Relativistic Modelling for Anisotropic Stellar Object

In this study, closed-form solutions for a spherically symmetric anisotropic matter distribution were obtained using the space-time geometry of Finch-Skea. We have shown that the class of solutions can be employed as strong models for 4U 1820-30, 4U 1608-52, Cen X-3 pulsars by looking at its physical admissibility. Using graphs, we have examined the many physical properties of our model, including energy density, pressures, anisotropy factor, mass, energy conditions, equilibrium, and stability analysis.