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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1187

Title: Gravitational radiation from inspiralling compact binaries completed at the third post-Newtonian order
Authors: Blanchet, Luc
Damour, Thibault
Esposito-Farese, G.
Iyer, B.R.
Issue Date: 26-Aug-2004
Publisher: The American Physical Society
Citation: Physical Review Letters, 2004, Vol.93, 091101
Abstract: 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.
URI: http://hdl.handle.net/2289/1187
ISSN: 0031-9007
1079-7114 (online)
Alternative Location: http://link.aps.org/abstract/PRL/v93/e091101
Copyright: (2004) by the American Physical Society
Appears in Collections:Research Papers (TP)

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