Bianchi type- I, III, V, VI\(_0\) and Kantowski-Sachs models in scalar-tensor theories with dynamic cosmological constant

DOI10.1007/S10509-008-9917-1zbMath1161.83474OpenAlexW2041462072MaRDI QIDQ1008430

R. Chaubey, Triloki Singh

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

zbMATH Keywords

scalar-tensor theoryBianchi type universedynamic cosmological constant

Mathematics Subject Classification ID

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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