Correspondence between entropy-corrected holographic and Gauss-Bonnet dark energy models

TL;DR

This paper explores the relationship between entropy-corrected holographic dark energy and Gauss-Bonnet dark energy models, showing their correspondence leads to an accelerating universe within a loop quantum gravity context.

Contribution

It establishes a novel correspondence between entropy-corrected holographic dark energy and Gauss-Bonnet dark energy models in flat universes.

Findings

The models are compatible with an accelerating universe.

A correspondence between ECHDE and Gauss-Bonnet phantom models is demonstrated.

Loop quantum gravity corrections influence dark energy modeling.

Abstract

In the present work we investigate the cosmological implications of the entropy-corrected holographic dark energy (ECHDE) density in the Gauss-Bonnet framework. This is motivated from the loop quantum gravity corrections to the entropy-area law. Assuming the two cosmological scenarios are valid simultaneously, we show that there is a correspondence between the ECHDE scenario in flat universe and the phantom dark energy model in the framework of Gauss-Bonnet theory with a potential. This correspondence leads consistently to an accelerating universe.