3.1 Spherically Symmetric Black Holes Stationary Black Holes: Uniqueness and 2.3 Black Holes with Degenerate

3 Beyond Einstein-Maxwell 

The purpose of this section is to estimate the generality of the various steps leading to the classification of electrovac black hole space-times. In particular, we shall argue that virtually all theorems displayed in Fig. 1 cease to exist in the presence of non-Abelian gauge fields. Unfortunately, this implies that we are far from having a classification of all stationary black hole space-times.





3.1 Spherically Symmetric Black Holes Stationary Black Holes: Uniqueness and 2.3 Black Holes with Degenerate

image Stationary Black Holes: Uniqueness and Beyond
Markus Heusler
http://www.livingreviews.org/lrr-1998-6
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