by raising the VBM, the relative change in <span class="hlt">band</span> gap is quantitatively validated by HDFT. These results demonstrate a powerful approach to quickly screen the impact of dopants on the <span class="hlt">electronic</span> structure of scintillator compounds, identifying those dopants which alter the <span class="hlt">band</span> edges in very specific ways to eliminate both <span class="hlt">electron</span> and hole traps responsible for performance limitations. Furthermore, this approach should be broadly applicable for the optimization of <span class="hlt">electronic</span> and optical performance for a wide range of compounds by tuning the VBM and CBM.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JPCM...30t5502H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JPCM...30t5502H"><span>Investigation of indirect excitons in bulk 2H-MoS2 using transmission <span class="hlt">electron</span> <span class="hlt">energy</span>-loss spectroscopy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Habenicht, Carsten; Schuster, Roman; Knupfer, Martin; Büchner, Bernd</p> <p>2018-05-01</p> <p>We have investigated indirect excitons in bulk 2H-MoS2 using transmission <span class="hlt">electron</span> <span class="hlt">energy</span>-loss spectroscopy. The <span class="hlt">electron</span> <span class="hlt">energy</span>-loss spectra were measured for various momentum transfer values parallel to the and directions of the Brillouin zone. The results allowed the identification of the indirect excitons between the valence <span class="hlt">band</span> K v and conduction <span class="hlt">band</span> Λc points, the Γv and K c points as well as adjacent K v and points. The <span class="hlt">energy</span>-momentum dispersions for the K v-Λc, Γv-K c and K v1- excitons along the line are presented. The former two transitions exhibit a quadratic dispersion which allowed calculating their effective exciton masses based on the effective mass approximation. The K v1- transition follows a more linear dispersion relationship.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22489482-tensile-strain-effect-inducing-indirect-direct-band-gap-transition-reducing-band-gap-energy-ge','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22489482-tensile-strain-effect-inducing-indirect-direct-band-gap-transition-reducing-band-gap-energy-ge"><span>Tensile-strain effect of inducing the indirect-to-direct <span class="hlt">band</span>-gap transition and reducing the <span class="hlt">band</span>-gap <span class="hlt">energy</span> of Ge</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Inaoka, Takeshi, E-mail: inaoka@phys.u-ryukyu.ac.jp; Furukawa, Takuro; Toma, Ryo</p> <p></p> <p>By means of a hybrid density-functional method, we investigate the tensile-strain effect of inducing the indirect-to-direct <span class="hlt">band</span>-gap transition and reducing the <span class="hlt">band</span>-gap <span class="hlt">energy</span> of Ge. We consider [001], [111], and [110] uniaxial tensility and (001), (111), and (110) biaxial tensility. Under the condition of no normal stress, we determine both normal compression and internal strain, namely, relative displacement of two atoms in the primitive unit cell, by minimizing the total <span class="hlt">energy</span>. We identify those strain types which can induce the <span class="hlt">band</span>-gap transition, and evaluate the critical strain coefficient where the gap transition occurs. Either normal compression or internal strain operatesmore » unfavorably to induce the gap transition, which raises the critical strain coefficient or even blocks the transition. We also examine how each type of tensile strain decreases the <span class="hlt">band</span>-gap <span class="hlt">energy</span>, depending on its orientation. Our analysis clearly shows that synergistic operation of strain orientation and <span class="hlt">band</span> anisotropy has a great influence on the gap transition and the gap <span class="hlt">energy</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015ApPhL.107f2104K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015ApPhL.107f2104K"><span>Compositional bowing of <span class="hlt">band</span> <span class="hlt">energies</span> and their deformation potentials in strained InGaAs ternary alloys: A first-principles study</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Khomyakov, Petr A.; Luisier, Mathieu; Schenk, Andreas</p> <p>2015-08-01</p> <p>Using first-principles calculations, we show that the conduction and valence <span class="hlt">band</span> <span class="hlt">energies</span> and their deformation potentials exhibit a non-negligible compositional bowing in strained ternary semiconductor alloys such as InGaAs. The <span class="hlt">electronic</span> structure of these compounds has been calculated within the framework of local density approximation and hybrid functional approach for large cubic supercells and special quasi-random structures, which represent two kinds of model structures for random alloys. We find that the predicted bowing effect for the <span class="hlt">band</span> <span class="hlt">energy</span> deformation potentials is rather insensitive to the choice of the functional and alloy structural model. The direction of bowing is determined by In cations that give a stronger contribution to the formation of the InxGa1-xAs valence <span class="hlt">band</span> states with x ≳ 0.5, compared to Ga cations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvM...2e4602B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvM...2e4602B"><span>Optical and <span class="hlt">electronic</span> properties of 2 H -Mo S2 under pressure: Revealing the spin-polarized nature of bulk <span class="hlt">electronic</span> <span class="hlt">bands</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brotons-Gisbert, Mauro; Segura, Alfredo; Robles, Roberto; Canadell, Enric; Ordejón, Pablo; Sánchez-Royo, Juan F.</p> <p>2018-05-01</p> <p>Monolayers of transition-metal dichalcogenide semiconductors present spin-valley locked <span class="hlt">electronic</span> <span class="hlt">bands</span>, a property with applications in valleytronics and spintronics that is usually believed to be absent in their centrosymmetric (as the bilayer or bulk) counterparts. Here we show that bulk 2 H -Mo S2 hides a spin-polarized nature of states determining its direct <span class="hlt">band</span> gap, with the spin sequence of valence and conduction <span class="hlt">bands</span> expected for its single layer. This relevant finding is attained by investigating the behavior of the binding <span class="hlt">energy</span> of A and B excitons under high pressure, by means of absorption measurements and density-functional-theory calculations. These results raise an unusual situation in which bright and dark exciton degeneracy is naturally broken in a centrosymmetric material. Additionally, the phonon-assisted scattering process of excitons has been studied by analyzing the pressure dependence of the linewidth of discrete excitons observed at the absorption coefficient edge of 2 H -Mo S2 . Also, the pressure dependence of the indirect optical transitions of bulk 2 H -Mo S2 has been analyzed by absorption measurements and density-functional-theory calculations. These results reflect a progressive closure of the indirect <span class="hlt">band</span> gap as pressure increases, indicating that metallization of bulk Mo S2 may occur at pressures higher than 26 GPa.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014CoPhC.185.1195S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014CoPhC.185.1195S"><span>Improved cache performance in Monte Carlo transport calculations using <span class="hlt">energy</span> <span class="hlt">banding</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Siegel, A.; Smith, K.; Felker, K.; Romano, P.; Forget, B.; Beckman, P.</p> <p>2014-04-01</p> <p>We present an <span class="hlt">energy</span> <span class="hlt">banding</span> algorithm for Monte Carlo (MC) neutral particle transport simulations which depend on large cross section lookup tables. In MC codes, read-only cross section data tables are accessed frequently, exhibit poor locality, and are typically too much large to fit in fast memory. Thus, performance is often limited by long latencies to RAM, or by off-node communication latencies when the data footprint is very large and must be decomposed on a distributed memory machine. The proposed <span class="hlt">energy</span> <span class="hlt">banding</span> algorithm allows maximal temporal reuse of data in <span class="hlt">band</span> sizes that can flexibly accommodate different architectural features. The <span class="hlt">energy</span> <span class="hlt">banding</span> algorithm is general and has a number of benefits compared to the traditional approach. In the present analysis we explore its potential to achieve improvements in time-to-solution on modern cache-based architectures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26226296','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26226296"><span>Esaki Diodes in van der Waals Heterojunctions with Broken-Gap <span class="hlt">Energy</span> <span class="hlt">Band</span> Alignment.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yan, Rusen; Fathipour, Sara; Han, Yimo; Song, Bo; Xiao, Shudong; Li, Mingda; Ma, Nan; Protasenko, Vladimir; Muller, David A; Jena, Debdeep; Xing, Huili Grace</p> <p>2015-09-09</p> <p>van der Waals (vdW) heterojunctions composed of two-dimensional (2D) layered materials are emerging as a solid-state materials family that exhibits novel physics phenomena that can power a range of <span class="hlt">electronic</span> and photonic applications. Here, we present the first demonstration of an important building block in vdW solids: room temperature Esaki tunnel diodes. The Esaki diodes were realized in vdW heterostructures made of black phosphorus (BP) and tin diselenide (SnSe2), two layered semiconductors that possess a broken-gap <span class="hlt">energy</span> <span class="hlt">band</span> offset. The presence of a thin insulating barrier between BP and SnSe2 enabled the observation of a prominent negative differential resistance (NDR) region in the forward-bias current-voltage characteristics, with a peak to valley ratio of 1.8 at 300 K and 2.8 at 80 K. A weak temperature dependence of the NDR indicates <span class="hlt">electron</span> tunneling being the dominant transport mechanism, and a theoretical model shows excellent agreement with the experimental results. Furthermore, the broken-gap <span class="hlt">band</span> alignment is confirmed by the junction photoresponse, and the phosphorus double planes in a single layer of BP are resolved in transmission <span class="hlt">electron</span> microscopy (TEM) for the first time. Our results represent a significant advance in the fundamental understanding of vdW heterojunctions and broaden the potential applications of 2D layered materials.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29150657','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29150657"><span>Specific heat, Electrical resistivity and <span class="hlt">Electronic</span> <span class="hlt">band</span> structure properties of noncentrosymmetric Th7Fe3 superconductor.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tran, V H; Sahakyan, M</p> <p>2017-11-17</p> <p>Noncentrosymmetric superconductor Th 7 Fe 3 has been investigated by means of specific heat, electrical resisitivity measurements and <span class="hlt">electronic</span> properties calculations. Sudden drop in the resistivity at 2.05 ± 0.15 K and specific heat jump at 1.98 ± 0.02 K are observed, rendering the superconducting transition. A model of two BCS-type gaps appears to describe the zero-magnetic-field specific heat better than those based on the isotropic BCS theory or anisotropic functions. A positive curvature of the upper critical field H c2 (T c ) and nonlinear field dependence of the Sommerfeld coefficient at 0.4 K qualitatively support the two-gap scenario, which predicts H c2 (0) = 13 kOe. The theoretical densities of states and <span class="hlt">electronic</span> <span class="hlt">band</span> structures (EBS) around the Fermi <span class="hlt">energy</span> show a mixture of Th 6d- and Fe 3d-<span class="hlt">electrons bands</span>, being responsible for the superconductivity. Furthermore, the EBS and Fermi surfaces disclose significantly anisotropic splitting associated with asymmetric spin-orbit coupling (ASOC). The ASOC sets up also multiband structure, which presumably favours a multigap superconductivity. <span class="hlt">Electron</span> Localization Function reveals the existence of both metallic and covalent bonds, the latter may have different strengths depending on the regions close to the Fe or Th atoms. The superconducting, <span class="hlt">electronic</span> properties and implications of asymmetric spin-orbit coupling associated with noncentrosymmetric structure are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22591505-class-monolayer-metal-halogenides-mx-sub-electronic-structures-band-alignments','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22591505-class-monolayer-metal-halogenides-mx-sub-electronic-structures-band-alignments"><span>A class of monolayer metal halogenides MX{sub 2}: <span class="hlt">Electronic</span> structures and <span class="hlt">band</span> alignments</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Lu, Feng; Wang, Weichao; Luo, Xiaoguang</p> <p>2016-03-28</p> <p>With systematic first principles calculations, a class of monolayer metal halogenides MX{sub 2} (M = Mg, Ca, Zn, Cd, Ge, Pb; M = Cl, Br, I) has been proposed. Our study indicates that these monolayer materials are semiconductors with the <span class="hlt">band</span> gaps ranging from 2.03 eV of ZnI{sub 2} to 6.08 eV of MgCl{sub 2}. Overall, the <span class="hlt">band</span> gap increases with the increase of the electronegativity of the X atom or the atomic number of the metal M. Meanwhile, the <span class="hlt">band</span> gaps of monolayer MgX{sub 2} (X = Cl, Br) are direct while those of other monolayers are indirect. Based on the <span class="hlt">band</span> edge curvatures, the derived electronmore » (m{sub e}) and hole (m{sub h}) effective masses of MX{sub 2} monolayers are close to their corresponding bulk values except that the m{sub e} of CdI{sub 2} is three times larger and the m{sub h} for PbI{sub 2} is twice larger. Finally, the <span class="hlt">band</span> alignments of all the studied MX{sub 2} monolayers are provided using the vacuum level as <span class="hlt">energy</span> reference. These theoretical results may not only introduce the monolayer metal halogenides family MX{sub 2} into the emerging two-dimensional materials, but also provide insights into the applications of MX{sub 2} in future <span class="hlt">electronic</span>, visible and ultraviolet optoelectronic devices.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA462510','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA462510"><span>Organic <span class="hlt">Electronic</span> Devices Using Crosslinked Polyelectrolyte Multilayers as an Ultra-Thin Dielectric Material</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2006-09-01</p> <p><span class="hlt">energy</span> <span class="hlt">band</span> diagram illustrating the allowed <span class="hlt">energies</span> for valence and conducting <span class="hlt">electrons</span>. The dashes within the <span class="hlt">band</span> gap (Eg) represent localized ...allowed <span class="hlt">energies</span> for valence and conducting <span class="hlt">electrons</span>. The dashes within the <span class="hlt">band</span> gap (Eg) represent localized <span class="hlt">electron</span> <span class="hlt">energy</span> states, or traps, that...been observed with the formation of alternating bond lengths along the backbone.43 The localization of the π-<span class="hlt">electrons</span> while forming the shorter double</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23142740','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23142740"><span>Extraction of topographic and material contrasts on surfaces from SEM images obtained by <span class="hlt">energy</span> filtering detection with low-<span class="hlt">energy</span> primary <span class="hlt">electrons</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Nagoshi, Masayasu; Aoyama, Tomohiro; Sato, Kaoru</p> <p>2013-01-01</p> <p>Secondary <span class="hlt">electron</span> microscope (SEM) images have been obtained for practical materials using low primary <span class="hlt">electron</span> <span class="hlt">energies</span> and an in-lens type annular detector with changing negative bias voltage supplied to a grid placed in front of the detector. The kinetic-<span class="hlt">energy</span> distribution of the detected <span class="hlt">electrons</span> was evaluated by the gradient of the bias-<span class="hlt">energy</span> dependence of the brightness of the images. This is divided into mainly two parts at about 500 V, high and low brightness in the low- and high-<span class="hlt">energy</span> regions, respectively and shows difference among the surface regions having different composition and topography. The combination of the negative grid bias and the pixel-by-pixel image subtraction provides the <span class="hlt">band</span>-pass filtered images and extracts the material and topographic information of the specimen surfaces. Copyright © 2012 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ApPRv...4b1301H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ApPRv...4b1301H"><span><span class="hlt">Energy</span> <span class="hlt">band</span> offsets of dielectrics on InGaZnO4</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hays, David C.; Gila, B. P.; Pearton, S. J.; Ren, F.</p> <p>2017-06-01</p> <p>Thin-film transistors (TFTs) with channels made of hydrogenated amorphous silicon (a-Si:H) and polycrystalline silicon (poly-Si) are used extensively in the display industry. Amorphous silicon continues to dominate large-format display technology, but a-Si:H has a low <span class="hlt">electron</span> mobility, μ ˜ 1 cm2/V s. Transparent, conducting metal-oxide materials such as Indium-Gallium-Zinc Oxide (IGZO) have demonstrated <span class="hlt">electron</span> mobilities of 10-50 cm2/V s and are candidates to replace a-Si:H for TFT backplane technologies. The device performance depends strongly on the type of <span class="hlt">band</span> alignment of the gate dielectric with the semiconductor channel material and on the <span class="hlt">band</span> offsets. The factors that determine the conduction and valence <span class="hlt">band</span> offsets for a given material system are not well understood. Predictions based on various models have historically been unreliable and <span class="hlt">band</span> offset values must be determined experimentally. This paper provides experimental <span class="hlt">band</span> offset values for a number of gate dielectrics on IGZO for next generation TFTs. The relationship between <span class="hlt">band</span> offset and interface quality, as demonstrated experimentally and by previously reported results, is also explained. The literature shows significant variations in reported <span class="hlt">band</span> offsets and the reasons for these differences are evaluated. The biggest contributor to conduction <span class="hlt">band</span> offsets is the variation in the bandgap of the dielectrics due to differences in measurement protocols and stoichiometry resulting from different deposition methods, chemistry, and contamination. We have investigated the influence of valence <span class="hlt">band</span> offset values of strain, defects/vacancies, stoichiometry, chemical bonding, and contamination on IGZO/dielectric heterojunctions. These measurements provide data needed to further develop a predictive theory of <span class="hlt">band</span> offsets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29578678','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29578678"><span><span class="hlt">Band</span> Edge Dynamics and Multiexciton Generation in Narrow <span class="hlt">Band</span> Gap HgTe Nanocrystals.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Livache, Clément; Goubet, Nicolas; Martinez, Bertille; Jagtap, Amardeep; Qu, Junling; Ithurria, Sandrine; Silly, Mathieu G; Dubertret, Benoit; Lhuillier, Emmanuel</p> <p>2018-04-11</p> <p>Mercury chalcogenide nanocrystals and especially HgTe appear as an interesting platform for the design of low cost mid-infrared (mid-IR) detectors. Nevertheless, their <span class="hlt">electronic</span> structure and transport properties remain poorly understood, and some critical aspects such as the carrier relaxation dynamics at the <span class="hlt">band</span> edge have been pushed under the rug. Some of the previous reports on dynamics are setup-limited, and all of them have been obtained using photon <span class="hlt">energy</span> far above the <span class="hlt">band</span> edge. These observations raise two main questions: (i) what are the carrier dynamics at the <span class="hlt">band</span> edge and (ii) should we expect some additional effect (multiexciton generation (MEG)) as such narrow <span class="hlt">band</span> gap materials are excited far above the <span class="hlt">band</span> edge? To answer these questions, we developed a high-bandwidth setup that allows us to understand and compare the carrier dynamics resonantly pumped at the <span class="hlt">band</span> edge in the mid-IR and far above the <span class="hlt">band</span> edge. We demonstrate that fast (>50 MHz) photoresponse can be obtained even in the mid-IR and that MEG is occurring in HgTe nanocrystal arrays with a threshold around 3 times the <span class="hlt">band</span> edge <span class="hlt">energy</span>. Furthermore, the photoresponse can be effectively tuned in magnitude and sign using a phototransistor configuration.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_9 --> <div id="page_10" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="181"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JPhD...50NLT02G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JPhD...50NLT02G"><span>A novel theoretical model for the temperature dependence of <span class="hlt">band</span> gap <span class="hlt">energy</span> in semiconductors</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Geng, Peiji; Li, Weiguo; Zhang, Xianhe; Zhang, Xuyao; Deng, Yong; Kou, Haibo</p> <p>2017-10-01</p> <p>We report a novel theoretical model without any fitting parameters for the temperature dependence of <span class="hlt">band</span> gap <span class="hlt">energy</span> in semiconductors. This model relates the <span class="hlt">band</span> gap <span class="hlt">energy</span> at the elevated temperature to that at the arbitrary reference temperature. As examples, the <span class="hlt">band</span> gap <span class="hlt">energies</span> of Si, Ge, AlN, GaN, InP, InAs, ZnO, ZnS, ZnSe and GaAs at temperatures below 400 K are calculated and are in good agreement with the experimental results. Meanwhile, the <span class="hlt">band</span> gap <span class="hlt">energies</span> at high temperatures (T  >  400 K) are predicted, which are greater than the experimental results, and the reasonable analysis is carried out as well. Under low temperatures, the effect of lattice expansion on the <span class="hlt">band</span> gap <span class="hlt">energy</span> is very small, but it has much influence on the <span class="hlt">band</span> gap <span class="hlt">energy</span> at high temperatures. Therefore, it is necessary to consider the effect of lattice expansion at high temperatures, and the method considering the effect of lattice expansion has also been given. The model has distinct advantages compared with the widely quoted Varshni’s semi-empirical equation from the aspect of modeling, physical meaning and application. The study provides a convenient method to determine the <span class="hlt">band</span> gap <span class="hlt">energy</span> under different temperatures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JPCM...30m5501P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JPCM...30m5501P"><span><span class="hlt">Band</span> structure and unconventional <span class="hlt">electronic</span> topology of CoSi</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pshenay-Severin, D. A.; Ivanov, Y. V.; Burkov, A. A.; Burkov, A. T.</p> <p>2018-04-01</p> <p>Semimetals with certain crystal symmetries may possess unusual <span class="hlt">electronic</span> structure topology, distinct from that of the conventional Weyl and Dirac semimetals. Characteristic property of these materials is the existence of <span class="hlt">band</span>-touching points with multiple (higher than two-fold) degeneracy and nonzero Chern number. CoSi is a representative of this group of materials exhibiting the so-called ‘new fermions’. We report on an ab initio calculation of the <span class="hlt">electronic</span> structure of CoSi using density functional methods, taking into account the spin-orbit interactions. The linearized \</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013NatSR...3E2849W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013NatSR...3E2849W"><span>Hydrogen production by Tuning the Photonic <span class="hlt">Band</span> Gap with the <span class="hlt">Electronic</span> <span class="hlt">Band</span> Gap of TiO2</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Waterhouse, G. I. N.; Wahab, A. K.; Al-Oufi, M.; Jovic, V.; Anjum, D. H.; Sun-Waterhouse, D.; Llorca, J.; Idriss, H.</p> <p>2013-10-01</p> <p>Tuning the photonic <span class="hlt">band</span> gap (PBG) to the <span class="hlt">electronic</span> <span class="hlt">band</span> gap (EBG) of Au/TiO2 catalysts resulted in considerable enhancement of the photocatalytic water splitting to hydrogen under direct sunlight. Au/TiO2 (PBG-357 nm) photocatalyst exhibited superior photocatalytic performance under both UV and sunlight compared to the Au/TiO2 (PBG-585 nm) photocatalyst and both are higher than Au/TiO2 without the 3 dimensionally ordered macro-porous structure materials. The very high photocatalytic activity is attributed to suppression of a fraction of <span class="hlt">electron</span>-hole recombination route due to the co-incidence of the PBG with the EBG of TiO2 These materials that maintain their activity with very small amount of sacrificial agents (down to 0.5 vol.% of ethanol) are poised to find direct applications because of their high activity, low cost of the process, simplicity and stability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012ApPhL.100f2102Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012ApPhL.100f2102Y"><span><span class="hlt">Energy</span> <span class="hlt">band</span> engineering and controlled p-type conductivity of CuAlO2 thin films by nonisovalent Cu-O alloying</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yao, Z. Q.; He, B.; Zhang, L.; Zhuang, C. Q.; Ng, T. W.; Liu, S. L.; Vogel, M.; Kumar, A.; Zhang, W. J.; Lee, C. S.; Lee, S. T.; Jiang, X.</p> <p>2012-02-01</p> <p>The <span class="hlt">electronic</span> <span class="hlt">band</span> structure and p-type conductivity of CuAlO2 films were modified via synergistic effects of <span class="hlt">energy</span> <span class="hlt">band</span> offset and partial substitution of less-dispersive Cu+ 3d10 with Cu2+ 3d9 orbitals in the valence <span class="hlt">band</span> maximum by alloying nonisovalent Cu-O with CuAlO2 host. The Cu-O/CuAlO2 alloying films show excellent <span class="hlt">electronic</span> properties with tunable wide direct bandgaps (˜3.46-3.87 eV); Hall measurements verify the highest hole mobilities (˜11.3-39.5 cm2/Vs) achieved thus far for CuAlO2 thin films and crystals. Top-gate thin film transistors constructed on p-CuAlO2 films were presented, and the devices showed pronounced performance with Ion/Ioff of ˜8.0 × 102 and field effect mobility of 0.97 cm2/Vs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22598820-sensitivity-electron-transport-within-bulk-zinc-blende-gallium-nitride-variations-crystal-temperature-doping-concentration-non-parabolicity-coefficient-associated-lowest-energy-conduction-band-valley','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22598820-sensitivity-electron-transport-within-bulk-zinc-blende-gallium-nitride-variations-crystal-temperature-doping-concentration-non-parabolicity-coefficient-associated-lowest-energy-conduction-band-valley"><span>The sensitivity of the <span class="hlt">electron</span> transport within bulk zinc-blende gallium nitride to variations in the crystal temperature, the doping concentration, and the non-parabolicity coefficient associated with the lowest <span class="hlt">energy</span> conduction <span class="hlt">band</span> valley</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Siddiqua, Poppy; O'Leary, Stephen K., E-mail: stephen.oleary@ubc.ca</p> <p>2016-09-07</p> <p>Within the framework of a semi-classical three-valley Monte Carlo simulation approach, we analyze the steady-state and transient <span class="hlt">electron</span> transport that occurs within bulk zinc-blende gallium nitride. In particular, we examine how the steady-state and transient <span class="hlt">electron</span> transport that occurs within this material changes in response to variations in the crystal temperature, the doping concentration, and the non-parabolicity coefficient associated with the lowest <span class="hlt">energy</span> conduction <span class="hlt">band</span> valley. These results are then contrasted with those corresponding to a number of other compound semiconductors of interest.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA615115','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA615115"><span>First Principles Study of <span class="hlt">Band</span> Structure and <span class="hlt">Band</span> Gap Engineering in Graphene for Device Applications</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2015-03-20</p> <p>In the bandstructure of graphene which is dominated by Dirac description, valence and conduction <span class="hlt">bands</span> cross the Fermi level at a single point (K...of <span class="hlt">energy</span> <span class="hlt">bands</span> and appearance of Dirac cones near the ‘K’ point and Fermi level the <span class="hlt">electrons</span> behave like massless Dirac fermions. For applications...results. Introduction Graphene, the super carbon , is now accepted as wonder material with new physics and it has caused major</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017OptMa..66..149L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017OptMa..66..149L"><span><span class="hlt">Electronic</span> structure and optical properties of noncentrosymmetric LiGaSe2: Experimental measurements and DFT <span class="hlt">band</span> structure calculations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lavrentyev, A. A.; Gabrelian, B. V.; Vu, V. T.; Ananchenko, L. N.; Isaenko, L. I.; Yelisseyev, A. P.; Khyzhun, O. Y.</p> <p>2017-04-01</p> <p>We report on measurements of X-ray photoelectron (XP) spectra for pristine and Ar+ ion-irradiated surfaces of LiGaSe2 single crystal grown by Bridgman-Stockbarger method. <span class="hlt">Electronic</span> structure of the LiGaSe2 compound is studied from a theoretical and experimental viewpoint. In particular, total and partial densities of states of LiGaSe2 are investigated by density functional theory (DFT) calculations employing the augmented plane wave + local orbitals (APW + lo) method and they are verified by data of X-ray spectroscopy measurements. The DFT calculations indicate that the main contributors to the valence <span class="hlt">band</span> of LiGaSe2 are the Se 4p states, which contribute mainly at the top and in the upper portion of the valence <span class="hlt">band</span>, with also essential contributions of these states in the lower portion of the <span class="hlt">band</span>. Other substantial contributions to the valence <span class="hlt">band</span> of LiGaSe2 emerge from the Ga 4s and Ga 4p states contributing mainly at the lower ant upper portions of the valence <span class="hlt">band</span>, respectively. With respect to the conduction <span class="hlt">band</span>, the calculations indicate that its bottom is composed mainly from contributions of the unoccupied Ga s and Se p states. The present calculations are confirmed experimentally when comparing the XP valence-<span class="hlt">band</span> spectrum of the LiGaS2 single crystal on a common <span class="hlt">energy</span> scale with the X-ray emission <span class="hlt">bands</span> representing the <span class="hlt">energy</span> distribution of the Ga 4p and Se 4p states. Measurements of the fundamental absorption edges at room temperature reveal that bandgap value, Eg, of LiGaSe2 is equal to 3.47 eV and the Eg value increases up to 3.66 eV when decreasing temperature to 80 K. The main optical characteristics of the LiGaSe2 compound are clarified by the DFT calculations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhSS...60..804K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhSS...60..804K"><span>Density of <span class="hlt">Electronic</span> States in the Conduction <span class="hlt">Band</span> of Ultrathin Films of Naphthalenedicarboxylic Anhydride and Naphthalenetetracarboxylic Dianhydride on the Surface of Oxidized Silicon</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Komolov, A. S.; Lazneva, E. F.; Gerasimova, N. B.; Panina, Yu. A.; Baramygin, A. V.; Zashikhin, G. D.; Pshenichnyuk, S. A.</p> <p>2018-04-01</p> <p>The results of examination of the <span class="hlt">electronic</span> structure of the conduction <span class="hlt">band</span> of naphthalenedicarboxylic anhydride (NDCA) films in the process of their deposition on the surface of oxidized silicon are presented. These results were obtained using total current spectroscopy (TCS) in the <span class="hlt">energy</span> range from 5 to 20 eV above the Fermi level. The <span class="hlt">energy</span> position of the primary maxima of the density of unoccupied states (DOUS) of an NDCA film was determined based on the experimental TCS data and calculated data and compared with the position of the DOUS maxima of a naphthalenetetracarboxylic dianhydride (NTCDA) film. The theoretical analysis involved calculating the <span class="hlt">energies</span> and the spatial distribution of orbitals of the molecules under study at the B3LYP/6-31G(d) DFT (density functional theory) level and correcting the obtained <span class="hlt">energies</span> in accordance with the procedure that was proven effective in earlier studies of the conduction <span class="hlt">band</span> of films of small conjugated organic molecules. It was found that the DOUS maxima of the NTCDA film in the studied <span class="hlt">energy</span> interval from 5 to 20 eV above the Fermi level are shifted toward lower <span class="hlt">electron</span> <span class="hlt">energies</span> by 1-2 eV relative to the corresponding DOUS maxima of the NDCA film Subdivision of the Ufa Federal Research Centre of the.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24283411','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24283411"><span>The dependence of graphene Raman D-<span class="hlt">band</span> on carrier density.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Liu, Junku; Li, Qunqing; Zou, Yuan; Qian, Qingkai; Jin, Yuanhao; Li, Guanhong; Jiang, Kaili; Fan, Shoushan</p> <p>2013-01-01</p> <p>Raman spectroscopy has been an integral part of graphene research and can provide information about graphene structure, <span class="hlt">electronic</span> characteristics, and <span class="hlt">electron</span>-phonon interactions. In this study, the characteristics of the graphene Raman D-<span class="hlt">band</span>, which vary with carrier density, are studied in detail, including the frequency, full width half-maximum, and intensity. We find the Raman D-<span class="hlt">band</span> frequency increases for hole doping and decreases for <span class="hlt">electron</span> doping. The Raman D-<span class="hlt">band</span> intensity increases when the Fermi level approaches half of the excitation <span class="hlt">energy</span> and is higher in the case of <span class="hlt">electron</span> doping than that of hole doping. These variations can be explained by <span class="hlt">electron</span>-phonon interaction theory and quantum interference between different Raman pathways in graphene. The intensity ratio of Raman D- and G-<span class="hlt">band</span>, which is important for defects characterization in graphene, shows a strong dependence on carrier density.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018npjQM...3....1T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018npjQM...3....1T"><span>Observation of Dirac-like <span class="hlt">energy</span> <span class="hlt">band</span> and ring-torus Fermi surface associated with the nodal line in topological insulator CaAgAs</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Takane, Daichi; Nakayama, Kosuke; Souma, Seigo; Wada, Taichi; Okamoto, Yoshihiko; Takenaka, Koshi; Yamakawa, Youichi; Yamakage, Ai; Mitsuhashi, Taichi; Horiba, Koji; Kumigashira, Hiroshi; Takahashi, Takashi; Sato, Takafumi</p> <p>2018-01-01</p> <p>One of key challenges in current material research is to search for new topological materials with inverted bulk-<span class="hlt">band</span> structure. In topological insulators, the <span class="hlt">band</span> inversion caused by strong spin-orbit coupling leads to opening of a <span class="hlt">band</span> gap in the entire Brillouin zone, whereas an additional crystal symmetry such as point-group and nonsymmorphic symmetries sometimes prohibits the gap opening at/on specific points or line in momentum space, giving rise to topological semimetals. Despite many theoretical predictions of topological insulators/semimetals associated with such crystal symmetries, the experimental realization is still relatively scarce. Here, using angle-resolved photoemission spectroscopy with bulk-sensitive soft-x-ray photons, we experimentally demonstrate that hexagonal pnictide CaAgAs belongs to a new family of topological insulators characterized by the inverted <span class="hlt">band</span> structure and the mirror reflection symmetry of crystal. We have established the bulk valence-<span class="hlt">band</span> structure in three-dimensional Brillouin zone, and observed the Dirac-like <span class="hlt">energy</span> <span class="hlt">band</span> and ring-torus Fermi surface associated with the line node, where bulk valence and conducting <span class="hlt">bands</span> cross on a line in the momentum space under negligible spin-orbit coupling. Intriguingly, we found that no other <span class="hlt">bands</span> cross the Fermi level and therefore the low-<span class="hlt">energy</span> excitations are solely characterized by the Dirac-like <span class="hlt">band</span>. CaAgAs provides an excellent platform to study the interplay among low-<span class="hlt">energy</span> <span class="hlt">electron</span> dynamics, crystal symmetry, and exotic topological properties.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29265821','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29265821"><span>A Unifying Perspective on Oxygen Vacancies in Wide <span class="hlt">Band</span> Gap Oxides.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Linderälv, Christopher; Lindman, Anders; Erhart, Paul</p> <p>2018-01-04</p> <p>Wide <span class="hlt">band</span> gap oxides are versatile materials with numerous applications in research and technology. Many properties of these materials are intimately related to defects, with the most important defect being the oxygen vacancy. Here, using <span class="hlt">electronic</span> structure calculations, we show that the charge transition level (CTL) and eigenstates associated with oxygen vacancies, which to a large extent determine their <span class="hlt">electronic</span> properties, are confined to a rather narrow <span class="hlt">energy</span> range, even while <span class="hlt">band</span> gap and the <span class="hlt">electronic</span> structure of the conduction <span class="hlt">band</span> vary substantially. Vacancies are classified according to their character (deep versus shallow), which shows that the alignment of <span class="hlt">electronic</span> eigenenergies and CTL can be understood in terms of the transition between cavity-like localized levels in the large <span class="hlt">band</span> gap limit and strong coupling between conduction <span class="hlt">band</span> and vacancy states for small to medium <span class="hlt">band</span> gaps. We consider both conventional and hybrid functionals and demonstrate that the former yields results in very good agreement with the latter provided that <span class="hlt">band</span> edge alignment is taken into account.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3794377','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3794377"><span>Hydrogen production by Tuning the Photonic <span class="hlt">Band</span> Gap with the <span class="hlt">Electronic</span> <span class="hlt">Band</span> Gap of TiO2</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Waterhouse, G. I. N.; Wahab, A. K.; Al-Oufi, M.; Jovic, V.; Anjum, D. H.; Sun-Waterhouse, D.; Llorca, J.; Idriss, H.</p> <p>2013-01-01</p> <p>Tuning the photonic <span class="hlt">band</span> gap (PBG) to the <span class="hlt">electronic</span> <span class="hlt">band</span> gap (EBG) of Au/TiO2 catalysts resulted in considerable enhancement of the photocatalytic water splitting to hydrogen under direct sunlight. Au/TiO2 (PBG-357 nm) photocatalyst exhibited superior photocatalytic performance under both UV and sunlight compared to the Au/TiO2 (PBG-585 nm) photocatalyst and both are higher than Au/TiO2 without the 3 dimensionally ordered macro-porous structure materials. The very high photocatalytic activity is attributed to suppression of a fraction of <span class="hlt">electron</span>-hole recombination route due to the co-incidence of the PBG with the EBG of TiO2 These materials that maintain their activity with very small amount of sacrificial agents (down to 0.5 vol.% of ethanol) are poised to find direct applications because of their high activity, low cost of the process, simplicity and stability. PMID:24108361</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017NatPh..13..799W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017NatPh..13..799W"><span>Quasiparticle interference and strong <span class="hlt">electron</span>-mode coupling in the quasi-one-dimensional <span class="hlt">bands</span> of Sr2RuO4</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Zhenyu; Walkup, Daniel; Derry, Philip; Scaffidi, Thomas; Rak, Melinda; Vig, Sean; Kogar, Anshul; Zeljkovic, Ilija; Husain, Ali; Santos, Luiz H.; Wang, Yuxuan; Damascelli, Andrea; Maeno, Yoshiteru; Abbamonte, Peter; Fradkin, Eduardo; Madhavan, Vidya</p> <p>2017-08-01</p> <p>The single-layered ruthenate Sr2RuO4 is presented as a potential spin-triplet superconductor with an order parameter that may break time-reversal invariance and host half-quantized vortices with Majorana zero modes. Although the actual nature of the superconducting state is still a matter of controversy, it is believed to condense from a metallic state that is well described by a conventional Fermi liquid. In this work we use a combination of Fourier transform scanning tunnelling spectroscopy (FT-STS) and momentum-resolved <span class="hlt">electron</span> <span class="hlt">energy</span> loss spectroscopy (M-EELS) to probe interaction effects in the normal state of Sr2RuO4. Our high-resolution FT-STS data show signatures of the β-<span class="hlt">band</span> with a distinctly quasi-one-dimensional (1D) character. The <span class="hlt">band</span> dispersion reveals surprisingly strong interaction effects that dramatically renormalize the Fermi velocity, suggesting that the normal state of Sr2RuO4 is that of a `correlated metal' where correlations are strengthened by the quasi-1D nature of the <span class="hlt">bands</span>. In addition, kinks at <span class="hlt">energies</span> of approximately 10 meV, 38 meV and 70 meV are observed. By comparing STM and M-EELS data we show that the two higher <span class="hlt">energy</span> features arise from coupling with collective modes. The strong correlation effects and the kinks in the quasi-1D <span class="hlt">bands</span> could provide important information for understanding the superconducting state.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29633954','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29633954"><span>Investigation of indirect excitons in bulk 2H-MoS2 using transmission <span class="hlt">electron</span> <span class="hlt">energy</span>-loss spectroscopy.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Habenicht, Carsten; Schuster, Roman; Knupfer, Martin; Büchner, Bernd</p> <p>2018-05-23</p> <p>We have investigated indirect excitons in bulk 2H-MoS 2 using transmission <span class="hlt">electron</span> <span class="hlt">energy</span>-loss spectroscopy. The <span class="hlt">electron</span> <span class="hlt">energy</span>-loss spectra were measured for various momentum transfer values parallel to the [Formula: see text] and [Formula: see text] directions of the Brillouin zone. The results allowed the identification of the indirect excitons between the valence <span class="hlt">band</span> K v and conduction <span class="hlt">band</span> Λ c points, the Γ v and K c points as well as adjacent K v and [Formula: see text] points. The <span class="hlt">energy</span>-momentum dispersions for the K v -Λ c , Γ v -K c and K v1 -[Formula: see text] excitons along the [Formula: see text] line are presented. The former two transitions exhibit a quadratic dispersion which allowed calculating their effective exciton masses based on the effective mass approximation. The K v1 -[Formula: see text] transition follows a more linear dispersion relationship.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..GECHT6022O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..GECHT6022O"><span>Measurement of <span class="hlt">Electron</span> Density Using the Multipole Resonance Probe, Langmuir Probe and Optical Emission Spectroscopy in Low Pressure Plasmas with Different <span class="hlt">Electron</span> <span class="hlt">Energy</span> Distribution Functions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Oberberg, Moritz; Bibinov, Nikita; Ries, Stefan; Awakowicz, Peter; Institute of Electrical Engineering; Plasma Technology Team</p> <p>2016-09-01</p> <p>In recently publication, the young diagnostic tool Multipole Resonance Probe (MRP) for <span class="hlt">electron</span> density measurements was introduced. It is based on active plasma resonance spectroscopy (APRS). The probe was simulated und evaluated for different devices. The geometrical and electrical symmetry simplifies the APRS model, so that the <span class="hlt">electron</span> density can be easily calculated from the measured resonance. In this work, low pressure nitrogen mixture plasmas with different <span class="hlt">electron</span> <span class="hlt">energy</span> distribution functions (EEDF) are investigated. The results of the MRP measurement are compared with measurements of a Langmuir Probe (LP) and Optical Emission Spectroscopy (OES). Probes and OES measure in different regimes of kinetic <span class="hlt">electron</span> <span class="hlt">energy</span>. Both probes measure <span class="hlt">electrons</span> with low kinetic <span class="hlt">energy</span> (<10 eV), whereas the OES is influenced by <span class="hlt">electrons</span> with high kinetic <span class="hlt">energy</span> which are needed for transitions of molecule <span class="hlt">bands</span>. By the determination of the absolute intensity of N2(C-B) and N2+(B-X)<span class="hlt">electron</span> temperature and density can be calculated. In a non-maxwellian plasma, all plasma diagnostics need to be combined.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..MARB23008B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..MARB23008B"><span>Advancing Efficient All-<span class="hlt">Electron</span> <span class="hlt">Electronic</span> Structure Methods Based on Numeric Atom-Centered Orbitals for <span class="hlt">Energy</span> Related Materials</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Blum, Volker</p> <p></p> <p>This talk describes recent advances of a general, efficient, accurate all-<span class="hlt">electron</span> <span class="hlt">electronic</span> theory approach based on numeric atom-centered orbitals; emphasis is placed on developments related to materials for <span class="hlt">energy</span> conversion and their discovery. For total <span class="hlt">energies</span> and <span class="hlt">electron</span> <span class="hlt">band</span> structures, we show that the overall accuracy is on par with the best benchmark quality codes for materials, but scalable to large system sizes (1,000s of atoms) and amenable to both periodic and non-periodic simulations. A recent localized resolution-of-identity approach for the Coulomb operator enables O (N) hybrid functional based descriptions of the <span class="hlt">electronic</span> structure of non-periodic and periodic systems, shown for supercell sizes up to 1,000 atoms; the same approach yields accurate results for many-body perturbation theory as well. For molecular systems, we also show how many-body perturbation theory for charged and neutral quasiparticle excitation <span class="hlt">energies</span> can be efficiently yet accurately applied using basis sets of computationally manageable size. Finally, the talk highlights applications to the <span class="hlt">electronic</span> structure of hybrid organic-inorganic perovskite materials, as well as to graphene-based substrates for possible future transition metal compound based electrocatalyst materials. All methods described here are part of the FHI-aims code. VB gratefully acknowledges contributions by numerous collaborators at Duke University, Fritz Haber Institute Berlin, TU Munich, USTC Hefei, Aalto University, and many others around the globe.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JEMat..45.3842U','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JEMat..45.3842U"><span>Design and Implementation of RF <span class="hlt">Energy</span> Harvesting System for Low-Power <span class="hlt">Electronic</span> Devices</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Uzun, Yunus</p> <p>2016-08-01</p> <p>Radio frequency (RF) <span class="hlt">energy</span> harvester systems are a good alternative for energizing of low-power <span class="hlt">electronics</span> devices. In this work, an RF <span class="hlt">energy</span> harvester is presented to obtain <span class="hlt">energy</span> from Global System for Mobile Communications (GSM) 900 MHz signals. The <span class="hlt">energy</span> harvester, consisting of a two-stage Dickson voltage multiplier circuit and L-type impedance matching circuits, was designed, simulated, fabricated and tested experimentally in terms of its performance. Simulation and experimental works were carried out for various input power levels, load resistances and input frequencies. Both simulation and experimental works have been carried out for this frequency <span class="hlt">band</span>. An efficiency of 45% is obtained from the system at 0 dBm input power level using the impedance matching circuit. This corresponds to the power of 450 μW and this value is sufficient for many low-power devices. The most important parameters affecting the efficiency of the RF <span class="hlt">energy</span> harvester are the input power level, frequency <span class="hlt">band</span>, impedance matching and voltage multiplier circuits, load resistance and the selection of diodes. RF <span class="hlt">energy</span> harvester designs should be optimized in terms of these parameters.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014PhRvB..90g5203F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014PhRvB..90g5203F"><span><span class="hlt">Band</span> gap renormalization and Burstein-Moss effect in silicon- and germanium-doped wurtzite GaN up to 1020 cm-3</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Feneberg, Martin; Osterburg, Sarah; Lange, Karsten; Lidig, Christian; Garke, Bernd; Goldhahn, Rüdiger; Richter, Eberhard; Netzel, Carsten; Neumann, Maciej D.; Esser, Norbert; Fritze, Stephanie; Witte, Hartmut; Bläsing, Jürgen; Dadgar, Armin; Krost, Alois</p> <p>2014-08-01</p> <p>The interplay between <span class="hlt">band</span> gap renormalization and <span class="hlt">band</span> filling (Burstein-Moss effect) in n-type wurtzite GaN is investigated. For a wide range of <span class="hlt">electron</span> concentrations up to 1.6×1020cm-3 spectroscopic ellipsometry and photoluminescence were used to determine the dependence of the <span class="hlt">band</span> gap <span class="hlt">energy</span> and the Fermi edge on <span class="hlt">electron</span> density. The <span class="hlt">band</span> gap renormalization is the dominating effect up to an <span class="hlt">electron</span> density of about 9×1018cm-3; at higher values the Burstein-Moss effect is stronger. Exciton screening, the Mott transition, and formation of Mahan excitons are discussed. A quantitative understanding of the near gap transition <span class="hlt">energies</span> on <span class="hlt">electron</span> density is obtained. Higher <span class="hlt">energy</span> features in the dielectric functions up to 10eV are not influenced by <span class="hlt">band</span> gap renormalization.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007PhRvB..76c5309T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007PhRvB..76c5309T"><span>Influence of defects on the absorption edge of InN thin films: The <span class="hlt">band</span> gap value</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Thakur, J. S.; Danylyuk, Y. V.; Haddad, D.; Naik, V. M.; Naik, R.; Auner, G. W.</p> <p>2007-07-01</p> <p>We investigate the optical-absorption spectra of InN thin films whose <span class="hlt">electron</span> density varies from ˜1017tõ1021cm-3 . The low-density films are grown by molecular-beam-epitaxy deposition while highly degenerate films are grown by plasma-source molecular-beam epitaxy. The optical-absorption edge is found to increase from 0.61to1.90eV as the carrier density of the films is increased from low to high density. Since films are polycrystalline and contain various types of defects, we discuss the <span class="hlt">band</span> gap values by studying the influence of <span class="hlt">electron</span> degeneracy, <span class="hlt">electron-electron</span>, <span class="hlt">electron</span>-ionized impurities, and <span class="hlt">electron</span>-LO-phonon interaction self-<span class="hlt">energies</span> on the spectral absorption coefficients of these films. The quasiparticle self-<span class="hlt">energies</span> of the valence and conduction <span class="hlt">bands</span> are calculated using dielectric screening within the random-phase approximation. Using one-particle Green’s function analysis, we self-consistently determine the chemical potential for films by coupling equations for the chemical potential and the single-particle scattering rate calculated within the effective-mass approximation for the <span class="hlt">electron</span> scatterings from ionized impurities and LO phonons. By subtracting the influence of self-<span class="hlt">energies</span> and chemical potential from the optical-absorption edge <span class="hlt">energy</span>, we estimate the intrinsic <span class="hlt">band</span> gap values for the films. We also determine the variations in the calculated <span class="hlt">band</span> gap values due to the variations in the <span class="hlt">electron</span> effective mass and static dielectric constant. For the lowest-density film, the estimated <span class="hlt">band</span> gap <span class="hlt">energy</span> is ˜0.59eV , while for the highest-density film, it varies from ˜0.60tõ0.68eV depending on the values of <span class="hlt">electron</span> effective mass and dielectric constant.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JaJAP..57fKA08O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JaJAP..57fKA08O"><span>Total photoelectron yield spectroscopy of <span class="hlt">energy</span> distribution of <span class="hlt">electronic</span> states density at GaN surface and SiO2/GaN interface</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ohta, Akio; Truyen, Nguyen Xuan; Fujimura, Nobuyuki; Ikeda, Mitsuhisa; Makihara, Katsunori; Miyazaki, Seiichi</p> <p>2018-06-01</p> <p>The <span class="hlt">energy</span> distribution of the <span class="hlt">electronic</span> state density of wet-cleaned epitaxial GaN surfaces and SiO2/GaN structures has been studied by total photoelectron yield spectroscopy (PYS). By X-ray photoelectron spectroscopy (XPS) analysis, the <span class="hlt">energy</span> <span class="hlt">band</span> diagram for a wet-cleaned epitaxial GaN surface such as the <span class="hlt">energy</span> level of the valence <span class="hlt">band</span> top and <span class="hlt">electron</span> affinity has been determined to obtain a better understanding of the measured PYS signals. The <span class="hlt">electronic</span> state density of GaN surface with different carrier concentrations in the <span class="hlt">energy</span> region corresponding to the GaN bandgap has been evaluated. Also, the interface defect state density of SiO2/GaN structures was also estimated by not only PYS analysis but also capacitance–voltage (C–V) characteristics. We have demonstrated that PYS analysis enables the evaluation of defect state density filled with <span class="hlt">electrons</span> at the SiO2/GaN interface in the <span class="hlt">energy</span> region corresponding to the GaN midgap, which is difficult to estimate by C–V measurement of MOS capacitors.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_10 --> <div id="page_11" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="201"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27020395','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27020395"><span>Toward Revealing the Critical Role of Perovskite Coverage in Highly Efficient <span class="hlt">Electron</span>-Transport Layer-Free Perovskite Solar Cells: An <span class="hlt">Energy</span> <span class="hlt">Band</span> and Equivalent Circuit Model Perspective.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Huang, Like; Xu, Jie; Sun, Xiaoxiang; Du, Yangyang; Cai, Hongkun; Ni, Jian; Li, Juan; Hu, Ziyang; Zhang, Jianjun</p> <p>2016-04-20</p> <p>Currently, most efficient perovskite solar cells (PVKSCs) with a p-i-n structure require simultaneously <span class="hlt">electron</span> transport layers (ETLs) and hole transport layers (HTLs) to help collecting photogenerated <span class="hlt">electrons</span> and holes for obtaining high performance. ETL free planar PVKSC is a relatively new and simple structured solar cell that gets rid of the complex and high temperature required ETL (such as compact and mesoporous TiO2). Here, we demonstrate the critical role of high coverage of perovskite in efficient ETL free PVKSCs from an <span class="hlt">energy</span> <span class="hlt">band</span> and equivalent circuit model perspective. From an electrical point of view, we confirmed that the low coverage of perovskite does cause localized short circuit of the device. With coverage optimization, a planar p-i-n(++) device with a power conversion efficiency of over 11% was achieved, implying that the ETL layer may not be necessary for an efficient device as long as the perovskite coverage is approaching 100%.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012PhDT.......211M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012PhDT.......211M"><span><span class="hlt">Band</span> structure engineering for solar <span class="hlt">energy</span> applications: Zinc oxide(1-x) selenium(x) films and devices</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mayer, Marie Annette</p> <p></p> <p>New technologies motivate the development of new semiconducting materials, for which structural, electrical and chemical properties are not well understood. In addition to new materials systems, there are huge opportunities for new applications, especially in solar <span class="hlt">energy</span> conversion. In this dissertation I explore the role of <span class="hlt">band</span> structure engineering of semiconducting oxides for solar <span class="hlt">energy</span>. Due to the abundance and electrochemical stability of oxides, the appropriate modification could make them appealing for applications in both photovoltaics and photoelectrochemical hydrogen production. This dissertation describes the design, synthesis and evaluation of the alloy ZnO1-xSe x for these purposes. I review several methods of <span class="hlt">band</span> structure engineering including strain, quantum confinement and alloying. A detailed description of the <span class="hlt">band</span> anticrossing (BAC) model for highly mismatched alloys is provided, including the derivation of the BAC model as well as recent work and potential applications. Thin film ZnOxSe1-x samples are grown by pulsed laser deposition (PLD). I describe in detail the effect of growth conditions (temperature, pressure and laser fluence) on the chemistry, structure and optoelectronic properties of ZnOxSe1-x. The films are grown using different combinations of PLD conditions and characterized with a variety of techniques. Phase pure films with low roughness and high crystallinity were obtained at temperatures below 450¢ªC, pressures less than 10-4 Torr and laser fluences on the order of 1.5 J/cm 2. Electrical conduction was still observed despite heavy concentrations of grain boundaries. The <span class="hlt">band</span> structure of ZnO1-xSex is then examined in detail. The bulk <span class="hlt">electron</span> affinity of a ZnO thin film was measured to be 4.5 eV by pinning the Fermi level with native defects. This is explained in the framework of the amphoteric defect model. A shift in the ZnO1-xSe x valence <span class="hlt">band</span> edge with x is observed using synchrotron x-ray absorption and emission</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JSemi..36a3001A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JSemi..36a3001A"><span>The calculation of <span class="hlt">band</span> gap <span class="hlt">energy</span> in zinc oxide films</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Arif, Ali; Belahssen, Okba; Gareh, Salim; Benramache, Said</p> <p>2015-01-01</p> <p>We investigated the optical properties of undoped zinc oxide thin films as the n-type semiconductor; the thin films were deposited at different precursor molarities by ultrasonic spray and spray pyrolysis techniques. The thin films were deposited at different substrate temperatures ranging between 200 and 500 °C. In this paper, we present a new approach to control the optical gap <span class="hlt">energy</span> of ZnO thin films by concentration of the ZnO solution and substrate temperatures from experimental data, which were published in international journals. The model proposed to calculate the <span class="hlt">band</span> gap <span class="hlt">energy</span> with the Urbach <span class="hlt">energy</span> was investigated. The relation between the experimental data and theoretical calculation suggests that the <span class="hlt">band</span> gap <span class="hlt">energies</span> are predominantly estimated by the Urbach <span class="hlt">energies</span>, film transparency, and concentration of the ZnO solution and substrate temperatures. The measurements by these proposal models are in qualitative agreements with the experimental data; the correlation coefficient values were varied in the range 0.96-0.99999, indicating high quality representation of data based on Equation (2), so that the relative errors of all calculation are smaller than 4%. Thus, one can suppose that the undoped ZnO thin films are chemically purer and have many fewer defects and less disorder owing to an almost complete chemical decomposition and contained higher optical <span class="hlt">band</span> gap <span class="hlt">energy</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1419468-dual-roles-electrons-mixing-al-character-orbital-conduction-bands-lanthanide-actinide-dialuminides','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1419468-dual-roles-electrons-mixing-al-character-orbital-conduction-bands-lanthanide-actinide-dialuminides"><span>Dual roles of f <span class="hlt">electrons</span> in mixing Al 3 p character into d -orbital conduction <span class="hlt">bands</span> for lanthanide and actinide dialuminides</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Altman, Alison B.; Pemmaraju, C. D.; Alayoglu, Selim; ...</p> <p>2018-01-15</p> <p>Correlated <span class="hlt">electron</span> phenomena in lanthanide and actinide materials are driven by a complex interplay between the f and d orbitals. Here in this study, aluminum K-edge x-ray absorption spectroscopy and density functional theory calculations are used to evaluate the <span class="hlt">electronic</span> structure of the dialuminides, MAl 2 (M = Ce, Sm, Eu, Yb, Lu, U, and Pu). The results show how the <span class="hlt">energy</span> and occupancy of the 4f or 5f orbitals impacts mixing of Al 3p character into the 5d or 6d conduction <span class="hlt">bands</span>, which has implications for understanding the magnetic and structural properties of correlated <span class="hlt">electron</span> systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19970009409','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19970009409"><span>Time-Resolved IR-Absorption Spectroscopy of Hot-<span class="hlt">Electron</span> Dynamics in Satellite and Upper Conduction <span class="hlt">Bands</span> in GaP</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cavicchia, M. A.; Alfano, R. R.</p> <p>1995-01-01</p> <p>The relaxation dynamics of hot <span class="hlt">electrons</span> in the X6 and X7 satellite and upper conduction <span class="hlt">bands</span> in GaP was directly measured by femtosecond UV-pump-IR-probe absorption spectroscopy. From a fit to the induced IR-absorption spectra the dominant scattering mechanism giving rise to the absorption at early delay times was determined to be intervalley scattering of <span class="hlt">electrons</span> out of the X7 upper conduction-<span class="hlt">band</span> valley. For long delay times the dominant scattering mechanism is <span class="hlt">electron</span>-hole scattering. <span class="hlt">Electron</span> transport dynamics of the upper conduction <span class="hlt">band</span> of GaP has been time resolved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JaJAP..55dEG08N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JaJAP..55dEG08N"><span>Analysis of <span class="hlt">energy</span> states where <span class="hlt">electrons</span> and holes coexist in pseudomorphically strained InAs high-<span class="hlt">electron</span>-mobility transistors</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nishio, Yui; Sato, Takato; Hirayama, Naomi; Iida, Tsutomu; Takanashi, Yoshifumi</p> <p>2016-04-01</p> <p>In strained high-<span class="hlt">electron</span>-mobility transistors (HEMTs) with InAs as the channel, excess <span class="hlt">electrons</span> and holes are generated in the drain region by impact ionization. In the source region, <span class="hlt">electrons</span> are injected to recombine with accumulated holes by the Auger process. This causes the shift of the gate potential, V GS,shift, for HEMTs. For a system where <span class="hlt">electrons</span> and holes coexist, we established a theory taking into account the nonparabolicity of the conduction <span class="hlt">band</span> in the InAs channel. This theory enables us to rigorously determine not only the <span class="hlt">energy</span> states and the concentration profiles for both carriers but also the V GS,shift due to an accumulation of holes. We have derived the Auger recombination theory which takes into account the Fermi-Dirac statistics and is applicable to an arbitrary shape of potential <span class="hlt">energy</span>. The Auger recombination lifetime τA for InAs-PHEMTs was estimated as a function of the sheet hole concentration, p s, and τA was on the order of psec for p s exceeding 1012 cm-2.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..MAR.G1179S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..MAR.G1179S"><span>The <span class="hlt">electronic</span> and transport properties of monolayer transition metal dichalcogenides: a complex <span class="hlt">band</span> structure analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Szczesniak, Dominik</p> <p></p> <p>Recently, monolayer transition metal dichalcogenides have attracted much attention due to their potential use in both nano- and opto-<span class="hlt">electronics</span>. In such applications, the <span class="hlt">electronic</span> and transport properties of group-VIB transition metal dichalcogenides (MX2 , where M=Mo, W; X=S, Se, Te) are particularly important. Herein, new insight into these properties is presented by studying the complex <span class="hlt">band</span> structures (CBS's) of MX2 monolayers while accounting for spin-orbit coupling effects. By using the symmetry-based tight-binding model a nonlinear generalized eigenvalue problem for CBS's is obtained. An efficient method for solving such class of problems is presented and gives a complete set of physically relevant solutions. Next, these solutions are characterized and classified into propagating and evanescent states, where the latter states present not only monotonic but also oscillatory decay character. It is observed that some of the oscillatory evanescent states create characteristic complex loops at the direct <span class="hlt">band</span> gaps, which describe the tunneling currents in the MX2 materials. The importance of CBS's and tunneling currents is demonstrated by the analysis of the quantum transport across MX2 monolayers within phase field matching theory. Present work has been prepared within the Qatar <span class="hlt">Energy</span> and Environment Research Institute (QEERI) grand challenge ATHLOC project (Project No. QEERI- GC-3008).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhDT.........5N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhDT.........5N"><span>Photoinduced <span class="hlt">electron</span> transfer at the tetrapyrrole-TiO2 interface: Effect of the <span class="hlt">energy</span> alignment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nieto-Pescador, Jesus S.</p> <p></p> <p>Photoinduced <span class="hlt">electron</span> transfer is a ubiquitous process behind several physical, chemical, and biological processes. Its potential applications, ranging from solar cell technologies to photodynamic cancer therapy, require a thorough understanding of the basics of the reaction. This dissertation addresses open questions for a particular case of <span class="hlt">electron</span> transfer processes: Heterogeneous <span class="hlt">Electron</span> Transfer (HET). In this process, an <span class="hlt">electron</span> is transferred between a localized donor and a multitude of delocalized acceptor states. HET between photoexcited tetrapyrroles and colloidal TiO2 has been investigated using femtosecond transient absorption spectroscopy. Specifically, this work explores the not well-understood influence of the availability of states on the HET reaction. This problem is addressed by measuring <span class="hlt">electron</span> injection times as a function of the <span class="hlt">energy</span> difference between the LUMO and the conduction <span class="hlt">band</span> of TiO2. The change in the <span class="hlt">energy</span> alignment was done using two experimental strategies. The first one employs a recently synthesized phlorin with two different excited states above the conduction <span class="hlt">band</span> of TiO2. This molecule allows comparing HET rates from two different excited states. The second strategy measures the <span class="hlt">electron</span> injection rates after exciting the same <span class="hlt">electronic</span> state of a set of specially designed porphyrins. The novelty of the approach is that the difference in <span class="hlt">energy</span> alignment is attained by the introduction of dipole groups within the bridge group of the molecule. This strategy generates a difference in <span class="hlt">energy</span> alignment of up to 200 meV. The reported measurements were carried in a high vacuum environment with an apparatus capable of resolving sub 30 fs processes. Disentanglement of the <span class="hlt">electron</span> transfer processes was done, after careful study of the relaxation dynamics of the molecules in solution, by monitoring the decay of the excited state absorption and the rise of the cation spectral signatures. Within our time resolution, our results</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JPSJ...87d4701S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JPSJ...87d4701S"><span>Valence-<span class="hlt">Band</span> <span class="hlt">Electronic</span> Structures of High-Pressure-Phase PdF2-type Platinum-Group Metal Dioxides MO2 (M = Ru, Rh, Ir, and Pt)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Soda, Kazuo; Kobayashi, Daichi; Mizui, Tatsuya; Kato, Masahiko; Shirako, Yuichi; Niwa, Ken; Hasegawa, Masashi; Akaogi, Masaki; Kojitani, Hiroshi; Ikenaga, Eiji; Muro, Takayuki</p> <p>2018-04-01</p> <p>The valence-<span class="hlt">band</span> <span class="hlt">electronic</span> structures of high-pressure-phase PdF2-type (HP-PdF2-type) platinum-group metal dioxides MO2 (M = Ru, Rh, Ir, and Pt) were studied by synchrotron radiation photoelectron spectroscopy and first-principles calculations. The obtained photoelectron spectra for HP-PdF2-type RuO2, RhO2, and IrO2 agree well with the calculated valence-<span class="hlt">band</span> densities of states (DOSs) for these compounds, indicating their metallic properties, whereas the DOS of HP-PdF2-type PtO2 (calculated in the presence and absence of spin-orbit interactions) predicts that this material may be metallic or semimetallic, which is inconsistent with the electric conductivity reported to date and the charging effect observed in current photoelectron measurements. Compared with the calculated results, the valence-<span class="hlt">band</span> spectrum of PtO2 appears to have shifted toward the high-binding-<span class="hlt">energy</span> side and reveals a gradual intensity decrease toward the Fermi <span class="hlt">energy</span> EF, implying a semiconductor-like <span class="hlt">electronic</span> structure. Spin-dependent calculations predict a ferromagnetic ground state with a magnetization of 0.475 μB per formula unit for HP-PdF2-type RhO2.