Radiation reaction for spinning bodies in effective field theory. I. Spin-orbit effects
Autor(a) principal: | |
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Data de Publicação: | 2017 |
Outros Autores: | , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1103/PhysRevD.96.084064 http://hdl.handle.net/11449/163436 |
Resumo: | We compute the leading post-Newtonian (PN) contributions at linear order in the spin to the radiationreaction acceleration and spin evolution for binary systems, which enter at fourth PN order. The calculation is carried out, from first principles, using the effective field theory framework for spinning compact objects, in both the Newton-Wigner and covariant spin supplementary conditions. A nontrivial consistency check is performed on our results by showing that the energy loss induced by the resulting radiation-reaction force is equivalent to the total emitted power in the far zone, up to so-called Schott terms. We also find that, at this order, the radiation reaction has no net effect on the evolution of the spins. The spin-spin contributions to radiation reaction are reported in a companion paper. |
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Radiation reaction for spinning bodies in effective field theory. I. Spin-orbit effectsWe compute the leading post-Newtonian (PN) contributions at linear order in the spin to the radiationreaction acceleration and spin evolution for binary systems, which enter at fourth PN order. The calculation is carried out, from first principles, using the effective field theory framework for spinning compact objects, in both the Newton-Wigner and covariant spin supplementary conditions. A nontrivial consistency check is performed on our results by showing that the energy loss induced by the resulting radiation-reaction force is equivalent to the total emitted power in the far zone, up to so-called Schott terms. We also find that, at this order, the radiation reaction has no net effect on the evolution of the spins. The spin-spin contributions to radiation reaction are reported in a companion paper.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/article14application/pdfhttp://dx.doi.org/10.1103/PhysRevD.96.084064Physical Review D. College Pk: Amer Physical Soc, v. 96, n. 8, 14 p., 2017.2470-0010http://hdl.handle.net/11449/16343610.1103/PhysRevD.96.084064WOS:000413900000009WOS000413900000009.pdfWeb of Sciencereponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review D1,801info:eu-repo/semantics/openAccess2023-10-05T06:02:04Zoai:repositorio.unesp.br:11449/163436Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T14:02:20.922775Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Radiation reaction for spinning bodies in effective field theory. I. Spin-orbit effects |
title |
Radiation reaction for spinning bodies in effective field theory. I. Spin-orbit effects |
spellingShingle |
Radiation reaction for spinning bodies in effective field theory. I. Spin-orbit effects Maia, Natalia T. [UNESP] |
title_short |
Radiation reaction for spinning bodies in effective field theory. I. Spin-orbit effects |
title_full |
Radiation reaction for spinning bodies in effective field theory. I. Spin-orbit effects |
title_fullStr |
Radiation reaction for spinning bodies in effective field theory. I. Spin-orbit effects |
title_full_unstemmed |
Radiation reaction for spinning bodies in effective field theory. I. Spin-orbit effects |
title_sort |
Radiation reaction for spinning bodies in effective field theory. I. Spin-orbit 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 linear order in the spin to the radiationreaction acceleration and spin evolution for binary systems, which enter at fourth PN order. The calculation is carried out, from first principles, using the effective field theory framework for spinning compact objects, in both the Newton-Wigner and covariant spin supplementary conditions. A nontrivial consistency check is performed on our results by showing that the energy loss induced by the resulting radiation-reaction force is equivalent to the total emitted power in the far zone, up to so-called Schott terms. We also find that, at this order, the radiation reaction has no net effect on the evolution of the spins. The spin-spin contributions to radiation reaction are reported in a companion paper. |
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.96.084064 Physical Review D. College Pk: Amer Physical Soc, v. 96, n. 8, 14 p., 2017. 2470-0010 http://hdl.handle.net/11449/163436 10.1103/PhysRevD.96.084064 WOS:000413900000009 WOS000413900000009.pdf |
url |
http://dx.doi.org/10.1103/PhysRevD.96.084064 http://hdl.handle.net/11449/163436 |
identifier_str_mv |
Physical Review D. College Pk: Amer Physical Soc, v. 96, n. 8, 14 p., 2017. 2470-0010 10.1103/PhysRevD.96.084064 WOS:000413900000009 WOS000413900000009.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 |
14 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 |
|
_version_ |
1808128308006617088 |