Galaxy cluster Sunyaev-Zel'dovich effect scaling-relation and type Ia supernova observations as a test for the cosmic distance duality relation

Detalhes bibliográficos
Autor(a) principal: Holanda, R. F.L.
Data de Publicação: 2019
Outros Autores: Colaço, L. R., Pereira, S. H. [UNESP], Silva, R.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1088/1475-7516/2019/06/008
http://hdl.handle.net/11449/189430
Resumo: In this paper, we propose a new test to the cosmic distance duality relation (CDDR), DL=DA(1+z)2, where DL and DA are the luminosity and angular diameter distances, respectively. The data used correspond to 61 Type Ia Supernova luminosity distances and YSZE-YX measurements of 61 galaxy clusters obtained by the Planck mission and the deep XMM-Newton X-ray data, where YSZE is the integrated comptonization parameter obtained via Sunyaev-Zel'dovich effect observations and YX is the X-ray counterpart. More precisely, we use the YSZEDA 2/CXSZEYX scaling-relation and a deformed CDDR, such as DL/DA(1+z)2=η(z), to verify if η(z) is compatible with the unity. Two η(z) functions are used, namely, η(z)=1+η0 z and η(z)=1+η0 z /(1+z). We obtain that the CDDR validity (η0=0) is verified within 1.5σ c.l. for both η(z) functions.
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spelling Galaxy cluster Sunyaev-Zel'dovich effect scaling-relation and type Ia supernova observations as a test for the cosmic distance duality relationGalaxy clustersSunyaev-Zeldovich effectSupernovasIn this paper, we propose a new test to the cosmic distance duality relation (CDDR), DL=DA(1+z)2, where DL and DA are the luminosity and angular diameter distances, respectively. The data used correspond to 61 Type Ia Supernova luminosity distances and YSZE-YX measurements of 61 galaxy clusters obtained by the Planck mission and the deep XMM-Newton X-ray data, where YSZE is the integrated comptonization parameter obtained via Sunyaev-Zel'dovich effect observations and YX is the X-ray counterpart. More precisely, we use the YSZEDA 2/CXSZEYX scaling-relation and a deformed CDDR, such as DL/DA(1+z)2=η(z), to verify if η(z) is compatible with the unity. Two η(z) functions are used, namely, η(z)=1+η0 z and η(z)=1+η0 z /(1+z). We obtain that the CDDR validity (η0=0) is verified within 1.5σ c.l. for both η(z) functions.Departamento de Física Teórica e Experimental Universidade Federal Do Rio Grande Do NorteDepartamento de Física Universidade Federal de SergipeUniversidade Estadual Paulista (Unesp) Faculdade de Engenharia Guaratinguetá Departamento de Física e Química, Av. Dr. Ariberto Pereira da Cunha 333Departamento de Física Universidade Do Estado Do Rio Grande Do NorteUniversidade Estadual Paulista (Unesp) Faculdade de Engenharia Guaratinguetá Departamento de Física e Química, Av. Dr. Ariberto Pereira da Cunha 333Universidade Federal Do Rio Grande Do NorteUniversidade Federal de Sergipe (UFS)Universidade Estadual Paulista (Unesp)Universidade Do Estado Do Rio Grande Do NorteHolanda, R. F.L.Colaço, L. R.Pereira, S. H. [UNESP]Silva, R.2019-10-06T16:40:30Z2019-10-06T16:40:30Z2019-06-05info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1088/1475-7516/2019/06/008Journal of Cosmology and Astroparticle Physics, v. 2019, n. 6, 2019.1475-7516http://hdl.handle.net/11449/18943010.1088/1475-7516/2019/06/0082-s2.0-85069506417Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengJournal of Cosmology and Astroparticle Physicsinfo:eu-repo/semantics/openAccess2021-10-22T22:17:21Zoai:repositorio.unesp.br:11449/189430Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462021-10-22T22:17:21Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Galaxy cluster Sunyaev-Zel'dovich effect scaling-relation and type Ia supernova observations as a test for the cosmic distance duality relation
title Galaxy cluster Sunyaev-Zel'dovich effect scaling-relation and type Ia supernova observations as a test for the cosmic distance duality relation
spellingShingle Galaxy cluster Sunyaev-Zel'dovich effect scaling-relation and type Ia supernova observations as a test for the cosmic distance duality relation
Holanda, R. F.L.
