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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1293
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dc.contributor.authorGopakumar, A.-
dc.contributor.authorIyer, B.R.-
dc.contributor.authorIyer, Sai-
dc.date.accessioned2006-05-23T11:09:26Z-
dc.date.available2006-05-23T11:09:26Z-
dc.date.issued1997-05-15-
dc.identifier.citationPhysical Review D, 1997, Vol.55, 6030-6053en
dc.identifier.issn1550-2368 (online)-
dc.identifier.issn1550-7998 (print)-
dc.identifier.urihttp://hdl.handle.net/2289/1293-
dc.description.abstractStarting from the recently obtained post-post-Newtonian (2PN) accurate forms of the energy and angular momentum fluxes from inspiraling compact binaries, we deduce the gravitational radiation reaction to 2PN order beyond the quadrupole approximation—4.5PN terms in the equation of motion—using the refined balance method proposed by Iyer and Will. We explore critically the features of their construction and illustrate them by contrast with other possible variants. The equations of motion are valid for general binary orbits and for a class of coordinate gauges. The limiting cases of circular orbits and radial infall are also discussed.en
dc.format.extent401073 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherThe American Physical Societyen
dc.rights() by the American Physical Societyen
dc.titleSecond post-Newtonian gravitational radiation reaction for two-body systems: Nonspinning bodiesen
dc.typeArticleen
dc.additionalErratum: A. Gopakumar, Bala R. Iyer, and Sai Iyer, Erratum: Second post-Newtonian gravitational radiation reaction for two-body systems: Nonspinning bodies [Phys. Rev. D 55, 6030 (1997)], Phys. Rev. D 57, 6562 (1998).en
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