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Open Access Article

14 pages 1892 KB

Charged Anisotropic Stellar Models with the MIT Bag Model Equation of State

Manuel Malaver

Universal Journal of Physics Research 1(1); 10.31586/ujpr.2022.338 - June 19, 2022

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Abstract

In this paper we present a new classes of solutions for the Einstein-Maxwell system of field equations in a spherically symmetric spacetime under the influence of an electric field considering the MIT... Read more

Figure 1. Energy density against radial coordinate. It has been considered that n=1(solid line) ; n=2 (long-dash line).

Figure 2. Density gradient against radial coordinate. It has been considered that n=1(solid line) ; n=2 (long-dash line).

Figure 3. Radial pressure against radial coordinate. It has been considered that n=1(solid line) ; n=2 (long-dash line).

Figure 4. Radial pressure against radial coordinate. It has been considered that n=1(solid line) ; n=2 (long-dash line).

Figure 5. Mass function against radial coordinate. It has been considered that n=1(solid line) ; n=2 (long-dash line).

Figure 6. Anisotropy against radial coordinate. It has been considered that n=1(solid line) ; n=2 (long-dash line).

Figure 7. Charge density against radial coordinate. It has been considered that n=1(solid line) ; n=2 (long-dash line).

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