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An Effective Field Theory Analysis of the First LUX Dark Matter Search

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arxiv 2003.11141 v1 pith:D7NGM4I6 submitted 2020-03-24 astro-ph.CO

An Effective Field Theory Analysis of the First LUX Dark Matter Search

classification astro-ph.CO
keywords searchfirstspin-independentcouplingsdarkeffectivefieldmass
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The Large Underground Xenon (LUX) dark matter search was a 250-kg active mass dual-phase time projection chamber that operated by detecting light and ionization signals from particles incident on a xenon target. In December 2015, LUX reported a minimum 90% upper C.L. of 6e-46 cm^2 on the spin-independent WIMP-nucleon elastic scattering cross section based on a 1.4e4 kg*day exposure in its first science run. Tension between experiments and the absence of a definitive positive detection suggest it would be prudent to search for WIMPs outside the standard spin-independent/spin-dependent paradigm. Recent theoretical work has identified a complete basis of 14 independent effective field theory (EFT) operators to describe WIMP-nucleon interactions. In addition to spin-independent and spin-dependent nuclear responses, these operators can produce novel responses such as angular-momentum-dependent and spin-orbit couplings. Here we report on a search for all 14 of these EFT couplings with data from LUX's first science run. Limits are placed on each coupling as a function of WIMP mass.

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