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Gravitational radiation reaction

Takahiro Tanaka
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Abstract

We give a short personally-biased review on the recent progress in our understanding of gravitational radiation reaction acting on a point particle orbiting a black hole. The main motivation of this study is to obtain sufficiently precise gravitational waveforms from inspiraling binary compact stars with a large mass ratio. For this purpose, various new concepts and techniques have been developed to compute the orbital evolution taking into account the gravitational self-force. Combining these ideas with a few supplementary new ideas, we try to outline a path to our goal here.

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Takahiro Tanaka. 2005-10-04. Gravitational radiation reaction. https://doi.org/10.1143/ptps.163.120

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