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来自GRB 120308A中稳定的有序磁场的高度极化光
C G Mundell1, D Kopač, D M Arnold
1Astrophysics Research Institute, Liverpool John Moores University, IC2, Liverpool Science Park, 146 Brownlow Hill, Liverpool L3 5RF, UK.
Nature
|December 6, 2013
概括
玛射线爆发后光中的高极化表明磁性喷射具有稳定的场. 这一发现支持了喷射中大规模磁场在爆炸中存活的模型,排除了等离子体的不稳定性.
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
- 血物理学的等离子体物理学
背景情况:
- 马射线爆发 (GRB) 是一种强大的宇宙爆炸.
- 余照是由GRB喷射物与周围物质相撞的冲击产生的.
- 来自反射冲击的光的极化可以揭示GRB射流磁场的特性.
研究的目的:
- 为了研究GRB早期后照的光的两极分化.
- 为了测试GRB喷射结构和磁场行为的竞争模型.
- 为了确定GRB喷射是否具有全球排序的磁场.
主要方法:
- 观测到Swift GRB 120308A在马射线检测后四分钟的光学偏振.
- 在接下来的10分钟内测量极化水平和位置角度.
- 分析了极化数据,以推断GRB喷射磁场的特性.
主要成果:
- 检测到高线性偏振 (P=28%,降至16%) 在即时后光.
- 观察到一个稳定的极化位置角度与最小的变化 (≤15度).
- 这些极化特性与因等离子体不稳定性而产生的随机磁场不一致.
结论:
- GRB的特点是磁化巴里昂喷射器具有大规模,均的磁场.
- 这些有序的磁场可以在最初的GRB爆炸后持续很长时间.
- 这些发现支持GRB喷射中向导,有序磁场的模型.
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