The purpose of this section is to reexamine the various steps leading to the classification of electrovacuum
black-hole spacetimes for other matter models. In particular, it will be seen that several steps in Figure 3
cease to hold in the presence of non-Abelian gauge fields. Unfortunately, this implies that we are far
from having a classification of all stationary black-hole spacetimes with physically-interesting
sources.
http://www.livingreviews.org/lrr-2012-7 |
Living Rev. Relativity 15, (2012), 7
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