Embedding of the Kerr-Newman Black Hole Surface in Euclidean Space
arXiv:gr-qc/0601104 · doi:10.1103/PhysRevD.73.064021
Abstract
We obtain a global embedding of the surface of a rapidly rotating Kerr-Newman black hole in an Euclidean 4-dimensional space.
arXiv comment5 pages, 6 figures
References in corpus (3)
Cited by in corpus (13)
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