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018CPL...701..126D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018CPL...701..126D"><span><span class="hlt">Electron</span> transfer dynamics and yield from gold nanoparticle to different semiconductors induced by plasmon <span class="hlt">band</span> excitation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Du, L. C.; Xi, W. D.; Zhang, J. B.; Matsuzaki, H.; Furube, A.</p> <p>2018-06-01</p> <p>Photoinduced <span class="hlt">electron</span> transfer from gold nanoparticles (NPs) to semiconductor under plasmon excitation is an important phenomenon in photocatalysis and solar cell applications. Femtosecond plasmon-induced <span class="hlt">electron</span> transfer from gold NPs to the conduction <span class="hlt">band</span> of different semiconductor like TiO2, SnO2, and ZnO was monitored at 3440 nm upon optical excitation of the surface plasmon <span class="hlt">band</span> of gold NPs. It was found that <span class="hlt">electron</span> injection was completed within 240 fs and the <span class="hlt">electron</span> injection yield reached 10-30% under 570 nm excitation. It means TiO2 is not the only proper semiconductor as <span class="hlt">electron</span> acceptors in such gold/semiconductor nanoparticle systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015APS..MARM16001J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015APS..MARM16001J"><span>Topologically nontrivial <span class="hlt">electronic</span> <span class="hlt">bands</span> and tunable Dirac cones in graphynes with spin-orbit coupling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Juricic, Vladimir; van Miert, Guido; Morais Smith, Cristiane</p> <p>2015-03-01</p> <p>Graphynes represent an emerging family of carbon allotropes that differ from graphene by the presence of the triple bonds (-C ≡C-) in their <span class="hlt">band</span> structure. They have recently attracted much interest due to the tunability of the Dirac cones in the <span class="hlt">band</span> structure. I will show that the spin-orbit coupling in β-graphyne could produce various effects related to the topological properties of its <span class="hlt">electronic</span> <span class="hlt">bands</span>. Intrinsic spin-orbit coupling yields high- and tunable Chern-number <span class="hlt">bands</span>, which may host both topological and Chern insulators, in the presence and absence of time-reversal symmetry, respectively. Furthermore, Rashba spin-orbit coupling can be used to control the position and the number of Dirac cones in the Brillouin zone. Finally, I will also discuss the <span class="hlt">electronic</span> properties of α - and γ - graphyne in the presence of the spin-orbit coupling within recently developed general theory of spin-orbit couplings in graphynes. Work supported by the Netherlands Organization for Scientific Research (NWO).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015OptMa..42..351L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015OptMa..42..351L"><span><span class="hlt">Electronic</span> structure and optical properties of Cs2HgI4: Experimental study and <span class="hlt">band</span>-structure DFT calculations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lavrentyev, A. A.; Gabrelian, B. V.; Vu, V. T.; Shkumat, P. N.; Myronchuk, G. L.; Khvyshchun, M.; Fedorchuk, A. O.; Parasyuk, O. V.; Khyzhun, O. Y.</p> <p>2015-04-01</p> <p>High-quality single crystal of cesium mercury tetraiodide, Cs2HgI4, has been synthesized by the vertical Bridgman-Stockbarger method and its crystal structure has been refined. In addition, <span class="hlt">electronic</span> structure and optical properties of Cs2HgI4 have been studied. For the crystal under study, X-ray photoelectron core-level and valence-<span class="hlt">band</span> spectra for pristine and Ar+-ion irradiated surfaces have been measured. The present X-ray photoelectron spectroscopy (XPS) results indicate that the Cs2HgI4 single crystal surface is very sensitive with respect to Ar+ ion-irradiation. In particular, Ar+ bombardment of the single crystal surface alters the elemental stoichiometry of the Cs2HgI4 surface. To elucidate peculiarities of the <span class="hlt">energy</span> distribution of the <span class="hlt">electronic</span> states within the valence-<span class="hlt">band</span> and conduction-<span class="hlt">band</span> regions of the Cs2HgI4 compound, we have performed first-principles <span class="hlt">band</span>-structure calculations based on density functional theory (DFT) as incorporated in the WIEN2k package. Total and partial densities of states for Cs2HgI4 have been calculated. The DFT calculations reveal that the I p states make the major contributions in the upper portion of the valence <span class="hlt">band</span>, while the Hg d, Cs p and I s states are the dominant contributors in its lower portion. Temperature dependence of the light absorption coefficient and specific electrical conductivity has been explored for Cs2HgI4 in the temperature range of 77-300 K. Main optical characteristics of the Cs2HgI4 compound have been elucidated by the first-principles calculations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25247447','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25247447"><span><span class="hlt">Energy</span> <span class="hlt">band</span> gap and optical transition of metal ion modified double crossover DNA lattices.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Dugasani, Sreekantha Reddy; Ha, Taewoo; Gnapareddy, Bramaramba; Choi, Kyujin; Lee, Junwye; Kim, Byeonghoon; Kim, Jae Hoon; Park, Sung Ha</p> <p>2014-10-22</p> <p>We report on the <span class="hlt">energy</span> <span class="hlt">band</span> gap and optical transition of a series of divalent metal ion (Cu(2+), Ni(2+), Zn(2+), and Co(2+)) modified DNA (M-DNA) double crossover (DX) lattices fabricated on fused silica by the substrate-assisted growth (SAG) method. We demonstrate how the degree of coverage of the DX lattices is influenced by the DX monomer concentration and also analyze the <span class="hlt">band</span> gaps of the M-DNA lattices. The <span class="hlt">energy</span> <span class="hlt">band</span> gap of the M-DNA, between the lowest unoccupied molecular orbital (LUMO) and the highest occupied molecular orbital (HOMO), ranges from 4.67 to 4.98 eV as judged by optical transitions. Relative to the <span class="hlt">band</span> gap of a pristine DNA molecule (4.69 eV), the <span class="hlt">band</span> gap of the M-DNA lattices increases with metal ion doping up to a critical concentration and then decreases with further doping. Interestingly, except for the case of Ni(2+), the onset of the second absorption <span class="hlt">band</span> shifts to a lower <span class="hlt">energy</span> until a critical concentration and then shifts to a higher <span class="hlt">energy</span> with further increasing the metal ion concentration, which is consistent with the evolution of electrical transport characteristics. Our results show that controllable metal ion doping is an effective method to tune the <span class="hlt">band</span> gap <span class="hlt">energy</span> of DNA-based nanostructures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016OptMa..53..134K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016OptMa..53..134K"><span>Effects of optical <span class="hlt">band</span> gap <span class="hlt">energy</span>, <span class="hlt">band</span> tail <span class="hlt">energy</span> and particle shape on photocatalytic activities of different ZnO nanostructures prepared by a hydrothermal method</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Klubnuan, Sarunya; Suwanboon, Sumetha; Amornpitoksuk, Pongsaton</p> <p>2016-03-01</p> <p>The dependence of the crystallite size and the <span class="hlt">band</span> tail <span class="hlt">energy</span> on the optical properties, particle shape and oxygen vacancy of different ZnO nanostructures to catalyse photocatalytic degradation was investigated. The ZnO nanoplatelets and mesh-like ZnO lamellae were synthesized from the PEO19-b-PPO3 modified zinc acetate dihydrate using aqueous KOH and CO(NH2)2 solutions, respectively via a hydrothermal method. The <span class="hlt">band</span> tail <span class="hlt">energy</span> of the ZnO nanostructures had more influence on the <span class="hlt">band</span> gap <span class="hlt">energy</span> than the crystallite size. The photocatalytic degradation of methylene blue increased as a function of the irradiation time, the amount of oxygen vacancy and the intensity of the (0 0 0 2) plane. The ZnO nanoplatelets exhibited a better photocatalytic degradation of methylene blue than the mesh-like ZnO lamellae due to the migration of the photoelectrons and holes to the (0 0 0 1) and (0 0 0 -1) planes, respectively under the internal electric field, that resulted in the enhancement of the photocatalytic activities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26222731','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26222731"><span>On Valence-<span class="hlt">Band</span> Splitting in Layered MoS2.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhang, Youwei; Li, Hui; Wang, Haomin; Liu, Ran; Zhang, Shi-Li; Qiu, Zhi-Jun</p> <p>2015-08-25</p> <p>As a representative two-dimensional semiconducting transition-metal dichalcogenide (TMD), the <span class="hlt">electronic</span> structure in layered MoS2 is a collective result of quantum confinement, interlayer interaction, and crystal symmetry. A prominent <span class="hlt">energy</span> splitting in the valence <span class="hlt">band</span> gives rise to many intriguing <span class="hlt">electronic</span>, optical, and magnetic phenomena. Despite numerous studies, an experimental determination of valence-<span class="hlt">band</span> splitting in few-layer MoS2 is still lacking. Here, we show how the valence-<span class="hlt">band</span> maximum (VBM) splits for one to five layers of MoS2. Interlayer coupling is found to contribute significantly to phonon <span class="hlt">energy</span> but weakly to VBM splitting in bilayers, due to a small interlayer hopping <span class="hlt">energy</span> for holes. Hence, spin-orbit coupling is still predominant in the splitting. A temperature-independent VBM splitting, known for single-layer MoS2, is, thus, observed for bilayers. However, a Bose-Einstein type of temperature dependence of VBM splitting prevails in three to five layers of MoS2. In such few-layer MoS2, interlayer coupling is enhanced with a reduced interlayer distance, but thermal expansion upon temperature increase tends to decouple adjacent layers and therefore decreases the splitting <span class="hlt">energy</span>. Our findings that shed light on the distinctive behaviors about VBM splitting in layered MoS2 may apply to other hexagonal TMDs as well. They will also be helpful in extending our understanding of the TMD <span class="hlt">electronic</span> structure for potential applications in <span class="hlt">electronics</span> and optoelectronics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EPJB...85..324G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EPJB...85..324G"><span>Plasmon satellites in valence-<span class="hlt">band</span> photoemission spectroscopy. Ab initio study of the photon-<span class="hlt">energy</span> dependence in semiconductors</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Guzzo, M.; Kas, J. J.; Sottile, F.; Silly, M. G.; Sirotti, F.; Rehr, J. J.; Reining, L.</p> <p>2012-09-01</p> <p>We present experimental data and theoretical results for valence-<span class="hlt">band</span> satellites in semiconductors, using the prototypical example of bulk silicon. In a previous publication we introduced a new approach that allows us to describe satellites in valence photoemission spectroscopy, in good agreement with experiment. Here we give more details; we show how the the spectra change with photon <span class="hlt">energy</span>, and how the theory explains this behaviour. We also describe how we include several effects which are important to obtain a correct comparison between theory and experiment, such as secondary <span class="hlt">electrons</span> and photon cross sections. In particular the inclusion of extrinsic losses and their dependence on the photon <span class="hlt">energy</span> are key to the description of the <span class="hlt">energy</span> dependence of spectra.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JPCM...28r5501L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JPCM...28r5501L"><span>The <span class="hlt">electronic</span> <span class="hlt">band</span> structures of gadolinium chalcogenides: a first-principles prediction for neutron detecting</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Kexue; Liu, Lei; Yu, Peter Y.; Chen, Xiaobo; Shen, D. Z.</p> <p>2016-05-01</p> <p>By converting the <span class="hlt">energy</span> of nuclear radiation to excited <span class="hlt">electrons</span> and holes, semiconductor detectors have provided a highly efficient way for detecting them, such as photons or charged particles. However, for detecting the radiated neutrons, those conventional semiconductors hardly behave well, as few of them possess enough capability for capturing these neutral particles. While the element Gd has the highest nuclear cross section, here for searching proper neutron-detecting semiconductors, we investigate theoretically the Gd chalcogenides whose <span class="hlt">electronic</span> <span class="hlt">band</span> structures have never been characterized clearly. Among them, we identify that γ-phase Gd2Se3 should be the best candidate for neutron detecting since it possesses not only the right bandgap of 1.76 eV for devices working under room temperature but also the desired indirect gap nature for charge carriers surviving longer. We propose further that semiconductor neutron detectors with single-neutron sensitivity can be realized with such a Gd-chalcogenide on the condition that their crystals can be grown with good quality.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27049355','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27049355"><span>The <span class="hlt">electronic</span> <span class="hlt">band</span> structures of gadolinium chalcogenides: a first-principles prediction for neutron detecting.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Li, Kexue; Liu, Lei; Yu, Peter Y; Chen, Xiaobo; Shen, D Z</p> <p>2016-05-11</p> <p>By converting the <span class="hlt">energy</span> of nuclear radiation to excited <span class="hlt">electrons</span> and holes, semiconductor detectors have provided a highly efficient way for detecting them, such as photons or charged particles. However, for detecting the radiated neutrons, those conventional semiconductors hardly behave well, as few of them possess enough capability for capturing these neutral particles. While the element Gd has the highest nuclear cross section, here for searching proper neutron-detecting semiconductors, we investigate theoretically the Gd chalcogenides whose <span class="hlt">electronic</span> <span class="hlt">band</span> structures have never been characterized clearly. Among them, we identify that γ-phase Gd2Se3 should be the best candidate for neutron detecting since it possesses not only the right bandgap of 1.76 eV for devices working under room temperature but also the desired indirect gap nature for charge carriers surviving longer. We propose further that semiconductor neutron detectors with single-neutron sensitivity can be realized with such a Gd-chalcogenide on the condition that their crystals can be grown with good quality.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1259764-electronic-structure-descriptor-discovery-narrow-band-red-emitting-phosphors','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1259764-electronic-structure-descriptor-discovery-narrow-band-red-emitting-phosphors"><span><span class="hlt">Electronic</span> structure descriptor for the discovery of narrow-<span class="hlt">band</span> red-emitting phosphors</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Wang, Zhenbin; Chu, Iek -Heng; Zhou, Fei; ...</p> <p>2016-05-09</p> <p>Narrow-<span class="hlt">band</span> red-emitting phosphors are a critical component of phosphor-converted light-emitting diodes for highly efficient illumination-grade lighting. In this work, we report the discovery of a quantitative descriptor for narrow-<span class="hlt">band</span> Eu 2+-activated emission identified through a comparison of the <span class="hlt">electronic</span> structures of known narrow-<span class="hlt">band</span> and broad-<span class="hlt">band</span> phosphors. We find that a narrow emission bandwidth is characterized by a large splitting of more than 0.1 eV between the two highest Eu 2+ 4 f 7 <span class="hlt">bands</span>. By incorporating this descriptor in a high-throughput first-principles screening of 2259 nitride compounds, we identify five promising new nitride hosts for Eu 2+-activated red-emitting phosphors thatmore » are predicted to exhibit good chemical stability, thermal quenching resistance, and quantum efficiency, as well as narrow-<span class="hlt">band</span> emission. Lastly, our findings provide important insights into the emission characteristics of rare-earth activators in phosphor hosts and a general strategy to the discovery of phosphors with a desired emission peak and bandwidth.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1259764','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1259764"><span><span class="hlt">Electronic</span> structure descriptor for the discovery of narrow-<span class="hlt">band</span> red-emitting phosphors</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Wang, Zhenbin; Chu, Iek -Heng; Zhou, Fei</p> <p></p> <p>Narrow-<span class="hlt">band</span> red-emitting phosphors are a critical component of phosphor-converted light-emitting diodes for highly efficient illumination-grade lighting. In this work, we report the discovery of a quantitative descriptor for narrow-<span class="hlt">band</span> Eu 2+-activated emission identified through a comparison of the <span class="hlt">electronic</span> structures of known narrow-<span class="hlt">band</span> and broad-<span class="hlt">band</span> phosphors. We find that a narrow emission bandwidth is characterized by a large splitting of more than 0.1 eV between the two highest Eu 2+ 4 f 7 <span class="hlt">bands</span>. By incorporating this descriptor in a high-throughput first-principles screening of 2259 nitride compounds, we identify five promising new nitride hosts for Eu 2+-activated red-emitting phosphors thatmore » are predicted to exhibit good chemical stability, thermal quenching resistance, and quantum efficiency, as well as narrow-<span class="hlt">band</span> emission. Lastly, our findings provide important insights into the emission characteristics of rare-earth activators in phosphor hosts and a general strategy to the discovery of phosphors with a desired emission peak and bandwidth.« less</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_11 --> <div id="page_12" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="221"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22661508-suprathermal-electron-strahl-widths-presence-narrow-band-whistler-waves-solar-wind','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22661508-suprathermal-electron-strahl-widths-presence-narrow-band-whistler-waves-solar-wind"><span>SUPRATHERMAL <span class="hlt">ELECTRON</span> STRAHL WIDTHS IN THE PRESENCE OF NARROW-<span class="hlt">BAND</span> WHISTLER WAVES IN THE SOLAR WIND</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Kajdič, P.; Alexandrova, O.; Maksimovic, M.</p> <p>2016-12-20</p> <p>We perform the first statistical study of the effects of the interaction of suprathermal <span class="hlt">electrons</span> with narrow-<span class="hlt">band</span> whistler mode waves in the solar wind (SW). We show that this interaction does occur and that it is associated with enhanced widths of the so-called strahl component. The latter is directed along the interplanetary magnetic field away from the Sun. We do the study by comparing the strahl pitch angle widths in the SW at 1 AU in the absence of large scale discontinuities and transient structures, such as interplanetary shocks, interplanetary coronal mass ejections, stream interaction regions, etc. during times whenmore » the whistler mode waves were present and when they were absent. This is done by using the data from two Cluster instruments: Spatio Temporal Analysis of Field Fluctuations experiment (STAFF) data in the frequency range between ∼0.1 and ∼200 Hz were used for determining the wave properties and Plasma <span class="hlt">Electron</span> And Current Experiment (PEACE) data sets at 12 central <span class="hlt">energies</span> between ∼57 eV (equivalent to ∼10 typical <span class="hlt">electron</span> thermal <span class="hlt">energies</span> in the SW, E{sub T}) and ∼676 eV (∼113 E{sub T}) for pitch angle measurements. Statistical analysis shows that, during the intervals with the whistler waves, the strahl component on average exhibits pitch angle widths between 2° and 12° larger than during the intervals when these waves are not present. The largest difference is obtained for the <span class="hlt">electron</span> central <span class="hlt">energy</span> of ∼344 eV (∼57 ET).« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=%22light-emitting+diode%22+OR+lighting&pg=3&id=EJ829407','ERIC'); return false;" href="https://eric.ed.gov/?q=%22light-emitting+diode%22+OR+lighting&pg=3&id=EJ829407"><span>Simple Experimental Verification of the Relation between the <span class="hlt">Band</span>-Gap <span class="hlt">Energy</span> and the <span class="hlt">Energy</span> of Photons Emitted by LEDs</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Precker, Jurgen W.</p> <p>2007-01-01</p> <p>The wavelength of the light emitted by a light-emitting diode (LED) is intimately related to the <span class="hlt">band</span>-gap <span class="hlt">energy</span> of the semiconductor from which the LED is made. We experimentally estimate the <span class="hlt">band</span>-gap <span class="hlt">energies</span> of several types of LEDs, and compare them with the <span class="hlt">energies</span> of the emitted light, which ranges from infrared to white. In spite of…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvB..97p5130E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvB..97p5130E"><span>Location of the valence <span class="hlt">band</span> maximum in the <span class="hlt">band</span> structure of anisotropic 1 T'-ReSe2</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Eickholt, P.; Noky, J.; Schwier, E. F.; Shimada, K.; Miyamoto, K.; Okuda, T.; Datzer, C.; Drüppel, M.; Krüger, P.; Rohlfing, M.; Donath, M.</p> <p>2018-04-01</p> <p>Transition-metal dichalcogenides (TMDCs) are a focus of current research due to their fascinating optical and <span class="hlt">electronic</span> properties with possible technical applications. ReSe2 is an interesting material of the TMDC family, with unique anisotropic properties originating from its distorted 1 T structure (1 T '). To develop a fundamental understanding of the optical and electric properties, we studied the underlying <span class="hlt">electronic</span> structure with angle-resolved photoemission (ARPES) as well as <span class="hlt">band</span>-structure calculations within the density functional theory (DFT)-local density approximation (LDA) and GdW approximations. We identified the Γ ¯M¯1 direction, which is perpendicular to the a axis, as a distinct direction in k space with the smallest bandwidth of the highest valence <span class="hlt">band</span>. Using photon-<span class="hlt">energy</span>-dependent ARPES, two valence <span class="hlt">band</span> maxima are identified within experimental limits of about 50 meV: one at the high-symmetry point Z , and a second one at a non-high-symmetry point in the Brillouin zone. Thus, the position in k space of the global valence <span class="hlt">band</span> maximum is undecided experimentally. Theoretically, an indirect <span class="hlt">band</span> gap is predicted on a DFT-LDA level, while quasiparticle corrections lead to a direct <span class="hlt">band</span> gap at the Z point.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1998RaPC...52...73H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998RaPC...52...73H"><span>Sterilization of foods with low-<span class="hlt">energy</span> <span class="hlt">electrons</span> (``soft-<span class="hlt">electrons</span>'')</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hayashi, Toru; Takahashi, Yoko; Todoriki, Setsuko</p> <p>1998-06-01</p> <p><span class="hlt">Electrons</span> with an <span class="hlt">energy</span> of 300 keV or lower were defined as "Soft-<span class="hlt">electrons</span>", which showed several advantages over conventional irradiation with gamma-rays or high-<span class="hlt">energy</span> <span class="hlt">electrons</span> in decontamination of grains and spices. <span class="hlt">Energies</span> of <span class="hlt">electrons</span> necessary to reduce microbial loads to levels lower than 10 CFU/g were 60 keV for brown rice, 75 keV for wheat, 100 keV for white pepper, coriander and basil, 130 keV for buckwheat, 160 keV for rough rice, and 210 keV for black pepper. <span class="hlt">Electrons</span> with such <span class="hlt">energies</span> did not significantly influence the quality.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1254851','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1254851"><span>Valence-<span class="hlt">band</span> <span class="hlt">electronic</span> structure evolution of graphene oxide upon thermal annealing for optoelectronics</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Yamaguchi, Hisato; Ogawa, Shuichi; Watanabe, Daiki</p> <p></p> <p>We report valence <span class="hlt">band</span> <span class="hlt">electronic</span> structure evolution of graphene oxide (GO) upon its thermal reduction. Degree of oxygen functionalization was controlled by annealing temperatures, and an <span class="hlt">electronic</span> structure evolution was monitored using real-time ultraviolet photoelectron spectroscopy. We observed a drastic increase in density of states around the Fermi level upon thermal annealing at ~600 °C. The result indicates that while there is an apparent <span class="hlt">band</span> gap for GO prior to a thermal reduction, the gap closes after an annealing around that temperature. This trend of <span class="hlt">band</span> gap closure was correlated with electrical, chemical, and structural properties to determine a setmore » of GO material properties that is optimal for optoelectronics. The results revealed that annealing at a temperature of ~500 °C leads to the desired properties, demonstrated by a uniform and an order of magnitude enhanced photocurrent map of an individual GO sheet compared to as-synthesized counterpart.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1254851-valence-band-electronic-structure-evolution-graphene-oxide-upon-thermal-annealing-optoelectronics','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1254851-valence-band-electronic-structure-evolution-graphene-oxide-upon-thermal-annealing-optoelectronics"><span>Valence-<span class="hlt">band</span> <span class="hlt">electronic</span> structure evolution of graphene oxide upon thermal annealing for optoelectronics</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Yamaguchi, Hisato; Ogawa, Shuichi; Watanabe, Daiki; ...</p> <p>2016-09-01</p> <p>We report valence <span class="hlt">band</span> <span class="hlt">electronic</span> structure evolution of graphene oxide (GO) upon its thermal reduction. Degree of oxygen functionalization was controlled by annealing temperatures, and an <span class="hlt">electronic</span> structure evolution was monitored using real-time ultraviolet photoelectron spectroscopy. We observed a drastic increase in density of states around the Fermi level upon thermal annealing at ~600 °C. The result indicates that while there is an apparent <span class="hlt">band</span> gap for GO prior to a thermal reduction, the gap closes after an annealing around that temperature. This trend of <span class="hlt">band</span> gap closure was correlated with electrical, chemical, and structural properties to determine a setmore » of GO material properties that is optimal for optoelectronics. The results revealed that annealing at a temperature of ~500 °C leads to the desired properties, demonstrated by a uniform and an order of magnitude enhanced photocurrent map of an individual GO sheet compared to as-synthesized counterpart.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1393189-shear-band-thickness-shear-band-cavities-zr-based-metallic-glass','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1393189-shear-band-thickness-shear-band-cavities-zr-based-metallic-glass"><span>Shear-<span class="hlt">band</span> thickness and shear-<span class="hlt">band</span> cavities in a Zr-based metallic glass</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Liu, C.; Roddatis, V.; Kenesei, P.; ...</p> <p>2017-08-14</p> <p>Strain localization into shear <span class="hlt">bands</span> in metallic glasses is typically described as a mechanism that occurs at the nano-scale, leaving behind a shear defect with a thickness of 10–20 nm. Here we sample the structure of a single system-spanning shear <span class="hlt">band</span> that has carried all plastic flow with high-angle annular dark field scanning transmission <span class="hlt">electron</span> microscopy (HAADF-STEM) and high-<span class="hlt">energy</span> x-ray tomography (XRT). It is found that the shear-<span class="hlt">band</span> thickness and the density change relative to the matrix sensitively depend on position along the shear <span class="hlt">band</span>. A wide distribution of shear-<span class="hlt">band</span> thickness (10 nm–210 nm) and density change (–1% to –12%)more » is revealed. There is no obvious correlation between shear-<span class="hlt">band</span> thickness and density change, but larger thicknesses correspond typically to higher density changes. More than 100 micron-size shear-<span class="hlt">band</span> cavities were identified on the shear-<span class="hlt">band</span> plane, and their three-dimensional arrangement suggests a strongly fluctuating local curvature of the shear plane. As a result, these findings urge for a more complex view of a shear <span class="hlt">band</span> than a simple nano-scale planar defect.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1393189-shear-band-thickness-shear-band-cavities-zr-based-metallic-glass','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1393189-shear-band-thickness-shear-band-cavities-zr-based-metallic-glass"><span>Shear-<span class="hlt">band</span> thickness and shear-<span class="hlt">band</span> cavities in a Zr-based metallic glass</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Liu, C.; Roddatis, V.; Kenesei, P.</p> <p></p> <p>Strain localization into shear <span class="hlt">bands</span> in metallic glasses is typically described as a mechanism that occurs at the nano-scale, leaving behind a shear defect with a thickness of 10–20 nm. Here we sample the structure of a single system-spanning shear <span class="hlt">band</span> that has carried all plastic flow with high-angle annular dark field scanning transmission <span class="hlt">electron</span> microscopy (HAADF-STEM) and high-<span class="hlt">energy</span> x-ray tomography (XRT). It is found that the shear-<span class="hlt">band</span> thickness and the density change relative to the matrix sensitively depend on position along the shear <span class="hlt">band</span>. A wide distribution of shear-<span class="hlt">band</span> thickness (10 nm–210 nm) and density change (–1% to –12%)more » is revealed. There is no obvious correlation between shear-<span class="hlt">band</span> thickness and density change, but larger thicknesses correspond typically to higher density changes. More than 100 micron-size shear-<span class="hlt">band</span> cavities were identified on the shear-<span class="hlt">band</span> plane, and their three-dimensional arrangement suggests a strongly fluctuating local curvature of the shear plane. As a result, these findings urge for a more complex view of a shear <span class="hlt">band</span> than a simple nano-scale planar defect.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17280325','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17280325"><span>Production of photocurrent due to intermediate-to-conduction-<span class="hlt">band</span> transitions: a demonstration of a key operating principle of the intermediate-<span class="hlt">band</span> solar cell.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Martí, A; Antolín, E; Stanley, C R; Farmer, C D; López, N; Díaz, P; Cánovas, E; Linares, P G; Luque, A</p> <p>2006-12-15</p> <p>We present intermediate-<span class="hlt">band</span> solar cells manufactured using quantum dot technology that show for the first time the production of photocurrent when two sub-<span class="hlt">band</span>-gap <span class="hlt">energy</span> photons are absorbed simultaneously. One photon produces an optical transition from the intermediate-<span class="hlt">band</span> to the conduction <span class="hlt">band</span> while the second pumps an <span class="hlt">electron</span> from the valence <span class="hlt">band</span> to the intermediate-<span class="hlt">band</span>. The detection of this two-photon absorption process is essential to verify the principles of operation of the intermediate-<span class="hlt">band</span> solar cell. The phenomenon is the cornerstone physical principle that ultimately allows the production of photocurrent in a solar cell by below <span class="hlt">band</span> gap photon absorption, without degradation of its output voltage.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..MAR.Y6002G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..MAR.Y6002G"><span>Phonon-induced ultrafast <span class="hlt">band</span> gap control in LaTiO3</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gu, Mingqiang; Rondinelli, James M.</p> <p></p> <p>We propose a route for ultrafast <span class="hlt">band</span> gap engineering in correlated transition metal oxides by using optically driven phonons. We show that the ∖Gamma-point <span class="hlt">electron</span> <span class="hlt">band</span> <span class="hlt">energies</span> can be deterministically tuned in the nonequilibrium state. Taking the Mott insulator LaTiO3 as an example, we show that such phonon-assisted processes dynamically induce an indirect-to-direct <span class="hlt">band</span> gap transition or even a metal-to-insulator transition, depending on the <span class="hlt">electron</span> correlation strength. We explain the origin of the dynamical <span class="hlt">band</span> structure control and also establish its generality by examining related oxides. Lastly, we describe experimental routes to realize the <span class="hlt">band</span> structure control with impulsive stimulated Raman scattering.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017IJMPB..3150095O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017IJMPB..3150095O"><span>The angular <span class="hlt">electronic</span> <span class="hlt">band</span> structure and free particle model of aromatic molecules: High-frequency photon-induced ring current</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Öncan, Mehmet; Koç, Fatih; Şahin, Mehmet; Köksal, Koray</p> <p>2017-05-01</p> <p>This work introduces an analysis of the relationship of first-principles calculations based on DFT method with the results of free particle model for ring-shaped aromatic molecules. However, the main aim of the study is to reveal the angular <span class="hlt">electronic</span> <span class="hlt">band</span> structure of the ring-shaped molecules. As in the case of spherical molecules such as fullerene, it is possible to observe a parabolic dispersion of <span class="hlt">electronic</span> states with the variation of angular quantum number in the planar ring-shaped molecules. This work also discusses the transition probabilities between the occupied and virtual states by analyzing the angular <span class="hlt">electronic</span> <span class="hlt">band</span> structure and the possibility of ring currents in the case of spin angular momentum (SAM) or orbital angular momentum (OAM) carrying light. Current study focuses on the benzene molecule to obtain its angular <span class="hlt">electronic</span> <span class="hlt">band</span> structure. The obtained <span class="hlt">electronic</span> <span class="hlt">band</span> structure can be considered as a useful tool to see the transition probabilities between the <span class="hlt">electronic</span> states and possible contribution of the states to the ring currents. The photoinduced current due to the transfer of SAM into the benzene molecule has been investigated by using analytical calculations within the frame of time-dependent perturbation theory.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015MNRAS.452.3666S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015MNRAS.452.3666S"><span><span class="hlt">Energy</span> dependence of the <span class="hlt">band</span>-limited noise in black hole X-ray binaries★</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stiele, H.; Yu, W.</p> <p>2015-10-01</p> <p>Black hole low-mass X-ray binaries show a variety of variability features, which manifest as narrow peak-like structures superposed on broad noise components in power density spectra in the hard X-ray emission. In this work, we study variability properties of the <span class="hlt">band</span>-limited noise component during the low-hard state for a sample of black hole X-ray binaries. We investigate the characteristic frequency and amplitude of the <span class="hlt">band</span>-limited noise component and study covariance spectra. For observations that show a noise component with a characteristic frequency above 1 Hz in the hard <span class="hlt">energy</span> <span class="hlt">band</span> (4-8 keV), we found this very same component at a lower frequency in the soft <span class="hlt">band</span> (1-2 keV). This difference in characteristic frequency is an indication that while both the soft and the hard <span class="hlt">band</span> photons contribute to the same <span class="hlt">band</span>-limited noise component, which likely represents the modulation of the mass accretion rate, the origin of the soft photons is actually further away from the black hole than the hard photons. Thus, the soft photons are characterized by larger radii, lower frequencies and softer <span class="hlt">energies</span>, and are probably associated with a smaller optical depth for Comptonization up-scattering from the outer layer of the corona, or suggest a temperature gradient of the corona. We interpret this <span class="hlt">energy</span> dependence within the picture of <span class="hlt">energy</span>-dependent power density states as a hint that the contribution of the up-scattered photons originating in the outskirts of the Comptonizing corona to the overall emission in the soft <span class="hlt">band</span> is becoming significant.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..MARH47005T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..MARH47005T"><span>New insights into the opening <span class="hlt">band</span> gap of graphene oxides</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tran, Ngoc Thanh Thuy; Lin, Shih-Yang; Lin, Ming-Fa</p> <p></p> <p><span class="hlt">Electronic</span> properties of oxygen absorbed few-layer graphenes are investigated using first-principle calculations. They are very sensitive to the changes in the oxygen concentration, number of graphene layer, and stacking configuration. The feature-rich <span class="hlt">band</span> structures exhibit the destruction or distortion of the Dirac cone, opening of <span class="hlt">band</span> gap, anisotropic <span class="hlt">energy</span> dispersions, O- and (C,O)-dominated <span class="hlt">energy</span> dispersions, and extra critical points. The <span class="hlt">band</span> decomposed charge distributions reveal the π-bonding dominated <span class="hlt">energy</span> gap. The orbital-projected density of states (DOS) have many special structures mainly coming from a composite <span class="hlt">energy</span> <span class="hlt">band</span>, the parabolic and partially flat ones. The DOS and spatial charge distributions clearly indicate the critical orbital hybridizations in O-O, C-O and C-C bonds, being responsible for the diversified properties. All of the few-layer graphene oxides are semi-metals except for the semiconducting monolayer ones.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PhRvB..94k5135N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhRvB..94k5135N"><span>Influence of Fröhlich polaron coupling on renormalized <span class="hlt">electron</span> <span class="hlt">bands</span> in polar semiconductors: Results for zinc-blende GaN</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nery, Jean Paul; Allen, Philip B.</p> <p>2016-09-01</p> <p>We develop a simple method to study the zero-point and thermally renormalized <span class="hlt">electron</span> <span class="hlt">energy</span> ɛk n(T ) for k n the conduction <span class="hlt">band</span> minimum or valence maximum in polar semiconductors. We use the adiabatic approximation, including an imaginary broadening parameter i δ to suppress noise in the density-functional integrations. The finite δ also eliminates the polar divergence which is an artifact of the adiabatic approximation. Nonadiabatic Fröhlich polaron methods then provide analytic expressions for the missing part of the contribution of the problematic optical phonon mode. We use this to correct the renormalization obtained from the adiabatic approximation. Test calculations are done for zinc-blende GaN for an 18 ×18 ×18 integration grid. The Fröhlich correction is of order -0.02 eV for the zero-point <span class="hlt">energy</span> shift of the conduction <span class="hlt">band</span> minimum, and +0.03 eV for the valence <span class="hlt">band</span> maximum; the correction to renormalization of the 3.28 eV gap is -0.05 eV, a significant fraction of the total zero point renormalization of -0.15 eV.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGRD..12111852T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGRD..12111852T"><span>Mesospheric ozone destruction by high-<span class="hlt">energy</span> <span class="hlt">electron</span> precipitation associated with pulsating aurora</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Turunen, Esa; Kero, Antti; Verronen, Pekka T.; Miyoshi, Yoshizumi; Oyama, Shin-Ichiro; Saito, Shinji</p> <p>2016-10-01</p> <p>Energetic particle precipitation into the upper atmosphere creates excess amounts of odd nitrogen and odd hydrogen. These destroy mesospheric and upper stratospheric ozone in catalytic reaction chains, either in situ at the altitude of the <span class="hlt">energy</span> deposition or indirectly due to transport to other altitudes and latitudes. Recent statistical analysis of satellite data on mesospheric ozone reveals that the variations during energetic <span class="hlt">electron</span> precipitation from Earth's radiation belts can be tens of percent. Here we report model calculations of ozone destruction due to a single event of pulsating aurora early in the morning on 17 November 2012. The presence of high-<span class="hlt">energy</span> component in the precipitating <span class="hlt">electron</span> flux (>200 keV) was detected as ionization down to 68 km altitude, by the VHF incoherent scatter radar of European Incoherent Scatter (EISCAT) Scientific Association (EISCAT VHF) in Tromsø, Norway. Observations by the Van Allen Probes satellite B showed the occurrence of rising tone lower <span class="hlt">band</span> chorus waves, which cause the precipitation. We model the effect of high-<span class="hlt">energy</span> <span class="hlt">electron</span> precipitation on ozone concentration using a detailed coupled ion and neutral chemistry model. Due to a 30 min, recorded <span class="hlt">electron</span> precipitation event we find 14% odd oxygen depletion at 75 km altitude. The uncertainty of the higher-<span class="hlt">energy</span> <span class="hlt">electron</span> fluxes leads to different possible <span class="hlt">energy</span> deposition estimates during the pulsating aurora event. We find depletion of odd oxygen by several tens of percent, depending on the precipitation characteristics used in modeling. The effect is notably maximized at the sunset time following the occurrence of the precipitation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvB..97d1203Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvB..97d1203Z"><span>Flat <span class="hlt">band</span> in disorder-driven non-Hermitian Weyl semimetals</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zyuzin, A. A.; Zyuzin, A. Yu.</p> <p>2018-01-01</p> <p>We study the interplay of disorder and <span class="hlt">band</span>-structure topology in a Weyl semimetal with a tilted conical spectrum around the Weyl points. The spectrum of particles is given by the eigenvalues of a non-Hermitian matrix, which contains contributions from a Weyl Hamiltonian and complex self-<span class="hlt">energy</span> due to <span class="hlt">electron</span> elastic scattering on disorder. We find that the tilt-induced matrix structure of the self-<span class="hlt">energy</span> gives rise to either a flat <span class="hlt">band</span> or a nodal line segment at the interface of the <span class="hlt">electron</span> and hole pockets in the bulk <span class="hlt">band</span> structure of type-II Weyl semimetals depending on the Weyl cone inclination. For the tilt in a single direction in momentum space, each Weyl point expands into a flat <span class="hlt">band</span> lying on the plane, which is transverse to the direction of the tilt. The spectrum of the flat <span class="hlt">band</span> is fully imaginary and is separated from the in-plane dispersive part of the spectrum by the "exceptional nodal ring" where the matrix of the Green's function in momentum-frequency space is defective. The tilt in two directions might shrink a flat <span class="hlt">band</span> into a nodal line segment with "exceptional edge points." We discuss the connection to the non-Hermitian topological theory.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvB..97x5113S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvB..97x5113S"><span>Correlation between superconductivity, <span class="hlt">band</span> filling, and <span class="hlt">electron</span> confinement at the LaAlO3/SrTiO3 interface</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Smink, A. E. M.; Stehno, M. P.; de Boer, J. C.; Brinkman, A.; van der Wiel, W. G.; Hilgenkamp, H.</p> <p>2018-06-01</p> <p>By combined top- and backgating, we explore the correlation of superconductivity with <span class="hlt">band</span> filling and <span class="hlt">electron</span> confinement at the LaAlO3/SrTiO3 interface. We find that the top- and backgate voltages have distinctly different effects on the superconducting critical temperature, implying that the confining potential well has a profound effect on superconductivity. We investigate the origin of this behavior by comparing the gate dependence of Tc to the corresponding evolution of the <span class="hlt">band</span> filling with gate voltage. For several backgate voltages, we observe maximum Tc to consistently coincide with a kink in tuning the <span class="hlt">band</span> filling for high topgate voltage. Self-consistent Schrödinger-Poisson calculations relate this kink to a Lifshitz transition of the second dx y subband. These results establish a major role for confinement-induced subbands in the phase diagram of SrTiO3 surface states, and establish gating as a means to control the relative <span class="hlt">energy</span> of these states.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014PhyE...63..264M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014PhyE...63..264M"><span><span class="hlt">Band</span> gap opening in α-graphyne by adsorption of organic molecule</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Majidi, R.; Karami, A. R.</p> <p>2014-09-01</p> <p>The lack of a <span class="hlt">band</span> gap limits the application of graphyne in nanoelectronic devices. We have investigated possibility of opening a <span class="hlt">band</span> gap in α-graphyne by adsorption of tetracyanoethylene. The <span class="hlt">electronic</span> property of α-graphyne in the presence of different numbers of tetracyanoethylene has been studied using density functional theory. It is found that charge is transferred from graphyne sheet to tetracyanoethylene molecules. In the presence of this <span class="hlt">electron</span> acceptor molecule, a semimetal α-graphyne shows semiconducting property. The <span class="hlt">energy</span> <span class="hlt">band</span> gap at the Dirac point is enhanced by increasing the number of tetracyanoethylene. Our results provide a simple method to create and control the <span class="hlt">band</span> gap in α-graphyne.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016OptMa..58...51C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016OptMa..58...51C"><span>Optical <span class="hlt">band</span> gaps of organic semiconductor materials</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Costa, José C. S.; Taveira, Ricardo J. S.; Lima, Carlos F. R. A. C.; Mendes, Adélio; Santos, Luís M. N. B. F.</p> <p>2016-08-01</p> <p>UV-Vis can be used as an easy and forthright technique to accurately estimate the <span class="hlt">band</span> gap <span class="hlt">energy</span> of organic π-conjugated materials, widely used as thin films/composites in organic and hybrid <span class="hlt">electronic</span> devices such as OLEDs, OPVs and OFETs. The <span class="hlt">electronic</span> and optical properties, including HOMO-LUMO <span class="hlt">energy</span> gaps of π-conjugated systems were evaluated by UV-Vis spectroscopy in CHCl3 solution for a large number of relevant π-conjugated systems: tris-8-hydroxyquinolinatos (Alq3, Gaq3, Inq3, Al(qNO2)3, Al(qCl)3, Al(qBr)3, In(qNO2)3, In(qCl)3 and In(qBr)3); triphenylamine derivatives (DDP, p-TTP, TPB, TPD, TDAB, m-MTDAB, NPB, α-NPD); oligoacenes (naphthalene, anthracene, tetracene and rubrene); oligothiophenes (α-2T, β-2T, α-3T, β-3T, α-4T and α-5T). Additionally, some <span class="hlt">electronic</span> properties were also explored by quantum chemical calculations. The experimental UV-Vis data are in accordance with the DFT predictions and indicate that the <span class="hlt">band</span> gap <span class="hlt">energies</span> of the OSCs dissolved in CHCl3 solution are consistent with the values presented for thin films.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22392404-energy-analyzer-low-energy-electrons','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22392404-energy-analyzer-low-energy-electrons"><span>2-D <span class="hlt">energy</span> analyzer for low <span class="hlt">energy</span> <span class="hlt">electrons</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Karkare, Siddharth, E-mail: ssk226@cornell.edu; Cultrera, Luca; Hwang, Yoon-Woo</p> <p>2015-03-15</p> <p>A 2-D <span class="hlt">electron</span> <span class="hlt">energy</span> analyzer is designed and constructed to measure the transverse and longitudinal <span class="hlt">energy</span> distribution of low <span class="hlt">energy</span> (<1 eV) <span class="hlt">electrons</span>. The analyzer operates on the principle of adiabatic invariance and motion of low <span class="hlt">energy</span> <span class="hlt">electrons</span> in a strong longitudinal magnetic field. The operation of the analyzer is studied in detail and a design to optimize the <span class="hlt">energy</span> resolution, signal to noise ratio, and physical size is presented. An <span class="hlt">energy</span> resolution better than 6 meV has been demonstrated. Such an analyzer is a powerful tool to study the process of photoemission which limits the beam quality in modernmore » accelerators.« less</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_12 --> <div id="page_13" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="241"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22668077','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22668077"><span>Microdosimetry of low-<span class="hlt">energy</span> <span class="hlt">electrons</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Liamsuwan, Thiansin; Emfietzoglou, Dimitris; Uehara, Shuzo; Nikjoo, Hooshang</p> <p>2012-12-01</p> <p>To investigate differences in <span class="hlt">energy</span> depositions and microdosimetric parameters of low-<span class="hlt">energy</span> <span class="hlt">electrons</span> in liquid and gaseous water using Monte Carlo track structure simulations. KURBUC-liq (Kyushu University and Radiobiology Unit Code for liquid water) was used for simulating <span class="hlt">electron</span> tracks in liquid water. The inelastic scattering cross sections of liquid water were obtained from the dielectric response model of Emfietzoglou et al. (Radiation Research 2005;164:202-211). Frequencies of <span class="hlt">energy</span> deposited in nanometre-size cylindrical targets per unit absorbed dose and associated lineal <span class="hlt">energies</span> were calculated for 100-5000 eV monoenergetic <span class="hlt">electrons</span> and the <span class="hlt">electron</span> spectrum of carbon K edge X-rays. The results for liquid water were compared with those for water vapour. Regardless of <span class="hlt">electron</span> <span class="hlt">energy</span>, there is a limit how much <span class="hlt">energy</span> <span class="hlt">electron</span> tracks can deposit in a target. Phase effects on the frequencies of <span class="hlt">energy</span> depositions are largely visible for the targets with diameters and heights smaller than 30 nm. For the target of 2.3 nm by 2.3 nm (similar to dimension of DNA segments), the calculated frequency- and dose-mean lineal <span class="hlt">energies</span> for liquid water are up to 40% smaller than those for water vapour. The corresponding difference is less than 12% for the targets with diameters ≥ 30 nm. Condensed-phase effects are non-negligible for microdosimetry of low-<span class="hlt">energy</span> <span class="hlt">electrons</span> for targets with sizes smaller than a few tens of nanometres, similar to dimensions of DNA molecular structures and nucleosomes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/874723','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/874723"><span>Permanent magnet focused X-<span class="hlt">band</span> photoinjector</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Yu, David U. L.; Rosenzweig, James</p> <p>2002-09-10</p> <p>A compact high <span class="hlt">energy</span> photoelectron injector integrates the photocathode directly into a multicell linear accelerator with no drift space between the injection and the linac. High <span class="hlt">electron</span> beam brightness is achieved by accelerating a tightly focused <span class="hlt">electron</span> beam in an integrated, multi-cell, X-<span class="hlt">band</span> rf linear accelerator (linac). The photoelectron linac employs a Plane-Wave-Transformer (PWT) design which provides strong cell-to-cell coupling, easing manufacturing tolerances and costs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19900033699&hterms=vk&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dvk','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19900033699&hterms=vk&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dvk"><span>Auroral excitation of the N2 2P(0,0) and VK(0,9) <span class="hlt">bands</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Solomon, Stanley C.</p> <p>1989-01-01</p> <p>The low-<span class="hlt">energy</span> secondary <span class="hlt">electron</span> flux caused by auroral <span class="hlt">electron</span> precipitation is examined using data from the Atmosphere Explorer C satellite. An energetic <span class="hlt">electron</span> transport algorithm is used to compute the differential <span class="hlt">electron</span> flux produced by measured primaries. Emissions of N2 in the 2P(0,0) <span class="hlt">band</span> at 337 nm and the VK(0,9) <span class="hlt">band</span> at 335 nm predicted by the model are compared with photometric observation of their combined volume emission rate altitude profile made by the visible airglow experiment. Reasonable correspondence between model and measurement is obtained. Ratios of emissions at 337 nm and 630 nm to the N2(+) 1N(0,0) <span class="hlt">band</span> at 428 nm are also studied. It is concluded that the 337/428 nm ratio responds to changes in the characteristic <span class="hlt">energy</span> of primary auroral <span class="hlt">electrons</span> only insofar as part of the 337 nm brightness is due to N2 VK(0,9) emission. The 630/428 nm ratio, which is strongly dependent on characteristic <span class="hlt">energy</span>, also varies significantly with changes in atomic oxygen density.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2013-title41-vol2/pdf/CFR-2013-title41-vol2-sec101-26-508.pdf','CFR2013'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2013-title41-vol2/pdf/CFR-2013-title41-vol2-sec101-26-508.pdf"><span>41 CFR 101-26.508 - <span class="hlt">Electronic</span> data processing (EDP) tape and instrumentation tape (wide and intermediate <span class="hlt">band</span>).</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2013&page.go=Go">Code of Federal Regulations, 2013 CFR</a></p> <p></p> <p>2013-07-01</p> <p>... processing (EDP) tape and instrumentation tape (wide and intermediate <span class="hlt">band</span>). 101-26.508 Section 101-26.508... Programs § 101-26.508 <span class="hlt">Electronic</span> data processing (EDP) tape and instrumentation tape (wide and intermediate <span class="hlt">band</span>). Procurement by Federal agencies of EDP tape and instrumentation tape (wide and intermediate <span class="hlt">band</span>...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2014-title41-vol2/pdf/CFR-2014-title41-vol2-sec101-26-508.pdf','CFR2014'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2014-title41-vol2/pdf/CFR-2014-title41-vol2-sec101-26-508.pdf"><span>41 CFR 101-26.508 - <span class="hlt">Electronic</span> data processing (EDP) tape and instrumentation tape (wide and intermediate <span class="hlt">band</span>).</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2014&page.go=Go">Code of Federal Regulations, 2014 CFR</a></p> <p></p> <p>2014-07-01</p> <p>... processing (EDP) tape and instrumentation tape (wide and intermediate <span class="hlt">band</span>). 101-26.508 Section 101-26.508... Programs § 101-26.508 <span class="hlt">Electronic</span> data processing (EDP) tape and instrumentation tape (wide and intermediate <span class="hlt">band</span>). Procurement by Federal agencies of EDP tape and instrumentation tape (wide and intermediate <span class="hlt">band</span>...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2010-title41-vol2/pdf/CFR-2010-title41-vol2-sec101-26-508.pdf','CFR'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2010-title41-vol2/pdf/CFR-2010-title41-vol2-sec101-26-508.pdf"><span>41 CFR 101-26.508 - <span class="hlt">Electronic</span> data processing (EDP) tape and instrumentation tape (wide and intermediate <span class="hlt">band</span>).</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2010&page.go=Go">Code of Federal Regulations, 2010 CFR</a></p> <p></p> <p>2010-07-01</p> <p>... processing (EDP) tape and instrumentation tape (wide and intermediate <span class="hlt">band</span>). 101-26.508 Section 101-26.508... Programs § 101-26.508 <span class="hlt">Electronic</span> data processing (EDP) tape and instrumentation tape (wide and intermediate <span class="hlt">band</span>). Procurement by Federal agencies of EDP tape and instrumentation tape (wide and intermediate <span class="hlt">band</span>...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2012-title41-vol2/pdf/CFR-2012-title41-vol2-sec101-26-508.pdf','CFR2012'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2012-title41-vol2/pdf/CFR-2012-title41-vol2-sec101-26-508.pdf"><span>41 CFR 101-26.508 - <span class="hlt">Electronic</span> data processing (EDP) tape and instrumentation tape (wide and intermediate <span class="hlt">band</span>).</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2012&page.go=Go">Code of Federal Regulations, 2012 CFR</a></p> <p></p> <p>2012-07-01</p> <p>... processing (EDP) tape and instrumentation tape (wide and intermediate <span class="hlt">band</span>). 101-26.508 Section 101-26.508... Programs § 101-26.508 <span class="hlt">Electronic</span> data processing (EDP) tape and instrumentation tape (wide and intermediate <span class="hlt">band</span>). Procurement by Federal agencies of EDP tape and instrumentation tape (wide and intermediate <span class="hlt">band</span>...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2011-title41-vol2/pdf/CFR-2011-title41-vol2-sec101-26-508.pdf','CFR2011'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2011-title41-vol2/pdf/CFR-2011-title41-vol2-sec101-26-508.pdf"><span>41 CFR 101-26.508 - <span class="hlt">Electronic</span> data processing (EDP) tape and instrumentation tape (wide and intermediate <span class="hlt">band</span>).</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2011&page.go=Go">Code of Federal Regulations, 2011 CFR</a></p> <p></p> <p>2011-07-01</p> <p>... processing (EDP) tape and instrumentation tape (wide and intermediate <span class="hlt">band</span>). 101-26.508 Section 101-26.508... Programs § 101-26.508 <span class="hlt">Electronic</span> data processing (EDP) tape and instrumentation tape (wide and intermediate <span class="hlt">band</span>). Procurement by Federal agencies of EDP tape and instrumentation tape (wide and intermediate <span class="hlt">band</span>...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JMOp...62.1158R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JMOp...62.1158R"><span>A multi-<span class="hlt">band</span>, multi-level, multi-<span class="hlt">electron</span> model for efficient FDTD simulations of electromagnetic interactions with semiconductor quantum wells</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ravi, Koustuban; Wang, Qian; Ho, Seng-Tiong</p> <p>2015-08-01</p> <p>We report a new computational model for simulations of electromagnetic interactions with semiconductor quantum well(s) (SQW) in complex electromagnetic geometries using the finite-difference time-domain method. The presented model is based on an approach of spanning a large number of <span class="hlt">electron</span> transverse momentum states in each SQW sub-<span class="hlt">band</span> (multi-<span class="hlt">band</span>) with a small number of discrete multi-<span class="hlt">electron</span> states (multi-level, multi-<span class="hlt">electron</span>). This enables accurate and efficient two-dimensional (2-D) and three-dimensional (3-D) simulations of nanophotonic devices with SQW active media. The model includes the following features: (1) Optically induced interband transitions between various SQW conduction and heavy-hole or light-hole sub-<span class="hlt">bands</span> are considered. (2) Novel intra sub-<span class="hlt">band</span> and inter sub-<span class="hlt">band</span> transition terms are derived to thermalize the <span class="hlt">electron</span> and hole occupational distributions to the correct Fermi-Dirac distributions. (3) The terms in (2) result in an explicit update scheme which circumvents numerically cumbersome iterative procedures. This significantly augments computational efficiency. (4) Explicit update terms to account for carrier leakage to unconfined states are derived, which thermalize the bulk and SQW populations to a common quasi-equilibrium Fermi-Dirac distribution. (5) Auger recombination and intervalence <span class="hlt">band</span> absorption are included. The model is validated by comparisons to analytic <span class="hlt">band</span>-filling calculations, simulations of SQW optical gain spectra, and photonic crystal lasers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22608762-effect-doping-electronic-properties-hgse','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22608762-effect-doping-electronic-properties-hgse"><span>Effect of doping on <span class="hlt">electronic</span> properties of HgSe</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Nag, Abhinav, E-mail: abhinavn76@gmail.com; Sastri, O. S. K. S., E-mail: sastri.osks@gmail.com; Kumar, Jagdish, E-mail: jagdishphysicist@gmail.com</p> <p>2016-05-23</p> <p>First principle study of <span class="hlt">electronic</span> properties of pure and doped HgSe have been performed using all <span class="hlt">electron</span> Full Potential Linearized Augmented Plane Wave (FP-LAPW) method using ELK code. The <span class="hlt">electronic</span> exchange and co-relations are considered using Generalized Gradient Approach (GGA). Lattice parameter, Density of States (DOS) and <span class="hlt">Band</span> structure calculations have been performed. The total <span class="hlt">energy</span> curve (<span class="hlt">Energy</span> vs Lattice parameter), DOS and <span class="hlt">band</span> structure calculations are in good agreement with the experimental values and those obtained using other DFT codes. The doped material is studied within the Virtual Crystal Approximation (VCA) with doping levels of 10% to 25% ofmore » <span class="hlt">electrons</span> (hole) per unit cell. Results predict zero <span class="hlt">band</span> gap in undopedHgSe and <span class="hlt">bands</span> meet at Fermi level near the symmetry point Γ. For doped HgSe, we found that by <span class="hlt">electron</span> (hole) doping, the point where conduction and valence <span class="hlt">bands</span> meet can be shifted below (above) the fermi level.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1181633-band-rf-driven-free-electron-laser-driver-optics-linearization','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1181633-band-rf-driven-free-electron-laser-driver-optics-linearization"><span>X -<span class="hlt">band</span> rf driven free <span class="hlt">electron</span> laser driver with optics linearization</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Sun, Yipeng; Emma, Paul; Raubenheimer, Tor; ...</p> <p>2014-11-13</p> <p>In this paper, a compact hard X-ray free <span class="hlt">electron</span> lasers (FEL) design is proposed with all X-<span class="hlt">band</span> rf acceleration and two stage bunch compression. It eliminates the need of a harmonic rf linearization section by employing optics linearization in its first stage bunch compression. Quadrupoles and sextupoles are employed in a bunch compressor one (BC1) design, in such a way that second order longitudinal dispersion of BC1 cancels the second order <span class="hlt">energy</span> correlation in the <span class="hlt">electron</span> beam. Start-to-end 6-D simulations are performed with all the collective effects included. Emittance growth in the horizontal plane due to coherent synchrotron radiation ismore » investigated and minimized, to be on a similar level with the successfully operating Linac coherent light source (LCLS). At a FEL radiation wavelength of 0.15 nm, a saturation length of 40 meters can be achieved by employing an undulator with a period of 1.5 cm. Without tapering, a FEL radiation power above 10 GW is achieved with a photon pulse length of 50 fs, which is LCLS-like performance. The overall length of the accelerator plus undulator is around 250 meters which is much shorter than the LCLS length of 1230 meters. That makes it possible to build hard X-ray FEL in a laboratory with limited size.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JPhD...50zLT02L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JPhD...50zLT02L"><span>First determination of the valence <span class="hlt">band</span> dispersion of CH3NH3PbI3 hybrid organic-inorganic perovskite</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lee, Min-I.; Barragán, Ana; Nair, Maya N.; Jacques, Vincent L. R.; Le Bolloc'h, David; Fertey, Pierre; Jemli, Khaoula; Lédée, Ferdinand; Trippé-Allard, Gaëlle; Deleporte, Emmanuelle; Taleb-Ibrahimi, Amina; Tejeda, Antonio</p> <p>2017-07-01</p> <p>The family of hybrid organic-inorganic halide perovskites is in the limelight because of their recently discovered high photovoltaic efficiency. These materials combine photovoltaic <span class="hlt">energy</span> conversion efficiencies exceeding 22% and low-temperature and low-cost processing in solution; a breakthrough in the panorama of renewable <span class="hlt">energy</span>. Solar cell operation relies on the excitation of the valence <span class="hlt">band</span> <span class="hlt">electrons</span> to the conduction <span class="hlt">band</span> by solar photons. One factor strongly impacting the absorption efficiency is the <span class="hlt">band</span> dispersion. The <span class="hlt">band</span> dispersion has been extensively studied theoretically, but no experimental information was available. Herein, we present the first experimental determination of the valence <span class="hlt">band</span> dispersion of methylammonium lead halide in the tetragonal phase. Our results pave the way for contrasting the <span class="hlt">electronic</span> hopping or the <span class="hlt">electron</span> effective masses in different theories by comparing to our experimental <span class="hlt">bands</span>. We also show a significant broadening of the <span class="hlt">electronic</span> states, promoting relaxed conditions for photon absorption, and demonstrate that the tetragonal structure associated to the octahedra network distortion below 50 °C induces only a minor modification of the <span class="hlt">electronic</span> <span class="hlt">bands</span>, with respect to the cubic phase at high temperature, thus minimizing the impact of the cubic-tetragonal transition on solar cell efficiencies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AIPC.1920b0040S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AIPC.1920b0040S"><span>The effect of carbon nanotubes functionalization on the <span class="hlt">band</span>-gap <span class="hlt">energy</span> of TiO2-CNT nanocomposite</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shahbazi, Hessam; Shafei, Alireza; Sheibani, Saeed</p> <p>2018-01-01</p> <p>In this paper the morphology and structure of TiO2-CNT nanocomposite powder obtained by an in situ sol-gel process were investigated. The synthesized nanocomposite powders were characterized by X-ray diffraction (XRD), field emission scanning <span class="hlt">electron</span> microscopy (FESEM) and diffuse reflectance spectroscopy (DRS). The effect of functionalizing of CNT on the properties was studied. XRD results showed amorphous structure before calcination. Also, anatase phase TiO2 was formed after calcination at 400 °C. The SEM results indicate different distributions of TiO2 on CNTs. As a result, well dispersed TiO2 microstructure on the surface of CNTs was observed after functionalizing, while compact and large aggregated particles were found without functionalizing. The average thickness of uniform and well-defined coated TiO2 layer was in the range of 30-40 nm. The DRS results have determined the reflective properties and <span class="hlt">band</span> gap <span class="hlt">energies</span> of nanocomposite powders and have shown that functionalizing of CNTs caused the change of <span class="hlt">band</span>-gap <span class="hlt">energy</span> from 2.98 to 2.87 eV.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24690441','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24690441"><span>Local <span class="hlt">band</span> gap measurements by VEELS of thin film solar cells.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Keller, Debora; Buecheler, Stephan; Reinhard, Patrick; Pianezzi, Fabian; Pohl, Darius; Surrey, Alexander; Rellinghaus, Bernd; Erni, Rolf; Tiwari, Ayodhya N</p> <p>2014-08-01</p> <p>This work presents a systematic study that evaluates the feasibility and reliability of local <span class="hlt">band</span> gap measurements of Cu(In,Ga)Se2 thin films by valence <span class="hlt">electron</span> <span class="hlt">energy</span>-loss spectroscopy (VEELS). The compositional gradients across the Cu(In,Ga)Se2 layer cause variations in the <span class="hlt">band</span> gap <span class="hlt">energy</span>, which are experimentally determined using a monochromated scanning transmission <span class="hlt">electron</span> microscope (STEM). The results reveal the expected <span class="hlt">band</span> gap variation across the Cu(In,Ga)Se2 layer and therefore confirm the feasibility of local <span class="hlt">band</span> gap measurements of Cu(In,Ga)Se2 by VEELS. The precision and accuracy of the results are discussed based on the analysis of individual error sources, which leads to the conclusion that the precision of our measurements is most limited by the acquisition reproducibility, if the signal-to-noise ratio of the spectrum is high enough. Furthermore, we simulate the impact of radiation losses on the measured <span class="hlt">band</span> gap value and propose a thickness-dependent correction. In future work, localized <span class="hlt">band</span> gap variations will be measured on a more localized length scale to investigate, e.g., the influence of chemical inhomogeneities and dopant accumulations at grain boundaries.