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We present a spherically symmetric solution of the general relativistic fieldequations in isotropic coordinates for charged fluid with pressure anisotropy,compatible with a super dense star modeling. Further, we have constructed ananisotropic model of super dense star with all degree of suitability. We alsoobserved that by increasing anisotropy, the maximum mass of super dense starsalso decreases.

Modeling anisotropic charged neutron star in isotropic coordinates