Relativistic Stellar Modeling with generalized Chapligyn Equation of State

Abstract

In this study, we obtained a new model for a charged anisotropic matter distribution by using the generalized Chaplygin equation of state. The Einstein-Maxwell field equations have been solved with a specific form of metric potential and electric field intensity. The graphical plots describe that physical features such as radial pressure, charge density, energy density, anisotropy, radial speed sound, and the mass are fully well explained and remain regular in the interior of the star. We have found models consistent with stellar objects.