Rotating solitons and non-rotating, non-static black holes

Details Rotating solitons and non-rotating, non-static black holes Rotating solitons and non-rotating, non-static black holes

1997-07-29

arxiv.org/abs/gr-qc/9707057v1

Phys.Rev.Lett. 79 (1997) 4310-4313

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

5 pages, REVTeX

Scientific paper

10.1103/PhysRevLett.79.4310

It is shown that the non-Abelian black hole solutions have stationary generalizations which are parameterized by their angular momentum and electric Yang-Mills charge. In particular, there exists a non-static class of stationary black holes with vanishing angular momentum. It is also argued that the particle-like Bartnik-McKinnon solutions admit slowly rotating, globally regular excitations. In agreement with the non-Abelian version of the staticity theorem, these non-static soliton excitations carry electric charge, although their non-rotating limit is neutral.

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