f(T) modified teleparallel gravity models as an alternative for holographic and new agegraphic dark energy models

TL;DR

This paper reconstructs f(T)-gravity models to emulate holographic and new agegraphic dark energy behaviors, showing they can mimic phantom or quintessence states and explain transitions consistent with observations.

Contribution

It introduces specific f(T)-gravity models aligned with holographic and agegraphic dark energy, including entropy corrections, and analyzes their equation of state parameters.

Findings

Models behave like phantom or quintessence.

Entropy-corrected models show transition from quintessence to phantom.

Results align with recent cosmological observations.

Abstract

In the present work, we reconstruct different f(T)-gravity models corresponding to the original and entropy-corrected version of the holographic and new agegraphic dark energy models. We also obtain the equation of state parameters of the corresponding f(T)-gravity models. We conclude that the holographic and new agegraphic f(T)-gravity models behave like phantom or quintessence model. Whereas in the entropy-corrected models, the equation of state parameter can justify the transition from the quintessence state to the phantom regime as indicated by the recent observations.