Observational Consequences of GRBs as Sources of Ultra High Energy Cosmic Rays

Details Observational Consequences of GRBs as Sources of Ultra High Energy Cosmic Rays Observational Consequences of GRBs as Sources of Ultra High Energy Cosmic Rays

2009-01-30

arxiv.org/abs/0901.4973v1

AIP Conf.Proc.1133:328-333,2009

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

6 pages and 4 figures. Contribution to the proceedings of the Huntsville GRB Symposium 2008

Scientific paper

10.1063/1.3155912

Gamma-ray bursts (GRBs) have long been considered as candidates of ultrahigh-energy cosmic rays (UHECRs). We investigate the signatures of CR proton acceleration in the GRBs by consistently taking into account their hadronic and electromagnetic interactions. We discuss the implications of our findings for high-energy gamma ray observations with the recently launched Fermi Gamma-ray Space Telescope.

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