<?xml version="1.0" encoding="UTF-8"?><xml><records><record><source-app name="Biblio" version="7.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">M. Xu</style></author><author><style face="normal" font="default" size="100%">D. George</style></author><author><style face="normal" font="default" size="100%">R. Jimenez</style></author><author><style face="normal" font="default" size="100%">A. Markelz</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Photo-Switching of Protein Dynamical Collectivity</style></title><secondary-title><style face="normal" font="default" size="100%">Photonics</style></secondary-title></titles><dates><year><style  face="normal" font="default" size="100%">2021</style></year></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://www.mdpi.com/2304-6732/8/8/302</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">8</style></volume><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">&lt;p class=&quot;rtejustify&quot;&gt;We examine changes in the picosecond structural dynamics with irreversible photobleaching of red fluorescent proteins (RFP) mCherry, mOrange2 and TagRFP-T. Measurements of the protein dynamical transition using terahertz time-domain spectroscopy show in all cases an increase in the turn-on temperature in the bleached state. The result is surprising given that there is little change in the protein surface, and thus, the solvent dynamics held responsible for the transition should not change. A spectral analysis of the measurements guided by quasiharmonic calculations of the protein absorbance reveals that indeed the solvent dynamical turn-on temperature is independent of the thermal stability/photostate however the protein dynamical turn-on temperature shifts to higher temperatures. This is the first demonstration of switching the protein dynamical turn-on temperature with protein functional state. The observed shift in protein dynamical turn-on temperature relative to the solvent indicates an increase in the required mobile waters necessary for the protein picosecond motions, that is, these motions are more collective. Melting-point measurements reveal that the photobleached state is more thermally stable, and structural analysis of related RFP’s shows that there is an increase in internal water channels as well as a more uniform atomic root mean squared displacement. These observations are consistent with previous suggestions that water channels form with extended light excitation providing O&lt;sub&gt;2 &lt;/sub&gt;access to the chromophore and subsequent fluorescence loss. We report that these same channels increase internal coupling enhancing thermal stability and collectivity of the picosecond protein motions. The terahertz spectroscopic characterization of the protein and solvent dynamical onsets can be applied generally to measure changes in collectivity of protein motions.&lt;/p&gt;
</style></abstract><section><style face="normal" font="default" size="100%">302</style></section></record><record><source-app name="Biblio" version="7.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Xu, M.</style></author><author><style face="normal" font="default" size="100%">George, D. K.</style></author><author><style face="normal" font="default" size="100%">Jimenez, R.</style></author><author><style face="normal" font="default" size="100%">Markelz, A. G.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Photo Switching of Protein Dynamical Collectivity</style></title><secondary-title><style face="normal" font="default" size="100%">arXiv:1906.00893</style></secondary-title></titles><dates><year><style  face="normal" font="default" size="100%">2019</style></year></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://arxiv.org/abs/1906.00893</style></url></web-urls></urls><language><style face="normal" font="default" size="100%">eng</style></language></record><record><source-app name="Biblio" version="7.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Dhillon, S. S.