Non-Singular Gravity Without Black Holes
| dc.creator | Cornish, N. J. | |
| dc.creator | Moffat, J. W. | |
| dc.date | 1994-06-03 | |
| dc.date.accessioned | 2026-07-07T11:46:22Z | |
| dc.date.available | 2026-07-07T11:46:22Z | |
| dc.description | 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. | |
| dc.description | 26 pages, UTPT-94-08 | |
| dc.identifier | https://arxiv.org/abs/gr-qc/9406007 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/9406007 | |
| dc.identifier | J.Math.Phys.35:6628-6643,1994 | |
| dc.identifier | doi:10.1063/1.530697 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/202202 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Non-Singular Gravity Without Black Holes | |
| dc.type | text |