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...
- 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
- Rights
- openAccess
- License
- http://creativecommons.org/licenses/by/2.5/co/
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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 |
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2024-09-04T16:27:45Z |
| dc.type.spa.fl_str_mv |
Artículo de investigación |
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http://purl.org/coar/resource_type/c_2df8fbb1 |
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https://purl.org/redcol/resource_type/ART |
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http://purl.org/coar/version/c_970fb48d4fbd8a85 |
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info:eu-repo/semantics/article |
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http://purl.org/coar/resource_type/c_2df8fbb1 |
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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. |
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7 |
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4 |
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1 |
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76 |
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European Physical Journal C |
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http://creativecommons.org/licenses/by/2.5/co/ |
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https://creativecommons.org/licenses/by/4.0/ |
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info:eu-repo/semantics/openAccess |
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openAccess |
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7 páginas |
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application/pdf |
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Springer |
| dc.publisher.place.spa.fl_str_mv |
Les Ulis, Francia |
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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. Phys. J. 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