Power Law Entropy Corrected New-Agegraphic Dark Energy in Ho\v{r}ava-Lifshitz Cosmology

TL;DR

This paper explores a modified dark energy model within Hořava-Lifshitz cosmology, revealing phantom crossing behavior influenced by interaction parameters, and providing insights into the universe's accelerated expansion.

Contribution

It introduces a power-law entropy corrected new agegraphic dark energy model in Hořava-Lifshitz cosmology and analyzes its evolution and interaction effects.

Findings

Phantom crossing occurs for non-zero coupling parameter.

The model's evolution depends on the form of the state parameter.

Interaction influences the dark energy dynamics.

Abstract

We investigate the new agegraphic dark energy (NADE) model with power-law corrected entropy in the framework of Ho\v{r}ava-Lifshitz cosmology. For a non-flat universe containing the interacting power-law entropy-corrected NADE (PLECNADE) with dark matter, we obtain the differential equation of the evolution of density parameter as well as the deceleration parameter. To study parametric behavior, we used an interesting form of state parameter as function of redshift $\omega_{\Lambda}(z)=\omega_0+\omega_1 z$. We found that phantom crossing occurs for the state parameter for a non-zero coupling parameter, thus supporting interacting dark energy model.