Holographic Dark Energy Model with Modified Variable Chaplygin Gas

TL;DR

This paper develops a holographic dark energy model linked with a modified variable Chaplygin gas, reconstructs the scalar field potential, and analyzes the model's stability, offering a new approach to understanding cosmic acceleration.

Contribution

It introduces a novel correspondence between holographic dark energy and modified variable Chaplygin gas, including potential reconstruction and stability analysis.

Findings

Successful reconstruction of scalar field potential.

Demonstration of model stability under certain conditions.

Provides a new framework for dark energy modeling.

Abstract

In this letter we consider a correspondence between holographic dark energy and variable modified Chaplygin gas to obtain a holographic dark energy model of the universe. The corresponding potential of the scalar field has been reconstructed which describes the modified variable Chaplygin gas. The stability of the holographic dark energy in this case is also discussed.