C
C. Chiller
Researcher at University of South Dakota
Publications - 19
Citations - 3564
C. Chiller is an academic researcher from University of South Dakota. The author has contributed to research in topics: WIMP & Dark matter. The author has an hindex of 12, co-authored 18 publications receiving 3314 citations.
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Journal ArticleDOI
First results from the LUX dark matter experiment at the Sanford Underground Research Facility
D. S. Akerib,Henrique Araujo,X. Bai,A. J. Bailey,J. Balajthy,S. Bedikian,Ethan Bernard,A. Bernstein,Alexander Bolozdynya,A. W. Bradley,D. Byram,Sidney Cahn,M. C. Carmona-Benitez,C. Chan,J.J. Chapman,A. A. Chiller,C. Chiller,K. Clark,T. Coffey,A. Currie,A. Curioni,Steven Dazeley,L. de Viveiros,A. Dobi,J. E. Y. Dobson,E. M. Dragowsky,E. Druszkiewicz,B. N. Edwards,C. H. Faham,S. Fiorucci,C. E. Flores,R. J. Gaitskell,V. M. Gehman,C. Ghag,K.R. Gibson,Murdock Gilchriese,C. R. Hall,M. Hanhardt,S. A. Hertel,M. Horn,D. Q. Huang,M. Ihm,R. G. Jacobsen,L. Kastens,K. Kazkaz,R. Knoche,S. Kyre,R. L. Lander,N. A. Larsen,C. Lee,David Leonard,K. T. Lesko,A. Lindote,M.I. Lopes,A. Lyashenko,D.C. Malling,R. L. Mannino,Daniel McKinsey,Dongming Mei,J. Mock,M. Moongweluwan,J. A. Morad,M. Morii,A. St. J. Murphy,C. Nehrkorn,H. N. Nelson,F. Neves,James Nikkel,R. A. Ott,M. Pangilinan,P. D. Parker,E. K. Pease,K. Pech,P. Phelps,L. Reichhart,T. A. Shutt,C. Silva,W. Skulski,C. Sofka,V. N. Solovov,P. Sorensen,T.M. Stiegler,K. O'Sullivan,T. J. Sumner,Robert Svoboda,M. Sweany,Matthew Szydagis,D. J. Taylor,B. P. Tennyson,D. R. Tiedt,Mani Tripathi,S. Uvarov,J.R. Verbus,N. Walsh,R. C. Webb,J. T. White,D. White,M. S. Witherell,M. Wlasenko,F.L.H. Wolfs,M. Woods,Chao Zhang +101 more
TL;DR: The first WIMP search data set is reported, taken during the period from April to August 2013, presenting the analysis of 85.3 live days of data, finding that the LUX data are in disagreement with low-mass W IMP signal interpretations of the results from several recent direct detection experiments.
Journal ArticleDOI
The Large Underground Xenon (LUX) experiment
D. S. Akerib,X. Bai,S. Bedikian,Ethan Bernard,A. Bernstein,Alexander Bolozdynya,A. W. Bradley,D. Byram,Sidney 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. M. Dragowsky,E. Druszkiewicz,B. N. Edwards,C.H. Faham,S. Fiorucci,R. J. Gaitskell,K.R. Gibson,Murdock Gilchriese,C. R. Hall,M. Hanhardt,B. Holbrook,M. Ihm,R. G. Jacobsen,L. Kastens,K. Kazkaz,R. Knoche,S. Kyre,J. Kwong,R. L. Lander,N. A. Larsen,C. Lee,David Leonard,K. T. Lesko,A. Lindote,M.I. Lopes,A. Lyashenko,D.C. Malling,R. L. Mannino,Z. Marquez,Daniel McKinsey,Dongming Mei,J. Mock,M. Moongweluwan,M. Morii,H. N. Nelson,F. Neves,James Nikkel,M. Pangilinan,P.D. Parker,E. K. Pease,K. Pech,P. Phelps,A. Rodionov,P. Roberts,Alexander Shei,T. A. Shutt,C. Silva,W. Skulski,V. N. Solovov,C. Sofka,P. Sorensen,J. Spaans,T.M. Stiegler,D. Stolp,Robert Svoboda,M. Sweany,Matthew Szydagis,D. J. Taylor,J. Thomson,Mani Tripathi,S. Uvarov,J.R. Verbus,N. Walsh,R. C. Webb,D. White,J. T. White,T. J. Whitis,M. Wlasenko,F.L.H. Wolfs,M. Woods,Chao Zhang +93 more
TL;DR: The Large Underground Xenon (LUX) detector as mentioned in this paper is a dual-phase Xenon detector with a spin independent cross-section per nucleon of 2 × 10 − 46 cm 2, equivalent to ∼ 1 event / 100 kg / month in the inner 100-kg fiducial volume (FV) of the 370-kg detector.
