Sample records for ground-state energy bands

  1. Ground-state energies of simple metals

    NASA Technical Reports Server (NTRS)

    Hammerberg, J.; Ashcroft, N. W.

    1974-01-01

    A structural expansion for the static ground-state energy of a simple metal is derived. Two methods are presented, one an approach based on single-particle band structure which treats the electron 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 band-structure effects, Fermi-surface distortions, and chemical-potential shifts affect the total energy. These are of special interest in corrections to the total energy beyond third order in the electron-ion interaction and hence to systems where differences in energies for various crystal structures are exceptionally small. Preliminary calculations using these methods for the zero-temperature thermodynamic functions of atomic hydrogen are reported.

  2. Ground-state properties of the three-band Hubbard model

    NASA Astrophysics Data System (ADS)

    Zhang, Shiwei; Vitali, Ettore; Chiciak, Adam; Shi, Hao

    The three-band Hubbard model proposed by Emery describes the CuO2 plane in cuprate superconductors by retaining both Cu and O orbitals in a minimal sense. Applying the latest developments in the auxiliary-field quantum Monte Carlo (AFQMC) method, we investigate ground-state properties of this model at half-filling and when lightly (under-)doped. The AFQMC uses generalized Hartree-Fock (GHF) trial wave functions to control the sign problem. A self-consistent constraint is applied. We also determine the unrestricted Hartree-Fock (UHF) and GHF ground states and compare their predictions with those from AFQMC. Similarities and differences between the three-band model and one-band Hubbard model will be discussed. Supported by NSF, and the Simons Foundation. Computing is carried out at the Extreme Science and Engineering Discovery Environment(XSEDE).

  3. Ground state energy of electrons in a static point-ion lattice

    NASA Technical Reports Server (NTRS)

    Styer, D. F.; Ashcroft, N. W.

    1983-01-01

    The ground state energy of a neutral collection of protons and electrons 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 band-minimum energy and wave functions are derived. For each of the three potentials, the approximate minimum ground state energy per proton (relative to isolated electrons 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.

  4. Ground-state and pairing-vibrational bands with equal quadrupole collectivity in 124Xe

    NASA Astrophysics Data System (ADS)

    Radich, A. J.; Garrett, P. E.; Allmond, J. M.; Andreoiu, C.; Ball, G. C.; Bianco, L.; Bildstein, V.; Chagnon-Lessard, S.; Cross, D. S.; Demand, G. A.; Diaz Varela, A.; Dunlop, R.; Finlay, P.; Garnsworthy, A. B.; Hackman, G.; Hadinia, B.; Jigmeddorj, B.; Laffoley, A. T.; Leach, K. G.; Michetti-Wilson, J.; Orce, J. N.; Rajabali, M. M.; Rand, E. T.; Starosta, K.; Sumithrarachchi, C. S.; Svensson, C. E.; Triambak, S.; Wang, Z. M.; Wood, J. L.; Wong, J.; Williams, S. J.; Yates, S. W.

    2015-04-01

    The nuclear structure of 124Xe has been investigated via measurements of the β+/EC decay of 124Cs with the 8 π γ -ray spectrometer at the TRIUMF-ISAC facility. The data collected have enabled branching ratio measurements of weak, low-energy transitions from highly excited states, and the 2+→0+ in-band transitions have been observed. Combining these results with those from a previous Coulomb excitation study, B (E 2 ;23+→02+) =78 (13 ) W.u. and B (E 2 ;24+→03+) =53 (12 ) W.u. were determined. The 03+ state, in particular, is interpreted as the main fragment of the proton-pairing vibrational band identified in a previous 122Te (3He,n )124Xe measurement, and has quadrupole collectivity equal to, within uncertainty, that of the ground-state band.

  5. Ground-state and pairing-vibrational bands with equal quadrupole collectivity in 124Xe

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

    Radich, A. J.; Garrett, P. E.; Allmond, J. M.

    The nuclear structure of 124Xe has been investigated via measurements of the β +/EC decay of 124Cs with the 8π γ-ray spectrometer at the TRIUMF-ISAC facility. The data collected have enabled branching ratio measurements of weak, low-energy transitions from highly excited states, and the 2 + → 0 + in-band transitions have been observed. Combining these results with those from a previous Coulomb excitation study,more » $$B(E2; 2^+_3 → 0^+_2)$$ = 78(13) W.u. and $$B(E2; 2^+_4 → 0^+_3)$$ = 53(12) W.u. were determined. The $$0^+_3$$ state, in particular, is interpreted as the main fragment of the proton-pairing vibrational band identified in a previous 122Te( 3He,n) 124Xe measurement, and has quadrupole collectivity equal to, within uncertainty, that of the ground-state band.« less

  6. Ground-state and pairing-vibrational bands with equal quadrupole collectivity in 124Xe

    DOE PAGES

    Radich, A. J.; Garrett, P. E.; Allmond, J. M.; ...

    2015-04-01

    The nuclear structure of 124Xe has been investigated via measurements of the β +/EC decay of 124Cs with the 8π γ-ray spectrometer at the TRIUMF-ISAC facility. The data collected have enabled branching ratio measurements of weak, low-energy transitions from highly excited states, and the 2 + → 0 + in-band transitions have been observed. Combining these results with those from a previous Coulomb excitation study,more » $$B(E2; 2^+_3 → 0^+_2)$$ = 78(13) W.u. and $$B(E2; 2^+_4 → 0^+_3)$$ = 53(12) W.u. were determined. The $$0^+_3$$ state, in particular, is interpreted as the main fragment of the proton-pairing vibrational band identified in a previous 122Te( 3He,n) 124Xe measurement, and has quadrupole collectivity equal to, within uncertainty, that of the ground-state band.« less

  7. 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

  8. Structural expansions for the ground state energy of a simple metal

    NASA Technical Reports Server (NTRS)

    Hammerberg, J.; Ashcroft, N. W.

    1973-01-01

    A structural expansion for the static ground state energy of a simple metal is derived. An approach based on single particle band structure which treats the electron gas as a non-linear dielectric is presented, along with a more general many particle analysis using finite temperature perturbation theory. The two methods are compared, and it is shown in detail how band-structure effects, Fermi surface distortions, and chemical potential shifts affect the total energy. These are of special interest in corrections to the total energy beyond third order in the electron ion interaction, and hence to systems where differences in energies for various crystal structures are exceptionally small. Preliminary calculations using these methods for the zero temperature thermodynamic functions of atomic hydrogen are reported.

  9. E 2 / M 1 Mixing Ratios in Transitions From the Gamma-Vibrational-Bands to the Ground-State-Rotational-Bands of 102 , 104 , 106 , 108Mo, 108 , 110 , 112Ru, and 112 , 114 , 116Pd

    NASA Astrophysics Data System (ADS)

    Eldridge, Jonathan M.; Fenker, B.; Goodin, C.; Hamilton, J. H.; Wang, E. H.; Ramayya, A. V.; Daniel, A. V.; Ter-Akopian, G. M.; Luo, Y. X.; Rasmussen, J. O.; Oganesson, Yu. Ts.; Zhu, S. J.

    2017-09-01

    E 2 / M 1 mixing ratios have been measured for transitions from states in the γ-vibrational-bands (Iγ+) to states in the ground-state-bands (Ig+ or [I- 1 ] g +) of the neutron rich, deformed isotopes, 102 , 104 , 106 , 108Mo, 108 , 110 , 112Ru, and 112 , 114 , 116Pd, including from states as high as 9γ+. These measurements were done using the GAMMASPHERE detector array, which, at the time of the experiment, had 101 working HPGe detectors, arranged at 64 different angles. A 62 μCi source of 252Cf was placed inside GAMMASPHERE yielding 5.7 ×1011 γ - γ - γ and higher coincidence events. The angular correlation between the transitions from the γ-band to the ground band, and the pure E2 transitions within the ground band were then measured. These angular correlations yielded the mixing ratios, demonstrating that these transitions are all pure or nearly pure E2, in agreement with theory. In order to correct for possible attenuation due to the lifetime of the intermediate state in these correlations, the g-factors of the intermediate states needed to be known. Therefore, the g-factors of the 2g+ states in the ground state band have been measured. Supported by the US Department of Energy; Grant No. DE-FG0588ER40407, Contract No. DE-AC03-76SF00098.

  10. The nu sub 2 band CHD3; ground state parameters for CHD3 from combination differences

    NASA Technical Reports Server (NTRS)

    Jennings, D. E.; Blass, W. E.

    1974-01-01

    The nu sub 2 fundamental band of CHD3, centered near 2143/cm, was recorded at a resolution of 0.015-0.25/cm. Analysis of ground state combination differences yielded well-determined values for the ground state molecular parameters for CHD3. These parameters were used in the determination of the alpha and beta molecular parameters for nu sub 2.

  11. Transition from one revolving cluster to two revolving clusters in the ground-state rotational bands of nuclei in the lanthanon region.

    PubMed

    Pauling, L

    1991-02-01

    Whereas 234(92)U142 and other actinon nuclei have ground-state bands that indicate that each nucleus consists of a sphere and a single revolving cluster with constant composition and with only a steady increase in the moment of inertia with increase in J, the angular-momentum quantum number, many of the lanthanon ground-state bands show discontinuities, usually with an initial slightly or strongly curved segment followed by one or two nearly straight segments. The transition to nearly straight segments is interpreted as a change in structure from one revolving cluster to two revolving clusters. The proton-neutron compositions of the clusters and the central sphere are assigned, leading to values of the radius of revolution. The approximation of the two-cluster sequences to linearity is attributed to the very small values of the quadrupole polarizability of the central sphere. Values of the nucleon numbers of clusters and spheres, of the radius of revolution, and of promotion energy are discussed.

  12. E2/M1 mixing ratios in transitions from the gamma vibrational bands to the ground state rotational bands of 102, 104, 106, 108Mo, 108, 110, 112Ru, and 112, 114, 116Pd

    NASA Astrophysics Data System (ADS)

    Eldridge, J. M.; Fenker, B.; Hamilton, J. H.; Goodin, C.; Zachary, C. J.; Wang, E.; Ramayya, A. V.; Daniel, A. V.; Ter-Akopian, G. M.; Oganessian, Yu. Ts.; Luo, Y. X.; Rasmussen, J. O.; Zhu, S. J.

    2018-02-01

    E2/ M1 mixing ratios have been measured for transitions from states in the γ vibrational bands ( I+_{γ}) to states in the ground state bands (I+ or [I-1]+) of the neutron rich, even-even, deformed isotopes, 102, 104, 106, 108Mo, 108, 110, 112Ru, and 112, 114, 116Pd, including from states as high as 9+_{γ}. These measurements were done using the GAMMASPHERE detector array, which, at the time of the experiment, had 101 working HPGe detectors, arranged at 64 different angles. A 62 μCi source of 252Cf was placed inside GAMMASPHERE yielding 5.7× 10^{11} γ-γ-γ and higher coincidence events. The angular correlations between the transitions from the γ-bands to the ground bands, and the pure E2 transitions within the ground band were then measured. These angular correlations yielded the mixing ratios, demonstrating that these transitions are pure or nearly pure E2, in agreement with theory. In order to correct for possible attenuation due to the lifetime of the intermediate state in these correlations, the g-factors of the intermediate states needed to be known. Therefore, the g-factors of the 2+ states in the ground state band have been measured.

  13. Nitric oxide excited under auroral conditions: Excited state densities and band emissions

    NASA Astrophysics Data System (ADS)

    Cartwright, D. C.; Brunger, M. J.; Campbell, L.; Mojarrabi, B.; Teubner, P. J. O.

    2000-09-01

    Electron impact excitation of vibrational levels in the ground electronic state and nine excited electronic 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 band emission intensities. New integral electron impact excitation cross sections for NO were combined with a measured IBC II auroral secondary electron distribution, and the vibrational populations of 10 NO electronic states were determined under conditions of statistical equilibrium. This model predicts an extended vibrational distribution in the NO ground electronic state produced by radiative cascade from the seven higher-lying doublet excited electronic states populated by electron impact. In addition to significant energy storage in vibrational excitation of the ground electronic state, both the a 4Π and L2 Φ excited electronic states are predicted to have relatively high number densities because they are only weakly connected to lower electronic states by radiative decay. Fundamental mode radiative transitions involving the lowest nine excited vibrational levels in the ground electronic state are predicted to produce infrared (IR) radiation from 5.33 to 6.05 μm with greater intensity than any single NO electronic emission band. Fundamental mode radiative transitions within the a 4Π electronic state, in the 10.08-11.37 μm region, are predicted to have IR intensities comparable to individual electronic emission bands in the Heath and ɛ band systems. Results from this model quantitatively predict the vibrational quantum number dependence of the NO IR measurements of Espy et al. [1988].

  14. Ground-state energy of HeH+

    NASA Astrophysics Data System (ADS)

    Zhou, Bing-Lu; Zhu, Jiong-Ming; Yan, Zong-Chao

    2006-06-01

    The nonrelativistic ground-state energy of He4H+ is calculated using a variational method in Hylleraas coordinates. Convergence to a few parts in 1010 is achieved, which improves the best previous result of Pavanello [J. Chem. Phys. 123, 104306 (2005)]. Expectation values of the interparticle distances are evaluated. Similar results for He3H+ are also presented.

  15. Ground-state energies of the nonlinear sigma model and the Heisenberg spin chains

    NASA Technical Reports Server (NTRS)

    Zhang, Shoucheng; Schulz, H. J.; Ziman, Timothy

    1989-01-01

    A theorem on the O(3) nonlinear sigma model with the topological theta term is proved, which states that the ground-state energy at theta = pi is always higher than the ground-state energy at theta = 0, for the same value of the coupling constant g. Provided that the nonlinear sigma model gives the correct description for the Heisenberg spin chains in the large-s limit, this theorem makes a definite prediction relating the ground-state energies of the half-integer and the integer spin chains. The ground-state energies obtained from the exact Bethe ansatz solution for the spin-1/2 chain and the numerical diagonalization on the spin-1, spin-3/2, and spin-2 chains support this prediction.

  16. Variable energy, high flux, ground-state atomic oxygen source

    NASA Technical Reports Server (NTRS)

    Chutjian, Ara (Inventor); Orient, Otto J. (Inventor)

    1987-01-01

    A variable energy, high flux atomic oxygen source is described which is comprised of a means for producing a high density beam of molecules which will emit O(-) ions when bombarded with electrons; a means of producing a high current stream of electrons at a low energy level passing through the high density beam of molecules to produce a combined stream of electrons and O(-) ions; means for accelerating the combined stream to a desired energy level; means for producing an intense magnetic field to confine the electrons and O(-) ions; means for directing a multiple pass laser beam through the combined stream to strip off the excess electrons from a plurality of the O(-) ions to produce ground-state O atoms within the combined stream; electrostatic deflection means for deflecting the path of the O(-) ions and the electrons in the combined stream; and, means for stopping the O(-) ions and the electrons and for allowing only the ground-state O atoms to continue as the source of the atoms of interest. The method and apparatus are also adaptable for producing other ground-state atoms and/or molecules.

  17. Ground-state-entanglement bound for quantum energy teleportation of general spin-chain models

    NASA Astrophysics Data System (ADS)

    Hotta, Masahiro

    2013-03-01

    Many-body quantum systems in the ground states have zero-point energy due to the uncertainty relation. In many cases, the system in the ground state accompanies spatially entangled energy density fluctuation via the noncommutativity of the energy density operators, though the total energy takes a fixed value, i.e., the lowest eigenvalue of the Hamiltonian. Quantum energy teleportation (QET) is a protocol for the extraction of the zero-point energy out of one subsystem using information of a remote measurement of another subsystem. From an operational viewpoint of protocol users, QET can be regarded as an effective rapid energy transportation without breaking all physical laws, including causality and local energy conservation. In the protocol, the ground-state entanglement plays a crucial role. In this paper, we show analytically for a general class of spin-chain systems that the entanglement entropy is lower bounded by a positive quadratic function of the teleported energy between the regions of a QET protocol. This supports a general conjecture that ground-state entanglement is an evident physical resource for energy transportation in the context of QET. The result may also deepen our understanding of the energy density fluctuation in condensed-matter systems from a perspective of quantum information theory.

  18. Population shuffling between ground and high energy excited states

    PubMed Central

    Sabo, T Michael; Trent, John O; Lee, Donghan

    2015-01-01

    Stochastic processes powered by thermal energy lead to protein motions traversing time-scales from picoseconds to seconds. Fundamental to protein functionality is the utilization of these dynamics for tasks such as catalysis, folding, and allostery. A hierarchy of motion is hypothesized to connect and synergize fast and slow dynamics toward performing these essential activities. Population shuffling predicts a “top-down” temporal hierarchy, where slow time-scale conformational interconversion leads to a shuffling of the free energy landscape for fast time-scale events. Until now, population shuffling was only applied to interconverting ground states. Here, we extend the framework of population shuffling to be applicable for a system interconverting between low energy ground and high energy excited states, such as the SH3 domain mutants G48M and A39V/N53P/V55L from the Fyn tyrosine kinase, providing another tool for accessing the structural dynamics of high energy excited states. Our results indicate that the higher energy gauche− rotameric state for the leucine χ2 dihedral angle contributes significantly to the distribution of rotameric states in both the major and minor forms of the SH3 domain. These findings are corroborated with unrestrained molecular dynamics (MD) simulations on both the major and minor states of the SH3 domain demonstrating high correlations between experimental and back-calculated leucine χ2 rotameric populations. Taken together, we demonstrate how fast time-scale rotameric side-chain population distributions can be extracted from slow time-scale conformational exchange data further extending the scope and the applicability of the population shuffling model. PMID:26316263

  19. Population shuffling between ground and high energy excited states.

    PubMed

    Sabo, T Michael; Trent, John O; Lee, Donghan

    2015-11-01

    Stochastic processes powered by thermal energy lead to protein motions traversing time-scales from picoseconds to seconds. Fundamental to protein functionality is the utilization of these dynamics for tasks such as catalysis, folding, and allostery. A hierarchy of motion is hypothesized to connect and synergize fast and slow dynamics toward performing these essential activities. Population shuffling predicts a "top-down" temporal hierarchy, where slow time-scale conformational interconversion leads to a shuffling of the free energy landscape for fast time-scale events. Until now, population shuffling was only applied to interconverting ground states. Here, we extend the framework of population shuffling to be applicable for a system interconverting between low energy ground and high energy excited states, such as the SH3 domain mutants G48M and A39V/N53P/V55L from the Fyn tyrosine kinase, providing another tool for accessing the structural dynamics of high energy excited states. Our results indicate that the higher energy gauche - rotameric state for the leucine χ2 dihedral angle contributes significantly to the distribution of rotameric states in both the major and minor forms of the SH3 domain. These findings are corroborated with unrestrained molecular dynamics (MD) simulations on both the major and minor states of the SH3 domain demonstrating high correlations between experimental and back-calculated leucine χ2 rotameric populations. Taken together, we demonstrate how fast time-scale rotameric side-chain population distributions can be extracted from slow time-scale conformational exchange data further extending the scope and the applicability of the population shuffling model. © 2015 The Protein Society.

  20. Ground-state energy of HeH{sup +}

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

    Zhou Binglu; Zhu Jiongming; Yan Zongchao

    2006-06-15

    The nonrelativistic ground-state energy of {sup 4}HeH{sup +} is calculated using a variational method in Hylleraas coordinates. Convergence to a few parts in 10{sup 10} is achieved, which improves the best previous result of Pavanello et al. [J. Chem. Phys. 123, 104306 (2005)]. Expectation values of the interparticle distances are evaluated. Similar results for {sup 3}HeH{sup +} are also presented.

  1. Ground-state splitting of ultrashallow thermal donors with negative central-cell corrections in silicon

    NASA Astrophysics Data System (ADS)

    Hara, Akito; Awano, Teruyoshi

    2017-06-01

    Ultrashallow thermal donors (USTDs), which consist of light element impurities such as carbon, hydrogen, and oxygen, have been found in Czochralski silicon (CZ Si) crystals. To the best of our knowledge, these are the shallowest hydrogen-like donors with negative central-cell corrections in Si. We observed the ground-state splitting of USTDs by far-infrared optical absorption at different temperatures. The upper ground-state levels are approximately 4 meV higher than the ground-state levels. This energy level splitting is also consistent with that obtained by thermal excitation from the ground state to the upper ground state. This is direct evidence that the wave function of the USTD ground state is made up of a linear combination of conduction band minimums.

  2. NiTi shape memory via solid-state nudge-elastic band

    NASA Astrophysics Data System (ADS)

    Zarkevich, Nikolai A.; Johnson, Duane D.

    2014-03-01

    We determine atomic mechanisms of the shape memory effect in NiTi from a generalized solid-state nudge elastic band (SSNEB) method. We consider transformation between the austenite B2 and the ground-state base-centered orthorhombic (BCO) structures. In these pathways we obtain the R-phase and discuss its structure. We confirm that BCO is the ground state, and determine the pathways to BCO martensite, which dictate transition barriers. While ideal B2 is unstable, we find a B2-like NiTi high-temperature solid phase with significant local displacement disorder, which is B2 on average. This B2-like phase appears to be entropically stabilized. This work is supported by the U.S. Department of Energy, Office of Basic Energy Science, Division of Materials Science and Engineering. Ames Laboratory is operated for the U.S. DOE by Iowa State University under contract DE-AC02-07CH11358.

  3. Ground state energies from converging and diverging power series expansions

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

    Lisowski, C.; Norris, S.; Pelphrey, R.

    2016-10-15

    It is often assumed that bound states of quantum mechanical systems are intrinsically non-perturbative in nature and therefore any power series expansion methods should be inapplicable to predict the energies for attractive potentials. However, if the spatial domain of the Schrödinger Hamiltonian for attractive one-dimensional potentials is confined to a finite length L, the usual Rayleigh–Schrödinger perturbation theory can converge rapidly and is perfectly accurate in the weak-binding region where the ground state’s spatial extension is comparable to L. Once the binding strength is so strong that the ground state’s extension is less than L, the power expansion becomes divergent,more » consistent with the expectation that bound states are non-perturbative. However, we propose a new truncated Borel-like summation technique that can recover the bound state energy from the diverging sum. We also show that perturbation theory becomes divergent in the vicinity of an avoided-level crossing. Here the same numerical summation technique can be applied to reproduce the energies from the diverging perturbative sums.« less

  4. Structures and Binding Energies of the Naphthalene Dimer in Its Ground and Excited States.

    PubMed

    Dubinets, N O; Safonov, A A; Bagaturyants, A A

    2016-05-05

    Possible structures of the naphthalene dimer corresponding to local energy minima in the ground and excited (excimer) electronic states are comprehensively investigated using DFT-D and TDDFT-D methods with a special accent on the excimer structures. The corresponding binding and electronic transition energies are calculated, and the nature of the electronic states in different structures is analyzed. Several parallel (stacked) and T-shaped structures were found in both the ground and excited (excimer) states in a rather narrow energy range. The T-shaped structure with the lowest energy in the excited state exhibits a marked charge transfer from the upright molecule to the base one.

  5. Kinetic energy partition method applied to ground state helium-like atoms.

    PubMed

    Chen, Yu-Hsin; Chao, Sheng D

    2017-03-28

    We have used the recently developed kinetic energy partition (KEP) method to solve the quantum eigenvalue problems for helium-like atoms and obtain precise ground state energies and wave-functions. The key to treating properly the electron-electron (repulsive) Coulomb potential energies for the KEP method to be applied is to introduce a "negative mass" term into the partitioned kinetic energy. A Hartree-like product wave-function from the subsystem wave-functions is used to form the initial trial function, and the variational search for the optimized adiabatic parameters leads to a precise ground state energy. This new approach sheds new light on the all-important problem of solving many-electron Schrödinger equations and hopefully opens a new way to predictive quantum chemistry. The results presented here give very promising evidence that an effective one-electron model can be used to represent a many-electron system, in the spirit of density functional theory.

  6. Free-end adaptive nudged elastic band method for locating transition states in minimum energy path calculation.

    PubMed

    Zhang, Jiayong; Zhang, Hongwu; Ye, Hongfei; Zheng, Yonggang

    2016-09-07

    A free-end adaptive nudged elastic band (FEA-NEB) method is presented for finding transition states on minimum energy paths, where the energy barrier is very narrow compared to the whole paths. The previously proposed free-end nudged elastic band method may suffer from convergence problems because of the kinks arising on the elastic band if the initial elastic band is far from the minimum energy 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 band 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.

  7. The ground state of two-dimensional silicon

    NASA Astrophysics Data System (ADS)

    Borlido, Pedro; Rödl, Claudia; Marques, Miguel A. L.; Botti, Silvana

    2018-07-01

    We perform ab initio structure-prediction calculations of the low-energy crystal structures of two-dimensional silicon. Besides the well-known silicene and a few other allotropes proposed earlier in the literature, we discover a wealth of new phases with interesting properties. In particular, we find that the ground state of two-dimensional silicon is an unreported structure formed by a honeycomb lattice with dumbbell atoms arranged in a zigzag pattern. This material, that we call zigzag dumbbell silicene, is 218 meV/atom more stable than silicene and displays a quasi-direct band gap of around 1.11 eV, with a very dispersive electron band. These properties should make it easier to synthesize than silicene and interesting for a wealth of opto-electronic applications.

  8. Lower bounds to energies for cusped-gaussian wavefunctions. [hydrogen atom ground state

    NASA Technical Reports Server (NTRS)

    Eaves, J. O.; Walsh, B. C.; Steiner, E.

    1974-01-01

    Calculations for the ground states of H, He, and Be, conducted by Steiner and Sykes (1972), show that the inclusion of a very small number of cusp functions can lead to a substantial enhancement of the quality of the Gaussian basis used in molecular wavefunction computations. The properties of the cusped-Gaussian basis are investigated by a calculation of lower bounds concerning the ground state energy of the hydrogen atom.

  9. Ground-state energy of an exciton-(LO) phonon system in a parabolic quantum well

    NASA Astrophysics Data System (ADS)

    Gerlach, B.; Wüsthoff, J.; Smondyrev, M. A.

    1999-12-01

    This paper presents a variational study of the ground-state energy of an exciton-(LO) phonon system, which is spatially confined to a quantum well. The exciton-phonon interaction is of Fröhlich type, the confinement potentials are assumed to be parabolic functions of the coordinates. Making use of functional integral techniques, the phonon part of the problem can be eliminated exactly, leading us to an effective two-particle system, which has the same spectral properties as the original one. Subsequently, Jensen's inequality is applied to obtain an upper bound on the ground-state energy. The main intention of this paper is to analyze the influence of the quantum-well-induced localization of the exciton on its ground-state energy (or its binding energy, respectively). To do so, we neglect any mismatch of the masses or the dielectric constants, but admit an arbitrary strength of the confinement potentials. Our approach allows for a smooth interpolation of the ultimate limits of vanishing and infinite confinement, corresponding to the cases of a free three-dimensional and a free two-dimensional exciton-phonon system. The interpolation formula for the ground-state energy bound corresponds to similar formulas for the free polaron or the free exciton-phonon system. These bounds in turn are known to compare favorably with all previous ones, which we are aware of.

  10. A toy model to investigate the existence of excitons in the ground state of strongly-correlated semiconductor

    NASA Astrophysics Data System (ADS)

    Karima, H. R.; Majidi, M. A.

    2018-04-01

    Excitons, quasiparticles associated with bound states between an electron and a hole and are typically created when photons with a suitable energy are absorbed in a solid-state material. We propose to study a possible emergence of excitons, created not by photon absorption but the effect of strong electronic correlations. This study is motivated by a recent experimental study of a substrate material SrTiO3 (STO) that reveals strong exitonic signals in its optical conductivity. Here we conjecture that some excitons may already exist in the ground state as a result of the electronic correlations before the additional excitons being created later by photon absorption. To investigate the existence of excitons in the ground state, we propose to study a simple 4-energy-level model that mimics a situation in strongly-correlated semiconductors. The four levels are divided into two groups, lower and upper groups separated by an energy gap, Eg , mimicking the valence and the conduction bands, respectively. Further, we incorporate repulsive Coulomb interactions between the electrons. The model is then solved by exact diagonalization method. Our result shows that the toy model can demonstrate band gap widening or narrowing and the existence of exciton in the ground state depending on interaction parameter values.

  11. Effect of temperature on the single-particle ground-state energy of a polar quantum dot with Gaussian confinement

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

    Jahan, Luhluh K., E-mail: luhluhjahan@gmail.com; Chatterjee, Ashok

    2016-05-23

    The temperature and size dependence of the ground-state energy of a polaron in a Gaussian quantum dot have been investigated by using a variational technique. It is found that the ground-state energy increases with increasing temperature and decreases with the size of the quantum dot. Also, it is found that the ground-state energy is larger for a three-dimensional quantum dot as compared to a two-dimensional dot.

  12. Van der Waals potential and vibrational energy levels of the ground state radon dimer

    NASA Astrophysics Data System (ADS)

    Sheng, Xiaowei; Qian, Shifeng; Hu, Fengfei

    2017-08-01

    In the present paper, the ground state van der Waals potential of the Radon dimer is described by the Tang-Toennies potential model, which requires five essential parameters. Among them, the two dispersion coefficients C6 and C8 are estimated from the well determined dispersion coefficients C6 and C8 of Xe2. C10 is estimated by using the approximation equation that C6C10/C82 has an average value of 1.221 for all the rare gas dimers. With these estimated dispersion coefficients and the well determined well depth De and Re the Born-Mayer parameters A and b are derived. Then the vibrational energy levels of the ground state radon dimer are calculated. 40 vibrational energy levels are observed in the ground state of Rn2 dimer. The last vibrational energy level is bound by only 0.0012 cm-1.

  13. New analytical model for the ozone electronic ground state potential surface and accurate ab initio vibrational predictions at high energy range.

    PubMed

    Tyuterev, Vladimir G; Kochanov, Roman V; Tashkun, Sergey A; Holka, Filip; Szalay, Péter G

    2013-10-07

    An accurate description of the complicated shape of the potential energy 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 electronic 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 energy path. The impact of the shape of the PES near the transition state (existence of the "reef structure") on vibration energy levels was studied for the first time. The major purpose of this work was to provide accurate theoretical predictions for ozone vibrational band centres at the energy 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 electronic structure calculations were carried out enabling the determination of the parameters of a minimum energy 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 band centres up to 90% of the dissociation energy. New ab initio vibrational predictions represent a significant improvement with respect to all previously available calculations.

  14. a New Phenomenological Formula for Ground-State Binding Energies

    NASA Astrophysics Data System (ADS)

    Gangopadhyay, G.

    A phenomenological formula based on liquid drop model has been proposed for ground-state binding energies of nuclei. The effect due to bunching of single particle levels has been incorporated through a term resembling the one-body Hamiltonian. The effect of n-p interaction has been included through a function of valence nucleons. A total of 50 parameters has been used in the present calculation. The root mean square (r.m.s.) deviation for the binding energy values for 2140 nuclei comes out to be 0.376 MeV, and that for 1091 alpha decay energies is 0.284 MeV. The correspondence with the conventional liquid drop model is discussed.

  15. Analysis of the energy of the first four excited states of the ground-state rotational bands of the even-even nuclei from 6C8 to 56Ba90 with the model of a single cluster of nucleons revolving about a sphere.

    PubMed Central

    Pauling, L

    1991-01-01

    The results of the analysis of the first four energy levels of the ground-state rotational bands of even-even nuclei from 6C8 to 56Ba90 on the basis of the revolving-cluster model are reported. Values of the nucleon number of the revolving cluster are assigned on the basis in part of the shell model and in part of the expectation that the corresponding values of the radius of revolution would change only slightly from one energy level to an adjacent level or from one nucleus to an adjacent nucleus. The values of the radius of revolution are found to change gradually from about 5 to 6 fm for the lighter nuclei to 7 to 8 fm for the heavier nuclei in the sequence studied. PMID:11607232

  16. Pair Formation of Hard Core Bosons in Flat Band Systems

    NASA Astrophysics Data System (ADS)

    Mielke, Andreas

    2018-05-01

    Hard core bosons in a large class of one or two dimensional flat band systems have an upper critical density, below which the ground states can be described completely. At the critical density, the ground states are Wigner crystals. If one adds a particle to the system at the critical density, the ground state and the low lying multi particle states of the system can be described as a Wigner crystal with an additional pair of particles. The energy band for the pair is separated from the rest of the multi-particle spectrum. The proofs use a Gerschgorin type of argument for block diagonally dominant matrices. In certain one-dimensional or tree-like structures one can show that the pair is localised, for example in the chequerboard chain. For this one-dimensional system with periodic boundary condition the energy band for the pair is flat, the pair is localised.

  17. Computational Design of Flat-Band Material.

    PubMed

    Hase, I; Yanagisawa, T; Kawashima, K

    2018-02-26

    Quantum mechanics states that hopping integral between local orbitals makes the energy band dispersive. However, in some special cases, there are bands with no dispersion due to quantum interference. These bands are called as flat band. Many models having flat band have been proposed, and many interesting physical properties are predicted. However, no real compound having flat band has been found yet despite the 25 years of vigorous researches. We have found that some pyrochlore oxides have quasi-flat band just below the Fermi level by first principles calculation. Moreover, their valence bands are well described by a tight-binding model of pyrochlore lattice with isotropic nearest neighbor hopping integral. This model belongs to a class of Mielke model, whose ground state is known to be ferromagnetic with appropriate carrier doping and on-site repulsive Coulomb interaction. We have also performed a spin-polarized band calculation for the hole-doped system from first principles and found that the ground state is ferromagnetic for some doping region. Interestingly, these compounds do not include magnetic element, such as transition metal and rare-earth elements.

  18. Computational Design of Flat-Band Material

    NASA Astrophysics Data System (ADS)

    Hase, I.; Yanagisawa, T.; Kawashima, K.

    2018-02-01

    Quantum mechanics states that hopping integral between local orbitals makes the energy band dispersive. However, in some special cases, there are bands with no dispersion due to quantum interference. These bands are called as flat band. Many models having flat band have been proposed, and many interesting physical properties are predicted. However, no real compound having flat band has been found yet despite the 25 years of vigorous researches. We have found that some pyrochlore oxides have quasi-flat band just below the Fermi level by first principles calculation. Moreover, their valence bands are well described by a tight-binding model of pyrochlore lattice with isotropic nearest neighbor hopping integral. This model belongs to a class of Mielke model, whose ground state is known to be ferromagnetic with appropriate carrier doping and on-site repulsive Coulomb interaction. We have also performed a spin-polarized band calculation for the hole-doped system from first principles and found that the ground state is ferromagnetic for some doping region. Interestingly, these compounds do not include magnetic element, such as transition metal and rare-earth elements.

  19. Regularities in the sequences of the number of nucleons in the revolving clusters for the ground-state energy bands of the even-even nuclei with neutron number equal to or greater than 126.

    PubMed

    Pauling, L

    1990-06-01

    Values of m, the number of nucleons in the revolving cluster, and of R, the radius of revolution of the cluster about the center of mass of the spherical part of the nucleus, are calculated from the observed values of the energy for the ground-state bands of all nuclei with neutron number N >/= 126 on the basis of the assumptions (i) that both m and R change in a reasonable way with increase in the angular momentum quantum number J and with change in the proton number Z and the neutron number N, (ii) that m is usually an even integer, (iii) that certain clusters are especially stable, and (iv) that there is a special stability of the doubly magic sphere p82n126.

  20. Structure, strain, and control of ground state property in LaTiO3/LaAlO3 superlattice

    NASA Astrophysics Data System (ADS)

    Lee, Alex Taekyung; Han, Myung Joon

    2014-03-01

    We examined the ground state property of LaTiO3/LaAlO3 superlattice through density functional band calculations. Total energy calculations, including the structural distortions, U dependence, and the exchange correlation functional dependence, clearly showed that the spin and orbital ground state can be controlled systematically by the epitaxial strain. In the wide range of strain, the ferromagnetic-spin and antiferro-orbital order are stabilized, which is notably different from the previously reported ground state in the titanate systems. By applying +2.8% of tensile strains, we showed that the antiferromagnetic-spin and ferro-orbital ordered phase become stabilized.

  1. Graphene ground states

    NASA Astrophysics Data System (ADS)

    Friedrich, Manuel; Stefanelli, Ulisse

    2018-06-01

    Graphene is locally two-dimensional but not flat. Nanoscale ripples appear in suspended samples and rolling up often occurs when boundaries are not fixed. We address this variety of graphene geometries by classifying all ground-state deformations of the hexagonal lattice with respect to configurational energies including two- and three-body terms. As a consequence, we prove that all ground-state deformations are either periodic in one direction, as in the case of ripples, or rolled up, as in the case of nanotubes.

  2. The ground state tunneling splitting and the zero point energy of malonaldehyde: a quantum Monte Carlo determination.

    PubMed

    Viel, Alexandra; Coutinho-Neto, Maurício D; Manthe, Uwe

    2007-01-14

    Quantum dynamics calculations of the ground state tunneling splitting and of the zero point energy of malonaldehyde on the full dimensional potential energy surface proposed by Yagi et al. [J. Chem. Phys. 1154, 10647 (2001)] are reported. The exact diffusion Monte Carlo and the projection operator imaginary time spectral evolution methods are used to compute accurate benchmark results for this 21-dimensional ab initio potential energy surface. A tunneling splitting of 25.7+/-0.3 cm-1 is obtained, and the vibrational ground state energy is found to be 15 122+/-4 cm-1. Isotopic substitution of the tunneling hydrogen modifies the tunneling splitting down to 3.21+/-0.09 cm-1 and the vibrational ground state energy to 14 385+/-2 cm-1. The computed tunneling splittings are slightly higher than the experimental values as expected from the potential energy surface which slightly underestimates the barrier height, and they are slightly lower than the results from the instanton theory obtained using the same potential energy surface.

  3. The ground-state energy of the ± J sping glass. A comparison of various biologically motivated algorithms

    NASA Astrophysics Data System (ADS)

    Gropengiesser, Uwe

    1995-06-01

    We compare various evlutionary strategies to determine the ground-state energy of the ± J spin glass. We show that the choice of different evolution laws is less important than a suitable treatment of the "free spins" of the system At least one combination of these strategies does not give the correct results, but the ground states of the other different strategies coincide. Therefore we are able to extrapolate the infinit-size ground-state energy for the square lattice to -1.401±0.0015 and for the simple cubic lattice to -1.786±0.004.

  4. Regularities in the sequences of the number of nucleons in the revolving clusters for the ground-state energy bands of the even-even nuclei with neutron number equal to or greater than 126.

    PubMed Central

    Pauling, L

    1990-01-01

    Values of m, the number of nucleons in the revolving cluster, and of R, the radius of revolution of the cluster about the center of mass of the spherical part of the nucleus, are calculated from the observed values of the energy for the ground-state bands of all nuclei with neutron number N >/= 126 on the basis of the assumptions (i) that both m and R change in a reasonable way with increase in the angular momentum quantum number J and with change in the proton number Z and the neutron number N, (ii) that m is usually an even integer, (iii) that certain clusters are especially stable, and (iv) that there is a special stability of the doubly magic sphere p82n126. PMID:11607085

  5. Use of ground-based radiometers for L-Band Freeze/Thaw retrieval in a boreal forest site

    NASA Astrophysics Data System (ADS)

    Roy, A.; Sonnentag, O.; Derksen, C.; Toose, P.; Pappas, C.; Mavrovic, A.; El Amine, M.; Royer, A.; Berg, A. A.; Rowlandson, T. L.; Barr, A.; Black, T. A.

    2017-12-01

    The boreal forest is the second largest land biome in the world and thus plays a major role in the global and regional climate systems. The extent, timing and duration of the seasonal freeze/thaw (F/T) state influences vegetation developmental stages (phenology) and, consequently, constitutes an important control on how boreal forest ecosystems exchange carbon, water and energy with the atmosphere. Recently, new L-Band satellite-derived F/T information has become available. However, disentangling the seasonally differing contributions from forest overstory and understory vegetation, and the ground surface to the satellite signal remains challenging. Here we present results from an ongoing campaign with two L-Band surface-based radiometers (SBR) installed on a micrometeorological tower at the Southern Old Black Spruce site (53.99°N / 105.12°W) in central Saskatchewan. One radiometer unit is installed on top of the tower viewing the multi-layer vegetation canopy from above. A second radiometer unit is installed within the multi-layer canopy, viewing the understory and the ground surface only. The objectives of our study are to (i) disentangle the L-Band F/T signal contribution of boreal forest overstory from the combined understory and ground surface contribution, and (ii) link the L-Band F/T signal to related boreal forest structural and functional characteristics. Analysis of these radiometer measurements made from September to November 2016 shows that when the ground surface is thawed, the main contributor to both radiometer signals is soil moisture. The Pearson correlation coefficient between brightness temperature (TB) at vertical polarization (V-pol) and soil permittivity is 0.79 for the radiometer above the canopy and 0.74 for the radiometer below the canopy. Under cold conditions when the soil was thawed (snow insulation) and the trees were frozen (below 0°C), TB at V-pol is negatively correlated with tree permittivity. The freezing tree contribution to

  6. Direct imaging of band profile in single layer MoS2 on graphite: quasiparticle energy gap, metallic edge states, and edge band bending.

    PubMed

    Zhang, Chendong; Johnson, Amber; Hsu, Chang-Lung; Li, Lain-Jong; Shih, Chih-Kang

    2014-05-14

    Using scanning tunneling microscopy and spectroscopy, we probe the electronic structures of single layer MoS2 on graphite. The apparent quasiparticle energy gap of single layer MoS2 is measured to be 2.15 ± 0.06 eV at 77 K, albeit a higher second conduction band threshold at 0.2 eV above the apparent conduction band minimum is also observed. Combining it with photoluminescence studies, we deduce an exciton binding energy 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 band maximum, possibly due to the formation of a graphite/MoS2 heterojunction. At the edge, however, we observe an upward band 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.

  7. On the ground state energy of the delta-function Fermi gas

    NASA Astrophysics Data System (ADS)

    Tracy, Craig A.; Widom, Harold

    2016-10-01

    The weak coupling asymptotics to order γ of the ground state energy of the delta-function Fermi gas, derived heuristically in the literature, is here made rigorous. Further asymptotics are in principle computable. The analysis applies to the Gaudin integral equation, a method previously used by one of the authors for the asymptotics of large Toeplitz matrices.

  8. Orbital stability and energy estimate of ground states of saturable nonlinear Schrödinger equations with intensity functions in R2

    NASA Astrophysics Data System (ADS)

    Lin, Tai-Chia; Wang, Xiaoming; Wang, Zhi-Qiang

    2017-10-01

    Conventionally, the existence and orbital stability of ground states of nonlinear Schrödinger (NLS) equations with power-law nonlinearity (subcritical case) can be proved by an argument using strict subadditivity of the ground state energy and the concentration compactness method of Cazenave and Lions [4]. However, for saturable nonlinearity, such an argument is not applicable because strict subadditivity of the ground state energy fails in this case. Here we use a convexity argument to prove the existence and orbital stability of ground states of NLS equations with saturable nonlinearity and intensity functions in R2. Besides, we derive the energy estimate of ground states of saturable NLS equations with intensity functions using the eigenvalue estimate of saturable NLS equations without intensity function.

  9. 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

  10. Conduction Band-Edge Non-Parabolicity Effects on Impurity States in (In,Ga)N/GaN Cylindrical QWWs

    NASA Astrophysics Data System (ADS)

    Haddou El, Ghazi; Anouar, Jorio

    2014-02-01

    In this paper, the conduction band-edge non-parabolicity (NP) and the circular cross-section radius effects on hydrogenic shallow-donor impurity ground-state binding energy in zinc-blende (ZB) InGaN/GaN cylindrical QWWs are reported. The finite potential barrier between (In,Ga)N well and GaN environment is considered. Two models of the conduction band-edge non-parabolicity are taking into account. The variational approach is used within the framework of single band effective-mass approximation with one-parametric 1S-hydrogenic trial wave-function. It is found that NP effect is more pronounced in the wire of radius equal to effective Bohr radius than in large and narrow wires. Moreover, the binding energy peak shifts to narrow wire under NP effect. A good agreement is shown compared to the findings results.

  11. On the ground state energy of the δ-function Bose gas

    NASA Astrophysics Data System (ADS)

    Tracy, Craig A.; Widom, Harold

    2016-07-01

    The weak coupling asymptotics, to order {(c/ρ )}2, of the ground state energy of the delta-function Bose gas is derived. Here 2c≥slant 0 is the delta-function potential amplitude and ρ the density of the gas in the thermodynamic limit. The analysis uses the electrostatic interpretation of the Lieb-Liniger integral equation. Dedicated to Professor Tony Guttmann on the occasion of his 70th birthday.

  12. The laboratory millimeter-wave spectrum of methyl formate in its ground torsional E state

    NASA Technical Reports Server (NTRS)

    Plummer, G. M.; Herbst, E.; De Lucia, F. C.; Blake, G. A.

    1986-01-01

    Over 250 rotational transitions of the internal rotor methyl formate (HCOOCH3) in its ground v(t) = 0 degenerate (E) torsional substate have been measured in the millimeter-wave spectral region. These data and a number of E-state lines identified by several other workers have been analyzed using an extension of the classical principal-axis method in the high barrier limit. The resulting rotational constants allow accurate prediction of the v(t) = 0 E substate methyl formate spectrum below 300 GHz between states with angular momentum J not greater than 30 and rotational energy of not more than 350/cm. The calculated transition frequencies for the E state, when combined with the results of the previous analysis of the ground-symmetric, nondegenerate state, account for over 200 of the emission lines observed toward Orion in a recent survey of the 215-265 GHz band.

  13. Temperature Effect of Hydrogen-Like Impurity on the Ground State Energy of Strong Coupling Polaron in a RbCl Quantum Pseudodot

    NASA Astrophysics Data System (ADS)

    Xiao, Jing-Lin

    2016-11-01

    We study the ground state energy and the mean number of LO phonons of the strong-coupling polaron in a RbCl quantum pseudodot (QPD) with hydrogen-like impurity at the center. The variations of the ground state energy and the mean number of LO phonons with the temperature and the strength of the Coulombic impurity potential are obtained by employing the variational method of Pekar type and the quantum statistical theory (VMPTQST). Our numerical results have displayed that [InlineMediaObject not available: see fulltext.] the absolute value of the ground state energy increases (decreases) when the temperature increases at lower (higher) temperature regime, [InlineMediaObject not available: see fulltext.] the mean number of the LO phonons increases with increasing temperature, [InlineMediaObject not available: see fulltext.] the absolute value of ground state energy and the mean number of LO phonons are increasing functions of the strength of the Coulombic impurity potential.

  14. Pulsed-field ionization zero electron kinetic energy spectrum of the ground electronic state of BeOBe+.

    PubMed

    Antonov, Ivan O; Barker, Beau J; Heaven, Michael C

    2011-01-28

    The ground electronic state of BeOBe(+) was probed using the pulsed-field ionization zero electron kinetic energy photoelectron technique. Spectra were rotationally resolved and transitions to the zero-point level, the symmetric stretch fundamental and first two bending vibrational levels were observed. The rotational state symmetry selection rules confirm that the ground electronic state of the cation is (2)Σ(g)(+). Detachment of an electron from the HOMO of neutral BeOBe results in little change in the vibrational or rotational constants, indicating that this orbital is nonbonding in nature. The ionization energy of BeOBe [65480(4) cm(-1)] was refined over previous measurements. Results from recent theoretical calculations for BeOBe(+) (multireference configuration interaction) were found to be in good agreement with the experimental data.

  15. Electronic states and potential energy curves of molybdenum carbide and its ions

    NASA Astrophysics Data System (ADS)

    Denis, Pablo A.; Balasubramanian, K.

    2006-07-01

    The potential energy curves and spectroscopic constants of the ground and 29 low-lying excited states of MoC with different spin and spatial symmetries within 48000cm-1 have been investigated. We have used the complete active space multiconfiguration self-consistent field methodology, followed by multireference configuration interaction (MRCI) methods. Relativistic effects were considered with the aid of relativistic effective core potentials in conjunction with these methods. The results are in agreement with previous studies that determined the ground state as XΣ-3. At the MRCISD +Q level, the transition energies to the 1Δ3 and 4Δ1 states are 3430 and 8048cm-1, respectively, in fair agreement with the results obtained by DaBell et al. [J. Chem. Phy. 114, 2938 (2001)], namely, 4003 and 7834cm-1, respectively. The three band systems located at 18 611, 20 700, and 22520cm-1 observed by Brugh et al. [J. Chem. Phy. 109, 7851 (1998)] were attributed to the excited 11Σ-3, 14Π3, and 15Π1 states respectively. At the MRCISD level, these states are 17 560, 20 836, and 20952cm-1 above the ground state respectively. We have also identified a Π3 state lying 14309cm-1 above the ground state. The ground states of the molecular ions are predicted to be Σ-4 and Δ2 for MoC- and MoC+, respectively.

  16. Global potential energy surface of ground state singlet spin O4

    NASA Astrophysics Data System (ADS)

    Mankodi, Tapan K.; Bhandarkar, Upendra V.; Puranik, Bhalchandra P.

    2018-02-01

    A new global potential energy for the singlet spin state O4 system is reported using CASPT2/aug-cc-pVTZ ab initio calculations. The geometries for the six-dimensional surface are constructed using a novel point generation scheme that employs randomly generated configurations based on the beta distribution. The advantage of this scheme is apparent in the reduction of the number of required geometries for a reasonably accurate potential energy surface (PES) and the consequent decrease in the overall computational effort. The reported surface matches well with the recently published singlet surface by Paukku et al. [J. Chem. Phys. 147, 034301 (2017)]. In addition to the O4 PES, the ground state N4 PES is also constructed using the point generation scheme and compared with the existing PES [Y. Paukku et al., J. Chem. Phys. 139, 044309 (2013)]. The singlet surface is constructed with the aim of studying high energy O2-O2 collisions and predicting collision induced dissociation cross section to be used in simulating non-equilibrium aerothermodynamic flows.

  17. Derivation of the RPA (Random Phase Approximation) Equation of ATDDFT (Adiabatic Time Dependent Density Functional Ground State Response Theory) from an Excited State Variational Approach Based on the Ground State Functional.

    PubMed

    Ziegler, Tom; Krykunov, Mykhaylo; Autschbach, Jochen

    2014-09-09

    The random phase approximation (RPA) equation of adiabatic time dependent density functional ground state response theory (ATDDFT) has been used extensively in studies of excited states. It extracts information about excited states from frequency dependent ground state response properties and avoids, thus, in an elegant way, direct Kohn-Sham calculations on excited states in accordance with the status of DFT as a ground state theory. Thus, excitation energies can be found as resonance poles of frequency dependent ground state polarizability from the eigenvalues of the RPA equation. ATDDFT is approximate in that it makes use of a frequency independent energy kernel derived from the ground state functional. It is shown in this study that one can derive the RPA equation of ATDDFT from a purely variational approach in which stationary states above the ground state are located using our constricted variational DFT (CV-DFT) method and the ground state functional. Thus, locating stationary states above the ground state due to one-electron excitations with a ground state functional is completely equivalent to solving the RPA equation of TDDFT employing the same functional. The present study is an extension of a previous work in which we demonstrated the equivalence between ATDDFT and CV-DFT within the Tamm-Dancoff approximation.

  18. Implementation of rigorous renormalization group method for ground space and low-energy states of local Hamiltonians

    NASA Astrophysics Data System (ADS)

    Roberts, Brenden; Vidick, Thomas; Motrunich, Olexei I.

    2017-12-01

    The success of polynomial-time tensor network methods for computing ground states of certain quantum local Hamiltonians has recently been given a sound theoretical basis by Arad et al. [Math. Phys. 356, 65 (2017), 10.1007/s00220-017-2973-z]. The convergence proof, however, relies on "rigorous renormalization group" (RRG) techniques which differ fundamentally from existing algorithms. We introduce a practical adaptation of the RRG procedure which, while no longer theoretically guaranteed to converge, finds matrix product state ansatz approximations to the ground spaces and low-lying excited spectra of local Hamiltonians in realistic situations. In contrast to other schemes, RRG does not utilize variational methods on tensor networks. Rather, it operates on subsets of the system Hilbert space by constructing approximations to the global ground space in a treelike manner. We evaluate the algorithm numerically, finding similar performance to density matrix renormalization group (DMRG) in the case of a gapped nondegenerate Hamiltonian. Even in challenging situations of criticality, large ground-state degeneracy, or long-range entanglement, RRG remains able to identify candidate states having large overlap with ground and low-energy eigenstates, outperforming DMRG in some cases.

  19. Resonant two-photon ionization spectroscopy of jet-cooled UN: determination of the ground state.

    PubMed

    Matthew, Daniel J; Morse, Michael D

    2013-05-14

    The optical transitions of supersonically cooled uranium nitride (UN) have been investigated in the range from 19,200 to 23,900 cm(-1) using resonant two-photon ionization spectroscopy. A large number of bands have been observed, of which seven have been rotationally resolved and analyzed. All are found to arise from the same state, which is presumably the ground state of the molecule. From the analysis of the bands, the ground state has Ω = 3.5, with a bond length of 1.7650(12) Å. Comparisons to the known isovalent molecules are made, and the variations in ground state configuration are explained in terms of the configurational reordering that occurs with changes in the nuclear and ligand charges. It is concluded that the UN molecule is best considered as a U(3+)N(3-) species in which the closed shell nitride ligand interacts with a U(3+) ion. The ground state of the molecule derives from a U(3+) ion in its 7s(1)5f 2) atomic configuration.

  20. Ground Levels and Ionization Energies for the Neutral Atoms

    National Institute of Standards and Technology Data Gateway

    SRD 111 Ground Levels and Ionization Energies for the Neutral Atoms (Web, free access)   Data for ground state electron configurations and ionization energies for the neutral atoms (Z = 1-104) including references.

  1. Theoretical Electric Dipole Moments and Dissociation Energies for the Ground States of GaH-BrH

    NASA Technical Reports Server (NTRS)

    Pettersson, Lars G. M.; Langhoff, Stephen R.

    1986-01-01

    Reliable experimental diople moments are available for the ground states of SeH and BrH whereas no values have been reported for GaH and AsH a recently reported experimental dipole moment for GeH of 1.24 + or -0.01 D has been seriously questioned, and a much lower value of, 0.1 + or - 0.05 D, suggested. In this work, we report accurate theoretical dipole moments, dipole derivatives, dissociation energies, and spectroscopic constants (tau(sub e), omega(sub e)) for the ground states of GaH through BrH.

  2. Classical many-particle systems with unique disordered ground states

    NASA Astrophysics Data System (ADS)

    Zhang, G.; Stillinger, F. H.; Torquato, S.

    2017-10-01

    Classical ground states (global energy-minimizing configurations) of many-particle systems are typically unique crystalline structures, implying zero enumeration entropy of distinct patterns (aside from trivial symmetry operations). By contrast, the few previously known disordered classical ground states of many-particle systems are all high-entropy (highly degenerate) states. Here we show computationally that our recently proposed "perfect-glass" many-particle model [Sci. Rep. 6, 36963 (2016), 10.1038/srep36963] possesses disordered classical ground states with a zero entropy: a highly counterintuitive situation . For all of the system sizes, parameters, and space dimensions that we have numerically investigated, the disordered ground states are unique such that they can always be superposed onto each other or their mirror image. At low energies, the density of states obtained from simulations matches those calculated from the harmonic approximation near a single ground state, further confirming ground-state uniqueness. Our discovery provides singular examples in which entropy and disorder are at odds with one another. The zero-entropy ground states provide a unique perspective on the celebrated Kauzmann-entropy crisis in which the extrapolated entropy of a supercooled liquid drops below that of the crystal. We expect that our disordered unique patterns to be of value in fields beyond glass physics, including applications in cryptography as pseudorandom functions with tunable computational complexity.

  3. FeRh ground state and martensitic transformation

    NASA Astrophysics Data System (ADS)

    Zarkevich, Nikolai A.; Johnson, Duane D.

    2018-01-01

    Cubic B 2 FeRh exhibits a metamagnetic transition [(111) antiferromagnet (AFM) to ferromagnet (FM)] around 353 K and remains structurally stable at higher temperatures. However, the calculated zero-Kelvin phonons of AFM FeRh exhibit imaginary modes at M points in the Brillouin zone, indicating a premartensitic instability, which is a precursor to a martensitic transformation at low temperatures. Combining electronic-structure calculations with ab initio molecular dynamics, conjugate gradient relaxation, and the solid-state nudged-elastic band methods, we predict that AFM B 2 FeRh becomes unstable at ambient pressure and transforms without a barrier to an AFM(111) orthorhombic (martensitic) ground state below 90 ±10 K . We also consider competing structures, in particular, a tetragonal AFM(100) phase that is not the global ground state, as proposed [Phys. Rev. B 94, 180407(R) (2016), 10.1103/PhysRevB.94.180407], but a constrained solution.

  4. FeRh ground state and martensitic transformation

    DOE PAGES

    Zarkevich, Nikolai A.; Johnson, Duane D.

    2018-01-09

    Cubic B2 FeRh exhibits a metamagnetic transition [(111) antiferromagnet (AFM) to ferromagnet (FM)] around 353 K and remains structurally stable at higher temperatures. However, the calculated zero-Kelvin phonons of AFM FeRh exhibit imaginary modes at M points in the Brillouin zone, indicating a premartensitic instability, which is a precursor to a martensitic transformation at low temperatures. Combining electronic-structure calculations with ab initio molecular dynamics, conjugate gradient relaxation, and the solid-state nudged-elastic band methods, we predict that AFM B2 FeRh becomes unstable at ambient pressure and transforms without a barrier to an AFM(111) orthorhombic (martensitic) ground state below 90±10K. In conclusion,more » we also consider competing structures, in particular, a tetragonal AFM(100) phase that is not the global ground state, as proposed, but a constrained solution.« less

  5. High-resolution spectroscopy of the C-N stretching band of methylamine

    NASA Astrophysics Data System (ADS)

    Lees, Ronald M.; Sun, Zhen-Dong; Billinghurst, B. E.

    2011-09-01

    The C-N stretching infrared fundamental of CH3NH2 has been investigated by high-resolution laser sideband and Fourier transform synchrotron spectroscopy to explore the energy level structure and to look for possible interactions with high-lying torsional levels of the ground state and other vibrational modes. The spectrum is complicated by two coupled large-amplitude motions in the molecule, the CH3 torsion and the NH2 inversion, which lead to rich spectral structure with a wide range of energy level splittings and relative line intensities. Numerous sub-bands have been assigned for K values ranging up to 12 for the stronger a inversion species for the vt = 0 torsional state, along with many of the weaker sub-bands of the s species. The C-N stretching sub-state origins have been determined by fitting the upper-state term values to J(J + 1) power-series expansions. For comparison with the ground-state behaviour, both ground and C-N stretch origins have been fitted to a phenomenological Fourier series model that produces an interesting pattern with the differing periodicities of the torsional and inversion energies. The amplitude of the torsional energy oscillation increases substantially for the C-N stretch, while the amplitude of the inversion energy oscillation is relatively unchanged. Independent inertial scale factors ρ were fitted for the torsion and the inversion and differ significantly in the upper state. The C-N stretching vibrational energy is determined to be 1044.817 cm-1, while the effective upper state B-value is 0.7318 cm-1. Several anharmonic resonances with vt = 4 ground-state levels have been observed and partially characterized. A variety of J-localized level-crossing resonances have also been seen, five of which display forbidden transitions arising from intensity borrowing that allow determination of the interaction coupling constants.

  6. Evolution from quasivibrational to quasirotational structure in 155Tm and yrast 27 /2- to 25 /2- energy anomaly in the A ≈150 mass region

    NASA Astrophysics Data System (ADS)

    Liu, L.; Wang, S. Y.; Wang, S.; Hua, H.; Zhang, S. Q.; Meng, J.; Bark, R. A.; Wyngaardt, S. M.; Qi, B.; Sun, D. P.; Liu, C.; Li, Z. Q.; Jia, H.; Li, X. Q.; Xu, C.; Li, Z. H.; Sun, J. J.; Zhu, L. H.; Jones, P.; Lawrie, E. A.; Lawrie, J. J.; Wiedeking, M.; Bucher, T. D.; Dinoko, T.; Makhathini, L.; Majola, S. N. T.; Noncolela, S. P.; Shirinda, O.; Gál, J.; Kalinka, G.; Molnár, J.; Nyakó, B. M.; Timár, J.; Juhász, K.; Arogunjo, M.

    2018-04-01

    Excited states in 155Tm have been populated via the reaction 144Sm(16O, p 4 n )155Tm at a beam energy of 118 MeV. The ground-state band has been extended and a new side band of the ground-state band is identified. E-GOS curves and potential energy surface calculations are employed to discuss the structure evolution of the ground-state band. The newly observed side band in 155Tm is discussed based on the spin/energy systematics. In particular, the phenomenon of seniority inversion is proposed in 155Tm, and a systematic study of this phenomenon in the A ≈150 mass region is performed.

  7. Ground and excited states of zinc phthalocyanine, zinc tetrabenzoporphyrin, and azaporphyrin analogs using DFT and TDDFT with Franck-Condon analysis

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

    Theisen, Rebekah F., E-mail: rtheisen@asu.edu; Huang, Liang; Fleetham, Tyler

    2015-03-07

    The electronic structure of eight zinc-centered porphyrin macrocyclic molecules are investigated using density functional theory for ground-state properties, time-dependent density functional theory (TDDFT) for excited states, and Franck-Condon (FC) analysis for further characterization of the UV-vis spectrum. Symmetry breaking was utilized to find the lowest energy of the excited states for many states in the spectra. To confirm the theoretical modeling, the spectroscopic result from zinc phthalocyanine (ZnPc) is used to compare to the TDDFT and FC result. After confirmation of the modeling, five more planar molecules are investigated: zinc tetrabenzoporphyrin (ZnTBP), zinc tetrabenzomonoazaporphyrin (ZnTBMAP), zinc tetrabenzocisdiazaporphyrin (ZnTBcisDAP), zinc tetrabenzotransdiazaporphyrinmore » (ZnTBtransDAP), and zinc tetrabenzotriazaporphyrin (ZnTBTrAP). The two latter molecules are then compared to their phenylated sister molecules: zinc monophenyltetrabenzotriazaporphyrin (ZnMPTBTrAP) and zinc diphenyltetrabenzotransdiazaporphyrin (ZnDPTBtransDAP). The spectroscopic results from the synthesis of ZnMPTBTrAP and ZnDPTBtransDAP are then compared to their theoretical models and non-phenylated pairs. While the Franck-Condon results were not as illuminating for every B-band, the Q-band results were successful in all eight molecules, with a considerable amount of spectral analysis in the range of interest between 300 and 750 nm. The π-π{sup ∗} transitions are evident in the results for all of the Q bands, while satellite vibrations are also visible in the spectra. In particular, this investigation finds that, while ZnPc has a D{sub 4h} symmetry at ground state, a C{sub 4v} symmetry is predicted in the excited-state Q band region. The theoretical results for ZnPc found an excitation energy at the Q-band 0-0 transition of 1.88 eV in vacuum, which is in remarkable agreement with published gas-phase spectroscopy, as well as our own results of ZnPc in solution

  8. Full-dimensional ground- and excited-state potential energy surfaces and state couplings for photodissociation of thioanisole

    NASA Astrophysics Data System (ADS)

    Li, Shaohong L.; Truhlar, Donald G.

    2017-02-01

    Analytic potential energy surfaces (PESs) and state couplings of the ground and two lowest singlet excited states of thioanisole (C6H5SCH3) are constructed in a diabatic representation based on electronic structure calculations including dynamic correlation. They cover all 42 internal degrees of freedom and a wide range of geometries including the Franck-Condon region and the reaction valley along the breaking S-CH3 bond with the full ranges of the torsion angles. The parameters in the PESs and couplings are fitted to the results of smooth diabatic electronic structure calculations including dynamic electron correlation by the extended multi-configurational quasi-degenerate perturbation theory method for the adiabatic state energies followed by diabatization by the fourfold way. The fit is accomplished by the anchor points reactive potential method with two reactive coordinates and 40 nonreactive degrees of freedom, where the anchor-point force fields are obtained with a locally modified version of the QuickFF package. The PESs and couplings are suitable for study of the topography of the trilayer potential energy landscape and for electronically nonadiabatic molecular dynamics simulations of the photodissociation of the S-CH3 bond.

  9. Tuning the Ground State Symmetry of Acetylenyl Radicals

    PubMed Central

    2015-01-01

    The lowest excited state of the acetylenyl radical, HCC, is a 2Π state, only 0.46 eV above the ground state, 2Σ+. The promotion of an electron from a π bond pair to a singly occupied σ hybrid orbital is all that is involved, and so we set out to tune those orbital energies, and with them the relative energetics of 2Π and 2Σ+ states. A strategy of varying ligand electronegativity, employed in a previous study on substituted carbynes, RC, was useful, but proved more difficult to apply for substituted acetylenyl radicals, RCC. However, π-donor/acceptor substitution is effective in modifying the state energies. We are able to design molecules with 2Π ground states (NaOCC, H2NCC (2A″), HCSi, FCSi, etc.) and vary the 2Σ+–2Π energy gap over a 4 eV range. We find an inconsistency between bond order and bond dissociation energy measures of the bond strength in the Si-containing molecules; we provide an explanation through an analysis of the relevant potential energy curves. PMID:27162981

  10. Spin dependence of intra-ground-state-band E2 transitions in the SU(3) limit of the sdg interacting boson model

    NASA Astrophysics Data System (ADS)

    Long, G. L.; Ji, H. Y.

    1998-04-01

    B(E2, L+2-->L) transitions in the sdg interacting boson model SU(3) limit are studied with a general E2 transition operator. Analytical expressions are obtained using a group theoretic method. It is found that when using transition operators of the form (d†g~+g†d~)2 or (g†g~)2, the B(E2, L+2-->L) values in the ground-state band have an L(L+3) dependent term. As L increases, the B(E2) values can be larger than the rigid rotor model value. Application to 236,238U is discussed.

  11. Valence-band states in Bi2(Ca,Sr,La)3Cu2O8

    NASA Astrophysics Data System (ADS)

    Wells, B. O.; Lindberg, P. A. P.; Shen, Z.-X.; Dessau, D. S.; Spicer, W. E.; Lindau, I.; Mitzi, D. B.; Kapitulnik, A.

    1989-09-01

    We have used photoemission spectroscopy to examine the symmetry of the occupied states of the valence band for the La-doped superconductor Bi2(Ca,Sr,La)3Cu2O8. While the oxygen states near the bottom of the 7-eV wide valence band exhibit predominantly O 2pz symmetry, the states at the top of the valence band extending to the Fermi level are found to have primarily O 2px and O 2py character. We have also examined anomalous intensity enhancements in the valence-band features for photon energies near 18 eV. These enhancements, which occur at photon energies ranging from 15.8 to 18.0 eV for the different valence-band features, are not consistent with either simple final-state effects or direct O 2s transitions to unoccupied O 2p states.

  12. Dynamics Near the Ground State for the Energy Critical Nonlinear Heat Equation in Large Dimensions

    NASA Astrophysics Data System (ADS)

    Collot, Charles; Merle, Frank; Raphaël, Pierre

    2017-05-01

    We consider the energy critical semilinear heat equation partial_tu = Δ u + |u|^{4/d-2}u, \\quad x \\in {R}^d and give a complete classification of the flow near the ground state solitary wave Q(x) = 1/(1+{|x|^2{d(d-2)})^{d-2/2}} in dimension {d ≥ 7}, in the energy critical topology and without radial symmetry assumption. Given an initial data {Q + ɛ_0} with {|\

  13. Nuts and Bolts of the Ion Band State Theory

    NASA Astrophysics Data System (ADS)

    Chubb, Scott R.

    2005-12-01

    The nuts and bolts of our ion band state 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 PdHx, this bonding is strongly correlated with loading. In ambient loading conditions (x ≲ 0.6), bonding inhibits ion band 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 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. In the past, implicitly, we have used these facts to justify our ion band state theory. Here, we present a more formal justification, based on the relationship between H(D) ion band 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.

  14. Nudged-elastic band method with two climbing images: Finding transition states in complex energy landscapes

    DOE PAGES

    Zarkevich, Nikolai A.; Johnson, Duane D.

    2015-01-09

    The nudged-elastic band (NEB) method is modified with concomitant two climbing images (C2-NEB) to find a transition state (TS) in complex energy landscapes, such as those with a serpentine minimal energy path (MEP). If a single climbing image (C1-NEB) successfully finds the TS, then C2-NEB finds it too. Improved stability of C2-NEB makes it suitable for more complex cases, where C1-NEB misses the TS because the MEP and NEB directions near the saddle point are different. Generally, C2-NEB not only finds the TS, but guarantees, by construction, that the climbing images approach it from the opposite sides along the MEP.more » In addition, C2-NEB provides an accuracy estimate from the three images: the highest-energy one and its climbing neighbors. C2-NEB is suitable for fixed-cell NEB and the generalized solid-state NEB.« less

  15. High-resolution Fourier transform synchrotron spectroscopy of the C-S stretching band of methyl mercaptan, CH332SH

    NASA Astrophysics Data System (ADS)

    Lees, R. M.; Xu, Li-Hong; Billinghurst, B. E.

    2016-01-01

    The C-S stretching fundamental band of 12CH332SH, the principal isotopologue of methyl mercaptan, has been investigated by Fourier transform infrared spectroscopy on the Far-Infrared beamline at the Canadian Light Source synchrotron. The band is centered around 710 cm-1 and shows well-resolved a-type parallel structure. Most of the A and E spectral sub-bands have been assigned up to K = 12 for the vt = 0 torsional state and K = 9 for the vt = 1 state, along with a smaller variety of sub-bands for vt = 2. C-S stretching energy term values have been determined employing known ground-state energies, and have been fitted to series expansions in powers of J(J + 1) to determine the substate origins. The origins have in turn been fitted to a Fourier model to characterize the oscillatory torsional energy structure of the C-S stretching state. The amplitude of oscillation of the vt = 0 torsional curves is significantly larger for the C-S stretch state compared to the ground state. A strategy devised to relate this amplitude to an effective torsional barrier height indicates a decrease of about 7% in the effective V3 for the C-S stretch. The vibrational frequency determined for the stretching fundamental from the Fourier fit is 710.3 cm-1. The C-S stretching manifold is crossed by excited vt = 4 torsional levels of the ground state, and strong torsion-vibrational resonant coupling is observed via perturbations in the spectrum together with forbidden sub-bands induced by mixing and intensity borrowing.

  16. Observation of double-well potential of NaH C 1Σ+ state: Deriving the dissociation energy of its ground state

    NASA Astrophysics Data System (ADS)

    Chu, Chia-Ching; Huang, Hsien-Yu; Whang, Thou-Jen; Tsai, Chin-Chun

    2018-03-01

    Vibrational levels (v = 6-42) of the NaH C 1Σ+ state including the inner and outer wells and the near-dissociation region were observed by pulsed optical-optical double resonance fluorescence depletion spectroscopy. The absolute vibrational quantum number is identified by comparing the vibrational energy difference of this experiment with the ab initio calculations. The outer well with v up to 34 is analyzed using the Dunham expansion and a Rydberg-Klein-Rees (RKR) potential energy curve is constructed. A hybrid double-well potential combined with the RKR potential, the ab initio calculation, and a long-range potential is able to describe the whole NaH C 1Σ+ state including the higher vibrational levels (v = 35-42). The dissociation energy of the NaH C 1Σ+ state is determined to be De(C) = 6595.10 ± 5 cm-1 and then the dissociation energy of the NaH ground state De(X) = 15 807.87 ± 5 cm-1 can be derived.

  17. Scaling behavior of ground-state energy cluster expansion for linear polyenes

    NASA Astrophysics Data System (ADS)

    Griffin, L. L.; Wu, Jian; Klein, D. J.; Schmalz, T. G.; Bytautas, L.

    Ground-state energies for linear-chain polyenes are additively expanded in a sequence of terms for chemically relevant conjugated substructures of increasing size. The asymptotic behavior of the large-substructure limit (i.e., high-polymer limit) is investigated as a means of characterizing the rapidity of convergence and consequent utility of this energy cluster expansion. Consideration is directed to computations via: simple Hückel theory, a refined Hückel scheme with geometry optimization, restricted Hartree-Fock self-consistent field (RHF-SCF) solutions of fixed bond-length Parisier-Parr-Pople (PPP)/Hubbard models, and ab initio SCF approaches with and without geometry optimization. The cluster expansion in what might be described as the more "refined" approaches appears to lead to qualitatively more rapid convergence: exponentially fast as opposed to an inverse power at the simple Hückel or SCF-Hubbard levels. The substructural energy cluster expansion then seems to merit special attention. Its possible utility in making accurate extrapolations from finite systems to extended polymers is noted.

  18. Novel solution of power law for γ-bands

    NASA Astrophysics Data System (ADS)

    Gupta, J. B.

    The power law expression E = aIb offers a single-term formula with just two parameters for expressing the level energies in the spectra of even-Z even-N nuclei. Its application to ground band spectra for a wide range of nuclei has been demonstrated in our earlier works. Here, we extend its application to the rotational bands built on an excited state of K = 2 γ-vibration band and Kπ = 0 2+ beta band. A novel assumption of a virtual level with spin zero for γ-bands is made and its validity and use is illustrated. Here, the constancy of the parameters “b” and “a” with spin, offers a more realistic view of the dependence of the nuclear core deformation on spin, in the excited bands. Also, it enables a spinwise view, not available in the other energy fit expressions.

  19. High-resolution infrared spectroscopy of the asymmetric NO stretch band of jet-cooled nitromethane and assignment of the lowest four torsional states

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

    Dawadi, Mahesh B.; Degliumberto, Lou; Perry, David S.

    A high-throughput CW slit-jet apparatus coupled to a high-resolution FTIR was used to record the asymmetric NO stretch band of nitromethane. The b-type band, including torsionally excited states with m ≤ 3, has been assigned for Ka" ≤ 10, J" ≤ 20. The ground state combination differences derived from these assigned levels were fit with the RAM36 program to give an RMS deviation of 0.0006 cm-1. The band origin is 1583.0 (+/- 0.1) cm-1 and the torsional level spacing is nearly identical to that in the ground state. The upper state levels are split into multiplets by perturbations. A subsetmore » of the available upper state combination differences for m = 0, Ka' ≤ 7, J' ≤ 10 were fit with the same program, but with rather poorer precision (0.01 cm-1) than for the ground state.« less

  20. High-resolution infrared spectroscopy of the asymmetric NO stretch band of jet-cooled nitromethane and assignment of the lowest four torsional states

    NASA Astrophysics Data System (ADS)

    Dawadi, Mahesh B.; Degliumberto, Lou; Perry, David S.; Mettee, Howard D.; Sams, Robert L.

    2018-01-01

    A high-throughput CW slit-jet apparatus coupled to a high-resolution FTIR was used to record the asymmetric NO stretch band of nitromethane. The b-type band, including torsionally excited states with m ≤ 3, has been assigned for Ka″ ≤ 10, J″ ≤ 20. The ground state combination differences derived from these assigned levels were fit with the RAM36 program to give an RMS deviation of 0.0006 cm-1. The band origin is 1583.0 (±0.1) cm-1 and the torsional level spacing is nearly identical to that in the ground state. The upper state levels are split into multiplets by perturbations. A subset of the available upper state combination differences for m = 0, Ka‧ ≤ 7, J‧ ≤ 10 were fit with the same program, but with rather poorer precision (0.01 cm-1) than for the ground state.

  1. Ground-state properties of light kaonic nuclei signaling symmetry energy at high densities

    NASA Astrophysics Data System (ADS)

    Yang, Rongyao; Wei, Sina; Jiang, Weizhou

    2018-01-01

    A sensitive correlation between the ground-state properties of light kaonic nuclei and the symmetry energy at high densities is constructed under the framework of relativistic mean-field theory. Taking oxygen isotopes as an example, we see that a high-density core is produced in kaonic oxygen nuclei, due to the strongly attractive antikaon-nucleon interaction. It is found that the 1{S}1/2 state energy in the high-density core of kaonic nuclei can directly probe the variation of the symmetry energy at supranormal nuclear density, and a sensitive correlation between the neutron skin thickness and the symmetry energy at supranormal density is established directly. Meanwhile, the sensitivity of the neutron skin thickness to the low-density slope of the symmetry energy is greatly increased in the corresponding kaonic nuclei. These sensitive relationships are established upon the fact that the isovector potential in the central region of kaonic nuclei becomes very sensitive to the variation of the symmetry energy. These findings might provide another perspective to constrain high-density symmetry energy, and await experimental verification in the future. Supported by National Natural Science Foundation of China (11775049, 11275048) and the China Jiangsu Provincial Natural Science Foundation (BK20131286)

  2. Communication: Broad manifold of excitonic states in light-harvesting complex 1 promotes efficient unidirectional energy transfer in vivo

    NASA Astrophysics Data System (ADS)

    Sohail, Sara H.; Dahlberg, Peter D.; Allodi, Marco A.; Massey, Sara C.; Ting, Po-Chieh; Martin, Elizabeth C.; Hunter, C. Neil; Engel, Gregory S.

