Gravitational radiation from inspiralling compact binaries completed at the third post-Newtonian order

Details Gravitational radiation from inspiralling compact binaries completed at the third post-Newtonian order Gravitational radiation from inspiralling compact binaries completed at the third post-Newtonian order

2004-06-03

arxiv.org/abs/gr-qc/0406012v1

Phys.Rev.Lett.93:091101,2004

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

4 pages in 2-column format, LaTeX 2e, REVTeX 4, no figure

Scientific paper

10.1103/PhysRevLett.93.091101

The gravitational radiation from point particle binaries is computed at the third post-Newtonian (3PN) approximation of general relativity. Three previously introduced ambiguity parameters, coming from the Hadamard self-field regularization of the 3PN source-type mass quadrupole moment, are consistently determined by means of dimensional regularization, and proved to have the values xi = -9871/9240, kappa = 0 and zeta = -7/33. These results complete the derivation of the general relativistic prediction for compact binary inspiral up to 3.5PN order, and should be of use for searching and deciphering the signals in the current network of gravitational wave detectors.

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