Journal ArticleDOI
Improved WIMP scattering limits from the LUX experiment
X. Bai,J. Balajthy,P. Beltrame,Adam Bernstein,A. W. Bradley,R. Bramante,C. Chan,C. Chiller,A. Currie,A. Dobi,S. Fiorucci,C. Ghag,M. Hanhardt,M. Horn,M. Ihm,W. Ji,K. Kazkaz,D. Khaitan,C. Lee,A. Lindote,A. Manalaysay,M. Mei,J. Mock,J. Murphy,C. Nehrkorn,F. Neves,M. Pangilinan,P. Phelps,L. Reichhart,C. Rhyne,S. Shaw,C. Silva,P. Sorensen,S. Stephenson,Matthew Szydagis,W. C. Taylor,Mani Tripathi,L. Tvrznikova,S. Uvarov,K. Yazdani,Chao Zhang,Sanford Underground +41 more
TL;DR: In this paper, the authors present constraints on WIMP-nucleus scattering from the 2013 data of the Large Underground Xenon (LUX) dark matter experiment, including $1.4\times10^{4}\,\mathrm{kg\cdot days}$ of search exposure.
Journal ArticleDOI
Limits on Spin-Dependent WIMP-Nucleon Cross Section Obtained from the Complete LUX Exposure
D. S. Akerib,D. S. Akerib,D. S. Akerib,S. Alsum,Henrique Araujo,X. Bai,A. J. Bailey,J. Balajthy,P. Beltrame,Ethan Bernard,Ethan Bernard,A. Bernstein,T. P. Biesiadzinski,T. P. Biesiadzinski,T. P. Biesiadzinski,E. M. Boulton,E. M. Boulton,E. M. Boulton,P. Brás,D. Byram,Sidney Cahn,M. C. Carmona-Benitez,M. C. Carmona-Benitez,C. Chan,A. A. Chiller,C. Chiller,A. Currie,J. E. Cutter,T. J. R. Davison,A. Dobi,J. E. Y. Dobson,E. Druszkiewicz,B. N. Edwards,C. H. Faham,S. R. Fallon,S. Fiorucci,S. Fiorucci,R. J. Gaitskell,V. M. Gehman,C. Ghag,M. G. D. Gilchriese,C. R. Hall,M. Hanhardt,S. J. Haselschwardt,S. A. Hertel,S. A. Hertel,S. A. Hertel,D. P. Hogan,M. Horn,M. Horn,D. Q. Huang,C. M. Ignarra,C. M. Ignarra,R. G. Jacobsen,W. Ji,W. Ji,W. Ji,K. Kamdin,K. Kazkaz,D. Khaitan,R. Knoche,N. A. Larsen,Ching Hua Lee,Ching Hua Lee,Ching Hua Lee,B. G. Lenardo,B. G. Lenardo,K. T. Lesko,A. Lindote,M.I. Lopes,A. Manalaysay,R. L. Mannino,M. F. Marzioni,Daniel McKinsey,Daniel McKinsey,Daniel McKinsey,Dongming Mei,J. Mock,M. Moongweluwan,J. A. Morad,A. St. J. Murphy,C. Nehrkorn,H. N. Nelson,F. Neves,K. O’Sullivan,K. O’Sullivan,K. O’Sullivan,K. C. Oliver-Mallory,K. J. Palladino,K. J. Palladino,K. J. Palladino,E. K. Pease,E. K. Pease,E. K. Pease,L. Reichhart,C. Rhyne,S. Shaw,S. Shaw,T. A. Shutt,T. A. Shutt,C. Silva,M. Solmaz,V. N. Solovov,P. Sorensen,S. Stephenson,T. J. Sumner,Matthew Szydagis,D. J. Taylor,W. C. Taylor,B. P. Tennyson,P. A. Terman,D. R. Tiedt,W. H. To,Mani Tripathi,L. Tvrznikova,L. Tvrznikova,L. Tvrznikova,S. Uvarov,V. Velan,J.R. Verbus,R. C. Webb,J. T. White,T. J. Whitis,T. J. Whitis,T. J. Whitis,M. S. Witherell,F.L.H. Wolfs,Jilei Xu,K. Yazdani,Sarah Young,Chao Zhang +130 more
TL;DR: The spin-dependent WIMP-neutron limit is the most sensitive constraint to date.
