Radiation reaction for spinning bodies in effective field theory. II. Spin-spin effects

Detalhes bibliográficos
Autor(a) principal: Maia, Natalia T. [UNESP]
Data de Publicação: 2017
Outros Autores: Galley, Chad R., Leibovich, Adam K., Porto, Rafael A. [UNESP]
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1103/PhysRevD.96.084065
http://hdl.handle.net/11449/163437
Resumo: We 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.
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spelling Radiation reaction for spinning bodies in effective field theory. II. Spin-spin effectsWe 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.Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)NSFSimons FoundationFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)National Aeronautics and Space AdministrationUniv Estadual Paulista, Inst Fis Teor, Rua Dr Bento Teobaldo Ferraz 271, BR-01140070 Sao Paulo, SP, BrazilCALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USACALTECH, Theoret Astrophys, Walter Burke Inst Theoret Phys, Pasadena, CA 91125 USAUniv Pittsburgh, Dept Phys & Astron, Pittsburgh Particle Phys Astrophys & Cosmol Ctr, Pittsburgh, PA 15260 USAICTP South Amer Inst Fundamental Res, Rua Dr Bento Teobaldo Ferraz 271, BR-01140070 Sao Paulo, SP, BrazilUniv Estadual Paulista, Inst Fis Teor, Rua Dr Bento Teobaldo Ferraz 271, BR-01140070 Sao Paulo, SP, BrazilNSF: PHY-1404569NSF: PHY-1519175FAPESP: 2014/25212-3FAPESP: 2014/10748-5Amer Physical SocUniversidade Estadual Paulista (Unesp)CALTECHUniv PittsburghICTP South Amer Inst Fundamental ResMaia, Natalia T. [UNESP]Galley, Chad R.Leibovich, Adam K.Porto, Rafael A. [UNESP]2018-11-26T17:42:01Z2018-11-26T17:42:01Z2017-10-30info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article9application/pdfhttp://dx.doi.org/10.1103/PhysRevD.96.084065Physical Review D. College Pk: Amer Physical Soc, v. 96, n. 8, 9 p., 2017.2470-0010http://hdl.handle.net/11449/16343710.1103/PhysRevD.96.084065WOS:000413900000010WOS000413900000010.pdfWeb of Sciencereponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review D1,801info:eu-repo/semantics/openAccess2023-11-30T06:17:24Zoai:repositorio.unesp.br:11449/163437Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T19:09:33.266255Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Radiation reaction for spinning bodies in effective field theory. II. Spin-spin effects
title Radiation reaction for spinning bodies in effective field theory. II. Spin-spin effects
spellingShingle Radiation reaction for spinning bodies in effective field theory. II. Spin-spin effects
Maia, Natalia T. [UNESP]
title_short Radiation reaction for spinning bodies in effective field theory. II. Spin-spin effects
title_full Radiation reaction for spinning bodies in effective field theory. II. Spin-spin effects
title_fullStr Radiation reaction for spinning bodies in effective field theory. II. Spin-spin effects
title_full_unstemmed Radiation reaction for spinning bodies in effective field theory. II. Spin-spin effects
title_sort Radiation reaction for spinning bodies in effective field theory. II. Spin-spin effects
author Maia, Natalia T. [UNESP]
author_facet Maia, Natalia T. [UNESP]
Galley, Chad R.
Leibovich, Adam K.
Porto, Rafael A. [UNESP]
author_role author
author2 Galley, Chad R.
Leibovich, Adam K.
Porto, Rafael A. [UNESP]
author2_role author
author
author
dc.contributor.none.fl_str_mv Universidade Estadual Paulista (Unesp)
CALTECH
Univ Pittsburgh
ICTP South Amer Inst Fundamental Res
dc.contributor.author.fl_str_mv Maia, Natalia T. [UNESP]
Galley, Chad R.
Leibovich, Adam K.
Porto, Rafael A. [UNESP]
description We 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.
publishDate 2017
dc.date.none.fl_str_mv 2017-10-30
2018-11-26T17:42:01Z
2018-11-26T17:42:01Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://dx.doi.org/10.1103/PhysRevD.96.084065
Physical Review D. College Pk: Amer Physical Soc, v. 96, n. 8, 9 p., 2017.
2470-0010
http://hdl.handle.net/11449/163437
10.1103/PhysRevD.96.084065
WOS:000413900000010
WOS000413900000010.pdf
url http://dx.doi.org/10.1103/PhysRevD.96.084065
http://hdl.handle.net/11449/163437
identifier_str_mv Physical Review D. College Pk: Amer Physical Soc, v. 96, n. 8, 9 p., 2017.
2470-0010
10.1103/PhysRevD.96.084065
WOS:000413900000010
WOS000413900000010.pdf
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Physical Review D
1,801
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 9
application/pdf
dc.publisher.none.fl_str_mv Amer Physical Soc
publisher.none.fl_str_mv Amer Physical Soc
dc.source.none.fl_str_mv Web of Science
reponame:Repositório Institucional da UNESP
instname:Universidade Estadual Paulista (UNESP)
instacron:UNESP
instname_str Universidade Estadual Paulista (UNESP)
instacron_str UNESP
institution UNESP
reponame_str Repositório Institucional da UNESP
collection Repositório Institucional da UNESP
repository.name.fl_str_mv Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)
repository.mail.fl_str_mv
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