    2017-10-01

    In photosynthetic organisms, the pigment-protein complexes that comprise the light-harvesting antenna exhibit complex electronic structures and ultrafast dynamics due to the coupling among the chromophores. Here, we present absorptive two-dimensional (2D) electronic spectra from living cultures of the purple bacterium, Rhodobacter sphaeroides, acquired using gradient assisted photon echo spectroscopy. Diagonal slices through the 2D lineshape of the LH1 stimulated emission/ground state bleach feature reveal a resolvable higher energy population within the B875 manifold. The waiting time evolution of diagonal, horizontal, and vertical slices through the 2D lineshape shows a sub-100 fs intra-complex relaxation as this higher energy population red shifts. The absorption (855 nm) of this higher lying sub-population of B875 before it has red shifted optimizes spectral overlap between the LH1 B875 band and the B850 band of LH2. Access to an energetically broad distribution of excitonic states within B875 offers a mechanism for efficient energy transfer from LH2 to LH1 during photosynthesis while limiting back transfer. Two-dimensional lineshapes reveal a rapid decay in the ground-state bleach/stimulated emission of B875. This signal, identified as a decrease in the dipole strength of a strong transition in LH1 on the red side of the B875 band, is assigned to the rapid localization of an initially delocalized exciton state, a dephasing process that frustrates back transfer from LH1 to LH2.

  3. A long-range-corrected density functional that performs well for both ground-state properties and time-dependent density functional theory excitation energies, including charge-transfer excited states.

    PubMed

    Rohrdanz, Mary A; Martins, Katie M; Herbert, John M

    2009-02-07

    We introduce a hybrid density functional that asymptotically incorporates full Hartree-Fock exchange, based on the long-range-corrected exchange-hole model of Henderson et al. [J. Chem. Phys. 128, 194105 (2008)]. The performance of this functional, for ground-state properties and for vertical excitation energies within time-dependent density functional theory, is systematically evaluated, and optimal values are determined for the range-separation parameter, omega, and for the fraction of short-range Hartree-Fock exchange. We denote the new functional as LRC-omegaPBEh, since it reduces to the standard PBEh hybrid functional (also known as PBE0 or PBE1PBE) for a certain choice of its two parameters. Upon optimization of these parameters against a set of ground- and excited-state benchmarks, the LRC-omegaPBEh functional fulfills three important requirements: (i) It outperforms the PBEh hybrid functional for ground-state atomization energies and reaction barrier heights; (ii) it yields statistical errors comparable to PBEh for valence excitation energies in both small and medium-sized molecules; and (iii) its performance for charge-transfer excitations is comparable to its performance for valence excitations. LRC-omegaPBEh, with the parameters determined herein, is the first density functional that satisfies all three criteria. Notably, short-range Hartree-Fock exchange appears to be necessary in order to obtain accurate ground-state properties and vertical excitation energies using the same value of omega.

  4. Dynamic Electron Correlation Effects on the Ground State Potential Energy Surface of a Retinal Chromophore Model.

    PubMed

    Gozem, Samer; Huntress, Mark; Schapiro, Igor; Lindh, Roland; Granovsky, Alexander A; Angeli, Celestino; Olivucci, Massimo

    2012-11-13

    The ground state potential energy surface of the retinal chromophore of visual pigments (e.g., bovine rhodopsin) features a low-lying conical intersection surrounded by regions with variable charge-transfer and diradical electronic structures. This implies that dynamic electron correlation may have a large effect on the shape of the force fields driving its reactivity. To investigate this effect, we focus on mapping the potential energy for three paths located along the ground state CASSCF potential energy surface of the penta-2,4-dieniminium cation taken as a minimal model of the retinal chromophore. The first path spans the bond length alternation coordinate and intercepts a conical intersection point. The other two are minimum energy paths along two distinct but kinetically competitive thermal isomerization coordinates. We show that the effect of introducing the missing dynamic electron correlation variationally (with MRCISD) and perturbatively (with the CASPT2, NEVPT2, and XMCQDPT2 methods) leads, invariably, to a stabilization of the regions with charge transfer character and to a significant reshaping of the reference CASSCF potential energy surface and suggesting a change in the dominating isomerization mechanism. The possible impact of such a correction on the photoisomerization of the retinal chromophore is discussed.

  5. A theoretical study on the geometry and spectroscopic properties of ground-state and local minima isomers of (CuS)n=2-6 clusters

    NASA Astrophysics Data System (ADS)

    Luque-Ceballos, Jonathan C.; Posada-Borbón, Alvaro; Herrera-Urbina, Ronaldo; Aceves, R.; Juárez-Sánchez, J. Octavio; Posada-Amarillas, Alvaro

    2018-03-01

    Spectroscopic properties of gas-phase copper sulfide clusters (CuS)n (n = 2-6) are calculated using Density Functional Theory (DFT) and time-dependent (TD) DFT approaches. The energy landscape of the potential energy surface is explored through a basin-hopping DFT methodology. Ground-state and low-lying isomer structures are obtained. The global search was performed at the B3PW91/SDD level of theory. Normal modes are calculated to validate the existence of optimal cluster structures. Energetic properties are obtained for the ground-state and isomer clusters and their relative energies are evaluated for probing isomerization. This is a few tenths of an eV, except for (CuS)2 cluster, which presents energy differences of ∼1 eV. Notable differences in the infrared spectra exist between the ground-state and first isomer structures, even for the (CuS)5 cluster, which has in both configurations a core copper pyramid. TDDFT provides the simulated absorption spectrum, presenting a theoretical description of optical absorption bands in terms of electronic excitations in the UV and visible regions. Results exhibit a significant dependence of the calculated UV/vis spectra on clusters size and shape regarding the ground state structures. Optical absorption is strong in the UV region, and weak or forbidden in the visible region of the spectrum.

  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. Does a 5/2 sup + -5/2 sup minus ground-state parity doublet exist in sup 229 Pa

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

    Grafen, V.; Ackermann, B.; Baltzer, H.

    1991-11-01

    The 1/2(530) decoupled band in {sup 229}Pa has been identified up to the 19/2{sup {minus}} level in ({ital p},{ital t}) and ({ital p},2{ital n}{gamma}) experiments. It is found that the 3/2{sup {minus}} band head has an excitation energy of 19(10) keV, and can thus not be identified with a 123 keV level observed in the {sup 229}U electron capture decay. This removes the evidence presented earlier for a spin-parity assignment of 5/2{sup +-}5/2{sup {minus}} to a proposed nearly degenerate ground-state doublet in {sup 229}Pa.

  8. High-resolution infrared spectroscopy of the asymmetric NO stretch band of jet-cooled nitromethane and assignment of the lowest four torsional states

    DOE PAGES

    Dawadi, Mahesh B.; Degliumberto, Lou; Perry, David S.; ...

    2017-08-10

    We used a high-throughput CW slit-jet apparatus coupled to a high-resolution FTIR to record the asymmetric NO stretch band of nitromethane. The b-type band, including torsionally excited states with m ≤ 3, has been assigned for Ka" ≤ 10, J" ≤ 20. The ground state combination differences derived from these assigned levels were fit with the RAM36 program to give an RMS deviation of 0.0006 cm -1. The band origin is 1583.0 (±0.1) cm -1 and the torsional level spacing is nearly identical to that in the ground state. The upper state levels are split into multiplets by perturbations. Wemore » also fit a subset of the available upper state combination differences for m = 0, Ka' ≤ 7, J' ≤ 10 with the same program, but with rather poorer precision (0.01 cm -1) than for the ground state.« less

  9. High-resolution infrared spectroscopy of the asymmetric NO stretch band of jet-cooled nitromethane and assignment of the lowest four torsional states

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

    Dawadi, Mahesh B.; Degliumberto, Lou; Perry, David S.

    We used a high-throughput CW slit-jet apparatus coupled to a high-resolution FTIR to record the asymmetric NO stretch band of nitromethane. The b-type band, including torsionally excited states with m ≤ 3, has been assigned for Ka" ≤ 10, J" ≤ 20. The ground state combination differences derived from these assigned levels were fit with the RAM36 program to give an RMS deviation of 0.0006 cm -1. The band origin is 1583.0 (±0.1) cm -1 and the torsional level spacing is nearly identical to that in the ground state. The upper state levels are split into multiplets by perturbations. Wemore » also fit a subset of the available upper state combination differences for m = 0, Ka' ≤ 7, J' ≤ 10 with the same program, but with rather poorer precision (0.01 cm -1) than for the ground state.« less

  10. Evidence of a Shockley-Read-Hall Defect State Independent of Band-Edge Energy in InAs / In ( As , Sb ) Type-II Superlattices

    DOE PAGES

    Aytac, Y.; Olson, B. V.; Kim, J. K.; ...

    2016-06-01

    A set of seven InAs/InAsSb type-II superlattices (T2SLs) were designed to have speci c bandgap energies between 290 meV (4.3 m) and 135 meV (9.2 m) in order to study the e ects of the T2SL bandgap energy on the minority carrier lifetime. A temperature dependent optical pump-probe technique is used to measure the carrier lifetimes, and the e ect of a mid-gap defect level on the carrier recombination dynamics is reported. The Shockley-Read-Hall (SRH) defect state is found to be at energy of approximately -250 12 meV relative to the valence band edge of bulk GaSb for the entiremore » set of T2SL structures, even though the T2SL valence band edge shifts by 155 meV on the same scale. These results indicate that the SRH defect state in InAs/InAsSb T2SLs is singular and is nearly independent of the exact position of the T2SL bandgap or band edge energies. They also suggest the possibility of engineering the T2SL structure such that the SRH state is removed completely from the bandgap, a result that should signi cantly increase the minority carrier lifetime.« less

  11. Evidence of a Shockley-Read-Hall Defect State Independent of Band-Edge Energy in InAs / In ( As , Sb ) Type-II Superlattices

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

    Aytac, Y.; Olson, B. V.; Kim, J. K.

    A set of seven InAs/InAsSb type-II superlattices (T2SLs) were designed to have speci c bandgap energies between 290 meV (4.3 m) and 135 meV (9.2 m) in order to study the e ects of the T2SL bandgap energy on the minority carrier lifetime. A temperature dependent optical pump-probe technique is used to measure the carrier lifetimes, and the e ect of a mid-gap defect level on the carrier recombination dynamics is reported. The Shockley-Read-Hall (SRH) defect state is found to be at energy of approximately -250 12 meV relative to the valence band edge of bulk GaSb for the entiremore » set of T2SL structures, even though the T2SL valence band edge shifts by 155 meV on the same scale. These results indicate that the SRH defect state in InAs/InAsSb T2SLs is singular and is nearly independent of the exact position of the T2SL bandgap or band edge energies. They also suggest the possibility of engineering the T2SL structure such that the SRH state is removed completely from the bandgap, a result that should signi cantly increase the minority carrier lifetime.« less

  12. 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.

  13. Magnetic ground state and electronic structure of CeRu(2)Al(10).

    PubMed

    Goraus, Jerzy; Ślebarski, Andrzej

    2012-03-07

    We present a combined theoretical and experimental study of the electronic structure for CeRu(2)Al(10) based on ab initio band structure calculations and x-ray photoemission spectroscopy (XPS) data. Our calculations were performed for the base unit cell and for the hypothetical unit cell which enables antiferromagnetic ordering. The stability of the magnetic phase was investigated within fixed spin moment calculations. When additional 4f correlations are not included in the LSDA C U approach, CeRu(2)Al(10) exhibits an unstable magnetic configuration with the difference in total energy per unit cell between the weakly magnetic state and the non-magnetic one of the order ~0.3 meV. We found that Coulomb correlations among 4f electrons, when they are included in the LSDA C U approach, stabilize the magnetic structure. In the weakly correlated system (small U) an antiferromagnetic (AFM) ground state with the lowest total energy is preferred. The situation is, however, the opposite when the 4f correlations are strong. In this case the ferromagnetic (FM) ground state is preferred. By comparing our calculations with the experimental data we conclude that the 4f correlations in CeRu(2)Al(10) are weak. We also carried out a structural relaxation of atomic positions within the Cmcm unit cell and we found that the Al atoms exhibit noticeable displacement from their positions known from x-ray diffraction (XRD) analysis.

  14. New more accurate calculations of the ground state potential energy surface of H(3) (+).

    PubMed

    Pavanello, Michele; Tung, Wei-Cheng; Leonarski, Filip; Adamowicz, Ludwik

    2009-02-21

    Explicitly correlated Gaussian functions with floating centers have been employed to recalculate the ground state potential energy surface (PES) of the H(3) (+) ion with much higher accuracy than it was done before. The nonlinear parameters of the Gaussians (i.e., the exponents and the centers) have been variationally optimized with a procedure employing the analytical gradient of the energy with respect to these parameters. The basis sets for calculating new PES points were guessed from the points already calculated. This allowed us to considerably speed up the calculations and achieve very high accuracy of the results.

  15. State-to-state quantum dynamics of the F + HCl (vi = 0, ji = 0) → HF(vf, jf) + Cl reaction on the ground state potential energy surface.

    PubMed

    Li, Anyang; Guo, Hua; Sun, Zhigang; Kłos, Jacek; Alexander, Millard H

    2013-10-07

    The state-to-state reaction dynamics of the title reaction is investigated on the ground electronic state potential energy surface using two quantum dynamical methods. The results obtained using the Chebyshev real wave packet method are in excellent agreement with those obtained using the time-independent method, except at low translational energies. It is shown that this exothermic hydrogen abstraction reaction is direct, resulting in a strong back-scattered bias in the product angular distribution. The HF product is highly excited internally. Agreement with available experimental data is only qualitative. We discuss several possible causes of disagreement with experiment.

  16. Spectroscopic study of hafnium silicate alloys prepared by RPECVD: Comparisons between conduction/valence band offset energies and optical band gaps

    NASA Astrophysics Data System (ADS)

    Hong, Joon Goo

    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 band offset energies 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 electron 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 band offset energies was observed. Hf 5d* state is fixed at the bottom of the conduction band and located at 1.3 +/- 0.2 eV above the top of the Si conduction band as a conduction band offset by x-ray absorption spectroscopy (XAS). Optical band gap energy changes were observed with vacuum ultra violet spectroscopic ellipsometry (VUVSE) to verify compositional dependence of conduction and valence band offset energy changes. 1 nm EOT normalized tunneling current with Wentzel-Kramer-Brillouin (WKB) simulation based on the band offset study and Franz two band 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 band offset energies and effective mass for tunneling. C-V curves were compared

  17. 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.

  18. Ground and excited state dissociation dynamics of ionized 1,1-difluoroethene.

    PubMed

    Gridelet, E; Dehareng, D; Locht, R; Lorquet, A J; Lorquet, J C; Leyh, B

    2005-09-22

    The kinetic energy release distributions (KERDs) for the fluorine atom loss from the 1,1-difluoroethene cation have been recorded with two spectrometers in two different energy ranges. A first experiment uses dissociative photoionization with the He(I) and Ne(I) resonance lines, providing the ions with a broad internal energy range, up to 7 eV above the dissociation threshold. The second experiment samples the metastable range, and the average ion internal energy is limited to about 0.2 eV above the threshold. In both energy domains, KERDs are found to be bimodal. Each component has been analyzed by the maximum entropy method. The narrow, low kinetic energy components display for both experiments the characteristics of a statistical, simple bond cleavage reaction: constraint equal to the square root of the fragment kinetic energy and ergodicity index higher than 90%. Furthermore, this component is satisfactorily accounted for in the metastable time scale by the orbiting transition state theory. Potential energy surfaces corresponding to the five lowest electronic states of the dissociating 1,1-C2H2F2+ ion have been investigated by ab initio calculations at various levels. The equilibrium geometry of these states, their dissociation energies, and their vibrational wavenumbers have been calculated, and a few conical intersections between these surfaces have been identified. It comes out that the ionic ground state X2B1 is adiabatically correlated with the lowest dissociation asymptote. Its potential energy curve increases in a monotonic way along the reaction coordinate, giving rise to the narrow KERD component. Two states embedded in the third photoelectron band (B2A1 at 15.95 eV and C2B2 at 16.17 eV) also correlate with the lowest asymptote at 14.24 eV. We suggest that their repulsive behavior along the reaction coordinate be responsible for the KERD high kinetic energy contribution.

  19. 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.

  20. Triplet and ground state potential energy surfaces of 1,4-diphenyl-1,3-butadiene: theory and experiment.

    PubMed

    Saltiel, J; Dmitrenko, O; Pillai, Z S; Klima, R; Wang, S; Wharton, T; Huang, Z-N; van de Burgt, L J; Arranz, J

    2008-05-01

    Relative energies of the ground state isomers of 1,4-diphenyl-1,3-butadiene (DPB) are determined from the temperature dependence of equilibrium isomer compositions obtained with the use of diphenyl diselenide as catalyst. Temperature and concentration effects on photostationary states and isomerization quantum yields with biacetyl or fluorenone as triplet sensitizers with or without the presence of O(2), lead to significant modification of the proposed DPB triplet potential energy surface. Quantum yields for ct-DPB formation from tt-DPB increase with [tt-DPB] revealing a quantum chain process in the tt --> ct direction, as had been observed for the ct --> tt direction, and suggesting an energy minimum at the (3)ct* geometry. They confirm the presence of planar and twisted isomeric triplets in equilibrium (K), with energy transfer from planar or quasi-planar geometries (quantum chain events from tt and ct triplets) and unimolecular decay (k(d)) from twisted geometries. Starting from cc-DPB, varphi(cc-->tt) increases with increasing [cc-DPB] whereas varphi(cc-->ct) is relatively insensitive to concentration changes. The concentration and temperature dependencies of the decay rate constants of DPB triplets in cyclohexane are consistent with the mechanism deduced from the photoisomerization quantum yields. The experimental DeltaH between (3)tt-DPB* and (3)tp-DPB*, 2.7 kcal mol(-1), is compared with the calculated energy difference [DFT with B3LYP/6-31+G(d,p) basis set]. Use of the calculated DeltaS = 4.04 eu between the two triplets gives k(d) = (2.4-6.4) x 10(7) s(-1), close to 1.70 x 10(7) s(-1), the value for twisted stilbene triplet decay. Experimental and calculated relative energies of DPB isomers on the ground and triplet state surfaces agree and theory is relied upon to deduce structural characteristics of the equilibrated conformers in the DPB triplet state.

  1. Energy bands and acceptor binding energies of GaN

    NASA Astrophysics Data System (ADS)

    Xia, Jian-Bai; Cheah, K. W.; Wang, Xiao-Liang; Sun, Dian-Zhao; Kong, Mei-Ying

    1999-04-01

    The energy bands 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 energy bands 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 energies of acceptor states are calculated by solving strictly the effective-mass equations. The binding energies 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 energy 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.

  2. Nature of ground and electronic excited states of higher acenes

    PubMed Central

    Yang, Yang; Yang, Weitao

    2016-01-01

    Higher acenes have drawn much attention as promising organic semiconductors with versatile electronic properties. However, the nature of their ground state and electronic excited states is still not fully clear. Their unusual chemical reactivity and instability are the main obstacles for experimental studies, and the potentially prominent diradical character, which might require a multireference description in such large systems, hinders theoretical investigations. Here, we provide a detailed answer with the particle–particle random-phase approximation calculation. The 1Ag ground states of acenes up to decacene are on the closed-shell side of the diradical continuum, whereas the ground state of undecacene and dodecacene tilts more to the open-shell side with a growing polyradical character. The ground state of all acenes has covalent nature with respect to both short and long axes. The lowest triplet state 3B2u is always above the singlet ground state even though the energy gap could be vanishingly small in the polyacene limit. The bright singlet excited state 1B2u is a zwitterionic state to the short axis. The excited 1Ag state gradually switches from a double-excitation state to another zwitterionic state to the short axis, but always keeps its covalent nature to the long axis. An energy crossing between the 1B2u and excited 1Ag states happens between hexacene and heptacene. Further energetic consideration suggests that higher acenes are likely to undergo singlet fission with a low photovoltaic efficiency; however, the efficiency might be improved if a singlet fission into multiple triplets could be achieved. PMID:27528690

  3. The ground state infrared spectrum of the MnH radical ( 7Σ) from diode laser spectroscopy

    NASA Astrophysics Data System (ADS)

    Urban, Rolf-Dieter; Jones, Harold

    1989-11-01

    The infrared spectrum of the manganese hydride radical ( 55MnH) in its ground electronic state ( 7Σ) has been observed using a diode laser spectrometer. The wavenumbers of twelve transitions of the v=1→0 band, five of the v=2→1 band and seven of the v=3→2 band have been measured with a nominal accuracy of ±0.001 cm -1. Coupling between the electronic spin ( S=3) and the overall molecular rotation causes each ro-vibrational transition with N>3 to be split (γ splitting) into seven components each separated by a few hundredths of a wavenumber. In most cases the complete structure was resolved. Correction terms arising from spin-spin coupling had to be included in the analysis. This work has produced the most accurate set of ground-state parameters available for MnH.

  4. Stabilities and defect-mediated lithium-ion conduction in a ground state cubic Li 3 N structure

    DOE PAGES

    Nguyen, Manh Cuong; Hoang, Khang; Wang, Cai-Zhuang; ...

    2016-01-07

    A stable ground state structure with cubic symmetry of Li 3N (c-Li 3N) is found by ab initio initially symmetric random-generated crystal structure search method. Gibbs free energy, calculated within quasi-harmonic approximation, shows that c-Li 3N is the ground state structure for a wide range of temperature. The c-Li 3N structure has a negative thermal expansion coefficient at temperatures lower than room temperature, due mainly to two transverse acoustic phonon modes. This c-Li 3N phase is a semiconductor with an indirect band gap of 1.90 eV within hybrid density functional calculation. We also investigate the migration and energetics of nativemore » point defects in c-Li 3N, including lithium and nitrogen vacancies, interstitials, and anti-site defects. Lithium interstitials are found to have a very low migration barrier (~0.12 eV) and the lowest formation energy among all possible defects. Thus, the ionic conduction in c-Li 3N is expected to occur via an interstitial mechanism, in contrast to that in the well-known α-Li 3N phase which occurs via a vacancy mechanism.« less

  5. Nature of the valence band states in Bi2(Ca, Sr, La)3Cu2O8

    NASA Astrophysics Data System (ADS)

    Wells, B. O.; Lindberg, P. A. P.; Shen, Z.-X.; Dessau, D. S.; Spicer, W. E.; Lindau, I.; Mitzi, D. B.; Kapitulnik, A.

    1990-01-01

    We have used photoemission spectroscopy to examine the symmetry of the occupied states of the valence band for the La doped superconductor Bi2(Ca, Sr, La)3Cu2O8. While the oxygen states near the bottom of the 7 eV wide valence band exhibit predominantly O 2pz symmetry, the states at the top of the valence band extending to the Fermi level are found to have primarily O 2px and O 2py character. We have also examined anomalous intensity enhancements in the valence band feature for photon energies near 18 eV. These enhancements, which occur at photon energies ranging from 15.8 to 18.0 eV for the different valence band features, are not consistent with either simple final state effects or direct O2s transitions to unoccupied O2p states.

  6. Far-infrared laser vibration-rotation-tunneling spectroscopy of water clusters in the librational band region of liquid water

    NASA Astrophysics Data System (ADS)

    Keutsch, Frank N.; Fellers, Ray S.; Viant, Mark R.; Saykally, Richard J.

    2001-03-01

    We report the first high resolution spectrum of a librational vibration for a water cluster. Four parallel bands of (H2O)3 were measured between 510 and 525 cm-1 using diode laser vibration-rotation-tunneling (VRT) spectroscopy. The bands lie in the "librational band" region of liquid water and are assigned to the nondegenerate out of plane librational vibration. The observation of at least three distinct bands within 8 cm-1 originating in the vibrational ground state is explained by a dramatically increased splitting of the rovibrational levels relative to the ground state by bifurcation tunneling and is indicative of a greatly reduced barrier height in the excited state. This tunneling motion is of special significance, as it is the lowest energy pathway for breaking and reforming of hydrogen bonds, a salient aspect of liquid water dynamics.

  7. Negative Ion Photoelectron Spectroscopy Confirms the Prediction that D-3h Carbontrioxide (CO 3) Has a Singlet Ground State

    DOE PAGES

    Hrovat, David; Hou, Gao-Lei; Chen, Bo; ...

    2015-11-13

    The CO 3 radical anion (CO 3 •–) has been formed by electrospraying carbonate dianion (CO 3 2–) into the gas phase. The negative ion photoelectron (NIPE) spectrum of CO 3 •– shows that, unlike trimethylenemethane [C(CH 2) 3], carbontrioxide (CO 3) has a singlet ground state. From the NIPE spectrum, the electron affinity of CO 3 was determined to be EA = 4.06 ± 0.03 eV, and the singlet-triplet energy difference was found to be ΔEST = - 17.8 ± 0.9 kcal/mol. B3LYP, CCSD(T), and CASPT2 calculations all find that the two lowest triplet states of CO 3 aremore » very close in energy, a prediction that is confirmed by the relative intensities of the bands in the NIPE spectrum of CO 3 •–. The 560 cm -1 vibrational progression, seen in the low energy region of the triplet band, enables the identification of the lowest, Jahn-Teller-distorted, triplet state as 3A 1, in which both unpaired electrons reside in σ MOs, rather than 3A 2, in which one unpaired electron occupies the b 2 σ MO, and the other occupies the b 1 π MO.« less

  8. Exponential vanishing of the ground-state gap of the quantum random energy model via adiabatic quantum computing

    NASA Astrophysics Data System (ADS)

    Adame, J.; Warzel, S.

    2015-11-01

    In this note, we use ideas of Farhi et al. [Int. J. Quantum. Inf. 6, 503 (2008) and Quantum Inf. Comput. 11, 840 (2011)] who link a lower bound on the run time of their quantum adiabatic search algorithm to an upper bound on the energy gap above the ground-state of the generators of this algorithm. We apply these ideas to the quantum random energy model (QREM). Our main result is a simple proof of the conjectured exponential vanishing of the energy gap of the QREM.

  9. Exponential vanishing of the ground-state gap of the quantum random energy model via adiabatic quantum computing

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

    Adame, J.; Warzel, S., E-mail: warzel@ma.tum.de

    In this note, we use ideas of Farhi et al. [Int. J. Quantum. Inf. 6, 503 (2008) and Quantum Inf. Comput. 11, 840 (2011)] who link a lower bound on the run time of their quantum adiabatic search algorithm to an upper bound on the energy gap above the ground-state of the generators of this algorithm. We apply these ideas to the quantum random energy model (QREM). Our main result is a simple proof of the conjectured exponential vanishing of the energy gap of the QREM.

  10. Investigation of high spin states in 133Cs

    NASA Astrophysics Data System (ADS)

    Xu, Q.; Xiao, Z. G.; Zhu, S. J.; Qi, C.; Jia, H.; Qi, B.; Wang, R. S.; Cheng, W. J.; Zhang, Y.; Yi, H.; Lü, L. M.; Wang, Y. J.; Li, H. J.; Huang, Y.; Zhang, Z.; Wu, X. G.; Li, C. B.; Zheng, Y.; Chen, Q. M.; Zhou, W. K.; Li, G. S.

    2018-05-01

    High spin states in 133Cs nucleus have been studied with the reaction 130Te (7Li, 4n) at a beam energy of 38 MeV. The level scheme has been expanded with spin up to 31/2 \\hbar. Compared with a recent paper, ground state band and other two collective band structures at lower spin states have been confirmed. Another collective band structure at higher spin states as well as some levels and transitions are updated. Compared with the experimental data, large-scale shell model and tilted axis cranking model calculations have been carried out. The results show that the band-head configuration of yrast band based on 7/2+ ground state and the side band built on the 5/2+ state are a pair of pseudospin partner states with π \\tilde{f}_{7/2,5/2}. The negative parity band based on 1071.5 keV level originates from π h_{11/2} orbital. Another band built on 2642.9 keV level at high spin states has been proposed with oblate deformation. Other characteristics for these bands were also discussed.

