Abstract
In this talk, I review an analytic method for calculating gravitational radiation from a small mass particle orbiting a massive black hole. This method allows a systematic evalutation of the gravitational radiation to a very high order in post-Newtonian expansion, hence gives us useful information on the evolution of coalescing compact binary stars.
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Sasaki, M. Analytic black hole perturbation approach. J Astrophys Astron 20, 281–289 (1999). https://doi.org/10.1007/BF02702359
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DOI: https://doi.org/10.1007/BF02702359