Abstract

We present the first experimental constraints on the spin-dependent WIMP-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 × 104 kg⋅ days1.4~\times~10^{4}~\text{kg}\cdot~\text{days} of fiducial exposure allows 90% CL upper limits to be set on the WIMP-neutron (WIMP-proton) cross section of σn = 9.4 × 10−41 cm2σ_n~=~9.4~\times~10^{-41}~\text{cm}^2 (σp = 2.9 × 10−39 cm2σ_p~=~2.9~\times~10^{-39}~\text{cm}^2) at 33 GeV/c2^2. The spin-dependent WIMP-neutron limit is the most sensitive constraint to date.

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