Is ΛCDM an effective CCDM cosmology?

Detalhes bibliográficos
Autor(a) principal: Cunha Junior, Joao Vital
Data de Publicação: 2016
Outros Autores: Lima, J. A. S., Santos, R.C.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UFRN
Texto Completo: https://repositorio.ufrn.br/handle/123456789/30961
Resumo: We show that a cosmology driven by gravitationally induced particle production of all non-relativistic species existing in the present Universe mimics exactly the observed flat accelerating ΛCDM cosmology with just one dynamical free parameter. This kind of scenario includes the creation cold dark matter (CCDM) model [1] as a particular case and also provides a natural reduction of the dark sector since the vacuum component is not needed to accelerate the Universe. The new cosmic scenario is equivalent to ΛCDM both at the background and perturbative levels and the associated creation process is also in agreement with the universality of the gravitational interaction and equivalence principle. Implicitly, it also suggests that the present day astronomical observations cannot be considered the ultimate proof of cosmic vacuum effects in the evolved Universe because ΛCDM may be only an effective cosmology
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spelling Cunha Junior, Joao VitalLima, J. A. S.Santos, R.C.2020-12-11T15:55:44Z2020-12-11T15:55:44Z2016-03-15LIMA, J.A.S.; SANTOS, R.C.; CUNHA, J.V.. Is ΛCDM an effective CCDM cosmology? Journal of Cosmology and Astroparticle Physics, [S.L.], v. 2016, n. 03, p. 027-027, 15 mar. 2016. Disponível em: https://iopscience.iop.org/article/10.1088/1475-7516/2016/03/027. Acesso em: 16 out. 2020. http://dx.doi.org/10.1088/1475-7516/2016/03/027.1475-7516https://repositorio.ufrn.br/handle/123456789/3096110.1088/1475-7516/2016/03/027IOP PublishingDark matter theoryGalaxy clusteringIs ΛCDM an effective CCDM cosmology?info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleWe show that a cosmology driven by gravitationally induced particle production of all non-relativistic species existing in the present Universe mimics exactly the observed flat accelerating ΛCDM cosmology with just one dynamical free parameter. This kind of scenario includes the creation cold dark matter (CCDM) model [1] as a particular case and also provides a natural reduction of the dark sector since the vacuum component is not needed to accelerate the Universe. The new cosmic scenario is equivalent to ΛCDM both at the background and perturbative levels and the associated creation process is also in agreement with the universality of the gravitational interaction and equivalence principle. Implicitly, it also suggests that the present day astronomical observations cannot be considered the ultimate proof of cosmic vacuum effects in the evolved Universe because ΛCDM may be only an effective cosmologyengreponame:Repositório Institucional da UFRNinstname:Universidade Federal do Rio Grande do Norte (UFRN)instacron:UFRNinfo:eu-repo/semantics/openAccessCC-LICENSElicense_rdflicense_rdfapplication/rdf+xml; charset=utf-8914https://repositorio.ufrn.br/bitstream/123456789/30961/2/license_rdf4d2950bda3d176f570a9f8b328dfbbefMD52LICENSElicense.txtlicense.txttext/plain; charset=utf-81484https://repositorio.ufrn.br/bitstream/123456789/30961/3/license.txte9597aa2854d128fd968be5edc8a28d9MD53TEXTΛCDMEffective_CUNHA_2016.pdf.txtΛCDMEffective_CUNHA_2016.pdf.txtExtracted texttext/plain30792https://repositorio.ufrn.br/bitstream/123456789/30961/4/%ce%9bCDMEffective_CUNHA_2016.pdf.txt5ed4369bc59cab9983976f16d6635d99MD54THUMBNAILΛCDMEffective_CUNHA_2016.pdf.jpgΛCDMEffective_CUNHA_2016.pdf.jpgGenerated Thumbnailimage/jpeg1234https://repositorio.ufrn.br/bitstream/123456789/30961/5/%ce%9bCDMEffective_CUNHA_2016.pdf.jpg8b8e287881abbdf8c19143067a72df7aMD55123456789/309612022-10-19 18:37:40.195oai:https://repositorio.ufrn.br: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Repositório de PublicaçõesPUBhttp://repositorio.ufrn.br/oai/opendoar:2022-10-19T21:37:40Repositório Institucional da UFRN - Universidade Federal do Rio Grande do Norte (UFRN)false
dc.title.pt_BR.fl_str_mv Is ΛCDM an effective CCDM cosmology?
title Is ΛCDM an effective CCDM cosmology?
spellingShingle Is ΛCDM an effective CCDM cosmology?
Cunha Junior, Joao Vital
Dark matter theory
Galaxy clustering
title_short Is ΛCDM an effective CCDM cosmology?
title_full Is ΛCDM an effective CCDM cosmology?
title_fullStr Is ΛCDM an effective CCDM cosmology?
title_full_unstemmed Is ΛCDM an effective CCDM cosmology?
title_sort Is ΛCDM an effective CCDM cosmology?
author Cunha Junior, Joao Vital
author_facet Cunha Junior, Joao Vital
Lima, J. A. S.
Santos, R.C.
author_role author
author2 Lima, J. A. S.
Santos, R.C.
author2_role author
author
dc.contributor.author.fl_str_mv Cunha Junior, Joao Vital
Lima, J. A. S.
Santos, R.C.
dc.subject.por.fl_str_mv Dark matter theory
Galaxy clustering
topic Dark matter theory
Galaxy clustering
description We show that a cosmology driven by gravitationally induced particle production of all non-relativistic species existing in the present Universe mimics exactly the observed flat accelerating ΛCDM cosmology with just one dynamical free parameter. This kind of scenario includes the creation cold dark matter (CCDM) model [1] as a particular case and also provides a natural reduction of the dark sector since the vacuum component is not needed to accelerate the Universe. The new cosmic scenario is equivalent to ΛCDM both at the background and perturbative levels and the associated creation process is also in agreement with the universality of the gravitational interaction and equivalence principle. Implicitly, it also suggests that the present day astronomical observations cannot be considered the ultimate proof of cosmic vacuum effects in the evolved Universe because ΛCDM may be only an effective cosmology
publishDate 2016
dc.date.issued.fl_str_mv 2016-03-15
dc.date.accessioned.fl_str_mv 2020-12-11T15:55:44Z
dc.date.available.fl_str_mv 2020-12-11T15:55:44Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
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dc.identifier.citation.fl_str_mv LIMA, J.A.S.; SANTOS, R.C.; CUNHA, J.V.. Is ΛCDM an effective CCDM cosmology? Journal of Cosmology and Astroparticle Physics, [S.L.], v. 2016, n. 03, p. 027-027, 15 mar. 2016. Disponível em: https://iopscience.iop.org/article/10.1088/1475-7516/2016/03/027. Acesso em: 16 out. 2020. http://dx.doi.org/10.1088/1475-7516/2016/03/027.
dc.identifier.uri.fl_str_mv https://repositorio.ufrn.br/handle/123456789/30961
dc.identifier.issn.none.fl_str_mv 1475-7516
dc.identifier.doi.none.fl_str_mv 10.1088/1475-7516/2016/03/027
identifier_str_mv LIMA, J.A.S.; SANTOS, R.C.; CUNHA, J.V.. Is ΛCDM an effective CCDM cosmology? Journal of Cosmology and Astroparticle Physics, [S.L.], v. 2016, n. 03, p. 027-027, 15 mar. 2016. Disponível em: https://iopscience.iop.org/article/10.1088/1475-7516/2016/03/027. Acesso em: 16 out. 2020. http://dx.doi.org/10.1088/1475-7516/2016/03/027.
1475-7516
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