Panorama behaviors of Holographic Dark Energy models in f(R,T) gravity

TL;DR

This paper explores solutions of holographic dark energy models within f(R,T) gravity for Bianchi type I spacetime, analyzing cosmic phases using statefinder diagnostics and jerk parameters.

Contribution

It provides exact solutions for holographic dark energy in f(R,T) gravity with specific expansion laws and analyzes their cosmological implications.

Findings

Solutions for volumetrical power and exponential expansion laws.

Analysis of statefinder parameters and jerk to characterize universe phases.

Detailed physical and geometrical parameter descriptions.

Abstract

Classes of solutions of field equations in gravity for a Bianchi sort I (Kasner form) space-time with matter and Holographic Dark Energy (HDE) is mentioned. Precise solutions of field equations are obtained with volumetrical power and exponential expansion laws .The physical and geometrical parameters of the models are mentioned well. The statefinder diagnostic pair and jerk parameter are analyzed to characterize utterly totally different phases of the universe.