Geodesic
Post-Newtonian approximation in the test particle limit
Banach Center Publications, Tome 41 (1997) no. 2, pp. 75-83.

Voir la notice de l'article provenant de la source Institute of Mathematics Polish Academy of Sciences

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.
DOI : 10.4064/-41-2-75-83

Misao Sasaki 1

1 
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Misao Sasaki. Post-Newtonian approximation in the test particle limit. Banach Center Publications, Tome 41 (1997) no. 2, pp. 75-83. doi : 10.4064/-41-2-75-83. http://geodesic.mathdoc.fr/articles/10.4064/-41-2-75-83/

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