Interacting entropy-corrected new agegraphic dark energy in non-flat universe

TL;DR

This paper explores an entropy-corrected new agegraphic dark energy model in a non-flat universe, deriving its evolution equations, analyzing its behavior, and reconstructing the associated scalar field dynamics.

Contribution

It introduces an entropy-corrected version of the new agegraphic dark energy model, including interaction effects and scalar field reconstruction, which are novel extensions.

Findings

Derived the evolution equation for the energy density parameter.

Identified conditions for crossing the phantom divide.

Reconstructed the scalar field potential and dynamics.

Abstract

Here we consider the entropy-corrected version of the new agegraphic dark energy model in the non-flat FRW universe. We derive the exact differential equation that determines the evolution of the entropy-corrected new agegraphic dark energy density parameter in the presence of interaction with dark matter. We also obtain the equation of state and deceleration parameters and present a necessary condition for the selected model to cross the phantom divide. Moreover, we reconstruct the potential and the dynamics of the phantom scalar field according to the evolutionary behavior of the interacting entropy-corrected new agegraphic model.