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/11449/228162 |
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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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) |
repository.mail.fl_str_mv |
|
_version_ |
1808129078524379136 |