Post-Newtonian approximation in the test particle limit

Misao Sasaki

Banach Center Publications (1997)

  • Volume: 41, Issue: 2, page 75-83
  • ISSN: 0137-6934

Abstract

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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.

How to cite

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Sasaki, Misao. "Post-Newtonian approximation in the test particle limit." Banach Center Publications 41.2 (1997): 75-83. <http://eudml.org/doc/252191>.

@article{Sasaki1997,
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.},
author = {Sasaki, Misao},
journal = {Banach Center Publications},
keywords = {gravitational radiation; black-hole perturbation approach},
language = {eng},
number = {2},
pages = {75-83},
title = {Post-Newtonian approximation in the test particle limit},
url = {http://eudml.org/doc/252191},
volume = {41},
year = {1997},
}

TY - JOUR
AU - Sasaki, Misao
TI - Post-Newtonian approximation in the test particle limit
JO - Banach Center Publications
PY - 1997
VL - 41
IS - 2
SP - 75
EP - 83
AB - 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.
LA - eng
KW - gravitational radiation; black-hole perturbation approach
UR - http://eudml.org/doc/252191
ER -

References

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