  11. 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/2016PhRvB..93q4516C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhRvB..93q4516C"><span>Superconductivity versus bound-<span class="hlt">state</span> 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 <span class="hlt">state</span> forms at arbitrary weak interaction, and already at weak coupling, one has to distinguish between the bound-<span class="hlt">state</span> 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 electron <span class="hlt">band</span> and another with two hole or two electron <span class="hlt">bands</span>. In each case, we obtain the bound-<span class="hlt">state</span> <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 electron <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 electron <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 electron <span class="hlt">band</span> to</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 <span class="hlt">state</span> 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 <span class="hlt">states</span> 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('https://www.osti.gov/biblio/22382119-projection-gradient-method-computing-ground-state-spin-boseeinstein-condensates','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22382119-projection-gradient-method-computing-ground-state-spin-boseeinstein-condensates"><span>A projection gradient method for computing <span class="hlt">ground</span> <span class="hlt">state</span> of spin-2 Bose–Einstein condensates</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, Hanquan, E-mail: hanquan.wang@gmail.com; Yunnan Tongchang Scientific Computing and Data Mining Research Center, Kunming, Yunnan Province, 650221</p> <p></p> <p>In this paper, a projection gradient method is presented for computing <span class="hlt">ground</span> <span class="hlt">state</span> of spin-2 Bose–Einstein condensates (BEC). We first propose the general projection gradient method for solving <span class="hlt">energy</span> functional minimization problem under multiple constraints, in which the <span class="hlt">energy</span> functional takes real functions as independent variables. We next extend the method to solve a similar problem, where the <span class="hlt">energy</span> functional now takes complex functions as independent variables. We finally employ the method into finding the <span class="hlt">ground</span> <span class="hlt">state</span> of spin-2 BEC. The key of our method is: by constructing continuous gradient flows (CGFs), the <span class="hlt">ground</span> <span class="hlt">state</span> of spin-2 BEC can bemore » computed as the steady <span class="hlt">state</span> solution of such CGFs. We discretized the CGFs by a conservative finite difference method along with a proper way to deal with the nonlinear terms. We show that the numerical discretization is normalization and magnetization conservative and <span class="hlt">energy</span> diminishing. Numerical results of the <span class="hlt">ground</span> <span class="hlt">state</span> and their <span class="hlt">energy</span> of spin-2 BEC are reported to demonstrate the effectiveness of the numerical method.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvA..97a3605K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvA..97a3605K"><span>Entropy of the Bose-Einstein-condensate <span class="hlt">ground</span> <span class="hlt">state</span>: Correlation versus <span class="hlt">ground-state</span> entropy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kim, Moochan B.; Svidzinsky, Anatoly; Agarwal, Girish S.; Scully, Marlan O.</p> <p>2018-01-01</p> <p>Calculation of the entropy of an ideal Bose-Einstein condensate (BEC) in a three-dimensional trap reveals unusual, previously unrecognized, features of the canonical ensemble. It is found that, for any temperature, the entropy of the Bose gas is equal to the entropy of the excited particles although the entropy of the particles in the <span class="hlt">ground</span> <span class="hlt">state</span> is nonzero. We explain this by considering the correlations between the <span class="hlt">ground-state</span> particles and particles in the excited <span class="hlt">states</span>. These correlations lead to a correlation entropy which is exactly equal to the contribution from the <span class="hlt">ground</span> <span class="hlt">state</span>. The correlations themselves arise from the fact that we have a fixed number of particles obeying quantum statistics. We present results for correlation functions between the <span class="hlt">ground</span> and excited <span class="hlt">states</span> in a Bose gas, so as to clarify the role of fluctuations in the system. We also report the sub-Poissonian nature of the <span class="hlt">ground-state</span> fluctuations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.S53D..06R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.S53D..06R"><span>Earthquake <span class="hlt">Ground</span> Motion Simulations in the Central United <span class="hlt">States</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ramirez Guzman, L.; Boyd, O. S.; Hartzell, S.; Williams, R. A.</p> <p>2010-12-01</p> <p>The Central United <span class="hlt">States</span> (CUS) includes two of the major seismic zones east of the Rockies: the New Madrid and Wabash Valley Seismic Zones. The winter 1811-1812 New Madrid Seismic Zone (NMSZ) events were the largest intraplate sequence ever recorded in the United <span class="hlt">States</span>. Together with their aftershocks, these earthquakes produced large areas of liquefaction, new lakes, and landslides in the region. Seismicity in the early 1800’s was dominated by the NMSZ activity, although three low magnitude 5 earthquakes occurred in the last 40 years in the Wabash Valley Seismic Zone (WVSZ). The population and infrastructure of the CUS have drastically changed from that of the early nineteenth century, and a large earthquake would now cause significant casualties and economic losses within the country’s heartland. In this study we present three sets of numerical simulations depicting earthquakes in the region. These hypothetical ruptures are located on the Reelfoot fault and the southern axial arm of the NMSZ and in the WVSZ. Our broad-<span class="hlt">band</span> synthetic <span class="hlt">ground</span> motions are calculated following the Liu et al. (2006) hybrid method. Using a finite element solver we calculate low frequency <span class="hlt">ground</span> motion (< 1 Hz) which accounts for the heterogeneity and low velocity soils of the region by using a recently developed seismic velocity model (CUSVM1) and a minimum shear wave velocity of 300 m/s. The broad-<span class="hlt">band</span> <span class="hlt">ground</span> motions are then generated by combining high frequency synthetics computed in a 1D velocity model with the low frequency motions at a crossover frequency of 1 Hz. We primarily discuss the basin effects produced by the Mississippi embayment and investigate the effects of hypocentral location and slip distribution on <span class="hlt">ground</span> motions in densely populated areas within the CUS.</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 <span class="hlt">states</span> 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 electronic structure, such as changes in the <span class="hlt">band</span> edge <span class="hlt">states</span> 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 <span class="hlt">states</span> 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 <span class="hlt">states</span> 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 <span class="hlt">states</span> 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 electron <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 <span class="hlt">states</span> 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 electronic structure, such as changes in the <span class="hlt">band</span> edge <span class="hlt">states</span> 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 <span class="hlt">states</span> 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 <span class="hlt">states</span> 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 <span class="hlt">states</span> 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 electron <span class="hlt">energy</span> loss spectroscopy analyses. PMID:27812035</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PPNL...15..236A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PPNL...15..236A"><span>The Hyperfine Structure of the <span class="hlt">Ground</span> <span class="hlt">State</span> in the Muonic Helium Atoms</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Aznabayev, D. T.; Bekbaev, A. K.; Korobov, V. I.</p> <p>2018-05-01</p> <p>Non-relativistic ionization <span class="hlt">energies</span> 3He2+μ-e- and 4He2+μ-e- of helium-muonic atoms are calculated for <span class="hlt">ground</span> <span class="hlt">states</span>. The calculations are based on the variational method of the exponential expansion. Convergence of the variational <span class="hlt">energies</span> is studied by an increasing of a number of the basis functions N. This allows to claim that the obtained <span class="hlt">energy</span> values have 26 significant digits for <span class="hlt">ground</span> <span class="hlt">states</span>. With the obtained results we calculate hyperfine splitting of the muonic helium atoms.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PhRvC..91d4303C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PhRvC..91d4303C"><span>High-spin <span class="hlt">states</span> and possible "stapler" <span class="hlt">band</span> in 115In</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, Z. Q.; Wang, S. Y.; Liu, L.; Zhang, P.; Jia, H.; Qi, B.; Wang, S.; Sun, D. P.; Liu, C.; Li, Z. Q.; Wu, X. G.; Li, G. S.; He, C. Y.; Zheng, Y.; Zhu, L. H.</p> <p>2015-04-01</p> <p>High-spin <span class="hlt">states</span> of 115In have been studied using the 114Cd (7Li,α 2 n ) reaction at a beam <span class="hlt">energy</span> of 48 MeV. A total of 13 new transitions have been observed and added to the level scheme of 115In. Most of the <span class="hlt">states</span> in 115In can be interpreted in terms of the weak coupling of a g9 /2 proton hole to the core <span class="hlt">states</span> of 116Sn or a g7 /2 proton to the core <span class="hlt">states</span> of 114Cd. A Δ I =1 <span class="hlt">band</span> with the π (g9/2) -1⊗ν (h11/2) 2 configuration was suggested as an oblate <span class="hlt">band</span> built on the "stapler" mechanism with the aid of the tilted axis cranking model based on covariant density functional theory.</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/1988PhRvC..38.1083G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1988PhRvC..38.1083G"><span>Systematic features in the structure of doubly odd nuclei around A~=80 mass region: <span class="hlt">Band</span> structure in 76Rb</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>García Bermúdez, G.; Baktash, C.; Lister, C. J.; Cardona, M. A.</p> <p>1988-08-01</p> <p>Multiple-particle γ-ray coincidence techniques have been used to establish the high spin structure of 76Rb. Two ΔI=1 <span class="hlt">bands</span> were found built on the Iπ=1- <span class="hlt">ground</span> <span class="hlt">state</span> and on the Iπ=(4+) isomeric <span class="hlt">state</span> at 316.8 keV <span class="hlt">energy</span>. Systematic of positive parity <span class="hlt">bands</span> seen in the Br-Kr-Rb isotones with N=39 and 41 is discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20020048706','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20020048706"><span>Theoretical Study of Tautomerization Reactions for the <span class="hlt">Ground</span> and First Excited Electronic <span class="hlt">States</span> of Adenine</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Salter, Latasha M.; Chaban, Galina M.; Kwak, Dochan (Technical Monitor)</p> <p>2002-01-01</p> <p>Geometrical structures and energetic properties for different tautomers of adenine are calculated in this study, using multi-configurational wave functions. Both the <span class="hlt">ground</span> and the lowest singlet excited <span class="hlt">state</span> potential <span class="hlt">energy</span> surfaces are studied. Four tautomeric forms are considered, and their energetic order is found to be different on the <span class="hlt">ground</span> and the excited <span class="hlt">state</span> potential <span class="hlt">energy</span> surfaces. Minimum <span class="hlt">energy</span> reaction paths are obtained for hydrogen atom transfer (tautomerization) reactions in the <span class="hlt">ground</span> and the lowest excited electronic <span class="hlt">states</span>. It is found that the barrier heights and the shapes of the reaction paths are different for the <span class="hlt">ground</span> and the excited electronic <span class="hlt">states</span>, suggesting that the probability of such tautomerization reaction is higher on the excited <span class="hlt">state</span> potential <span class="hlt">energy</span> surface. This tautomerization process should become possible in the presence of water or other polar solvent molecules and should play an important role in the photochemistry of adenine.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1007240','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1007240"><span><span class="hlt">Ground</span>-Based Radiometric Measurements of Slant Path Attenuation in the V/W <span class="hlt">Bands</span></span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2016-04-01</p> <p><span class="hlt">GROUND</span>-BASED RADIOMETRIC MEASUREMENTS OF SLANT PATH ATTENUATION IN THE V/W <span class="hlt">BANDS</span> APRIL 2016 FINAL TECHNICAL REPORT APPROVED FOR PUBLIC RELEASE...2. REPORT TYPE FINAL TECHNICAL REPORT 3. DATES COVERED (From - To) OCT 2012 – SEP 2015 4. TITLE AND SUBTITLE <span class="hlt">GROUND</span>-BASED RADIOMETRIC MEASUREMENTS ...SUPPLEMENTARY NOTES 14. ABSTRACT <span class="hlt">Ground</span>-based radiometric techniques were applied to measure the slant path attenuation cumulative distribution function to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.C12A..06K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.C12A..06K"><span>Modelling <span class="hlt">Ground</span> Based X- and Ku-<span class="hlt">Band</span> Observations of Tundra Snow</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kasurak, A.; King, J. M.; Kelly, R. E.</p> <p>2012-12-01</p> <p>As part of a radar-based remote sensing field experiment in Churchill, Manitoba <span class="hlt">ground</span> based Ku- and X-<span class="hlt">band</span> scatterometers were deployed to observe changing tundra snowpack conditions from November 2010 to March 2011. The research is part of the validation effort for the Cold Regions Hydrology High-resolution Observatory (CoReH2O) mission, a candidate in the European Space Agency's Earth Explorer program. This paper focuses on the local validation of the semi-empirical radiative transfer (sRT) model proposed for use in snow property retrievals as part of the CoReH2O mission. In this validation experiment, sRT was executed in the forward mode, simulating backscatter to assess the ability of the model. This is a necessary precursor to any inversion attempt. Two experiments are considered, both conducted in a hummocky tundra environment with shallow snow cover. In both cases, scatterometer observations were acquired over a field of view of approximately 10 by 20 meters. In the first experiment, radar observations were made of a snow field and then repeated after the snow had been removed. A <span class="hlt">ground</span>-based scanning LiDAR system was used to characterize the spatial variability of snow depth through measurements of the snow and <span class="hlt">ground</span> surface. Snow properties were determined in the field of view from two snow pits, 12 density core measurements, and Magnaprobe snow depth measurements. In the second experiment, a site was non-destructively observed from November through March, with snow properties measured out-of-scene, to characterize the snow evolution response. The model results from sRT fit the form of the observations from the two scatterometer field experiments but do not capture the backscatter magnitude. A constant offset for the season of 5 dB for X-<span class="hlt">band</span> co- and cross-polarization response was required to match observations, in addition to a 3 dB X- and Ku-<span class="hlt">band</span> co-polarization offset after the 6th of December. To explain these offsets, it is recognized that the two</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JPSJ...87f3703K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JPSJ...87f3703K"><span><span class="hlt">Ground-state</span> and Thermodynamic Properties of an S = 1 Kitaev Model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Koga, Akihisa; Tomishige, Hiroyuki; Nasu, Joji</p> <p>2018-06-01</p> <p>We study the <span class="hlt">ground-state</span> and thermodynamic properties of an S = 1 Kitaev model. We first clarify the existence of global parity symmetry in addition to the local symmetry on each plaquette, which enables us to perform large-scale calculations on up to 24 sites. It is found that the <span class="hlt">ground</span> <span class="hlt">state</span> should be singlet, and its <span class="hlt">energy</span> is estimated as E/N ˜ -0.65J, where J is the Kitaev exchange coupling. We find that the lowest excited <span class="hlt">state</span> belongs to the same subspace as the <span class="hlt">ground</span> <span class="hlt">state</span>, and that the gap decreases monotonically with increasing system size, which suggests that the <span class="hlt">ground</span> <span class="hlt">state</span> of the S = 1 Kitaev model is gapless. Using the thermal pure quantum <span class="hlt">states</span>, we clarify the finite temperature properties characteristic of the Kitaev models with S ≤ 2.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhRvB..96d1112M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvB..96d1112M"><span>Antibonding <span class="hlt">ground</span> <span class="hlt">state</span> of adatom molecules in bulk Dirac semimetals</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marques, Y.; Obispo, A. E.; Ricco, L. S.; de Souza, M.; Shelykh, I. A.; Seridonio, A. C.</p> <p>2017-07-01</p> <p>The <span class="hlt">ground</span> <span class="hlt">state</span> of the diatomic molecules in nature is inevitably bonding, and its first excited <span class="hlt">state</span> is antibonding. We demonstrate theoretically that, for a pair of distant adatoms placed buried in three-dimensional-Dirac semimetals, this natural order of the <span class="hlt">states</span> can be reversed and an antibonding <span class="hlt">ground</span> <span class="hlt">state</span> occurs at the lowest <span class="hlt">energy</span> of the so-called bound <span class="hlt">states</span> in the continuum. We propose an experimental protocol with the use of a scanning tunneling microscope tip to visualize the topographic map of the local density of <span class="hlt">states</span> on the surface of the system to reveal the emerging physics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JPhB...51h5202T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JPhB...51h5202T"><span>Low <span class="hlt">energy</span> collisions of spin-polarized metastable argon atoms with <span class="hlt">ground</span> <span class="hlt">state</span> argon atoms</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Taillandier-Loize, T.; Perales, F.; Baudon, J.; Hamamda, M.; Bocvarski, V.; Ducloy, M.; Correia, F.; Fabre, N.; Dutier, G.</p> <p>2018-04-01</p> <p>The collision between a spin-polarized metastable argon atom in Ar* (3p54s, 3P2, M = +2) <span class="hlt">state</span> slightly decelerated by the Zeeman slower-laser technique and a co-propagating thermal <span class="hlt">ground</span> <span class="hlt">state</span> argon atom Ar (3p6, 1S0), both merged from the same supersonic beam, but coming through adjacent slots of a rotating disk, is investigated at the center of mass <span class="hlt">energies</span> ranging from 1 to 10 meV. The duration of the laser pulse synchronised with the disk allows the tuning of the relative velocity and thus the collision <span class="hlt">energy</span>. At these sub-thermal <span class="hlt">energies</span>, the ‘resonant metastability transfer’ signal is too small to be evidenced. The explored <span class="hlt">energy</span> range requires using indiscernibility amplitudes for identical isotopes to have a correct interpretation of the experimental results. Nevertheless, excitation transfers are expected to increase significantly at much lower <span class="hlt">energies</span> as suggested by previous theoretical predictions of potentials 2g(3P2) and 2u(3P2). Limits at ultra-low collisional <span class="hlt">energies</span> of the order of 1 mK (0.086 μeV) or less, where gigantic elastic cross sections are expected, will also be discussed. The experimental method is versatile and could be applied using different isotopes of Argon like 36Ar combined with 40Ar, as well as other rare gases among which Krypton should be of great interest thanks to the available numerous isotopes present in a natural gas mixture.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JLTP..175..508K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JLTP..175..508K"><span>The Pressure Coefficients of the Superconducting Order Parameters at the <span class="hlt">Ground</span> <span class="hlt">State</span> of Ferromagnetic Superconductors</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Konno, R.; Hatayama, N.; Chaudhury, R.</p> <p>2014-04-01</p> <p>We investigated the pressure coefficients of the superconducting order parameters at the <span class="hlt">ground</span> <span class="hlt">state</span> of ferromagnetic superconductors based on the microscopic single <span class="hlt">band</span> model by Linder et al. The superconducting gaps (i) similar to the ones seen in the thin film of A2 phase in liquid 3He and (ii) with the line node were used. This study shows that we would be able to estimate the pressure coefficients of the superconducting and magnetic order parameters at the <span class="hlt">ground</span> <span class="hlt">state</span> of ferromagnetic superconductors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1248866-nuclear-ground-state-masses-deformations-frdm','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1248866-nuclear-ground-state-masses-deformations-frdm"><span>Nuclear <span class="hlt">ground-state</span> masses and deformations: FRDM(2012)</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Moller, P.; Sierk, A. J.; Ichikawa, T.; ...</p> <p>2016-03-25</p> <p>Here, we tabulate the atomic mass excesses and binding <span class="hlt">energies</span>, <span class="hlt">ground-state</span> shell-plus-pairing corrections, <span class="hlt">ground-state</span> microscopic corrections, and nuclear <span class="hlt">ground-state</span> deformations of 9318 nuclei ranging from 16O to A=339. The calculations are based on the finite-range droplet macroscopic and the folded-Yukawa single-particle microscopic nuclear-structure models, which are completely specified. Relative to our FRDM(1992) mass table in Möller et al. (1995), the results are obtained in the same model, but with considerably improved treatment of deformation and fewer of the approximations that were necessary earlier, due to limitations in computer power. The more accurate execution of the model and the more extensivemore » and more accurate experimental mass data base now available allow us to determine one additional macroscopic-model parameter, the density-symmetry coefficient LL, which was not varied in the previous calculation, but set to zero. Because we now realize that the FRDM is inaccurate for some highly deformed shapes occurring in fission, because some effects are derived in terms of perturbations around a sphere, we only adjust its macroscopic parameters to <span class="hlt">ground-state</span> masses.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JMoSp.324....6N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JMoSp.324....6N"><span>Rovibrational constants of the <span class="hlt">ground</span> <span class="hlt">state</span> and v8 = 1 <span class="hlt">state</span> of 13C2HD3 by high-resolution FTIR spectroscopy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ng, L. L.; Tan, T. L.</p> <p>2016-06-01</p> <p>The Fourier transform infrared (FTIR) spectrum of the c-type ν8 <span class="hlt">band</span> of 13C2HD3 was recorded for the first time at a unapodized resolution of 0.0063 cm-1 in the wavenumber region of 830-1000 cm-1. Through the fitting of a total of 1057 assigned infrared transitions using Watson's A-reduced Hamiltonian in the Ir representation, rovibrational constants for the upper <span class="hlt">state</span> (v8 = 1) up to five quartic centrifugal distortion terms were derived for the first time with a root-mean-square (rms) deviation of 0.00073 cm-1. The <span class="hlt">band</span> center of ν8 of 13C2HD3 was found to be 913.011021(55) cm-1. <span class="hlt">Ground</span> <span class="hlt">state</span> rovibrational constants up to five quartic terms of 13C2HD3 were also determined from a fit of 453 <span class="hlt">ground</span> <span class="hlt">state</span> combination-differences from the present infrared measurements with an rms deviation of 0.00072 cm-1 for the first time. The uncertainty of the measured infrared lines was estimated to be ±0.0012 cm-1. From the <span class="hlt">ground</span> <span class="hlt">state</span> rotational constants, the inertial defect of 13C2HD3 was calculated to be 0.06973(16) uÅ2, showing the high planarity of the molecule.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1990CPL...169..116O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1990CPL...169..116O"><span><span class="hlt">Ground</span> and excited <span class="hlt">states</span> of CaSH through electron propagator calculations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ortiz, J. V.</p> <p>1990-05-01</p> <p>Electron propagator calculations of electron affinities of CaSH + produce <span class="hlt">ground</span> and excited <span class="hlt">state</span> <span class="hlt">energies</span> at the optimized, C s minimum of the neutral <span class="hlt">ground</span> <span class="hlt">state</span> and at a C ∞v geometry. Feynman-Dyson amplitudes (FDAs) describe the distribution of the least bound electron in various <span class="hlt">states</span>. The neutral <span class="hlt">ground</span> <span class="hlt">state</span> differs from the cation by the occupation of a one-electron <span class="hlt">state</span> dominated by Ca s functions. Described by FDAs with Ca-S π pseudosymmetry, corresponding excited <span class="hlt">states</span> have unpaired electrons in orbitals displaying interference between Ca p and d functions. Above these lies a σ pseudosymmetry FDA with principal contributions from Ca d functions. Two FDAs with σ pseudosymmetry follow. Higher excited <span class="hlt">states</span> exhibit considerable delocalization onto S.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26609599','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26609599"><span>Some Fundamental Issues in <span class="hlt">Ground-State</span> Density Functional Theory: A Guide for the Perplexed.</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; Ruzsinszky, Adrienn; Constantin, Lucian A; Sun, Jianwei; Csonka, Gábor I</p> <p>2009-04-14</p> <p>Some fundamental issues in <span class="hlt">ground-state</span> density functional theory are discussed without equations: (1) The standard Hohenberg-Kohn and Kohn-Sham theorems were proven for a Hamiltonian that is not quite exact for real atoms, molecules, and solids. (2) The density functional for the exchange-correlation <span class="hlt">energy</span>, which must be approximated, arises from the tendency of electrons to avoid one another as they move through the electron density. (3) In the absence of a magnetic field, either spin densities or total electron density can be used, although the former choice is better for approximations. (4) "Spin contamination" of the determinant of Kohn-Sham orbitals for an open-shell system is not wrong but right. (5) Only to the extent that symmetries of the interacting wave function are reflected in the spin densities should those symmetries be respected by the Kohn-Sham noninteracting or determinantal wave function. Functionals below the highest level of approximations should however sometimes break even those symmetries, for good physical reasons. (6) Simple and commonly used semilocal (lower-level) approximations for the exchange-correlation <span class="hlt">energy</span> as a functional of the density can be accurate for closed systems near equilibrium and yet fail for open systems of fluctuating electron number. (7) The exact Kohn-Sham noninteracting <span class="hlt">state</span> need not be a single determinant, but common approximations can fail when it is not. (8) Over an open system of fluctuating electron number, connected to another such system by stretched bonds, semilocal approximations make the exchange-correlation <span class="hlt">energy</span> and hole-density sum rule too negative. (9) The gap in the exact Kohn-Sham <span class="hlt">band</span> structure of a crystal underestimates the real fundamental gap but may approximate the first exciton <span class="hlt">energy</span> in the large-gap limit. (10) Density functional theory is not really a mean-field theory, although it looks like one. The exact functional includes strong correlation, and semilocal approximations often</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JPhCS1023a2013G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JPhCS1023a2013G"><span>Structure of the low-lying positive parity <span class="hlt">states</span> in the proton-neutron symplectic model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ganev, H. G.</p> <p>2018-05-01</p> <p>The proton-neutron symplectic model with Sp(12, R) dynamical symmetry is applied for the simultaneous description of the microscopic structure of the low-lying <span class="hlt">states</span> of the <span class="hlt">ground</span> <span class="hlt">state</span>, γ and β <span class="hlt">bands</span> in 166 Er. For this purpose, the model Hamiltonian is diagonalized in the space of stretched <span class="hlt">states</span> by exploiting the SUp (3) ⊗ SUn (3) symmetry-adapted basis. The theoretical predictions are compared with experiment and some other microscopic collective models, like the one-component Sp(6, R) symplectic and pseudo-SU(3) models. A good description of the <span class="hlt">energy</span> levels of the three <span class="hlt">bands</span> under consideration, as well as the enhanced intraband B(E2) transition strengths between the <span class="hlt">states</span> of the <span class="hlt">ground</span> and γ <span class="hlt">bands</span> is obtained without the use of effective charges. The results show the presence of a good SU(3) dynamical symmetry. It is also shown that, in contrast to the Sp(6, R) case, the lowest excited <span class="hlt">bands</span>, e.g., the β and γ <span class="hlt">bands</span>, naturally appear together with the <span class="hlt">ground</span> <span class="hlt">state</span> <span class="hlt">band</span> within a single Sp(12, R) irreducible representation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=coulomb&pg=2&id=EJ963904','ERIC'); return false;" href="https://eric.ed.gov/?q=coulomb&pg=2&id=EJ963904"><span>Using Uncertainty Principle to Find the <span class="hlt">Ground-State</span> <span class="hlt">Energy</span> of the Helium and a Helium-like Hookean Atom</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>Harbola, Varun</p> <p>2011-01-01</p> <p>In this paper, we accurately estimate the <span class="hlt">ground-state</span> <span class="hlt">energy</span> and the atomic radius of the helium atom and a helium-like Hookean atom by employing the uncertainty principle in conjunction with the variational approach. We show that with the use of the uncertainty principle, electrons are found to be spread over a radial region, giving an electron…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.B43B0582R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.B43B0582R"><span>A Passive Microwave L-<span class="hlt">Band</span> Boreal Forest Freeze/Thaw and Vegetation Phenology Study</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Roy, A.; Sonnentag, O.; Pappas, C.; Mavrovic, A.; Royer, A.; Berg, A. A.; Rowlandson, T. L.; Lemay, J.; Helgason, W.; Barr, A.; Black, T. A.; Derksen, C.; Toose, P.</p> <p>2016-12-01</p> <p>The boreal forest is the second largest land biome in the world and thus plays a major role in the global and regional climate systems. The extent, timing and duration of seasonal freeze/thaw (F/T) <span class="hlt">state</span> influences vegetation developmental stages (phenology) and, consequently, constitute an important control on how boreal forest ecosystems exchange carbon, water and <span class="hlt">energy</span> with the atmosphere. The effective retrieval of seasonal F/T <span class="hlt">state</span> from L-<span class="hlt">Band</span> radiometry was demonstrated using satellite mission. However, disentangling the seasonally differing contributions from forest overstory and understory vegetation, and the soil surface to the satellite signal remains challenging. Here we present initial results from a radiometer field campaign to improve our understanding of the L-<span class="hlt">Band</span> derived boreal forest F/T signal and vegetation phenology. Two L-<span class="hlt">Band</span> surface-based radiometers (SBR) are installed on a micrometeorological tower at the Southern Old Black Spruce site in central Saskatchewan over the 2016-2017 F/T season. One radiometer unit is installed on the flux tower so it views forest including all overstory and understory vegetation and the moss-covered <span class="hlt">ground</span> surface. A second radiometer unit is installed within the boreal forest overstory, viewing the understory and the <span class="hlt">ground</span> surface. The objectives of our study are (i) to disentangle the L-<span class="hlt">Band</span> F/T signal contribution of boreal forest overstory from the understory and <span class="hlt">ground</span> surface, (ii) to link the L-<span class="hlt">Band</span> F/T signal to related boreal forest structural and functional characteristics, and (iii) to investigate the use of the L-<span class="hlt">Band</span> signal to characterize boreal forest carbon, water and <span class="hlt">energy</span> fluxes. The SBR observations above and within the forest canopy are used to retrieve the transmissivity (γ) and the scattering albedo (ω), two parameters that describe the emission of the forest canopy though the F/T season. These two forest parameters are compared with boreal forest structural and functional</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JChPh.144q4301K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JChPh.144q4301K"><span>New ab initio adiabatic potential <span class="hlt">energy</span> surfaces and bound <span class="hlt">state</span> calculations for the singlet <span class="hlt">ground</span> X˜ 1A1 and excited C˜ 1B2(21A') <span class="hlt">states</span> of SO2</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kłos, Jacek; Alexander, Millard H.; Kumar, Praveen; Poirier, Bill; Jiang, Bin; Guo, Hua</p> <p>2016-05-01</p> <p>We report new and more accurate adiabatic potential <span class="hlt">energy</span> surfaces (PESs) for the <span class="hlt">ground</span> X˜ 1A1 and electronically excited C˜ 1B2(21A') <span class="hlt">states</span> of the SO2 molecule. Ab initio points are calculated using the explicitly correlated internally contracted multi-reference configuration interaction (icMRCI-F12) method. A second less accurate PES for the <span class="hlt">ground</span> X ˜ <span class="hlt">state</span> is also calculated using an explicitly correlated single-reference coupled-cluster method with single, double, and non-iterative triple excitations [CCSD(T)-F12]. With these new three-dimensional PESs, we determine <span class="hlt">energies</span> of the vibrational bound <span class="hlt">states</span> and compare these values to existing literature data and experiment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1407026-coulomb-excitation-isomeric-band','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1407026-coulomb-excitation-isomeric-band"><span>Coulomb excitation of the K π= 8⁻ isomeric <span class="hlt">band</span> in 178Hf</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Napiorkovsk, P. J.; Srebrny, J.; Czosnyka, T.; ...</p> <p>2001-12-01</p> <p>The Coulomb excitation experiment on the 178Hf was performed using 650 MeV beam of 136Xe. The first observation of discrete transitions in the K π = 8 - isomeric <span class="hlt">band</span>. Coulomb excited from K π = 0+ <span class="hlt">ground</span> <span class="hlt">state</span>, is reported. The possible mechanisms of El coupling of the <span class="hlt">ground</span> <span class="hlt">state</span> <span class="hlt">band</span> and the isomeric <span class="hlt">band</span> is discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/21518425-energy-transition-characterization-mu-bands-bismuth-fiber-spectroscopy-transient-oscillations','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/21518425-energy-transition-characterization-mu-bands-bismuth-fiber-spectroscopy-transient-oscillations"><span><span class="hlt">Energy</span> transition characterization of 1.18 and 1.3 {mu}m <span class="hlt">bands</span> of bismuth fiber by spectroscopy of the transient oscillations</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>Gumenyuk, Regina; Okhotnikov, Oleg G.; Golant, Konstantin</p> <p>2011-05-09</p> <p>The experimental evidence of laser transition type in bismuth-doped silica fibers operating at different spectral <span class="hlt">bands</span> is presented. Spectrally resolved transient (relaxation) oscillations studied for a Bi-doped fiber laser at room and liquid-nitrogen temperatures allow to identify the three- and four-level <span class="hlt">energy</span> <span class="hlt">bands</span>. 1.18 {mu}m short-wavelength <span class="hlt">band</span> is found to be a three-level system at room temperature with highly populated terminal <span class="hlt">energy</span> level of laser transition. The depopulation of <span class="hlt">ground</span> level by cooling the fiber down to liquid-nitrogen temperature changes the transition to four-level type. Four-level <span class="hlt">energy</span> transition distinguished at 1.32 {mu}m exhibits the net gain at room temperature.</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-<span class="hlt">state</span> current in tunnel field-effect transistors (TFETs). In this paper, we reveal that the on-<span class="hlt">state</span> 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-<span class="hlt">state</span> performance, and it also suppresses the off-<span class="hlt">state</span> 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('https://www.osti.gov/biblio/22493114-measurement-inassb-bandgap-energy-inas-inassb-band-edge-positions-using-spectroscopic-ellipsometry-photoluminescence-spectroscopy','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22493114-measurement-inassb-bandgap-energy-inas-inassb-band-edge-positions-using-spectroscopic-ellipsometry-photoluminescence-spectroscopy"><span>Measurement of InAsSb bandgap <span class="hlt">energy</span> and InAs/InAsSb <span class="hlt">band</span> edge positions using spectroscopic ellipsometry and photoluminescence 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>Webster, P. T.; Riordan, N. A.; Liu, S.</p> <p>2015-12-28</p> <p>The structural and optical properties of lattice-matched InAs{sub 0.911}Sb{sub 0.089} bulk layers and strain-balanced InAs/InAs{sub 1−x}Sb{sub x} (x ∼ 0.1–0.4) superlattices grown on (100)-oriented GaSb substrates by molecular beam epitaxy are examined using X-ray diffraction, spectroscopic ellipsometry, and temperature dependent photoluminescence spectroscopy. The photoluminescence and ellipsometry measurements determine the <span class="hlt">ground</span> <span class="hlt">state</span> bandgap <span class="hlt">energy</span> and the X-ray diffraction measurements determine the layer thickness and mole fraction of the structures studied. Detailed modeling of the X-ray diffraction data is employed to quantify unintentional incorporation of approximately 1% Sb into the InAs layers of the superlattices. A Kronig-Penney model of the superlattice miniband structure ismore » used to analyze the valence <span class="hlt">band</span> offset between InAs and InAsSb, and hence the InAsSb <span class="hlt">band</span> edge positions at each mole fraction. The resulting composition dependence of the bandgap <span class="hlt">energy</span> and <span class="hlt">band</span> edge positions of InAsSb are described using the bandgap bowing model; the respective low and room temperature bowing parameters for bulk InAsSb are 938 and 750 meV for the bandgap, 558 and 383 meV for the conduction <span class="hlt">band</span>, and −380 and −367 meV for the valence <span class="hlt">band</span>.« 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/1998ChPhL..15..793Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998ChPhL..15..793Z"><span>Collective <span class="hlt">Band</span> Structures in the Neutron-Rich 107,109Ru Nuclei</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhu, Sheng-jiang; Gan, Cui-yun; J, Hamilton H.; A, Ramayya V.; B, Babu R. S.; M, Sakhaee; W, Ma C.; Long, Gui-lu; Deng, Jing-kang; Zhu, Ling-yan; Li, Ming; Yang, Li-ming; J, Komicki; J, Cole D.; R, Aryaeinejad; Y, Dardenne K.; M, Drigert W.; J, Rasmussen O.; M, Stoyer A.; S, Chu Y.; K, Gregorich E.; M, Mohar F.; S, Prussin G.; I, Lee Y.; N, Johnson R.; F, McGowan K.</p> <p>1998-11-01</p> <p>The levels in neutron-rich odd-A 107,109Ru nuclei have been investigated by using γ-γ- and γ-γ-γ-coincidence studies of the prompt γ-rays from the spontaneous fission of 252Cf. The <span class="hlt">ground</span> <span class="hlt">state</span> <span class="hlt">bands</span> and the negative parity <span class="hlt">bands</span> are identified and expanded in both nuclei. Triaxial rotor plus particle model calculations indicate the <span class="hlt">ground</span> <span class="hlt">state</span> <span class="hlt">bands</span> originate from ν(d5/2 + g7/2) quasiparticle configurations and the negative parity <span class="hlt">bands</span> are from νh11/2 orbital.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016MRE.....3i5005Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016MRE.....3i5005Y"><span>The dependence of the tunneling characteristic on the electronic <span class="hlt">energy</span> <span class="hlt">bands</span> and the carrier’s <span class="hlt">states</span> of Graphene superlattice</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, C. H.; Shen, G. Z.; Ao, Z. M.; Xu, Y. W.</p> <p>2016-09-01</p> <p>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 <span class="hlt">energy</span> and angle, the height and width of the potential. These carriers tunneling characteristic can be understood from the <span class="hlt">energy</span> <span class="hlt">band</span> structures in the corresponding superlattice systems and the carrier’s <span class="hlt">states</span> 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.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017isms.confEFA05D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017isms.confEFA05D"><span>First High Resolution IR Spectra of 1-^{13}C-PROPANE. the νb{9} B-Type <span class="hlt">Band</span> Near 366.404 \\wn and the νb{26} C-Type <span class="hlt">Band</span> Near 748.470 \\wn. Determination of <span class="hlt">Ground</span> and Upper <span class="hlt">State</span> Constants.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Daunt, S. J.; Grzywacz, Robert; Lafferty, Walter; Flaud, Jean-Marie; Billinghurst, Brant E.</p> <p>2017-06-01</p> <p>We report in this talk on the first high resolution IR spectra (Δν = 0.0009 \\wn) of the 1-^{13}C-Propane isotopologue. Spectra were taken on the Bruker FTS instrument on the Far-IR beamline at the Canadian National Synchrotron (CLS) located at the University of Saskatchewan. The νb{9} B-type <span class="hlt">band</span> centered near 366.404 \\wn appears unperturbed and lines were assigned up to K = 17 and J = 50. Since the 1960 MW study of Lide only used 6 J lines of K = 0 we had to use GSCD analyses to determine a fuller set of molecular constants for this molecule. Since normal propane has been detected using the νb{26} C-type <span class="hlt">band</span> in Titan and other astrophysical objects our main focus was on the analagous <span class="hlt">bands</span> for the both the 1-^{13}C and 2-^{13}C isotopologues. Assigned lines up to K = 17, J = 50 in νb{26} were analyzed with GSCD to independently obtain <span class="hlt">ground</span> <span class="hlt">state</span> rotational constants. These were consistent with those obtained from the νb{9} analysis. Upper <span class="hlt">state</span> constants were also determined that reproduce the vast majority of this <span class="hlt">band</span>. As in the normal and 2-^{13}C species a Coriolis resonance with the 2νb{9} <span class="hlt">state</span> causes lines of most K levels above 15 to be shifted. We did not have enough sample available at the time of these experiments to be able to record the 2νb{9} - νb{9} hot <span class="hlt">band</span> transitions in the low frequency study of νb{9}. Lide, J. Chem. Phys. 33, p. 1514 ff. (1960) Flaud, Kwabia Tchana, Lafferty & Nixon, Mol. Phys. 108, p. 699 ff. (2010)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/942079-nitrogen-induced-perturbation-valence-band-states-gap1-xnx-alloys','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/942079-nitrogen-induced-perturbation-valence-band-states-gap1-xnx-alloys"><span>Nitrogen-Induced Perturbation of the Valence <span class="hlt">Band</span> <span class="hlt">States</span> in GaP1-xNx Alloys</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>Dudiy, S. V.; Zunger, A.; Felici, M.</p> <p>2006-01-01</p> <p>The effects of diluted nitrogen impurities on the valence- and conduction-<span class="hlt">band</span> <span class="hlt">states</span> of GaP{sub 1-x}N{sub x} have been predicted and measured experimentally. The calculation uses <span class="hlt">state</span>-of-the-art atomistic modeling: we use large supercells with screened pseudopotentials and consider several random realizations of the nitrogen configurations. These calculations agree with photoluminescence excitation (PLE) measurements performed for nitrogen concentrations x up to 0.035 and photon <span class="hlt">energies</span> up to 1 eV above the GaP optical-absorption edge, as well as with published ellipsometry data. In particular, a predicted nitrogen-induced buildup of the L character near the valence- and conduction-<span class="hlt">band</span> edges accounts for the surprising broad-absorptionmore » plateau observed in PLE between the X{sub 1c} and the {Lambda}{sub 1c} critical points of GaP. Moreover, theory accounts quantitatively for the downward bowing of the indirect conduction-<span class="hlt">band</span> edge and for the upward bowing of the direct transition with increasing nitrogen concentration. We review some of the controversies in the literature regarding the shifts in the conduction <span class="hlt">band</span> with composition, and conclude that measured results at ultralow N concentration cannot be used to judge behavior at a higher concentration. In particular, we find that at the high concentrations of nitrogen studied here ({approx}1%) the conduction-<span class="hlt">band</span> edge (CBE) is a hybridized <span class="hlt">state</span> made from the original GaP X{sub 1c} <span class="hlt">band</span>-edge <span class="hlt">state</span> plus all cluster <span class="hlt">states</span>. In this limit, the CBE plunges down in <span class="hlt">energy</span> as the N concentration increases, in quantitative agreement with the measurements reported here. However, at ultralow nitrogen concentrations (<0.1%), the CBE is the nearly unperturbed host X{sub 1c}, which does not sense the nitrogen cluster levels. Thus, this <span class="hlt">state</span> does not move energetically as nitrogen is added and stays pinned in <span class="hlt">energy</span>, in agreement with experimental results.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004JMoSp.226..123S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004JMoSp.226..123S"><span><span class="hlt">Ground</span> <span class="hlt">state</span> spectrum of methylcyanide</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Šimečková, Marie; Urban, Štěpán; Fuchs, Ulrike; Lewen, Frank; Winnewisser, Gisbert; Morino, Isamu; Yamada, Koichi M. T.</p> <p>2004-08-01</p> <p>The rotational spectrum of methylcyanide (acetonitrile) in the <span class="hlt">ground</span> vibrational <span class="hlt">state</span> was measured in the spectral region from 91 to 810 GHz using the Cologne and Tsukuba spectrometers operated in the Doppler-limited and sub-Doppler saturation layouts. The resolution of the saturation Lamb-dip measurements is estimated to be about 1 kHz at the best of circumstances and the measuring accuracy of 10-60 kHz depending very sensitively on the quality of the spectrum. In the cases of rotational transitions with the low quantum number J ( J<18) and with a low difference of the rotational quantum numbers J- K, the resolved or partly resolved hyperfine structures of the rotational transitions were observed. Together with the most accurate data from the literature, the newly measured experimental data were analyzed using the traditional polynomial <span class="hlt">energy</span> formula as well as the Padè approximant for the effective rotational Hamiltonian. The resulting rotational, centrifugal distortion, and hyperfine structure spectroscopic constants were obtained with a significantly higher accuracy than the ones listed in the literature. In addition, an anomalous accidental resonance was detected between the K=14 <span class="hlt">ground</span> <span class="hlt">state</span> levels and the K=12, + l levels in the excited v8=1 vibrational <span class="hlt">state</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PhRvB..92k5137K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PhRvB..92k5137K"><span>Exact <span class="hlt">ground</span> <span class="hlt">states</span> and topological order in interacting Kitaev/Majorana chains</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Katsura, Hosho; Schuricht, Dirk; Takahashi, Masahiro</p> <p>2015-09-01</p> <p>We study a system of interacting spinless fermions in one dimension that, in the absence of interactions, reduces to the Kitaev chain [Kitaev, Phys. Usp. 44, 131 (2001), 10.1070/1063-7869/44/10S/S29]. In the noninteracting case, a signal of topological order appears as zero-<span class="hlt">energy</span> modes localized near the edges. We show that the exact <span class="hlt">ground</span> <span class="hlt">states</span> can be obtained analytically even in the presence of nearest-neighbor repulsive interactions when the on-site (chemical) potential is tuned to a particular function of the other parameters. As with the noninteracting case, the obtained <span class="hlt">ground</span> <span class="hlt">states</span> are twofold degenerate and differ in fermionic parity. We prove the uniqueness of the obtained <span class="hlt">ground</span> <span class="hlt">states</span> and show that they can be continuously deformed to the <span class="hlt">ground</span> <span class="hlt">states</span> of the noninteracting Kitaev chain without gap closing. We also demonstrate explicitly that there exists a set of operators each of which maps one of the <span class="hlt">ground</span> <span class="hlt">states</span> to the other with opposite fermionic parity. These operators can be thought of as an interacting generalization of Majorana edge zero modes.</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 <span class="hlt">states</span> 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://hdl.handle.net/2060/19950009428','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19950009428"><span>The C4H radical and the diffuse interstellar <span class="hlt">bands</span>. An ab initio study</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kolbuszewski, Marcin</p> <p>1994-01-01</p> <p>An ab initio study of the low-lying electronic <span class="hlt">states</span> of C4H has been presented where the species studied has a chi(2)sigma(+) <span class="hlt">ground</span> <span class="hlt">state</span> and two low lying pi <span class="hlt">states</span>. Based on the vertical and adiabatic excitation <span class="hlt">energies</span> between those <span class="hlt">states</span> it is suggested that the 4428 A diffuse interstellar <span class="hlt">band</span> is not carried by C4H. The application of the particle in a box model shows strong coincidences between the strong DIB's and predicted wavelengths of pi-pi transitions in C(2n)H series. Based on those coincidences, it is suggested the C(2n)H species as good candidates for carriers of diffuse interstellar <span class="hlt">bands</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhRvL.118m7202L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvL.118m7202L"><span>Gapless Spin-Liquid <span class="hlt">Ground</span> <span class="hlt">State</span> in the S =1 /2 Kagome Antiferromagnet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liao, H. J.; Xie, Z. Y.; Chen, J.; Liu, Z. Y.; Xie, H. D.; Huang, R. Z.; Normand, B.; Xiang, T.</p> <p>2017-03-01</p> <p>The defining problem in frustrated quantum magnetism, the <span class="hlt">ground</span> <span class="hlt">state</span> of the nearest-neighbor S =1 /2 antiferromagnetic Heisenberg model on the kagome lattice, has defied all theoretical and numerical methods employed to date. We apply the formalism of tensor-network <span class="hlt">states</span>, specifically the method of projected entangled simplex <span class="hlt">states</span>, which combines infinite system size with a correct accounting for multipartite entanglement. By studying the <span class="hlt">ground-state</span> <span class="hlt">energy</span>, the finite magnetic order appearing at finite tensor bond dimensions, and the effects of a next-nearest-neighbor coupling, we demonstrate that the <span class="hlt">ground</span> <span class="hlt">state</span> is a gapless spin liquid. We discuss the comparison with other numerical studies and the physical interpretation of this result.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20136303','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20136303"><span>Method and basis set dependence of anharmonic <span class="hlt">ground</span> <span class="hlt">state</span> nuclear wave functions and zero-point <span class="hlt">energies</span>: application to SSSH.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kolmann, Stephen J; Jordan, Meredith J T</p> <p>2010-02-07</p> <p>One of the largest remaining errors in thermochemical calculations is the determination of the zero-point <span class="hlt">energy</span> (ZPE). The fully coupled, anharmonic ZPE and <span class="hlt">ground</span> <span class="hlt">state</span> nuclear wave function of the SSSH radical are calculated using quantum diffusion Monte Carlo on interpolated potential <span class="hlt">energy</span> surfaces (PESs) constructed using a variety of method and basis set combinations. The ZPE of SSSH, which is approximately 29 kJ mol(-1) at the CCSD(T)/6-31G* level of theory, has a 4 kJ mol(-1) dependence on the treatment of electron correlation. The anharmonic ZPEs are consistently 0.3 kJ mol(-1) lower in <span class="hlt">energy</span> than the harmonic ZPEs calculated at the Hartree-Fock and MP2 levels of theory, and 0.7 kJ mol(-1) lower in <span class="hlt">energy</span> at the CCSD(T)/6-31G* level of theory. Ideally, for sub-kJ mol(-1) thermochemical accuracy, ZPEs should be calculated using correlated methods with as big a basis set as practicable. The <span class="hlt">ground</span> <span class="hlt">state</span> nuclear wave function of SSSH also has significant method and basis set dependence. The analysis of the nuclear wave function indicates that SSSH is localized to a single symmetry equivalent global minimum, despite having sufficient ZPE to be delocalized over both minima. As part of this work, modifications to the interpolated PES construction scheme of Collins and co-workers are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010JChPh.132e4105K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010JChPh.132e4105K"><span>Method and basis set dependence of anharmonic <span class="hlt">ground</span> <span class="hlt">state</span> nuclear wave functions and zero-point <span class="hlt">energies</span>: Application to SSSH</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kolmann, Stephen J.; Jordan, Meredith J. T.</p> <p>2010-02-01</p> <p>One of the largest remaining errors in thermochemical calculations is the determination of the zero-point <span class="hlt">energy</span> (ZPE). The fully coupled, anharmonic ZPE and <span class="hlt">ground</span> <span class="hlt">state</span> nuclear wave function of the SSSH radical are calculated using quantum diffusion Monte Carlo on interpolated potential <span class="hlt">energy</span> surfaces (PESs) constructed using a variety of method and basis set combinations. The ZPE of SSSH, which is approximately 29 kJ mol-1 at the CCSD(T)/6-31G∗ level of theory, has a 4 kJ mol-1 dependence on the treatment of electron correlation. The anharmonic ZPEs are consistently 0.3 kJ mol-1 lower in <span class="hlt">energy</span> than the harmonic ZPEs calculated at the Hartree-Fock and MP2 levels of theory, and 0.7 kJ mol-1 lower in <span class="hlt">energy</span> at the CCSD(T)/6-31G∗ level of theory. Ideally, for sub-kJ mol-1 thermochemical accuracy, ZPEs should be calculated using correlated methods with as big a basis set as practicable. The <span class="hlt">ground</span> <span class="hlt">state</span> nuclear wave function of SSSH also has significant method and basis set dependence. The analysis of the nuclear wave function indicates that SSSH is localized to a single symmetry equivalent global minimum, despite having sufficient ZPE to be delocalized over both minima. As part of this work, modifications to the interpolated PES construction scheme of Collins and co-workers are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=function+AND+wave&pg=2&id=EJ1032438','ERIC'); return false;" href="https://eric.ed.gov/?q=function+AND+wave&pg=2&id=EJ1032438"><span>Using a Spreadsheet to Solve the Schro¨dinger Equations for the <span class="hlt">Energies</span> of the <span class="hlt">Ground</span> Electronic <span class="hlt">State</span> and the Two Lowest Excited <span class="hlt">States</span> of H[subscript2</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>Ge, Yingbin; Rittenhouse, Robert C.; Buchanan, Jacob C.; Livingston, Benjamin</p> <p>2014-01-01</p> <p>We have designed an exercise suitable for a lab or project in an undergraduate physical chemistry course that creates a Microsoft Excel spreadsheet to calculate the <span class="hlt">energy</span> of the S[subscript 0] <span class="hlt">ground</span> electronic <span class="hlt">state</span> and the S[subscript 1] and T[subscript 1] excited <span class="hlt">states</span> of H[subscript 2]. The spreadsheet calculations circumvent the…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24784259','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24784259"><span>Local CC2 response method based on the Laplace transform: analytic <span class="hlt">energy</span> gradients for <span class="hlt">ground</span> and excited <span class="hlt">states</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ledermüller, Katrin; Schütz, Martin</p> <p>2014-04-28</p> <p>A multistate local CC2 response method for the calculation of analytic <span class="hlt">energy</span> gradients with respect to nuclear displacements is presented for <span class="hlt">ground</span> and electronically excited <span class="hlt">states</span>. The gradient enables the search for equilibrium geometries of extended molecular systems. Laplace transform is used to partition the eigenvalue problem in order to obtain an effective singles eigenvalue problem and adaptive, <span class="hlt">state</span>-specific local approximations. This leads to an approximation in the <span class="hlt">energy</span> Lagrangian, which however is shown (by comparison with the corresponding gradient method without Laplace transform) to be of no concern for geometry optimizations. The accuracy of the local approximation is tested and the efficiency of the new code is demonstrated by application calculations devoted to a photocatalytic decarboxylation process of present interest.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017SPIE10465E..08L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017SPIE10465E..08L"><span>Design and analysis of coplanar waveguide triple-<span class="hlt">band</span> antenna based on defected <span class="hlt">ground</span> structure</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lv, Hong; Chen, Wanli; Xia, Xinsheng; Qi, Peng; Sun, Quanling</p> <p>2017-11-01</p> <p>A kind of coplanar waveguide triple-<span class="hlt">band</span> antenna based on defected <span class="hlt">ground</span> structure is proposed, which has novel structure. Three batches with different frequency <span class="hlt">band</span> are constructed by utilizing line combination, overlapping, and symmetry method. Stop <span class="hlt">band</span> signals among three frequency <span class="hlt">bands</span> are effectively suppressed by slots with different structures. More satisfactory impedance matching is realized by means of changing slot structure and improving return-loss. The presented antenna can operates simultaneously in various systems such as 3G / 4G wireless communication, Bluetooth, Worldwide Interoperability for Microwave Access, Wireless LAN. Test results show that the antenna has good radiation and gain in its working frequency <span class="hlt">band</span>, and that it has great application potentials.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1999JAP....86.4419P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1999JAP....86.4419P"><span><span class="hlt">Band</span> gap narrowing in n-type and p-type 3C-, 2H-, 4H-, 6H-SiC, and Si</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Persson, C.; Lindefelt, U.; Sernelius, B. E.</p> <p>1999-10-01</p> <p>Doping-induced <span class="hlt">energy</span> shifts of the conduction <span class="hlt">band</span> minimum and the valence <span class="hlt">band</span> maximum have been calculated for n-type and p-type 3C-, 2H-, 4H-, 6H-SiC, and Si. The narrowing of the fundamental <span class="hlt">band</span> gap and of the optical <span class="hlt">band</span> gap are presented as functions of ionized impurity concentration. The calculations go beyond the common parabolic treatments of the <span class="hlt">ground</span> <span class="hlt">state</span> <span class="hlt">energy</span> dispersion by using <span class="hlt">energy</span> dispersion and overlap integrals from <span class="hlt">band</span> structure calculations. The nonparabolic valence <span class="hlt">band</span> curvatures influence strongly the <span class="hlt">energy</span> shifts especially in p-type materials. The utilized method is based on a zero-temperature Green's function formalism within the random phase approximation with local field correction according to Hubbard. We have parametrized the shifts of the conduction and the valence <span class="hlt">bands</span> and made comparisons with recently published results from a semi-empirical model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29676041','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29676041"><span>Engineering the <span class="hlt">Band</span> Gap <span class="hlt">States</span> of the Rutile TiO2 (110) Surface by Modulating the Active Heteroatom.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yu, Yaoguang; Yang, Xu; Zhao, Yanling; Zhang, Xiangbin; An, Liang; Huang, Miaoyan; Chen, Gang; Zhang, Ruiqin</p> <p>2018-04-19</p> <p>Introducing <span class="hlt">band</span> gap <span class="hlt">states</span> to TiO 2 photocatalysts is an efficient strategy for expanding the range of accessible <span class="hlt">energy</span> available in the solar spectrum. However, few approaches are able to introduce <span class="hlt">band</span> gap <span class="hlt">states</span> and improve photocatalytic performance simultaneously. Introducing <span class="hlt">band</span> gap <span class="hlt">states</span> by creating surface disorder can incapacitate reactivity where unambiguous adsorption sites are a prerequisite. An alternative method for introduction of <span class="hlt">band</span> gap <span class="hlt">states</span> is demonstrated in which selected heteroatoms are implanted at preferred surface sites. Theoretical prediction and experimental verification reveal that the implanted heteroatoms not only introduce <span class="hlt">band</span> gap <span class="hlt">states</span> without creating surface disorder, but also function as active sites for the Cr VI reduction reaction. This promising approach may be applicable to the surfaces of other solar harvesting materials where engineered <span class="hlt">band</span> gap <span class="hlt">states</span> could be used to tune photophysical and -catalytic properties. © 2018 Wiley-VCH Verlag GmbH & Co. KGaA, Weinheim.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvB..97c5161R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvB..97c5161R"><span>Compact localized <span class="hlt">states</span> and flat <span class="hlt">bands</span> from local symmetry partitioning</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Röntgen, M.; Morfonios, C. V.; Schmelcher, P.</p> <p>2018-01-01</p> <p>We propose a framework for the connection between local symmetries of discrete Hamiltonians and the design of compact localized <span class="hlt">states</span>. Such compact localized <span class="hlt">states</span> are used for the creation of tunable, local symmetry-induced bound <span class="hlt">states</span> in an <span class="hlt">energy</span> continuum and flat <span class="hlt">energy</span> <span class="hlt">bands</span> for periodically repeated local symmetries in one- and two-dimensional lattices. The framework is based on very recent theorems in graph theory which are here employed to obtain a block partitioning of the Hamiltonian induced by the symmetry of a given system under local site permutations. The diagonalization of the Hamiltonian is thereby reduced to finding the eigenspectra of smaller matrices, with eigenvectors automatically divided into compact localized and extended <span class="hlt">states</span>. We distinguish between local symmetry operations which commute with the Hamiltonian, and those which do not commute due to an asymmetric coupling to the surrounding sites. While valuable as a computational tool for versatile discrete systems with locally symmetric structures, the approach provides in particular a unified, intuitive, and efficient route to the flexible design of compact localized <span class="hlt">states</span> at desired <span class="hlt">energies</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1132327-alternative-ground-states-enable-pathway-switching-biological-electron-transfer','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1132327-alternative-ground-states-enable-pathway-switching-biological-electron-transfer"><span>Alternative <span class="hlt">ground</span> <span class="hlt">states</span> enable pathway switching in biological electron transfer</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Abriata, Luciano A.; Alvarez-Paggi, Damian; Ledesma, Gabirela N.; ...</p> <p>2012-10-10</p> <p>Electron transfer is the simplest chemical reaction and constitutes the basis of a large variety of biological processes, such as photosynthesis and cellular respiration. Nature has evolved specific proteins and cofactors for these functions. The mechanisms optimizing biological electron transfer have been matter of intense debate, such as the role of the protein milieu between donor and acceptor sites. Here we propose a mechanism regulating long-range electron transfer in proteins. Specifically, we report a spectroscopic, electrochemical, and theoretical study on WT and single-mutant CuA redox centers from Thermus thermophilus, which shows that thermal fluctuations may populate two alternative <span class="hlt">ground-state</span> electronicmore » wave functions optimized for electron entry and exit, respectively, through two different and nearly perpendicular pathways. In conclusion, these findings suggest a unique role for alternative or “invisible” electronic <span class="hlt">ground</span> <span class="hlt">states</span> in directional electron transfer. Moreover, it is shown that this <span class="hlt">energy</span> gap and, therefore, the equilibrium between <span class="hlt">ground</span> <span class="hlt">states</span> can be fine-tuned by minor perturbations, suggesting alternative ways through which protein–protein interactions and membrane potential may optimize and regulate electron–proton <span class="hlt">energy</span> transduction.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1339166-rotational-band-structure-mg32','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1339166-rotational-band-structure-mg32"><span>Rotational <span class="hlt">band</span> structure in Mg 32</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>Crawford, H. L.; Fallon, P.; Macchiavelli, A. O.</p> <p>2016-03-01</p> <p>There is significant evidence supporting the existence of deformed <span class="hlt">ground</span> <span class="hlt">states</span> within the neutron-rich N ≈ 20 neon, sodium, and magnesium isotopes that make up what is commonly called the “island of inversion.” However, the rotational <span class="hlt">band</span> structures, which are a characteristic fingerprint of a rigid nonspherical shape, have yet to be observed. In this work, we report on a measurement and analysis of the yrast (lowest lying) rotational <span class="hlt">band</span> in 32 Mg up to spin I = 6 + produced in a two-step projectile fragmentation reaction and observed using the <span class="hlt">state</span>-of-the-art γ -ray tracking detector array, GRETINA ( γmore » -ray <span class="hlt">energy</span> tracking in-beam nuclear array). Large-scale shell-model calculations using the SDPF-U-MIX effective interaction show excellent agreement with the new data. Moreover, a theoretical analysis of the spectrum of rotational <span class="hlt">states</span> as a function of the pairing gap, together with cranked-shell-model calculations, provides intriguing evidence for a reduction in pairing correlations with increased angular momentum, also in line with the shell-model results.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JMP....59c1504L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JMP....59c1504L"><span><span class="hlt">Ground</span> <span class="hlt">state</span> sign-changing solutions for fractional Kirchhoff equations in bounded domains</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Luo, Huxiao; Tang, Xianhua; Gao, Zu</p> <p>2018-03-01</p> <p>We study the existence of <span class="hlt">ground</span> <span class="hlt">state</span> sign-changing solutions for the fractional Kirchhoff problem. Under mild assumptions on the nonlinearity, by using some new analytical skills and the non-Nehari manifold method, we prove that the fractional Kirchhoff problem possesses a <span class="hlt">ground</span> <span class="hlt">state</span> sign-changing solution ub. Moreover, we show that the <span class="hlt">energy</span> of ub is strictly larger than twice that of the <span class="hlt">ground</span> <span class="hlt">state</span> solutions of Nehari-type. Finally, we establish the convergence property of ub as the parameter b ↘ 0. Our results generalize some results obtained by Shuai [J. Differ. Equations 259, 1256 (2015)] and Tang and Cheng [J. Differ. Equations 261, 2384 (2016)].</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/2017isms.confETK08G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017isms.confETK08G"><span>First High Resolution IR Spectra of 2,2-D_{2}-PROPANE. the νb{15} (B_{1}) A-Type <span class="hlt">Band</span> Near 954.709 \\wn. Determination of <span class="hlt">Ground</span> and Upper <span class="hlt">State</span> Constants.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gjuraj, Daniel; Daunt, S. J.; Grzywacz, Robert; Lafferty, Walter; Flaud, Jean-Marie; Billinghurst, Brant E.</p> <p>2017-06-01</p> <p>As part of our project on the study of isotopologues of propane we have taken the spectra of the 2-D and 2,2-D_2 substituted species. There have been no studies of these species since the early IR studies. We recorded high resolution (Δν = 0.0009 \\wn) FTS data on the Canadian Light Source Far-IR beamline. The spectra of all <span class="hlt">bands</span> of both species in the region examined (500 - 1250 \\wn) show torsionally perturbed lines, all but one <span class="hlt">band</span> appearing globally perturbed. Virtually all <span class="hlt">bands</span> were not amenable to analysis at present except for the νb{15} (B_{1}) A-type <span class="hlt">band</span> centered at 954.709 \\wn. One can still see a few perturbed lines with torsional components but overall most lines were single and could be readily assigned using traditional methods. The spectrum is modelled well using PGOPHER. No MW determined GS constants were available so we have analyzed about 3500 levels to determine both <span class="hlt">ground</span> <span class="hlt">state</span> and upper <span class="hlt">state</span> rotational constants. Friedman & Turkevich, J. Chem. Phys. 17, 1012 ff. (1949) McMurry, Thornton & Condon, J. Chem. Phys. 17, 918 ff. (1949) McMurry & Thornton, J. Chem. Phys. 19, 1014 ff.(1951) Gayles & King, Spectrochim. Acta 21, 543 ff.(1965) Kondo & Saeki, Spectrochim. Acta 29A, 735 ff. (1973) Western, J. Quant. Spectrosc. Rad. Transf. 186, 221 ff. (2017).</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 electronic <span class="hlt">states</span> 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 electronic <span class="hlt">states</span> 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 electronic wave function for quasi-Bloch <span class="hlt">states</span> yields a non-Hermitian Hamiltonian matrix characterized by matrix elements of constituent crystals and concentration of constituents. Solving secular equations for each k-<span class="hlt">state</span> 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.osti.gov/biblio/21189904-gamma-vibrational-states-superheavy-nuclei','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/21189904-gamma-vibrational-states-superheavy-nuclei"><span>{gamma}-vibrational <span class="hlt">states</span> in superheavy nuclei</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>Sun Yang; Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou 730000; Joint Institute for Nuclear Astrophysics, University of Notre Dame, Notre Dame, Indiana 46556</p> <p>2008-04-15</p> <p>Recent experimental advances have made it possible to study excited structure in superheavy nuclei. The observed <span class="hlt">states</span> have often been interpreted as quasiparticle excitations. We show that in superheavy nuclei collective vibrations systematically appear as low-<span class="hlt">energy</span> excitation modes. By using the microscopic Triaxial Projected Shell Model, we make a detailed prediction on {gamma}-vibrational <span class="hlt">states</span> and their E2 transition probabilities to the <span class="hlt">ground</span> <span class="hlt">state</span> <span class="hlt">band</span> in fermium and nobelium isotopes where active structure research is going on, and in {sup 270}Ds, the heaviest isotope where decay data have been obtained for the <span class="hlt">ground-state</span> and for an isomeric <span class="hlt">state</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JQSRT.208...39R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JQSRT.208...39R"><span>Photoionization <span class="hlt">bands</span> of rubidium molecule</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rakić, M.; Pichler, G.</p> <p>2018-03-01</p> <p>We studied the absorption spectrum of dense rubidium vapor generated in a T-type sapphire cell with a special emphasis on the structured photoionization continuum observed in the 200-300 nm spectral region. The photoionization spectrum has a continuous atomic contribution with a pronounced Seaton-Cooper minimum at about 250 nm and a molecular photoionization contribution with many broad <span class="hlt">bands</span>. We discuss the possible origin of the photoionization <span class="hlt">bands</span> as stemming from the absorption from the <span class="hlt">ground</span> <span class="hlt">state</span> of the Rb2 molecule to excited <span class="hlt">states</span> of Rb2+* and to doubly excited autoionizing <span class="hlt">states</span> of Rb2** molecule. All these photoionization <span class="hlt">bands</span> are located above the Rb+ and Rb2+ ionization limits.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22612584-description-alternating-parity-bands-within-dinuclear-system-model','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22612584-description-alternating-parity-bands-within-dinuclear-system-model"><span>Description of alternating-parity <span class="hlt">bands</span> within the dinuclear-system model</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>Shneidman, T. M.; Adamian, G. G., E-mail: adamian@theor.jinr.ru; Antonenko, N. V.</p> <p>2016-11-15</p> <p>A cluster approach is used to describe <span class="hlt">ground-state</span>-based alternating-parity <span class="hlt">bands</span> in even–even nuclei and to study the <span class="hlt">band</span>-termination mechanism. A method is proposed for testing the cluster nature of alternating-parity <span class="hlt">bands</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1984CPL...108..367F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1984CPL...108..367F"><span>Analytical ab initio potential-<span class="hlt">energy</span> surfaces for the <span class="hlt">ground</span> and the first singlet excited <span class="hlt">states</span> of HeH 2</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Farantos, Stavros C.; Murrell, J. N.; Carter, S.</p> <p>1984-07-01</p> <p>Analytical potential-<span class="hlt">energy</span> surfaces have been constructed for the <span class="hlt">ground</span> and the first excited <span class="hlt">states</span> of HeH 2. The functions fit ab initio MRD CI calculations with standard deviations of 0.05 and 0.13 eV for the <span class="hlt">ground</span> and the excited surface respectively. Classical trajectory calculations for collisions of 4Hc with HD(B 1Σ u+, υ = 3, J = 2) at the temperature T = 297 K yields the electronic quenching cross section σ Q = 6.5 A 2 and the vibrational cross section σ 3→2 = 3.8 A 2. The results are in qualitative agreement with the experimental values of Fink, Akins and Moore.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20100040589','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20100040589"><span>Advances in High <span class="hlt">Energy</span> Solid-<span class="hlt">State</span> 2-micron Laser Transmitter Development for <span class="hlt">Ground</span> and Airborne Wind and CO2 Measurements</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Singh, Upendra N.; Yu, Jirong; Petros, Mulugeta; Chen, Songsheng; Kavaya, Michael J.; Trieu, Bo; Bai, Yingxin; Petzar, Paul; Modlin, Edward A.; Koch, Grady; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20100040589'); toggleEditAbsImage('author_20100040589_show'); toggleEditAbsImage('author_20100040589_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20100040589_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20100040589_hide"></p> <p>2010-01-01</p> <p>Sustained research efforts at NASA Langley Research Center (LaRC) during last fifteen years have resulted in a significant advancement in 2-micron diode-pumped, solid-<span class="hlt">state</span> laser transmitter for wind and carbon dioxide measurement from <span class="hlt">ground</span>, air and space-borne platform. Solid-<span class="hlt">state</span> 2-micron laser is a key subsystem for a coherent Doppler lidar that measures the horizontal and vertical wind velocities with high precision and resolution. The same laser, after a few modifications, can also be used in a Differential Absorption Lidar (DIAL) system for measuring atmospheric CO2 concentration profiles. Researchers at NASA Langley Research Center have developed a compact, flight capable, high <span class="hlt">energy</span>, injection seeded, 2-micron laser transmitter for <span class="hlt">ground</span> and airborne wind and carbon dioxide measurements. It is capable of producing 250 mJ at 10 Hz by an oscillator and one amplifier. This compact laser transmitter was integrated into a mobile trailer based coherent Doppler wind and CO2 DIAL system and was deployed during field measurement campaigns. This paper will give an overview of 2-micron solid-<span class="hlt">state</span> laser technology development and discuss results from recent <span class="hlt">ground</span>-based field measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013PhDT........59D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013PhDT........59D"><span>Mission aware <span class="hlt">energy</span> saving strategies for Army <span class="hlt">ground</span> vehicles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dattathreya, Macam S.</p> <p></p> <p> on, gear is on neutral position, the vehicle is stationary, and the alternator powers the systems. The proposed <span class="hlt">energy</span> saving strategy for silent surveillance mission minimizes unnecessary battery discharges by controlling the power <span class="hlt">states</span> of systems according to the mission needs and available battery capacity. Initial experiments show that the proposed approach saves 3% <span class="hlt">energy</span> when compared with the baseline strategy for one scenario and 1.8% for the second scenario. The proposed <span class="hlt">energy</span> saving strategy for normal surveillance mission operates the engine at fuel-efficient speeds to meet vehicle demand and to save fuel. The experiment and simulation uses a computerized vehicle model and a test bench to validate the approach. In comparison to vehicles with fixed high-idle engine speed increments, experiments show that the proposed strategy saves fuel <span class="hlt">energy</span> in the range of 0-4.9% for the tested power demand range of 44-69 kW. It is hoped to implement the proposed strategies on a real Army <span class="hlt">ground</span> vehicle to start realizing the <span class="hlt">energy</span> savings.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20010047499','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20010047499"><span>Potential <span class="hlt">Energy</span> Curves and Transport Properties for the Interaction of He with Other <span class="hlt">Ground-state</span> Atoms</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Partridge, Harry; Stallcop, James R.; Levin, Eugene; Arnold, Jim (Technical Monitor)</p> <p>2001-01-01</p> <p>The interactions of a He atom with a heavier atom are examined for 26 different elements, which are consecutive members selected from three rows (Li - Ne, Na - Ar, and K,Ca, Ga - Kr) and column 12 (Zn,Cd) of the periodic table. Interaction <span class="hlt">energies</span> are determined wing high-quality ab initio calculations for the <span class="hlt">states</span> of the molecule that would be formed from each pair of atoms in their <span class="hlt">ground</span> <span class="hlt">states</span>. Potential <span class="hlt">energies</span> are tabulated for a broad range of Interatomic separation distances. The results show, for example, that the <span class="hlt">energy</span> of an alkali interaction at small separations is nearly the same as that of a rare-gas interaction with the same electron configuration for the dosed shells. Furthermore, the repulsive-range parameter for this region is very short compared to its length for the repulsion dominated by the alkali-valence electron at large separations (beyond about 3-4 a(sub 0)). The potential <span class="hlt">energies</span> in the region of the van der Waals minimum agree well with the most accurate results available. The ab initio <span class="hlt">energies</span> are applied to calculate scattering cross sections and obtain the collision integrals that are needed to determine transport properties to second order. The theoretical values of Li-He total scattering cross sections and the rare-gas atom-He transport properties agree well (to within about 1%) with the corresponding measured data. Effective potential <span class="hlt">energies</span> are constructed from the ab initio <span class="hlt">energies</span>; the results have been shown to reproduce known transport data and can be readily applied to predict unknown transport properties for like-atom interactions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015ChPhB..24i0301M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015ChPhB..24i0301M"><span><span class="hlt">Ground-state</span> information geometry and quantum criticality in an inhomogeneous spin model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ma, Yu-Quan</p> <p>2015-09-01</p> <p>We investigate the <span class="hlt">ground-state</span> Riemannian metric and the cyclic quantum distance of an inhomogeneous quantum spin-1/2 chain in a transverse field. This model can be diagonalized by using a general canonical transformation to the fermionic Hamiltonian mapped from the spin system. The <span class="hlt">ground-state</span> Riemannian metric is derived exactly on a parameter manifold ring S1, which is introduced by performing a gauge transformation to the spin Hamiltonian through a twist operator. The cyclic <span class="hlt">ground-state</span> quantum distance and the second derivative of the <span class="hlt">ground-state</span> <span class="hlt">energy</span> are studied in different exchange coupling parameter regions. Particularly, we show that, in the case of exchange coupling parameter Ja = Jb, the quantum ferromagnetic phase can be characterized by an invariant quantum distance and this distance will decay to zero rapidly in the paramagnetic phase. Project supported by the National Natural Science Foundation of China (Grant Nos. 11404023 and 11347131).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1989PhRvA..40.6084L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1989PhRvA..40.6084L"><span><span class="hlt">Ground-state</span> <span class="hlt">energies</span> and highest occupied eigenvalues of atoms in exchange-only 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>Li, Yan; Harbola, Manoj K.; Krieger, J. B.; Sahni, Viraht</p> <p>1989-11-01</p> <p>The exchange-correlation potential of the Kohn-Sham density-functional theory has recently been interpreted as the work required to move an electron against the electric field of its Fermi-Coulomb hole charge distribution. In this paper we present self-consistent results for <span class="hlt">ground-state</span> total <span class="hlt">energies</span> and highest occupied eigenvalues of closed subshell atoms as obtained by this formalism in the exchange-only approximation. The total <span class="hlt">energies</span>, which are an upper bound, lie within 50 ppm of Hartree-Fock theory for atoms heavier than Be. The highest occupied eigenvalues, as a consequence of this interpretation, approximate well the experimental ionization potentials. In addition, the self-consistently calculated exchange potentials are very close to those of Talman and co-workers [J. D. Talman and W. F. Shadwick, Phys. Rev. A 14, 36 (1976); K. Aashamar, T. M. Luke, and J. D. Talman, At. Data Nucl. Data Tables 22, 443 (1978)].</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19950906','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19950906"><span>Mid-infrared picosecond pump-dump-probe and pump-repump-probe experiments to resolve a <span class="hlt">ground-state</span> intermediate in cyanobacterial phytochrome Cph1.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>van Wilderen, Luuk J G W; Clark, Ian P; Towrie, Michael; van Thor, Jasper J</p> <p>2009-12-24</p> <p>Multipulse picosecond mid-infrared spectroscopy has been used to study photochemical reactions of the cyanobacterial phytochrome photoreceptor Cph1. Different photophysical schemes have been discussed in the literature to describe the pathways after photoexcitation, particularly, to identify reaction phases that are linked to photoisomerisation and electronic decay in the 1566-1772 cm(-1) region that probes C=C and C=O stretching modes of the tetrapyrrole chromophore. Here, multipulse spectroscopy is employed, where, compared to conventional visible pump-mid-infrared probe spectroscopy, an additional visible pulse is incorporated that interacts with populations that are evolving on the excited- and <span class="hlt">ground-state</span> potential <span class="hlt">energy</span> surfaces. The time delays between the pump and the dump pulse are chosen such that the dump pulse interacts with different phases in the reaction process. The pump and dump pulses are at the same wavelength, 640 nm, and are resonant with the Pr <span class="hlt">ground</span> <span class="hlt">state</span> as well as with the excited <span class="hlt">state</span> and intermediates. Because the dump pulse additionally pumps the remaining, partially recovered, and partially oriented <span class="hlt">ground-state</span> population, theory is developed for estimating the fraction of excited-<span class="hlt">state</span> molecules. The calculations take into account the model-dependent <span class="hlt">ground-state</span> recovery fraction, the angular dependence of the population transfer resulting from the finite bleach that occurs with linearly polarized intense femtosecond optical excitation, and the partially oriented population for the dump field. Distinct differences between the results from the experiments that use a 1 or a 14 ps dump time favor a branching evolution from S1 to an excited <span class="hlt">state</span> or reconfigured chromophore and to a newly identified <span class="hlt">ground-state</span> intermediate (GSI). Optical dumping at 1 ps shows the instantaneous induced absorption of a delocalized C=C stretching mode at 1608 cm(-1), where the increased cross section is associated with the electronic <span class="hlt">ground-state</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170010234','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170010234"><span>Exponentially-Biased <span class="hlt">Ground-State</span> Sampling of Quantum Annealing Machines with Transverse-Field Driving Hamiltonians</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mandra, Salvatore</p> <p>2017-01-01</p> <p>We study the performance of the D-Wave 2X quantum annealing machine on systems with well-controlled <span class="hlt">ground-state</span> degeneracy. While obtaining the <span class="hlt">ground</span> <span class="hlt">state</span> of a spin-glass benchmark instance represents a difficult task, the gold standard for any optimization algorithm or machine is to sample all solutions that minimize the Hamiltonian with more or less equal probability. Our results show that while naive transverse-field quantum annealing on the D-Wave 2X device can find the <span class="hlt">ground-state</span> <span class="hlt">energy</span> of the problems, it is not well suited in identifying all degenerate <span class="hlt">ground-state</span> configurations associated to a particular instance. Even worse, some <span class="hlt">states</span> are exponentially suppressed, in agreement with previous studies on toy model problems [New J. Phys. 11, 073021 (2009)]. These results suggest that more complex driving Hamiltonians are needed in future quantum annealing machines to ensure a fair sampling of the <span class="hlt">ground-state</span> manifold.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhDT.......102T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhDT.......102T"><span>Electronic <span class="hlt">Band</span> Structure Tuning of Highly-Mismatched-Alloys for <span class="hlt">Energy</span> Conversion Applications</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ting, Min</p> <p></p> <p>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 <span class="hlt">energy</span> conversion efficiency theoretical limit of a single junction solar cell. Combining with a material of 1.8 eV <span class="hlt">band</span> gap, SBTSC can theoretically achieve <span class="hlt">energy</span> conversion efficiency > 45%. ZnO and GaN are wide <span class="hlt">band</span> gap semiconductors. Alloying Te in ZnO and alloying Sb in GaN result in large <span class="hlt">band</span> gap reduction to < 2 eV from 3.3 eV and 3.4 eV respectively. The <span class="hlt">band</span> gap reduction is majorly achieved by the upward shift of valence <span class="hlt">band</span> (VB). Incorporating Te in ZnO modifies the VB of ZnO through the valence-<span class="hlt">band</span> anticrossing (VBAC) interaction between localized Te <span class="hlt">states</span> and ZnO VB delocalized <span class="hlt">states</span>, which forms a Te-derived VB at 1 eV above the host VB. Similar <span class="hlt">band</span> 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 <span class="hlt">band</span> 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 <span class="hlt">band</span> 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 (<span class="hlt">band</span> gap at 1.8 eV) on Si bottom cell is proposed as a promising SBTSC device.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/21290054-energy-ground-sup-excited-states-sub-lambda-sub-lambda-sup-partial-ten-body-model','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/21290054-energy-ground-sup-excited-states-sub-lambda-sub-lambda-sup-partial-ten-body-model"><span><span class="hlt">Energy</span> of the <span class="hlt">ground</span> and 2{sup +} excited <span class="hlt">states</span> of {sub {lambda}}{sub {lambda}}{sup 10}Be: A partial ten-body model</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>Shoeb, Mohammad; Sonika</p> <p>2009-08-15</p> <p>The <span class="hlt">energies</span> of the <span class="hlt">ground</span> and excited 2{sup +} <span class="hlt">states</span> of {sub {lambda}}{sub {lambda}}{sup 10}Be have been calculated variationally in the Monte Carlo framework. The hypernucleus is treated as a partial ten-body problem in the {lambda}{lambda}+{alpha}{alpha} model where nucleonic degrees of freedom of {alpha}'s are taken into consideration ignoring the antisymmetrization between two {alpha}'s. The central two-body {lambda}N and {lambda}{lambda} and the three-body dispersive and two-pion exchange {lambda}NN forces, constrained by the {lambda}p scattering data and the observed <span class="hlt">ground</span> <span class="hlt">state</span> <span class="hlt">energies</span> of {sub {lambda}}{sup 5}He and {sub {lambda}}{sub {lambda}}{sup 6}He, are employed. The product-type trial wave function predicts binding energymore » for the <span class="hlt">ground</span> <span class="hlt">state</span> considerably less than for the event reported by Danysz et al.; however, it is consistent with the value deduced assuming a {gamma} ray of 3.04 MeV must have escaped undetected in the decay of the product {sub {lambda}}{sup 9}Be* {yields} {sub {lambda}}{sup 9}Be+{gamma} of the emulsion event {sub {lambda}}{sub {lambda}}{sup 10}Be{yields} {pi}{sup -}+p+{sub {lambda}}{sup 9}Be* and for the excited 2{sup +} <span class="hlt">state</span> closer to the value measured in the Demachi-Yanagi event. The hypernucleus {sub {lambda}}{sub {lambda}}{sup 10}Be has an oblate shape in the excited <span class="hlt">state</span>. These results are consistent with the earlier four-body {alpha} cluster model approach where {alpha}'s are assumed to be structureless entities.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvB..97l1113N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvB..97l1113N"><span>Emergent low-<span class="hlt">energy</span> bound <span class="hlt">states</span> in the two-orbital Hubbard model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Núñez-Fernández, Y.; Kotliar, G.; Hallberg, K.</p> <p>2018-03-01</p> <p>A repulsive Coulomb interaction between electrons in different orbitals in correlated materials can give rise to bound quasiparticle <span class="hlt">states</span>. We study the nonhybridized two-orbital Hubbard model with intra- (inter)orbital interaction U (U12) and different bandwidths using an improved dynamical mean-field theory numerical technique which leads to reliable spectra on the real <span class="hlt">energy</span> axis directly at zero temperature. We find that a finite density of <span class="hlt">states</span> at the Fermi <span class="hlt">energy</span> in one <span class="hlt">band</span> is correlated with the emergence of well-defined quasiparticle <span class="hlt">states</span> at excited <span class="hlt">energies</span> Δ =U -U12 in the other <span class="hlt">band</span>. These excitations are interband holon-doublon bound <span class="hlt">states</span>. At the symmetric point U =U12 , the quasiparticle peaks are located at the Fermi <span class="hlt">energy</span>, leading to a simultaneous and continuous Mott transition settling a long-standing controversy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..MAR.T1287M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..MAR.T1287M"><span><span class="hlt">Ground-State</span> of the Bose-Hubbard Model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mancini, J. D.; Fessatidis, V.; Bowen, S. P.; Murawski, R. K.; Maly, J.</p> <p></p> <p>The Bose-Hubbard Model represents a s simple theoretical model to describe the physics of interacting Boson systems. In particular it has proved to be an effective description of a number of physical systems such as arrays of Josephson arrays as well as dilute alkali gases in optical lattices. Here we wish to study the <span class="hlt">ground-state</span> of this system using two disparate but related moments calculational schemes: the Lanczos (tridiagonal) method as well as a Generalized moments approach. The Hamiltonian to be studied is given by (in second-quantized notation): H = - t ∑ < i , j > bi†bj +U/2 ∑ ini<m:mfenced close=")" open="(" separators="">ni - 1</m:mfenced> - μ ∑ ini . Here i is summed over all lattice sites, and < i , j > denotes summation over all neighbhoring sites i and j, while bi† and bi are bosonic creation and annihilation operators. ni = bi†bi gives the number of particles on site i. Parameter t is the hopping amplitude, describing mobility of bosons in the lattice. Parameter U describes the on-site interaction, repulsive, if U > 0 , and attractive for U < 0 . μ is the chemical potential. Both the <span class="hlt">ground-state</span> <span class="hlt">energy</span> and <span class="hlt">energy</span> gap are evaluated as a function of t, U and μ.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009JSP...135..175F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009JSP...135..175F"><span>High-Order Coupled Cluster Method (CCM) Calculations for Quantum Magnets with Valence-Bond <span class="hlt">Ground</span> <span class="hlt">States</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Farnell, D. J. J.; Richter, J.; Zinke, R.; Bishop, R. F.