Collisional mechanism for GRB emission

Monthly Notices of the Royal Astronomical Society, no. 2 (2010): 1033-1047

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Nuclear and Coulomb collisions in gamma-ray burst (GRB) jets create a hot e± plasma. This collisional heating starts when the jet is still opaque, and extends to the transparent region. The e± plasma radiates its energy. As a result, a large fraction of the jet energy is converted to escaping radiation with a well-defined spectrum. The pr...更多

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