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arXiv · 1206.1694

Direct conversion of the flux of kinetic energy into radiation in gamma-ray burst

L. Zaninetti
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Abstract

The time evolution of a Gamma-ray burst (GRB) is associated with the evolution of a supernova remnant (SNR). The time evolution of the flux of a GRB is modeled introducing a law for the density of the medium in the advancing layer. The adopted radiative model for the GRB in the various e.m. frequencies is synchrotron emission. The X-ray ring which appears a few hours after a GRB is simulated.

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L. Zaninetti. 2012-06-08. Direct conversion of the flux of kinetic energy into radiation in gamma-ray burst. https://arxiv.org/abs/1206.1694

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