来自中子星的引力波：前景与挑战
Gravitational waves from neutron stars: Promises and challenges
摘要：
我们讨论了不同的方式，中子星可以产生引力波，描述了最近的改进，在提高探测器灵敏度的背景下，相关的场景建模，并显示如何观测开始测试我们的理解基础物理。讨论的主要目的是为第三代地基探测器（如爱因斯坦望远镜）建立有前途的科学目标，并确定如果我们想使用引力波数据来探测中子星物理学，需要满足的各种挑战。
英文摘要：
We discuss different ways that neutron stars can generate gravitational waves, describe recent improvements in modelling the relevant scenarios in the context of improving detector sensitivity, and show how observations are beginning to test our understanding of fundamental physics. The main purpose of the discussion is to establish promising science goals for third-generation ground-based detectors, like the Einstein Telescope, and identify the various challenges that need to be met if we want to use gravitational-wave data to probe neutron star physics.
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