Is ΛCDM an effective CCDM cosmology?
Autor(a) principal: | |
---|---|
Data de Publicação: | 2016 |
Outros Autores: | , |
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 |
id |
UFRN_0765d3a5c6d175fbfb1f4edec4c78f16 |
---|---|
oai_identifier_str |
oai:https://repositorio.ufrn.br:123456789/30961 |
network_acronym_str |
UFRN |
network_name_str |
Repositório Institucional da UFRN |
repository_id_str |
|
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 |
format |
article |
status_str |
publishedVersion |
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 10.1088/1475-7516/2016/03/027 |
url |
https://repositorio.ufrn.br/handle/123456789/30961 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.publisher.none.fl_str_mv |
IOP Publishing |
publisher.none.fl_str_mv |
IOP Publishing |
dc.source.none.fl_str_mv |
reponame:Repositório Institucional da UFRN instname:Universidade Federal do Rio Grande do Norte (UFRN) instacron:UFRN |
instname_str |
Universidade Federal do Rio Grande do Norte (UFRN) |
instacron_str |
UFRN |
institution |
UFRN |
reponame_str |
Repositório Institucional da UFRN |
collection |
Repositório Institucional da UFRN |
bitstream.url.fl_str_mv |
https://repositorio.ufrn.br/bitstream/123456789/30961/2/license_rdf https://repositorio.ufrn.br/bitstream/123456789/30961/3/license.txt https://repositorio.ufrn.br/bitstream/123456789/30961/4/%ce%9bCDMEffective_CUNHA_2016.pdf.txt https://repositorio.ufrn.br/bitstream/123456789/30961/5/%ce%9bCDMEffective_CUNHA_2016.pdf.jpg |
bitstream.checksum.fl_str_mv |
4d2950bda3d176f570a9f8b328dfbbef e9597aa2854d128fd968be5edc8a28d9 5ed4369bc59cab9983976f16d6635d99 8b8e287881abbdf8c19143067a72df7a |
bitstream.checksumAlgorithm.fl_str_mv |
MD5 MD5 MD5 MD5 |
repository.name.fl_str_mv |
Repositório Institucional da UFRN - Universidade Federal do Rio Grande do Norte (UFRN) |
repository.mail.fl_str_mv |
|
_version_ |
1814833025833238528 |