X
X. Bai
Researcher at South Dakota School of Mines and Technology
Publications - 260
Citations - 18345
X. Bai is an academic researcher from South Dakota School of Mines and Technology. The author has contributed to research in topics: Neutrino & IceCube Neutrino Observatory. The author has an hindex of 60, co-authored 247 publications receiving 15742 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
Results from a Search for Dark Matter in the Complete LUX Exposure
D. S. Akerib,S. Alsum,Henrique Araujo,X. Bai,A. J. Bailey,J. Balajthy,P. Beltrame,Ethan Bernard,A. Bernstein,T. P. Biesiadzinski,E. M. Boulton,R. Bramante,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. 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,D. Q. Huang,C. M. Ignarra,M. Ihm,R.G. Jacobsen,W. Ji,K. Kamdin,K. Kazkaz,D. Khaitan,R. Knoche,N.A. Larsen,C. Lee,B. G. Lenardo,K. T. Lesko,A. Lindote,M.I. Lopes,A. Manalaysay,R. L. Mannino,M. F. Marzioni,Daniel McKinsey,D. M. Mei,J. Mock,M. Moongweluwan,J. A. Morad,A. St. J. Murphy,C. Nehrkorn,H. N. Nelson,F. Neves,K. O’Sullivan,K. C. Oliver-Mallory,K. J. Palladino,E. K. Pease,P. Phelps,L. Reichhart,C. Rhyne,S. Shaw,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,S. Uvarov,J.R. Verbus,R. C. Webb,J. T. White,T. J. Whitis,M. S. Witherell,F.L.H. Wolfs,Jilei Xu,K. Yazdani,Sarah Young,Chao Zhang +100 more
TL;DR: This search yields no evidence of WIMP nuclear recoils and constraints on spin-independent weakly interacting massive particle (WIMP)-nucleon scattering using a 3.35×10^{4} kg day exposure of the Large Underground Xenon experiment are reported.
Journal ArticleDOI
Evidence for High-Energy Extraterrestrial Neutrinos at the IceCube Detector
M. G. Aartsen,Rasha Abbasi,Y. Abdou,Markus Ackermann,Jenni Adams,Juanan Aguilar,Markus Ahlers,D. Altmann,J. Auffenberg,X. Bai,Michael J. Baker,S. W. Barwick,V. Baum,R. C. Bay,J. J. Beatty,S. Bechet,J. Becker Tjus,K.-H. Becker,M. L. Benabderrahmane,Segev BenZvi,P. Berghaus,D. Berley,Elisa Bernardini,A. Bernhard,D. Bertrand,D. Z. Besson,Gary Binder,Gary Binder,Daniel Bindig,M. Bissok,E. Blaufuss,J. Blumenthal,D. J. Boersma,S. Bohaichuk,C. Bohm,D. Bose,S. Böser,Olga Botner,L. Brayeur,H.-P. Bretz,A. M. Brown,R. Bruijn,Jürgen Brunner,M. J. Carson,J. Casey,M. Casier,Dmitry Chirkin,A. Christov,B. Christy,K. Clark,F. Clevermann,S. Coenders,Seth M. Cohen,D. F. Cowen,A. H. Cruz Silva,M. Danninger,J. Daughhetee,J. C. Davis,M. Day,C. De Clercq,S. De Ridder,Paolo Desiati,K. D. de Vries,Tyce DeYoung,Juan Carlos Diaz-Velez,Matt Dunkman,R. Eagan,B. Eberhardt,B. Eichmann,J. Eisch,R. W. Ellsworth,S. Euler,Paul Evenson,O. Fadiran,A. R. Fazely,Anatoli Fedynitch,J. Feintzeig,T. Feusels,Kirill Filimonov,Chad Finley,T. Fischer-Wasels,S. Flis,A. Franckowiak,K. Frantzen,T. Fuchs,Thomas K. Gaisser,J. C. Gallagher,L. Gerhardt,L. Gerhardt,L. Gladstone,Thorsten Glusenkamp,A. Goldschmidt,G. Golup,J. G. Gonzalez,J. A. Goodman,Dariusz Gora,Dylan T. Grandmont +96 more
TL;DR: The presence of a high-energy neutrino flux containing the most energetic neutrinos ever observed is revealed, including 28 events at energies between 30 and 1200 TeV, although the origin of this flux is unknown and the findings are consistent with expectations for a neutRino population with origins outside the solar system.
Journal ArticleDOI
Improved limits on scattering of weakly interacting massive particles from reanalysis of 2013 LUX data
D. S. Akerib,Henrique Araujo,X. Bai,A. J. Bailey,J. Balajthy,P. Beltrame,Ethan Bernard,A. Bernstein,T. P. Biesiadzinski,E. M. Boulton,A. W. Bradley,R. Bramante,Sidney Cahn,M. C. Carmona-Benitez,C. Chan,J.J. Chapman,A.A. Chiller,C. Chiller,A. Currie,J. E. Cutter,T. J. R. Davison,L. de Viveiros,A. Dobi,J. E. Y. Dobson,E. Druszkiewicz,B. N. Edwards,C. H. Faham,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,D. Q. Huang,C. M. Ignarra,M. Ihm,R.G. Jacobsen,W. Ji,K. Kazkaz,D. Khaitan,R. Knoche,N.A. Larsen,C. Lee,B. G. Lenardo,K. T. Lesko,A. Lindote,M.I. Lopes,D.C. Malling,A. Manalaysay,R. L. Mannino,M. F. Marzioni,Daniel McKinsey,D. M. Mei,J. Mock,M. Moongweluwan,J. A. Morad,A. St. J. Murphy,C. Nehrkorn,H. N. Nelson,F. Neves,K. O'Sullivan,K. C. Oliver-Mallory,R. A. Ott,K. J. Palladino,M. Pangilinan,E. K. Pease,P. Phelps,L. Reichhart,C. Rhyne,S. Shaw,T. A. Shutt,C. Silva,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,S. Uvarov,J.R. Verbus,R. C. Webb,J. T. White,T. J. Whitis,M. S. Witherell,F.L.H. Wolfs,K. Yazdani,Sarah Young,Chao Zhang +100 more
TL;DR: This new analysis incorporates several advances: single-photon calibration at the scintillation wavelength, improved event-reconstruction algorithms, a revised background model including events originating on the detector walls in an enlarged fiducial volume, and new calibrations from decays of an injected tritium β source and from kinematically constrained nuclear recoils down to 1.1 keV.
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.