</p> <p>2009-04-01</p> <p>In this article, we prove that exact representations of dimer and plaquette valence-bond ket <span class="hlt">ground</span> <span class="hlt">states</span> for quantum Heisenberg antiferromagnets may be formed via the usual coupled cluster method (CCM) from independent-spin product (e.g. Néel) model <span class="hlt">states</span>. We show that we are able to provide good results for both the <span class="hlt">ground-state</span> <span class="hlt">energy</span> and the sublattice magnetization for dimer and plaquette valence-bond phases within the CCM. As a first example, we investigate the spin-half J 1- J 2 model for the linear chain, and we show that we are able to reproduce exactly the dimerized <span class="hlt">ground</span> (ket) <span class="hlt">state</span> at J 2/ J 1=0.5. The dimerized phase is stable over a range of values for J 2/ J 1 around 0.5, and results for the <span class="hlt">ground-state</span> <span class="hlt">energies</span> are in good agreement with the results of exact diagonalizations of finite-length chains in this regime. We present evidence of symmetry breaking by considering the ket- and bra-<span class="hlt">state</span> correlation coefficients as a function of J 2/ J 1. A radical change is also observed in the behavior of the CCM sublattice magnetization as we enter the dimerized phase. We then consider the Shastry-Sutherland model and demonstrate that the CCM can span the correct <span class="hlt">ground</span> <span class="hlt">states</span> in both the Néel and the dimerized phases. Once again, very good results for the <span class="hlt">ground-state</span> <span class="hlt">energies</span> are obtained. We find CCM critical points of the bra-<span class="hlt">state</span> equations that are in agreement with the known phase transition point for this model. The results for the sublattice magnetization remain near to the "true" value of zero over much of the dimerized regime, although they diverge exactly at the critical point. Finally, we consider a spin-half system with nearest-neighbor bonds for an underlying lattice corresponding to the magnetic material CaV4O9 (CAVO). We show that we are able to provide excellent results for the <span class="hlt">ground-state</span> <span class="hlt">energy</span> in each of the plaquette-ordered, Néel-ordered, and dimerized regimes of this model. The exact plaquette and dimer <span class="hlt">ground</span> <span class="hlt">states</span> are</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007PhRvL..99r6801Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007PhRvL..99r6801Y"><span>Quasiparticle <span class="hlt">Energies</span> and <span class="hlt">Band</span> Gaps in Graphene Nanoribbons</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, Li; Park, Cheol-Hwan; Son, Young-Woo; Cohen, Marvin L.; Louie, Steven G.</p> <p>2007-11-01</p> <p>We present calculations of the quasiparticle <span class="hlt">energies</span> and <span class="hlt">band</span> 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 <span class="hlt">band</span> gap. Compared with previous tight-binding and density functional theory studies, our calculated quasiparticle <span class="hlt">band</span> gaps show significant self-<span class="hlt">energy</span> 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 <span class="hlt">band</span> gaps found here suggest that use of GNRs for electronic device components in ambient conditions may be viable.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/203878','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/biblio/203878"><span>Wide <span class="hlt">band</span> stepped frequency <span class="hlt">ground</span> penetrating radar</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Bashforth, M.B.; Gardner, D.; Patrick, D.; Lewallen, T.A.; Nammath, S.R.; Painter, K.D.; Vadnais, K.G.</p> <p>1996-03-12</p> <p>A wide <span class="hlt">band</span> <span class="hlt">ground</span> penetrating radar system is described embodying a method wherein a series of radio frequency signals is produced by a single radio frequency source and provided to a transmit antenna for transmission to a target and reflection therefrom to a receive antenna. A phase modulator modulates those portions of the radio frequency signals to be transmitted and the reflected modulated signal is combined in a mixer with the original radio frequency signal to produce a resultant signal which is demodulated to produce a series of direct current voltage signals, the envelope of which forms a cosine wave shaped plot which is processed by a Fast Fourier Transform Unit 44 into frequency domain data wherein the position of a preponderant frequency is indicative of distance to the target and magnitude is indicative of the signature of the target. 6 figs.</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://hdl.handle.net/2060/20150000886','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150000886"><span>Multi-<span class="hlt">Band</span> (K- Q- and E-<span class="hlt">Band</span>) Multi-Tone Millimeter-Wave Frequency Synthesizer for Radio Wave Propagation Studies</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Simons, Rainee N.; Wintucky, Edwin G.</p> <p>2014-01-01</p> <p>This paper presents the design and test results of a multi-<span class="hlt">band</span> multi-tone millimeter-wave frequency synthesizer, based on a solid-<span class="hlt">state</span> frequency comb generator. The intended application of the synthesizer is in a space-borne transmitter for radio wave atmospheric studies at K-<span class="hlt">band</span> (18 to 26.5 GHz), Q-<span class="hlt">band</span> (37 to 42 GHz), and E-<span class="hlt">band</span> (71 to 76 GHz). These studies would enable the design of robust multi-Gbps data rate space-to-<span class="hlt">ground</span> satellite communication links. Lastly, the architecture for a compact multi-tone beacon transmitter, which includes a high frequency synthesizer, a polarizer, and a conical horn antenna, has been investigated for a notional CubeSat based space-to-<span class="hlt">ground</span> radio wave propagation experiment.</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 <span class="hlt">state</span> associated with the coexistence of line and point nodes.</p> </li> <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 electron 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-electron <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 <span class="hlt">ground</span> <span class="hlt">state</span> 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('http://adsabs.harvard.edu/abs/2017EPJWC.14612031M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EPJWC.14612031M"><span>Optical model with multiple <span class="hlt">band</span> couplings using soft rotator structure</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Martyanov, Dmitry; Soukhovitskii, Efrem; Capote, Roberto; Quesada, Jose Manuel; Chiba, Satoshi</p> <p>2017-09-01</p> <p>A new dispersive coupled-channel optical model (DCCOM) is derived that describes nucleon scattering on 238U and 232Th targets using a soft-rotator-model (SRM) description of the collective levels of the target nucleus. SRM Hamiltonian parameters are adjusted to the observed collective levels of the target nucleus. SRM nuclear wave functions (mixed in K quantum number) have been used to calculate coupling matrix elements of the generalized optical model. Five rotational <span class="hlt">bands</span> are coupled: the <span class="hlt">ground-state</span> <span class="hlt">band</span>, β-, γ-, non-axial- <span class="hlt">bands</span>, and a negative parity <span class="hlt">band</span>. Such coupling scheme includes almost all levels below 1.2 MeV of excitation <span class="hlt">energy</span> of targets. The "effective" deformations that define inter-<span class="hlt">band</span> couplings are derived from SRM Hamiltonian parameters. Conservation of nuclear volume is enforced by introducing a monopolar deformed potential leading to additional couplings between rotational <span class="hlt">bands</span>. The present DCCOM describes the total cross section differences between 238U and 232Th targets within experimental uncertainty from 50 keV up to 200 MeV of neutron incident <span class="hlt">energy</span>. SRM couplings and volume conservation allow a precise calculation of the compound-nucleus (CN) formation cross sections, which is significantly different from the one calculated with rigid-rotor potentials with any number of coupled levels.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1391649-mixed-configuration-ground-state-iron-ii-phthalocyanine','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1391649-mixed-configuration-ground-state-iron-ii-phthalocyanine"><span>Mixed configuration <span class="hlt">ground</span> <span class="hlt">state</span> in iron(II) phthalocyanine</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>Fernández-Rodríguez, Javier; Toby, Brian; van Veenendaal, Michel</p> <p>2015-06-01</p> <p>We calculate the angular dependence of the x-ray linear and circular dichroism at the L2,3 edges of α-Fe(II) Phthalocyanine (FePc) thin films using a ligand-field model with full configuration interaction. We find the best agreement with the experimental spectra for a mixed <span class="hlt">ground</span> <span class="hlt">state</span> of 3E (a2 e3b1 ) and 3B (a1 e4b1 ) g 1g g 2g 2g 1g g 2g with the two configurations coupled by the spin-orbit interaction. The 3Eg(b) and 3B2g <span class="hlt">states</span> have easy-axis and easy-plane anisotropies, respectively. Our model accounts for an easy-plane magnetic anisotropy and the measured magnitudes of the in-plane orbital and spinmore » moments. The proximity in <span class="hlt">energy</span> of the two configurations allows a switching of the magnetic anisotropy from easy plane to easy axis with a small change in the crystal field, as recently observed for FePc adsorbed on an oxidized Cu surface. We also discuss the possibility of a quintet <span class="hlt">ground</span> <span class="hlt">state</span> (5A1g is 250 meV above the <span class="hlt">ground</span> <span class="hlt">state</span>) with planar anisotropy by manipulation of the Fe-C bond length by depositing the complex on a substrate that is subjected to a mechanical strain.« less</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 electronics, 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 <span class="hlt">States</span> 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('https://www.ncbi.nlm.nih.gov/pubmed/26301835','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26301835"><span>A Computational Study on the <span class="hlt">Ground</span> and Excited <span class="hlt">States</span> of Nickel Silicide.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Schoendorff, George; Morris, Alexis R; Hu, Emily D; Wilson, Angela K</p> <p>2015-09-17</p> <p>Nickel silicide has been studied with a range of computational methods to determine the nature of the Ni-Si bond. Additionally, the physical effects that need to be addressed within calculations to predict the equilibrium bond length and bond dissociation <span class="hlt">energy</span> within experimental error have been determined. The <span class="hlt">ground</span> <span class="hlt">state</span> is predicted to be a (1)Σ(+) <span class="hlt">state</span> with a bond order of 2.41 corresponding to a triple bond with weak π bonds. It is shown that calculation of the <span class="hlt">ground</span> <span class="hlt">state</span> equilibrium geometry requires a polarized basis set and treatment of dynamic correlation including up to triple excitations with CR-CCSD(T)L resulting in an equilibrium bond length of only 0.012 Å shorter than the experimental bond length. Previous calculations of the bond dissociation <span class="hlt">energy</span> resulted in <span class="hlt">energies</span> that were only 34.8% to 76.5% of the experimental bond dissociation <span class="hlt">energy</span>. It is shown here that use of polarized basis sets, treatment of triple excitations, correlation of the valence and subvalence electrons, and a Λ coupled cluster approach is required to obtain a bond dissociation <span class="hlt">energy</span> that deviates as little as 1% from experiment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1457350-emergent-low-energy-bound-states-two-orbital-hubbard-model','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1457350-emergent-low-energy-bound-states-two-orbital-hubbard-model"><span>Emergent low-<span class="hlt">energy</span> bound <span class="hlt">states</span> in the two-orbital Hubbard model</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Nunez-Fernandez, Y.; Kotliar, G.; Hallberg, K.</p> <p>2018-03-30</p> <p>A repulsive Coulomb interaction between electrons in different orbitals in correlated materials can give rise to bound quasiparticle <span class="hlt">states</span>. We study the nonhybridized two-orbital Hubbard model with intra- (inter)orbital interaction U (U 12) and different bandwidths using an improved dynamical mean-field theory numerical technique which leads to reliable spectra on the real <span class="hlt">energy</span> axis directly at zero temperature. We find that a finite density of <span class="hlt">states</span> at the Fermi <span class="hlt">energy</span> in one <span class="hlt">band</span> is correlated with the emergence of well-defined quasiparticle <span class="hlt">states</span> at excited <span class="hlt">energies</span> Δ = U - U 12 in the other <span class="hlt">band</span>. These excitations are interband holon-doublonmore » bound <span class="hlt">states</span>. At the symmetric point U = U 12, the quasiparticle peaks are located at the Fermi <span class="hlt">energy</span>, leading to a simultaneous and continuous Mott transition settling a long-standing controversy.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22255164-zethrene-biradicals-how-pro-aromaticity-expressed-ground-electronic-state-lowest-energy-singlet-triplet-ionic-states','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22255164-zethrene-biradicals-how-pro-aromaticity-expressed-ground-electronic-state-lowest-energy-singlet-triplet-ionic-states"><span>Zethrene biradicals: How pro-aromaticity is expressed in the <span class="hlt">ground</span> electronic <span class="hlt">state</span> and in the lowest <span class="hlt">energy</span> singlet, triplet, and ionic <span class="hlt">states</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>Zafra, José Luis; González Cano, Rafael C.; Ruiz Delgado, M. Carmen</p> <p></p> <p>A analysis of the electronic and molecular structures of new molecular materials based on zethrene is presented with particular attention to those systems having a central benzo-quinoidal core able to generate Kekulé biradicals whose stability is provided by the aromaticity recovery in this central unit. These Kekulé biradicals display singlet <span class="hlt">ground</span> electronic <span class="hlt">states</span> thanks to double spin polarization and have low-<span class="hlt">energy</span> lying triplet excited <span class="hlt">states</span> also featured by the aromaticity gain. Pro-aromatization is also the driving force for the stabilization of the ionized species. Moreover, the low <span class="hlt">energy</span> lying singlet excited <span class="hlt">states</span> also display a profound biradical fingerprint allowing tomore » singlet exciton fission. These properties are discussed in the context of the size of the zethrene core and of its substitution. The work encompasses all known long zethrenes and makes use of a variety of experimental techniques, such as Raman, UV-Vis-NIR absorption, transient absorption, in situ spectroelectrochemistry and quantum chemical calculations. This study reveals how the insertion of suitable molecular modules (i.e., quinoidal) opens the door to new intriguing molecular properties exploitable in organic electronics.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19850062559&hterms=poor+performances&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dpoor%2Bperformances','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19850062559&hterms=poor+performances&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dpoor%2Bperformances"><span>Performance of a normalized <span class="hlt">energy</span> metric without jammer <span class="hlt">state</span> information for an FH/MFSK system in worst case partial <span class="hlt">band</span> jamming</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lee, P. J.</p> <p>1985-01-01</p> <p>For a frequency-hopped noncoherent MFSK communication system without jammer <span class="hlt">state</span> information (JSI) in a worst case partial <span class="hlt">band</span> jamming environment, it is well known that the use of a conventional unquantized metric results in very poor performance. In this paper, a 'normalized' unquantized <span class="hlt">energy</span> metric is suggested for such a system. It is shown that with this metric, one can save 2-3 dB in required signal <span class="hlt">energy</span> over the system with hard decision metric without JSI for the same desired performance. When this very robust metric is compared to the conventional unquantized <span class="hlt">energy</span> metric with JSI, the loss in required signal <span class="hlt">energy</span> is shown to be small. Thus, the use of this normalized metric provides performance comparable to systems for which JSI is known. Cutoff rate and bit error rate with dual-k coding are used for the performance measures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JKPS...69...56S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JKPS...69...56S"><span>Effects of temperature on the <span class="hlt">ground</span> <span class="hlt">state</span> of a strongly-coupling magnetic polaron and mean phonon number in RbCl quantum pseudodot</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sun, Yong; Ding, Zhao-Hua; Xiao, Jing-Lin</p> <p>2016-07-01</p> <p>On the condition of strong electron-LO phonon coupling in a RbCl quantum pseudodot (QPD), the <span class="hlt">ground</span> <span class="hlt">state</span> <span class="hlt">energy</span> and the mean number of phonons are calculated by using the Pekar variational method and quantum statistical theory. The variations of the <span class="hlt">ground</span> <span class="hlt">state</span> <span class="hlt">energy</span> and the mean number with respect to the temperature and the cyclotron frequency of the magnetic field are studied in detail. We find that the absolute value of the <span class="hlt">ground</span> <span class="hlt">state</span> <span class="hlt">energy</span> increases (decreases) with increasing temperature when the temperature is in the lower (higher) temperature region, and that the mean number increases with increasing temperature. The absolute value of the <span class="hlt">ground</span> <span class="hlt">state</span> <span class="hlt">energy</span> is a decreasing function of the cyclotron frequency of the magnetic field whereas the mean number is an increasing function of it. We find two ways to tune the <span class="hlt">ground</span> <span class="hlt">state</span> <span class="hlt">energy</span> and the mean number: controlling the temperature and controlling the cyclotron frequency of the magnetic field.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/21199548-identification-yrast-high-intrinsic-states-sup-os','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/21199548-identification-yrast-high-intrinsic-states-sup-os"><span>Identification of yrast high-K intrinsic <span class="hlt">states</span> in {sup 188}Os</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>Modamio, V.; Jungclaus, A.; Instituto de Estructura de la Materia, CSIC, Serrano 113bis, E-28006 Madrid</p> <p>2009-02-15</p> <p>The high-spin structure of the Z=76 nucleus {sup 188}Os has been studied using the incomplete fusion reaction {sup 7}Li+{sup 186}W. A K{sup {pi}}=10{sup +} <span class="hlt">band</span> has been established up to spin (24{sup +}) and its crossing with the <span class="hlt">ground-state</span> <span class="hlt">band</span> has been studied. In addition, intrinsic high-K <span class="hlt">states</span> have been identified and on top of two of them, K{sup {pi}}=7{sup -} and K{sup {pi}}=10{sup -}, regular <span class="hlt">bands</span> have been observed. The K{sup {pi}}=16{sup +} and K{sup {pi}}=18{sup +} <span class="hlt">states</span> are yrast whereas the K{sup {pi}}=14{sup +} level lies only 33 keV above the yrast line and decays with a lowmore » reduced hindrance of f{sub {nu}}<1.3 to the <span class="hlt">ground-state</span> <span class="hlt">band</span> ({delta}K=14). The results are discussed by means of a systematic comparison with the even-even neighboring nucleus {sup 186}Os. Configuration-constrained multiquasiparticle potential-<span class="hlt">energy</span>-surface calculations have been performed to identify the configurations of multiquasiparticle <span class="hlt">states</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1194163-rayleigh-approximation-ground-state-bose-coulomb-glasses','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1194163-rayleigh-approximation-ground-state-bose-coulomb-glasses"><span>Rayleigh approximation to <span class="hlt">ground</span> <span class="hlt">state</span> of the Bose and Coulomb glasses</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Ryan, S. D.; Mityushev, V.; Vinokur, V. M.; ...</p> <p>2015-01-16</p> <p>Glasses are rigid systems in which competing interactions prevent simultaneous minimization of local <span class="hlt">energies</span>. This leads to frustration and highly degenerate <span class="hlt">ground</span> <span class="hlt">states</span> the nature and properties of which are still far from being thoroughly understood. We report an analytical approach based on the method of functional equations that allows us to construct the Rayleigh approximation to the <span class="hlt">ground</span> <span class="hlt">state</span> of a two-dimensional (2D) random Coulomb system with logarithmic interactions. We realize a model for 2D Coulomb glass as a cylindrical type II superconductor containing randomly located columnar defects (CD) which trap superconducting vortices induced by applied magnetic field. Ourmore » findings break <span class="hlt">ground</span> for analytical studies of glassy systems, marking an important step towards understanding their properties.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4296301','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4296301"><span>Rayleigh approximation to <span class="hlt">ground</span> <span class="hlt">state</span> of the Bose and Coulomb glasses</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ryan, S. D.; Mityushev, V.; Vinokur, V. M.; Berlyand, L.</p> <p>2015-01-01</p> <p>Glasses are rigid systems in which competing interactions prevent simultaneous minimization of local <span class="hlt">energies</span>. This leads to frustration and highly degenerate <span class="hlt">ground</span> <span class="hlt">states</span> the nature and properties of which are still far from being thoroughly understood. We report an analytical approach based on the method of functional equations that allows us to construct the Rayleigh approximation to the <span class="hlt">ground</span> <span class="hlt">state</span> of a two-dimensional (2D) random Coulomb system with logarithmic interactions. We realize a model for 2D Coulomb glass as a cylindrical type II superconductor containing randomly located columnar defects (CD) which trap superconducting vortices induced by applied magnetic field. Our findings break <span class="hlt">ground</span> for analytical studies of glassy systems, marking an important step towards understanding their properties. PMID:25592417</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1998CoTPh..30..491M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998CoTPh..30..491M"><span>The g Factors of <span class="hlt">Ground</span> <span class="hlt">State</span> of Ruby and Their Pressure-Induced Shifts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ma, Dongping; Zhang, Hongmei; Chen, Jurong; Liu, Yanyun</p> <p>1998-12-01</p> <p>By using the theory of pressure-induced shifts and the eigenfunctions at normal and various pressures obtained from the diagonalization of the complete d3 <span class="hlt">energy</span> matrix adopting C3v symmetry, g factors of the <span class="hlt">ground</span> <span class="hlt">state</span> of ruby and their pressure-induced shifts have been calculated. The results are in very good agreement with the experimental data. For the precise calculation of properties of the <span class="hlt">ground</span> skate, it is necessary to take into account the effects of all the excited <span class="hlt">states</span> by the diagonalization of the complete <span class="hlt">energy</span> matrix. The project (Grant No. 19744001) supported by National Natural Science Foundation of China</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26871327','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26871327"><span>Electron Elevator: Excitations across the <span class="hlt">Band</span> Gap via a Dynamical Gap <span class="hlt">State</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lim, A; Foulkes, W M C; Horsfield, A P; Mason, D R; Schleife, A; Draeger, E W; Correa, A A</p> <p>2016-01-29</p> <p>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 <span class="hlt">energy</span> transferred to the electrons per unit path length by an ion of kinetic <span class="hlt">energy</span> 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 <span class="hlt">band</span> 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 <span class="hlt">state</span> induced in the gap by the moving ion acts like an elevator and carries electrons across the <span class="hlt">band</span> gap.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JMoSp.315...63L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JMoSp.315...63L"><span>Fourier transform synchrotron spectroscopy of the in-plane methyl-rocking <span class="hlt">band</span> of CD3OH</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lees, R. M.; Xu, Li-Hong; Gao, Song; Billinghurst, B. E.</p> <p>2015-09-01</p> <p>Infrared Fourier transform spectra of the 12CD3OH isotopologue of methanol recorded at the Canadian Light Source synchrotron have been investigated in the 750-950 cm-1 region to explore the torsional <span class="hlt">energy</span> pattern of the in-plane methyl-rocking mode. The in-plane CD3-rocking <span class="hlt">band</span> is primarily of parallel a-type character with relatively widely spaced K-structure, and the central Q-branch region is well-resolved. Sub-<span class="hlt">bands</span> have been assigned for the vt = 0 <span class="hlt">ground</span> torsional <span class="hlt">state</span> from K = 0 to 15 for both A and E torsional species, as well as a number of sub-<span class="hlt">bands</span> in the vt = 1 excited torsional <span class="hlt">state</span>. A variety of perturbations due to asymmetry-induced, anharmonic Fermi and level-crossing resonances is seen in the spectra. Mapping of K-reduced torsional <span class="hlt">energies</span> determined from the upper-<span class="hlt">state</span> term values shows that the K-dependence is severely distorted from the usual pattern of smoothly oscillating, near-sinusoidal interlocking τ-curves. Although the K = 0 levels are nominally inverted for vt = 0, the torsional splitting is very small with the A level higher than the E level by only 0.625 cm-1, and the anomalous behavior precludes a definite conclusion about torsional inversion. However, the range of variation with K of the vt = 0 CD3-rocking τ-curves is about half that of the <span class="hlt">ground</span> vibrational <span class="hlt">state</span>, similar to previous observations for CH3OH isotopologues, suggesting a comparable reduction of about 25% in the effective torsional barrier height for the in-plane rocking mode.</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 electrons 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 <span class="hlt">ground</span> <span class="hlt">state</span> of an exciton formed from an electron and a hole spatially separated from each other (the hole is moving within a quantum dot, and the electron 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 <span class="hlt">states</span> (formed from spatiallymore » separated electrons and holes) appears. It is shown that there exists the possibility of experimentally detecting the <span class="hlt">ground</span> and excited exciton <span class="hlt">states</span> 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/2016EPJC...76...64B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EPJC...76...64B"><span>Traces of Lorentz symmetry breaking in a hydrogen atom at <span class="hlt">ground</span> <span class="hlt">state</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Borges, L. H. C.; Barone, F. A.</p> <p>2016-02-01</p> <p>Some traces of a specific Lorentz symmetry breaking scenario in the <span class="hlt">ground</span> <span class="hlt">state</span> of the hydrogen atom are investigated. We use standard Rayleigh-Schrödinger perturbation theory in order to obtain the corrections to the <span class="hlt">ground</span> <span class="hlt">state</span> <span class="hlt">energy</span> and the wave function. It is shown that an induced four-pole moment arises, due to the Lorentz symmetry breaking. The model considered is the one studied in Borges et al. (Eur Phys J C 74:2937, 2014), where the Lorentz symmetry is broken in the electromagnetic sector.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JMoSp.340...29N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JMoSp.340...29N"><span>The ν8 <span class="hlt">band</span> of C2HD3 by high-resolution synchrotron FTIR spectroscopy: Coriolis interactions between the v8 = 1 and v6 = 1 <span class="hlt">states</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ng, L. L.; Tan, T. L.; Akasyah, Luqman; Wong, Andy; Appadoo, Dominique R. T.; McNaughton, Don</p> <p>2017-10-01</p> <p>The synchrotron Fourier transform infrared (FTIR) spectrum of the ν8 <span class="hlt">band</span> of ethylene-d3 (C2HD3) was measured at an unapodized resolution of 0.00096 cm-1 from 830 to 1010 cm-1. Rovibrational constants up to five quartic terms were derived with improved precision for the v8 = 1 <span class="hlt">state</span> through the fitting of 1566 unperturbed infrared transitions using the Watson's A-reduced Hamiltonian in the Ir representation with a root-mean-square (rms) deviation of 0.00044 cm-1. For the first time, 446 perturbed IR transitions of the ν8 <span class="hlt">band</span> were fitted together with the 1566 unperturbed infrared transitions to obtain the a- and b-Coriolis resonance parameters from its interaction with the v6 = 1 <span class="hlt">state</span>, with an rms deviation of 0.00039 cm-1. The IR lines of the ν6 <span class="hlt">band</span> were too weak for detection. Three rotational constants, a quartic constant and <span class="hlt">band</span> center of the v6 = 1 <span class="hlt">state</span> were also derived for the first time in this work. <span class="hlt">Ground</span> <span class="hlt">state</span> rovibrational constants of C2HD3 up to five quartic constants were also derived from a fit of 906 <span class="hlt">ground</span> <span class="hlt">state</span> combination differences with an rms deviation of 0.00030 cm-1 from infrared transitions of the present analysis. The <span class="hlt">ground</span> <span class="hlt">state</span> rotational constants are in close agreement with theoretically calculated values using the cc-pVTZ basis set at CCSD(T), MP2 and B3LYP levels of theory. Alpha constants determined from the rotational constants of the v8 = 1 <span class="hlt">state</span> derived from the perturbed IR fit compared favourably with those from anharmonic calculations.</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('http://adsabs.harvard.edu/abs/1996CPL...262..807B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1996CPL...262..807B"><span>Predictions of <span class="hlt">ground</span> <span class="hlt">states</span> of LiGa and NaGa</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Boldyrev, Alexander I.; Simons, Jack</p> <p>1996-11-01</p> <p>The <span class="hlt">ground</span> and very low-lying excited <span class="hlt">states</span> of LiGa and NaGa have been studied using high level ab initio techniques. At the QCISD(T)/6-311 + G(2df) level of theory, the 1Σ + <span class="hlt">state</span> was found to be the most stable for both molecules. The equilibrium bond lengths and dissociation <span class="hlt">energies</span> were found to be: R( LiGa) = 2.865 Å and D0(LiGa) = 22.3 kcal/mol and R( NaGa) = 3.174 Å and D0(NaGa) = 17.1 kcal/mol. Trends within the <span class="hlt">ground</span> electronic <span class="hlt">states</span> of LiB, NaB, LiAl, NaAl, LiGa and NaGa are discussed and predictions for related AlkM (Alk LiCs and MBTl) species are made.</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://hdl.handle.net/2060/19890007088','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19890007088"><span><span class="hlt">Ground</span> <span class="hlt">state</span> of high-density matter</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Copeland, ED; Kolb, Edward W.; Lee, Kimyeong</p> <p>1988-01-01</p> <p>It is shown that if an upper bound to the false vacuum <span class="hlt">energy</span> of the electroweak Higgs potential is satisfied, the true <span class="hlt">ground</span> <span class="hlt">state</span> of high-density matter is not nuclear matter, or even strange-quark matter, but rather a non-topological soliton where the electroweak symmetry is exact and the fermions are massless. This possibility is examined in the standard SU(3) sub C tensor product SU(2) sub L tensor product U(1) sub Y model. The bound to the false vacuum <span class="hlt">energy</span> is satisfied only for a narrow range of the Higgs boson masses in the minimal electroweak model (within about 10 eV of its minimum allowed value of 6.6 GeV) and a somewhat wider range for electroweak models with a non-minimal Higgs sector.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26567645','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26567645"><span><span class="hlt">Ground-state</span> densities from the Rayleigh-Ritz variation principle and from density-functional theory.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kvaal, Simen; Helgaker, Trygve</p> <p>2015-11-14</p> <p>The relationship between the densities of <span class="hlt">ground-state</span> wave functions (i.e., the minimizers of the Rayleigh-Ritz variation principle) and the <span class="hlt">ground-state</span> densities in density-functional theory (i.e., the minimizers of the Hohenberg-Kohn variation principle) is studied within the framework of convex conjugation, in a generic setting covering molecular systems, solid-<span class="hlt">state</span> systems, and more. Having introduced admissible density functionals as functionals that produce the exact <span class="hlt">ground-state</span> <span class="hlt">energy</span> for a given external potential by minimizing over densities in the Hohenberg-Kohn variation principle, necessary and sufficient conditions on such functionals are established to ensure that the Rayleigh-Ritz <span class="hlt">ground-state</span> densities and the Hohenberg-Kohn <span class="hlt">ground-state</span> densities are identical. We apply the results to molecular systems in the Born-Oppenheimer approximation. For any given potential v ∈ L(3/2)(ℝ(3)) + L(∞)(ℝ(3)), we establish a one-to-one correspondence between the mixed <span class="hlt">ground-state</span> densities of the Rayleigh-Ritz variation principle and the mixed <span class="hlt">ground-state</span> densities of the Hohenberg-Kohn variation principle when the Lieb density-matrix constrained-search universal density functional is taken as the admissible functional. A similar one-to-one correspondence is established between the pure <span class="hlt">ground-state</span> densities of the Rayleigh-Ritz variation principle and the pure <span class="hlt">ground-state</span> densities obtained using the Hohenberg-Kohn variation principle with the Levy-Lieb pure-<span class="hlt">state</span> constrained-search functional. In other words, all physical <span class="hlt">ground-state</span> densities (pure or mixed) are recovered with these functionals and no false densities (i.e., minimizing densities that are not physical) exist. The importance of topology (i.e., choice of Banach space of densities and potentials) is emphasized and illustrated. The relevance of these results for current-density-functional theory is examined.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JAP...122m5702S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JAP...122m5702S"><span>The effect of density-of-<span class="hlt">state</span> tails on <span class="hlt">band-to-band</span> tunneling: Theory and application to tunnel 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>Sant, S.; Schenk, A.</p> <p>2017-10-01</p> <p>It is demonstrated how <span class="hlt">band</span> tail <span class="hlt">states</span> in the semiconductor influence the performance of a Tunnel Field Effect Transistor (TFET). As a consequence of the smoothened density of <span class="hlt">states</span> (DOS) around the <span class="hlt">band</span> edges, the energetic overlap of conduction and valence <span class="hlt">band</span> <span class="hlt">states</span> occurs gradually at the onset of <span class="hlt">band-to-band</span> tunneling (BTBT), thus degrading the sub-threshold swing (SS) of the TFET. The effect of the <span class="hlt">band</span> tail <span class="hlt">states</span> on the current-voltage characteristics is modelled quantum-mechanically based on the idea of zero-phonon trap-assisted tunneling between <span class="hlt">band</span> and tail <span class="hlt">states</span>. The latter are assumed to arise from a 3-dimensional pseudo-delta potential proposed by Vinogradov [1]. This model potential allows the derivation of analytical expressions for the generation rate covering the whole range from very strong to very weak localization of the tail <span class="hlt">states</span>. Comparison with direct BTBT in the one-<span class="hlt">band</span> effective mass approximation reveals the essential features of tail-to-<span class="hlt">band</span> tunneling. Furthermore, an analytical solution for the problem of tunneling from continuum <span class="hlt">states</span> of the disturbed DOS to <span class="hlt">states</span> in the opposite <span class="hlt">band</span> is found, and the differences to direct BTBT are worked out. Based on the analytical expressions, a semi-classical model is implemented in a commercial device simulator which involves numerical integration along the tunnel paths. The impact of the tail <span class="hlt">states</span> on the device performance is analyzed for a nanowire Gate-All-Around TFET. The simulations show that tail <span class="hlt">states</span> notably impact the transfer characteristics of a TFET. It is found that exponentially decaying <span class="hlt">band</span> tails result in a stronger degradation of the SS than tail <span class="hlt">states</span> with a Gaussian decay of their density. The developed model allows more realistic simulations of TFETs including their non-idealities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ChPhC..41a4102S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ChPhC..41a4102S"><span>Systematic study of α preformation probability of nuclear isomeric and <span class="hlt">ground</span> <span class="hlt">states</span></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-Dong; Wu, Xi-Jun; Zheng, Bo; Xiang, Dong; Guo, Ping; Li, Xiao-Hua</p> <p>2017-01-01</p> <p>In this paper, based on the two-potential approach combining with the isospin dependent nuclear potential, we systematically compare the α preformation probabilities of odd-A nuclei between nuclear isomeric <span class="hlt">states</span> and <span class="hlt">ground</span> <span class="hlt">states</span>. The results indicate that during the process of α particle preforming, the low lying nuclear isomeric <span class="hlt">states</span> are similar to <span class="hlt">ground</span> <span class="hlt">states</span>. Meanwhile, in the framework of single nucleon <span class="hlt">energy</span> level structure, we find that for nuclei with nucleon number below the magic numbers, the α preformation probabilities of high-spin <span class="hlt">states</span> seem to be larger than low ones. For nuclei with nucleon number above the magic numbers, the α preformation probabilities of isomeric <span class="hlt">states</span> are larger than those of <span class="hlt">ground</span> <span class="hlt">states</span>. Supported by National Natural Science Foundation of China (11205083), Construct Program of Key Discipline in Hunan Province, Research Foundation of Education Bureau of Hunan Province, China (15A159), Natural Science Foundation of Hunan Province, China (2015JJ3103, 2015JJ2123), Innovation Group of Nuclear and Particle Physics in USC, Hunan Provincial Innovation Foundation for Postgraduate (CX2015B398)</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 electronics, 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 <span class="hlt">States</span> 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('https://www.osti.gov/servlets/purl/870338','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/870338"><span>Wide <span class="hlt">band</span> stepped frequency <span class="hlt">ground</span> penetrating radar</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Bashforth, Michael B.; Gardner, Duane; Patrick, Douglas; Lewallen, Tricia A.; Nammath, Sharyn R.; Painter, Kelly D.; Vadnais, Kenneth G.</p> <p>1996-01-01</p> <p>A wide <span class="hlt">band</span> <span class="hlt">ground</span> penetrating radar system (10) embodying a method wherein a series of radio frequency signals (60) is produced by a single radio frequency source (16) and provided to a transmit antenna (26) for transmission to a target (54) and reflection therefrom to a receive antenna (28). A phase modulator (18) modulates those portion of the radio frequency signals (62) to be transmitted and the reflected modulated signal (62) is combined in a mixer (34) with the original radio frequency signal (60) to produce a resultant signal (53) which is demodulated to produce a series of direct current voltage signals (66) the envelope of which forms a cosine wave shaped plot (68) which is processed by a Fast Fourier Transform unit 44 into frequency domain data (70) wherein the position of a preponderant frequency is indicative of distance to the target (54) and magnitude is indicative of the signature of the target (54).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PhRvB..93r4415K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhRvB..93r4415K"><span><span class="hlt">Ground</span> <span class="hlt">state</span> of Ho atoms on Pt(111) metal surfaces: Implications for magnetism</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Karbowiak, M.; Rudowicz, C.</p> <p>2016-05-01</p> <p>We investigated the <span class="hlt">ground</span> <span class="hlt">state</span> of Ho atoms adsorbed on the Pt(111) surface, for which conflicting results exist. The density functional theory (DFT) calculations yielded the Ho <span class="hlt">ground</span> <span class="hlt">state</span> as | Jz=±8 > . Interpretation of x-ray absorption spectroscopy and x-ray magnetic circular dichroism spectra and the magnetization curves indicated the <span class="hlt">ground</span> <span class="hlt">state</span> as | Jz=±6 > . Superposition model is employed to predict the crystal-field (CF) parameters based on the structural data for the system Ho/Pt(111) obtained from the DFT modeling. Simultaneous diagonalization of the free-ion (HFI) and the trigonal CF Hamiltonian (HCF) within the whole configuration 4 f10 of H o3 + ion was performed. The role of the trigonal CF terms, neglected in the pure uniaxial CF model used previously for interpretation of experimental spectra, is found significant, whereas the sixth-rank CF terms may be neglected in agreement with the DFT predictions. The results provide substantial support for the experimental designation of the | Jz=±6 > <span class="hlt">ground</span> <span class="hlt">state</span>, albeit with subtle difference due to admixture of other | Jz> <span class="hlt">states</span>, but run against the DFT-based designation of the | Jz=±8 > <span class="hlt">ground</span> <span class="hlt">state</span>. A subtle splitting of the <span class="hlt">ground</span> <span class="hlt">energy</span> level with the <span class="hlt">state</span> (predominantly), | Jz=±6 > is predicted. This paper provides better insight into the single-ion magnetic behavior of the Ho/Pt(111) system by helping to resolve the controversy concerning the Ho <span class="hlt">ground</span> <span class="hlt">state</span>. Experimental techniques with greater resolution powers are suggested for direct confirmation of this splitting and C3 v symmetry experienced by the Ho atom.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1351137-electron-elevator-excitations-across-band-gap-via-dynamical-gap-state','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1351137-electron-elevator-excitations-across-band-gap-via-dynamical-gap-state"><span>Electron elevator: Excitations across the <span class="hlt">band</span> gap via a dynamical gap <span class="hlt">state</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Lim, Anthony; Foulkes, W. M. C.; Horsfield, A. P.; ...</p> <p>2016-01-27</p> <p>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 <span class="hlt">energy</span> transferred to the electrons per unit path length by an ion of kinetic <span class="hlt">energy</span> 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 <span class="hlt">band</span> 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 <span class="hlt">state</span> induced in the gap by the moving ion acts like an elevator and carries electrons across the <span class="hlt">band</span> gap.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19910005500','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19910005500"><span>Surface modification using low <span class="hlt">energy</span> <span class="hlt">ground</span> <span class="hlt">state</span> ion beams</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chutjian, Ara (Inventor); Hecht, Michael H. (Inventor); Orient, Otto J. (Inventor)</p> <p>1990-01-01</p> <p>A method of effecting modifications at the surfaces of materials using low <span class="hlt">energy</span> ion beams of known quantum <span class="hlt">state</span>, purity, flux, and <span class="hlt">energy</span> is presented. The ion beam is obtained by bombarding ion-generating molecules with electrons which are also at low <span class="hlt">energy</span>. The electrons used to bombard the ion generating molecules are separated from the ions thus obtained and the ion beam is directed at the material surface to be modified. Depending on the type of ion generating molecules used, different ions can be obtained for different types of surface modifications such as oxidation and diamond film formation. One area of application is in the manufacture of semiconductor devices from semiconductor wafers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JPhB...51i5302L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JPhB...51i5302L"><span>Exact <span class="hlt">ground-state</span> correlation functions of an atomic-molecular Bose–Einstein condensate model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Links, Jon; Shen, Yibing</p> <p>2018-05-01</p> <p>We study the <span class="hlt">ground-state</span> properties of an atomic-molecular Bose–Einstein condensate model through an exact Bethe Ansatz solution. For a certain range of parameter choices, we prove that the <span class="hlt">ground-state</span> Bethe roots lie on the positive real-axis. We then use a continuum limit approach to obtain a singular integral equation characterising the distribution of these Bethe roots. Solving this equation leads to an analytic expression for the <span class="hlt">ground-state</span> <span class="hlt">energy</span>. The form of the expression is consistent with the existence of a line of quantum phase transitions, which has been identified in earlier studies. This line demarcates a molecular phase from a mixed phase. Certain correlation functions, which characterise these phases, are then obtained through the Hellmann–Feynman theorem.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EPJA...53..209M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EPJA...53..209M"><span>α-cluster <span class="hlt">states</span> in 46,54Cr from double-folding potentials</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mohr, Peter</p> <p>2017-10-01</p> <p>α-cluster <span class="hlt">states</span> in 46Cr and 54Cr are investigated in the double-folding model. This study complements a recent similar work by Souza and Miyake, Eur. Phys. J. A 53, 146 (2017), which was based on a specially shaped potential. Excitation <span class="hlt">energies</span>, reduced widths, intercluster separations, and intra-<span class="hlt">band</span> transition strengths are calculated and compared to experimental values for the <span class="hlt">ground</span> <span class="hlt">state</span> <span class="hlt">bands</span> in 46Cr and 54Cr . The α-cluster potential is also applied to elastic scattering at low and intermediate <span class="hlt">energies</span>. Here, as a byproduct, a larger radial extent of the neutron density in 50Ti is found.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/662212-ground-state-structure-random-magnets','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/662212-ground-state-structure-random-magnets"><span><span class="hlt">Ground</span> <span class="hlt">state</span> structure of random magnets</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>Bastea, S.; Duxbury, P.M.</p> <p>1998-10-01</p> <p>Using exact optimization methods, we find all of the <span class="hlt">ground</span> <span class="hlt">states</span> of ({plus_minus}h) random-field Ising magnets (RFIM) and of dilute antiferromagnets in a field (DAFF). The degenerate <span class="hlt">ground</span> <span class="hlt">states</span> are usually composed of isolated clusters (two-level systems) embedded in a frozen background. We calculate the paramagnetic response (sublattice response) and the <span class="hlt">ground</span> <span class="hlt">state</span> entropy for the RFIM (DAFF) due to these clusters. In both two and three dimensions there is a broad regime in which these quantities are strictly positive, even at irrational values of h/J (J is the exchange constant). {copyright} {ital 1998} {ital The American Physical Society}</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/21428685-influence-ground-state-scattering-properties-photoassociation-spectra-near-intercombination-line-bosonic-ytterbium','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/21428685-influence-ground-state-scattering-properties-photoassociation-spectra-near-intercombination-line-bosonic-ytterbium"><span>Influence of <span class="hlt">ground-state</span> scattering properties on photoassociation spectra near the intercombination line of bosonic ytterbium</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>Borkowski, M.; Ciurylo, R.; Julienne, P. S.</p> <p>2010-10-29</p> <p>We study theoretically the properties of photoassociation spectra near the {sup 1}S{sub 0}-{sup 3}P{sub 1} inter-combination line of bosonic ytterbium. We construct a mass scaled model of the excited <span class="hlt">state</span> interaction potential that well describes bound <span class="hlt">state</span> <span class="hlt">energies</span> obtained in a previous photoassociation experiment. We then use it to calculate theoretical photoassociation spectra in a range of ultracold temperatures using semianalytical theory developed by Bohn and Julienne.Photoassociation spectra not only give us the <span class="hlt">energies</span> of excited bound <span class="hlt">states</span>, but also provide information about the behavior of the <span class="hlt">ground</span> <span class="hlt">state</span> wavefunction. In fact, it can be shown that within the so-calledmore » reflection approximation the line intensity is proportional to the <span class="hlt">ground</span> <span class="hlt">state</span> wavefunction at the transition's Condon point. We show that in the case of ytterbium, the rotational structure of the photoassociation spectra depends heavily on the behavior of the <span class="hlt">ground-state</span> wavefunction. The change of the scattering length from one isotope to another and the resulting occurence of shape resonances in higher partial waves determines the appearance and disapperance of rotational components, especially in the deeper lying <span class="hlt">states</span>, whose respective Condon points lie near the <span class="hlt">ground</span> <span class="hlt">state</span> centrifugal barrier. Thus, photoassociation spectra differ qualitatively between isotopes.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006JAP...100i3511E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006JAP...100i3511E"><span>Optical <span class="hlt">band</span> gap studies on lithium aluminum silicate glasses doped with Cr3+ ions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>El-Diasty, Fouad; Abdel Wahab, Fathy A.; Abdel-Baki, Manal</p> <p>2006-11-01</p> <p>Lithium aluminum silicate glass system (LAS) implanted with chromium ions is prepared. The reflectance and transmittance measurements are used to determine the dispersion of absorption coefficient. The optical data are explained in terms of the different oxidation <span class="hlt">states</span> adopted by the chromium ions into the glass network. It is found that the oxidation <span class="hlt">state</span> of the chromium depends on its concentration. Across a wide spectral range, 0.2-1.6μm, analysis of the fundamental absorption edge provides values for the average <span class="hlt">energy</span> <span class="hlt">band</span> gaps for allowed direct and indirect transitions. The optical absorption coefficient just below the absorption edge varies exponentially with photon <span class="hlt">energy</span> indicating the presence of Urbach's tail. Such tail is decreased with the increase of the chromium dopant. From the analysis of the optical absorption data, the absorption peak at <span class="hlt">ground</span> <span class="hlt">state</span> exciton <span class="hlt">energy</span>, the absorption at <span class="hlt">band</span> gap, and the free exciton binding <span class="hlt">energy</span> are determined. The extinction coefficient data are used to determine the Fermi <span class="hlt">energy</span> level of the studied glasses. The metallization criterion is obtained and discussed exploring the nature of the glasses. The measured IR spectra of the different glasses are used to throw some light on the optical properties of the present glasses correlating them with their structure and composition.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28325035','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28325035"><span>Calculation of <span class="hlt">Energy</span> Diagram of Asymmetric Graded-<span class="hlt">Band</span>-Gap Semiconductor Superlattices.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Monastyrskii, Liubomyr S; Sokolovskii, Bogdan S; Alekseichyk, Mariya P</p> <p>2017-12-01</p> <p>The paper theoretically investigates the peculiarities of <span class="hlt">energy</span> diagram of asymmetric graded-<span class="hlt">band</span>-gap superlattices with linear coordinate dependences of <span class="hlt">band</span> gap and electron affinity. For calculating the <span class="hlt">energy</span> diagram of asymmetric graded-<span class="hlt">band</span>-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 <span class="hlt">bands</span> demonstrate substantial transformation of the shape of the <span class="hlt">energy</span> diagram at changing the period of the lattice and the ratio of width of the adjacent layers. The most marked changes in the <span class="hlt">energy</span> 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 <span class="hlt">energy</span> diagram has the shape of a sawtooth-like pattern.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27722444','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27722444"><span>An ab initio potential <span class="hlt">energy</span> surface for the formic acid dimer: zero-point <span class="hlt">energy</span>, selected anharmonic fundamental <span class="hlt">energies</span>, and <span class="hlt">ground-state</span> tunneling splitting calculated in relaxed 1-4-mode subspaces.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Qu, Chen; Bowman, Joel M</p> <p>2016-09-14</p> <p>We report a full-dimensional, permutationally invariant potential <span class="hlt">energy</span> surface (PES) for the cyclic formic acid dimer. This PES is a least-squares fit to 13475 CCSD(T)-F12a/haTZ (VTZ for H and aVTZ for C and O) <span class="hlt">energies</span>. The <span class="hlt">energy</span>-weighted, root-mean-square fitting error is 11 cm -1 and the barrier for the double-proton transfer on the PES is 2848 cm -1 , in good agreement with the directly-calculated ab initio value of 2853 cm -1 . The zero-point vibrational <span class="hlt">energy</span> of 15 337 ± 7 cm -1 is obtained from diffusion Monte Carlo calculations. <span class="hlt">Energies</span> of fundamentals of fifteen modes are calculated using the vibrational self-consistent field and virtual-<span class="hlt">state</span> configuration interaction method. The <span class="hlt">ground-state</span> tunneling splitting is computed using a reduced-dimensional Hamiltonian with relaxed potentials. The highest-level, four-mode coupled calculation gives a tunneling splitting of 0.037 cm -1 , which is roughly twice the experimental value. The tunneling splittings of (DCOOH) 2 and (DCOOD) 2 from one to three mode calculations are, as expected, smaller than that for (HCOOH) 2 and consistent with experiment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008PhRvD..78c4504H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008PhRvD..78c4504H"><span>Is the <span class="hlt">ground</span> <span class="hlt">state</span> of Yang-Mills theory Coulombic?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Heinzl, T.; Ilderton, A.; Langfeld, K.; Lavelle, M.; Lutz, W.; McMullan, D.</p> <p>2008-08-01</p> <p>We study trial <span class="hlt">states</span> modelling the heavy quark-antiquark <span class="hlt">ground</span> <span class="hlt">state</span> in SU(2) Yang-Mills theory. A <span class="hlt">state</span> describing the flux tube between quarks as a thin string of glue is found to be a poor description of the continuum <span class="hlt">ground</span> <span class="hlt">state</span>; the infinitesimal thickness of the string leads to UV artifacts which suppress the overlap with the <span class="hlt">ground</span> <span class="hlt">state</span>. Contrastingly, a <span class="hlt">state</span> which surrounds the quarks with non-Abelian Coulomb fields is found to have a good overlap with the <span class="hlt">ground</span> <span class="hlt">state</span> for all charge separations. In fact, the overlap increases as the lattice regulator is removed. This opens up the possibility that the Coulomb <span class="hlt">state</span> is the true <span class="hlt">ground</span> <span class="hlt">state</span> in the continuum limit.</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('http://hdl.handle.net/2060/20140017163','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140017163"><span>Comparing On-Orbit and <span class="hlt">Ground</span> Performance for an S-<span class="hlt">Band</span> Software-Defined Radio</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chelmins, David T.; Welch, Bryan W.</p> <p>2014-01-01</p> <p>NASA's Space Communications and Navigation Testbed was installed on an external truss of the International Space Station in 2012. The testbed contains several software-defined radios (SDRs), including the Jet Propulsion Laboratory (JPL) SDR, which underwent performance testing throughout 2013 with NASAs Tracking and Data Relay Satellite System (TDRSS). On-orbit testing of the JPL SDR was conducted at S-<span class="hlt">band</span> with the Glenn Goddard TDRSS waveform and compared against an extensive dataset collected on the <span class="hlt">ground</span> prior to launch. This paper will focus on the development of a waveform power estimator on the <span class="hlt">ground</span> post-launch and discuss the performance challenges associated with operating the power estimator in space.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140017772','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140017772"><span>Comparing On-Orbit and <span class="hlt">Ground</span> Performance for an S-<span class="hlt">Band</span> Software-Defined Radio</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chelmins, David; Welch, Bryan</p> <p>2014-01-01</p> <p>NASA's Space Communications and Navigation Testbed was installed on an external truss of the International Space Station in 2012. The testbed contains several software-defined radios (SDRs), including the Jet Propulsion Laboratory (JPL) SDR, which underwent performance testing throughout 2013 with NASA's Tracking and Data Relay Satellite System (TDRSS). On-orbit testing of the JPL SDR was conducted at S-<span class="hlt">band</span> with the Glenn Goddard TDRSS waveform and compared against an extensive dataset collected on the <span class="hlt">ground</span> prior to launch. This paper will focus on the development of a waveform power estimator on the <span class="hlt">ground</span> post-launch and discuss the performance challenges associated with operating the power estimator in space.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvL.120x8001K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvL.120x8001K"><span>Universal Features of Metastable <span class="hlt">State</span> <span class="hlt">Energies</span> in Cellular Matter</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kim, Sangwoo; Wang, Yiliang; Hilgenfeldt, Sascha</p> <p>2018-06-01</p> <p>Mechanical equilibrium <span class="hlt">states</span> of cellular matter are overwhelmingly metastable and separated from each other by topology changes. Using theory and simulations, it is shown that for a wide class of <span class="hlt">energy</span> functionals in 2D, including those describing tissue cell layers, local <span class="hlt">energy</span> differences between neighboring metastable <span class="hlt">states</span> as well as global <span class="hlt">energy</span> differences between initial <span class="hlt">states</span> and <span class="hlt">ground</span> <span class="hlt">states</span> are governed by simple, universal relations. Knowledge of instantaneous length of an edge undergoing a T 1 transition is sufficient to predict local <span class="hlt">energy</span> changes, while the initial edge length distribution yields a successful prediction for the global <span class="hlt">energy</span> difference. An analytical understanding of the model parameters is provided.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70193799','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70193799"><span>Migratory connectivity of american woodcock using <span class="hlt">band</span> return data</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Moore, Joseph D.; Krementz, David G.</p> <p>2017-01-01</p> <p>American woodcock (Scolopax minor) are managed as a Central and an Eastern population in the United <span class="hlt">States</span> and Canada based on <span class="hlt">band</span> return data showing little crossover between populations or management regions. The observed proportion of crossover between management regions, however, depends on the criteria used to subset the <span class="hlt">band</span> return data. We analyzed the amount of crossover between management regions using only <span class="hlt">band</span> return records that represent complete migrations between the breeding and wintering <span class="hlt">grounds</span> by using only <span class="hlt">band</span> return records in which the capture took place during the breeding season and the <span class="hlt">band</span> recovery took place during the wintering season or vice versa (n = 224). Additionally, we applied spatial statistics and a clustering algorithm to investigate woodcock migratory connectivity using this subset of migratory woodcock <span class="hlt">band</span> return records. Using raw counts, 17.9% of records showed crossover between management regions, a higher proportion than the <5% crossover reported in studies that did not use only migratory <span class="hlt">band</span> returns. Our results showed woodcock from the breeding <span class="hlt">grounds</span> in the Central Region largely migrate to destinations within the Central Region, whereas woodcock from the breeding <span class="hlt">grounds</span> in the Eastern Region migrate to destinations across the entire wintering range and mix with individuals from the Central Region. Using the division coefficient, we estimated that 54% of woodcock from the breeding <span class="hlt">grounds</span> of the Eastern Region migrate to the Central Region wintering <span class="hlt">grounds</span>. Our result that many woodcock from separate regions of the breeding <span class="hlt">grounds</span> mix on the wintering <span class="hlt">grounds</span> has implications for the 2-region basis for woodcock management. Elucidating finer scale movement patterns among regions provides a basis for reassessing the need for separate management regions to ensure optimal conservation and management of the species.</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.osti.gov/pages/biblio/1183876-observation-vibrations-alignments-built-non-ground-state-configurations-dy','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1183876-observation-vibrations-alignments-built-non-ground-state-configurations-dy"><span>Observation of γ-vibrations and alignments built on non-<span class="hlt">ground-state</span> configurations in ¹⁵⁶Dy</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Zhu, C. -H.; Hartley, D. J.; Riedinger, L. L.; ...</p> <p>2015-03-26</p> <p>The exact nature of the lowest K π=2⁺ rotational <span class="hlt">bands</span> in all deformed nuclei remains obscure. Traditionally they are assumed to be collective vibrations of the nuclear shape in the γ degree of freedom perpendicular to the nuclear symmetry axis. Very few such γ-<span class="hlt">bands</span> have been traced past the usual back-bending rotational alignments of high-j nucleons. We have investigated the structure of positive-parity <span class="hlt">bands</span> in the N=90 nucleus ¹⁵⁶Dy, using the ¹⁴⁸Nd(¹²C,4n)¹⁵⁶Dy reaction at 65 MeV, observing the resulting γ-ray transitions with the Gammasphere array. The even- and odd-spin members of the π=2⁺ γ-<span class="hlt">band</span> are observed to 32⁺ and 31⁺more » respectively. This rotational <span class="hlt">band</span> faithfully tracks the <span class="hlt">ground-state</span> configuration to the highest spins. The members of a possible γ-vibration built on the aligned yrast S-<span class="hlt">band</span> are observed to spins 28⁺ and 27⁺. An even-spin positive-parity <span class="hlt">band</span>, observed to spin 24⁺, is a candidate for an aligned S-<span class="hlt">band</span> built on the seniority-zero configuration of the 0₂⁺ <span class="hlt">state</span> at 676 keV. As a result, the crossing of this <span class="hlt">band</span> with the 0₂⁺ <span class="hlt">band</span> is at hw c = 0.28(1) MeV and is consistent with the configuration of the 0₂⁺ <span class="hlt">band</span> not producing any blocking of the monopole pairing.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvL.120e7002B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvL.120e7002B"><span>Unconventional Superconductivity in Luttinger Semimetals: Theory of Complex Tensor Order and the Emergence of the Uniaxial Nematic <span class="hlt">State</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Boettcher, Igor; Herbut, Igor F.</p> <p>2018-02-01</p> <p>We investigate unconventional superconductivity in three-dimensional electronic systems with the chemical potential close to a quadratic <span class="hlt">band</span> touching point in the <span class="hlt">band</span> dispersion. Short-range interactions can lead to d -wave superconductivity, described by a complex tensor order parameter. We elucidate the general structure of the corresponding Ginzburg-Landau free <span class="hlt">energy</span> and apply these concepts to the case of an isotropic <span class="hlt">band</span> touching point. For a vanishing chemical potential, the <span class="hlt">ground</span> <span class="hlt">state</span> of the system is given by the superconductor analogue of the uniaxial nematic <span class="hlt">state</span>, which features line nodes in the excitation spectrum of quasiparticles. In contrast to the theory of real tensor order in liquid crystals, however, the <span class="hlt">ground</span> <span class="hlt">state</span> is selected here by the sextic terms in the free <span class="hlt">energy</span>. At a finite chemical potential, the nematic <span class="hlt">state</span> has an additional instability at weak coupling and low temperatures. In particular, the one-loop coefficients in the free <span class="hlt">energy</span> indicate that at weak coupling genuinely complex orders, which break time-reversal symmetry, are energetically favored. We relate our analysis to recent measurements in the half-Heusler compound YPtBi and discuss the role of cubic crystal symmetry.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JChPh.147j4301S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JChPh.147j4301S"><span>Re-examination of the Cs2 <span class="hlt">ground</span> singlet X1Σg+ and triplet a3Σu+ <span class="hlt">states</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sovkov, Vladimir B.; Xie, Feng; Lyyra, A. Marjatta; Ahmed, Ergin H.; Ma, Jie; Jia, Suotang</p> <p>2017-09-01</p> <p>This paper clarifies the disagreement in the depth of the potential <span class="hlt">energy</span> curve of the cesium dimer singlet <span class="hlt">ground</span> <span class="hlt">state</span> which has lasted for nearly a decade. We point out that the origin of this disagreement must be a technical misprint in the values of the three binding <span class="hlt">energies</span> reported by Danzl et al. [Science 321, 1062 (2008)], while the X1Σg+ <span class="hlt">state</span> potential reported by Coxon and Hajigeorgiou [J. Chem. Phys. 132, 094105 (2010)], based on experimental data by Amiot and Dulieu [J. Chem. Phys. 117, 5155 (2002)], is quite correct. We have recalculated the potential <span class="hlt">energy</span> function of the triplet <span class="hlt">ground</span> <span class="hlt">state</span> a3Σu+ by using the available experimental data spanning both the attractive and the repulsive branches so that the potential <span class="hlt">energy</span> function complies asymptotically with the singlet <span class="hlt">ground</span> <span class="hlt">state</span> X1Σg+ potential <span class="hlt">energy</span> function by Coxon and Hajigeorgiou. This is important for the simulation of the near dissociation properties such as Feshbach resonances, which are typically observed in modern experiments with ultracold atoms and molecules.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22613995-ground-state-properties-neutron-magic-nuclei','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22613995-ground-state-properties-neutron-magic-nuclei"><span><span class="hlt">Ground-state</span> properties of neutron magic nuclei</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>Saxena, G., E-mail: gauravphy@gmail.com; Kaushik, M.</p> <p>2017-03-15</p> <p>A systematic study of the <span class="hlt">ground-state</span> properties of the entire chains of even–even neutron magic nuclei represented by isotones of traditional neutron magic numbers N = 8, 20, 40, 50, 82, and 126 has been carried out using relativistic mean-field plus Bardeen–Cooper–Schrieffer approach. Our present investigation includes deformation, binding <span class="hlt">energy</span>, two-proton separation <span class="hlt">energy</span>, single-particle <span class="hlt">energy</span>, rms radii along with proton and neutron density profiles, etc. Several of these results are compared with the results calculated using nonrelativistic approach (Skyrme–Hartree–Fock method) along with available experimental data and indeed they are found with excellent agreement. In addition, the possible locations of themore » proton and neutron drip-lines, the (Z, N) values for the new shell closures, disappearance of traditional shell closures as suggested by the detailed analyzes of results are also discussed in detail.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JChPh.144w4309G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JChPh.144w4309G"><span>An experimental and theoretical study of the A˜ 2A″Π -X˜ 2A' <span class="hlt">band</span> system of the jet-cooled HBBr/DBBr free radical</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gharaibeh, Mohammed; Clouthier, Dennis J.; Tarroni, Riccardo</p> <p>2016-06-01</p> <p>The electronic spectra of the HBBr and DBBr free radicals have been studied in depth. These species were prepared in a pulsed electric discharge jet using a precursor mixture of BBr3 vapor and H2 or D2 in high pressure argon. Transitions to the electronic excited <span class="hlt">state</span> of the jet-cooled radicals were probed with laser-induced fluorescence and the <span class="hlt">ground</span> <span class="hlt">state</span> <span class="hlt">energy</span> levels were measured from the single vibronic level emission spectra. HBBr has an extensive <span class="hlt">band</span> system in the red which involves a linear-bent transition between the two Renner-Teller components of what would be a 2Π <span class="hlt">state</span> at linearity. We have used high level ab initio theory to calculate potential <span class="hlt">energy</span> surfaces for the bent 2A' <span class="hlt">ground</span> <span class="hlt">state</span> and the linear A˜ 2A″Π excited <span class="hlt">state</span> and we have determined the ro-vibronic <span class="hlt">energy</span> levels variationally, including spin orbit effects. The correspondence between the computed and experimentally observed transition frequencies, upper <span class="hlt">state</span> level symmetries, and H and B isotope shifts was used to make reliable assignments. We have shown that the <span class="hlt">ground</span> <span class="hlt">state</span> barriers to linearity, which range from 10 000 cm-1 in HBF to 2700 cm-1 in BH2, are inversely related to the <span class="hlt">energy</span> of the first excited 2Σ (2A') electronic <span class="hlt">state</span>. This suggests that a vibronic coupling mechanism is responsible for the nonlinear equilibrium geometries of the <span class="hlt">ground</span> <span class="hlt">states</span> of the HBX free radicals.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JChPh.148l4116S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JChPh.148l4116S"><span>Path integral molecular dynamic simulation of flexible molecular systems in their <span class="hlt">ground</span> <span class="hlt">state</span>: Application to the water dimer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schmidt, Matthew; Roy, Pierre-Nicholas</p> <p>2018-03-01</p> <p>We extend the Langevin equation Path Integral <span class="hlt">Ground</span> <span class="hlt">State</span> (LePIGS), a <span class="hlt">ground</span> <span class="hlt">state</span> quantum molecular dynamics method, to simulate flexible molecular systems and calculate both energetic and structural properties. We test the approach with the H2O and D2O monomers and dimers. We systematically optimize all simulation parameters and use a unity trial wavefunction. We report <span class="hlt">ground</span> <span class="hlt">state</span> <span class="hlt">energies</span>, dissociation <span class="hlt">energies</span>, and structural properties using three different water models, two of which are empirically based, q-TIP4P/F and q-SPC/Fw, and one which is ab initio, MB-pol. We demonstrate that our <span class="hlt">energies</span> calculated from LePIGS can be merged seamlessly with low temperature path integral molecular dynamics calculations and note the similarities between the two methods. We also benchmark our <span class="hlt">energies</span> against previous diffusion Monte Carlo calculations using the same potentials and compare to experimental results. We further demonstrate that accurate vibrational <span class="hlt">energies</span> of the H2O and D2O monomer can be calculated from imaginary time correlation functions generated from the LePIGS simulations using solely the unity trial wavefunction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017RpMP...80..233W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017RpMP...80..233W"><span>Bogolyubov inequality for the <span class="hlt">ground</span> <span class="hlt">state</span> and its application to interacting rotor systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wojtkiewicz, Jacek; Pusz, Wiesław; Stachura, Piotr</p> <p>2017-10-01</p> <p>We have formulated and proved the Bogolyubov inequality for operators at zero temperature. So far this inequality has been known for matrices, and we were able to extend it to certain class of operators. We have also applied this inequality to the system of interacting rotors. We have shown that if: (i) the dimension of the lattice is 1 or 2, (ii) the interaction decreases sufficiently fast with a distance, and (iii) there is an <span class="hlt">energy</span> gap over the <span class="hlt">ground</span> <span class="hlt">state</span>, then the spontaneous magnetization in the <span class="hlt">ground</span> <span class="hlt">state</span> is zero, i.e. there is no LRO in the system. We present also heuristic arguments (of perturbation-theoretic nature) suggesting that one- and two-dimensional systems of interacting rotors have the <span class="hlt">energy</span> gap independent of the system size if the interaction is sufficiently small.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016NatCo...710418C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016NatCo...710418C"><span>Engineered Mott <span class="hlt">ground</span> <span class="hlt">state</span> in a LaTiO3+δ/LaNiO3 heterostructure</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cao, Yanwei; Liu, Xiaoran; Kareev, M.; Choudhury, D.; Middey, S.; Meyers, D.; Kim, J.-W.; Ryan, P. J.; Freeland, J. W.; Chakhalian, J.</p> <p>2016-01-01</p> <p>In pursuit of creating cuprate-like electronic and orbital structures, artificial heterostructures based on LaNiO3 have inspired a wealth of exciting experimental and theoretical results. However, to date there is a very limited experimental understanding of the electronic and orbital <span class="hlt">states</span> emerging from interfacial charge transfer and their connections to the modified <span class="hlt">band</span> structure at the interface. Towards this goal, we have synthesized a prototypical superlattice composed of a correlated metal LaNiO3 and a doped Mott insulator LaTiO3+δ, and investigated its electronic structure by resonant X-ray absorption spectroscopy combined with X-ray photoemission spectroscopy, electrical transport and theory calculations. The heterostructure exhibits interfacial charge transfer from Ti to Ni sites, giving rise to an insulating <span class="hlt">ground</span> <span class="hlt">state</span> with orbital polarization and eg orbital <span class="hlt">band</span> splitting. Our findings demonstrate how the control over charge at the interface can be effectively used to create exotic electronic, orbital and spin <span class="hlt">states</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4735946','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4735946"><span>Engineered Mott <span class="hlt">ground</span> <span class="hlt">state</span> in a LaTiO3+δ/LaNiO3 heterostructure</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Cao, Yanwei; Liu, Xiaoran; Kareev, M.; Choudhury, D.; Middey, S.; Meyers, D.; Kim, J.-W.; Ryan, P. J.; Freeland, J.W.; Chakhalian, J.</p> <p>2016-01-01</p> <p>In pursuit of creating cuprate-like electronic and orbital structures, artificial heterostructures based on LaNiO3 have inspired a wealth of exciting experimental and theoretical results. However, to date there is a very limited experimental understanding of the electronic and orbital <span class="hlt">states</span> emerging from interfacial charge transfer and their connections to the modified <span class="hlt">band</span> structure at the interface. Towards this goal, we have synthesized a prototypical superlattice composed of a correlated metal LaNiO3 and a doped Mott insulator LaTiO3+δ, and investigated its electronic structure by resonant X-ray absorption spectroscopy combined with X-ray photoemission spectroscopy, electrical transport and theory calculations. The heterostructure exhibits interfacial charge transfer from Ti to Ni sites, giving rise to an insulating <span class="hlt">ground</span> <span class="hlt">state</span> with orbital polarization and eg orbital <span class="hlt">band</span> splitting. Our findings demonstrate how the control over charge at the interface can be effectively used to create exotic electronic, orbital and spin <span class="hlt">states</span>. PMID:26791402</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1241364-engineered-mott-ground-state-latio3+-lanio3-heterostructure','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1241364-engineered-mott-ground-state-latio3+-lanio3-heterostructure"><span>Engineered Mott <span class="hlt">ground</span> <span class="hlt">state</span> in a LaTiO 3+δ/LaNiO 3 heterostructure</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Cao, Yanwei; Liu, Xiaoran; Kareev, M.; ...</p> <p>2016-01-21</p> <p>In pursuit of creating cuprate-like electronic and orbital structures, artificial heterostructures based on LaNiO 3 have inspired a wealth of exciting experimental and theoretical results. However, to date there is a very limited experimental understanding of the electronic and orbital <span class="hlt">states</span> emerging from interfacial charge transfer and their connections to the modified <span class="hlt">band</span> structure at the interface. Towards this goal, we have synthesized a prototypical superlattice composed of a correlated metal LaNiO 3 and a doped Mott insulator LaTiO 3+δ, and investigated its electronic structure by resonant X-ray absorption spectroscopy combined with X-ray photoemission spectroscopy, electrical transport and theory calculations.more » The heterostructure exhibits interfacial charge transfer from Ti to Ni sites, giving rise to an insulating <span class="hlt">ground</span> <span class="hlt">state</span> with orbital polarization and e g orbital <span class="hlt">band</span> splitting. Here, our findings demonstrate how the control over charge at the interface can be effectively used to create exotic electronic, orbital and spin <span class="hlt">states</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PhRvB..93h5202G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhRvB..93h5202G"><span>Quasiparticle <span class="hlt">band</span> gap of organic-inorganic hybrid perovskites: Crystal structure, spin-orbit coupling, and self-<span class="hlt">energy</span> effects</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gao, Weiwei; Gao, Xiang; Abtew, Tesfaye A.; Sun, Yi-Yang; Zhang, Shengbai; Zhang, Peihong</p> <p>2016-02-01</p> <p>The quasiparticle <span class="hlt">band</span> gap is one of the most important materials properties for photovoltaic applications. Often the <span class="hlt">band</span> 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 <span class="hlt">band</span> gap formation mechanism in organic-inorganic hybrid perovskites by decoupling various contributing factors which ultimately determine their electronic structure and quasiparticle <span class="hlt">band</span> gap. Major factors, namely, quasiparticle self-<span class="hlt">energy</span>, spin-orbit coupling, and structural distortions due to the presence of organic molecules, and their influences on the quasiparticle <span class="hlt">band</span> structure of organic-inorganic hybrid perovskites are illustrated. We find that although methylammonium cations do not contribute directly to the electronic <span class="hlt">states</span> near <span class="hlt">band</span> edges, they play an important role in defining the <span class="hlt">band</span> 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 <span class="hlt">energies</span>.</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 electronic <span class="hlt">states</span>. In the electronic <span class="hlt">states</span> calculations using plane wave basis functions, a large number of plane waves are often required to obtain precise results. Even using <span class="hlt">state</span>-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/2017AGUFM.H21E1507Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.H21E1507Z"><span>Comparison of High Resolution Quantitative Extreme Precipitation Estimation from GPM Dual-frequency Radar and S-<span class="hlt">band</span> Radar Observation over Southern China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, A.; Chen, S.; Fan, S.; Min, C.</p> <p>2017-12-01</p> <p>Precipitation is one of the basic elements of regional and global climate change. Not only does the precipitation have a great impact on the earth's hydrosphere, but also plays a crucial role in the global <span class="hlt">energy</span> balance. S-<span class="hlt">band</span> <span class="hlt">ground</span>-based dual-polarization radar has the excellent performance of identifying the different phase <span class="hlt">states</span> of precipitation, which can dramatically improve the accuracy of hail identification and quantitative precipitation estimation (QPE). However, the <span class="hlt">ground</span>-based radar cannot measure the precipitation in mountains, sparsely populated plateau, desert and ocean because of the <span class="hlt">ground</span>-based radar void. The Unites <span class="hlt">States</span> National Aeronautics and Space Administration (NASA) and Japan Aerospace Exploration Agency (JAXA) have launched the Global Precipitation Measurement (GPM) for almost three years. GPM is equipped with a GPM Microwave Imager (GMI) and a Dual-frequency (Ku- and Ka-<span class="hlt">band</span>) Precipitation Radar (DPR) that covers the globe between 65°S and 65°N. The main parameters and the detection method of DPR are different from those of <span class="hlt">ground</span>-based radars, thus, the DPR's reliability and capability need to be investigated and evaluated by the <span class="hlt">ground</span>-based radar. This study compares precipitation derived from the <span class="hlt">ground</span>-based radar measurement to that derived from the DPR's observations. The <span class="hlt">ground</span>-based radar is a S-<span class="hlt">band</span> dual-polarization radar deployed near an airport in the west of Zhuhai city. The <span class="hlt">ground</span>-based quantitative precipitation estimates are with a high resolution of 1km×1km×6min. It shows that this radar covers the whole Pearl River Delta of China, including Hong Kong and Macao. In order to quantify the DPR precipitation quantification capabilities relative to the S-<span class="hlt">band</span> radar, statistical metrics used in this study are as follows: the difference (Dif) between DPR and the S-<span class="hlt">band</span> radar observation, root-mean-squared error (RMSE) and correlation coefficient (CC). Additionally, Probability of Detection (POD) and False Alarm Ratio</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001LNP...570..672K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001LNP...570..672K"><span><span class="hlt">Ground-State</span> Hyperfine Structure of Heavy Hydrogen-Like Ions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kühl, T.; Borneis, S.; Dax, A.; Engel, T.; Faber, S.; Gerlach, M.; Holbrow, C.; Huber, G.; Marx, D.; Merz, P.; Quint, W.; Schmitt, F.; Seelig, P.; Tomaselli, M.; Winter, H.; Wuertz, M.; Beckert, K.; Franzke, B.; Nolden, F.; Reich, H.; Steck, M.</p> <p></p> <p>Contributions of quantum electrodynamics (QED) to the combined electric and magnetic interaction between the electron and the nucleus can be studied by optical spectroscopy in high-Z hydrogen-like heavy ions. The transition studied is the <span class="hlt">ground-state</span> hyperfine structure transition, well known from the 21 cm line in atomic hydrogen. The hyperfine splitting of the is <span class="hlt">ground</span> <span class="hlt">state</span> of hydrogen-like systems constitutes the simplest and most basic magnetic interaction in atomic physics. The Z3-increase leads to a transition <span class="hlt">energy</span> in the UV-region of the optical spectrum for the case of Bi82+. At the same time, the QED correction rises to nearly 1 fraction of higher order contributions. This situation is particularly useful for a comparison with non-perturbative QED calculations. The combination of exceptionally intense electric and magnetic fields electric and magnetic fields is unique. This transition has become accessible to precision laser spectroscopy at the high-<span class="hlt">energy</span> heavy-ion storage ring at GSI-Darmstadt in the hydrogen-like 209Bi82+ and 207Pb81+. In the meantime, 165Ho66+ and 185,187Re74+ were also studied with reduced resolution by conventional optical spectroscopy at the SuperEBIT ion trap at Lawrence Livermore National Laboratory.</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-electronics 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 <span class="hlt">ground</span> <span class="hlt">state</span> <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 electronic properties of quasi-one-dimensional materials such as bio-molecular chains, organic and inorganic nanoribbons by performing edge engineering. PMID:27808172</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('http://adsabs.harvard.edu/abs/2008JChPh.128v4314W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008JChPh.128v4314W"><span>Full-dimensional quantum calculations of <span class="hlt">ground-state</span> tunneling splitting of malonaldehyde using an accurate ab initio potential <span class="hlt">energy</span> surface</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Yimin; Braams, Bastiaan J.; Bowman, Joel M.; Carter, Stuart; Tew, David P.</p> <p>2008-06-01</p> <p>Quantum calculations of the <span class="hlt">ground</span> vibrational <span class="hlt">state</span> tunneling splitting of H-atom and D-atom transfer in malonaldehyde are performed on a full-dimensional ab initio potential <span class="hlt">energy</span> surface (PES). The PES is a fit to 11 147 near basis-set-limit frozen-core CCSD(T) electronic <span class="hlt">energies</span>. This surface properly describes the invariance of the potential with respect to all permutations of identical atoms. The saddle-point barrier for the H-atom transfer on the PES is 4.1 kcal/mol, in excellent agreement with the reported ab initio value. Model one-dimensional and ``exact'' full-dimensional calculations of the splitting for H- and D-atom transfer are done using this PES. The tunneling splittings in full dimensionality are calculated using the unbiased ``fixed-node'' diffusion Monte Carlo (DMC) method in Cartesian and saddle-point normal coordinates. The <span class="hlt">ground-state</span> tunneling splitting is found to be 21.6 cm-1 in Cartesian coordinates and 22.6 cm-1 in normal coordinates, with an uncertainty of 2-3 cm-1. This splitting is also calculated based on a model which makes use of the exact single-well zero-point <span class="hlt">energy</span> (ZPE) obtained with the MULTIMODE code and DMC ZPE and this calculation gives a tunneling splitting of 21-22 cm-1. The corresponding computed splittings for the D-atom transfer are 3.0, 3.1, and 2-3 cm-1. These calculated tunneling splittings agree with each other to within less than the standard uncertainties obtained with the DMC method used, which are between 2 and 3 cm-1, and agree well with the experimental values of 21.6 and 2.9 cm-1 for the H and D transfer, respectively.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18554020','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18554020"><span>Full-dimensional quantum calculations of <span class="hlt">ground-state</span> tunneling splitting of malonaldehyde using an accurate ab initio potential <span class="hlt">energy</span> surface.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Yimin; Braams, Bastiaan J; Bowman, Joel M; Carter, Stuart; Tew, David P</p> <p>2008-06-14</p> <p>Quantum calculations of the <span class="hlt">ground</span> vibrational <span class="hlt">state</span> tunneling splitting of H-atom and D-atom transfer in malonaldehyde are performed on a full-dimensional ab initio potential <span class="hlt">energy</span> surface (PES). The PES is a fit to 11 147 near basis-set-limit frozen-core CCSD(T) electronic <span class="hlt">energies</span>. This surface properly describes the invariance of the potential with respect to all permutations of identical atoms. The saddle-point barrier for the H-atom transfer on the PES is 4.1 kcalmol, in excellent agreement with the reported ab initio value. Model one-dimensional and "exact" full-dimensional calculations of the splitting for H- and D-atom transfer are done using this PES. The tunneling splittings in full dimensionality are calculated using the unbiased "fixed-node" diffusion Monte Carlo (DMC) method in Cartesian and saddle-point normal coordinates. The <span class="hlt">ground-state</span> tunneling splitting is found to be 21.6 cm(-1) in Cartesian coordinates and 22.6 cm(-1) in normal coordinates, with an uncertainty of 2-3 cm(-1). This splitting is also calculated based on a model which makes use of the exact single-well zero-point <span class="hlt">energy</span> (ZPE) obtained with the MULTIMODE code and DMC ZPE and this calculation gives a tunneling splitting of 21-22 cm(-1). The corresponding computed splittings for the D-atom transfer are 3.0, 3.1, and 2-3 cm(-1). These calculated tunneling splittings agree with each other to within less than the standard uncertainties obtained with the DMC method used, which are between 2 and 3 cm(-1), and agree well with the experimental values of 21.6 and 2.9 cm(-1) for the H and D transfer, respectively.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19840011558&hterms=Exciter&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DExciter','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19840011558&hterms=Exciter&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DExciter"><span>X-<span class="hlt">band</span> Uplink <span class="hlt">Ground</span> Systems Development</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Johns, C. E.</p> <p>1984-01-01</p> <p>The development of the X-<span class="hlt">band</span> exciter and Doppler extractor equipment for the X-<span class="hlt">band</span> uplink was completed. Stability measurements were made on the exciter and Doppler reference signals and the results are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/21550238-analytical-ground-state-jaynes-cummings-model-ultrastrong-coupling','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/21550238-analytical-ground-state-jaynes-cummings-model-ultrastrong-coupling"><span>Analytical <span class="hlt">ground</span> <span class="hlt">state</span> for the Jaynes-Cummings model with ultrastrong coupling</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>Zhang Yuanwei; Institute of Theoretical Physics, Shanxi University, Taiyuan 030006; Chen Gang</p> <p>2011-06-15</p> <p>We present a generalized variational method to analytically obtain the <span class="hlt">ground-state</span> properties of the Jaynes-Cummings model with the ultrastrong coupling. An explicit expression for the <span class="hlt">ground-state</span> <span class="hlt">energy</span>, which agrees well with the numerical simulation in a wide range of the experimental parameters, is given. In particular, the introduced method can successfully solve this Jaynes-Cummings model with the positive detuning (the atomic resonant level is larger than the photon frequency), which cannot be treated in the adiabatical approximation and the generalized rotating-wave approximation. Finally, we also demonstrate analytically how to control the mean photon number by means of the current experimentalmore » parameters including the photon frequency, the coupling strength, and especially the atomic resonant level.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PrPNP.101...96R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PrPNP.101...96R"><span>Nuclear equation of <span class="hlt">state</span> from <span class="hlt">ground</span> and collective excited <span class="hlt">state</span> properties of nuclei</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Roca-Maza, X.; Paar, N.</p> <p>2018-07-01</p> <p>This contribution reviews the present status on the available constraints to the nuclear equation of <span class="hlt">state</span> (EoS) around saturation density from nuclear structure calculations on <span class="hlt">ground</span> and collective excited <span class="hlt">state</span> properties of atomic nuclei. It concentrates on predictions based on self-consistent mean-field calculations, which can be considered as an approximate realization of an exact <span class="hlt">energy</span> density functional (EDF). EDFs are derived from effective interactions commonly fitted to nuclear masses, charge radii and, in many cases, also to pseudo-data such as nuclear matter properties. Although in a model dependent way, EDFs constitute nowadays a unique tool to reliably and consistently access bulk <span class="hlt">ground</span> <span class="hlt">state</span> and collective excited <span class="hlt">state</span> properties of atomic nuclei along the nuclear chart as well as the EoS. For comparison, some emphasis is also given to the results obtained with the so called ab initio approaches that aim at describing the nuclear EoS based on interactions fitted to few-body data only. Bridging the existent gap between these two frameworks will be essential since it may allow to improve our understanding on the diverse phenomenology observed in nuclei. Examples on observations from astrophysical objects and processes sensitive to the nuclear EoS are also briefly discussed. As the main conclusion, the isospin dependence of the nuclear EoS around saturation density and, to a lesser extent, the nuclear matter incompressibility remain to be accurately determined. Experimental and theoretical efforts in finding and measuring observables specially sensitive to the EoS properties are of paramount importance, not only for low-<span class="hlt">energy</span> nuclear physics but also for nuclear astrophysics applications.</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/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 <span class="hlt">states</span>. 