</style></author><author><style face="normal" font="default" size="100%">Vitiello, M. S.</style></author><author><style face="normal" font="default" size="100%">Linfield, E. H.</style></author><author><style face="normal" font="default" size="100%">Davies, A. G.</style></author><author><style face="normal" font="default" size="100%">Hoffmann, M. C.</style></author><author><style face="normal" font="default" size="100%">Booske, J.</style></author><author><style face="normal" font="default" size="100%">Paoloni, C.</style></author><author><style face="normal" font="default" size="100%">Gensch, M.</style></author><author><style face="normal" font="default" size="100%">Weightman, P.</style></author><author><style face="normal" font="default" size="100%">Williams, G. P.</style></author><author><style face="normal" font="default" size="100%">Castro-Camus, E.</style></author><author><style face="normal" font="default" size="100%">Cumming, D. R. S.</style></author><author><style face="normal" font="default" size="100%">Simoens, F.</style></author><author><style face="normal" font="default" size="100%">Escorcia-Carranza, I.</style></author><author><style face="normal" font="default" size="100%">Grant, J.</style></author><author><style face="normal" font="default" size="100%">Lucyszyn, S.</style></author><author><style face="normal" font="default" size="100%">Kuwata-Gonokami, M.</style></author><author><style face="normal" font="default" size="100%">Konishi, K.</style></author><author><style face="normal" font="default" size="100%">Koch, M.</style></author><author><style face="normal" font="default" size="100%">Schmuttenmaer, C. A.</style></author><author><style face="normal" font="default" size="100%">Cocker, T. L.</style></author><author><style face="normal" font="default" size="100%">Huber, R.</style></author><author><style face="normal" font="default" size="100%">Markelz, A. G.</style></author><author><style face="normal" font="default" size="100%">Taylor, Z. D.</style></author><author><style face="normal" font="default" size="100%">Wallace, V. P.</style></author><author><style face="normal" font="default" size="100%">Zeitler, J. A.</style></author><author><style face="normal" font="default" size="100%">Sibik, J.</style></author><author><style face="normal" font="default" size="100%">Korter, T. M.</style></author><author><style face="normal" font="default" size="100%">Ellison, B.</style></author><author><style face="normal" font="default" size="100%">Rea, S.</style></author><author><style face="normal" font="default" size="100%">Goldsmith, P.</style></author><author><style face="normal" font="default" size="100%">Cooper, K. 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B.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">The 2017 terahertz science and technology roadmap</style></title><secondary-title><style face="normal" font="default" size="100%">Journal of Physics D-Applied Physics</style></secondary-title><alt-title><style face="normal" font="default" size="100%">J. Phys. D-Appl. Phys.</style></alt-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">ex-vivo</style></keyword><keyword><style  face="normal" font="default" size="100%">generation</style></keyword><keyword><style  face="normal" font="default" size="100%">metal wave-guides</style></keyword><keyword><style  face="normal" font="default" size="100%">near-field</style></keyword><keyword><style  face="normal" font="default" size="100%">performance</style></keyword><keyword><style  face="normal" font="default" size="100%">photoconductive emitters</style></keyword><keyword><style  face="normal" font="default" size="100%">Physics</style></keyword><keyword><style  face="normal" font="default" size="100%">quantum-cascade lasers</style></keyword><keyword><style  face="normal" font="default" size="100%">radiation</style></keyword><keyword><style  face="normal" font="default" size="100%">semiconductors</style></keyword><keyword><style  