R. Gomez
Rice University
16 Papers
45 Citations
R. Gomez is an academic researcher from Rice University. The author has contributed to research in topics: Dark matter & Time projection chamber. The author has an hindex of 11, co-authored 16 publications.
Chat about Author
Papers
First results from the XENON10 dark matter experiment at the gran sasso national laboratory
J. Angle,J. Angle,Elena Aprile,F. Arneodo,Laura Baudis,A. Bernstein,Alexander Bolozdynya,P. P. Brusov,Luis Coelho,C. E. Dahl,C. E. Dahl,L. DeViveiros,A. D. Ferella,L.M.P. Fernandes,S. Fiorucci,R. J. Gaitskell,Karl Giboni,R. Gomez,R. Hasty,L. Kastens,J. Kwong,J. Kwong,J. A. M. Lopes,N. Madden,A. Manalaysay,A. Manalaysay,A. Manzur,Daniel McKinsey,M. E. Monzani,Kaixuan Ni,Uwe Oberlack,J. Orboeck,Guillaume Plante,R. Santorelli,J.M.F. dos Santos,P. Shagin,T. A. Shutt,P. Sorensen,S. Schulte,C. Winant,Masaki Yamashita +40 more
TL;DR: A blind analysis of 58.6 live days of data excludes previously unexplored parameter space, setting a new 90% C.L. upper limit for the WIMP-nucleon spin-independent cross section of 8.8x10(-44) cm2 for a W IMP mass of 100 GeV/c2, which further constrains predictions of supersymmetric models.
Search for light dark matter in XENON10 data.
J. Angle,J. Angle,Elena Aprile,F. Arneodo,Laura Baudis,A. Bernstein,Alexander Bolozdynya,Luis Coelho,C. E. Dahl,L. DeViveiros,A. D. Ferella,L.M.P. Fernandes,S. Fiorucci,R. J. Gaitskell,Karl Giboni,R. Gomez,R. Hasty,L. Kastens,J. Kwong,J. A. M. Lopes,Norman W. Madden,A. Manalaysay,A. Manalaysay,A. Manzur,Daniel McKinsey,M. E. Monzani,Kaixuan Ni,Uwe Oberlack,Uwe Oberlack,J. Orboeck,Guillaume Plante,R. Santorelli,J.M.F. dos Santos,S. Schulte,P. Shagin,T. A. Shutt,P. Sorensen,C. Winant,Masaki Yamashita +38 more
TL;DR: The data strongly constrain recent elastic dark matter interpretations of excess low-energy events observed by CoGeNT and CRESST-II, as well as the DAMA annual modulation signal.
734
Erratum: Search for light dark matter in XENON10 data (Physical Review Letters (2011) 107 (051301))
J. Angle,J. Angle,Elena Aprile,F. Arneodo,Laura Baudis,Adam Bernstein,Alexander Bolozdynya,Luis Coelho,C. E. Dahl,L. DeViveiros,A. D. Ferella,L.M.P. Fernandes,S. Fiorucci,R. J. Gaitskell,Karl Giboni,R. Gomez,R. Hasty,L. Kastens,J. Kwong,J. A. M. Lopes,Norman W. Madden,A. Manalaysay,A. Manalaysay,A. Manzur,Daniel McKinsey,M. E. Monzani,Kaixuan Ni,Uwe Oberlack,Uwe Oberlack,J. Orboeck,Guillaume Plante,R. Santorelli,J.M.F. dos Santos,S. Schulte,P. Shagin,T. A. Shutt,P. Sorensen,C. Winant,Masaki Yamashita +38 more
194
Design and performance of the XENON10 dark matter experiment
Elena Aprile,J. Angle,J. Angle,F. Arneodo,Laura Baudis,Laura Baudis,Adam Bernstein,Alexander Bolozdynya,P. P. Brusov,Luis Coelho,C. E. Dahl,C. E. Dahl,L. DeViveiros,A. D. Ferella,L.M.P. Fernandes,S. Fiorucci,R. J. Gaitskell,Karl Giboni,R. Gomez,R. Hasty,L. Kastens,J. Kwong,J. Kwong,J. A. M. Lopes,Norman W. Madden,A. Manalaysay,A. Manalaysay,A. Manzur,Daniel McKinsey,M. E. Monzani,Kaixuan Ni,Kaixuan Ni,Uwe Oberlack,J. Orboeck,D. Orlandi,Guillaume Plante,R. Santorelli,J.M.F. dos Santos,P. Shagin,T. A. Shutt,P. Sorensen,S. Schulte,E. Tatananni,C. Winant,Masaki Yamashita +44 more
TL;DR: XENON10 as mentioned in this paper is the first two-phase Xenon time projection chamber (TPC) developed within the XENON dark matter search program, with an active liquid xenon (LXe) mass of about 14 kg.
173
The scintillation and ionization yield of liquid xenon for nuclear recoils
P. Sorensen,A. Manzur,C. E. Dahl,J. Angle,J. Angle,Elena Aprile,F. Arneodo,Laura Baudis,Adam Bernstein,Alexander Bolozdynya,Luis Coelho,L. DeViveiros,A. D. Ferella,L.M.P. Fernandes,S. Fiorucci,R. J. Gaitskell,Karl Giboni,R. Gomez,R. Hasty,L. Kastens,J. Kwong,J. A. M. Lopes,Norman W. Madden,A. Manalaysay,A. Manalaysay,Daniel McKinsey,M. E. Monzani,Kaixuan Ni,Uwe Oberlack,J. Orboeck,G. Plante,R. Santorelli,J.M.F. dos Santos,P. Shagin,T. A. Shutt,S. Schulte,C. Winant,Masaki Yamashita +37 more
TL;DR: In this paper, the relative scintillation yield and the absolute ionization yield for nuclear recoils in xenon were measured in two ways, both in agreement with previous measurements and with a factor of 10 lower energy threshold.