Marion Wirschins

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SU(4) Einstein-Yang-Mills theory possesses sequences of static spherically symmetric globally regular and black hole solutions. Considering solutions with a purely magnetic gauge field, based on the 4-dimensional embedding of su(2) in su(4), these solutions are labelled by the node numbers (n1, n2, n3) of the three gauge field functions u1, u2 and u3. We(More)
In Einstein-Maxwell theory black holes are uniquely determined by their mass, their charge and their angular momentum. This is no longer true in EinsteinYang-Mills theory. We discuss sequences of neutral and charged SU(N) EinsteinYang-Mills black holes, which are static spherically symmetric and asymptotically flat, and which carry Yang-Mills hair.(More)
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