A note on the radiation reaction in the 2.5PN waveform from inspiralling binaries in quasi-circular orbits

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/3444

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DC Field	Value	Language
dc.contributor.author	Kidder, Lawrence E.	-
dc.contributor.author	Blanchet, Luc	-
dc.contributor.author	Iyer, B.R.	-
dc.date.accessioned	2008-03-08T05:30:59Z	-
dc.date.available	2008-03-08T05:30:59Z	-
dc.date.issued	2007-10	-
dc.identifier.citation	Classical and Quantum Gravity, 2007, Vol.24, p5307-5312	en
dc.identifier.issn	E-ISSN(s): 1361-6382	-
dc.identifier.issn	P-ISSN(s): 0264-9381	-
dc.identifier.uri	http://hdl.handle.net/2289/3444	-
dc.description	Restricted Access. An open-access version is available at arXiv.org (one of the alternative locations)	en
dc.description.abstract	In this note we compute the contributions of the radiation reaction force in the 2.5 post-Newtonian (PN) gravitational wave polarizations for compact binaries in quasi-circular orbits. (i) We point out and correct an inconsistency in the derivation of [1]. (ii) We prove that all contributions from the radiation reaction in the 2.5PN waveform are actually negligible since they can be absorbed into a modification of the orbital phase at the 5PN order.	en
dc.format.extent	104295 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Instititute of Physics Publishing Ltd.	en
dc.relation.uri	http://arxiv.org/abs/arXiv:0706.0726	en
dc.relation.uri	http://dx.doi.org/10.1088/0264-9381/24/20/N01	en
dc.rights	2007 IOP Publishing Ltd.	en
dc.title	A note on the radiation reaction in the 2.5PN waveform from inspiralling binaries in quasi-circular orbits	en
dc.type	Article	en
Appears in Collections:	Research Papers (TP)

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