Reconstructing interacting entropy-corrected holographic scalar field models of dark energy in non-flat universe

TL;DR

This paper reconstructs various scalar field models of dark energy based on an entropy-corrected holographic dark energy framework in a non-flat universe, analyzing their dynamics and interactions.

Contribution

It introduces a reconstruction of scalar field models from an entropy-corrected holographic dark energy model considering non-flat geometry and interaction effects.

Findings

Derived the equation of state parameter with dark energy-dark matter interaction.

Reconstructed potentials and dynamics for quintessence, tachyon, K-essence, and dilaton fields.

Analyzed the evolutionary behavior of these scalar field models.

Abstract

Here we consider the entropy-corrected version of the holographic dark energy model in the non-flat universe. We obtain the equation of state parameter in the presence of interaction between dark energy and dark matter. Moreover, we reconstruct the potential and the dynamics of the quintessence, tachyon, K-essence and dilaton scalar field models according to the evolutionary behavior of the interacting entropy-corrected holographic dark energy model.