Showing 121–140 of 280 results
/ Date/ Name
Mar 12, 2023Measurement of electrons from open heavy-flavor hadron decays in Au+Au collisions at $\sqrt{s_{\rm NN}}=200$ GeV with the STAR detectorDec 19, 2022Highly-parallelized simulation of a pixelated LArTPC on a GPUNov 30, 2022Background Determination for the LUX-ZEPLIN (LZ) Dark Matter ExperimentNov 14, 2022Search for boosted keV-MeV light dark matter particles from evaporating primordial black holes at the CDEX-10 experimentNov 2, 2022Identification and reconstruction of low-energy electrons in the ProtoDUNE-SP detectorOct 4, 2022Search for exotic interactions of solar neutrinos in the CDEX-10 experimentSep 2, 2022Exotic Dark Matter Search with CDEX-10 Experiment at China's Jinping Underground LaboratoryAug 1, 2022Pion, kaon, and (anti-)proton production in U+U Collisions at $\sqrt{s_{NN}}$ = 193 GeV measured with the STAR detectorJul 8, 2022First Dark Matter Search Results from the LUX-ZEPLIN (LZ) ExperimentJul 2, 2022Measurement of $\rm ^4_ΛH$ and $\rm ^4_ΛHe$ binding energy in Au+Au collisions at $\sqrt{s_\mathrm{NN}}$ = 3 GeVJun 29, 2022Reconstruction of interactions in the ProtoDUNE-SP detector with PandoraJun 8, 2022Constraints on Sub-GeV Dark Matter--Electron Scattering from the CDEX-10 ExperimentMay 24, 2022Azimuthal transverse single-spin asymmetries of inclusive jets and identified hadrons within jets from polarized $pp$ collisions at $\sqrt{s}$ = 200 GeVMay 22, 2022Search for Neutrinoless Double-Beta Decay of $^{76}$Ge with a Natural Broad Energy Germanium DetectorMar 31, 2022Separation of track- and shower-like energy deposits in ProtoDUNE-SP using a convolutional neural networkMar 30, 2022Scintillation light detection in the 6-m drift-length ProtoDUNE Dual Phase liquid argon TPCMar 11, 2022A Gaseous Argon-Based Near Detector to Enhance the Physics Capabilities of DUNEMar 11, 2022Snowmass Neutrino Frontier: DUNE Physics SummaryMar 4, 2022A Next-Generation Liquid Xenon Observatory for Dark Matter and Neutrino PhysicsJan 8, 2022Cosmogenic production of $^{37}$Ar in the context of the LUX-ZEPLIN experiment