Numerical Simulations of Charged Analogues of Isentropic Superdense Star Model


Numerical simulations of charged analogues of isentropic super-dense star model by using a particular eclectic field, which involves a parameter K have been obtained and the general solution for star is derived for all negative values K. Runge-Kutta method has been used to represent superdense star models with ultrahigh surface density of the order . The physical properties have been studied and analyzed numerically subject to the energy conditions throughout the star and found to be physically acceptable.