短玛射线爆发中的千赫兹半周期性振荡
Cecilia Chirenti1,2,3,4, Simone Dichiara5, Amy Lien6
1Department of Astronomy, University of Maryland, College Park, MD, USA. chirenti@umd.edu.
Nature
|January 9, 2023
概括
科学家从档案数据中发现了马射线爆发 (GRB) 的准周期性振荡,与二进制中子星合并后形成的短寿命中子星的预测相匹配. 这一发现为这些极端宇宙事件的物理提供了洞察力.
科学领域:
- 天文学
- 天体物理学
- 引力波天文学
背景情况:
- 短马射线爆发与双中子恒星的合并有关,通过引力波和电磁信号观察到.
- 合并后的引力波信号可能包含可被未来观测站检测的功率光谱特征 (1-5 kHz).
- 一个短命的中子星可能会在合并后形成, 在几毫秒内崩成黑洞.
研究的目的:
- 在短GRB信号中寻找和识别准周期调制.
- 调查这些调制与二进制星合并后短命中子星的形成之间的潜在联系.
- 将观测数据与数字相对论模拟的预测进行比较.
主要方法:
- 来自爆发和短暂源实验 (BATSE) 的档案数据分析.
- 显示准周期调制的信号的识别.
- 识别的信号与数值相对论的理论预测进行比较.
主要成果:
- 两个信号,GRB 910711和GRB 931101B,被确定为半周期调节.
- 这些信号与合并后形成的短命中子星的预测行为相符.
- 观察到的调制与1-5kHz范围内的理论功率光谱特征保持一致.
结论:
- 这些发现为短GRB的准周期性振荡提供了观察证据.
- 这支持了短寿命中子星在二进制中子星合并的子集中形成的假设.
- 这项研究强调了未来探测器观察这些现象的潜力.
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