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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)

We construct regular and black hole solutions in SU(2) Einstein-Born-Infeld theory. These solutions have many features in common with the corresponding SU(2) Einstein-Yang-Mills solutions. In particular, sequences of neutral nonabelian solutions tend to magnetically charged limiting solutions, related to embedded abelian solutions. Thermodynamic properties… (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)

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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