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

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

1999-09-08

arxiv.org/abs/hep-ph/9909286v2

Astrophys.J.541:707-711,2000

Physics

High Energy Physics

High Energy Physics - Phenomenology

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

Scientific paper

10.1086/309462

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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