A class of solutions for anisotropic stars admitting conformal motion

TL;DR

This paper introduces a new class of interior solutions for anisotropic stars that admit conformal motion, solving Einstein's equations for specific density/mass functions and analyzing key physical parameters.

Contribution

It presents a novel class of solutions for anisotropic stars with conformal symmetry, expanding the theoretical models available for such stellar objects.

Findings

Model parameters like pressures and density are explicitly characterized.

The solutions demonstrate physically plausible behavior for anisotropic stellar models.

Surface tension and other parameters are analyzed for stability and realism.

Abstract

We provide a new class of interior solutions for anisotropic stars admitting conformal motion. The Einstein's field equations in this construction are solved for specific choices of the density/mass functions. We analyze the behavior of the model parameters like radial and transverse pressures, density and surface tension.