Direct conversion of the flux of kinetic energy into radiation in gamma-ray burst
arXiv:1206.1694
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.
18 pages, 10 figures; published on Advanced Studies in Theoretical Physics 6, 529, (2012)