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.osti.gov/biblio/22416015-theoretical-study-ground-state-polar-alkali-metal-barium-molecules-potential-energy-curve-permanent-dipole-moment','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22416015-theoretical-study-ground-state-polar-alkali-metal-barium-molecules-potential-energy-curve-permanent-dipole-moment"><span>Theoretical study on the <span class="hlt">ground</span> <span class="hlt">state</span> of the polar alkali-metal-barium molecules: Potential <span class="hlt">energy</span> curve and permanent dipole moment</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>Gou, Dezhi; Kuang, Xiaoyu, E-mail: scu-kuang@163.com; Gao, Yufeng</p> <p>2015-01-21</p> <p>In this paper, we systematically investigate the electronic structure for the {sup 2}Σ{sup +} <span class="hlt">ground</span> <span class="hlt">state</span> of the polar alkali-metal-alkaline-earth-metal molecules BaAlk (Alk = Li, Na, K, Rb, and Cs). Potential <span class="hlt">energy</span> curves and permanent dipole moments (PDMs) are determined using power quantum chemistry complete active space self-consistent field and multi-reference configuration interaction methods. Basic spectroscopic constants are derived from ro-vibrational bound <span class="hlt">state</span> calculation. From the calculations, it is shown that BaK, BaRb, and BaCs molecules have moderate values of PDM at the equilibrium bond distance (BaK:1.62 D, BaRb:3.32 D, and BaCs:4.02 D). Besides, the equilibrium bond length (4.93 Åmore » and 5.19 Å) and dissociation <span class="hlt">energy</span> (0.1825 eV and 0.1817 eV) for the BaRb and BaCs are also obtained.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvB..97d1403L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvB..97d1403L"><span>Contributions of oxygen vacancies and titanium interstitials to <span class="hlt">band</span>-gap <span class="hlt">states</span> of reduced titania</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Jingfeng; Lazzari, Rémi; Chenot, Stéphane; Jupille, Jacques</p> <p>2018-01-01</p> <p>The spectroscopic fingerprints of the point defects of titanium dioxide remain highly controversial. Seemingly indisputable experiments lead to conflicting conclusions in which oxygen vacancies and titanium interstitials are alternately referred to as the primary origin of the Ti 3 d <span class="hlt">band</span>-gap <span class="hlt">states</span>. We report on experiments performed by electron <span class="hlt">energy</span> loss spectroscopy whose key is the direct annealing of only the very surface of rutile TiO2(110 ) crystals and the simultaneous measurement of its temperature via the Bose-Einstein loss/gain ratio. By surface preparations involving reactions with oxygen and water vapor, in particular, under electron irradiation, vacancy- and interstitial-related <span class="hlt">band</span>-gap <span class="hlt">states</span> are singled out. Off-specular measurements reveal that both types of defects contribute to a unique charge distribution that peaks in subsurface layers with a common dispersive behavior.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011APS..DMP.P4001M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011APS..DMP.P4001M"><span>Cavity optomechanics -- beyond the <span class="hlt">ground</span> <span class="hlt">state</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Meystre, Pierre</p> <p>2011-05-01</p> <p>The coupling of coherent optical systems to micromechanical devices, combined with breakthroughs in nanofabrication and in ultracold science, has opened up the exciting new field of cavity optomechanics. Cooling of the vibrational motion of a broad range on oscillating cantilevers and mirrors near their <span class="hlt">ground</span> <span class="hlt">state</span> has been demonstrated, and the <span class="hlt">ground</span> <span class="hlt">state</span> of at least one such system has now been reached. Cavity optomechanics offers much promise in addressing fundamental physics questions and in applications such as the detection of feeble forces and fields, or the coherent control of AMO systems and of nanoscale electromechanical devices. However, these applications require taking cavity optomechanics ``beyond the <span class="hlt">ground</span> <span class="hlt">state</span>.'' This includes the generation and detection of squeezed and other non-classical <span class="hlt">states</span>, the transfer of squeezing between electromagnetic fields and motional quadratures, and the development of measurement schemes for the characterization of nanomechanical structures. The talk will present recent ``beyond <span class="hlt">ground</span> <span class="hlt">state</span>'' developments in cavity optomechanics. We will show how the magnetic coupling between a mechanical membrane and a BEC - or between a mechanical tuning fork and a nanoscale cantilever - permits to control and monitor the center-of-mass position of the mechanical system, and will comment on the measurement back-action on the membrane motion. We will also discuss of <span class="hlt">state</span> transfer between optical and microwave fields and micromechanical devices. Work done in collaboration with Dan Goldbaum, Greg Phelps, Keith Schwab, Swati Singh, Steve Steinke, Mehmet Tesgin, and Mukund Vengallatore and supported by ARO, DARPA, NSF, and ONR.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AnPhy.326.2165B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AnPhy.326.2165B"><span>On the <span class="hlt">ground</span> <span class="hlt">state</span> of Yang-Mills theory</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bakry, Ahmed S.; Leinweber, Derek B.; Williams, Anthony G.</p> <p>2011-08-01</p> <p>We investigate the overlap of the <span class="hlt">ground</span> <span class="hlt">state</span> meson potential with sets of mesonic-trial wave functions corresponding to different gluonic distributions. We probe the transverse structure of the flux tube through the creation of non-uniform smearing profiles for the string of glue connecting two color sources in Wilson loop operator. The non-uniformly UV-regulated flux-tube operators are found to optimize the overlap with the <span class="hlt">ground</span> <span class="hlt">state</span> and display interesting features in the <span class="hlt">ground</span> <span class="hlt">state</span> overlap.</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.osti.gov/biblio/5013655-ground-state-excitonic-molecules-green-function-monte-carlo-method','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5013655-ground-state-excitonic-molecules-green-function-monte-carlo-method"><span><span class="hlt">Ground</span> <span class="hlt">state</span> of excitonic molecules by the Green's-function Monte Carlo method</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>Lee, M.A.; Vashishta, P.; Kalia, R.K.</p> <p>1983-12-26</p> <p>The <span class="hlt">ground-state</span> <span class="hlt">energy</span> of excitonic molecules is evaluated as a function of the ratio of electron and hole masses, sigma, with use of the Green's-function Monte Carlo method. For all sigma, the Green's-function Monte Carlo <span class="hlt">energies</span> are significantly lower than the variational estimates and in favorable agreement with experiments. In excitonic rydbergs, the binding <span class="hlt">energy</span> of the positronium molecule (sigma = 1) is predicted to be -0.06 and for sigma<<1, the Green's-function Monte Carlo <span class="hlt">energies</span> agree with the ''exact'' limiting behavior, E = -2.346+0.764sigma.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011PhRvL.107d3005S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011PhRvL.107d3005S"><span>QED Effects in Molecules: Test on Rotational Quantum <span class="hlt">States</span> of H2</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Salumbides, E. J.; Dickenson, G. D.; Ivanov, T. I.; Ubachs, W.</p> <p>2011-07-01</p> <p>Quantum electrodynamic effects have been systematically tested in the progression of rotational quantum <span class="hlt">states</span> in the XΣg+1, v=0 vibronic <span class="hlt">ground</span> <span class="hlt">state</span> of molecular hydrogen. High-precision Doppler-free spectroscopy of the EFΣg+1-XΣg+1 (0,0) <span class="hlt">band</span> was performed with 0.005cm-1 accuracy on rotationally hot H2 (with rotational quantum <span class="hlt">states</span> J up to 16). QED and relativistic contributions to rotational level <span class="hlt">energies</span> as high as 0.13cm-1 are extracted, and are in perfect agreement with recent calculations of QED and high-order relativistic effects for the H2 <span class="hlt">ground</span> <span class="hlt">state</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1281077-theoretical-modeling-low-energy-electronic-absorption-bands-reduced-cobaloximes','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1281077-theoretical-modeling-low-energy-electronic-absorption-bands-reduced-cobaloximes"><span>Theoretical modeling of low-<span class="hlt">energy</span> electronic absorption <span class="hlt">bands</span> in reduced cobaloximes</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Bhattacharjee, Anirban; Chavarot-Kerlidou, Murielle; Dempsey, Jillian L.; ...</p> <p>2014-08-11</p> <p>Here, we report that the reduced Co(I) <span class="hlt">states</span> 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 <span class="hlt">energy</span> electronic absorption <span class="hlt">bands</span> 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.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PhRvL.117f2501H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhRvL.117f2501H"><span>Superdeformed and Triaxial <span class="hlt">States</span> in 42Ca</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hadyńska-KlÈ©k, K.; Napiorkowski, P. J.; Zielińska, M.; Srebrny, J.; Maj, A.; Azaiez, F.; Valiente Dobón, J. J.; Kicińska-Habior, M.; Nowacki, F.; Naïdja, H.; Bounthong, B.; Rodríguez, T. R.; de Angelis, G.; Abraham, T.; Anil Kumar, G.; Bazzacco, D.; Bellato, M.; Bortolato, D.; Bednarczyk, P.; Benzoni, G.; Berti, L.; Birkenbach, B.; Bruyneel, B.; Brambilla, S.; Camera, F.; Chavas, J.; Cederwall, B.; Charles, L.; Ciemała, M.; Cocconi, P.; Coleman-Smith, P.; Colombo, A.; Corsi, A.; Crespi, F. C. L.; Cullen, D. M.; Czermak, A.; Désesquelles, P.; Doherty, D. T.; Dulny, B.; Eberth, J.; Farnea, E.; Fornal, B.; Franchoo, S.; Gadea, A.; Giaz, A.; Gottardo, A.; Grave, X.; GrÈ©bosz, J.; Görgen, A.; Gulmini, M.; Habermann, T.; Hess, H.; Isocrate, R.; Iwanicki, J.; Jaworski, G.; Judson, D. S.; Jungclaus, A.; Karkour, N.; Kmiecik, M.; Karpiński, D.; Kisieliński, M.; Kondratyev, N.; Korichi, A.; Komorowska, M.; Kowalczyk, M.; Korten, W.; Krzysiek, M.; Lehaut, G.; Leoni, S.; Ljungvall, J.; Lopez-Martens, A.; Lunardi, S.; Maron, G.; Mazurek, K.; Menegazzo, R.; Mengoni, D.; Merchán, E.; MÈ©czyński, W.; Michelagnoli, C.; Mierzejewski, J.; Million, B.; Myalski, S.; Napoli, D. R.; Nicolini, R.; Niikura, M.; Obertelli, A.; Özmen, S. F.; Palacz, M.; Próchniak, L.; Pullia, A.; Quintana, B.; Rampazzo, G.; Recchia, F.; Redon, N.; Reiter, P.; Rosso, D.; Rusek, K.; Sahin, E.; Salsac, M.-D.; Söderström, P.-A.; Stefan, I.; Stézowski, O.; Styczeń, J.; Theisen, Ch.; Toniolo, N.; Ur, C. A.; Vandone, V.; Wadsworth, R.; Wasilewska, B.; Wiens, A.; Wood, J. L.; Wrzosek-Lipska, K.; ZiÈ©bliński, M.</p> <p>2016-08-01</p> <p>Shape parameters of a weakly deformed <span class="hlt">ground-state</span> <span class="hlt">band</span> and highly deformed slightly triaxial sideband in 42Ca were determined from E 2 matrix elements measured in the first low-<span class="hlt">energy</span> Coulomb excitation experiment performed with AGATA. The picture of two coexisting structures is well reproduced by new <span class="hlt">state</span>-of-the-art large-scale shell model and beyond-mean-field calculations. Experimental evidence for superdeformation of the <span class="hlt">band</span> built on 02+ has been obtained and the role of triaxiality in the A ˜40 mass region is discussed. Furthermore, the potential of Coulomb excitation as a tool to study superdeformation has been demonstrated for the first time.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19549837','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19549837"><span>Baseline brain <span class="hlt">energy</span> supports the <span class="hlt">state</span> of consciousness.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Shulman, Robert G; Hyder, Fahmeed; Rothman, Douglas L</p> <p>2009-07-07</p> <p>An individual, human or animal, is defined to be in a conscious <span class="hlt">state</span> empirically by the behavioral ability to respond meaningfully to stimuli, whereas the loss of consciousness is defined by unresponsiveness. PET measurements of glucose or oxygen consumption show a widespread approximately 45% reduction in cerebral <span class="hlt">energy</span> consumption with anesthesia-induced loss of consciousness. Because baseline brain <span class="hlt">energy</span> consumption has been shown by (13)C magnetic resonance spectroscopy to be almost exclusively dedicated to neuronal signaling, we propose that the high level of brain <span class="hlt">energy</span> is a necessary property of the conscious <span class="hlt">state</span>. Two additional neuronal properties of the conscious <span class="hlt">state</span> change with anesthesia. The delocalized fMRI activity patterns in rat brain during sensory stimulation at a higher <span class="hlt">energy</span> <span class="hlt">state</span> (close to the awake) collapse to a contralateral somatosensory response at lower <span class="hlt">energy</span> <span class="hlt">state</span> (deep anesthesia). Firing rates of an ensemble of neurons in the rat somatosensory cortex shift from the gamma-<span class="hlt">band</span> range (20-40 Hz) at higher <span class="hlt">energy</span> <span class="hlt">state</span> to <10 Hz at lower <span class="hlt">energy</span> <span class="hlt">state</span>. With the conscious <span class="hlt">state</span> defined by the individual's behavior and maintained by high cerebral <span class="hlt">energy</span>, measurable properties of that <span class="hlt">state</span> are the widespread fMRI patterns and high frequency neuronal activity, both of which support the extensive interregional communication characteristic of consciousness. This usage of high brain <span class="hlt">energies</span> when the person is in the "<span class="hlt">state</span>" of consciousness differs from most studies, which attend the smaller <span class="hlt">energy</span> increments observed during the stimulations that form the "contents" of that <span class="hlt">state</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26574447','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26574447"><span>Multiconfiguration Pair-Density Functional Theory Outperforms Kohn-Sham Density Functional Theory and Multireference Perturbation Theory for <span class="hlt">Ground-State</span> and Excited-<span class="hlt">State</span> Charge Transfer.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ghosh, Soumen; Sonnenberger, Andrew L; Hoyer, Chad E; Truhlar, Donald G; Gagliardi, Laura</p> <p>2015-08-11</p> <p>The correct description of charge transfer in <span class="hlt">ground</span> and excited <span class="hlt">states</span> is very important for molecular interactions, photochemistry, electrochemistry, and charge transport, but it is very challenging for Kohn-Sham (KS) density functional theory (DFT). KS-DFT exchange-correlation functionals without nonlocal exchange fail to describe both <span class="hlt">ground</span>- and excited-<span class="hlt">state</span> charge transfer properly. We have recently proposed a theory called multiconfiguration pair-density functional theory (MC-PDFT), which is based on a combination of multiconfiguration wave function theory with a new type of density functional called an on-top density functional. Here we have used MC-PDFT to study challenging <span class="hlt">ground</span>- and excited-<span class="hlt">state</span> charge-transfer processes by using on-top density functionals obtained by translating KS exchange-correlation functionals. For <span class="hlt">ground-state</span> charge transfer, MC-PDFT performs better than either the PBE exchange-correlation functional or CASPT2 wave function theory. For excited-<span class="hlt">state</span> charge transfer, MC-PDFT (unlike KS-DFT) shows qualitatively correct behavior at long-range with great improvement in predicted excitation <span class="hlt">energies</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25398159','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25398159"><span><span class="hlt">Ground</span> <span class="hlt">state</span>, collective mode, phase soliton and vortex in multiband superconductors.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lin, Shi-Zeng</p> <p>2014-12-10</p> <p>This article reviews theoretical and experimental work on the novel physics in multiband superconductors. Multiband superconductors are characterized by multiple superconducting <span class="hlt">energy</span> gaps in different <span class="hlt">bands</span> with interaction between Cooper pairs in these <span class="hlt">bands</span>. The discovery of prominent multiband superconductors MgB2 and later iron-based superconductors, has triggered enormous interest in multiband superconductors. The most recently discovered superconductors exhibit multiband features. The multiband superconductors possess novel properties that are not shared with their single-<span class="hlt">band</span> counterpart. Examples include: the time-reversal symmetry broken <span class="hlt">state</span> in multiband superconductors with frustrated interband couplings; the collective oscillation of number of Cooper pairs between different <span class="hlt">bands</span>, known as the Leggett mode; and the phase soliton and fractional vortex, which are the main focus of this review. This review presents a survey of a wide range of theoretical exploratory and experimental investigations of novel physics in multiband superconductors. A vast amount of information derived from these studies is shown to highlight unusual and unique properties of multiband superconductors and to reveal the challenges and opportunities in the research on the multiband superconductivity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27660919','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27660919"><span><span class="hlt">Band</span> gap <span class="hlt">states</span> in nanocrystalline WO3 thin films studied by soft x-ray spectroscopy and optical spectrophotometry.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Johansson, M B; Kristiansen, P T; Duda, L; Niklasson, G A; Österlund, L</p> <p>2016-11-30</p> <p>Nanocrystalline tungsten trioxide (WO3) thin films prepared by DC magnetron sputtering have been studied using soft x-ray spectroscopy and optical spectrophotometry. Resonant inelastic x-ray scattering (RIXS) measurements reveal <span class="hlt">band</span> gap <span class="hlt">states</span> in sub-stoichiometric γ-WO3-x with x  =  0.001-0.005. The <span class="hlt">energy</span> positions of these <span class="hlt">states</span> are in good agreement with recently reported density functional calculations. The results were compared with optical absorption measurements in the near infrared spectral region. An optical absorption peak at 0.74 eV is assigned to intervalence transfer of polarons between W sites. A less prominent peak at <span class="hlt">energies</span> between 0.96 and 1.16 eV is assigned to electron excitation of oxygen vacancies. The latter results are supported by RIXS measurements, where an <span class="hlt">energy</span> loss in this <span class="hlt">energy</span> range was observed, and this suggests that electron transfer processes involving transitions from oxygen vacancy <span class="hlt">states</span> can be observed in RIXS. Our results have implications for the interpretation of optical properties of WO3, and the optical transitions close to the <span class="hlt">band</span> gap, which are important in photocatalytic and photoelectrochemical applications.</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/2017PhRvC..96c4311V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvC..96c4311V"><span>Search for the 73Ga <span class="hlt">ground-state</span> doublet splitting in the β decay of 73Zn</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vedia, V.; Paziy, V.; Fraile, L. M.; Mach, H.; Walters, W. B.; Aprahamian, A.; Bernards, C.; Briz, J. A.; Bucher, B.; Chiara, C. J.; Dlouhý, Z.; Gheorghe, I.; GhiÅ£ǎ, D.; Hoff, P.; Jolie, J.; Köster, U.; Kurcewicz, W.; Licǎ, R.; Mǎrginean, N.; Mǎrginean, R.; Olaizola, B.; Régis, J.-M.; Rudigier, M.; Sava, T.; Simpson, G. S.; Stǎnoiu, M.; Stroe, L.</p> <p>2017-09-01</p> <p>The existence of two close-lying nuclear <span class="hlt">states</span> in 73Ga has recently been experimentally determined: a 1 /2- spin-parity for the <span class="hlt">ground</span> <span class="hlt">state</span> was measured in a laser spectroscopy experiment, while a Jπ=3 /2- level was observed in transfer reactions. This scenario is supported by Coulomb excitation studies, which set a limit for the <span class="hlt">energy</span> splitting of 0.8 keV. In this work, we report on the study of the excited structure of 73Ga populated in the β decay of 73Zn produced at ISOLDE, CERN. Using β -gated, γ -ray singles, and γ -γ coincidences, we have searched for <span class="hlt">energy</span> differences to try to delimit the <span class="hlt">ground-state</span> <span class="hlt">energy</span> splitting, providing a more stringent <span class="hlt">energy</span> difference limit. Three new half-lives of excited <span class="hlt">states</span> in 73Ga have been measured using the fast-timing method with LaBr3(Ce) detectors. From our study, we help clarify the excited structure of 73Ga and we extend the existing 73Zn decay to 73Ga with 8 new <span class="hlt">energy</span> levels and 35 γ transitions. We observe a 195-keV transition consistent with a γ ray de-exciting a short-lived <span class="hlt">state</span> in the β -decay parent 73Zn.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19910012263','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19910012263"><span><span class="hlt">Ground</span>-based testing of the dynamics of flexible space structures using <span class="hlt">band</span> mechanisms</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Yang, L. F.; Chew, Meng-Sang</p> <p>1991-01-01</p> <p>A suspension system based on a <span class="hlt">band</span> mechanism is studied to provide the free-free conditions for <span class="hlt">ground</span> based validation testing of flexible space structures. The <span class="hlt">band</span> mechanism consists of a noncircular disk with a convex profile, preloaded by torsional springs at its center of rotation so that static equilibrium of the test structure is maintained at any vertical location; the gravitational force will be directly counteracted during dynamic testing of the space structure. This noncircular disk within the suspension system can be configured to remain unchanged for test articles with the different weights as long as the torsional spring is replaced to maintain the originally designed frequency ratio of W/k sub s. Simulations of test articles which are modeled as lumped parameter as well as continuous parameter systems, are also presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..DMP.D1147E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..DMP.D1147E"><span>Toward Triplet <span class="hlt">Ground</span> <span class="hlt">State</span> NaLi Molecules</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ebadi, Sepehr; Jamison, Alan; Rvachov, Timur; Jing, Li; Son, Hyungmok; Jiang, Yijun; Zwierlein, Martin; Ketterle, Wolfgang</p> <p>2016-05-01</p> <p>The NaLi molecule is expected to have a long lifetime in the triplet <span class="hlt">ground-state</span> due to its fermionic nature, large rotational constant, and weak spin-orbit coupling. The triplet <span class="hlt">state</span> has both electric and magnetic dipole moments, affording unique opportunities in quantum simulation and ultracold chemistry. We have mapped the excited <span class="hlt">state</span> NaLi triplet potential by means of photoassociation spectroscopy. We report on this and our further progress toward the creation of the triplet <span class="hlt">ground-state</span> molecules using STIRAP. NSF, ARO-MURI, Samsung, NSERC.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29431681','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29431681"><span>Hartree-Fock implementation using a Laguerre-based wave function for the <span class="hlt">ground</span> <span class="hlt">state</span> and correlation <span class="hlt">energies</span> of two-electron atoms.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>King, Andrew W; Baskerville, Adam L; Cox, Hazel</p> <p>2018-03-13</p> <p>An implementation of the Hartree-Fock (HF) method using a Laguerre-based wave function is described and used to accurately study the <span class="hlt">ground</span> <span class="hlt">state</span> of two-electron atoms in the fixed nucleus approximation, and by comparison with fully correlated (FC) <span class="hlt">energies</span>, used to determine accurate electron correlation <span class="hlt">energies</span>. A variational parameter A is included in the wave function and is shown to rapidly increase the convergence of the <span class="hlt">energy</span>. The one-electron integrals are solved by series solution and an analytical form is found for the two-electron integrals. This methodology is used to produce accurate wave functions, <span class="hlt">energies</span> and expectation values for the helium isoelectronic sequence, including at low nuclear charge just prior to electron detachment. Additionally, the critical nuclear charge for binding two electrons within the HF approach is calculated and determined to be Z HF C =1.031 177 528.This article is part of the theme issue 'Modern theoretical chemistry'. © 2018 The Author(s).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1321722-heavily-doped-type-pbse-pbs-nanocrystals-using-ground-state-charge-transfer-from-cobaltocene','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1321722-heavily-doped-type-pbse-pbs-nanocrystals-using-ground-state-charge-transfer-from-cobaltocene"><span>Heavily doped n-type PbSe and PbS nanocrystals using <span class="hlt">ground-state</span> charge transfer from cobaltocene</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Koh, Weon-kyu; Koposov, Alexey Y.; Stewart, John T.; ...</p> <p>2013-06-18</p> <p>Colloidal nanocrystals (NCs) of lead chalcogenides are a promising class of tunable infrared materials for applications in devices such as photodetectors and solar cells. Such devices typically employ electronic materials in which charge carrier concentrations are manipulated through “doping;” however, persistent electronic doping of these NCs remains a challenge. In this paper, we demonstrate that heavily doped n-type PbSe and PbS NCs can be realized utilizing <span class="hlt">ground-state</span> electron transfer from cobaltocene. This allows injecting up to eight electrons per NC into the <span class="hlt">band</span>-edge <span class="hlt">state</span> and maintaining the doping level for at least a month at room temperature. Doping is confirmedmore » by inter- and intra-<span class="hlt">band</span> optical absorption, as well as by carrier dynamics. In conclusion, FET measurements of doped NC films and the demonstration of a p-n diode provide additional evidence that the developed doping procedure allows for persistent incorporation of electrons into the quantum-confined NC <span class="hlt">states</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=festival&pg=7&id=EJ1087349','ERIC'); return false;" href="https://eric.ed.gov/?q=festival&pg=7&id=EJ1087349"><span>Warm-Up Activities of Middle and High School <span class="hlt">Band</span> Directors Participating in <span class="hlt">State</span>-Level Concert <span class="hlt">Band</span> Assessments</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>Ward, Justin P.; Hancock, Carl B.</p> <p>2016-01-01</p> <p>The purpose of this study was to examine the warm-ups chosen by concert <span class="hlt">band</span> directors participating in <span class="hlt">state</span>-level performance assessments. We observed 29 middle and high school <span class="hlt">bands</span> and coded the frequency and duration of warm-up activities and behaviors. Results indicated that most <span class="hlt">bands</span> rehearsed music and played scales, long tones, and…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5402741','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5402741"><span>Identification of <span class="hlt">ground-state</span> spin ordering in antiferromagnetic transition metal oxides using the Ising model and a genetic algorithm</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Lee, Kyuhyun; Youn, Yong; Han, Seungwu</p> <p>2017-01-01</p> <p>Abstract We identify <span class="hlt">ground-state</span> collinear spin ordering in various antiferromagnetic transition metal oxides by constructing the Ising model from first-principles results and applying a genetic algorithm to find its minimum <span class="hlt">energy</span> <span class="hlt">state</span>. The present method can correctly reproduce the <span class="hlt">ground</span> <span class="hlt">state</span> of well-known antiferromagnetic oxides such as NiO, Fe2O3, Cr2O3 and MnO2. Furthermore, we identify the <span class="hlt">ground-state</span> spin ordering in more complicated materials such as Mn3O4 and CoCr2O4. PMID:28458746</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040141448&hterms=zinc&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dzinc','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040141448&hterms=zinc&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dzinc"><span>A semiempirical study for the <span class="hlt">ground</span> and excited <span class="hlt">states</span> of free-base and zinc porphyrin-fullerene dyads</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Parusel, A. B.</p> <p>2000-01-01</p> <p>The <span class="hlt">ground</span> and excited <span class="hlt">states</span> of a covalently linked porphyrin-fullerene dyad in both its free-base and zinc forms (D. Kuciauskas et al., J. Phys. Chem. 100 (1996) 15926) have been investigated by semiempirical methods. The excited-<span class="hlt">state</span> properties are discussed by investigation of the character of the molecular orbitals. All frontier MOs are mainly localized on either the donor or the acceptor subunit. Thus, the absorption spectra of both systems are best described as the sum of the spectra of the single components. The experimentally observed spectra are well reproduced by the theoretical computations. Both molecules undergo efficient electron transfer in polar but not in apolar solvents. This experimental finding is explained theoretically by explicitly considering solvent effects. The tenth excited <span class="hlt">state</span> in the gas phase is of charge-separated character where an electron is transferred from the porphyrin donor to the fullerene acceptor subunit. This <span class="hlt">state</span> is stabilized in <span class="hlt">energy</span> in polar solvents due to its large formal dipole moment. The stabilization <span class="hlt">energy</span> for an apolar environment such as benzene is not sufficient to lower this <span class="hlt">state</span> to become the first excited singlet <span class="hlt">state</span>. Thus, no electron transfer is observed, in agreement with experiment. In a polar environment such as acetonitrile, the charge-separated <span class="hlt">state</span> becomes the S, <span class="hlt">state</span> and electron transfer takes place, as observed experimentally. The flexible single bond connecting both the donor and acceptor subunits allows free rotation by ca. +/- 30 degrees about the optimized <span class="hlt">ground-state</span> conformation. For the charge-separated <span class="hlt">state</span> this optimized geometry has a maximum dipole moment. The geometry of the charge-separated <span class="hlt">state</span> thus does not change relatively to the <span class="hlt">ground-state</span> conformation. The electron-donating properties of porphyrin are enhanced in the zinc derivative due to a reduced porphyrin HOMO-LUMO <span class="hlt">energy</span> gap. This yields a lower <span class="hlt">energy</span> for the charge-separated <span class="hlt">state</span> compared to the free</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1399117-methodology-energy-strategy-prescreen-feasibility-ground-source-heat-pump-systems-residential-commercial-buildings-united-states','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1399117-methodology-energy-strategy-prescreen-feasibility-ground-source-heat-pump-systems-residential-commercial-buildings-united-states"><span>Methodology for <span class="hlt">energy</span> strategy to prescreen the feasibility of <span class="hlt">Ground</span> Source Heat Pump systems in residential and commercial buildings in the United <span class="hlt">States</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Cho, Soolyeon; Ray, Saurabh; Im, Piljae; ...</p> <p>2017-09-21</p> <p>Geothermal resources have potential to reduce dependence on fossil fuels. The viability of geothermal heat pumps or <span class="hlt">ground</span> source heat pumps (GSHPs) is significant as a potential alternative <span class="hlt">energy</span> source with substantial savings potential. While the prospect of these systems is promising for <span class="hlt">energy</span> efficiency, careful feasibility analysis is required before implementation. Here, this paper presents the results of evaluation of the application feasibility for GSHPs in buildings across seven climate zones in three United <span class="hlt">States</span> regions. A comprehensive methodology is developed to measure the integrated feasibility of GSHPs using compiled data for <span class="hlt">energy</span> use intensity, <span class="hlt">energy</span> cost and designmore » parameters. Four different feasibility metrics are utilized: <span class="hlt">ground</span> temperature, outdoor weather condition, <span class="hlt">energy</span> savings potential, and cost benefits. For each metric, a corresponding feasibility score system is developed. The defined integrated feasibility score classifies the locations into five different feasibility levels ranging from Fair (0–20), Moderate (21–40), Good (41–60), High (61–80), and Very High (81–100). Conclusions show the GSHP feasibility level is High for 3 sites, Good for 8 sites and Moderate for 4 sites. Through the methodology, it is possible to develop a practical <span class="hlt">energy</span> strategy for more economic and sustainable GSHP systems at an early design stage in the various viewpoints of geometries, climate conditions, operational factors, and <span class="hlt">energy</span> costs.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1399117-methodology-energy-strategy-prescreen-feasibility-ground-source-heat-pump-systems-residential-commercial-buildings-united-states','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1399117-methodology-energy-strategy-prescreen-feasibility-ground-source-heat-pump-systems-residential-commercial-buildings-united-states"><span>Methodology for <span class="hlt">energy</span> strategy to prescreen the feasibility of <span class="hlt">Ground</span> Source Heat Pump systems in residential and commercial buildings in the United <span class="hlt">States</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>Cho, Soolyeon; Ray, Saurabh; Im, Piljae</p> <p></p> <p>Geothermal resources have potential to reduce dependence on fossil fuels. The viability of geothermal heat pumps or <span class="hlt">ground</span> source heat pumps (GSHPs) is significant as a potential alternative <span class="hlt">energy</span> source with substantial savings potential. While the prospect of these systems is promising for <span class="hlt">energy</span> efficiency, careful feasibility analysis is required before implementation. Here, this paper presents the results of evaluation of the application feasibility for GSHPs in buildings across seven climate zones in three United <span class="hlt">States</span> regions. A comprehensive methodology is developed to measure the integrated feasibility of GSHPs using compiled data for <span class="hlt">energy</span> use intensity, <span class="hlt">energy</span> cost and designmore » parameters. Four different feasibility metrics are utilized: <span class="hlt">ground</span> temperature, outdoor weather condition, <span class="hlt">energy</span> savings potential, and cost benefits. For each metric, a corresponding feasibility score system is developed. The defined integrated feasibility score classifies the locations into five different feasibility levels ranging from Fair (0–20), Moderate (21–40), Good (41–60), High (61–80), and Very High (81–100). Conclusions show the GSHP feasibility level is High for 3 sites, Good for 8 sites and Moderate for 4 sites. Through the methodology, it is possible to develop a practical <span class="hlt">energy</span> strategy for more economic and sustainable GSHP systems at an early design stage in the various viewpoints of geometries, climate conditions, operational factors, and <span class="hlt">energy</span> costs.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/4352889-isomer-rotational-bands-sup-os','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/4352889-isomer-rotational-bands-sup-os"><span>A 6.1 s isomer and rotational <span class="hlt">bands</span> in $sup 192$Os</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>Pakkanen, A.; Heikkinen, D.W.</p> <p></p> <p>A 6.1 plus or minus 0.2 s activity has been observed when natural Os targets were bombarded with 14.5 MeV neutrons. The activity is assigned to the decay of a high-spin isomer in /sup 192/Os at 2015.4 keV, which is depopulated by M2 and E3 transitions. Singles and coincidence gamma -ray spectra have allowed the identification of seven new <span class="hlt">states</span> in /sup 192/Os. Several of these levels have been placed in either the <span class="hlt">ground</span>- <span class="hlt">state</span> or gamma -vibrational <span class="hlt">bands</span>, which are strongly mixed. Excitation <span class="hlt">energies</span>, B(E2) ratios for these <span class="hlt">bands</span> are compared with different theoretical models. (auth) It is shownmore » that, if one uses single-particle <span class="hlt">energies</span> from experiment and a delta residual interaction, it is not possible to obtain the <span class="hlt">energy</span> of the giant dipole and spurious <span class="hlt">states</span> of /sup 208/Pb, and at the same time obtain reasonable results for the low-lying two- particle spectra of /sup 210/Pb or /sup 210/Po. Related to the above problem, the isobaric analog <span class="hlt">state</span> of /sup 208/Pb (in /sup 208/Bi) comes much too low in calculations using realistic interactions. It is noted that the above difficulties can be overcome, phenomenologically at least, by adding to the effective interaction some longrange repulsive components. The Bansal- French and the Schiffer interactions are examples of these; however, the dipole--dipole component of the Schiffer interaction gives much too large a splitting between the dipole <span class="hlt">state</span> and spurious <span class="hlt">state</span>. (auth)« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25539153','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25539153"><span>Theoretical and Experimental Photoelectron Spectroscopy Characterization of the <span class="hlt">Ground</span> <span class="hlt">State</span> of Thymine Cation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Majdi, Youssef; Hochlaf, Majdi; Pan, Yi; Lau, Kai-Chung; Poisson, Lionel; Garcia, Gustavo A; Nahon, Laurent; Al-Mogren, Muneerah Mogren; Schwell, Martin</p> <p>2015-06-11</p> <p>We report on the vibronic structure of the <span class="hlt">ground</span> <span class="hlt">state</span> X̃(2)A″ of the thymine cation, which has been measured using a threshold photoelectron photoion coincidence technique and vacuum ultraviolet synchrotron radiation. The threshold photoelectron spectrum, recorded over ∼0.7 eV above the ionization potential (i.e., covering the whole <span class="hlt">ground</span> <span class="hlt">state</span> of the cation) shows rich vibrational structure that has been assigned with the help of calculated anharmonic modes of the <span class="hlt">ground</span> electronic cation <span class="hlt">state</span> at the PBE0/aug-cc-pVDZ level of theory. The adiabatic ionization <span class="hlt">energy</span> has been experimentally determined as AIE = 8.913 ± 0.005 eV, in very good agreement with previous high resolution results. The corresponding theoretical value of AIE = 8.917 eV has been calculated in this work with the explicitly correlated method/basis set (R)CCSD(T)-F12/cc-pVTZ-F12, which validates the theoretical approach and benchmarks its accuracy for future studies of medium-sized biological molecules.</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 electron 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 <span class="hlt">stated</span> 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 electron 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 <span class="hlt">states</span> 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 <span class="hlt">ground</span> <span class="hlt">state</span> (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 <span class="hlt">ground</span> <span class="hlt">state</span> bandstructure calculation. The method is based on integer electron systems, fractional electron systems (an ensemble of N- and (N + 1)-electron systems) and the derivative discontinuity are not invoked.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011JMoSp.268..211M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011JMoSp.268..211M"><span>Fourier transform synchrotron spectroscopy of torsional and CO-stretching <span class="hlt">bands</span> of CH 3 17 OH</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moruzzi, G.; Murphy, R. J.; Vos, J.; Lees, R. M.; Predoi-Cross, A.; Billinghurst, B. E.</p> <p>2011-07-01</p> <p>The Fourier transform spectrum of the CH 317OH isotopologue of methanol has been recorded in the 65-1200 cm -1 spectral region at a resolution of 0.00096 cm -1 using synchrotron source radiation at the Canadian Light Source. Here we present an extension to higher torsional <span class="hlt">states</span> of our investigation of the torsion-rotation transitions within the small-amplitude vibrational <span class="hlt">ground</span> <span class="hlt">state</span>, now including assignments of more than 16 500 lines involving quantum numbers in the ranges v t ⩽ 3, J ⩽ 30 and | K| ⩽ 12, as well as a study of the strong CO-stretching <span class="hlt">band</span> centered at 1020 cm -1. <span class="hlt">Energy</span> term values have been determined for assigned <span class="hlt">ground</span> and CO-stretching levels by use of the Ritz program, and have been fitted to series expansions in powers of J( J + 1) to determine substate origins and effective B values. Several Fermi anharmonic and Coriolis level-crossing resonances coupling the CO stretch with high torsional <span class="hlt">ground-state</span> levels have been identified and characterized. The study is motivated by astrophysical applications, with a principal aim being the compilation of an extensive set of <span class="hlt">energy</span> term values to permit prediction of astronomically observable sub-millimetre transitions to within an uncertainty of a few MHz.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JMoSp.315...10D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JMoSp.315...10D"><span>High-resolution Fourier transform infrared synchrotron spectroscopy of the NO2 in-plane rock <span class="hlt">band</span> of nitromethane</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dawadi, Mahesh B.; Twagirayezu, Sylvestre; Perry, David S.; Billinghurst, Brant E.</p> <p>2015-09-01</p> <p>The high-resolution rotationally resolved Fourier-transform infrared spectrum of the NO2 in-plane rock <span class="hlt">band</span> (440-510 cm-1) of nitromethane (CH3NO2) has been recorded using the Far-Infrared Beamline at the Canadian Light Source, with a resolution of 0.00096 cm-1. About 1773 transitions reaching the upper <span class="hlt">state</span> levels m‧ = 0; Ka‧ ⩽ 7;J‧ ⩽ 50 have been assigned using an automated <span class="hlt">ground-state</span> combination difference program together with the traditional Loomis-Wood approach. These data from the lowest torsional <span class="hlt">state</span>, m‧ = 0, were fit using the six-fold torsion-rotation program developed by Ilyushin et al. (2010). The analysis reveals that the rotational <span class="hlt">energy</span> level structure in the upper vibrational <span class="hlt">state</span> is similar to that of the <span class="hlt">ground</span> vibrational <span class="hlt">state</span>, but the sign and magnitude of high-order constants are significantly changed suggesting the presence of multiple perturbations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017NuPhA.968...48J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017NuPhA.968...48J"><span>Intrinsic properties of high-spin <span class="hlt">band</span> structures in triaxial nuclei</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jehangir, S.; Bhat, G. H.; Sheikh, J. A.; Palit, R.; Ganai, P. A.</p> <p>2017-12-01</p> <p>The <span class="hlt">band</span> structures of 68,70Ge, 128,130,132,134Ce and 132,134,136,138Nd are investigated using the triaxial projected shell model (TPSM) approach. These nuclei depict forking of the <span class="hlt">ground-state</span> <span class="hlt">band</span> into several s-<span class="hlt">bands</span> and in some cases, both the lowest two observed s-<span class="hlt">bands</span> depict neutron or proton character. It was discussed in our earlier work that this anomalous behaviour can be explained by considering γ-<span class="hlt">bands</span> based on two-quasiparticle configurations. As the parent <span class="hlt">band</span> and the γ-<span class="hlt">band</span> built on it have the same intrinsic structure, g-factors of the two <span class="hlt">bands</span> are expected to be similar. In the present work, we have undertaken a detailed investigation of g-factors for the excited <span class="hlt">band</span> structures of the studied nuclei and the available data for a few high-spin <span class="hlt">states</span> are shown to be in fair agreement with the predicted values.</p> </li> <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/1981SSCom..39..831K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1981SSCom..39..831K"><span>Positron and electron <span class="hlt">energy</span> <span class="hlt">bands</span> in several ionic crystals using restricted Hartree-Fock method</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kunz, A. B.; Waber, J. T.</p> <p>1981-08-01</p> <p>Using a restricted Hartree-Fock formalism and suitably localized and symmetrized wave functions, both the positron and electron <span class="hlt">energy</span> <span class="hlt">bands</span> were calculated for NaF, MgO and NiO. The lowest positron <span class="hlt">state</span> 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.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26918977','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26918977"><span><span class="hlt">Ground</span> <span class="hlt">State</span> of the Universe and the Cosmological Constant. A Nonperturbative Analysis.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Husain, Viqar; Qureshi, Babar</p> <p>2016-02-12</p> <p>The physical Hamiltonian of a gravity-matter system depends on the choice of time, with the vacuum naturally identified as its <span class="hlt">ground</span> <span class="hlt">state</span>. We study the expanding Universe with scalar field in the volume time gauge. We show that the vacuum <span class="hlt">energy</span> density computed from the resulting Hamiltonian is a nonlinear function of the cosmological constant and time. This result provides a new perspective on the relation between time, the cosmological constant, and vacuum <span class="hlt">energy</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20070015992&hterms=atom&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Datom','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20070015992&hterms=atom&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Datom"><span>Formation of Triplet Positron-helium Bound <span class="hlt">State</span> by Stripping of Positronium Atoms in Collision with <span class="hlt">Ground</span> <span class="hlt">State</span> Helium</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Drachman, Richard J.</p> <p>2006-01-01</p> <p>Formation of triplet positron-helium bound <span class="hlt">state</span> by stripping of positronium atoms in collision with <span class="hlt">ground</span> <span class="hlt">state</span> helium JOSEPH DI RlENZI, College of Notre Dame of Maryland, RICHARD J. DRACHMAN, NASA/Goddard Space Flight Center - The system consisting of a positron and a helium atom in the triplet <span class="hlt">state</span> e(+)He(S-3)(sup e) was conjectured long ago to be stable [1]. Its stability has recently been established rigorously [2], and the values of the <span class="hlt">energies</span> of dissociation into the <span class="hlt">ground</span> <span class="hlt">states</span> of Ps and He(+) have also been reported [3] and [4]. We have evaluated the cross-section for this system formed by radiative attachment of a positron in triplet He <span class="hlt">state</span> and found it to be small [5]. The mechanism of production suggested here should result in a larger cross-section (of atomic size) which we are determining using the Born approximation with simplified initial and final wave functions.</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/2017APS..MARX48003C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..MARX48003C"><span>Exact <span class="hlt">ground</span> <span class="hlt">states</span> for the nearest neighbor quantum XXZ model on the kagome and other lattices with triangular motifs at Jz /Jxy = - 1 / 2</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Changlani, Hitesh; Kumar, Krishna; Kochkov, Dmitrii; Fradkin, Eduardo; Clark, Bryan</p> <p></p> <p>We report the existence of a quantum macroscopically degenerate <span class="hlt">ground</span> <span class="hlt">state</span> manifold on the nearest neighbor XXZ model on the kagome lattice at the point Jz /Jxy = - 1 / 2 . On many lattices with triangular motifs (including the kagome, sawtooth, icosidodecahedron and Shastry-Sutherland lattice for a certain choice of couplings) this Hamiltonian is found to be frustration-free with exact <span class="hlt">ground</span> <span class="hlt">states</span> which correspond to three-colorings of these lattices. Several results also generalize to the case of variable couplings and to other motifs (albeit with possibly more complex Hamiltonians). The degenerate manifold on the kagome lattice corresponds to a ''many-body flat <span class="hlt">band</span>'' of interacting hard-core bosons; and for the one boson case our results also explain the well-known non-interacting flat <span class="hlt">band</span>. On adding realistic perturbations, <span class="hlt">state</span> selection in this manifold of quantum many-body <span class="hlt">states</span> is discussed along with the implications for the phase diagram of the kagome lattice antiferromagnet. supported by DE-FG02-12ER46875, DMR 1408713, DE-FG02-08ER46544.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JChPh.146l4308G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JChPh.146l4308G"><span>Molecular symmetry group analysis of the low-wavenumber torsions and vibration-torsions in the S1 <span class="hlt">state</span> and <span class="hlt">ground</span> <span class="hlt">state</span> cation of p-xylene: An investigation using resonance-enhanced multiphoton ionization (REMPI) and zero-kinetic-<span class="hlt">energy</span> (ZEKE) spectroscopy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gardner, Adrian M.; Tuttle, William D.; Groner, Peter; Wright, Timothy G.</p> <p>2017-03-01</p> <p>For the first time, a molecular symmetry group (MSG) analysis has been undertaken in the investigation of the electronic spectroscopy of p-xylene (p-dimethylbenzene). Torsional and vibration-torsional (vibtor) levels in the S1 <span class="hlt">state</span> and <span class="hlt">ground</span> <span class="hlt">state</span> of the cation of p-xylene are investigated using resonance-enhanced multiphoton ionization (REMPI) and zero-kinetic-<span class="hlt">energy</span> (ZEKE) spectroscopy. In the present work, we concentrate on the 0-350 cm-1 region, where there are a number of torsional and vibtor <span class="hlt">bands</span> and we discuss the assignment of this region. In Paper II [W. D. Tuttle et al., J. Chem. Phys. 146, 124309 (2017)], we examine the 350-600 cm-1 region where vibtor levels are observed as part of a Fermi resonance. The similarity of much of the observed spectral activity to that in the related substituted benzenes, toluene and para-fluorotoluene, is striking, despite the different symmetries. The discussion necessitates a consideration of the MSG of p-xylene, which has been designated G72, but we shall also designate [{3,3}]D2h and we include the symmetry operations, character table, and direct product table for this. We also discuss the symmetries of the internal rotor (torsional) levels and the selection rules for the particular electronic transition of p-xylene investigated here.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19770062429&hterms=laser+darpa&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dlaser%2Bdarpa','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19770062429&hterms=laser+darpa&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dlaser%2Bdarpa"><span>Measurements of copper <span class="hlt">ground-state</span> and metastable level population densities in a copper-chloride laser</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Nerheim, N. M.</p> <p>1977-01-01</p> <p>The population densities of both the <span class="hlt">ground</span> and the 2D(5/2) metastable <span class="hlt">states</span> of copper atoms in a double-pulsed copper-chloride laser are correlated with laser <span class="hlt">energy</span> as a function of time after the dissociation current pulse. Time-resolved density variations of the <span class="hlt">ground</span> and excited copper atoms were derived from measurements of optical absorption at 324.7 and 510.6 nm, respectively, over a wide range of operating conditions in laser tubes with diameters of 4 to 40 mm. The minimum delay between the two current pulses at which lasing was observed is shown to be a function of the initial density and subsequent decay of the metastable <span class="hlt">state</span>. Similarly, the maximum delay is shown to be a function of the initial density and decay of the <span class="hlt">ground</span> <span class="hlt">state</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5062575','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5062575"><span><span class="hlt">Ground-state</span> oxygen holes and the metal–insulator transition in the negative charge-transfer rare-earth nickelates</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Bisogni, Valentina; Catalano, Sara; Green, Robert J.; Gibert, Marta; Scherwitzl, Raoul; Huang, Yaobo; Strocov, Vladimir N.; Zubko, Pavlo; Balandeh, Shadi; Triscone, Jean-Marc; Sawatzky, George; Schmitt, Thorsten</p> <p>2016-01-01</p> <p>The metal–insulator transition and the intriguing physical properties of rare-earth perovskite nickelates have attracted considerable attention in recent years. Nonetheless, a complete understanding of these materials remains elusive. Here we combine X-ray absorption and resonant inelastic X-ray scattering (RIXS) spectroscopies to resolve important aspects of the complex electronic structure of rare-earth nickelates, taking NdNiO3 thin film as representative example. The unusual coexistence of bound and continuum excitations observed in the RIXS spectra provides strong evidence for abundant oxygen holes in the <span class="hlt">ground</span> <span class="hlt">state</span> of these materials. Using cluster calculations and Anderson impurity model interpretation, we show that distinct spectral signatures arise from a Ni 3d8 configuration along with holes in the oxygen 2p valence <span class="hlt">band</span>, confirming suggestions that these materials do not obey a conventional positive charge-transfer picture, but instead exhibit a negative charge-transfer <span class="hlt">energy</span> in line with recent models interpreting the metal–insulator transition in terms of bond disproportionation. PMID:27725665</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1992SSCom..83..871F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1992SSCom..83..871F"><span>A note on AB INITIO semiconductor <span class="hlt">band</span> structures</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fiorentini, Vincenzo</p> <p>1992-09-01</p> <p>We point out that only the internal features of the DFT ab initio theoretical picture of a crystal should be used in a consistent ab initio calculation of the <span class="hlt">band</span> structure. As a consequence, we show that <span class="hlt">ground-state</span> <span class="hlt">band</span> structure calculations should be performed for the system in equilibrium at zero pressure, i.e. at the computed equilibrium cell volume ω th. Examples of consequences of this attitude are considered.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2000STIN...0171553M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2000STIN...0171553M"><span>Mars Global Surveyor Ka-<span class="hlt">Band</span> Frequency Data Analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Morabito, D.; Butman, S.; Shambayati, S.</p> <p>2000-01-01</p> <p>The Mars Global Surveyor (MGS) spacecraft, launched on November 7, 1996, carries an experimental space-to-<span class="hlt">ground</span> telecommunications link at Ka-<span class="hlt">band</span> (32 GHz) along with the primary X-<span class="hlt">band</span> (8.4 GHz) downlink. The signals are simultaneously transmitted from a 1.5-in diameter parabolic high gain antenna (HGA) on MGS and received by a beam-waveguide (BWG) R&D 34-meter antenna located in NASA's Goldstone Deep Space Network (DSN) complex near Barstow, California. The projected 5-dB link advantage of Ka-<span class="hlt">band</span> relative to X-<span class="hlt">band</span> was confirmed in previous reports using measurements of MGS signal strength data acquired during the first two years of the link experiment from December 1996 to December 1998. Analysis of X-<span class="hlt">band</span> and Ka-<span class="hlt">band</span> frequency data and difference frequency (fx-fka)/3.8 data will be presented here. On board the spacecraft, a low-power sample of the X-<span class="hlt">band</span> downlink from the transponder is upconverted to 32 GHz, the Ka-<span class="hlt">band</span> frequency, amplified to I-W using a Solid <span class="hlt">State</span> Power Amplifier, and radiated from the dual X/Ka HGA. The X-<span class="hlt">band</span> signal is amplified by one of two 25 W TWTAs. An upconverter first downconverts the 8.42 GHz X-<span class="hlt">band</span> signal to 8 GHz and then multiplies using a X4 multiplier producing the 32 GHz Ka-<span class="hlt">band</span> frequency. The frequency source selection is performed by an RF switch which can be commanded to select a VCO (Voltage Controlled Oscillator) or USO (Ultra-Stable Oscillator) reference. The Ka-<span class="hlt">band</span> frequency can be either coherent with the X-<span class="hlt">band</span> downlink reference or a hybrid combination of the USO and VCO derived frequencies. The data in this study were chosen such that the Ka-<span class="hlt">band</span> signal is purely coherent with the X-<span class="hlt">band</span> signal, that is the downconverter is driven by the same frequency source as the X-<span class="hlt">band</span> downlink). The <span class="hlt">ground</span> station used to acquire the data is DSS-13, a 34-meter BWG antenna which incorporates a series of mirrors inside beam waveguide tubes which guide the <span class="hlt">energy</span> to a subterranean pedestal room, providing a stable environment</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19980201487&hterms=diversity&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Ddiversity','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19980201487&hterms=diversity&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Ddiversity"><span>Narrow Angle Diversity using ACTS Ka-<span class="hlt">band</span> Signal with Two USAT <span class="hlt">Ground</span> Stations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kalu, A.; Emrich, C.; Ventre, J.; Wilson, W.; Acosta, R.</p> <p>1998-01-01</p> <p>Two ultra small aperture terminal (USAT) <span class="hlt">ground</span> stations, separated by 1.2 km in a narrow angle diversity configuration, received a continuous Ka-<span class="hlt">band</span> tone sent from Cleveland Link Evaluation Terminal (LET). The signal was transmitted to the USAT <span class="hlt">ground</span> stations via NASA's Advanced Communications Technology Satellite (ACTS) steerable beam. Received signal power at the two sites was measured and analyzed. A dedicated datalogger at each site recorded time-of-tip data from tipping bucket rain gauges, providing rain amount and instantaneous rain rate. WSR-88D data was also obtained for the collection period. Eleven events with <span class="hlt">ground</span>-to-satellite slant-path precipitation and resultant signal attenuation were observed during the data collection period. Fade magnitude and duration were compared at the two sites and diversity gain was calculated. These results exceeded standard diversity gain model predictions by several decibels. Rain statistics from tipping bucket data and from radar data were also compared to signal attenuation. The nature of Florida's subtropical rainfall, specifically its impact on signal attenuation at the sites, was addressed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3216574','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3216574"><span>Solving Quantum <span class="hlt">Ground-State</span> Problems with Nuclear Magnetic Resonance</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Li, Zhaokai; Yung, Man-Hong; Chen, Hongwei; Lu, Dawei; Whitfield, James D.; Peng, Xinhua; Aspuru-Guzik, Alán; Du, Jiangfeng</p> <p>2011-01-01</p> <p>Quantum <span class="hlt">ground-state</span> problems are computationally hard problems for general many-body Hamiltonians; there is no classical or quantum algorithm known to be able to solve them efficiently. Nevertheless, if a trial wavefunction approximating the <span class="hlt">ground</span> <span class="hlt">state</span> is available, as often happens for many problems in physics and chemistry, a quantum computer could employ this trial wavefunction to project the <span class="hlt">ground</span> <span class="hlt">state</span> by means of the phase estimation algorithm (PEA). We performed an experimental realization of this idea by implementing a variational-wavefunction approach to solve the <span class="hlt">ground-state</span> problem of the Heisenberg spin model with an NMR quantum simulator. Our iterative phase estimation procedure yields a high accuracy for the eigenenergies (to the 10−5 decimal digit). The <span class="hlt">ground-state</span> fidelity was distilled to be more than 80%, and the singlet-to-triplet switching near the critical field is reliably captured. This result shows that quantum simulators can better leverage classical trial wave functions than classical computers PMID:22355607</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JMoSp.347...19T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JMoSp.347...19T"><span>High-resolution far-infrared synchrotron FTIR spectrum of the ν12 <span class="hlt">band</span> of formamide-d1 (DCONH2)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tan, T. L.; Wu, Q. Y.; Ng, L. L.; Appadoo, Dominique R. T.; McNaughton, Don</p> <p>2018-05-01</p> <p>The spectrum of the ν12 <span class="hlt">band</span> of formamide-d1 (DCONH2) was recorded using a synchrotron Fourier transform infrared (FTIR) spectrometer coupled to the Australian Synchrotron THz/Far-IR beamline, with an unapodized resolution of 0.00096 cm-1 in the 350-210 cm-1 region. For the first time, rovibrational constants up to five quartic and two sextic terms were derived for the v12 = 1 <span class="hlt">state</span> through the fitting of a total of 2072 far-infrared transitions using Watson's A-reduced Hamiltonian in the Ir representation with a root-mean-square (rms) deviation of 0.000073 cm-1. The <span class="hlt">band</span> centre of the ν12 <span class="hlt">band</span> of DCONH2 was found to be 289.3327553(47) cm-1 although the experimental uncertainty was limited to ±0.0002 cm-1. <span class="hlt">Ground</span> <span class="hlt">state</span> rovibrational constants of DCONH2 up to five quartic and two sextic constants were derived from a fit of 847 <span class="hlt">ground</span> <span class="hlt">state</span> combination differences (GSCDs) obtained from the infrared transitions of the ν12 <span class="hlt">band</span>, together with 6 previously reported microwave transitions, with a rms deviation of 0.000108 cm-1. The <span class="hlt">ground</span> <span class="hlt">state</span> rotational constants (A, B, and C) of DCONH2 were improved while the <span class="hlt">ground</span> <span class="hlt">state</span> centrifugal distortion constants were accurately obtained for the first time. The uncertainty of the measured infrared lines was estimated to be ±0.0002 cm-1. From the <span class="hlt">ground</span> <span class="hlt">state</span> rotational constants, the inertial defect of DCONH2 was calculated to be 0.0169412(11) uÅ2.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhRvC..96c4321G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvC..96c4321G"><span>Outstanding problems in the <span class="hlt">band</span> structures of 152Sm</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gupta, J. B.; Hamilton, J. H.</p> <p>2017-09-01</p> <p>The recent data on B (E 2 ) values, deduced from the multi-Coulex excitation of the low spin <span class="hlt">states</span> in the decay of 152Sm, and other experimental findings in the last two decades are compared with the predictions from the microscopic dynamic pairing plus quadrupole model of Kumar and Baranger. The 1292.8 keV 2+ <span class="hlt">state</span> is assigned to the 03 + <span class="hlt">band</span>, and the K =2 assignment of the 1769 keV 2+ <span class="hlt">state</span> is confirmed. The anomaly of the shape coexistence of the assumed spherical β <span class="hlt">band</span> versus the deformed <span class="hlt">ground</span> <span class="hlt">band</span> is resolved. The values from the critical point symmetry X(5) support the collective character of the β <span class="hlt">band</span>. The problem with the two-term interacting boson model Hamiltonian in predicting β and γ <span class="hlt">bands</span> in 152Sm leads to interesting consequences. The collective features of the second excited Kπ=03 + <span class="hlt">band</span> are preferred over the "pairing isomer" view. Also the multiphonon nature of the higher lying Kπ=22 +β γ <span class="hlt">band</span> and Kπ=4+ <span class="hlt">band</span> are illustrated vis-à-vis the new data and the nuclear structure theory.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PhyA..444..397S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhyA..444..397S"><span>Analysis of <span class="hlt">ground</span> <span class="hlt">state</span> in random bipartite matching</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shi, Gui-Yuan; Kong, Yi-Xiu; Liao, Hao; Zhang, Yi-Cheng</p> <p>2016-02-01</p> <p>Bipartite matching problems emerge in many human social phenomena. In this paper, we study the <span class="hlt">ground</span> <span class="hlt">state</span> of the Gale-Shapley model, which is the most popular bipartite matching model. We apply the Kuhn-Munkres algorithm to compute the numerical <span class="hlt">ground</span> <span class="hlt">state</span> of the model. For the first time, we obtain the number of blocking pairs which is a measure of the system instability. We also show that the number of blocking pairs formed by each person follows a geometric distribution. Furthermore, we study how the connectivity in the bipartite matching problems influences the instability of the <span class="hlt">ground</span> <span class="hlt">state</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22415934-long-range-interactions-between-polar-bialkali-ground-state-molecules-arbitrary-vibrational-levels','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22415934-long-range-interactions-between-polar-bialkali-ground-state-molecules-arbitrary-vibrational-levels"><span>Long-range interactions between polar bialkali <span class="hlt">ground-state</span> molecules in arbitrary vibrational levels</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>Vexiau, R.; Lepers, M., E-mail: maxence.lepers@u-psud.fr; Aymar, M.</p> <p>2015-06-07</p> <p>We have calculated the isotropic C{sub 6} coefficients characterizing the long-range van der Waals interaction between two identical heteronuclear alkali-metal diatomic molecules in the same arbitrary vibrational level of their <span class="hlt">ground</span> electronic <span class="hlt">state</span> X{sup 1}Σ{sup +}. We consider the ten species made up of {sup 7}Li, {sup 23}Na, {sup 39}K, {sup 87}Rb, and {sup 133}Cs. Following our previous work [Lepers et al., Phys. Rev. A 88, 032709 (2013)], we use the sum-over-<span class="hlt">state</span> formula inherent to the second-order perturbation theory, composed of the contributions from the transitions within the <span class="hlt">ground</span> <span class="hlt">state</span> levels, from the transition between <span class="hlt">ground-state</span> and excited <span class="hlt">state</span> levels,more » and from a crossed term. These calculations involve a combination of experimental and quantum-chemical data for potential <span class="hlt">energy</span> curves and transition dipole moments. We also investigate the case where the two molecules are in different vibrational levels and we show that the Moelwyn-Hughes approximation is valid provided that it is applied for each of the three contributions to the sum-over-<span class="hlt">state</span> formula. Our results are particularly relevant in the context of inelastic and reactive collisions between ultracold bialkali molecules in deeply bound or in Feshbach levels.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..MARB27005B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..MARB27005B"><span>Revealing the electronic <span class="hlt">ground</span> <span class="hlt">state</span> of ReNiO3 combining Ni-L3 x-ray absorption and resonant inelastic x-ray scattering</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bisogni, Valentina; Catalano, Sara; Green, Robert; Gibert, Marta; Scherwitzl, Raoul; Huang, Yaobo; Balandesh, Shadi; Strocov, Vladimir N.; Zubko, Pavlo; Sawatzky, George; Triscone, Jean-Marc; Schmitt, Thorsten</p> <p></p> <p>Rare-earth nickelates ReNiO3 attract a lot of interest thanks to their intriguing physical properties like sharp metal to insulator transition, unusual magnetic order and expected superconductivity in nickelate-based heterostructures. Full understanding of these materials, however, is hampered by the difficulties in describing their electronic <span class="hlt">ground</span> <span class="hlt">state</span> (GS). Taking a NdNiO3 thin film as a representative example, we reveal with x-ray absorption and resonant inelastic x-ray scattering unusual coexistence of bound and continuum excitations, providing strong evidence for abundant O 2p holes in the GS of these materials. Using an Anderson impurity model interpretation, we show that these distinct spectral signatures arise from a Ni 3d8 configuration along with holes in the O 2p valence <span class="hlt">band</span>, confirming suggestions that these materials exhibit a negative charge-transfer <span class="hlt">energy</span>, with O 2p <span class="hlt">states</span> extending across the Fermi level.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910030254&hterms=1575&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3D%2526%25231575','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910030254&hterms=1575&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3D%2526%25231575"><span><span class="hlt">Ground</span> <span class="hlt">states</span> of partially connected binary neural networks</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Baram, Yoram</p> <p>1990-01-01</p> <p>Neural networks defined by outer products of vectors over (-1, 0, 1) are considered. Patterns over (-1, 0, 1) define by their outer products partially connected neural networks consisting of internally strongly connected, externally weakly connected subnetworks. Subpatterns over (-1, 1) define subnetworks, and their combinations that agree in the common bits define permissible words. It is shown that the permissible words are locally stable <span class="hlt">states</span> of the network, provided that each of the subnetworks stores mutually orthogonal subwords, or, at most, two subwords. It is also shown that when each of the subnetworks stores two mutually orthogonal binary subwords at most, the permissible words, defined as the combinations of the subwords (one corresponding to each subnetwork), that agree in their common bits are the unique <span class="hlt">ground</span> <span class="hlt">states</span> of the associated <span class="hlt">energy</span> function.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013mss..confETJ03A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013mss..confETJ03A"><span>Accurate Determination of Rotational <span class="hlt">Energy</span> Levels in the <span class="hlt">Ground</span> <span class="hlt">State</span> of ^{12}CH_4</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Abe, M.; Iwakuni, K.; Okubo, S.; Sasada, H.</p> <p>2013-06-01</p> <p>We have measured absolute frequencies of saturated absorption of 183 allowed and 21 forbidden transitions in the νb{3} <span class="hlt">band</span> of ^{12}CH_4 using an optical comb-referenced difference-frequency-generation spectrometer from 86.8 to 93.1 THz (from 2890 to 3100 wn). The pump and signal sources are a 1.06-μ m Nd:YAG laser and a 1.5-μ m extended-cavity laser diode. An enhanced-cavity absorption cell increases the optical electric field and enhances the sensitivity. The typical uncertainty is 3 kHz for the allowed transitions and 12 kHz for the forbidden transitions. Twenty combination differences are precisely determined, and the scalar rotational and centrifugal distortion constants of the <span class="hlt">ground</span> <span class="hlt">state</span> are thereby yielded as r@ = l@ r@ = l B_{{s}} (157 122 614.2 ± 1.5) kHz, D_{{s}} (3 328.545 ± 0.031) kHz, H_{{s}} (190.90 ± 0.26) Hz, and L_{{s}} (-13.16 ± 0.76) mHz. Here, B_{{s}} is the rotational constant and D_{{s}}, H_{{s}} and L_{{s}} are the scalar quartic, sextic, octic distortion constants. The relative uncertainties are considerably smaller than those obtained from global analysis of Fourier-transform infrared spectroscopy. S. Okubo, H. Nakayama, K. Iwakuni, H. Inaba and H. Sasada, Opt. Express 19, 23878 (2011). M. Abe, K. Iwakuni, S. Okubo, and H. Sasada, J. Opt. Soc. Am. B (to be published). S. Albert, S. Bauerecker, V. Boudon, L. R. Brown, J. -P. Champion, M. Loëte, A. Nikitin, and M. Quack, Chem. Phys. 356, 131 (2009).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvB..97c5159A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvB..97c5159A"><span>Stability of fractional Chern insulators in the effective continuum limit of Harper-Hofstadter <span class="hlt">bands</span> with Chern number |C |>1</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Andrews, Bartholomew; Möller, Gunnar</p> <p>2018-01-01</p> <p>We study the stability of composite fermion fractional quantum Hall <span class="hlt">states</span> in Harper-Hofstadter <span class="hlt">bands</span> with Chern number |C |>1 . From composite fermion theory, <span class="hlt">states</span> are predicted to be found at filling factors ν =r /(k r |C |+1 ),r ∈Z , with k =1 for bosons and k =2 for fermions. Here, we closely analyze these series in both cases, with contact interactions for bosons and nearest-neighbor interactions for (spinless) fermions. In particular, we analyze how the many-body gap scales as the <span class="hlt">bands</span> are tuned to the effective continuum limit of Chern number |C | <span class="hlt">bands</span>, realized near flux density nϕ=1 /|C | . Near these points, the Hofstadter model requires large magnetic unit cells that yield <span class="hlt">bands</span> with perfectly flat dispersion and Berry curvature. We exploit the known scaling of <span class="hlt">energies</span> in the effective continuum limit in order to maintain a fixed square aspect ratio in finite-size calculations. Based on exact diagonalization calculations of the <span class="hlt">band</span>-projected Hamiltonian for these lattice geometries, we show that for both bosons and fermions, the vast majority of finite-size spectra yield the <span class="hlt">ground-state</span> degeneracy predicted by composite fermion theory. For the chosen interactions, we confirm that <span class="hlt">states</span> with filling factor ν =1 /(k |C |+1 ) are the most robust and yield a clear gap in the thermodynamic limit. For bosons with contact interactions in |C |=2 and |C |=3 <span class="hlt">bands</span>, our data for the composite fermion <span class="hlt">states</span> are compatible with a finite gap in the thermodynamic limit. We also report new evidence for gapped incompressible <span class="hlt">states</span> stabilized for fermions with nearest-neighbor interactions in |C |>1 <span class="hlt">bands</span>. For cases with a clear gap, we confirm that the thermodynamic limit commutes with the effective continuum limit within finite-size error bounds. We analyze the nature of the correlation functions for the Abelian composite fermion <span class="hlt">states</span> and find that the correlation functions for |C |>1 <span class="hlt">states</span> are smooth functions for positions separated by |C | sites</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ApSS..407...99K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ApSS..407...99K"><span><span class="hlt">Energy</span> <span class="hlt">band</span> alignment of antiferroelectric (Pb,La)(Zr,Sn,Ti)O3</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Klein, Andreas; Lohaus, Christian; Reiser, Patrick; Dimesso, Lucangelo; Wang, Xiucai; Yang, Tongqing</p> <p>2017-06-01</p> <p>The <span class="hlt">energy</span> <span class="hlt">band</span> 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 <span class="hlt">band</span> maximum <span class="hlt">energy</span> 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 <span class="hlt">band</span> maximum, which is directly related to the electrical properties of such compounds. The results also verify that the <span class="hlt">energy</span> <span class="hlt">band</span> 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 <span class="hlt">energy</span> density capacitors. Moreover, the position of the <span class="hlt">energy</span> <span class="hlt">bands</span> should result in a great freedom of selecting electrode materials in terms of avoiding charge injection.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011ITEIS.131.2034I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011ITEIS.131.2034I"><span>Size Effect of <span class="hlt">Ground</span> Patterns on FM-<span class="hlt">Band</span> Cross-Talks between Two Parallel Signal Traces of Printed Circuit Boards for Vehicles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Iida, Michihira; Maeno, Tsuyoshi; Wang, Jianqing; Fujiwara, Osamu</p> <p></p> <p>Electromagnetic disturbances in vehicle-mounted radios are mainly caused by conducted noise currents flowing through wiring-harnesses from vehicle-mounted printed circuit boards (PCBs) with common slitting <span class="hlt">ground</span> patterns. To suppress these kinds of noise currents, we previously measured them for simple two-layer PCBs with two parallel signal traces and slitting or non-slitting <span class="hlt">ground</span> patterns, and then investigated by the FDTD simulation the reduction characteristics of the FM-<span class="hlt">band</span> cross-talk noise levels between two parallel signal traces on six simple PCB models having different slitting <span class="hlt">ground</span> or different divided <span class="hlt">ground</span> patterns parallel to the traces. As a result, we found that the contributory factor for the FM-<span class="hlt">band</span> cross-talk reduction is the reduction of mutual inductance between the two parallel traces, and also the noise currents from PCBs can rather be suppressed even if the size of the return <span class="hlt">ground</span> becomes small. In this study, to investigate this finding, we further simulated the frequency characteristics of cross-talk reduction for additional six simple PCB models with different dividing dimensions <span class="hlt">ground</span> patterns parallel to the traces, which revealed an interesting phenomenon that cross-talk reduction characteristics do not always decrease with increasing the width between the divided <span class="hlt">ground</span> patterns.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22251539-multireference-perturbation-method-using-non-orthogonal-hartree-fock-determinants-ground-excited-states','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22251539-multireference-perturbation-method-using-non-orthogonal-hartree-fock-determinants-ground-excited-states"><span>A multireference perturbation method using non-orthogonal Hartree-Fock determinants for <span class="hlt">ground</span> and excited <span class="hlt">states</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>Yost, Shane R.; Kowalczyk, Tim; Van Voorhis, Troy, E-mail: tvan@mit.edu</p> <p>2013-11-07</p> <p>In this article we propose the ΔSCF(2) framework, a multireference strategy based on second-order perturbation theory, for <span class="hlt">ground</span> and excited electronic <span class="hlt">states</span>. Unlike the complete active space family of methods, ΔSCF(2) employs a set of self-consistent Hartree-Fock determinants, also known as ΔSCF <span class="hlt">states</span>. Each ΔSCF electronic <span class="hlt">state</span> is modified by a first-order correction from Møller-Plesset perturbation theory and used to construct a Hamiltonian in a configuration interactions like framework. We present formulas for the resulting matrix elements between nonorthogonal <span class="hlt">states</span> that scale as N{sub occ}{sup 2}N{sub virt}{sup 3}. Unlike most active space methods, ΔSCF(2) treats the <span class="hlt">ground</span> and excited statemore » determinants even-handedly. We apply ΔSCF(2) to the H{sub 2}, hydrogen fluoride, and H{sub 4} systems and show that the method provides accurate descriptions of <span class="hlt">ground</span>- and excited-<span class="hlt">state</span> potential <span class="hlt">energy</span> surfaces with no single active space containing more than 10 ΔSCF <span class="hlt">states</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19730023383','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19730023383"><span>Solid <span class="hlt">state</span>, S-<span class="hlt">band</span>, power amplifier</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Digrindakis, M.</p> <p>1973-01-01</p> <p>The final design and specifications for a solid <span class="hlt">state</span>, S-<span class="hlt">band</span>, power amplifier is reported. Modifications from a previously proposed design were incorporated to improve efficiency and meet input overdrive and noise floor requirements. Reports on the system design, driver amplifier, power amplifier, and voltage and current limiter are included along with a discussion of the testing program.</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/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.ncbi.nlm.nih.gov/pubmed/28432287','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28432287"><span>Advantages of Unfair Quantum <span class="hlt">Ground-State</span> Sampling.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhang, Brian Hu; Wagenbreth, Gene; Martin-Mayor, Victor; Hen, Itay</p> <p>2017-04-21</p> <p>The debate around the potential superiority of quantum annealers over their classical counterparts has been ongoing since the inception of the field. Recent technological breakthroughs, which have led to the manufacture of experimental prototypes of quantum annealing optimizers with sizes approaching the practical regime, have reignited this discussion. However, the demonstration of quantum annealing speedups remains to this day an elusive albeit coveted goal. We examine the power of quantum annealers to provide a different type of quantum enhancement of practical relevance, namely, their ability to serve as useful samplers from the <span class="hlt">ground-state</span> manifolds of combinatorial optimization problems. We study, both numerically by simulating stoquastic and non-stoquastic quantum annealing processes, and experimentally, using a prototypical quantum annealing processor, the ability of quantum annealers to sample the <span class="hlt">ground-states</span> of spin glasses differently than thermal samplers. We demonstrate that (i) quantum annealers sample the <span class="hlt">ground-state</span> manifolds of spin glasses very differently than thermal optimizers (ii) the nature of the quantum fluctuations driving the annealing process has a decisive effect on the final distribution, and (iii) the experimental quantum annealer samples <span class="hlt">ground-state</span> manifolds significantly differently than thermal and ideal quantum annealers. We illustrate how quantum annealers may serve as powerful tools when complementing standard sampling algorithms.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvB..97q4501I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvB..97q4501I"><span>Symmetry conditions of a nodal superconductor for generating robust flat-<span class="hlt">band</span> Andreev bound <span class="hlt">states</span> at its dirty surface</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ikegaya, Satoshi; Kobayashi, Shingo; Asano, Yasuhiro</p> <p>2018-05-01</p> <p>We discuss the symmetry property of a nodal superconductor that hosts robust flat-<span class="hlt">band</span> zero-<span class="hlt">energy</span> <span class="hlt">states</span> at its surface under potential disorder. Such robust zero-<span class="hlt">energy</span> <span class="hlt">states</span> are known to induce the anomalous proximity effect in a dirty normal metal attached to a superconductor. A recent study has shown that a topological index NZES describes the number of zero-<span class="hlt">energy</span> <span class="hlt">states</span> at the dirty surface of a p -wave superconductor. We generalize the theory to clarify the conditions required for a superconductor that enables NZES≠0 . Our results show that NZES≠0 is realized in a topological material that belongs to either the BDI or CII class. We also present two realistic Hamiltonians that result in NZES≠0 .</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22047595-band-ground-based-detection-secondary-eclipse-wasp','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22047595-band-ground-based-detection-secondary-eclipse-wasp"><span>z'-<span class="hlt">BAND</span> <span class="hlt">GROUND</span>-BASED DETECTION OF THE SECONDARY ECLIPSE OF WASP-19b</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>Burton, J. R.; Watson, C. A.; Pollacco, D.</p> <p>2012-08-01</p> <p>We present the <span class="hlt">ground</span>-based detection of the secondary eclipse of the transiting exoplanet WASP-19b. The observations were made in the Sloan z' <span class="hlt">band</span> using the ULTRACAM triple-beam CCD camera mounted on the New Technology Telescope. The measurement shows a 0.088% {+-} 0.019% eclipse depth, matching previous predictions based on H- and K-<span class="hlt">band</span> measurements. We discuss in detail our approach to the removal of errors arising due to systematics in the data set, in addition to fitting a model transit to our data. This fit returns an eclipse center, T{sub 0}, of 2455578.7676 HJD, consistent with a circular orbit. Our measurementmore » of the secondary eclipse depth is also compared to model atmospheres of WASP-19b and is found to be consistent with previous measurements at longer wavelengths for the model atmospheres we investigated.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018EPJB...91..108P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018EPJB...91..108P"><span>Density-functional <span class="hlt">energy</span> gaps of solids demystified</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Perdew, John P.; Ruzsinszky, Adrienn</p> <p>2018-06-01</p> <p>The fundamental <span class="hlt">energy</span> gap of a solid is a <span class="hlt">ground-state</span> second <span class="hlt">energy</span> difference. Can one find the fundamental gap from the gap in the <span class="hlt">band</span> structure of Kohn-Sham density functional theory? An argument of Williams and von Barth (WB), 1983, suggests that one can. In fact, self-consistent <span class="hlt">band</span>-structure calculations within the local density approximation or the generalized gradient approximation (GGA) yield the fundamental gap within the same approximation for the <span class="hlt">energy</span>. Such a calculation with the exact density functional would yield a <span class="hlt">band</span> gap that also underestimates the fundamental gap, because the exact Kohn-Sham potential in a solid jumps up by an additive constant when one electron is added, and the WB argument does not take this effect into account. The WB argument has been extended recently to generalized Kohn-Sham theory, the simplest way to implement meta-GGAs and hybrid functionals self-consistently, with an exchange-correlation potential that is a non-multiplication operator. Since this operator is continuous, the <span class="hlt">band</span> gap is again the fundamental gap within the same approximation, but, because the approximations are more realistic, so is the <span class="hlt">band</span> gap. What approximations might be even more realistic?</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003SSCom.128..369X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003SSCom.128..369X"><span><span class="hlt">Ground</span> <span class="hlt">state</span> transitions in vertically coupled N-layer single electron quantum dots</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xie, Wenfang; Wang, Anmei</p> <p>2003-12-01</p> <p>A method is proposed to exactly diagonalize the Hamiltonian of a N-layer quantum dot containing a single electron in each dot in arbitrary magnetic fields. For N=4, the <span class="hlt">energy</span> spectra of the dot are calculated as a function of the applied magnetic field. We find discontinuous <span class="hlt">ground-state</span> <span class="hlt">energy</span> transitions induced by an external magnetic field in the case of strong coupling. However, in the case of weak coupling, such a transition does not occur and the angular momentum remains zero.</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 electronic <span class="hlt">band</span> structure. Each <span class="hlt">band</span> represents a series of allowed <span class="hlt">states</span> inside a material, relating electron <span class="hlt">energy</span> and momentum. The occupied <span class="hlt">bands</span>, that is, the filled electron <span class="hlt">states</span> 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> electron microscopy. It relies on the dependence of the electron 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 electronic <span class="hlt">band</span> structure. Each <span class="hlt">band</span> represents a series of allowed <span class="hlt">states</span> inside a material, relating electron <span class="hlt">energy</span> and momentum. The occupied <span class="hlt">bands</span>, that is, the filled electron <span class="hlt">states</span> 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> electron microscopy. It relies on the dependence of the electron 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/29327688','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29327688"><span>Empirical optimization of DFT  +  U and HSE for the <span class="hlt">band</span> structure of ZnO.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bashyal, Keshab; Pyles, Christopher K; Afroosheh, Sajjad; Lamichhane, Aneer; Zayak, Alexey T</p> <p>2018-02-14</p> <p>ZnO is a well-known wide <span class="hlt">band</span> gap semiconductor with promising potential for applications in optoelectronics, transparent electronics, and spintronics. Computational simulations based on the density functional theory (DFT) play an important role in the research of ZnO, but the standard functionals, like Perdew-Burke-Erzenhof, result in largely underestimated values of the <span class="hlt">band</span> gap and the binding <span class="hlt">energies</span> of the Zn 3d electrons. Methods like DFT  +  U and hybrid functionals are meant to remedy the weaknesses of plain DFT. However, both methods are not parameter-free. Direct comparison with experimental data is the best way to optimize the computational parameters. X-ray photoemission spectroscopy (XPS) is commonly considered as a benchmark for the computed electronic densities of <span class="hlt">states</span>. In this work, both DFT  +  U and HSE methods were parametrized to fit almost exactly the binding <span class="hlt">energies</span> of electrons in ZnO obtained by XPS. The optimized parameterizations of DFT  +  U and HSE lead to significantly worse results in reproducing the ion-clamped static dielectric tensor, compared to standard high-level calculations, including GW, which in turn yield a perfect match for the dielectric tensor. The failure of our XPS-based optimization reveals the fact that XPS does not report the <span class="hlt">ground</span> <span class="hlt">state</span> electronic structure for ZnO and should not be used for benchmarking <span class="hlt">ground</span> <span class="hlt">state</span> electronic structure calculations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JPCM...30f5501B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JPCM...30f5501B"><span>Empirical optimization of DFT  +  U and HSE for the <span class="hlt">band</span> structure of ZnO</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bashyal, Keshab; Pyles, Christopher K.; Afroosheh, Sajjad; Lamichhane, Aneer; Zayak, Alexey T.</p> <p>2018-02-01</p> <p>ZnO is a well-known wide <span class="hlt">band</span> gap semiconductor with promising potential for applications in optoelectronics, transparent electronics, and spintronics. Computational simulations based on the density functional theory (DFT) play an important role in the research of ZnO, but the standard functionals, like Perdew-Burke-Erzenhof, result in largely underestimated values of the <span class="hlt">band</span> gap and the binding <span class="hlt">energies</span> of the Zn3d electrons. Methods like DFT  +  U and hybrid functionals are meant to remedy the weaknesses of plain DFT. However, both methods are not parameter-free. Direct comparison with experimental data is the best way to optimize the computational parameters. X-ray photoemission spectroscopy (XPS) is commonly considered as a benchmark for the computed electronic densities of <span class="hlt">states</span>. In this work, both DFT  +  U and HSE methods were parametrized to fit almost exactly the binding <span class="hlt">energies</span> of electrons in ZnO obtained by XPS. The optimized parameterizations of DFT  +  U and HSE lead to significantly worse results in reproducing the ion-clamped static dielectric tensor, compared to standard high-level calculations, including GW, which in turn yield a perfect match for the dielectric tensor. The failure of our XPS-based optimization reveals the fact that XPS does not report the <span class="hlt">ground</span> <span class="hlt">state</span> electronic structure for ZnO and should not be used for benchmarking <span class="hlt">ground</span> <span class="hlt">state</span> electronic structure calculations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002APS..MAR.G2004P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002APS..MAR.G2004P"><span>Spin-polarized <span class="hlt">ground</span> <span class="hlt">state</span> and exact quantization at ν=5/2</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pan, Wei</p> <p>2002-03-01</p> <p>The nature of the even-denominator fractional quantum Hall effect at ν=5/2 remains elusive, in particular, its <span class="hlt">ground</span> <span class="hlt">state</span> spin-polarization. An earlier, so-called "hollow core" model arrived at a spin-unpolarized wave function. The more recent calculations based on a model of BCS-like pairing of composite fermions, however, suggest that its <span class="hlt">ground</span> <span class="hlt">state</span> is spin-polarized. In this talk, I will first review the earlier experiments and then present our recent experimental results showing evidence for a spin-polarized <span class="hlt">state</span> at ν=5/2. Our ultra-low temperature experiments on a high quality sample established the fully developed FQHE <span class="hlt">state</span> at ν=5/2 as well as at ν=7/3 and 8/3, manifested by a vanishing R_xx and exact quantization of the Hall plateau. The tilted field experiments showed that the added in-plane magnetic fields not only destroyed the FQHE at ν=5/2, as seen before, but also induced an electrical anisotropy, which is now interpreted as a phase transition from a paired, spin-polarized ν=5/2 <span class="hlt">state</span> to a stripe phase, not unlike the ones at ν=9/2, 11/2, etc in the N > 1 higher Landau levels. Furthermore, in the experiments on the heterojunction insulated-gate field-effect transistors (HIGFET) at dilution refrigerator temperatures, a strong R_xx minimum and a concomitant developing Hall plateau were observed at ν=5/2 in a magnetic field as high as 12.6 Tesla. This and the subsequent density dependent studies of its <span class="hlt">energy</span> gap largely rule out a spin-singlet <span class="hlt">state</span> and point quite convincingly towards a spin-polarized <span class="hlt">ground</span> <span class="hlt">state</span> at ν=5/2.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/979197-multi-quasiparticle-gamma-band-structure-neutron-deficient-ce-nd-isotopes','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/979197-multi-quasiparticle-gamma-band-structure-neutron-deficient-ce-nd-isotopes"><span>Multi-Quasiparticle Gamma-<span class="hlt">Band</span> Structure in Neutron-Deficient Ce and Nd Isotopes</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>Sheikh, Javid; Bhat, G. H.; Palit, R.</p> <p>2009-01-01</p> <p>The newly developed multi-quasiparticle triaxial projected shell-model approach is employed to study the high-spin <span class="hlt">band</span> structures in neutron-deficient even-even Ce and Nd isotopes. It is observed that gamma <span class="hlt">bands</span> are built on each intrinsic configuration of the triaxial mean-field deformation. Due to the fact that a triaxial configuration is a superposition of several K <span class="hlt">states</span>, the projection from these <span class="hlt">states</span> results in several low-lying <span class="hlt">bands</span> originating from the same intrinsic configuration. This generalizes the well-known concept of the surface gamma oscillation in deformed nuclei based on the <span class="hlt">ground</span> <span class="hlt">state</span> to gamma <span class="hlt">bands</span> built on multi-quasiparticle configurations. This new feature providesmore » an alternative explanation on the observation of two I=10 aligning <span class="hlt">states</span> in ^{134}Ce and both exhibiting a neutron character.