Volume 241, Issue5 (April 2004)
Articles in the Current Issue:
Cover Picture
Horizontal line nodes in superconducting Sr2RuO4
NASA Astrophysics Data System (ADS)
Litak, G.; Annett, J. F.; Györffy, B. L.; Wysokiski, K. I.
2004-04-01
Superconductivity in Sr2RuO4 is one of the most interesting phenomena in current condensed matter physics, since it is revealed to be a triplet-pairing state. Our Editor's Choice [1] considers an important problem related to the type of order parameter in this material.The position of line nodes on the Fermi surface, as evident from recent measurements, has been determined for various scenarios shown in the cover picture. Using these models, the temperature dependence of heat capacity and penetration depth has been calculated for easy comparison with experiments.The first author, Grzegorz Litak, is assistant professor at Technical University of Lublin and visiting scientist at the Max Planck Institute in Dresden. He is working on the effect of disorder on correlated and exotic superconductors, nonlinear dynamics, and superconductivity in strontium ruthenate.
The Front-End System For MARE In Milano
NASA Astrophysics Data System (ADS)
Arnaboldi, Claudio; Pessina, Gianluigi
2009-12-01
The first phase of MARE consists of 72 μ-bolometers composed each of a crystal of AgReO4 readout by Si thermistors. The spread in the thermistor characteristics and bolometer thermal coupling leads to different energy conversion gains and optimum operating points of the detectors. Detector biasing levels and voltage gains are completely remote-adjustable by the front end system developed, the subject of this paper, achieving the same signal range at the input of the DAQ system. The front end consists of a cold buffer stage, a second pseudo differential stage followed by a gain stage, an antialiasing filter, and a battery powered detector biasing set up. The DAQ system can be used to set all necessary parameters of the electronics remotely, by writing to a μ-controller located on each board. Fiber optics are used for the serial communication between the DAQ and the front end. To suppress interference noise during normal operation, the clocked devices of the front end are maintained in sleep-mode, except during the set-up phase of the experiment. An automatic DC detector characterization procedure is used to establish the optimum operating point of every detector of the array. A very low noise level has been achieved: about 3nV/□Hz at 1 Hz and 1 nV/□Hz for the white component, high frequencies.
Mapping TES Aerobreaking Data of The Martian Polar Caps
NASA Astrophysics Data System (ADS)
Altunaiji, E. S.; Edwards, C. S.; Smith, M. D.; AlShamsi, M. R.; AlJanaahi, A. A.
2016-12-01
The purpose of this paper is to create maps of the north and south Mars polar caps using Thermal Emission Spectrometer (TES) aerobreaking surface temperature data in south and north as well as Lambert albedo data in the south. TES is an instrument on board the Mars Global Surveyor (MGS) spacecraft. It has six detectors arranged in a 2x3 array with a nominal spot size of 3 × 6 km; however, given the elliptical nature of the orbit during aerobreaking the footprint can be significantly larger (10s of km), especially over the southern hemisphere. TES is a Fourier transform infrared spectrometer designed to study the Martian surface and atmosphere using thermal infrared emission spectroscopy. It is composed of 2 separate channels, a broadband visible/near-infrared bolometer and hyperspectral thermal infrared spectrometer with a broadband thermal infrared bolometer. TES aerobraking spectra were taken between Mars Year 23, Ls=180° and Mars Year 24, Ls=30°. To determine the footprint location on the surface, geometry is calculated using the Spacecraft Planet Instrument Camera Matrix and Event (SPICE) Toolkit. These data were then binned and mapped to surface in polar stereographic projection. While some early studies focused on these data, we have expanded upon the ranges, generated time-/seasonally-binned data, and re-examined this largely underutilized set of data from TES ultimately extending the record of polar science on Mars.
