Probing the Emission Sites of GRBs
| dc.creator | Papathanassiou, H. | |
| dc.date | 1998-10-05 | |
| dc.date.accessioned | 2026-07-07T02:28:13Z | |
| dc.date.available | 2026-07-07T02:28:13Z | |
| dc.description | I present a computationally efficient way to account for synchrotron and its inverse Compton scattered emission along with the resulting radiative losses, in a self-consistent way, for a relativistic distribution of electrons continuously injected in an expanding region. This approach permits the exploration of the wide parameter space of the physical processes in a shock. I apply it to the picture of ``internal shocks'' for the description of Gamma Ray Bursts. I use the properties of the time-integrated spectra as defined mainly by observations by BATSE, EGRET, and Ginga to impose constrains on the parameter space. I discuss the corresponding shock properties and one of the ways in which INTEGRAL can provide further insight. | |
| dc.description | 4 pages, submitted to Proc. of the 3rd INTEGRAL Workshop: The Etxreme Universe | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9810068 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9810068 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/13031 | |
| dc.subject | Astrophysics | |
| dc.title | Probing the Emission Sites of GRBs | |
| dc.type | text |