Journal ArticleDOI
First Searches for Axions and Axionlike Particles with the LUX Experiment.
D. S. Akerib,D. S. Akerib,S. Alsum,C. Aquino,Henrique Araujo,X. Bai,A. J. Bailey,J. Balajthy,P. Beltrame,Ethan Bernard,Ethan Bernard,Adam Bernstein,T. P. Biesiadzinski,T. P. Biesiadzinski,E. M. Boulton,E. M. Boulton,P. Brás,D. Byram,Sidney Cahn,M. C. Carmona-Benitez,C. Chan,A. A. Chiller,C. Chiller,A. Currie,J. E. Cutter,T. J. R. Davison,A. Dobi,J. E. Y. Dobson,E. Druszkiewicz,B. N. Edwards,C. H. Faham,S. R. Fallon,S. Fiorucci,S. Fiorucci,R. J. Gaitskell,V. M. Gehman,C. Ghag,K.R. Gibson,M. G. D. Gilchriese,C. R. Hall,M. Hanhardt,S. J. Haselschwardt,S. A. Hertel,D. P. Hogan,M. Horn,M. Horn,D. Q. Huang,C. M. Ignarra,R. G. Jacobsen,W. Ji,W. Ji,K. Kamdin,K. Kazkaz,D. Khaitan,R. Knoche,N. A. Larsen,Ching Hua Lee,Ching Hua Lee,B. G. Lenardo,B. G. Lenardo,K. T. Lesko,A. Lindote,M.I. Lopes,A. Manalaysay,R. L. Mannino,M. F. Marzioni,Daniel McKinsey,Daniel McKinsey,Daniel McKinsey,Dongming Mei,J. Mock,M. Moongweluwan,J. A. Morad,A. St. J. Murphy,C. Nehrkorn,H. N. Nelson,F. Neves,K. O’Sullivan,K. O’Sullivan,K. O’Sullivan,K. C. Oliver-Mallory,K. J. Palladino,K. J. Palladino,E. K. Pease,E. K. Pease,L. Reichhart,C. Rhyne,S. Shaw,T. A. Shutt,T. A. Shutt,C. Silva,M. Solmaz,V. N. Solovov,P. Sorensen,S. Stephenson,T. J. Sumner,Matthew Szydagis,D. J. Taylor,W. C. Taylor,B. P. Tennyson,P. A. Terman,D. R. Tiedt,W. H. To,W. H. To,Mani Tripathi,L. Tvrznikova,L. Tvrznikova,S. Uvarov,V. Velan,J.R. Verbus,R. C. Webb,J. T. White,T. J. Whitis,T. J. Whitis,M. S. Witherell,F.L.H. Wolfs,Jilei Xu,K. Yazdani,S. K. Young,Chao Zhang +119 more
TL;DR: The first searches for axions and axionlike particles with the Large Underground Xenon experiment are presented and the coupling constant between axion and electrons g_{Ae} is tested using data collected in 2013.