"fireshell" 模型与"标准"伽马射线暴场景
天体物理学
2008-11-26 v1
摘要
在"fireshell"模型中，我们定义了一个"标准"伽马射线暴光变曲线，包含两个截然不同的成分：原生伽马射线暴（P-GRB），当源自该现象的 optically thick fireshell of electron-positron plasma 达到透明时发射；以及余辉，由剩余的光学薄 fireshell 与 CircumBurst Medium (CBM) 碰撞产生。我们概述了我们的"标准"伽马射线暴场景，源自黑洞的引力坍缩，特别强调对"真实"和"虚假"短伽马射线暴的区分。
引用
@article{arxiv.0712.0495,
title = {The "fireshell" model and the "canonical" GRB scenario},
author = {Carlo Luciano Bianco and Maria Grazia Bernardini and Letizia Caito and Maria Giovanna Dainotti and Roberto Guida and Remo Ruffini},
journal= {arXiv preprint arXiv:0712.0495},
year = {2008}
}
备注
4 pages, 5 figures, in the Proceedings of the "4th Italian-Sino Workshop on Relativistic Astrophysics", held in Pescara, Italy, July 20-28, 2007, C.L. Bianco, S.-S. Xue, Editors