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

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dc.contributor.authorKidder, Lawrence E.
dc.contributor.authorBlanchet, Luc
dc.contributor.authorIyer, B.R.
dc.date.accessioned2008-03-08T05:30:59Z
dc.date.available2008-03-08T05:30:59Z
dc.date.issued2007-10
dc.descriptionRestricted Access. An open-access version is available at arXiv.org (one of the alternative locations)en
dc.description.abstractIn 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.extent104295 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.citationClassical and Quantum Gravity, 2007, Vol.24, p5307-5312en
dc.identifier.issnE-ISSN(s): 1361-6382
dc.identifier.issnP-ISSN(s): 0264-9381
dc.identifier.urihttp://hdl.handle.net/2289/3444
dc.language.isoenen
dc.publisherInstititute of Physics Publishing Ltd.en
dc.relation.urihttp://arxiv.org/abs/arXiv:0706.0726en
dc.relation.urihttp://dx.doi.org/10.1088/0264-9381/24/20/N01en
dc.rights2007 IOP Publishing Ltd.en
dc.titleA note on the radiation reaction in the 2.5PN waveform from inspiralling binaries in quasi-circular orbitsen
dc.typeArticleen

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