Late time acceleration in scalar-tensor theory with GB interaction

DOI10.1007/S10773-011-0912-XzbMath1242.83086OpenAlexW2092918217MaRDI QIDQ432115

B. Modak, R. N. Bose

Publication date: 3 July 2012

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

Full work available at URL: https://doi.org/10.1007/s10773-011-0912-x

zbMATH Keywords

cosmologychameleon mechanism and late time accelerationGauss-Bonnet interaction

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Cites Work

• Modified Gauss-Bonnet theory as gravitational alternative for dark energy
• Dynamical relaxation of dark energy: a solution to early inflation, late-time acceleration and the cosmological constant problem
• A new type of isotropic cosmological models without singularity
• Acceleration of the universe with a simple trigonometric potential
• On compatibility of string effective action with an accelerating universe
• Cosmological Imprint of an Energy Component with General Equation of State
• Dark energy and cosmological solutions in second-order string gravity
• Mach's Principle and Invariance under Transformation of Units
• Evolution of dynamical coupling in scalar tensor theory from Noether symmetry
• \(k\)-inflation

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