Quasi-elastic neutrino-nucleus scattering produces an azimuthal asymmetry in outgoing nucleons due to weak parity violation, sensitive to nuclear modeling and observable with O(10^4) events on carbon.
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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.
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Azimuthal asymmetry in exclusive quasi-elastic neutrino-nucleus interactions
Quasi-elastic neutrino-nucleus scattering produces an azimuthal asymmetry in outgoing nucleons due to weak parity violation, sensitive to nuclear modeling and observable with O(10^4) events on carbon.
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Continuum contribution to charged-current absorption of low-energy $\nu_e$ on $^{40}$Ar
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.