QUANTUM EFFECTS AND STABILITY OF CHAMELEON COSMOLOGY

DOI10.1142/S0217732304013933zbMath1076.83538arXivhep-th/0310296MaRDI QIDQ5708227

Sergei D. Odintsov, Shin'ichi Nojiri

Publication date: 28 November 2005

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

Full work available at URL: https://arxiv.org/abs/hep-th/0310296

zbMATH Keywords

conformal anomalycosmic accelerationDark energy

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Anomalies in quantum field theory (81T50) Methods of quantum field theory in general relativity and gravitational theory (83C47)

Related Items (13)

Phase space correspondence between Jordan and Einstein frames ⋮ Observational constraints on FRW cosmologies with dark energy-dark matter interaction ⋮ Cosmographic test of chameleon gravity ⋮ Chameleonic generalized Brans-Dicke model and late-time acceleration ⋮ Dynamics of the self-interacting chameleon cosmology ⋮ A reconstruction scheme for f(T) gravity and its consequences in the perturbation level ⋮ Knot universes in Bianchi type I cosmology ⋮ An exponential \(F(R)\) dark energy model ⋮ \(k\)-essential phantom energy: revisited ⋮ COSMIC DYNAMICS IN CHAMELEON COSMOLOGY ⋮ Future singularity avoidance in semiclassical cosmology ⋮ THE UNIVERSE DYNAMICS IN THE TACHYON COSMOLOGY WITH NON-MINIMAL COUPLING TO MATTER ⋮ Symmetron and de Sitter attractor in a teleparallel model of cosmology

Cites Work

• A new type of isotropic cosmological models without singularity
• QUANTUM DILATONIC GRAVITY IN d=2,4 AND 5 DIMENSIONS
• Inflationary Brans-Dicke quantum universe

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