Modelling of a Binary System with a Quadratic Equation of State
DOI:
https://doi.org/10.47363/JPSOS/2025(7)307Keywords:
Einstein-Maxwell Equations, Anisotropic Pressures, Quadratic Equation of State, Anisotropy, Binary SystemAbstract
This study investigates Einstein-Maxwell field equations with anisotropic pressure by means of a quadratic equation of state (Bose-Einstein equation of state) in the presence of an electric field and a modified version of the metric potential proposed for Korkina and Orlyanskii (1991). We obtain new classes of models that satisfy all the physical conditions for a realistic star. According to visual analysis, physical properties including energy density, radial pressure, charge density, and anisotropy are consistent with the stellar binary system GW191219, which is composed of a neutron star and a black hole.
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Published
2025-11-26
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