Please use this identifier to cite or link to this item:
http://hdl.handle.net/2289/1187
Title: | Gravitational radiation from inspiralling compact binaries completed at the third post-Newtonian order |
Authors: | Blanchet, Luc Damour, Thibault Esposito-Farese, G. Iyer, B.R. |
Issue Date: | 26-Aug-2004 |
Publisher: | The American Physical Society |
Citation: | Physical Review Letters, 2004, Vol.93, 091101 |
Abstract: | The gravitational radiation from point particle binaries is computed at the third post-Newtonian (3PN) approximation of general relativity. Three previously introduced ambiguity parameters, coming from the Hadamard self-field regularization of the 3PN source-type mass quadrupole moment, are consistently determined by means of dimensional regularization, and proved to have the values xi= –9871/9240, kappa= 0, and zeta= –7/33. These results complete the derivation of the general relativistic prediction for compact binary inspiral up to 3.5PN order, and should be of use for searching and deciphering the signals in the current network of gravitational wave detectors. |
URI: | http://hdl.handle.net/2289/1187 |
ISSN: | 0031-9007 1079-7114 (online) |
Alternative Location: | http://link.aps.org/abstract/PRL/v93/e091101 |
Copyright: | (2004) by the American Physical Society |
Appears in Collections: | Research Papers (TP) |
Files in This Item:
File | Description | Size | Format | |
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2004 PRL 93 p091101.pdf | 4p. | 107.93 kB | Adobe PDF | View/Open |
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