First Results of the LUX Dark Matter Experiment

First Results of the LUX Dark Matter Experiment
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DOI：
10.1016/j.nuclphysbps.2015.09.043
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发表时间：
2016-04
期刊：
Nuclear and Particle Physics Proceedings
影响因子：
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通讯作者：
M. Carmona-Benitez;D. Akerib;H. Araújo;X. Bai;A. Bailey;J. Balajthy;P. Beltrame;E. Bernard;A. Bernstein;A. Bradley;D. Byram;S. Cahn;C. Chan;J. Chapman;A. A. Chiller-A.;C. Chiller;A. Currie;L. D. Viveiros;A. Dobi;J. Dobson;E. Druszkiewicz;B. Edwards;C. Faham;S. Fiorucci;C. Flores;R. Gaitskell;V. Gehman;C. Ghag;K. Gibson;M. Gilchriese;C. Hall;M. Hanhardt;S. Haselschwardt;S. Hertel;M. Horn;D. Huang;M. Ihm;R. Jacobsen;K. Kazkaz;R. Knoche;N. Larsen;C. Lee;B. Lenardo;K. Lesko;A. Lindote;M. Lopes;D. Malling;A. Manalaysay;R. Mannino;D. McKinsey;D. Mei;J. Mock;M. Moongweluwan;J. Morad;A. Murphy;C. Nehrkorn;H. Nelson;F. Neves;R. Ott;M. Pangilinan;P. Parker;E. K. Pease;K. Pech;P. Phelps;L. Reichhart;T. Shutt;Catarina Silva;V. Solovov;P. Sorensen;K. O'Sullivan;T. Sumner;M. Szydagis;D. Taylor;B. Tennyson;D. Tiedt;M. Tripathi;L. Tvrznikova;S. Uvarov;J. Verbus;N. Walsh;R. Webb;J. White;M. Witherell;F. Wolfs;M. Woods;C. Zhang
M. Carmona-Benitez;D. Akerib;H. Araújo;X. Bai;A. Bailey;J. Balajthy;P. Beltrame;E. Bernard;A. Bernstein;A. Bradley;D. Byram;S. Cahn;C. Chan;J. Chapman;A. A. Chiller-A.;C. Chiller;A. Currie;L. D. Viveiros;A. Dobi;J. Dobson;E. Druszkiewicz;B. Edwards;C. Faham;S. Fiorucci;C. Flores;R. Gaitskell;V. Gehman;C. Ghag;K. Gibson;M. Gilchriese;C. Hall;M. Hanhardt;S. Haselschwardt;S. Hertel;M. Horn;D. Huang;M. Ihm;R. Jacobsen;K. Kazkaz;R. Knoche;N. Larsen;C. Lee;B. Lenardo;K. Lesko;A. Lindote;M. Lopes;D. Malling;A. Manalaysay;R. Mannino;D. McKinsey;D. Mei;J. Mock;M. Moongweluwan;J. Morad;A. Murphy;C. Nehrkorn;H. Nelson;F. Neves;R. Ott;M. Pangilinan;P. Parker;E. K. Pease;K. Pech;P. Phelps;L. Reichhart;T. Shutt;Catarina Silva;V. Solovov;P. Sorensen;K. O'Sullivan;T. Sumner;M. Szydagis;D. Taylor;B. Tennyson;D. Tiedt;M. Tripathi;L. Tvrznikova;S. Uvarov;J. Verbus;N. Walsh;R. Webb;J. White;M. Witherell;F. Wolfs;M. Woods;C. Zhang
中科院分区：
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文献类型：
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作者：
M. Carmona-Benitez;D. Akerib;H. Araújo;X. Bai;A. Bailey;J. Balajthy;P. Beltrame;E. Bernard;A. Bernstein;A. Bradley;D. Byram;S. Cahn;C. Chan;J. Chapman;A. A. Chiller-A.;C. Chiller;A. Currie;L. D. Viveiros;A. Dobi;J. Dobson;E. Druszkiewicz;B. Edwards;C. Faham;S. Fiorucci;C. Flores;R. Gaitskell;V. Gehman;C. Ghag;K. Gibson;M. Gilchriese;C. Hall;M. Hanhardt;S. Haselschwardt;S. Hertel;M. Horn;D. Huang;M. Ihm;R. Jacobsen;K. Kazkaz;R. Knoche;N. Larsen;C. Lee;B. Lenardo;K. Lesko;A. Lindote;M. Lopes;D. Malling;A. Manalaysay;R. Mannino;D. McKinsey;D. Mei;J. Mock;M. Moongweluwan;J. Morad;A. Murphy;C. Nehrkorn;H. Nelson;F. Neves;R. Ott;M. Pangilinan;P. Parker;E. K. Pease;K. Pech;P. Phelps;L. Reichhart;T. Shutt;Catarina Silva;V. Solovov;P. Sorensen;K. O'Sullivan;T. Sumner;M. Szydagis;D. Taylor;B. Tennyson;D. Tiedt;M. Tripathi;L. Tvrznikova;S. Uvarov;J. Verbus;N. Walsh;R. Webb;J. White;M. Witherell;F. Wolfs;M. Woods;C. Zhang

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LUX (Large Underground Xenon) is a dark matter direct detection experiment deployed at the 4850' level of the Sanford Underground Research Facility (SURF) in Lead, SD, operating a 370 kg dual-phase xenon TPC. Results of the first WIMP search run were presented in late 2013, for the analysis of 85.3 live-days with a fiducial volume of 118 kg, taken during the period of April to August 2013. The experiment exhibited a sensitivity to spin-independent WIMP-nucleon elastic scattering with a minimum upper limit on the cross section of 7.6×10−46cm2 at a WIMP mass of 33 GeV/c 2 , becoming the world's leading WIMP search result, in conflict with several previous claimed hints of discovery.