Tail effect in gravitational radiation reaction: Time nonlocality and renormalization group evolution
Autor(a) principal: | |
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Data de Publicação: | 2016 |
Outros Autores: | , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1103/PhysRevD.93.124010 http://hdl.handle.net/11449/161574 |
Resumo: | We use the effective field theory (EFT) framework to calculate the tail effect in gravitational radiation reaction, which enters at the fourth post-Newtonian order in the dynamics of a binary system. The computation entails a subtle interplay between the near (or potential) and far (or radiation) zones. In particular, we find that the tail contribution to the effective action is nonlocal in time and features both a dissipative and a conservative term. The latter includes a logarithmic ultraviolet (UV) divergence, which we show cancels against an infrared (IR) singularity found in the (conservative) near zone. The origin of this behavior in the long-distance EFT is due to the point-particle limit-shrinking the binary to a point-which transforms a would-be infrared singularity into an ultraviolet divergence. This is a common occurrence in an EFT approach, which furthermore allows us to use renormalization group (RG) techniques to resum the resulting logarithmic contributions. We then derive the RG evolution for the binding potential and total mass/energy, and find agreement with the results obtained imposing the conservation of the (pseudo) stress-energy tensor in the radiation theory. While the calculation of the leading tail contribution to the effective action involves only one diagram, five are needed for the one-point function. This suggests logarithmic corrections may be easier to incorporate in this fashion. We conclude with a few remarks on the nature of these IR/UV singularities, the (lack of) ambiguities recently discussed in the literature, and the completeness of the analytic post-Newtonian framework. |
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Tail effect in gravitational radiation reaction: Time nonlocality and renormalization group evolutionWe use the effective field theory (EFT) framework to calculate the tail effect in gravitational radiation reaction, which enters at the fourth post-Newtonian order in the dynamics of a binary system. The computation entails a subtle interplay between the near (or potential) and far (or radiation) zones. In particular, we find that the tail contribution to the effective action is nonlocal in time and features both a dissipative and a conservative term. The latter includes a logarithmic ultraviolet (UV) divergence, which we show cancels against an infrared (IR) singularity found in the (conservative) near zone. The origin of this behavior in the long-distance EFT is due to the point-particle limit-shrinking the binary to a point-which transforms a would-be infrared singularity into an ultraviolet divergence. This is a common occurrence in an EFT approach, which furthermore allows us to use renormalization group (RG) techniques to resum the resulting logarithmic contributions. We then derive the RG evolution for the binding potential and total mass/energy, and find agreement with the results obtained imposing the conservation of the (pseudo) stress-energy tensor in the radiation theory. While the calculation of the leading tail contribution to the effective action involves only one diagram, five are needed for the one-point function. This suggests logarithmic corrections may be easier to incorporate in this fashion. We conclude with a few remarks on the nature of these IR/UV singularities, the (lack of) ambiguities recently discussed in the literature, and the completeness of the analytic post-Newtonian framework.NSFBrinson FoundationSimons FoundationFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)NASACALTECH, Walter Burke Inst Theoret Phys, Theoret Astrophys TAPIR, Pasadena, CA 91125 USAUniv Pittsburgh, Dept Phys & Astron, Pittsburgh Particle Phys Astrophys & Cosmol Ctr P, Pittsburgh, PA 15260 USAUniv Estadual Paulista, Inst Fis Teor, ICTP South Amer Inst Fundamental Res, Rua Dr Bento Teobaldo Ferraz 271, BR-01140070 Sao Paulo, BrazilCarnegie Mellon Univ, Dept Phys & Astron, Pittsburgh, PA 15213 USAUniv Estadual Paulista, Inst Fis Teor, ICTP South Amer Inst Fundamental Res, Rua Dr Bento Teobaldo Ferraz 271, BR-01140070 Sao Paulo, BrazilNSF: PHY-1404569NSF: PHY-1519175FAPESP: 2014/25212-3FAPESP: 2014/10748-5NASA: 22645.1.1110173Amer Physical SocCALTECHUniv