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/11449/228162
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.California Institute of TechnologyFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)National Aeronautics and Space AdministrationNational Stroke FoundationTheoretical Astrophysics (TAPIR) Walter Burke Institute for Theoretical Physics California Institute of TechnologyPittsburgh Particle Physics Astrophysics and Cosmology Center (PITT PACC) Department of Physics and Astronomy University of PittsburghICTP South American Institute for Fundamental Research Instituto de Física Teórica Universidade Estadual Paulista, Rua Dr. Bento Teobaldo Ferraz 271Department of Physics Astronomy Carnegie Mellon UniversityICTP South American Institute for Fundamental Research Instituto de Física Teórica Universidade Estadual Paulista, Rua Dr. Bento Teobaldo Ferraz 271FAPESP: 2014/10748-5FAPESP: 2014/25212-3National Aeronautics and Space Administration: 22645.1.1110173National Stroke Foundation: PHY-1404569National Stroke Foundation: PHY-1519175California Institute of TechnologyUniversity of PittsburghUniversidade Estadual Paulista (UNESP)Astronomy Carnegie Mellon UniversityGalley, Chad R.Leibovich, Adam K.Porto, Rafael A. [UNESP]Ross, Andreas2022-04-29T07:37:28Z2022-04-29T07:37:28Z2016-06-06info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1103/PhysRevD.93.124010Physical Review D, v. 93, n. 12, 2016.2470-00292470-0010http://hdl.handle.net/11449/22816210.1103/PhysRevD.93.1240102-s2.0-84974530666Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review Dinfo:eu-repo/semantics/openAccess2022-04-29T07:37:28Zoai:repositorio.unesp.br:11449/228162Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T19:30:06.597441Repositório 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 California Institute of Technology
University of Pittsburgh
Universidade Estadual Paulista (UNESP)
Astronomy Carnegie Mellon University
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
2022-04-29T07:37:28Z
2022-04-29T07:37:28Z
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, v. 93, n. 12, 2016.
2470-0029
2470-0010
http://hdl.handle.net/11449/228162
10.1103/PhysRevD.93.124010
2-s2.0-84974530666
url http://dx.doi.org/10.1103/PhysRevD.93.124010
http://hdl.handle.net/11449/228162
identifier_str_mv Physical Review D, v. 93, n. 12, 2016.
2470-0029
2470-0010
10.1103/PhysRevD.93.124010
2-s2.0-84974530666
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Physical Review D
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.source.none.fl_str_mv Scopus
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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