  A new version of nonsymmetric gravitational theory is presented. The field
equations are expanded about the Minkowski metric, giving in lowest order the
linear Einstein field equations and massive Proca field equations for the
antisymmetric field $g_{[\mu\nu]}$. An expansion about an arbitrary Einstein
background metric yields massive Proca field equations with couplings to only
physical modes. It follows that the new version of NGT is free of ghost poles,
tachyons and higher-order poles and there are no problems with asymptotic
boundary conditions. A static spherically symmetric solution of the field
equations in the short-range approximation is everywhere regular and does not
contain a black hole event horizon.
