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Scientific paper
May 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..906...40m&link_type=abstract
GAMMA-RAY BURSTS: PROSPECTS FOR GLAST: Stockholm Symposium on GRB's. AIP Conference Proceedings, Volume 906, pp. 40-50 (2007).
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1
Gamma-Ray Sources, Gamma-Ray Bursts, Neutrino, Muon, Pion, And Other Elementary Particles, Cosmic Rays, X- And Gamma-Ray Sources, Mirrors, Gratings, And Detectors
Scientific paper
Gamma-ray bursts are thought to be capable of accelerating cosmic rays up to GZK energies Ep ~ 1020 eV, leading to a flux at Earth comparable to that observed by large EAS arrays such as AUGER. Both leptonic, e.g. synchrotron and inverse Compton, as well as photomeson processes can lead to GeV-TeV gamma-rays measurable by GLAST, AGILE, or ACTs, providing useful probes of the burst physics and model parameters. Photomeson interactions also produce neutrinos at energies ranging from sub-TeV to EeV, which will be probed with forthcoming experiments such as IceCube, ANITA and KM3NeT. This would provide information about the fundamental interaction physics, the acceleration mechanism, the nature of the sources and their environment.
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