Non-Singular Gravity Without Black Holes

Abstract

A non-singular, static spherically symmetric solution to the nonsymmetric gravitational and electromagnetic theory field equations is derived, which depends on the four parameters m, l^2, Q and s, where m is the mass, Q is the electric charge, l^2 is the NGT charge of a body and s is a dimensionless constant. The electromagnetic field invariants are also singularity-free, so that it is possible to construct regular particle-like solutions in the theory. All the curvature invariants are finite, there are no null surfaces in the spacetime and there are no black holes. A new stable, superdense object (SDO) replaces black holes.

26 pages, UTPT-94-08

References in corpus (2)

• The Structure of Naked Singularity in Self-similar Gravitational Collapse II
• A Non-singular Theory of Gravity

Cited by in corpus (7)

• Nonsymmetric Gravitational Theory
• On the nonsymmetric purely affine gravity
• Regularity Theorems in the Nonsymmetric Gravitational Theory
• On the formation of black holes in non-symmetric gravity
• Short Distance Repulsive Gravity as a Consequence of Non Trivial PPN Parameters $\beta$ and $\gamma$
• Homothetic Wyman Spacetimes
• 5D non-symmetric gravity and geodesic confinement