The LUCIFER Project: Achievements and Near Future Prospects
NASA Astrophysics Data System (ADS)
Beeman, J. W.; Bellini, F.; Benetti, P.; Cardani, L.; Casali, N.; Chiesa, D.; Clemenza, M.; Dafinei, I.; Di Domizio, S.; Ferroni, F.; Gironi, L.; Giuliani, A.; Gotti, C.; Maino, M.; Nagorny, S. S.; Nisi, S.; Nones, C.; Pagnanini, L.; Pattavina, L.; Pessina, G.; Piperno, G.; Pirro, S.; Previtali, E.; Rusconi, C.; Schäffner, K.; Tomei, C.; Vignati, M.
2016-08-01
In the view of exploring the inverted hierarchy region future experiments investigating the neutrinoless double beta decay have to demand for detectors with excellent energy resolution and zero background in the energy region of interest. Cryogenic scintillating bolometers are very suitable detectors for this task since they provide particle discrimination: the simultaneous detection of the phonon and light signal allows us to identify the interacting type of particle and thus guarantees a suppression of α -induced backgrounds, the key-issue for next-generation tonne-scale bolometric experiments. The LUCIFER project aims at running the first array of enriched scintillating Zn^{ {82}}Se bolometers (total mass of about 8kg of ^{ {82}}Se) with a background level as low as 10^{ {-3}} counts/(keV kg y) in the energy region of interest. The main effort is currently focused on the finalization of the crystal growth procedure in order to achieve high quality Zn^{ {82}}Se crystals both in terms of radiopurity and bolometric properties. We present results from tests of such crystals operated at mK temperatures which demonstrate the excellent background rejection capabilities of this detection approach towards a background-free demonstrator experiment. Besides, the high purity of the enriched ^{ {82}}Se material allows us to establish the most stringent limits on the half-life of the double beta decay of ^{ {82}}Se on excited levels.
NASA Astrophysics Data System (ADS)
Ward, Jonathan; Advanced ACT Collaboration, NASA Space Technology Research Fellowship
2017-06-01
The Atacama Cosmology Telescope is a six-meter diameter telescope located at 17,000 feet (5,200 meters) on Cerro Toco in the Andes Mountains of northern Chile. The next generation Advanced ACT (AdvACT) experiment is currently underway and will consist of three multichroic TES bolometer arrays operating together, totaling 5800 detectors on the sky. Each array will be sensitive to two frequency bands: a high frequency (HF) array at 150 and 230 GHz, two middle frequency (MF) arrays at 90 and 150 GHz, and a low frequency (LF) array at 28 and 41 GHz. The AdACT detector arrays will feature a revamped design when compared to ACTPol, including a transition to 150mm wafers equipped with multichroic pixels, allowing for a more densely packed focal plane. Each set of detectors consists of a feedhorn array of stacked silicon wafers which form a corrugated profile leading to each pixel. This is then followed by a four-piece detector stack assembly of silicon wafers which includes a waveguide interface plate, detector wafer, backshort cavity plate, and backshort cap. Each array is housed in a custom designed structure manufactured out of gold-plated, high purity copper. In addition to the detector array assembly, the array package also encloses the majority of our readout electronics. We present the full mechanical design of the AdvACT HF and MF detector array packages along with a detailed look at the detector array assemblies. We also highlight the use of continuously rotating warm half-wave plates (HWPs) at the front of the AdvACT receiver. We review the design of the rotation system and also early pipeline data analysis results. This experiment will also make use of extensive hardware and software previously developed for ACT, which will be modified to incorporate the new AdvACT instruments. Therefore, we discuss the integration of all AdvACT instruments with pre-existing ACTPol infrastructure.
The Green Bank Telescope: Transformational Science for the Next Decade.
