Abstract:
This thesis investigates a charged anisotropic stellar model in paraboloidal geometry, using
the Chaplygin equation of state. We develop a new solution to Einstein’s field equations
that investigates the interaction of electromagnetic fields and, anisotropic pressures. This
solution satisfies all physically admissible conditions. This model also fulfills all stability
conditions, including hydrostatic equilibrium, the adiabatic index and, Abreu’s criterion.
By assuming the values of parameters, we can develop detailed profiles of the compact
stars in our model. These profiles show how density, pressure, and electric field vary
throughout the star.
