Modelling of a Binary System with a Quadratic Equation of State

Authors

  • Manuel Malaver Department of Basic Sciences, Maritime University of the Caribbean, Catia la Mar, Venezuela Author
  • Rajan Iyer Environmental Materials Theoretical Physicist, Department of Physical Mathematics Sciences Engineering Project Technologies, Engineeringinc International Operational Teknet Earth Global, Tempe, Arizona, United States of America Author

DOI:

https://doi.org/10.47363/JPSOS/2025(7)307

Keywords:

Einstein-Maxwell Equations, Anisotropic Pressures, Quadratic Equation of State, Anisotropy, Binary System

Abstract

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.

Author Biographies

  • Manuel Malaver, Department of Basic Sciences, Maritime University of the Caribbean, Catia la Mar, Venezuela

    Manuel Malaver de la Fuente, Department of Basic Sciences, Maritime University of the Caribbean, Catia la Mar, Venezuela.

  • Rajan Iyer, Environmental Materials Theoretical Physicist, Department of Physical Mathematics Sciences Engineering Project Technologies, Engineeringinc International Operational Teknet Earth Global, Tempe, Arizona, United States of America

    Environmental Materials Theoretical Physicist, Department of Physical Mathematics Sciences Engineering Project Technologies, Engineeringinc International Operational Teknet Earth Global, Tempe, Arizona, United States of America

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Published

2025-11-26