NASA Astrophysics Data System (ADS)
Wootten, Al; GBO Staff
2018-01-01
The Robert C Byrd Green Bank Telescope has met its design goal of providing high-quality observations at 115 GHz. The accurate small beam of the telescope at high frequencies is leveraged by deployment of multi beam receivers. An overview is presented. Observers now have access to the new, 16-pixel, 3-mm Argus receiver, which is providing high-dynamic range images over wide fields for the multitude of spectral lines between 85 and 115 GHz. The successful performance of Argus, and its modular design, demonstrates that receivers with many more pixels could be built for the GBT. A 12 x 12 array of the Argus design would have mapping speeds about nine times faster than Argus without suffering any degradation in performance for the outer pixels in the array. The Observatory plans to build the next-generation Argus instrument (Argus+) with 144-pixels, a footprint 5'x5', and 7" resolution at 110 GHz. The project will be a collaboration between the Green Bank Observatory and university groups, who will supply key components. The key science drivers for Argus+ are studies of molecular filaments in the Milky Way, studies of molecular clouds in nearby galaxies, and the observations of rapidly evolving solar system objects. Observers also have access to MUSTANG-2, a 223-feedhorn bolometer camera which was commissioned on the GBT in spring 2016, and was offered for observations on a shared risk basis, in collaboration with the instrument team, in the 2018A GBO proposal call. Several features distinguish it from its predecessor, MUSTANG: A new, microstrip-coupled detector design yields higher sensitivity and less susceptibility to environmental microphonics. Detectors are feedhorn coupled, with the sum of two linear polarizations measured by a single TES per feed. The instantaneous field of view is 4 arcminutes (vs 42 arcseconds for MUSTANG) The receiver design incorporates a tilted refrigerator and receiver rotator, resulting in much lower dependence of cooling performance on telescope elevation. The detector readout is the first astronomical use of microwave resonators to multiplex TES bolometers. MUSTANG-2 has been developed by a collaboration including the University of Pennsylvania, NIST, NRAO, the University of Michigan, and Cardiff University. A 7-pixel K-band Feed Array covering 18-28 GHz with Dual polarization feeds and a noise temperature < 40-50 K has been available for several years. The array offers an instantaneous bandwidth/beam of 1.8 GHz. Future upgrade concepts under study envision increasing the number of beams by an order of magnitude.
NASA Astrophysics Data System (ADS)
Foley, C. P.
2007-11-01
The main theme at ISEC 2007 for superconducting materials, fabrication and analogue electronics was the description of incremental developments, including a few new directions that indicate breakthroughs in this area of research. The work on applications focused on their cost-benefit analysis (in order to improve their appeal), the development of simpler systems, making more of the data collected, improving packaging and being responsive to the power handling requirements for commercial systems. All papers presenting this level of research highlighted the importance of obtaining all the necessary details in order to investigate analogue devices and the effectiveness and commercial viability of their systems. This stage of development is important if we are to achieve the transition of superconducting electronics from the laboratory to commercial use. There were some exciting disruptive breakthroughs reported. These were in the areas of nano-SQUIDs, rotating gradiometers, superconducting scanning tunnelling microscopy (Hayashi et al) and the potential of superconducting photonics using optical interfaces with superconducting vortex flow transistors, for example. The materials research in low (LTS), high (HTS) and medium (MTS) critical temperature superconductors was reported. In LTS, nitrides emerged as important materials for use as new tunnel barriers, either insulating or semiconducting. Papers on BaN, NbN, TaN, GaN and Nb-Si superconducting materials were also presented. The MTS material of MgB2 is still under development (Zhao et al). There were also new research groups from South Africa and Turkey attending the conference. The fabrication research presented covered the areas of critical current Ic spread, which is still an issue in reducing the reproducibility of Josephson junctions, a 150 mm process for Nb/Al-AlOx/Nb and methods to improve barrier layers using both new materials and smooth surfaces at thin film interfaces (Du et al). New methods to make sub-micron Josephson junctions using laser etching (Büttner et al) and the development of passivation layers using amorphous YBCO and SiO2 (Seidel et al) were also presented. Characterization methods using Raman and photo-emission spectroscopy (Kikunaga et al) emerged as fresh approaches. Josephson junction (JJ) research covered the areas of critical current fluctuations where results on Tl-based junctions suggested a 40 times lower δI/Ic, and LTS junctions for voltage standards using a Nb-Si barrier for improved SNS junctions (Kieler et al). Development of MTS junctions based on MgB2 are yet to be realized with the interface barrier appearing to be the limiting factor. HTS Josephson junctions were reviewed by asking the question: `Are all HTS JJs the same?' with a clear `no' as the answer. Research