Showing 1–20 of 24 results
/ Date/ Name
Apr 23, 2026Precision measurement of positron decay modes of Xe-125 in the LUX-ZEPLIN experimentMar 27, 2026Pushing the Limits of Pulse Shape Discrimination in a Large Liquid Xenon DetectorFeb 24, 2026Low-Energy Radon Backgrounds from Electrode Grids in Dual-Phase Xenon TPCsFeb 18, 2026Measurement of the Muon Flux at the Sanford Underground Research Facility with the LUX-ZEPLIN Dark Matter DetectorDec 8, 2025Searches for Light Dark Matter and Evidence of Coherent Elastic Neutrino-Nucleus Scattering of Solar Neutrinos with the LUX-ZEPLIN (LZ) ExperimentNov 21, 2025Search for New Physics via Low-Energy Electron Recoils with a 4.2 Tonne\times Year Exposure from the LZ ExperimentOct 7, 2025Study of few-electron backgrounds in the LUX-ZEPLIN detectorSep 18, 2025Low-energy nuclear recoil calibration of the LUX-ZEPLIN experiment with a photoneutron sourceAug 26, 2025Flow-dependent tagging of $^{214}$Pb decays in the LZ dark matter detectorMar 23, 2025New constraints on cosmic ray-boosted dark matter from the LUX-ZEPLIN experimentMar 7, 2025Measurements and models of enhanced recombination following inner-shell vacancies in liquid xenonDec 6, 2024First constraint for atmospheric millicharged particles with the LUX-ZEPLIN experimentOct 23, 2024Neutrinoless Double Beta Decay Sensitivity of the XLZD Rare Event ObservatoryOct 22, 2024The XLZD Design Book: Towards the Next-Generation Liquid Xenon Observatory for Dark Matter and Neutrino PhysicsOct 22, 2024Dark Matter Search Results from 4.2 Tonne-Years of Exposure of the LUX-ZEPLIN (LZ) ExperimentAug 30, 2024Two-neutrino double electron capture of $^{124}$Xe in the first LUX-ZEPLIN exposureJun 4, 2024Probing the Scalar WIMP-Pion Coupling with the first LUX-ZEPLIN dataMay 23, 2024The Data Acquisition System of the LZ Dark Matter Detector: FADRMay 2, 2024The Design, Implementation, and Performance of the LZ Calibration SystemsApr 26, 2024Constraints On Covariant WIMP-Nucleon Effective Field Theory Interactions from the First Science Run of the LUX-ZEPLIN Experiment