平坦谱伽马射线暴尾后glow
天体物理学
2007-05-23 v2
摘要
推导当电子能量分布相对平坦（幂指数p位于1.0至2.0之间）时，GRB尾后glow光度曲线的时序行为。证明当电子能量分布的上截至随喷流冲击波的批量洛伦兹因子直接成比例演化时，预期的行为将与p>2.0的情况相同。
引用
@article{arxiv.astro-ph/0104250,
title = {Flat Spectrum Gamma Ray Burst Afterglows},
author = {Dipankar Bhattacharya},
journal= {arXiv preprint arXiv:astro-ph/0104250},
year = {2007}
}
备注
8 pages, uses basi.sty (included). Revised according to referees' comments. Added discussion on Dai & Cheng (2001) astro-ph/0105055. Accepted for publication in Bull. Astr. Soc. India