# Anisotropic stars for spherically symmetric spacetimes satisfying the Karmarkar condition

## TL;DR

This paper introduces a new class of anisotropic stellar models satisfying the Karmarkar condition, demonstrating their physical viability and applicability to real compact stars like Vela X-1 and 4U1608-52.

## Contribution

It presents a novel solution for anisotropic stars satisfying the Karmarkar condition, ensuring physical stability and realistic modeling of compact stars.

## Key findings

- Model satisfies all physical stability criteria
- Accurately describes observed compact stars
- Ensures hydrostatic equilibrium

## Abstract

A new class of solution describing an anisotropic stellar configuration satisfying Karmarkar's condition i.e. spherically symmetric metric of embedding class 1, is reported. It has been shown that the compact star model is physically well-behaved and meet all the physical requirements for a stable configuration in hydrostatic equilibrium. Our model describes compact stars like Vela X-1 and 4U1608-52 to a very good approximation.