Bianchi type- I, III, V, VI\(_0\) and Kantowski-Sachs models in scalar-tensor theories with dynamic cosmological constant
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Publication:1008430
DOI10.1007/S10509-008-9917-1zbMath1161.83474OpenAlexW2041462072MaRDI QIDQ1008430
Publication date: 27 March 2009
Published in: Astrophysics and Space Science (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10509-008-9917-1
Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15)
Related Items (2)
Bianchi type-V bulk viscous cosmological models with particle creation in Brans-Dicke theory ⋮ SOME COSMOLOGICAL MODELS IN SCALAR–TENSOR THEORIES
Cites Work
- Bianchi type I cosmological models with variable \(G\) and \(\Lambda\)
- Bianchi type I cosmological models with variable \(G\) and \(\Lambda\): A comment
- COASTING COSMOLOGIES WITH TIME DEPENDENT COSMOLOGICAL CONSTANT
- REQUIRED CONDITIONS FOR LATE TIME ACCELERATION AND EARLY TIME DECELERATION IN GENERALIZED SCALAR–TENSOR THEORIES
- The cosmological constant problem
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