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

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Autor(es): dc.contributorCalifornia Institute of Technology-
Autor(es): dc.contributorUniversity of Pittsburgh-
Autor(es): dc.contributorUniversidade Estadual Paulista (UNESP)-
Autor(es): dc.contributorAstronomy Carnegie Mellon University-
Autor(es): dc.creatorGalley, Chad R.-
Autor(es): dc.creatorLeibovich, Adam K.-
Autor(es): dc.creatorPorto, Rafael A.-
Autor(es): dc.creatorRoss, Andreas-
Data de aceite: dc.date.accessioned2025-08-21T19:47:52Z-
Data de disponibilização: dc.date.available2025-08-21T19:47:52Z-
Data de envio: dc.date.issued2022-04-29-
Data de envio: dc.date.issued2022-04-29-
Data de envio: dc.date.issued2016-06-06-
Fonte completa do material: dc.identifierhttp://dx.doi.org/10.1103/PhysRevD.93.124010-
Fonte completa do material: dc.identifierhttp://hdl.handle.net/11449/228162-
Fonte: dc.identifier.urihttp://educapes.capes.gov.br/handle/11449/228162-
Descrição: dc.descriptionWe 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.-
Descrição: dc.descriptionCalifornia Institute of Technology-
Descrição: dc.descriptionFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)-
Descrição: dc.descriptionNational Aeronautics and Space Administration-
Descrição: dc.descriptionNational Stroke Foundation-
Descrição: dc.descriptionTheoretical Astrophysics (TAPIR) Walter Burke Institute for Theoretical Physics California Institute of Technology-
Descrição: dc.descriptionPittsburgh Particle Physics Astrophysics and Cosmology Center (PITT PACC) Department of Physics and Astronomy University of Pittsburgh-
Descrição: dc.descriptionICTP South American Institute for Fundamental Research Instituto de Física Teórica Universidade Estadual Paulista, Rua Dr. Bento Teobaldo Ferraz 271-
Descrição: dc.descriptionDepartment of Physics Astronomy Carnegie Mellon University-
Descrição: dc.descriptionICTP South American Institute for Fundamental Research Instituto de Física Teórica Universidade Estadual Paulista, Rua Dr. Bento Teobaldo Ferraz 271-
Descrição: dc.descriptionFAPESP: 2014/10748-5-
Descrição: dc.descriptionFAPESP: 2014/25212-3-
Descrição: dc.descriptionNational Aeronautics and Space Administration: 22645.1.1110173-
Descrição: dc.descriptionNational Stroke Foundation: PHY-1404569-
Descrição: dc.descriptionNational Stroke Foundation: PHY-1519175-
Idioma: dc.languageen-
Relação: dc.relationPhysical Review D-
???dc.source???: dc.sourceScopus-
Título: dc.titleTail effect in gravitational radiation reaction: Time nonlocality and renormalization group evolution-
Tipo de arquivo: dc.typelivro digital-
Aparece nas coleções:Repositório Institucional - Unesp

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