Physics
Scientific paper
Aug 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aipc.1358...59b&link_type=abstract
GAMMA RAY BURSTS 2010. AIP Conference Proceedings, Volume 1358, pp. 59-62 (2011).
Physics
Gamma-Rays, Telescopes, Spectral Analysis, Relativity, Gamma-Ray, X- And Gamma-Ray Telescopes And Instrumentation, Luminosities, Magnitudes, Effective Temperatures, Colors, And Spectral Classification, Relativity And Gravitation
Scientific paper
Using a time-dependent numerical model in which the prompt gamma-ray burst (GRB) emission is calculated in the framework of the internal shock model on a broad energy range (from soft X-ray to GeV energies), we compute GRB lightcurves and time-evolving spectra. We show how the spectral evolution in this model is determined by the evolution of the physical conditions in the shocked regions and by the dominant radiative process for the effective microphysics parameters. The predictions of a model are confronted by the observations in the standard sub-MeV energy range, as well as with high energy bands observed by Fermi.
Bosnjak Z.
Daigne Frederic
Dubus Guillaume
No associations
LandOfFree
Gamma-ray burst spectral evolution in the internal shock model: comparison with the observations does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Gamma-ray burst spectral evolution in the internal shock model: comparison with the observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gamma-ray burst spectral evolution in the internal shock model: comparison with the observations will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1738872