Estimation of the post-Newtonian parameters in the gravitational-wave emission of a coalescing binary-Reference-Cited by-同舟云学术

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Estimation of the post-Newtonian parameters in the gravitational-wave emission of a coalescing binary

Published:1995-08-15 Issue:4 Volume:52 Page:2089-2111
ISSN:0556-2821
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Królak Andrzej,Kokkotas Kostas D.,Schäfer Gerhard

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.52.2089/fulltext

Reference42 articles.

1. Neutron star and black hole binaries in the Galaxy

2. The rate of neutron star binary mergers in the universe - Minimal predictions for gravity wave detectors

3. The merger rate of neutron star and black hole binaries

4. Gravitational Radiation and the Motion of Two Point Masses

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