on intrinsic stacked junctions, sub-micron junctions, the manipulation of electronic band structure to increase energy gap and mid-gap states was also presented. Developments in packaging and cooling were not as dominant at this conference as in previous years. However, there was research reported on the importance of non-magnetic structures in packaging, the design of magnetic shielding improvement by using finite element analysis to optimize design (Tanaka et al) and the use of cryocoolers (Vernik et al). SQUID research reported some breakthrough developments with new ideas presented on nano-SQUIDs with the possible detection of a ferritin spin-flip, a successful airborne trial using a rotating gradiometer and the development of a new 4 cm long baseline planar gradiometer, achieving a sensitivity of 35 fT cm-1 Hz-½. Applications in non-destructive evaluation (NDE) covered the use of SQUIDs in the detection of stainless steel foreign objects in food, defects in wire and circuit boards and surface imaging with most developments focusing on potential customer requirements. Biomagnetic applications have continued to be embraced in the use of SQUIDs in MRI (Zotev et al), NMR, MEG (including one paper that did not use SQUIDs), immunoassays (close to single cell detection—30 cells to date) and in spinal cord injury detection using quadrapoles. Instrumentation using various devices for thermometers (fast response), micro-susceptometers, current comparators and spin-flip measurements were reported. There were few papers on the use of SQUIDs for geophysical prospecting. This area of application is now commercially mature with research in the field being presented at mineral exploration conferences. However, one paper reported the development of an HTS transient electromagnetic (TEM) system with similar sensitivities to those demonstrated by LTS systems due to improved electronics. The application of nuclear quadrupole resonance for explosives using gate arrays for noise reduction was also reported. There were some novel devices presented with an excellent overview on SQUIFs which were first suggested by Richard Feynman in his well-known university lecture series in physics. This work continues with the aim of achieving the measurement of the absolute value (or true field) of magnetic fields with the question being asked: `Can you really create a zero magnetic field environment?'. Detector research presented at the conference considered the exciting applications in THz imaging. Superconducting bolometers with anti-reflection coatings and using MgB2 (Portesi et al) were reported suggesting improved performance. The application for the improvedr discrimination of radioactive materials by spectroscopy will be very important in the implementation of the Nuclear Non-proliferation Treaty. Single-photon detectors were reported using Nb nanowires (NbN), ferromagnets in nanolayers and SiN transition edge absorbers. Resonators based on SQUID arrays (He et al) and frequency adjustable Josephson junctions were also reported, along with receivers for radio astronomy. Filters have been found to be improved using MgB2, which showed increased Q factors using a split-ring element design (68000 at 5 GHz). This author also used the summing-up session to talk about the need for cooperation leading up to the setting of international standards for superconducting devices. For instance, in the standardization of connections to coolers to enable black box operation, in order to achieve the long-term vision that one day anyone could source a superconducting component from a standard electronics catalogue! Finally, some general comments on the conference. There were not many students (or females) as attendees, which suggests we need to consider more closely the future generation to take the current research to fruition. Nevertheless there was a clear movement forward with some exciting new developments and some new research groups participating, but some important superconducting electronics research groups did not attend. This calls into question the status of the funding of research into superconducting electronics. However, some clear applications, where superconducting electronics provides the only solution, are clearly achieving maturity in their development and adoption. Our research community needs to make sure these developments are recognized to ensure a healthy future for superconducting electronics research, development and commercialization.
Physical implementation of protected qubits
NASA Astrophysics Data System (ADS)
Douçot, B.; Ioffe, L. B.
2012-07-01
We review the general notion of topological protection of quantum states in spin models and its relation with the ideas of quantum error correction. We show that topological protection can be viewed as a Hamiltonian realization of error correction: for a quantum code for which the minimal number of errors that remain undetected is N, the corresponding Hamiltonian model of the effects of the environment noise appears only in the Nth order of the perturbation theory. We discuss the simplest model Hamiltonians that realize topological protection and their implementation in superconducting arrays. We focus on two dual realizations: in one the protected state is stored in the parity of the Cooper pair number, in the other, in the parity of the flux number. In both cases the superconducting arrays allow a number of fault-tolerant operations that should make the universal quantum computation possible.