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

Blanchet, Luc; Damour, Thibault; Esposito-Farese, G.; Iyer, B.R.

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

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DC Field	Value	Language
dc.contributor.author	Blanchet, Luc	-
dc.contributor.author	Damour, Thibault	-
dc.contributor.author	Esposito-Farese, G.	-
dc.contributor.author	Iyer, B.R.	-
dc.date.accessioned	2006-05-11T10:41:06Z	-
dc.date.available	2006-05-11T10:41:06Z	-
dc.date.issued	2004-08-26	-
dc.identifier.citation	Physical Review Letters, 2004, Vol.93, 091101	en
dc.identifier.issn	0031-9007	-
dc.identifier.issn	1079-7114 (online)	-
dc.identifier.uri	http://hdl.handle.net/2289/1187	-
dc.description.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.	en
dc.format.extent	110521 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	The American Physical Society	en
dc.relation.uri	http://link.aps.org/abstract/PRL/v93/e091101	en
dc.rights	(2004) by the American Physical Society	en
dc.title	Gravitational radiation from inspiralling compact binaries completed at the third post-Newtonian order	en
dc.type	Article	en
Appears in Collections:	Research Papers (TP)

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