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JaJAP..55e1202K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JaJAP..55e1202K"><span>Interacting quasi-<span class="hlt">band</span> theory for <span class="hlt">electronic</span> states in compound semiconductor alloys: Wurtzite structure</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kishi, Ayaka; Oda, Masato; Shinozuka, Yuzo</p> <p>2016-05-01</p> <p>This paper reports on the <span class="hlt">electronic</span> states of compound semiconductor alloys of wurtzite structure calculated by the recently proposed interacting quasi-<span class="hlt">band</span> (IQB) theory combined with empirical sp3 tight-binding models. Solving derived quasi-Hamiltonian 24 × 24 matrix that is characterized by the crystal parameters of the constituents facilitates the calculation of the conduction and valence <span class="hlt">bands</span> of wurtzite alloys for arbitrary concentrations under a unified scheme. The theory is applied to III-V and II-VI wurtzite alloys: cation-substituted Al1- x Ga x N and Ga1- x In x N and anion-substituted CdS1- x Se x and ZnO1- x S x . The obtained results agree well with the experimental data, and are discussed in terms of mutual mixing between the quasi-localized states (QLS) and quasi-average <span class="hlt">bands</span> (QAB): the latter <span class="hlt">bands</span> are approximately given by the virtual crystal approximation (VCA). The changes in the valence and conduction <span class="hlt">bands</span>, and the origin of the <span class="hlt">band</span> gap bowing are discussed on the basis of mixing character.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016NatSR...622938H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016NatSR...622938H"><span>Directly tailoring photon-<span class="hlt">electron</span> coupling for sensitive photoconductance</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huang, Zhiming; Zhou, Wei; Huang, Jingguo; Wu, Jing; Gao, Yanqing; Qu, Yue; Chu, Junhao</p> <p>2016-03-01</p> <p>The coupling between photons and <span class="hlt">electrons</span> is at the heart of many fundamental phenomena in nature. Despite tremendous advances in controlling <span class="hlt">electrons</span> by photons in engineered <span class="hlt">energy-band</span> systems, control over their coupling is still widely lacking. Here we demonstrate an unprecedented ability to couple photon-<span class="hlt">electron</span> interactions in real space, in which the incident electromagnetic wave directly tailors <span class="hlt">energy</span> <span class="hlt">bands</span> of solid to generate carriers for sensitive photoconductance. By spatially coherent manipulation of metal-wrapped material system through anti-symmetric electric field of the irradiated electromagnetic wave, <span class="hlt">electrons</span> in the metals are injected and accumulated in the induced potential well (EIW) produced in the solid. Respective positive and negative electric conductances are easily observed in n-type and p-type semiconductors into which <span class="hlt">electrons</span> flow down from the two metallic sides under light irradiation. The photoconductivity is further confirmed by sweeping the injected <span class="hlt">electrons</span> out of the semiconductor before recombination applied by sufficiently strong electric fields. Our work opens up new perspectives for tailoring <span class="hlt">energy</span> <span class="hlt">bands</span> of solids and is especially relevant to develop high effective photon detection, spin injection, and <span class="hlt">energy</span> harvesting in optoelectronics and <span class="hlt">electronics</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011JPhCS.326a2028A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011JPhCS.326a2028A"><span>Accurate calibration for the quantification of the Al content in AlGaN epitaxial layers by <span class="hlt">energy</span>-dispersive X-ray spectroscopy in a Transmission <span class="hlt">Electron</span> Microscope</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Amari, H.; Lari, L.; Zhang, H. Y.; Geelhaar, L.; Chèze, C.; Kappers, M. J.; McAleese, C.; Humphreys, C. J.; Walther, T.</p> <p>2011-11-01</p> <p>Since the <span class="hlt">band</span> structure of group III- nitrides presents a direct <span class="hlt">electronic</span> transition with a <span class="hlt">band</span>-gap <span class="hlt">energy</span> covering the range from 3.4 eV for (GaN) to 6.2 eV (for AlN) at room temperature as well as a high thermal conductivity, aluminium gallium nitride (AlGaN) is a strong candidate for high-power and high-temperature <span class="hlt">electronic</span> devices and short-wavelength (visible and ultraviolet) optoelectronic devices. We report here a study by <span class="hlt">energy</span>-filtered transmission <span class="hlt">electron</span> microscopy (EFTEM) and <span class="hlt">energy</span>-dispersive X-ray spectroscopy (EDXS) of the micro structure and elemental distribution in different aluminium gallium nitride epitaxial layers grown by different research groups. A calibration procedure is out-lined that yields the Al content from EDXS to within ~1 at % precision.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25884131','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25884131"><span>Low-dimensional transport and large thermoelectric power factors in bulk semiconductors by <span class="hlt">band</span> engineering of highly directional <span class="hlt">electronic</span> states.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bilc, Daniel I; Hautier, Geoffroy; Waroquiers, David; Rignanese, Gian-Marco; Ghosez, Philippe</p> <p>2015-04-03</p> <p>Thermoelectrics are promising for addressing <span class="hlt">energy</span> issues but their exploitation is still hampered by low efficiencies. So far, much improvement has been achieved by reducing the thermal conductivity but less by maximizing the power factor. The latter imposes apparently conflicting requirements on the <span class="hlt">band</span> structure: a narrow <span class="hlt">energy</span> distribution and a low effective mass. Quantum confinement in nanostructures and the introduction of resonant states were suggested as possible solutions to this paradox, but with limited success. Here, we propose an original approach to fulfill both requirements in bulk semiconductors. It exploits the highly directional character of some orbitals to engineer the <span class="hlt">band</span> structure and produce a type of low-dimensional transport similar to that targeted in nanostructures, while retaining isotropic properties. Using first-principle calculations, the theoretical concept is demonstrated in Fe2YZ Heusler compounds, yielding power factors 4 to 5 times larger than in classical thermoelectrics at room temperature. Our findings are totally generic and rationalize the search of alternative compounds with similar behavior. Beyond thermoelectricity, these might be relevant also in the context of <span class="hlt">electronic</span>, superconducting, or photovoltaic applications.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22310942-band-gap-engineering-graphene-using-na-sup-ions','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22310942-band-gap-engineering-graphene-using-na-sup-ions"><span><span class="hlt">Band</span> gap engineering for graphene by using Na{sup +} ions</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Sung, S. J.; Lee, P. R.; Kim, J. G.</p> <p>2014-08-25</p> <p>Despite the noble <span class="hlt">electronic</span> properties of graphene, its industrial application has been hindered mainly by the absence of a stable means of producing a <span class="hlt">band</span> gap at the Dirac point (DP). We report a new route to open a <span class="hlt">band</span> gap (E{sub g}) at DP in a controlled way by depositing positively charged Na{sup +} ions on single layer graphene formed on 6H-SiC(0001) surface. The doping of low <span class="hlt">energy</span> Na{sup +} ions is found to deplete the π* <span class="hlt">band</span> of graphene above the DP, and simultaneously shift the DP downward away from Fermi <span class="hlt">energy</span> indicating the opening of E{sub g}.more » The <span class="hlt">band</span> gap increases with increasing Na{sup +} coverage with a maximum E{sub g}≥0.70 eV. Our core-level data, C 1s, Na 2p, and Si 2p, consistently suggest that Na{sup +} ions do not intercalate through graphene, but produce a significant charge asymmetry among the carbon atoms of graphene to cause the opening of a <span class="hlt">band</span> gap. We thus provide a reliable way of producing and tuning the <span class="hlt">band</span> gap of graphene by using Na{sup +} ions, which may play a vital role in utilizing graphene in future nano-<span class="hlt">electronic</span> devices.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011LTP....37...69K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011LTP....37...69K"><span>Anomalous resistivity and superconductivity in the two-<span class="hlt">band</span> Hubbard model with one narrow <span class="hlt">band</span> (Review)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kagan, M. Yu.; Valkov, V. V.</p> <p>2011-01-01</p> <p>We search for marginal Fermi-liquid behavior in the two-<span class="hlt">band</span> Hubbard model with one narrow <span class="hlt">band</span>. We consider the limit of low <span class="hlt">electron</span> densities in the <span class="hlt">bands</span> and strong intraband and interband Hubbard interactions. We analyze the influence of <span class="hlt">electron</span>-polaron effects and other mechanisms for mass-enhancement (related to the momentum dependence of the self-<span class="hlt">energies</span>) on the effective mass and scattering times of light and heavy components in the clean case (<span class="hlt">electron-electron</span> scattering and no impurities). We find a tendency towards phase separation (towards negative partial compressibility of heavy particles) in the 3D case with a large mismatch between the densities of heavy and light <span class="hlt">bands</span> in the strong coupling limit. We also find that for low temperatures and equal densities, the resistivity in a homogeneous state R(T )∝T2 behaves as a Fermi-liquid in both 3D and 2D. For temperatures greater than the effective bandwidth for heavy <span class="hlt">electrons</span> T >Wh*, the coherence of the heavy component breaks down completely. The heavy particles move diffusively in the surrounding light particles. At the same time, light particles scatter on heavy particles as if on immobile (static) impurities. Under these conditions, the heavy component is marginal, while the light component is not. The resistivity approaches saturation for T >Wh* in the 3D case. In 2D the resistivity has a maximum and a localization tail owing to weak-localization corrections of the Altshuler-Aronov type. This behavior of resistivity in 3D could be relevant for some uranium-based heavy-fermion compounds such as UNi2Al3 and in 2D, for some other mixed-valence compounds, possibly including layered manganites. We also consider briefly the superconductive (SC) instability in this model. The leading instability tends to p-wave pairing and is governed by an enhanced Kohn-Luttinger mechanism for SC at low <span class="hlt">electron</span> densities. The critical temperature corresponds to the pairing of heavy <span class="hlt">electrons</span> via polarization of</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_13 --> <div id="page_14" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="261"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MsT.........13T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MsT.........13T"><span><span class="hlt">Band</span> Gap Engineering of Titania Systems Purposed for Photocatalytic Activity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Thurston, Cameron</p> <p></p> <p>Ab initio computer aided design drastically increases candidate population for highly specified material discovery and selection. These simulations, carried out through a first-principles computational approach, accurately extrapolate material properties and behavior. Titanium Dioxide (TiO2 ) is one such material that stands to gain a great deal from the use of these simulations. In its anatase form, titania (TiO2 ) has been found to exhibit a <span class="hlt">band</span> gap nearing 3.2 eV. If titania is to become a viable alternative to other contemporary photoactive materials exhibiting <span class="hlt">band</span> gaps better suited for the solar spectrum, then the <span class="hlt">band</span> gap must be subsequently reduced. To lower the <span class="hlt">energy</span> needed for <span class="hlt">electronic</span> excitation, both transition metals and non-metals have been extensively researched and are currently viable candidates for the continued reduction of titania's <span class="hlt">band</span> gap. The introduction of multicomponent atomic doping introduces new <span class="hlt">energy</span> <span class="hlt">bands</span> which tend to both reduce the <span class="hlt">band</span> gap and recombination loss. Ta-N, Nb-N, V-N, Cr-N, Mo-N, and W-N substitutions were studied in titania and subsequent <span class="hlt">energy</span> and <span class="hlt">band</span> gap calculations show a favorable <span class="hlt">band</span> gap reduction in the case of passivated systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012JChPh.137s4112K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012JChPh.137s4112K"><span><span class="hlt">Electronic</span> <span class="hlt">energy</span> transfer: Localized operator partitioning of <span class="hlt">electronic</span> <span class="hlt">energy</span> in composite quantum systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Khan, Yaser; Brumer, Paul</p> <p>2012-11-01</p> <p>A Hamiltonian based approach using spatially localized projection operators is introduced to give precise meaning to the chemically intuitive idea of the <span class="hlt">electronic</span> <span class="hlt">energy</span> on a quantum subsystem. This definition facilitates the study of <span class="hlt">electronic</span> <span class="hlt">energy</span> transfer in arbitrarily coupled quantum systems. In particular, the decomposition scheme can be applied to molecular components that are strongly interacting (with significant orbital overlap) as well as to isolated fragments. The result defines a consistent <span class="hlt">electronic</span> <span class="hlt">energy</span> at all internuclear distances, including the case of separated fragments, and reduces to the well-known Förster and Dexter results in their respective limits. Numerical calculations of coherent <span class="hlt">energy</span> and charge transfer dynamics in simple model systems are presented and the effect of collisionally induced decoherence is examined.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1402656-generation-lower-upper-bands-electrostatic-electron-cyclotron-harmonic-waves-van-allen-radiation-belts','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1402656-generation-lower-upper-bands-electrostatic-electron-cyclotron-harmonic-waves-van-allen-radiation-belts"><span>Generation of lower and upper <span class="hlt">bands</span> of electrostatic <span class="hlt">electron</span> cyclotron harmonic waves in the Van Allen radiation belts</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Zhou, Qinghua; Xiao, Fuliang; Yang, Chang; ...</p> <p>2017-05-22</p> <p>Electrostatic <span class="hlt">electron</span> cyclotron harmonic (ECH) waves generated by the <span class="hlt">electron</span> loss cone distribution can produce efficient scattering loss of plasma sheet <span class="hlt">electrons</span>, which has a significant effect on the dynamics in the outer magnetosphere. Here we report two ECH emission events around the same location L≈ 5.7–5.8, MLT ≈ 12 from Van Allen Probes on 11 February (event A) and 9 January 2014 (event B), respectively. The spectrum of ECH waves was centered at the lower half of the harmonic <span class="hlt">bands</span> during event A, but the upper half during event B. The observed <span class="hlt">electron</span> phase space density in both eventsmore » is fitted by the subtracted bi-Maxwellian distribution, and the fitting functions are used to evaluate the local growth rates of ECH waves based on a linear theory for homogeneous plasmas. ECH waves are excited by the loss cone instability of 50 eV–1 keV <span class="hlt">electrons</span> in the lower half of harmonic <span class="hlt">bands</span> in the low-density plasmasphere in event A, and 1–10 keV <span class="hlt">electrons</span> in the upper half of harmonic <span class="hlt">bands</span> in a relatively high-density region in event B. Here, the current results successfully explain observations and provide a first direct evidence on how ECH waves are generated in the lower and upper half of harmonic frequency <span class="hlt">bands</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1402656','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1402656"><span>Generation of lower and upper <span class="hlt">bands</span> of electrostatic <span class="hlt">electron</span> cyclotron harmonic waves in the Van Allen radiation belts</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Zhou, Qinghua; Xiao, Fuliang; Yang, Chang</p> <p></p> <p>Electrostatic <span class="hlt">electron</span> cyclotron harmonic (ECH) waves generated by the <span class="hlt">electron</span> loss cone distribution can produce efficient scattering loss of plasma sheet <span class="hlt">electrons</span>, which has a significant effect on the dynamics in the outer magnetosphere. Here we report two ECH emission events around the same location L≈ 5.7–5.8, MLT ≈ 12 from Van Allen Probes on 11 February (event A) and 9 January 2014 (event B), respectively. The spectrum of ECH waves was centered at the lower half of the harmonic <span class="hlt">bands</span> during event A, but the upper half during event B. The observed <span class="hlt">electron</span> phase space density in both eventsmore » is fitted by the subtracted bi-Maxwellian distribution, and the fitting functions are used to evaluate the local growth rates of ECH waves based on a linear theory for homogeneous plasmas. ECH waves are excited by the loss cone instability of 50 eV–1 keV <span class="hlt">electrons</span> in the lower half of harmonic <span class="hlt">bands</span> in the low-density plasmasphere in event A, and 1–10 keV <span class="hlt">electrons</span> in the upper half of harmonic <span class="hlt">bands</span> in a relatively high-density region in event B. Here, the current results successfully explain observations and provide a first direct evidence on how ECH waves are generated in the lower and upper half of harmonic frequency <span class="hlt">bands</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29488385','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29488385"><span>Origin of the Two <span class="hlt">Bands</span> in the B800 Ring and Their Involvement in the <span class="hlt">Energy</span> Transfer Network of Allochromatium vinosum.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Schröter, Marco; Alcocer, Marcelo J P; Cogdell, Richard J; Kühn, Oliver; Zigmantas, Donatas</p> <p>2018-03-15</p> <p>Bacterial photosynthesis features robust and adaptable <span class="hlt">energy</span>-harvesting processes in which light-harvesting proteins play a crucial role. The peripheral light-harvesting complex of the purple bacterium Allochromatium vinosum is particularly distinct, featuring a double peak structure in its B800 absorption <span class="hlt">band</span>. Two hypotheses-not necessarily mutually exclusive-concerning the origin of this splitting have been proposed; either two distinct B800 bacteriochlorophyll site <span class="hlt">energies</span> are involved, or an excitonic dimerization of bacteriochlorophylls within the B800 ring takes place. Through the use of two-dimensional <span class="hlt">electronic</span> spectroscopy, we present unambiguous evidence that excitonic interaction shapes the split <span class="hlt">band</span>. We further identify and characterize all of the <span class="hlt">energy</span> transfer pathways within this complex by using a global kinetic fitting procedure. Our approach demonstrates how the combination of two-dimensional spectral resolution and self-consistent fitting allows for extraction of information on light-harvesting processes, which would otherwise be inaccessible due to signal congestion.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014SSCom.190...44G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014SSCom.190...44G"><span>Excitonic and <span class="hlt">band-band</span> transitions of Cu2ZnSiS4 determined from reflectivity spectra</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Guc, M.; Levcenko, S.; Dermenji, L.; Gurieva, G.; Schorr, S.; Syrbu, N. N.; Arushanov, E.</p> <p>2014-07-01</p> <p>Exciton spectra of Cu2ZnSiS4 single crystals are investigated by reflection spectroscopy at 10 and 300 K for light polarized perpendicular (E⊥c) and parallel (E∥c) to the optical axis. The parameters of the excitons and dielectric constant are determined. The free carriers effective masses have been estimated. The room temperature reflectivity spectra at photon <span class="hlt">energies</span> higher than the fundamental <span class="hlt">band</span> gap in the polarization Е⊥с and E∥с were measured and related to the <span class="hlt">electronic</span> <span class="hlt">band</span> structure of Cu2ZnSiS4.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvB..97m4521L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvB..97m4521L"><span>Exotic superconductivity with enhanced <span class="hlt">energy</span> scales in materials with three <span class="hlt">band</span> crossings</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lin, Yu-Ping; Nandkishore, Rahul M.</p> <p>2018-04-01</p> <p>Three <span class="hlt">band</span> crossings can arise in three-dimensional quantum materials with certain space group symmetries. The low <span class="hlt">energy</span> Hamiltonian supports spin one fermions and a flat <span class="hlt">band</span>. We study the pairing problem in this setting. We write down a minimal BCS Hamiltonian and decompose it into spin-orbit coupled irreducible pairing channels. We then solve the resulting gap equations in channels with zero total angular momentum. We find that in the s-wave spin singlet channel (and also in an unusual d-wave `spin quintet' channel), superconductivity is enormously enhanced, with a possibility for the critical temperature to be linear in interaction strength. Meanwhile, in the p-wave spin triplet channel, the superconductivity exhibits features of conventional BCS theory due to the absence of flat <span class="hlt">band</span> pairing. Three <span class="hlt">band</span> crossings thus represent an exciting new platform for realizing exotic superconducting states with enhanced <span class="hlt">energy</span> scales. We also discuss the effects of doping, nonzero temperature, and of retaining additional terms in the k .p expansion of the Hamiltonian.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EL....11520008R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EL....11520008R"><span>Revivals of <span class="hlt">electron</span> currents and topological-<span class="hlt">band</span> insulator transitions in 2D gapped Dirac materials</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Romera, E.; Bolívar, J. C.; Roldán, J. B.; de los Santos, F.</p> <p>2016-07-01</p> <p>We have studied the time evolution of <span class="hlt">electron</span> wave packets in silicene under perpendicular magnetic and electric fields to characterize topological-<span class="hlt">band</span> insulator transitions. We have found that at the charge neutrality points, the periodicities exhibited by the wave packet dynamics (classical and revival times) reach maximum values, and that the <span class="hlt">electron</span> currents reflect the transition from a topological insulator to a <span class="hlt">band</span> insulator. This provides a signature of topological phase transition in silicene that can be extended to other 2D Dirac materials isostructural to graphene and with a buckled structure and a significant spin-orbit coupling.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005cmns.conf..735C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005cmns.conf..735C"><span>Nuts and Bolts of the Ion <span class="hlt">Band</span> State Theory</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chubb, Scott R.</p> <p>2005-12-01</p> <p>The nuts and bolts of our ion <span class="hlt">band</span> state theory of low <span class="hlt">energy</span> nuclear reactions (LENR's) in palladium-deuteride (PdD) and palladium-hydride (PdH) are the <span class="hlt">electrons</span> that hold together or tear apart the bonds (or lack of bonds) between deuterons (d's) or protons (p's) and the host material. In PdDx and PdHx, this bonding is strongly correlated with loading. In ambient loading conditions (x ≲ 0.6), bonding inhibits ion <span class="hlt">band</span> state occupation. As x → 1, slight increases and decreases in loading can induce "vibrations" (which have conventionally been thought to occur from phonons) that can induce potential losses or increases of p/d. Naive assumptions about phonons fail to include these losses and increases. These effects can occur because neither H or D has core <span class="hlt">electrons</span> and because in either PdD or PdH, the <span class="hlt">electrons</span> near the Fermi <span class="hlt">energy</span> have negligible overlap with the nucleus of either D or H. In the past, implicitly, we have used these facts to justify our ion <span class="hlt">band</span> state theory. Here, we present a more formal justification, based on the relationship between H(D) ion <span class="hlt">band</span> states (IBS's) and H(D) phonons that includes a microscopic picture that explains why occupation of IBS's can occur in PdD and PdH and how this can lead to nuclear reactions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JChPh.148t4109F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JChPh.148t4109F"><span><span class="hlt">Band</span> structures in coupled-cluster singles-and-doubles Green's function (GFCCSD)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Furukawa, Yoritaka; Kosugi, Taichi; Nishi, Hirofumi; Matsushita, Yu-ichiro</p> <p>2018-05-01</p> <p>We demonstrate that the coupled-cluster singles-and-doubles Green's function (GFCCSD) method is a powerful and prominent tool drawing the <span class="hlt">electronic</span> <span class="hlt">band</span> structures and the total <span class="hlt">energies</span>, which many theoretical techniques struggle to reproduce. We have calculated single-<span class="hlt">electron</span> <span class="hlt">energy</span> spectra via the GFCCSD method for various kinds of systems, ranging from ionic to covalent and van der Waals, for the first time: the one-dimensional LiH chain, one-dimensional C chain, and one-dimensional Be chain. We have found that the bandgap becomes narrower than in HF due to the correlation effect. We also show that the <span class="hlt">band</span> structures obtained from the GFCCSD method include both quasiparticle and satellite peaks successfully. Besides, taking one-dimensional LiH as an example, we discuss the validity of restricting the active space to suppress the computational cost of the GFCCSD method. We show that the calculated results without <span class="hlt">bands</span> that do not contribute to the chemical bonds are in good agreement with full-<span class="hlt">band</span> calculations. With the GFCCSD method, we can calculate the total <span class="hlt">energies</span> and spectral functions for periodic systems in an explicitly correlated manner.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28205063','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28205063"><span>Excitation <span class="hlt">energy</span> transfer from the bacteriochlorophyll Soret <span class="hlt">band</span> to carotenoids in the LH2 light-harvesting complex from Ectothiorhodospira haloalkaliphila is negligible.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Razjivin, A P; Lukashev, E P; Kompanets, V O; Kozlovsky, V S; Ashikhmin, A A; Chekalin, S V; Moskalenko, A A; Paschenko, V Z</p> <p>2017-09-01</p> <p>Pathways of intramolecular conversion and intermolecular <span class="hlt">electronic</span> excitation <span class="hlt">energy</span> transfer (EET) in the photosynthetic apparatus of purple bacteria remain subject to debate. Here we experimentally tested the possibility of EET from the bacteriochlorophyll (BChl) Soret <span class="hlt">band</span> to the singlet S 2 level of carotenoids using femtosecond pump-probe measurements and steady-state fluorescence excitation and absorption measurements in the near-ultraviolet and visible spectral ranges. The efficiency of EET from the Soret <span class="hlt">band</span> of BChl to S 2 of the carotenoids in light-harvesting complex LH2 from the purple bacterium Ectothiorhodospira haloalkaliphila appeared not to exceed a few percent.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011APS..GECJW2002H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011APS..GECJW2002H"><span><span class="hlt">Electronic</span> Excitation of Furan by Low <span class="hlt">Energy</span> <span class="hlt">Electrons</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hargreaves, Leigh R.; Khakoo, Murtadha A.; Lopes, Maria Cristina A.; da Costa, Romarly; Bettega, Marcio H. F.; Lima, Marco A. P.</p> <p>2011-10-01</p> <p>We present absolute differential cross section (DCS) measurements and calculations of <span class="hlt">electron</span> impact excitation of the lowest lying triplet 3B2 and 3A1 <span class="hlt">electronic</span> states of furan. The incident <span class="hlt">electron</span> <span class="hlt">energy</span> range of the present study was 5-15eV. The experimental data were normalized to the elastic DCS data of. The cross sections were determined by unfolding <span class="hlt">electron</span> <span class="hlt">energy</span> loss spectra, using an open source data analysis package and the spectroscopic assignments of. The calculations employ a Multichannel Schwinger method with a 9-state closed coupling CI configuration including polarized pseudo-potentials. The preliminary theoretical results show reasonable agreement with experiment below 10eV, but differ at higher <span class="hlt">energies</span>. Funded by the US NSF and the Brazilian funding agencies CNPq, CAPES and FAPESP.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015NIMPB.360..103C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015NIMPB.360..103C"><span><span class="hlt">Band</span> structure effects in the <span class="hlt">energy</span> loss of low-<span class="hlt">energy</span> protons and deuterons in thin films of Pt</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Celedón, C. E.; Sánchez, E. A.; Salazar Alarcón, L.; Guimpel, J.; Cortés, A.; Vargas, P.; Arista, N. R.</p> <p>2015-10-01</p> <p>We have investigated experimentally and by computer simulations the <span class="hlt">energy</span>-loss and angular distribution of low <span class="hlt">energy</span> (E < 10 keV) protons and deuterons transmitted through thin polycrystalline platinum films. The experimental results show significant deviations from the expected velocity dependence of the stopping power in the range of very low <span class="hlt">energies</span> with respect to the predictions of the Density Functional Theory for a jellium model. This behavior is similar to those observed in other transition metals such as Cu, Ag and Au, but different from the linear dependence recently observed in another transition metal, Pd, which belongs to the same Group of Pt in the Periodic Table. These differences are analyzed in term of the properties of the <span class="hlt">electronic</span> <span class="hlt">bands</span> corresponding to Pt and Pd, represented in terms of the corresponding density of states. The present experiments include also a detailed study of the angular dependence of the <span class="hlt">energy</span> loss and the angular distributions of transmitted protons and deuterons. The results are compared with computer simulations based on the Monte Carlo method and with a theoretical model that evaluates the contributions of elastic collisions, path length effects in the inelastic <span class="hlt">energy</span> losses, and the effects of the foil roughness. The results of the analysis obtained from these various approaches provide a consistent and comprehensive description of the experimental findings.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AIPC.1953k0019B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AIPC.1953k0019B"><span>Ab-initio study on <span class="hlt">electronic</span> properties of rocksalt SnAs</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Babariya, Bindiya; Vaghela, M. V.; Gajjar, P. N.</p> <p>2018-05-01</p> <p>Within the frame work of Local Density Approximation of Exchange and Correlation, ab-initio method of density functional theory with Abinit code is used to compute <span class="hlt">electronic</span> <span class="hlt">energy</span> <span class="hlt">band</span> structure, density of States and charge density of SnAs in rocksalt phase. Our result after optimization for lattice constant agrees with experimental value within 0.59% deviation. The computed <span class="hlt">electronic</span> <span class="hlt">energy</span> <span class="hlt">bands</span> in high symmetry directions Γ→K→X→Γ→L→X→W→L→U shown metallic nature. The lowest <span class="hlt">band</span> in the <span class="hlt">electronic</span> <span class="hlt">band</span> structure is showing <span class="hlt">band</span>-gap approximately 1.70 eV from next higher <span class="hlt">band</span> and no crossing between lowest two <span class="hlt">bands</span> are seen. The density of states revels p-p orbit hybridization between Sn and As atoms. The spherical contour around Sn and As in the charge density plot represent partly ionic and partly covalent bonding. Fermi surface topology is the resultant effect of the single <span class="hlt">band</span> crossing along L direction at Ef.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JMPSo..75...45X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JMPSo..75...45X"><span>Atomistic potentials based <span class="hlt">energy</span> flux integral criterion for dynamic adiabatic shear <span class="hlt">banding</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xu, Yun; Chen, Jun</p> <p>2015-02-01</p> <p>The <span class="hlt">energy</span> flux integral criterion based on atomistic potentials within the framework of hyperelasticity-plasticity is proposed for dynamic adiabatic shear <span class="hlt">banding</span> (ASB). System Helmholtz <span class="hlt">energy</span> decomposition reveals that the dynamic influence on the integral path dependence is originated from the volumetric strain <span class="hlt">energy</span> and partial deviatoric strain <span class="hlt">energy</span>, and the plastic influence only from the rest part of deviatoric strain <span class="hlt">energy</span>. The concept of critical shear <span class="hlt">banding</span> <span class="hlt">energy</span> is suggested for describing the initiation of ASB, which consists of the dynamic recrystallization (DRX) threshold <span class="hlt">energy</span> and the thermal softening <span class="hlt">energy</span>. The criterion directly relates <span class="hlt">energy</span> flux to the basic physical processes that induce shear instability such as dislocation nucleations and multiplications, without introducing ad-hoc parameters in empirical constitutive models. It reduces to the classical path independent J-integral for quasi-static loading and elastic solids. The atomistic-to-continuum multiscale coupling method is used to simulate the initiation of ASB. Atomic configurations indicate that DRX induced microstructural softening may be essential to the dynamic shear localization and hence the initiation of ASB.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JAP...123j4301G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JAP...123j4301G"><span><span class="hlt">Band</span>-offset-induced lateral shift of valley <span class="hlt">electrons</span> in ferromagnetic MoS2/WS2 planar heterojunctions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ghadiri, Hassan; Saffarzadeh, Alireza</p> <p>2018-03-01</p> <p>Low-<span class="hlt">energy</span> coherent transport and a Goos-Hänchen (GH) lateral shift of valley <span class="hlt">electrons</span> in planar heterojunctions composed of normal MoS2 and ferromagnetic WS2 monolayers are theoretically investigated. Two types of heterojunctions in the forms of WS2/MoS2/WS2 (type-A) and MoS2/WS2/MoS2 (type-B) with incident <span class="hlt">electrons</span> in the MoS2 region are considered in which the lateral shift of <span class="hlt">electrons</span> is induced by <span class="hlt">band</span> alignments of the two constituent semiconductors. It is shown that the type-A heterojunction can act as an <span class="hlt">electron</span> waveguide due to <span class="hlt">electron</span> confinement between the two WS2/MoS2 interfaces which cause the incident <span class="hlt">electrons</span> with an appropriate incidence angle to propagate along the interfaces. In this case, the spin- and valley-dependent GH shifts of totally reflected <span class="hlt">electrons</span> from the interface lead to separated <span class="hlt">electrons</span> with distinct spin-valley indexes after traveling a sufficiently long distance. In the type-B heterojunction, however, transmission resonances occur for incident <span class="hlt">electron</span> beams passing through the structure, and large spin- and valley-dependent lateral shift values in propagating states can be achieved. Consequently, the transmitted <span class="hlt">electrons</span> are spatially well-separated into <span class="hlt">electrons</span> with distinct spin-valley indexes. Our findings reveal that the planar heterojunctions of transition metal dichalcogenides can be utilized as spin-valley beam filters and/or splitters without external gating.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018SuMi..115...88D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018SuMi..115...88D"><span>Structural analysis, <span class="hlt">electronic</span> properties, and <span class="hlt">band</span> gaps of a graphene nanoribbon: A new 2D materials</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dass, Devi</p> <p>2018-03-01</p> <p>Graphene nanoribbon (GNR), a new 2D carbon nanomaterial, has some unique features and special properties that offer a great potential for interconnect, nanoelectronic devices, optoelectronics, and nanophotonics. This paper reports the structural analysis, <span class="hlt">electronic</span> properties, and <span class="hlt">band</span> gaps of a GNR considering different chirality combinations obtained using the pz orbital tight binding model. In structural analysis, the analytical expressions for GNRs have been developed and verified using the simulation for the first time. It has been found that the total number of unit cells and carbon atoms within an overall unit cell and molecular structure of a GNR have been changed with the change in their chirality values which are similar to the values calculated using the developed analytical expressions thus validating both the simulation as well as analytical results. Further, the <span class="hlt">electronic</span> <span class="hlt">band</span> structures at different chirality values have been shown for the identification of metallic and semiconductor properties of a GNR. It has been concluded that all zigzag edge GNRs are metallic with very small <span class="hlt">band</span> gaps range whereas all armchair GNRs show both the metallic and semiconductor nature with very small and high <span class="hlt">band</span> gaps range. Again, the total number of subbands in each <span class="hlt">electronic</span> <span class="hlt">band</span> structure is equal to the total number of carbon atoms present in overall unit cell of the corresponding GNR. The semiconductors GNRs can be used as a channel material in field effect transistor suitable for advanced CMOS technology whereas the metallic GNRs could be used for interconnect.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22253966-electron-tunneling-spectroscopy-study-electrically-active-traps-algan-gan-high-electron-mobility-transistors','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22253966-electron-tunneling-spectroscopy-study-electrically-active-traps-algan-gan-high-electron-mobility-transistors"><span><span class="hlt">Electron</span> tunneling spectroscopy study of electrically active traps in AlGaN/GaN high <span class="hlt">electron</span> mobility transistors</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Yang, Jie, E-mail: jie.yang@yale.edu; Cui, Sharon; Ma, T. P.</p> <p>2013-11-25</p> <p>We investigate the <span class="hlt">energy</span> levels of <span class="hlt">electron</span> traps in AlGaN/GaN high <span class="hlt">electron</span> mobility transistors by the use of <span class="hlt">electron</span> tunneling spectroscopy. Detailed analysis of a typical spectrum, obtained in a wide gate bias range and with both bias polarities, suggests the existence of <span class="hlt">electron</span> traps both in the bulk of AlGaN and at the AlGaN/GaN interface. The <span class="hlt">energy</span> levels of the <span class="hlt">electron</span> traps have been determined to lie within a 0.5 eV <span class="hlt">band</span> below the conduction <span class="hlt">band</span> minimum of AlGaN, and there is strong evidence suggesting that these traps contribute to Frenkel-Poole conduction through the AlGaN barrier.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ApSS..429....2C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ApSS..429....2C"><span>Selectivity of photoelectrochemical CO2 reduction modulated with <span class="hlt">electron</span> transfer from size-tunable quantized <span class="hlt">energy</span> states of CdSe nanocrystals</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cho, Hyunjin; Kim, Whi Dong; Lee, Kangha; Lee, Seokwon; Kang, Gil-Seong; Joh, Han-Ik; Lee, Doh C.</p> <p>2018-01-01</p> <p>We investigate the product selectivity of CO2 reduction using NiO photocathodes decorated with CdSe quantum dots (QDs) of varying size in a photoelectrochemical (PEC) cell. Size-tunable and quantized <span class="hlt">energy</span> states of conduction <span class="hlt">band</span> in CdSe QDs enable systematic control of <span class="hlt">electron</span> transfer kinetics from CdSe QDs to NiO. It turns out that different size of CdSe QDs results in variation in product selectivity for CO2 reduction. The <span class="hlt">energy</span> gap between conduction <span class="hlt">band</span> edge and redox potential of each reduction product (e.g., CO and CH4) correlates with their production rate. The size dependence of the <span class="hlt">electron</span> transfer rate estimated from the <span class="hlt">energy</span> gap is in agreement with the selectivity of CO2 reduction products for all reduction products but CO. The deviation in the case of CO is attributed to sequential conversion of CO into CH4 with CO adsorbed on electrode surface. Based on a premise that the CdSe QDs would exhibit similar surface configuration regardless of QD size, it is concluded that the <span class="hlt">electron</span> transfer kinetics proves to alter the selectivity of CO2 reduction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3957363','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3957363"><span>Inter-spin distance determination using L-<span class="hlt">band</span> (1-2 GHz) non-adiabatic rapid sweep <span class="hlt">electron</span> paramagnetic resonance (NARS EPR)</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Kittell, Aaron W.; Hustedt, Eric J.; Hyde, James S.</p> <p>2014-01-01</p> <p>Site-directed spin-labeling <span class="hlt">electron</span> paramagnetic resonance (SDSL EPR) provides insight into the local structure and motion of a spin probe strategically attached to a molecule. When a second spin is introduced to the system, macromolecular information can be obtained through measurement of inter-spin distances either by continuous wave (CW) or pulsed <span class="hlt">electron</span> double resonance (ELDOR) techniques. If both methodologies are considered, inter-spin distances of 8 to 80 Å can be experimentally determined. However, there exists a region at the upper limit of the conventional X-<span class="hlt">band</span> (9.5 GHz) CW technique and the lower limit of the four-pulse double <span class="hlt">electron-electron</span> resonance (DEER) experiment where neither method is particularly reliable. The work presented here utilizes L-<span class="hlt">band</span> (1.9 GHz) in combination with non-adiabatic rapid sweep (NARS) EPR to address this opportunity by increasing the upper limit of the CW technique. Because L-<span class="hlt">band</span> linewidths are three to seven times narrower than those at X-<span class="hlt">band</span>, dipolar broadenings that are small relative to the X-<span class="hlt">band</span> inhomogeneous linewidth become observable, but the signal loss due to the frequency dependence of the Boltzmann factor, has made L-<span class="hlt">band</span> especially challenging. NARS has been shown to increase sensitivity by a factor of five, and overcomes much of this loss, making L-<span class="hlt">band</span> distance determination more feasible [1]. Two different systems are presented and distances of 18–30 Å have been experimentally determined at physiologically relevant temperatures. Measurements are in excellent agreement with a helical model and values determined by DEER. PMID:22750251</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_14 --> <div id="page_15" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="281"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015ApPhL.107r3301G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015ApPhL.107r3301G"><span>Experimental and theoretical investigations of the <span class="hlt">electronic</span> <span class="hlt">band</span> structure of metal-organic frameworks of HKUST-1 type</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gu, Zhi-Gang; Heinke, Lars; Wöll, Christof; Neumann, Tobias; Wenzel, Wolfgang; Li, Qiang; Fink, Karin; Gordan, Ovidiu D.; Zahn, Dietrich R. T.</p> <p>2015-11-01</p> <p>The <span class="hlt">electronic</span> properties of metal-organic frameworks (MOFs) are increasingly attracting the attention due to potential applications in sensor techniques and (micro-) <span class="hlt">electronic</span> engineering, for instance, as low-k-dielectric in semiconductor technology. Here, the <span class="hlt">band</span> gap and the <span class="hlt">band</span> structure of MOFs of type HKUST-1 are studied in detail by means of spectroscopic ellipsometry applied to thin surface-mounted MOF films and by means of quantum chemical calculations. The analysis of the density of states, the <span class="hlt">band</span> structure, and the excitation spectrum reveal the importance of the empty Cu-3d orbitals for the <span class="hlt">electronic</span> properties of HKUST-1. This study shows that, in contrast to common belief, even in the case of this fairly "simple" MOF, the excitation spectra cannot be explained by a superposition of "intra-unit" excitations within the individual building blocks. Instead, "inter-unit" excitations also have to be considered.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015SeScT..30g5001M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015SeScT..30g5001M"><span><span class="hlt">Electronic</span> structure of germanium selenide investigated using ultra-violet photo-<span class="hlt">electron</span> spectroscopy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mishra, P.; Lohani, H.; Kundu, A. K.; Patel, R.; Solanki, G. K.; Menon, Krishnakumar S. R.; Sekhar, B. R.</p> <p>2015-07-01</p> <p>The valence <span class="hlt">band</span> <span class="hlt">electronic</span> structure of GeSe single crystals has been investigated using angle resolved photoemission spectroscopy (ARPES) and x-ray photoelectron spectroscopy. The experimentally observed <span class="hlt">bands</span> from ARPES, match qualitatively with our LDA-based <span class="hlt">band</span> structure calculations along the Γ-Z, Γ-Y and Γ-T symmetry directions. The valence <span class="hlt">band</span> maximum occurs nearly midway along the Γ-Z direction, at a binding <span class="hlt">energy</span> of -0.5 eV, substantiating the indirect <span class="hlt">band</span> gap of GeSe. Non-dispersive features associated with surface states and indirect transitions have been observed. The difference in hybridization of Se and Ge 4p orbitals leads to the variation of dispersion along the three symmetry directions. The predominance of the Se 4pz orbitals, evidenced from theoretical calculations, may be the cause for highly dispersive <span class="hlt">bands</span> along the Γ-T direction. Detailed <span class="hlt">electronic</span> structure analysis reveals the significance of the cation-anion 4p orbitals hybridization in the valence <span class="hlt">band</span> dispersion of IV-VI semiconductors. This is the first comprehensive report of the <span class="hlt">electronic</span> structure of a GeSe single crystal using ARPES in conjugation with theoretical <span class="hlt">band</span> structure analysis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4533319','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4533319"><span>Anomalous High-<span class="hlt">Energy</span> Waterfall-Like <span class="hlt">Electronic</span> Structure in 5 d Transition Metal Oxide Sr2IrO4 with a Strong Spin-Orbit Coupling</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Liu, Yan; Yu, Li; Jia, Xiaowen; Zhao, Jianzhou; Weng, Hongming; Peng, Yingying; Chen, Chaoyu; Xie, Zhuojin; Mou, Daixiang; He, Junfeng; Liu, Xu; Feng, Ya; Yi, Hemian; Zhao, Lin; Liu, Guodong; He, Shaolong; Dong, Xiaoli; Zhang, Jun; Xu, Zuyan; Chen, Chuangtian; Cao, Gang; Dai, Xi; Fang, Zhong; Zhou, X. J.</p> <p>2015-01-01</p> <p>The low <span class="hlt">energy</span> <span class="hlt">electronic</span> structure of Sr2IrO4 has been well studied and understood in terms of an effective Jeff = 1/2 Mott insulator model. However, little work has been done in studying its high <span class="hlt">energy</span> <span class="hlt">electronic</span> behaviors. Here we report a new observation of the anomalous high <span class="hlt">energy</span> <span class="hlt">electronic</span> structure in Sr2IrO4. By taking high-resolution angle-resolved photoemission measurements on Sr2IrO4 over a wide <span class="hlt">energy</span> range, we have revealed for the first time that the high <span class="hlt">energy</span> <span class="hlt">electronic</span> structures show unusual nearly-vertical <span class="hlt">bands</span> that extend over a large <span class="hlt">energy</span> range. Such anomalous high <span class="hlt">energy</span> behaviors resemble the high <span class="hlt">energy</span> waterfall features observed in the cuprate superconductors. While strong <span class="hlt">electron</span> correlation plays an important role in producing high <span class="hlt">energy</span> waterfall features in the cuprate superconductors, the revelation of the high <span class="hlt">energy</span> anomalies in Sr2IrO4, which exhibits strong spin-orbit coupling and a moderate <span class="hlt">electron</span> correlation, points to an unknown and novel route in generating exotic <span class="hlt">electronic</span> excitations. PMID:26267653</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015NatSR...513036L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015NatSR...513036L"><span>Anomalous High-<span class="hlt">Energy</span> Waterfall-Like <span class="hlt">Electronic</span> Structure in 5 d Transition Metal Oxide Sr2IrO4 with a Strong Spin-Orbit Coupling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liu, Yan; Yu, Li; Jia, Xiaowen; Zhao, Jianzhou; Weng, Hongming; Peng, Yingying; Chen, Chaoyu; Xie, Zhuojin; Mou, Daixiang; He, Junfeng; Liu, Xu; Feng, Ya; Yi, Hemian; Zhao, Lin; Liu, Guodong; He, Shaolong; Dong, Xiaoli; Zhang, Jun; Xu, Zuyan; Chen, Chuangtian; Cao, Gang; Dai, Xi; Fang, Zhong; Zhou, X. J.</p> <p>2015-08-01</p> <p>The low <span class="hlt">energy</span> <span class="hlt">electronic</span> structure of Sr2IrO4 has been well studied and understood in terms of an effective Jeff = 1/2 Mott insulator model. However, little work has been done in studying its high <span class="hlt">energy</span> <span class="hlt">electronic</span> behaviors. Here we report a new observation of the anomalous high <span class="hlt">energy</span> <span class="hlt">electronic</span> structure in Sr2IrO4. By taking high-resolution angle-resolved photoemission measurements on Sr2IrO4 over a wide <span class="hlt">energy</span> range, we have revealed for the first time that the high <span class="hlt">energy</span> <span class="hlt">electronic</span> structures show unusual nearly-vertical <span class="hlt">bands</span> that extend over a large <span class="hlt">energy</span> range. Such anomalous high <span class="hlt">energy</span> behaviors resemble the high <span class="hlt">energy</span> waterfall features observed in the cuprate superconductors. While strong <span class="hlt">electron</span> correlation plays an important role in producing high <span class="hlt">energy</span> waterfall features in the cuprate superconductors, the revelation of the high <span class="hlt">energy</span> anomalies in Sr2IrO4, which exhibits strong spin-orbit coupling and a moderate <span class="hlt">electron</span> correlation, points to an unknown and novel route in generating exotic <span class="hlt">electronic</span> excitations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26267653','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26267653"><span>Anomalous High-<span class="hlt">Energy</span> Waterfall-Like <span class="hlt">Electronic</span> Structure in 5 d Transition Metal Oxide Sr2IrO4 with a Strong Spin-Orbit Coupling.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Liu, Yan; Yu, Li; Jia, Xiaowen; Zhao, Jianzhou; Weng, Hongming; Peng, Yingying; Chen, Chaoyu; Xie, Zhuojin; Mou, Daixiang; He, Junfeng; Liu, Xu; Feng, Ya; Yi, Hemian; Zhao, Lin; Liu, Guodong; He, Shaolong; Dong, Xiaoli; Zhang, Jun; Xu, Zuyan; Chen, Chuangtian; Cao, Gang; Dai, Xi; Fang, Zhong; Zhou, X J</p> <p>2015-08-12</p> <p>The low <span class="hlt">energy</span> <span class="hlt">electronic</span> structure of Sr2IrO4 has been well studied and understood in terms of an effective Jeff = 1/2 Mott insulator model. However, little work has been done in studying its high <span class="hlt">energy</span> <span class="hlt">electronic</span> behaviors. Here we report a new observation of the anomalous high <span class="hlt">energy</span> <span class="hlt">electronic</span> structure in Sr2IrO4. By taking high-resolution angle-resolved photoemission measurements on Sr2IrO4 over a wide <span class="hlt">energy</span> range, we have revealed for the first time that the high <span class="hlt">energy</span> <span class="hlt">electronic</span> structures show unusual nearly-vertical <span class="hlt">bands</span> that extend over a large <span class="hlt">energy</span> range. Such anomalous high <span class="hlt">energy</span> behaviors resemble the high <span class="hlt">energy</span> waterfall features observed in the cuprate superconductors. While strong <span class="hlt">electron</span> correlation plays an important role in producing high <span class="hlt">energy</span> waterfall features in the cuprate superconductors, the revelation of the high <span class="hlt">energy</span> anomalies in Sr2IrO4, which exhibits strong spin-orbit coupling and a moderate <span class="hlt">electron</span> correlation, points to an unknown and novel route in generating exotic <span class="hlt">electronic</span> excitations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JChPh.147v4104J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JChPh.147v4104J"><span>Complex <span class="hlt">band</span> structure and <span class="hlt">electronic</span> transmission eigenchannels</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jensen, Anders; Strange, Mikkel; Smidstrup, Søren; Stokbro, Kurt; Solomon, Gemma C.; Reuter, Matthew G.</p> <p>2017-12-01</p> <p>It is natural to characterize materials in transport junctions by their conductance length dependence, β. Theoretical estimations of β are made employing two primary theories: complex <span class="hlt">band</span> structure and density functional theory (DFT) Landauer transport. It has previously been shown that the β value derived from total Landauer transmission can be related to the β value from the smallest |ki| complex <span class="hlt">band</span>; however, it is an open question whether there is a deeper relationship between the two. Here we probe the details of the relationship between transmission and complex <span class="hlt">band</span> structure, in this case individual eigenchannel transmissions and different complex <span class="hlt">bands</span>. We present calculations of decay constants for the two most conductive states as determined by complex <span class="hlt">band</span> structure and standard DFT Landauer transport calculations for one semi-conductor and two molecular junctions. The molecular junctions show that both the length dependence of the total transmission and the individual transmission eigenvalues can be, almost always, found through the complex <span class="hlt">band</span> structure. The complex <span class="hlt">band</span> structure of the semi-conducting material, however, does not predict the length dependence of the total transmission but only of the individual channels, at some k-points, due to multiple channels contributing to transmission. We also observe instances of vertical <span class="hlt">bands</span>, some of which are the smallest |ki| complex <span class="hlt">bands</span>, that do not contribute to transport. By understanding the deeper relationship between complex <span class="hlt">bands</span> and individual transmission eigenchannels, we can make a general statement about when the previously accepted wisdom linking transmission and complex <span class="hlt">band</span> structure will fail, namely, when multiple channels contribute significantly to the transmission.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27711601','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27711601"><span>Low <span class="hlt">energy</span> <span class="hlt">electron</span> catalyst: the <span class="hlt">electronic</span> origin of catalytic strategies.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Davis, Daly; Sajeev, Y</p> <p>2016-10-12</p> <p>Using a low <span class="hlt">energy</span> <span class="hlt">electron</span> (LEE) as a catalyst, the <span class="hlt">electronic</span> origin of the catalytic strategies corresponding to substrate selectivity, reaction specificity and reaction rate enhancement is investigated for a reversible unimolecular elementary reaction. An <span class="hlt">electronic</span> <span class="hlt">energy</span> complementarity between the catalyst and the substrate molecule is the origin of substrate selectivity and reaction specificity. The <span class="hlt">electronic</span> <span class="hlt">energy</span> complementarity is induced by tuning the <span class="hlt">electronic</span> <span class="hlt">energy</span> of the catalyst. The <span class="hlt">energy</span> complementarity maximizes the binding forces between the catalyst and the molecule. Consequently, a new <span class="hlt">electronically</span> metastable high-<span class="hlt">energy</span> reactant state and a corresponding new low barrier reaction path are resonantly created for a specific reaction of the substrate through the formation of a catalyst-substrate transient adduct. The LEE catalysis also reveals a fundamental structure-<span class="hlt">energy</span> correspondence in the formation of the catalyst-substrate transient adduct. Since the <span class="hlt">energy</span> complementarities corresponding to the substrate molecules of the forward and the backward steps of the reversible reactions are not the same due to their structural differences, the LEE catalyst exhibits a unique one-way catalytic strategy, i.e., the LEE catalyst favors the reversible reaction more effectively in one direction. A characteristic stronger binding of the catalyst to the transition state of the reaction than in the initial reactant state and the final product state is the molecular origin of barrier lowering.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PhRvB..94h5403L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhRvB..94h5403L"><span>Valley-dependent <span class="hlt">band</span> structure and valley polarization in periodically modulated graphene</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lu, Wei-Tao</p> <p>2016-08-01</p> <p>The valley-dependent <span class="hlt">energy</span> <span class="hlt">band</span> and transport property of graphene under a periodic magnetic-strained field are studied, where the time-reversal symmetry is broken and the valley degeneracy is lifted. The considered superlattice is composed of two different barriers, providing more degrees of freedom for engineering the <span class="hlt">electronic</span> structure. The <span class="hlt">electrons</span> near the K and K' valleys are dominated by different effective superlattices. It is found that the <span class="hlt">energy</span> <span class="hlt">bands</span> for both valleys are symmetric with respect to ky=-(AM+ξ AS) /4 under the symmetric superlattices. More finite-<span class="hlt">energy</span> Dirac points, more prominent collimation behavior, and new crossing points are found for K' valley. The degenerate miniband near the K valley splits into two subminibands and produces a new <span class="hlt">band</span> gap under the asymmetric superlattices. The velocity for the K' valley is greatly renormalized compared with the K valley, and so we can achieve a finite velocity for the K valley while the velocity for the K' valley is zero. Especially, the miniband and <span class="hlt">band</span> gap could be manipulated independently, leading to an increase of the conductance. The characteristics of the <span class="hlt">band</span> structure are reflected in the transmission spectra. The Dirac points and the crossing points appear as pronounced peaks in transmission. A remarkable valley polarization is obtained which is robust to the disorder and can be controlled by the strain, the period, and the voltage.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22004886-electron-electron-interaction-spin-orbit-coupling-inas-alsb-heterostructures-two-dimensional-electron-gas','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22004886-electron-electron-interaction-spin-orbit-coupling-inas-alsb-heterostructures-two-dimensional-electron-gas"><span><span class="hlt">Electron-electron</span> interaction and spin-orbit coupling in InAs/AlSb heterostructures with a two-dimensional <span class="hlt">electron</span> gas</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Gavrilenko, V. I.; Krishtopenko, S. S., E-mail: ds_a-teens@mail.ru; Goiran, M.</p> <p>2011-01-15</p> <p>The effect of <span class="hlt">electron-electron</span> interaction on the spectrum of two-dimensional <span class="hlt">electron</span> states in InAs/AlSb (001) heterostructures with a GaSb cap layer with one filled size-quantization subband. The <span class="hlt">energy</span> spectrum of two-dimensional <span class="hlt">electrons</span> is calculated in the Hartree and Hartree-Fock approximations. It is shown that the exchange interaction decreasing the <span class="hlt">electron</span> <span class="hlt">energy</span> in subbands increases the <span class="hlt">energy</span> gap between subbands and the spin-orbit splitting of the spectrum in the entire region of <span class="hlt">electron</span> concentrations, at which only the lower size-quantization <span class="hlt">band</span> is filled. The nonlinear dependence of the Rashba splitting constant at the Fermi wave vector on the concentration of two-dimensionalmore » <span class="hlt">electrons</span> is demonstrated.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010NIMPA.614..335F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010NIMPA.614..335F"><span><span class="hlt">Energy</span> monitoring device for 1.5-2.4 MeV <span class="hlt">electron</span> beams</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fuochi, P. G.; Lavalle, M.; Martelli, A.; Kovács, A.; Mehta, K.; Kuntz, F.; Plumeri, S.</p> <p>2010-03-01</p> <p>An easy-to-use and robust <span class="hlt">energy</span> monitoring device has been developed for reliable detection of day-to-day small variations in the <span class="hlt">electron</span> beam <span class="hlt">energy</span>, a critical parameter for quality control and quality assurance in industrial radiation processing. It has potential for using on-line, thus providing real-time information. Its working principle is based on the measurement of currents, or charges, collected by two aluminium absorbers of specific thicknesses (dependent on the beam <span class="hlt">energy</span>), insulated from each other and positioned within a faraday cup-style aluminium cage connected to the ground. The device has been extensively tested in the <span class="hlt">energy</span> range of 4-12 MeV under standard laboratory conditions at Institute of Isotopes and CNR-ISOF using different types of <span class="hlt">electron</span> accelerators; namely, a TESLA LPR-4 LINAC (3-6 MeV) and a L-<span class="hlt">band</span> Vickers LINAC (7-12 MeV), respectively. This device has been also tested in high power <span class="hlt">electron</span> beam radiation processing facilities, one equipped with a 7-MeV LUE-8 linear accelerator used for crosslinking of cables and medical device sterilization, and the other equipped with a 10 MeV Rhodotron TT100 recirculating accelerator used for in-house sterilization of medical devices. In the present work, we have extended the application of this method to still lower <span class="hlt">energy</span> region, i.e. from 1.5 to 2.4 MeV. Also, we show that such a device is capable of detecting deviation in the beam <span class="hlt">energy</span> as small as 40 keV.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007EPJB...59..391D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007EPJB...59..391D"><span><span class="hlt">Energy</span> diffusion controlled reaction rate of reacting particle driven by broad-<span class="hlt">band</span> noise</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Deng, M. L.; Zhu, W. Q.</p> <p>2007-10-01</p> <p>The <span class="hlt">energy</span> diffusion controlled reaction rate of a reacting particle with linear weak damping and broad-<span class="hlt">band</span> noise excitation is studied by using the stochastic averaging method. First, the stochastic averaging method for strongly nonlinear oscillators under broad-<span class="hlt">band</span> noise excitation using generalized harmonic functions is briefly introduced. Then, the reaction rate of the classical Kramers' reacting model with linear weak damping and broad-<span class="hlt">band</span> noise excitation is investigated by using the stochastic averaging method. The averaged Itô stochastic differential equation describing the <span class="hlt">energy</span> diffusion and the Pontryagin equation governing the mean first-passage time (MFPT) are established. The <span class="hlt">energy</span> diffusion controlled reaction rate is obtained as the inverse of the MFPT by solving the Pontryagin equation. The results of two special cases of broad-<span class="hlt">band</span> noises, i.e. the harmonic noise and the exponentially corrected noise, are discussed in details. It is demonstrated that the general expression of reaction rate derived by the authors can be reduced to the classical ones via linear approximation and high potential barrier approximation. The good agreement with the results of the Monte Carlo simulation verifies that the reaction rate can be well predicted using the stochastic averaging method.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AIPC.1953i0066S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AIPC.1953i0066S"><span>Optical absorption spectra and <span class="hlt">energy</span> <span class="hlt">band</span> gap in manganese containing sodium zinc phosphate glasses</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sardarpasha, K. R.; Hanumantharaju, N.; Gowda, V. C. Veeranna</p> <p>2018-05-01</p> <p>Optical <span class="hlt">band</span> gap <span class="hlt">energy</span> in the system 25Na2O-(75-x)[0.6P2O5-0.4ZnO]-xMnO2 (where x = 0.5,1,5,10 and 20 mol.%) have been studied. The intensity of the absorption <span class="hlt">band</span> found to increase with increase of MnO2 content. The decrease in the optical <span class="hlt">band</span> gap <span class="hlt">energy</span> with increase in MnO2 content in the investigated glasses is attributed to shifting of absorption edge to a longer wavelength region. The obtained results were discussed in view of the structure of phosphate glass network.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1345934-unraveling-excitation-mechanisms-highly-oblique-lower-band-chorus-waves','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1345934-unraveling-excitation-mechanisms-highly-oblique-lower-band-chorus-waves"><span>Unraveling the excitation mechanisms of highly oblique lower-<span class="hlt">band</span> chorus waves</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Li, Wen; Mourenas, D.; Artemyev, A. V.; ...</p> <p>2016-08-17</p> <p>Excitation mechanisms of highly oblique, quasi-electrostatic lower <span class="hlt">band</span> chorus waves are investigated using Van Allen Probes observations near the equator of the Earth's magnetosphere. Linear growth rates are evaluated based on in situ, measured <span class="hlt">electron</span> velocity distributions and plasma conditions and compared with simultaneously observed wave frequency spectra and wave normal angles. Accordingly, two distinct excitation mechanisms of highly oblique lower <span class="hlt">band</span> chorus have been clearly identified for the first time. The first mechanism relies on cyclotron resonance with <span class="hlt">electrons</span> possessing both a realistic temperature anisotropy at keV <span class="hlt">energies</span> and a plateau at 100–500 eV in the parallel velocity distribution.more » The second mechanism corresponds to Landau resonance with a 100–500 eV beam. In both cases, a small low-<span class="hlt">energy</span> beam-like component is necessary for suppressing an otherwise dominating Landau damping. In conclusion, our new findings suggest that small variations in the <span class="hlt">electron</span> distribution could have important impacts on energetic <span class="hlt">electron</span> dynamics.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22486015-experimental-theoretical-investigations-electronic-band-structure-metal-organic-frameworks-hkust-type','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22486015-experimental-theoretical-investigations-electronic-band-structure-metal-organic-frameworks-hkust-type"><span>Experimental and theoretical investigations of the <span class="hlt">electronic</span> <span class="hlt">band</span> structure of metal-organic frameworks of HKUST-1 type</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Gu, Zhi-Gang; State Key Laboratory of Structural Chemistry, Fujian Institute of Research on the Structure of Matter, Chinese Academy of Sciences, 350002 Fuzhou; Heinke, Lars, E-mail: Lars.Heinke@KIT.edu</p> <p></p> <p>The <span class="hlt">electronic</span> properties of metal-organic frameworks (MOFs) are increasingly attracting the attention due to potential applications in sensor techniques and (micro-) <span class="hlt">electronic</span> engineering, for instance, as low-k-dielectric in semiconductor technology. Here, the <span class="hlt">band</span> gap and the <span class="hlt">band</span> structure of MOFs of type HKUST-1 are studied in detail by means of spectroscopic ellipsometry applied to thin surface-mounted MOF films and by means of quantum chemical calculations. The analysis of the density of states, the <span class="hlt">band</span> structure, and the excitation spectrum reveal the importance of the empty Cu-3d orbitals for the <span class="hlt">electronic</span> properties of HKUST-1. This study shows that, in contrast tomore » common belief, even in the case of this fairly “simple” MOF, the excitation spectra cannot be explained by a superposition of “intra-unit” excitations within the individual building blocks. Instead, “inter-unit” excitations also have to be considered.