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http://hdl.handle.net/2289/6192
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DC Field | Value | Language |
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dc.contributor.author | Faye, Guillaume | - |
dc.contributor.author | Blanchet, Luc | - |
dc.contributor.author | Iyer, B.R. | - |
dc.date.accessioned | 2015-03-10T02:08:41Z | - |
dc.date.available | 2015-03-10T02:08:41Z | - |
dc.date.issued | 2015-02-19 | - |
dc.identifier.citation | Classical and Quantum Gravity, 2015, Vol.32, p045016 | en |
dc.identifier.issn | 0264-9381 | - |
dc.identifier.uri | http://hdl.handle.net/2289/6192 | - |
dc.description | Open Access - IOP select | en |
dc.description.abstract | This paper is motivated by the need to improve the post-Newtonian (PN) amplitude accuracy of waveforms for gravitational waves generated by inspiralling compact binaries, both for use in data analysis and in the comparison between post-Newtonian approximations and numerical relativity computations. It presents (i) the non-linear couplings between multipole moments of general post-Newtonian matter sources up to order 3.5PN, including all contributions from tails, tails-of-tails and the non-linear memory effect; and (ii) the source mass-type octupole moment of (non-spinning) compact binaries up to order 3PN, which permits completion of the expressions of the octupole modes $(3,3)$ and $(3,1)$ of the gravitational waveform to order 3.5PN. On this occasion we reconfirm by means of independent calculations our earlier results concerning the source mass-type quadrupole moment to order 3PN. Related discussions on factorized resummed waveforms and the occurence of logarithmic contributions to high order are also included. | en |
dc.language.iso | en | en |
dc.publisher | IOP Publishing Ltd. | en |
dc.relation.uri | http://arxiv.org/abs/1409.3546 | en |
dc.relation.uri | http://dx.doi.org/10.1088/0264-9381/32/4/045016 | en |
dc.relation.uri | http://adsabs.harvard.edu/abs/2015CQGra..32d5016F | en |
dc.rights | 2015 IOP Publishing Ltd. | en |
dc.subject | approximation | en |
dc.subject | gravitational waves | en |
dc.title | Non-linear multipole interactions and gravitational-wave octupole modes for inspiralling compact binaries to third-and-a-half post-Newtonian order | en |
dc.type | Article | en |
Appears in Collections: | Research Papers (TP) |
Files in This Item:
File | Description | Size | Format | |
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2015_CQG_32_045016.pdf | Open Access | 616.86 kB | Adobe PDF | View/Open |
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