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- W2023704436 endingPage "011" @default.
- W2023704436 startingPage "011" @default.
- W2023704436 abstract "We derive the redshift and the angular diameter distance in rotationless dust universes which are statistically homogeneous and isotropic, but have otherwise arbitrary geometry. The calculation from first principles shows that the Dyer-Roeder approximation does not correctly describe the effect of clumping. Instead, the redshift and the distance are determined by the average expansion rate, the matter density today and the null geodesic shear. In particular, the position of the CMB peaks is consistent with significant spatial curvature provided the expansion history is sufficiently close to the spatially flat LambdaCDM model." @default.
- W2023704436 created "2016-06-24" @default.
- W2023704436 creator A5090219201 @default.
- W2023704436 date "2009-02-09" @default.
- W2023704436 modified "2023-10-04" @default.
- W2023704436 title "Light propagation in statistically homogeneous and isotropic dust universes" @default.
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