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29 March 2024
 
  » arxiv » astro-ph/0211609

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Stellar collapse and gravitational waves
Chris L. Fryer ; Daniel E. Holz ; Scott A. Hughes ; Michael S. Warren ;
Date 27 Nov 2002
Subject astro-ph gr-qc
AbstractThe 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.
Source arXiv, astro-ph/0211609
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