通过LIGO-Virgo黑洞合并测试宇宙中的镜像对称性
Juan Calderón Bustillo1,2, Adrian Del Rio3,4, Nicolas Sanchis-Gual5
1Universidade de Santiago de Compostela, Instituto Galego de Física de Altas Enerxías, 15782 Santiago de Compostela, Galicia, Spain.
Physical review letters
|February 10, 2025
概括
引力波分析显示,大多数黑洞合并都表现出循环极化,挑战了宇宙学原理.
科学领域:
- 天体物理学和宇宙学
- 引力波天文学 引力波天文学
- 一般相对论一般相对论.
背景情况:
- 黑洞的合并可以产生带有净圆极化的引力波.
- 宇宙学原理预测这种辐射应该平均为零,以保持镜像反射对称性.
研究的目的:
- 对宇宙学原理关于净圆极化预测进行独立的引力波测试.
- 用黑洞合并数据调查宇宙中大规模的镜像不对称性.
主要方法:
- 利用一种新的可观测量,切尔恩 - 庞特里亚金伪尺度,来测量净圆极化.
- 分析了47个黑洞的合并,使用最先进的广义相对论模型来预先处理合并.
- 对特定事件进行参数推断,包括GW200129,使用新的和公开的数据.
主要成果:
- 在所有分析的合并中,平均净循环偏振与零一致.
- 在分析的黑洞合并中,至少有82%的黑洞合并显示出产生净循环偏振的证据.
- 事件GW200129显示了镜像不对称的强有力的证据 (93.1%的概率).
结论:
- 虽然平均值为零,但绝大多数黑洞合并显示净圆极化,这表明局部镜像不对称.
- 这些发现暗示存在能够通过量子效应自发发射循环偏振光子的天体物理源.
- 未来的黑洞合并检测将完善大规模镜像不对称性和宇宙学原理的约束.
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