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1185348-quenched-crystal-field-disorder-magnetic-liquid-ground-states-tb2sn2-xtixo7-crystal-field-disorder-quantum-spin-ice-ground-state-tb2sn2-xtixo7','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1185348-quenched-crystal-field-disorder-magnetic-liquid-ground-states-tb2sn2-xtixo7-crystal-field-disorder-quantum-spin-ice-ground-state-tb2sn2-xtixo7"><span>Quenched crystal-field disorder and magnetic liquid <span class="hlt">ground</span> <span class="hlt">states</span> in Tb 2 Sn 2 - x Ti x O 7 [Crystal field disorder in the quantum spin ice <span class="hlt">ground</span> <span class="hlt">state</span> of Tb2Sn2-xTixO7</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Gaulin, B. D.; Kermarrec, E.; Dahlberg, M. L.; ...</p> <p>2015-06-01</p> <p>Solid-solutions of the "soft" quantum spin ice pyrochlore magnets Tb 2B 2O 7 with B=Ti and Sn display a novel magnetic <span class="hlt">ground</span> <span class="hlt">state</span> in the presence of strong B-site disorder, characterized by a low susceptibility and strong spin fluctuations to temperatures below 0.1 K. These materials have been studied using ac-susceptibility and muSR techniques to very low temperatures, and time-of-flight inelastic neutron scattering techniques to 1.5 K. Remarkably, neutron spectroscopy of the Tb 3+ crystal field levels appropriate to at high B-site mixing (0.5 < x < 1.5 in Tb 2Sn 2-xTi xO 7) reveal that the doublet <span class="hlt">ground</span> andmore » first excited <span class="hlt">states</span> present as continua in <span class="hlt">energy</span>, while transitions to singlet excited <span class="hlt">states</span> at higher <span class="hlt">energies</span> simply interpolate between those of the end members of the solid solution. The resulting <span class="hlt">ground</span> <span class="hlt">state</span> suggests an extreme version of a random-anisotropy magnet, with many local moments and anisotropies, depending on the precise local configuration of the six B sites neighboring each magnetic Tb 3+ ion.« less</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 <span class="hlt">State</span> Density Determines the <span class="hlt">Energy</span> Level Alignment at Hybrid Perovskite/Electron 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 electronic 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 <span class="hlt">states</span> 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 electron acceptor layer interfaces using photoelectron spectroscopy. When forming the interfaces, it is found that electron transfer from surface <span class="hlt">states</span> to acceptor molecules occurs, leading to a strong decrease in the density of ionized surface <span class="hlt">states</span>. As a consequence, for perovskite samples with low surface <span class="hlt">state</span> 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 <span class="hlt">state</span> 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 <span class="hlt">state</span> 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/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> electrons in graphene by a time-dependent finite-step potential barrier. Our results demonstrate that, after Klein tunneling through the barrier, the electron 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 electron loses <span class="hlt">energy</span> and ends up as a valence <span class="hlt">band</span> <span class="hlt">state</span> 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/20639799-ground-state-properties-trapped-bose-fermi-mixtures-role-exchange-correlation','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/20639799-ground-state-properties-trapped-bose-fermi-mixtures-role-exchange-correlation"><span><span class="hlt">Ground-state</span> properties of trapped Bose-Fermi mixtures: Role of exchange correlation</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>Albus, Alexander P.; Wilkens, Martin; Illuminati, Fabrizio</p> <p>2003-06-01</p> <p>We introduce density-functional theory for inhomogeneous Bose-Fermi mixtures, derive the associated Kohn-Sham equations, and determine the exchange-correlation <span class="hlt">energy</span> in local-density approximation. We solve numerically the Kohn-Sham system, and determine the boson and fermion density distributions and the <span class="hlt">ground-state</span> <span class="hlt">energy</span> of a trapped, dilute mixture beyond mean-field approximation. The importance of the corrections due to exchange correlation is discussed by a comparison with current experiments; in particular, we investigate the effect of the repulsive potential-<span class="hlt">energy</span> contribution due to exchange correlation on the stability of the mixture against collapse.</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 electron 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 <span class="hlt">state</span> having the most advantageous formation <span class="hlt">energy</span>. Also, doping effects on the electronic 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/447532-optimised-effective-potential-ground-states-excited-states-time-dependent-phenomena','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/447532-optimised-effective-potential-ground-states-excited-states-time-dependent-phenomena"><span>Optimised effective potential for <span class="hlt">ground</span> <span class="hlt">states</span>, excited <span class="hlt">states</span>, and time-dependent phenomena</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>Gross, E.K.U.</p> <p>1996-12-31</p> <p>(1) The optimized effective potential method is a variant of the traditional Kohn-Sham scheme. In this variant, the exchange-correlation <span class="hlt">energy</span> E{sub xc} is an explicit functional of single-particle orbitals. The exchange-correlation potential, given as usual by the functional derivative v{sub xc} = {delta}E{sub xc}/{delta}{rho}, then satisfies as integral equation involving the single-particle orbitals. This integral equation in solved semi-analytically using a scheme recently proposed by Krieger, Li and Iafrate. If the exact (Fock) exchange-<span class="hlt">energy</span> functional is employed together with the Colle-Salvetti orbital functional for the correlation <span class="hlt">energy</span>, the mean absolute deviation of the resulting <span class="hlt">ground-state</span> <span class="hlt">energies</span> from the exact nonrelativisticmore » values is CT mH for the first-row atoms, as compared to 4.5 mH in a <span class="hlt">state</span>-of-the-art CI calculation. The proposed scheme is thus significantly more accurate than the conventional Kohn-Sham method while the numerical effort involved is about the same as for an ordinary Hanree-Fock calculation. (2) A time-dependent generalization of the optimized-potential method is presented and applied to the linear-response regime. Since time-dependent density functional theory leads to a formally exact representation of the frequency-dependent linear density response and since the latter, as a function of frequency, has poles at the excitation <span class="hlt">energies</span> of the fully interacting system, the formalism is suitable for the calculation of excitation <span class="hlt">energies</span>. A simple additive correction to the Kohn-Sham single-particle excitation <span class="hlt">energies</span> will be deduced and first results for atomic and molecular singlet and triplet excitation <span class="hlt">energies</span> will be presented. (3) Beyond the regime of linear response, the time-dependent optimized-potential method is employed to describe atoms in strong emtosecond laser pulses. Ionization yields and harmonic spectra will be presented and compared with experimental data.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AIPC..819..550P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AIPC..819..550P"><span>Spin-isospin excitations from the <span class="hlt">ground-state</span> of 64Ni</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Popescu, L.; Adachi, T.; Bäumer, C.; Berg, G. P. A.; van den Berg, A. M.; von Brentano, P.; Frekers, D.; de Frenne, D.; Fujita, K.; Fujita, Y.; Grewe, E. W.; Haefner, P.; Hatanaka, K.; Hunyadi, M.; de Huu, M.; Jacobs, E.; Johansson, H.; Korff, A.; Negret, A.; Nakanishi, K.; von Neumann-Cosel, P.; Rakers, S.; Ryezayeva, N.; Sakemi, Y.; Shevchenko, A.; Shimbara, Y.; Shimizu, Y.; Simon, H.; Tameshige, Y.; Tamii, A.; Uchida, M.; Wörtche, H. J.; Yosoi, M.</p> <p>2006-03-01</p> <p>Spin-isospin (Gamow-Teller) excitations in 64Cu and 64Co have been studied using (3He,t) and (d,2He) charge-exchange reactions on 64Ni. As the isospin of the 64Ni <span class="hlt">ground-state</span> is T0=4, <span class="hlt">states</span> with T=3, 4 and 5 in 64Cu are excited via the (3He,t) reaction and <span class="hlt">states</span> with T=5 in 64Co via (d,2He). If we assume that the nuclear interaction is charge symmetric, the T=5 <span class="hlt">states</span> in 64Cu should appear at corresponding excitation <span class="hlt">energies</span> (if corrected for the Coulomb displacement) and with similar strengths as the T=5 <span class="hlt">states</span> in 64Co. As in the 64Cu spectrum the T=5 <span class="hlt">states</span> are very weakly excited, only by combining the results of the two complementary experiments one can estimate the Gamow-Teller strength starting from 64Ni in a consistent way.</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> </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/2018JPSJ...87c4002K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JPSJ...87c4002K"><span><span class="hlt">Ground-State</span> Wave Function with Interactions between Different Species in M-Component Miscible Bose-Einstein Condensates</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kohno, Wataru; Kirikoshi, Akimitsu; Kita, Takafumi</p> <p>2018-03-01</p> <p>We construct a variational <span class="hlt">ground-state</span> wave function of weakly interacting M-component Bose-Einstein condensates beyond the mean-field theory by incorporating the dynamical 3/2-body processes, where one of the two colliding particles drops into the condensate and vice versa. Our numerical results with various masses and particle numbers show that the 3/2-body processes between different particles make finite contributions to lowering the <span class="hlt">ground-state</span> <span class="hlt">energy</span>, implying that many-body correlation effects between different particles are essential even in the weak-coupling regime of the Bose-Einstein condensates. We also consider the stability condition for 2-component miscible <span class="hlt">states</span> using the new <span class="hlt">ground-state</span> wave function. Through this calculation, we obtain the relation UAB2/UAAUBB < 1 + α , where Uij is the effective contact potential between particles i and j and α is the correction, which originates from the 3/2- and 2-body processes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018MS%26E..306a2124H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MS%26E..306a2124H"><span>Design and Simulation of Microstrip Hairpin Bandpass Filter with Open Stub and Defected <span class="hlt">Ground</span> Structure (DGS) at X-<span class="hlt">Band</span> Frequency</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hariyadi, T.; Mulyasari, S.; Mukhidin</p> <p>2018-02-01</p> <p>In this paper we have designed and simulated a <span class="hlt">Band</span> Pass Filter (BPF) at X-<span class="hlt">band</span> frequency. This filter is designed for X-<span class="hlt">band</span> weather radar application with 9500 MHz center frequency and bandwidth -3 dB is 120 MHz. The filter design was performed using a hairpin microstrip combined with an open stub and defected <span class="hlt">ground</span> structure (DGS). The substrate used is Rogers RT5880 with a dielectric constant of 2.2 and a thickness of 1.575 mm. Based on the simulation results, it is found that the filter works on frequency 9,44 - 9,56 GHz with insertion loss value at pass <span class="hlt">band</span> is -1,57 dB.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PMag...97.1884N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PMag...97.1884N"><span>The under-pressure behaviour of mechanical, electronic and optical properties of calcium titanate and its <span class="hlt">ground</span> <span class="hlt">state</span> thermoelectric response</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Noor, N. A.; Alay-e-Abbas, S. M.; Hassan, M.; Mahmood, I.; Alahmed, Z. A.; Reshak, A. H.</p> <p>2017-08-01</p> <p>In this study, the elastic, electronic, optical and thermoelectric properties of CaTiO3 perovskite oxide have been investigated using first-principles calculations. The generalised gradient approximation (GGA) has been employed for evaluating structural and elastic properties, while the modified Becke Johnson functional is used for studying the optical response of this compound. In addition to <span class="hlt">ground</span> <span class="hlt">state</span> physical properties, we also investigate the effects of pressure (0, 30, 60, 90 and 120 GPa) on the electronic structure of CaTiO3. The application of pressure from 0 to 90 GPa shows that the indirect <span class="hlt">band</span> gap (Γ-M) of CaTiO3 increases with increasing pressure and at 120 GPa it spontaneously decreases transforming cubic CaTiO3 to a direct (Γ-Γ) <span class="hlt">band</span> gap material. The complex dielectric function and some optical parameters are also investigated under the application of pressures. All the calculated optical properties have been found to exhibit a shift to the higher <span class="hlt">energies</span> with the increase of applied pressure suggesting potential optoelectronic device applications of CaTiO3. The thermoelectric properties of CaTiO3 have been computed at 0 GPa in terms of electrical conductivity, thermal conductivity and Seebeck coefficient.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20020032683&hterms=singlet+oxygen&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dsinglet%2Boxygen','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20020032683&hterms=singlet+oxygen&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dsinglet%2Boxygen"><span>Quantum Mechanical Determination of Potential <span class="hlt">Energy</span> Surfaces for TiO and H2O</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Langhoff, Stephen R.</p> <p>1996-01-01</p> <p>We discuss current ab initio methods for determining potential <span class="hlt">energy</span> surfaces, in relation to the TiO and H2O molecules, both of which make important contributions to the opacity of oxygen-rich stars. For the TiO molecule we discuss the determination of the radiative lifetimes of the excited <span class="hlt">states</span> and <span class="hlt">band</span> oscillator strengths for both the triplet and singlet <span class="hlt">band</span> systems. While the theoretical radiative lifetimes for TiO agree well with recent measurements, the <span class="hlt">band</span> oscillator strengths differ significantly from those currently employed in opacity calculations. For the H2O molecule we discuss the current results for the potential <span class="hlt">energy</span> and dipole moment <span class="hlt">ground</span> <span class="hlt">state</span> surfaces generated at NASA Ames. We show that it is necessary to account for such effects as core-valence Correlation <span class="hlt">energy</span> to generate a PES of near spectroscopic accuracy. We also describe how we solve the ro-vibrational problem to obtain the line positions and intensities that are needed for opacity sampling.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1346533','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1346533"><span>Solid-<span class="hlt">State</span> Powered X-<span class="hlt">band</span> Accelerator</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>Othman, Mohamed A.K.; Nann, Emilio A.; Dolgashev, Valery A.</p> <p>2017-03-06</p> <p>In this report we disseminate the hot test results of an X-<span class="hlt">band</span> 100-W solid <span class="hlt">state</span> amplifier chain for linear accelerator (linac) applications. Solid <span class="hlt">state</span> power amplifiers have become increasingly attractive solutions for achieving high power in radar and maritime applications. Here the performance of solid <span class="hlt">state</span> amplifiers when driving an RF cavity is investigated. Commercially available, matched and fully-packaged GaN on SiC HEMTs are utilized, comprising a wideband driver stage and two power stages. The amplifier chain has a high poweradded- efficiency and is able to supply up to ~1.2 MV/m field gradient at 9.2 GHz in a simple testmore » cavity, with a peak power exceeding 100 W. These findings set forth the enabling technology for solid-<span class="hlt">state</span> powered linacs.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ApPhL.112s3901L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ApPhL.112s3901L"><span>Calcium doped MAPbI3 with better <span class="hlt">energy</span> <span class="hlt">state</span> alignment in perovskite solar cells</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lu, Chaojie; Zhang, Jing; Hou, Dagang; Gan, Xinlei; Sun, Hongrui; Zeng, Zhaobing; Chen, Renjie; Tian, Hui; Xiong, Qi; Zhang, Ying; Li, Yuanyuan; Zhu, Yuejin</p> <p>2018-05-01</p> <p>The organic-inorganic perovskite material with better <span class="hlt">energy</span> alignment in the solar cell device will have a profound impact on the solar cell performance. It is valuable to tune the <span class="hlt">energy</span> <span class="hlt">states</span> by element substitution and doping in perovskites. Here, we present that Ca2+ is incorporated into CH3NH3PbI3, which up-shifts the valence <span class="hlt">band</span> maximum and the conduction <span class="hlt">band</span> minimum, leading to a difference between the bandgap and the Fermi level in the device. Consequently, Ca2+ incorporation results in an enhancement of the photovoltage and photocurrent, achieving a summit efficiency of 18.3% under standard 1 sun (AM 1.5). This work reveals the doped perovskite to improve the solar cell performance by tuning the <span class="hlt">energy</span> <span class="hlt">state</span>.</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('http://adsabs.harvard.edu/abs/2017APS..MARB25004Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..MARB25004Y"><span>σ -SCF: A Direct <span class="hlt">Energy</span>-targeting Method To Mean-field Excited <span class="hlt">States</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ye, Hongzhou; Welborn, Matthew; Ricke, Nathan; van Voorhis, Troy</p> <p></p> <p>The mean-field solutions of electronic excited <span class="hlt">states</span> are much less accessible than <span class="hlt">ground</span> <span class="hlt">state</span> (e.g. Hartree-Fock) solutions. <span class="hlt">Energy</span>-based optimization methods for excited <span class="hlt">states</span>, like Δ-SCF, tend to fall into the lowest solution consistent with a given symmetry - a problem known as ``variational collapse''. In this work, we combine the ideas of direct <span class="hlt">energy</span>-targeting and variance-based optimization in order to describe excited <span class="hlt">states</span> at the mean-field level. The resulting method, σ-SCF, has several advantages. First, it allows one to target any desired excited <span class="hlt">state</span> by specifying a single parameter: a guess of the <span class="hlt">energy</span> of that <span class="hlt">state</span>. It can therefore, in principle, find all excited <span class="hlt">states</span>. Second, it avoids variational collapse by using a variance-based, unconstrained local minimization. As a consequence, all <span class="hlt">states</span> - <span class="hlt">ground</span> or excited - are treated on an equal footing. Third, it provides an alternate approach to locate Δ-SCF solutions that are otherwise hardly accessible by the usual non-aufbau configuration initial guess. We present results for this new method for small atoms (He, Be) and molecules (H2, HF). This work was funded by a Grant from NSF (CHE-1464804).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160006685','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160006685"><span>Multi-<span class="hlt">Band</span> Multi-Tone Tunable Millimeter-Wave Frequency Synthesizer For Satellite Beacon Transmitter</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Simons, Rainee N.; Wintucky, Edwin G.</p> <p>2016-01-01</p> <p>This paper presents the design and test results of a multi-<span class="hlt">band</span> multi-tone tunable millimeter-wave frequency synthesizer, based on a solid-<span class="hlt">state</span> frequency comb generator. The intended application of the synthesizer is in a satellite beacon transmitter for radio wave propagation studies at K-<span class="hlt">band</span> (18 to 26.5 GHz), Q-<span class="hlt">band</span> (37 to 42 GHz), and E-<span class="hlt">band</span> (71 to 76 GHz). In addition, the architecture for a compact beacon transmitter, which includes the multi-tone synthesizer, polarizer, horn antenna, and power/control electronics, has been investigated for a notional space-to-<span class="hlt">ground</span> radio wave propagation experiment payload on a small satellite. The above studies would enable the design of robust high throughput multi-Gbps data rate future space-to-<span class="hlt">ground</span> satellite communication links.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1998JMoSp.191..306K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998JMoSp.191..306K"><span>High-Resolution Analysis of the ν 6, ν 7, ν 8, and ν 9<span class="hlt">Bands</span> of H 15N 16O 3Measured by Fourier Transform Spectroscopy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Keller, F.; Perrin, A.; Flaud, J.-M.; Johns, J. W. C.; Lu, Z.; Looi, E. C.</p> <p>1998-10-01</p> <p>The analysis of the ν6, ν7, ν8, and ν9<span class="hlt">bands</span> of H15N16O3located at 646.9641, 578.4719, 743.6166, and 458.2917 cm-1, respectively, has been carried out in the 400-800 cm-1region using high-resolution Fourier transform spectra recorded at Ottawa. Using the <span class="hlt">ground</span> <span class="hlt">state</span> <span class="hlt">energy</span> levels calculated from thev= 0 rotational constants of H15N16O3[A. P. Cox, M. C. Ellis, C. J. Attfield, and A. C. Ferris,J. Mol. Struct.320, 91-106 (1994)], it was possible to assign theA-type ν6and ν7<span class="hlt">bands</span> and theC-type ν8and ν9<span class="hlt">bands</span> of H15N16O3up to highJandKarotational quantum numbers. Thev6= 1,v7= 1, v8= 1, andv9= 1 experimental <span class="hlt">energy</span> levels were then introduced in a least-squares fit calculation and precise upper <span class="hlt">state</span> Hamiltonian constants (<span class="hlt">band</span> centers and rotational constants) were determined allowing one to reproduce the infrared data to within the experimental uncertainty.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22590793-high-spin-polarization-origin-unique-ferromagnetic-ground-state-cufesb','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22590793-high-spin-polarization-origin-unique-ferromagnetic-ground-state-cufesb"><span>High spin polarization and the origin of unique ferromagnetic <span class="hlt">ground</span> <span class="hlt">state</span> in CuFeSb</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>Sirohi, Anshu; Saha, Preetha; Gayen, Sirshendu</p> <p></p> <p>CuFeSb is isostructural to the ferro-pnictide and chalcogenide superconductors and it is one of the few materials in the family that are known to stabilize in a ferromagnetic <span class="hlt">ground</span> <span class="hlt">state</span>. Majority of the members of this family are either superconductors or antiferromagnets. Therefore, CuFeSb may be used as an ideal source of spin polarized current in spin-transport devices involving pnictide and the chalcogenide superconductors. However, for that the Fermi surface of CuFeSb needs to be sufficiently spin polarized. In this paper we report direct measurement of transport spin polarization in CuFeSb by spin-resolved Andreev reflection spectroscopy. From a number ofmore » measurements using multiple superconducting tips we found that the intrinsic transport spin polarization in CuFeSb is high (∼47%). In order to understand the unique <span class="hlt">ground</span> <span class="hlt">state</span> of CuFeSb and the origin of large spin polarization at the Fermi level, we have evaluated the spin-polarized <span class="hlt">band</span> structure of CuFeSb through first principles calculations. Apart from supporting the observed 47% transport spin polarization, such calculations also indicate that the Sb-Fe-Sb angles and the height of Sb from the Fe plane are strikingly different for CuFeSb than the equivalent parameters in other members of the same family thereby explaining the origin of the unique <span class="hlt">ground</span> <span class="hlt">state</span> of CuFeSb.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014APS..MARF45005C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014APS..MARF45005C"><span><span class="hlt">State</span> Counting for Excited <span class="hlt">Bands</span> of the Fractional Quantum Hall Effect: Exclusion Rules for Bound Excitons</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Coimbatore Balram, Ajit; Wójs, Arkadiusz; Jain, Jainendra</p> <p>2014-03-01</p> <p>Exact diagonalization studies have revealed that the <span class="hlt">energy</span> spectrum of interacting electrons in the lowest Landau level splits, non-perturbatively, into <span class="hlt">bands</span>. The theory of nearly free composite fermions (CFs) has been shown to be valid for the lowest <span class="hlt">band</span>, and thus to capture the low temperature physics, but it over-predicts the number of <span class="hlt">states</span> for the excited <span class="hlt">bands</span>. We explain the <span class="hlt">state</span> counting of higher <span class="hlt">bands</span> in terms of composite fermions with an infinitely strong short range interaction between a CF particle and a CF hole. This interaction, the form of which we derive from the microscopic CF theory, eliminates configurations containing certain tightly bound CF excitons. With this modification, the CF theory reproduces, for all well-defined excited <span class="hlt">bands</span>, an exact counting for ν > 1 / 3 , and an almost exact counting for ν <= 1 / 3 . The resulting insight clarifies that the corrections to the nearly free CF theory are not thermodynamically significant at sufficiently low temperatures, thus providing a microscopic explanation for why it has proved successful for the analysis of the various properties of the CF Fermi sea. NSF grants DMR-1005536 and DMR-0820404, Polish NCN grant 2011/01/B/ST3/04504 and EU Marie Curie Grant PCIG09-GA-2011-294186, Research Computing and Cyberinfrastructure, PSU and Wroclaw Centre for Networking and Supercomputing</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.H21H1491N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.H21H1491N"><span>Satellite Based Soil Moisture Product Validation Using NOAA-CREST <span class="hlt">Ground</span> and L-<span class="hlt">Band</span> Observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Norouzi, H.; Campo, C.; Temimi, M.; Lakhankar, T.; Khanbilvardi, R.</p> <p>2015-12-01</p> <p>Soil moisture content is among most important physical parameters in hydrology, climate, and environmental studies. Many microwave-based satellite observations have been utilized to estimate this parameter. The Advanced Microwave Scanning Radiometer 2 (AMSR2) is one of many remotely sensors that collects daily information of land surface soil moisture. However, many factors such as ancillary data and vegetation scattering can affect the signal and the estimation. Therefore, this information needs to be validated against some "<span class="hlt">ground</span>-truth" observations. NOAA - Cooperative Remote Sensing and Technology (CREST) center at the City University of New York has a site located at Millbrook, NY with several insitu soil moisture probes and an L-<span class="hlt">Band</span> radiometer similar to Soil Moisture Passive and Active (SMAP) one. This site is among SMAP Cal/Val sites. Soil moisture information was measured at seven different locations from 2012 to 2015. Hydra probes are used to measure six of these locations. This study utilizes the observations from insitu data and the L-<span class="hlt">Band</span> radiometer close to <span class="hlt">ground</span> (at 3 meters height) to validate and to compare soil moisture estimates from AMSR2. Analysis of the measurements and AMSR2 indicated a weak correlation with the hydra probes and a moderate correlation with Cosmic-ray Soil Moisture Observing System (COSMOS probes). Several differences including the differences between pixel size and point measurements can cause these discrepancies. Some interpolation techniques are used to expand point measurements from 6 locations to AMSR2 footprint. Finally, the effect of penetration depth in microwave signal and inconsistencies with other ancillary data such as skin temperature is investigated to provide a better understanding in the analysis. The results show that the retrieval algorithm of AMSR2 is appropriate under certain circumstances. This validation algorithm and similar study will be conducted for SMAP mission. Keywords: Remote Sensing, Soil</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22573937-atomic-solid-state-energy-scale-universality-periodic-trends-oxidation-state','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22573937-atomic-solid-state-energy-scale-universality-periodic-trends-oxidation-state"><span>Atomic solid <span class="hlt">state</span> <span class="hlt">energy</span> scale: Universality and periodic trends in oxidation <span class="hlt">state</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>Pelatt, Brian D.; Kokenyesi, Robert S.; Ravichandran, Ram</p> <p>2015-11-15</p> <p>The atomic solid <span class="hlt">state</span> <span class="hlt">energy</span> (SSE) scale originates from a plot of the electron affinity (EA) and ionization potential (IP) versus <span class="hlt">band</span> gap (E{sub G}). SSE is estimated for a given atom by assessing an average EA (for a cation) or an average IP (for an anion) for binary inorganic compounds having that specific atom as a constituent. Physically, SSE is an experimentally-derived average frontier orbital <span class="hlt">energy</span> referenced to the vacuum level. In its original formulation, 69 binary closed-shell inorganic semiconductors and insulators were employed as a database, providing SSE estimates for 40 elements. In this contribution, EA and IPmore » versus E{sub G} are plotted for an additional 92 compounds, thus yielding SSE estimates for a total of 64 elements from the s-, p-, d-, and f-blocks of the periodic table. Additionally, SSE is refined to account for its dependence on oxidation <span class="hlt">state</span>. Although most cations within the SSE database are found to occur in a single oxidation <span class="hlt">state</span>, data are available for nine d-block transition metals and one p-block main group metal in more than one oxidation <span class="hlt">state</span>. SSE is deeper in <span class="hlt">energy</span> for a higher cation oxidation <span class="hlt">state</span>. Two p-block main group non-metals within the SSE database are found to exist in both positive and negative oxidation <span class="hlt">states</span> so that they can function as a cation or anion. SSEs for most cations are positioned above −4.5 eV with respect to the vacuum level, and SSEs for all anions are positioned below. Hence, the <span class="hlt">energy</span> −4.5 eV, equal to the hydrogen donor/acceptor ionization <span class="hlt">energy</span> ε(+/−) or equivalently the standard hydrogen electrode <span class="hlt">energy</span>, is considered to be an absolute <span class="hlt">energy</span> reference for chemical bonding in the solid <span class="hlt">state</span>. - Highlights: • Atomic solid-<span class="hlt">state</span> <span class="hlt">energies</span> are estimated for 64 elements from experimental data. • The relationship between atomic SSEs and oxidation <span class="hlt">state</span> is assessed. • Cations are positioned above and absolute <span class="hlt">energy</span> of −4.5 eV and anions below.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017isms.confETD07D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017isms.confETD07D"><span>Analysis of the νb{6} Asymmetric no Stretch <span class="hlt">Band</span> of Nitromethane</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dawadi, Mahesh B.; Degliumberto, Lou; Perry, David S.; Mettee, Howard; Sams, Robert L.</p> <p>2017-06-01</p> <p>The b-type <span class="hlt">band</span> near 1583 \\wn has been assigned for m ≤ 3, K''_{a} ≤ 10, J'' ≤ 20. The <span class="hlt">ground</span> <span class="hlt">state</span> combination differences derived from these assigned levels were fit with the RAM36 program with an RMS deviation of 0.0006 \\wn. The upper <span class="hlt">state</span> levels are split into multiplets by perturbations. A subset of the available upper <span class="hlt">state</span> combination differences for m = 0, K'_{a} ≤ 7, J' ≤ 10 were fit with the same program, but with rather poorer precision (0.01 \\wn) than for the <span class="hlt">ground</span> <span class="hlt">state</span>.</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('https://www.osti.gov/biblio/20798350-spin-isospin-excitations-from-ground-state','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/20798350-spin-isospin-excitations-from-ground-state"><span>Spin-isospin excitations from the <span class="hlt">ground-state</span> of 64Ni</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>Popescu, L.; Frenne, D. de; Jacobs, E.</p> <p>2006-03-13</p> <p>Spin-isospin (Gamow-Teller) excitations in 64Cu and 64Co have been studied using (3He,t) and (d,2He) charge-exchange reactions on 64Ni. As the isospin of the 64Ni <span class="hlt">ground-state</span> is T0=4, <span class="hlt">states</span> with T=3, 4 and 5 in 64Cu are excited via the (3He,t) reaction and <span class="hlt">states</span> with T=5 in 64Co via (d,2He). If we assume that the nuclear interaction is charge symmetric, the T=5 <span class="hlt">states</span> in 64Cu should appear at corresponding excitation <span class="hlt">energies</span> (if corrected for the Coulomb displacement) and with similar strengths as the T=5 <span class="hlt">states</span> in 64Co. As in the 64Cu spectrum the T=5 <span class="hlt">states</span> are very weakly excited, only bymore » combining the results of the two complementary experiments one can estimate the Gamow-Teller strength starting from 64Ni in a consistent way.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011JFuE...30...21A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011JFuE...30...21A"><span>An Investigation for <span class="hlt">Ground</span> <span class="hlt">State</span> Features of Some Structural Fusion Materials</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Aytekin, H.; Tel, E.; Baldik, R.; Aydin, A.</p> <p>2011-02-01</p> <p>Environmental concerns associated with fossil fuels are creating increased interest in alternative non-fossil <span class="hlt">energy</span> sources. Nuclear fusion can be one of the most attractive sources of <span class="hlt">energy</span> from the viewpoint of safety and minimal environmental impact. When considered in all <span class="hlt">energy</span> systems, the requirements for performance of structural materials in a fusion reactor first wall, blanket or diverter, are arguably more demanding or difficult than for other <span class="hlt">energy</span> system. The development of fusion materials for the safety of fusion power systems and understanding nuclear properties is important. In this paper, <span class="hlt">ground</span> <span class="hlt">state</span> properties for some structural fusion materials as 27Al, 51V, 52Cr, 55Mn, and 56Fe are investigated using Skyrme-Hartree-Fock method. The obtained results have been discussed and compared with the available experimental data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JQSRT.198..155C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JQSRT.198..155C"><span>Collision induced broadening of ν1 <span class="hlt">band</span> and <span class="hlt">ground</span> <span class="hlt">state</span> spectral lines of sulfur dioxide perturbed by N2 and O2</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ceselin, Giorgia; Tasinato, Nicola; Puzzarini, Cristina; Charmet, Andrea Pietropolli; Stoppa, Paolo; Giorgianni, Santi</p> <p>2017-09-01</p> <p>To monitor the constituents and trace pollutants of Earth atmosphere and understand its evolution, accurate spectroscopic parameters are fundamental information. SO2 is produced by both natural and anthropogenic sources and it is one of the principal causes of acid rains as well as an important component of fine aerosol particles, once oxidized to sulfate. The present work aims at determining SO2 broadening parameters using N2 and O2 as atmospherically relevant damping gases. Measurements are carried out in the infrared (IR) and mm-/sub-mm wave regions, around 8.8 μm and in the 104 GHz-1.1 THz interval, respectively. IR ro-vibrational transitions are recorded by using a tunable diode laser spectrometer, whereas the microwave spectra are recorded by using a frequency-modulated millimeter-/submillimeter-wave spectrometer. SO2-N2 and SO2-O2 collisional cross sections are retrieved for several ν1 <span class="hlt">band</span> ro-vibrational transitions of 32S16O2, for some transitions belonging to either ν1 + ν2 - ν2 of 32S16O2 or ν1 of 34S16O2 as well as for about 20 pure rotational transitions in the vibrational <span class="hlt">ground</span> <span class="hlt">state</span> of the main isotopic species. From N2- and O2- broadening coefficients the broadening parameters of SO2 in air are derived. The work is completed with the study of the dependence of foreign broadening coefficients on the rotational quantum numbers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1999JMoSp.195..324T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1999JMoSp.195..324T"><span>FTIR Spectrum of the ν 4<span class="hlt">Band</span> of DCOOD</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tan, T. L.; Goh, K. L.; Ong, P. P.; Teo, H. H.</p> <p>1999-06-01</p> <p>The FTIR spectrum of the ν4<span class="hlt">band</span> of deuterated formic acid (DCOOD) has been measured with a resolution of 0.004 cm-1in the frequency range of 1120 to 1220 cm-1. A total of 1866 assigned transitions have been analyzed and fitted using a Watson'sA-reduced Hamiltonian in theIrrepresentation to derive rovibrational constants for the upper <span class="hlt">state</span> (v4= 1) with a standard deviation of 0.00036 cm-1. In the course of the analysis, the constants for the <span class="hlt">ground</span> <span class="hlt">state</span> were improved by a simultaneous fit of microwave frequencies and combination differences from the infrared measurements. Due to the relatively unperturbed nature of the <span class="hlt">band</span>, the constants can be used to accurately calculate the infrared line positions for the whole <span class="hlt">band</span>. Although the <span class="hlt">band</span> is a hybrid typeAandB, onlya-type transitions were strong enough to be observed. The <span class="hlt">band</span> center is at 1170.79980 ± 0.00002 cm-1.</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/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 electronic 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> <span class="hlt">states</span> with x ≳ 0.5, compared to Ga cations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1341699','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1341699"><span><span class="hlt">Ground-state</span> oxygen holes and the metal–insulator transition in the negative charge-transfer rare-earth nickelates</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>Bisogni, Valentina; Catalano, Sara; Green, Robert J.</p> <p></p> <p>The metal-insulator transitions and the intriguing physical properties of rare-earth perovskite nickelates have attracted considerable attention in recent years. However, a complete understanding of these materials remains elusive. Here, taking a NdNiO 3 thin film as a representative example, we utilize a combination of x-ray absorption (XAS) and resonant inelastic x-ray scattering (RIXS) spectroscopies to resolve important aspects of the complex electronic structure of the rare-earth nickelates. The unusual coexistence of bound and continuum excitations observed in the RIXS spectra provides strong evidence for the abundance of oxygen 2p holes in the <span class="hlt">ground</span> <span class="hlt">state</span> of these materials. Using cluster calculationsmore » and Anderson impurity model interpretation, we show that these distinct spectral signatures arise from a Ni 3d 8 configuration along with holes in the oxygen 2p valence <span class="hlt">band</span>, confirming suggestions that these materials do not obey a “conventional” positive charge-transfer picture, but instead exhibit a negative charge-transfer <span class="hlt">energy</span>, in line with recent models interpreting the metal to insulator transition in terms of bond disproportionation.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1341699-ground-state-oxygen-holes-metalinsulator-transition-negative-charge-transfer-rare-earth-nickelates','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1341699-ground-state-oxygen-holes-metalinsulator-transition-negative-charge-transfer-rare-earth-nickelates"><span><span class="hlt">Ground-state</span> oxygen holes and the metal–insulator transition in the negative charge-transfer rare-earth nickelates</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Bisogni, Valentina; Catalano, Sara; Green, Robert J.; ...</p> <p>2016-10-11</p> <p>The metal-insulator transitions and the intriguing physical properties of rare-earth perovskite nickelates have attracted considerable attention in recent years. However, a complete understanding of these materials remains elusive. Here, taking a NdNiO 3 thin film as a representative example, we utilize a combination of x-ray absorption (XAS) and resonant inelastic x-ray scattering (RIXS) spectroscopies to resolve important aspects of the complex electronic structure of the rare-earth nickelates. The unusual coexistence of bound and continuum excitations observed in the RIXS spectra provides strong evidence for the abundance of oxygen 2p holes in the <span class="hlt">ground</span> <span class="hlt">state</span> of these materials. Using cluster calculationsmore » and Anderson impurity model interpretation, we show that these distinct spectral signatures arise from a Ni 3d 8 configuration along with holes in the oxygen 2p valence <span class="hlt">band</span>, confirming suggestions that these materials do not obey a “conventional” positive charge-transfer picture, but instead exhibit a negative charge-transfer <span class="hlt">energy</span>, in line with recent models interpreting the metal to insulator transition in terms of bond disproportionation.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvL.120u0604A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvL.120u0604A"><span>Fast Preparation of Critical <span class="hlt">Ground</span> <span class="hlt">States</span> Using Superluminal Fronts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Agarwal, Kartiek; Bhatt, R. N.; Sondhi, S. L.</p> <p>2018-05-01</p> <p>We propose a spatiotemporal quench protocol that allows for the fast preparation of <span class="hlt">ground</span> <span class="hlt">states</span> of gapless models with Lorentz invariance. Assuming the system initially resides in the <span class="hlt">ground</span> <span class="hlt">state</span> of a corresponding massive model, we show that a superluminally moving "front" that locally quenches the mass, leaves behind it (in space) a <span class="hlt">state</span> arbitrarily close to the <span class="hlt">ground</span> <span class="hlt">state</span> of the gapless model. Importantly, our protocol takes time O (L ) to produce the <span class="hlt">ground</span> <span class="hlt">state</span> of a system of size ˜Ld (d spatial dimensions), while a fully adiabatic protocol requires time ˜O (L2) to produce a <span class="hlt">state</span> with exponential accuracy in L . The physics of the dynamical problem can be understood in terms of relativistic rarefaction of excitations generated by the mass front. We provide proof of concept by solving the proposed quench exactly for a system of free bosons in arbitrary dimensions, and for free fermions in d =1 . We discuss the role of interactions and UV effects on the free-theory idealization, before numerically illustrating the usefulness of the approach via simulations on the quantum Heisenberg spin chain.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29221390','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29221390"><span>σ-SCF: A direct <span class="hlt">energy</span>-targeting method to mean-field excited <span class="hlt">states</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ye, Hong-Zhou; Welborn, Matthew; Ricke, Nathan D; Van Voorhis, Troy</p> <p>2017-12-07</p> <p>The mean-field solutions of electronic excited <span class="hlt">states</span> are much less accessible than <span class="hlt">ground</span> <span class="hlt">state</span> (e.g., Hartree-Fock) solutions. <span class="hlt">Energy</span>-based optimization methods for excited <span class="hlt">states</span>, like Δ-SCF (self-consistent field), tend to fall into the lowest solution consistent with a given symmetry-a problem known as "variational collapse." In this work, we combine the ideas of direct <span class="hlt">energy</span>-targeting and variance-based optimization in order to describe excited <span class="hlt">states</span> at the mean-field level. The resulting method, σ-SCF, has several advantages. First, it allows one to target any desired excited <span class="hlt">state</span> by specifying a single parameter: a guess of the <span class="hlt">energy</span> of that <span class="hlt">state</span>. It can therefore, in principle, find all excited <span class="hlt">states</span>. Second, it avoids variational collapse by using a variance-based, unconstrained local minimization. As a consequence, all <span class="hlt">states-ground</span> or excited-are treated on an equal footing. Third, it provides an alternate approach to locate Δ-SCF solutions that are otherwise hardly accessible by the usual non-aufbau configuration initial guess. We present results for this new method for small atoms (He, Be) and molecules (H 2 , HF). We find that σ-SCF is very effective at locating excited <span class="hlt">states</span>, including individual, high <span class="hlt">energy</span> excitations within a dense manifold of excited <span class="hlt">states</span>. Like all single determinant methods, σ-SCF shows prominent spin-symmetry breaking for open shell <span class="hlt">states</span> and our results suggest that this method could be further improved with spin projection.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25396366','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25396366"><span>Trapping cold <span class="hlt">ground</span> <span class="hlt">state</span> argon atoms.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Edmunds, P D; Barker, P F</p> <p>2014-10-31</p> <p>We trap cold, <span class="hlt">ground</span> <span class="hlt">state</span> argon atoms in a deep optical dipole trap produced by a buildup cavity. The atoms, which are a general source for the sympathetic cooling of molecules, are loaded in the trap by quenching them from a cloud of laser-cooled metastable argon atoms. Although the <span class="hlt">ground</span> <span class="hlt">state</span> atoms cannot be directly probed, we detect them by observing the collisional loss of cotrapped metastable argon atoms and determine an elastic cross section. Using a type of parametric loss spectroscopy we also determine the polarizability of the metastable 4s[3/2](2) <span class="hlt">state</span> to be (7.3±1.1)×10(-39)  C m(2)/V. Finally, Penning and associative losses of metastable atoms in the absence of light assisted collisions, are determined to be (3.3±0.8)×10(-10)  cm(3) s(-1).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/circ/1323/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/circ/1323/"><span><span class="hlt">Ground</span>-Water Availability in the United <span class="hlt">States</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Reilly, Thomas E.; Dennehy, Kevin F.; Alley, William M.; Cunningham, William L.</p> <p>2008-01-01</p> <p><span class="hlt">Ground</span> water is among the Nation's most important natural resources. It provides half our drinking water and is essential to the vitality of agriculture and industry, as well as to the health of rivers, wetlands, and estuaries throughout the country. Large-scale development of <span class="hlt">ground</span>-water resources with accompanying declines in <span class="hlt">ground</span>-water levels and other effects of pumping has led to concerns about the future availability of <span class="hlt">ground</span> water to meet domestic, agricultural, industrial, and environmental needs. The challenges in determining <span class="hlt">ground</span>-water availability are many. This report examines what is known about the Nation's <span class="hlt">ground</span>-water availability and outlines a program of study by the U.S. Geological Survey <span class="hlt">Ground</span>-Water Resources Program to improve our understanding of <span class="hlt">ground</span>-water availability in major aquifers across the Nation. The approach is designed to provide useful regional information for <span class="hlt">State</span> and local agencies who manage <span class="hlt">ground</span>-water resources, while providing the building blocks for a national assessment. The report is written for a wide audience interested or involved in the management, protection, and sustainable use of the Nation's water resources.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JMOp...65..501M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JMOp...65..501M"><span>Experimental apparatus for overlapping a <span class="hlt">ground-state</span> cooled ion with ultracold atoms</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Meir, Ziv; Sikorsky, Tomas; Ben-shlomi, Ruti; Akerman, Nitzan; Pinkas, Meirav; Dallal, Yehonatan; Ozeri, Roee</p> <p>2018-03-01</p> <p>Experimental realizations of charged ions and neutral atoms in overlapping traps are gaining increasing interest due to their wide research application ranging from chemistry at the quantum level to quantum simulations of solid <span class="hlt">state</span> systems. In this paper, we describe our experimental system in which we overlap a single <span class="hlt">ground-state</span> cooled ion trapped in a linear Paul trap with a cloud of ultracold atoms such that both constituents are in the ?K regime. Excess micromotion (EMM) currently limits atom-ion interaction <span class="hlt">energy</span> to the mK <span class="hlt">energy</span> scale and above. We demonstrate spectroscopy methods and compensation techniques which characterize and reduce the ion's parasitic EMM <span class="hlt">energy</span> to the ?K regime even for ion crystals of several ions. We further give a substantial review on the non-equilibrium dynamics which governs atom-ion systems. The non-equilibrium dynamics is manifested by a power law distribution of the ion's <span class="hlt">energy</span>. We also give an overview on the coherent and non-coherent thermometry tools which can be used to characterize the ion's <span class="hlt">energy</span> distribution after single to many atom-ion collisions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhRvB..96m4426H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvB..96m4426H"><span>Quantifying confidence in density functional theory predictions of magnetic <span class="hlt">ground</span> <span class="hlt">states</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Houchins, Gregory; Viswanathan, Venkatasubramanian</p> <p>2017-10-01</p> <p>Density functional theory (DFT) simulations, at the generalized gradient approximation (GGA) level, are being routinely used for material discovery based on high-throughput descriptor-based searches. The success of descriptor-based material design relies on eliminating bad candidates and keeping good candidates for further investigation. While DFT has been widely successfully for the former, oftentimes good candidates are lost due to the uncertainty associated with the DFT-predicted material properties. Uncertainty associated with DFT predictions has gained prominence and has led to the development of exchange correlation functionals that have built-in error estimation capability. In this work, we demonstrate the use of built-in error estimation capabilities within the BEEF-vdW exchange correlation functional for quantifying the uncertainty associated with the magnetic <span class="hlt">ground</span> <span class="hlt">state</span> of solids. We demonstrate this approach by calculating the uncertainty estimate for the <span class="hlt">energy</span> difference between the different magnetic <span class="hlt">states</span> of solids and compare them against a range of GGA exchange correlation functionals as is done in many first-principles calculations of materials. We show that this estimate reasonably bounds the range of values obtained with the different GGA functionals. The estimate is determined as a postprocessing step and thus provides a computationally robust and systematic approach to estimating uncertainty associated with predictions of magnetic <span class="hlt">ground</span> <span class="hlt">states</span>. We define a confidence value (c-value) that incorporates all calculated magnetic <span class="hlt">states</span> in order to quantify the concurrence of the prediction at the GGA level and argue that predictions of magnetic <span class="hlt">ground</span> <span class="hlt">states</span> from GGA level DFT is incomplete without an accompanying c-value. We demonstrate the utility of this method using a case study of Li-ion and Na-ion cathode materials and the c-value metric correctly identifies that GGA-level DFT will have low predictability for NaFePO4F . Further, there</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19880003321','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19880003321"><span>X-<span class="hlt">band</span> uplink <span class="hlt">ground</span> systems development: Part 2</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Johns, C. E.</p> <p>1987-01-01</p> <p>The prototype X-<span class="hlt">band</span> exciter testing has been completed. Stability and single-sideband phase noise measurements have been made on the X-<span class="hlt">band</span> exciter signal (7.145-7.235 GHz) and on the coherent X- and S-<span class="hlt">band</span> receiver test signals (8.4-8.5 GHz and 2.29-2.3 GHz) generated within the exciter equipment. Outputs are well within error budgets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22657861-transition-state-region-band-photodissociation-allyl-iodidea-femtosecond-extreme-ultraviolet-transient-absorption-study','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22657861-transition-state-region-band-photodissociation-allyl-iodidea-femtosecond-extreme-ultraviolet-transient-absorption-study"><span>Transition <span class="hlt">state</span> region in the A-<span class="hlt">Band</span> photodissociation of allyl iodide—A femtosecond extreme ultraviolet transient absorption study</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>Bhattacherjee, Aditi, E-mail: abhattacherjee@berkeley.edu, E-mail: andrewattar@berkeley.edu; Attar, Andrew R., E-mail: abhattacherjee@berkeley.edu, E-mail: andrewattar@berkeley.edu; Chemical Sciences Division, Lawrence Berkeley National Laboratory, Berkeley, California 94720</p> <p>2016-03-28</p> <p>Femtosecond extreme ultraviolet (XUV) transient absorption spectroscopy based on a high-harmonic generation source is used to study the 266 nm induced A-<span class="hlt">band</span> photodissociation dynamics of allyl iodide (CH{sub 2} =CHCH{sub 2}I). The photolysis of the C—I bond at this wavelength produces iodine atoms both in the <span class="hlt">ground</span> ({sup 2}P{sub 3/2}, I) and spin-orbit excited ({sup 2}P{sub 1/2}, I*) <span class="hlt">states</span>, with the latter as the predominant channel. Using XUV absorption at the iodine N{sub 4/5} edge (45–60 eV), the experiments constitute a direct probe of not only the long-lived atomic iodine reaction products but also the fleeting transition <span class="hlt">state</span> region ofmore » the repulsive n{sub I}σ{sup ∗}{sub C—I} excited <span class="hlt">states</span>. Specifically, three distinct features are identified in the XUV transient absorption spectrum at 45.3 eV, 47.4 eV, and 48.4 eV (denoted transients A, B, and C, respectively), which arise from the repulsive valence-excited nσ{sup ∗} <span class="hlt">states</span> and project onto the high-lying core-excited <span class="hlt">states</span> of the dissociating molecule via excitation of 4d(I) core electrons. Transients A and B originate from 4d(I) → n(I) core-to-valence transitions, whereas transient C is best assigned to a 4d(I) →σ{sup ∗}(C—I) transition. The measured differential absorbance of these new features along with the I/I* branching ratios known from the literature is used to suggest a more definitive assignment, albeit provisional, of the transients to specific dissociative <span class="hlt">states</span> within the A-<span class="hlt">band</span> manifold. The transients are found to peak around 55 fs–65 fs and decay completely by 145 fs–185 fs, demonstrating the ability of XUV spectroscopy to map the evolution of reactants into products in real time. The similarity in the <span class="hlt">energies</span> of transients A and B with analogous features observed in methyl iodide [Attar et al. J. Phys. Chem. Lett. 6, 5072, (2015)] together with the new observation of transient C in the present work provides a more complete picture of the valence</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JChPh.147u4104Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JChPh.147u4104Y"><span>σ-SCF: A direct <span class="hlt">energy</span>-targeting method to mean-field excited <span class="hlt">states</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ye, Hong-Zhou; Welborn, Matthew; Ricke, Nathan D.; Van Voorhis, Troy</p> <p>2017-12-01</p> <p>The mean-field solutions of electronic excited <span class="hlt">states</span> are much less accessible than <span class="hlt">ground</span> <span class="hlt">state</span> (e.g., Hartree-Fock) solutions. <span class="hlt">Energy</span>-based optimization methods for excited <span class="hlt">states</span>, like Δ-SCF (self-consistent field), tend to fall into the lowest solution consistent with a given symmetry—a problem known as "variational collapse." In this work, we combine the ideas of direct <span class="hlt">energy</span>-targeting and variance-based optimization in order to describe excited <span class="hlt">states</span> at the mean-field level. The resulting method, σ-SCF, has several advantages. First, it allows one to target any desired excited <span class="hlt">state</span> by specifying a single parameter: a guess of the <span class="hlt">energy</span> of that <span class="hlt">state</span>. It can therefore, in principle, find all excited <span class="hlt">states</span>. Second, it avoids variational collapse by using a variance-based, unconstrained local minimization. As a consequence, all states—<span class="hlt">ground</span> or excited—are treated on an equal footing. Third, it provides an alternate approach to locate Δ-SCF solutions that are otherwise hardly accessible by the usual non-aufbau configuration initial guess. We present results for this new method for small atoms (He, Be) and molecules (H2, HF). We find that σ-SCF is very effective at locating excited <span class="hlt">states</span>, including individual, high <span class="hlt">energy</span> excitations within a dense manifold of excited <span class="hlt">states</span>. Like all single determinant methods, σ-SCF shows prominent spin-symmetry breaking for open shell <span class="hlt">states</span> and our results suggest that this method could be further improved with spin projection.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009A%26A...493L..35D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009A%26A...493L..35D"><span><span class="hlt">Ground</span>-based K-<span class="hlt">band</span> detection of thermal emission from the exoplanet TrES-3b</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>de Mooij, E. J. W.; Snellen, I. A. G.</p> <p>2009-01-01</p> <p>Context: Secondary eclipse measurements of transiting extrasolar planets with the Spitzer Space Telescope have yielded several direct detections of thermal exoplanet light. Since Spitzer operates at wavelengths longward of 3.6 μm, arguably one of the most interesting parts of the planet spectrum (from 1 to 3 μm) is inaccessible with this satellite. This region is at the peak of the planet's spectral <span class="hlt">energy</span> distribution and is also the regime where molecular absorption <span class="hlt">bands</span> can significantly influence the measured emission. Aims: So far, 2.2 μm K-<span class="hlt">band</span> secondary eclipse measurements, which are possible from the <span class="hlt">ground</span>, have not yet lead to secure detections. The aim of this paper is to measure the secondary eclipse of the very hot Jupiter TrES-3b in K-<span class="hlt">band</span>, and in addition to observe its transit, to obtain an accurate planet radius in the near infrared. Methods: We have used the william herschell telescope (WHT) to observe the secondary eclipse, and the united kingdom infrared telescope (UKIRT) to observe the transit of TrES-3b. Both observations involved significant defocusing of the telescope, aimed to produce high-cadence time series of several thousand frames at high efficiency, with the starlight spread out over many pixels. Results: We detect the secondary eclipse of TrES-3b with a depth of -0.241 ± 0.043% (~6σ). This corresponds to a day-side brightness temperature of TB(2.2 μm) = 2040 ± 185 K, which is consistent with current models of the physical properties of this planet's upper atmosphere. The centre of the eclipse seems slightly offset from phase φ=0.5 by Δφ = -0.0042 ± 0.0027, which could indicate that the orbit of TrES-3b is non-circular. Analysis of the transit data shows that TrES-3b has a near-infrared radius of 1.338 ± 0.016 R_Jup, showing no significant deviation from optical measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018NuPhA.970..398I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018NuPhA.970..398I"><span>The Gamow-<span class="hlt">state</span> description of the decay <span class="hlt">energy</span> spectrum of neutron-unbound 25O</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Id Betan, R. M.; de la Madrid, R.</p> <p>2018-02-01</p> <p>We show the feasibility of calculating the decay <span class="hlt">energy</span> spectrum of neutron emitting nuclei within the Gamow-<span class="hlt">state</span> description of resonances by obtaining the decay <span class="hlt">energy</span> spectrum of 25O. We model this nucleus as a valence neutron interacting with an 24O inert core, and we obtain the resulting resonant <span class="hlt">energies</span>, widths and decay <span class="hlt">energy</span> spectra for the <span class="hlt">ground</span> and first excited <span class="hlt">states</span>. We also discuss the similarities and differences between the decay <span class="hlt">energy</span> spectrum of a Gamow <span class="hlt">state</span> and the Breit-Wigner distribution with <span class="hlt">energy</span>-dependent width.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29462724','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29462724"><span>Maturation trajectories of cortical resting-<span class="hlt">state</span> networks depend on the mediating frequency <span class="hlt">band</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Khan, Sheraz; Hashmi, Javeria A; Mamashli, Fahimeh; Michmizos, Konstantinos; Kitzbichler, Manfred G; Bharadwaj, Hari; Bekhti, Yousra; Ganesan, Santosh; Garel, Keri-Lee A; Whitfield-Gabrieli, Susan; Gollub, Randy L; Kong, Jian; Vaina, Lucia M; Rana, Kunjan D; Stufflebeam, Steven M; Hämäläinen, Matti S; Kenet, Tal</p> <p>2018-07-01</p> <p>The functional significance of resting <span class="hlt">state</span> networks and their abnormal manifestations in psychiatric disorders are firmly established, as is the importance of the cortical rhythms in mediating these networks. Resting <span class="hlt">state</span> networks are known to undergo substantial reorganization from childhood to adulthood, but whether distinct cortical rhythms, which are generated by separable neural mechanisms and are often manifested abnormally in psychiatric conditions, mediate maturation differentially, remains unknown. Using magnetoencephalography (MEG) to map frequency <span class="hlt">band</span> specific maturation of resting <span class="hlt">state</span> networks from age 7 to 29 in 162 participants (31 independent), we found significant changes with age in networks mediated by the beta (13-30 Hz) and gamma (31-80 Hz) <span class="hlt">bands</span>. More specifically, gamma <span class="hlt">band</span> mediated networks followed an expected asymptotic trajectory, but beta <span class="hlt">band</span> mediated networks followed a linear trajectory. Network integration increased with age in gamma <span class="hlt">band</span> mediated networks, while local segregation increased with age in beta <span class="hlt">band</span> mediated networks. Spatially, the hubs that changed in importance with age in the beta <span class="hlt">band</span> mediated networks had relatively little overlap with those that showed the greatest changes in the gamma <span class="hlt">band</span> mediated networks. These findings are relevant for our understanding of the neural mechanisms of cortical maturation, in both typical and atypical development. Copyright © 2018. Published by Elsevier Inc.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25553979','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25553979"><span>Resting-<span class="hlt">state</span> theta-<span class="hlt">band</span> connectivity and verbal memory in schizophrenia and in the high-risk <span class="hlt">state</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Andreou, Christina; Leicht, Gregor; Nolte, Guido; Polomac, Nenad; Moritz, Steffen; Karow, Anne; Hanganu-Opatz, Ileana L; Engel, Andreas K; Mulert, Christoph</p> <p>2015-02-01</p> <p>Disturbed functional connectivity is assumed to underlie neurocognitive deficits in patients with schizophrenia. As neurocognitive deficits are already present in the high-risk <span class="hlt">state</span>, identification of the neural networks involved in this core feature of schizophrenia is essential to our understanding of the disorder. Resting-<span class="hlt">state</span> studies enable such investigations, while at the same time avoiding the known confounder of impaired task performance in patients. The aim of the present study was to investigate EEG resting-<span class="hlt">state</span> connectivity in high-risk individuals (HR) compared to first episode patients with schizophrenia (SZ) and to healthy controls (HC), and its association with cognitive deficits. 64-channel resting-<span class="hlt">state</span> EEG recordings (eyes closed) were obtained for 28 HR, 19 stable SZ, and 23 HC, matched for age, education, and parental education. The imaginary coherence-based multivariate interaction measure (MIM) was used as a measure of connectivity across 80 cortical regions and six frequency <span class="hlt">bands</span>. Mean connectivity at each region was compared across groups using the non-parametric randomization approach. Additionally, the network-based statistic was applied to identify affected networks in patients. SZ displayed increased theta-<span class="hlt">band</span> resting-<span class="hlt">state</span> MIM connectivity across midline, sensorimotor, orbitofrontal regions and the left temporoparietal junction. HR displayed intermediate theta-<span class="hlt">band</span> connectivity patterns that did not differ from either SZ or HC. Mean theta-<span class="hlt">band</span> connectivity within the above network partially mediated verbal memory deficits in SZ and HR. Aberrant theta-<span class="hlt">band</span> connectivity may represent a trait characteristic of schizophrenia associated with neurocognitive deficits. As such, it might constitute a promising target for novel treatment applications. Copyright © 2014 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1371922-ground-state-properties-h5-from-he6-he3-h5-reaction','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1371922-ground-state-properties-h5-from-he6-he3-h5-reaction"><span><span class="hlt">Ground-state</span> properties of H 5 from the He 6 ( d , He 3 ) H 5 reaction</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>Wuosmaa, A. H.; Bedoor, S.; Brown, K. W.</p> <p>2017-01-01</p> <p>We have studied the <span class="hlt">ground</span> <span class="hlt">state</span> of the unbound, very neutron-rich isotope of hydrogen 5H, using the 6He(d,3He)5H reaction in inverse kinematics at a bombarding <span class="hlt">energy</span> of E(6He)=55A MeV. The present results suggest a <span class="hlt">ground-state</span> resonance <span class="hlt">energy</span> ER=2.4±0.3 MeV above the 3H+2n threshold, with an intrinsic width of Γ=5.3±0.4 MeV in the 5H system. Both the resonance <span class="hlt">energy</span> and width are higher than those reported in some, but not all previous studies of 5H. The previously unreported 6He(d,t)5Heg.s. reaction is observed in the same measurement, providing a check on the understanding of the response of the apparatus. The data aremore » compared to expectations from direct two-neutron and dineutron decay. The possibility of excited <span class="hlt">states</span> of 5H populated in this reaction is discussed using different calculations of the 6He→5H+p spectroscopic overlaps from shell-model and ab initio nuclear-structure calculations.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JQSRT.210...44H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JQSRT.210...44H"><span>Line list for the <span class="hlt">ground</span> <span class="hlt">state</span> of CaF</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hou, Shilin; Bernath, Peter F.</p> <p>2018-05-01</p> <p>The molecular potential <span class="hlt">energy</span> function and electronic dipole moment function for the <span class="hlt">ground</span> <span class="hlt">state</span> of CaF were studied with MRCI, ACPF, and RCCSD(T) ab initio calculations. The RCCSD(T) potential function reproduces the experimental vibrational intervals to within ∼2 cm-1. The RCCSD(T) dipole moment at the equilibrium internuclear separation agrees well with the experimental value. Over a wide range of internuclear separations, far beyond the range associated with the observed spectra, the ab initio dipole moment functions are similar and highly linear. An extended Morse oscillator (EMO) potential function was also obtained by fitting the observed lines of the laboratory vibration-rotation and pure rotation spectra of the 40CaF X2Σ+ <span class="hlt">ground</span> <span class="hlt">state</span>. The fitted potential reproduces the observed transitions (v ≤ 8, N ≤ 121, Δv = 0, 1) within their experimental uncertainties. With this EMO potential and the RCCSD(T) dipole moment function, line lists for 40CaF, 42CaF, 43CaF, 44CaF, 46CaF, and 48CaF were computed for v ≤ 10, N ≤ 121, Δv = 0-10. The calculated emission spectra are in good agreement with an observed laboratory spectrum of CaF at a sample temperature of 1873 K.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1356572-simultaneous-low-state-spectral-energy-distribution-from-radio-very-high-energies','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1356572-simultaneous-low-state-spectral-energy-distribution-from-radio-very-high-energies"><span>The simultaneous low <span class="hlt">state</span> spectral <span class="hlt">energy</span> distribution of 1ES 2344+514 from radio to very high <span class="hlt">energies</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Aleksić, J.; Antonelli, L. A.; Antoranz, P.; ...</p> <p>2013-07-31</p> <p>Here, BL Lacertae objects are variable at all <span class="hlt">energy</span> <span class="hlt">bands</span> on time scales down to minutes. To construct and interpret their spectral <span class="hlt">energy</span> distribution (SED), simultaneous broad-<span class="hlt">band</span> observations are mandatory. Up to now, the number of objects studied during such campaigns is very limited and biased towards high flux <span class="hlt">states</span>. Furthermore, we present the results of a dedicated multi-wavelength study of the high-frequency peaked BL Lacertae (HBL) object and known TeV emitter 1ES 2344+514 by means of a pre-organised campaign. The observations were conducted during simultaneous visibility windows of MAGIC and AGILE in late 2008. The measurements were complemented bymore » Metsähovi, RATAN-600, KVA+Tuorla, Swift and VLBA pointings. Additional coverage was provided by the ongoing long-term F-GAMMA and MOJAVE programs, the OVRO 40-m and CrAO telescopes as well as the Fermi satellite. The obtained SEDs are modelled using a one-zone as well as a self-consistent two-zone synchrotron self-Compton model. As a result, 1ES 2344+514 was found at very low flux <span class="hlt">states</span> in both X-rays and very high <span class="hlt">energy</span> gamma rays. Variability was detected in the low frequency radio and X-ray <span class="hlt">bands</span> only, where for the latter a small flare was observed. The X-ray flare was possibly caused by shock acceleration characterised by similar cooling and acceleration time scales. MOJAVE VLBA monitoring reveals a static jet whose components are stable over time scales of eleven years, contrary to previous findings. There appears to be no significant correlation between the 15 GHz and R-<span class="hlt">band</span> monitoring light curves. The observations presented here constitute the first multi-wavelength campaign on 1ES 2344+514 from radio to VHE <span class="hlt">energies</span> and one of the few simultaneous SEDs during low activity <span class="hlt">states</span>. The quasi-simultaneous Fermi-LAT data poses some challenges for SED modelling, but in general the SEDs are described well by both applied models. The resulting parameters are typical for TeV emitting HBLs</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19800019173','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19800019173"><span>The GSFC Mark-2 three <span class="hlt">band</span> hand-held radiometer. [thematic mapper for <span class="hlt">ground</span> truth data collection</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Tucker, C. J.; Jones, W. H.; Kley, W. A.; Sundstrom, G. J.</p> <p>1980-01-01</p> <p>A self-contained, portable, hand-radiometer designed for field usage was constructed and tested. The device, consisting of a hand-held probe containing three sensors and a strap supported electronic module, weighs 4 1/2 kilograms. It is powered by flashlight and transistor radio batteries, utilizes two silicon and one lead sulfide detectors, has three liquid crystal displays, sample and hold radiometric sampling, and its spectral configuration corresponds to LANDSAT-D's thematic mapper <span class="hlt">bands</span>. The device was designed to support thematic mapper <span class="hlt">ground</span>-truth data collection efforts and to facilitate 'in situ' <span class="hlt">ground</span>-based remote sensing studies of natural materials. Prototype instruments were extensively tested under laboratory and field conditions with excellent results.</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/2016APS..DMP.D1128W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..DMP.D1128W"><span>Molecular spectroscopy for producing ultracold <span class="hlt">ground-state</span> NaRb molecules</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Dajun; Guo, Mingyang; Zhu, Bing; Lu, Bo; Ye, Xin; Wang, Fudong; Vexiau, Romain; Bouloufa-Maafa, Nadia; Quéméner, Goulven; Dulieu, Olivier</p> <p>2016-05-01</p> <p>Recently, we have successfully created an ultracold sample of absolute <span class="hlt">ground-state</span> NaRb molecules by two-photon Raman transfer of weakly bound Feshbach molecules. Here we will present the detailed spectroscopic investigations on both the excited and the rovibrational <span class="hlt">ground</span> <span class="hlt">states</span> for finding the two-photon path. For the excited <span class="hlt">state</span>, we focus on the A1Σ+ /b3 Π singlet and triplet admixture. We discovered an anomalously strong coupling between the Ω =0+ and 0- components which renders efficient population transfer possible. In the <span class="hlt">ground</span> <span class="hlt">state</span>, the pure nuclear hyperfine levels have been clearly resolved, which allows us to create molecules in the absolute <span class="hlt">ground</span> <span class="hlt">state</span> directly with Raman transfer. This work is jointly supported by Agence Nationale de la Recherche (#ANR-13- IS04-0004-01) and Hong Kong Research Grant Council (#A-CUHK403/13) through the COPOMOL project.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4960298','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4960298"><span>Magnetic <span class="hlt">ground</span> <span class="hlt">state</span> of FeSe</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Wang, Qisi; Shen, Yao; Pan, Bingying; Zhang, Xiaowen; Ikeuchi, K.; Iida, K.; Christianson, A. D.; Walker, H. C.; Adroja, D. T.; Abdel-Hafiez, M.; Chen, Xiaojia; Chareev, D. A.; Vasiliev, A. N.; Zhao, Jun</p> <p>2016-01-01</p> <p>Elucidating the nature of the magnetism of a high-temperature superconductor is crucial for establishing its pairing mechanism. The parent compounds of the cuprate and iron-pnictide superconductors exhibit Néel and stripe magnetic order, respectively. However, FeSe, the structurally simplest iron-based superconductor, shows nematic order (Ts=90 K), but not magnetic order in the parent phase, and its magnetic <span class="hlt">ground</span> <span class="hlt">state</span> is intensely debated. Here we report inelastic neutron-scattering experiments that reveal both stripe and Néel spin fluctuations over a wide <span class="hlt">energy</span> range at 110 K. On entering the nematic phase, a substantial amount of spectral weight is transferred from the Néel to the stripe spin fluctuations. Moreover, the total fluctuating magnetic moment of FeSe is ∼60% larger than that in the iron pnictide BaFe2As2. Our results suggest that FeSe is a novel S=1 nematic quantum-disordered paramagnet interpolating between the Néel and stripe magnetic instabilities. PMID:27431986</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27431986','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27431986"><span>Magnetic <span class="hlt">ground</span> <span class="hlt">state</span> of FeSe.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Qisi; Shen, Yao; Pan, Bingying; Zhang, Xiaowen; Ikeuchi, K; Iida, K; Christianson, A D; Walker, H C; Adroja, D T; Abdel-Hafiez, M; Chen, Xiaojia; Chareev, D A; Vasiliev, A N; Zhao, Jun</p> <p>2016-07-19</p> <p>Elucidating the nature of the magnetism of a high-temperature superconductor is crucial for establishing its pairing mechanism. The parent compounds of the cuprate and iron-pnictide superconductors exhibit Néel and stripe magnetic order, respectively. However, FeSe, the structurally simplest iron-based superconductor, shows nematic order (Ts=90 K), but not magnetic order in the parent phase, and its magnetic <span class="hlt">ground</span> <span class="hlt">state</span> is intensely debated. Here we report inelastic neutron-scattering experiments that reveal both stripe and Néel spin fluctuations over a wide <span class="hlt">energy</span> range at 110 K. On entering the nematic phase, a substantial amount of spectral weight is transferred from the Néel to the stripe spin fluctuations. Moreover, the total fluctuating magnetic moment of FeSe is ∼60% larger than that in the iron pnictide BaFe2As2. Our results suggest that FeSe is a novel S=1 nematic quantum-disordered paramagnet interpolating between the Néel and stripe magnetic instabilities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1999SPIE.3797..178S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1999SPIE.3797..178S"><span><span class="hlt">Energy</span> level alignment and <span class="hlt">band</span> bending at organic interfaces</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Seki, Kazuhiko; Oji, Hiroshi; Ito, Eisuke; Hayashi, Naoki; Ouchi, Yukio; Ishii, Hisao</p> <p>1999-12-01</p> <p>Recent progress in the study of the <span class="hlt">energy</span> level alignment and <span class="hlt">band</span> 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 <span class="hlt">energy</span> 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 <span class="hlt">band</span> bending, the careful examination of the existence/absence of <span class="hlt">band</span> bending of purified TPD* molecule deposited on various metals in ultrahigh vacuum (UHV) revealed negligible <span class="hlt">band</span> 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).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17995195','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17995195"><span>NiO: correlated <span class="hlt">band</span> structure of a charge-transfer insulator.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kunes, J; Anisimov, V I; Skornyakov, S L; Lukoyanov, A V; Vollhardt, D</p> <p>2007-10-12</p> <p>The <span class="hlt">band</span> structure of the prototypical charge-transfer insulator NiO is computed by using a combination of an ab initio <span class="hlt">band</span> structure method and the dynamical mean-field theory with a quantum Monte-Carlo impurity solver. Employing a Hamiltonian which includes both Ni d and O p orbitals we find excellent agreement with the <span class="hlt">energy</span> <span class="hlt">bands</span> determined from angle-resolved photoemission spectroscopy. This brings an important progress in a long-standing problem of solid-<span class="hlt">state</span> theory. Most notably we obtain the low-<span class="hlt">energy</span> Zhang-Rice <span class="hlt">bands</span> with strongly k-dependent orbital character discussed previously in the context of low-<span class="hlt">energy</span> model theories.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22251750-trap-density-states-channel-organic-transistors-variable-temperature-characteristics-band-transport','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22251750-trap-density-states-channel-organic-transistors-variable-temperature-characteristics-band-transport"><span>Trap density of <span class="hlt">states</span> in n-channel organic transistors: variable temperature characteristics and <span class="hlt">band</span> transport</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>Cho, Joung-min, E-mail: cho.j.ad@m.titech.ac.jp; Akiyama, Yuto; Kakinuma, Tomoyuki</p> <p>2013-10-15</p> <p>We have investigated trap density of <span class="hlt">states</span> (trap DOS) in n-channel organic field-effect transistors based on N,N ’-bis(cyclohexyl)naphthalene diimide (Cy-NDI) and dimethyldicyanoquinonediimine (DMDCNQI). A new method is proposed to extract trap DOS from the Arrhenius plot of the temperature-dependent transconductance. Double exponential trap DOS are observed, in which Cy-NDI has considerable deep <span class="hlt">states</span>, by contrast, DMDCNQI has substantial tail <span class="hlt">states</span>. In addition, numerical simulation of the transistor characteristics has been conducted by assuming an exponential trap distribution and the interface approximation. Temperature dependence of transfer characteristics are well reproduced only using several parameters, and the trap DOS obtained from the simulatedmore » characteristics are in good agreement with the assumed trap DOS, indicating that our analysis is self-consistent. Although the experimentally obtained Meyer-Neldel temperature is related to the trap distribution width, the simulation satisfies the Meyer-Neldel rule only very phenomenologically. The simulation also reveals that the subthreshold swing is not always a good indicator of the total trap amount, because it also largely depends on the trap distribution width. Finally, <span class="hlt">band</span> transport is explored from the simulation having a small number of traps. A crossing point of the transfer curves and negative activation <span class="hlt">energy</span> above a certain gate voltage are observed in the simulated characteristics, where the critical V{sub G} above which <span class="hlt">band</span> transport is realized is determined by the sum of the trapped and free charge <span class="hlt">states</span> below the conduction <span class="hlt">band</span> edge.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19790011018','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19790011018"><span>Shuttle Ku-<span class="hlt">band</span> and S-<span class="hlt">band</span> communications implementations study</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Huth, G. K.; Nessibou, T.; Nilsen, P. W.; Simon, M. K.; Weber, C. L.</p> <p>1979-01-01</p> <p>The interfaces between the Ku-<span class="hlt">band</span> system and the TDRSS, between the S-<span class="hlt">band</span> system and the TDRSS, GSTDN and SGLS networks, and between the S-<span class="hlt">band</span> payload communication equipment and the other Orbiter avionic equipment were investigated. The principal activities reported are: (1) performance analysis of the payload narrowband bent-pipe through the Ku-<span class="hlt">band</span> communication system; (2) performance evaluation of the TDRSS user constraints placed on the S-<span class="hlt">band</span> and Ku-<span class="hlt">band</span> communication systems; (3) assessment of the shuttle-unique S-<span class="hlt">band</span> TDRSS <span class="hlt">ground</span> station false lock susceptibility; (4) development of procedure to make S-<span class="hlt">band</span> antenna measurements during orbital flight; (5) development of procedure to make RFI measurements during orbital flight to assess the performance degradation to the TDRSS S-<span class="hlt">band</span> communication link; and (6) analysis of the payload interface integration problem areas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014APS..DNP.EB003M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014APS..DNP.EB003M"><span><span class="hlt">Ground-state</span> <span class="hlt">energies</span> and charge radii of medium-mass nuclei in the unitary-model-operator approach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Miyagi, Takayuki; Abe, Takashi; Okamoto, Ryoji; Otsuka, Takaharu</p> <p>2014-09-01</p> <p>In nuclear structure theory, one of the most fundamental problems is to understand the nuclear structure based on nuclear forces. This attempt has been enabled due to the progress of the computational power and nuclear many-body approaches. However, it is difficult to apply the first-principle methods to medium-mass region, because calculations demand the huge model space as increasing the number of nucleons. The unitary-model-operator approach (UMOA) is one of the methods which can be applied to medium-mass nuclei. The essential point of the UMOA is to construct the effective Hamiltonian which does not induce the two-particle-two-hole excitations. A many-body problem is reduced to the two-body subsystem problem in an entire many-body system with the two-body effective interaction and one-body potential determined self-consistently. In this presentation, we will report the numerical results of <span class="hlt">ground-state</span> <span class="hlt">energies</span> and charge radii of 16O, 40Ca, and 56Ni in the UMOA, and discuss the saturation property by comparing our results with those in the other many-body methods and also experimental data. In nuclear structure theory, one of the most fundamental problems is to understand the nuclear structure based on nuclear forces. This attempt has been enabled due to the progress of the computational power and nuclear many-body approaches. However, it is difficult to apply the first-principle methods to medium-mass region, because calculations demand the huge model space as increasing the number of nucleons. The unitary-model-operator approach (UMOA) is one of the methods which can be applied to medium-mass nuclei. The essential point of the UMOA is to construct the effective Hamiltonian which does not induce the two-particle-two-hole excitations. A many-body problem is reduced to the two-body subsystem problem in an entire many-body system with the two-body effective interaction and one-body potential determined self-consistently. In this presentation, we will report the</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 electronic and optoelectronic devices requires a fundamental understanding in their electronic structure as a function of strain. Previous experimental and theoretical studies assume that an identical strain and/or stress <span class="hlt">state</span> 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 electronic <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 electronic 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://www.ncbi.nlm.nih.gov/pubmed/19948132','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19948132"><span>Low light adaptation: <span class="hlt">energy</span> transfer processes in different types of light harvesting complexes from Rhodopseudomonas palustris.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Moulisová, Vladimíra; Luer, Larry; Hoseinkhani, Sajjad; Brotosudarmo, Tatas H P; Collins, Aaron M; Lanzani, Guglielmo; Blankenship, Robert E; Cogdell, Richard J</p> <p>2009-12-02</p> <p><span class="hlt">Energy</span> transfer processes in photosynthetic light harvesting 2 (LH2) complexes isolated from purple bacterium Rhodopseudomonas palustris grown at different light intensities were studied by <span class="hlt">ground</span> <span class="hlt">state</span> and transient absorption spectroscopy. The decomposition of <span class="hlt">ground</span> <span class="hlt">state</span> absorption spectra shows contributions from B800 and B850 bacteriochlorophyll (BChl) a rings, the latter component splitting into a low <span class="hlt">energy</span> and a high <span class="hlt">energy</span> <span class="hlt">band</span> in samples grown under low light (LL) conditions. A spectral analysis reveals strong inhomogeneity of the B850 excitons in the LL samples that is well reproduced by an exponential-type distribution. Transient spectra show a bleach of both the low <span class="hlt">energy</span> and high <span class="hlt">energy</span> <span class="hlt">bands</span>, together with the respective blue-shifted exciton-to-biexciton transitions. The different spectral evolutions were analyzed by a global fitting procedure. <span class="hlt">Energy</span> transfer from B800 to B850 occurs in a mono-exponential process and the rate of this process is only slightly reduced in LL compared to high light samples. In LL samples, spectral relaxation of the B850 exciton follows strongly nonexponential kinetics that can be described by a reduction of the bleach of the high <span class="hlt">energy</span> excitonic component and a red-shift of the low energetic one. We explain these spectral changes by picosecond exciton relaxation caused by a small coupling parameter of the excitonic splitting of the BChl a molecules to the surrounding bath. The splitting of exciton <span class="hlt">energy</span> into two excitonic <span class="hlt">bands</span> in LL complex is most probably caused by heterogenous composition of LH2 apoproteins that gives some of the BChls in the B850 ring B820-like site <span class="hlt">energies</span>, and causes a disorder in LH2 structure.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007CoPhC.177..787D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007CoPhC.177..787D"><span><span class="hlt">Ground</span> <span class="hlt">state</span> of the time-independent Gross Pitaevskii equation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dion, Claude M.; Cancès, Eric</p> <p>2007-11-01</p> <p>We present a suite of programs to determine the <span class="hlt">ground</span> <span class="hlt">state</span> of the time-independent Gross-Pitaevskii equation, used in the simulation of Bose-Einstein condensates. The calculation is based on the Optimal Damping Algorithm, ensuring a fast convergence to the true <span class="hlt">ground</span> <span class="hlt">state</span>. Versions are given for the one-, two-, and three-dimensional equation, using either a spectral method, well suited for harmonic trapping potentials, or a spatial grid. Program summaryProgram title: GPODA Catalogue identifier: ADZN_v1_0 Program summary URL:http://cpc.cs.qub.ac.uk/summaries/ADZN_v1_0.html Program obtainable from: CPC Program Library, Queen's University, Belfast, N. Ireland Licensing provisions: Standard CPC licence, http://cpc.cs.qub.ac.uk/licence/licence.html No. of lines in distributed program, including test data, etc.: 5339 No. of bytes in distributed program, including test data, etc.: 19 426 Distribution format: tar.gz Programming language: Fortran 90 Computer: ANY (Compilers under which the program has been tested: Absoft Pro Fortran, The Portland Group Fortran 90/95 compiler, Intel Fortran Compiler) RAM: From <1 MB in 1D to ˜10 MB for a large 3D grid Classification: 2.7, 4.9 External routines: LAPACK, BLAS, DFFTPACK Nature of problem: The order parameter (or wave function) of a Bose-Einstein condensate (BEC) is obtained, in a mean field approximation, by the Gross-Pitaevskii equation (GPE) [F. Dalfovo, S. Giorgini, L.P. Pitaevskii, S. Stringari, Rev. Mod. Phys. 71 (1999) 463]. The GPE is a nonlinear Schrödinger-like equation, including here a confining potential. The stationary <span class="hlt">state</span> of a BEC is obtained by finding the <span class="hlt">ground</span> <span class="hlt">state</span> of the time-independent GPE, i.e., the order parameter that minimizes the <span class="hlt">energy</span>. In addition to the standard three-dimensional GPE, tight traps can lead to effective two- or even one-dimensional BECs, so the 2D and 1D GPEs are also considered. Solution method: The <span class="hlt">ground</span> <span class="hlt">state</span> of the time-independent of the GPE is calculated using the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhRvB..95p5110L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvB..95p5110L"><span><span class="hlt">Ground-state</span> phase diagram of an anisotropic spin-1/2 model on the triangular lattice</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Luo, Qiang; Hu, Shijie; Xi, Bin; Zhao, Jize; Wang, Xiaoqun</p> <p>2017-04-01</p> <p>Motivated by a recent experiment on the rare-earth material YbMgGaO4 [Y. Li et al., Phys. Rev. Lett. 115, 167203 (2015), 10.1103/PhysRevLett.115.167203], which found that the <span class="hlt">ground</span> <span class="hlt">state</span> of YbMgGaO4 is a quantum spin liquid, we study the <span class="hlt">ground-state</span> phase diagram of an anisotropic spin-1 /2 model that was proposed to describe YbMgGaO4. Using the density matrix renormalization-group method in combination with the exact-diagonalization method, we calculate a variety of physical quantities, including the <span class="hlt">ground-state</span> <span class="hlt">energy</span>, the fidelity, the entanglement entropy and spin-spin correlation functions. Our studies show that in the quantum phase diagram, there is a 120∘ phase and two distinct stripe phases. The transitions from the two stripe phases to the 120∘ phase are of the first order. However, the transition between the two stripe phases is not of the first order, which is different from its classical counterpart. Additionally, we find no evidence for a quantum spin liquid in this model. Our results suggest that additional terms may also be important to model the material YbMgGaO4. These findings will stimulate further experimental and theoretical works in understanding the quantum spin-liquid <span class="hlt">ground</span> <span class="hlt">state</span> in YbMgGaO4.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014APS..MARQ20006M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014APS..MARQ20006M"><span>Charge <span class="hlt">Energy</span> Transport in Hopping Systems with Rapidly Decreasing Density of <span class="hlt">States</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mendels, Dan; Organic Electronics Group Technion Team</p> <p>2014-03-01</p> <p>An accurate description of the carrier hopping topology in the <span class="hlt">energy</span> domain of hopping systems incorporating a rapidly decreasing density of <span class="hlt">states</span> and the subsequent energetic position of these systems' so called effective conduction <span class="hlt">band</span> is crucial for rationalizing and quantifying these systems' thermo-electric properties, doping related phenomena and carrier gradient effects such as the emergence of the General Einstein Relation under degenerate conditions. Additionally, as will be shown, the 'mobile' carriers propagating through the system can have excess <span class="hlt">energies</span> reaching 0.3eV above the system quasi-Fermi <span class="hlt">energy</span>. Hence, since these mobile carriers are most prone to reach systems interfaces and interact with oppositely charged carriers, their excess <span class="hlt">energy</span> should be considered in determining the efficiencies of <span class="hlt">energy</span> dependent processes such as carrier recombination and exciton dissociation. In light of the <span class="hlt">stated</span> motivations, a comprehensive numerical and analytical study of the topology of hopping in the energetic density of such systems (i.e. the statistics regarding which <span class="hlt">energy</span> values carriers visit most and in what manner) was implemented and the main statistical features of the hopping process that determine the position in <span class="hlt">energy</span> of the system's effective conduction <span class="hlt">band</span> were distilled. The obtained results also help shed light on yet to be elucidated discrepancies between predictions given by the widely employed transport <span class="hlt">energy</span> concept and Monte Carlo simulations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19006413','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19006413"><span>Determination of <span class="hlt">ground-state</span> hole-transfer rates between equivalent sites in oxidized multiporphyrin arrays using time-resolved optical spectroscopy.