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/
