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使用闪制约的快速无线电爆发的磁层起源
Kenzie Nimmo1, Ziggy Pleunis2,3,4, Paz Beniamini5,6
1MIT Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA. knimmo@mit.edu.
Nature
|January 1, 2025
概括
快速无线电爆发 (FRB) 是一种神秘的宇宙信号. 新的研究使用闪来测量FRB 20221022A的辐射大小,
科学领域:
- 天体物理学与宇宙学
- 无线电天文学
- 短暂的现象
背景情况:
- 快速无线电爆发 (FRB) 是来自银河系外的强烈,持续数毫秒的无线电短暂.
- 关于FRB的发射机制进行了讨论,模型提出其起源于中央发动机附近或大规模相对论冲击.
- 射频雷射发射区域的大小是这些模型之间的关键差异.
研究的目的:
- 为了限制快速无线电爆发FRB 20221022A的横向发射区域大小.
- 使用天体物理散射来区分竞争中的FRB发射模型.
- 研究闪作为理解FRB物理学的工具的实用性.
主要方法:
- 在FRB20221022A的频谱中测量了两个相互连贯的闪尺度.
- 在银河系和FRB的主星系中利用散射介质作为天体物理镜头.
- 使用闪特性限制了FRB侧面发射区域的大小.
主要成果:
- FRB 20221022A的横向发射区域大小被限制为小于或等于3 × 10^4公里.
- 这种测量大小与涉及大辐射距离相对论冲击的模型不一致.
- 结果支持来自中央紧物体磁层或附近的辐射.
结论:
- 闪测量独立支持FRB 20221022A的磁层发射过程.
- 这一发现与最近在同一FRB中观察到的S形偏振角度相一致.
- 闪被证实是探测FRB发射机制和原始环境的有价值工具.
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