通过使用先进的LIGO引力波引力透镜检测单个无脊柱恒星质量黑洞的可检测性
1School of Astronomy and Space Science, Nanjing University, Nanjing 210093, People's Republic of China and Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, Nanjing 210023, People's Republic of China.
Physical review letters
|January 19, 2024
概括
黑洞透视的引力波产生独特的信号,可以被先进的LIGO检测到. 这项研究表明,可以观察到强大的重力效应,改善了对恒星质量黑洞的检测能力.
科学领域:
- 天体物理学 天体物理学
- 一般相对论一般相对论.
- 引力波天文学 引力波天文学
背景情况:
- 引力波 (GWs) 为宇宙提供了一个独特的窗口.
- 黑洞是天体物理学中的关键物体,但它们对GWs强大的重力效应需要详细研究.
研究的目的:
- 通过使用先进的LIGO,研究由无旋转恒星质量黑洞透镜的引力波的可检测性.
- 分析强引力对镜头GW波形的影响.
主要方法:
- 在施瓦茨柴尔德黑洞时空中解决全相对主义线性波形方程.
- 使用配合因子,比较透镜波形与未透镜的广义相对论模板.
- 使用贝叶斯推理来评估可区分性.
主要成果:
- 强大的重力在透镜式GW波形中产生独特的信号,特别是在合并和回落过程中.
- 对于70M和133.33M之间的黑洞质量,发现的配合因子差异>5%.
- 透镜特征可以区分,信号噪声比高达19.2,可以通过先进的LIGO实现.
结论:
- 该研究表明,与弱场近似相比,透镜GWs的检测能力提高了.
- 可观察到的透镜效应覆盖了预测的恒星黑洞质量差距的很大一部分.
- 先进的LIGO可以检测到这些强重力透镜签名.
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