Anisotropic Quintessence stars

TL;DR

This paper introduces a relativistic model for anisotropic quintessence stars combining normal matter and dark energy, demonstrating their physical viability and stability under certain conditions.

Contribution

It presents a novel relativistic model for anisotropic quintessence stars with specific dark energy parameters, ensuring regularity and stability.

Findings

Model satisfies all regularity conditions

Provides stable equilibrium configurations

Incorporates anisotropic pressure and dark energy

Abstract

We propose a relativistic model for quintessence stars with the combination of an anisotropic pressure corresponding to normal matter and a quintessence dark energy having a characteristic parameter {\omega}q such that -1 <{\omega}q < - 1/3. We discuss various physical features of the model and show that the model satisfies all the regularity conditions and can provide stable equilibrium configurations.