Galaxy clusters
Sunyaev-Zeldovich effect
Supernovas
title_short Galaxy cluster Sunyaev-Zel'dovich effect scaling-relation and type Ia supernova observations as a test for the cosmic distance duality relation
title_full Galaxy cluster Sunyaev-Zel'dovich effect scaling-relation and type Ia supernova observations as a test for the cosmic distance duality relation
title_fullStr Galaxy cluster Sunyaev-Zel'dovich effect scaling-relation and type Ia supernova observations as a test for the cosmic distance duality relation
title_full_unstemmed Galaxy cluster Sunyaev-Zel'dovich effect scaling-relation and type Ia supernova observations as a test for the cosmic distance duality relation
title_sort Galaxy cluster Sunyaev-Zel'dovich effect scaling-relation and type Ia supernova observations as a test for the cosmic distance duality relation
author Holanda, R. F.L.
author_facet Holanda, R. F.L.
Colaço, L. R.
Pereira, S. H. [UNESP]
Silva, R.
author_role author
author2 Colaço, L. R.
Pereira, S. H. [UNESP]
Silva, R.
author2_role author
author
author
dc.contributor.none.fl_str_mv Universidade Federal Do Rio Grande Do Norte
Universidade Federal de Sergipe (UFS)
Universidade Estadual Paulista (Unesp)
Universidade Do Estado Do Rio Grande Do Norte
dc.contributor.author.fl_str_mv Holanda, R. F.L.
Colaço, L. R.
Pereira, S. H. [UNESP]
Silva, R.
dc.subject.por.fl_str_mv Galaxy clusters
Sunyaev-Zeldovich effect
Supernovas
topic Galaxy clusters
Sunyaev-Zeldovich effect
Supernovas
description In this paper, we propose a new test to the cosmic distance duality relation (CDDR), DL=DA(1+z)2, where DL and DA are the luminosity and angular diameter distances, respectively. The data used correspond to 61 Type Ia Supernova luminosity distances and YSZE-YX measurements of 61 galaxy clusters obtained by the Planck mission and the deep XMM-Newton X-ray data, where YSZE is the integrated comptonization parameter obtained via Sunyaev-Zel'dovich effect observations and YX is the X-ray counterpart. More precisely, we use the YSZEDA 2/CXSZEYX scaling-relation and a deformed CDDR, such as DL/DA(1+z)2=η(z), to verify if η(z) is compatible with the unity. Two η(z) functions are used, namely, η(z)=1+η0 z and η(z)=1+η0 z /(1+z). We obtain that the CDDR validity (η0=0) is verified within 1.5σ c.l. for both η(z) functions.
publishDate 2019
dc.date.none.fl_str_mv 2019-10-06T16:40:30Z
2019-10-06T16:40:30Z
2019-06-05
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/10.1088/1475-7516/2019/06/008
Journal of Cosmology and Astroparticle Physics, v. 2019, n. 6, 2019.
1475-7516
http://hdl.handle.net/11449/189430
10.1088/1475-7516/2019/06/008
2-s2.0-85069506417
url http://dx.doi.org/10.1088/1475-7516/2019/06/008
http://hdl.handle.net/11449/189430
identifier_str_mv Journal of Cosmology and Astroparticle Physics, v. 2019, n. 6, 2019.
1475-7516
10.1088/1475-7516/2019/06/008
2-s2.0-85069506417
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Journal of Cosmology and Astroparticle Physics
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
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