Statefinder Description in Generalized Holographic and Ricci Dark Energy Models
arXiv:1106.5689 · doi:10.1007/s10773-011-0992-7
Abstract
We have considered the generalized holographic and generalized Ricci dark energy models for acceleration of the universe. If the universe filled with only GHDE/GRDE the corresponding decel- eration parameter, EOS parameter and statefinder parameters have been calculated. Next we have considered that the mixture of GHDE/GRDE and dark matter in interacting and non-interacting situations. Also the mixture of GHDE/GRDE and generalized Chaplygin gas have been analyzed during evolution of the universe. The natures of above mentioned parameters have been investigated for interacting and non-interacting situations. Finally, it follows that the prescribed models derive the acceleration of the universe.
18 pages and 19 figures
References in corpus (12)
- A Holographic Dark Energy Model from Ricci Scalar Curvature
- Statefinder Diagnosis for Ricci Dark Energy
- Viscous Ricci Dark Energy
- Interacting HDE and NADE in Brans-Dicke Chameleon Cosmology
- Statefinder diagnostic and stability of modified gravity consistent with holographic and new agegraphic dark energy
- Reconstructing Quintom from Ricci Dark Energy
- Correspondence between entropy-corrected holographic and Gauss-Bonnet dark energy models
- Generalized Holographic and Ricci Dark Energy Models
- Cosmic accelerated expansion and the entropy corrected holographic dark energy
- Reconstructing interacting entropy-corrected holographic scalar field models of dark energy in non-flat universe
- Interacting modified Chaplygin gas in loop quantum cosmology
- Variable G correction to statefinder parameters of dark energy