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First results from the LUX dark matter experiment at the Sanford underground research facility.
TLDR
The first WIMP search data set is reported, taken during the period from April to August 2013, presenting the analysis of 85.3 live days of data, finding that the LUX data are in disagreement with low-mass W IMP signal interpretations of the results from several recent direct detection experiments. Expand
Results from a Search for Dark Matter in the Complete LUX Exposure.
TLDR
This search yields no evidence of WIMP nuclear recoils and constraints on spin-independent weakly interacting massive particle (WIMP)-nucleon scattering using a 3.35×10^{4}  kg day exposure of the Large Underground Xenon experiment are reported. Expand
Improved Limits on Scattering of Weakly Interacting Massive Particles from Reanalysis of 2013 LUX Data.
TLDR
This new analysis incorporates several advances: single-photon calibration at the scintillation wavelength, improved event-reconstruction algorithms, a revised background model including events originating on the detector walls in an enlarged fiducial volume, and new calibrations from decays of an injected tritium β source and from kinematically constrained nuclear recoils down to 1.1 keV. Expand
First results from the XENON10 dark matter experiment at the Gran Sasso National Laboratory.
TLDR
A blind analysis of 58.6 live days of data excludes previously unexplored parameter space, setting a new 90% C.L. upper limit for the WIMP-nucleon spin-independent cross section of 8.8x10(-44) cm2 for a W IMP mass of 100 GeV/c2, which further constrains predictions of supersymmetric models. Expand
Search for light dark matter in XENON10 data.
TLDR
The data strongly constrain recent elastic dark matter interpretations of excess low-energy events observed by CoGeNT and CRESST-II, as well as the DAMA annual modulation signal. Expand
Limits on spin-dependent WIMP-nucleon cross sections from the XENON10 experiment.
TLDR
XENON10 is an experiment to directly detect weakly interacting massive particles (WIMPs), which may comprise the bulk of the nonbaryonic dark matter in the authors' Universe, and excludes previously unexplored regions in the theoretically allowed parameter space for neutralinos. Expand
The Large Underground Xenon (LUX) experiment
The Large Underground Xenon (LUX) collaboration has designed and constructed a dual-phase xenon detector, in order to conduct a search for Weakly Interacting Massive Particles (WIMPs), a leading darkExpand
Results on the Spin-Dependent Scattering of Weakly Interacting Massive Particles on Nucleons from the Run 3 Data of the LUX Experiment.
TLDR
The spin-dependent WIMP-neutron limit is the most sensitive constraint to date. Expand
Scintillation efficiency and ionization yield of liquid xenon for monoenergetic nuclear recoils down to 4 keV
Liquid xenon (LXe) is an excellent material for experiments designed to detect dark matter in the form of weakly interacting massive particles (WIMPs). A low energy detection threshold is essentialExpand
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