face="normal" font="default" size="100%">Terahertz</style></keyword><keyword><style  face="normal" font="default" size="100%">thz</style></keyword><keyword><style  face="normal" font="default" size="100%">time-domain spectroscopy</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2017</style></year><pub-dates><date><style  face="normal" font="default" size="100%">Feb</style></date></pub-dates></dates><number><style face="normal" font="default" size="100%">4</style></number><volume><style face="normal" font="default" size="100%">50</style></volume><pages><style face="normal" font="default" size="100%">49</style></pages><isbn><style face="normal" font="default" size="100%">0022-3727</style></isbn><language><style face="normal" font="default" size="100%">English</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;Science and technologies based on terahertz frequency electromagnetic radiation (100 GHz-30 THz) have developed rapidly over the last 30 years. For most of the 20th Century, terahertz radiation, then referred to as sub-millimeter wave or far-infrared radiation, was mainly utilized by astronomers and some spectroscopists. Following the development of laser based terahertz time-domain spectroscopy in the 1980s and 1990s the field of THz science and technology expanded rapidly, to the extent that it now touches many areas from fundamental science to &#039;real world&#039; applications. For example THz radiation is being used to optimize materials for new solar cells, and may also be a key technology for the next generation of airport security scanners. While the field was emerging it was possible to keep track of all new developments, however now the field has grown so much that it is increasingly difficult to follow the diverse range of new discoveries and applications that are appearing. At this point in time, when the field of THz science and technology is moving from an emerging to a more established and interdisciplinary field, it is apt to present a roadmap to help identify the breadth and future directions of the field. The aim of this roadmap is to present a snapshot of the present state of THz science and technology in 2017, and provide an opinion on the challenges and opportunities that the future holds. To be able to achieve this aim, we have invited a group of international experts to write 18 sections that cover most of the key areas of THz science and technology. We hope that The 2017 Roadmap on THz science and technology will prove to be a useful resource by providing a wide ranging introduction to the capabilities of THz radiation for those outside or just entering the field as well as providing perspective and breadth for those who are well established. 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S. Vitiello, M. S. Linfield, E. H. Davies, A. G. Hoffmann, Matthias C. Booske, John Paoloni, Claudio Gensch, M. Weightman, P. Williams, G. P. Castro-Camus, E. Cumming, D. R. S. Simoens, F. Escorcia-Carranza, I. Grant, J. Lucyszyn, Stepan Kuwata-Gonokami, Makoto Konishi, Kuniaki Koch, Martin Schmuttenmaer, Charles A. Cocker, Tyler L. Huber, Rupert Markelz, A. G. Taylor, Z. D. Wallace, Vincent P. Zeitler, J. Axel Sibik, Juraj Korter, Timothy M. Ellison, B. Rea, S. Goldsmith, P. Cooper, Ken B. Appleby, Roger Pardo, D. Huggard, P. G. Krozer, V. Shams, Haymen Fice, Martyn Renaud, Cyril Seeds, Alwyn Stoehr, Andreas Naftaly, Mira Ridler, Nick Clarke, Roland Cunningham, John E. Johnston, Michael B.