Reconstructing interacting new agegraphic polytropic gas model in non-flat FRW universe

TL;DR

This paper establishes a connection between the interacting new agegraphic dark energy and the polytropic gas model in a non-flat FRW universe, enabling the reconstruction of scalar field dynamics for cosmic acceleration.

Contribution

It introduces a novel correspondence that reconstructs scalar field potential and dynamics for dark energy models in a non-flat universe setting.

Findings

Reconstructed scalar field potential for dark energy.

Derived dynamics of the scalar field in the polytropic model.

Showed compatibility with accelerated cosmic expansion.

Abstract

We study the correspondence between the interacting new agegraphic dark energy and the polytropic gas model of dark energy in the non-flat FRW universe. This correspondence allows to reconstruct the potential and the dynamics for the scalar field of the polytropic model, which describe accelerated expansion of the universe.