Tail effect in gravitational radiation reaction: Time nonlocality and renormalization group evolution

Detalhes bibliográficos
Autor(a) principal: Galley, Chad R.
Data de Publicação: 2016
Outros Autores: Leibovich, Adam K., Porto, Rafael A. [UNESP], Ross, Andreas
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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spelling 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)
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