SOME COSMOLOGICAL MODELS IN SCALAR–TENSOR THEORIES

DOI10.1142/S0217732310033177zbMath1194.83025MaRDI QIDQ3590684

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Publication date: 13 September 2010

Published in: Modern Physics Letters A (Search for Journal in Brave)

zbMATH Keywords

magnetic fieldcosmologyscalar-tensor theoryBianchi type-V model

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Electromagnetic fields in general relativity and gravitational theory (83C50) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Exact solutions to problems in general relativity and gravitational theory (83C15)

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Some exact solutions of Bianchi type-II string cosmological models with magnetic field in Brans-Dicke theory of gravitation ⋮ A Bianchi type-II dark-energy cosmology with a decaying \(\Lambda\)-term in the Brans-Dicke theory of gravity ⋮ Modified Chaplygin gas cosmology with observational constraints ⋮ Unnamed Item ⋮ Bianchi type-I cosmological model with null radiation flow ⋮ Bianchi type-II string cosmological model with magnetic field in scalar-tensor theory of gravitation

Cites Work

• Bianchi type- I, III, V, VI\(_0\) and Kantowski-Sachs models in scalar-tensor theories with dynamic cosmological constant
• 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
• The cosmological constant problem
• Cosmological models in generalized scalar-tensor theory with cosmological term and bulk viscosity

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