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A new type of nonsingular black-hole solution in general relativity | F.R. Klinkhamer
; | Date: |
26 Sep 2013 | Abstract: | Certain exact solutions of the Einstein field equations over
nonsimply-connected manifolds are reviewed. These solutions are spherically
symmetric and have no curvature singularity. They can be considered to
regularize the Schwarzschild solution with a curvature singularity at the
center. Spherically symmetric collapse of matter in R^4 may result in these
nonsingular black-hole solutions, if quantum-gravity effects allow for topology
change near the center or if the nontrivial topology is already present as a
remnant from a quantum spacetime foam. | Source: | arXiv, 1309.7011 | Services: | Forum | Review | PDF | Favorites |
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