Astronomy and Astrophysics – Astrophysics
Scientific paper
1999-11-21
Phys.Scripta T85 (2000) 117-126
Astronomy and Astrophysics
Astrophysics
Physica Scripta, in press; Talk presented at the Nobel Symposium: Particle Physics and The Universe (Sweden, August 1998)
Scientific paper
10.1238/Physica.Topical.085a0011
The recent detection of delayed, low energy emission from Gamma-Ray Burst (GRB) sources confirmed the cosmological origin of the bursts and provided support for models where GRBs are produced by the dissipation of the kinetic energy of relativistic fireballs. In this review, ultra high energy, >10^{19} eV, cosmic-ray and high energy, 100 TeV, 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. The predicted neutrino intensity, E^2 dN/dE=3\times 10^{-9} GeV/(cm^2 s sr) for 10^{14} eV
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