REQUIRED CONDITIONS FOR LATE TIME ACCELERATION AND EARLY TIME DECELERATION IN GENERALIZED SCALAR–TENSOR THEORIES

DOI10.1142/S0217751X03012205zbMath1036.83032arXivgr-qc/0208061MaRDI QIDQ4803937

Luz M. Diaz-Rivera, Luis O. Pimentel

Publication date: 2003

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

Full work available at URL: https://arxiv.org/abs/gr-qc/0208061

zbMATH Keywords

cosmological modelscalar fieldeffective cosmological constantgeneralized scalar tensor theory

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Methods of quantum field theory in general relativity and gravitational theory (83C47) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Related Items (7)

Semi-Symmetric Curvature Properties of Robertson–Walker Spacetimes ⋮ SOME COSMOLOGICAL MODELS IN SCALAR–TENSOR THEORIES ⋮ Generalized Brans-Dicke cosmology in the presence of matter and dark energy ⋮ Living with phantoms fields in a sheet spacetime ⋮ Bianchi type- I, III, V, VI\(_0\) and Kantowski-Sachs models in scalar-tensor theories with dynamic cosmological constant ⋮ COSMIC ACCELERATION IN A MODEL OF SCALAR–TENSOR GRAVITATION ⋮ Self-similar scalar cosmologies

Cites Work

• Dynamical cosmological constant from a very recent phase transition
• COASTING COSMOLOGIES WITH TIME DEPENDENT COSMOLOGICAL CONSTANT
• The cosmological constant problem

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