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Very high energy phenomena in GRBs
Reviews production of very high energy particles and expected radiations from them in the standard relativistic blastwave model of GRBs. Electrons and protons can be accelerated in the internal shock of GRBs up to ~10/sup 14/ and 10/sup 20/ eV, respectively, and GRBs are one of the possible sites of...
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| Lenguaje: | eng |
| Publicado: |
2001
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| Acceso en línea: | http://cds.cern.ch/record/516219 |