FRW Bulk Viscous Cosmology with Modified Chaplygin Gas in Flat Space
arXiv:1612.00304 · doi:10.1007/s10509-012-1268-2
Abstract
In this paper we study FRW bulk viscous cosmology in presence of modified Chaplygin gas. We write modified Friedmann equations due to bulk viscosity and Chaplygin gas and obtain time-dependent energy density for the special case of flat space.
arXiv commentpublished by Astrophysics and Space Science see http://inspirehep.net/record/1215969
References in corpus (24)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- The Cosmological Constant and Dark Energy
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
- Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
- A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state
- Cosmological Constant - the Weight of the Vacuum
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- New Constraints on , , and w from an Independent Set of Eleven High-Redshift Supernovae Observed with HST
- Dark Energy Constraints from the Cosmic Age and Supernova
- Cosmological Evolution of a Quintom Model of Dark Energy
- CDM Models with a Smooth Component
- Role of Modified Chaplygin Gas in Accelerated Universe
- Holographic Chaplygin gas model
- Interacting holographic generalized Chaplygin gas model
- Categorizing Different Approaches to the Cosmological Constant Problem
- Interacting generalized Chaplygin gas model in non-flat universe
- Two-Fluid Scenario for Dark Energy Models in an FRW Universe-Revisited
- Holographic Chaplygin DGP cosmologies
- FRW and Bianchi type I cosmology of f-essence
- Thermodynamics of viscous dark energy in an RSII braneworld
- Bouncing Universe and Reconstructing Vector Field
- Dynamics of Modified Chaplygin Gas in Brane World Scenario: Phase Plane Analysis
- FRW Cosmological model with Modified Chaplygin Gas and Dynamical System
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- Toy models of Universe with an Effective varying -Term in Lyra Manifold
- Perturbations with bulk viscosity in modified chaplygin gas cosmology