Showing 1–20 of 33 results
/ Date/ Name
Aug 22, 2024DUNE Phase II: Scientific Opportunities, Detector Concepts, Technological SolutionsAug 1, 2024First Measurement of the Total Inelastic Cross-Section of Positively-Charged Kaons on Argon at Energies Between 5.0 and 7.5 GeVJul 14, 2024Supernova Pointing Capabilities of DUNEApr 12, 2024Technical Design Report of the Spin Physics Detector at NICAMar 5, 2024Performance of a modular ton-scale pixel-readout liquid argon time projection chamberFeb 2, 2024Doping Liquid Argon with Xenon in ProtoDUNE Single-Phase: Effects on Scintillation LightDec 5, 2023The DUNE Far Detector Vertical Drift Technology, Technical Design ReportMar 29, 2023Impact of cross-section uncertainties on supernova neutrino spectral parameter fitting in the Deep Underground Neutrino ExperimentDec 19, 2022Highly-parallelized simulation of a pixelated LArTPC on a GPUNov 9, 2022Updated constraints on sterile neutrino mixing in the OPERA experiment using a new $ν_e$ identification methodNov 2, 2022Identification and reconstruction of low-energy electrons in the ProtoDUNE-SP detectorJun 29, 2022Reconstruction of interactions in the ProtoDUNE-SP detector with PandoraMar 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 SummaryJul 19, 2021Searching for solar KDAR with DUNEMar 25, 2021Deep Underground Neutrino Experiment (DUNE) Near Detector Conceptual Design ReportDec 23, 2019First observation of a tau neutrino charged current interaction with charm production in the Opera experimentApr 11, 2019Final results on neutrino oscillation parameters from the OPERA experiment in the CNGS beam