The fact that the stationary electrovac black holes are parametrized by their mass, angular momentum and
electric charge is due to the distinguished structure of the Einstein–Maxwell equations in the presence of a
Killing symmetry. In general, the classification of the stationary black hole space-times within a given
matter model is a difficult task, involving the investigation of Einstein’s equations with a low degree of
symmetries. The variety of black hole configurations in the
Einstein–Yang–Mills system indicates
that – in spite of its beautiful and intuitive content – the uniqueness theorem is a distinguished feature of
electrovac space-times. In general, the stationary black hole solutions of self-gravitating matter fields are
considerably less simple than one might have expected from the experience with the Einstein–Maxwell
system.
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