Gamma-ray burst models with general dynamics and fits to Fermi LAT bursts
classification
🌌 astro-ph.HE
keywords
arisesaroundburstsemissiongamma-raygeneralmodelphotospheric
read the original abstract
We present a dissipative photospheric model for gamma-ray bursts where the usual Band peak around MeV energies arises as synchrotron emission from around the photosphere. We treat the initial acceleration in a general way and the GeV emission arises as the interaction of photospheric radiation and the shocked electrons at the deceleration radius. We show some applications of this model.
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.