Self-consistent cooling and synchrotron-self-compton emission of relativistic electrons in gamma-ray bursts

被引：0
|
作者：
Derishev, EV [1 ]
Kocharovsky, VV [1 ]
Kocharovsky, VV [1 ]
机构：
[1] Russian Acad Sci, Inst Appl Phys, Nizhnii Novgorod 603600, Russia
来源：
COSMOLOGY AND PARTICLE PHYSICS | 2001年 / 555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：
The spectra of Gamma-Ray Burst (GRB) emission have been investigated theoretically by a number of authors (e.g., [1-3]) for different versions of a general fireball-shock scenario [4,5]. However, the existing analytical works give rather coarse predictions and suffer from many uncertainties. We develop a refined analytical model of synchrotron-self-Compton emission, in which we take into account both synchrotron and inverse Compton cooling of relativistic electrons. The principal role of Klein-Nishina cut-off is shown. We discuss the delay of inverse Compton (IC) component of GRB emission with respect to sub-MeV radiation and describe its energy dependence.
引用
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页码：461 / 464
页数：4
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