# Anisotropic strange quark stars with a non-linear equation-of-state

## TL;DR

This paper presents an exact analytical model of anisotropic strange quark stars using a non-linear equation-of-state, satisfying all energy conditions and providing insights into their mass-radius relationship within General Relativity.

## Contribution

It introduces a new exact solution for anisotropic strange quark stars with a non-linear equation-of-state, expanding the understanding of their internal structure.

## Key findings

- Energy conditions are fully satisfied.
- Mass-to-radius profile is derived.
- Star compactness is computed.

## Abstract

We obtain an exact analytical solution to Einstein's field equations assuming a non-linear equation-of-state and a particular mass function. Our solution describes the interior of anisotropic color flavor locked strange quark stars. All energy conditions are fulfilled, and therefore the solution obtained here is a realistic solution within General Relativity. The mass-to-radius profile is obtained, and the compactness of the star is computed.