Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1206
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dc.contributor.authorGopakumar, A.-
dc.contributor.authorIyer, B.R.-
dc.date.accessioned2006-05-12T05:44:03Z-
dc.date.available2006-05-12T05:44:03Z-
dc.date.issued2002-04-15-
dc.identifier.citationPhysical Review D, 2002, Vol.65, 084011en
dc.identifier.issn1550-7998-
dc.identifier.issn1550-2368 (online)-
dc.identifier.urihttp://hdl.handle.net/2289/1206-
dc.description.abstractThe 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.extent341375 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherThe American Physical Societyen
dc.relation.urihttp://prola.aps.org/abstract/PRD/v65/i8/e084011en
dc.rights(2002) by the American Physical Societyen
dc.titleSecond post-Newtonian gravitational wave polarizations for compact binaries in elliptical orbitsen
dc.typeArticleen
Appears in Collections:Research Papers (TP)

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