Abstract
We generate a three-layered super dense charged star with Van der Waals equation of state at the intermediate layer of stellar spheres. Our model comprises of three interior layers: the core, the intermediate, and the envelope described by linear, Van der Waals, and Chaplygin equations of state, respectively. The plots for the physical variables such as energy density, radial and tangential pressures, mass, anisotropy, and metric potentials are well behaved and agree with the astrophysical results. The stability and equilibrium factors are continuous and defined at some values of the parameters. We have also generated new stellar masses and radii which are in acceptable ranges. We have also regained previous masses and radii for the stars like PSRJ1903+0327, PSRJ1614-2230, SAXJ1808.4-3658, EXO1745-248, and EXO1785-248.
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