Modified Chaplygin Gas Cosmology with Bulk Viscosity
arXiv:1401.8002 · doi:10.1142/S0218271814500825
Abstract
In this paper, we investigate the viscous modified Chaplygin gas cosmological model. Solutions for different values of the viscosity parameter are obtained using both analytical and numerical methods. We have calculated the deceleration and defined {\em newly} statefinder pair in D dimensions. It is shown that when , the usual statefinder parameters are recovered. Furthermore, we apply the statefinder diagnostic to the MCG model with and without viscosity in dimensions and explore these parameters graphically.
11 pages, 4 figures
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- Holographic Dark Energy from Fluid/Gravity Duality Constraint by Cosmological Observations
- Dynamics of Modified Chaplygin Gas Inflation on the Brane with Bulk Viscous Pressure
- Modified Cosmic Chaplygin AdS Black Hole
- Israel-Stewart approach to viscous dissipative extended holographic Ricci dark energy dominated universe
- Constraining Cosmological Parameters with Viscous Modified Chaplygin Gas and Generalized Cosmic Chaplygin Gas Models in Horava-Lifshitz Gravity: Utilizing Late-time Datasets
- Perturbations with bulk viscosity in modified chaplygin gas cosmology