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Song, Hee-eun; Kirmaier, Christine; Taniguchi, Masahiko; Diers, James R; Bocian, David F; Lindsey, Jonathan S; Holten, Dewey</p> <p>2008-11-19</p> <p>Excited-<span class="hlt">state</span> charge separation in molecular architectures has been widely explored, yet <span class="hlt">ground-state</span> hole (or electron) transfer, particularly involving equivalent pigments, has been far less studied, and direct quantitation of the rate of transfer often has proved difficult. Prior studies of <span class="hlt">ground-state</span> hole transfer between equivalent zinc porphyrins using electron paramagnetic resonance techniques give a lower limit of approximately (50 ns)(-1) on the rates. Related transient optical studies of hole transfer between inequivalent sites [zinc porphyrin (Zn) and free base porphyrin (Fb)] give an upper limit of approximately (20 ps)(-1). Thus, a substantial window remains for the unknown rates of <span class="hlt">ground-state</span> hole transfer between equivalent sites. Herein, the <span class="hlt">ground-state</span> hole-transfer processes are probed in a series of oxidized porphyrin triads (ZnZnFb) with the focus being on determination of the rates between the nominally equivalent sites (Zn/Zn). The strategy builds upon recent time-resolved optical studies of the photodynamics of dyads wherein a zinc porphyrin is electrochemically oxidized and the attached free base porphyrin is photoexcited. The resulting <span class="hlt">energy</span>- and hole-transfer processes in the oxidized ZnFb dyads are typically complete within 100 ps of excitation. Such processes are also present in the triads and serve as a starting point for determining the rates of <span class="hlt">ground-state</span> hole transfer between equivalent sites in the triads. The rate constant of the Zn/Zn hole transfer is found to be (0.8 ns)(-1) for diphenylethyne-linked zinc porphyrins and increases only slightly to (0.6 ns)(-1) when a shorter phenylene linker is utilized. The rate decreases slightly to (1.1 ns)(-1) when steric constraints are introduced in the diarylethyne linker. In general, the rate constants for <span class="hlt">ground-state</span> Zn/Zn hole transfer in oxidized arrays are a factor of 40 slower than those for Zn/Fb transfer. Collectively, the findings should aid the design of next</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007JChPh.126m4315C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007JChPh.126m4315C"><span>Ab initio <span class="hlt">ground</span> and excited <span class="hlt">state</span> potential <span class="hlt">energy</span> surfaces for NO-Kr complex and dynamics of Kr solids with NO impurity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Castro-Palacios, Juan Carlos; Rubayo-Soneira, Jesús; Ishii, Keisaku; Yamashita, Koichi</p> <p>2007-04-01</p> <p>The intermolecular potentials for the NO(XΠ2)-Kr and NO(AΣ+2)-Kr systems have been calculated using highly accurate ab initio calculations. The spin-restricted coupled cluster method for the <span class="hlt">ground</span> 1A'2 <span class="hlt">state</span> [NO(XΠ2)-Kr ] and the multireference singles and doubles configuration interaction method for the excited 2A'2 <span class="hlt">state</span> [NO(AΣ+2)-Kr], respectively, were used. The potential <span class="hlt">energy</span> surfaces (PESs) show two linear wells and one that is almost in the perpendicular position. An analytical representation of the PESs has been constructed for the triatomic systems and used to carry out molecular dynamics (MD) simulations of the NO-doped krypton matrix response after excitation of NO. MD results are shown comparatively for three sets of potentials: (1) anisotropic ab initio potentials [NO molecule direction fixed during the dynamics and considered as a point (its center of mass)], (2) isotropic ab initio potentials (isotropic part in a Legendre polynomial expansion of the PESs), and (3) fitted Kr-NO potentials to the spectroscopic data. An important finding of this work is that the anisotropic and isotropic ab initio potentials calculated for the Kr-NO triatomic system are not suitable for describing the dynamics of structural relaxation upon Rydberg excitation of a NO impurity in the crystal. However, the isotropic ab initio potential in the <span class="hlt">ground</span> <span class="hlt">state</span> almost overlaps the published experimental potential, being almost independent of the angle asymmetry. This fact is also manifested in the radial distribution function around NO. However, in the case of the excited <span class="hlt">state</span> the isotropic ab initio potential differs from the fitted potentials, which indicates that the Kr-NO interaction in the matrix is quite different because of the presence of the surrounding Kr atoms acting on the NO molecule. MD simulations for isotropic potentials reasonably reproduce the experimental observables for the femtosecond response and the bubble size but do not match spectroscopic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..MAR.G1071Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..MAR.G1071Y"><span>Theoretical study on electronic structure of bathocuproine: Renormalization of the <span class="hlt">band</span> gap in the crystalline <span class="hlt">state</span> and the large exciton binding <span class="hlt">energy</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yanagisawa, Susumu; Hatada, Shin-No-Suke; Morikawa, Yoshitada</p> <p></p> <p>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 <span class="hlt">states</span> 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 <span class="hlt">band</span> gap of the BCP single crystal is 4.39 eV, and it is in agreement with the recent low-<span class="hlt">energy</span> inverse photoemission spectroscopy measurement. The polarization <span class="hlt">energy</span> 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 <span class="hlt">energy</span> is 3.68 eV, and the exciton binding <span class="hlt">energy</span> 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.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.S53G..08I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.S53G..08I"><span>Synthesis of High-Frequency <span class="hlt">Ground</span> Motion Using Information Extracted from Low-Frequency <span class="hlt">Ground</span> Motion</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Iwaki, A.; Fujiwara, H.</p> <p>2012-12-01</p> <p>Broadband <span class="hlt">ground</span> motion computations of scenario earthquakes are often based on hybrid methods that are the combinations of deterministic approach in lower frequency <span class="hlt">band</span> and stochastic approach in higher frequency <span class="hlt">band</span>. Typical computation methods for low-frequency and high-frequency (LF and HF, respectively) <span class="hlt">ground</span> motions are the numerical simulations, such as finite-difference and finite-element methods based on three-dimensional velocity structure model, and the stochastic Green's function method, respectively. In such hybrid methods, LF and HF wave fields are generated through two different methods that are completely independent of each other, and are combined at the matching frequency. However, LF and HF wave fields are essentially not independent as long as they are from the same event. In this study, we focus on the relation among acceleration envelopes at different frequency <span class="hlt">bands</span>, and attempt to synthesize HF <span class="hlt">ground</span> motion using the information extracted from LF <span class="hlt">ground</span> motion, aiming to propose a new method for broad-<span class="hlt">band</span> strong motion prediction. Our study area is Kanto area, Japan. We use the K-NET and KiK-net surface acceleration data and compute RMS envelope at four frequency <span class="hlt">bands</span>: 0.5-1.0 Hz, 1.0-2.0 Hz, 2.0-4.0 Hz, .0-8.0 Hz, and 8.0-16.0 Hz. Taking the ratio of the envelopes of adjacent <span class="hlt">bands</span>, we find that the envelope ratios have stable shapes at each site. The empirical envelope-ratio characteristics are combined with low-frequency envelope of the target earthquake to synthesize HF <span class="hlt">ground</span> motion. We have applied the method to M5-class earthquakes and a M7 target earthquake that occurred in the vicinity of Kanto area, and successfully reproduced the observed HF <span class="hlt">ground</span> motion of the target earthquake. The method can be applied to a broad <span class="hlt">band</span> <span class="hlt">ground</span> motion simulation for a scenario earthquake by combining numerically-computed low-frequency (~1 Hz) <span class="hlt">ground</span> motion with the empirical envelope ratio characteristics to generate broadband <span class="hlt">ground</span> motion</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29393900','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29393900"><span>Accurate <span class="hlt">Energy</span> Consumption Modeling of IEEE 802.15.4e TSCH Using Dual-<span class="hlt">Band</span>OpenMote Hardware.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Daneels, Glenn; Municio, Esteban; Van de Velde, Bruno; Ergeerts, Glenn; Weyn, Maarten; Latré, Steven; Famaey, Jeroen</p> <p>2018-02-02</p> <p>The Time-Slotted Channel Hopping (TSCH) mode of the IEEE 802.15.4e amendment aims to improve reliability and <span class="hlt">energy</span> efficiency in industrial and other challenging Internet-of-Things (IoT) environments. This paper presents an accurate and up-to-date <span class="hlt">energy</span> consumption model for devices using this IEEE 802.15.4e TSCH mode. The model identifies all network-related CPU and radio <span class="hlt">state</span> changes, thus providing a precise representation of the device behavior and an accurate prediction of its <span class="hlt">energy</span> consumption. Moreover, <span class="hlt">energy</span> measurements were performed with a dual-<span class="hlt">band</span> OpenMote device, running the OpenWSN firmware. This allows the model to be used for devices using 2.4 GHz, as well as 868 MHz. Using these measurements, several network simulations were conducted to observe the TSCH <span class="hlt">energy</span> consumption effects in end-to-end communication for both frequency <span class="hlt">bands</span>. Experimental verification of the model shows that it accurately models the consumption for all possible packet sizes and that the calculated consumption on average differs less than 3% from the measured consumption. This deviation includes measurement inaccuracies and the variations of the guard time. As such, the proposed model is very suitable for accurate <span class="hlt">energy</span> consumption modeling of TSCH networks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5855993','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5855993"><span>Accurate <span class="hlt">Energy</span> Consumption Modeling of IEEE 802.15.4e TSCH Using Dual-<span class="hlt">Band</span>OpenMote Hardware</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Municio, Esteban; Van de Velde, Bruno; Latré, Steven</p> <p>2018-01-01</p> <p>The Time-Slotted Channel Hopping (TSCH) mode of the IEEE 802.15.4e amendment aims to improve reliability and <span class="hlt">energy</span> efficiency in industrial and other challenging Internet-of-Things (IoT) environments. This paper presents an accurate and up-to-date <span class="hlt">energy</span> consumption model for devices using this IEEE 802.15.4e TSCH mode. The model identifies all network-related CPU and radio <span class="hlt">state</span> changes, thus providing a precise representation of the device behavior and an accurate prediction of its <span class="hlt">energy</span> consumption. Moreover, <span class="hlt">energy</span> measurements were performed with a dual-<span class="hlt">band</span> OpenMote device, running the OpenWSN firmware. This allows the model to be used for devices using 2.4 GHz, as well as 868 MHz. Using these measurements, several network simulations were conducted to observe the TSCH <span class="hlt">energy</span> consumption effects in end-to-end communication for both frequency <span class="hlt">bands</span>. Experimental verification of the model shows that it accurately models the consumption for all possible packet sizes and that the calculated consumption on average differs less than 3% from the measured consumption. This deviation includes measurement inaccuracies and the variations of the guard time. As such, the proposed model is very suitable for accurate <span class="hlt">energy</span> consumption modeling of TSCH networks. PMID:29393900</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990111473&hterms=DURAND&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAuthor-Name%26N%3D0%26No%3D50%26Ntt%3DDURAND','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990111473&hterms=DURAND&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAuthor-Name%26N%3D0%26No%3D50%26Ntt%3DDURAND"><span>ACTS Ka-<span class="hlt">band</span> Propagation Research in a Spatially Diversified Network with Two USAT <span class="hlt">Ground</span> Stations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kalu, Alex; Acousta, R.; Durand, S.; Emrich, Carol; Ventre, G.; Wilson, W.</p> <p>1999-01-01</p> <p>Congestion in the radio spectrum below 18 GHz is stimulating greater interest in the Ka (20/30 GHz) frequency <span class="hlt">band</span>. Transmission at these shorter wavelengths is greatly influenced by rain resulting in signal attenuation and decreased link availability. The size and projected cost of Ultra Small Aperture Terminals (USATS) make site diversity methodology attractive for rain fade compensation. Separation distances between terminals must be small to be of interest commercially. This study measures diversity gain at a separation distance <5 km and investigates utilization of S-<span class="hlt">band</span> weather radar reflectivity in predicting diversity gain. Two USAT <span class="hlt">ground</span> stations, separated by 2.43 km for spatial diversity, received a continuous Ka-<span class="hlt">band</span> tone sent from NASA Glenn Research Center via the Advanced Communications Technology Satellite (ACTS) steerable antenna beam. Received signal power and rainfall were measured, and Weather Surveillance Radar-1998 Doppler (WSR-88D) data were obtained as a measure of precipitation along the USAT-to-ACTS slant path. Signal attenuation was compared for the two sites, and diversity gain was calculated for fades measured on eleven days. Correlation of WSR-88D S-<span class="hlt">band</span> reflectivity with measured Ka-<span class="hlt">band</span> attenuation consisted of locating radar volume elements along each slant path, converting reflectivity to Ka-<span class="hlt">band</span> attenuation with rain rate calculation as an intermediate step. Specific attenuation for each associated path segment was summed, resulting in total attenuation along the slant path. Derived Ka-<span class="hlt">band</span> attenuation did not correlate closely with empirical data (r = 0.239), but a measured signal fade could be matched with an increase in radar reflectivity in all fade events. Applying a low pass filter to radar reflectivity prior to deriving Ka-<span class="hlt">band</span> attenuation improved the correlation between measured and derived signal attenuation (r = 0.733). Results indicate that site diversity at small separation distances is a viable means of rain fade</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://ntrs.nasa.gov/search.jsp?R=19920073738&hterms=ICT&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DWhat%2BICT','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19920073738&hterms=ICT&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DWhat%2BICT"><span>The low-<span class="hlt">energy</span>, charge-transfer excited <span class="hlt">states</span> of 4-amino-4-prime-nitrodiphenyl sulfide</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>O'Connor, Donald B.; Scott, Gary W.; Tran, Kim; Coulter, Daniel R.; Miskowski, Vincent M.; Stiegman, Albert E.; Wnek, Gary E.</p> <p>1992-01-01</p> <p>Absorption and emission spectra of 4-amino-4-prime-nitrodiphenyl sulfide in polar and nonpolar solvents were used to characterize and assign the low-<span class="hlt">energy</span> excited <span class="hlt">states</span> of the molecule. Fluorescence-excitation anisotropy spectra and fluorescence quantum yields were also used to characterize the photophysics of these <span class="hlt">states</span>. The lowest-<span class="hlt">energy</span> fluorescent singlet <span class="hlt">state</span> was determined to be an intramolecular charge transfer (ICT) <span class="hlt">state</span> involving transfer of a full electron charge from the amino to the nitro group yielding a dipole moment of about 50 D. A low-<span class="hlt">energy</span>, intense absorption <span class="hlt">band</span> is assigned as a transition to a different ICT <span class="hlt">state</span> involving a partial electron charge transfer from sulfur to the nitro group.</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 electronic-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/1341642-magnetostriction-driven-ground-state-stabilization-perovskites','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1341642-magnetostriction-driven-ground-state-stabilization-perovskites"><span>Magnetostriction-driven <span class="hlt">ground-state</span> stabilization in 2H perovskites</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Porter, D. G.; Senn, M. S.; Khalyavin, D. D.; ...</p> <p>2016-10-04</p> <p>In this paper, the magnetic <span class="hlt">ground</span> <span class="hlt">state</span> of Sr 3ARuO 6, with A =(Li,Na), is studied using neutron diffraction, resonant x-ray scattering, and laboratory characterization measurements of high-quality crystals. Combining these results allows us to observe the onset of long-range magnetic order and distinguish the symmetrically allowed magnetic models, identifying in-plane antiferromagnetic moments and a small ferromagnetic component along the c axis. While the existence of magnetic domains masks the particular in-plane direction of the moments, it has been possible to elucidate the <span class="hlt">ground</span> <span class="hlt">state</span> using symmetry considerations. We find that due to the lack of local anisotropy, antisymmetric exchangemore » interactions control the magnetic order, first through structural distortions that couple to in-plane antiferromagnetic moments and second through a high-order magnetoelastic coupling that lifts the degeneracy of the in-plane moments. Finally, the symmetry considerations used to rationalize the magnetic <span class="hlt">ground</span> <span class="hlt">state</span> are very general and will apply to many systems in this family, such as Ca 3ARuO 6, with A = (Li,Na), and Ca 3LiOsO 6 whose magnetic <span class="hlt">ground</span> <span class="hlt">states</span> are still not completely understood.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JMoSp.297....4R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JMoSp.297....4R"><span>First analysis of the 2ν1 + 3ν3 <span class="hlt">band</span> of NO2 at 7192.159 cm-1</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Raghunandan, R.; Perrin, A.; Ruth, A. A.; Orphal, J.</p> <p>2014-03-01</p> <p>The first investigation of the very weak 2ν1 + 3ν3 absorption <span class="hlt">band</span> of nitrogen dioxide, 14N16O2, located at 7192.1587(1) cm-1 was performed using Fourier-transform incoherent broadband cavity-enhanced absorption spectroscopy (FT-IBBCEAS) in the 7080-7210 cm-1 spectral range. The assigned 2ν1 + 3ν3 lines involve <span class="hlt">energy</span> levels of the (2 0 3) vibrational <span class="hlt">state</span> with rotational quantum numbers up to Ka = 7 and N = 47. Furthermore, due to local resonances involving <span class="hlt">energy</span> levels from the (2,2,2)⇔(2,0,3) and (5,1,0)⇔(2,0,3) <span class="hlt">states</span>, several transitions were also observed for the 2ν1 + 2ν2 + 2ν3 and 5ν1 + ν3 dark <span class="hlt">bands</span>, respectively. The <span class="hlt">energy</span> levels were satisfactorily reproduced within their experimental uncertainty using a theoretical model which takes explicitly into account the Coriolis interactions between the levels of the (2, 0, 3) vibrational <span class="hlt">state</span> and those of (2, 2, 2) and of (5, 1, 0). As a consequence, precise vibrational <span class="hlt">energies</span>, rotational, and coupling constants were achieved for the triad {(5, 0, 1), (2, 2, 2), (2, 0, 3)} of interacting <span class="hlt">states</span> of 14N16O2. This theoretical model also accounts for the electron spin-rotation resonances within the (2, 0, 3), (2, 2, 2) and (5, 1, 0) vibrational <span class="hlt">states</span>. However, owing to the limited experimental resolution (˜0.075 cm-1), it was not possible to observe the spin-rotation doublet structure. As a consequence, the spin-rotation constants in the {(2, 2, 2), (2, 0, 3), (5, 1, 0)} excited <span class="hlt">states</span> were maintained fixed to their <span class="hlt">ground</span> <span class="hlt">state</span> values in this study. Using these parameters a comprehensive list of line positions and line intensities was generated for the 2ν1 + 3ν3 <span class="hlt">band</span> of NO2.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016isms.confEWF12G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016isms.confEWF12G"><span>Progress in the Rotational Analysis of the <span class="hlt">Ground</span> and Low-Lying Vibrationally Excited <span class="hlt">States</span> of Malonaldehyde</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Goudreau, E. S.; Tokaryk, Dennis W.; Ross, Stephen Cary; Billinghurst, Brant E.</p> <p>2016-06-01</p> <p>Despite being an important prototype molecule for intramolecular proton tunnelling, the far-IR spectrum of the internally hydrogen-bonded species malonaldehyde (C_3O_2H_4) is not yet well understood. In the talk I gave at the ISMS meeting in 2015 I discussed the high-resolution spectra we obtained at the Canadian Light Source synchrotron in Saskatoon, Saskatchewan. These spectra include a number of fundamental vibrational <span class="hlt">bands</span> in the 100-2000 cm-1 region. In our efforts to analyze these <span class="hlt">bands</span> we have noticed that our <span class="hlt">ground</span> <span class="hlt">state</span> combination differences show a large drift (up to an order of magnitude larger than our experimental error) away from those calculated using constants established by Baba et al., particularly in regions of high J (above 30) and low Ka (below 5). An examination of the previous microwave and far-IR studies reveals that this region of J-Ka space was not represented in the lines that Baba et al. used to generate the values for their fitting parameters. By including our own measurements in the fitting, we were able to improve the characterization of the <span class="hlt">ground</span> <span class="hlt">state</span> so that it is now consistent with all of the existing data. This characterization now covers a much larger range of J-Ka space and has enabled us to make significant progress in analyzing our far-IR synchrotron spectra. These include an excited vibrational <span class="hlt">state</span> at 241 cm-1 as well as several <span class="hlt">states</span> split by the tunnelling effect at higher wavenumber. T. Baba, T. Tanaka, I. Morino, K. M. T. Yamada, K. Tanaka. Detection of the tunneling-rotation transitions of malonaldehyde in the submillimeter-wave region. J. Chem. Phys., 110. 4131-4133 (1999) P. Turner, S. L. Baughcum, S. L. Coy, Z. Smith. Microwave Spectroscopic Study of Malonaldehyde. 4. Vibration-Rotation Interaction in Parent Species. J. Am. Chem. Soc., 106. 2265-2267 (1984) D. W. Firth, K. Beyer, M. A. Dvorak, S. W. Reeve, A. Grushow, K. R. Leopold. Tunable far-infrared spectroscopy of malonaldehyde. J. Chem. Phys., 94. 1812</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..DMP.D1140Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..DMP.D1140Y"><span>Coherent Control of <span class="hlt">Ground</span> <span class="hlt">State</span> NaK Molecules</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yan, Zoe; Park, Jee Woo; Loh, Huanqian; Will, Sebastian; Zwierlein, Martin</p> <p>2016-05-01</p> <p>Ultracold dipolar molecules exhibit anisotropic, tunable, long-range interactions, making them attractive for the study of novel <span class="hlt">states</span> of matter and quantum information processing. We demonstrate the creation and control of 23 Na40 K molecules in their rovibronic and hyperfine <span class="hlt">ground</span> <span class="hlt">state</span>. By applying microwaves, we drive coherent Rabi oscillations of spin-polarized molecules between the rotational <span class="hlt">ground</span> <span class="hlt">state</span> (J=0) and J=1. The control afforded by microwave manipulation allows us to pursue engineered dipolar interactions via microwave dressing. By driving a two-photon transition, we are also able to observe Ramsey fringes between different J=0 hyperfine <span class="hlt">states</span>, with coherence times as long as 0.5s. The realization of long coherence times between different molecular <span class="hlt">states</span> is crucial for applications in quantum information processing. NSF, AFOSR- MURI, Alfred P. Sloan Foundation, DARPA-OLE</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ARCMP...9..105H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ARCMP...9..105H"><span>Experimental Insights into <span class="hlt">Ground-State</span> Selection of Quantum XY Pyrochlores</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hallas, Alannah M.; Gaudet, Jonathan; Gaulin, Bruce D.</p> <p>2018-03-01</p> <p>Extensive experimental investigations of the magnetic structures and excitations in the XY pyrochlores have been carried out over the past decade. Three families of XY pyrochlores have emerged: Yb2B2O7, Er2B2O7, and, most recently, [Formula: see text]Co2F7. In each case, the magnetic cation (either Yb, Er, or Co) exhibits XY anisotropy within the local pyrochlore coordinates, a consequence of crystal field effects. Materials in these families display rich phase behavior and are candidates for exotic <span class="hlt">ground</span> <span class="hlt">states</span>, such as quantum spin ice, and exotic <span class="hlt">ground-state</span> selection via order-by-disorder mechanisms. In this review, we present an experimental summary of the <span class="hlt">ground-state</span> properties of the XY pyrochlores, including evidence that they are strongly influenced by phase competition. We empirically demonstrate the signatures for phase competition in a frustrated magnet: multiple heat capacity anomalies, suppressed TN or TC, sample- and pressure-dependent <span class="hlt">ground</span> <span class="hlt">states</span>, and unconventional spin dynamics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29938269','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29938269"><span>A first-principles study of the electrically tunable <span class="hlt">band</span> gap in few-layer penta-graphene.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Jinjin; Wang, Zhanyu; Zhang, R J; Zheng, Y X; Chen, L Y; Wang, S Y; Tsoo, Chia-Chin; Huang, Hung-Ji; Su, Wan-Sheng</p> <p>2018-06-25</p> <p>The structural and electronic properties of bilayer (AA- and AB-stacked) and tri-layer (AAA-, ABA- and AAB-stacked) penta-graphene (PG) have been investigated in the framework of density functional theory. The present results demonstrate that the <span class="hlt">ground</span> <span class="hlt">state</span> <span class="hlt">energy</span> in AB stacking is lower than that in AA stacking, whereas ABA stacking is found to be the most energetically favorable, followed by AAB and AAA stackings. All considered model configurations are found to be semiconducting, independent of the stacking sequence. In the presence of a perpendicular electric field, their <span class="hlt">band</span> gaps can be significantly reduced and completely closed at a specific critical electric field strength, demonstrating a Stark effect. These findings show that few-layer PG will have tremendous opportunities to be applied in nanoscale electronic and optoelectronic devices owing to its tunable <span class="hlt">band</span> gap.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5290264','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5290264"><span>Charge transfer to <span class="hlt">ground-state</span> ions produces free electrons</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>You, D.; Fukuzawa, H.; Sakakibara, Y.; Takanashi, T.; Ito, Y.; Maliyar, G. G.; Motomura, K.; Nagaya, K.; Nishiyama, T.; Asa, K.; Sato, Y.; Saito, N.; Oura, M.; Schöffler, M.; Kastirke, G.; Hergenhahn, U.; Stumpf, V.; Gokhberg, K.; Kuleff, A. I.; Cederbaum, L. S.; Ueda, K</p> <p>2017-01-01</p> <p>Inner-shell ionization of an isolated atom typically leads to Auger decay. In an environment, for example, a liquid or a van der Waals bonded system, this process will be modified, and becomes part of a complex cascade of relaxation steps. Understanding these steps is important, as they determine the production of slow electrons and singly charged radicals, the most abundant products in radiation chemistry. In this communication, we present experimental evidence for a so-far unobserved, but potentially very important step in such relaxation cascades: Multiply charged ionic <span class="hlt">states</span> after Auger decay may partially be neutralized by electron transfer, simultaneously evoking the creation of a low-<span class="hlt">energy</span> free electron (electron transfer-mediated decay). This process is effective even after Auger decay into the dicationic <span class="hlt">ground</span> <span class="hlt">state</span>. In our experiment, we observe the decay of Ne2+ produced after Ne 1s photoionization in Ne–Kr mixed clusters. PMID:28134238</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('https://www.ncbi.nlm.nih.gov/pubmed/15379532','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15379532"><span>Relocation of the disulfonic stilbene sites of AE1 (<span class="hlt">band</span> 3) on the basis of fluorescence <span class="hlt">energy</span> transfer measurements.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Knauf, Philip A; Law, Foon-Yee; Leung, Tze-Wah Vivian; Atherton, Stephen J</p> <p>2004-09-28</p> <p>Previous fluorescence resonance <span class="hlt">energy</span> transfer (FRET) measurements, using BIDS (4-benzamido-4'-isothiocyanostilbene-2,2'-disulfonate) as a label for the disulfonic stilbene site and FM (fluorescein-5-maleimide) as a label for the cytoplasmic SH groups on <span class="hlt">band</span> 3 (AE1), combined with data showing that the cytoplasmic SH groups lie about 40 A from the cytoplasmic surface of the lipid bilayer, would place the BIDS sites very near the membrane's inner surface, a location that seems to be inconsistent with current models of AE1 structure and mechanism. We reinvestigated the BIDS-FM distance, using laser single photon counting techniques as well as steady-<span class="hlt">state</span> fluorescence of AE1, in its native membrane environment. Both techniques agree that there is very little <span class="hlt">energy</span> transfer from BIDS to FM. The mean <span class="hlt">energy</span> transfer (E), based on three-exponential fits to the fluorescence decay data, is 2.5 +/- 0.7% (SEM, N = 12). Steady-<span class="hlt">state</span> fluorescence measurements also indicate <3% <span class="hlt">energy</span> transfer from BIDS to FM. These data indicate that the BIDS sites are probably over 63 A from the cytoplasmic SH groups, placing them near the middle or the external half of the lipid bilayer. This relocation of the BIDS sites fits with other evidence that the disulfonic stilbene sites are located farther toward the external membrane surface than Glu-681, a residue near the inner membrane surface whose modification affects the pH dependence and anion selectivity of <span class="hlt">band</span> 3. The involvement of two relatively distant parts of the AE1 protein in transport function suggests that the transport mechanism requires coordinated large-scale conformational changes in the <span class="hlt">band</span> 3 protein.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009ITEIS.129.1642U','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009ITEIS.129.1642U"><span>FDTD Calculation of FM-<span class="hlt">Band</span> Crosstalks between Perpendicular Traces on Printed Circuit Board with <span class="hlt">Ground</span>-Pattern Slits</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ueyama, Hiroya; Maeno, Tsuyoshi; Hirata, Akimasa; Wang, Jianqing; Fujiwara, Osamu</p> <p></p> <p>Electromagnetic disturbances for vehicle-mounted radios are well known to be caused mainly by conduction noise currents flowing out wire harnesses from printed circuit boards (PCBs) having a common <span class="hlt">ground</span> layer with slits. In this study, in order to investigate how <span class="hlt">ground</span>-layer slits affect the above conduction noise currents, we paid FM <span class="hlt">band</span> induced voltages or crosstalks on the trace connected to the wire harnesss, and simulated with the FDTD method the crosstalk levels between two traces perpendicularly fabricated on three kinds of simple PCBs with different <span class="hlt">ground</span>-layer slits, which were compared with measurement in the frequency range from 10 MHz to 1 GHz. As a result, we could confirm that the FDTD calculation approximately agrees with the measured results, and also that the crosstalk levels do not always increase with the slit number, which can be reduced by the slit layout.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhRvB..95k5135M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvB..95k5135M"><span>Compact localized <span class="hlt">states</span> and flat-<span class="hlt">band</span> generators in one dimension</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Maimaiti, Wulayimu; Andreanov, Alexei; Park, Hee Chul; Gendelman, Oleg; Flach, Sergej</p> <p>2017-03-01</p> <p>Flat <span class="hlt">bands</span> (FB) are strictly dispersionless <span class="hlt">bands</span> in the Bloch spectrum of a periodic lattice Hamiltonian, recently observed in a variety of photonic and dissipative condensate networks. FB Hamiltonians are fine-tuned networks, still lacking a comprehensive generating principle. We introduce a FB generator based on local network properties. We classify FB networks through the properties of compact localized <span class="hlt">states</span> (CLS) which are exact FB eigenstates and occupy U unit cells. We obtain the complete two-parameter FB family of two-<span class="hlt">band</span> d =1 networks with nearest unit cell interaction and U =2 . We discover a novel high symmetry sawtooth chain with identical hoppings in a transverse dc field, easily accessible in experiments. Our results pave the way towards a complete description of FBs in networks with more <span class="hlt">bands</span> and in higher dimensions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017isms.confETB05L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017isms.confETB05L"><span>Hot <span class="hlt">Band</span> Analysis and Kinetics Measurements for Ethynyl Radical, C_2H, in the 1.49 μm Region</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Le, Anh T.; Hall, Gregory; Sears, Trevor</p> <p>2017-06-01</p> <p>Ethynyl, C_2H, is an important intermediate in combustion processes and has been widely observed in interstellar space. Spectroscopically, it is of particular interest because it possesses three low-lying electronic surfaces: a <span class="hlt">ground</span> ^2Σ^+<span class="hlt">state</span>, and a low-lying ^2Π excited electronic <span class="hlt">state</span>, which splits due to the Renner-Teller effect. Vibronic coupling among these <span class="hlt">states</span> leads to a complicated, mixed-character, <span class="hlt">energy</span> level structure. We have previously reported work on three <span class="hlt">bands</span> originating from the ˜{X}(0,0,0) ^2Σ <span class="hlt">ground</span> <span class="hlt">state</span> to excited vibronic <span class="hlt">states</span>: two ^2Σ - ^2 Σ transitions at 6696 and 7088 \\wn and a ^2Π - ^2Σ transition at 7108 \\wn. In this work, the radicals were formed in a hot, non-thermal, population distribution by u.v. pulsed laser photolysis of a precursor. Kinetic measurements of the time-evolution of the <span class="hlt">ground</span> <span class="hlt">state</span> populations following collisional relaxation and reactive loss were also made, using some of the stronger rotational lines observed. Time-dependent signals in mixtures containing a variable concentration of precursor in argon suggested that vibronically hot C_2H radicals were less reactive than the relaxed, thermalized, radical. Two additional hot <span class="hlt">bands</span> originating in <span class="hlt">states</span> ˜{X}(0,1^1,0) ^2Π and ˜{X}(0,2^0,0) ^2Σ, have now been identified in the same spectral region. In a new series of experiments, we have measured the kinetics of formation and decay of representative levels involving all the assigned transitions, i.e. originating in ˜{X}(0,v_2,0), with v_2 =0 ,1, and 2, in various concentrations of mixtures of precursor, inert gas and hydrogen. The new spectra also show greatly improved signal-to-noise ratio in comparison to our previous work, due to the use of a transient FM detection scheme, and additional spectral assignments seem likely. Both kinetics and spectroscopic results will be described in the talk. Acknowledgments: Work at Brookhaven National Laboratory was carried out under Contract No. DE-SC0012704</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1994JChPh.101.7255S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1994JChPh.101.7255S"><span>An analysis of the à 2Π-X˜ 2Σ+ <span class="hlt">band</span> system of isotopically substituted calcium isocyanide CaNC</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Scurlock, C. T.; Fletcher, D. A.; Steimle, T. C.</p> <p>1994-11-01</p> <p>The strong visible <span class="hlt">band</span> systems of a supersonic molecular beam sample of isotopically substituted CaNC (13C and 15N individually) have been recorded at high resolution by laser-induced fluorescence spectroscopy. The spectra have the general appearance of the expected à 2Π-X˜ 2Σ+ <span class="hlt">band</span> systems, but the <span class="hlt">energy</span> levels of both the ‖Ω‖=1/2 and 3/2 excited substates have localized perturbations. Spectroscopic parameters for the X˜ 2Σ+ <span class="hlt">state</span> of the isotopomers were extracted from a least-squares fit to the appropriate combinations differences of the observed transitions frequencies. Excited <span class="hlt">state</span> effective parameters were extracted by directly fitting the unperturbed portions of the optical spectra. The rs-structure bond lengths for the <span class="hlt">ground</span> electronic <span class="hlt">state</span> were determined to be Ca-N=2.2065(58) Å and N-C=1.1186(58) Å. The permanent electric dipole moments for the Ca15NC isotopomer were determined to be 5.93(8) and 6.69(9) D for the à 2Π and X˜ 2Σ+ <span class="hlt">states</span>, respectively.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/21254327-ground-states-baryoleptonic-balls-supersymmetric-models','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/21254327-ground-states-baryoleptonic-balls-supersymmetric-models"><span><span class="hlt">Ground</span> <span class="hlt">states</span> of baryoleptonic Q-balls in supersymmetric models</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>Shoemaker, Ian M.; Kusenko, Alexander</p> <p>2008-10-01</p> <p>In supersymmetric generalizations of the standard model, all stable Q-balls are associated with some flat directions. We show that, if the flat direction has both the baryon number and the lepton number, the scalar field inside the Q-ball can deviate slightly from the flat direction in the <span class="hlt">ground</span> <span class="hlt">state</span>. We identify the true <span class="hlt">ground</span> <span class="hlt">states</span> of such nontopological solitons, including the electrically neutral and electrically charged Q-balls.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18518481','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18518481"><span>Theory of <span class="hlt">ground</span> <span class="hlt">state</span> factorization in quantum cooperative systems.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Giampaolo, Salvatore M; Adesso, Gerardo; Illuminati, Fabrizio</p> <p>2008-05-16</p> <p>We introduce a general analytic approach to the study of factorization points and factorized <span class="hlt">ground</span> <span class="hlt">states</span> in quantum cooperative systems. The method allows us to determine rigorously the existence, location, and exact form of separable <span class="hlt">ground</span> <span class="hlt">states</span> in a large variety of, generally nonexactly solvable, spin models belonging to different universality classes. The theory applies to translationally invariant systems, irrespective of spatial dimensionality, and for spin-spin interactions of arbitrary range.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3549080','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3549080"><span>Regulating <span class="hlt">energy</span> transfer of excited carriers and the case for excitation-induced hydrogen dissociation on hydrogenated 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>Bang, Junhyeok; Meng, Sheng; Sun, Yi-Yang; West, Damien; Wang, Zhiguo; Gao, Fei; Zhang, S. B.</p> <p>2013-01-01</p> <p>Understanding and controlling of excited carrier dynamics is of fundamental and practical importance, particularly in photochemistry and solar <span class="hlt">energy</span> applications. However, theory of <span class="hlt">energy</span> relaxation of excited carriers is still in its early stage. Here, using ab initio molecular dynamics (MD) coupled with time-dependent density functional theory, we show a coverage-dependent <span class="hlt">energy</span> transfer of photoexcited carriers in hydrogenated graphene, giving rise to distinctively different ion dynamics. Graphene with sparsely populated H is difficult to dissociate due to inefficient transfer of the excitation <span class="hlt">energy</span> into kinetic <span class="hlt">energy</span> of the H. In contrast, H can easily desorb from fully hydrogenated graphane. The key is to bring down the H antibonding <span class="hlt">state</span> to the conduction <span class="hlt">band</span> minimum as the <span class="hlt">band</span> gap increases. These results can be contrasted to those of standard <span class="hlt">ground-state</span> MD that predict H in the sparse case should be much less stable than that in fully hydrogenated graphane. Our findings thus signify the importance of carrying out explicit electronic dynamics in excited-<span class="hlt">state</span> simulations. PMID:23277576</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..SHK.E8001Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..SHK.E8001Y"><span>Temperature dependent of IVR investigated by steady-<span class="hlt">state</span> and time-frequency resolved CARS for liquid nitrobenzene and nitromethane</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, Yanqiang; Zhu, Gangbei; Yan, Lin; Liu, Xiaosong; Yang's Ultrafast Spectroscopy Group Team</p> <p>2017-06-01</p> <p>Intramolecular vibrational <span class="hlt">energy</span> redistribution (IVR) is important process in thermal decomposition, shock chemistry and photochemistry. Anti-Stokes Raman scattering is sensitive to the vibrational population in excited <span class="hlt">states</span> because only vibrational excited <span class="hlt">states</span> are responsible to the anti-Stokes Raman scattering, does not vibrational <span class="hlt">ground</span> <span class="hlt">states</span>. In this report, steady-<span class="hlt">state</span> anti-Stokes Raman spectroscopy and broad <span class="hlt">band</span> ultrafast coherent anti-Stokes Raman scattering (CARS) are performed. The steady-<span class="hlt">state</span> anti-Stokes Raman spectroscopy shows temperature dependent of vibrational <span class="hlt">energy</span> redistribution in vibrational excited-<span class="hlt">state</span> molecule, and reveal that, in liquid nitrobenzene, with temperature increasing, vibrational <span class="hlt">energy</span> is mainly redistributed in NO2 symmetric stretching mode, and phenyl ring stretching mode of νCC. For liquid nitromethane, it is found that, with temperature increasing, vibrational <span class="hlt">energy</span> concentrate in CN stretching mode and methyl umbrella vibrational mode. In the broad <span class="hlt">band</span> ultrafast CARS experiment, multiple vibrational modes are coherently excited to vibrational excited <span class="hlt">states</span>, and the time-frequency resolved CARS spectra show the coincident IVR processes. This work is supported by the National Natural Science Foundation of China (Grant Numbers 21673211 and 11372053), and the Science Challenging Program (Grant Number JCKY2016212A501).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013JPhCS.428a2004W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013JPhCS.428a2004W"><span>Vibronic <span class="hlt">bands</span> in the HOMO-LUMO excitation of linear polyyne molecules</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wakabayashi, Tomonari; Wada, Yoriko; Iwahara, Naoya; Sato, Tohru</p> <p>2013-04-01</p> <p>Hydrogen-capped linear carbon chain molecules, namely polyynes H(C≡C)nH (n>=2), give rise to three excited <span class="hlt">states</span> in the HOMO-LUMO excitation. Electric dipole transition from the <span class="hlt">ground</span> <span class="hlt">state</span> is fully allowed to one of the three excited <span class="hlt">states</span>, while forbidden for the other two low-lying excited <span class="hlt">states</span>. In addition to the strong absorption <span class="hlt">bands</span> in the UV for the allowed transition, the molecules exhibit weak absorption and emission <span class="hlt">bands</span> in the near UV and visible wavelength regions. The weak features are the vibronic <span class="hlt">bands</span> in the forbidden transition. In this article, symmetry considerations are presented for the optical transitions in the centrosymmetric linear polyyne molecule. The argument includes Herzberg-Teller expansion for the <span class="hlt">state</span> mixing induced by nuclear displacements along the normal coordinate of the molecule, intensity borrowing from fully allowed transitions, and inducing vibrational modes excited in the vibronic transition. The vibronic coupling considered here includes off-diagonal matrix elements for second derivatives along the normal coordinate. The vibronic selection rule for the forbidden transition is derived and associated with the transition moment with respect to the molecular axis. Experimental approaches are proposed for the assignment of the observed vibronic <span class="hlt">bands</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_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/2018JPSJ...87d4701S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JPSJ...87d4701S"><span>Valence-<span class="hlt">Band</span> Electronic 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> electronic 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 <span class="hlt">states</span> (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 electronic structure. Spin-dependent calculations predict a ferromagnetic <span class="hlt">ground</span> <span class="hlt">state</span> 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/2017PhRvB..96q4410A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvB..96q4410A"><span>Evidence of tetragonal distortion as the origin of the ferromagnetic <span class="hlt">ground</span> <span class="hlt">state</span> in γ -Fe nanoparticles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Augustyns, V.; van Stiphout, K.; Joly, V.; Lima, T. A. L.; Lippertz, G.; Trekels, M.; Menéndez, E.; Kremer, F.; Wahl, U.; Costa, A. R. G.; Correia, J. G.; Banerjee, D.; Gunnlaugsson, H. P.; von Bardeleben, J.; Vickridge, I.; Van Bael, M. J.; Hadermann, J.; Araújo, J. P.; Temst, K.; Vantomme, A.; Pereira, L. M. C.</p> <p>2017-11-01</p> <p>γ -Fe and related alloys are model systems of the coupling between structure and magnetism in solids. Since different electronic <span class="hlt">states</span> (with different volumes and magnetic ordering <span class="hlt">states</span>) are closely spaced in <span class="hlt">energy</span>, small perturbations can alter which one is the actual <span class="hlt">ground</span> <span class="hlt">state</span>. Here, we demonstrate that the ferromagnetic <span class="hlt">state</span> of γ -Fe nanoparticles is associated with a tetragonal distortion of the fcc structure. Combining a wide range of complementary experimental techniques, including low-temperature Mössbauer spectroscopy, advanced transmission electron microscopy, and synchrotron radiation techniques, we unambiguously identify the tetragonally distorted ferromagnetic <span class="hlt">ground</span> <span class="hlt">state</span>, with lattice parameters a =3.76 (2 )Å and c =3.50 (2 )Å , and a magnetic moment of 2.45(5) μB per Fe atom. Our findings indicate that the ferromagnetic order in nanostructured γ -Fe is generally associated with a tetragonal distortion. This observation motivates a theoretical reassessment of the electronic structure of γ -Fe taking tetragonal distortion into account.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110024152','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110024152"><span>High-Performance Solid-<span class="hlt">State</span> W-<span class="hlt">Band</span> Power Amplifiers</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gaier, Todd; Samoska, Lorene; Wells, Mary; Ferber, Robert; Pearson, John; Campbell, April; Peralta, Alejandro; Swift, Gerald; Yocum, Paul; Chung, Yun</p> <p>2003-01-01</p> <p>The figure shows one of four solid-<span class="hlt">state</span> power amplifiers, each capable of generating an output power greater than or equal to 240 mW over one of four overlapping frequency <span class="hlt">bands</span> from 71 to 106 GHz. (The <span class="hlt">bands</span> are 71 to 84, 80 to 92, 88 to 99, and 89 to 106 GHz.) The amplifiers are designed for optimum performance at a temperature of 130 K. These amplifiers were developed specifically for incorporation into frequency-multiplier chains in local oscillators in a low-noise, far-infrared receiving instrument to be launched into outer space to make astrophysical observations. The designs of these amplifiers may also be of interest to designers and manufacturers of terrestrial W-<span class="hlt">band</span> communication and radar systems. Each amplifier includes a set of six high-electron-mobility transistor (HEMT) GaAs monolithic microwave integrated-circuit (MMIC) chips, microstrip cavities, and other components packaged in a housing made from A-40 silicon-aluminum alloy. This alloy was chosen because, for the original intended spacecraft application, it offers an acceptable compromise among the partially competing requirements for high thermal conductivity, low mass, and low thermal expansion. Problems that were solved in designing the amplifiers included designing connectors and packages to fit the available space; designing microstrip signal-power splitters and combiners; matching of impedances across the frequency <span class="hlt">bands</span>; matching of the electrical characteristics of those chips installed in parallel power-combining arms; control and levelling of output power across the <span class="hlt">bands</span>; and designing the MMICs, microstrips, and microstrip cavities to suppress tendencies toward oscillation in several modes, both inside and outside the desired frequency <span class="hlt">bands</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19800016453','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19800016453"><span>Determination of the Solar <span class="hlt">Energy</span> Microclimate of the United <span class="hlt">States</span> Using Satellite Data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Vonderharr, T. H.; Ellis, J. S.</p> <p>1978-01-01</p> <p>The determination of total solar <span class="hlt">energy</span> reaching the <span class="hlt">ground</span> over the United <span class="hlt">States</span> using measurements from meteorological satellites as the basic data set is examined. The methods of satellite data processing are described. Uncertainty analysis and comparison of results with well calibrated surface pyranometers are used to estimate the probable error in the satellite-based determination of <span class="hlt">ground</span> insolation. It is 10 to 15 percent for daily information, and about 5 percent for monthly values. However, the natural space and time variability of insolation is much greater than the uncertainty in the method. The most important aspect of the satellite-based technique is the ability to determine the solar <span class="hlt">energy</span> reaching the <span class="hlt">ground</span> over small areas where no other measurements are available. Thus, it complements the widely spaced solar radiation measurement network of <span class="hlt">ground</span> stations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29379225','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29379225"><span>Hylleraas-Configuration Interaction study of the 1S <span class="hlt">ground</span> <span class="hlt">state</span> of the negative Li ion.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sims, James S</p> <p>2017-12-28</p> <p>In a previous work Sims and Hagstrom [J. Chem. Phys. 140, 224312 (2014)] reported Hylleraas-Configuration Interaction (Hy-CI) method variational calculations for the neutral atom and positive ion 1 S <span class="hlt">ground</span> <span class="hlt">states</span> of the beryllium isoelectronic sequence. The Li - ion, nominally the first member of this series, has a decidedly different electronic structure. This paper reports the results of a large, comparable calculation for the Li - <span class="hlt">ground</span> <span class="hlt">state</span> to explore how well the Hy-CI method can represent the more diffuse L shell of Li - which is representative of the Be(2sns) excited <span class="hlt">states</span> as well. The best non-relativistic <span class="hlt">energy</span> obtained was -7.500 776 596 hartree, indicating that 10 - 20 nh accuracy is attainable in Hy-CI and that convergence of the r 12 r 34 double cusp is fast and that this correlation type can be accurately represented within the Hy-CI model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19830050168&hterms=thermal+insulator&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dthermal%2Binsulator','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19830050168&hterms=thermal+insulator&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dthermal%2Binsulator"><span>The electrical behavior of GaAs-insulator interfaces - A discrete <span class="hlt">energy</span> interface <span class="hlt">state</span> model</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kazior, T. E.; Lagowski, J.; Gatos, H. C.</p> <p>1983-01-01</p> <p>The relationship between the electrical behavior of GaAs Metal Insulator Semiconductor (MIS) structures and the high density discrete <span class="hlt">energy</span> interface <span class="hlt">states</span> (0.7 and 0.9 eV below the conduction <span class="hlt">band</span>) was investigated utilizing photo- and thermal emission from the interface <span class="hlt">states</span> in conjunction with capacitance measurements. It was found that all essential features of the anomalous behavior of GaAs MIS structures, such as the frequency dispersion and the C-V hysteresis, can be explained on the basis of nonequilibrium charging and discharging of the high density discrete <span class="hlt">energy</span> interface <span class="hlt">states</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014isms.confERJ02D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014isms.confERJ02D"><span>Assignment and Analysis of the NO2 In-Plane Rock <span class="hlt">Band</span> of Nitromethane Recorded by High-Resolution FTIR Synchrotron Spectroscopy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dawadi, Mahesh B.; Perry, David S.; Twagirayezu, Sylvestre; Billinghurst, Brant E.</p> <p>2014-06-01</p> <p>The high-resolution rotationally resolved Fourier Transform Far-infrared spectrum of the NO2 in plane-rock <span class="hlt">band</span> (440-510 cm-1) of nitromethane (CH3NO2) has been recorded using the Far-Infrared Beamline at the Canadian Light Source, with a resolution of 0.00096 cm-1. More than 1500 transitions lines have been assigned for ' = 0; {_a}' {≤ 7}; ' {≤ 50}; using an automated <span class="hlt">ground</span> <span class="hlt">state</span> combination difference program together with the traditional Loomis Wood approach. Transitions involving ' = 0; {_a}' {≤7}; ' {≤ 20}; in the upper vibrational <span class="hlt">state</span> are fit using the six-fold torsion-rotation program developed by Ilyushin et.al. The torsion-rotation <span class="hlt">energy</span> pattern in the lowest torsional <span class="hlt">state</span> ( ' = 0) of the upper vibrational <span class="hlt">state</span> is similar to that of the vibrational <span class="hlt">ground</span> <span class="hlt">state</span>. C. F. Neese., An Interactive Loomis-Wood Package, V2.0, {56th},OSU Interanational Symposium on Molecular Spectroscopy (2001). V. V. Ilyushin, Z. Kisiel, L. Pszczolkowski, H. Mader, and J. T. Hougen, M. Mol. Spectrosc., 259, 26, (2010).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004JChPh.12011500K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004JChPh.12011500K"><span>Ab initio investigation of the <span class="hlt">ground</span> and low-lying <span class="hlt">states</span> of the diatomic fluorides TiF, VF, CrF, and MnF</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Koukounas, Constantine; Kardahakis, Stavros; Mavridis, Aristides</p> <p>2004-06-01</p> <p>The electronic structure of the <span class="hlt">ground</span> and low-lying <span class="hlt">states</span> of the diatomic fluorides TiF, VF, CrF, and MnF was examined by multireference and coupled cluster methods in conjunction with extended basis sets. For a total of 34 <span class="hlt">states</span> we report binding <span class="hlt">energies</span>, spectroscopic constants, dipole moments, separation <span class="hlt">energies</span>, and charge distributions. In addition, for all <span class="hlt">states</span> we have constructed full potential curves. The suggested <span class="hlt">ground</span> <span class="hlt">state</span> binding <span class="hlt">energies</span> of TiF(X 4Φ), VF(X 5Π), CrF(X 6Σ+), and MnF(X 7Σ+) are 135, 130, 110, and 108 kcal/mol, respectively, with first excited <span class="hlt">states</span> A 4Σ-, A 5Δ, A 6Π, and a 5Σ+ about 2, 3, 23, and 19 kcal/mol higher. In essence all our numerical findings are in harmony with experimental results. For all molecules and <span class="hlt">states</span> studied it is clear that the in situ metal atom (M) shows highly ionic character, therefore the binding is described realistically by M+F-.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15268185','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15268185"><span>Ab initio investigation of the <span class="hlt">ground</span> and low-lying <span class="hlt">states</span> of the diatomic fluorides TiF, VF, CrF, and MnF.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Koukounas, Constantine; Kardahakis, Stavros; Mavridis, Aristides</p> <p>2004-06-22</p> <p>The electronic structure of the <span class="hlt">ground</span> and low-lying <span class="hlt">states</span> of the diatomic fluorides TiF, VF, CrF, and MnF was examined by multireference and coupled cluster methods in conjunction with extended basis sets. For a total of 34 <span class="hlt">states</span> we report binding <span class="hlt">energies</span>, spectroscopic constants, dipole moments, separation <span class="hlt">energies</span>, and charge distributions. In addition, for all <span class="hlt">states</span> we have constructed full potential curves. The suggested <span class="hlt">ground</span> <span class="hlt">state</span> binding <span class="hlt">energies</span> of TiF(X (4)Phi), VF(X (5)Pi), CrF(X (6)Sigma(+)), and MnF(X (7)Sigma(+)) are 135, 130, 110, and 108 kcal/mol, respectively, with first excited <span class="hlt">states</span> A (4)Sigma(-), A (5)Delta, A (6)Pi, and a (5)Sigma(+) about 2, 3, 23, and 19 kcal/mol higher. In essence all our numerical findings are in harmony with experimental results. For all molecules and <span class="hlt">states</span> studied it is clear that the in situ metal atom (M) shows highly ionic character, therefore the binding is described realistically by M(+)F(-). (c) 2004 American Institute of Physics.</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/2009JMoSp.256...91L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009JMoSp.256...91L"><span>Fourier transform spectroscopy of the CO-stretching <span class="hlt">band</span> of O-18 methanol</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lees, R. M.; Murphy, Reba-Jean; Moruzzi, Giovanni; Predoi-Cross, Adriana; Xu, Li-Hong; Appadoo, D. R. T.; Billinghurst, B.; Goulding, R. R. J.; Zhao, Saibei</p> <p>2009-07-01</p> <p>The high-resolution Fourier transform spectrum of the ν8 CO-stretching <span class="hlt">band</span> of CH 318OH between 900 and 1100 cm -1 has been recorded at the Canadian Light Source (CLS) synchrotron facility in Saskatoon, and the majority of the torsion-rotation structure has been analyzed. For the ν t = 0 torsional <span class="hlt">ground</span> <span class="hlt">state</span>, subbands have been identified for K values from 0 to 11 for A and E torsional symmetries up to J values typically well over 30. For ν t = 1, A and E subbands have been assigned up to K = 7, and several ν t = 2 subbands have also been identified. Upper-<span class="hlt">state</span> term values determined from the assigned transitions using the Ritz program have been fitted to J( J + 1) power-series expansions to obtain substate origins and sets of <span class="hlt">state</span>-specific parameters giving a compact representation of the substate J-dependence. The ν t = 0 subband origins have been fitted to effective molecular constants for the excited CO-stretching <span class="hlt">state</span> and a torsional barrier of 377.49(32) cm -1 is found, representing a 0.89% increase over the <span class="hlt">ground-state</span> value. The vibrational <span class="hlt">energy</span> for the CO-stretch <span class="hlt">state</span> was found to be 1007.49(7) cm -1. A number of subband-wide and J-localized perturbations have been seen in the spectrum, arising both from anharmonic and Coriolis interactions, and several of the interacting <span class="hlt">states</span> have been identified.</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('http://adsabs.harvard.edu/abs/2018ResPh...9..297I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ResPh...9..297I"><span>Optical properties of InAs/GaAs quantum dot superlattice structures</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Imran, Ali; Jiang, Jianliang; Eric, Deborah; Zahid, M. Noaman; Yousaf, M.; Shah, Z. H.</p> <p>2018-06-01</p> <p>Quantum dot (QD) structure has potential applications in modern highly efficient optoelectronic devices due to their <span class="hlt">band</span>-tuning. The device dimensions have been miniatured with increased efficiencies by virtue of this discovery. In this research, we have presented modified analytical and simulation results of InAs/GaAs QD superlattice (QDSL). We have applied tight binding model for the investigation of <span class="hlt">ground</span> <span class="hlt">state</span> <span class="hlt">energies</span> using timeindependent Schrödinger equation (SE) with effective mass approximation. It has been investigated that the electron <span class="hlt">energies</span> are confined due to wave function delocalization in closely coupled QD structures. The minimum <span class="hlt">ground</span> <span class="hlt">state</span> <span class="hlt">energy</span> can be obtained by increasing the periodicity and decreasing the barrier layer thickness. We have calculated electronics and optical properties which includes <span class="hlt">ground</span> <span class="hlt">state</span> <span class="hlt">energies</span>, transition <span class="hlt">energies</span>, density of <span class="hlt">states</span> (DOS), absorption coefficient and refractive index, which can be tuned by structure modification. In our results, the minimum <span class="hlt">ground</span> <span class="hlt">state</span> <span class="hlt">energy</span> of QDSL is achieved to be 0.25 eV with a maximum period of 10 QDs. The minimum <span class="hlt">band</span> to <span class="hlt">band</span> and <span class="hlt">band</span> to continuum transition <span class="hlt">energies</span> are 63 meV and 130 meV with 2 nm barrier layer thickness respectively. The absorption coefficient of our proposed QDSL model is found to be maximum 1.2 × 104 cm-1 and can be used for highly sensitive infrared detector and high efficiency solar cells.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013APS..MARJ23015J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013APS..MARJ23015J"><span>Metal-induced gap <span class="hlt">states</span> in ferroelectric capacitors and its relationship with complex <span class="hlt">band</span> structures</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Junquera, Javier; Aguado-Puente, Pablo</p> <p>2013-03-01</p> <p>At metal-isulator interfaces, the metallic wave functions with an <span class="hlt">energy</span> eigenvalue within the <span class="hlt">band</span> gap decay exponentially inside the dielectric (metal-induced gap <span class="hlt">states</span>, MIGS). These MIGS can be actually regarded as Bloch functions with an associated complex wave vector. Usually only real values of the wave vectors are discussed in text books, since infinite periodicity is assumed and, in that situation, wave functions growing exponentially in any direction would not be physically valid. However, localized wave functions with an exponential decay are indeed perfectly valid solution of the Schrodinger equation in the presence of defects, surfaces or interfaces. For this reason, properties of MIGS have been typically discussed in terms of the complex <span class="hlt">band</span> structure of bulk materials. The probable dependence on the interface particulars has been rarely taken into account explicitly due to the difficulties to include them into the model or simulations. We aim to characterize from first-principles simulations the MIGS in realistic ferroelectric capacitors and their connection with the complex <span class="hlt">band</span> structure of the ferroelectric material. We emphasize the influence of the real interface beyond the complex <span class="hlt">band</span> structure of bulk materials. Financial support provided by MICINN Grant FIS2009-12721-C04-02, and by the European Union Grant No. CP-FP 228989-2 ``OxIDes''. Computer resources provided by the RES.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018SedG..367..135B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018SedG..367..135B"><span>Visualisation and analysis of shear-deformation <span class="hlt">bands</span> in unconsolidated Pleistocene sand using <span class="hlt">ground</span>-penetrating radar: Implications for paleoseismological studies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brandes, Christian; Igel, Jan; Loewer, Markus; Tanner, David C.; Lang, Jörg; Müller, Katharina; Winsemann, Jutta</p> <p>2018-05-01</p> <p>Deformation <span class="hlt">bands</span> in unconsolidated sediments are of great value for paleoseismological studies in sedimentary archives. Using <span class="hlt">ground</span>-penetrating radar (GPR), we investigated an array of shear-deformation <span class="hlt">bands</span> that developed in unconsolidated Pleistocene glacifluvial Gilbert-type delta sediments. A dense grid (spacing 0.6 m) of GPR profiles was measured on top of a 20 m-long outcrop that exposes shear-deformation <span class="hlt">bands</span>. Features in the radargrams could be directly tied to the exposure. The shear-deformation <span class="hlt">bands</span> are partly represented by inclined reflectors and partly by the offset of reflections at delta clinoforms. 3-D interpretation of the 2-D radar sections shows that the <span class="hlt">bands</span> have near-planar geometries that can be traced throughout the entire sediment volume. Thin sections of sediment samples show that the analysed shear-deformation <span class="hlt">bands</span> have a denser grain packing than the host sediment. Thus they have a lower porosity and smaller pore sizes and therefore, in the vadose zone, the deformation <span class="hlt">bands</span> have a higher water content due to enhanced capillary forces. This, together with the partially-developed weak calcite cementation and the distinct offset along the <span class="hlt">bands</span>, are likely the main reasons for the clear and unambiguous expression of the shear-deformation <span class="hlt">bands</span> in the radar survey. The study shows that deformation-<span class="hlt">band</span> arrays can clearly be detected using GPR and quickly mapped over larger sediment volumes. With the 3-D analysis, it is further possible to derive the orientation and geometry of the <span class="hlt">bands</span>. This allows correlation of the <span class="hlt">bands</span> with the regional fault trend. Studying deformation <span class="hlt">bands</span> in unconsolidated sediments with GPR is therefore a powerful approach in paleoseismological studies. Based on our data, we postulate that the outcrop is part of a dextral strike-slip zone that was reactivated by glacial isostatic adjustment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017isms.confEFA04D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017isms.confEFA04D"><span>First High Resolution IR Spectra of 2-^{13}C-PROPANE. the νb{9} B-Type <span class="hlt">Band</span> Near 366.767 \\wn and the νb{26} C-Type <span class="hlt">Band</span> Near 746.615 \\wn. Determination of <span class="hlt">Ground</span> and Upper <span class="hlt">State</span> Constants.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Daunt, S. J.; Grzywacz, Robert; Lafferty, Walter; Flaud, Jean-Marie; Billinghurst, Brant E.</p> <p>2017-06-01</p> <p>This is the first report in a project to record high resolution IR data of the ^{13}C and D substituted isotopologues of propane. In this talk we will give details on the first high resolution (Δν = 0.0009 \\wn) IR investigation of 2-^{13}C-propane. Spectra of the CCC skeletal bending mode near 336.767 \\wn (B-type) and the wagging mode near 746.615 \\wn (C-type) were recorded using the FTS on the Far-IR beamline of the Canadian Light Source (CLS). The spectra were assigned both traditionally and with the aid of the PGOPHER program of Colin Western. The only available MW data on this molecule are the six K =0 J lines from Lide. We therefore had to use the present data to determine a new set of <span class="hlt">ground</span> <span class="hlt">state</span> constants that included centrifugal distortion terms for this molecule. We compare these experimentally determined values with the recent ab initio values of Villa, Senent & Carvajal. Upper <span class="hlt">state</span> constants for both <span class="hlt">bands</span> have been found that provide a good simulation of the spectra. The hope is that this data will be useful in identifying isotopic propane lines in Titan and other astrophysical objects. C. Western, J. Quant. Spectrosc. & Rad. Transf. 186, 221 ff. (2017). Lide, J.Chem. Phys. 33, p.1514ff. (1960). Villa, Senent & Carvajal, PCCP 15, 10258 (2013).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=36068&Lab=ORD&keyword=water+AND+leaks&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=36068&Lab=ORD&keyword=water+AND+leaks&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span><span class="hlt">GROUND</span>-WATER POLLUTION PROBLEMS IN THE SOUTHEASTERN UNITED <span class="hlt">STATES</span></span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>An evaluation of principal sources of <span class="hlt">ground</span>-water contamination has been carried out in seven southeastern <span class="hlt">States</span>--Alabama, Florida, Georgia, Mississippi, North Carolina, South Carolina, and Virginia. Natural <span class="hlt">ground</span>-water quality is good to excellent, except for the presence of ...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20867055','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20867055"><span>Probing quantum frustrated systems via factorization of the <span class="hlt">ground</span> <span class="hlt">state</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Giampaolo, Salvatore M; Adesso, Gerardo; Illuminati, Fabrizio</p> <p>2010-05-21</p> <p>The existence of definite orders in frustrated quantum systems is related rigorously to the occurrence of fully factorized <span class="hlt">ground</span> <span class="hlt">states</span> below a threshold value of the frustration. <span class="hlt">Ground-state</span> separability thus provides a natural measure of frustration: strongly frustrated systems are those that cannot accommodate for classical-like solutions. The exact form of the factorized <span class="hlt">ground</span> <span class="hlt">states</span> and the critical frustration are determined for various classes of nonexactly solvable spin models with different spatial ranges of the interactions. For weak frustration, the existence of disentangling transitions determines the range of applicability of mean-field descriptions in biological and physical problems such as stochastic gene expression and the stability of long-period modulated structures.</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 electronic <span class="hlt">states</span> 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 electronic <span class="hlt">states</span> 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 <span class="hlt">states</span> (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('https://www.ncbi.nlm.nih.gov/pubmed/25978775','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25978775"><span>Dispersion Corrected Structural Properties and Quasiparticle <span class="hlt">Band</span> Gaps of Several Organic Energetic Solids.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Appalakondaiah, S; Vaitheeswaran, G; Lebègue, S</p> <p>2015-06-18</p> <p>We have performed ab initio calculations for a series of energetic solids to explore their structural and electronic properties. To evaluate the <span class="hlt">ground</span> <span class="hlt">state</span> volume of these molecular solids, different dispersion correction methods were accounted in DFT, namely the Tkatchenko-Scheffler method (with and without self-consistent screening), Grimme's methods (D2, D3(BJ)), and the vdW-DF method. Our results reveal that dispersion correction methods are essential in understanding these complex structures with van der Waals interactions and hydrogen bonding. The calculated <span class="hlt">ground</span> <span class="hlt">state</span> volumes and bulk moduli show that the performance of each method is not unique, and therefore a careful examination is mandatory for interpreting theoretical predictions. This work also emphasizes the importance of quasiparticle calculations in predicting the <span class="hlt">band</span> gap, which is obtained here with the GW approximation. We find that the obtained <span class="hlt">band</span> gaps are ranging from 4 to 7 eV for the different compounds, indicating their insulating nature. In addition, we show the essential role of quasiparticle <span class="hlt">band</span> structure calculations to correlate the gap with the energetic properties.</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://www.osti.gov/biblio/22590979-computation-energy-states-hydrogenic-quantum-dot-two-electrons','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22590979-computation-energy-states-hydrogenic-quantum-dot-two-electrons"><span>Computation of <span class="hlt">energy</span> <span class="hlt">states</span> of hydrogenic quantum dot with two-electrons</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>Yakar, Y., E-mail: yuyakar@yahoo.com; Özmen, A., E-mail: aozmen@selcuk.edu.tr; Çakır, B., E-mail: bcakir@selcuk.edu.tr</p> <p>2016-03-25</p> <p>In this study we have investigated the electronic structure of the hydrogenic quantum dot with two electrons inside an impenetrable potential surface. The <span class="hlt">energy</span> eigenvalues and wavefunctions of the <span class="hlt">ground</span> and excited <span class="hlt">states</span> of spherical quantum dot have been calculated by using the Quantum Genetic Algorithm (QGA) and Hartree-Fock Roothaan (HFR) method, and the <span class="hlt">energies</span> are investigated as a function of dot radius. The results show that as dot radius increases, the <span class="hlt">energy</span> of quantum dot decreases.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JMoSp.344...27N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JMoSp.344...27N"><span>First analysis of the hybrid A/B-type 2ν8 <span class="hlt">band</span> of C2HD3 and the Coriolis interactions with the ν3 + ν4 <span class="hlt">band</span> by high-resolution FTIR spectroscopy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ng, L. L.; Tan, T. L.; Chia, A. H.</p> <p>2018-02-01</p> <p>Using a Fourier transform infrared (FTIR) spectrometer, the spectrum of the 2ν8 <span class="hlt">band</span> of ethylene-d3 (C2HD3) was measured between 1745 to 1905 cm-1 at an unapodized resolution of 0.0063 cm-1. For the first time, 1664 perturbed and unperturbed a- and b-type absorption lines of the <span class="hlt">band</span> were recorded, assigned and fitted using the Watson's A-reduced Hamiltonian in the Ir representation to derive rovibrational constants up to four quartic terms for the v8 = 2 <span class="hlt">state</span>. Three rotational constants of the v3 = v4 = 1 <span class="hlt">state</span> were also derived for the first time in this work from the analysis of the a- and b-Coriolis resonances with the v8 = 2 <span class="hlt">state</span>, together with a set of resonance parameters. The root-mean-square (rms) deviation of the FTIR fit was 0.0010 cm-1. The <span class="hlt">band</span> centers of the 2ν8 and ν3 + ν4 <span class="hlt">bands</span> were determined to be 1831.457508 ± 0.000071 cm-1 and 1812.629 ± 0.022 cm-1, respectively. A set of <span class="hlt">ground</span> <span class="hlt">state</span> rovibrational constants of C2HD3 up to five quartic constants was also derived with improved precision from a simultaneous fit of 377 <span class="hlt">ground</span> <span class="hlt">state</span> combination differences (GSCDs) from a-type infrared transitions of the present analysis and 906 GSCDs from the previous work on the C-type ν8 <span class="hlt">band</span>, with an rms deviation of 0.00043 cm-1. The transition dipole moment ratio | μa/μb | was found to be 2.194 ± 0.072.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19770023223','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19770023223"><span>Shuttle program: <span class="hlt">Ground</span> tracking data program document shuttle OFT launch/landing</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lear, W. M.</p> <p>1977-01-01</p> <p>The equations for processing <span class="hlt">ground</span> tracking data during a space shuttle ascent or entry, or any nonfree flight phase of a shuttle mission are given. The resulting computer program processes data from up to three stations simultaneously: C-<span class="hlt">band</span> station number 1; C-<span class="hlt">band</span> station number 2; and an S-<span class="hlt">band</span> station. The C-<span class="hlt">band</span> data consists of range, azimuth, and elevation angle measurements. The S-<span class="hlt">band</span> data consists of range, two angles, and integrated Doppler data in the form of cycle counts. A nineteen element <span class="hlt">state</span> vector is used in Kalman filter to process the measurements. The acceleration components of the shuttle are taken to be independent exponentially-correlated random variables. Nine elements of the <span class="hlt">state</span> vector are the measurement bias errors associated with range and two angles for each tracking station. The biases are all modeled as exponentially-correlated random variables with a typical time constant of 108 seconds. All time constants are taken to be the same for all nine <span class="hlt">state</span> variables. This simplifies the logic in propagating the <span class="hlt">state</span> error covariance matrix ahead in time.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70012976','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70012976"><span><span class="hlt">STATE</span> WATER RESOURCES RESEARCH INSTITUTE PROGRAM: <span class="hlt">GROUND</span> WATER RESEARCH.</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Burton, James S.; ,</p> <p>1985-01-01</p> <p>This paper updates a review of the accomplishments of the <span class="hlt">State</span> Water Resources Research Program in <span class="hlt">ground</span> water contamination research. The aim is to assess the progress made towards understanding the mechanisms of <span class="hlt">ground</span> water contamination and based on this understanding, to suggest procedures for the prevention and control of <span class="hlt">ground</span> water contamination. The following research areas are covered: (1) mechanisms of organic contaminant transport in the subsurface environment; (2) bacterial and viral contamination of <span class="hlt">ground</span> water from landfills and septic tank systems; (3) fate and persistence of pesticides in the subsurface; (4) leachability and transport of <span class="hlt">ground</span> water pollutants from coal production and utilization; and (5) pollution of <span class="hlt">ground</span> water from mineral mining activities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1001115-high-resolution-infrared-spectroscopy-propellane-region-band','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1001115-high-resolution-infrared-spectroscopy-propellane-region-band"><span>High resolution infrared spectroscopy of [1.1.1]propellane: The region of the ν 9 <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>Maki, Arthur; Weber, Alfons; Nibler, Joseph W.</p> <p>2010-11-01</p> <p>The region of the infrared-active <span class="hlt">band</span> of the ν 9 CH2 bending mode [1.1.1]propellane has been recorded at a resolution (0.0025 cm -1) sufficient to distinguish individual rovibrational lines. This region includes the partially overlapping <span class="hlt">bands</span> ν 9 (e') = 1459 cm -1, 2ν 18 (l = 2, E') = 1430 cm -1, ν 6 + ν 12 (E') = 1489 cm-1, and ν 4 + ν 15 (A 2") = 1518 cm -1. In addition, the difference <span class="hlt">band</span> ν 4 - ν 15 (A2") was observed in the far infrared near 295 cm -1 and analyzed to give goodmore » constants for the upper ν 4 levels. The close proximities of the four <span class="hlt">bands</span> in the ν 9 region suggest that Coriolis and Fermi resonance couplings could be significant and theoretical <span class="hlt">band</span> parameters obtained from Gaussian ab initio calculations were helpful in guiding the <span class="hlt">band</span> analyses. The analyses of all four <span class="hlt">bands</span> were accomplished, based on our earlier report of <span class="hlt">ground</span> <span class="hlt">state</span> constants determined from combination differences involving more than 4000 pairs of transitions from five fundamental and four combination <span class="hlt">bands</span>. This paper presents the analyses and the determination of the upper <span class="hlt">state</span> constants of all four <span class="hlt">bands</span> in the region of the ν 9 <span class="hlt">band</span>. Complications were most evident in the 2ν 18 (l = 2, E') <span class="hlt">band</span>, which showed significant perturbations due to mixing with the nearby 2ν 18 (l = 0, A 1') and ν 4 + ν 12 (E') levels which are either infrared inactive as transitions from the <span class="hlt">ground</span> <span class="hlt">state</span>, or, in the latter case, too weak to observe. Finally, these complications are discussed and a comparison of all molecular constants with those available from the ab initio calculations at the anharmonic level is presented.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008SPIE.7132E..06G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008SPIE.7132E..06G"><span><span class="hlt">Energy</span> dependence of effective electron mass and laser-induced ionization of wide <span class="hlt">band</span>-gap solids</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gruzdev, V. E.</p> <p>2008-10-01</p> <p>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 <span class="hlt">energy</span>. Those assumptions exclude from consideration all the effects resulting from significant increase of the effective mass with increasing of electron <span class="hlt">energy</span> in real the conduction <span class="hlt">band</span>. Promotion of electrons to the <span class="hlt">states</span> 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 <span class="hlt">energy</span>, 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 <span class="hlt">energy</span>, we demonstrate that special regimes of high-intensity photo-ionization are possible depending on laser and material parameters. Qualitative analysis of the <span class="hlt">energy</span> dependence of the effective mass also leads to conclusion that the avalanche ionization can be stopped by the effect of electron trapping in the <span class="hlt">states</span> with large values of the effective mass.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22391925-stability-quantum-dot-excited-state-laser-emission-under-simultaneous-ground-state-perturbation','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22391925-stability-quantum-dot-excited-state-laser-emission-under-simultaneous-ground-state-perturbation"><span>Stability of quantum-dot excited-<span class="hlt">state</span> laser emission under simultaneous <span class="hlt">ground-state</span> perturbation</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>Kaptan, Y., E-mail: yuecel.kaptan@physik.tu-berlin.de; Herzog, B.; Schöps, O.</p> <p>2014-11-10</p> <p>The impact of <span class="hlt">ground</span> <span class="hlt">state</span> amplification on the laser emission of In(Ga)As quantum dot excited <span class="hlt">state</span> lasers is studied in time-resolved experiments. We find that a depopulation of the quantum dot <span class="hlt">ground</span> <span class="hlt">state</span> is followed by a drop in excited <span class="hlt">state</span> lasing intensity. The magnitude of the drop is strongly dependent on the wavelength of the depletion pulse and the applied injection current. Numerical simulations based on laser rate equations reproduce the experimental results and explain the wavelength dependence by the different dynamics in lasing and non-lasing sub-ensembles within the inhomogeneously broadened quantum dots. At high injection levels, the observedmore » response even upon perturbation of the lasing sub-ensemble is small and followed by a fast recovery, thus supporting the capacity of fast modulation in dual-<span class="hlt">state</span> devices.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011SPIE.8123E..1HV','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011SPIE.8123E..1HV"><span><span class="hlt">Energy</span>-saving approaches to solid <span class="hlt">state</span> street lighting</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vitta, Pranciškus; Stanikūnas, Rytis; Tuzikas, Arūnas; Reklaitis, Ignas; Stonkus, Andrius; Petrulis, Andrius; Vaitkevičius, Henrikas; Žukauskas, Artūras</p> <p>2011-10-01</p> <p>We consider the <span class="hlt">energy</span>-saving potential of solid-<span class="hlt">state</span> street lighting due to improved visual performance, weather sensitive luminance control and tracking of pedestrians and vehicles. A psychophysical experiment on the measurement of reaction time with a decision making task was performed under mesopic levels of illumination provided by a highpressure sodium (HPS) lamp and different solid-<span class="hlt">state</span> light sources, such as daylight and warm-white phosphor converted light-emitting diodes (LEDs) and red-green-blue LED clusters. The results of the experiment imply that photopic luminances of road surface provided by solid-<span class="hlt">state</span> light sources with an optimized spectral power distribution might be up to twice as low as those provided by the HPS lamp. Dynamical correction of road luminance against road surface conditions typical of Lithuanian climate was estimated to save about 20% of <span class="hlt">energy</span> in comparison with constant-level illumination. The estimated <span class="hlt">energy</span> savings due to the tracking of pedestrians and vehicles amount at least 25% with the cumulative effect of intelligent control of at least 40%. A solid-<span class="hlt">state</span> street lighting system with intelligent control was demonstrated using a 300 m long test <span class="hlt">ground</span> consisting of 10 solid-<span class="hlt">state</span> street luminaires, a meteorological station and microwave motion sensor network operated via power line communication.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26431178','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26431178"><span>Moving Toward the <span class="hlt">Ground</span> <span class="hlt">State</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kumar, Ishan; Ivanova, Natalia</p> <p>2015-10-01</p> <p>Transferring mouse ESCs to a media supplemented with Mek and Gsk3β inhibitors (2i) provokes marked transcriptional and epigenetic changes, embodying a shift toward <span class="hlt">ground-state</span> pluripotency. In this issue of Cell Stem Cell, Kolodziejczyk et al. (2015) examine population structures of ESCs while Galonska et al. (2015) unravel the mechanisms underlying regulatory network rewiring during 2i-mediated reprogramming. Copyright © 2015 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012ApPhL.100z3902Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012ApPhL.100z3902Y"><span>Photon ratchet intermediate <span class="hlt">band</span> solar cells</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yoshida, M.; Ekins-Daukes, N. J.; Farrell, D. J.; Phillips, C. C.</p> <p>2012-06-01</p> <p>In this paper, we propose an innovative concept for solar power conversion—the "photon ratchet" intermediate <span class="hlt">band</span> solar cell (IBSC)—which may increase the photovoltaic <span class="hlt">energy</span> conversion efficiency of IBSCs by increasing the lifetime of charge carriers in the intermediate <span class="hlt">state</span>. The limiting efficiency calculation for this concept shows that the efficiency can be increased by introducing a fast thermal transition of carriers into a non-emissive <span class="hlt">state</span>. At 1 sun, the introduction of a "ratchet <span class="hlt">band</span>" results in an increase of efficiency from 46.8% to 48.5%, due to suppression of entropy generation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29389047','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29389047"><span>Multiscale <span class="hlt">energy</span> reallocation during low-frequency steady-<span class="hlt">state</span> brain response.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Yifeng; Chen, Wang; Ye, Liangkai; Biswal, Bharat B; Yang, Xuezhi; Zou, Qijun; Yang, Pu; Yang, Qi; Wang, Xinqi; Cui, Qian; Duan, Xujun; Liao, Wei; Chen, Huafu</p> <p>2018-05-01</p> <p>Traditional task-evoked brain activations are based on detection and estimation of signal change from the mean signal. By contrast, the low-frequency steady-<span class="hlt">state</span> brain response (lfSSBR) reflects frequency-tagging activity at the fundamental frequency of the task presentation and its harmonics. Compared to the activity at these resonant frequencies, brain responses at nonresonant frequencies are largely unknown. Additionally, because the lfSSBR is defined by power change, we hypothesize using Parseval's theorem that the power change reflects brain signal variability rather than the change of mean signal. Using a face recognition task, we observed power increase at the fundamental frequency (0.05 Hz) and two harmonics (0.1 and 0.15 Hz) and power decrease within the infra-slow frequency <span class="hlt">band</span> (<0.1 Hz), suggesting a multifrequency <span class="hlt">energy</span> reallocation. The consistency of power and variability was demonstrated by the high correlation (r > .955) of their spatial distribution and brain-behavior relationship at all frequency <span class="hlt">bands</span>. Additionally, the reallocation of finite <span class="hlt">energy</span> was observed across various brain regions and frequency <span class="hlt">bands</span>, forming a particular spatiotemporal pattern. Overall, results from this study strongly suggest that frequency-specific power and variability may measure the same underlying brain activity and that these results may shed light on different mechanisms between lfSSBR and brain activation, and spatiotemporal characteristics of <span class="hlt">energy</span> reallocation induced by cognitive tasks. © 2018 Wiley Periodicals, Inc.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2000EPJD....8..227K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2000EPJD....8..227K"><span><span class="hlt">Energy</span> transfer studies in krypton-xenon mixtures excited in a cooled DC discharge</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Krylov, B.; Gerasimov, G.; Morozov, A.; Arnesen, A.; Hallin, R.; Heijkenskjold, F.</p> <p>2000-01-01</p> <p>The VUV spectrum of gaseous mixtures of krypton with a small amount of xenon added was investigated in the range 115-200 nm. The mixtures were excited in a capillary DC discharge where the capillary could be cooled by using liquid nitrogen. The mixed molecule <span class="hlt">band</span> around the Xe I resonance line at λ = 147 nm and the mixed molecule continuum to the long wavelength side from the line were analysed. The <span class="hlt">band</span> around λ = 147 nm was identified as transitions between a weakly bound excited <span class="hlt">state</span> and the weakly bound <span class="hlt">ground</span> <span class="hlt">state</span> of XeKr molecules. When cooling the capillary wall, the appearance of the Xe2 continuum was observed. The effect is ascribed to <span class="hlt">energy</span> transfer between molecular <span class="hlt">states</span> as a consequence of radiation trapping in the <span class="hlt">band</span> around λ = 147 nm. The role of the mixed molecule in the formation of the VUV spectrum of the gas mixture is discussed and underlined.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhRvA..96f3411B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvA..96f3411B"><span>Optical Feshbach resonances and <span class="hlt">ground-state</span>-molecule production in the RbHg system</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Borkowski, Mateusz; Muñoz Rodriguez, Rodolfo; Kosicki, Maciej B.; Ciuryło, Roman; Żuchowski, Piotr S.</p> <p>2017-12-01</p> <p>We present the prospects for photoassociation, optical control of interspecies scattering lengths, and, finally, the production of ultracold absolute <span class="hlt">ground-state</span> molecules in the Rb+Hg system. We use the <span class="hlt">state</span>-of-the-art ab initio methods for the calculations of <span class="hlt">ground</span>- [CCSD(T)] and excited-<span class="hlt">state</span> (EOM-CCSD) potential curves. The RbHg system, thanks to the wide range of stable Hg bosonic isotopes, offers possibilities for mass tuning of <span class="hlt">ground-state</span> interactions. The optical lengths describing the strengths of optical Feshbach resonances near the Rb transitions are favorable even at large laser detunings. <span class="hlt">Ground-state</span> RbHg molecules can be produced with efficiencies ranging from about 20% for deeply bound to at least 50% for weakly bound <span class="hlt">states</span> close to the dissociation limit. Finally, electronic transitions with favorable Franck-Condon factors can be found for the purposes of a STIRAP transfer of the weakly bound RbHg molecules to the absolute <span class="hlt">ground</span> <span class="hlt">state</span> using commercially available lasers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JChPh.147a3934D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JChPh.147a3934D"><span>Electron affinity and excited <span class="hlt">states</span> of methylglyoxal</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dauletyarov, Yerbolat; Dixon, Andrew R.; Wallace, Adam A.; Sanov, Andrei</p> <p>2017-07-01</p> <p>Using photoelectron imaging spectroscopy, we characterized the anion of methylglyoxal (X2A″ electronic <span class="hlt">state</span>) and three lowest electronic <span class="hlt">states</span> of the neutral methylglyoxal molecule: the closed-shell singlet <span class="hlt">ground</span> <span class="hlt">state</span> (X1A'), the lowest triplet <span class="hlt">state</span> (a3A″), and the open-shell singlet <span class="hlt">state</span> (A1A″). The adiabatic electron affinity (EA) of the <span class="hlt">ground</span> <span class="hlt">state</span>, EA(X1A') = 0.87(1) eV, spectroscopically determined for the first time, compares to 1.10(2) eV for unsubstituted glyoxal. The EAs (adiabatic attachment <span class="hlt">energies</span>) of two excited <span class="hlt">states</span> of methylglyoxal were also determined: EA(a3A″) = 3.27(2) eV and EA(A1A″) = 3.614(9) eV. The photodetachment of the anion to each of these two <span class="hlt">states</span> produces the neutral species near the respective structural equilibria; hence, the a3A″ ← X2A″ and A1A″ ← X2A″ photodetachment transitions are dominated by intense peaks at their respective origins. The lowest-<span class="hlt">energy</span> photodetachment transition, on the other hand, involves significant geometry relaxation in the X1A' <span class="hlt">state</span>, which corresponds to a 60° internal rotation of the methyl group, compared to the anion structure. Accordingly, the X1A' ← X2A″ transition is characterized as a broad, congested <span class="hlt">band</span>, whose vertical detachment <span class="hlt">energy</span>, VDE = 1.20(4) eV, significantly exceeds the adiabatic EA. The experimental results are in excellent agreement with the ab initio predictions using several equation-of-motion methodologies, combined with coupled-cluster theory.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22482216-effect-dielectric-stoichiometry-interface-chemical-state-band-alignment-between-tantalum-oxide-platinum','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22482216-effect-dielectric-stoichiometry-interface-chemical-state-band-alignment-between-tantalum-oxide-platinum"><span>Effect of dielectric stoichiometry and interface chemical <span class="hlt">state</span> on <span class="hlt">band</span> alignment between tantalum oxide and platinum</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>Lebedinskii, Yu. Yu.; National Research Nuclear University MEPhI; Chernikova, A. G.