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

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.

Accepted ApJ; added sentence re: sterile neutrinos; related material at http://www.sns.ias.edu/~jnb

References in corpus (2)

• Wind Interaction Models for Gamma-Ray Burst Afterglows: The Case for Two Types of Progenitors
• High energy cosmic-rays and neutrinos from cosmological gamma-ray burst fireballs

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