Treatment of a static spherically symmetric matter distribution on the basis of the projective unified field theory

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Gravitational Fields, Stellar Models, Unified Field Theory, Einstein Equations, Equations Of State, Isotropism, Mass Distribution, Neutron Stars, Numerical Integration

Scientific paper

The projective unified field theory developed by Schmutzer (1990) is applied to the astrophysically interesting case of a static spherically symmetric matter distribution (e.g., a star, neutron star, or other starlike object). The basic four-dimensional equations for an electrically neutral object are derived; their specialization to the case in question is outlined; and particular attention is given to the exterior solution in isotropic coordinates, an analytical approach to the interior solution, and the first steps of a numerical integration based on the resulting system of seven differential equations.

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