Study of Some Cosmological Parameters for Interacting New Holographic Dark Energy Model in f(T) Gravity

TL;DR

This study explores an interacting holographic dark energy model within f(T) gravity, analyzing cosmological parameters and stability, and finds results consistent with an accelerating universe.

Contribution

It introduces a new interacting holographic dark energy model in f(T) gravity and investigates its cosmological implications and stability.

Findings

Model aligns with an accelerating universe

Cosmological parameters are consistent with observations

Stability analysis supports the model's viability

Abstract

The present work is based on the idea of an interacting framework of new holographic dark energy with cold dark matter in the background of $f(T)$ gravity. Here, we have considered the flat modified Friedmann universe for $f(T)$ gravity which is filled with new Holographic dark energy and dark matter. We have derived some cosmological parameters like Deceleration parameter, EoS parameter, State-finder parameters, Cosmographic parameters, {\it Om} parameter and graphically investigated the nature of these parameters for the above mentioned interacting scenario. The results are found to be consistent with the accelerating universe. Also we have graphically investigated the trajectories in $\omega $--$ \omega'$ plane for different values of the interacting parameter and explored the freezing region and thawing region in $\omega $--$ \omega'$ plane. Finally, we have analyzed the stability of this model.