The origin of the prompt GRB spectrum
arXiv:0912.3743
Abstract
Using a detailed model of the internal shock phase, we discuss the origin of the prompt emission in gamma-ray bursts. We focus on the identification of the dominant radiative process (Fermi-GBM range) and propose an explanation for some features observed by Fermi-LAT at high energy in some GRB lightcurves.
2009 Fermi Symposium, eConf Proceedings C091122;