Low-redshift effects of local structure on the Hubble parameter in presence of a cosmological constant

ABSTRACT: In order to estimate the effects of a local structure on the Hubble parameter we calculate the low-redshift expansion for H(z) and δH H for an observer at the center of a spherically symmetric matter distribution in the presence of a cosmological constant. We then test the accuracy of the...

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Autores:
Romano, Antonio Enea
Vallejo Peña, Sergio Andrés
Tipo de recurso:
Article of investigation
Fecha de publicación:
2016
Institución:
Universidad de Antioquia
Repositorio:
Repositorio UdeA
Idioma:
eng
OAI Identifier:
oai:bibliotecadigital.udea.edu.co:10495/41768
Acceso en línea:
https://hdl.handle.net/10495/41768
Palabra clave:
Energía oscura (Astronomía)
Dark energy (Astronomy)
Constantes cosmológicas
Cosmological constants
Campo profundo del Hubble
Hubble Deep Field
Desplazamiento hacia el rojo
Red shift
Astronomía geodesica
Geodetic astronomy
http://id.loc.gov/authorities/subjects/sh2001002908
http://id.loc.gov/authorities/subjects/sh2006000063
http://id.loc.gov/authorities/subjects/sh98004348
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openAccess
License
http://creativecommons.org/licenses/by/2.5/co/
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dc.title.spa.fl_str_mv Low-redshift effects of local structure on the Hubble parameter in presence of a cosmological constant
title Low-redshift effects of local structure on the Hubble parameter in presence of a cosmological constant
spellingShingle Low-redshift effects of local structure on the Hubble parameter in presence of a cosmological constant
Energía oscura (Astronomía)
Dark energy (Astronomy)
Constantes cosmológicas
Cosmological constants
Campo profundo del Hubble
Hubble Deep Field
Desplazamiento hacia el rojo
Red shift
Astronomía geodesica
Geodetic astronomy
http://id.loc.gov/authorities/subjects/sh2001002908
http://id.loc.gov/authorities/subjects/sh2006000063
http://id.loc.gov/authorities/subjects/sh98004348
title_short Low-redshift effects of local structure on the Hubble parameter in presence of a cosmological constant
title_full Low-redshift effects of local structure on the Hubble parameter in presence of a cosmological constant
title_fullStr Low-redshift effects of local structure on the Hubble parameter in presence of a cosmological constant
title_full_unstemmed Low-redshift effects of local structure on the Hubble parameter in presence of a cosmological constant
title_sort Low-redshift effects of local structure on the Hubble parameter in presence of a cosmological constant
dc.creator.fl_str_mv Romano, Antonio Enea
Vallejo Peña, Sergio Andrés
dc.contributor.author.none.fl_str_mv Romano, Antonio Enea
Vallejo Peña, Sergio Andrés
dc.contributor.researchgroup.spa.fl_str_mv COSMOGRAV
Grupo de Fenomenología de Interacciones Fundamentales
dc.subject.lcsh.none.fl_str_mv Energía oscura (Astronomía)
Dark energy (Astronomy)
Constantes cosmológicas
Cosmological constants
Campo profundo del Hubble
Hubble Deep Field
topic Energía oscura (Astronomía)
Dark energy (Astronomy)
Constantes cosmológicas
Cosmological constants
Campo profundo del Hubble
Hubble Deep Field
Desplazamiento hacia el rojo
Red shift
Astronomía geodesica
Geodetic astronomy
http://id.loc.gov/authorities/subjects/sh2001002908
http://id.loc.gov/authorities/subjects/sh2006000063
http://id.loc.gov/authorities/subjects/sh98004348
dc.subject.lemb.none.fl_str_mv Desplazamiento hacia el rojo
Red shift
Astronomía geodesica
Geodetic astronomy
dc.subject.lcshuri.none.fl_str_mv http://id.loc.gov/authorities/subjects/sh2001002908
http://id.loc.gov/authorities/subjects/sh2006000063
http://id.loc.gov/authorities/subjects/sh98004348
description ABSTRACT: In order to estimate the effects of a local structure on the Hubble parameter we calculate the low-redshift expansion for H(z) and δH H for an observer at the center of a spherically symmetric matter distribution in the presence of a cosmological constant. We then test the accuracy of the formulas comparing them with fully relativistic non perturbative numerical calculations for different cases for the density profile. The low-redshift expansion we obtain gives results more precise than perturbation theory since it is based on the use of an exact solution of Einstein’s field equations. For larger density contrasts the low-redshift formulas accuracy improves respect to the perturbation theory accuracy because the latter is based on the assumption of a small density contrast, while the former does not rely on such an assumption. The formulas can be used to take into account the effects on the Hubble expansion parameter due to the monopole component of the local structure. If the H(z) observations will show deviations from the CDM prediction compatible with the formulas we have derived, this could be considered an independent evidence of the existence of a local inhomogeneity, and the formulas could be used to determine the characteristics of this local structure.
