粘性物体对引力波的动态反应
Valentin Boyanov1, Vitor Cardoso1,2, Kostas D Kokkotas3
1Instituto Superior Técnico-IST, Universidade de Lisboa-UL, CENTRA, Departamento de Física, Avenida Rovisco Pais 1, 1049-001 Lisboa, Portugal.
粘性恒星吸收高频引力波,模仿黑洞. 然而,因果关系阻止它们成为完美的波反射器,尽管旋转的恒星可能会放大辐射.
科学领域:
- 相对论天体物理学 相对论天体物理学
- 流体动力学 流体动力学
- 引力波天文学 引力波天文学
背景情况:
- 了解天体在极端物理条件下的行为至关重要.
- 引力波为动态天体物理过程提供了一个独特的窗口.
研究的目的:
- 研究粘性恒星对引力波的动态反应.
- 首次计算粘性恒星的振荡模式和散射特性.
主要方法:
- 使用完全相对论的流体动力学理论.
- 计算粘性恒星的振荡模式和散射特性.
主要成果:
- 粘性恒星吸收高频辐射,遵循Press的散射关系.
- 最大粘度的恒星模仿黑洞的吸收.
- 因果界限禁止恒星成为完美的波反射器.
结论:
- 旋转的粘性恒星可能会放大传入的辐射.
- 粘性恒星为黑洞物理和波浪相互作用提供了洞察力.
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