&lt;br/&gt;Huggard, Peter/U-2150-2019; Konishi, Kuniaki/AAN-3624-2020; Zeitler, J. Axel/B-4885-2008; Paoloni, Claudio/AAH-9824-2019; Hoffmann, Matthias C./N-1082-2019; Wallace, Vincent P/A-9320-2012; Johnston, Michael/B-9813-2008; Castro-Camus, Enrique/V-6861-2019; Krozer, Viktor/P-5623-2014; Hoffmann, Matthias C/B-3893-2009; PAOLONI, CLAUDIO/AAA-3211-2020; Gonokami, Makoto/F-3641-2012; Shams, Haymen/H-3754-2012; Ridler, Nick/AAN-9637-2020; Huber, Rupert/N-4126-2018&lt;br/&gt;Konishi, Kuniaki/0000-0003-2389-9787; Zeitler, J. Axel/0000-0002-4958-0582; Hoffmann, Matthias C./0000-0002-3596-9853; Wallace, Vincent P/0000-0003-3814-5400; Johnston, Michael/0000-0002-0301-8033; Krozer, Viktor/0000-0002-2387-1947; Hoffmann, Matthias C/0000-0002-3596-9853; PAOLONI, CLAUDIO/0000-0002-0265-0862; Shams, Haymen/0000-0002-5333-6478; Huber, Rupert/0000-0001-6617-9283; Davies, Alexander/0000-0002-1987-4846; Seeds, Alwyn/0000-0002-5228-627X; Castro-Camus, Enrique/0000-0002-8218-9155; Cunningham, John/0000-0002-1805-9743; Naftaly, Mira/0000-0002-0671-822X; Cumming, David/0000-0002-7838-8362&lt;br/&gt;Engineering and Physical Sciences Research CouncilUK Research &amp; Innovation (UKRI)Engineering &amp; Physical Sciences Research Council (EPSRC) [EP/P015883/1, EP/M00306X/1, EP/K023349/1, EP/M017095/1, EP/L026597/1, EP/J017671/1] Funding Source: researchfish; Natural Environment Research CouncilUK Research &amp; Innovation (UKRI)NERC Natural Environment Research Council [NER/Z/S/2003/00642, NE/L012375/1, NER/Z/S/2000/01292] Funding Source: researchfish; Science and Technology Facilities CouncilUK Research &amp; Innovation (UKRI)Science &amp; Technology Facilities Council (STFC) [ST/P002056/1] Funding Source: researchfish; Direct For Biological SciencesNational Science Foundation (NSF)NSF - Directorate for Biological Sciences (BIO) [1556359] Funding Source: National Science Foundation; Div Of Biological InfrastructureNational Science Foundation (NSF)NSF - Directorate for Biological Sciences (BIO) [1556359] Funding Source: National Science Foundation; Div Of Molecular and Cellular BioscienceNational Science Foundation (NSF)NSF - Directorate for Biological Sciences (BIO) [1616529] Funding Source: National Science Foundation&lt;br/&gt;566&lt;br/&gt;30&lt;br/&gt;462&lt;br/&gt;Iop publishing ltd&lt;br/&gt;Bristol&lt;br/&gt;1361-6463</style></notes><custom7><style face="normal" font="default" size="100%">043001</style></custom7><auth-address><style face="normal" font="default" size="100%">[Dhillon, S. S.] Univ Paris 06, Univ Paris Diderot, Sorbonne Univ,CNRS,Lab Pierre Aigrain, Sorbonne Paris Cite,Ecole Normale Super,PSL Res U, F-75231 Paris, France. [Vitiello, M. S.] CNR, Ist Nanosci, NEST, Piazza San Silvestro 12, I-56127 Pisa, Italy. [Vitiello, M. S.] Scuola Normale Super Pisa, Piazza San Silvestro 12, I-56127 Pisa, Italy. [Linfield, E. H.|Davies, A. G.|Cunningham, John E.] Univ Leeds, Sch Elect &amp; Elect Engn, Leeds LS2 9JT, W Yorkshire, England. [Hoffmann, Matthias C.] SLAC Natl Accelerator Lab, Linac Coherent Light Source, Menlo Pk, CA 94025 USA. [Booske, John] Univ Wisconsin Madison, Dept Elect &amp; Comp Engn, Madison, WI USA. [Paoloni, Claudio] Univ Lancaster, Dept Engn, Lancaster, England. [Gensch, M.] Helmholtz Zentrum Dresden Rossendorf, Inst Radiat Phys, Bautzner Landstr 400, D-01328 Dresden, Germany. [Weightman, P.] Univ Liverpool, Dept Phys, Liverpool L69 7ZE, Merseyside, England. [Williams, G. P.] Jefferson Lab, 12000 Jefferson Ave Suite 21, Newport News, VA 23606 USA. [Castro-Camus, E.] Ctr Invest Opt AC, Loma Bosque 115, Guanajuato 37150, Mexico. [Cumming, D. R. S.|Escorcia-Carranza, I.|Grant, J.] Glasgow, Sch Engn, Microsyst Technol Grp, Glasgow G12 8LT, Lanark, Scotland. [Simoens, F.] CEA Leti MINATEC, 17 Rue Martyrs, F-38054 Grenoble 9, France. [Lucyszyn, Stepan] Imperial Coll London, Dept EEE, Ctr Terahertz Sci &amp; Engn, London, England. [Kuwata-Gonokami, Makoto|Konishi, Kuniaki] Univ Tokyo, Dept Phys, Tokyo, Japan. [Koch, Martin] Philipps Univ Marburg, Fac Phys, D-35032 Marburg, Germany. [Koch, Martin] Philipps Univ Marburg, Ctr Mat Sci, D-35032 Marburg, Germany. [Schmuttenmaer, Charles A.] Yale Univ, Dept Chem, 225 Prospect St,POB 208107, New Haven, CT 06520 USA. [Schmuttenmaer, Charles A.] Yale Univ, Energy Sci Inst, 225 Prospect St,POB 208107, New Haven, CT 06520 USA. [Cocker, Tyler L.