We provide a bird’s-eye view of neutron-star seismology, which aims to probe the extreme physics associated with these objects, in the context of gravitational-wave astronomy. Focussing on the fundamental mode of oscillation, which is an efficient gravitational-wave emitter, we consider the seismology aspects of a number of astrophysically relevant scenarios, ranging from transients (like pulsar glitches and magnetar flares), to the dynamics of tides in inspiralling compact binaries and the eventual merged object and instabilities acting in isolated, rapidly rotating, neutron stars. The aim is not to provide a thorough review, but rather to introduce (some of) the key ideas and highlight issues that need further attention.

中文翻译：

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中子星地震学的引力波透视

我们提供了中子星地震学的鸟瞰图，其目的是在引力波天文学的背景下探究与这些天体有关的极端物理学。着眼于振荡的基本模式（一种有效的重力波发射器），我们考虑了与天体有关的许多场景的地震学方面，从瞬变（例如脉冲星故障和电磁耀斑）到励志紧凑型中的潮汐动力学，不一而足。双星以及最终合并的物体和不稳定性作用于孤立的，快速旋转的中子星。目的不是提供全面的审查，而是介绍（某些）关键思想并强调需要进一步关注的问题。