Post-Newtonian prediction for the (2,2) mode of the gravitational wave emitted by compact binaries
| dc.contributor.author | Marsat, Sylvain | |
| dc.contributor.author | Faye, Guillaume | |
| dc.contributor.author | Blanchet, Luc | |
| dc.contributor.author | Iyer, B.R. | |
| dc.date.accessioned | 2013-02-27T13:42:04Z | |
| dc.date.available | 2013-02-27T13:42:04Z | |
| dc.date.issued | 2012 | |
| dc.description | Restricted Access. Proceedings of 9th LISA Symposium Paris, France from 21-25 may 2012. Edited by Gerard Auger, Pierre Binétruy, and Eric Plagnol ( | en |
| dc.description.abstract | We present our 3.5PN computation of the (2,2) mode of the gravitational wave amplitude emitted by compact binaries, on quasi-circular orbits and in the absence of spins. We use the multipolar post-Newtonian wave generation formalism, extending and building on previous works which computed the 3PN order. This calculation required the extension of the multipolar post-Minkowskian algorithm, as well as the computation of the mass source quadrupole at 3.5PN order. Our result will allow more accurate comparisons to numerical relativity, and is a first step towards the computation of the full 3.5PN waveform amplitude, which would improve the estimation of the source parameters by gravitational wave detectors | en |
| dc.identifier.citation | ASP Conference Series, 2012, Vol.467, p197 (Book Chapter) | en |
| dc.identifier.issn | 978-1-58381-816-9 | |
| dc.identifier.uri | http://hdl.handle.net/2289/5401 | |
| dc.language.iso | en | en |
| dc.relation.uri | http://arxiv.org/abs/1210.2339 | en |
| dc.relation.uri | http://adsabs.harvard.edu/abs/bib_query?arXiv:1210.2339 | en |
| dc.rights | 2012 Astronomical Society of the Pacific | en |
| dc.title | Post-Newtonian prediction for the (2,2) mode of the gravitational wave emitted by compact binaries | en |
| dc.type | Book chapter | en |