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Title: | Post-Newtonian prediction for the (2,2) mode of the gravitational wave emitted by compact binaries |
Authors: | Marsat, Sylvain Faye, Guillaume Blanchet, Luc Iyer, B.R. |
Issue Date: | 2012 |
Citation: | ASP Conference Series, 2012, Vol.467, p197 (Book Chapter) |
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 |
Description: | Restricted Access. Proceedings of 9th LISA Symposium Paris, France from 21-25 may 2012. Edited by Gerard Auger, Pierre Binétruy, and Eric Plagnol ( |
URI: | http://hdl.handle.net/2289/5401 |
ISSN: | 978-1-58381-816-9 |
Alternative Location: | http://arxiv.org/abs/1210.2339 http://adsabs.harvard.edu/abs/bib_query?arXiv:1210.2339 |
Copyright: | 2012 Astronomical Society of the Pacific |
Appears in Collections: | Research Papers (TP) |
Files in This Item:
File | Description | Size | Format | |
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2012_ASP_567_197.pdf Restricted Access | Restricted Access | 46.68 kB | Adobe PDF | View/Open Request a copy |
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