Uniqueness of Kerr–Newman–de Sitter Black Holes with Small Angular Momenta

We show that a stationary solution of the Einstein–Maxwell equations which is close to a non-degenerate Reissner–Nordström–de Sitter solution is in fact equal to a slowly rotating Kerr–Newman–de Sitter solution. The proof uses the nonlinear stability of the Kerr–Newman–de Sitter family of black hole...

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Veröffentlicht in:	Annales Henri Poincaré 2018-02, Vol.19 (2), p.607-617
1. Verfasser:	Hintz, Peter
Format:	Artikel
Sprache:	eng
Schlagworte:	Black holes Classical and Quantum Gravitation Dynamical Systems and Ergodic Theory Elementary Particles Fields (mathematics) Mathematical and Computational Physics Mathematical Methods in Physics Maxwell's equations Physics Physics and Astronomy Quantum Field Theory Quantum Physics Relativity Theory Theoretical Uniqueness
Online-Zugang:	Volltext
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