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Stellar collapse and gravitational waves

Chris L. Fryer·Daniel E. Holz·Scott A. Hughes·Michael S. Warren
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Abstract

The new generation of gravitational wave (GW) detectors have the potential to open a novel window onto the violent dynamics of core collapse. Although it is certain that core collapse events generate gravitational radiation, understanding the characteristics of the radiation -- whether it can be measured with these detectors, and the best way to go about doing so -- is a challenging problem. In this chapter we review the promise of GWs as observational probes, including a discussion of the current state of GW detectors, and discuss the status of work to understand the waves generated by stellar core collapse.

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Chris L. Fryer, Daniel E. Holz, Scott A. Hughes, Michael S. Warren. 2002-11-27. Stellar collapse and gravitational waves. https://arxiv.org/abs/astro-ph/0211609

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