Interacting Holographic Viscous Dark Energy Model
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.
0
Turn this paper into a lesson
ArcXiv compiles a structured reading guide from this paper's metadata: plain-English importance, contributions, prerequisite concepts, which sections to read first, flashcards, and a quiz. Grounded in the abstract, never invented.