Radiation reaction for spinning bodies in effective field theory. I. Spin-orbit effects
Autor(a) principal: | |
---|---|
Data de Publicação: | 2017 |
Outros Autores: | , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1103/PhysRevD.96.084064 http://hdl.handle.net/11449/228408 |
Resumo: | We compute the leading post-Newtonian (PN) contributions at linear order in the spin to the radiation-reaction acceleration and spin evolution for binary systems, which enter at fourth PN order. The calculation is carried out, from first principles, using the effective field theory framework for spinning compact objects, in both the Newton-Wigner and covariant spin supplementary conditions. A nontrivial consistency check is performed on our results by showing that the energy loss induced by the resulting radiation-reaction force is equivalent to the total emitted power in the far zone, up to so-called Schott terms. We also find that, at this order, the radiation reaction has no net effect on the evolution of the spins. The spin-spin contributions to radiation reaction are reported in a companion paper. |
id |
UNSP_67fabd7424c0aaa7fead75a9512c75d0 |
---|---|
oai_identifier_str |
oai:repositorio.unesp.br:11449/228408 |
network_acronym_str |
UNSP |
network_name_str |
Repositório Institucional da UNESP |
repository_id_str |
2946 |
spelling |
Radiation reaction for spinning bodies in effective field theory. I. Spin-orbit effectsWe compute the leading post-Newtonian (PN) contributions at linear order in the spin to the radiation-reaction acceleration and spin evolution for binary systems, which enter at fourth PN order. The calculation is carried out, from first principles, using the effective field theory framework for spinning compact objects, in both the Newton-Wigner and covariant spin supplementary conditions. A nontrivial consistency check is performed on our results by showing that the energy loss induced by the resulting radiation-reaction force is equivalent to the total emitted power in the far zone, up to so-called Schott terms. We also find that, at this order, the radiation reaction has no net effect on the evolution of the spins. The spin-spin contributions to radiation reaction are reported in a companion paper.Instituto de Física Teórica Universidade Estadual Paulista, Rua Dr. Bento Teobaldo Ferraz 271Jet Propulsion Laboratory California Institute of TechnologyTheoretical Astrophysics Walter Burke Institute for Theoretical Physics California Institute of TechnologyPittsburgh Particle Physics Astrophysics and Cosmology Center Department of Physics and Astronomy University of PittsburghICTP South American Institute for Fundamental Research, Rua Dr. Bento Teobaldo Ferraz 271Instituto de Física Teórica Universidade Estadual Paulista, Rua Dr. Bento Teobaldo Ferraz 271Universidade Estadual Paulista (UNESP)California Institute of TechnologyUniversity of PittsburghICTP South American Institute for Fundamental ResearchMaia, Natália T. [UNESP]Galley, Chad R.Leibovich, Adam K.Porto, Rafael A. [UNESP]2022-04-29T08:14:39Z2022-04-29T08:14:39Z2017-10-15info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1103/PhysRevD.96.084064Physical Review D, v. 96, n. 8, 2017.2470-00292470-0010http://hdl.handle.net/11449/22840810.1103/PhysRevD.96.0840642-s2.0-85033224686Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review Dinfo:eu-repo/semantics/openAccess2022-04-29T08:14:39Zoai:repositorio.unesp.br:11449/228408Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T21:45:18.129023Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Radiation reaction for spinning bodies in effective field theory. I. Spin-orbit effects |
title |
Radiation reaction for spinning bodies in effective field theory. I. Spin-orbit effects |
spellingShingle |
Radiation reaction for spinning bodies in effective field theory. I. Spin-orbit effects Maia, Natália T. [UNESP] |
title_short |
Radiation reaction for spinning bodies in effective field theory. I. Spin-orbit effects |
title_full |
Radiation reaction for spinning bodies in effective field theory. I. Spin-orbit effects |
title_fullStr |
Radiation reaction for spinning bodies in effective field theory. I. Spin-orbit effects |
title_full_unstemmed |
Radiation reaction for spinning bodies in effective field theory. I. Spin-orbit effects |
title_sort |
Radiation reaction for spinning bodies in effective field theory. I. Spin-orbit effects |
author |
Maia, Natália T. [UNESP] |
author_facet |
Maia, Natália T. [UNESP] Galley, Chad R. Leibovich, Adam K. Porto, Rafael A. [UNESP] |
author_role |
author |
author2 |
Galley, Chad R. Leibovich, Adam K. Porto, Rafael A. [UNESP] |
author2_role |
author author author |
dc.contributor.none.fl_str_mv |
Universidade Estadual Paulista (UNESP) California Institute of Technology University of Pittsburgh ICTP South American Institute for Fundamental Research |
dc.contributor.author.fl_str_mv |
Maia, Natália T. [UNESP] Galley, Chad R. Leibovich, Adam K. Porto, Rafael A. [UNESP] |
description |
We compute the leading post-Newtonian (PN) contributions at linear order in the spin to the radiation-reaction acceleration and spin evolution for binary systems, which enter at fourth PN order. The calculation is carried out, from first principles, using the effective field theory framework for spinning compact objects, in both the Newton-Wigner and covariant spin supplementary conditions. A nontrivial consistency check is performed on our results by showing that the energy loss induced by the resulting radiation-reaction force is equivalent to the total emitted power in the far zone, up to so-called Schott terms. We also find that, at this order, the radiation reaction has no net effect on the evolution of the spins. The spin-spin contributions to radiation reaction are reported in a companion paper. |
publishDate |
2017 |
dc.date.none.fl_str_mv |
2017-10-15 2022-04-29T08:14:39Z 2022-04-29T08:14:39Z |
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.96.084064 Physical Review D, v. 96, n. 8, 2017. 2470-0029 2470-0010 http://hdl.handle.net/11449/228408 10.1103/PhysRevD.96.084064 2-s2.0-85033224686 |
url |
http://dx.doi.org/10.1103/PhysRevD.96.084064 http://hdl.handle.net/11449/228408 |
identifier_str_mv |
Physical Review D, v. 96, n. 8, 2017. 2470-0029 2470-0010 10.1103/PhysRevD.96.084064 2-s2.0-85033224686 |
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_ |
1808129355135582208 |