大量粘度对合并后来自合并中子星的引力波信号的影响
Michail Chabanov1,2, Luciano Rezzolla1,3,4
1Institut für Theoretische Physik, Goethe Universität, Max-von-Laue-Straße 1, 60438 Frankfurt am Main, Germany.
Physical review letters
|March 7, 2025
概括
双质中子星合并中的大量粘度显著影响引力波信号. 较高的粘度减轻了振荡,但增强了GW排放,改变了合并后的光谱.
科学领域:
- 天体物理学 天体物理学
- 核物理 核物理 核物理
- 一般相对论一般相对论.
背景情况:
- 双质中子星的合并会产生强烈的合并后振荡,影响引力波 (GW) 信号.
- 高温和高密度可以通过弱相互作用破坏化学平衡,从而诱导散装粘度.
研究的目的:
- 为了研究散体粘度对二进制中子星合并动态和GW发射的影响.
- 为了执行第一个模拟使用一个自相一致的,二阶相对论液态动力学公式消散流体.
主要方法:
- 采用了一种自相一致的,二次相对论的液体动力学公式,用于消耗性流体.
- 基于直接和修改的Urca反应建模的散装粘度,在三个场景 (低,中,高) 中强度不同.
主要成果:
- 高质量粘度抑制了合并后的碰撞和反弹振荡.
- 增加的粘度保留了m=2变形,增强了GW发射,并将GW频谱转移高达100Hz.
- 大量粘度增加了辐射的GW能量~2% (小粘度) 到~30% (大粘度).
结论:
- 大量粘度在中子星合并的动态和GW排放中起着至关重要的作用.
- 在模拟中包含散装粘度对于准确建模合并后现象至关重要.
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