dc.contributorUniversidade Estadual Paulista (Unesp)
dc.contributorCALTECH
dc.contributorUniv Pittsburgh
dc.contributorICTP South Amer Inst Fundamental Res
dc.date.accessioned2018-11-26T17:42:01Z
dc.date.available2018-11-26T17:42:01Z
dc.date.created2018-11-26T17:42:01Z
dc.date.issued2017-10-30
dc.identifierPhysical Review D. College Pk: Amer Physical Soc, v. 96, n. 8, 9 p., 2017.
dc.identifier2470-0010
dc.identifierhttp://hdl.handle.net/11449/163437
dc.identifier10.1103/PhysRevD.96.084065
dc.identifierWOS:000413900000010
dc.identifierWOS000413900000010.pdf
dc.description.abstractWe compute the leading post-Newtonian (PN) contributions at quadratic order in the spins to the radiation-reaction acceleration and spin evolution for binary systems, entering at four-and-a-half PN order. Our calculation includes the backreaction from finite-size spin effects, which is presented for the first time. The computation is carried out, from first principles, using the effective field theory framework for spinning extended objects. At this order, nonconservative effects in the spin-spin sector are independent of the spin supplementary conditions. A nontrivial consistency check is performed by showing that the energy loss induced by the resulting radiation-reaction force is equivalent to the total emitted power in the far zone. We find that, in contrast to the spin-orbit contributions (reported in a companion paper), the radiation reaction affects the evolution of the spin vectors once spin-spin effects are incorporated.
dc.languageeng
dc.publisherAmer Physical Soc
dc.relationPhysical Review D
dc.relation1,801
dc.rightsAcesso aberto
dc.sourceWeb of Science
dc.titleRadiation reaction for spinning bodies in effective field theory. II. Spin-spin effects
dc.typeArtículos de revistas


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