Direct conversion of the flux of kinetic energy into radiation in gamma-ray burst
classification
🌌 astro-ph.HE
keywords
evolutionburstfluxgamma-raytimeadoptedadvancingappears
read the original 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.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.