On the classification of stationary electro-vacuum black holes
arXiv:0912.0834 · doi:10.1088/0264-9381/27/3/035010
Abstract
We obtain a classification of stationary, --regular, non-degenerate and analytic electro-vacuum space-times in terms of Weinstein solutions. In particular, for connected horizons, we prove uniqueness of the Kerr-Newman black holes.
References in corpus (5)
- Mass and angular-momentum inequalities for axi-symmetric initial data sets. II. Angular-momentum
- Mass and angular-momentum inequalities for axi-symmetric initial data sets I. Positivity of mass
- Non-existence of stationary two-black-hole configurations
- Uniqueness of Extremal Kerr and Kerr-Newman Black Holes
- Proof of the angular momentum-mass inequality for axisymmetric black holes
Cited by in corpus (7)
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- Integrability of Five Dimensional Minimal Supergravity and Charged Rotating Black Holes
- Constructive proof of the Kerr-Newman black hole uniqueness including the extreme case
- A Dain Inequality with charge
- A uniqueness theorem for degenerate Kerr-Newman black holes
- Generalizations and challenges for the spacetime block-diagonalization
- Soliton methods and the black hole balance problem