Interior problem in a ponsymmetric theory of gravitation

Abstract

The field equations of a previous metric nonsymmetric theory of gravitation are considered for the interior of a static spherically symmetric perfect fluid with a view to a study of stellar equilibrium. The equations are put into a form of four first-order differential equations which are ready for numerical integration.

Metric nonsymmetric theory of gravitation: the analogue of the theorem of Birkhoff

“…The conservation laws associated to the theory were studied by one of us in [3]. Then [4], we have established the equations governing the interior problem of a static spherically symmetric perfect fluid with a view to a study of stelar equilibrium.…”