INHOMOGENEOUS COSMOLOGICAL MODELS AND H0 OBSERVATIONS
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Publication:4921241
DOI10.1142/S021827181250085XzbMath1263.83194arXiv1112.1777OpenAlexW2963613779MaRDI QIDQ4921241
Publication date: 23 May 2013
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1112.1777
Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Exact solutions to problems in general relativity and gravitational theory (83C15) General questions in astronomy and astrophysics (85A04) Astrophysical cosmology (85A40)
Related Items (2)
Coordinate independent approach to the calculation of the effects of local structure on the luminosity distance ⋮ Reconstructing the metric of the local Universe from number counts observations
Cites Work
- Complete solutions to the metric of spherically collapsing dust in an expanding spacetime with a cosmological constant
- Oscillating Friedman cosmology
- Phantom Friedmann cosmologies and higher-order characteristics of expansion
- Can the acceleration of our universe be explained by the effects of inhomogeneities?
- Effect of Inhomogeneity on Cosmological Models
- A (giant) void is not mandatory to explain away dark energy with a Lemaître-Tolman model
- Solving the Inverse Problem with Inhomogeneous Universes
- Spherically Symmetrical Models in General Relativity
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