Constructive proof of the Kerr-Newman black hole uniqueness: derivation of the full solution from scratch
arXiv:1208.0294 · doi:10.1142/9789814623995_0290
Abstract
The Kerr-Newman black hole solution can be constructed straightforwardly as the unique solution to the boundary value problem of the Einstein-Maxwell equations corresponding to an asymptotically flat, stationary and axisymmetric electro-vacuum spacetime surrounding a connected Killing horizon.
3 pages, contribution to the Proceedings of the Thirteenth Marcel Grossmann Meeting on General Relativity (Stockholm, July 1-7, 2012)