|Huber, Rupert] Univ Regensburg, Inst Expt &amp; Angew Phys, Univ Str 31, D-93053 Regensburg, Germany. [Markelz, A. G.] Univ Buffalo State Univ New York, Dept Phys, Buffalo, NY 14620 USA. [Taylor, Z. D.] Univ Calif Los Angeles, Dept Bioengn, Los Angeles, CA 90095 USA. [Wallace, Vincent P.] Univ Western Australia M013, 35 Stirling Highway, Crawley, WA 6009, Australia. [Zeitler, J. Axel|Sibik, Juraj] Magnet Resonance Res Ctr, Dept Chem Engn, JJ Thompson Ave, Cambridge CB3 0HE, England. [Korter, Timothy M.] Syracuse Univ, Dept Chem, 1-014 CST,111 Coll Pl, Syracuse, NY 13244 USA. [Ellison, B.|Rea, S.|Pardo, D.|Huggard, P. G.] RAL Space, STFC, Millimetre Wave Technol Grp, Didcot OX11 0QX, Oxon, England. [Goldsmith, P.] Jet Prop Lab, M-S 180-703,4800 Oak Grove Dr, Pasadena, CA 91109 USA. [Cooper, Ken B.] CALTECH, Jet Prop Lab, Pasadena, CA USA. [Appleby, Roger] Innovasec Ltd, 212b West Malvern Rd, Malvern WR14 4BA, Worcs, England. [Krozer, V.] Goethe Univ Frankfurt Main, Goethe Leibniz Terahertz Ctr, D-60323 Frankfurt, Germany. [Shams, Haymen|Fice, Martyn|Renaud, Cyril|Seeds, Alwyn] UCL, Dept Elect &amp; Elect Engn, Torrington Pl, London WC1E 7JE, England. [Stoehr, Andreas] Univ Duisburg Essen, Fac Engn, Dept Optoelect, Lotharstr 55, D-47057 Duisburg, Germany. [Naftaly, Mira|Ridler, Nick] Natl Phys Lab, Div Time Quantum &amp; Electromagnet, Teddington TW11 0LW, Middx, England. [Clarke, Roland] Univ Leeds, Sch Elect &amp; Elect Engn, Leeds LS2 9JT, W Yorkshire, England. [Johnston, Michael B.] Univ Oxford, Dept Phys, Clarendon Lab, Parks Rd, Oxford OX1 3PU, England.&lt;br/&gt;Cunningham, JE (corresponding author), Univ Leeds, Sch Elect &amp; Elect Engn, Leeds LS2 9JT, W Yorkshire, England.|Johnston, MB (corresponding author), Univ Oxford, Dept Phys, Clarendon Lab, Parks Rd, Oxford OX1 3PU, England.&lt;br/&gt;enrique@cio.mx|david.cumming.2@glasgow.ac.uk|J.E.Cunningham@leeds.ac.uk|michael.johnston@physics.ox.ac.uk</style></auth-address></record><record><source-app name="Biblio" version="7.x">Drupal-Biblio</source-app><ref-type>10</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Xu, M. Y.</style></author><author><style face="normal" font="default" size="100%">George, D. K.</style></author><author><style face="normal" font="default" size="100%">Jimenez, R.</style></author><author><style face="normal" font="default" size="100%">Markelz, A. G.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Probing the Stability of Fluorescent Proteins by Terahertz Spectroscopy</style></title><secondary-title><style face="normal" font="default" size="100%">2014 39th International Conference on Infrared, Millimeter, and Terahertz Waves</style></secondary-title><tertiary-title><style face="normal" font="default" size="100%">International Conference on Infrared Millimeter and Terahertz Waves</style></tertiary-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">dynamics</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2014</style></year></dates><publisher><style face="normal" font="default" size="100%">Ieee</style></publisher><pub-location><style face="normal" font="default" size="100%">New York</style></pub-location><isbn><style face="normal" font="default" size="100%">978-1-4799-3877-3</style></isbn><language><style face="normal" font="default" size="100%">English</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;The higher transmission through tissues of long wavelength light motivates the development of fluorescent proteins with excitation shifted to the red. However red fluorescent proteins (RFPs) are more susceptible to photobleaching than their shorter wavelength counterparts. In particular RFPs are more susceptible to photobleaching [1]. A possible reason for this is a decrease in the structural stability of the beta barrel. Measurements of structural stability include atomic root mean squared displacement &amp;lt;x(2)&amp;gt; measured by the X-ray B-factor and neutron quasi elastic scattering. To date, X-ray measurements of RFP&#039;s do not indicate a structural stability change and systematic scattering studies have not been performed. Using THz dielectric response we examine if the picosecond structural flexibility decreases with increasing FP stability.