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001JChPh.115.3497T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001JChPh.115.3497T"><span><span class="hlt">Electronic</span> <span class="hlt">energy</span> density in chemical reaction systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tachibana, Akitomo</p> <p>2001-08-01</p> <p>The <span class="hlt">energy</span> of chemical reaction is visualized in real space using the <span class="hlt">electronic</span> <span class="hlt">energy</span> density nE(r⃗) associated with the <span class="hlt">electron</span> density n(r⃗). The <span class="hlt">electronic</span> <span class="hlt">energy</span> density nE(r⃗) is decomposed into the kinetic <span class="hlt">energy</span> density nT(r⃗), the external potential <span class="hlt">energy</span> density nV(r⃗), and the interelectron potential <span class="hlt">energy</span> density nW(r⃗). Using the <span class="hlt">electronic</span> <span class="hlt">energy</span> density nE(r⃗) we can pick up any point in a chemical reaction system and find how the <span class="hlt">electronic</span> <span class="hlt">energy</span> E is assigned to the selected point. We can then integrate the <span class="hlt">electronic</span> <span class="hlt">energy</span> density nE(r⃗) in any region R surrounding the point and find out the regional <span class="hlt">electronic</span> <span class="hlt">energy</span> ER to the global E. The kinetic <span class="hlt">energy</span> density nT(r⃗) is used to identify the intrinsic shape of the reactants, the <span class="hlt">electronic</span> transition state, and the reaction products along the course of the chemical reaction coordinate. The intrinsic shape is identified with the <span class="hlt">electronic</span> interface S that discriminates the region RD of the <span class="hlt">electronic</span> drop from the region RA of the <span class="hlt">electronic</span> atmosphere in the density distribution of the <span class="hlt">electron</span> gas. If the R spans the whole space, then the integral gives the total E. The regional <span class="hlt">electronic</span> <span class="hlt">energy</span> ER in thermodynamic ensemble is realized in electrochemistry as the intrinsic Volta electric potential φR and the intrinsic Herring-Nichols work function ΦR. We have picked up first a hydrogen-like atom for which we have analytical exact expressions of the relativistic kinetic <span class="hlt">energy</span> density nTM(r⃗) and its nonrelativistic version nT(r⃗). These expressions are valid for any excited bound states as well as the ground state. Second, we have selected the following five reaction systems and show the figures of the nT(r⃗) as well as the other <span class="hlt">energy</span> densities along the intrinsic reaction coordinates: a protonation reaction to He, addition reactions of HF to C2H4 and C2H2, hydrogen abstraction reactions of NH3+ from HF and NH3. Valence <span class="hlt">electrons</span> possess their unique</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26563679','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26563679"><span><span class="hlt">Electronic</span> <span class="hlt">band</span>-gap modified passive silicon optical modulator at telecommunications wavelengths.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhang, Rui; Yu, Haohai; Zhang, Huaijin; Liu, Xiangdong; Lu, Qingming; Wang, Jiyang</p> <p>2015-11-13</p> <p>The silicon optical modulator is considered to be the workhorse of a revolution in communications. In recent years, the capabilities of externally driven active silicon optical modulators have dramatically improved. Self-driven passive modulators, especially passive silicon modulators, possess advantages in compactness, integration, low-cost, etc. Constrained by a large indirect <span class="hlt">band</span>-gap and sensitivity-related loss, the passive silicon optical modulator is scarce and has been not advancing, especially at telecommunications wavelengths. Here, a passive silicon optical modulator is fabricated by introducing an impurity <span class="hlt">band</span> in the <span class="hlt">electronic</span> <span class="hlt">band</span>-gap, and its nonlinear optics and applications in the telecommunications-wavelength lasers are investigated. The saturable absorption properties at the wavelength of 1.55 μm was measured and indicates that the sample is quite sensitive to light intensity and has negligible absorption loss. With a passive silicon modulator, pulsed lasers were constructed at wavelengths at 1.34 and 1.42 μm. It is concluded that the sensitive self-driven passive silicon optical modulator is a viable candidate for photonics applications out to 2.5 μm.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1994TSF...253..269S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1994TSF...253..269S"><span>Use of valence <span class="hlt">band</span> Auger <span class="hlt">electron</span> spectroscopy to study thin film growth: oxide and diamond-like carbon films</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Steffen, H. J.</p> <p>1994-12-01</p> <p>It is demonstrated how Auger line shape analysis with factor analysis (FA), least-squares fitting and even simple peak height measurements may provide detailed information about the composition, different chemical states and also defect concentration or crystal order. Advantage is taken of the capability of Auger <span class="hlt">electron</span> spectroscopy to give valence <span class="hlt">band</span> structure information with high surface sensitivity and the special aspect of FA to identify and discriminate quantitatively unknown chemical species. Valence <span class="hlt">band</span> spectra obtained from Ni, Fe, Cr and NiFe40Cr20 during oxygen exposure at room temperature reveal the oxidation process in the initial stage of the thin layer formation. Furthermore, the carbon chemical states that were formed during low <span class="hlt">energy</span> C(+) and Ne(+) ion irradiation of graphite are delineated and the evolution of an amorphous network with sp3 bonds is disclosed. The analysis represents a unique method to quantify the fraction of sp3-hybridized carbon in diamond-like materials.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018MRE.....5a6301M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MRE.....5a6301M"><span>Enhancement of Seebeck coefficient in graphene superlattices by <span class="hlt">electron</span> filtering technique</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mishra, Shakti Kumar; Kumar, Amar; Kaushik, Chetan Prakash; Dikshit, Biswaranjan</p> <p>2018-01-01</p> <p>We show theoretically that the Seebeck coefficient and the thermoelectric figure of merit can be increased by using <span class="hlt">electron</span> filtering technique in graphene superlattice based thermoelectric devices. The average Seebeck coefficient for graphene-based thermoelectric devices is proportional to the integral of the distribution of Seebeck coefficient versus <span class="hlt">energy</span> of <span class="hlt">electrons</span>. The low <span class="hlt">energy</span> <span class="hlt">electrons</span> in the distribution curve are found to reduce the average Seebeck coefficient as their contribution is negative. We show that, with <span class="hlt">electron</span> <span class="hlt">energy</span> filtering technique using multiple graphene superlattice heterostructures, the low <span class="hlt">energy</span> <span class="hlt">electrons</span> can be filtered out and the Seebeck coefficient can be increased. The multiple graphene superlattice heterostructures can be formed by graphene superlattices with different periodic electric potentials applied above the superlattice. The overall <span class="hlt">electronic</span> <span class="hlt">band</span> gap of the multiple heterostructures is dependent upon the individual <span class="hlt">band</span> gap of the graphene superlattices and can be tuned by varying the periodic electric potentials. The overall <span class="hlt">electronic</span> <span class="hlt">band</span> gap of the multiple heterostructures has to be properly chosen such that, the low <span class="hlt">energy</span> <span class="hlt">electrons</span> which cause negative Seebeck distribution in single graphene superlattice thermoelectric devices fall within the overall <span class="hlt">band</span> gap formed by the multiple heterostructures. Although the electrical conductance is decreased in this technique reducing the thermoelectric figure of merit, the overall figure of merit is increased due to huge increase in Seebeck coefficient and its square dependency upon the Seebeck coefficient. This is an easy technique to make graphene superlattice based thermoelectric devices more efficient and has the potential to significantly improve the technology of <span class="hlt">energy</span> harvesting and sensors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JAP...123p1599W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JAP...123p1599W"><span>A density functional study of the effect of hydrogen on <span class="hlt">electronic</span> properties and <span class="hlt">band</span> discontinuity at anatase TiO2/diamond interface</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wu, Kongping; Liao, Meiyong; Sang, Liwen; Liu, Jiangwei; Imura, Masataka; Ye, Haitao; Koide, Yasuo</p> <p>2018-04-01</p> <p>Tailoring the <span class="hlt">electronic</span> states of the dielectric oxide/diamond interface is critical to the development of next generation semiconductor devices like high-power high-frequency field-effect transistors. In this work, we investigate the <span class="hlt">electronic</span> states of the TiO2/diamond 2 × 1-(100) interface by using first principles total <span class="hlt">energy</span> calculations. Based on the calculation of the chemical potentials for the TiO2/diamond interface, it is observed that the hetero-interfaces with the C-OTi configuration or with two O vacancies are the most energetically favorable structures under the O-rich condition and under Ti-rich condition, respectively. The <span class="hlt">band</span> structure and density of states of both TiO2/diamond and TiO2/H-diamond hetero-structures are calculated. It is revealed that there are considerable interface states at the interface of the anatase TiO2/diamond hetero-structure. By introducing H on the diamond surface, the interface states are significantly suppressed. A type-II alignment <span class="hlt">band</span> structure is disclosed at the interface of the TiO2/diamond hetero-structure. The valence <span class="hlt">band</span> offset increases from 0.6 to 1.7 eV when H is introduced at the TiO2/diamond interface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhPl...25d3120Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhPl...25d3120Z"><span>Optimization of a triode-type cusp <span class="hlt">electron</span> gun for a W-<span class="hlt">band</span> gyro-TWA</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Liang; Donaldson, Craig R.; He, Wenlong</p> <p>2018-04-01</p> <p>A triode-type cusp <span class="hlt">electron</span> gun was optimized through numerical simulations for a W-<span class="hlt">band</span> gyrotron traveling wave amplifier. An additional electrode in front of the cathode could switch the <span class="hlt">electron</span> beam on and off instantly when its electric potential is properly biased. An optimal <span class="hlt">electron</span> beam of current 1.7 A and a velocity ratio (alpha) of 1.12 with an alpha spread of ˜10.7% was achieved when the triode gun was operated at 40 kV.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_15 --> <div id="page_16" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="301"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JSP...170..399T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JSP...170..399T"><span>Ferromagnetism in the Hubbard Model with a Gapless Nearly-Flat <span class="hlt">Band</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tanaka, Akinori</p> <p>2018-01-01</p> <p>We present a version of the Hubbard model with a gapless nearly-flat lowest <span class="hlt">band</span> which exhibits ferromagnetism in two or more dimensions. The model is defined on a lattice obtained by placing a site on each edge of the hypercubic lattice, and <span class="hlt">electron</span> hopping is assumed to be only between nearest and next nearest neighbor sites. The lattice, where all the sites are identical, is simple, and the corresponding single-<span class="hlt">electron</span> <span class="hlt">band</span> structure, where two cosine-type <span class="hlt">bands</span> touch without an <span class="hlt">energy</span> gap, is also simple. We prove that the ground state of the model is unique and ferromagnetic at half-filling of the lower <span class="hlt">band</span>, if the lower <span class="hlt">band</span> is nearly flat and the strength of on-site repulsion is larger than a certain value which is independent of the lattice size. This is the first example of ferromagnetism in three dimensional non-singular models with a gapless <span class="hlt">band</span> structure.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23396813','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23396813"><span>Quasiparticle semiconductor <span class="hlt">band</span> structures including spin-orbit interactions.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Malone, Brad D; Cohen, Marvin L</p> <p>2013-03-13</p> <p>We present first-principles calculations of the quasiparticle <span class="hlt">band</span> structure of the group IV materials Si and Ge and the group III-V compound semiconductors AlP, AlAs, AlSb, InP, InAs, InSb, GaP, GaAs and GaSb. Calculations are performed using the plane wave pseudopotential method and the 'one-shot' GW method, i.e. G(0)W(0). Quasiparticle <span class="hlt">band</span> structures, augmented with the effects of spin-orbit, are obtained via a Wannier interpolation of the obtained quasiparticle <span class="hlt">energies</span> and calculated spin-orbit matrix. Our calculations explicitly treat the shallow semicore states of In and Ga, which are known to be important in the description of the <span class="hlt">electronic</span> properties, as valence states in the quasiparticle calculation. Our calculated quasiparticle <span class="hlt">energies</span>, combining both the ab initio evaluation of the <span class="hlt">electron</span> self-<span class="hlt">energy</span> and the vector part of the pseudopotential representing the spin-orbit effects, are in generally very good agreement with experimental values. These calculations illustrate the predictive power of the methodology as applied to group IV and III-V semiconductors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ApSS..396.1562P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ApSS..396.1562P"><span>Reconstructing the <span class="hlt">energy</span> <span class="hlt">band</span> <span class="hlt">electronic</span> structure of pulsed laser deposited CZTS thin films intended for solar cell absorber applications</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pandiyan, Rajesh; Oulad Elhmaidi, Zakaria; Sekkat, Zouheir; Abd-lefdil, Mohammed; El Khakani, My Ali</p> <p>2017-02-01</p> <p>We report here on the use of pulsed KrF-laser deposition (PLD) technique for the growth of high-quality Cu2ZnSnS4 (CZTS) thin films onto Si, and glass substrates without resorting to any post sulfurization process. The PLD-CZTS films were deposited at room temperature (RT) and then subjected to post annealing at different temperatures ranging from 200 to 500 °C in Argon atmosphere. The X-ray diffraction and Raman spectroscopy confirmed that the PLD films crystallize in the characteristic kesterite CZTS structure regardless of their annealing temperature (Ta), but their crystallinity is much improved for Ta ≥ 400 °C. The PLD-CZTS films were found to exhibit a relatively dense morphology with a surface roughness (RMS) that increases with Ta (from ∼14 nm at RT to 70 nm at Ta = 500 °C with a value around 40 nm for Ta = 300-400 °C). The optical bandgap of the PLD-CZTS films, was derived from UV-vis transmission spectra analysis, and found to decrease from 1.73 eV for non-annealed films to ∼1.58 eV for those annealed at Ta = 300 °C. These <span class="hlt">band</span> gap values are very close to the optimum value needed for an ideal solar cell absorber. In order to achieve a complete reconstruction of the one-dimensional <span class="hlt">energy</span> <span class="hlt">band</span> structure of these PLD-CZTS absorbers, we have combined both XPS and UPS spectroscopies to determine their chemical bondings, the position of their valence <span class="hlt">band</span> maximum (relative to Fermi level), and their work function values. This enabled us to sketch out, as accurately as possible, the <span class="hlt">band</span> alignment of the heterojunction interface formed between CZTS and both CdS and ZnS buffer layer materials.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990018629&hterms=Magnetic+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DMagnetic%2Benergy','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990018629&hterms=Magnetic+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DMagnetic%2Benergy"><span>Spatial and Temporal <span class="hlt">Energy</span> Characterization of Precipitating <span class="hlt">Electrons</span> for the January 10th, 1997 Magnetic Cloud Event</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Spann, J. F., Jr.; Germany, G. A.; Brittnacher, M. J.; Parks, G. K.; Elsen, R.</p> <p>1997-01-01</p> <p>The January 10-11, 1997 magnetic cloud event provided a rare opportunity to study auroral <span class="hlt">energy</span> deposition under varying but intense IMF conditions. The Wind spacecraft located about 100 RE upstream monitored the IMF and plasma parameters during the passing of the cloud. The Polar Ultraviolet Imager (UVI) observed the aurora[ precipitation during the first encounter of the cloud with Earth's magnetosphere and during several subsequent substorm events. The UVI has the unique capability of measuring the <span class="hlt">energy</span> flux and characteristic <span class="hlt">energy</span> of the precipitating <span class="hlt">electrons</span> through the use of narrow <span class="hlt">band</span> filters that distinguish short and long wavelength molecular nitrogen emissions. The spatial and temporal characteristics of the precipitating <span class="hlt">electron</span> <span class="hlt">energy</span> will be discussed beginning with the inception of the event at the Earth early January 1 Oth and continuing through the subsidence of auroral activity on January 11th.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27812035','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27812035"><span>Engineering of <span class="hlt">band</span> gap states of amorphous SiZnSnO semiconductor as a function of Si doping concentration.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Choi, Jun Young; Heo, Keun; Cho, Kyung-Sang; Hwang, Sung Woo; Kim, Sangsig; Lee, Sang Yeol</p> <p>2016-11-04</p> <p>We investigated the <span class="hlt">band</span> gap of SiZnSnO (SZTO) with different Si contents. <span class="hlt">Band</span> gap engineering of SZTO is explained by the evolution of the <span class="hlt">electronic</span> structure, such as changes in the <span class="hlt">band</span> edge states and <span class="hlt">band</span> gap. Using ultraviolet photoelectron spectroscopy (UPS), it was verified that Si atoms can modify the <span class="hlt">band</span> gap of SZTO thin films. Carrier generation originating from oxygen vacancies can modify the <span class="hlt">band</span>-gap states of oxide films with the addition of Si. Since it is not easy to directly derive changes in the <span class="hlt">band</span> gap states of amorphous oxide semiconductors, no reports of the relationship between the Fermi <span class="hlt">energy</span> level of oxide semiconductor and the device stability of oxide thin film transistors (TFTs) have been presented. The addition of Si can reduce the total density of trap states and change the <span class="hlt">band</span>-gap properties. When 0.5 wt% Si was used to fabricate SZTO TFTs, they showed superior stability under negative bias temperature stress. We derived the <span class="hlt">band</span> gap and Fermi <span class="hlt">energy</span> level directly using data from UPS, Kelvin probe, and high-resolution <span class="hlt">electron</span> <span class="hlt">energy</span> loss spectroscopy analyses.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5095643','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5095643"><span>Engineering of <span class="hlt">band</span> gap states of amorphous SiZnSnO semiconductor as a function of Si doping concentration</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Choi, Jun Young; Heo, Keun; Cho, Kyung-Sang; Hwang, Sung Woo; Kim, Sangsig; Lee, Sang Yeol</p> <p>2016-01-01</p> <p>We investigated the <span class="hlt">band</span> gap of SiZnSnO (SZTO) with different Si contents. <span class="hlt">Band</span> gap engineering of SZTO is explained by the evolution of the <span class="hlt">electronic</span> structure, such as changes in the <span class="hlt">band</span> edge states and <span class="hlt">band</span> gap. Using ultraviolet photoelectron spectroscopy (UPS), it was verified that Si atoms can modify the <span class="hlt">band</span> gap of SZTO thin films. Carrier generation originating from oxygen vacancies can modify the <span class="hlt">band</span>-gap states of oxide films with the addition of Si. Since it is not easy to directly derive changes in the <span class="hlt">band</span> gap states of amorphous oxide semiconductors, no reports of the relationship between the Fermi <span class="hlt">energy</span> level of oxide semiconductor and the device stability of oxide thin film transistors (TFTs) have been presented. The addition of Si can reduce the total density of trap states and change the <span class="hlt">band</span>-gap properties. When 0.5 wt% Si was used to fabricate SZTO TFTs, they showed superior stability under negative bias temperature stress. We derived the <span class="hlt">band</span> gap and Fermi <span class="hlt">energy</span> level directly using data from UPS, Kelvin probe, and high-resolution <span class="hlt">electron</span> <span class="hlt">energy</span> loss spectroscopy analyses. PMID:27812035</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PhDT........81W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhDT........81W"><span>Probing the <span class="hlt">band</span> structure and local <span class="hlt">electronic</span> properties of low-dimensional semiconductor structures</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Walrath, Jenna Cherie</p> <p></p> <p>Low-dimensional semiconductor structures are important for a wide variety of applications, and recent advances in nanoscale fabrication are paving the way for increasingly precise nano-engineering of a wide range of materials. It is therefore essential that the physics of materials at the nanoscale are thoroughly understood to unleash the full potential of nanotechnology, requiring the development of increasingly sophisticated instrumentation and modeling. Of particular interest is the relationship between the local density of states (LDOS) of low-dimensional structures and the <span class="hlt">band</span> structure and local <span class="hlt">electronic</span> properties. This dissertation presents the investigation of the <span class="hlt">band</span> structure, LDOS, and local <span class="hlt">electronic</span> properties of nanostructures ranging from zero-dimensional (0D) quantum dots (QDs) to two-dimensional (2D) thin films, synthesizing computational and experimental approaches including Poisson-Schrodinger <span class="hlt">band</span> structure calculations, scanning tunneling microscopy (STM), scanning tunneling spectroscopy (STS), and scanning thermoelectric microscopy (SThEM). A method is presented for quantifying the local Seebeck coefficient (S) with SThEM, using a quasi-3D conversion matrix approach to directly convert temperature gradient-induced voltages S. For a GaAs p-n junction, the resulting S-profile is consistent with that computed using the free carrier concentration profile. This combined computational-experimental approach is expected to enable nanoscale measurements of S across a wide variety of heterostructure interfaces. The local carrier concentration, n, is profiled across epitaxial InAs/GaAs QDs, where SThEM is used to profile the temperature gradient-induced voltage, which is converted to a profile of the local S and finally to an n profile. The S profile is converted to a conduction <span class="hlt">band</span>-edge profile and compared with Poisson-Schrodinger <span class="hlt">band</span>-edge simulations. The combined computational-experimental approach suggests a reduced n in the QD center in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22657899-effective-hamiltonians-correlated-narrow-energy-band-systems-magnetic-insulators-role-spin-orbit-interactions-metal-insulator-transitions-magnetic-phase-transitions','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22657899-effective-hamiltonians-correlated-narrow-energy-band-systems-magnetic-insulators-role-spin-orbit-interactions-metal-insulator-transitions-magnetic-phase-transitions"><span>Effective Hamiltonians for correlated narrow <span class="hlt">energy</span> <span class="hlt">band</span> systems and magnetic insulators: Role of spin-orbit interactions in metal-insulator transitions and magnetic phase transitions</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Chakraborty, Subrata; Vijay, Amrendra, E-mail: avijay@iitm.ac.in</p> <p></p> <p>Using a second-quantized many-<span class="hlt">electron</span> Hamiltonian, we obtain (a) an effective Hamiltonian suitable for materials whose <span class="hlt">electronic</span> properties are governed by a set of strongly correlated <span class="hlt">bands</span> in a narrow <span class="hlt">energy</span> range and (b) an effective spin-only Hamiltonian for magnetic materials. The present Hamiltonians faithfully include phonon and spin-related interactions as well as the external fields to study the electromagnetic response properties of complex materials and they, in appropriate limits, reduce to the model Hamiltonians due to Hubbard and Heisenberg. With the Hamiltonian for narrow-<span class="hlt">band</span> strongly correlated materials, we show that the spin-orbit interaction provides a mechanism for metal-insulator transition, whichmore » is distinct from the Mott-Hubbard (driven by the <span class="hlt">electron</span> correlation) and the Anderson mechanism (driven by the disorder). Next, with the spin-only Hamiltonian, we demonstrate the spin-orbit interaction to be a reason for the existence of antiferromagnetic phase in materials which are characterized by a positive isotropic spin-exchange <span class="hlt">energy</span>. This is distinct from the Néel-VanVleck-Anderson paradigm which posits a negative spin-exchange for the existence of antiferromagnetism. We also find that the Néel temperature increases as the absolute value of the spin-orbit coupling increases.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22590494-band-gap-tuning-amorphous-al-oxides-zr-alloying','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22590494-band-gap-tuning-amorphous-al-oxides-zr-alloying"><span><span class="hlt">Band</span> gap tuning of amorphous Al oxides by Zr alloying</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Canulescu, S., E-mail: stec@fotonik.dtu.dk; Schou, J.; Jones, N. C.</p> <p>2016-08-29</p> <p>The optical <span class="hlt">band</span> gap and <span class="hlt">electronic</span> structure of amorphous Al-Zr mixed oxides with Zr content ranging from 4.8 to 21.9% were determined using vacuum ultraviolet and X-ray absorption spectroscopy. The light scattering by the nano-porous structure of alumina at low wavelengths was estimated based on the Mie scattering theory. The dependence of the optical <span class="hlt">band</span> gap of the Al-Zr mixed oxides on the Zr content deviates from linearity and decreases from 7.3 eV for pure anodized Al{sub 2}O{sub 3} to 6.45 eV for Al-Zr mixed oxides with a Zr content of 21.9%. With increasing Zr content, the conduction <span class="hlt">band</span> minimum changes non-linearlymore » as well. Fitting of the <span class="hlt">energy</span> <span class="hlt">band</span> gap values resulted in a bowing parameter of ∼2 eV. The <span class="hlt">band</span> gap bowing of the mixed oxides is assigned to the presence of the Zr d-<span class="hlt">electron</span> states localized below the conduction <span class="hlt">band</span> minimum of anodized Al{sub 2}O{sub 3}.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22486039-elimination-surface-band-bending-polar-inn-thin-gan-capping','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22486039-elimination-surface-band-bending-polar-inn-thin-gan-capping"><span>Elimination of surface <span class="hlt">band</span> bending on N-polar InN with thin GaN capping</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Kuzmík, J., E-mail: Jan.Kuzmik@savba.sk; Haščík, Š.; Kučera, M.</p> <p>2015-11-09</p> <p>0.5–1 μm thick InN (0001) films grown by molecular-beam epitaxy with N- or In-polarity are investigated for the presence of native oxide, surface <span class="hlt">energy</span> <span class="hlt">band</span> bending, and effects introduced by 2 to 4 monolayers of GaN capping. Ex situ angle-resolved x-ray photo-<span class="hlt">electron</span> spectroscopy is used to construct near-surface (GaN)/InN <span class="hlt">energy</span> profiles, which is combined with deconvolution of In3d signal to trace the presence of InN native oxide for different types of polarity and capping. Downwards surface <span class="hlt">energy</span> <span class="hlt">band</span> bending was observed on bare samples with native oxide, regardless of the polarity. It was found that the In-polar InN surface is mostmore » readily oxidized, however, with only slightly less <span class="hlt">band</span> bending if compared with the N-polar sample. On the other hand, InN surface oxidation was effectively mitigated by GaN capping. Still, as confirmed by ultra-violet photo-<span class="hlt">electron</span> spectroscopy and by <span class="hlt">energy</span> <span class="hlt">band</span> diagram calculations, thin GaN cap layer may provide negative piezoelectric polarization charge at the GaN/InN hetero-interface of the N-polar sample, in addition to the passivation effect. These effects raised the <span class="hlt">band</span> diagram up by about 0.65 eV, reaching a flat-<span class="hlt">band</span> profile.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1997APS..PAC..7P48N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1997APS..PAC..7P48N"><span>High Peak Power Test and Evaluation of S-<span class="hlt">band</span> Waveguide Switches</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nassiri, A.; Grelick, A.; Kustom, R. L.; White, M.</p> <p>1997-05-01</p> <p>The injector and source of particles for the Advanced Photon Source is a 2856-MHz S-<span class="hlt">band</span> <span class="hlt">electron</span>-positron linear accelerator (linac) which produces <span class="hlt">electrons</span> with <span class="hlt">energies</span> up to 650 MeV or positrons with <span class="hlt">energies</span> up to 450 MeV. To improve the linac rf system availability, an additional modulator-klystron subsystem is being constructed to provide a switchable hot spare unit for each of the five exsisting S-<span class="hlt">band</span> transmitters. The switching of the transmitters will require the use of SF6-pressurized S-<span class="hlt">band</span> waveguide switches at a peak operating power of 35 MW. Such rf switches have been successfully operated at other accelerator facilities but at lower peak powers. A test stand has been set up at the Stanford Linear Accelerator Center (SLAC) Klystron Factory to conduct tests comparing the power handling characteristics of two WR-284 and one WR-340 switches. Test results are presented and their implications for the design of the switching system are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhRvB..96s5103M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvB..96s5103M"><span><span class="hlt">Electronic</span> properties and bonding in Zr Hx thin films investigated by valence-<span class="hlt">band</span> x-ray photoelectron spectroscopy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Magnuson, Martin; Schmidt, Susann; Hultman, Lars; Högberg, Hans</p> <p>2017-11-01</p> <p>The <span class="hlt">electronic</span> structure and chemical bonding in reactively magnetron sputtered Zr Hx (x =0.15 , 0.30, 1.16) thin films with oxygen content as low as 0.2 at.% are investigated by 4d valence <span class="hlt">band</span>, shallow 4p core-level, and 3d core-level x-ray photoelectron spectroscopy. With increasing hydrogen content, we observe significant reduction of the 4d valence states close to the Fermi level as a result of redistribution of intensity toward the H 1s-Zr 4d hybridization region at ˜6 eV below the Fermi level. For low hydrogen content (x =0.15 , 0.30), the films consist of a superposition of hexagonal closest-packed metal (α phase) and understoichiometric δ -Zr Hx (Ca F2 -type structure) phases, while for x =1.16 , the films form single-phase Zr Hx that largely resembles that of stoichiometric δ -Zr H2 phase. We show that the cubic δ -Zr Hx phase is metastable as thin film up to x =1.16 , while for higher H contents the structure is predicted to be tetragonally distorted. For the investigated Zr H1.16 film, we find chemical shifts of 0.68 and 0.51 eV toward higher binding <span class="hlt">energies</span> for the Zr 4 p3 /2 and 3 d5 /2 peak positions, respectively. Compared to the Zr metal binding <span class="hlt">energies</span> of 27.26 and 178.87 eV, this signifies a charge transfer from Zr to H atoms. The change in the <span class="hlt">electronic</span> structure, spectral line shapes, and chemical shifts as a function of hydrogen content is discussed in relation to the charge transfer from Zr to H that affects the conductivity by charge redistribution in the valence <span class="hlt">band</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016SPIE.9748E..27M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016SPIE.9748E..27M"><span>Wurtzite/zinc-blende <span class="hlt">electronic-band</span> alignment in basal-plane stacking faults in semi-polar GaN</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Monavarian, Morteza; Hafiz, Shopan; Izyumskaya, Natalia; Das, Saikat; Özgür, Ümit; Morkoç, Hadis; Avrutin, Vitaliy</p> <p>2016-02-01</p> <p>Heteroepitaxial semipolar and nonpolar GaN layers often suffer from high densities of extended defects including basal plane stacking faults (BSFs). BSFs which are considered as inclusions of cubic zinc-blende phase in wurtzite matrix act as quantum wells strongly affecting device performance. <span class="hlt">Band</span> alignment in BSFs has been discussed as type of <span class="hlt">band</span> alignment at the wurtzite/zinc blende interface governs the response in differential transmission; fast decay after the pulse followed by slow recovery due to spatial splitting of <span class="hlt">electrons</span> and heavy holes for type- II <span class="hlt">band</span> alignment in contrast to decay with no recovery in case of type I <span class="hlt">band</span> alignment. Based on the results, <span class="hlt">band</span> alignment is demonstrated to be of type II in zinc-blende segments in wurtzite matrix as in BSFs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1988AcSpA..44..505S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1988AcSpA..44..505S"><span>Potential <span class="hlt">energy</span> surface and vibrational <span class="hlt">band</span> origins of the triatomic lithium cation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Searles, Debra J.; Dunne, Simon J.; von Nagy-Felsobuki, Ellak I.</p> <p></p> <p>The 104 point CISD Li +3 potential <span class="hlt">energy</span> surface and its analytical representation is reported. The calculations predict the minimum <span class="hlt">energy</span> geometry to be an equilateral triangle of side RLiLi = 3.0 Å and of <span class="hlt">energy</span> - 22.20506 E h. A fifth-order Morse—Dunham type analytical force field is used in the Carney—Porter normal co-ordinate vibrational Hamiltonian, the corresponding eigenvalue problem being solved variationally using a 560 configurational finite-element basis set. The predicted assignment of the vibrational <span class="hlt">band</span> origins is in accord with that reported for H +3. Moreover, for 6Li +3 and 7Li +3 the lowest i.r. accessible <span class="hlt">band</span> origin is the overlineν0,1,±1 predicted to be at 243.6 and 226.0 cm -1 respectively.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JChPh.144l4309J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JChPh.144l4309J"><span>Theoretical and experimental differential cross sections for <span class="hlt">electron</span> impact excitation of the <span class="hlt">electronic</span> <span class="hlt">bands</span> of furfural</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jones, D. B.; Neves, R. F. C.; Lopes, M. C. A.; da Costa, R. F.; do N. Varella, M. T.; Bettega, M. H. F.; Lima, M. A. P.; García, G.; Limão-Vieira, P.; Brunger, M. J.</p> <p>2016-03-01</p> <p>We report results from a joint experimental and theoretical investigation into <span class="hlt">electron</span> scattering from the important industrial species furfural (C5H4O2). Specifically, differential cross sections (DCSs) have been measured and calculated for the <span class="hlt">electron</span>-impact excitation of the <span class="hlt">electronic</span> states of C5H4O2. The measurements were carried out at <span class="hlt">energies</span> in the range 20-40 eV, and for scattered-<span class="hlt">electron</span> angles between 10° and 90°. The <span class="hlt">energy</span> resolution of those experiments was typically ˜80 meV. Corresponding Schwinger multichannel method with pseudo-potential calculations, for <span class="hlt">energies</span> between 6-50 eV and with and without Born-closure, were also performed for a sub-set of the excited <span class="hlt">electronic</span>-states that were accessed in the measurements. Those calculations were undertaken at the static exchange plus polarisation-level using a minimum orbital basis for single configuration interaction (MOB-SCI) approach. Agreement between the measured and calculated DCSs was qualitatively quite good, although to obtain quantitative accord, the theory would need to incorporate even more channels into the MOB-SCI. The role of multichannel coupling on the computed <span class="hlt">electronic</span>-state DCSs is also explored in some detail.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1990JAP....67..908W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1990JAP....67..908W"><span><span class="hlt">Energy</span> <span class="hlt">band</span>-gap calculations of short-period (ZnTe)m(ZnSe)n and (ZnS)m(ZnSe)n strained-layer superlattices</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wu, Yi-hong; Fujita, Shizuo; Fujita, Shigeo</p> <p>1990-01-01</p> <p>We report on the calculations of <span class="hlt">energy</span> <span class="hlt">band</span> gaps based on the semiempirical tight-binding model for short-period (ZnTe)m(ZnSe)n and (ZnS)m(ZnSe)n strained-layer superlattices (SLSs). During the calculation, much attention has been paid to the modeling of strain effect. It is found that (ZnTe)m(ZnSe)n superlattices grown on InAs, InP, and GaAs substrates show very different <span class="hlt">electronic</span> properties from each other, which is consistent with experimental results now available. Assuming that the emission observed for (ZnTe)m(ZnSe)n SLS originates from intrinsic luminescence, we obtain an unstrained valence-<span class="hlt">band</span> offset of 1.136±0.1 eV for this superlattice. On the other hand, the <span class="hlt">band</span> gap of (ZnS)m(ZnSe)n superlattice grown coherently on GaP is found to exhibit a much stronger structure dependence than that grown coherently on GaAs. The difference of <span class="hlt">energy</span> gap between superlattice with equal monolayers (m=n) and the corresponding alloy with equal chalcogenide composition is also discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990041055&hterms=diamond+structure&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Ddiamond%2Bstructure','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990041055&hterms=diamond+structure&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Ddiamond%2Bstructure"><span>Fine Structure in the Secondary <span class="hlt">Electron</span> Emission Peak for Diamond Crystal with (100) Negative <span class="hlt">Electron</span> Affinity Surface</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Asnin, V. M.; Krainsky, I. L.</p> <p>1998-01-01</p> <p>A fine structure was discovered in the low-<span class="hlt">energy</span> peak of the secondary <span class="hlt">electron</span> emission spectra of the diamond surface with negative <span class="hlt">electron</span> affinity. We studied this structure for the (100) surface of the natural type-IIb diamond crystal. We have found that the low-<span class="hlt">energy</span> peak consists of a total of four maxima. The relative <span class="hlt">energy</span> positions of three of them could be related to the <span class="hlt">electron</span> <span class="hlt">energy</span> minima near the bottom of the conduction <span class="hlt">band</span>. The fourth peak, having the lowest <span class="hlt">energy</span>, was attributed to the breakup of the bulk exciton at the surface during the process of secondary <span class="hlt">electron</span> emission.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhyE...88..142R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhyE...88..142R"><span>Multi-shell spherical GaAs /AlxGa1-x As quantum dot shells-size distribution as a mechanism to generate intermediate <span class="hlt">band</span> <span class="hlt">energy</span> levels</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rodríguez-Magdaleno, K. A.; Pérez-Álvarez, R.; Martínez-Orozco, J. C.; Pernas-Salomón, R.</p> <p>2017-04-01</p> <p>In this work the generation of an intermediate <span class="hlt">band</span> of <span class="hlt">energy</span> levels from multi-shell spherical GaAs /AlxGa1-x As quantum dot shells-size distribution is reported. Within the effective mass approximation the <span class="hlt">electronic</span> structure of a GaAs spherical quantum-dot surrounded by one, two and three shells is studied in detail using a numerically stable transfer matrix method. We found that a shells-size distribution characterized by continuously wider GaAs domains is a suitable mechanism to generate the intermediate <span class="hlt">band</span> whose width is also dependent on the Aluminium concentration x. Our results suggest that this effective mechanism can be used for the design of wider intermediate <span class="hlt">band</span> than reported in other quantum systems with possible solar cells enhanced performance.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AIPC.1942e0111S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AIPC.1942e0111S"><span>Determination of shift in <span class="hlt">energy</span> of <span class="hlt">band</span> edges and <span class="hlt">band</span> gap of ZnSe spherical quantum dot</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Siboh, Dutem; Kalita, Pradip Kumar; Sarma, Jayanta Kumar; Nath, Nayan Mani</p> <p>2018-04-01</p> <p>We have determined the quantum confinement induced shifts in <span class="hlt">energy</span> of <span class="hlt">band</span> edges and <span class="hlt">band</span> gap with respect to size of ZnSe spherical quantum dot employing an effective confinement potential model developed in our earlier communication "arXiv:1705.10343". We have also performed phenomenological analysis of our theoretical results in comparison with available experimental data and observe a very good agreement in this regard. Phenomenological success achieved in this regard confirms validity of the confining potential model as well as signifies the capability and applicability of the ansatz for the effective confining potential to have reasonable information in the study of real nano-structured spherical systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29521391','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29521391"><span>Colloidal nanocrystals as LEGO® bricks for building <span class="hlt">electronic</span> <span class="hlt">band</span> structure models.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tadjine, Athmane; Delerue, Christophe</p> <p>2018-03-28</p> <p>The synthesis of self-assembled semiconductor nanocrystal (NC) superlattices using oriented attachment recently became a flourishing research topic. This technique already produced remarkable forms of NC superlattices, such as linear chains, mono and multilayer square lattices, and silicene-like honeycomb lattices. In the case of lead chalcogenide semiconductors where NCs are in the form of truncated nanocubes, the attachment mostly occurs via (100) facets. In this work, we show that all these structures can be seen as sub-structures of a simple cubic lattice. From this, we investigate a rich variety of one-dimensional or two-dimensional superlattices that could be built as few lines or few layers taken from the same cubic system following different crystallographic orientations. Each NC can be therefore considered as a LEGO® brick, and any superlattice can be obtained from another one by rearranging the bricks. Moreover, we show that this concept of LEGO® bricks can be extended to the calculation of the <span class="hlt">electronic</span> <span class="hlt">band</span> structure of the superlattices. This leads to a simple yet powerful way to build analytical Hamiltonians that present <span class="hlt">band</span> structures in excellent agreement with more elaborate atomistic tight-binding calculations. This LEGO® concept could guide the synthesis of superlattices and LEGO® Hamiltonians should greatly simplify further studies on the (opto-)<span class="hlt">electronic</span> properties of such structures.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_16 --> <div id="page_17" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="321"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JAP...115n3107D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JAP...115n3107D"><span>Inter-<span class="hlt">band</span> optoelectronic properties in quantum dot structure of low <span class="hlt">band</span> gap III-V semiconductors</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dey, Anup; Maiti, Biswajit; Chanda Sarkar, Debasree</p> <p>2014-04-01</p> <p>A generalized theory is developed to study inter-<span class="hlt">band</span> optical absorption coefficient (IOAC) and material gain (MG) in quantum dot structures of narrow gap III-V compound semiconductor considering the wave-vector (k→) dependence of the optical transition matrix element. The <span class="hlt">band</span> structures of these low <span class="hlt">band</span> gap semiconducting materials with sufficiently separated split-off valance <span class="hlt">band</span> are frequently described by the three <span class="hlt">energy</span> <span class="hlt">band</span> model of Kane. This has been adopted for analysis of the IOAC and MG taking InAs, InSb, Hg1-xCdxTe, and In1-xGaxAsyP1-y lattice matched to InP, as example of III-V compound semiconductors, having varied split-off <span class="hlt">energy</span> <span class="hlt">band</span> compared to their bulk <span class="hlt">band</span> gap <span class="hlt">energy</span>. It has been found that magnitude of the IOAC for quantum dots increases with increasing incident photon <span class="hlt">energy</span> and the lines of absorption are more closely spaced in the three <span class="hlt">band</span> model of Kane than those with parabolic <span class="hlt">energy</span> <span class="hlt">band</span> approximations reflecting the direct the influence of <span class="hlt">energy</span> <span class="hlt">band</span> parameters. The results show a significant deviation to the MG spectrum of narrow-gap materials having <span class="hlt">band</span> nonparabolicity compared to the parabolic <span class="hlt">band</span> model approximations. The results reflect the important role of valence <span class="hlt">band</span> split-off <span class="hlt">energies</span> in these narrow gap semiconductors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JChPh.148l4312J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JChPh.148l4312J"><span><span class="hlt">Electron</span>-impact <span class="hlt">electronic</span>-state excitation of para-benzoquinone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jones, D. B.; da Costa, R. F.; Kossoski, F.; Varella, M. T. do N.; Bettega, M. H. F.; Ferreira da Silva, F.; Limão-Vieira, P.; García, G.; Lima, M. A. P.; White, R. D.; Brunger, M. J.</p> <p>2018-03-01</p> <p>Angle resolved <span class="hlt">electron</span> <span class="hlt">energy</span> loss spectra (EELS) for para-benzoquinone (C6H4O2) have been recorded for incident <span class="hlt">electron</span> <span class="hlt">energies</span> of 20, 30, and 40 eV. Measured differential cross sections (DCSs) for <span class="hlt">electronic</span> <span class="hlt">band</span> features, composed of a combination of energetically unresolved <span class="hlt">electronic</span> states, are subsequently derived from those EELS. Where possible, the obtained DCSs are compared with those calculated using the Schwinger multichannel method with pseudopotentials. These calculations were performed using a minimum orbital basis single configuration interaction framework at the static exchange plus polarisation level. Here, quite reasonable agreement between the experimental cross sections and the theoretical cross sections for the summation of unresolved states was observed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21393805','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21393805"><span>Importance of conduction <span class="hlt">electron</span> correlation in a Kondo lattice, Ce₂CoSi₃.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Patil, Swapnil; Pandey, Sudhir K; Medicherla, V R R; Singh, R S; Bindu, R; Sampathkumaran, E V; Maiti, Kalobaran</p> <p>2010-06-30</p> <p>Kondo systems are usually described by the interaction of the correlation induced local moments with the highly itinerant conduction <span class="hlt">electrons</span>. Here, we study the role of <span class="hlt">electron</span> correlations among conduction <span class="hlt">electrons</span> in the <span class="hlt">electronic</span> structure of a Kondo lattice compound, Ce₂CoSi₃, using high resolution photoemission spectroscopy and ab initio <span class="hlt">band</span> structure calculations, where Co 3d <span class="hlt">electrons</span> contribute in the conduction <span class="hlt">band</span>. High <span class="hlt">energy</span> resolution employed in the measurements helped to reveal the signatures of Ce 4f states derived Kondo resonance features at the Fermi level and the dominance of Co 3d contributions at higher binding <span class="hlt">energies</span> in the conduction <span class="hlt">band</span>. The lineshape of the experimental Co 3d <span class="hlt">band</span> is found to be significantly different from that obtained from the <span class="hlt">band</span> structure calculations within the local density approximations, LDA. Consideration of <span class="hlt">electron-electron</span> Coulomb repulsion, U, among Co 3d <span class="hlt">electrons</span> within the LDA + U method leads to a better representation of experimental results. The signature of an <span class="hlt">electron</span> correlation induced satellite feature is also observed in the Co 2p core level spectrum. These results clearly demonstrate the importance of the <span class="hlt">electron</span> correlation among conduction <span class="hlt">electrons</span> in deriving the microscopic description of such Kondo systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2000JGR...10520857C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2000JGR...10520857C"><span>Nitric oxide excited under auroral conditions: Excited state densities and <span class="hlt">band</span> emissions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cartwright, D. C.; Brunger, M. J.; Campbell, L.; Mojarrabi, B.; Teubner, P. J. O.</p> <p>2000-09-01</p> <p><span class="hlt">Electron</span> impact excitation of vibrational levels in the ground <span class="hlt">electronic</span> state and nine excited <span class="hlt">electronic</span> states in NO has been simulated for an IBC II aurora (i.e., ˜10 kR in 3914 Å radiation) in order to predict NO excited state number densities and <span class="hlt">band</span> emission intensities. New integral <span class="hlt">electron</span> impact excitation cross sections for NO were combined with a measured IBC II auroral secondary <span class="hlt">electron</span> distribution, and the vibrational populations of 10 NO <span class="hlt">electronic</span> states were determined under conditions of statistical equilibrium. This model predicts an extended vibrational distribution in the NO ground <span class="hlt">electronic</span> state produced by radiative cascade from the seven higher-lying doublet excited <span class="hlt">electronic</span> states populated by <span class="hlt">electron</span> impact. In addition to significant <span class="hlt">energy</span> storage in vibrational excitation of the ground <span class="hlt">electronic</span> state, both the a 4Π and L2 Φ excited <span class="hlt">electronic</span> states are predicted to have relatively high number densities because they are only weakly connected to lower <span class="hlt">electronic</span> states by radiative decay. Fundamental mode radiative transitions involving the lowest nine excited vibrational levels in the ground <span class="hlt">electronic</span> state are predicted to produce infrared (IR) radiation from 5.33 to 6.05 μm with greater intensity than any single NO <span class="hlt">electronic</span> emission <span class="hlt">band</span>. Fundamental mode radiative transitions within the a 4Π <span class="hlt">electronic</span> state, in the 10.08-11.37 μm region, are predicted to have IR intensities comparable to individual <span class="hlt">electronic</span> emission <span class="hlt">bands</span> in the Heath and ɛ <span class="hlt">band</span> systems. Results from this model quantitatively predict the vibrational quantum number dependence of the NO IR measurements of Espy et al. [1988].</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvB..97l5203Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvB..97l5203Z"><span>Spin-to-charge conversion for hot photoexcited <span class="hlt">electrons</span> in germanium</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zucchetti, C.; Bottegoni, F.; Isella, G.; Finazzi, M.; Rortais, F.; Vergnaud, C.; Widiez, J.; Jamet, M.; Ciccacci, F.</p> <p>2018-03-01</p> <p>We investigate the spin-to-charge conversion in highly doped germanium as a function of the kinetic <span class="hlt">energy</span> of the carriers. Spin-polarized <span class="hlt">electrons</span> are optically generated in the Ge conduction <span class="hlt">band</span>, and their kinetic <span class="hlt">energy</span> is varied by changing the photon <span class="hlt">energy</span> in the 0.7-2.2 eV range. The spin detection scheme relies on spin-dependent scattering inside Ge, which yields an inverse spin-Hall electromotive force. The detected signal shows a sign inversion for h ν ≈1 eV which can be related to an interplay between the spin relaxation of high-<span class="hlt">energy</span> <span class="hlt">electrons</span> photoexcited from the heavy-hole and light-hole <span class="hlt">bands</span> and that of low-<span class="hlt">energy</span> <span class="hlt">electrons</span> promoted from the split-off <span class="hlt">band</span>. The inferred spin-Hall angle increases by about 3 orders of magnitude within the analyzed photon <span class="hlt">energy</span> range. Since, for increasing photon <span class="hlt">energies</span>, the phonon contribution to spin scattering exceeds that of impurities, our result indicates that the spin-to-charge conversion mediated by phonons is much more efficient than the one mediated by impurities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017CoMP..172...56D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017CoMP..172...56D"><span>Mechanisms of fine extinction <span class="hlt">band</span> development in vein quartz: new insights from correlative light and <span class="hlt">electron</span> microscopy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Derez, Tine; Van Der Donck, Tom; Plümper, Oliver; Muchez, Philippe; Pennock, Gill; Drury, Martyn R.; Sintubin, Manuel</p> <p>2017-07-01</p> <p>Fine extinction <span class="hlt">bands</span> (FEBs) (also known as deformation lamellae) visible with polarized light microscopy in quartz consist of a range of nanostructures, inferring different formation processes. Previous transmission <span class="hlt">electron</span> microscopy studies have shown that most FEB nanostructures in naturally deformed quartz are elongated subgrains formed by recovery of dislocation slip <span class="hlt">bands</span>. Here we show that three types of FEB nanostructure occur in naturally deformed vein quartz from the low-grade metamorphic High-Ardenne slate belt (Belgium). Prismatic oriented FEBs are defined by <span class="hlt">bands</span> of dislocation walls. Dauphiné twin boundaries present along the FEB boundaries probably formed after FEB formation. In an example of two sub-rhombohedral oriented FEBs, developed as two sets in one grain, the finer FEB set consists of elongated subgrains, similar to FEBs described in previous transmission <span class="hlt">electron</span> microscopy studies. The second wider FEB set consists of <span class="hlt">bands</span> with different dislocation density and fluid-inclusion content. The wider FEB set is interpreted as <span class="hlt">bands</span> with different plastic strain associated with the primary growth <span class="hlt">banding</span> of the vein quartz grain. The nanometre-scale fluid inclusions are interpreted to have formed from structurally bounded hydroxyl groups that moreover facilitated formation of the elongate subgrains. Larger fluid inclusions aligned along FEBs are explained by fluid-inclusion redistribution along dislocation cores. The prismatic FEB nanostructure and the relation between FEBs and growth <span class="hlt">bands</span> have not been recognized before, although related structures have been reported in experimentally deformed quartz.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005PhRvB..72p5406G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005PhRvB..72p5406G"><span>Ultrafast dynamics and decoherence of quasiparticles in surface <span class="hlt">bands</span>: Development of the formalism</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gumhalter, Branko</p> <p>2005-10-01</p> <p>We describe a formalism suitable for studying the ultrafast dynamics and nonadiabatic effects associated with propagation of a single <span class="hlt">electron</span> injected into an empty <span class="hlt">band</span>. Within the <span class="hlt">band</span> the <span class="hlt">electron</span> is coupled to vibrational or <span class="hlt">electronic</span> excitations that can be modeled by bosons. The formalism is based on the application of cumulant expansion to calculations of diagonal single particle propagators that are used in the interpretations of time resolved measurements of the surface <span class="hlt">electronic</span> structure. Second and fourth order cumulants which arise from linear coupling to bosonic excitations and give leading contributions to the renormalization of propagators are explicitly calculated in the real time domain and their properties analyzed. This approach enables the assessment of transient effects and <span class="hlt">energy</span> transfer associated with nonadiabatic response of the system to promotion of <span class="hlt">electrons</span> into unoccupied <span class="hlt">bands</span>, as well as of higher order corrections to the lifetimes and <span class="hlt">energy</span> shifts of the initial <span class="hlt">electronic</span> states that in the adiabatic regime are obtained from Fermi’s golden rule approach or its improvements such as the GW approximation. In the form presented the formalism is particularly suitable for studying the non-Markovian evolution and ultrafast decoherence of <span class="hlt">electronic</span> states encountered in <span class="hlt">electron</span> spectroscopies of quasi-two-dimensional <span class="hlt">bands</span> on metal surfaces whose descriptions are inaccessible to the approaches based on the adiabatic hypothesis. The fast convergence of the results obtained by this procedure is demonstrated for a simple model system relevant to surface problems. On the basis of this and some general properties of cumulants it is argued that in the majority of surface problems involving <span class="hlt">electron</span>-boson interactions the ultrafast dynamics of quasiparticles is accurately described by the second order cumulant, which can be calculated with the effort not exceeding those encountered in the standard GW approximation calculations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29370376','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29370376"><span>Development of a secondary <span class="hlt">electron</span> <span class="hlt">energy</span> analyzer for a transmission <span class="hlt">electron</span> microscope.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Magara, Hideyuki; Tomita, Takeshi; Kondo, Yukihito; Sato, Takafumi; Akase, Zentaro; Shindo, Daisuke</p> <p>2018-04-01</p> <p>A secondary <span class="hlt">electron</span> (SE) <span class="hlt">energy</span> analyzer was developed for a transmission <span class="hlt">electron</span> microscope. The analyzer comprises a microchannel plate (MCP) for detecting <span class="hlt">electrons</span>, a coil for collecting SEs emitted from the specimen, a tube for reducing the number of backscattered <span class="hlt">electrons</span> incident on the MCP, and a retarding mesh for selecting the <span class="hlt">energy</span> of SEs incident on the MCP. The detection of the SEs associated with charging phenomena around a charged specimen was attempted by performing <span class="hlt">electron</span> holography and SE spectroscopy using the <span class="hlt">energy</span> analyzer. The results suggest that it is possible to obtain the <span class="hlt">energy</span> spectra of SEs using the analyzer and the charging states of a specimen by <span class="hlt">electron</span> holography simultaneously.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AIPC.1299..451F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AIPC.1299..451F"><span>Ultra-High Gradient S-<span class="hlt">band</span> Linac for Laboratory and Industrial Applications</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Faillace, L.; Agustsson, R.; Dolgashev, V.; Frigola, P.; Murokh, A.; Rosenzweig, J.; Yakimenko, V.</p> <p>2010-11-01</p> <p>A strong demand for high gradient structures arises from the limited real estate available for linear accelerators. RadiaBeam Technologies is developing a Doubled <span class="hlt">Energy</span> Compact Accelerator (DECA) structure: an S-<span class="hlt">band</span> standing wave <span class="hlt">electron</span> linac designed to operate at accelerating gradients of up to 50 MV/m. In this paper, we present the radio-frequency design of the DECA S-<span class="hlt">band</span> accelerating structure, operating at 2.856 GHz in the π-mode. The structure design is heavily influenced by NLC collaboration experience with ultra high gradient X-<span class="hlt">band</span> structures; S-<span class="hlt">band</span>, however, is chosen to take advantage of commonly available high power S-<span class="hlt">band</span> klystrons.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28805062','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28805062"><span>Ultrafast <span class="hlt">Electron</span> Dynamics in Solar <span class="hlt">Energy</span> Conversion.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ponseca, Carlito S; Chábera, Pavel; Uhlig, Jens; Persson, Petter; Sundström, Villy</p> <p>2017-08-23</p> <p><span class="hlt">Electrons</span> are the workhorses of solar <span class="hlt">energy</span> conversion. Conversion of the <span class="hlt">energy</span> of light to electricity in photovoltaics, or to <span class="hlt">energy</span>-rich molecules (solar fuel) through photocatalytic processes, invariably starts with photoinduced generation of <span class="hlt">energy</span>-rich <span class="hlt">electrons</span>. The harvesting of these <span class="hlt">electrons</span> in practical devices rests on a series of <span class="hlt">electron</span> transfer processes whose dynamics and efficiencies determine the function of materials and devices. To capture the <span class="hlt">energy</span> of a photogenerated <span class="hlt">electron</span>-hole pair in a solar cell material, charges of opposite sign have to be separated against electrostatic attractions, prevented from recombining and being transported through the active material to electrodes where they can be extracted. In photocatalytic solar fuel production, these <span class="hlt">electron</span> processes are coupled to chemical reactions leading to storage of the <span class="hlt">energy</span> of light in chemical bonds. With the focus on the ultrafast time scale, we here discuss the light-induced <span class="hlt">electron</span> processes underlying the function of several molecular and hybrid materials currently under development for solar <span class="hlt">energy</span> applications in dye or quantum dot-sensitized solar cells, polymer-fullerene polymer solar cells, organometal halide perovskite solar cells, and finally some photocatalytic systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AIPA....8e5123X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AIPA....8e5123X"><span>Temperature-induced <span class="hlt">band</span> shift in bulk γ-InSe by angle-resolved photoemission spectroscopy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xu, Huanfeng; Wang, Wei; Zhao, Yafei; Zhang, Xiaoqian; Feng, Yue; Tu, Jian; Gu, Chenyi; Sun, Yizhe; Liu, Chang; Nie, Yuefeng; Edmond Turcu, Ion C.; Xu, Yongbing; He, Liang</p> <p>2018-05-01</p> <p>Indium selenide (InSe) has recently become popular research topics because of its unique layered crystal structure, direct <span class="hlt">band</span> gap and high <span class="hlt">electron</span> mobilities. In this work, we have acquired the <span class="hlt">electronic</span> structure of bulk γ-InSe at various temperatures using angle-resolved photoemission spectroscopy (ARPES). We have also found that as the temperature decreases, the valence <span class="hlt">bands</span> of γ-InSe exhibit a monotonic shift to lower binding <span class="hlt">energies</span>. This <span class="hlt">band</span> shift is attributed to the change of lattice parameters and has been validated by variable temperature X-ray diffraction measurements and theoretical calculations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1436077-demonstration-transmission-high-energy-electron-microscopy','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1436077-demonstration-transmission-high-energy-electron-microscopy"><span>Demonstration of transmission high <span class="hlt">energy</span> <span class="hlt">electron</span> microscopy</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Merrill, F. E.; Goett, J.; Gibbs, J. W.; ...</p> <p>2018-04-06</p> <p>High <span class="hlt">energy</span> <span class="hlt">electrons</span> have been used to investigate an extension of transmission <span class="hlt">electron</span> microscopy. This technique, transmission high <span class="hlt">energy</span> <span class="hlt">electron</span> microscopy (THEEM), provides two additional capabilities to <span class="hlt">electron</span> microscopy. First, high <span class="hlt">energy</span> <span class="hlt">electrons</span> are more penetrating than low <span class="hlt">energy</span> <span class="hlt">electrons</span>, and thus, they are able to image through thicker samples. Second, the accelerating mode of a radio-frequency linear accelerator provides fast exposures, down to 1 ps, which are ideal for flash radiography, making THEEM well suited to study the evolution of fast material processes under dynamic conditions. Lastly, initial investigations with static objects and during material processing have been performedmore » to investigate the capabilities of this technique.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27350094','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27350094"><span>Importance of doping, dopant distribution, and defects on <span class="hlt">electronic</span> <span class="hlt">band</span> structure alteration of metal oxide nanoparticles: Implications for reactive oxygen species.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Saleh, Navid B; Milliron, Delia J; Aich, Nirupam; Katz, Lynn E; Liljestrand, Howard M; Kirisits, Mary Jo</p> <p>2016-10-15</p> <p>Metal oxide nanoparticles (MONPs) are considered to have the potency to generate reactive oxygen species (ROS), one of the key mechanisms underlying nanotoxicity. However, the nanotoxicology literature demonstrates a lack of consensus on the dominant toxicity mechanism(s) for a particular MONP. Moreover, recent literature has studied the correlation between <span class="hlt">band</span> structure of pristine MONPs to their ability to introduce ROS and thus has downplayed the ROS-mediated toxicological relevance of a number of such materials. On the other hand, material science can control the <span class="hlt">band</span> structure of these materials to engineer their <span class="hlt">electronic</span> and optical properties and thereby is constantly modulating the pristine <span class="hlt">electronic</span> structure. Since <span class="hlt">band</span> structure is the fundamental material property that controls ROS-producing ability, <span class="hlt">band</span> tuning via introduction of dopants and defects needs careful consideration in toxicity assessments. This commentary critically evaluates the existing material science and nanotoxicity literature and identifies the gap in our understanding of the role of important crystal structure features (i.e., dopants and defects) on MONPs' <span class="hlt">electronic</span> structure alteration as well as their ROS-generation capability. Furthermore, this commentary provides suggestions on characterization techniques to evaluate dopants and defects on the crystal structure and identifies research needs for advanced theoretical predictions of their <span class="hlt">electronic</span> <span class="hlt">band</span> structures and ROS-generation abilities. Correlation of <span class="hlt">electronic</span> <span class="hlt">band</span> structure and ROS will not only aid in better mechanistic assessment of nanotoxicity but will be impactful in designing and developing ROS-based applications ranging from water disinfection to next-generation antibiotics and even cancer therapeutics. Copyright © 2016 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007JAP...101i3106F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007JAP...101i3106F"><span>Effect of elastic strain redistribution on <span class="hlt">electronic</span> <span class="hlt">band</span> structures of compressively strained GaInAsP/InP membrane quantum wires</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ferdous, F.; Haque, A.</p> <p>2007-05-01</p> <p>The effect of redistribution of elastic strain relaxation on the <span class="hlt">energy</span> <span class="hlt">band</span> structures of GaInAsP/InP compressively strained membrane quantum wires fabricated by <span class="hlt">electron</span>-beam lithography, reactive-ion etching and two-step epitaxial growth is theoretically studied using an 8-<span class="hlt">band</span> k ṡp method. Anisotropic strain analysis by the finite element method shows that due to etching away the top and the bottom InP clad layers in membrane structures, redistribution of strain occurs. It is found that strain redistribution increases the effective bandgap of membrane quantum wire structures causing a blueshift of the emission frequency. Comparison with effective bandgap calculations neglecting confinement and <span class="hlt">band</span> mixing demonstrates that neglect of these effects leads to an overestimation of the change in the bandgap. We have also investigated the effect of variation of wire width, barrier strain compensation, number of stacked quantum wire layers, and thickness of the top and the bottom residual InP layers in membrane structures on the change in the effective bandgap of membrane structures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1992PhRvB..46.4899A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1992PhRvB..46.4899A"><span>Diffraction of <span class="hlt">electrons</span> at intermediate <span class="hlt">energies</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ascolani, H.; Barrachina, R. O.; Guraya, M. M.; Zampieri, G.</p> <p>1992-08-01</p> <p>We present a theory of the elastic scattering of <span class="hlt">electrons</span> from crystalline surfaces that contains both low-<span class="hlt">energy-electron</span>-diffraction (LEED) effects at low <span class="hlt">energies</span> and x-ray-photoelectron- and Auger-<span class="hlt">electron</span>-diffraction (XPD/AED) effects at intermediate <span class="hlt">energies</span>. The theory is based on a cluster-type approach to the scattering problem and includes temperature effects. The transition from one regime to the other may be explained as follows: At low <span class="hlt">energies</span> all the scattered waves add coherently, and the intensity is dominated by LEED effects. At intermediate <span class="hlt">energies</span> the thermal vibration of the atoms destroys the long-range coherency responsible for the LEED peaks, but affects little the interference of those waves that share parts of their paths inside the solid. Thus, the interference of these waves comes to dominate the intensity, giving rise to structures similar to those observed in XPD/AED experiments. We perform a calculation of the elastic reflection of <span class="hlt">electrons</span> from Cu(001) that is in good agreement with the experiment in the range 200-1500 eV. At low <span class="hlt">energies</span> the intensity is dominated by LEED peaks; at 400 eV LEED peaks and XPD/AED structures coexist; and above this <span class="hlt">energy</span> the intensity is dominated by the latter. We analyze the contributions to the intensity at intermediate <span class="hlt">energies</span> of the interferences in the incoming and outgoing parts of the <span class="hlt">electron</span> path.