Charged perfect fluid stellar structures with Bardeen model

This paper is devoted to study static spherically symmetric model in the presence of charged perfect fluid. This is the generalization of neutral perfect fluid (when there is no charge) through the solution of Einstein Maxwell equations. For this purpose, we consider a suitable form of gravitational potential g(tt) and the electric field E(r), already used in the literature. The value of mass-radius ratio or compactness u = M/R, which depends upon the chosen model exceeds the value 4/9 corresponding to neutral stars. The most important feature of the current study is to use the Bardeen model geometry instead of usual Reissner-Nordstrom model for the matching conditions. In this case the energy density and pressure remain positive, bounded and monotonically decreasing whereas electric field is monotonically increasing. Also the causality condition, i.e. the magnitude of speed of sound must be less than the speed of light, is satisfied. Moreover, the behavior of all the physical parameters at the center and on surface of star of mass M similar to M-circle dot and for Her X-1 are tabulated. All the results by graphical analysis and tabular information suggest that Bardeen model provides physically realistic stellar structures.