&lt;/p&gt;</style></abstract><accession-num><style face="normal" font="default" size="100%">WOS:000378889200449</style></accession-num><notes><style face="normal" font="default" size="100%">ISI Document Delivery No.: BF0IL&lt;br/&gt;Times Cited: 0&lt;br/&gt;Cited Reference Count: 7&lt;br/&gt;Cited References: &lt;br/&gt;     Dean KM, 2011, BIOPHYS J, V101, P961, DOI 10.1016/j.bpj.2011.06.055&lt;br/&gt;     He YF, 2011, BIOPHYS J, V100, P1058, DOI 10.1016/j.bpj.2010.12.3731&lt;br/&gt;     Helms V, 2007, CHEMPHYSCHEM, V8, P23, DOI 10.1002/cphc.200600298&lt;br/&gt;     Leu BM, 2008, BIOPHYS J, V95, P5874, DOI 10.1529/biophysj.108.138198&lt;br/&gt;     Markelz AG, 2007, CHEM PHYS LETT, V442, P413, DOI 10.1016/j.cplett.2007.05.080&lt;br/&gt;     Nagy A, 2004, THERMOCHIM ACTA, V410, P161, DOI 10.1016/S0040-6031(03)00397-6&lt;br/&gt;     Zaccai G, 2000, SCIENCE, V288, P1604, DOI 10.1126/science.288.5471.1604&lt;br/&gt;Xu, Mengyang George, D. K. Jimenez, R. Markelz, A. G.&lt;br/&gt;Irmmw-thz&lt;br/&gt;Proceedings Paper&lt;br/&gt;39th International Conference on Infrared, Millimeter, and Terahertz waves (IRMMW-THz)&lt;br/&gt;Sep 14-19, 2014&lt;br/&gt;Tucson, AZ&lt;br/&gt;THORLABS, Tydex, TOPTICA Photon, Bruker, Gentec EO, Lake Shore Cryotron, Ekspla, Zomega, TeraSense, Insight Product, Emcore, QMC Instruments, TeraView, NeaSpec, Advantest, MenloSystems, Traycer, Microtech Instruments Inc, LongWave Photon, Virginia Diodes Inc, ASU, MTT S, Journal Infrared Millimeter &amp; Tera Hertz Waves, Tera Hertz Sci &amp; Technol, Army Res Off&lt;br/&gt;George, Deepu/J-9882-2014&lt;br/&gt;George, Deepu/0000-0003-0021-0705&lt;br/&gt;345 e 47th st, new york, ny 10017 usa&lt;br/&gt;2162-2027</style></notes><auth-address><style face="normal" font="default" size="100%">[Xu, Mengyang|George, D. K.|Markelz, A. G.] SUNY Buffalo, Buffalo, NY 14260 USA. [Jimenez, R.] Univ Colorado, Boulder, CO 80309 USA.&lt;br/&gt;Xu, MY (corresponding author), SUNY Buffalo, Buffalo, NY 14260 USA.</style></auth-address></record><record><source-app name="Biblio" version="7.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Kabir, N. A.</style></author><author><style face="normal" font="default" size="100%">Yoon, Y.</style></author><author><style face="normal" font="default" size="100%">Knab, J. R.</style></author><author><style face="normal" font="default" size="100%">Chen, J. Y.</style></author><author><style face="normal" font="default" size="100%">Markelz, A. G.</style></author><author><style face="normal" font="default" size="100%">Reno, J. L.</style></author><author><style face="normal" font="default" size="100%">Sadofyev, Y.</style></author><author><style face="normal" font="default" size="100%">Johnson, S.</style></author><author><style face="normal" font="default" size="100%">Zhang, Y. H.</style></author><author><style face="normal" font="default" size="100%">Bird, J. P.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Terahertz transmission characteristics of high-mobility GaAs and InAs two-dimensional-electron-gas systems</style></title><secondary-title><style face="normal" font="default" size="100%">Applied Physics Letters</style></secondary-title><alt-title><style face="normal" font="default" size="100%">Appl. Phys. Lett.</style></alt-title><short-title><style face="normal" font="default" size="100%">Appl. Phys. Lett.Appl. Phys. Lett.