Gamma-Ray Bursts
Abstract
Ultra-high-energy, >1019 eV, cosmic-ray and high energy, ~1014 eV, neutrino production in GRBs is discussed in the light of recent GRB and cosmic-ray observations. Emphasis is put on model predictions that can be tested with operating and planned cosmic-ray and neutrino detectors, and on the prospects of testing for neutrino properties.
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