Bayesian correction of H(z) data uncertainties

Detalhes bibliográficos
Autor(a) principal: Jesus, J. F. [UNESP]
Data de Publicação: 2018
Outros Autores: Gregório, T. M. [UNESP], Andrade-Oliveira, F. [UNESP], Valentim, R., Matos, C. A.O. [UNESP]
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1093/mnras/sty813
http://hdl.handle.net/11449/176338
Resumo: We compile 41 H(z) data from literature and use them to constrain OΛCDM and flat ΛCDM parameters. We show that the available H(z) suffers from uncertainties overestimation and propose a Bayesian method to reduce them. As a result of this method, using H(z) only, we find, in the context of OΛCDM, H0 = 69.5 ± 2.5 kms-1 Mpc-1, Ωm = 0.242 ± 0.036, and ΩΛ = 0.68 ± 0.14. In the context of flatΛCDMmodel,we have foundH0 =70.4±1.2 kms-1 Mpc-1 and Ωm = 0.256 ± 0.014. This corresponds to an uncertainty reduction of up to ≈30 per cent when compared to the uncorrected analysis in both cases.
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spelling Bayesian correction of H(z) data uncertaintiesCosmological parametersCosmology: ObservationsDark energyDark matterWe compile 41 H(z) data from literature and use them to constrain OΛCDM and flat ΛCDM parameters. We show that the available H(z) suffers from uncertainties overestimation and propose a Bayesian method to reduce them. As a result of this method, using H(z) only, we find, in the context of OΛCDM, H0 = 69.5 ± 2.5 kms-1 Mpc-1, Ωm = 0.242 ± 0.036, and ΩΛ = 0.68 ± 0.14. In the context of flatΛCDMmodel,we have foundH0 =70.4±1.2 kms-1 Mpc-1 and Ωm = 0.256 ± 0.014. This corresponds to an uncertainty reduction of up to ≈30 per cent when compared to the uncorrected analysis in both cases.Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)Universidade Estadual Paulista (UNESP) Câmpus Experimental de Itapeva, Rua Geraldo Alckmin 519, Vila N. Sra. de FátimaUniversidade Estadual Paulista (UNESP) Faculdade de Engenharia Guaratinguetá Departamento de Física e Química, Av. Dr. Ariberto Pereira da Cunha 333Universidade Estadual Paulista (UNESP) Instituto de Física TeóricaLaboratório Interinstitucional de e-Astronomia - LIneA, Rua General José Cristino, 77Departamento de Física Instituto de Ciências Ambientais Químicas e Farmacêuticas - ICAQF Universidade Federal de São Paulo (UNIFESP) Unidade José Alencar, Rua São Nicolau No. 210Universidade Estadual Paulista (UNESP) Câmpus Experimental de Itapeva, Rua Geraldo Alckmin 519, Vila N. Sra. de FátimaUniversidade Estadual Paulista (UNESP) Faculdade de Engenharia Guaratinguetá Departamento de Física e Química, Av. Dr. Ariberto Pereira da Cunha 333Universidade Estadual Paulista (UNESP) Instituto de Física TeóricaCNPq: 465376/2014-2Universidade Estadual Paulista (Unesp)Laboratório Interinstitucional de e-Astronomia - LIneAUniversidade Federal de São Paulo (UNIFESP)Jesus, J. F. [UNESP]Gregório, T. M. [UNESP]Andrade-Oliveira, F. [UNESP]Valentim, R.Matos, C. A.O. [UNESP]2018-12-11T17:20:11Z2018-12-11T17:20:11Z2018-07-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article2867-2873application/pdfhttp://dx.doi.org/10.1093/mnras/sty813Monthly Notices of the Royal Astronomical Society, v. 477, n. 3, p. 2867-2873, 2018.1365-29660035-8711http://hdl.handle.net/11449/17633810.1093/mnras/sty8132-s2.0-850471073682-s2.0-85047107368.pdfScopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengMonthly Notices of the Royal Astronomical Society2,3462,346info:eu-repo/semantics/openAccess2024-01-08T06:23:50Zoai:repositorio.unesp.br:11449/176338Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-01-08T06:23:50Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Bayesian correction of H(z) data uncertainties
title Bayesian correction of H(z) data uncertainties
spellingShingle Bayesian correction of H(z) data uncertainties
Jesus, J. F. [UNESP]
Cosmological parameters
Cosmology: Observations
Dark energy
Dark matter
title_short Bayesian correction of H(z) data uncertainties
title_full Bayesian correction of H(z) data uncertainties
title_fullStr Bayesian correction of H(z) data uncertainties
title_full_unstemmed Bayesian correction of H(z) data uncertainties
title_sort Bayesian correction of H(z) data uncertainties
author Jesus, J. F. [UNESP]
author_facet Jesus, J. F. [UNESP]
Gregório, T. M. [UNESP]
Andrade-Oliveira, F. [UNESP]
Valentim, R.
Matos, C. A.O. [UNESP]
author_role author
author2 Gregório, T. M. [UNESP]
Andrade-Oliveira, F. [UNESP]
Valentim, R.
Matos, C. A.O. [UNESP]
author2_role author
author
author
author
dc.contributor.none.fl_str_mv Universidade Estadual Paulista (Unesp)
Laboratório Interinstitucional de e-Astronomia - LIneA
Universidade Federal de São Paulo (UNIFESP)
dc.contributor.author.fl_str_mv Jesus, J. F. [UNESP]
Gregório, T. M. [UNESP]
Andrade-Oliveira, F. [UNESP]
Valentim, R.
Matos, C. A.O. [UNESP]
dc.subject.por.fl_str_mv Cosmological parameters
Cosmology: Observations
Dark energy
Dark matter
topic Cosmological parameters
Cosmology: Observations
Dark energy
Dark matter
description We compile 41 H(z) data from literature and use them to constrain OΛCDM and flat ΛCDM parameters. We show that the available H(z) suffers from uncertainties overestimation and propose a Bayesian method to reduce them. As a result of this method, using H(z) only, we find, in the context of OΛCDM, H0 = 69.5 ± 2.5 kms-1 Mpc-1, Ωm = 0.242 ± 0.036, and ΩΛ = 0.68 ± 0.14. In the context of flatΛCDMmodel,we have foundH0 =70.4±1.2 kms-1 Mpc-1 and Ωm = 0.256 ± 0.014. This corresponds to an uncertainty reduction of up to ≈30 per cent when compared to the uncorrected analysis in both cases.
publishDate 2018
dc.date.none.fl_str_mv 2018-12-11T17:20:11Z
2018-12-11T17:20:11Z
2018-07-01
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/10.1093/mnras/sty813
Monthly Notices of the Royal Astronomical Society, v. 477, n. 3, p. 2867-2873, 2018.
1365-2966
0035-8711
http://hdl.handle.net/11449/176338
10.1093/mnras/sty813
2-s2.0-85047107368
2-s2.0-85047107368.pdf
url http://dx.doi.org/10.1093/mnras/sty813
http://hdl.handle.net/11449/176338
identifier_str_mv Monthly Notices of the Royal Astronomical Society, v. 477, n. 3, p. 2867-2873, 2018.
1365-2966
0035-8711
10.1093/mnras/sty813
2-s2.0-85047107368
2-s2.0-85047107368.pdf
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Monthly Notices of the Royal Astronomical Society
2,346
2,346
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 2867-2873
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
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