Interacting Holographic Viscous Dark Energy Model
arXiv:0901.3724 · doi:10.1007/s10773-009-0176-x
Abstract
In this manuscript, we present a generalization of the interacting holographic dark energy model using the viscous generalized Chaplygin gas. We also study the model by considering a dynamical Newton's constant $G$. Then we reconstruct the potential and the dynamics of the scalar field which describe the viscous Chaplygin cosmology.
11 pages, accepted for publication in Int. J. Theor. Phys