Abstract
In this paper, we present an anisotropic analogue of charged Tolman’s solution of the general relativistic field equations in curvature coordinates compatible with a super dense star model. These exact solutions are well behaved in all respect for a wide range of anisotropy parameter and charged parameter. We found that new solutions have advantages for modeling super-dense stars as neutron stars and quark stars because they have wide range of masses and radii with a simple mathematical expression.
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