arXiv · gr-qc/9407006
Extended Geometry of Black Holes
Abstract
We reconsider space-time singularities in classical Einsteinian general relativity: with the help of several new co-ordinate systems we show that the Schwarzschild solution can be extended beyond the curvature singularity at r=0. The extension appears as an infinite covering of standard Kruskal space-time. While the two-dimensional reduction of this infinite sequence of Kruskal-Szekeres domains obtained by suppressing the angular degrees of freedom is still a topological manifold - albeit one for which the metric structure is singular on one-dimensional submanifolds - we obtain for the full four-dimensional geometry the more general structure of a stratified variety.
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K. Peeters, C. Schweigert, J. W. van Holten. 1994-07-08. Extended Geometry of Black Holes. https://doi.org/10.1088/0264-9381%2F12%2F1%2F015
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