Overall evolution of realistic gamma-ray burst remnant and its afterglow

被引：34

作者：

Huang, YF ^{[1
]}

Dai, ZG

Lu, T

机构：

[1] Nanjing Univ, Dept Astron, Nanjing 210093, Peoples R China

[2] Chinese Acad Sci, Inst High Energy Phys, Lab Cosm Ray & High Energy Astrophys, Beijing 100039, Peoples R China

来源：

CHINESE PHYSICS LETTERS | 1999年 / 16卷 / 10期

关键词：

D O I：

10.1088/0256-307X/16/10/027

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Conventional dynamic model of gamma-ray burst remnants is found to be incorrect for adiabatic blastwaves during the non-relativistic phase. A new model is derived, which is shown to be correct for both radiative and adiabatic blastwaves during both ultra-relativistic and non-relativistic phases. Our model also takes the evolution of the radiative efficiency into account. The importance of the transition from the ultra-relativistic phase to the non-relativistic phase is stressed.

引用

页码：775 / 777

页数：3

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