Interaction between modified Chaplygin gas and ghost dark energy in presence of extra dimensions
arXiv:1402.3256 · doi:10.1140/epjp/i2014-14119-x
Abstract
In this paper, we consider three different models of dark energy in higher dimensional space-time and discuss about some cosmological parameters numerically. The first model is a single component universe including viscous varying modified Chaplygin gas. In the second model, we consider two-component universe including viscous varying modified Chaplygin gas and ghost dark energy. In the third model, we consider another two-component universe including viscous modified cosmic Chaplygin gas and ghost dark energy. In the cases of two-component fluids we also consider possibility of interaction between components.
References in corpus (18)
- Bouncing Universe with Quintom Matter
- Interacting holographic generalized Chaplygin gas model
- Quintessence and phantom cosmology with non-minimal derivative coupling
- Interacting Agegraphic Dark Energy
- The cosmological constant from the ghost. A toy model
- Parametrizations of the Dark Energy Density and Scalar Potentials
- A Tracker Solution for a Holographic Dark Energy Model
- FRW Bulk Viscous Cosmology with Modified Chaplygin Gas in Flat Space
- Braneworld models with a non-minimally coupled phantom bulk field: a simple way to obtain the -1-crossing at late times
- Holographic Dark Energy in Braneworld Models with Moving Branes and the w=-1 Crossing
- Interacting Quintessence Models of Dark Energy
- Cosmic coincidence problem and variable constants of physics
- Higher derivative corrections of gravity with varying equation of state in the case of variable and
- Latest Observational Constraints to the Ghost Dark Energy Model by Using Markov Chain Monte Carlo Approach
- Interacting two-component fluid models with varying EoS parameter
- Theoretical Aspects of Quintom Models
- Variable Correction for Dark Energy Model in Higher Dimensional Cosmology
- Phenomenological models of Universe with varying and
Cited by in corpus (9)
- Interacting quintessence dark energy models in Lyra manifold
- Thermodynamics of the viscous gravity in the new agegraphic dark energy model
- Thermodynamics and stability of gravity with viscous fluid by observational constraints
- Stability and interacting gravity with modified Chaplygin gas
- Cosmological Tests of Dark Energy Model in FRW Universe
- Observational constraints and stability in viscous gravity
- Non-linear logarithmic interactions and a varying polytropic gas
- Viscous interacting and stability on dark matter Bose-Einstein condensation with modified Chaplygin gas
- Toy models of Universe with an Effective varying -Term in Lyra Manifold