Comparisons between analytic and numerical calculations of GRB spectra

被引:0
|
作者
Dermer, CD [1 ]
Böttcher, M [1 ]
Chiang, J [1 ]
机构
[1] USN, Res Lab, Washington, DC 20375 USA
来源
GAMMA-RAY BURSTS | 2000年 / 526卷
关键词
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Formulas of Sari, Piran, and Narayan for the spectral energy distributions of gamma-ray burst blast waves are extended to include synchrotron self-absorption and Compton scattering and, given a simple numerical integration, to apply to general radiative regimes. The expressions are compared with detailed numerical simulation results and are most accurate (within a factor of similar to 3) in the optical/X-ray regime during the afterglow phase. Comparison of spectral energy distributions are made for the parameters used by Wijers and Galama to fit GRB 970508.
引用
收藏
页码:470 / 474
页数:5
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