Neural posterior estimation reconstructs neutrino energy, direction, and flavor from radio signals in ice detectors, reporting median resolutions of 0.30 log(E) and 18 sq deg (shallow) and 0.08 log(E) and 28 sq deg (deep) for NC events at 1 EeV.
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Collective nucleon scattering in neutron-star matter suppresses the effective absorption of ultralight bosons at the long wavelengths relevant for superradiance, weakening the link between stellar cooling bounds and superradiant instability rates.
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Event Reconstruction for Radio-Based In-Ice Neutrino Detectors with Neural Posterior Estimation
Neural posterior estimation reconstructs neutrino energy, direction, and flavor from radio signals in ice detectors, reporting median resolutions of 0.30 log(E) and 18 sq deg (shallow) and 0.08 log(E) and 28 sq deg (deep) for NC events at 1 EeV.
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Stellar Superradiance and Low-Energy Absorption in Dense Nuclear Media
Collective nucleon scattering in neutron-star matter suppresses the effective absorption of ultralight bosons at the long wavelengths relevant for superradiance, weakening the link between stellar cooling bounds and superradiant instability rates.