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Listening for Ringing Black Holes

Jolien D. E. Creighton
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Abstract

The gravitational radiation produced by binary black holes during their inspiral, merger, and ringdown phases is a promising candidate for detection by the first or second generation of kilometer-scale interferometric gravitational wave antennas. Waveforms for the last phase, the quasinormal ringing, are well understood. I discuss the feasibility of detection of the quasinormal ringing of a black hole based on an analysis of the Caltech 40-meter interferometer data.

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Jolien D. E. Creighton. 1997-12-10. Listening for Ringing Black Holes. https://arxiv.org/abs/gr-qc/9712044

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