R. Svoboda
University of California, Davis
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Featured researches published by R. Svoboda.
Physical Review Letters | 2014
X. Bai; J. Balajthy; S. Bedikian; E. Bernard; A. Bernstein; A. Bolozdynya; A. Bradley; D. Byram; C. Chan; C. Chiller; K. Clark; T. Coey; A. Currie; A. Curioni; S. Dazeley; L. de Viveiros; A. Dobi; J. Dobson; E. Druszkiewicz; S. Fiorucci; C. Flores; C. Ghag; M. Hanhardt; M. Horn; M. Ihm; L. Kastens; K. Kazkaz; R. Knoche; S. Kyre; R. Lander
The Large Underground Xenon (LUX) experiment is a dual-phase xenon time-projection chamber operating at the Sanford Underground Research Facility (Lead, South Dakota). The LUX cryostat was filled for the first time in the underground laboratory in February 2013. We report results of the first WIMP search data set, taken during the period from April to August 2013, presenting the analysis of 85.3 live days of data with a fiducial volume of 118 kg. A profile-likelihood analysis technique shows our data to be consistent with the background-only hypothesis, allowing 90% confidence limits to be set on spin-independent WIMP-nucleon elastic scattering with a minimum upper limit on the cross section of 7.6 × 10(-46) cm(2) at a WIMP mass of 33 GeV/c(2). We find that the LUX data are in disagreement with low-mass WIMP signal interpretations of the results from several recent direct detection experiments.
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2013
D. S. Akerib; X. Bai; S. Bedikian; E. Bernard; A. Bernstein; A. Bolozdynya; A. Bradley; D. Byram; S. B. Cahn; C. Camp; M.C. Carmona-Benitez; D. Carr; J.J. Chapman; A.A. Chiller; C. Chiller; K. Clark; T. Classen; T. Coffey; A. Curioni; E. Dahl; S. Dazeley; L. de Viveiros; A. Dobi; E. Dragowsky; E. Druszkiewicz; B. Edwards; C.H. Faham; S. Fiorucci; R.J. Gaitskell; K.R. Gibson
The Large Underground Xenon (LUX) collaboration has designed and constructed a dual-phase xenon detector, in order to conduct a search for Weakly Interacting Massive Particles (WIMPs), a leading dark matter candidate. The goal of the LUX detector is to clearly detect (or exclude) WIMPS with a spin independent cross-section per nucleon of 2×10-46cm2, equivalent to ∼1event/100kg/month in the inner 100-kg fiducial volume (FV) of the 370-kg detector. The overall background goals are set to have <1 background events characterized as possible WIMPs in the FV in 300 days of running. This paper describes the design and construction of the LUX detector.
Physical Review Letters | 2004
K. Eguchi; Z. Djurcic; L. A. Winslow; T. Mitsui; K. Ishihara; Koji Inoue; S. Dazeley; Kimimasa Ikeda; P. Vogel; K. Ishii; J. A. Detwiler; H. Watanabe; P. Gorham; W. Bugg; K. Tada; C. E. Okada; A. R. Young; K. Owada; D. A. Dwyer; B. E. Berger; T. Kawashima; J. Shirai; Y.D. Chan; F. Piquemal; M. Koga; I. Shimizu; A. Kozlov; F. Suekane; B.D. Dieterle; T. Iwamoto
Data corresponding to a KamLAND detector exposure of 0.28 kton-year has been used to search for
Physical Review D | 2008
J. G. Learned; S. T. Dye; Sandip Pakvasa; R. Svoboda
\bar{\nu}_e
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 1993
R. Becker-Szendy; R. M. Bionta; C. B. Bratton; David William Casper; R. Claus; B. G. Cortez; S. T. Dye; S. Errede; G. W. Foster; W. Gajewski; K. S. Ganezer; M. Goldhaber; P. G. Halverson; Eric Hazen; T. W. Jones; D. Kielczewska; W. R. Kropp; J. G. Learned; J. M. LoSecco; S. Matsuno; J. A. J. Matthews; G. McGrath; C. McGrew; R. S. Miller; M. S. Mudan; Hae-Sim Park; L. R. Price; F. Reines; J. Schultz; Sally Seidel
s in the energy range 8.3 MeV
Journal of Physics: Conference Series | 2010
D. N. McKinsey; D. S. Akerib; S. Bedikian; A. Bernstein; A. Bolozdynya; A. Bradley; J.J. Chapman; K. Clark; T. Classen; A. Curioni; E Dahl; S. Dazeley; M. R. Dragowsky; L. de Viveiros; E. Druszkiewicz; S. Fiorucci; R.J. Gaitskell; C. Hall; C. Hernandez Faham; L. Kastens; K. Kazkaz; R. Lander; D.S. Leonard; D.C. Malling; R. Mannino; Dongming Mei; J. Mock; J.A. Nikkel; P. Phelps; T. Shutt
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Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2012
D. S. Akerib; X. Bai; S. Bedikian; E. Bernard; A. Bernstein; A. Bradley; S. B. Cahn; M.C. Carmona-Benitez; D. Carr; J.J. Chapman; K. Clark; T. Classen; T. Coffey; S. Dazeley; L. de Viveiros; A. Dobi; M. R. Dragowsky; E. Druszkiewicz; C.H. Faham; S. Fiorucci; R.J. Gaitskell; K.R. Gibson; C. Hall; M. Hanhardt; B. Holbrook; M. Ihm; R. G. Jacobsen; L. Kastens; K. Kazkaz; R. Lander
E
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2012
D. S. Akerib; X. Bai; S. Bedikian; E. Bernard; A. Bernstein; A. Bradley; S. B. Cahn; M.C. Carmona-Benitez; D. Carr; J.J. Chapman; K. Clark; T. Classen; T. Coffey; A. Curioni; S. Dazeley; L. de Viveiros; M. R. Dragowsky; E. Druszkiewicz; C.H. Faham; S. Fiorucci; R.J. Gaitskell; K.R. Gibson; C. Hall; M. Hanhardt; B. Holbrook; M. Ihm; R. G. Jacobsen; L. Kastens; K. Kazkaz; R. Lander
_{\bar{\nu}_e}
Lawrence Berkeley National Laboratory | 2008
A. Bernstein; E. Blucher; D. Cline; M. V. Diwan; B. T. Fleming; R. Kadel; E. Kearns; Jeff Klein; K. Lande; Francesco Lanni; D. Lissauer; R. D. McKeown; W. M. Morse; R. Radeika; K. Scholberg; M. Smy; H. W. Sobel; G. W. Sullivan; R. Svoboda; M. R. Vagins; C. W. Walter; R. Zwaska
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2013
D. S. Akerib; X. Bai; S. Bedikian; A. Bernstein; A. Bolozdynya; A. Bradley; S. B. Cahn; D. Carr; J.J. Chapman; K. Clark; T. Classen; A. Curioni; C.E. Dahl; S. Dazeley; L. de Viveiros; M. R. Dragowsky; E. Druszkiewicz; S. Fiorucci; R.J. Gaitskell; C. Hall; C.H. Faham; B. Holbrook; L. Kastens; K. Kazkaz; J. Kwong; R. Lander; D.S. Leonard; D.C. Malling; R. Mannino; D. N. McKinsey
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