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/873026','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/873026"><span>Thermophotovoltaic conversion using selective infrared line emitters and large <span class="hlt">band</span> gap photovoltaic devices</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Brandhorst, Jr., Henry W.; Chen, Zheng</p> <p>2000-01-01</p> <p>Efficient thermophotovoltaic conversion can be performed using photovoltaic devices with a <span class="hlt">band</span> gap in the 0.75-1.4 <span class="hlt">electron</span> volt range, and selective infrared emitters chosen from among the rare earth oxides which are thermally stimulated to emit infrared radiation whose <span class="hlt">energy</span> very largely corresponds to the aforementioned <span class="hlt">band</span> gap. It is possible to use thermovoltaic devices operating at relatively high temperatures, up to about 300.degree. C., without seriously impairing the efficiency of <span class="hlt">energy</span> conversion.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27420635','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27420635"><span>Direct characterization of the <span class="hlt">energy</span> level alignments and molecular components in an organic hetero-junction by integrated photoemission spectroscopy and reflection <span class="hlt">electron</span> <span class="hlt">energy</span> loss spectroscopy analysis.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yun, Dong-Jin; Shin, Weon-Ho; Bulliard, Xavier; Park, Jong Hwan; Kim, Seyun; Chung, Jae Gwan; Kim, Yongsu; Heo, Sung; Kim, Seong Heon</p> <p>2016-08-26</p> <p>A novel, direct method for the characterization of the <span class="hlt">energy</span> level alignments at bulk-heterojunction (BHJ)/electrode interfaces on the basis of <span class="hlt">electronic</span> spectroscopy measurements is proposed. The home-made in situ photoemission system is used to perform x-ray/ultraviolet photoemission spectroscopy (XPS/UPS), reflection <span class="hlt">electron</span> <span class="hlt">energy</span> loss spectroscopy (REELS) and inverse photoemission spectroscopy of organic-semiconductors (OSCs) deposited onto a Au substrate. Through this analysis system, we are able to obtain the <span class="hlt">electronic</span> structures of a boron subphthalocyanine chloride:fullerene (SubPC:C60) BHJ and those of the separate OSC/electrode structures (SubPC/Au and C60/Au). Morphology and chemical composition analyses confirm that the original SubPC and C60 <span class="hlt">electronic</span> structures remain unchanged in the electrodes prepared. Using this technique, we ascertain that the position and area of the nearest peak to the Fermi <span class="hlt">energy</span> (EF = 0 eV) in the UPS (REELS) spectra of SubPC:C60 BHJ provide information on the highest occupied molecular orbital level (optical <span class="hlt">band</span> gap) and combination ratio of the materials, respectively. Thus, extracting the adjusted spectrum from the corresponding SubPC:C60 BHJ UPS (REELS) spectrum reveals its <span class="hlt">electronic</span> structure, equivalent to that of the C60 materials. This novel analytical approach allows complete <span class="hlt">energy</span>-level determination for each combination ratio by separating its <span class="hlt">electronic</span> structure information from the BHJ spectrum.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JPhD...49V5103B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JPhD...49V5103B"><span>Influence of non-collisional laser heating on the <span class="hlt">electron</span> dynamics in dielectric materials</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barilleau, L.; Duchateau, G.; Chimier, B.; Geoffroy, G.; Tikhonchuk, V.</p> <p>2016-12-01</p> <p>The <span class="hlt">electron</span> dynamics in dielectric materials induced by intense femtosecond laser pulses is theoretically addressed. The laser driven temporal evolution of the <span class="hlt">energy</span> distribution of <span class="hlt">electrons</span> in the conduction <span class="hlt">band</span> is described by a kinetic Boltzmann equation. In addition to the collisional processes for <span class="hlt">energy</span> transfer such as <span class="hlt">electron</span>-phonon-photon and <span class="hlt">electron-electron</span> interactions, a non-collisional process for photon absorption in the conduction <span class="hlt">band</span> is included. It relies on direct transitions between sub-<span class="hlt">bands</span> of the conduction <span class="hlt">band</span> through multiphoton absorption. This mechanism is shown to significantly contribute to the laser heating of conduction <span class="hlt">electrons</span> for large enough laser intensities. It also increases the time required for the <span class="hlt">electron</span> distribution to reach the equilibrium state as described by the Fermi-Dirac statistics. Quantitative results are provided for quartz irradiated by a femtosecond laser pulse with a wavelength of 800 nm and for intensities in the range of tens of TW cm-2, lower than the ablation threshold. The change in the <span class="hlt">energy</span> deposition induced by this non-collisional heating process is expected to have a significant influence on the laser processing of dielectric materials.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008PhLA..372.5999C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008PhLA..372.5999C"><span>Magneto-<span class="hlt">electronic</span> properties of graphene nanoribbons in the spatially modulated electric field</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, S. C.; Wang, T. S.; Lee, C. H.; Lin, M. F.</p> <p>2008-09-01</p> <p>The Peierls tight-binding model with the nearest-neighbor interactions is used to calculate the magneto-<span class="hlt">electronic</span> structure of graphene nanoribbons under a spatially modulated electric field along the y-axis. A uniform perpendicular magnetic field could make <span class="hlt">energy</span> dispersions change into the quasi-Landau levels. Such levels are composed of the dispersionless and parabolic <span class="hlt">energy</span> <span class="hlt">bands</span>. A spatially modulated electric field would further induce a lot of oscillating parabolic <span class="hlt">bands</span> with several <span class="hlt">band</span>-edge states. It drastically modifies <span class="hlt">energy</span> dispersions, alters subband spacings, destroys symmetry of <span class="hlt">energy</span> spectrum about k=0, and changes features of <span class="hlt">band</span>-edge states (number and <span class="hlt">energy</span>). The above-mentioned magneto-<span class="hlt">electronic</span> structures are directly reflected in density of states (DOS). The modulation effect changes shape, number, positions, and intensities of peaks in DOS. The predicted result could be tested by the optical measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011JETP..113..156K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011JETP..113..156K"><span>Anomalous resistivity and the origin of heavy mass in the two-<span class="hlt">band</span> Hubbard model with one narrow <span class="hlt">band</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kagan, M. Yu.; Val'kov, V. V.</p> <p>2011-07-01</p> <p>We search for marginal Fermi-liquid behavior [1] in the two-<span class="hlt">band</span> Hubbard model with one narrow <span class="hlt">band</span>. We consider the limit of low <span class="hlt">electron</span> densities in the <span class="hlt">bands</span> and strong intraband and interband Hubbard interactions. We analyze the influence of <span class="hlt">electron</span> polaron effect [2] and other mechanisms of mass enhancement (related to momentum dependence of the self-<span class="hlt">energies</span>) on the effective mass and scattering times of light and heavy components in the clean case (<span class="hlt">electron-electron</span> scattering and no impurities). We find the tendency towards phase separation (towards negative partial compressibility of heavy particles) in the 3D case for a large mismatch between the densities of heavy and light <span class="hlt">bands</span> in the strong-coupling limit. We also observe that for low temperatures and equal densities, the homogeneous state resistivity R( T) ˜ T 2 behaves in a Fermi-liquid fashion in both 3D and 2D cases. For temperatures higher than the effective bandwidth for heavy <span class="hlt">electrons</span> T > W {*/ h }, the coherent behavior of the heavy component is totally destroyed. The heavy particles move diffusively in the surrounding of light particles. At the same time, the light particles scatter on the heavy ones as if on immobile (static) impurities. In this regime, the heavy component is marginal, while the light one is not. The resistivity saturates for T > W {*/ h } in the 3D case. In 2D, the resistivity has a maximum and a localization tail due to weak-localization corrections of the Altshuler-Aronov type [3]. Such behavior of resistivity could be relevant for some uranium-based heavy-fermion compounds like UNi2Al3 in 3D and for some other mixed-valence compounds possibly including layered manganites in 2D. We also briefly consider the superconductive (SC) instability in the model. The leading instability is towards the p-wave pairing and is governed by the enhanced Kohn-Luttinger [4] mechanism of SC at low <span class="hlt">electron</span> density. The critical temperature corresponds to the pairing of heavy <span class="hlt">electrons</span></p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_17 --> <div id="page_18" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="341"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhyE...85..253D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhyE...85..253D"><span>Sizable <span class="hlt">band</span> gap in organometallic topological insulator</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Derakhshan, V.; Ketabi, S. A.</p> <p>2017-01-01</p> <p>Based on first principle calculation when Ceperley-Alder and Perdew-Burke-Ernzerh type exchange-correlation <span class="hlt">energy</span> functional were adopted to LSDA and GGA calculation, <span class="hlt">electronic</span> properties of organometallic honeycomb lattice as a two-dimensional topological insulator was calculated. In the presence of spin-orbit interaction bulk <span class="hlt">band</span> gap of organometallic lattice with heavy metals such as Au, Hg, Pt and Tl atoms were investigated. Our results show that the organometallic topological insulator which is made of Mercury atom shows the wide bulk <span class="hlt">band</span> gap of about ∼120 meV. Moreover, by fitting the conduction and valence <span class="hlt">bands</span> to the <span class="hlt">band</span>-structure which are produced by Density Functional Theory, spin-orbit interaction parameters were extracted. Based on calculated parameters, gapless edge states within bulk insulating gap are indeed found for finite width strip of two-dimensional organometallic topological insulators.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/20787016-transmission-effects-unfolding-electronic-vibrational-electron-molecule-energy-loss-spectra','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/20787016-transmission-effects-unfolding-electronic-vibrational-electron-molecule-energy-loss-spectra"><span>Transmission effects in unfolding <span class="hlt">electronic</span>-vibrational <span class="hlt">electron</span>-molecule <span class="hlt">energy</span>-loss spectra</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Wang Shiyang; Khakoo, Murtadha A.; Johnson, Paul V.</p> <p>2006-03-15</p> <p>The results of an investigation concerning the sensitivity of conventional unfolding methods applied to <span class="hlt">electronic</span>-vibrational <span class="hlt">electron-energy</span>-loss spectra to the transmission efficiency of <span class="hlt">electron</span> spectrometers are presented. This investigation was made in an effort to understand differences in the differential cross sections for excitation of low-lying <span class="hlt">electronic</span> states determined experimentally by various groups using <span class="hlt">electronic</span>-vibrational <span class="hlt">energy</span>-loss spectra of N{sub 2}. In these experiments, very similar spectral unfolding methods were used, which relied on similar Franck-Condon factors. However, the overall analyses of the <span class="hlt">electron</span> scattering spectra (by the individual groups) resulted in large differences among the differential cross sections determined from thesemore » <span class="hlt">energy</span>-loss spectra. The transmission response of the experimental apparatus to different-<span class="hlt">energy</span> scattered <span class="hlt">electrons</span> has often been discussed as a key factor that caused these disagreements. The present investigation shows in contrast that the effect of transmission is smaller than that required to independently explain such differences, implying that other systematic effects are responsible for the existing differences between measurements.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JQSRT.210..127P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JQSRT.210..127P"><span>Potential <span class="hlt">energy</span> surface, dipole moment surface and the intensity calculations for the 10 μm, 5 μm and 3 μm <span class="hlt">bands</span> of ozone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Polyansky, Oleg L.; Zobov, Nikolai F.; Mizus, Irina I.; Kyuberis, Aleksandra A.; Lodi, Lorenzo; Tennyson, Jonathan</p> <p>2018-05-01</p> <p>Monitoring ozone concentrations in the Earth's atmosphere using spectroscopic methods is a major activity which undertaken both from the ground and from space. However there are long-running issues of consistency between measurements made at infrared (IR) and ultraviolet (UV) wavelengths. In addition, key O3 IR <span class="hlt">bands</span> at 10 μm, 5 μm and 3 μm also yield results which differ by a few percent when used for retrievals. These problems stem from the underlying laboratory measurements of the line intensities. Here we use quantum chemical techniques, first principles <span class="hlt">electronic</span> structure and variational nuclear-motion calculations, to address this problem. A new high-accuracy ab initio dipole moment surface (DMS) is computed. Several spectroscopically-determined potential <span class="hlt">energy</span> surfaces (PESs) are constructed by fitting to empirical <span class="hlt">energy</span> levels in the region below 7000 cm-1 starting from an ab initio PES. Nuclear motion calculations using these new surfaces allow the unambiguous determination of the intensities of 10 μm <span class="hlt">band</span> transitions, and the computation of the intensities of 10 μm and 5 μm <span class="hlt">bands</span> within their experimental error. A decrease in intensities within the 3 μm is predicted which appears consistent with atmospheric retrievals. The PES and DMS form a suitable starting point both for the computation of comprehensive ozone line lists and for future calculations of <span class="hlt">electronic</span> transition intensities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AIPC.1728b0141R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AIPC.1728b0141R"><span><span class="hlt">Electronic</span> properties of <span class="hlt">electron</span> and hole in type-II semiconductor nano-heterostructures</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rahul, K. Suseel; Souparnika, C.; Salini, K.; Mathew, Vincent</p> <p>2016-05-01</p> <p>In this project, we record the orbitals of <span class="hlt">electron</span> and hole in type-II (CdTe/CdSe/CdTe/CdSe) semiconductor nanocrystal using effective mass approximation. In type-II the <span class="hlt">band</span> edges of both valance and conduction <span class="hlt">band</span> are higher than that of shell. So the <span class="hlt">electron</span> and hole get confined in different layers of the hetero-structure. The <span class="hlt">energy</span> eigen values and eigen functions are calculated by solving Schrodinger equation using finite difference matrix method. Based on this we investigate the effect of shell thickness and well width on <span class="hlt">energy</span> and probability distribution of ground state (1s) and few excited states (1p,1d,etc). Our results predict that, type-II quantum dots have significant importance in photovoltaic applications.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29082994','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29082994"><span>Investigation of <span class="hlt">energy</span> <span class="hlt">band</span> alignments and interfacial properties of rutile NMO2/TiO2 (NM = Ru, Rh, Os, and Ir) by first-principles calculations.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yang, Chen; Zhao, Zong-Yan</p> <p>2017-11-08</p> <p>In the field of photocatalysis, constructing hetero-structures is an efficient strategy to improve quantum efficiency. However, a lattice mismatch often induces unfavorable interfacial states that can act as recombination centers for photo-generated <span class="hlt">electron</span>-hole pairs. If the hetero-structure's components have the same crystal structure, this disadvantage can be easily avoided. Conversely, in the process of loading a noble metal co-catalyst onto the TiO 2 surface, a transition layer of noble metal oxides is often formed between the TiO 2 layer and the noble metal layer. In this article, interfacial properties of hetero-structures composed of a noble metal dioxide and TiO 2 with a rutile crystal structure have been systematically investigated using first-principles calculations. In particular, the Schottky barrier height, <span class="hlt">band</span> bending, and <span class="hlt">energy</span> <span class="hlt">band</span> alignments are studied to provide evidence for practical applications. In all cases, no interfacial states exist in the forbidden <span class="hlt">band</span> of TiO 2 , and the interfacial formation <span class="hlt">energy</span> is very small. A strong internal electric field generated by interfacial <span class="hlt">electron</span> transfer leads to an efficient separation of photo-generated carriers and <span class="hlt">band</span> bending. Because of the differences in the atomic properties of the components, RuO 2 /TiO 2 and OsO 2 /TiO 2 hetero-structures demonstrate <span class="hlt">band</span> dividing, while RhO 2 /TiO 2 and IrO 2 /TiO 2 hetero-structures have a pseudo-gap near the Fermi <span class="hlt">energy</span> level. Furthermore, NMO 2 /TiO 2 hetero-structures show upward <span class="hlt">band</span> bending. Conversely, RuO 2 /TiO 2 and OsO 2 /TiO 2 hetero-structures present a relatively strong infrared light absorption, while RhO 2 /TiO 2 and IrO 2 /TiO 2 hetero-structures show an obvious absorption edge in the visible light region. Overall, considering all aspects of their properties, RuO 2 /TiO 2 and OsO 2 /TiO 2 hetero-structures are more suitable than others for improving the photocatalytic performance of TiO 2 . These findings will provide useful information</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16413678','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16413678"><span>Image acquisition with immersion objective lenses using <span class="hlt">electrons</span> emitted with several tenths of an <span class="hlt">electron</span> volt <span class="hlt">energies</span>: towards high spatial resolution ESCA analysis.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bernheim, M</p> <p>2006-03-01</p> <p>This study aims to evaluate the spatial resolution achievable with photoelectrons in order to perform localised UPS or XPS analyses on various heterogeneous samples. This investigation is intentionally restricted to direct image acquisition by immersion objective lenses, involving <span class="hlt">electrons</span> ejected with initial <span class="hlt">energies</span> of several tenths of an <span class="hlt">electron</span>-volt. In order to characterise the contribution of all optical elements, analytical investigations were associated to numerical simulations based on SIMION 7 software. The acquisition of high-quality images implies a simultaneous reduction in spherical and chromatic aberrations by a narrow aperture stop placed at the output pupil of the objective. With such limitations in useful emission angles, it is shown that monochromatic <span class="hlt">electron</span> beams build images with a resolution of about 1 nm, especially for the acceleration bias mode where the focussing electrode is biased at a positive high voltage. Even <span class="hlt">energy</span> dispersed <span class="hlt">electron</span> beams, limited by a 4 eV <span class="hlt">band</span> pass spectrometer, can produce images convenient for highly localised ESCA analyses (resolution 3 nm), where the objective lens is associated with an aperture stop of 30 microm in diameter without using acceleration voltages above 5000 V.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JPhCS.901a2171P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JPhCS.901a2171P"><span>First Principles Study of <span class="hlt">Electronic</span> <span class="hlt">Band</span> Structure and Structural Stability of Al2C Monolayer and Nanotubes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pramchu, S.; Jaroenjittichai, A. P.; Laosiritaworn, Y.</p> <p>2017-09-01</p> <p>We used density functional theory (DFT) based on generalized gradient approximation (GGA) and hybrid functional (HSE06) to investigate <span class="hlt">band</span> gap and structural stability of Al2C monolayer and nanotubes. From the results, both GGA and HSE06 <span class="hlt">band</span> gaps of Al2C monolayer agree well with previously reported data. For the Al2C nanotubes, we found that their <span class="hlt">band</span> gaps are more sensitive to the size and the chirality than that of the widely studied SiC2 nanotubes, indicating the Al2C nanotubes may have higher <span class="hlt">band</span> gap tuning capabilities (with varying diameter size and chirality) compared with those of SiC2 nanotubes. We have also discovered a desirable direct <span class="hlt">band</span> gap in the case of (n,0) nanotubes, although Al2C monolayer <span class="hlt">band</span> gap is indirect. The calculated strain <span class="hlt">energy</span> reveals that (n,0) nanotubes constructed by wrapping up Al2C monolayer consume less <span class="hlt">energy</span> than (0,n) nanotubes. Thus, (n,0) nanotubes is easier to synthesize than (0,n) nanotubes. This discovery of direct <span class="hlt">band</span> gap in (n,0) Al2C nanotubes and their adjustable <span class="hlt">band</span> gap suggests them as promising sensitizer for enhancing power conversion efficiency of excitonic solar cells.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5307316','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5307316"><span>Strain Dependent <span class="hlt">Electronic</span> Structure and <span class="hlt">Band</span> Offset Tuning at Heterointerfaces of ASnO3 (A=Ca, Sr, and Ba) and SrTiO3</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Baniecki, John D.; Yamazaki, Takashi; Ricinschi, Dan; Van Overmeere, Quentin; Aso, Hiroyuki; Miyata, Yusuke; Yamada, Hiroaki; Fujimura, Norifumi; Maran, Ronald; Anazawa, Toshihisa; Valanoor, Nagarajan; Imanaka, Yoshihiko</p> <p>2017-01-01</p> <p>The valence <span class="hlt">band</span> (VB) <span class="hlt">electronic</span> structure and VB alignments at heterointerfaces of strained epitaxial stannate ASnO3 (A=Ca, Sr, and Ba) thin films are characterized using in situ X-ray and ultraviolet photoelectron spectroscopies, with <span class="hlt">band</span> gaps evaluated using spectroscopic ellipsometry. Scanning transmission <span class="hlt">electron</span> microscopy with geometric phase analysis is used to resolve strain at atomic resolution. The VB <span class="hlt">electronic</span> structure is strain state dependent in a manner that correlated with a directional change in Sn-O bond lengths with strain. However, VB offsets are found not to vary significantly with strain, which resulted in ascribing most of the difference in <span class="hlt">band</span> alignment, due to a change in the <span class="hlt">band</span> gaps with strain, to the conduction <span class="hlt">band</span> edge. Our results reveal significant strain tuning of conduction <span class="hlt">band</span> offsets using epitaxial buffer layers, with strain-induced offset differences as large as 0.6 eV possible for SrSnO3. Such large conduction <span class="hlt">band</span> offset tunability through elastic strain control may provide a pathway to minimize the loss of charge confinement in 2-dimensional <span class="hlt">electron</span> gases and enhance the performance of photoelectrochemical stannate-based devices. PMID:28195149</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMED41A0490H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMED41A0490H"><span>Examining the Displacement of <span class="hlt">Energy</span> during Formation of Shear <span class="hlt">Bands</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hernandez, M.; Hilley, G. E.</p> <p>2011-12-01</p> <p>M.X. Hernandez, G. Hilley Department of Geological and Environmental Sciences, Stanford University, Stanford, CA This study has originated from an experimental (sandbox) setting that we have previously used to document the link between the kinematics and dynamics of deforming sand in the verge of frictional failure. Our initial experimental setting included a load control system that allowed us to track the changes in load, that when applied to the sand, deform and generate individual shear <span class="hlt">bands</span> or localized faults. Over the course of earlier experiments, three cameras located at different positions outside the sandbox monitored the movement throughout the run. This current stage of analysis includes using computer programs such as QuickTime to create image sequences of the shear <span class="hlt">band</span> formation, and Microsoft Excel to visually graph and plot each data sequence. This allows us to investigate the correlation between changes in work measured within our experiments, the construction of topography, slip along shear <span class="hlt">bands</span>, and the creation of new shear <span class="hlt">bands</span>. We observed that the measured load generally increased during the experiment to maintain a constant displacement rate as the sand wedge thickened and modeled topography increased. Superposed on this trend were periodic drops in load that appeared temporally coincident with the formation of shear <span class="hlt">bands</span> in the sand. Using the time series of the loads applied during the experiment, changes in the position of the backstop over time, and the loads measured before, during, and after the time of each shear <span class="hlt">band</span> formation, we are examining the fraction of the apples work that is absorbed by friction and shear <span class="hlt">band</span> formation, and what fraction of the apples work is expended in increasing the potential <span class="hlt">energy</span> of the thickening sand wedge. Our results indicate that before the formation of a continuous shear <span class="hlt">band</span>, the rate of work done on the sand by the experimental apparatus decreases. This may suggest that once formed, work</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JaJAP..57dFP09K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JaJAP..57dFP09K"><span>Origin of <span class="hlt">band</span> bending at domain boundaries of MoS2: First-principles study</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kaneko, Tomoaki; Saito, Riichiro</p> <p>2018-04-01</p> <p>Using first-principles calculations based on density functional theory, the energetics and <span class="hlt">electronic</span> structure of domain boundaries of MoS2, in which the same polar edges face each other, are investigated. We find that the interface model with homoelemental bonds is not energetically preferred in this system. The domain boundaries have defect levels that have wide distributions inside the <span class="hlt">band</span> gap of MoS2. The upshift (or downshift) of the MoS2 <span class="hlt">energy</span> <span class="hlt">band</span> occurs around the domain boundaries when the occupation number of <span class="hlt">electrons</span> in the defect levels increases (or decreases). The charge transfer of <span class="hlt">electrons</span> from the graphite substrate plays an important role in <span class="hlt">band</span> bending, which is observed in the recent experiments by scanning tunneling microscopy/spectroscopy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27998144','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27998144"><span><span class="hlt">Electronic</span> Structure and <span class="hlt">Band</span> Gap of Fullerenes on Tungsten Surfaces: Transition from a Semiconductor to a Metal Triggered by Annealing.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Monazami, Ehsan; McClimon, John B; Rondinelli, James; Reinke, Petra</p> <p>2016-12-21</p> <p>The understanding and control of molecule-metal interfaces is critical to the performance of molecular <span class="hlt">electronics</span> and photovoltaics devices. We present a study of the interface between C 60 and W, which is a carbide-forming transition metal. The complex solid-state reaction at the interface can be exploited to adjust the <span class="hlt">electronic</span> properties of the molecule layer. Scanning tunneling microscopy/spectroscopy measurements demonstrate the progression of this reaction from wide <span class="hlt">band</span> gap (>2.5 eV) to metallic molecular surface during annealing from 300 to 800 K. Differential conduction maps with 10 4 scanning tunneling spectra are used to quantify the transition in the density of states and the reduction of the <span class="hlt">band</span> gap during annealing with nanometer spatial resolution. The <span class="hlt">electronic</span> transition is spatially homogeneous, and the surface <span class="hlt">band</span> gap can therefore be adjusted by a targeted annealing step. The modified molecules, which we call nanospheres, are quite resistant to ripening and coalescence, unlike any other metallic nanoparticle of the same size. Densely packed C 60 and isolated C 60 molecules show the same transition in <span class="hlt">electronic</span> structure, which confirms that the transformation is controlled by the reaction at the C 60 -W interface. Density functional theory calculations are used to develop possible reaction pathways in agreement with experimentally observed <span class="hlt">electronic</span> structure modulation. Control of the <span class="hlt">band</span> gap by the choice of annealing temperature is a unique route to tailoring molecular-layer <span class="hlt">electronic</span> properties.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22491746','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22491746"><span>Controlled growth of ZnO/Zn₁-xPbxSe core-shell nanowires and their interfacial <span class="hlt">electronic</span> <span class="hlt">energy</span> alignment.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chen, Z H; Yeung, S Y; Li, H; Qian, J C; Zhang, W J; Li, Y Y; Bello, I</p> <p>2012-05-21</p> <p>ZnO/Zn(1-x)Pb(x)Se core-shell nanowires (NWs) have been synthesized by a solution based surface ion transfer method at various temperatures. The <span class="hlt">energy</span> dispersive spectroscopic (EDS) mapping of single NWs suggests that the Zn, Pb and Se atoms are uniformly distributed in their shell layers. The ternary Zn(1-x)Pb(x)Se layers with tunable bandgaps extend the <span class="hlt">band</span>-edge of optical absorption from 450 nm to 700 nm contrasting with the binary ZnSe layers. The ultraviolet photoelectron spectroscopic (UPS) analysis reveals a transition from the type I to type II <span class="hlt">band</span> alignment when the x fraction decreases from 0.66 to the value of 0.36 in the nanoshell layers. This quantitative investigation of <span class="hlt">electronic</span> <span class="hlt">energy</span> levels at ZnO and Zn(1-x)Pb(x)Se interfaces indicates that the proper type II <span class="hlt">band</span> alignment is well suited for photovoltaic <span class="hlt">energy</span> conversion. The photovoltaic cells comprising a ZnO/Zn(1-x)Pb(x)Se nano-heterojunction with the optimized Pb content are expected to be more efficient than the devices sensitized by binary ZnSe or PbSe.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22310945-role-suprathermal-electrons-during-nanosecond-laser-energy-deposit-fused-silica','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22310945-role-suprathermal-electrons-during-nanosecond-laser-energy-deposit-fused-silica"><span>Role of suprathermal <span class="hlt">electrons</span> during nanosecond laser <span class="hlt">energy</span> deposit in fused silica</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Grua, P.; Hébert, D.; Lamaignère, L.</p> <p>2014-08-25</p> <p>An accurate description of interaction between a nanosecond laser pulse and a wide <span class="hlt">band</span> gap dielectric, such as fused silica, requires the understanding of <span class="hlt">energy</span> deposit induced by temperature changes occurring in the material. In order to identify the fundamental processes involved in laser-matter interaction, we have used a 1D computational model that allows us to describe a wide set of physical mechanisms and intended for comparison with specially designed “1D experiments.” We have pointed out that suprathermal <span class="hlt">electrons</span> are very likely implicated in heat conduction, and this assumption has allowed the model to reproduce the experiments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013JKPS...63..809M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013JKPS...63..809M"><span><span class="hlt">Electronic</span> structures of of PuX (X=S, Se, Te)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Maehira, Takahiro; Sakai, Eijiro; Tatetsu, Yasutomi</p> <p>2013-08-01</p> <p>We have calculated the <span class="hlt">energy</span> <span class="hlt">band</span> structures and the Fermi surfaces of PuS, PuSe, and PuTe by using a self-consistent relativistic linear augmented-plane-wave method with the exchange and correlation potential in the local density approximation. In general, the <span class="hlt">energy</span> <span class="hlt">bands</span> near the Fermi level are mainly caused by the hybridization between the Pu 5 f and the monochalcogenide p <span class="hlt">electrons</span>. The obtained main Fermi surfaces consisted of two hole sheets and one <span class="hlt">electron</span> sheet, which were constructed from the <span class="hlt">band</span> having both the Pu 5 f state and the monochalcogenide p state.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AIPC.1942i0028A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AIPC.1942i0028A"><span><span class="hlt">Electronic</span> structure modifications and <span class="hlt">band</span> gap narrowing in Zn0.95V0.05O</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ahad, Abdul; Majid, S. S.; Rahman, F.; Shukla, D. K.; Phase, D. M.</p> <p>2018-04-01</p> <p>We present here, structural, optical and <span class="hlt">electronic</span> structure studies on Zn0.95V0.05O, synthesized using solid state method. Rietveld refinement of x-ray diffraction pattern indicates no considerable change in the lattice of doped ZnO. The <span class="hlt">band</span> gap of doped sample, as calculated by Kubelka-Munk transformed reflectance spectra, has been found reduced compared to pure ZnO. Considerable changes in absorbance in UV-Vis range is observed in doped sample. V doping induced decrease in <span class="hlt">band</span> gap is supported by x-ray absorption spectroscopy measurements. It is experimentally confirmed that conduction <span class="hlt">band</span> edge in Zn0.95V0.05O has shifted towards Fermi level than in pure ZnO.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19437632','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19437632"><span><span class="hlt">Energy</span> spectrum of cosmic-ray <span class="hlt">electrons</span> at TeV <span class="hlt">energies</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Aharonian, F; Akhperjanian, A G; Barres de Almeida, U; Bazer-Bachi, A R; Becherini, Y; Behera, B; Benbow, W; Bernlöhr, K; Boisson, C; Bochow, A; Borrel, V; Braun, I; Brion, E; Brucker, J; Brun, P; Brucker, R; Bulik, T; Büsching, I; Boutelier, T; Carrigan, S; Chadwick, P M; Charbonnier, A; Chaves, R C G; Cheesebrough, A; Chounet, L M; Clapson, A C; Coignet, G; Costamante, L; Dalton, M; Degrange, B; Deil, C; Dickinson, H J; Djannati-Ataï, A; Domainko, W; Drury, L O'C; Dubois, F; Dubus, G; Dyks, J; Dyrda, M; Egberts, K; Emmanoulopoulos, D; Espigat, P; Farnier, C; Feinstein, F; Fiasson, A; Fontaine, G; Füsling, M; Gabici, S; Gallant, Y A; Gérard, L; Giebels, B; Glicenstein, J F; Glück, B; Goret, P; Hadjichristidis, C; Hauser, D; Hauser, M; Heinz, S; Heinzelmann, G; Henri, G; Hermann, G; Hinton, J A; Hoffmann, A; Hofmann, W; Holleran, M; Hoppe, S; Horns, D; Jacholkowska, A; de Jager, O C; Jung, I; Katarzyński, K; Kaufmann, S; Kendziorra, E; Kerschhaggl, M; Khangulyan, D; Khélifi, B; Keogh, D; Komin, Nu; Kosack, K; Lamanna, G; Lenain, J P; Lohse, T; Marandon, V; Martin, J M; Martineau-Huynh, O; Marcowith, A; Maurin, D; McComb, T J L; Medina, C; Moderski, R; Moulin, E; Naumann-Godo, M; de Naurois, M; Nedbal, D; Nekrassov, D; Niemiec, J; Nolan, S J; Ohm, S; Olive, J F; de Oña Wilhelmi, E; Orford, K J; Osborne, J L; Ostrowski, M; Panter, M; Pedaletti, G; Pelletier, G; Petrucci, P O; Pita, S; Pühlhofer, G; Punch, M; Quirrenbach, A; Raubenheimer, B C; Raue, M; Rayner, S M; Renaud, M; Rieger, F; Ripken, J; Rob, L; Rosier-Lees, S; Rowell, G; Rudak, B; Rulten, C B; Ruppel, J; Sahakian, V; Santangelo, A; Schlickeiser, R; Schöck, F M; Schröder, R; Schwanke, U; Schwarzburg, S; Schwemmer, S; Shalchi, A; Skilton, J L; Sol, H; Spangler, D; Stawarz, Ł; Steenkamp, R; Stegmann, C; Superina, G; Tam, P H; Tavernet, J P; Terrier, R; Tibolla, O; van Eldik, C; Vasileiadis, G; Venter, C; Vialle, J P; Vincent, P; Vivier, M; Völk, H J; Volpe, F; Wagner, S J; Ward, M; Zdziarski, A A; Zech, A</p> <p>2008-12-31</p> <p>The very large collection area of ground-based gamma-ray telescopes gives them a substantial advantage over balloon or satellite based instruments in the detection of very-high-<span class="hlt">energy</span> (>600 GeV) cosmic-ray <span class="hlt">electrons</span>. Here we present the <span class="hlt">electron</span> spectrum derived from data taken with the High <span class="hlt">Energy</span> Stereoscopic System (H.E.S.S.) of imaging atmospheric Cherenkov telescopes. In this measurement, the first of this type, we are able to extend the measurement of the <span class="hlt">electron</span> spectrum beyond the range accessible to direct measurements. We find evidence for a substantial steepening in the <span class="hlt">energy</span> spectrum above 600 GeV compared to lower <span class="hlt">energies</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PhRvB..92u4514K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PhRvB..92u4514K"><span>Fragile surface zero-<span class="hlt">energy</span> flat <span class="hlt">bands</span> in three-dimensional chiral superconductors</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kobayashi, Shingo; Tanaka, Yukio; Sato, Masatoshi</p> <p>2015-12-01</p> <p>We study surface zero-<span class="hlt">energy</span> flat <span class="hlt">bands</span> in three-dimensional chiral superconductors with pz(px+i py) ν -wave pairing symmetry (ν is a nonzero integer), based on topological arguments and tunneling conductance. It is shown that the surface flat <span class="hlt">bands</span> are fragile against (i) the surface misorientation and (ii) the surface Rashba spin-orbit interaction. The fragility of (i) is specific to chiral SCs, whereas that of (ii) happens for general odd-parity SCs. We demonstrate that these flat-<span class="hlt">band</span> instabilities vanish or suppress a zero-bias conductance peak in a normal/insulator/superconductor junction, which behavior is clearly different from high-Tc cuprates and noncentrosymmetric superconductors. By calculating the angle-resolved conductance, we also discuss a topological surface state associated with the coexistence of line and point nodes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/8724739','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/8724739"><span>Thermoluminescent dosimetry in <span class="hlt">electron</span> beams: <span class="hlt">energy</span> dependence.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Robar, V; Zankowski, C; Olivares Pla, M; Podgorsak, E B</p> <p>1996-05-01</p> <p>The response of thermoluminescent dosimeters to <span class="hlt">electron</span> irradiations depends on the radiation dose, mean <span class="hlt">electron</span> <span class="hlt">energy</span> at the position of the dosimeter in phantom, and the size of the dosimeter. In this paper the semi-empirical expression proposed by Holt et al. [Phys. Med. Biol. 20, 559-570 (1975)] is combined with the calculated <span class="hlt">electron</span> dose fraction to determine the thermoluminescent dosimetry (TLD) response as a function of the mean <span class="hlt">electron</span> <span class="hlt">energy</span> and the dosimeter size. The <span class="hlt">electron</span> and photon dose fractions, defined as the relative contributions of <span class="hlt">electrons</span> and bremsstrahlung photons to the total dose for a clinical <span class="hlt">electron</span> beam, are calculated with Monte Carlo techniques using EGS4. Agreement between the calculated and measured TLD response is very good. We show that the considerable reduction in TLD response per unit dose at low <span class="hlt">electron</span> <span class="hlt">energies</span>, i.e., at large depths in phantom, is offset by an ever-increasing relative contribution of bremsstrahlung photons to the total dose of clinical <span class="hlt">electron</span> beams. This renders the TLD sufficiently reliable for dose measurements over the entire <span class="hlt">electron</span> depth dose distribution despite the dependence of the TLD response on <span class="hlt">electron</span> beam <span class="hlt">energy</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018APExp..11f1301D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018APExp..11f1301D"><span>Modulating the <span class="hlt">band</span> structure and sub-bandgap absorption of Co-hyperdoped silicon by co-doping with shallow-level elements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dong, Xiao; Fang, Xiuxiu; Wang, Yongyong; Song, Xiaohui; Lu, Zhansheng</p> <p>2018-06-01</p> <p>Hyperdoped group-III elements can lower the Fermi <span class="hlt">energy</span> in the <span class="hlt">band</span> structures of Co-hyperdoped silicon. When the Co-to-X (X = B, Al, Ga) ratio is 2:1, the intermediate <span class="hlt">band</span> (IB) in the bandgap includes the Fermi <span class="hlt">energy</span> and is partially filled by <span class="hlt">electrons</span>, which is in accordance with the requirement of an IB material. The hyperdoped X atoms can cause the blueshift of the sub-bandgap absorption of the compound compared with the material with no shallow-level elements, which is due to the enlargement of the <span class="hlt">electronic</span> excitation <span class="hlt">energy</span> of the Co,X-co-doped silicon.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23214551','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23214551"><span><span class="hlt">Energy</span> transport in weakly nonlinear wave systems with narrow frequency <span class="hlt">band</span> excitation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kartashova, Elena</p> <p>2012-10-01</p> <p>A novel discrete model (D model) is presented describing nonlinear wave interactions in systems with small and moderate nonlinearity under narrow frequency <span class="hlt">band</span> excitation. It integrates in a single theoretical frame two mechanisms of <span class="hlt">energy</span> transport between modes, namely, intermittency and <span class="hlt">energy</span> cascade, and gives the conditions under which each regime will take place. Conditions for the formation of a cascade, cascade direction, conditions for cascade termination, etc., are given and depend strongly on the choice of excitation parameters. The <span class="hlt">energy</span> spectra of a cascade may be computed, yielding discrete and continuous <span class="hlt">energy</span> spectra. The model does not require statistical assumptions, as all effects are derived from the interaction of distinct modes. In the example given-surface water waves with dispersion function ω(2)=gk and small nonlinearity-the D model predicts asymmetrical growth of side-<span class="hlt">bands</span> for Benjamin-Feir instability, while the transition from discrete to continuous <span class="hlt">energy</span> spectrum, excitation parameters properly chosen, yields the saturated Phillips' power spectrum ~g(2)ω(-5). The D model can be applied to the experimental and theoretical study of numerous wave systems appearing in hydrodynamics, nonlinear optics, electrodynamics, plasma, convection theory, etc.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_18 --> <div id="page_19" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="361"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011PhDT........61F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011PhDT........61F"><span><span class="hlt">Band</span> alignment measurements at heterojunction interfaces in layered thin film solar cells & thermoelectrics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fang, Fang</p> <p>2011-12-01</p> <p>Public awareness of the increasing <span class="hlt">energy</span> crisis and the related serious environmental concerns has led to a significantly growing demand for alternative clean and renewable <span class="hlt">energy</span> resources. Thin film are widely applied in multiple renewable <span class="hlt">energy</span> devices owing to the reduced amount of raw materials and increase flexibility of choosing from low-cost candidates, which translates directly into reduced capital cost. This is a key driving force to make renewable technology competitive in the <span class="hlt">energy</span> market. This thesis is focused on the measurement of <span class="hlt">energy</span> level alignments at interfaces of thin film structures for renewable <span class="hlt">energy</span> applications. There are two primary foci: II -VI semiconductor ZnSe/ZnTe thin film solar cells and Bi2Te3/Sb2Te3 thin film structures for thermoelectric applications. In both cases, the <span class="hlt">electronic</span> structure and <span class="hlt">energy</span> <span class="hlt">band</span> alignment at interfaces usually controls the carrier transport behavior and determines the quality of the device. High-resolution photoemission spectroscopy (lab-based XPS & synchrotron-based UPS) was used to investigate the chemical and <span class="hlt">electronic</span> properties of epitaxial Bi2Te3 and Sb2Te3 thin films, in order to validate the anticipated <span class="hlt">band</span> alignment at interfaces in Bi 2Te3/Sb2Te3 superlattices as one favoring <span class="hlt">electron</span>-transmission. A simple, thorough two-step treatment of a chemical etching in dilute hydrochloric acid solution and a subsequent annealing at ˜150°C under ultra-high vacuum environment is established to remove the surface oxides completely. It is an essential step to ensure the measurements on <span class="hlt">electronic</span> states are acquired on stoichimetric, oxide-free clean surface of Bi 2Te3 and Sb2Te3 films. The direct measurement of valence <span class="hlt">band</span> offsets (VBO) at a real Sb 2Te3/Bi2Te3 interface is designed based on the Kraut model; a special stacking film structure is prepared intentionally: sufficiently thin Sb2Te3 film on top of Bi2Te 3 that photoelectrons from both of them are collected simultaneously. From a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29460856','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29460856"><span>Ultraviolet photoelectron spectroscopy reveals <span class="hlt">energy-band</span> dispersion for π-stacked 7,8,15,16-tetraazaterrylene thin films in a donor-acceptor bulk heterojunction.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Aghdassi, Nabi; Wang, Qi; Ji, Ru-Ru; Wang, Bin; Fan, Jian; Duhm, Steffen</p> <p>2018-05-11</p> <p>7,8,15,16-tetraazaterrylene (TAT) thin films grown on highly oriented pyrolytic graphite (HOPG) substrates were studied extensively with regard to their intrinsic and interfacial <span class="hlt">electronic</span> properties by means of ultraviolet photoelectron spectroscopy (UPS). Merely weak substrate-adsorbate interaction occurs at the TAT/HOPG interface, with interface energetics being only little affected by the nominal film thickness. Photon <span class="hlt">energy</span>-dependent UPS performed perpendicular to the molecular planes of TAT multilayer films at room temperature clearly reveals <span class="hlt">band</span>-like intermolecular dispersion of the TAT highest occupied molecular orbital (HOMO) <span class="hlt">energy</span>. Based on a comparison with a tight-binding model, a relatively narrow bandwidth of 54 meV is derived, which points to the presence of an intermediate regime between hopping and <span class="hlt">band</span>-like hole transport. Upon additional deposition of 2,2':5',2″:5″,2″'-quaterthiophene (4T), a 4T:TAT donor-acceptor bulk heterojunction with a considerable HOMO-level offset at the donor-acceptor interface is formed. The 4T:TAT bulk heterojunction likewise exhibits intermolecular dispersion of the TAT HOMO <span class="hlt">energy</span>, yet with a significant decreased bandwidth.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EPJD...66...26C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EPJD...66...26C"><span><span class="hlt">Electron</span> impact excitation of higher <span class="hlt">energy</span> states of molecular oxygen in the atmosphere of Europa</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Campbell, L.; Tanaka, H.; Kato, H.; Jayaraman, S.; Brunger, M. J.</p> <p>2012-01-01</p> <p>Recent measurements of integral cross sections for <span class="hlt">electron</span> impact excitation of the Schumann-Runge continuum, longest <span class="hlt">band</span> and second <span class="hlt">band</span> of molecular oxygen are applied to calculations of emissions from the atmosphere of Europa. Molecules excited to these <span class="hlt">bands</span> predissociate, producing O(1D) (excited oxygen) atoms which subsequently decay to produce 630.0-nm radiation. Radiation of this wavelength is also produced by direct excitation of O atoms and by the recombination of O _2^+ + 2 with <span class="hlt">electrons</span>, but these two processes also produce O(1S) atoms which then emit at 557.7 nm. It is shown by modeling that the ratio of 630.0-nm to 557.7-nm is sensitive to the relative importance of the three processes, suggesting that the ratio would be a useful remote sensing probe in the atmosphere of Europa. In particular, the excitation of the Schumann-Runge continuum, longest <span class="hlt">band</span> and second <span class="hlt">band</span> is produced by magnetospheric <span class="hlt">electrons</span> while the recombination is produced by secondary <span class="hlt">electrons</span> produced in the atmosphere. This difference raises the possibility of determination of the secondary <span class="hlt">electron</span> spectrum by measurement of light emissions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA412962','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA412962"><span>C (G)-<span class="hlt">Band</span> & X (I) - <span class="hlt">Band</span> Noncoherent Radar Transponder Performance Specification Standard</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2002-04-01</p> <p>TRAINING RANGE NEVADA TEST SITE STANDARD 262-02 <span class="hlt">ELECTRONIC</span> TRAJECTORY MEASUREMENTS GROUP C (G) – <span class="hlt">BAND</span> & X (I) – <span class="hlt">BAND</span> NONCOHERENT RADAR...Date 00 Apr 2002 Report Type N/A Dates Covered (from... to) - Title and Subtitle C (G)-<span class="hlt">Band</span> & X (I) - <span class="hlt">Band</span> Noncoherent Radar Transponder...Number of Pages 157 i STANDARD 262-02 C (G) – <span class="hlt">BAND</span> & X (I) – <span class="hlt">BAND</span> NONCOHERENT RADAR TRANSPONDER PERFORMANCE SPECIFICATION STANDARD APRIL 2002 Prepared by</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AIPC.1953k0026M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AIPC.1953k0026M"><span><span class="hlt">Electronic</span> structure and <span class="hlt">electron</span> momentum densities of Ag2CrO4</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Meena, Seema Kumari; Ahuja, B. L.</p> <p>2018-05-01</p> <p>We present the first-ever experimental <span class="hlt">electron</span> momentum density of Ag2CrO4 using 661.65 keV γ-rays from 20 Ci 137Cs source. To validate our experimental data, we have also deduced theoretical Compton profiles, <span class="hlt">energy</span> <span class="hlt">bands</span> and density of states using linear combination of atomic orbitals (LCAO) method in the framework of density functional theory. It is seen that the DFT-LDA gives a better agreement with experimental data than free atom model. The <span class="hlt">energy</span> <span class="hlt">bands</span> and density of states are also discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1399563-experimental-determination-ionization-energies-mose2-ws2-mos2-sio2-using-photoemission-electron-microscopy','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1399563-experimental-determination-ionization-energies-mose2-ws2-mos2-sio2-using-photoemission-electron-microscopy"><span>Experimental Determination of the Ionization <span class="hlt">Energies</span> of MoSe 2, WS 2, and MoS 2 on SiO 2 Using Photoemission <span class="hlt">Electron</span> Microscopy</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Keyshar, Kunttal; Berg, Morgann; Zhang, Xiang; ...</p> <p>2017-07-19</p> <p>Here, the values of the ionization <span class="hlt">energies</span> of transition metal dichalcogenides (TMDs) are needed to assess their potential usefulness in semiconductor heterojunctions for high-performance optoelectronics. Here, we report on the systematic determination of ionization <span class="hlt">energies</span> for three prototypical TMD monolayers (MoSe 2, WS 2, and MoS 2) on SiO 2 using photoemission <span class="hlt">electron</span> microscopy with deep ultraviolet illumination. The ionization <span class="hlt">energy</span> displays a progressive decrease from MoS 2, to WS 2, to MoSe 2, in agreement with predictions of density functional theory calculations. Combined with the measured <span class="hlt">energy</span> positions of the valence <span class="hlt">band</span> edge at the Brillouin zone center, wemore » deduce that, in the absence of interlayer coupling, a vertical heterojunction comprising any of the three TMD monolayers would form a staggered (type-II) <span class="hlt">band</span> alignment. This <span class="hlt">band</span> alignment could give rise to long-lived interlayer excitons that are potentially useful for valleytronics or efficient electron–hole separation in photovoltaics.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhRvP...8e4017L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvP...8e4017L"><span>Femtosecond MeV <span class="hlt">Electron</span> <span class="hlt">Energy</span>-Loss Spectroscopy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, R. K.; Wang, X. J.</p> <p>2017-11-01</p> <p>Pump-probe <span class="hlt">electron</span> <span class="hlt">energy</span>-loss spectroscopy (EELS) with femtosecond temporal resolution will be a transformative research tool for studying nonequilibrium chemistry and <span class="hlt">electronic</span> dynamics of matter. In this paper, we propose a concept of femtosecond EELS utilizing mega-<span class="hlt">electron</span>-volt <span class="hlt">electron</span> beams from a radio-frequency (rf) photocathode source. The high acceleration gradient and high beam <span class="hlt">energy</span> of the rf gun are critical to the generation of 10-fs <span class="hlt">electron</span> beams, which enables an improvement of the temporal resolution by more than 1 order of magnitude beyond the state of the art. In our proposal, the "reference-beam technique" relaxes the <span class="hlt">energy</span> stability requirement of the rf power source by roughly 2 orders of magnitude. The requirements for the <span class="hlt">electron</span>-beam quality, photocathode, spectrometer, and detector are also discussed. Supported by particle-tracking simulations, we demonstrate the feasibility of achieving sub-<span class="hlt">electron</span>-volt <span class="hlt">energy</span> resolution and approximately 10-fs temporal resolution with existing or near-future hardware performance.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27608986','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27608986"><span>Free-end adaptive nudged elastic <span class="hlt">band</span> method for locating transition states in minimum <span class="hlt">energy</span> path calculation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhang, Jiayong; Zhang, Hongwu; Ye, Hongfei; Zheng, Yonggang</p> <p>2016-09-07</p> <p>A free-end adaptive nudged elastic <span class="hlt">band</span> (FEA-NEB) method is presented for finding transition states on minimum <span class="hlt">energy</span> paths, where the <span class="hlt">energy</span> barrier is very narrow compared to the whole paths. The previously proposed free-end nudged elastic <span class="hlt">band</span> method may suffer from convergence problems because of the kinks arising on the elastic <span class="hlt">band</span> if the initial elastic <span class="hlt">band</span> is far from the minimum <span class="hlt">energy</span> path and weak springs are adopted. We analyze the origin of the formation of kinks and present an improved free-end algorithm to avoid the convergence problem. Moreover, by coupling the improved free-end algorithm and an adaptive strategy, we develop a FEA-NEB method to accurately locate the transition state with the elastic <span class="hlt">band</span> cut off repeatedly and the density of images near the transition state increased. Several representative numerical examples, including the dislocation nucleation in a penta-twinned nanowire, the twin boundary migration under a shear stress, and the cross-slip of screw dislocation in face-centered cubic metals, are investigated by using the FEA-NEB method. Numerical results demonstrate both the stability and efficiency of the proposed method.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvB..97k5433P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvB..97k5433P"><span><span class="hlt">Electron</span> affinity and surface states of GaN m -plane facets: Implication for <span class="hlt">electronic</span> self-passivation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Portz, V.; Schnedler, M.; Eisele, H.; Dunin-Borkowski, R. E.; Ebert, Ph.</p> <p>2018-03-01</p> <p>The <span class="hlt">electron</span> affinity and surface states are of utmost importance for designing the potential landscape within (heterojunction) nanowires and hence for tuning conductivity and carrier lifetimes. Therefore, we determined for stoichiometric nonpolar GaN (10 1 ¯0 ) m -plane facets, i.e., the dominating sidewalls of GaN nanowires, the <span class="hlt">electron</span> affinity to 4.06 ±0.07 eV and the <span class="hlt">energy</span> of the empty Ga-derived surface state in the <span class="hlt">band</span> gap to 0.99 ±0.08 eV below the conduction <span class="hlt">band</span> minimum using scanning tunneling spectroscopy. These values imply that the potential landscape within GaN nanowires is defined by a surface state-induced Fermi-level pinning, creating an upward <span class="hlt">band</span> bending at the sidewall facets, which provides an <span class="hlt">electronic</span> passivation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMSH21A2385W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMSH21A2385W"><span>The <span class="hlt">Energy</span> Spectrum of Solar Energetic <span class="hlt">Electrons</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, L.; Yang, L.; Krucker, S.; Wimmer-Schweingruber, R. F.; Bale, S. D.</p> <p>2015-12-01</p> <p>Here we present a statistical survey of the <span class="hlt">energy</span> spectrum of solar energetic <span class="hlt">electron</span> events (SEEs) observed by the WIND 3DP instrument from 1995 though 2014. For SEEs with the minimum <span class="hlt">energy</span> below 10 keV and the maximum <span class="hlt">energy</span> above 100 keV, ~85% (~2%) have a double-power-law <span class="hlt">energy</span> spectrum with a steepening (hardening) above the break <span class="hlt">energy</span>, while ~13% have a single-power-law <span class="hlt">energy</span> spectrum at all <span class="hlt">energies</span>. The average spectral index is ~2.4 below the <span class="hlt">energy</span> break and is ~4.0 above the <span class="hlt">energy</span> break. For SEEs detected only at <span class="hlt">energies</span> <10 keV (>20 keV), they generally show a single-power-law spectrum with the average index of ~3.0 (~3.3). The spectrum of SEEs detected only below 10 keV appears to get harder with increasing solar activity, but the spectrum of SEEs with higher-<span class="hlt">energy</span> <span class="hlt">electrons</span> shows no clear correlation with solar activity. We will also investigate whether the observed <span class="hlt">energy</span> spectrum of SEEs at 1 AU mainly reflects the <span class="hlt">electron</span> acceleration at the Sun or the <span class="hlt">electron</span> transport in the interplanetary medium.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JKPS...71.1048S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JKPS...71.1048S"><span>Design of 6 MeV X-<span class="hlt">band</span> <span class="hlt">electron</span> linac for dual-head gantry radiotherapy system</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shin, Seung-wook; Lee, Seung-Hyun; Lee, Jong-Chul; Kim, Huisu; Ha, Donghyup; Ghergherehchi, Mitra; Chai, Jongseo; Lee, Byung-no; Chae, Moonsik</p> <p>2017-12-01</p> <p>A compact 6 MeV <span class="hlt">electron</span> linac is being developed at Sungkyunkwan University, in collaboration with the Korea atomic <span class="hlt">energy</span> research institute (KAERI). The linac will be used as an X-ray source for a dual-head gantry radiotherapy system. X-<span class="hlt">band</span> technology has been employed to satisfy the size requirement of the dual-head gantry radiotherapy machine. Among the several options available, we selected a pi/2-mode, standing-wave, side-coupled cavity. This choice of radiofrequency (RF) cavity design is intended to enhance the shunt impedance of each cavity in the linac. An optimum structure of the RF cavity with a high-performance design was determined by applying a genetic algorithm during the optimization procedure. This paper describes the detailed design process for a single normal RF cavity and the entire structure, including the RF power coupler and coupling cavity, as well as the beam dynamics results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1176927','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1176927"><span>Strategic <span class="hlt">Energy</span> Management Plan for the Santa Ynez <span class="hlt">Band</span> of Chumash Indians</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Davenport, Lars; Smythe, Louisa; Sarquilla, Lindsey</p> <p>2015-03-27</p> <p>This plan outlines the Santa Ynez <span class="hlt">Band</span> of Chumash Indians’ comprehensive <span class="hlt">energy</span> management strategy including an assessment of current practices, a commitment to improving <span class="hlt">energy</span> performance and reducing overall <span class="hlt">energy</span> use, and recommended actions to achieve these goals. Vision Statement The primary objective of the Strategic <span class="hlt">Energy</span> Management Plan is to implement <span class="hlt">energy</span> efficiency, <span class="hlt">energy</span> security, conservation, education, and renewable <span class="hlt">energy</span> projects that align with the economic goals and cultural values of the community to improve the health and welfare of the tribe. The intended outcomes of implementing the <span class="hlt">energy</span> plan include job creation, capacity building, and reduced <span class="hlt">energy</span> costsmore » for tribal community members, and tribal operations. By encouraging <span class="hlt">energy</span> independence and local power production the plan will promote self-sufficiency. Mission & Objectives The Strategic <span class="hlt">Energy</span> Plan will provide information and suggestions to guide tribal decision-making and provide a foundation for effective management of <span class="hlt">energy</span> resources within the Santa Ynez <span class="hlt">Band</span> of Chumash Indians (SYBCI) community. The objectives of developing this plan include; Assess current <span class="hlt">energy</span> demand and costs of all tribal enterprises, offices, and facilities; Provide a baseline assessment of the SYBCI’s <span class="hlt">energy</span> resources so that future progress can be clearly and consistently measured, and current usage better understood; Project future <span class="hlt">energy</span> demand; Establish a system for centralized, ongoing tracking and analysis of tribal <span class="hlt">energy</span> data that is applicable across sectors, facilities, and activities; Develop a unifying vision that is consistent with the tribe’s long-term cultural, social, environmental, and economic goals; Identify and evaluate the potential of opportunities for development of long-term, cost effective <span class="hlt">energy</span> sources, such as renewable <span class="hlt">energy</span>, <span class="hlt">energy</span> efficiency and conservation, and other feasible supply- and demand-side options; and Build the SYBCI’s capacity for</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PhRvB..92t5301V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PhRvB..92t5301V"><span>Digital direct <span class="hlt">electron</span> imaging of <span class="hlt">energy</span>-filtered <span class="hlt">electron</span> backscatter diffraction patterns</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vespucci, S.; Winkelmann, A.; Naresh-Kumar, G.; Mingard, K. P.; Maneuski, D.; Edwards, P. R.; Day, A. P.; O'Shea, V.; Trager-Cowan, C.</p> <p>2015-11-01</p> <p><span class="hlt">Electron</span> backscatter diffraction is a scanning <span class="hlt">electron</span> microscopy technique used to obtain crystallographic information on materials. It allows the nondestructive mapping of crystal structure, texture, and strain with a lateral and depth resolution on the order of tens of nanometers. <span class="hlt">Electron</span> backscatter diffraction patterns (EBSPs) are presently acquired using a detector comprising a scintillator coupled to a digital camera, and the crystallographic information obtainable is limited by the conversion of <span class="hlt">electrons</span> to photons and then back to <span class="hlt">electrons</span> again. In this article we will report the direct acquisition of <span class="hlt">energy</span>-filtered EBSPs using a digital complementary metal-oxide-semiconductor hybrid pixel detector, Timepix. We show results from a range of samples with different mass and density, namely diamond, silicon, and GaN. Direct <span class="hlt">electron</span> detection allows the acquisition of EBSPs at lower (≤5 keV) <span class="hlt">electron</span> beam <span class="hlt">energies</span>. This results in a reduction in the depth and lateral extension of the volume of the specimen contributing to the pattern and will lead to a significant improvement in lateral and depth resolution. Direct <span class="hlt">electron</span> detection together with <span class="hlt">energy</span> filtering (<span class="hlt">electrons</span> having <span class="hlt">energy</span> below a specific value are excluded) also leads to an improvement in spatial resolution but in addition provides an unprecedented increase in the detail in the acquired EBSPs. An increase in contrast and higher-order diffraction features are observed. In addition, excess-deficiency effects appear to be suppressed on <span class="hlt">energy</span> filtering. This allows the fundamental physics of pattern formation to be interrogated and will enable a step change in the use of <span class="hlt">electron</span> backscatter diffraction (EBSD) for crystal phase identification and the mapping of strain. The enhancement in the contrast in high-pass <span class="hlt">energy</span>-filtered EBSD patterns is found to be stronger for lighter, less dense materials. The improved contrast for such materials will enable the application of the EBSD</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/569607','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/569607"><span>High <span class="hlt">energy</span> <span class="hlt">electron</span> cooling</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Parkhomchuk, V.</p> <p>1997-09-01</p> <p>High <span class="hlt">energy</span> <span class="hlt">electron</span> cooling requires a very cold <span class="hlt">electron</span> beam. The questions of using <span class="hlt">electron</span> cooling with and without a magnetic field are presented for discussion at this workshop. The <span class="hlt">electron</span> cooling method was suggested by G. Budker in the middle sixties. The original idea of the <span class="hlt">electron</span> cooling was published in 1966. The design activities for the NAP-M project was started in November 1971 and the first run using a proton beam occurred in September 1973. The first experiment with both <span class="hlt">electron</span> and proton beams was started in May 1974. In this experiment good result was achieved very closemore » to theoretical prediction for a usual two component plasma heat exchange.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JIEIB..98..213K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JIEIB..98..213K"><span><span class="hlt">Electronic</span> Power Conditioner for Ku-<span class="hlt">band</span> Travelling Wave Tube</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kowstubha, Palle; Krishnaveni, K.; Ramesh Reddy, K.</p> <p>2017-04-01</p> <p>A highly sophisticated regulated power supply is known as <span class="hlt">electronic</span> power conditioner (EPC) is required to energise travelling wave tubes (TWTs), which are used as RF signal amplifiers in satellite payloads. The assembly consisting of TWT and EPC together is known as travelling wave tube amplifier (TWTA). EPC is used to provide isolated and conditioned voltage rails with tight regulation to various electrodes of TWT and makes its RF performance independent of solar bus variations which are caused due to varying conditions of eclipse and sunlit. The payload mass and their power consumption is mainly due to the existence of TWTAs that represent about 35 % of total mass and about 70-90 % (based on the type of satellite application) of overall dc power consumption. This situation ensures a continuous improvement in the design of TWTAs and their associated EPCs to realize more efficient and light products. Critical technologies involved in EPCs are design and configuration, closed loop regulation, component and material selection, <span class="hlt">energy</span> limiting of high voltage (HV) outputs and potting of HV card etc. This work addresses some of these critical technologies evolved in realizing and testing the state of art of EPC and it focuses on the design of HV supply with a HV and high power capability, up to 6 kV and 170 WRF, respectively required for a space TWTA. Finally, an experimental prototype of EPC with a dc power of 320 W provides different voltages required by Ku-<span class="hlt">band</span> TWT in open loop configuration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JPhD...47G5103P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JPhD...47G5103P"><span>Spectroscopic analysis of <span class="hlt">electron</span> trapping levels in pentacene field-effect transistors</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Park, Chang Bum</p> <p>2014-08-01</p> <p><span class="hlt">Electron</span> trapping phenomena have been investigated with respect to the <span class="hlt">energy</span> levels of localized trap states and bias-induced device instability effects in pentacene field-effect transistors. The mechanism of the photoinduced threshold voltage shift (ΔVT) is presented by providing a ΔVT model governed by the <span class="hlt">electron</span> trapping. The trap-and-release behaviour functionalized by photo-irradiation also shows that the trap state for <span class="hlt">electrons</span> is associated with the <span class="hlt">energy</span> levels in different positions in the forbidden gap of pentacene. Spectroscopic analysis identifies two kinds of <span class="hlt">electron</span> trap states distributed above and below the <span class="hlt">energy</span> of 2.5 eV in the <span class="hlt">band</span> gap of the pentacene crystal. The study of photocurrent spectra shows the specific trap levels of <span class="hlt">electrons</span> in <span class="hlt">energy</span> space that play a substantial role in causing device instability. The shallow and deep trapping states are distributed at two centroidal <span class="hlt">energy</span> levels of ˜1.8 and ˜2.67 eV in the pentacene <span class="hlt">band</span> gap. Moreover, we present a systematic <span class="hlt">energy</span> profile of <span class="hlt">electron</span> trap states in the pentacene crystal for the first time.