Galaxy cluster Sunyaev-Zel'dovich effect scaling-relation and type Ia supernova observations as a test for the cosmic distance duality relation
Autor(a) principal: | |
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Data de Publicação: | 2019 |
Outros Autores: | , , |
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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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 |
|
_version_ |
1799964940372541440 |