Slowly Rotating Non-Abelian Black Holes

Details Slowly Rotating Non-Abelian Black Holes Slowly Rotating Non-Abelian Black Holes

1997-04-03

arxiv.org/abs/hep-th/9704026v1

Phys.Rev.Lett.79:1428-1431,1997

Physics

High Energy Physics

High Energy Physics - Theory

8 pages, LaTeX

Scientific paper

10.1103/PhysRevLett.79.1428

It is shown that the well-known non-Abelian static SU(2) black hole solutions have rotating generalizations, provided that the hypothesis of linearization stability is accepted. Surprisingly, this rotating branch has an asymptotically Abelian gauge field with an electric charge that cannot vanish, although the non-rotating limit is uncharged. We argue that this may be related to our second finding, namely that there are no globally regular slowly rotating excitations of the particle-like Bartnik-McKinnon solutions.

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