Charged Stellar Model with Quadratic Equation of State in Tolman VII Spacetime
In this paper, we studied the behavior of relativistic objects considering Tolman VII form for the gravitational potential Z and a quadratic equation of state for the charged anisotropic matter distribution. A physical analysis of electromagnetic field indicates that is regular in the origin and well behaved. The new obtained solution not admits singularities in the matter, charge density and metric functions. A graphical analysis indicates that the new stellar model satisfy all physical properties expected in a realistic star.
Relativistic Objects, Anisotropic Matter, Tolman VII Potential, Quadratic Equation of State, Gravitational Potential
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