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|a (TOE)ost1257741
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|a SLAC-PUB-16557
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|a LLNL-JRNL-833845
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|a Results on the spin-dependent scattering of weakly interacting massive particles on nucleons from the Run 3 Data of the LUX Experiment
|h [electronic resource]
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|a Washington, D.C. :
|b United States. Department of Energy. Office of High Energy Physics ;
|a Oak Ridge, Tenn. :
|b Distributed by the Office of Scientific and Technical Information, U.S. Department of Energy,
|c 2016.
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| 300 |
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|a Size: Article No. 161302 :
|b digital, PDF file.
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|a text
|b txt
|2 rdacontent.
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|a computer
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|2 rdamedia.
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|a online resource
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|a Published through Scitech Connect.
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|a 04/20/2016.
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|a "SLAC-PUB-16557."
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|a "LLNL-JRNL-833845."
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|a "Journal ID: ISSN 0031-9007."
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|a "PRLTAO."
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|a Akerib, D. S. ;
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|a SLAC National Accelerator Lab., Menlo Park, CA (United States)
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|a Univ. of California, Santa Barbara, CA (United States)
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3 |
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|a Here, we present experimental constraints on the spin-dependent WIMP (weakly interacting massive particle)-nucleon elastic cross sections from LUX data acquired in 2013. LUX is a dual-phase xenon time projection chamber operating at the Sanford Underground Research Facility (Lead, South Dakota), which is designed to observe the recoil signature of galactic WIMPs scattering from xenon nuclei. A profile likelihood ratio analysis of 1.4 × 10<sup>4</sup> kg day of fiducial exposure allows 90% C.L. upper limits to be set on the WIMP-neutron (WIMP-proton) cross section of ?<sub>n</sub> = 9.4 × 10<sup>?41</sup> cm<sup>2</sup> (?<sub>p</sub> = 2.9 × 10<sup>?39</sup> cm<sup>2</sup>) at 33 GeV/c<sup>2</sup>. The spin-dependent WIMP-neutron limit is the most sensitive constraint to date.
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|b AC02-76SF00515.
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|b AC52-07NA27344.
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|b RA0350.
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|b PTDC/FIS-NUC/1525/2014.
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|a 72 physics of elementary particles and fields
|2 local.
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|a 79 astronomy and astrophysics
|2 local.
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|a Particle dark matter
|2 local.
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|a Weakly interacting massive particles
|2 local.
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|a Dark matter detectors
|2 local.
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|a Timeprojection chambers
|2 local.
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|a Physics of elementary particles and fields
|2 local.
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|a Astronomy and astrophysics
|2 local.
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|a Time-projection chambers
|2 local.
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|a Lawrence Berkeley National Laboratory.
|4 res.
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|a Lawrence Livermore National Laboratory.
|4 res.
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| 710 |
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|a United States.
|b Department of Energy.
|b Office of High Energy Physics.
|4 spn.
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| 710 |
2 |
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|a National Science Foundation (U.S.).
|4 spn.
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2 |
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|a Stanford Linear Accelerator Center.
|f res.
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| 710 |
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|a United States.
|b Department of Energy.
|b Office of Scientific and Technical Information
|4 dst.
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|u https://www.osti.gov/servlets/purl/1257741
|z Full Text (via OSTI)
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|a .b91186213
|b 02-20-23
|c 05-12-17
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|a web
|b 12-08-22
|c f
|d m
|e p
|f eng
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|h 0
|i 3
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|a Information bridge
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|s 7f60e02f-0191-526e-b5a3-95d5b18ed290
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| 952 |
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|p Can circulate
|a University of Colorado Boulder
|b Online
|c Online
|d Online
|e E 1.99:LLNL-JRNL-833845
|h Superintendent of Documents classification
|i web
|n 1
|
