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arXiv · hep-ph/0004102

Gamma-Ray Bursts

E. Waxman
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Abstract

Ultra-high-energy, >10^19 eV, cosmic-ray and high energy, ~10^14 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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E. Waxman. 2000-04-11. Gamma-Ray Bursts. https://doi.org/10.1142/9789812792433_0061

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