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20020017758','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20020017758"><span><span class="hlt">Band</span> Anticrossing in Highly Mismatched Compound Semiconductor Alloys</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Yu, Kin Man; Wu, J.; Walukiewicz, W.; Ager, J. W.; Haller, E. E.; Miotkowski, I.; Ramdas, A.; Su, Ching-Hua; Whitaker, Ann F. (Technical Monitor)</p> <p>2001-01-01</p> <p>Compound semiconductor alloys in which metallic anions are partially replaced with more electronegative isoelectronic atoms have recently attracted significant attention. Group IIIN(x)V(1-x), alloys with a small amount of the electronegative N substituting more metallic column V elements has been the most extensively studied class of such Highly Mismatched Alloys (HMAs). We have shown that many of the unusual properties of the IIIN(x),V(1-x) alloys can be well explained by the <span class="hlt">Band</span> Anticrossing (BAC) model that describes the <span class="hlt">electronic</span> structure in terms of an interaction between highly localized levels of substitutional N and the extended states of the host semiconductor matrix. Most recently the BAC model has been also used to explain similar modifications of the <span class="hlt">electronic</span> <span class="hlt">band</span> structure observed in Te-rich ZnS(x)Te(l-x) and ZnSe(Y)Te(1-y) alloys. To date studies of HMAs have been limited to materials with relatively small concentrations of highly electronegative atoms. Here we report investigations of the <span class="hlt">electronic</span> structure of ZnSe(y)Te(1-y) alloys in the entire composition range, 0 less than or equal to y less than or equal to 1. The samples used in this study are bulk ZnSe(y)Te(1-y) crystals grown by either a modified Bridgman method or by physical vapor transport. Photomodulated reflection (PR) spectroscopy was used to measure the composition dependence of optical transitions from the valence <span class="hlt">band</span> edge and from the spin-orbit split off <span class="hlt">band</span> to the conduction <span class="hlt">band</span>. The pressure dependence of the <span class="hlt">band</span> gap was measured using optical absorption in a diamond anvil cell. We find that the <span class="hlt">energy</span> of the spin-orbit split off valence <span class="hlt">band</span> edge does not depend on composition and is located at about 3 eV below the conduction <span class="hlt">band</span> edge of ZnSe. On the Te-rich side the pressure and the composition dependence of the optical transitions are well explained by the BAC model which describes the downward shift of the conduction <span class="hlt">band</span> edge in terms of the interaction between</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19750044014&hterms=molecular+electronics&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dmolecular%2Belectronics','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19750044014&hterms=molecular+electronics&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dmolecular%2Belectronics"><span>Monte Carlo simulation of <span class="hlt">energy</span> deposition by low-<span class="hlt">energy</span> <span class="hlt">electrons</span> in molecular hydrogen</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Heaps, M. G.; Furman, D. R.; Green, A. E. S.</p> <p>1975-01-01</p> <p>A set of detailed atomic cross sections has been used to obtain the spatial deposition of <span class="hlt">energy</span> by 1-20-eV <span class="hlt">electrons</span> in molecular hydrogen by a Monte Carlo simulation of the actual trajectories. The <span class="hlt">energy</span> deposition curve (<span class="hlt">energy</span> per distance traversed) is quite peaked in the forward direction about the entry point for <span class="hlt">electrons</span> with <span class="hlt">energies</span> above the threshold of the <span class="hlt">electronic</span> states, but the peak decreases and broadens noticeably as the <span class="hlt">electron</span> <span class="hlt">energy</span> decreases below 10 eV (threshold for the lowest excitable <span class="hlt">electronic</span> state of H2). The curve also assumes a very symmetrical shape for <span class="hlt">energies</span> below 10 eV, indicating the increasing importance of elastic collisions in determining the shape of the curve, although not the mode of <span class="hlt">energy</span> deposition.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22330471','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22330471"><span><span class="hlt">Electronic</span> <span class="hlt">band</span> structures and optical properties of type-II superlattice photodetectors with interfacial effect.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Qiao, Peng-Fei; Mou, Shin; Chuang, Shun Lien</p> <p>2012-01-30</p> <p>The <span class="hlt">electronic</span> <span class="hlt">band</span> structures and optical properties of type-II superlattice (T2SL) photodetectors in the mid-infrared (IR) range are investigated. We formulate a rigorous <span class="hlt">band</span> structure model using the 8-<span class="hlt">band</span> k · p method to include the conduction and valence <span class="hlt">band</span> mixing. After solving the 8 × 8 Hamiltonian and deriving explicitly the new momentum matrix elements in terms of envelope functions, optical transition rates are obtained through the Fermi's golden rule under various doping and injection conditions. Optical measurements on T2SL photodetectors are compared with our model and show good agreement. Our modeling results of quantum structures connect directly to the device-level design and simulation. The predicted doping effect is readily applicable to the optimization of photodetectors. We further include interfacial (IF) layers to study the significance of their effect. Optical properties of T2SLs are expected to have a large tunable range by controlling the thickness and material composition of the IF layers. Our model provides an efficient tool for the designs of novel photodetectors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005NIMPA.545..744O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005NIMPA.545..744O"><span>Avalanche photodiode for measurement of low-<span class="hlt">energy</span> <span class="hlt">electrons</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ogasawara, K.; Asamura, K.; Mukai, T.; Saito, Y.</p> <p>2005-06-01</p> <p>We report on the performance of an Avalanche Photodiode (APD) produced by Hamamatsu Photonics Co. Ltd. (Type Z7966-20) for measurements of low <span class="hlt">energy</span> <span class="hlt">electrons</span>. We have set up an <span class="hlt">electron</span> gun, which can generate a 1-20 keV <span class="hlt">electron</span> beam impinging onto the APD in a vacuum chamber. The result shows that the pulse height distribution (PHD) of the APD signal exhibits a significant peak for <span class="hlt">electrons</span> with <span class="hlt">energies</span> above 8 keV, and the variation of the PHD peak shows a good linearity with the <span class="hlt">energy</span> of incident <span class="hlt">electrons</span>. The <span class="hlt">energy</span> resolution is quite good, though it slightly depends on the <span class="hlt">electron</span> <span class="hlt">energy</span>. In the case of low-<span class="hlt">energies</span> (lower than 10 keV), the pulse height distribution has a characteristic tail on the low <span class="hlt">energy</span> side, and the <span class="hlt">energy</span> resolution becomes a little worse. The position of the peak appears on a slightly lower channel than is expected from data at higher <span class="hlt">energies</span> (near 20 keV). Qualitatively, the low-<span class="hlt">energy</span> tail is caused by the dead-layer on the surface of the device. The nonlinearity and the worse resolution of the peaks for higher <span class="hlt">energy</span> <span class="hlt">electrons</span> may have resulted from a space-charge effect due to created e-h pairs. For a quantitative understanding, we have made a Monte Carlo particle simulation of charge transport and collection inside the APD.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_19 --> <div id="page_20" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="381"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1182486-observation-electron-band-above-fermi-level-fete-se-from-situ-surface-doping','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1182486-observation-electron-band-above-fermi-level-fete-se-from-situ-surface-doping"><span>Observation of an <span class="hlt">electron</span> <span class="hlt">band</span> above the Fermi level in FeTe₀.₅₅Se₀.₄₅ from in-situ surface doping</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Zhang, P.; Richard, P.; Xu, N.; ...</p> <p>2014-10-27</p> <p>We used in-situ potassium (K) evaporation to dope the surface of the iron-based superconductor FeTe₀.₅₅Se₀.₄₅. The systematic study of the <span class="hlt">bands</span> near the Fermi level confirms that <span class="hlt">electrons</span> are doped into the system, allowing us to tune the Fermi level of this material and to access otherwise unoccupied <span class="hlt">electronic</span> states. In particular, we observe an <span class="hlt">electron</span> <span class="hlt">band</span> located above the Fermi level before doping that shares similarities with a small three-dimensional pocket observed in the cousin, heavily-<span class="hlt">electron</span>-doped KFe₂₋ xSe₂ compound.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ApSS..422..179C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ApSS..422..179C"><span><span class="hlt">Band</span> offsets in ITO/Ga2O3 heterostructures</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carey, Patrick H.; Ren, F.; Hays, David C.; Gila, B. P.; Pearton, S. J.; Jang, Soohwan; Kuramata, Akito</p> <p>2017-11-01</p> <p>The valence <span class="hlt">band</span> offsets in rf-sputtered Indium Tin Oxide (ITO)/single crystal β-Ga2O3 (ITO/Ga2O3) heterostructures were measured with X-Ray Photoelectron Spectroscopy using the Kraut method. The bandgaps of the component materials in the heterostructure were determined by Reflection <span class="hlt">Electron</span> <span class="hlt">Energy</span> Loss Spectroscopy as 4.6 eV for Ga2O3 and 3.5 eV for ITO. The valence <span class="hlt">band</span> offset was determined to be -0.78 ± 0.30 eV, while the conduction <span class="hlt">band</span> offset was determined to be -0.32 ± 0.13 eV. The ITO/Ga2O3 system has a nested gap (type I) alignment. The use of a thin layer of ITO between a metal and the Ga2O3 is an attractive approach for reducing contact resistance on Ga2O3-based power <span class="hlt">electronic</span> devices and solar-blind photodetectors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22494995-energies-valleys-sub-ga-sub-from-electronic-structure-calculations','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22494995-energies-valleys-sub-ga-sub-from-electronic-structure-calculations"><span><span class="hlt">Energies</span> of the X- and L-valleys in In{sub 0.53}Ga{sub 0.47}As from <span class="hlt">electronic</span> structure calculations</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Greene-Diniz, Gabriel; Greer, J. C.; Fischetti, M. V.</p> <p>2016-02-07</p> <p>Several theoretical <span class="hlt">electronic</span> structure methods are applied to study the relative <span class="hlt">energies</span> of the minima of the X- and L-conduction-<span class="hlt">band</span> satellite valleys of In{sub x}Ga{sub 1−x}As with x = 0.53. This III-V semiconductor is a contender as a replacement for silicon in high-performance n-type metal-oxide-semiconductor transistors. The <span class="hlt">energy</span> of the low-lying valleys relative to the conduction-<span class="hlt">band</span> edge governs the population of channel carriers as the transistor is brought into inversion, hence determining current drive and switching properties at gate voltages above threshold. The calculations indicate that the position of the L- and X-valley minima are ∼1 eV and ∼1.2 eV, respectively, higher in energymore » with respect to the conduction-<span class="hlt">band</span> minimum at the Γ-point.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26166580','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26166580"><span>Quantitative operando visualization of the <span class="hlt">energy</span> <span class="hlt">band</span> depth profile in solar cells.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chen, Qi; Mao, Lin; Li, Yaowen; Kong, Tao; Wu, Na; Ma, Changqi; Bai, Sai; Jin, Yizheng; Wu, Dan; Lu, Wei; Wang, Bing; Chen, Liwei</p> <p>2015-07-13</p> <p>The <span class="hlt">energy</span> <span class="hlt">band</span> alignment in solar cell devices is critically important because it largely governs elementary photovoltaic processes, such as the generation, separation, transport, recombination and collection of charge carriers. Despite the expenditure of considerable effort, the measurement of <span class="hlt">energy</span> <span class="hlt">band</span> depth profiles across multiple layers has been extremely challenging, especially for operando devices. Here we present direct visualization of the surface potential depth profile over the cross-sections of operando organic photovoltaic devices using scanning Kelvin probe microscopy. The convolution effect due to finite tip size and cantilever beam crosstalk has previously prohibited quantitative interpretation of scanning Kelvin probe microscopy-measured surface potential depth profiles. We develop a bias voltage-compensation method to address this critical problem and obtain quantitatively accurate measurements of the open-circuit voltage, built-in potential and electrode potential difference.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AIPC.1942i0031T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AIPC.1942i0031T"><span><span class="hlt">Bands</span> dispersion and charge transfer in β-BeH2</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Trivedi, D. K.; Galav, K. L.; Joshi, K. B.</p> <p>2018-04-01</p> <p>Predictive capabilities of ab-initio method are utilised to explore <span class="hlt">bands</span> dispersion and charge transfer in β-BeH2. Investigations are carried out using the linear combination of atomic orbitals method at the level of density functional theory. The crystal structure and related parameters are settled by coupling total <span class="hlt">energy</span> calculations with the Murnaghan equation of state. <span class="hlt">Electronic</span> <span class="hlt">bands</span> dispersion from PBE-GGA is reported. The PBE-GGA, and PBE0 hybrid functional, show that β-BeH2 is a direct gap semiconductor with 1.18 and 2.40 eV <span class="hlt">band</span> gap. The <span class="hlt">band</span> gap slowly decreases with pressure and beyond l00 GPa overlap of conduction and valence <span class="hlt">bands</span> at the r point is observed. Charge transfer is studied by means of Mullikan population analysis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1994SPIE.2142..261H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1994SPIE.2142..261H"><span>New results on thermalization of <span class="hlt">electrons</span> in GaAs</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hannak, Reinhard M.; Ruehle, Wolfgang W.</p> <p>1994-05-01</p> <p>The transition from a nonthermal into a thermal distribution of <span class="hlt">electrons</span> at low densities (< 1014 cm-3) is traced on a picosecond time-scale by the time evolution of a <span class="hlt">band</span>-to-acceptor transition in GaAs:Be. Two narrow, nonthermal <span class="hlt">electron</span> distributions are detected during the first picoseconds originating from the heavy- and light-hole valence <span class="hlt">band</span>, respectively. Measurements with circular polarization of excitation and luminescence confirm this assignment. The variation of their energetic peak-positions with excitation <span class="hlt">energy</span> allows the experimental determination of the valence <span class="hlt">band</span> dispersions for very small wave vectors near k equals 0, where only parabolic <span class="hlt">energy</span> terms contribute to the dispersions. The results are consistent with the commonly used effective hole masses.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1410519-femtosecond-mev-electron-energy-loss-spectroscopy','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1410519-femtosecond-mev-electron-energy-loss-spectroscopy"><span>Femtosecond MeV <span class="hlt">Electron</span> <span class="hlt">Energy</span>-Loss Spectroscopy</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Li, R. K.; Wang, X. J.</p> <p>2017-11-09</p> <p>Pump-probe <span class="hlt">electron</span> <span class="hlt">energy</span>-loss spectroscopy (EELS) with femtosecond temporal resolution will be a transformative research tool for studying nonequilibrium chemistry and <span class="hlt">electronic</span> dynamics of matter. Here in this article, we propose a concept of femtosecond EELS utilizing mega-<span class="hlt">electron</span>-volt <span class="hlt">electron</span> beams from a radio-frequency (rf) photocathode source. The high acceleration gradient and high beam <span class="hlt">energy</span> of the rf gun are critical to the generation of 10-fs <span class="hlt">electron</span> beams, which enables an improvement of the temporal resolution by more than 1 order of magnitude beyond the state of the art. In our proposal, the “referencebeam technique” relaxes the <span class="hlt">energy</span> stability requirement of themore » rf power source by roughly 2 orders of magnitude. The requirements for the <span class="hlt">electron</span>-beam quality, photocathode, spectrometer, and detector are also discussed. Supported by particle-tracking simulations, we demonstrate the feasibility of achieving subelectron- volt <span class="hlt">energy</span> resolution and approximately 10-fs temporal resolution with existing or near-future hardware performance.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1410519-femtosecond-mev-electron-energy-loss-spectroscopy','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1410519-femtosecond-mev-electron-energy-loss-spectroscopy"><span>Femtosecond MeV <span class="hlt">Electron</span> <span class="hlt">Energy</span>-Loss Spectroscopy</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Li, R. K.; Wang, X. J.</p> <p></p> <p>Pump-probe <span class="hlt">electron</span> <span class="hlt">energy</span>-loss spectroscopy (EELS) with femtosecond temporal resolution will be a transformative research tool for studying nonequilibrium chemistry and <span class="hlt">electronic</span> dynamics of matter. Here in this article, we propose a concept of femtosecond EELS utilizing mega-<span class="hlt">electron</span>-volt <span class="hlt">electron</span> beams from a radio-frequency (rf) photocathode source. The high acceleration gradient and high beam <span class="hlt">energy</span> of the rf gun are critical to the generation of 10-fs <span class="hlt">electron</span> beams, which enables an improvement of the temporal resolution by more than 1 order of magnitude beyond the state of the art. In our proposal, the “referencebeam technique” relaxes the <span class="hlt">energy</span> stability requirement of themore » rf power source by roughly 2 orders of magnitude. The requirements for the <span class="hlt">electron</span>-beam quality, photocathode, spectrometer, and detector are also discussed. Supported by particle-tracking simulations, we demonstrate the feasibility of achieving subelectron- volt <span class="hlt">energy</span> resolution and approximately 10-fs temporal resolution with existing or near-future hardware performance.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23635138','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23635138"><span>High-resolution <span class="hlt">electron</span> spectroscopy of lanthanide (Ce, Pr, and Nd) complexes of cyclooctatetraene: the role of 4f <span class="hlt">electrons</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kumari, Sudesh; Roudjane, Mourad; Hewage, Dilrukshi; Liu, Yang; Yang, Dong-Sheng</p> <p>2013-04-28</p> <p>Cerium, praseodymium, and neodymium complexes of 1,3,5,7-cyclooctatetraene (COT) complexes were produced in a laser-vaporization metal cluster source and studied by pulsed-field ionization zero <span class="hlt">electron</span> kinetic <span class="hlt">energy</span> spectroscopy and quantum chemical calculations. The computations included the second-order Møller-Plesset perturbation theory, the coupled cluster method with single, double, and perturbative triple excitations, and the state-average complete active space self-consistent field method. The spectrum of each complex exhibits multiple <span class="hlt">band</span> systems and is assigned to ionization of several low-<span class="hlt">energy</span> <span class="hlt">electronic</span> states of the neutral complex. This observation is different from previous studies of M(COT) (M = Sc, Y, La, and Gd), for which a single <span class="hlt">band</span> system was observed. The presence of the multiple low-<span class="hlt">energy</span> <span class="hlt">electronic</span> states is caused by the splitting of the partially filled lanthanide 4f orbitals in the ligand field, and the number of the low-<span class="hlt">energy</span> states increases rapidly with increasing number of the metal 4f <span class="hlt">electrons</span>. On the other hand, the 4f <span class="hlt">electrons</span> have a small effect on the geometries and vibrational frequencies of these lanthanide complexes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22573976-first-principles-energy-band-calculation-ruddlesdenpopper-compound-sr-sub-sn-sub-sub-using-modified-beckejohnson-exchange-potential','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22573976-first-principles-energy-band-calculation-ruddlesdenpopper-compound-sr-sub-sn-sub-sub-using-modified-beckejohnson-exchange-potential"><span>First-principles <span class="hlt">energy</span> <span class="hlt">band</span> calculation of Ruddlesden–Popper compound Sr{sub 3}Sn{sub 2}O{sub 7} using modified Becke–Johnson exchange potential</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Kamimura, Sunao, E-mail: kamimura-sunao@che.kyutech.ac.jp; National Institute of Advanced Industrial Science and Technology; Department of Molecular and Material Sciences, Interdisciplinary Graduate School of Engineering Science, Kyushu University, 6-1 Kasuga Kouen, Kasuga, Fukuoka 816-8580 Japan</p> <p></p> <p>The <span class="hlt">electronic</span> structure of Sr{sub 3}Sn{sub 2}O{sub 7} is evaluated by the scalar-relativistic full potential linearized augmented plane wave (FLAPW+lo) method using the modified Becke–Johnson potential (Tran–Blaha potential) combined with the local density approximation correlation (MBJ–LDA). The fundamental gap between the valence <span class="hlt">band</span> (VB) and conduction <span class="hlt">band</span> (CB) is estimated to be 3.96 eV, which is close to the experimental value. Sn 5s states and Sr 4d states are predominant in the lower and upper CB, respectively. On the other hand, the lower VB is mainly composed of Sn 5s, 5p, and O 2p states, while the upper VB mainlymore » consists of O 2p states. These features of the DOS are well reflected by the optical transition between the upper VB and lower CB, as seen in the <span class="hlt">energy</span> dependence of the dielectric function. Furthermore, the absorption coefficient estimated from the MBJ–LDA is similar to the experimental result. - Graphical abstract: Calculated <span class="hlt">energy</span> <span class="hlt">band</span> structure along the symmetry lines of the first BZ of Sr{sub 3}Sn{sub 2}O{sub 7} crystal obtained using the MBJ potential. - Highlights: • <span class="hlt">Electronic</span> structure of Sr{sub 3}Sn{sub 2}O{sub 7} is calculated on the basis of MBJ–LDA method for the first time. • <span class="hlt">Band</span> gap of Sr{sub 3}Sn{sub 2}O{sub 7} is determined accurately on the basis of MBJ–LDA method. • The experimental absorption spectrum of Sr{sub 3}Sn{sub 2}O{sub 7} produced by MBJ–LDA is more accurate than that obtained by GGA method.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21544143','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21544143"><span>Convergence of <span class="hlt">electronic</span> <span class="hlt">bands</span> for high performance bulk thermoelectrics.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pei, Yanzhong; Shi, Xiaoya; LaLonde, Aaron; Wang, Heng; Chen, Lidong; Snyder, G Jeffrey</p> <p>2011-05-05</p> <p>Thermoelectric generators, which directly convert heat into electricity, have long been relegated to use in space-based or other niche applications, but are now being actively considered for a variety of practical waste heat recovery systems-such as the conversion of car exhaust heat into electricity. Although these devices can be very reliable and compact, the thermoelectric materials themselves are relatively inefficient: to facilitate widespread application, it will be desirable to identify or develop materials that have an intensive thermoelectric materials figure of merit, zT, above 1.5 (ref. 1). Many different concepts have been used in the search for new materials with high thermoelectric efficiency, such as the use of nanostructuring to reduce phonon thermal conductivity, which has led to the investigation of a variety of complex material systems. In this vein, it is well known that a high valley degeneracy (typically ≤6 for known thermoelectrics) in the <span class="hlt">electronic</span> <span class="hlt">bands</span> is conducive to high zT, and this in turn has stimulated attempts to engineer such degeneracy by adopting low-dimensional nanostructures. Here we demonstrate that it is possible to direct the convergence of many valleys in a bulk material by tuning the doping and composition. By this route, we achieve a convergence of at least 12 valleys in doped PbTe(1-x)Se(x) alloys, leading to an extraordinary zT value of 1.8 at about 850 kelvin. <span class="hlt">Band</span> engineering to converge the valence (or conduction) <span class="hlt">bands</span> to achieve high valley degeneracy should be a general strategy in the search for and improvement of bulk thermoelectric materials, because it simultaneously leads to a high Seebeck coefficient and high electrical conductivity. ©2011 Macmillan Publishers Limited. All rights reserved</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008JPCM...20g5233E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008JPCM...20g5233E"><span>Determination of the optical <span class="hlt">band</span>-gap <span class="hlt">energy</span> of cubic and hexagonal boron nitride using luminescence excitation spectroscopy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Evans, D. A.; McGlynn, A. G.; Towlson, B. M.; Gunn, M.; Jones, D.; Jenkins, T. E.; Winter, R.; Poolton, N. R. J.</p> <p>2008-02-01</p> <p>Using synchrotron-based luminescence excitation spectroscopy in the <span class="hlt">energy</span> range 4-20 eV at 8 K, the indirect Γ-X optical <span class="hlt">band</span>-gap transition in cubic boron nitride is determined as 6.36 ± 0.03 eV, and the quasi-direct <span class="hlt">band</span>-gap <span class="hlt">energy</span> of hexagonal boron nitride is determined as 5.96 ± 0.04 eV. The composition and structure of the materials are self-consistently established by optically detected x-ray absorption spectroscopy, and both x-ray diffraction and Raman measurements on the same samples give independent confirmation of their chemical and structural purity: together, the results are therefore considered as providing definitive measurements of the optical <span class="hlt">band</span>-gap <span class="hlt">energies</span> of the two materials.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26698057','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26698057"><span>Application of mid-infrared free-<span class="hlt">electron</span> laser tuned to amide <span class="hlt">bands</span> for dissociation of aggregate structure of protein.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kawasaki, Takayasu; Yaji, Toyonari; Ohta, Toshiaki; Tsukiyama, Koichi</p> <p>2016-01-01</p> <p>A mid-infrared free-<span class="hlt">electron</span> laser (FEL) is a linearly polarized, high-peak powered pulse laser with tunable wavelength within the mid-infrared absorption region. It was recently found that pathogenic amyloid fibrils could be partially dissociated to the monomer form by the irradiation of the FEL targeting the amide I <span class="hlt">band</span> (C=O stretching vibration), amide II <span class="hlt">band</span> (N-H bending vibration) and amide III <span class="hlt">band</span> (C-N stretching vibration). In this study, the irradiation effect of the FEL on keratin aggregate was tested as another model to demonstrate an applicability of the FEL for dissociation of protein aggregates. Synchrotron radiation infrared microscopy analysis showed that the α-helix content in the aggregate structure decreased to almost the same level as that in the monomer state after FEL irradiation tuned to 6.06 µm (amide I <span class="hlt">band</span>). Both irradiations at 6.51 µm (amide II <span class="hlt">band</span>) and 8.06 µm (amide III <span class="hlt">band</span>) also decreased the content of the aggregate but to a lesser extent than for the irradiation at the amide I <span class="hlt">band</span>. On the contrary, the irradiation tuned to 5.6 µm (non-absorbance region) changed little the secondary structure of the aggregate. Scanning-<span class="hlt">electron</span> microscopy observation at the submicrometer order showed that the angular solid of the aggregate was converted to non-ordered fragments by the irradiation at each amide <span class="hlt">band</span>, while the aggregate was hardly deformed by the irradiation at 5.6 µm. These results demonstrate that the amide-specific irradiation by the FEL was effective for dissociation of the protein aggregate to the monomer form.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014ApPhL.105g2402Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014ApPhL.105g2402Y"><span>Ferromagnetism and the <span class="hlt">electronic</span> <span class="hlt">band</span> structure in (Ga,Mn)(Bi,As) epitaxial layers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yastrubchak, O.; Sadowski, J.; Gluba, L.; Domagala, J. Z.; Rawski, M.; Żuk, J.; Kulik, M.; Andrearczyk, T.; Wosinski, T.</p> <p>2014-08-01</p> <p>Impact of Bi incorporation into (Ga,Mn)As layers on their <span class="hlt">electronic</span>- and <span class="hlt">band</span>-structures as well as their magnetic and structural properties has been studied. Homogenous (Ga,Mn)(Bi,As) layers of high structural perfection have been grown by the low-temperature molecular-beam epitaxy technique. Post-growth annealing treatment of the layers results in an improvement of their structural and magnetic properties and an increase in the hole concentration in the layers. The modulation photoreflectance spectroscopy results are consistent with the valence-<span class="hlt">band</span> model of hole-mediated ferromagnetism in the layers. This material combines the properties of (Ga,Mn)As and Ga(Bi,As) ternary compounds and offers the possibility of tuning its electrical and magnetic properties by controlling the alloy composition.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28695740','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28695740"><span><span class="hlt">Electronic</span> Structure and <span class="hlt">Band</span> Alignment at the NiO and SrTiO3 p-n Heterojunctions.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhang, Kelvin H L; Wu, Rui; Tang, Fengzai; Li, Weiwei; Oropeza, Freddy E; Qiao, Liang; Lazarov, Vlado K; Du, Yingge; Payne, David J; MacManus-Driscoll, Judith L; Blamire, Mark G</p> <p>2017-08-09</p> <p>Understanding the energetics at the interface, including the alignment of valence and conduction <span class="hlt">bands</span>, built-in potentials, and ionic and <span class="hlt">electronic</span> reconstructions, is an important challenge in designing oxide interfaces that have controllable multifunctionalities for novel (opto-)<span class="hlt">electronic</span> devices. In this work, we report detailed investigations on the heterointerface of wide-<span class="hlt">band</span>-gap p-type NiO and n-type SrTiO 3 (STO). We show that despite a large lattice mismatch (∼7%) and dissimilar crystal structure, high-quality NiO and Li-doped NiO (LNO) thin films can be epitaxially grown on STO(001) substrates through a domain-matching epitaxy mechanism. X-ray photoelectron spectroscopy studies indicate that NiO/STO heterojunctions form a type II "staggered" <span class="hlt">band</span> alignment. In addition, a large built-in potential of up to 0.97 eV was observed at the interface of LNO and Nb-doped STO (NbSTO). The LNO/NbSTO p-n heterojunctions exhibit not only a large rectification ratio of 2 × 10 3 but also a large ideality factor of 4.3. The NiO/STO p-n heterojunctions have important implications for applications in photocatalysis and photodetectors as the interface provides favorable energetics for facile separation and transport of photogenerated <span class="hlt">electrons</span> and holes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhRvB..96t5206S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvB..96t5206S"><span>Simple vertex correction improves G W <span class="hlt">band</span> <span class="hlt">energies</span> of bulk and two-dimensional crystals</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schmidt, Per S.; Patrick, Christopher E.; Thygesen, Kristian S.</p> <p>2017-11-01</p> <p>The G W self-<span class="hlt">energy</span> method has long been recognized as the gold standard for quasiparticle (QP) calculations of solids in spite of the fact that the neglect of vertex corrections and the use of a density-functional theory starting point lack rigorous justification. In this work we remedy this situation by including a simple vertex correction that is consistent with a local-density approximation starting point. We analyze the effect of the self-<span class="hlt">energy</span> by splitting it into short-range and long-range terms which are shown to govern, respectively, the center and size of the <span class="hlt">band</span> gap. The vertex mainly improves the short-range correlations and therefore has a small effect on the <span class="hlt">band</span> gap, while it shifts the <span class="hlt">band</span> gap center up in <span class="hlt">energy</span> by around 0.5 eV, in good agreement with experiments. Our analysis also explains how the relative importance of short- and long-range interactions in structures of different dimensionality is reflected in their QP <span class="hlt">energies</span>. Inclusion of the vertex comes at practically no extra computational cost and even improves the basis set convergence compared to G W . Taken together, the method provides an efficient and rigorous improvement over the G W approximation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015APS..MARG24011H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015APS..MARG24011H"><span>Kohn-Sham <span class="hlt">Band</span> Structure Benchmark Including Spin-Orbit Coupling for 2D and 3D Solids</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huhn, William; Blum, Volker</p> <p>2015-03-01</p> <p>Accurate <span class="hlt">electronic</span> <span class="hlt">band</span> structures serve as a primary indicator of the suitability of a material for a given application, e.g., as <span class="hlt">electronic</span> or catalytic materials. Computed <span class="hlt">band</span> structures, however, are subject to a host of approximations, some of which are more obvious (e.g., the treatment of the exchange-correlation of self-<span class="hlt">energy</span>) and others less obvious (e.g., the treatment of core, semicore, or valence <span class="hlt">electrons</span>, handling of relativistic effects, or the accuracy of the underlying basis set used). We here provide a set of accurate Kohn-Sham <span class="hlt">band</span> structure benchmarks, using the numeric atom-centered all-<span class="hlt">electron</span> <span class="hlt">electronic</span> structure code FHI-aims combined with the ``traditional'' PBE functional and the hybrid HSE functional, to calculate core, valence, and low-lying conduction <span class="hlt">bands</span> of a set of 2D and 3D materials. Benchmarks are provided with and without effects of spin-orbit coupling, using quasi-degenerate perturbation theory to predict spin-orbit splittings. This work is funded by Fritz-Haber-Institut der Max-Planck-Gesellschaft.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011JAP...110l3702P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011JAP...110l3702P"><span>Transition temperature from <span class="hlt">band</span> to hopping direct current conduction in crystalline semiconductors with hydrogen-like impurities: Heat versus Coulomb attraction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Poklonski, N. A.; Vyrko, S. A.; Poklonskaya, O. N.; Zabrodskii, A. G.</p> <p>2011-12-01</p> <p>For nondegenerate bulk semiconductors, we have used the virial theorem to derive an expression for the temperature Tj of the transition from the regime of "free" motion of <span class="hlt">electrons</span> in the c-<span class="hlt">band</span> (or holes in the υ-<span class="hlt">band</span>) to their hopping motion between donors (or acceptors). Distribution of impurities over the crystal was assumed to be of the Poisson type, while distribution of their <span class="hlt">energy</span> levels was assumed to be of the Gaussian type. Our conception of the virial theorem implementation is that the transition from the <span class="hlt">band</span>-like conduction to hopping conduction occurs when the average kinetic <span class="hlt">energy</span> of an <span class="hlt">electron</span> in the c-<span class="hlt">band</span> (hole in the υ-<span class="hlt">band</span>) is equal to the half of the absolute value of the average <span class="hlt">energy</span> of the Coulomb interaction of an <span class="hlt">electron</span> (hole) with the nearest neighbor ionized donor (acceptor). Calculations of Tj according to our model agree with experimental data for crystals of Ge, Si, diamond, etc. up to the concentrations of a hydrogen-like impurity, at which the phase insulator-metal transition (Mott transition) occurs. Under the temperature Th ≈ Tj /3, when the nearest neighbor hopping conduction via impurity atoms dominates, we obtained expressions for the electrostatic field screening length Λh in the Debye-Hückel approximation, taking into account a nonzero width of the impurity <span class="hlt">energy</span> <span class="hlt">band</span>. It is shown that the measurements of quasistatic capacitance of the semiconductor in a metal-insulator-semiconductor structure in the regime of the flat <span class="hlt">bands</span> at the temperature Th allow to determine the concentration of doping impurity or its compensation ratio by knowing Λh.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19800059462&hterms=high+current+electron+beam&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dhigh%2Bcurrent%2Belectron%2Bbeam','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19800059462&hterms=high+current+electron+beam&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dhigh%2Bcurrent%2Belectron%2Bbeam"><span><span class="hlt">Electron</span> <span class="hlt">energy</span> distributions measured during <span class="hlt">electron</span> beam/plasma interactions. [in E region</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jost, R. J.; Anderson, H. R.; Mcgarity, J. O.</p> <p>1980-01-01</p> <p>In the large vacuum facility at the NASA-Johnson Space Center an <span class="hlt">electron</span> beam was projected 20 m parallel to B from a gun with variable accelerating potential (1.0 to 2.5 kV) to an aluminum target. The ionospheric neutral pressure and field were approximated. Beam <span class="hlt">electron</span> <span class="hlt">energy</span> distributions were measured directly using an electrostatic deflection analyzer and indirectly with a detector that responded to the X-rays produced by <span class="hlt">electron</span> impact on the target. At low currents the distribution is sharply peaked at the acceleration potential. At high currents a beam plasma discharge occurs and <span class="hlt">electrons</span> are redistributed in <span class="hlt">energy</span> so that the former <span class="hlt">energy</span> peak broadens to 10-15 percent FWHM with a strongly enhanced low <span class="hlt">energy</span> tail. At the 10% of maximum point the <span class="hlt">energy</span> spectrum ranges from less than 1/2 to 1.2 times the gun <span class="hlt">energy</span>. The effect is qualitatively the same at all pitch angles and locations sampled.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4513282','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4513282"><span>Quasiparticle self-consistent GW study of cuprates: <span class="hlt">electronic</span> structure, model parameters, and the two-<span class="hlt">band</span> theory for Tc</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Jang, Seung Woo; Kotani, Takao; Kino, Hiori; Kuroki, Kazuhiko; Han, Myung Joon</p> <p>2015-01-01</p> <p>Despite decades of progress, an understanding of unconventional superconductivity still remains elusive. An important open question is about the material dependence of the superconducting properties. Using the quasiparticle self-consistent GW method, we re-examine the <span class="hlt">electronic</span> structure of copper oxide high-Tc materials. We show that QSGW captures several important features, distinctive from the conventional LDA results. The <span class="hlt">energy</span> level splitting between and is significantly enlarged and the van Hove singularity point is lowered. The calculated results compare better than LDA with recent experimental results from resonant inelastic xray scattering and angle resolved photoemission experiments. This agreement with the experiments supports the previously suggested two-<span class="hlt">band</span> theory for the material dependence of the superconducting transition temperature, Tc. PMID:26206417</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_20 --> <div id="page_21" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="401"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhRvB..96g5433D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvB..96g5433D"><span>Ab initio study of the <span class="hlt">electron</span> <span class="hlt">energy</span> loss function in a graphene-sapphire-graphene composite system</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Despoja, Vito; Djordjević, Tijana; Karbunar, Lazar; Radović, Ivan; Mišković, Zoran L.</p> <p>2017-08-01</p> <p>The propagator of a dynamically screened Coulomb interaction W in a sandwichlike structure consisting of two graphene layers separated by a slab of Al2O3 (or vacuum) is derived from single-layer graphene response functions and by using a local dielectric function for the bulk Al2O3 . The response function of graphene is obtained using two approaches within the random phase approximation (RPA): an ab initio method that includes all <span class="hlt">electronic</span> <span class="hlt">bands</span> in graphene and a computationally less demanding method based on the massless Dirac fermion (MDF) approximation for the low-<span class="hlt">energy</span> excitations of <span class="hlt">electrons</span> in the π <span class="hlt">bands</span>. The propagator W is used to derive an expression for the effective dielectric function of our sandwich structure, which is relevant for the reflection <span class="hlt">electron</span> <span class="hlt">energy</span> loss spectroscopy of its surface. Focusing on the range of frequencies from THz to mid-infrared, special attention is paid to finding an accurate optical limit in the ab initio method, where the response function is expressed in terms of a frequency-dependent conductivity of graphene. It was shown that the optical limit suffices for describing hybridization between the Dirac plasmons in graphene layers and the Fuchs-Kliewer phonons in both surfaces of the Al2O3 slab, and that the spectra obtained from both the ab initio method and the MDF approximation in the optical limit agree perfectly well for wave numbers up to about 0.1 nm-1. Going beyond the optical limit, the agreement between the full ab initio method and the MDF approximation was found to extend to wave numbers up to about 0.3 nm-1 for doped graphene layers with the Fermi <span class="hlt">energy</span> of 0.2 eV.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4202206','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4202206"><span>Layer-dependent <span class="hlt">Band</span> Alignment and Work Function of Few-Layer Phosphorene</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Cai, Yongqing; Zhang, Gang; Zhang, Yong-Wei</p> <p>2014-01-01</p> <p>Using first-principles calculations, we study the <span class="hlt">electronic</span> properties of few-layer phosphorene focusing on layer-dependent behavior of <span class="hlt">band</span> gap, work function <span class="hlt">band</span> alignment and carrier effective mass. It is found that few-layer phosphorene shows a robust direct <span class="hlt">band</span> gap character, and its <span class="hlt">band</span> gap decreases with the number of layers following a power law. The work function decreases rapidly from monolayer (5.16 eV) to trilayer (4.56 eV), and then slowly upon further increasing the layer number. Compared to monolayer phosphorene, there is a drastic decrease of hole effective mass along the ridge (zigzag) direction for bilayer phosphorene, indicating a strong interlayer coupling and screening effect. Our study suggests that 1). Few-layer phosphorene with a layer-dependent <span class="hlt">band</span> gap and a robust direct <span class="hlt">band</span> gap character is promising for efficient solar <span class="hlt">energy</span> harvest. 2). Few-layer phosphorene outperforms monolayer counterpart in terms of a lighter carrier effective mass, a higher carrier density and a weaker scattering due to enhanced screening. 3). The layer-dependent <span class="hlt">band</span> edges and work functions of few-layer phosphorene allow for modification of Schottky barrier with enhanced carrier injection efficiency. It is expected that few-layer phosphorene will present abundant opportunities for a plethora of new <span class="hlt">electronic</span> applications. PMID:25327586</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvB..97l5121M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvB..97l5121M"><span>Interplay of Coulomb interactions and disorder in three-dimensional quadratic <span class="hlt">band</span> crossings without time-reversal symmetry and with unequal masses for conduction and valence <span class="hlt">bands</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mandal, Ipsita; Nandkishore, Rahul M.</p> <p>2018-03-01</p> <p>Coulomb interactions famously drive three-dimensional quadratic <span class="hlt">band</span> crossing semimetals into a non-Fermi liquid phase of matter. In a previous work [Nandkishore and Parameswaran, Phys. Rev. B 95, 205106 (2017), 10.1103/PhysRevB.95.205106], the effect of disorder on this non-Fermi liquid phase was investigated, assuming that the <span class="hlt">band</span> structure was isotropic, assuming that the conduction and valence <span class="hlt">bands</span> had the same <span class="hlt">band</span> mass, and assuming that the disorder preserved exact time-reversal symmetry and statistical isotropy. It was shown that the non-Fermi liquid fixed point is unstable to disorder and that a runaway flow to strong disorder occurs. In this paper, we extend that analysis by relaxing the assumption of time-reversal symmetry and allowing the <span class="hlt">electron</span> and hole masses to differ (but continuing to assume isotropy of the low <span class="hlt">energy</span> <span class="hlt">band</span> structure). We first incorporate time-reversal symmetry breaking disorder and demonstrate that there do not appear any new fixed points. Moreover, while the system continues to flow to strong disorder, time-reversal-symmetry-breaking disorder grows asymptotically more slowly than time-reversal-symmetry-preserving disorder, which we therefore expect should dominate the strong-coupling phase. We then allow for unequal <span class="hlt">electron</span> and hole masses. We show that whereas asymmetry in the two masses is irrelevant in the clean system, it is relevant in the presence of disorder, such that the `effective masses' of the conduction and valence <span class="hlt">bands</span> should become sharply distinct in the low-<span class="hlt">energy</span> limit. We calculate the RG flow equations for the disordered interacting system with unequal <span class="hlt">band</span> masses and demonstrate that the problem exhibits a runaway flow to strong disorder. Along the runaway flow, time-reversal-symmetry-preserving disorder grows asymptotically more rapidly than both time-reversal-symmetry-breaking disorder and the Coulomb interaction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/865752','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/865752"><span>Broad-<span class="hlt">band</span> beam buncher</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Goldberg, David A.; Flood, William S.; Arthur, Allan A.; Voelker, Ferdinand</p> <p>1986-01-01</p> <p>A broad-<span class="hlt">band</span> beam buncher is disclosed, comprising an evacuated housing, an <span class="hlt">electron</span> gun therein for producing an <span class="hlt">electron</span> beam, a buncher cavity having entrance and exit openings through which the beam is directed, grids across such openings, a source providing a positive DC voltage between the cavity and the <span class="hlt">electron</span> gun, a drift tube through which the <span class="hlt">electron</span> beam travels in passing through such cavity, grids across the ends of such drift tube, gaps being provided between the drift tube grids and the entrance and exit grids, a modulator for supplying an ultrahigh frequency modulating signal to the drift tube for producing velocity modulation of the <span class="hlt">electrons</span> in the beam, a drift space in the housing through which the velocity modulated <span class="hlt">electron</span> beam travels and in which the beam is bunched, and a discharge opening from such drift tube and having a grid across such opening through which the bunched <span class="hlt">electron</span> beam is discharged into an accelerator or the like. The buncher cavity and the drift tube may be arranged to constitute an extension of a coaxial transmission line which is employed to deliver the modulating signal from a signal source. The extended transmission line may be terminated in its characteristic impedance to afford a broad-<span class="hlt">band</span> response and the device as a whole designed to effect broad-<span class="hlt">band</span> beam coupling, so as to minimize variations of the output across the response <span class="hlt">band</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JEMat..47.3277P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JEMat..47.3277P"><span><span class="hlt">Electronic</span> Structure and Thermoelectric Properties of Transition Metal Monosilicides</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pshenay-Severin, D. A.; Ivanov, Yu. V.; Burkov, A. T.; Novikov, S. V.; Zaitsev, V. K.; Reith, H.</p> <p>2018-06-01</p> <p>We present theoretical and experimental results on <span class="hlt">electronic</span> structure and thermoelectric properties of cobalt monosilicide (CoSi) and of Co1- x M x Si diluted alloys (M = Fe and Ni) at temperatures from 2 K to 800 K. CoSi crystallizes into a non-centrosymmetric cubic B20 structure, which suggests the possibility of a topologically non-trivial <span class="hlt">electronic</span> structure. We show that the <span class="hlt">electronic</span> structure of CoSi exhibits linear <span class="hlt">band</span> crossings in close vicinity to Fermi <span class="hlt">energy</span>, confirming the possibility of non-trivial topology. The proximity of the linear-dispersion <span class="hlt">bands</span> to Fermi <span class="hlt">energy</span> implies their important contribution to the <span class="hlt">electronic</span> transport. Calculation of thermopower of CoSi, using ab initio <span class="hlt">band</span> structure and the constant relaxation time approximation, is carried out. It reveals that many body corrections to the <span class="hlt">electronic</span> spectrum are important in order to obtain qualitative agreement of theoretical and experimental temperature dependences of thermopower. Phonon dispersion and lattice thermal conductivity are calculated. The phonons give a major contribution to the thermal conductivity of the compound below room temperature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011APS..MARP37005K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011APS..MARP37005K"><span>Spectromicroscopy measurements of surface morphology and <span class="hlt">band</span> structure of exfoliated graphene</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Knox, Kevin; Locatelli, Andrea; Cvetko, Dean; Mentes, Tevfik; Nino, Miguel; Wang, Shancai; Yilmaz, Mehmet; Kim, Philip; Osgood, Richard; Morgante, Alberto</p> <p>2011-03-01</p> <p>Monolayer-thick crystals, such as graphene, are an area of intense interest in condensed matter research. ~However, crystal deformations in these 2D systems are known to adversely affect conductivity and increase local chemical reactivity. Additionally, surface roughness in graphene complicates <span class="hlt">band</span>-mapping and limits resolution in techniques such as angle resolved photoemission spectroscopy (ARPES), the theory of which was developed for atomically flat surfaces. Thus, an understanding of the surface morphology of graphene is essential to making high quality devices and important for interpreting ARPES results. In this talk, we will describe a non-invasive approach to examining the corrugation in exfoliated graphene using a combination of low <span class="hlt">energy</span> <span class="hlt">electron</span> microscopy (LEEM) and micro-spot low <span class="hlt">energy</span> <span class="hlt">electron</span> diffraction (LEED). We will also describe how such knowledge of surface roughness can be used in the analysis of ARPES data to improve resolution and extract useful information about the <span class="hlt">band</span>-structure.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhPl...24l3104Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhPl...24l3104Z"><span>Characteristics of a KA-<span class="hlt">band</span> third-harmonic peniotron driven by a high-quality linear axis-encircling <span class="hlt">electron</span> beam</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhao, Xiaoyun; Tuo, Xianguo; Ge, Qing; Peng, Ying</p> <p>2017-12-01</p> <p>We employ a high-quality linear axis-encircling <span class="hlt">electron</span> beam generated by a Cuccia coupler to drive a Ka-<span class="hlt">band</span> third-harmonic peniotron and develop a self-consistent nonlinear calculation code to numerically analyze the characteristics of the designed peniotron. It is demonstrated that through a Cuccia coupler, a 6 kV, 0.5 A pencil beam and an input microwave power of 16 kW at 10 GHz can generate a 37 kV, 0.5 A linear axis-encircling beam, and it is characterized by a very low velocity spread. Moreover, the <span class="hlt">electron</span> beam guiding center deviation can be adjusted easily. Driven by such a beam, a 30 GHz, Ka-<span class="hlt">band</span> third-harmonic peniotron is predicted to achieve a conversion efficiency of 51.0% and a microwave output power of 9.44 kW; the results are in good agreement with the Magic3D simulation. Using this code, we studied the factors influencing the peniotron performance, and it can provide some guidelines for the design of a Ka-<span class="hlt">band</span> third-harmonic peniotron driven by a linear <span class="hlt">electron</span> beam and can promote the application of high-harmonic peniotrons in practice.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012OptSp.113....5C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012OptSp.113....5C"><span>Excitation of lowest <span class="hlt">electronic</span> states of the uracil molecule by slow <span class="hlt">electrons</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chernyshova, I. V.; Kontros, J. E.; Markush, P. P.; Shpenik, O. B.</p> <p>2012-07-01</p> <p>The excitation of lowest <span class="hlt">electronic</span> states of the uracil molecule in the gas phase has been studied by <span class="hlt">electron</span> <span class="hlt">energy</span> loss spectroscopy. Along with excitation of lowest singlet states, excitation of two lowest triplet states at 3.75 and 4.76 eV (±0.05 eV) and vibrational excitation of the molecule in two resonant ranges (1-2 and 3-4 eV) have been observed for the first time. The peak of the excitation <span class="hlt">band</span> related to the lowest singlet state (5.50 eV) is found to be blueshifted by 0.4 eV in comparison with the optical absorption spectroscopy data. The threshold excitation spectra have been measured for the first time, with detection of <span class="hlt">electrons</span> inelastically scattered by an angle of 180°. These spectra exhibit clear separation of the 5.50-eV-wide <span class="hlt">band</span> into two <span class="hlt">bands</span>, which are due to the excitation of the triplet 13 A″ and singlet 11 A' states.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18729418','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18729418"><span>Carrier multiplication in semiconductor nanocrystals: theoretical screening of candidate materials based on <span class="hlt">band</span>-structure effects.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Luo, Jun-Wei; Franceschetti, Alberto; Zunger, Alex</p> <p>2008-10-01</p> <p>Direct carrier multiplication (DCM) occurs when a highly excited <span class="hlt">electron</span>-hole pair decays by transferring its excess <span class="hlt">energy</span> to the <span class="hlt">electrons</span> rather than to the lattice, possibly exciting additional <span class="hlt">electron</span>-hole pairs. Atomistic <span class="hlt">electronic</span> structure calculations have shown that DCM can be induced by <span class="hlt">electron</span>-hole Coulomb interactions, in an impact-ionization-like process whose rate is proportional to the density of biexciton states rho XX. Here we introduce a DCM "figure of merit" R2(E) which is proportional to the ratio between the biexciton density of states rhoXX and the single-exciton density of states rhoX, restricted to single-exciton and biexciton states that are coupled by Coulomb interactions. Using R2(E), we consider GaAs, InAs, InP, GaSb, InSb, CdSe, Ge, Si, and PbSe nanocrystals of different sizes. Although DCM can be affected by both quantum-confinement effects (reflecting the underly <span class="hlt">electronic</span> structure of the confined dot-interior states) and surface effects, here we are interested to isolate the former. To this end the nanocrystal <span class="hlt">energy</span> levels are obtained from the corresponding bulk <span class="hlt">band</span> structure via the truncated crystal approximation. We find that PbSe, Si, GaAs, CdSe, and InP nanocrystals have larger DCM figure of merit than the other nanocrystals. Our calculations suggest that high DCM efficiency requires high degeneracy of the corresponding bulk <span class="hlt">band</span>-edge states. Interestingly, by considering <span class="hlt">band</span> structure effects we find that as the dot size increases the DCM critical <span class="hlt">energy</span> E0 (the <span class="hlt">energy</span> at which R2(E) becomes >or=1) is reduced, suggesting improved DCM. However, whether the normalized E0/epsilong increases or decreases as the dot size increases depends on dot material.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvM...2c5801G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvM...2c5801G"><span>Spectroscopic investigation of the <span class="hlt">electronic</span> structure of yttria-stabilized zirconia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Götsch, Thomas; Bertel, Erminald; Menzel, Alexander; Stöger-Pollach, Michael; Penner, Simon</p> <p>2018-03-01</p> <p>The <span class="hlt">electronic</span> structure and optical properties of yttria-stabilized zirconia are investigated as a function of the yttria content using multiple experimental and theoretical methods, including <span class="hlt">electron</span> <span class="hlt">energy</span>-loss spectroscopy, Kramers-Kronig analysis to obtain the optical parameters, photoelectron spectroscopy, and density functional theory. It is shown that many properties, including the <span class="hlt">band</span> gaps, the crystal field splitting, the so-called defect gap between acceptor (YZr') and donor (VO••) states, as well as the index of refraction in the visible range exhibit the same "zig-zag-like" trend as the unit cell height does, showing the influence of an increased yttria content as well as of the tetragonal-cubic phase transition between 8 mol % and 20 mol %Y2O3 . Also, with Čerenkov spectroscopy (CS), a new technique is presented, providing information complementary to <span class="hlt">electron</span> <span class="hlt">energy</span>-loss spectroscopy. In CS, the Čerenkov radiation emitted inside the TEM is used to measure the onset of optical absorption. The apparent absorption edges in the Čerenkov spectra correspond to the energetic difference between the disorder states close to the valence <span class="hlt">band</span> and the oxygen-vacancy-related <span class="hlt">electronic</span> states within the <span class="hlt">band</span> gap. Theoretical computations corroborate this assignment: they find both, the acceptor states and the donor states, at the expected <span class="hlt">energies</span> in the <span class="hlt">band</span> structures for diverse yttria concentrations. In the end, a schematic <span class="hlt">electronic</span> structure diagram of the area around the <span class="hlt">band</span> gap is constructed, including the chemical potential of the <span class="hlt">electrons</span> obtained from photoelectron spectroscopy. The latter reveal that tetragonal YSZ corresponds to a p -type semiconductor, whereas the cubic samples exhibit n -type semiconductor properties.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1995PhRvB..52.8788S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1995PhRvB..52.8788S"><span>Bulk and surface <span class="hlt">electronic</span> structures of MgO</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schönberger, U.; Aryasetiawan, F.</p> <p>1995-09-01</p> <p>The bulk <span class="hlt">electronic</span> structure of MgO is calculated from first principles including correlation effects within the GW approximation. The <span class="hlt">band</span> gap, the position of the 2s O <span class="hlt">band</span>, and the valence <span class="hlt">band</span> width are in good agreement with experiment. From the quasiparticle <span class="hlt">band</span> structure, optical transitions corresponding to the main optical absorption peaks are identified. The <span class="hlt">energy</span>-loss spectrum is also calculated and compared with experiment. The surface <span class="hlt">electronic</span> structure of MgO(100) is calculated self-consistently within the local-density approximation. It is found that states observed in a recent photoemission experiment outside the bulk allowed states are close to surface states.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012JPhCS.400d2042M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012JPhCS.400d2042M"><span><span class="hlt">Electronic</span> structures of Plutonium compounds with the NaCl-type monochalcogenides structure</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Maehira, Takahiro; Tatetsu, Yasutomi</p> <p>2012-12-01</p> <p>We calculate the <span class="hlt">energy</span> <span class="hlt">band</span> structure and the Fermi surface of PuS, PuSe and PuTe by using a self-consistent relativistic linear augmented-plane-wave method with the exchange and correlation potential in a local density approximation. It is found in common that the <span class="hlt">energy</span> <span class="hlt">bands</span> in the vicinity of the Fermi level are mainly due to the hybridization between Pu 5/ and monochalcogenide p <span class="hlt">electrons</span>. The obtained main Fermi surfaces are composed of two hole sheets and one <span class="hlt">electron</span> sheet, all of which are constructed from the <span class="hlt">band</span> having the Pu 5/ state and the monochalcogenide p state.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4510960','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4510960"><span>Quantitative operando visualization of the <span class="hlt">energy</span> <span class="hlt">band</span> depth profile in solar cells</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Chen, Qi; Mao, Lin; Li, Yaowen; Kong, Tao; Wu, Na; Ma, Changqi; Bai, Sai; Jin, Yizheng; Wu, Dan; Lu, Wei; Wang, Bing; Chen, Liwei</p> <p>2015-01-01</p> <p>The <span class="hlt">energy</span> <span class="hlt">band</span> alignment in solar cell devices is critically important because it largely governs elementary photovoltaic processes, such as the generation, separation, transport, recombination and collection of charge carriers. Despite the expenditure of considerable effort, the measurement of <span class="hlt">energy</span> <span class="hlt">band</span> depth profiles across multiple layers has been extremely challenging, especially for operando devices. Here we present direct visualization of the surface potential depth profile over the cross-sections of operando organic photovoltaic devices using scanning Kelvin probe microscopy. The convolution effect due to finite tip size and cantilever beam crosstalk has previously prohibited quantitative interpretation of scanning Kelvin probe microscopy-measured surface potential depth profiles. We develop a bias voltage-compensation method to address this critical problem and obtain quantitatively accurate measurements of the open-circuit voltage, built-in potential and electrode potential difference. PMID:26166580</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PhRvB..93p5105H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhRvB..93p5105H"><span>Interpretation of monoclinic hafnia valence <span class="hlt">electron</span> <span class="hlt">energy</span>-loss spectra by time-dependent density functional theory</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hung, L.; Guedj, C.; Bernier, N.; Blaise, P.; Olevano, V.; Sottile, F.</p> <p>2016-04-01</p> <p>We present the valence <span class="hlt">electron</span> <span class="hlt">energy</span>-loss spectrum and the dielectric function of monoclinic hafnia (m -HfO2) obtained from time-dependent density-functional theory (TDDFT) predictions and compared to <span class="hlt">energy</span>-filtered spectroscopic imaging measurements in a high-resolution transmission-<span class="hlt">electron</span> microscope. Fermi's golden rule density-functional theory (DFT) calculations can capture the qualitative features of the <span class="hlt">energy</span>-loss spectrum, but we find that TDDFT, which accounts for local-field effects, provides nearly quantitative agreement with experiment. Using the DFT density of states and TDDFT dielectric functions, we characterize the excitations that result in the m -HfO2 <span class="hlt">energy</span>-loss spectrum. The sole plasmon occurs between 13 and 16 eV, although the peaks ˜28 and above 40 eV are also due to collective excitations. We furthermore elaborate on the first-principles techniques used, their accuracy, and remaining discrepancies among spectra. More specifically, we assess the influence of Hf semicore <span class="hlt">electrons</span> (5 p and 4 f ) on the <span class="hlt">energy</span>-loss spectrum, and find that the inclusion of transitions from the 4 f <span class="hlt">band</span> damps the <span class="hlt">energy</span>-loss intensity in the region above 13 eV. We study the impact of many-body effects in a DFT framework using the adiabatic local-density approximation (ALDA) exchange-correlation kernel, as well as from a many-body perspective using "scissors operators" matched to an ab initio G W calculation to account for self-<span class="hlt">energy</span> corrections. These results demonstrate some cancellation of errors between self-<span class="hlt">energy</span> and excitonic effects, even for excitations from the Hf 4 f shell. We also simulate the dispersion with increasing momentum transfer for plasmon and collective excitation peaks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017SeScT..32i5002C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017SeScT..32i5002C"><span>Effect of conduction <span class="hlt">band</span> non-parabolicity on the optical gain of quantum cascade lasers based on the effective two-<span class="hlt">band</span> finite difference method</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cho, Gookbin; Kim, Jungho</p> <p>2017-09-01</p> <p>We theoretically investigate the effect of conduction <span class="hlt">band</span> non-parabolicity (NPB) on the optical gain spectrum of quantum cascade lasers (QCLs) using the effective two-<span class="hlt">band</span> finite difference method. Based on the effective two-<span class="hlt">band</span> model to consider the NPB effect in the multiple quantum wells (QWs), the wave functions and confined <span class="hlt">energies</span> of <span class="hlt">electron</span> states are calculated in two different active-region structures, which correspond to three-QW single-phonon and four-QW double-phonon resonance designs. In addition, intersubband optical dipole moments and polar-optical-phonon scattering times are calculated and compared without and with the conduction <span class="hlt">band</span> NPB effect. Finally, the calculation results of optical gain spectra are compared in the two QCL structures having the same peak gain wavelength of 8.55 μm. The gain peaks are greatly shifted to longer wavelengths and the overall gain magnitudes are slightly reduced when the NPB effect is considered. Compared with the three-QW active-region design, the redshift of the peak gain is more prominent in the four-QW active-region design, which makes use of higher <span class="hlt">electronic</span> states for the lasing transition.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20020022486&hterms=selenium&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dselenium','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20020022486&hterms=selenium&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dselenium"><span><span class="hlt">Band</span> Anticrossing in Highly Mismatched Compound Semiconductor Alloys</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Yu, Kin Man; Wu, J.; Walukiewicz, W.; Ager, J. W.; Haller, E. E.; Miotkowski, I.; Su, Ching-Hua; Curreri, Peter A. (Technical Monitor)</p> <p>2001-01-01</p> <p>Compound semiconductor alloys in which metallic anions are partially replaced with more electronegative isoelectronic atoms have recently attracted significant attention. Group IIIN(sub x)V(sub 1-x) alloys with a small amount of the electronegative N substituting more metallic column V elements has been the most extensively studied class of such Highly Mismatched Alloys (HMAs). We have shown that many of the unusual properties of the IIIN(sub x)V(sub 1-x) alloys can be well explained by the <span class="hlt">Band</span> Anticrossing (BAC) model that describes the <span class="hlt">electronic</span> structure in terms of an interaction between highly localized levels of substitutional N and the extended states of the host semiconductor matrix. Most recently the BAC model has been also used to explain similar modifications of the <span class="hlt">electronic</span> <span class="hlt">band</span> structure observed in Te-rich ZnS(sub x)Te(sub 1-x) and ZnSe(sub y)Te(sub 1-y) alloys. To date studies of HMAs have been limited to materials with relatively small concentrations of highly electronegative atoms. Here we report investigations of the <span class="hlt">electronic</span> structure of ZnSe(sub y)Te(sub 1-y) alloys in the entire composition range, y between 0 and 1. The samples used in this study are bulk ZnSe(sub y)Te(sub 1-y) crystals grown by either a modified Bridgman method or by physical vapor transport. Photomodulated reflection (PR) spectroscopy was used to measure the composition dependence of optical transitions from the valence <span class="hlt">band</span> edge and from the spin-orbit split off <span class="hlt">band</span> to the conduction <span class="hlt">band</span>. The pressure dependence of the <span class="hlt">band</span> gap was measured using optical absorption in a diamond anvil cell. We find that the <span class="hlt">energy</span> of the spin-orbit split off valence <span class="hlt">band</span> edge does not depend on composition and is located at about 3 eV below the conduction <span class="hlt">band</span> edge of ZnSe. On the Te-rich side the pressure and the composition dependence of the optical transitions are well explained by the BAC model which describes the downward shift of the conduction <span class="hlt">band</span> edge in terms of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27701861','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27701861"><span>Photoemission of Energetic Hot <span class="hlt">Electrons</span> Produced via Up-Conversion in Doped Quantum Dots.