We find two new classes of exact solutions to the Einstein-Maxwell system of equations. The matter distribution satisfies a linear equation of state consistent with quark matter. The field equations are integrated by specifying forms for the measure of anisotropy and a gravitational potential which are physically reasonable. The first class has a constant potential and is regular in the stellar interior. It contains the familiar Einstein model as a limiting case and we can generate finite masses for the star. The second class has a variable potential and singularity at the centre. A graphical analysis indicates that the matter variables are well behaved.
Sunzu, J , Maharaj, S & Ray, S (2021). Quark Star Model With Charged Anisotropic Matter. Afribary. Retrieved from https://afribary.com/works/quark-star-model-with-charged-anisotropic-matter
Sunzu, Jefta et. al. "Quark Star Model With Charged Anisotropic Matter" Afribary. Afribary, 20 May. 2021, https://afribary.com/works/quark-star-model-with-charged-anisotropic-matter. Accessed 08 Jun. 2023.
Sunzu, Jefta, Sunil Maharaj and Subharthi Ray . "Quark Star Model With Charged Anisotropic Matter". Afribary, Afribary, 20 May. 2021. Web. 08 Jun. 2023. < https://afribary.com/works/quark-star-model-with-charged-anisotropic-matter >.
Sunzu, Jefta , Maharaj, Sunil and Ray, Subharthi . "Quark Star Model With Charged Anisotropic Matter" Afribary (2021). Accessed June 08, 2023. https://afribary.com/works/quark-star-model-with-charged-anisotropic-matter