Post-Newtonian approximation in the test particle limit
Volume 41 / 1997
Banach Center Publications 41 (1997), 75-83
DOI: 10.4064/-41-2-75-83
Abstract
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.