</p> <p>2015-10-05</p> <p>The tantalum oxide–platinum interface electronic properties determined by X-ray photoelectron spectroscopy are found to depend on the dielectric stoichiometry and platinum chemical <span class="hlt">state</span>. We demonstrate the slow charging of the tantalum oxide in cases of Ta{sub 2}O{sub 5}/Pt and Ta{sub 2}O{sub 5−y}/Pt interfaces under the X-ray irradiation. This behavior is proposed to be related to the charge accumulation at oxygen vacancies induced traps. Based on the proposed methodology, we define the intrinsic conductive <span class="hlt">band</span> offset (CBO) ∼1.3 eV (both for Ta{sub 2}O{sub 5}/Pt and Ta{sub 2}O{sub 5−y}/Pt) and CBO after the full saturation of the traps charging ∼0.5 eV, while the lastmore » one defines the <span class="hlt">energy</span> position of charged traps below the bottom of conduction <span class="hlt">band</span>. We demonstrate also the pining at the both Ta{sub 2}O{sub 5}/Pt and Ta{sub 2}O{sub 5−y}/Pt interfaces even in the “intrinsic” <span class="hlt">state</span>, apparently induced by the presence of additional interfacial <span class="hlt">states</span>. No shifts of Ta4f line and <span class="hlt">band</span> alignment in over stoichiometric Ta{sub 2}O{sub 5+x}/Pt structure during X-ray irradiation, as well as the absence of pinning, resulting in increase of CBO up to 2.3 eV are found. This behavior is related to the PtO{sub 2} interfacing layer formation at Ta{sub 2}O{sub 5+x}/Pt, blocking the charging of the surface <span class="hlt">states</span> and associated dipole formation.« less</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/2016PhRvB..93w5123F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhRvB..93w5123F"><span><span class="hlt">Ground-state</span> ordering of the J1-J2 model on the simple cubic and body-centered cubic lattices</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Farnell, D. J. J.; Götze, O.; Richter, J.</p> <p>2016-06-01</p> <p>The J1-J2 Heisenberg model is a "canonical" model in the field of quantum magnetism in order to study the interplay between frustration and quantum fluctuations as well as quantum phase transitions driven by frustration. Here we apply the coupled cluster method (CCM) to study the spin-half J1-J2 model with antiferromagnetic nearest-neighbor bonds J1>0 and next-nearest-neighbor bonds J2>0 for the simple cubic (sc) and body-centered cubic (bcc) lattices. In particular, we wish to study the <span class="hlt">ground-state</span> ordering of these systems as a function of the frustration parameter p =z2J2/z1J1 , where z1 (z2) is the number of nearest (next-nearest) neighbors. We wish to determine the positions of the phase transitions using the CCM and we aim to resolve the nature of the phase transition points. We consider the <span class="hlt">ground-state</span> <span class="hlt">energy</span>, order parameters, spin-spin correlation functions, as well as the spin stiffness in order to determine the <span class="hlt">ground-state</span> phase diagrams of these models. We find a direct first-order phase transition at a value of p =0.528 from a <span class="hlt">state</span> of nearest-neighbor Néel order to next-nearest-neighbor Néel order for the bcc lattice. For the sc lattice the situation is more subtle. CCM results for the <span class="hlt">energy</span>, the order parameter, the spin-spin correlation functions, and the spin stiffness indicate that there is no direct first-order transition between <span class="hlt">ground-state</span> phases with magnetic long-range order, rather it is more likely that two phases with antiferromagnetic long range are separated by a narrow region of a spin-liquid-like quantum phase around p =0.55 . Thus the strong frustration present in the J1-J2 Heisenberg model on the sc lattice may open a window for an unconventional quantum <span class="hlt">ground</span> <span class="hlt">state</span> in this three-dimensional spin model.</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>Electronic 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 <span class="hlt">states</span> (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('https://www.ncbi.nlm.nih.gov/pubmed/18698752','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18698752"><span>The hyperbolic chemical bond: Fourier analysis of <span class="hlt">ground</span> and first excited <span class="hlt">state</span> potential <span class="hlt">energy</span> curves of HX (X = H-Ne).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Harrison, John A</p> <p>2008-09-04</p> <p>RHF/aug-cc-pVnZ, UHF/aug-cc-pVnZ, and QCISD/aug-cc-pVnZ, n = 2-5, potential <span class="hlt">energy</span> curves of H2 X (1) summation g (+) are analyzed by Fourier transform methods after transformation to a new coordinate system via an inverse hyperbolic cosine coordinate mapping. The Fourier frequency domain spectra are interpreted in terms of underlying mathematical behavior giving rise to distinctive features. There is a clear difference between the underlying mathematical nature of the potential <span class="hlt">energy</span> curves calculated at the HF and full-CI levels. The method is particularly suited to the analysis of potential <span class="hlt">energy</span> curves obtained at the highest levels of theory because the Fourier spectra are observed to be of a compact nature, with the envelope of the Fourier frequency coefficients decaying in magnitude in an exponential manner. The finite number of Fourier coefficients required to describe the CI curves allows for an optimum sampling strategy to be developed, corresponding to that required for exponential and geometric convergence. The underlying random numerical noise due to the finite convergence criterion is also a clearly identifiable feature in the Fourier spectrum. The methodology is applied to the analysis of MRCI potential <span class="hlt">energy</span> curves for the <span class="hlt">ground</span> and first excited <span class="hlt">states</span> of HX (X = H-Ne). All potential <span class="hlt">energy</span> curves exhibit structure in the Fourier spectrum consistent with the existence of resonances. The compact nature of the Fourier spectra following the inverse hyperbolic cosine coordinate mapping is highly suggestive that there is some advantage in viewing the chemical bond as having an underlying hyperbolic nature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011PhRvC..83b4316B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011PhRvC..83b4316B"><span>Experimental study of ΔI=1 <span class="hlt">bands</span> in In111</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Banerjee, P.; Ganguly, S.; Pradhan, M. K.; Sharma, H. P.; Muralithar, S.; Singh, R. P.; Bhowmik, R. K.</p> <p>2011-02-01</p> <p>The two ΔI=1 <span class="hlt">bands</span> in In111, built upon the 3461.0 and 4931.8 keV <span class="hlt">states</span>, have been studied. The <span class="hlt">bands</span> were populated in the reaction Mo100(F19,α4nγ) at a beam <span class="hlt">energy</span> of 105 MeV. Mean lifetimes of nine <span class="hlt">states</span>, four in the first and five in the second <span class="hlt">band</span>, have been determined for the first time from Doppler shift attenuation data. The deduced B(M1) rates and their behavior as a function of level spin support the interpretation of these <span class="hlt">bands</span> within the framework of the shears mechanism. The geometrical model of Machiavelli has been used to derive the effective gyromagnetic ratios for the two <span class="hlt">bands</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_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('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('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/2001nspc.book..249K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001nspc.book..249K"><span><roman>B</roman>(<roman>M</roman>1) values in the <span class="hlt">band</span>-crossing of shears <span class="hlt">bands</span> in 197<roman>Pb</roman></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Krücken, R.; Cooper, J. R.; Beausang, C. W.; Novak, J. R.; Dewald, A.; Klug, T.; Kemper, G.; von Brentano, P.; Carpenter, M.; Wiedenhöver, I.</p> <p></p> <p>We present details of the <span class="hlt">band</span> crossing mechanism of shears <span class="hlt">bands</span> using the example of 197Pb. Absolute reduced matrix elements B(M1) were determined by means of a RDM lifetime measurement in one of the shears <span class="hlt">bands</span> in 197Pb. The experiment was performed using the New Yale Plunger Device (NYPD) in conjunction with the Gammasphere array. <span class="hlt">Band</span> mixing calculations on the basis of the semi-classical model of the shears mechanism are used to describe the transition matrix elements B(M1) and <span class="hlt">energies</span> throughout the <span class="hlt">band</span>-crossing regions. Good agreement with the data was obtained and the detailed composition of the <span class="hlt">states</span> in the shears <span class="hlt">band</span> are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940006888','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940006888"><span>Electronic excitation of <span class="hlt">ground</span> <span class="hlt">state</span> atoms by collision with heavy gas particles</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hansen, C. Frederick</p> <p>1993-01-01</p> <p>Most of the important chemical reactions which occur in the very high temperature air produced around space vehicles as they enter the atmosphere were investigated both experimentally and theoretically, to some extent at least. One remaining reaction about which little is known, and which could be quite important at the extremely high temperatures that will be produced by the class of space vehicles now contemplated - such as the AOTV - is the excitation of bound electron <span class="hlt">states</span> due to collisions between heavy gas particles. Rates of electronic excitation due to free electron collisions are known to be very rapid, but because these collisions quickly equilibrate the free and bound electron <span class="hlt">energy</span>, the approach to full equilibrium with the heavy particle kinetic <span class="hlt">energy</span> will depend primarily on the much slower process of bound electron excitation in heavy particle collisions and the subsequent rapid transfer to free electron <span class="hlt">energy</span>. This may be the dominant mechanism leading to full equilibrium in the gas once the dissociation process has depleted the molecular <span class="hlt">states</span> so the transfer between molecular vibrational <span class="hlt">energy</span> and free electron <span class="hlt">energy</span> is no longer available as a channel for equilibration of free electron and heavy particle kinetic <span class="hlt">energies</span>. Two mechanisms seem probable in electronic excitation by heavy particle impact. One of these is the collision excitation and deexcitation of higher electronic <span class="hlt">states</span> which are Rydberg like. A report, entitled 'Semi-Classical Theory of Electronic Excitation Rates', was submitted previously. This presented analytic expressions for the transition probabilities, assuming that the interaction potential is an exponential repulsion with a perturbation ripple due to the dipole-induced dipole effect in the case of neutral-neutral collisions, and to the ion-dipole interaction in the case of ion-neutral collisions. However the above may be, there is little doubt that excitation of <span class="hlt">ground</span> <span class="hlt">state</span> species by collision occurs at the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/ha/730a/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/ha/730a/report.pdf"><span><span class="hlt">Ground</span> Water Atlas of the United <span class="hlt">States</span>: Introduction and national summary</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Miller, James A.</p> <p>1999-01-01</p> <p>The <span class="hlt">Ground</span> Water Atlas of the United <span class="hlt">States</span> provides a summary of the most important information available for each principal aquifer, or rock unit that will yield usable quantities of water to wells, throughout the 50 <span class="hlt">States</span>, Puerto Rico, and the U.S. Virgin Islands. The Atlas is an outgrowth of the Regional Aquifer-System Analysis (RASA) program of the U.S. Geological Survey (USGS), a program that investigated 24 of the most important aquifers and aquifer systems of the Nation and one in the Caribbean Islands (fig. 1). The objectives of the RASA program were to define the geologic and hydrologic frameworks of each aquifer system, to assess the geochemistry of the water in the system, to characterize the <span class="hlt">ground</span>-water flow system, and to describe the effects of development on the flow system. Although the RASA studies did not cover the entire Nation, they compiled much of the data needed to make the National assessments of <span class="hlt">ground</span>-water resources presented in the <span class="hlt">Ground</span> Water Atlas of the United <span class="hlt">States</span>. The Atlas, however, describes the location, extent, and geologic and hydrologic characteristics of all the important aquifers in the United <span class="hlt">States</span>, including those not studied by the RASA program. The Atlas is written so that it can be understood by readers who are not hydrologists. Simple language is used to explain technical terms. The principles that control the presence, movement, and chemical quality of <span class="hlt">ground</span> water in different climatic, topographic, and geologic settings are clearly illustrated. The Atlas is, therefore, useful as a teaching tool for introductory courses in hydrology or hydrogeology at the college level and as an overview of <span class="hlt">ground</span>-water conditions for consultants who need information about an individual aquifer. It also serves as an introduction to regional and National <span class="hlt">ground</span>-water resources for lawmakers, personnel of local, <span class="hlt">State</span>, or Federal agencies, or anyone who needs to understand <span class="hlt">ground</span>-water occurrence, movement, and quality. The</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.jstor.org/stable/3798230','USGSPUBS'); return false;" href="http://www.jstor.org/stable/3798230"><span>Reward <span class="hlt">banding</span> to determine reporting rate of recovered mourning dove <span class="hlt">bands</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Tomlinson, R.E.</p> <p>1968-01-01</p> <p>Reward <span class="hlt">bands</span> placed on the other leg of certain regularly <span class="hlt">banded</span> immature mourning doves (Zenaidura macroura) were used to develop information on reporting rates of recovered dove <span class="hlt">bands</span>. Reports from 15 widely separated sections of the United <span class="hlt">States</span> showed considerable variation in recovery rate of doves both with and without reward <span class="hlt">bands</span>. The overall percentages of <span class="hlt">banded</span> doves that were reported as recovered were 9.69% for those with reward <span class="hlt">bands</span> and 3.83% for controls. The bandreporting rate for <span class="hlt">states</span> influenced by publicity was 66%; that for <span class="hlt">states</span> not influenced was 32%.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009NuPhA.825...16B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009NuPhA.825...16B"><span><span class="hlt">Band</span> structures in near spherical 138Ce</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bhattacharjee, T.; Chanda, S.; Bhattacharyya, S.; Basu, S. K.; Bhowmik, R. K.; Das, J. J.; Pramanik, U. Datta; Ghugre, S. S.; Madhavan, N.; Mukherjee, A.; Mukherjee, G.; Muralithar, S.; Singh, R. P.</p> <p>2009-06-01</p> <p>The high spin <span class="hlt">states</span> of N=80138Ce have been populated in the fusion evaporation reaction 130Te( 12C, 4n) 138Ce at E=65 MeV. The γ transitions belonging to various <span class="hlt">band</span> structures were detected and characterized using an array of five Clover Germanium detectors. The level scheme has been established up to a maximum spin and excitation <span class="hlt">energy</span> of 23 ℏ and 9511.3 keV, respectively, by including 53 new transitions. The negative parity ΔI=1 <span class="hlt">band</span>, developed on the 6536.3 keV 15 level, has been conjectured to be a magnetic rotation <span class="hlt">band</span> following a semiclassical analysis and comparing the systematics of similar <span class="hlt">bands</span> in the neighboring nuclei. The said <span class="hlt">band</span> is proposed to have a four quasiparticle configuration of [πgh]⊗[. Other <span class="hlt">band</span> structures are interpreted in terms of multi-quasiparticle configurations, based on Total Routhian Surface (TRS) calculations. For the low and medium spin <span class="hlt">states</span>, a shell model calculation using a realistic two body interaction has been performed using the code OXBASH.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015isms.confERI11K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015isms.confERI11K"><span>Reactions of <span class="hlt">Ground</span> <span class="hlt">State</span> Nitrogen Atoms N(4S) with Astrochemically-Relevant Molecules on Interstellar Dusts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Krim, Lahouari; Nourry, Sendres</p> <p>2015-06-01</p> <p>In the last few years, ambitious programs were launched to probe the interstellar medium always more accurately. One of the major challenges of these missions remains the detection of prebiotic compounds and the understanding of reaction pathways leading to their formation. These complex heterogeneous reactions mainly occur on icy dust grains, and their studies require the coupling of laboratory experiments mimicking the extreme conditions of extreme cold and dilute media. For that purpose, we have developed an original experimental approach that combine the study of heterogeneous reactions (by exposing neutral molecules adsorbed on ice to non-energetic radicals H, OH, N...) and a neon matrix isolation study at very low temperatures, which is of paramount importance to isolate and characterize highly reactive reaction intermediates. Such experimental approach has already provided answers to many questions raised about some astrochemically-relevant reactions occurring in the <span class="hlt">ground</span> <span class="hlt">state</span> on the surface of dust grain ices in dense molecular clouds. The aim of this new present work is to show the implication of <span class="hlt">ground</span> <span class="hlt">state</span> atomic nitrogen on hydrogen atom abstraction reactions from some astrochemically-relevant species, at very low temperatures (3K-20K), without providing any external <span class="hlt">energy</span>. Under cryogenic temperatures and with high barrier heights, such reactions involving N(4S) nitrogen atoms should not occur spontaneously and require an initiating <span class="hlt">energy</span>. However, the detection of some radicals species as byproducts, in our solid samples left in the dark for hours at 10K, proves that hydrogen abstraction reactions involving <span class="hlt">ground</span> <span class="hlt">state</span> N(4S) nitrogen atoms may occur in solid phase at cryogenic temperatures. Our results show the efficiency of radical species formation stemming from non-energetic N-atoms and astrochemically-relevant molecules. We will then discuss how such reactions, involving nitrogen atoms in their <span class="hlt">ground</span> <span class="hlt">states</span>, might be the first key step</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..MAR.K2001B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..MAR.K2001B"><span>The magnetic <span class="hlt">ground</span> <span class="hlt">state</span> and relationship to Kitaev physics in α-RuCl3</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Banerjee, Arnab</p> <p></p> <p>The 2D Kitaev candidate alpha-RuCl3 consists of stacked honeycomb layers weakly coupled by Van der Waals interactions. Here we report the measurements of bulk properties and neutron diffraction in both powder and single crystal samples. Our results show that the full three dimensional magnetic <span class="hlt">ground</span> <span class="hlt">state</span> is highly pliable with at least two dominant phases corresponding to two different out-of-plane magnetic orders. They have different Neel temperatures dependent on the stacking of the 2D layers, such as a broad magnetic transition at TN = 14 K as observed in phase-pure powder samples, or a sharp magnetic transition at a lower TN = 7 K as observed in homogeneous single crystals with no evidence for stacking faults. The magnetic refinements of the neutron scattering data will be discussed, which in all cases shows the in-plane magnetic <span class="hlt">ground</span> <span class="hlt">state</span> is the zigzag phase common in Kitaev related materials including the honeycomb lattice Iridates. Inelastic neutron scattering in all cases shows that this material consistently exhibit strong two-dimensional magnetic fluctuations leading to a break-down of the classical spin-wave picture. Work performed at ORNL is supported by U.S. Dept. of <span class="hlt">Energy</span>, Office of Basic <span class="hlt">Energy</span> Sciences and Office of User Facilities Division.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19173507','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19173507"><span>High-accuracy calculations of the <span class="hlt">ground</span>, 1 1A1', and the 2 1A1', 2 3A1', and 1 1E' excited <span class="hlt">states</span> of H3+.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pavanello, Michele; Adamowicz, Ludwik</p> <p>2009-01-21</p> <p>Accurate variational Born-Oppenheimer calculations of the 1 (1)A(1) ('), 2 (1)A(1) ('), 2 (3)A(1) ('), and 1 (1)E(') <span class="hlt">states</span> of the H(3) (+) ion at the <span class="hlt">ground-state</span> equilibrium geometry are reported. The wave functions of the <span class="hlt">states</span> are expanded in terms of explicitly correlated spherical Gaussian functions with shifted centers. In the variational optimization the analytical gradient of the <span class="hlt">energy</span> with respect to the nonlinear exponential parameters of the Gaussians has been employed. The <span class="hlt">energies</span> obtained in the calculations are the best variational estimates ever calculated for the four <span class="hlt">states</span>. One-electron densities for the <span class="hlt">states</span>, as well as a D(3h)-restricted potential <span class="hlt">energy</span> surface of the <span class="hlt">ground</span> <span class="hlt">state</span> calculated around the equilibrium geometry, are also presented and discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JPCM...29z5801S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JPCM...29z5801S"><span>Evidence for the antiferromagnetic <span class="hlt">ground</span> <span class="hlt">state</span> of Zr2TiAl: 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>Sreenivasa Reddy, P. V.; Kanchana, V.; Vaitheeswaran, G.; Ruban, Andrei V.; Christensen, N. E.</p> <p>2017-07-01</p> <p>A detailed study on the ternary Zr-based intermetallic compound Zr2TiAl has been carried out using first-principles electronic structure calculations. From the total <span class="hlt">energy</span> calculations, we find an antiferromagnetic L11-like (AFM) phase with alternating (1 1 1) spin-up and spin-down layers to be a stable phase among some others with magnetic moment on Ti being 1.22 {μ\\text{B}} . The calculated magnetic exchange interaction parameters of the Heisenberg Hamiltonian and subsequent Heisenberg Monte Carlo simulations confirm that this phase is the magnetic <span class="hlt">ground</span> structure with Néel temperature between 30 and 100 K. The phonon dispersion relations further confirm the stability of the magnetic phase while the non-magnetic phase is found to have imaginary phonon modes and the same is also found from the calculated elastic constants. The magnetic moment of Ti is found to decrease under pressure eventually driving the system to the non-magnetic phase at around 46 GPa, where the phonon modes are found to be positive indicating stability of the non-magnetic phase. A continuous change in the <span class="hlt">band</span> structure under compression leads to the corresponding change of the Fermi surface topology and electronic topological transitions (ETT) in both majority and minority spin cases, which are also evident from the calculated elastic constants and density of <span class="hlt">state</span> calculations for the material under compression.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19820011462','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19820011462"><span>A High Resolution Spectroscopic Study of the Nu2 <span class="hlt">Band</span> of Hydrogen Sulfide and the 1-0 <span class="hlt">Band</span> of Hydrogen Iodide. Ph.D. Thesis - Maryland Univ.</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Strow, L. L.</p> <p>1981-01-01</p> <p>A tunable diode laser spectrometer was constructed and used to study: (1) the effects of centrifugal distortion on the transition frequencies and strengths of the nu sub 2 <span class="hlt">band</span> of H2S, and (2) nuclear quadrupole hyperfine structure in the 1-0 <span class="hlt">band</span> of HI. A total of 126 line frequencies and 94 line strengths in the nu sub 2 <span class="hlt">band</span> of H2S were measured. The average accuracy of the line frequency measurements was + or - 0.0016 cm. The line strengths were measured to an average accuracy of about 3 percent. The effect of the finite spectral width of the diode laser on the measurement of line strengths is discussed. The observed H2S line frequencies were fit to Watson's AS and NS reduced Hamiltonian in both the Ir and IIIr coordinate representations in order to determine the best set of rotation distortion constants for the upper <span class="hlt">state</span> of the nu sub 2 <span class="hlt">band</span>. Comparisons of the observed line strengths in this <span class="hlt">band</span> to rigid rotor line strengths are also presented. Nuclear quadrupole hyperfine structure in the low J lines of the 1-0 <span class="hlt">band</span> of HI was observed. The upper vibrational <span class="hlt">state</span> nuclear quadrupole coupling constant, determined from the observed splittings, was -1850 MHz + or - 12 MHz or 1.2 percent + or - 0.7 percent larger than the <span class="hlt">ground</span> <span class="hlt">state</span> coupling constant.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvB..97o5422E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvB..97o5422E"><span>Topological nanophononic <span class="hlt">states</span> by <span class="hlt">band</span> inversion</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Esmann, Martin; Lamberti, Fabrice Roland; Senellart, Pascale; Favero, Ivan; Krebs, Olivier; Lanco, Loïc; Gomez Carbonell, Carmen; Lemaître, Aristide; Lanzillotti-Kimura, Norberto Daniel</p> <p>2018-04-01</p> <p>Nanophononics is essential for the engineering of thermal transport in nanostructured electronic devices, it greatly facilitates the manipulation of mechanical resonators in the quantum regime, and it could unveil a new route in quantum communications using phonons as carriers of information. Acoustic phonons also constitute a versatile platform for the study of fundamental wave dynamics, including Bloch oscillations, Wannier-Stark ladders, and other localization phenomena. Many of the phenomena studied in nanophononics were inspired by their counterparts in optics and electronics. In these fields, the consideration of topological invariants to control wave dynamics has already had a great impact for the generation of robust confined <span class="hlt">states</span>. Interestingly, the use of topological phases to engineer nanophononic devices remains an unexplored and promising field. Conversely, the use of acoustic phonons could constitute a rich platform to study topological <span class="hlt">states</span>. Here, we introduce the concept of topological invariants to nanophononics and experimentally implement a nanophononic system supporting a robust topological interface <span class="hlt">state</span> at 350 GHz. The <span class="hlt">state</span> is constructed through <span class="hlt">band</span> inversion, i.e., by concatenating two semiconductor superlattices with inverted spatial mode symmetries. The existence of this <span class="hlt">state</span> is purely determined by the Zak phases of the constituent superlattices, i.e., the one-dimensional Berry phase. We experimentally evidenced the mode through Raman spectroscopy. The reported robust topological interface <span class="hlt">states</span> could become part of nanophononic devices requiring resonant structures such as sensors or phonon lasers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018CPL...700...36R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018CPL...700...36R"><span><span class="hlt">Energy</span>-switching potential <span class="hlt">energy</span> surface for <span class="hlt">ground-state</span> C3</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rocha, C. M. R.; Varandas, A. J. C.</p> <p>2018-05-01</p> <p>The multiple <span class="hlt">energy</span> switching scheme [J. Chem. Phys. 119 (2003) 2596] has been used to improve the double many-body expansion (DMBE II) potential <span class="hlt">energy</span> surface of C3 near its linear global minima by morphing it with an accurate Taylor-series expansion [J. Chem. Phys. 144 (2016) 044307]. The final ES form attains the accuracy of the local form in reproducing the rovibrational spectrum of C3 while keeping unaltered all key attributes of the original DMBE II, namely conical intersection seams and dissociative channels. The ES form is therefore commended for adiabatic spectroscopic and reaction dynamics studies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27603228','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27603228"><span><span class="hlt">Energy</span>-Looping Nanoparticles: Harnessing Excited-<span class="hlt">State</span> Absorption for Deep-Tissue Imaging.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Levy, Elizabeth S; Tajon, Cheryl A; Bischof, Thomas S; Iafrati, Jillian; Fernandez-Bravo, Angel; Garfield, David J; Chamanzar, Maysamreza; Maharbiz, Michel M; Sohal, Vikaas S; Schuck, P James; Cohen, Bruce E; Chan, Emory M</p> <p>2016-09-27</p> <p>Near infrared (NIR) microscopy enables noninvasive imaging in tissue, particularly in the NIR-II spectral range (1000-1400 nm) where attenuation due to tissue scattering and absorption is minimized. Lanthanide-doped upconverting nanocrystals are promising deep-tissue imaging probes due to their photostable emission in the visible and NIR, but these materials are not efficiently excited at NIR-II wavelengths due to the dearth of lanthanide <span class="hlt">ground-state</span> absorption transitions in this window. Here, we develop a class of lanthanide-doped imaging probes that harness an <span class="hlt">energy</span>-looping mechanism that facilitates excitation at NIR-II wavelengths, such as 1064 nm, that are resonant with excited-<span class="hlt">state</span> absorption transitions but not <span class="hlt">ground-state</span> absorption. Using computational methods and combinatorial screening, we have identified Tm(3+)-doped NaYF4 nanoparticles as efficient looping systems that emit at 800 nm under continuous-wave excitation at 1064 nm. Using this benign excitation with standard confocal microscopy, <span class="hlt">energy</span>-looping nanoparticles (ELNPs) are imaged in cultured mammalian cells and through brain tissue without autofluorescence. The 1 mm imaging depths and 2 μm feature sizes are comparable to those demonstrated by <span class="hlt">state</span>-of-the-art multiphoton techniques, illustrating that ELNPs are a promising class of NIR probes for high-fidelity visualization in cells and tissue.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/fs/2007/3007/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/fs/2007/3007/"><span><span class="hlt">Ground</span>-water recharge in humid areas of the United <span class="hlt">States</span>: A summary of <span class="hlt">Ground</span>-Water Resources Program studies, 2003-2006</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Delin, Geoffrey N.; Risser, Dennis W.</p> <p>2007-01-01</p> <p>Increased demands on water resources by a growing population and recent droughts have raised awareness about the adequacy of <span class="hlt">ground</span>-water resources in humid areas of the United <span class="hlt">States</span>. The spatial and temporal variability of <span class="hlt">ground</span>-water recharge are key factors that need to be quantified to determine the sustainability of <span class="hlt">ground</span>-water resources. <span class="hlt">Ground</span>-water recharge is defined herein as the entry into the saturated zone of water made available at the water-table surface, together with the associated flow away from the water table within the saturated zone (Freeze and Cherry, 1979). In response to the need for better estimates of <span class="hlt">ground</span>-water recharge, the <span class="hlt">Ground</span>-Water Resources Program (GWRP) of the U.S. Geological Survey (USGS) began an initiative in 2003 to estimate <span class="hlt">ground</span>-water recharge rates in the relatively humid areas of the United <span class="hlt">States</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17302473','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17302473"><span>Real-time observation of intramolecular proton transfer in the electronic <span class="hlt">ground</span> <span class="hlt">state</span> of chloromalonaldehyde: an ab initio study of time-resolved 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>do N Varella, Márcio T; Arasaki, Yasuki; Ushiyama, Hiroshi; Takatsuka, Kazuo; Wang, Kwanghsi; McKoy, Vincent</p> <p>2007-02-07</p> <p>The authors report on studies of time-resolved photoelectron spectra of intramolecular proton transfer in the <span class="hlt">ground</span> <span class="hlt">state</span> of chloromalonaldehyde, employing ab initio photoionization matrix elements and effective potential surfaces of reduced dimensionality, wherein the couplings of proton motion to the other molecular vibrational modes are embedded by averaging over classical trajectories. In the simulations, population is transferred from the vibrational <span class="hlt">ground</span> <span class="hlt">state</span> to vibrationally hot wave packets by pumping to an excited electronic <span class="hlt">state</span> and dumping with a time-delayed pulse. These pump-dump-probe simulations demonstrate that the time-resolved photoelectron spectra track proton transfer in the electronic <span class="hlt">ground</span> <span class="hlt">state</span> well and, furthermore, that the geometry dependence of the matrix elements enhances the tracking compared with signals obtained with the Condon approximation. Photoelectron kinetic <span class="hlt">energy</span> distributions arising from wave packets localized in different basins are also distinguishable and could be understood, as expected, on the basis of the strength of the optical couplings in different regions of the <span class="hlt">ground</span> <span class="hlt">state</span> potential surface and the Franck-Condon overlaps of the <span class="hlt">ground</span> <span class="hlt">state</span> wave packets with the vibrational eigenstates of the ion potential surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008JMAA..338..675R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008JMAA..338..675R"><span>Semistable extremal <span class="hlt">ground</span> <span class="hlt">states</span> for nonlinear evolution equations in unbounded domains</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rodríguez-Bernal, Aníbal; Vidal-López, Alejandro</p> <p>2008-02-01</p> <p>In this paper we show that dissipative reaction-diffusion equations in unbounded domains posses extremal semistable <span class="hlt">ground</span> <span class="hlt">states</span> equilibria, which bound asymptotically the global dynamics. Uniqueness of such positive <span class="hlt">ground</span> <span class="hlt">state</span> and their approximation by extremal equilibria in bounded domains is also studied. The results are then applied to the important case of logistic equations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013APS..DMP.D1116D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013APS..DMP.D1116D"><span>Effects of inter-fullerene π-<span class="hlt">band</span> mixings in the photoexcitation of hybrid plasmons in the C60@C240 molecule</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>de, Rume; Madjet, Mohamed; Chakraborty, Himadri</p> <p>2013-05-01</p> <p>We perform a detailed study of the <span class="hlt">ground</span> <span class="hlt">state</span> electronic structure of a two-layer fullerene onion molecule C60@C240. Calculations are carried out in a quantum mechanical framework of local density approximation (LDA) where the onion's ion-core of sixty C4+ ions from C60 and two hundred and forty of those from C240 is smeared into a classical jellium distribution. Significant inter-fullerene mixing between the <span class="hlt">bands</span> of single-node radial symmetry, the π-<span class="hlt">bands</span>, is found. We then compute the photoionization from all the levels of the system using a time-dependent version of LDA at photon <span class="hlt">energies</span> where the ionization is dominated by the inter-layer hybridization of collective plasmon resonances. It is determined, by comparing the isolated fullerene cross sections with the cross section of the onion system for both π and σ (having nodeless radial waves) symmetry, that the π-<span class="hlt">band</span> mixing is predominantly responsible for the production of plasmon hybrids. Supported by NSF and DOE.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JAP...119x5701P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JAP...119x5701P"><span>Ionization equilibrium at the transition from valence-<span class="hlt">band</span> to acceptor-<span class="hlt">band</span> migration of holes in boron-doped diamond</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.; Kovalev, A. I.; Zabrodskii, A. G.</p> <p>2016-06-01</p> <p>A quasi-classical model of ionization equilibrium in the p-type diamond between hydrogen-like acceptors (boron atoms which substitute carbon atoms in the crystal lattice) and holes in the valence <span class="hlt">band</span> (v-<span class="hlt">band</span>) is proposed. The model is applicable on the insulator side of the insulator-metal concentration phase transition (Mott transition) in p-Dia:B crystals. The densities of the spatial distributions of impurity atoms (acceptors and donors) and of holes in the crystal are considered to be Poissonian, and the fluctuations of their electrostatic potential <span class="hlt">energy</span> are considered to be Gaussian. The model accounts for the decrease in thermal ionization <span class="hlt">energy</span> of boron atoms with increasing concentration, as well as for electrostatic fluctuations due to the Coulomb interaction limited to two nearest point charges (impurity ions and holes). The mobility edge of holes in the v-<span class="hlt">band</span> is assumed to be equal to the sum of the threshold <span class="hlt">energy</span> for diffusion percolation and the exchange <span class="hlt">energy</span> of the holes. On the basis of the virial theorem, the temperature Tj is determined, in the vicinity of which the dc <span class="hlt">band</span>-like conductivity of holes in the v-<span class="hlt">band</span> is approximately equal to the hopping conductivity of holes via the boron atoms. For compensation ratio (hydrogen-like donor to acceptor concentration ratio) K ≈ 0.15 and temperature Tj, the concentration of "free" holes in the v-<span class="hlt">band</span> and their jumping (turbulent) drift mobility are calculated. Dependence of the differential <span class="hlt">energy</span> of thermal ionization of boron atoms (at the temperature 3Tj/2) as a function of their concentration N is calculated. The estimates of the extrapolated into the temperature region close to Tj hopping drift mobility of holes hopping from the boron atoms in the charge <span class="hlt">states</span> (0) to the boron atoms in the charge <span class="hlt">states</span> (-1) are given. Calculations based on the model show good agreement with electrical conductivity and Hall effect measurements for p-type diamond with boron atom concentrations in the</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/biblio/22606440-energy-band-gap-spectroscopic-studies-mn-sub-cu-sub-wo-sub','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22606440-energy-band-gap-spectroscopic-studies-mn-sub-cu-sub-wo-sub"><span><span class="hlt">Energy</span> <span class="hlt">band</span> gap and spectroscopic studies in Mn{sub 1-x}Cu{sub x}WO{sub 4} (0 ≤ x ≤ 0.125)</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>Mal, Priyanath; Rambabu, P.; Turpu, G. R.</p> <p>2016-05-06</p> <p>A study on the effect of nonmagnetic Cu{sup 2+} substitution at Mn{sup 2+} site on the structural and <span class="hlt">energy</span> <span class="hlt">band</span> gap of the MnWO{sub 4} is reported. Convenient solid <span class="hlt">state</span> reaction route has been adopted for the synthesis of Mn{sub 1-x}Cu{sub x}WO{sub 4}. X-ray diffraction (XRD) pattern showed high crystalline quality of the prepared samples. Raman spectroscopic studies were carried out to understand the structural aspects of the doping. 15 Raman active modes were identified out of 18, predicted for wolframite type monoclinic structure of MnWO{sub 4}. UV-visible diffuse reflectance spectra were recorded and analyzed to get <span class="hlt">energy</span> <span class="hlt">band</span> gapmore » of the studied system and are found in the range of 2.5 eV to 2.04 eV with a systematic decrease with the increase in Cu{sup 2+} concentration. <span class="hlt">Energy</span> <span class="hlt">band</span> gap values are verified by Density Functional Theory calculations based on projector augmented wave (PAW) method. The calculated values are in good agreement with the experimental data.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910055819&hterms=Dissociative&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DDissociative','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910055819&hterms=Dissociative&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DDissociative"><span>Dissociative recombination of the <span class="hlt">ground</span> <span class="hlt">state</span> of N2(+)</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Guberman, Steven L.</p> <p>1991-01-01</p> <p>Large-scale calculations of the dissociative recombination cross sections and rates for the v = 0 level of the N2(+) <span class="hlt">ground</span> <span class="hlt">state</span> are reported, and the important role played by vibrationally excited Rydberg <span class="hlt">states</span> lying both below and above the v = 0 level of the ion is demonstrated. The large-scale electronic wave function calculations were done using triple zeta plus polarization nuclear-centered-valence Gaussian basis sets. The electronic widths were obtained using smaller wave functions, and the cross sections were calculated on the basis of the multichannel quantum defect theory. The DR rate is calculated at 1.6 x 10 to the -7th x (Te/300) to the -0.37 cu cm/sec for Te in the range of 100 to 1000 K, and is found to be in excellent agreement with prior microwave afterglow experiments but in disagreement with recent merged beam results. It is inferred that the dominant mechanism for DR imparts sufficient <span class="hlt">energy</span> to the product atoms to allow for escape from the Martian atmosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19466824','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19466824"><span>Nested variant of the method of moments of coupled cluster equations for vertical excitation <span class="hlt">energies</span> and excited-<span class="hlt">state</span> potential <span class="hlt">energy</span> surfaces.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kowalski, Karol</p> <p>2009-05-21</p> <p>In this article we discuss the problem of proper balancing of the noniterative corrections to the <span class="hlt">ground</span>- and excited-<span class="hlt">state</span> <span class="hlt">energies</span> obtained with approximate coupled cluster (CC) and equation-of-motion CC (EOMCC) approaches. It is demonstrated that for a class of excited <span class="hlt">states</span> dominated by single excitations and for <span class="hlt">states</span> with medium doubly excited component, the newly introduced nested variant of the method of moments of CC equations provides mathematically rigorous way of balancing the <span class="hlt">ground</span>- and excited-<span class="hlt">state</span> correlation effects. The resulting noniterative methodology accounting for the effect of triples is tested using its parallel implementation on the systems, for which iterative CC/EOMCC calculations with full inclusion of triply excited configurations or their most important subset are numerically feasible.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011mss..confEMF03L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011mss..confEMF03L"><span>An Accurate New Potential Function for <span class="hlt">Ground-State</span> X{e}_2 from UV and Virial Coefficient Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Le Roy, Robert J.; Mackie, J. Cameron; Chandrasekhar, Pragna</p> <p>2011-06-01</p> <p>Determining accurate analytic pair potentials for rare gas dimers has been a longstanding goal in molecular physics. However, most potential <span class="hlt">energy</span> functions reported to date fail to optimally represent the available spectroscopic data, in spite of the fact that such data provide constraints of unparalleled precision on the attractive potential <span class="hlt">energy</span> wells of these species. A recent study of ArXe showed that it is a straightforward matter to combine multi-isotopologue spectroscopic data (in that case, microwave, and high resolution UV measurements) and virial coefficients in a direct fit to obtain a flexible analytic potential function that incorporates the theoretically predicted damped inverse-power long-range behaviour. The present work reports the application of this approach to Xe_2, with a direct fit to high resolution rotationally resolved UV emission data for v''=0 and 1, <span class="hlt">band</span> head data for v''=0-9, and virial coefficient data for T=165-950 K being used to obtain an accurate new potential <span class="hlt">energy</span> function for the <span class="hlt">ground</span> <span class="hlt">state</span> of this Van der Waals molecule. Analogous results for other rare-gas pairs will also be presented, as time permits. L. Piticco, F. Merkt, A.A. Cholewinski, F.R. McCourt and R.J. Le Roy, J. Mol. Spectrosc. 264, 83 (2010). A. Wüest and K.G. Bruin and F. Merkt, Can. J. Chem. 82, 750 (2004). D.E. Freeman, K. Yoshino, and Y. Tanaka, J. Chem. Phys. 61, 4880 (1974). J.H. Dymond, K.N. Marsh, R.C. Wilhoit and K.C. Wong, in Landold-Börnstein, New Series, Group IV, edited by M. Frenkel and K.N. Marsh, Vol. 21 (2003).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011PhRvA..83d2108F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011PhRvA..83d2108F"><span>Classification of matrix-product <span class="hlt">ground</span> <span class="hlt">states</span> corresponding to one-dimensional chains of two-<span class="hlt">state</span> sites of nearest neighbor interactions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fatollahi, Amir H.; Khorrami, Mohammad; Shariati, Ahmad; Aghamohammadi, Amir</p> <p>2011-04-01</p> <p>A complete classification is given for one-dimensional chains with nearest-neighbor interactions having two <span class="hlt">states</span> in each site, for which a matrix product <span class="hlt">ground</span> <span class="hlt">state</span> exists. The Hamiltonians and their corresponding matrix product <span class="hlt">ground</span> <span class="hlt">states</span> are explicitly obtained.</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('https://www.ncbi.nlm.nih.gov/pubmed/28526885','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28526885"><span>Experimental linear-optics simulation of <span class="hlt">ground-state</span> of an Ising spin chain.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Xue, Peng; Zhan, Xian; Bian, Zhihao</p> <p>2017-05-19</p> <p>We experimentally demonstrate a photonic quantum simulator: by using a two-spin Ising chain (an isolated dimer) as an example, we encode the wavefunction of the <span class="hlt">ground</span> <span class="hlt">state</span> with a pair of entangled photons. The effect of magnetic fields, leading to a critical modification of the correlation between two spins, can be simulated by just local operations. With the ratio of simulated magnetic fields and coupling strength increasing, the <span class="hlt">ground</span> <span class="hlt">state</span> of the system changes from a product <span class="hlt">state</span> to an entangled <span class="hlt">state</span> and back to another product <span class="hlt">state</span>. The simulated <span class="hlt">ground</span> <span class="hlt">states</span> can be distinguished and the transformations between them can be observed by measuring correlations between photons. This simulation of the Ising model with linear quantum optics opens the door to the future studies which connect quantum information and condensed matter physics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015isms.confETI11C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015isms.confETI11C"><span>Vibrationally-Resolved Kinetic Isotope Effects in the Proton-Transfer Dynamics of <span class="hlt">Ground-State</span> Tropolone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chew, Kathryn; Vealey, Zachary; Vaccaro, Patrick</p> <p>2015-06-01</p> <p>The vibrational and isotopic dependence of the hindered (tunneling-mediated) proton-transfer reaction taking place in the <span class="hlt">ground</span> electronic <span class="hlt">state</span> ( X1{A}1) of monodeuterated tropolone (TrOD) has been explored under ambient (bulk-gas) conditions by applying two-color variants of resonant four-wave mixing (RFWM) spectroscopy in conjunction with polarization-resolved detection schemes designed to alleviate spectral complexity and facilitate rovibrational assignments. Full rotation-tunneling analyses of high-resolution spectral profiles acquired for the fundamental and first-overtone <span class="hlt">bands</span> of a reaction-promoting O-D\\cdotsO deformation/ring-breathing mode, νb{36}(a1), were performed, thereby extracting refined structural and dynamical information that affords benchmarks for the quantitative interpretation of tunneling-induced signatures found in long-range scans of X1{A}1 vibrational levels residing below Etilde{X}vib = 1700 wn}. Observed kinetic isotope effects, which reflect changes in both reaction kinematics and vibrational displacements, will be discussed, with high-level quantum-chemical calculations serving to elucidate <span class="hlt">state</span>-resolved propensities for proton transfer in TrOH and TrOD.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017CPL...690...20K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017CPL...690...20K"><span>Restoring the Pauli principle in the random phase approximation <span class="hlt">ground</span> <span class="hlt">state</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kosov, D. S.</p> <p>2017-12-01</p> <p>Random phase approximation <span class="hlt">ground</span> <span class="hlt">state</span> contains electronic configurations where two (and more) identical electrons can occupy the same molecular spin-orbital violating the Pauli exclusion principle. This overcounting of electronic configurations happens due to quasiboson approximation in the treatment of electron-hole pair operators. We describe the method to restore the Pauli principle in the RPA wavefunction. The proposed theory is illustrated by the calculations of molecular dipole moments and electronic kinetic <span class="hlt">energies</span>. The Hartree-Fock based RPA, which is corrected for the Pauli principle, gives the results of comparable accuracy with Møller-Plesset second order perturbation theory and coupled-cluster singles and doubles method.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012PhRvC..86d4305W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012PhRvC..86d4305W"><span>Rotational <span class="hlt">band</span> properties of 173W</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, H. X.; Zhang, Y. H.; Zhou, X. H.; Liu, M. L.; Ding, B.; Li, G. S.; Hua, W.; Zhou, H. B.; Guo, S.; Qiang, Y. H.; Oshima, M.; Koizumi, M.; Toh, Y.; Kimura, A.; Harada, H.; Furutaka, K.; Kitatani, F.; Nakamura, S.; Hatsukawa, Y.; Ohta, M.; Hara, K.; Kin, T.; Meng, J.</p> <p>2012-10-01</p> <p>High-spin <span class="hlt">states</span> in 173W have been studied using the 150Nd(28Si,5n)173W reaction at beam <span class="hlt">energies</span> of 135 and 140 MeV. The previously known <span class="hlt">bands</span> associated with the 7/2+[633], 5/2-[512], and 1/2-[521] configurations are extended significantly, and the unfavored signature branch of the 1/2-[521] <span class="hlt">band</span> is established for the first time. The <span class="hlt">band</span> properties, such as level spacings, <span class="hlt">band</span>-crossing frequencies, alignment gains, and signature splittings, are discussed with an emphasis on the low-spin signature inversion observed in the 5/2-[512] <span class="hlt">band</span>. By comparing the experimental B(M1)/B(E2) ratios with the theoretical values, we conclude that the configuration of the 5/2-[512] <span class="hlt">band</span> is quite pure at low spins without appreciable admixture of the 5/2-[523] orbit, in conflict with the particle rotor model calculated results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015OptMa..49..319S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015OptMa..49..319S"><span>Excitonic spectra and <span class="hlt">energy</span> <span class="hlt">band</span> structure of ZnAl2Se4 crystals</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Syrbu, N. N.; Zalamai, V. V.; Tiron, A. V.; Tiginyanu, I. M.</p> <p>2015-11-01</p> <p>Absorption, reflection and wavelength modulated reflection spectra were investigated in ZnAl2Se4 crystals. The <span class="hlt">energy</span> positions of <span class="hlt">ground</span> and excited <span class="hlt">states</span> for three excitonic series (А, В and С) were determined. The main parameters of excitons and more precise values of <span class="hlt">energy</span> intervals V1(Γ7)-C1(Γ6), V2(Γ6)-C1(Γ6), and V3(Γ7)-C1(Γ6) were estimated. Values of splitting due to crystal field and spin-orbital interaction were calculated. Effective masses of electrons (mC1∗) and holes (mV1∗, mV2∗, mV3∗) were estimated. Reflection spectra contours in excitonic region were calculated using dispersion equations. Optical functions for E > Eg from measured reflection spectra were assigned on the base of Kramers-Kronig relations.</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 electronic <span class="hlt">bands</span> corresponding to Pt and Pd, represented in terms of the corresponding density of <span class="hlt">states</span>. 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('https://www.osti.gov/pages/biblio/1344110-superconducting-transitions-flat-band-systems','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1344110-superconducting-transitions-flat-band-systems"><span>Superconducting transitions in flat-<span class="hlt">band</span> systems</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Iglovikov, V. I.; Hébert, F.; Grémaud, B.; ...</p> <p>2014-09-11</p> <p>The physics of strongly correlated quantum particles within a flat <span class="hlt">band</span> was originally explored as a route to itinerant ferromagnetism and, indeed, a celebrated theorem by Lieb rigorously establishes that the <span class="hlt">ground</span> <span class="hlt">state</span> of the repulsive Hubbard model on a bipartite lattice with unequal number of sites in each sublattice must have nonzero spin S at half-filling. Recently, there has been interest in Lieb geometries due to the possibility of novel topological insulator, nematic, and Bose-Einstein condensed (BEC) phases. In this paper, we extend the understanding of the attractive Hubbard model on the Lieb lattice by using Determinant Quantum Montemore » Carlo to study real space charge and pair correlation functions not addressed by the Lieb theorems. Specifically, our results show unusual charge and charge transfer signatures within the flat <span class="hlt">band</span>, and a reduction in pairing order at ρ = 2/3 and ρ = 4/3, the points at which the flat <span class="hlt">band</span> is first occupied and then completely filled. Lastly, we compare our results to the case of flat <span class="hlt">bands</span> in the Kagome lattice and demonstrate that the behavior observed in the two cases is rather different.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JChPh.147l4305M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JChPh.147l4305M"><span>Interplay of spin-dependent delocalization and magnetic anisotropy in the <span class="hlt">ground</span> and excited <span class="hlt">states</span> of [Gd2@C78]- and [Gd2@C80]-</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mansikkamäki, Akseli; Popov, Alexey A.; Deng, Qingming; Iwahara, Naoya; Chibotaru, Liviu F.</p> <p>2017-09-01</p> <p>The magnetic properties and electronic structure of the <span class="hlt">ground</span> and excited <span class="hlt">states</span> of two recently characterized endohedral metallo-fullerenes, [Gd2@C78]- (1) and [Gd2@C80]- (2), have been studied by theoretical methods. The systems can be considered as [Gd2]5+ dimers encapsulated in a fullerene cage with the fifteen unpaired electrons ferromagnetically coupled into an S = 15/2 high-spin configuration in the <span class="hlt">ground</span> <span class="hlt">state</span>. The microscopic mechanisms governing the Gd-Gd interactions leading to the ferromagnetic <span class="hlt">ground</span> <span class="hlt">state</span> are examined by a combination of density functional and ab initio calculations and the full <span class="hlt">energy</span> spectrum of the <span class="hlt">ground</span> and lowest excited <span class="hlt">states</span> is constructed by means of ab initio model Hamiltonians. The <span class="hlt">ground</span> <span class="hlt">state</span> is characterized by strong electron delocalization bordering on a σ type one-electron covalent bond and minor zero-field splitting (ZFS) that is successfully described as a second order spin-orbit coupling effect. We have shown that the observed ferromagnetic interaction originates from Hund's rule coupling and not from the conventional double exchange mechanism. The calculated ZFS parameters of 1 and 2 in their optimized geometries are in qualitative agreement with experimental EPR results. The higher excited <span class="hlt">states</span> display less electron delocalization, but at the same time they possess unquenched first-order angular momentum. This leads to strong spin-orbit coupling and highly anisotropic <span class="hlt">energy</span> spectrum. The analysis of the excited <span class="hlt">states</span> presented here constitutes the first detailed study of the effects of spin-dependent delocalization in the presence of first order orbital angular momentum and the obtained results can be applied to other mixed valence lanthanide systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70022646','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70022646"><span>Arsenic in <span class="hlt">ground</span> water of the United <span class="hlt">States</span>: occurrence and geochemistry</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Welch, Alan H.; Westjohn, D.B.; Helsel, Dennis R.; Wanty, Richard B.</p> <p>2000-01-01</p> <p>Concentrations of naturally occurring arsenic in <span class="hlt">ground</span> water vary regionally due to a combination of climate and geology. Although slightly less than half of 30,000 arsenic analyses of <span class="hlt">ground</span> water in the United <span class="hlt">States</span> were 1 μg/L, about 10% exceeded 10 μg/L. At a broad regional scale, arsenic concentrations exceeding 10 μg/L appear to be more frequently observed in the western United <span class="hlt">States</span> than in the eastern half. Arsenic concentrations in <span class="hlt">ground</span> water of the Appalachian Highlands and the Atlantic Plain generally are very low ( 1 μg/L). Concentrations are somewhat greater in the Interior Plains and the Rocky Mountain System. Investigations of <span class="hlt">ground</span> water in New England, Michigan, Minnesota, South Dakota, Oklahoma, and Wisconsin within the last decade suggest that arsenic concentrations exceeding 10 μg/L are more widespread and common than previously recognized.Arsenic release from iron oxide appears to be the most common cause of widespread arsenic concentrations exceeding 10 μg/L in <span class="hlt">ground</span> water. This can occur in response to different geochemical conditions, including release of arsenic to <span class="hlt">ground</span> water through reaction of iron oxide with either natural or anthropogenic (i.e., petroleum products) organic carbon. Iron oxide also can release arsenic to alkaline <span class="hlt">ground</span> water, such as that found in some felsic volcanic rocks and alkaline aquifers of the western United <span class="hlt">States</span>. Sulfide minerals are both a source and sink for arsenic. Geothermal water and high evaporation rates also are associated with arsenic concentrations 10g/L in <span class="hlt">ground</span> and surface water, particularly in the west.Arsenic release from iron oxide appears to be the most common cause of widespread arsenic concentrations exceeding 10 µg/L a <span class="hlt">ground</span> water. This can occur in response to different geochemical conditions, including release of arsenic to <span class="hlt">ground</span> water through reaction of iron oxide with either natural or anthropogenic (i.e., petroleum products) organic carbon. Iron oxide also can</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> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1236683-valence-fluctuating-ground-state-plutonium','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1236683-valence-fluctuating-ground-state-plutonium"><span>The valence-fluctuating <span class="hlt">ground</span> <span class="hlt">state</span> of plutonium</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Janoschek, Marc; Das, Pinaki; Chakrabarti, Bismayan; ...</p> <p>2015-07-10</p> <p>A central issue in material science is to obtain understanding of the electronic correlations that control complex materials. Such electronic correlations frequently arise because of the competition of localized and itinerant electronic degrees of freedom. Although the respective limits of well-localized or entirely itinerant <span class="hlt">ground</span> <span class="hlt">states</span> are well understood, the intermediate regime that controls the functional properties of complex materials continues to challenge theoretical understanding. We have used neutron spectroscopy to investigate plutonium, which is a prototypical material at the brink between bonding and nonbonding configurations. In addition, our study reveals that the <span class="hlt">ground</span> <span class="hlt">state</span> of plutonium is governed bymore » valence fluctuations, that is, a quantum mechanical superposition of localized and itinerant electronic configurations as recently predicted by dynamical mean field theory. Our results not only resolve the long-standing controversy between experiment and theory on plutonium’s magnetism but also suggest an improved understanding of the effects of such electronic dichotomy in complex materials.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AIPA....8e5316L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AIPA....8e5316L"><span>Electrical-field-induced magnetic Skyrmion <span class="hlt">ground</span> <span class="hlt">state</span> in a two-dimensional chromium tri-iodide ferromagnetic monolayer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liu, Jie; Shi, Mengchao; Mo, Pinghui; Lu, Jiwu</p> <p>2018-05-01</p> <p>Using fully first-principles non-collinear self-consistent field density functional theory (DFT) calculations with relativistic spin-orbital coupling effects, we show that, by applying an out-of-plane electrical field on a free-standing two-dimensional chromium tri-iodide (CrI3) ferromagnetic monolayer, the Néel-type magnetic Skyrmion spin configurations become more energetically-favorable than the ferromagnetic spin configurations. It is revealed that the topologically-protected Skyrmion <span class="hlt">ground</span> <span class="hlt">state</span> is caused by the breaking of inversion symmetry, which induces the non-trivial Dzyaloshinskii-Moriya interaction (DMI) and the energetically-favorable spin-canting configuration. Combining the ferromagnetic and the magnetic Skyrmion <span class="hlt">ground</span> <span class="hlt">states</span>, it is shown that 4-level data can be stored in a single monolayer-based spintronic device, which is of practical interests to realize the next-generation <span class="hlt">energy</span>-efficient quaternary logic devices and multilevel memory devices.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/15004546','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/15004546"><span>The 75As(n,2n) Cross Sections into the 74As Isomer and <span class="hlt">Ground</span> <span class="hlt">State</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>Younes, W; Garrett, P E; Becker, J A</p> <p>2003-06-30</p> <p>The {sup 75}As(n, 2n) cross section for the population of the T{sub 1/2} = 26.8-ns isomer at E{sub x} = 259.3 keV in {sup 74}As has been measured as a function of incident neutron <span class="hlt">energy</span>, from threshold to E{sub n} = 20 MeV. The cross section was measured using the GEANIE spectrometer at LANSCE/WNR. For convenience, the {sup 75}As(n, 2n) population cross section for the {sup 74}As <span class="hlt">ground</span> <span class="hlt">state</span> has been deduced as the difference between the previously-known (n, 2n) reaction cross section and the newly measured {sup 75}As(n, 2n){sup 74}As{sup m} cross section. The (n, 2n) reaction, <span class="hlt">ground-state</span>, andmore » isomer population cross sections are tabulated in this paper.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JEMat.tmp.2579B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JEMat.tmp.2579B"><span><span class="hlt">Band</span>-Like Behavior of Localized <span class="hlt">States</span> of Metal Silicide Precipitate in Silicon</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bondarenko, Anton; Vyvenko, Oleg</p> <p>2018-03-01</p> <p>Deep-level transient spectroscopy (DLTS) investigations of <span class="hlt">energy</span> levels of charge-carrier traps associated with precipitates of metal silicide often show that they behave not like localized monoenergetic traps but as a continuous density of allowed <span class="hlt">states</span> in the bandgap with fast carrier exchange between these <span class="hlt">states</span>, so-called <span class="hlt">band</span>-like behavior. This kind of behavior was ascribed to the dislocation loop bounding the platelet, which in addition exhibits an attractive potential caused by long-range elastic strain. In previous works, the presence of the dislocation-related deformation potential in combination with the external electric field of the Schottky diode was included to obtain a reasonable fit of the proposed model to experimental data. Another well-known particular property of extended defects—the presence of their own strong electric field in their vicinity that is manifested in the logarithmic kinetics of electron capture—was not taken into account. We derive herein a theoretical model that takes into account both the external electric field and the intrinsic electric field of dislocation self-charge as well as its deformation potential, which leads to strong temporal variation of the activation <span class="hlt">energy</span> during charge-carrier emission. We performed numerical simulations of the DLTS spectra based on such a model for a monoenergetic trap, finding excellent agreement with available experimental 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_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('https://ntrs.nasa.gov/search.jsp?R=19830044457&hterms=Pepper&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3DPepper','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19830044457&hterms=Pepper&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3DPepper"><span>Diamond /111/ studied by electron <span class="hlt">energy</span> loss spectroscopy in the characteristic loss region</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Pepper, S. V.</p> <p>1982-01-01</p> <p>Unoccupied surface <span class="hlt">states</span> on diamond (111) annealed at greater than 900 C are studied by electron <span class="hlt">energy</span> loss spectroscopy with valence <span class="hlt">band</span> excitation. A feature found at 2.1 eV loss <span class="hlt">energy</span> is attributed to an excitation from occupied surface <span class="hlt">states</span> into unoccupied surface <span class="hlt">states</span> of <span class="hlt">energy</span> within the bulk <span class="hlt">band</span> gap. A surface <span class="hlt">band</span> gap of approximately 1 eV is estimated. This result supports a previous suggestion for unoccupied <span class="hlt">band</span> gap <span class="hlt">states</span> based on core level <span class="hlt">energy</span> loss spectroscopy. Using the valence <span class="hlt">band</span> excitation <span class="hlt">energy</span> loss spectrosocpy, it is also suggested that hydrogen is removed from the as-polished diamond surface by a Menzel-Gomer-Redhead mechanism.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014PhRvC..89d4610W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014PhRvC..89d4610W"><span><span class="hlt">Ground-state</span> properties of neutron-rich Mg isotopes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Watanabe, S.; Minomo, K.; Shimada, M.; Tagami, S.; Kimura, M.; Takechi, M.; Fukuda, M.; Nishimura, D.; Suzuki, T.; Matsumoto, T.; Shimizu, Y. R.; Yahiro, M.</p> <p>2014-04-01</p> <p>We analyze recently measured total reaction cross sections for 24-38Mg isotopes incident on 12C targets at 240 MeV/nucleon by using the folding model and antisymmetrized molecular dynamics (AMD). The folding model well reproduces the measured reaction cross sections, when the projectile densities are evaluated by the deformed Woods-Saxon (def-WS) model with AMD deformation. Matter radii of 24-38Mg are then deduced from the measured reaction cross sections by fine tuning the parameters of the def-WS model. The deduced matter radii are largely enhanced by nuclear deformation. Fully microscopic AMD calculations with no free parameter well reproduce the deduced matter radii for 24-36Mg, but still considerably underestimate them for 37,38Mg. The large matter radii suggest that 37,38Mg are candidates for deformed halo nucleus. AMD also reproduces other existing measured <span class="hlt">ground-state</span> properties (spin parity, total binding <span class="hlt">energy</span>, and one-neutron separation <span class="hlt">energy</span>) of Mg isotopes. Neutron-number (N) dependence of deformation parameter is predicted by AMD. Large deformation is seen from 31Mg with N =19 to a drip-line nucleus 40Mg with N =28, indicating that both the N =20 and 28 magicities disappear. N dependence of neutron skin thickness is also predicted by AMD.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003CoTPh..39..607Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003CoTPh..39..607Y"><span>A Rigorous Investigation on the <span class="hlt">Ground</span> <span class="hlt">State</span> of the Penson-Kolb Model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, Kai-Hua; Tian, Guang-Shan; Han, Ru-Qi</p> <p>2003-05-01</p> <p>By using either numerical calculations or analytical methods, such as the bosonization technique, the <span class="hlt">ground</span> <span class="hlt">state</span> of the Penson-Kolb model has been previously studied by several groups. Some physicists argued that, as far as the existence of superconductivity in this model is concerned, it is canonically equivalent to the negative-U Hubbard model. However, others did not agree. In the present paper, we shall investigate this model by an independent and rigorous approach. We show that the <span class="hlt">ground</span> <span class="hlt">state</span> of the Penson-Kolb model is nondegenerate and has a nonvanishing overlap with the <span class="hlt">ground</span> <span class="hlt">state</span> of the negative-U Hubbard model. Furthermore, we also show that the <span class="hlt">ground</span> <span class="hlt">states</span> of both the models have the same good quantum numbers and may have superconducting long-range order at the same momentum q = 0. Our results support the equivalence between these models. The project partially supported by the Special Funds for Major <span class="hlt">State</span> Basic Research Projects (G20000365) and National Natural Science Foundation of China under Grant No. 10174002</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMSA23A2376S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMSA23A2376S"><span>Emission coefficients for the OH Meinel <span class="hlt">band</span> system; calculations and nightglow comparisons</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Slanger, T. G.</p> <p>2016-12-01</p> <p>The OH Meinel <span class="hlt">band</span> system is an extensive series of <span class="hlt">bands</span> that are transitions between the vibrational levels of the X2Π <span class="hlt">ground-state</span> of the molecule. The exothermicity of the source reaction is sufficient to populate up to OH(v = 9), and in fact the nascent reaction puts most of the product into that level. Subsequently, relaxation of the population to lower levels takes place via collisions with the ambient atmosphere and radiation within the OH(v) manifold. Considerable effort has been spent in determining the emission coefficients of the OH Meinel <span class="hlt">band</span> system. This emission is a prominent feature of the terrestrial nightglow, and because it is relatively intense, there have been numerous investigations, generally based on <span class="hlt">ground</span>-based instrumentation. The very exothermic source reaction, H + O3 → OH(v) + O2, results in the production of vibrationally and rotationally hot OH(v), and leads to a great number of OH emission lines, covering a wide spectral range, 500-2000 nm. The full range of <span class="hlt">energy</span>-accessible OH vibrational levels, up to v = 9, is produced in the reaction, and in this presentation we make the case that it is essential to simultaneously measure as many OH <span class="hlt">bands</span> as possible, to retrieve the maximum amount of spectroscopic and dynamic information. In order to do so, we must agree on the emission coefficients (A-factors) associated with the individual OH <span class="hlt">bands</span>, and this determination has presented problems in the past. A major advance in the study of atmospheric OH Meinel <span class="hlt">band</span> emission took place when astronomical sky spectra were utilized to record all accessible OH <span class="hlt">bands</span> simultaneously, from Mauna Kea [Cosby and Slanger, 2007]. Subsequently, similar studies were undertaken at the VLT [Noll et al. 2015 a,b], and at the GIANO-TNG [Oliva et al., 2015]. With these intensity-calibrated spectra, it becomes possible to compare the OH optical data with sets of A-factor calculations that have been presented over the years [Mies, 1974; Turnbull and Lowe</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009JChPh.131v4321H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009JChPh.131v4321H"><span>A benchmark theoretical study of the electronic <span class="hlt">ground</span> <span class="hlt">state</span> and of the singlet-triplet split of benzene and linear acenes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hajgató, B.; Szieberth, D.; Geerlings, P.; De Proft, F.; Deleuze, M. S.</p> <p>2009-12-01</p> <p>A benchmark theoretical study of the electronic <span class="hlt">ground</span> <span class="hlt">state</span> and of the vertical and adiabatic singlet-triplet (ST) excitation <span class="hlt">energies</span> of benzene (n =1) and n-acenes (C4n+2H2n+4) ranging from naphthalene (n =2) to heptacene (n =7) is presented, on the <span class="hlt">ground</span> of single- and multireference calculations based on restricted or unrestricted zero-order wave functions. High-level and large scale treatments of electronic correlation in the <span class="hlt">ground</span> <span class="hlt">state</span> are found to be necessary for compensating giant but unphysical symmetry-breaking effects in unrestricted single-reference treatments. The composition of multiconfigurational wave functions, the topologies of natural orbitals in symmetry-unrestricted CASSCF calculations, the T1 diagnostics of coupled cluster theory, and further <span class="hlt">energy</span>-based criteria demonstrate that all investigated systems exhibit a A1g singlet closed-shell electronic <span class="hlt">ground</span> <span class="hlt">state</span>. Singlet-triplet (S0-T1) <span class="hlt">energy</span> gaps can therefore be very accurately determined by applying the principles of a focal point analysis onto the results of a series of single-point and symmetry-restricted calculations employing correlation consistent cc-pVXZ basis sets (X=D, T, Q, 5) and single-reference methods [HF, MP2, MP3, MP4SDQ, CCSD, CCSD(T)] of improving quality. According to our best estimates, which amount to a dual extrapolation of <span class="hlt">energy</span> differences to the level of coupled cluster theory including single, double, and perturbative estimates of connected triple excitations [CCSD(T)] in the limit of an asymptotically complete basis set (cc-pV∞Z), the S0-T1 vertical excitation <span class="hlt">energies</span> of benzene (n =1) and n-acenes (n =2-7) amount to 100.79, 76.28, 56.97, 40.69, 31.51, 22.96, and 18.16 kcal/mol, respectively. Values of 87.02, 62.87, 46.22, 32.23, 24.19, 16.79, and 12.56 kcal/mol are correspondingly obtained at the CCSD(T)/cc-pV∞Z level for the S0-T1 adiabatic excitation <span class="hlt">energies</span>, upon including B3LYP/cc-PVTZ corrections for zero-point vibrational <span class="hlt">energies</span>. In line with</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009APS..MARL35006I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009APS..MARL35006I"><span>An LDA+U study of the photoemission spectra of <span class="hlt">ground</span> <span class="hlt">state</span> phase of americium and curium</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Islam, Md; Ray, Asok</p> <p>2009-03-01</p> <p>We have investigated the photoemission spectra and other <span class="hlt">ground</span> <span class="hlt">state</span> properties such as equilibrium volume and bulk modulus of dhcp americium and the density of <span class="hlt">states</span> and magnetic properties of dhcp curium using LDA+U method. Our calculations show that spin polarized americium is energetically favorable but spin degenerate configuration produces experimental quantities much better than that calculated using spin polarized configuration. The DOS calculated using LDA+U with both non-magnetic and spin polarized configurations is compared and the non-magnetic DOS is shown to be in good agreement with experimental photoemission spectra when U=4.5 eV. In spin polarized case, U is observed to increase the splitting between occupied and unoccupied <span class="hlt">bands</span> by enhancing Stoner parameter. The results are shown to be in good agreement with that calculated using dynamical mean field theory for these two heavy actinides. For curium, exchange interaction appears to play the dominant role in its magnetic stability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25105648','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25105648"><span><span class="hlt">Ground-state</span> cooling of a carbon nanomechanical resonator by spin-polarized current.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Stadler, P; Belzig, W; Rastelli, G</p> <p>2014-07-25</p> <p>We study the nonequilibrium steady <span class="hlt">state</span> of a mechanical resonator in the quantum regime realized by a suspended carbon nanotube quantum dot in contact with two ferromagnets. Because of the spin-orbit interaction and/or an external magnetic field gradient, the spin on the dot couples directly to the flexural eigenmodes. Accordingly, the nanomechanical motion induces inelastic spin flips of the tunneling electrons. A spin-polarized current at finite bias voltage causes either heating or active cooling of the mechanical modes. We show that maximal cooling is achieved at resonant transport when the <span class="hlt">energy</span> splitting between two dot levels of opposite spin equals the vibrational frequency. Even for weak electron-resonator coupling and moderate polarizations we can achieve <span class="hlt">ground-state</span> cooling with a temperature of the leads, for instance, of T = 10 ω.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AIPA....7e5704H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AIPA....7e5704H"><span>The first-principles investigations on magnetic <span class="hlt">ground-state</span> in Sm-doped phenanthrene</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Han, Jia-Xing; Zhong, Guo-Hua; Wang, Xiao-Hui; Chen, Xiao-Jia; Lin, Hai-Qing</p> <p>2017-05-01</p> <p>Based on the density functional theory plus the effective Coulomb repulsion U, we have investigated the crystal structure, electronic properties and magnetic characteristics in Sm-doped phenanthrene, recently characterized as a superconductor with Tc˜5 -6 Kelvin. Calculated total <span class="hlt">energies</span> of different magnetic <span class="hlt">states</span> indicate that Sm-doped phenanthrene is stable at the ferromagnetic <span class="hlt">ground-state</span>. Considered the strong electronic correlations effect due to the intercalation of Sm-4f electrons, we found that the Sm-4f contributes to the Fermi surface together with C-2p, which is different from K-doped phenanthrene. Compared with alkali-metal-doped phenanthrene, Sm atom has larger local magnetic moment, which suppresses the superconductivity in conventional superconductors. Our results indicate that the electron-electron correlations play an important role in superconductivity of Sm-doped phenanthrene.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22421987','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22421987"><span>Nanoscale charge distribution and <span class="hlt">energy</span> <span class="hlt">band</span> modification in defect-patterned graphene.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Shengnan; Wang, Rui; Wang, Xiaowei; Zhang, Dongdong; Qiu, Xiaohui</p> <p>2012-04-21</p> <p>Defects were introduced precisely to exfoliated graphene (G) sheets on a SiO(2)/n(+) Si substrate to modulate the local <span class="hlt">energy</span> <span class="hlt">band</span> structure and the electron pathway using solution-phase oxidation followed by thermal reduction. The resulting nanoscale charge distribution and <span class="hlt">band</span> 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 <span class="hlt">energy</span> 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.</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/2005PhRvB..71e4501N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005PhRvB..71e4501N"><span>Properties of the superconducting <span class="hlt">state</span> in a two-<span class="hlt">band</span> model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nicol, E. J.; Carbotte, J. P.</p> <p>2005-02-01</p> <p>Eliashberg theory is used to investigate the range of thermodynamic properties possible within a two-<span class="hlt">band</span> model for s -wave superconductivity and to identify signatures of its two-<span class="hlt">band</span> nature. We emphasize dimensionless BCS ratios [those for the <span class="hlt">energy</span> gaps, the specific heat jump, and the negative of its slope near Tc , the thermodynamic critical field Hc(0) , and the normalized slopes of the critical field and the penetration depth near Tc ], which are no longer universal even in weak coupling. We also give results for temperature-dependent quantities, such as the penetration depth and the <span class="hlt">energy</span> gap. Results are presented both for microscopic parameters appropriate to MgB2 and for variations away from these. Strong coupling corrections are identified and found to be significant. Analytic formulas are provided that show the role played by the anisotropy in coupling in some special limits. Particular emphasis is placed on small interband coupling and on the opposite limit of no diagonal coupling. The effect of impurity scattering is considered, particularly for the interband case.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22591250-flat-electronic-bands-fractal-kagome-network-effect-perturbation','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22591250-flat-electronic-bands-fractal-kagome-network-effect-perturbation"><span>Flat electronic <span class="hlt">bands</span> in fractal-kagomé network and the effect of perturbation</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>Nandy, Atanu, E-mail: atanunandy1989@gmail.com; Chakrabarti, Arunava, E-mail: arunava-chakrabarti@yahoo.co.in</p> <p>2016-05-06</p> <p>We demonstrate an analytical prescription of demonstrating the flat <span class="hlt">band</span> [FB] <span class="hlt">states</span> 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 <span class="hlt">energy</span> 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 <span class="hlt">energy</span> eigenvalue for which one can havemore » dispersionless flat electronic <span class="hlt">bands</span>. 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 <span class="hlt">states</span> and to generate absolutely continuous sub-<span class="hlt">bands</span> in the <span class="hlt">energy</span> spectrum and again an interesting re-entrant behavior of those FB <span class="hlt">states</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvA..97a2115H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvA..97a2115H"><span>Symmetry-breaking dynamics of the finite-size Lipkin-Meshkov-Glick model near <span class="hlt">ground</span> <span class="hlt">state</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huang, Yi; Li, Tongcang; Yin, Zhang-qi</p> <p>2018-01-01</p> <p>We study the dynamics of the Lipkin-Meshkov-Glick (LMG) model with a finite number of spins. In the thermodynamic limit, the <span class="hlt">ground</span> <span class="hlt">state</span> of the LMG model with an isotropic Hamiltonian in the broken phase breaks to a mean-field <span class="hlt">ground</span> <span class="hlt">state</span> with a certain direction. However, when the spin number N is finite, the exact <span class="hlt">ground</span> <span class="hlt">state</span> is always unique and is not given by a classical mean-field <span class="hlt">ground</span> <span class="hlt">state</span>. Here, we prove that when N is large but finite, through a tiny external perturbation, a localized <span class="hlt">state</span> which is close to a mean-field <span class="hlt">ground</span> <span class="hlt">state</span> can be prepared, which mimics spontaneous symmetry breaking. Also, we find the localized in-plane spin polarization oscillates with two different frequencies ˜O (1 /N ) , and the lifetime of the localized <span class="hlt">state</span> is long enough to exhibit this oscillation. We numerically test the analytical results and find that they agree very well with each other. Finally, we link the phenomena to quantum time crystals and time quasicrystals.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JMoSp.349...64L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JMoSp.349...64L"><span>Analysis of the A ∼ - X ∼ <span class="hlt">bands</span> of the ethynyl radical near 1.48 μ m and re-evaluation of X ∼ <span class="hlt">state</span> <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>Le, A. T.; Gross, Eisen C.; Hall, Gregory E.; Sears, Trevor J.</p> <p>2018-07-01</p> <p>We report the observation and analysis of spectra in part of the near-infrared spectrum of C2H, originating in rotational levels in the <span class="hlt">ground</span> and lowest two excited bending vibrational levels of the <span class="hlt">ground</span> X ˜ 2Σ+ <span class="hlt">state</span>. In the analysis, we have combined present and previously reported high resolution spectroscopic data for the lower levels involved in the transitions to determine significantly improved molecular constants to describe the fine and hyperfine split rotational levels of the radical in the zero point, v2 = 1 and the 2Σ+ component of v2 = 2 . Two of the upper <span class="hlt">state</span> vibronic levels involved had not been observed previously. The data and analysis indicate the electronic wavefunction character changes with bending vibrational excitation in the <span class="hlt">ground</span> <span class="hlt">state</span> and provide avenues for future measurements of reactivity of the radical as a function of vibrational excitation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009JChPh.130j4301L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009JChPh.130j4301L"><span>Characterization of the HSiN HNSi system in its electronic <span class="hlt">ground</span> <span class="hlt">state</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lind, Maria C.; Pickard, Frank C.; Ingels, Justin B.; Paul, Ankan; Yamaguchi, Yukio; Schaefer, Henry F.</p> <p>2009-03-01</p> <p>The electronic <span class="hlt">ground</span> <span class="hlt">states</span> (X˜Σ+1) of HSiN, HNSi, and the transition <span class="hlt">state</span> connecting the two isomers were systematically studied using configuration interaction with single and double (CISD) excitations, coupled cluster with single and double (CCSD) excitations, CCSD with perturbative triple corrections [CCSD(T)], multireference complete active space self-consistent field (CASSCF), and internally contracted multireference configuration interaction (ICMRCI) methods. The correlation-consistent polarized valence (cc-pVXZ), augmented correlation-consistent polarized valence (aug-cc-pVXZ) (X=T,Q,5), correlation-consistent polarized core-valence (cc-pCVYZ), and augmented correlation-consistent polarized core-valence (aug-cc-pCVYZ) (Y=T,Q) basis sets were used. Via focal point analyses, we confirmed the HNSi isomer as the global minimum on the <span class="hlt">ground</span> <span class="hlt">state</span> HSiN HNSi zero-point vibrational <span class="hlt">energy</span> corrected surface and is predicted to lie 64.7kcalmol-1 (22640cm-1, 2.81eV) below the HSiN isomer. The barrier height for the forward isomerization reaction (HSiN→HNSi) is predicted to be 9.7kcalmol-1, while the barrier height for the reverse process (HNSi→HSiN) is determined to be 74.4kcalmol-1. The dipole moments of the HSiN and HNSi isomers are predicted to be 4.36 and 0.26D, respectively. The theoretical vibrational isotopic shifts for the HSiN/DSiN and HNSi/DNSi isotopomers are in strong agreement with the available experimental values. The dissociation <span class="hlt">energy</span> for HSiN [HSiN(X˜Σ+1)→H(S2)+SiN(XΣ+2)] is predicted to be D0=59.6kcalmol-1, whereas the dissociation <span class="hlt">energy</span> for HNSi [HNSi(X˜Σ+1)→H(S2)+NSi(XΣ+2)] is predicted to be D0=125.0kcalmol-1 at the CCSD(T)/aug-cc-pCVQZ level of theory. Anharmonic vibrational frequencies computed using second order vibrational perturbation theory are in good agreement with available matrix isolation experimental data for both HSiN and HNSi isomers root mean squared derivation (RMSD=9cm-1).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015aris.confb0024W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015aris.confb0024W"><span><span class="hlt">Ground-State</span> Properties of Mg Isotopes in and Beyond the Island of Inversion through Reaction Cross Sections</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Watanabe, Shin; Minomo, Kosho; Shimada, Mitsuhiro; Tagami, Shingo; Kimura, Masaaki; Takechi, Maya; Fukuda, Mitsunori; Nishimura, Daiki; Suzuki, Takeshi; Matsumoto, Takuma; Shimizu, Yoshifumi R.; Yahiro, Masanobu</p> <p></p> <p>We analyze recently measured total reaction cross sections (σR) for 24-38Mg incident on 12C targets at 240 MeV/nucleon by using the microscopic framework based on the double folding model and antisymmetrized molecular dynamics (AMD). The framework reproduces not only the measured σR but also other existing measured <span class="hlt">ground-state</span> properties of Mg Isotopes (spin parity, total binding <span class="hlt">energy</span>, one-neutron separation <span class="hlt">energy</span>, and 2+ and 4+ excitation <span class="hlt">energies</span>) quite well. AMD predicts large deformation from 31Mg19 to a drip-line nucleus 40Mg28, indicating that both the N = 20 and 28 magicities disappear.</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 electronic 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 <span class="hlt">states</span> and Sr 4d <span class="hlt">states</span> 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 <span class="hlt">states</span>, while the upper VB mainlymore » consists of O 2p <span class="hlt">states</span>. 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: • Electronic 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.osti.gov/pages/biblio/1340509-measurement-high-energy-neutron-flux-above-ground-utilizing-spallation-based-multiplicity-technique','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1340509-measurement-high-energy-neutron-flux-above-ground-utilizing-spallation-based-multiplicity-technique"><span>Measurement of high-<span class="hlt">energy</span> neutron flux above <span class="hlt">ground</span> utilizing a spallation based multiplicity technique</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Roecker, Caleb; Bernstein, Adam; Marleau, Peter; ...</p> <p>2016-11-14</p> <p>Cosmogenic high-<span class="hlt">energy</span> neutrons are a ubiquitous, difficult to shield, poorly measured background. Above <span class="hlt">ground</span> the high-<span class="hlt">energy</span> neutron <span class="hlt">energy</span>-dependent flux has been measured, with significantly varying results. Below <span class="hlt">ground</span>, high-<span class="hlt">energy</span> neutron fluxes are largely unmeasured. Here we present a reconstruction algorithm to unfold the incident neutron <span class="hlt">energy</span>-dependent flux measured using the Multiplicity and Recoil Spectrometer (MARS), simulated test cases to verify the algorithm, and provide a new measurement of the above <span class="hlt">ground</span> high-<span class="hlt">energy</span> neutron <span class="hlt">energy</span>-dependent flux with a detailed systematic uncertainty analysis. Uncertainty estimates are provided based upon the measurement statistics, the incident angular distribution, the surrounding environment of the Montemore » Carlo model, and the MARS triggering efficiency. Quantified systematic uncertainty is dominated by the assumed incident neutron angular distribution and surrounding environment of the Monte Carlo model. The <span class="hlt">energy</span>-dependent neutron flux between 90 MeV and 400 MeV is reported. Between 90 MeV and 250 MeV the MARS results are comparable to previous Bonner sphere measurements. Over the total <span class="hlt">energy</span> regime measured, the MARS result are located within the span of previous measurements. Lastly, these results demonstrate the feasibility of future below <span class="hlt">ground</span> measurements with MARS.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1340509','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1340509"><span>Measurement of high-<span class="hlt">energy</span> neutron flux above <span class="hlt">ground</span> utilizing a spallation based multiplicity technique</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>Roecker, Caleb; Bernstein, Adam; Marleau, Peter</p> <p></p> <p>Cosmogenic high-<span class="hlt">energy</span> neutrons are a ubiquitous, difficult to shield, poorly measured background. Above <span class="hlt">ground</span> the high-<span class="hlt">energy</span> neutron <span class="hlt">energy</span>-dependent flux has been measured, with significantly varying results. Below <span class="hlt">ground</span>, high-<span class="hlt">energy</span> neutron fluxes are largely unmeasured. Here we present a reconstruction algorithm to unfold the incident neutron <span class="hlt">energy</span>-dependent flux measured using the Multiplicity and Recoil Spectrometer (MARS), simulated test cases to verify the algorithm, and provide a new measurement of the above <span class="hlt">ground</span> high-<span class="hlt">energy</span> neutron <span class="hlt">energy</span>-dependent flux with a detailed systematic uncertainty analysis. Uncertainty estimates are provided based upon the measurement statistics, the incident angular distribution, the surrounding environment of the Montemore » Carlo model, and the MARS triggering efficiency. Quantified systematic uncertainty is dominated by the assumed incident neutron angular distribution and surrounding environment of the Monte Carlo model. The <span class="hlt">energy</span>-dependent neutron flux between 90 MeV and 400 MeV is reported. Between 90 MeV and 250 MeV the MARS results are comparable to previous Bonner sphere measurements. Over the total <span class="hlt">energy</span> regime measured, the MARS result are located within the span of previous measurements. Lastly, these results demonstrate the feasibility of future below <span class="hlt">ground</span> measurements with MARS.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JChPh.148t4301P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JChPh.148t4301P"><span>Influence of the aggregate <span class="hlt">state</span> on <span class="hlt">band</span> structure and optical properties of C60 computed with different methods</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pal, Amrita; Arabnejad, Saeid; Yamashita, Koichi; Manzhos, Sergei</p> <p>2018-05-01</p> <p>C60 and C60 based molecules are efficient acceptors and electron transport layers for planar perovskite solar cells. While properties of these molecules are well studied by ab initio methods, those of solid C60, specifically its optical absorption properties, are not. We present a combined density functional theory-Density Functional Tight Binding (DFTB) study of the effect of solid <span class="hlt">state</span> packing on the <span class="hlt">band</span> structure and optical absorption of C60. The valence and conduction <span class="hlt">band</span> edge <span class="hlt">energies</span> of solid C60 differ on the order of 0.1 eV from single molecule frontier orbital <span class="hlt">energies</span>. We show that calculations of optical properties using linear response time dependent-DFT(B) or the imaginary part of the dielectric constant (dipole approximation) can result in unrealistically large redshifts in the presence of intermolecular interactions compared to available experimental data. We show that optical spectra computed from the frequency-dependent real polarizability can better reproduce the effect of C60 aggregation on optical absorption, specifically with a generalized gradient approximation functional, and may be more suited to study effects of molecular aggregation.</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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