PittsburghUniversidade Estadual Paulista (Unesp)Carnegie Mellon UnivGalley, Chad R.Leibovich, Adam K.Porto, Rafael A. [UNESP]Ross, Andreas2018-11-26T16:34:50Z2018-11-26T16:34:50Z2016-06-06info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article13http://dx.doi.org/10.1103/PhysRevD.93.124010Physical Review D. College Pk: Amer Physical Soc, v. 93, n. 12, 13 p., 2016.2470-0010http://hdl.handle.net/11449/16157410.1103/PhysRevD.93.124010WOS:000377303400005Web of Sciencereponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review D1,801info:eu-repo/semantics/openAccess2021-10-23T17:36:58Zoai:repositorio.unesp.br:11449/161574Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T13:41:19.827326Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Tail effect in gravitational radiation reaction: Time nonlocality and renormalization group evolution |
title |
Tail effect in gravitational radiation reaction: Time nonlocality and renormalization group evolution |
spellingShingle |
Tail effect in gravitational radiation reaction: Time nonlocality and renormalization group evolution Galley, Chad R. |
title_short |
Tail effect in gravitational radiation reaction: Time nonlocality and renormalization group evolution |
title_full |
Tail effect in gravitational radiation reaction: Time nonlocality and renormalization group evolution |
title_fullStr |
Tail effect in gravitational radiation reaction: Time nonlocality and renormalization group evolution |
title_full_unstemmed |
Tail effect in gravitational radiation reaction: Time nonlocality and renormalization group evolution |
title_sort |
Tail effect in gravitational radiation reaction: Time nonlocality and renormalization group evolution |
author |
Galley, Chad R. |
author_facet |
Galley, Chad R. Leibovich, Adam K. Porto, Rafael A. [UNESP] Ross, Andreas |
author_role |
author |
author2 |
Leibovich, Adam K. Porto, Rafael A. [UNESP] Ross, Andreas |
author2_role |
author author author |
dc.contributor.none.fl_str_mv |
CALTECH Univ Pittsburgh Universidade Estadual Paulista (Unesp) Carnegie Mellon Univ |
dc.contributor.author.fl_str_mv |
Galley, Chad R. Leibovich, Adam K. Porto, Rafael A. [UNESP] Ross, Andreas |
description |
We use the effective field theory (EFT) framework to calculate the tail effect in gravitational radiation reaction, which enters at the fourth post-Newtonian order in the dynamics of a binary system. The computation entails a subtle interplay between the near (or potential) and far (or radiation) zones. In particular, we find that the tail contribution to the effective action is nonlocal in time and features both a dissipative and a conservative term. The latter includes a logarithmic ultraviolet (UV) divergence, which we show cancels against an infrared (IR) singularity found in the (conservative) near zone. The origin of this behavior in the long-distance EFT is due to the point-particle limit-shrinking the binary to a point-which transforms a would-be infrared singularity into an ultraviolet divergence. This is a common occurrence in an EFT approach, which furthermore allows us to use renormalization group (RG) techniques to resum the resulting logarithmic contributions. We then derive the RG evolution for the binding potential and total mass/energy, and find agreement with the results obtained imposing the conservation of the (pseudo) stress-energy tensor in the radiation theory. While the calculation of the leading tail contribution to the effective action involves only one diagram, five are needed for the one-point function. This suggests logarithmic corrections may be easier to incorporate in this fashion. We conclude with a few remarks on the nature of these IR/UV singularities, the (lack of) ambiguities recently discussed in the literature, and the completeness of the analytic post-Newtonian framework. |
publishDate |
2016 |
dc.date.none.fl_str_mv |
2016-06-06 2018-11-26T16:34:50Z 2018-11-26T16:34:50Z |
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.93.124010 Physical Review D. College Pk: Amer Physical Soc, v. 93, n. 12, 13 p., 2016. 2470-0010 http://hdl.handle.net/11449/161574 10.1103/PhysRevD.93.124010 WOS:000377303400005 |
url |
http://dx.doi.org/10.1103/PhysRevD.93.124010 http://hdl.handle.net/11449/161574 |
identifier_str_mv |
Physical Review D. College Pk: Amer Physical Soc, v. 93, n. 12, 13 p., 2016. 2470-0010 10.1103/PhysRevD.93.124010 WOS:000377303400005 |
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 |
13 |
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_ |
1808128264975155200 |