English

Non-Singular Gravity Without Black Holes

General Relativity and Quantum Cosmology 2008-11-26 v1

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.

Keywords

Cite

@article{arxiv.gr-qc/9406007,
  title  = {Non-Singular Gravity Without Black Holes},
  author = {N. J. Cornish and J. W. Moffat},
  journal= {arXiv preprint arXiv:gr-qc/9406007},
  year   = {2008}
}

Comments

26 pages, UTPT-94-08