Viscous Ricci Dark Energy
arXiv:0905.0527 · doi:10.1016/j.physletb.2009.09.013
Abstract
We investigate the viscous Ricci dark energy (RDE) model by assuming that there is bulk viscosity in the linear barotropic fluid and the RDE. In the RDE model without bulk viscosity, the universe is younger than some old objects at some redshifts. Since the age of the universe should be longer than any objects in the universe, the RDE model suffers the age problem, especially when we consider the object APM 08279+5255 at , whose age is Gyr. In this letter, we find that once the viscosity is taken into account, this age problem is alleviated.
4 pages, 3 figures
References in corpus (10)
- A Holographic Dark Energy Model from Ricci Scalar Curvature
- Infrared cut-off proposal for the Holographic density
- New infrared cut-off for the holographic scalar fields models of dark energy
- Statefinder Diagnosis for Ricci Dark Energy
- Restoring Holographic Dark Energy in Brane Cosmology
- Holographic Dark Energy in Braneworld Models with a Gauss-Bonnet Term in the Bulk. Interacting Behavior and the w =-1 Crossing
- Some Issues Concerning Holographic Dark Energy
- Can a matter-dominated model with constant bulk viscosity drive the accelerated expansion of the universe?
- Reconstructing Quintom from Ricci Dark Energy
- Holographic Gas as Dark Energy