4.8 Article

Limits on Spin-Dependent WIMP-Nucleon Cross Section Obtained from the Complete LUX Exposure

期刊

PHYSICAL REVIEW LETTERS
卷 118, 期 25, 页码 -

出版社

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevLett.118.251302

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资金

  1. U.S. Department of Energy (DOE) [DE-AC02-05CH11231, DE-AC05-06OR23100, DE-AC52-07NA27344, DE-FG01-91ER40618, DE-FG02-08ER41549, DE-FG02-11ER41738, DE-FG02-91ER40674, DE-FG02-91ER40688, DE-FG02-95ER40917, DE-NA0000979, DE-SC0006605, DE-SC0010010, DE-SC0015535]
  2. U.S. National Science Foundation [PHY-0750671, PHY-0801536, PHY-1003660, PHY-1004661, PHY-1102470, PHY-1312561, PHY-1347449, PHY-1505868, PHY-1636738]
  3. Research Corporation Grant [RA0350]
  4. Center for Ultra-low Background Experiments in the Dakotas (CUBED)
  5. South Dakota School of Mines and Technology (SDSMT)
  6. Fundacao para a Ciencia e a Tecnologia (FCT) [PTDC/FIS-NUC/1525/2014]
  7. Imperial College London, University College London
  8. Edinburgh University
  9. Science and Technology Facilities Council for PhD studentships [ST/K502042/1, ST/K502406/1, ST/M503538/1]
  10. U.S. Department of Energy (DOE) [DE-SC0015535] Funding Source: U.S. Department of Energy (DOE)
  11. Science and Technology Facilities Council [ST/K502406/1, ST/K502042/1, ST/M503538/1] Funding Source: researchfish
  12. Direct For Mathematical & Physical Scien
  13. Division Of Physics [1636738] Funding Source: National Science Foundation
  14. STFC [ST/M503538/1, ST/M003744/1, ST/K502406/1, ST/K502042/1, ST/K003208/1] Funding Source: UKRI

向作者/读者索取更多资源

We present experimental constraints on the spin-dependentWIMP- nucleon elastic cross sections from the total 129.5 kg yr exposure acquired by the Large Underground Xenon experiment (LUX), operating at the Sanford Underground Research Facility in Lead, South Dakota (USA). A profile likelihood ratio analysis allows 90% C.L. upper limits to be set on the WIMP-neutron (WIMP-proton) cross section of sigma(n) = 1.6 x 10(-41) cm(2) (sigma(p) 5 x 10(-40) cm(2)) at 35 GeVc(-2), almost a sixfold improvement over the previous LUX spin-dependent results. The spin-dependent WIMP-neutron limit is the most sensitive constraint to date.

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