The Non-Thermal High Energy Emission from GRBs - Theoretical Predictions

Details The Non-Thermal High Energy Emission from GRBs - Theoretical Predictions The Non-Thermal High Energy Emission from GRBs - Theoretical Predictions

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ebhe.conf..136n&link_type=abstract

ENERGY BUDGET IN THE HIGH ENERGY UNIVERSE . Proceedings of the International Workshop. Held 22-24 February 2006 in Kashiwa, Japa

Physics

Scientific paper

Gamma-Ray bursts (GRBs) are considered to be one of the most promising
sources of ultra-high energy cosmic rays (UHECRs), detectable neutrino
flux and bright GeV photons. Here I briefly review the theoretical
predictions for the production of these types of emission in GRBs.

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