</style></short-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">field-effect transistors</style></keyword><keyword><style  face="normal" font="default" size="100%">photoconductivity</style></keyword><keyword><style  face="normal" font="default" size="100%">Physics</style></keyword><keyword><style  face="normal" font="default" size="100%">plasma-waves</style></keyword><keyword><style  face="normal" font="default" size="100%">radiation</style></keyword><keyword><style  face="normal" font="default" size="100%">resonant detection</style></keyword><keyword><style  face="normal" font="default" size="100%">subterahertz</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2006</style></year><pub-dates><date><style  face="normal" font="default" size="100%">Sep</style></date></pub-dates></dates><number><style face="normal" font="default" size="100%">13</style></number><volume><style face="normal" font="default" size="100%">89</style></volume><pages><style face="normal" font="default" size="100%">3</style></pages><isbn><style face="normal" font="default" size="100%">0003-6951</style></isbn><language><style face="normal" font="default" size="100%">English</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;Frequency-dependent complex conductivity of high-mobility GaAs and InAs two-dimensional-electron-gas (2DEG) systems is studied by terahertz time domain spectroscopy. Determining the momentum relaxation time from a Drude model, the authors find a lower value than that from dc measurements, particularly at high frequencies/low temperatures. These deviations are consistent with the ratio tau(t)/tau(q,) where tau(q) is the full scattering time. This suggests that small-angle scattering leads to weaker heating of 2DEGs at low temperatures than expected from dc mobilit9y. (c) 2006 American Institute of Physics.&lt;/p&gt;</style></abstract><work-type><style face="normal" font="default" size="100%">Article</style></work-type><accession-num><style face="normal" font="default" size="100%">WOS:000240875800066</style></accession-num><notes><style face="normal" font="default" size="100%">ISI Document Delivery No.: 089JE&lt;br/&gt;Times Cited: 18&lt;br/&gt;Cited Reference Count: 16&lt;br/&gt;Cited References: &lt;br/&gt;     ANDO T, 1982, REV MOD PHYS, V54, P437, DOI 10.1103/RevModPhys.54.437&lt;br/&gt;     ANDO T, 1989, HIGH MAGNETIC FIELDS, V2, P164&lt;br/&gt;     Ashcroft NW, 1976, SOLID STATE PHYS, P1&lt;br/&gt;     Beard MC, 2000, PHYS REV B, V62, P15764, DOI 10.1103/PhysRevB.62.15764&lt;br/&gt;     Cerne J, 2000, PHYS REV B, V61, P8133, DOI 10.1103/PhysRevB.61.8133&lt;br/&gt;     COLERIDGE PT, 1991, PHYS REV B, V44, P3793, DOI 10.1103/PhysRevB.44.3793&lt;br/&gt;     Dorozhkin PS, 2005, APPL PHYS LETT, V87, DOI 10.1063/1.2035883&lt;br/&gt;     Knap W, 2002, APPL PHYS LETT, V81, P4637, DOI 10.1063/1.1525851&lt;br/&gt;     Knap W, 2002, APPL PHYS LETT, V80, P3433, DOI 10.1063/1.1473685&lt;br/&gt;     Kukushkin IV, 2005, APPL PHYS LETT, V86, DOI 10.1063/1.1856143&lt;br/&gt;     MADELUNG O, 1996, SEMICONDUCTORS BASIC, P109&lt;br/&gt;     MCKNIGHT SW, 1987, INFRARED PHYS, V27, P327, DOI 10.1016/0020-0891(87)90074-1&lt;br/&gt;     Peralta XG, 2002, APPL PHYS LETT, V81, P1627, DOI 10.1063/1.1497433&lt;br/&gt;     Sadofyev YG, 2002, APPL PHYS LETT, V81, P1833, DOI 10.1063/1.1504882&lt;br/&gt;     Shaner EA, 2005, APPL PHYS LETT, V87, DOI 10.1063/1.2128057&lt;br/&gt;     ZAWADZKI W, 1974, ADV PHYS, V23, P435, DOI 10.1080/00018737400101371&lt;br/&gt;Kabir, N. A. Yoon, Y. Knab, J. R. Chen, J. -Y. Markelz, A. G. Reno, J. L. Sadofyev, Y. Johnson, S. Zhang, Y. -H. Bird, J. P.&lt;br/&gt;Bird, Jonathan P/G-4068-2010&lt;br/&gt;Bird, Jonathan P/0000-0002-6966-9007; Markelz, Andrea/0000-0003-0443-4319&lt;br/&gt;18&lt;br/&gt;&lt;br/&gt;15&lt;br/&gt;Amer inst physics&lt;br/&gt;Melville</style></notes><custom7><style face="normal" font="default" size="100%">132109</style></custom7><auth-address><style face="normal" font="default" size="100%">SUNY Buffalo, Dept Phys, Buffalo, NY 14260 USA. SUNY Buffalo, Dept Elect Engn, Buffalo, NY 14260 USA. Sandia Natl Labs, Nanostruct &amp; Semicond Phys Dept, Albuquerque, NM 87185 USA. Arizona State Univ, Dept Elect Engn, Tempe, AZ 85287 USA. Arizona State Univ, Ctr Solid State Elect Res, Tempe, AZ 85287 USA.&lt;br/&gt;Markelz, AG (corresponding author), SUNY Buffalo, Dept Phys, Buffalo, NY 14260 USA.&lt;br/&gt;jbird@buffalo.edu</style></auth-address></record></records></xml>