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Dong, Yitong; Parobek, David; Rossi, Daniel; Son, Dong Hee</p> <p>2016-11-09</p> <p>The benefits of the hot <span class="hlt">electrons</span> from semiconductor nanostructures in photocatalysis or photovoltaics result from their higher <span class="hlt">energy</span> compared to that of the <span class="hlt">band</span>-edge <span class="hlt">electrons</span> facilitating the <span class="hlt">electron</span>-transfer process. The production of high-<span class="hlt">energy</span> hot <span class="hlt">electrons</span> usually requires short-wavelength UV or intense multiphoton visible excitation. Here, we show that highly energetic hot <span class="hlt">electrons</span> capable of above-threshold ionization are produced via exciton-to-hot-carrier up-conversion in Mn-doped quantum dots under weak <span class="hlt">band</span> gap excitation (∼10 W/cm 2 ) achievable with the concentrated solar radiation. The <span class="hlt">energy</span> of hot <span class="hlt">electrons</span> is as high as ∼0.4 eV above the vacuum level, much greater than those observed in other semiconductor or plasmonic metal nanostructures, which are capable of performing energetically and kinetically more-challenging <span class="hlt">electron</span> transfer. Furthermore, the prospect of generating solvated <span class="hlt">electron</span> is unique for the energetic hot <span class="hlt">electrons</span> from up-conversion, which can open a new door for long-range <span class="hlt">electron</span> transfer beyond short-range interfacial <span class="hlt">electron</span> transfer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018InJPh..92..303C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018InJPh..92..303C"><span>A note on anomalous <span class="hlt">band</span>-gap variations in semiconductors with temperature</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chakraborty, P. K.; Mondal, B. N.</p> <p>2018-03-01</p> <p>An attempt is made to theoretically study the <span class="hlt">band</span>-gap variations (ΔEg) in semiconductors with temperature following the works, did by Fan and O'Donnell et al. based on thermodynamic functions. The semiconductor <span class="hlt">band</span>-gap reflects the bonding <span class="hlt">energy</span>. An increase in temperature changes the chemical bondings, and <span class="hlt">electrons</span> are promoted from valence <span class="hlt">band</span> to conduction <span class="hlt">band</span>. In their analyses, they made several approximations with respect to temperature and other fitting parameters leading to real values of <span class="hlt">band</span>-gap variations with linear temperature dependences. In the present communication, we have tried to re-analyse the works, specially did by Fan, and derived an analytical model for ΔEg(T). Because, it was based on the second-order perturbation technique of thermodynamic functions. Our analyses are made without any approximations with respect to temperatures and other fitting parameters mentioned in the text, leading to a complex functions followed by an oscillating nature of the variations of ΔEg. In support of the existence of the oscillating <span class="hlt">energy</span> <span class="hlt">band</span>-gap variations with temperature in a semiconductor, possible physical explanations are provided to justify the experimental observation for various materials.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010SurSR..65....1A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010SurSR..65....1A"><span>Low-<span class="hlt">energy</span> <span class="hlt">electron</span>-induced reactions in condensed matter</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Arumainayagam, Christopher R.; Lee, Hsiao-Lu; Nelson, Rachel B.; Haines, David R.; Gunawardane, Richard P.</p> <p>2010-01-01</p> <p>The goal of this review is to discuss post-irradiation analysis of low-<span class="hlt">energy</span> (≤50 eV) <span class="hlt">electron</span>-induced processes in nanoscale thin films. Because <span class="hlt">electron</span>-induced surface reactions in monolayer adsorbates have been extensively reviewed, we will instead focus on low-<span class="hlt">energy</span> <span class="hlt">electron</span>-induced reactions in multilayer adsorbates. The latter studies, involving nanoscale thin films, serve to elucidate the pivotal role that the low-<span class="hlt">energy</span> <span class="hlt">electron</span>-induced reactions play in high-<span class="hlt">energy</span> radiation-induced chemical reactions in condensed matter. Although <span class="hlt">electron</span>-stimulated desorption (ESD) experiments conducted during irradiation have yielded vital information relevant to primary or initial <span class="hlt">electron</span>-induced processes, we wish to demonstrate in this review that analyzing the products following low-<span class="hlt">energy</span> <span class="hlt">electron</span> irradiation can provide new insights into radiation chemistry. This review presents studies of <span class="hlt">electron</span>-induced reactions in nanoscale films of molecular species such as oxygen, nitrogen trifluoride, water, alkanes, alcohols, aldehydes, ketones, carboxylic acids, nitriles, halocarbons, alkane and phenyl thiols, thiophenes, ferrocene, amino acids, nucleotides, and DNA using post-irradiation techniques such as temperature-programmed desorption (TPD), reflection-absorption infrared spectroscopy (RAIRS), X-ray photoelectron spectroscopy (XPS), high-resolution <span class="hlt">electron</span> <span class="hlt">energy</span> loss spectroscopy (HREELS), gel electrophoresis, and microarray fluorescence. Post-irradiation temperature-programmed desorption, in particular, has been shown to be useful in identifying labile radiolysis products as demonstrated by the first identification of methoxymethanol as a reaction product of methanol radiolysis. Results of post-irradiation studies have been used not only to identify radiolysis products, but also to determine the dynamics of <span class="hlt">electron</span>-induced reactions. For example, studies of the radiolysis yield as a function of incident <span class="hlt">electron</span> <span class="hlt">energy</span> have shown that dissociative</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhyB..530...53D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhyB..530...53D"><span>Tuning of <span class="hlt">electronic</span> <span class="hlt">band</span> gaps and optoelectronic properties of binary strontium chalcogenides by means of doping of magnesium atom(s)- a first principles based theoretical initiative with mBJ, B3LYP and WC-GGA functionals</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Debnath, Bimal; Sarkar, Utpal; Debbarma, Manish; Bhattacharjee, Rahul; Chattopadhyaya, Surya</p> <p>2018-02-01</p> <p>First principle based theoretical initiative is taken to tune the optoelectronic properties of binary strontium chalcogenide semiconductors by doping magnesium atom(s) into their rock-salt unit cells at specific concentrations x = 0.0, 0.25, 0.50, 0.75 and 1.0 and such tuning is established by studying structural, <span class="hlt">electronic</span> and optical properties of designed binary compounds and ternary alloys employing WC-GGA, B3LYP and mBJ exchange-correlation functionals. <span class="hlt">Band</span> structure of each compound is constructed and respective <span class="hlt">band</span> gaps under all the potential schemes are measured. The <span class="hlt">band</span> gap bowing and its microscopic origin are calculated using quadratic fit and Zunger's approach, respectively. The atomic and orbital origins of <span class="hlt">electronic</span> states in the <span class="hlt">band</span> structure of any compound are explored from its density of states. The nature of chemical bonds between the constituent atoms in each compound is explored from the valence <span class="hlt">electron</span> density contour plots. Optical properties of any specimen are explored from the computed spectra of its dielectric function, refractive index, extinction coefficient, normal incidence reflectivity, optical conductivity optical absorption and <span class="hlt">energy</span> loss function. Several calculated results are compared with available experimental and earlier theoretical data.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_21 --> <div id="page_22" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="421"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20020024134&hterms=CERN&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DCERN','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20020024134&hterms=CERN&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DCERN"><span>High <span class="hlt">Energy</span> <span class="hlt">Electron</span> Detection with ATIC</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chang, J.; Schmidt, W. K. H.; Adams, James H., Jr.; Ahn, H.; Ampe, J.; Whitaker, Ann F. (Technical Monitor)</p> <p>2001-01-01</p> <p>The ATIC (Advanced Thin Ionization Calorimeter) balloon-borne ionization calorimeter is well suited to record and identify high <span class="hlt">energy</span> cosmic ray <span class="hlt">electrons</span>. The instrument was exposed to high-<span class="hlt">energy</span> beams at CERN H2 bean-dine in September of 1999. We have simulated the performance of the instrument, and compare the simulations with actual high <span class="hlt">energy</span> <span class="hlt">electron</span> exposures at the CERN accelerator. Simulations and measurements do not compare exactly, in detail, but overall the simulations have predicted actual measured behavior quite well.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018Nanot..29s4002A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018Nanot..29s4002A"><span>Ultraviolet photoelectron spectroscopy reveals <span class="hlt">energy-band</span> dispersion for π-stacked 7,8,15,16-tetraazaterrylene thin films in a donor–acceptor bulk heterojunction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Aghdassi, Nabi; Wang, Qi; Ji, Ru-Ru; Wang, Bin; Fan, Jian; Duhm, Steffen</p> <p>2018-05-01</p> <p>7,8,15,16-tetraazaterrylene (TAT) thin films grown on highly oriented pyrolytic graphite (HOPG) substrates were studied extensively with regard to their intrinsic and interfacial <span class="hlt">electronic</span> properties by means of ultraviolet photoelectron spectroscopy (UPS). Merely weak substrate–adsorbate interaction occurs at the TAT/HOPG interface, with interface energetics being only little affected by the nominal film thickness. Photon <span class="hlt">energy</span>-dependent UPS performed perpendicular to the molecular planes of TAT multilayer films at room temperature clearly reveals <span class="hlt">band</span>-like intermolecular dispersion of the TAT highest occupied molecular orbital (HOMO) <span class="hlt">energy</span>. Based on a comparison with a tight-binding model, a relatively narrow bandwidth of 54 meV is derived, which points to the presence of an intermediate regime between hopping and <span class="hlt">band</span>-like hole transport. Upon additional deposition of 2,2‧:5‧,2″:5″,2″‧-quaterthiophene (4T), a 4T:TAT donor–acceptor bulk heterojunction with a considerable HOMO-level offset at the donor–acceptor interface is formed. The 4T:TAT bulk heterojunction likewise exhibits intermolecular dispersion of the TAT HOMO <span class="hlt">energy</span>, yet with a significant decreased bandwidth.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/7067698','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/biblio/7067698"><span><span class="hlt">Electron</span> <span class="hlt">energy</span> recovery system for negative ion sources</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Dagenhart, W.K.; Stirling, W.L.</p> <p>1979-10-25</p> <p>An <span class="hlt">electron</span> <span class="hlt">energy</span> recovery system for negative ion sources is provided. The system, employing crossed electric and magnetic fields, separates the <span class="hlt">electrons</span> from the ions as they are extracted from the ion source plasma generator and before the ions are accelerated to their full <span class="hlt">energy</span>. With the electric and magnetic fields oriented 90/sup 0/ to each other, the <span class="hlt">electrons</span> remain at approximately the electrical potential at which they were generated. The electromagnetic forces cause the ions to be accelerated to the full accelerating supply voltage <span class="hlt">energy</span> while being deflected through an angle of less than 90/sup 0/. The <span class="hlt">electrons</span> precess out of the accelerating field region into an <span class="hlt">electron</span> recovery region where they are collected at a small fraction of the full accelerating supply <span class="hlt">energy</span>. It is possible, by this method, to collect > 90% of the <span class="hlt">electrons</span> extracted along with the negative ions from a negative ion source beam at < 4% of full <span class="hlt">energy</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1171474-controlling-band-alignments-artificial-interface-dipoles-perovskite-heterointerfaces','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1171474-controlling-band-alignments-artificial-interface-dipoles-perovskite-heterointerfaces"><span>Controlling <span class="hlt">band</span> alignments by artificial interface dipoles at perovskite heterointerfaces</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Yajima, Takeaki; Hikita, Yasuyuki; Minohara, Makoto; ...</p> <p>2015-04-07</p> <p>The concept ‘the interface is the device' is embodied in a wide variety of interfacial <span class="hlt">electronic</span> phenomena and associated applications in oxide materials, ranging from catalysts and clean <span class="hlt">energy</span> systems to emerging multifunctional devices. Many device properties are defined by the <span class="hlt">band</span> alignment, which is often influenced by interface dipoles. On the other hand, the ability to purposefully create and control interface dipoles is a relatively unexplored degree of freedom for perovskite oxides, which should be particularly effective for such ionic materials. Here we demonstrate tuning the <span class="hlt">band</span> alignment in perovskite metal-semiconductor heterojunctions over a broad range of 1.7 eV.more » This is achieved by the insertion of positive or negative charges at the interface, and the resultant dipole formed by the induced screening charge. This approach can be broadly used in applications where decoupling the <span class="hlt">band</span> alignment from the constituent work functions and <span class="hlt">electron</span> affinities can enhance device functionality.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5093554','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5093554"><span>Origin of multiple <span class="hlt">band</span> gap values in single width nanoribbons</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Goyal, Deepika; Kumar, Shailesh; Shukla, Alok; Kumar, Rakesh</p> <p>2016-01-01</p> <p>Deterministic <span class="hlt">band</span> gap in quasi-one-dimensional nanoribbons is prerequisite for their integrated functionalities in high performance molecular-<span class="hlt">electronics</span> based devices. However, multiple <span class="hlt">band</span> gaps commonly observed in graphene nanoribbons of the same width, fabricated in same slot of experiments, remain unresolved, and raise a critical concern over scalable production of pristine and/or hetero-structure nanoribbons with deterministic properties and functionalities for plethora of applications. Here, we show that a modification in the depth of potential wells in the periodic direction of a supercell on relative shifting of passivating atoms at the edges is the origin of multiple <span class="hlt">band</span> gap values in nanoribbons of the same width in a crystallographic orientation, although they carry practically the same ground state <span class="hlt">energy</span>. The results are similar when calculations are extended from planar graphene to buckled silicene nanoribbons. Thus, the findings facilitate tuning of the <span class="hlt">electronic</span> properties of quasi-one-dimensional materials such as bio-molecular chains, organic and inorganic nanoribbons by performing edge engineering. PMID:27808172</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhRvB..96k5438T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvB..96k5438T"><span>Low-<span class="hlt">energy</span> <span class="hlt">electron</span> diffraction from ferroelectric surfaces: Dead layers and surface dipoles in clean Pb(Zr ,Ti )O 3(001 )</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Teodorescu, Cristian M.; Pintilie, Lucian; Apostol, Nicoleta G.; Costescu, Ruxandra M.; Lungu, George A.; Hrib, LuminiÅ£a.; Trupinǎ, Lucian; Tǎnase, Liviu C.; Bucur, Ioana C.; Bocîrnea, Amelia E.</p> <p>2017-09-01</p> <p>The positions of the low <span class="hlt">energy</span> <span class="hlt">electron</span> diffraction (LEED) spots from ferroelectric single crystal films depend on its polarization state, due to electric fields generated outside of the sample. One may derive the surface potential <span class="hlt">energy</span>, yielding the depth where the mobile charge carriers compensating the depolarization field are located (δ ). On ferroelectric Pb (Zr ,Ti ) O3 (001) samples, surface potential <span class="hlt">energies</span> are between 6.7 and 10.6 eV, and δ values are unusually low, in the range of 1.8 ±0.4 Å . When δ is introduced in the values of the <span class="hlt">band</span> bending inside the ferroelectric, a considerably lower value of the dielectric constant and/or of the polarization near the surface than their bulk values is obtained, evidencing either that the intrinsic `dielectric constant' of the material has this lower value or the existence of a `dead layer' at the free surface of clean ferroelectric films. The inwards polarization of these films is explained in the framework of the present considerations by the formation of an <span class="hlt">electron</span> sheet on the surface. Possible explanations are suggested for discrepancies between the values found for surface potential <span class="hlt">energies</span> from LEED experiments and those derived from the transition between mirror <span class="hlt">electron</span> microscopy and low <span class="hlt">energy</span> <span class="hlt">electron</span> microscopy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19800032942&hterms=molecular+electronics&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dmolecular%2Belectronics','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19800032942&hterms=molecular+electronics&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dmolecular%2Belectronics"><span><span class="hlt">Electron</span> <span class="hlt">energy</span>-loss spectra in molecular fluorine</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Nishimura, H.; Cartwright, D. C.; Trajmar, S.</p> <p>1979-01-01</p> <p><span class="hlt">Electron</span> <span class="hlt">energy</span>-loss spectra in molecular fluorine, for <span class="hlt">energy</span> losses from 0 to 17.0 eV, have been taken at incident <span class="hlt">electron</span> <span class="hlt">energies</span> of 30, 50, and 90 eV and scattering angles from 5 to 140 deg. Features in the spectra above 11.5 eV <span class="hlt">energy</span> loss agree well with the assignments recently made from optical spectroscopy. Excitations of many of the eleven repulsive valence excited <span class="hlt">electronic</span> states are observed and their location correlates reasonably well with recent theoretical results. Several of these excitations have been observed for the first time and four features, for which there are no identifications, appear in the spectra.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22280620-fine-structure-red-luminescence-band-undoped-gan','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22280620-fine-structure-red-luminescence-band-undoped-gan"><span>Fine structure of the red luminescence <span class="hlt">band</span> in undoped GaN</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Reshchikov, M. A., E-mail: mreshchi@vcu.edu; Usikov, A.; Saint-Petersburg National Research University of Information Technologies, Mechanics and Optics, 49 Kronverkskiy Ave., 197101 Saint Petersburg</p> <p>2014-01-20</p> <p>Many point defects in GaN responsible for broad photoluminescence (PL) <span class="hlt">bands</span> remain unidentified. Their presence in thick GaN layers grown by hydride vapor phase epitaxy (HVPE) detrimentally affects the material quality and may hinder the use of GaN in high-power <span class="hlt">electronic</span> devices. One of the main PL <span class="hlt">bands</span> in HVPE-grown GaN is the red luminescence (RL) <span class="hlt">band</span> with a maximum at 1.8 eV. We observed the fine structure of this <span class="hlt">band</span> with a zero-phonon line (ZPL) at 2.36 eV, which may help to identify the related defect. The shift of the ZPL with excitation intensity and the temperature-related transformation of the RLmore » <span class="hlt">band</span> fine structure indicate that the RL <span class="hlt">band</span> is caused by transitions from a shallow donor (at low temperature) or from the conduction <span class="hlt">band</span> (above 50 K) to an unknown deep acceptor having an <span class="hlt">energy</span> level 1.130 eV above the valence <span class="hlt">band</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29617017','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29617017"><span>Study of the <span class="hlt">electronic</span> structure of <span class="hlt">electron</span> accepting cyano-films: TCNQversusTCNE.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Capitán, Maria J; Álvarez, Jesús; Navio, Cristina</p> <p>2018-04-18</p> <p>In this article, we perform systematic research on the <span class="hlt">electronic</span> structure of two closely related organic <span class="hlt">electron</span> acceptor molecules (TCNQ and TCNE), which are of technological interest due to their outstanding <span class="hlt">electronic</span> properties. These studies have been performed from the experimental point of view by the use <span class="hlt">electron</span> spectroscopies (XPS and UPS) and supported theoretically by the use of ab-initio DFT calculations. The cross-check between both molecules allows us to identify the characteristic <span class="hlt">electronic</span> features of each part of the molecules and their contribution to the final <span class="hlt">electronic</span> structure. We can describe the nature of the <span class="hlt">band</span> gap of these materials, and we relate this with the appearance of the shake-up features in the core level spectra. A <span class="hlt">band</span> bending and <span class="hlt">energy</span> gap reduction of the aforementioned <span class="hlt">electronic</span> structure in contact with a metal surface are seen in the experimental results as well in the theoretical calculations. This behavior implies that the TCNQ thin film accepts <span class="hlt">electrons</span> from the metal substrate becoming a Schottky n-junction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ApSS..423..100K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ApSS..423..100K"><span>Doping induced modifications in the <span class="hlt">electronic</span> structure and magnetism of ZnO films: Valence <span class="hlt">band</span> and conduction <span class="hlt">band</span> studies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Katba, Savan; Jethva, Sadaf; Udeshi, Malay; Trivedi, Priyanka; Vagadia, Megha; Shukla, D. K.; Choudhary, R. J.; Phase, D. M.; Kuberkar, D. G.</p> <p>2017-11-01</p> <p>The <span class="hlt">electronic</span> structure of Pulsed Laser Deposited (PLD) ZnO, Zn0.95Fe0.05O (ZFO), Zn0.98Al0.02O (ZAO) and Zn0.93Fe0.05Al0.02O (ZFAO) films were investigated by Photoelectron spectroscopy and X-ray absorption spectroscopy. X-ray diffraction and ϕ-scan measurements show epitaxial c-directional growth of the films. Temperature dependent magnetization and M-H loop measurements show the presence of room temperature magnetic ordering in all the films. Fittings of Fe 2p XPS and Fe L3,2 -edge XAS of ZFO and ZFAO films show the presence of Fe, in both, Fe+2 and Fe+3 states in tetrahedral symmetry. Valence <span class="hlt">band</span> spectra in resonance mode show resonance photon <span class="hlt">energy</span> at 56 eV showing the presence of Fe2+ state (∼2 eV) near the Fermi level. A significant effect of Fe and Al doping on the spectral shape of O K-edge XAS was observed. Results of the Spectroscopic studies reveal that, ferromagnetism in the films is due to the contribution of oxygen deficiency which increases the number of charge carriers that take part in the exchange interaction. Al co-doping with Fe (in ZFAO) results in the enhancement of saturation magnetization by increase in the carrier-mediated ferromagnetic exchange interaction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1408425','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1408425"><span>Multicolor emission from intermediate <span class="hlt">band</span> semiconductor ZnO 1-xSe x</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Welna, M.; Baranowski, M.; Linhart, W. M.</p> <p></p> <p>Photoluminescence and photomodulated reflectivity measurements of ZnOSe alloys are used to demonstrate a splitting of the valence <span class="hlt">band</span> due to the <span class="hlt">band</span> anticrossing interaction between localized Se states and the extended valence <span class="hlt">band</span> states of the host ZnO matrix. A strong multiband emission associated with optical transitions from the conduction <span class="hlt">band</span> to lower E - and upper E + valence subbands has been observed at room temperature. The composition dependence of the optical transition <span class="hlt">energies</span> is well explained by the <span class="hlt">electronic</span> <span class="hlt">band</span> structure calculated using the kp method combined with the <span class="hlt">band</span> anticrossing model. The observation of the multiband emissionmore » is possible because of relatively long recombination lifetimes. Longer than 1 ns lifetimes for holes photoexcited to the lower valence subband offer a potential of using the alloy as an intermediate <span class="hlt">band</span> semiconductor for solar power conversion applications.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1408425-multicolor-emission-from-intermediate-band-semiconductor-zno1-xsex','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1408425-multicolor-emission-from-intermediate-band-semiconductor-zno1-xsex"><span>Multicolor emission from intermediate <span class="hlt">band</span> semiconductor ZnO 1-xSe x</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Welna, M.; Baranowski, M.; Linhart, W. M.; ...</p> <p>2017-03-13</p> <p>Photoluminescence and photomodulated reflectivity measurements of ZnOSe alloys are used to demonstrate a splitting of the valence <span class="hlt">band</span> due to the <span class="hlt">band</span> anticrossing interaction between localized Se states and the extended valence <span class="hlt">band</span> states of the host ZnO matrix. A strong multiband emission associated with optical transitions from the conduction <span class="hlt">band</span> to lower E - and upper E + valence subbands has been observed at room temperature. The composition dependence of the optical transition <span class="hlt">energies</span> is well explained by the <span class="hlt">electronic</span> <span class="hlt">band</span> structure calculated using the kp method combined with the <span class="hlt">band</span> anticrossing model. The observation of the multiband emissionmore » is possible because of relatively long recombination lifetimes. Longer than 1 ns lifetimes for holes photoexcited to the lower valence subband offer a potential of using the alloy as an intermediate <span class="hlt">band</span> semiconductor for solar power conversion applications.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JAP...123k5701A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JAP...123k5701A"><span>Heterostructures with diffused interfaces: Luminescent technique for ascertainment of <span class="hlt">band</span> alignment type</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Abramkin, D. S.; Gutakovskii, A. K.; Shamirzaev, T. S.</p> <p>2018-03-01</p> <p>The experimental ascertainment of <span class="hlt">band</span> alignment type for semiconductor heterostructures with diffused interfaces is discussed. A method based on the analysis of the spectral shift of photoluminescence (PL) <span class="hlt">band</span> with excitation density (Pex) that takes into account state filling and <span class="hlt">band</span> bending effects on the PL <span class="hlt">band</span> shift is developed. It is shown that the shift of PL <span class="hlt">band</span> maximum position is proportional to ℏωmax ˜ (Ue + Uh).ln(Pex) + b.Pex1/3, where Ue (Uh) are <span class="hlt">electron</span> (hole) Urbach <span class="hlt">energy</span> tail, and parameter b characterizes the effect of <span class="hlt">band</span> bending or is equal to zero for heterostructures with type-II or type-I <span class="hlt">band</span> alignment, respectively. The method was approved with InAs/AlAs, GaAs/AlAs, GaSb/AlAs, and AlSb/AlAs heterostructures containing quantum wells.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012SPIE.8496E..0FM','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012SPIE.8496E..0FM"><span>Frequency tunable <span class="hlt">electronic</span> sources working at room temperature in the 1 to 3 THz <span class="hlt">band</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Maestrini, Alain; Mehdi, Imran; Siles, José V.; Lin, Robert; Lee, Choonsup; Chattopadhyay, Goutam; Pearson, John; Siegel, Peter</p> <p>2012-10-01</p> <p>Compact, room temperature terahertz sources are much needed in the 1 to 3 THz <span class="hlt">band</span> for developing multi-pixel heterodyne receivers for astrophysics and planetary science or for building short-range high spatial resolution THz imaging systems able to see through low water content and non metallic materials, smoke or dust for a variety of applications ranging from the inspection of art artifacts to the detection of masked or concealed objects. All solid-sate <span class="hlt">electronic</span> sources based on a W-<span class="hlt">band</span> synthesizer followed by a high-power W-<span class="hlt">band</span> amplifier and a cascade of Schottky diode based THz frequency multipliers are now capable of producing more than 1 mW at 0.9THz, 50 μW at 2 THz and 18 μW at 2.6 THz without the need of any cryogenic system. These sources are frequency agile and have a relative bandwidth of 10 to 15%, limited by the high power W-<span class="hlt">band</span> amplifiers. The paper will present the latest developments of this technology and its perspective in terms of frequency range, bandwidth and power.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhyC..549..159D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhyC..549..159D"><span>Cooper-pair size and binding <span class="hlt">energy</span> for unconventional superconducting systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dinóla Neto, F.; Neto, Minos A.; Salmon, Octavio D. Rodriguez</p> <p>2018-06-01</p> <p>The main proposal of this paper is to analyze the size of the Cooper pairs composed by unbalanced mass fermions from different <span class="hlt">electronic</span> <span class="hlt">bands</span> along the BCS-BEC crossover and study the binding <span class="hlt">energy</span> of the pairs. We are considering an interaction between fermions with different masses leading to an inter-<span class="hlt">band</span> pairing. In addiction to the attractive interaction we have an hybridization term to couple both <span class="hlt">bands</span>, which in general acts unfavorable for the pairing between the <span class="hlt">electrons</span>. We get first order phase transitions as the hybridization breaks the Cooper pairs for the s-wave symmetry of the gap amplitude. The results show the dependence of the Cooper-pair size as a function of the hybridization for T = 0 . We also propose the structure of the binding <span class="hlt">energy</span> of the inter-<span class="hlt">band</span> system as a function of the two-<span class="hlt">bands</span> quasi-particle <span class="hlt">energies</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhyB..536...48S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhyB..536...48S"><span><span class="hlt">Electronic</span> <span class="hlt">band</span> structure of 4d and 5d transition metal trichalcogenides</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sugita, Yusuke; Miyake, Takashi; Motome, Yukitoshi</p> <p>2018-05-01</p> <p>Transition metal trichalcogenides (TMTs), a family of van der Waals materials, have gained increasing interests from the discovery of magnetism in few-layer forms. Although TMTs with 3d transition metal elements have been studied extensively, much less is explored for the 4d and 5d cases, where the interesting interplay between <span class="hlt">electron</span> correlations and the relativistic spin-orbit coupling is expected. Using ab initio calculations, we here investigate the <span class="hlt">electronic</span> property of TMTs with 4d and 5d transition metal elements. We show that the <span class="hlt">band</span> structures exhibit multiple node-like features near the Fermi level. These are the remnant of multiple Dirac cones that were recently discovered in the monolayer cases. Our results indicate that the peculiar two-dimensional multiple Dirac cones are concealed even in the layered bulk systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1209521-electronic-structures-bonding-configurations-band-gap-opening-properties-graphene-binding-low-concentration-fluorine','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1209521-electronic-structures-bonding-configurations-band-gap-opening-properties-graphene-binding-low-concentration-fluorine"><span><span class="hlt">Electronic</span> Structures, Bonding Configurations, and <span class="hlt">Band</span>-Gap-Opening Properties of Graphene Binding with Low-Concentration Fluorine</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Duan, Yuhua; Stinespring, Charter D.; Chorpening, Benjamin</p> <p>2015-06-18</p> <p>To better understand the effects of low-level fluorine in graphene-based sensors, first-principles density functional theory (DFT) with van der Waals dispersion interactions has been employed to investigate the structure and impact of fluorine defects on the electrical properties of single-layer graphene films. The results show that both graphite-2H and graphene have zero <span class="hlt">band</span> gaps. When fluorine bonds to a carbon atom, the carbon atom is pulled slightly above the graphene plane, creating what is referred to as a CF defect. The lowest-binding <span class="hlt">energy</span> state is found to correspond to two CF defects on nearest neighbor sites, with one fluorine abovemore » the carbon plane and the other below the plane. Overall this has the effect of buckling the graphene. The results further show that the addition of fluorine to graphene leads to the formation of an <span class="hlt">energy</span> <span class="hlt">band</span> (BF) near the Fermi level, contributed mainly from the 2p orbitals of fluorine with a small contribution from the porbitals of the carbon. Among the 11 binding configurations studied, our results show that only in two cases does the BF serve as a conduction <span class="hlt">band</span> and open a <span class="hlt">band</span> gap of 0.37 eV and 0.24 eV respectively. The binding <span class="hlt">energy</span> decreases with decreasing fluorine concentration due to the interaction between neighboring fluorine atoms. The obtained results are useful for sensor development and nanoelectronics.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28561024','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28561024"><span>Giant <span class="hlt">electron</span>-hole transport asymmetry in ultra-short quantum transistors.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>McRae, A C; Tayari, V; Porter, J M; Champagne, A R</p> <p>2017-05-31</p> <p>Making use of bipolar transport in single-wall carbon nanotube quantum transistors would permit a single device to operate as both a quantum dot and a ballistic conductor or as two quantum dots with different charging <span class="hlt">energies</span>. Here we report ultra-clean 10 to 100 nm scale suspended nanotube transistors with a large <span class="hlt">electron</span>-hole transport asymmetry. The devices consist of naked nanotube channels contacted with sections of tube under annealed gold. The annealed gold acts as an n-doping top gate, allowing coherent quantum transport, and can create nanometre-sharp barriers. These tunnel barriers define a single quantum dot whose charging <span class="hlt">energies</span> to add an <span class="hlt">electron</span> or a hole are vastly different (e-h charging <span class="hlt">energy</span> asymmetry). We parameterize the e-h transport asymmetry by the ratio of the hole and <span class="hlt">electron</span> charging <span class="hlt">energies</span> η e-h . This asymmetry is maximized for short channels and small <span class="hlt">band</span> gap tubes. In a small <span class="hlt">band</span> gap device, we demonstrate the fabrication of a dual functionality quantum device acting as a quantum dot for holes and a much longer quantum bus for <span class="hlt">electrons</span>. In a 14 nm-long channel, η e-h reaches up to 2.6 for a device with a <span class="hlt">band</span> gap of 270 meV. The charging <span class="hlt">energies</span> in this device exceed 100 meV.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5460015','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5460015"><span>Giant <span class="hlt">electron</span>-hole transport asymmetry in ultra-short quantum transistors</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>McRae, A. C.; Tayari, V.; Porter, J. M.; Champagne, A. R.</p> <p>2017-01-01</p> <p>Making use of bipolar transport in single-wall carbon nanotube quantum transistors would permit a single device to operate as both a quantum dot and a ballistic conductor or as two quantum dots with different charging <span class="hlt">energies</span>. Here we report ultra-clean 10 to 100 nm scale suspended nanotube transistors with a large <span class="hlt">electron</span>-hole transport asymmetry. The devices consist of naked nanotube channels contacted with sections of tube under annealed gold. The annealed gold acts as an n-doping top gate, allowing coherent quantum transport, and can create nanometre-sharp barriers. These tunnel barriers define a single quantum dot whose charging <span class="hlt">energies</span> to add an <span class="hlt">electron</span> or a hole are vastly different (e−h charging <span class="hlt">energy</span> asymmetry). We parameterize the e−h transport asymmetry by the ratio of the hole and <span class="hlt">electron</span> charging <span class="hlt">energies</span> ηe−h. This asymmetry is maximized for short channels and small <span class="hlt">band</span> gap tubes. In a small <span class="hlt">band</span> gap device, we demonstrate the fabrication of a dual functionality quantum device acting as a quantum dot for holes and a much longer quantum bus for <span class="hlt">electrons</span>. In a 14 nm-long channel, ηe−h reaches up to 2.6 for a device with a <span class="hlt">band</span> gap of 270 meV. The charging <span class="hlt">energies</span> in this device exceed 100 meV. PMID:28561024</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19740039525&hterms=interest+simple&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dinterest%2Bsimple','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19740039525&hterms=interest+simple&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dinterest%2Bsimple"><span>Ground-state <span class="hlt">energies</span> of simple metals</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hammerberg, J.; Ashcroft, N. W.</p> <p>1974-01-01</p> <p>A structural expansion for the static ground-state <span class="hlt">energy</span> of a simple metal is derived. Two methods are presented, one an approach based on single-particle <span class="hlt">band</span> structure which treats the <span class="hlt">electron</span> gas as a nonlinear dielectric, the other a more general many-particle analysis using finite-temperature perturbation theory. The two methods are compared, and it is shown in detail how <span class="hlt">band</span>-structure effects, Fermi-surface distortions, and chemical-potential shifts affect the total <span class="hlt">energy</span>. These are of special interest in corrections to the total <span class="hlt">energy</span> beyond third order in the <span class="hlt">electron</span>-ion interaction and hence to systems where differences in <span class="hlt">energies</span> for various crystal structures are exceptionally small. Preliminary calculations using these methods for the zero-temperature thermodynamic functions of atomic hydrogen are reported.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_22 --> <div id="page_23" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="441"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/527015-ballistic-electron-emission-spectroscopy-al-sub-ga-sub-minus-gaas-heterostructures-conduction-band-offsets-transport-mechanisms-band-structure-effects','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/527015-ballistic-electron-emission-spectroscopy-al-sub-ga-sub-minus-gaas-heterostructures-conduction-band-offsets-transport-mechanisms-band-structure-effects"><span>Ballistic-<span class="hlt">electron</span>-emission spectroscopy of Al{sub x}Ga{sub 1{minus}x}As/GaAs heterostructures: Conduction-<span class="hlt">band</span> offsets, transport mechanisms, and <span class="hlt">band</span>-structure effects</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>OShea, J.J.; Brazel, E.G.; Rubin, M.E.</p> <p>1997-07-01</p> <p>We report an extensive investigation of semiconductor <span class="hlt">band</span>-structure effects in single-barrier Al{sub x}Ga{sub 1{minus}x}As/GaAs heterostructures using ballistic-<span class="hlt">electron</span>-emission spectroscopy (BEES). The transport mechanisms in these single-barrier structures were studied systematically as a function of temperature and Al composition over the full compositional range (0{le}x{le}1). The initial ({Gamma}) BEES thresholds for Al{sub x}Ga{sub 1{minus}x}As single barriers with 0{le}x{le}0.42 were extracted using a model which includes the complete transmission probability of the metal-semiconductor interface and the semiconductor heterostructure. <span class="hlt">Band</span> offsets measured by BEES are in good agreement with previous measurements by other techniques which demonstrates the accuracy of this technique. BEES measurements atmore » 77 K give the same <span class="hlt">band</span>-offset values as at room temperature. When a reverse bias is applied to the heterostructures, the BEES thresholds shift to lower voltages in good agreement with the expected bias-induced <span class="hlt">band</span>-bending. In the indirect <span class="hlt">band</span>-gap regime ({ital x}{gt}0.45), spectra show a weak ballistic-<span class="hlt">electron</span>-emission microscopy current contribution due to intervalley scattering through Al{sub x}Ga{sub 1{minus}x}As {ital X} valley states. Low-temperature spectra show a marked reduction in this intervalley current component, indicating that intervalley phonon scattering at the GaAs/Al{sub x}Ga{sub 1{minus}x}As interface produces a significant fraction of this{ital X} valley current. A comparison of the BEES thresholds with the expected composition dependence of the Al{sub x}Ga{sub 1{minus}x}As {Gamma}, {ital L}, and {ital X} points yields good agreement over the entire composition range. {copyright} {ital 1997} {ital The American Physical Society}« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/878935','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/878935"><span>Attainment of <span class="hlt">Electron</span> Beam Suitable for Medium <span class="hlt">Energy</span> <span class="hlt">Electron</span> Cooling</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Seletskiy, Sergei M.</p> <p></p> <p><span class="hlt">Electron</span> cooling of charged particle beams is a well-established technique at <span class="hlt">electron</span> <span class="hlt">energies</span> of up to 300 keV. However, up to the present time the advance of <span class="hlt">electron</span> cooling to the MeV-range <span class="hlt">energies</span> has remained a purely theoretical possibility. The <span class="hlt">electron</span> cooling project at Fermilab has recently demonstrated the ¯rst cooling of 8.9 GeV/c antiprotons in the Recycler ring, and therefore, has proved the validity of the idea of relativistic <span class="hlt">electron</span> cool- ing. The Recycler <span class="hlt">Electron</span> Cooler (REC) is the key component of the Teva- tron Run II luminosity upgrade project. Its performance depends critically on the quality of electronmore » beam. A stable <span class="hlt">electron</span> beam of 4.3 MeV car- rying 0.5 A of DC current is required. The beam suitable for the Recycler <span class="hlt">Electron</span> Cooler must have an angular spread not exceeding 200 ¹rad. The full-scale prototype of the REC was designed, built and tested at Fermilab in the Wideband laboratory to study the feasibility of attaining the high-quality <span class="hlt">electron</span> beam. In this thesis I describe various aspects of development of the Fermilab <span class="hlt">electron</span> cooling system, and the techniques used to obtain the <span class="hlt">electron</span> beam suitable for the cooling process. In particular I emphasize those aspects of the work for which I was principally responsible.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018RScI...89d3105W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018RScI...89d3105W"><span>Development of an <span class="hlt">electron</span>-ion coincidence apparatus for molecular-frame <span class="hlt">electron</span> <span class="hlt">energy</span> loss spectroscopy studies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Watanabe, Noboru; Hirayama, Tsukasa; Yamada, So; Takahashi, Masahiko</p> <p>2018-04-01</p> <p>We report details of an <span class="hlt">electron</span>-ion coincidence apparatus, which has been developed for molecular-frame <span class="hlt">electron</span> <span class="hlt">energy</span> loss spectroscopy studies. The apparatus is mainly composed of a pulsed <span class="hlt">electron</span> gun, an <span class="hlt">energy</span>-dispersive <span class="hlt">electron</span> spectrometer, and an ion momentum imaging spectrometer. Molecular-orientation dependence of the high-<span class="hlt">energy</span> <span class="hlt">electron</span> scattering cross section can be examined by conducting measurements of vector correlation between the momenta of the scattered <span class="hlt">electron</span> and fragment ion. Background due to false coincidences is significantly reduced by introducing a pulsed <span class="hlt">electron</span> beam and pulsing scheme of ion extraction. The experimental setup has been tested by measuring the inner-shell excitation of N2 at an incident <span class="hlt">electron</span> <span class="hlt">energy</span> of 1.5 keV and a scattering angle of 10.2°.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/4394338-energy-dependence-lithium-fluoride-dosemeter-high-energy-electrons','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/4394338-energy-dependence-lithium-fluoride-dosemeter-high-energy-electrons"><span><span class="hlt">Energy</span> dependence of lithium fluoride dosemeter for high <span class="hlt">energy</span> <span class="hlt">electrons</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Antoku, S.; Sunayashiki, T.; Takeoka, S.</p> <p>1973-11-01</p> <p>A lithium fluoride and a Fricke dosemeter have been exposed simultaneously to /sup 60/Co gamma -rays and 10, 20, and 30 MeV <span class="hlt">electrons</span> to study the <span class="hlt">energy</span> dependence of the lithium fluoride dosemeter for high-<span class="hlt">energy</span> <span class="hlt">electrons</span>, with particular reference to possible significant reductions in the sensitivity of LiF phosphors for <span class="hlt">electrons</span> as compared with /sup 60/Co gamma - rays. In the present study, the direct comparison excluded errors resulting from uncertainties about ion recombination and conversion factors from roentgens to rads for ionization chambers. The dosemeters were exposed to approximately 5000 rads of each radiation at the appropriate peak depthmore » in a water phantom. Corrections for the supra-linear response for LiF were made using a dose response curve for /sup 60/Co gamma -rays. The three types of LiF phosphor examined did not exhibit any <span class="hlt">energy</span> dependence for <span class="hlt">electrons</span> compared with /sup 60/Co gamma - rays. Within the statistical uncertainty (~3%) for the experiment. (UK)« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011JETP..112..140O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011JETP..112..140O"><span><span class="hlt">Electronic</span> structure, magnetic properties, and mechanism of the insulator-metal transition in LaCoO3 taking into account strong <span class="hlt">electron</span> correlations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ovchinnikov, S. G.; Orlov, Yu. S.; Nekrasov, I. A.; Pchelkina, Z. V.</p> <p>2011-01-01</p> <p>The <span class="hlt">electronic</span> structure of LaCoO3 at finite temperatures is calculated using the LDA+GTB method taking into account strong <span class="hlt">electron</span> correlations and possible spin crossover upon an increase in temperature. Gap states revealed in the <span class="hlt">energy</span> spectrum of LaCoO3 reduce the dielectric gap width upon heating; this allowed us to describe the insulator-metal transition observed in this compound at T = 500-600 K. The temperature dependence of the magnetic susceptibility with a peak at T ≈ 100 K is explained by the Curie contribution from thermally excited <span class="hlt">energy</span> levels of the Co3+ ion. At high temperatures, the Pauli contribution from a <span class="hlt">band</span> <span class="hlt">electron</span> is added and the total magnetization of LaCoO3 is considered as the sum M tot = M loc + M <span class="hlt">band</span>. The second term describes the <span class="hlt">band</span> contribution appearing as a result of the insulator-metal transition and facilitating the emergence of a high-temperature anomaly in the magnetic susceptibility of LaCoO3.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26206417','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26206417"><span>Quasiparticle self-consistent GW study of cuprates: <span class="hlt">electronic</span> structure, model parameters, and the two-<span class="hlt">band</span> theory for Tc.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jang, Seung Woo; Kotani, Takao; Kino, Hiori; Kuroki, Kazuhiko; Han, Myung Joon</p> <p>2015-07-24</p> <p>Despite decades of progress, an understanding of unconventional superconductivity still remains elusive. An important open question is about the material dependence of the superconducting properties. Using the quasiparticle self-consistent GW method, we re-examine the <span class="hlt">electronic</span> structure of copper oxide high-Tc materials. We show that QSGW captures several important features, distinctive from the conventional LDA results. The <span class="hlt">energy</span> level splitting between d(x(2)-y(2)) and d(3z(2)-r(2)) is significantly enlarged and the van Hove singularity point is lowered. The calculated results compare better than LDA with recent experimental results from resonant inelastic xray scattering and angle resolved photoemission experiments. This agreement with the experiments supports the previously suggested two-<span class="hlt">band</span> theory for the material dependence of the superconducting transition temperature, Tc.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1184847-photoemission-study-electronic-structure-charge-density-waves-natisbo','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1184847-photoemission-study-electronic-structure-charge-density-waves-natisbo"><span>Photoemission study of the <span class="hlt">electronic</span> structure and charge density waves of Na₂Ti₂Sb₂O</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Tan, S. Y.; Jiang, J.; Ye, Z. R.; ...</p> <p>2015-04-30</p> <p>The <span class="hlt">electronic</span> structure of Na₂Ti₂Sb₂O single crystal is studied by photon <span class="hlt">energy</span> and polarization dependent angle-resolved photoemission spectroscopy (ARPES). The obtained <span class="hlt">band</span> structure and Fermi surface agree well with the <span class="hlt">band</span> structure calculation of Na₂Ti₂Sb₂O in the non-magnetic state, which indicates that there is no magnetic order in Na₂Ti₂Sb₂O and the <span class="hlt">electronic</span> correlation is weak. Polarization dependent ARPES results suggest the multi-<span class="hlt">band</span> and multi-orbital nature of Na₂Ti₂Sb₂O. Photon <span class="hlt">energy</span> dependent ARPES results suggest that the <span class="hlt">electronic</span> structure of Na₂Ti₂Sb₂O is rather two-dimensional. Moreover, we find a density wave <span class="hlt">energy</span> gap forms below the transition temperature and reaches 65 meV atmore » 7 K, indicating that Na₂Ti₂Sb₂O is likely a weakly correlated CDW material in the strong <span class="hlt">electron</span>-phonon interaction regime. (author)« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011JChPh.134v4706P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011JChPh.134v4706P"><span>Hybrid density functional theory <span class="hlt">band</span> structure engineering in hematite</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pozun, Zachary D.; Henkelman, Graeme</p> <p>2011-06-01</p> <p>We present a hybrid density functional theory (DFT) study of doping effects in α-Fe2O3, hematite. Standard DFT underestimates the <span class="hlt">band</span> gap by roughly 75% and incorrectly identifies hematite as a Mott-Hubbard insulator. Hybrid DFT accurately predicts the proper structural, magnetic, and <span class="hlt">electronic</span> properties of hematite and, unlike the DFT+U method, does not contain d-<span class="hlt">electron</span> specific empirical parameters. We find that using a screened functional that smoothly transitions from 12% exact exchange at short ranges to standard DFT at long range accurately reproduces the experimental <span class="hlt">band</span> gap and other material properties. We then show that the antiferromagnetic symmetry in the pure α-Fe2O3 crystal is broken by all dopants and that the ligand field theory correctly predicts local magnetic moments on the dopants. We characterize the resulting <span class="hlt">band</span> gaps for hematite doped by transition metals and the p-block post-transition metals. The specific case of Pd doping is investigated in order to correlate calculated doping <span class="hlt">energies</span> and optical properties with experimentally observed photocatalytic behavior.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA154698','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA154698"><span>Microwave Semiconductor Research - Materials, Devices and Circuits and Gallium Arsenide Ballistic <span class="hlt">Electron</span> Transistors.</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1985-04-01</p> <p>activation <span class="hlt">energies</span> than previously possible. <span class="hlt">Electron</span> traps and hole traps with <span class="hlt">energies</span> less than 50 meV were observed for the first time in GaAs...developed in our laboratory to photoexcite <span class="hlt">electrons</span> in a given <span class="hlt">energy</span> range in the conduction <span class="hlt">band</span> and then measure the relaxation of these carriers...limitations on the <span class="hlt">electron</span> <span class="hlt">energy</span> may be required. CURRENT AND FUTURE EFFORTS The possibility of ballistic <span class="hlt">electron</span> transport in gallium arsenide has been</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1987JAP....61.4612W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1987JAP....61.4612W"><span>An <span class="hlt">energy</span>-dependent <span class="hlt">electron</span> backscattering coefficient</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Williamson, W., Jr.; Antolak, A. J.; Meredith, R. J.</p> <p>1987-05-01</p> <p>An <span class="hlt">energy</span>-dependent <span class="hlt">electron</span> backscattering coefficient is derived based on the continuous slowing down approximation and the Bethe stopping power. Backscattering coefficients are given for 10-50-keV <span class="hlt">electrons</span> incident on bulk and thin-film aluminum, silver, and gold targets. The results are compared with the Everhart theory and empirical fits to experimental data. The <span class="hlt">energy</span>-dependent theory agrees better with experimental work.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22479669-li-induced-effects-core-level-band-electronic-structure-graphene-grown-face-sic','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22479669-li-induced-effects-core-level-band-electronic-structure-graphene-grown-face-sic"><span>Li induced effects in the core level and π-<span class="hlt">band</span> <span class="hlt">electronic</span> structure of graphene grown on C-face SiC</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Johansson, Leif I., E-mail: lij@ifm.liu.se; Xia, Chao; Virojanadara, Chariya</p> <p></p> <p>Studies of the effects induced in the <span class="hlt">electronic</span> structure after Li deposition, and subsequent heating, on graphene samples prepared on C-face SiC are reported. The as prepared graphene samples are essentially undoped, but after Li deposition, the Dirac point shifts down to 1.2 eV below the Fermi level due to <span class="hlt">electron</span> doping. The shape of the C 1s level also indicates a doping concentration of around 10{sup 14 }cm{sup −2} after Li deposition, when compared with recent calculated results of core level spectra of graphene. The C 1s, Si 2p, and Li 1s core level results show little intercalation directly after depositionmore » but that most of the Li has intercalated after heating at 280 °C. Heating at higher temperatures leads to desorption of Li from the sample, and at 1030 °C, Li can no longer be detected on the sample. The single π-<span class="hlt">band</span> observable from multilayer C-face graphene samples in conventional angle resolved photoelectron spectroscopy is reasonably sharp both on the initially prepared sample and after Li deposition. After heating at 280 °C, the π-<span class="hlt">band</span> appears more diffuse and possibly split. The Dirac point becomes located at 0.4 eV below the Fermi level, which indicates occurrence of a significant reduction in the <span class="hlt">electron</span> doping concentration. Constant <span class="hlt">energy</span> photoelectron distribution patterns extracted from the as prepared graphene C-face sample and also after Li deposition and heating at 280 °C look very similar to earlier calculated distribution patterns for monolayer graphene.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PhPro..61..666C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PhPro..61..666C"><span>The new Wide-<span class="hlt">band</span> Solar Neutrino Trigger for Super-Kamiokande</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carminati, Giada</p> <p></p> <p>Super-Kamiokande observes low <span class="hlt">energy</span> <span class="hlt">electrons</span> induced by the elastic scattering of 8B solar neutrinos. The transition region between vacuum and matter oscillations, with neutrino <span class="hlt">energy</span> near 3 MeV, is still partially unexplored by any detector. Super-Kamiokande can study this intermediate regime adding a new software trigger. The Wide-<span class="hlt">band</span> Intelligent Trigger (WIT) has been developed to simultaneously trigger and reconstruct very low <span class="hlt">energy</span> <span class="hlt">electrons</span> (above 2.49 kinetic MeV) with an e_ciency close to 100%. The WIT system, comprising 256-Hyperthreaded CPU cores and one 10-Gigabit Ethernet network switch, has been recently installed and integrated in the online DAQ system of SK and the complete system is currently in an advanced status of online data testing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PlPhR..44...18O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PlPhR..44...18O"><span>Generation of Low-<span class="hlt">Energy</span> High-Current <span class="hlt">Electron</span> Beams in Plasma-Anode <span class="hlt">Electron</span> Guns</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ozur, G. E.; Proskurovsky, D. I.</p> <p>2018-01-01</p> <p>This paper is a review of studies on the generation of low-<span class="hlt">energy</span> high-current <span class="hlt">electron</span> beams in <span class="hlt">electron</span> guns with a plasma anode and an explosive-emission cathode. The problems related to the initiation of explosive <span class="hlt">electron</span> emission under plasma and the formation and transport of high-current <span class="hlt">electron</span> beams in plasma-filled systems are discussed consecutively. Considerable attention is given to the nonstationary effects that occur in the space charge layers of plasma. Emphasis is also placed on the problem of providing a uniform <span class="hlt">energy</span> density distribution over the beam cross section, which is of critical importance in using <span class="hlt">electron</span> beams of this type for surface treatment of materials. Examples of facilities based on low-<span class="hlt">energy</span> high-current <span class="hlt">electron</span> beam sources are presented and their applications in materials science and practice are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29114447','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29114447"><span>Comprehensive investigation of the <span class="hlt">electronic</span> excitation of W(CO)6 by photoabsorption and theoretical analysis in the <span class="hlt">energy</span> region from 3.9 to 10.8 eV.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mendes, Mónica; Regeta, Khrystyna; Ferreira da Silva, Filipe; Jones, Nykola C; Hoffmann, Søren Vrønning; García, Gustavo; Daniel, Chantal; Limão-Vieira, Paulo</p> <p>2017-01-01</p> <p>High-resolution vacuum ultraviolet photoabsorption measurements in the wavelength range of 115-320 nm (10.8-3.9 eV) have been performed together with comprehensive relativistic time-dependent density functional calculations (TDDFT) on the low-lying excited sates of tungsten hexacarbonyl, W(CO) 6 . The higher resolution obtained reveals previously unresolved spectral features of W(CO) 6 . The spectrum shows two higher-<span class="hlt">energy</span> <span class="hlt">bands</span> (in the <span class="hlt">energy</span> ranges of 7.22-8.12 eV and 8.15-9.05 eV), one of them with clear vibrational structure, and a few lower-<span class="hlt">energy</span> shoulders in addition to a couple of lower-<span class="hlt">energy</span> metal-to-ligand charge-transfer (MLCT) <span class="hlt">bands</span> reported in the literature before. Absolute photoabsorption cross sections are reported and, where possible, compared to previously published results. On the basis of this combined experimental/theoretical study the absorption spectrum of the complex has been totally re-assigned between 3.9 and 10.8 eV under the light of spin-orbit coupling (SOC) effects. The present comprehensive knowledge of the nature of the <span class="hlt">electronically</span> excited states may be of relevance to estimate neutral dissociation cross sections of W(CO) 6 , a precursor molecule in focused <span class="hlt">electron</span> beam induced deposition (FEBID) processes, from <span class="hlt">electron</span> scattering measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5669226','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5669226"><span>Comprehensive investigation of the <span class="hlt">electronic</span> excitation of W(CO)6 by photoabsorption and theoretical analysis in the <span class="hlt">energy</span> region from 3.9 to 10.8 eV</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Mendes, Mónica; Regeta, Khrystyna; Ferreira da Silva, Filipe; Jones, Nykola C; Hoffmann, Søren Vrønning; García, Gustavo</p> <p>2017-01-01</p> <p>High-resolution vacuum ultraviolet photoabsorption measurements in the wavelength range of 115–320 nm (10.8–3.9 eV) have been performed together with comprehensive relativistic time-dependent density functional calculations (TDDFT) on the low-lying excited sates of tungsten hexacarbonyl, W(CO)6. The higher resolution obtained reveals previously unresolved spectral features of W(CO)6. The spectrum shows two higher-<span class="hlt">energy</span> <span class="hlt">bands</span> (in the <span class="hlt">energy</span> ranges of 7.22–8.12 eV and 8.15–9.05 eV), one of them with clear vibrational structure, and a few lower-<span class="hlt">energy</span> shoulders in addition to a couple of lower-<span class="hlt">energy</span> metal-to-ligand charge-transfer (MLCT) <span class="hlt">bands</span> reported in the literature before. Absolute photoabsorption cross sections are reported and, where possible, compared to previously published results. On the basis of this combined experimental/theoretical study the absorption spectrum of the complex has been totally re-assigned between 3.9 and 10.8 eV under the light of spin–orbit coupling (SOC) effects. The present comprehensive knowledge of the nature of the <span class="hlt">electronically</span> excited states may be of relevance to estimate neutral dissociation cross sections of W(CO)6, a precursor molecule in focused <span class="hlt">electron</span> beam induced deposition (FEBID) processes, from <span class="hlt">electron</span> scattering measurements. PMID:29114447</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28147681','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28147681"><span>Retarding field <span class="hlt">energy</span> analyzer for high <span class="hlt">energy</span> pulsed <span class="hlt">electron</span> beam measurements.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hu, Jing; Rovey, Joshua L; Zhao, Wansheng</p> <p>2017-01-01</p> <p>A retarding field <span class="hlt">energy</span> analyzer (RFEA) designed specifically for high <span class="hlt">energy</span> pulsed <span class="hlt">electron</span> beam measurements is described in this work. By proper design of the entrance grid, attenuation grid, and beam collector, this RFEA is capable of determining the time-resolved <span class="hlt">energy</span> distribution of high <span class="hlt">energy</span> pulsed <span class="hlt">electron</span> beams normally generated under "soft vacuum" environment. The performance of the RFEA is validated by multiple tests of the leakage current, attenuation coefficient, and response time. The test results show that the retarding potential in the RFEA can go up to the same voltage as the <span class="hlt">electron</span> beam source, which is 20 kV for the maximum in this work. Additionally, an attenuation coefficient of 4.2 is obtained in the RFEA while the percent difference of the rise time of the <span class="hlt">electron</span> beam pulse before and after attenuation is lower than 10%. When compared with a reference source, the percent difference of the RFEA response time is less than 10% for fall times greater than 35 ns. Finally, the test results of the 10 kV pseudospark-based pulsed <span class="hlt">electron</span> beam currents collected under varying retarding potentials are presented in this paper.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22416106-electronic-excitation-carbonyl-sulphide-cos-high-resolution-vacuum-ultraviolet-photoabsorption-electron-impact-spectroscopy-energy-region-from-ev','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22416106-electronic-excitation-carbonyl-sulphide-cos-high-resolution-vacuum-ultraviolet-photoabsorption-electron-impact-spectroscopy-energy-region-from-ev"><span><span class="hlt">Electronic</span> excitation of carbonyl sulphide (COS) by high-resolution vacuum ultraviolet photoabsorption and <span class="hlt">electron</span>-impact spectroscopy in the <span class="hlt">energy</span> region from 4 to 11 eV</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Limão-Vieira, P., E-mail: plimaovieira@fct.unl.pt; Department of Physics, Sophia University, Tokyo 102-8554; Department of Physical Sciences, The Open University, Walton Hall, Milton Keynes MK7 6AA</p> <p>2015-02-14</p> <p>The <span class="hlt">electronic</span> state spectroscopy of carbonyl sulphide, COS, has been investigated using high resolution vacuum ultraviolet photoabsorption spectroscopy and <span class="hlt">electron</span> <span class="hlt">energy</span> loss spectroscopy in the <span class="hlt">energy</span> range of 4.0–10.8 eV. The spectrum reveals several new features not previously reported in the literature. Vibronic structure has been observed, notably in the low <span class="hlt">energy</span> absorption dipole forbidden <span class="hlt">band</span> assigned to the (4π←3π) ({sup 1}Δ←{sup 1}Σ{sup +}) transition, with a new weak transition assigned to ({sup 1}Σ{sup −}←{sup 1}Σ{sup +}) reported here for the first time. The absolute optical oscillator strengths are determined for ground state to {sup 1}Σ{sup +} and {sup 1}Πmore » transitions. Based on our recent measurements of differential cross sections for the optically allowed ({sup 1}Σ{sup +} and {sup 1}Π) transitions of COS by <span class="hlt">electron</span> impact, the optical oscillator strength f{sub 0} value and integral cross sections (ICSs) are derived by applying a generalized oscillator strength analysis. Subsequently, ICSs predicted by the scaling are confirmed down to 60 eV in the intermediate <span class="hlt">energy</span> region. The measured absolute photoabsorption cross sections have been used to calculate the photolysis lifetime of carbonyl sulphide in the upper stratosphere (20–50 km)« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013PhyB..410..112R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013PhyB..410..112R"><span><span class="hlt">Electronic</span> <span class="hlt">band</span> structure of LaCoO3/Y/Mn compounds</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rahnamaye Aliabad, H. A.; Hesam, V.; Ahmad, Iftikhar; Khan, Imad</p> <p>2013-02-01</p> <p>Spin polarization effects on <span class="hlt">electronic</span> properties of pure LaCoO3 and doped compounds (La0.5Y0.5CoO3, LaCo0.5Mn0.5O3) in the rhombohedral phase have been studied. We have employed the full potential linearized augmented plane wave (FP-LAPW) method with the generalized gradient approximation (GGA+U) under density functional theory (DFT). The calculated <span class="hlt">band</span> structures along with total as well as partial densities of states reveal that Y and Mn impurities have a significant effect on the structural and <span class="hlt">electronic</span> properties of LaCoO3. It is found that Mn alters insulating behavior of this compound to the half metallic for spin up state. Obtained results show that the magnetic moment for the Co-3d state is near 3.12μB in LaCoO3 compound which increases and decreases with addition of Y and Mn dopants respectively.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1434315-first-principles-study-electronic-structure-fermi-surface-semimetallic-yas','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1434315-first-principles-study-electronic-structure-fermi-surface-semimetallic-yas"><span>First-principles study of <span class="hlt">electronic</span> structure and Fermi surface in semimetallic YAs</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Swatek, Przemys?aw Wojciech</p> <p>2018-03-23</p> <p>In the course of searching for new systems, which exhibit nonsaturating and extremely large positive magnetoresistance, <span class="hlt">electronic</span> structure, Fermi surface, and de Haas-van Alphen characteristics of the semimetallic YAs compound were studied using the all-<span class="hlt">electron</span> full-potential linearized augmented-plane wave (FP–LAPW) approach in the framework of the generalized gradient approximation (GGA). In the scalar-relativistic calculation, the cubic symmetry splits fivefold degenerate Y- d orbital into low-<span class="hlt">energy</span> threefold-degenerate and twofold degenerate doublet states at point around the Fermi <span class="hlt">energy</span>. Furthermore one of them, together with the threefold degenerate character of As-p orbital, render the YAs semimetal with a topologically trivial <span class="hlt">band</span> ordermore » and fairly low density of states at the Fermi level. Including spin–orbit (SO) coupling into the calculation leads to pronounced splitting of the state and shifting the <span class="hlt">bands</span> in the <span class="hlt">energy</span> scale. Consequently, the determined four different 3-dimensional Fermi surface sheets of YAs consists of three concentric hole-like <span class="hlt">bands</span> at and one ellipsoidal <span class="hlt">electron</span>-like sheet centred at the X points. In full accordance with the previous first-principles calculations for isostructural YSb and YBi, the calculated Fermi surface of YAs originates from fairly compensated multi-<span class="hlt">band</span> <span class="hlt">electronic</span> structures.