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arXiv · hep-ph/9909286

Neutrino afterglow from Gamma-Ray Bursts: ~10^{18} eV

Eli Waxman·John Bahcall
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Abstract

We show that a significant fraction of the energy of a gamma-ray burst(GRB) is probably converted to a burst of 10^{17}-10^{19} eV neutrinos and multiple GeV gammas that follow the GRB by > 10 s . If, as previously suggested, GRB's accelerate protons to ~10^{20} eV, then both the neutrinos and the gammas may be detectable.

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Eli Waxman, John Bahcall. 2000-05-06. Neutrino afterglow from Gamma-Ray Bursts: ~10^{18} eV. https://doi.org/10.1086/309462

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