Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-12-06
Astronomy and Astrophysics
Astrophysics
12 pages, 5 figures, in proceedings of conference "Towards a Network of Atmospheric Cherenkov Detectors VII," 27-29 April, 200
Scientific paper
Gamma-ray bursts are known to be sources of high-energy gamma rays, and are likely to be sources of high-energy cosmic rays and neutrinos. Following a short review of observations of GRBs at multi-MeV energies and above, the physics of leptonic and hadronic models of GRBs is summarized. Evidence for two components in BATSE and EGRET/TASC data suggest that GRBs are sources of high-energy cosmic rays. GLAST observations will reveal the high-energy gamma-ray power and energy releases from GRBs, and will provide detailed knowledge of anomalous high-energy emission components, but confirmation of cosmic ray acceleration must await 100 TeV -- PeV neutrino detection from GRBs.
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