Geometric and thermodynamic properties in Gauss-Bonnet gravity
arXiv:1111.0232 · doi:10.1007/s10509-011-0911-7
Abstract
In this paper, the generalized second law (GSL) of thermodynamics and entropy is revisited in the context of cosmological models in Gauss-Bonnet gravity with the boundary of the universe is assumed to be enclosed by the dynamical apparent horizon. The model is best fitted with the observational data for distance modulus. The best fitted geometric and thermodynamic parameters such as equation of state parameter, deceleration parameter and entropy are derived. To link between thermodynamic and geometric parameters, the "entropy rate of change multiplied by the temperature" as a model independent thermodynamic state parameter is also derived. The results show that the model is in good agreement with the observational analysis.
13 pages, 13 figures, to be published in Astrophysics and Space Sci
References in corpus (26)
- Dark energy in modified Gauss-Bonnet gravity: late-time acceleration and the hierarchy problem
- Thermodynamic Behavior of Friedmann Equation at Apparent Horizon of FRW Universe
- Friedmann Equations of FRW Universe in Scalar-tensor Gravity, f(R) Gravity and First Law of Thermodynamics
- The holographic dark energy in non-flat Brans-Dicke cosmology
- Deep Connection Between Thermodynamics and Gravity in Gauss-Bonnet Braneworld
- Generalized Second Law of Thermodynamics in Quintom Dominated Universe
- Dark energy from modified F(R)-scalar-Gauss-Bonnet gravity
- Accelerating cosmologies from non-local higher-derivative gravity
- The generalized second law of thermodynamics in the accelerating universe
- Holographic dark energy in Brans-Dicke cosmology with chameleon scalar field
- Thermodynamical Interpretation of the Interacting Holographic Dark Energy Model in a non-flat Universe
- The Holographic Model of Dark Energy and Thermodynamics of Non-Flat Accelerated Expanding Universe
- The Effect of a Chameleon Scalar Field on the Cosmic Microwave Background
- Schwarzschild black hole and the generalized second law in phantom-dominated universe
- Stellar configurations in f(R) theories of gravity
- Modified gravity with
- Thermodynamical properties of dark energy
- Revisiting chameleon gravity - thin-shells and no-shells with appropriate boundary conditions
- Attractors, Statefinders and Observational Measurement for Chameleonic Brans--Dicke Cosmology
- Non-minimal Maxwell-Modified Gauss-Bonnet Cosmologies: Inflation and Dark Energy
- Cosmic acceleration and crossing of in non-minimal modified Gauss-Bonnet gravity
- Gauss-Bonnet Chameleon Mechanism of Dark Energy
- Bouncing Universe and phantom crossing in Modified Gravity and its reconstruction
- Interacting Holographic dark energy in chameleon tachyon cosmology
- Renormalization-group running cosmologies and the generalized second law
- Entropy and statefinder diagnosis in chameleon cosmology