Dark Viscous Fluid coupled with Dark Matter and future singularity
arXiv:1006.1610 · doi:10.1140/epjc/s10052-010-1398-z
Abstract
We study effects of viscous fluid coupled with dark matter in our universe. We consider bulk viscosity in the cosmic fluid and we suppose the existence of a coupling between fluid and dark matter, in order to reproduce a stable de Sitter universe protected against future-time singularities. More general inhomogeneous fluids are studied related to future singularities.
11 pages
References in corpus (10)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- New Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy
- Finite-time future singularities in modified Gauss-Bonnet and gravity and singularity avoidance
- Future of the universe in modified gravitational theories: Approaching to the finite-time future singularity
- The future evolution and finite-time singularities in -gravity unifying the inflation and cosmic acceleration
- Relativistic stars in f(R) gravity, and absence thereof
- Classifying and avoiding singularities in the alternative gravity dark energy models
- Viscous Dark Cosmology with Account of Quantum Effects
- Is the future universe singular: Dark Matter versus modified gravity?
Cited by in corpus (11)
- Viscous Little Rip Cosmology
- Inflationary universe in terms of a van der Waals viscous fluid
- Non-local -mimetic gravity
- Inhomogeneous viscous dark fluid coupled with dark matter in the FRW universe
- Viscous Coupled Fluids in Inflationary Cosmology
- Inhomogeneous viscous fluids for inflation
- The unified history of the viscous accelerating universe and phase transitions
- Inhomogeneous viscous fluids in FRW universe
- Viscous Accelerating Universe with Non-linear and Logarithmic Equation of State Fluid
- Holographic representation of the unified early and late universe via a viscous dark fluid
- Coupled fluids model in FRW space-time