Improved constraints on violations of the Einstein equivalence principle in the electromagnetic sector with complementary cosmic probes

Detalhes bibliográficos
Autor(a) principal: Holanda, R. F.L.
Data de Publicação: 2017
Outros Autores: Pereira, S. H. [UNESP], Busti, V. C., Bessa, C. H.G.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1088/1361-6382/aa8828
http://hdl.handle.net/11449/175501
Resumo: Recent results have shown that a field non-minimally coupled to the electromagnetic Lagrangian can induce a violation of the Einstein equivalence principle. This kind of coupling is present in a very wide class of gravitation theories. In a cosmological context, this would break the validity of the cosmic distance duality relation as well as cause a time variation of the fine structure constant. Here, we improve constraints on this scenario by using four different observables: the luminosity distance of type Ia supernovae, the angular diameter distance of galaxy clusters, the gas mass fraction of galaxy clusters and the temperature of the cosmic microwave background at different redshifts. We consider four standard parametrizations adopted in the literature and show that, due to a high complementarity of the data, the errors are shrunk between 20% and 40% depending on the parametrization. We also show that our constraints are weakly affected by the geometry considered to describe the galaxy clusters. In short, no violation of the Einstein equivalence principle is detected up to redshifts ∼3.
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spelling Improved constraints on violations of the Einstein equivalence principle in the electromagnetic sector with complementary cosmic probescosmologygeneral relativity theory modified, distance scaleRecent results have shown that a field non-minimally coupled to the electromagnetic Lagrangian can induce a violation of the Einstein equivalence principle. This kind of coupling is present in a very wide class of gravitation theories. In a cosmological context, this would break the validity of the cosmic distance duality relation as well as cause a time variation of the fine structure constant. Here, we improve constraints on this scenario by using four different observables: the luminosity distance of type Ia supernovae, the angular diameter distance of galaxy clusters, the gas mass fraction of galaxy clusters and the temperature of the cosmic microwave background at different redshifts. We consider four standard parametrizations adopted in the literature and show that, due to a high complementarity of the data, the errors are shrunk between 20% and 40% depending on the parametrization. We also show that our constraints are weakly affected by the geometry considered to describe the galaxy clusters. In short, no violation of the Einstein equivalence principle is detected up to redshifts ∼3.Departamento de Física Universidade Federal de SergipeDepartamento de Física Universidade Federal de Campina GrandeDepartamento de Física Universidade Federal Do Rio Grande Do NorteDepartamento de Física e Química Universidade Estadual Paulista (Unesp) Faculdade de Engenharia, Guaratingueta, Av. Dr. Ariberto Pereira da Cunha 333Department of Physics and Astronomy University of PennsylvaniaDepartamento de Física Matemática Universidade de São Paulo, Rua do Matão 1371Departamento de Física Universidade Federal da ParaíbaDepartamento de Física e Química Universidade Estadual Paulista (Unesp) Faculdade de Engenharia, Guaratingueta, Av. Dr. Ariberto Pereira da Cunha 333Universidade Federal de Sergipe (UFS)Universidade Federal de Campina GrandeUniversidade Federal Do Rio Grande Do NorteUniversidade Estadual Paulista (Unesp)University of PennsylvaniaUniversidade de São Paulo (USP)Universidade Federal da Paraíba (UFPB)Holanda, R. F.L.Pereira, S. H. [UNESP]Busti, V. C.Bessa, C. H.G.2018-12-11T17:16:04Z2018-12-11T17:16:04Z2017-09-11info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://dx.doi.org/10.1088/1361-6382/aa8828Classical and Quantum Gravity, v. 34, n. 19, 2017.1361-63820264-9381http://hdl.handle.net/11449/17550110.1088/1361-6382/aa88282-s2.0-850342627772-s2.0-85034262777.pdfScopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengClassical and Quantum Gravity1,809info:eu-repo/semantics/openAccess2023-10-02T06:08:18Zoai:repositorio.unesp.br:11449/175501Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462023-10-02T06:08:18Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Improved constraints on violations of the Einstein equivalence principle in the electromagnetic sector with complementary cosmic probes
title Improved constraints on violations of the Einstein equivalence principle in the electromagnetic sector with complementary cosmic probes
spellingShingle Improved constraints on violations of the Einstein equivalence principle in the electromagnetic sector with complementary cosmic probes
Holanda, R. F.L.
cosmology
general relativity theory modified, distance scale
title_short Improved constraints on violations of the Einstein equivalence principle in the electromagnetic sector with complementary cosmic probes
title_full Improved constraints on violations of the Einstein equivalence principle in the electromagnetic sector with complementary cosmic probes
title_fullStr Improved constraints on violations of the Einstein equivalence principle in the electromagnetic sector with complementary cosmic probes
title_full_unstemmed Improved constraints on violations of the Einstein equivalence principle in the electromagnetic sector with complementary cosmic probes
title_sort Improved constraints on violations of the Einstein equivalence principle in the electromagnetic sector with complementary cosmic probes
author Holanda, R. F.L.
author_facet Holanda, R. F.L.
Pereira, S. H. [UNESP]
Busti, V. C.
Bessa, C. H.G.
author_role author
author2 Pereira, S. H. [UNESP]
Busti, V. C.
Bessa, C. H.G.
author2_role author
author
author
dc.contributor.none.fl_str_mv Universidade Federal de Sergipe (UFS)
Universidade Federal de Campina Grande
Universidade Federal Do Rio Grande Do Norte
Universidade Estadual Paulista (Unesp)
University of Pennsylvania
Universidade de São Paulo (USP)
Universidade Federal da Paraíba (UFPB)
dc.contributor.author.fl_str_mv Holanda, R. F.L.
Pereira, S. H. [UNESP]
Busti, V. C.
Bessa, C. H.G.
dc.subject.por.fl_str_mv cosmology
general relativity theory modified, distance scale
topic cosmology
general relativity theory modified, distance scale
description Recent results have shown that a field non-minimally coupled to the electromagnetic Lagrangian can induce a violation of the Einstein equivalence principle. This kind of coupling is present in a very wide class of gravitation theories. In a cosmological context, this would break the validity of the cosmic distance duality relation as well as cause a time variation of the fine structure constant. Here, we improve constraints on this scenario by using four different observables: the luminosity distance of type Ia supernovae, the angular diameter distance of galaxy clusters, the gas mass fraction of galaxy clusters and the temperature of the cosmic microwave background at different redshifts. We consider four standard parametrizations adopted in the literature and show that, due to a high complementarity of the data, the errors are shrunk between 20% and 40% depending on the parametrization. We also show that our constraints are weakly affected by the geometry considered to describe the galaxy clusters. In short, no violation of the Einstein equivalence principle is detected up to redshifts ∼3.
publishDate 2017
dc.date.none.fl_str_mv 2017-09-11
2018-12-11T17:16:04Z
2018-12-11T17:16:04Z
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/10.1088/1361-6382/aa8828
Classical and Quantum Gravity, v. 34, n. 19, 2017.
1361-6382
0264-9381
http://hdl.handle.net/11449/175501
10.1088/1361-6382/aa8828
2-s2.0-85034262777
2-s2.0-85034262777.pdf
url http://dx.doi.org/10.1088/1361-6382/aa8828
http://hdl.handle.net/11449/175501
identifier_str_mv Classical and Quantum Gravity, v. 34, n. 19, 2017.
1361-6382
0264-9381
10.1088/1361-6382/aa8828
2-s2.0-85034262777
2-s2.0-85034262777.pdf
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Classical and Quantum Gravity
1,809
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
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_ 1799964408672157696