Interacting Holographic Viscous Dark Energy Model
Mubasher Jamil, M. Umar Farooq
TL;DR
This paper introduces a generalized interacting holographic dark energy model incorporating viscous generalized Chaplygin gas and a dynamical Newton's constant, analyzing scalar field dynamics and potential reconstruction.
Contribution
It presents a novel extension of holographic dark energy models with viscosity and variable G, including scalar field reconstruction and potential analysis.
Findings
Reconstructed scalar field potential for viscous Chaplygin cosmology.
Analyzed effects of a dynamical Newton's constant G.
Extended holographic dark energy models with viscosity and variable G.
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 . Then we reconstruct the potential and the dynamics of the scalar field which describe the viscous Chaplygin cosmology.
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