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1434315-first-principles-study-electronic-structure-fermi-surface-semimetallic-yas','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1434315-first-principles-study-electronic-structure-fermi-surface-semimetallic-yas"><span>First-principles study of <span class="hlt">electronic</span> structure and Fermi surface in semimetallic YAs</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Swatek, Przemys?aw Wojciech</p> <p></p> <p>In the course of searching for new systems, which exhibit nonsaturating and extremely large positive magnetoresistance, <span class="hlt">electronic</span> structure, Fermi surface, and de Haas-van Alphen characteristics of the semimetallic YAs compound were studied using the all-<span class="hlt">electron</span> full-potential linearized augmented-plane wave (FP–LAPW) approach in the framework of the generalized gradient approximation (GGA). In the scalar-relativistic calculation, the cubic symmetry splits fivefold degenerate Y- d orbital into low-<span class="hlt">energy</span> threefold-degenerate and twofold degenerate doublet states at point around the Fermi <span class="hlt">energy</span>. Furthermore one of them, together with the threefold degenerate character of As-p orbital, render the YAs semimetal with a topologically trivial <span class="hlt">band</span> ordermore » and fairly low density of states at the Fermi level. Including spin–orbit (SO) coupling into the calculation leads to pronounced splitting of the state and shifting the <span class="hlt">bands</span> in the <span class="hlt">energy</span> scale. Consequently, the determined four different 3-dimensional Fermi surface sheets of YAs consists of three concentric hole-like <span class="hlt">bands</span> at and one ellipsoidal <span class="hlt">electron</span>-like sheet centred at the X points. In full accordance with the previous first-principles calculations for isostructural YSb and YBi, the calculated Fermi surface of YAs originates from fairly compensated multi-<span class="hlt">band</span> <span class="hlt">electronic</span> structures.« less</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_23 --> <div id="page_24" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="461"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/15003703-properties-electron-cloud-high-energy-positron-electron-storage-ring','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/15003703-properties-electron-cloud-high-energy-positron-electron-storage-ring"><span>Properties of the <span class="hlt">electron</span> cloud in a high-<span class="hlt">energy</span> positron and <span class="hlt">electron</span> storage ring</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Harkay, K. C.; Rosenberg, R. A.</p> <p>2003-03-20</p> <p>Low-<span class="hlt">energy</span>, background <span class="hlt">electrons</span> are ubiquitous in high-<span class="hlt">energy</span> particle accelerators. Under certain conditions, interactions between this <span class="hlt">electron</span> cloud and the high-<span class="hlt">energy</span> beam can give rise to numerous effects that can seriously degrade the accelerator performance. These effects range from vacuum degradation to collective beam instabilities and emittance blowup. Although <span class="hlt">electron</span>-cloud effects were first observed two decades ago in a few proton storage rings, they have in recent years been widely observed and intensely studied in positron and proton rings. <span class="hlt">Electron</span>-cloud diagnostics developed at the Advanced Photon Source enabled for the first time detailed, direct characterization of the <span class="hlt">electron</span>-cloud properties in amore » positron and <span class="hlt">electron</span> storage ring. From in situ measurements of the <span class="hlt">electron</span> flux and <span class="hlt">energy</span> distribution at the vacuum chamber wall, <span class="hlt">electron</span>-cloud production mechanisms and details of the beam-cloud interaction can be inferred. A significant longitudinal variation of the <span class="hlt">electron</span> cloud is also observed, due primarily to geometrical details of the vacuum chamber. Furthermore, such experimental data can be used to provide realistic limits on key input parameters in modeling efforts, leading ultimately to greater confidence in predicting <span class="hlt">electron</span>-cloud effects in future accelerators.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016LaPhy..26f5005N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016LaPhy..26f5005N"><span><span class="hlt">Electron</span> <span class="hlt">energy</span> and <span class="hlt">electron</span> trajectories in an inverse free-<span class="hlt">electron</span> laser accelerator based on a novel electrostatic wiggler</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nikrah, M.; Jafari, S.</p> <p>2016-06-01</p> <p>We expand here a theory of a high-gradient laser-excited <span class="hlt">electron</span> accelerator based on an inverse free-<span class="hlt">electron</span> laser (inverse-FEL), but with innovations in the structure and design. The electrostatic wiggler used in our scheme, namely termed the Paul wiggler, is generated by segmented cylindrical electrodes with applied oscillatory voltages {{V}\\text{osc}}(t) over {{90}\\circ} segments. The inverse-FEL interaction can be described by the equations that govern the <span class="hlt">electron</span> motion in the combined fields of both the laser pulse and Paul wiggler field. A numerical study of <span class="hlt">electron</span> <span class="hlt">energy</span> and <span class="hlt">electron</span> trajectories has been made using the fourth-order Runge-Kutta method. The results indicate that the <span class="hlt">electron</span> attains a considerable <span class="hlt">energy</span> at short distances in this device. It is found that if the <span class="hlt">electron</span> has got sufficient suitable wiggler amplitude intensities, it can not only gain higher <span class="hlt">energy</span> in longer distances, but also can retain it even after the passing of the laser pulse. In addition, the results reveal that the <span class="hlt">electron</span> <span class="hlt">energy</span> gains different peaks for different initial axial velocities, so that a suitable small initial axial velocity of e-beam produces substantially high <span class="hlt">energy</span> gain. With regard to the transverse confinement of the <span class="hlt">electron</span> beam in a Paul wiggler, there is no applied axial guide magnetic field in this device.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..12.8909M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12.8909M"><span>Survey of upper <span class="hlt">band</span> chorus and ECH waves: Implications for the diffuse aurora</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Meredith, Nigel; Horne, Richard; Thorne, Richard; Anderson, Roger</p> <p>2010-05-01</p> <p>The origin of the diffuse aurora has been a source of controversy for many years. More recently the question has taken a new significance in view of the associated changes in atmospheric chemistry which may affect the middle atmosphere. Here we use CRRES data to assess the importance of upper <span class="hlt">band</span> chorus and <span class="hlt">electron</span> cyclotron harmonic (ECH) waves in the production of the diffuse aurora. Both wave modes increase with increasing geomagnetic activity, suggesting they are related to periods of enhanced convection and/or substorm activity. They are confined to the near-equatorial region which excludes the pre-noon sector from the wave survey. During active conditions intense ECH waves and upper <span class="hlt">band</span> chorus, with amplitudes exceeding 1 mVm-1, are observed in the region 4 < L < 7 from 2100 to 0600 MLT approximately 20% and 6% of the time respectively. This suggests that both wave modes can put <span class="hlt">electrons</span> on strong diffusion, but only during active conditions and not at all local times. Scattering rates fall below the strong diffusion limit at other times when the wave amplitudes are weaker. Fluxes of low <span class="hlt">energy</span> <span class="hlt">electrons</span> (100 eV < E < 30 keV) also increase with increasing geomagnetic activity in approximately the same region of geospace as the waves, suggesting that these <span class="hlt">electrons</span> are responsible for the generation of the waves. The patterns of the upper <span class="hlt">band</span> chorus, ECH waves and low <span class="hlt">energy</span> <span class="hlt">electrons</span> are similar to the global morphology of the diffuse aurora, suggesting that both wave modes play significant roles in the production of the diffuse aurora.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1022533','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1022533"><span>Insights on the Cuprate High <span class="hlt">Energy</span> Anomaly Observed in ARPES</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Moritz, Brian</p> <p>2011-08-16</p> <p>Recently, angle-resolved photoemission spectroscopy has been used to highlight an anomalously large <span class="hlt">band</span> renormalization at high binding <span class="hlt">energies</span> in cuprate superconductors: the high <span class="hlt">energy</span> 'waterfall' or high <span class="hlt">energy</span> anomaly (HEA). The anomaly is present for both hole- and <span class="hlt">electron</span>-doped cuprates as well as the half-filled parent insulators with different <span class="hlt">energy</span> scales arising on either side of the phase diagram. While photoemission matrix elements clearly play a role in changing the aesthetic appearance of the <span class="hlt">band</span> dispersion, i.e. creating a 'waterfall'-like appearance, they provide an inadequate description for the physics that underlies the strong <span class="hlt">band</span> renormalization giving rise to the HEA.more » Model calculations of the single-<span class="hlt">band</span> Hubbard Hamiltonian showcase the role played by correlations in the formation of the HEA and uncover significant differences in the HEA <span class="hlt">energy</span> scale for hole- and <span class="hlt">electron</span>-doped cuprates. In addition, this approach properly captures the transfer of spectral weight accompanying doping in a correlated material and provides a unifying description of the HEA across both sides of the cuprate phase diagram. We find that the anomaly demarcates a transition, or cross-over, from a quasiparticle <span class="hlt">band</span> at low binding <span class="hlt">energies</span> near the Fermi level to valence <span class="hlt">bands</span> at higher binding <span class="hlt">energy</span>, assumed to be of strong oxygen character.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25204839','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25204839"><span><span class="hlt">Energy</span>-filtered cold <span class="hlt">electron</span> transport at room temperature.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bhadrachalam, Pradeep; Subramanian, Ramkumar; Ray, Vishva; Ma, Liang-Chieh; Wang, Weichao; Kim, Jiyoung; Cho, Kyeongjae; Koh, Seong Jin</p> <p>2014-09-10</p> <p>Fermi-Dirac <span class="hlt">electron</span> thermal excitation is an intrinsic phenomenon that limits functionality of various <span class="hlt">electron</span> systems. Efforts to manipulate <span class="hlt">electron</span> thermal excitation have been successful when the entire system is cooled to cryogenic temperatures, typically <1 K. Here we show that <span class="hlt">electron</span> thermal excitation can be effectively suppressed at room temperature, and <span class="hlt">energy</span>-suppressed <span class="hlt">electrons</span>, whose <span class="hlt">energy</span> distribution corresponds to an effective <span class="hlt">electron</span> temperature of ~45 K, can be transported throughout device components without external cooling. This is accomplished using a discrete level of a quantum well, which filters out thermally excited <span class="hlt">electrons</span> and permits only <span class="hlt">energy</span>-suppressed <span class="hlt">electrons</span> to participate in <span class="hlt">electron</span> transport. The quantum well (~2 nm of Cr2O3) is formed between source (Cr) and tunnelling barrier (SiO2) in a double-barrier-tunnelling-junction structure having a quantum dot as the central island. Cold <span class="hlt">electron</span> transport is detected from extremely narrow differential conductance peaks in <span class="hlt">electron</span> tunnelling through CdSe quantum dots, with full widths at half maximum of only ~15 mV at room temperature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4175579','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4175579"><span><span class="hlt">Energy</span>-filtered cold <span class="hlt">electron</span> transport at room temperature</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Bhadrachalam, Pradeep; Subramanian, Ramkumar; Ray, Vishva; Ma, Liang-Chieh; Wang, Weichao; Kim, Jiyoung; Cho, Kyeongjae; Koh, Seong Jin</p> <p>2014-01-01</p> <p>Fermi-Dirac <span class="hlt">electron</span> thermal excitation is an intrinsic phenomenon that limits functionality of various <span class="hlt">electron</span> systems. Efforts to manipulate <span class="hlt">electron</span> thermal excitation have been successful when the entire system is cooled to cryogenic temperatures, typically <1 K. Here we show that <span class="hlt">electron</span> thermal excitation can be effectively suppressed at room temperature, and <span class="hlt">energy</span>-suppressed <span class="hlt">electrons</span>, whose <span class="hlt">energy</span> distribution corresponds to an effective <span class="hlt">electron</span> temperature of ~45 K, can be transported throughout device components without external cooling. This is accomplished using a discrete level of a quantum well, which filters out thermally excited <span class="hlt">electrons</span> and permits only <span class="hlt">energy</span>-suppressed <span class="hlt">electrons</span> to participate in <span class="hlt">electron</span> transport. The quantum well (~2 nm of Cr2O3) is formed between source (Cr) and tunnelling barrier (SiO2) in a double-barrier-tunnelling-junction structure having a quantum dot as the central island. Cold <span class="hlt">electron</span> transport is detected from extremely narrow differential conductance peaks in <span class="hlt">electron</span> tunnelling through CdSe quantum dots, with full widths at half maximum of only ~15 mV at room temperature. PMID:25204839</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28880064','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28880064"><span>Fullerene-Free Organic Solar Cells with an Efficiency of 10.2% and an <span class="hlt">Energy</span> Loss of 0.59 eV Based on a Thieno[3,4-c]Pyrrole-4,6-dione-Containing Wide <span class="hlt">Band</span> Gap Polymer Donor.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hadmojo, Wisnu Tantyo; Wibowo, Febrian Tri Adhi; Ryu, Du Yeol; Jung, In Hwan; Jang, Sung-Yeon</p> <p>2017-09-27</p> <p>Although the combination of wide <span class="hlt">band</span> gap polymer donors and narrow <span class="hlt">band</span> gap small-molecule acceptors achieved state-of-the-art performance as bulk heterojunction (BHJ) active layers for organic solar cells, there have been only several of the wide <span class="hlt">band</span> gap polymers that actually realized high-efficiency devices over >10%. Herein, we developed high-efficiency, low-<span class="hlt">energy</span>-loss fullerene-free organic solar cells using a weakly crystalline wide <span class="hlt">band</span> gap polymer donor, PBDTTPD-HT, and a nonfullerene small-molecule acceptor, ITIC. The excessive intermolecular stacking of ITIC is efficiently suppressed by the miscibility with PBDTTPD-HT, which led to a well-balanced nanomorphology in the PBDTTPD-HT/ITIC BHJ active films. The favorable optical, <span class="hlt">electronic</span>, and energetic properties of PBDTTPD-HT with respect to ITIC achieved panchromatic photon-to-current conversion with a remarkably low <span class="hlt">energy</span> loss (0.59 eV).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015APS..GECGT1091P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015APS..GECGT1091P"><span>Numerical <span class="hlt">band</span> structure calculations of plasma metamaterials</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pederson, Dylan; Kourtzanidis, Konstantinos; Raja, Laxminarayan</p> <p>2015-09-01</p> <p>Metamaterials (MM) are materials engineered to display negative macroscopic permittivity and permeability. These materials allow for designed control over electromagnetic <span class="hlt">energy</span> flow, especially at frequencies where natural materials do not interact. Plasmas have recently found application in MM as a negative permittivity component. The permittivity of a plasma depends on its <span class="hlt">electron</span> density, which can be controlled by an applied field. This means that plasmas can be used in MM to actively control the transmission or reflection of incident waves. This work focuses on a plasma MM geometry in which microplasmas are generated in perforations in a metal plate. We characterizethis material by its <span class="hlt">band</span> structure, which describes its interaction with incident waves. The plasma-EM interactions are obtained by coupling Maxwell's equations to a simplified plasma momentum equation. A plasma density profile is prescribed, and its effect on the <span class="hlt">band</span> structure is investigated. The <span class="hlt">band</span> structure calculations are typically done for static structures, whereas our current density responds to the incident waves. The resulting <span class="hlt">band</span> structures are compared with experimental results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..MARC21004L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..MARC21004L"><span>Molecularly Stretchable <span class="hlt">Electronics</span> for <span class="hlt">Energy</span> and Healthcare</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lipomi, Darren</p> <p></p> <p>The term ``plastic <span class="hlt">electronics</span>'' masks the wide range of mechanical behavior possessed by films of π-conjugated (semiconducting) small molecules and polymers. Such materials are promising for biosensors, large-area displays, low-<span class="hlt">energy</span> lighting, and low-cost photovoltaic modules. There is also an apparent trade-off between <span class="hlt">electronic</span> performance and mechanical compliance in films of some of the best-performing semiconducting polymers, which fracture at tensile strains not significantly greater than those at which conventional inorganic semiconductors fail. The design of intrinsically deformable <span class="hlt">electronic</span> materials-i.e., imagine a semiconducting rubber <span class="hlt">band</span>-would facilitate roll-to-roll production, mechanical robustness for potable applications, and conformal bonding to curved surfaces. This seminar describes my group's efforts to understand and control the structural parameters that influence the mechanical properties of π-conjugated polymers. The techniques we employ include synthetic chemistry, spectroscopy and microstructural characterization, computation from the molecular to continuum level, and electrical measurements of devices. A complex picture emerges for the interplay between molecular structure, the way the process of solidification influences the morphology, and how molecular structure and morphology combine to produce a film with a given modulus, elastic range, ductility, and toughness. We are also exploring ways to introduce other properties into organic semiconductors that are inspired by biological tissue. That is, not just elasticity and toughness, but also biodegradability and the capacity for self-repair. The seminar will also touch on our use of self-assembled metallic nanoislands on graphene for ultra-sensitive mechanical sensing using piezoresistive and ``piezoplasmonic'' mechanisms. The applications for these materials are in detecting human motion and measuring the mechanics of cardiac and musculoskeletal cells. My group is broadly</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1998CoTPh..30..381C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998CoTPh..30..381C"><span>Balance-Equation Approach to Nonuniform <span class="hlt">Electron</span> Transport in Nonparabolic Semiconductors</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cao, Juncheng; Lei, Xiaolin</p> <p>1998-10-01</p> <p>On the basis of the Lei-Ting balance-equation transport theory recently developed for nonparabolic <span class="hlt">energy</span> <span class="hlt">band</span>, we propose a hydrodynamic approach to the spatially inhomogeneous <span class="hlt">electron</span> transport in semiconductor devices. In the present approach, the momentum and <span class="hlt">energy</span> collision terms are expressed by two nonlinear functions, the frictional acceleration and <span class="hlt">energy</span>-loss rate, which give a detailed scattering-process-level description of nonstationary and nonlocal charge transport in the system. This approach allows one to calculate selfconsistently the transport parameters within the model itself based on the primary material data (<span class="hlt">band</span> structure, deformation potential constant, etc.), thus it minimizes the uncertainty associated with the use of some empirical relations for transport coefficients. As a demonstration of the approach, we have carried out a numerical calculation for a submicrometer Si n^+nn^+ diode by assuming an isotropic Kane-type <span class="hlt">energy</span> <span class="hlt">band</span>. The results for <span class="hlt">electron</span> velocity and <span class="hlt">energy</span>, obtained at much less computing cost than the Monte-Carlo (MC) method, are in good agreement with MC prediction. The influence of heat-flow term on <span class="hlt">electron</span> transport behaviour, especially on velocity overshoot, is also investigated. The project supported by National Natural Science Foundation of China, National and Shanghai Municipal Commission of Science and Technology, and the Shanghai Foundation for Research and Development of Applied Materials</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22482079-type-band-alignment-gaas-sub-sb-sub-gaas-core-shell-nanowires','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22482079-type-band-alignment-gaas-sub-sb-sub-gaas-core-shell-nanowires"><span>Type I <span class="hlt">band</span> alignment in GaAs{sub 81}Sb{sub 19}/GaAs core-shell nanowires</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Xu, T.; Key Laboratory of Advanced Display and System Application, Shanghai University, 149 Yanchang Road, Shanghai 200072; Wei, M. J.</p> <p>2015-09-14</p> <p>The composition and <span class="hlt">band</span> gap of the shell that formed during the growth of axial GaAs/GaAs{sub 81}Sb{sub 19}/ GaAs heterostructure nanowires have been investigated by transmission <span class="hlt">electron</span> microscopy combined with <span class="hlt">energy</span> dispersion spectroscopy, scanning tunneling spectroscopy, and density functional theory calculations. On the GaAs{sub 81}Sb{sub 19} intermediate segment, the shell is found to be free of Sb (pure GaAs shell) and transparent to the tunneling <span class="hlt">electrons</span>, despite the (110) biaxial strain that affects its <span class="hlt">band</span> gap. As a result, a direct measurement of the core <span class="hlt">band</span> gap allows the quantitative determination of the <span class="hlt">band</span> offset between the GaAs{sub 81}Sb{sub 19}more » core and the GaAs shell and identifies it as a type I <span class="hlt">band</span> alignment.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=foam&pg=5&id=EJ546509','ERIC'); return false;" href="https://eric.ed.gov/?q=foam&pg=5&id=EJ546509"><span>Housing <span class="hlt">Electrons</span>: Relating Quantum Numbers, <span class="hlt">Energy</span> Levels, and <span class="hlt">Electron</span> Configurations.</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Garofalo, Anthony</p> <p>1997-01-01</p> <p>Presents an activity that combines the concepts of quantum numbers and probability locations, <span class="hlt">energy</span> levels, and <span class="hlt">electron</span> configurations in a concrete, hands-on way. Uses model houses constructed out of foam board and colored beads to represent <span class="hlt">electrons</span>. (JRH)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28766610','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28766610"><span>Optical properties and magnetic flux-induced <span class="hlt">electronic</span> <span class="hlt">band</span> tuning of a T-graphene sheet and nanoribbon.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bandyopadhyay, Arka; Nandy, Atanu; Chakrabarti, Arunava; Jana, Debnarayan</p> <p>2017-08-16</p> <p>Tetragonal graphene (T-graphene) is a theoretically proposed dynamically stable, metallic allotrope of graphene. In this theoretical investigation, a tight binding (TB) model is used to unravel the metal to semiconductor transition of this 2D sheet under the influence of an external magnetic flux. In addition, the environment under which the sheet exposes an appreciable direct <span class="hlt">band</span> gap of 1.41 ± 0.01 eV is examined. Similarly, the <span class="hlt">electronic</span> <span class="hlt">band</span> structure of the narrowest armchair T-graphene nanoribbon (NATGNR) also gets modified with different combinations of magnetic fluxes through the elementary rings. The <span class="hlt">band</span> tuning parameters are critically identified for both systems. It is observed that the induced <span class="hlt">band</span> gaps vary remarkably with the tuning parameters. We have also introduced an exact analytical approach to address the <span class="hlt">band</span> structure of the NATGNR in the absence of any magnetic flux. Finally, the optical properties of the sheet and NATGNR are also critically analysed for both parallel and perpendicular polarizations with the help of density functional theory (DFT). Our study predicts that this material and its nanoribbons can be used in optoelectronic devices.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..DPPB10100G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..DPPB10100G"><span><span class="hlt">Energy</span> Conversion Mechanism for <span class="hlt">Electron</span> Perpendicular <span class="hlt">Energy</span> in High Guide-Field Reconnection</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Guo, Xuehan; Horiuchi, Ritoku; Kaminou, Yasuhiro; Cheng, Frank; Ono, Yasushi</p> <p>2016-10-01</p> <p>The <span class="hlt">energy</span> conversion mechanism for <span class="hlt">electron</span> perpendicular <span class="hlt">energy</span>, both the thermal and the kinetic <span class="hlt">energy</span>, is investigated by means of two-dimensional, full-particle simulations in an open system. It is shown that <span class="hlt">electron</span> perpendicular heating is mainly due to the breaking of magnetic moment conservation in separatrix region because the charge separation generates intense variation of electric field within the <span class="hlt">electron</span> Larmor radius. Meanwhile, <span class="hlt">electron</span> perpendicular acceleration takes place manly due to the polarization drift term as well as the curvature drift term of E . u⊥ in the downstream near the X-point. The enhanced electric field due to the charge separation there results in a significant effect of the polarization drift term on the dissipation of magnetic <span class="hlt">energy</span> within the ion inertia length in the downstream. Japan Society for the Promotion of Science (JSPS) Fellows 15J03758.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25166690','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25166690"><span>Direct measurement of the thickness-dependent <span class="hlt">electronic</span> <span class="hlt">band</span> structure of MoS2 using angle-resolved photoemission spectroscopy.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jin, Wencan; Yeh, Po-Chun; Zaki, Nader; Zhang, Datong; Sadowski, Jerzy T; Al-Mahboob, Abdullah; van der Zande, Arend M; Chenet, Daniel A; Dadap, Jerry I; Herman, Irving P; Sutter, Peter; Hone, James; Osgood, Richard M</p> <p>2013-09-06</p> <p>We report on the evolution of the thickness-dependent <span class="hlt">electronic</span> <span class="hlt">band</span> structure of the two-dimensional layered-dichalcogenide molybdenum disulfide (MoS2). Micrometer-scale angle-resolved photoemission spectroscopy of mechanically exfoliated and chemical-vapor-deposition-grown crystals provides direct evidence for the shifting of the valence <span class="hlt">band</span> maximum from Γ to K, for the case of MoS2 having more than one layer, to the case of single-layer MoS2, as predicted by density functional theory. This evolution of the <span class="hlt">electronic</span> structure from bulk to few-layer to monolayer MoS2 had earlier been predicted to arise from quantum confinement. Furthermore, one of the consequences of this progression in the <span class="hlt">electronic</span> structure is the dramatic increase in the hole effective mass, in going from bulk to monolayer MoS2 at its Brillouin zone center, which is known as the cause for the decreased carrier mobility of the monolayer form compared to that of bulk MoS2.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JPhD...51u5102B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JPhD...51u5102B"><span><span class="hlt">Band</span>-edges and <span class="hlt">band</span>-gap in few-layered transition metal dichalcogenides</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bhunia, Hrishikesh; Pal, Amlan J.</p> <p>2018-05-01</p> <p>We have considered liquid-exfoliated transition metal dichalcogenides (WS2, WSe2, MoS2, and MoSe2) and studied their <span class="hlt">band</span>-edges and <span class="hlt">band</span>-gap through scanning tunneling spectroscopy (STS) and density of states. A monolayer, bilayer (2L), and trilayer (3L) of each of the layered materials were characterized to derive the <span class="hlt">energies</span>. Upon an increase in the number of layers, both the <span class="hlt">band</span>-edges were found to shift towards the Fermi <span class="hlt">energy</span>. The results from the exfoliated nanosheets have been compared with reported STS studies of MoS2 and WSe2 formed through chemical vapor deposition or molecular beam epitaxy methods; an uncontrolled lattice strain existed in such 2L and 3L nanoflakes due to mismatch in stacking-patterns between the monolayers affecting their <span class="hlt">energies</span>. In the present work, the layers formed through the liquid-exfoliation process retained their interlayer coupling or stacking-sequence prevalent to the bulk and hence allowed determination of <span class="hlt">band-energies</span> in these strain-free two-dimensional materials.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24116568','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24116568"><span>New analytical model for the ozone <span class="hlt">electronic</span> ground state potential surface and accurate ab initio vibrational predictions at high <span class="hlt">energy</span> range.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tyuterev, Vladimir G; Kochanov, Roman V; Tashkun, Sergey A; Holka, Filip; Szalay, Péter G</p> <p>2013-10-07</p> <p>An accurate description of the complicated shape of the potential <span class="hlt">energy</span> surface (PES) and that of the highly excited vibration states is of crucial importance for various unsolved issues in the spectroscopy and dynamics of ozone and remains a challenge for the theory. In this work a new analytical representation is proposed for the PES of the ground <span class="hlt">electronic</span> state of the ozone molecule in the range covering the main potential well and the transition state towards the dissociation. This model accounts for particular features specific to the ozone PES for large variations of nuclear displacements along the minimum <span class="hlt">energy</span> path. The impact of the shape of the PES near the transition state (existence of the "reef structure") on vibration <span class="hlt">energy</span> levels was studied for the first time. The major purpose of this work was to provide accurate theoretical predictions for ozone vibrational <span class="hlt">band</span> centres at the <span class="hlt">energy</span> range near the dissociation threshold, which would be helpful for understanding the very complicated high-resolution spectra and its analyses currently in progress. Extended ab initio <span class="hlt">electronic</span> structure calculations were carried out enabling the determination of the parameters of a minimum <span class="hlt">energy</span> path PES model resulting in a new set of theoretical vibrational levels of ozone. A comparison with recent high-resolution spectroscopic data on the vibrational levels gives the root-mean-square deviations below 1 cm(-1) for ozone <span class="hlt">band</span> centres up to 90% of the dissociation <span class="hlt">energy</span>. New ab initio vibrational predictions represent a significant improvement with respect to all previously available calculations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JAP...121p4902R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JAP...121p4902R"><span>V-<span class="hlt">band</span> <span class="hlt">electronically</span> reconfigurable metamaterial</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Radisic, Vesna; Hester, Jimmy G.; Nguyen, Vinh N.; Caira, Nicholas W.; DiMarzio, Donald; Hilgeman, Theodore; Larouche, Stéphane; Kaneshiro, Eric; Gutierrez-Aitken, Augusto</p> <p>2017-04-01</p> <p>In this work, we report on a reconfigurable V-<span class="hlt">band</span> metamaterial fabricated using an InP heterojunction bipolar transistor production process. As designed and fabricated, the implementation uses complementary split ring resonators (cSRRs) and Schottky diodes in both single unit cell and three unit cell monolithic microwave integrated circuits. Each unit cell has two diodes embedded within the gaps of the cSRRs. Reconfigurability is achieved by applying an external bias that turns the diodes on and off, which effectively controls the resonant property of the structure. In order to measure the metamaterial properties, the unit cells are fed and followed by transmission lines. Measured data show good agreement with simulations and demonstrate that the metamaterial structure exhibits resonance at around 65 GHz that can be switched on and off. The three-unit cell transmission line metamaterial shows a deeper resonance and a larger phase change than a single cell, as expected. These are the first reported reconfigurable metamaterials operating at the V-<span class="hlt">band</span> using the InP high speed device fabrication process.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28753018','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28753018"><span>Temperature-Induced Large Broadening and Blue Shift in the <span class="hlt">Electronic</span> <span class="hlt">Band</span> Structure and Optical Absorption of Methylammonium Lead Iodide Perovskite.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yang, Jia-Yue; Hu, Ming</p> <p>2017-08-17</p> <p>The power conversion efficiency of hybrid halide perovskite solar cells is profoundly influenced by the operating temperature. Here we investigate the temperature influence on the <span class="hlt">electronic</span> <span class="hlt">band</span> structure and optical absorption of cubic CH 3 NH 3 PbI 3 from first-principles by accounting for both the <span class="hlt">electron</span>-phonon interaction and thermal expansion. Within the framework of density functional perturbation theory, the <span class="hlt">electron</span>-phonon coupling induces slightly enlarged <span class="hlt">band</span> gap and strongly broadened <span class="hlt">electronic</span> relaxation time as temperature increases. The large broadening effect is mainly due to the presence of cation organic atoms. Consequently, the temperature-dependent absorption peak exhibits blue-shift position, decreased amplitude, and broadened width. This work uncovers the atomistic origin of temperature influence on the optical absorption of cubic CH 3 NH 3 PbI 3 and can provide guidance to design high-performance hybrid halide perovskite solar cells at different operating temperatures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002APS..MARU22003T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002APS..MARU22003T"><span>Temperature dependent dispersion and <span class="hlt">electron</span>-phonon coupling surface states on Be(1010)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tang, Shu-Jung; Ismail; Sprunger, Philip; Plummer, Ward</p> <p>2002-03-01</p> <p>Temperature dependent dispersion and <span class="hlt">electron</span>-phonon coupling surface states on Be(10-10) S.-J Tang*, Ismail* , P.T . Sprunger#, E. W. Plummer* * Department of Physics and Astronomy, University of Tennessee, Knoxville, TN37996 , # Center for Advanced Microstructures and Devices (CAMD), Louisiana State University The surface states dispersing in a large <span class="hlt">band</span> gap from -A to -Γ in Be(10-10) were studied with high-resolution, angle-resolved photoemission. Spectra reveal that the two zone-boundary surface states, S1 and S2, behave significantly different with respect to <span class="hlt">band</span> dispersion, the temperature dependence of binding <span class="hlt">energies</span>, and the <span class="hlt">electron</span>-phonon coupling. The <span class="hlt">band</span> dispersion of S1 is purely free-<span class="hlt">electron</span> like with the maximum binding <span class="hlt">energy</span> of 0.37+-0.05 eV at -A and effective mass m*/m =0835. However, the maximum binding <span class="hlt">energy</span> 2.74+-0.05 eV of the S2 is located 0.2Åaway from -A and disperses into the bulk <span class="hlt">band</span> edge at a binding <span class="hlt">energy</span> of 1.75+-0.05 eV. Temperature dependent data reveal that the binding <span class="hlt">energies</span> of S1 and S2 at -A shift in opposite directions at the rate of (-0.61+-0.3)+- 10E-4 eV/K and (1.71+-0.8)+-10E-4 eV/K, respectively. Moreover, from the temperature-dependent spectral widths of the surface states S1 and S2 at , the <span class="hlt">electron</span>-phonon coupling parameters,λ, have been determined. Unusually different, the coupling strength λ for S1 and S2 are 0.67+-0.03 and 0.51+-0.04, respectively. The differences between the <span class="hlt">electron</span>-phonon coupling, temperature dependent binding <span class="hlt">energies</span>, and dispersions between these two zone-centered surface states will be discussed in light unique bonding at the surface and localization.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_24 --> <div id="page_25" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li class="active"><span>25</span></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="481"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhPl...25e3104Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhPl...25e3104Z"><span>Investigation on the optimal magnetic field of a cusp <span class="hlt">electron</span> gun for a W-<span class="hlt">band</span> gyro-TWA</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Liang; He, Wenlong; Donaldson, Craig R.; Cross, Adrian W.</p> <p>2018-05-01</p> <p>High efficiency and broadband operation of a gyrotron traveling wave amplifier (gyro-TWA) require a high-quality <span class="hlt">electron</span> beam with low-velocity spreads. The beam velocity spreads are mainly due to the differences of the electric and magnetic fields that the <span class="hlt">electrons</span> withstand the <span class="hlt">electron</span> gun. This paper investigates the possibility to decouple the design of <span class="hlt">electron</span> gun geometry and the magnet system while still achieving optimal results, through a case study of designing a cusp <span class="hlt">electron</span> gun for a W-<span class="hlt">band</span> gyro-TWA. A global multiple-objective optimization routing was used to optimize the <span class="hlt">electron</span> gun geometry for different predefined magnetic field profiles individually. Their results were compared and the properties of the required magnetic field profile are summarized.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22600107-electron-energy-distribution-function-effective-electron-temperature-dust-charge-temporal-afterglow-plasma','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22600107-electron-energy-distribution-function-effective-electron-temperature-dust-charge-temporal-afterglow-plasma"><span><span class="hlt">Electron</span> <span class="hlt">energy</span> distribution function, effective <span class="hlt">electron</span> temperature, and dust charge in the temporal afterglow of a plasma</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Denysenko, I. B.; Azarenkov, N. A.; Kersten, H.</p> <p>2016-05-15</p> <p>Analytical expressions describing the variation of <span class="hlt">electron</span> <span class="hlt">energy</span> distribution function (EEDF) in an afterglow of a plasma are obtained. Especially, the case when the <span class="hlt">electron</span> <span class="hlt">energy</span> loss is mainly due to momentum-transfer <span class="hlt">electron</span>-neutral collisions is considered. The study is carried out for different EEDFs in the steady state, including Maxwellian and Druyvesteyn distributions. The analytical results are not only obtained for the case when the rate for momentum-transfer <span class="hlt">electron</span>-neutral collisions is independent on <span class="hlt">electron</span> <span class="hlt">energy</span> but also for the case when the collisions are a power function of <span class="hlt">electron</span> <span class="hlt">energy</span>. Using analytical expressions for the EEDF, the effective <span class="hlt">electron</span> temperaturemore » and charge of the dust particles, which are assumed to be present in plasma, are calculated for different afterglow durations. An analytical expression for the rate describing collection of <span class="hlt">electrons</span> by dust particles for the case when the rate for momentum-transfer <span class="hlt">electron</span>-neutral collisions is independent on <span class="hlt">electron</span> <span class="hlt">energy</span> is also derived. The EEDF profile and, as a result, the effective <span class="hlt">electron</span> temperature and dust charge are sufficiently different in the cases when the rate for momentum-transfer <span class="hlt">electron</span>-neutral collisions is independent on <span class="hlt">electron</span> <span class="hlt">energy</span> and when the rate is a power function of <span class="hlt">electron</span> <span class="hlt">energy</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018A%26A...612A.106S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018A%26A...612A.106S"><span><span class="hlt">Energy</span> distribution of relativistic <span class="hlt">electrons</span> in the kiloparsec scale jet of M 87 with Chandra</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sun, Xiao-Na; Yang, Rui-Zhi; Rieger, Frank M.; Liu, Ruo-Yu; Aharonian, Felix</p> <p>2018-05-01</p> <p>The X-ray emission from the jets in active galactic nuclei (AGN) carries important information on the distributions of relativistic <span class="hlt">electrons</span> and magnetic fields on large scales. We reanalysed archival Chandra observations on the jet of M 87 from 2000 to 2016 with a total exposure of 1460 kiloseconds to explore the X-ray emission characteristics along the jet. We investigated the variability behaviours of the nucleus and the inner jet component HST-1, and confirm indications for day-scale X-ray variability in the nucleus contemporaneous to the 2010 high TeV γ-ray state. HST-1 shows a general decline in X-ray flux over the last few years consistent with its synchrotron interpretation. We extracted the X-ray spectra for the nucleus and all knots in the jet, showing that they are compatible with a single power law within the X-ray <span class="hlt">band</span>. There are indications that the resultant X-ray photon index exhibit a trend, with slight but significant index variations ranging from ≃ 2.2 (e.g. in knot D) to ≃ 2.4-2.6 (in the outer knots F, A, and B). When viewed in a multiwavelength context, a more complex situation can be seen. Fitting the radio to X-ray spectral <span class="hlt">energy</span> distributions (SEDs) assuming a synchrotron origin, we show that a broken power-law <span class="hlt">electron</span> spectrum with break <span class="hlt">energy</span> Eb around 1 (300 μG/B)1/2 TeV allows a satisfactory description of the multiband SEDs for most of the knots. However, in the case of knots B, C, and D we find indications that an additional high-<span class="hlt">energy</span> component is needed to adequately reproduce the broad-<span class="hlt">band</span> SEDs. We discuss the implications and suggest that a stratified jet model may account for the differences.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19850026468','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19850026468"><span>The <span class="hlt">Energy</span> Spectrum of Jovian <span class="hlt">Electrons</span> in Interplanetary Space</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Christon, S. P.; Cummings, A. C.; Stone, E. C.; Webber, W. R.</p> <p>1985-01-01</p> <p>The <span class="hlt">energy</span> spectrum of <span class="hlt">electrons</span> with <span class="hlt">energies</span> approx 10 to approx 180 MeV measured with the <span class="hlt">electron</span> telescope on the Voyager 1 and 2 spacecraft in interplanetary space from 1978 to 1983 is studied. The kinetic <span class="hlt">energy</span> of <span class="hlt">electrons</span> is determined by double dE/dx measurements from the first two detectors (D sub 1, D sub 2) of a stack of eight solid state detectors and by the range of particle penetration into the remaining six detectors (D sub 3 to D sub 8) which are interleaved with tungsten absorbers. From 1978 to 1983 (radial range approximately 2 to a pproximately 12 AU) <span class="hlt">electrons</span> of Jovian origin were clearly observable for <span class="hlt">electrons</span> stopping in D(sub 3(E approximately greater than 4 MeV)) and in D(sub 4 (E approximately greater than 8 MeV)). For <span class="hlt">electrons</span> stopping in D(sub 5(E approximately greather than 12 MeV)), the jovian flux dominated the galactic <span class="hlt">electron</span> flux for a period of approximately one year near the encounter with Jupiter. Jovian <span class="hlt">electrons</span> were also observed in D(sub 6(E approximately greater than 21 MeV)) but not in D(sub 7(E approximately greater than 28 MeV)). A detailed interpretation of the <span class="hlt">electron</span> variations in all <span class="hlt">energy</span> channels depends on an accurate subtraction of background induced by energetic protons of a few 100 MeV. This substraction is facilitated by laboratory calibration results at several <span class="hlt">energies</span>. Further results on the differential <span class="hlt">energy</span> spectrum of Jovian <span class="hlt">electrons</span> and limits on the maximum detected <span class="hlt">energies</span> will be reported.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EPJAP..7320301Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EPJAP..7320301Y"><span><span class="hlt">Energy</span> <span class="hlt">band</span> and transport properties in magnetic aperiodic graphene superlattices of Thue-Morse sequence</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yin, Yiheng; Niu, Yanxiong; Zhang, Huiyun; Zhang, Yuping; Liu, Haiyue</p> <p>2016-02-01</p> <p>Utilizing the transfer matrix method, we develop the <span class="hlt">electronic</span> <span class="hlt">band</span> structure and transport properties in Thue-Morse aperiodic graphene superlattices with magnetic barriers. It is found that the normal transmission is blocked and the position of the Dirac point can be shifted along the wavevector axis by changing the height and width ratio of magnetic barriers, which is intrinsic different from <span class="hlt">electronic</span> field modulated superlattices. In addition, the angular threshold property of the transmission spectra and the oscillatory property of the conductance have been studied.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvB..97p5421L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvB..97p5421L"><span>Probing quasi-one-dimensional <span class="hlt">band</span> structures by plasmon spectroscopy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lichtenstein, T.; Mamiyev, Z.; Braun, C.; Sanna, S.; Schmidt, W. G.; Tegenkamp, C.; Pfnür, H.</p> <p>2018-04-01</p> <p>The plasmon dispersion is inherently related to the continuum of <span class="hlt">electron</span>-hole pair excitations. Therefore, the comparison of this continuum, as derived from <span class="hlt">band</span> structure calculations, with experimental data of plasmon dispersion, can yield direct information about the form of the occupied as well as the unoccupied <span class="hlt">band</span> structure in the vicinity of the Fermi level. The relevance of this statement is illustrated by a detailed analysis of plasmon dispersions in quasi-one-dimensional systems combining experimental <span class="hlt">electron</span> <span class="hlt">energy</span> loss spectroscopy with quantitative density-functional theory (DFT) calculations. Si(557)-Au and Si(335)-Au with single atomic chains per terrace are compared with the Si(775)-Au system, which has a double Au chain on each terrace. We demonstrate that both hybridization between Si surface states and the Au chains as well as <span class="hlt">electronic</span> correlations lead to increasing deviations from the nearly free <span class="hlt">electron</span> picture that is suggested by a too simple interpretation of data of angular resolved photoemission (ARPES) of these systems, particularly for the double chain system. These deviations are consistently predicted by the DFT calculations. Thus also dimensional crossover can be explained.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ApPhL.112q1605Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ApPhL.112q1605Z"><span>Interface <span class="hlt">energy</span> <span class="hlt">band</span> alignment at the all-transparent p-n heterojunction based on NiO and BaSnO3</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Jiaye; Han, Shaobo; Luo, Weihuang; Xiang, Shuhuai; Zou, Jianli; Oropeza, Freddy E.; Gu, Meng; Zhang, Kelvin H. L.</p> <p>2018-04-01</p> <p>Transparent oxide semiconductors hold great promise for many optoelectronic devices such as transparent <span class="hlt">electronics</span>, UV-emitting devices, and photodetectors. A p-n heterojunction is the most ubiquitous building block to realize these devices. In this work, we report the fabrication and characterization of the interface properties of a transparent heterojunction consisting of p-type NiO and n-type perovskite BaSnO3. We show that high-quality NiO thin films can be epitaxially grown on BaSnO3 with sharp interfaces because of a small lattice mismatch (˜1.3%). The diode fabricated from this heterojunction exhibits rectifying behavior with a ratio of 500. X-ray photoelectron spectroscopy reveals a type II or "staggered" <span class="hlt">band</span> alignment with valence and conduction <span class="hlt">band</span> offsets of 1.44 eV and 1.86 eV, respectively. Moreover, a large upward <span class="hlt">band</span> bending potential of 0.90 eV for BaSnO3 and a downward <span class="hlt">band</span> bending potential of 0.15 eV for NiO were observed in the interface region. Such <span class="hlt">electronic</span> properties have important implication for optoelectronic applications as the large built-in potential provides favorable energetics for photo-generated <span class="hlt">electron</span>-hole separation/migration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017TePhL..43..998C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017TePhL..43..998C"><span>The interaction of low-<span class="hlt">energy</span> <span class="hlt">electrons</span> with fructose molecules</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chernyshova, I. V.; Kontrosh, E. E.; Markush, P. P.; Shpenik, O. B.</p> <p>2017-11-01</p> <p>Using a hypocycloidal <span class="hlt">electronic</span> spectrometer, the interactions of low <span class="hlt">energy</span> <span class="hlt">electrons</span> (0-8.50 eV) with fructose molecules, namely, <span class="hlt">electron</span> scattering and dissociative attachment, are studied. The results of these studies showed that the fragmentation of fructose molecules occurs effectively even at an <span class="hlt">electron</span> <span class="hlt">energy</span> close to zero. In the total <span class="hlt">electron</span>-scattering cross section by molecules, resonance features (at <span class="hlt">energies</span> 3.10 and 5.00 eV) were first observed near the formation thresholds of light ion fragments OH- and H-. The correlation of the features observed in the cross sections of <span class="hlt">electron</span> scattering and dissociative attachment is analyzed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150003431','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150003431"><span>Single-<span class="hlt">Band</span> and Dual-<span class="hlt">Band</span> Infrared Detectors</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ting, David Z. (Inventor); Gunapala, Sarath D. (Inventor); Soibel, Alexander (Inventor); Nguyen, Jean (Inventor); Khoshakhlagh, Arezou (Inventor)</p> <p>2015-01-01</p> <p>Bias-switchable dual-<span class="hlt">band</span> infrared detectors and methods of manufacturing such detectors are provided. The infrared detectors are based on a back-to-back heterojunction diode design, where the detector structure consists of, sequentially, a top contact layer, a unipolar hole barrier layer, an absorber layer, a unipolar <span class="hlt">electron</span> barrier, a second absorber, a second unipolar hole barrier, and a bottom contact layer. In addition, by substantially reducing the width of one of the absorber layers, a single-<span class="hlt">band</span> infrared detector can also be formed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170004927','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170004927"><span>Single-<span class="hlt">Band</span> and Dual-<span class="hlt">Band</span> Infrared Detectors</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ting, David Z. (Inventor); Gunapala, Sarath D. (Inventor); Soibel, Alexander (Inventor); Nguyen, Jean (Inventor); Khoshakhlagh, Arezou (Inventor)</p> <p>2017-01-01</p> <p>Bias-switchable dual-<span class="hlt">band</span> infrared detectors and methods of manufacturing such detectors are provided. The infrared detectors are based on a back-to-back heterojunction diode design, where the detector structure consists of, sequentially, a top contact layer, a unipolar hole barrier layer, an absorber layer, a unipolar <span class="hlt">electron</span> barrier, a second absorber, a second unipolar hole barrier, and a bottom contact layer. In addition, by substantially reducing the width of one of the absorber layers, a single-<span class="hlt">band</span> infrared detector can also be formed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1150022','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1150022"><span>Fundamental studies of <span class="hlt">energy</span>-and hole/<span class="hlt">electron</span>- transfer in hydroporphyrin architectures</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Bocian, David F.</p> <p>2014-08-20</p> <p>The long-term objective of the Bocian/Holten/Lindsey research program is to design, synthesize, and characterize tetrapyrrole-based molecular architectures that absorb sunlight, funnel <span class="hlt">energy</span>, and separate charge with high efficiency and in a manner compatible with current and future solar-<span class="hlt">energy</span> conversion schemes. The synthetic tetrapyrroles include porphyrins and hydroporphyrins; the latter classes of molecules encompass analogues of the naturally occurring chlorophylls and bacteriochlorophylls (e.g., chlorins, bacteriochlorins, and their derivatives). The attainment of the goals of the research program requires the close interplay of molecular design and synthesis (Lindsey group), static and time-resolved optical spectroscopic measurements (Holten group), and electrochemical, <span class="hlt">electron</span> paramagnetic resonance,more » and resonance Raman studies, as well as density functional theory calculations (Bocian Group). The proposed research encompasses four interrelated themes: (1) Determination of the rates of ground-state hole/<span class="hlt">electron</span> transfer between (hydro)porphyrins in multipigment arrays as a function of array size, distance between components, linker type, site of linker connection, and frontier molecular orbital composition. (2) Examination of excited-state <span class="hlt">energy</span> transfer among hydroporphyrins in multipigment arrrays, including both pairwise and non-adjacent transfer, with a chief aim to identify the relative contributions of through-space (Förster) and through-bond (Dexter) mechanisms of <span class="hlt">energy</span> transfer, including the roles of site of linker connection and frontier molecular orbital composition. (3) Elucidation of the role of substituents in tuning the spectral and <span class="hlt">electronic</span> properties of bacteriochlorins, with a primary aim of learning how to shift the long-wavelength absorption <span class="hlt">band</span> deeper into the near-infrared region. (4) Continued development of the software package PhotochemCAD for spectral manipulations and calculations through the compilation of a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhRvP...7c4011M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvP...7c4011M"><span>Substitutional <span class="hlt">Electron</span> and Hole Doping of WSe2 : Synthesis, Electrical Characterization, and Observation of <span class="hlt">Band-to-Band</span> Tunneling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mukherjee, R.; Chuang, H. J.; Koehler, M. R.; Combs, N.; Patchen, A.; Zhou, Z. X.; Mandrus, D.</p> <p>2017-03-01</p> <p>Transition-metal dichalcogenides (TMDs) such as MoS2 , MoSe2 , and WSe2 have emerged as promising two-dimensional semiconductors. Many anticipated applications of these materials require both p -type and n -type TMDs with long-term doping stability. Here, we report on the synthesis of substitutionally doped WSe2 crystals using Nb and Re as p - and n -type dopants, respectively. Hall coefficient and gate-dependent transport measurements reveal drastically different doping properties between nominally 0.5% Nb- and 0.5% Re-doped WSe2 . While 0.5% Nb-doped WSe2 (WSe2∶Nb ) is degenerately hole doped with a nearly temperature-independent carrier density of approximately 1019 cm-3 , <span class="hlt">electrons</span> in 0.5% Re-doped WSe2 (WSe2 ∶Re ) are largely trapped in localized states below the mobility edge and exhibit thermally activated behavior. Charge transport in both WSe2∶Nb and WSe2 ∶Re is found to be limited by Coulomb scattering from ionized impurities. Furthermore, we fabricate vertical van der Waals-junction diodes consisting of multilayers of WSe2∶Nb and WSe2 ∶Re . Finally, we demonstrate reverse rectifying behavior as a direct proof of <span class="hlt">band-to-band</span> tunneling in our WSe2∶Nb /WSe2∶Re diodes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1992PhDT.......264C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1992PhDT.......264C"><span>Intramolecular <span class="hlt">Electron</span> Transfer in Bis(tetraalkyl Hydrazine) and Bis(hydrazyl) Radical Cations.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chang, Hao</p> <p></p> <p>A series of multicyclic bis(hydrazine) and bis(diazenium) compounds connected by relatively rigid hydrocarbon frameworks were prepared for the study of intramolecular <span class="hlt">electron</span> transfer. The thermodynamics of <span class="hlt">electron</span> removal of these compounds was investigated by cyclic voltammetry. The difference between the first and second oxidation potentials for the 4 sigma-bonded species was found to be larger for the bis(hydrazyl) radical systems than for the bis(hydrazines) by ca. 0.2 V (4.6 kcal/mol). This indicates a greater degree of interaction between the two nitrogen moieties for the hydrazyl systems, which is consistent with a greater degree of <span class="hlt">electronic</span> coupling (H _{rm AB}) in these systems. The ESR spectra of the 4 sigma -bonded bis(hydrazine) radical cations indicate localized radical cations, which corresponds to slow intramolecular <span class="hlt">electron</span> transfer on the ESR timescale. Conversely, the ESR spectra of the corresponding bis(hydrazyl) radical cation systems show nitrogen hyperfine splittings of a(4N) of ca. 4.5 G. This indicates that intramolecular <span class="hlt">electron</span> transfer between the two nitrogen moieties is fast on the ESR timescale; the rate of exchange, k_ {rm ex} was estimated to be well above 1.9 times 10^8 s^{-1}. The contrast in exchange rates is consistent with the large geometry change upon oxidation which is characteristic of hydrazines. The hydrazyls undergo a smaller geometry change upon oxidation, and thus are expected to exhibit smaller inner-sphere reorganization <span class="hlt">energies</span>. The optical spectra of these radical species was investigated in hopes of observing absorption <span class="hlt">bands</span> corresponding to intramolecular <span class="hlt">electron</span> transfer, as predicted by Hush theory. A broad absorption <span class="hlt">band</span> was observed in the near IR region for the saturated bis(hydrazyl) radical cation system at 1060 nm (9420 cm^{-1} ) in acetonitrile at room temperature, and was accompanied by a narrower <span class="hlt">band</span> at 1430 nm (6993 cm^ {-1}). The width of this <span class="hlt">band</span> was estimated to be 545 nm (6496 cm^{-1</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1987ZPhyA.328..399Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1987ZPhyA.328..399Z"><span>In-beam spectroscopy of the k π=0- <span class="hlt">bands</span> in230 236U</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zeyen, P.; Ackermann, B.; Dämmrich, U.; Euler, K.; Grafen, V.; Günther, C.; Herzog, P.; Marten-Tölle, M.; Prillwitz, B.; Tölle, R.; Lauterbach, Ch.; Maier, H. J.</p> <p>1987-12-01</p> <p>The K π=0- <span class="hlt">bands</span> in even uranium nuclei were studied in the compound reactions231Pa( p, 2 n)230U,230, 232Th( α,2 n)232, 234U and236U( d, pn)236U. In-beam γ-rays were measured in coincidence with conversion-<span class="hlt">electrons</span>, which were detected with an iron-free orange spectrometer. The negative-parity levels are observed up to intermediate spins ( I<13-). In addition, the 1- and 3- levels in230U were confirmed by a decay study with an isotope separated230Pa source. For the heavier isotopes ( A≥232) the properties of the K π=0- <span class="hlt">bands</span> (<span class="hlt">energies</span> and γ-branchings) are consistent with a vibrational character of these <span class="hlt">bands</span>. For230U the K π=0- <span class="hlt">band</span> lies at rather low <span class="hlt">energy</span> ( E(1-)=367 keV), and the level spacings within this <span class="hlt">band</span> are very similar to those of the isotones228Th and226Ra, which might indicate the onset of a stable octupole deformation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AIPA....2b2111C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AIPA....2b2111C"><span>Lateral <span class="hlt">energy</span> <span class="hlt">band</span> profile modulation in tunnel field effect transistors based on gate structure engineering</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cui, Ning; Liang, Renrong; Wang, Jing; Xu, Jun</p> <p>2012-06-01</p> <p>Choosing novel materials and structures is important for enhancing the on-state current in tunnel field-effect transistors (TFETs). In this paper, we reveal that the on-state performance of TFETs is mainly determined by the <span class="hlt">energy</span> <span class="hlt">band</span> profile of the channel. According to this interpretation, we present a new concept of <span class="hlt">energy</span> <span class="hlt">band</span> profile modulation (BPM) achieved with gate structure engineering. It is believed that this approach can be used to suppress the ambipolar effect. Based on this method, a Si TFET device with a symmetrical tri-material-gate (TMG) structure is proposed. Two-dimensional numerical simulations demonstrated that the special <span class="hlt">band</span> profile in this device can boost on-state performance, and it also suppresses the off-state current induced by the ambipolar effect. These unique advantages are maintained over a wide range of gate lengths and supply voltages. The BPM concept can serve as a guideline for improving the performance of nanoscale TFET devices.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JEMat.tmp.2704M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JEMat.tmp.2704M"><span>Tuning the <span class="hlt">Energy</span> Gap of SiCH3 Nanomaterials Under Elastic Strain</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ma, Shengqian; Li, Feng; Geng, Jiguo; Zhu, Mei; Li, Suyan; Han, Juguang</p> <p>2018-05-01</p> <p>SiCH3 nanomaterials have been studied using the density functional theory. When the nanosheets and nanoribbons (armchair and zigzag) are introduced, their <span class="hlt">energy</span> gap is modulated under elastic strain and width. The results show that the <span class="hlt">band</span> gap of SiCH3 nanomaterials can be easily tuned using elastic strains and widths. Surprisingly, the <span class="hlt">band</span> gap can be modulated along two directions, namely, compressing and stretching. The <span class="hlt">band</span> gap decreases when increasing stretching strain or decreasing compressing strain. In addition, the <span class="hlt">band</span> gap decreases when increasing the nanoribbon width. For <span class="hlt">energy</span> gap engineering, the <span class="hlt">band</span> gap can be tuned by strains and widths. Therefore, the SiCH3 nanomaterials play important roles in potential applications for strain sensors, <span class="hlt">electronics</span>, and optical <span class="hlt">electronics</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140017833','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140017833"><span>Magnetosphere-Ionosphere <span class="hlt">Energy</span> Interchange in the <span class="hlt">Electron</span> Diffuse Aurora</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Khazanov, George V.; Glocer, Alex; Himwich, E. W.</p> <p>2014-01-01</p> <p>The diffuse aurora has recently been shown to be a major contributor of <span class="hlt">energy</span> flux into the Earth's ionosphere. Therefore, a comprehensive theoretical analysis is required to understand its role in <span class="hlt">energy</span> redistribution in the coupled ionosphere-magnetosphere system. In previous theoretical descriptions of precipitated magnetospheric <span class="hlt">electrons</span> (E is approximately 1 keV), the major focus has been the ionization and excitation rates of the neutral atmosphere and the <span class="hlt">energy</span> deposition rate to thermal ionospheric <span class="hlt">electrons</span>. However, these precipitating <span class="hlt">electrons</span> will also produce secondary <span class="hlt">electrons</span> via impact ionization of the neutral atmosphere. This paper presents the solution of the Boltzman-Landau kinetic equation that uniformly describes the entire <span class="hlt">electron</span> distribution function in the diffuse aurora, including the affiliated production of secondary <span class="hlt">electrons</span> (E greater than 600 eV) and their ionosphere-magnetosphere coupling processes. In this article, we discuss for the first time how diffuse <span class="hlt">electron</span> precipitation into the atmosphere and the associated secondary <span class="hlt">electron</span> production participate in ionosphere-magnetosphere <span class="hlt">energy</span> redistribution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5368653','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5368653"><span>Inelastic <span class="hlt">electron</span> injection in a water chain</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Rizzi, Valerio; Todorov, Tchavdar N.; Kohanoff, Jorge J.</p> <p>2017-01-01</p> <p>Irradiation of biological matter triggers a cascade of secondary particles that interact with their surroundings, resulting in damage. Low-<span class="hlt">energy</span> <span class="hlt">electrons</span> are one of the main secondary species and <span class="hlt">electron</span>-phonon interaction plays a fundamental role in their dynamics. We have developed a method to capture the <span class="hlt">electron</span>-phonon inelastic <span class="hlt">energy</span> exchange in real time and have used it to inject <span class="hlt">electrons</span> into a simple system that models a biological environment, a water chain. We simulated both an incoming <span class="hlt">electron</span> pulse and a steady stream of <span class="hlt">electrons</span> and found that <span class="hlt">electrons</span> with <span class="hlt">energies</span> just outside <span class="hlt">bands</span> of excited molecular states can enter the chain through phonon emission or absorption. Furthermore, this phonon-assisted dynamical behaviour shows great sensitivity to the vibrational temperature, highlighting a crucial controlling factor for the injection and propagation of <span class="hlt">electrons</span> in water. PMID:28350013</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..MARL33001M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..MARL33001M"><span><span class="hlt">Band</span> alignment in atomically precise graphene nanoribbon junctions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ma, Chuanxu; Liang, Liangbo; Hong, Kunlun; Li, An-Ping; Xiao, Zhongcan; Lu, Wenchang; Bernholc, Jerry</p> <p></p> <p>Building atomically precise graphene nanoribbon (GNR) heterojunctions down to molecular level opens a new realm to functional graphene-based devices. By employing a surface-assisted self-assembly process, we have synthesized heterojunctions of armchair GNRs (aGNR) with widths of seven, fourteen and twenty-one carbon atoms, denoted 7, 14 and 21-aGNR respectively. A combined study with scanning tunneling microscopy (STM) and density functional theory (DFT) allows the visualization of <span class="hlt">electronic</span> <span class="hlt">band</span> structures and <span class="hlt">energy</span> level alignments at the heterojunctions with varying widths. A wide bandgap ( 2.6 eV) has been identified on semiconducting 7-aGNR, while the 14-aGNR appears nearly metallic and the 21-aGNR possesses a narrow bandgap. The spatially modulations of the <span class="hlt">energy</span> <span class="hlt">bands</span> are strongly confined at the heterojunctions within a width of about 2 nm. Clear <span class="hlt">band</span> bending of about 0.4 eV and 0.1 eV are observed at the 7-14 and 14-21 aGNR heterojunctions, respectively. This research was conducted at the Center for Nanophase Materials Sciences, which is a DOE Office of Science User Facility.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22525678-optimal-electron-energies-driving-chromospheric-evaporation-solar-flares','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22525678-optimal-electron-energies-driving-chromospheric-evaporation-solar-flares"><span>OPTIMAL <span class="hlt">ELECTRON</span> <span class="hlt">ENERGIES</span> FOR DRIVING CHROMOSPHERIC EVAPORATION IN SOLAR FLARES</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Reep, J. W.; Bradshaw, S. J.; Alexander, D., E-mail: jr665@cam.ac.uk, E-mail: stephen.bradshaw@rice.edu, E-mail: dalex@rice.edu</p> <p>2015-08-01</p> <p>In the standard model of solar flares, <span class="hlt">energy</span> deposition by a beam of <span class="hlt">electrons</span> drives strong chromospheric evaporation leading to a significantly denser corona and much brighter emission across the spectrum. Chromospheric evaporation was examined in great detail by Fisher et al., who described a distinction between two different regimes, termed explosive and gentle evaporation. In this work, we examine the importance of <span class="hlt">electron</span> <span class="hlt">energy</span> and stopping depths on the two regimes and on the atmospheric response. We find that with explosive evaporation, the atmospheric response does not depend strongly on <span class="hlt">electron</span> <span class="hlt">energy</span>. In the case of gentle evaporation, lowermore » <span class="hlt">energy</span> <span class="hlt">electrons</span> are significantly more efficient at heating the atmosphere and driving up-flows sooner than higher <span class="hlt">energy</span> <span class="hlt">electrons</span>. We also find that the threshold between explosive and gentle evaporation is not fixed at a given beam <span class="hlt">energy</span> flux, but also depends strongly on the <span class="hlt">electron</span> <span class="hlt">energy</span> and duration of heating. Further, at low <span class="hlt">electron</span> <span class="hlt">energies</span>, a much weaker beam flux is required to drive explosive evaporation.« less</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li class="active"><span>25</span></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_25 --> <div class="footer-extlink text-muted" style="margin-bottom:1rem; text-align:center;">Some links on this page may take you to non-federal websites. 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