Post-Newtonian approximation in the test particle limit

Tom 41 / 1997

Misao Sasaki Banach Center Publications 41 (1997), 75-83 DOI: 10.4064/-41-2-75-83

Streszczenie

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.

Autorzy

  • Misao Sasaki

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