Solar neutrinos enable self-calibration of the ν_e + 40Ar cross section to ≲2% in 9-15 MeV via known 8B flux, survival probability, and distinctive Fermi/Gamow-Teller angular distributions.
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Proposes using solar ^8B and muon-decay-at-rest neutrinos as calibration sources to constrain the ν_e-Ar cross section and reduce nuclear model bias in DUNE supernova neutrino detection.
Joint analysis of neutrino detectors and CMB observables can constrain dark matter annihilation into neutrinos for MeV-GeV masses.
Hybrid HF-CRPA calculations predict lower allowed cross sections for charged-current ν_e on 40Ar at low energies, leading to ~20% fewer events in DUNE for a galactic supernova burst than the prior MARLEY model.
Fluka simulation of neutron-induced light in a small LArTPC matches experimental data in photoelectron count and decay time constant.
citing papers explorer
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Self-Calibration of the Neutrino-Argon Cross Section with Solar Neutrinos
Solar neutrinos enable self-calibration of the ν_e + 40Ar cross section to ≲2% in 9-15 MeV via known 8B flux, survival probability, and distinctive Fermi/Gamow-Teller angular distributions.
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Standard Candles for Supernova Neutrino Detection at DUNE
Proposes using solar ^8B and muon-decay-at-rest neutrinos as calibration sources to constrain the ν_e-Ar cross section and reduce nuclear model bias in DUNE supernova neutrino detection.
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Joint probes of dark matter annihilation from neutrino detectors and CMB targets
Joint analysis of neutrino detectors and CMB observables can constrain dark matter annihilation into neutrinos for MeV-GeV masses.
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Modeling Light Signals Using Data from the First Pulsed Neutron Source Program at the DUNE Vertical Drift ColdBox Test Facility at CERN Neutrino Platform
Fluka simulation of neutron-induced light in a small LArTPC matches experimental data in photoelectron count and decay time constant.