Rotating Einstein-Yang-Mills Black Holes

Details Rotating Einstein-Yang-Mills Black Holes Rotating Einstein-Yang-Mills Black Holes

2002-07-10

arxiv.org/abs/gr-qc/0207042v1

Phys.Rev. D66 (2002) 104001

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

63 pages, 10 figures

Scientific paper

10.1103/PhysRevD.66.104001

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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