publishDate 2016
dc.date.issued.none.fl_str_mv 2016
dc.date.accessioned.none.fl_str_mv 2024-09-04T16:27:45Z
dc.date.available.none.fl_str_mv 2024-09-04T16:27:45Z
dc.type.spa.fl_str_mv Artículo de investigación
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dc.identifier.citation.spa.fl_str_mv Romano, A. E., & Vallejo, S. A. (2016). Low-redshift effects of local structure on the Hubble parameter in presence of a cosmological constant. European Physical Journal C, 76(4), 1–7. https://doi.org/10.1140/epjc/s10052-016-4033-9
dc.identifier.issn.none.fl_str_mv 1434-6044
dc.identifier.uri.none.fl_str_mv https://hdl.handle.net/10495/41768
dc.identifier.doi.none.fl_str_mv 10.1140/epjc/s10052-016-4033-9
dc.identifier.eissn.none.fl_str_mv 1434-6052
identifier_str_mv Romano, A. E., & Vallejo, S. A. (2016). Low-redshift effects of local structure on the Hubble parameter in presence of a cosmological constant. European Physical Journal C, 76(4), 1–7. https://doi.org/10.1140/epjc/s10052-016-4033-9
1434-6044
10.1140/epjc/s10052-016-4033-9
1434-6052
url https://hdl.handle.net/10495/41768
dc.language.iso.spa.fl_str_mv eng
language eng
dc.relation.ispartofjournalabbrev.spa.fl_str_mv Eur. Phys. J. C.
dc.relation.citationendpage.spa.fl_str_mv 7
dc.relation.citationissue.spa.fl_str_mv 4
dc.relation.citationstartpage.spa.fl_str_mv 1
dc.relation.citationvolume.spa.fl_str_mv 76
dc.relation.ispartofjournal.spa.fl_str_mv European Physical Journal C
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dc.format.extent.spa.fl_str_mv 7 páginas
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dc.publisher.place.spa.fl_str_mv Les Ulis, Francia
institution Universidad de Antioquia
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spelling Romano, Antonio EneaVallejo Peña, Sergio AndrésCOSMOGRAVGrupo de Fenomenología de Interacciones Fundamentales2024-09-04T16:27:45Z2024-09-04T16:27:45Z2016Romano, A. E., & Vallejo, S. A. (2016). Low-redshift effects of local structure on the Hubble parameter in presence of a cosmological constant. European Physical Journal C, 76(4), 1–7. https://doi.org/10.1140/epjc/s10052-016-4033-91434-6044https://hdl.handle.net/10495/4176810.1140/epjc/s10052-016-4033-91434-6052ABSTRACT: In order to estimate the effects of a local structure on the Hubble parameter we calculate the low-redshift expansion for H(z) and δH H for an observer at the center of a spherically symmetric matter distribution in the presence of a cosmological constant. We then test the accuracy of the formulas comparing them with fully relativistic non perturbative numerical calculations for different cases for the density profile. The low-redshift expansion we obtain gives results more precise than perturbation theory since it is based on the use of an exact solution of Einstein’s field equations. For larger density contrasts the low-redshift formulas accuracy improves respect to the perturbation theory accuracy because the latter is based on the assumption of a small density contrast, while the former does not rely on such an assumption. The formulas can be used to take into account the effects on the Hubble expansion parameter due to the monopole component of the local structure. If the H(z) observations will show deviations from the CDM prediction compatible with the formulas we have derived, this could be considered an independent evidence of the existence of a local inhomogeneity, and the formulas could be used to determine the characteristics of this local structure.Universidad de Antioquia. Vicerrectoría de investigación. Comité para el Desarrollo de la Investigación - CODIUnión EuroperaCOL0147829COL00084237 páginasapplication/pdfengSpringerLes Ulis, Franciahttp://creativecommons.org/licenses/by/2.5/co/https://creativecommons.org/licenses/by/4.0/info:eu-repo/semantics/openAccesshttp://purl.org/coar/access_right/c_abf2Energía oscura (Astronomía)Dark energy (Astronomy)Constantes cosmológicasCosmological constantsCampo profundo del HubbleHubble Deep FieldDesplazamiento hacia el rojoRed shiftAstronomía geodesicaGeodetic astronomyhttp://id.loc.gov/authorities/subjects/sh2001002908http://id.loc.gov/authorities/subjects/sh2006000063http://id.loc.gov/authorities/subjects/sh98004348Low-redshift effects of local structure on the Hubble parameter in presence of a cosmological constantArtículo de investigaciónhttp://purl.org/coar/resource_type/c_2df8fbb1https://purl.org/redcol/resource_type/ARThttp://purl.org/coar/version/c_970fb48d4fbd8a85info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionEur. 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