Second post-Newtonian gravitational wave polarizations for compact binaries in elliptical orbits

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1206

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DC Field	Value	Language
dc.contributor.author	Gopakumar, A.	-
dc.contributor.author	Iyer, B.R.	-
dc.date.accessioned	2006-05-12T05:44:03Z	-
dc.date.available	2006-05-12T05:44:03Z	-
dc.date.issued	2002-04-15	-
dc.identifier.citation	Physical Review D, 2002, Vol.65, 084011	en
dc.identifier.issn	1550-7998	-
dc.identifier.issn	1550-2368 (online)	-
dc.identifier.uri	http://hdl.handle.net/2289/1206	-
dc.description.abstract	The second post-Newtonian (2PN) contribution to the “plus” and “cross” gravitational wave polarizations associated with gravitational radiation from non-spinning, compact binaries moving in elliptic orbits is computed. The computation starts from our earlier results on 2PN generation, crucially employs the 2PN accurate generalized quasi-Keplerian parametrization of elliptic orbits by Damour, Schäfer and Wex and provides 2PN accurate expressions modulo the tail terms for gravitational wave polarizations incorporating effects of eccentricity and periastron precession.	en
dc.format.extent	341375 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	The American Physical Society	en
dc.relation.uri	http://prola.aps.org/abstract/PRD/v65/i8/e084011	en
dc.rights	(2002) by the American Physical Society	en
dc.title	Second post-Newtonian gravitational wave polarizations for compact binaries in elliptical orbits	en
dc.type	Article	en
Appears in Collections:	Research Papers (TP)

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