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Rotating Einstein-Yang-Mills Black Holes

B. Kleihaus·J. Kunz·F. Navarro-Lerida
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Abstract

We construct rotating hairy black holes in SU(2) Einstein-Yang-Mills theory. These stationary axially symmetric black holes are asymptotically flat. They possess non-trivial non-Abelian gauge fields outside their regular event horizon, and they carry non-Abelian electric charge. In the limit of vanishing angular momentum, they emerge from the neutral static spherically symmetric Einstein-Yang-Mills black holes, labelled by the node number of the gauge field function. With increasing angular momentum and mass, the non-Abelian electric charge of the solutions increases, but remains finite. The asymptotic expansion for these black hole solutions includes non-integer powers of the radial variable.

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B. Kleihaus, J. Kunz, F. Navarro-Lerida. 2002-07-10. Rotating Einstein-Yang-Mills Black Holes. https://doi.org/10.1103/physrevd.66.104001

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