费米-LAT对马射线爆发GRB 130427A的观测结果
M Ackermann1, M Ajello, K Asano
1Deutsches Elektronen Synchrotron DESY, D-15738 Zeuthen, Germany.
概括
费米马射线太空望远镜观测到一个非常明亮的马射线爆发 (GRB) 130427A,挑战了标准模型. 它的独特性质表明了对天体物理源中高能发射的替代解释.
科学领域:
- 天体物理学 天体物理学
- 高能天体物理学 高能天体物理学
- 马射线天文学 马射线天文学
背景情况:
- 马射线爆发 (GRBs) 是强大的,神秘的宇宙爆炸.
- GRBs的后发光阶段通常由加速电子的同步子辐射解释.
- 了解GRB发射机制对于天体物理学至关重要.
研究的目的:
- 分析马射线爆发 (GRB) 130427A.A.的独特特征
- 为了限制特殊的天体物理源的物理性质,如GRB 130427A.
- 为了测试GRB后照中高能排放的现有模型.
主要方法:
- 使用费米马射线太空望远镜上的大面积望远镜 (LAT) 进行观测.
- 马射线光曲线的时间分析.
- 高能辐射的光谱分析.
主要成果:
- GRB 130427A表现出前所未有的特性:最大的流动性,最高能量的光子 (95 GeV),最长的持续时间 (20 小时),以及巨大的同位素能量释放.
- 观察到的时间和光谱特征与标准同步子发射模型的预测有很大差异.
- 这些数据挑战了广泛接受的非热高能排放的外部冲击模型.
结论:
- 由于GRB 130427A的特殊性,需要重新评估当前的GRB排放模型.
- 可能需要替代或修改的排放机制来解释观察到的现象.
- 对这种极端GRB的进一步研究对于进一步了解高能天体物理学至关重要.
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