“长”伽马射线暴与“短”伽马射线暴的理论解释
天体物理学
2016-11-15 v1
摘要
在“火壳”模型框架内，我们定义了一种具有两个截然不同分量的“ canonical GRB ”光变曲线：当产生该现象的正负电子等离子体光学厚火壳达到透明度时发射的 Proper-GRB (P-GRB)，以及由于剩余的光学薄火壳与 CircumBurst Medium (CBM) 碰撞而发射的余辉。在此，我们展示该场景对“长”伽马射线暴与“短”伽马射线暴本质理论解释的影响。
引用
@article{arxiv.0804.2818,
title = {Theoretical interpretation of "long" and "short" GRBs},
author = {Carlo Luciano Bianco and Maria Grazia Bernardini and Letizia Caito and Pascal Chardonnet and Maria Giovanna Dainotti and Federico Fraschetti and Roberto Guida and Remo Ruffini and She-Sheng Xue},
journal= {arXiv preprint arXiv:0804.2818},
year = {2016}
}
备注
3 pages, 1 figure, to appear on the Proceedings of the Eleventh Marcel Grossmann Meeting, Berlin (Germany), July 2006