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Universal properties of distorted Kerr-Newman black holes

MPG-Autoren
http://pubman.mpdl.mpg.de/cone/persons/resource/persons20688

Hennig,  Jörg
Geometric Analysis and Gravitation, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons20685

Cederbaum,  Carla
Geometric Analysis and Gravitation, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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Volltexte (frei zugänglich)

1005.3128
(Preprint), 94KB

GRG43_1205.pdf
(beliebiger Volltext), 113KB

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Zitation

Ansorg, M., Hennig, J., & Cederbaum, C. (2011). Universal properties of distorted Kerr-Newman black holes. General Relativity and Gravitation, 43(5), 1205-1210. doi:10.1007/s10714-010-1136-8.


Zitierlink: http://hdl.handle.net/11858/00-001M-0000-0012-BD38-D
Zusammenfassung
We discuss universal properties of axisymmetric and stationary configurations consisting of a central black hole and surrounding matter in Einstein-Maxwell theory. In particular, we find that certain physical equations and inequalities (involving angular momentum, electric charge and horizon area) are not restricted to the Kerr-Newman solution but can be generalized to the situation where the black hole is distorted by an arbitrary axisymmetric and stationary surrounding matter distribution.