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Light propagation in statistically homogeneous and isotropic universes with general matter content
We derive the relationship of the redshift and the angular diameter distance to the average expansion rate for universes which are statistically homogeneous and isotropic and where the distribution evolves slowly, but which have otherwise arbitrary geometry and matter content. The relevant average e...
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| Lenguaje: | eng |
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2009
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| Acceso en línea: | https://dx.doi.org/10.1088/1475-7516/2010/03/018 http://cds.cern.ch/record/1229532 |