Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4032
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dc.contributor.authorMishra, Chandrakanth-
dc.contributor.authorIyer, B.R.-
dc.date.accessioned2011-04-08T09:15:13Z-
dc.date.available2011-04-08T09:15:13Z-
dc.date.issued2010-11-03-
dc.identifier.citationPhysical Review D, 2010, Vol.82, p104005en
dc.identifier.issn1550-2368 (Online)-
dc.identifier.issn1550-7998-
dc.identifier.urihttp://hdl.handle.net/2289/4032-
dc.descriptionOpen Access.en
dc.description.abstractHead-on infall of two compact objects with arbitrary mass ratio is investigated using the multipolar post-Minkowskian approximation method. At the third post-Newtonian order the energy flux, in addition to the instantaneous contributions, also includes hereditary contributions consisting of the gravitational-wave tails, tails-of-tails, and the tail-squared terms. The results are given both for infall from infinity and also for infall from a finite distance. These analytical expressions should be useful for the comparison with the high accuracy numerical relativity results within the limit in which post-Newtonian approximations are valid.en
dc.language.isoenen
dc.publisherAmerican Physical Societyen
dc.relation.urihttp://arxiv.org/abs/1008.4009en
dc.relation.urihttp://dx.doi.org/10.1103/PhysRevD.82.104005en
dc.relation.urihttp://adsabs.harvard.edu/abs/2010PhRvD..82j4005Men
dc.rights2010 The American Physical Societyen
dc.titleHead-on infall of two compact objects: Third post-Newtonian energy fluxen
dc.typeArticleen
Appears in Collections:Research Papers (TP)

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