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快速无线电爆发的物理机制
1Department of Physics and Astronomy, University of Nevada, Las Vegas, Las Vegas, NV, USA. zhang@physics.unlv.edu.
Nature
|November 5, 2020
概括
快速无线电爆发是一种神秘的宇宙事件. 最近的数据表明磁星发动机可能为这些神秘的无线电短暂提供动力,
科学领域:
- 天文学与天体物理学
- 高能天体物理学
背景情况:
- 快速无线电爆发 (FRB) 是持续数毫秒的天体物理瞬态.
- 最近收集数据的进步有助于人们更好地了解FRB的起源.
- 来自马射线爆发和无线脉冲星的洞察力为FRB研究提供了信息.
研究的目的:
- 为了回顾最近在研究快速无线电爆发的进展.
- 讨论FRB产生的物理机制.
- 评估磁星在产生FRB中的作用.
主要方法:
- 对最近的观测数据和理论模型进行审查.
- 将FRB特征与相关天体物理领域的现象进行比较.
- 分析银河系FRB和软马射线反射器之间的关联.
主要成果:
- 讨论了两种主要的辐射模型:紧物体的磁层和相对论冲击.
- 一个银河系FRB被检测到与一个柔软的马射线重复器.
- 这种关联强烈地表明磁星发动机可以产生FRB.
结论:
- 磁星发动机可能是至少部分,甚至全部快速无线电爆发的来源.
- 虽然磁器是最受欢迎的,但其他FRB发动机的可能性不能完全排除.
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