Anisotropic Compact Star Model on Finch-Skea Spacetime

In this study, we demonstrate a new anisotropic solution to the Einstein field equations in Finch-Skea spacetime. The physical features of stellar configuration are studied in previous investigations. We create a model that meets all physical plausibility conditions for a variety of stars and plot graphs for $\mathbf{\text{4U}}\mathbf{\text{1820-30}}$.