长伽马射线暴余辉起源于双星驱动极超新星的同步辐射
高能天体物理现象
2022-02-02 v1
摘要
长伽马射线暴在 X 射线、光学和射电波段显示出余辉辐射，其光度随时间以近乎相同的幂律行为衰减。在本次报告中，我给出一个解析处理，表明该余辉由与双星驱动极超新星相关的超新星抛射物产生的同步辐射所致。
引用
@article{arxiv.2202.00316,
title = {On the Origin of the Long Gamma-Ray Burst Afterglow as Synchrotron Radiation from Binary-Driven Hypernovae},
author = {Jorge A. Rueda},
journal= {arXiv preprint arXiv:2202.00316},
year = {2022}
}
备注
To appear in AIP Conf. Proc. This article is a contribution to the proceedings of the "17th Italian-Korean Symposium on Relativistic Astrophysics" held on August 2-6, 2021