A new up-down flux ratio for sub-GeV atmospheric neutrinos enables Hyper-Kamiokande to measure the CP-violating phase with sensitivity surpassing T2HK near delta_CP of 90 and 270 degrees.
Abeet al.,Measurements of neutrino oscillation parameters from the T2K experiment using3.6×10 21 protons on target, Eur
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ICARUS measures flux-averaged differential CCQE-like cross sections in lepton angle, lepton-proton opening angle, and transverse kinematic imbalance variables, finding agreement with event generator predictions within current uncertainties.
Liquid scintillator detectors of a few kilotons can probe the CP-violating phase in atmospheric neutrino oscillations via rate, spectrum, and zenith-angle distributions analyzed with Poisson likelihood.
Dark dimension right-handed neutrino models are confronted with T2K and NOvA long-baseline oscillation data, yielding exclusion limits on model parameters while remaining compatible with standard three-neutrino oscillations.
citing papers explorer
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Towards Measuring the CP-Violating Phase with Atmospheric Neutrinos
A new up-down flux ratio for sub-GeV atmospheric neutrinos enables Hyper-Kamiokande to measure the CP-violating phase with sensitivity surpassing T2HK near delta_CP of 90 and 270 degrees.
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Measurement of muon (anti-)neutrino charged-current quasielastic-like cross section using off-axis NuMI beam at ICARUS
ICARUS measures flux-averaged differential CCQE-like cross sections in lepton angle, lepton-proton opening angle, and transverse kinematic imbalance variables, finding agreement with event generator predictions within current uncertainties.
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The sensitivity of liquid scintillator detectors to CP-violation with atmospheric neutrinos
Liquid scintillator detectors of a few kilotons can probe the CP-violating phase in atmospheric neutrino oscillations via rate, spectrum, and zenith-angle distributions analyzed with Poisson likelihood.
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Dark Dimension Right-handed Neutrinos Confronted with Long-Baseline Oscillation Experiments
Dark dimension right-handed neutrino models are confronted with T2K and NOvA long-baseline oscillation data, yielding exclusion limits on model parameters while remaining compatible with standard three-neutrino oscillations.