Curvature singularity of the distributional BTZ black hole geometry
arXiv:gr-qc/0205094 · doi:10.1063/1.1699482
Abstract
For the non-rotating BTZ black hole, the distributional curvature tensor field is found. It is shown to have singular parts proportional to a -distribution with support at the origin. This singularity is related, through Einstein field equations, to a point source. Coordinate invariance and independence on the choice of differentiable structure of the results are addressed.
Latex, 7 pages
References in corpus (3)
Cited by in corpus (7)
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