Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1294
Full metadata record
DC FieldValueLanguage
dc.contributor.authorGopakumar, A.-
dc.contributor.authorIyer, B.R.-
dc.date.accessioned2006-05-23T11:11:27Z-
dc.date.available2006-05-23T11:11:27Z-
dc.date.issued1997-12-15-
dc.identifier.citationPhysical Review D, 1997, Vol.56, 7708-7731en
dc.identifier.issn1550-2368 (online)-
dc.identifier.issn1550-7998 (print)-
dc.identifier.urihttp://hdl.handle.net/2289/1294-
dc.description.abstractThe post-post-Newtonian (2PN) accurate mass quadrupole moment, for compact binaries of arbitrary mass ratio, moving in general orbits is obtained by the multipolar post Minkowskian approach of Blanchet, Damour, and Iyer. Using this, for binaries in general orbits, the 2PN contributions to the gravitational waveform, and the associated far-zone energy and angular momentum fluxes are computed. For quasielliptic orbits, the energy and angular momentum fluxes are averaged over an orbital period, and employed to determine the 2PN corrections to the rate of decay of the orbital elements.en
dc.format.extent441343 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherThe American Physical Societyen
dc.relation.uri10.1103/PhysRevD.56.7708en
dc.relation.urihttp://link.aps.org/abstract/PRD/v56/p7708en
dc.rights(1997) by the American Physical Societyen
dc.titleGravitational waves from inspiraling compact binaries: Angular momentum flux, evolution of the orbital elements, and the waveform to the second post-Newtonian orderen
dc.typeArticleen
Appears in Collections:Research Papers (TP)

Files in This Item:
File Description SizeFormat 
1997 PRD V56 p7708.pdf24p.431 kBAdobe PDFView/Open


Items in RRI Digital Repository are protected by copyright, with all rights reserved, unless otherwise indicated.