Results on the Spin-Dependent Scattering of Weakly Interacting Massive Particles on Nucleons from the Run 3 Data of the LUX Experiment.

نویسندگان

  • D S Akerib
  • H M Araújo
  • X Bai
  • A J Bailey
  • J Balajthy
  • P Beltrame
  • E P Bernard
  • A Bernstein
  • T P Biesiadzinski
  • E M Boulton
  • A Bradley
  • R Bramante
  • S B 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
  • D N 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
  • M Szydagis
  • D J Taylor
  • W Taylor
  • B P Tennyson
  • P A Terman
  • D R Tiedt
  • W H To
  • M 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
  • S K Young
  • C Zhang
چکیده

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^{4}  kg day of fiducial exposure allows 90% C.L. upper limits to be set on the WIMP-neutron (WIMP-proton) cross section of σ_{n}=9.4×10^{-41}  cm^{2} (σ_{p}=2.9×10^{-39}  cm^{2}) at 33  GeV/c^{2}. The spin-dependent WIMP-neutron limit is the most sensitive constraint to date.

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عنوان ژورنال:
  • Physical review letters

دوره 116 16  شماره 

صفحات  -

تاریخ انتشار 2016