Gravitational wave emission from stellar collapse has been studied for more than three decades. Current state-of-the-art numerical investigations of collapse include those that use progenitors with more realistic angular momentum profiles, properly treat microphysics issues, account for general relativity, and examine non-axisymmetric effects in three dimensions. Such simulations predict that gravitational waves from various phenomena associated with gravitational collapse could be detectable with ground-based and space-based interferometric observatories. This review covers the entire range of stellar collapse sources of gravitational waves: from the accretion induced collapse of a white dwarf through the collapse down to neutron stars or black holes of massive stars to the collapse of supermassive stars. ELECTRONIC SUPPLEMENTARY MATERIAL Supplementary material is available for this article at 10.12942/lrr-2003-2.

中文翻译：

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引力塌缩产生的引力波。


恒星坍缩引起的引力波发射的研究已经有三十多年了。目前最先进的塌陷数值研究包括使用具有更真实角动量分布的前身、正确处理微观物理问题、解释广义相对论以及检查三个维度的非轴对称效应。这种模拟预测，与引力塌缩相关的各种现象产生的引力波可以通过地面和空间干涉观测站进行探测。这篇综述涵盖了引力波的恒星塌缩源的整个范围：从白矮星的吸积引起的塌缩，到中子星或大质量恒星的黑洞的塌缩，再到超大质量恒星的塌缩。电子补充材料 本文的补充材料可在 10.12942/lrr-2003-2 上找到。