Please use this identifier to cite or link to this item:
http://hdl.handle.net/2289/1206
Full metadata record
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) |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
2002 Physcial Review 'D' V65 084011p.pdf | 25p. | 333.37 kB | Adobe PDF | View/Open |
Items in RRI Digital Repository are protected by copyright, with all rights reserved, unless otherwise indicated.