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Very Strong TeV Emission as $\gamma$-Ray Burst Afterglows
Gamma-ray bursts (GRBs) and following afterglows are considered to be produced by dissipation of kinetic energy of a relativistic fireball and radiation process is widely believed as synchrotron radiation or inverse Compton scattering of electrons. We argue that the transfer of kinetic energy of eje...
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| Lenguaje: | eng |
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1998
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| Acceso en línea: | https://dx.doi.org/10.1086/311489 http://cds.cern.ch/record/357129 |