Gravitational radiation from a small mass particle orbiting a massive black hole can be analytically studied to a very high order in the post-Newtonian expansion. Thus it gives us useful information on the evolution of a coalescing compact binary star. In this talk, I report on recent progress made in the black-hole perturbation approach.
@article{bwmeta1.element.bwnjournal-article-bcpv41z2p75bwm,
author = {Sasaki, Misao},
title = {Post-Newtonian approximation in the test particle limit},
journal = {Banach Center Publications},
volume = {38},
year = {1997},
pages = {75-83},
zbl = {0891.53064},
language = {en},
url = {http://dml.mathdoc.fr/item/bwmeta1.element.bwnjournal-article-bcpv41z2p75bwm}
}
Sasaki, Misao. Post-Newtonian approximation in the test particle limit. Banach Center Publications, Tome 38 (1997) pp. 75-83. http://gdmltest.u-ga.fr/item/bwmeta1.element.bwnjournal-article-bcpv41z2p75bwm/
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