Universal properties of distorted Kerr-Newman black holes
arXiv:1005.3128 · doi:10.1007/s10714-010-1136-8
Abstract
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.
arXiv comment7 pages
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