X-ray Rich GRB, Photospheres and Variability
arXiv:astro-ph/0205144 · doi:10.1086/342611
Abstract
We investigate the relationship between the quasi-thermal baryon-related photosphere in relativistic outflows, and the internal shocks arising outside them, which out to a limiting radius may be able to create enough pairs to extend the optically thick region. Variable gamma-ray light curves are likely to arise outside this limiting pair-forming shock radius, while X-ray excess bursts may arise from shocks occurring below it; a possible relation to X-ray flashes is discussed. This model leads to a simple physical interpretation of the observational gamma-ray variability-luminosity relation.
accepted in Ap.J. 6/20/02; subm 5/8/02; aaspp4, 12 pages, 1 fig