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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Authors are grateful to the anonymous referees and editors for their rigorous review, constructive comments and useful suggestions.
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Singh, K.N., Pradhan, N. & Pant, N. Charge Analogue of Tolman IV Solution for Anisotropic Fluid. Int J Theor Phys 54, 3408–3423 (2015). https://doi.org/10.1007/s10773-015-2581-7
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DOI: https://doi.org/10.1007/s10773-015-2581-7