A physical derivation of the Kerr-Newman black hole solution
General Relativity and Quantum Cosmology
2017-11-08 v1 High Energy Astrophysical Phenomena
High Energy Physics - Theory
Abstract
According to the no-hair theorem, the Kerr-Newman black hole solution represents the most general asymptotically flat, stationary (electro-) vacuum black hole solution in general relativity. The procedure described here shows how this solution can indeed be constructed as the unique solution to the corresponding boundary value problem of the axially symmetric Einstein-Maxwell equations in a straightforward manner.
Keywords
Cite
@article{arxiv.1310.0640,
title = {A physical derivation of the Kerr-Newman black hole solution},
author = {Reinhard Meinel},
journal= {arXiv preprint arXiv:1310.0640},
year = {2017}
}
Comments
8 pages, contribution to the Proceedings of the Karl Schwarzschild Meeting (Frankfurt, July 22-26, 2013)