Rotating black holes with non-Abelian hair
arXiv:1609.07357 · doi:10.1088/0264-9381/33/23/234002
Abstract
We here review asymptotically flat rotating black holes in the presence of non-Abelian gauge fields. Like their static counterparts these black holes are no longer uniquely determined by their global charges. In the case of pure SU(2) Yang-Mills fields, the rotation generically induces an electric charge, while the black holes do not carry a magnetic charge. When a Higgs field is coupled, rotating black holes with monopole hair arise in the case of a Higgs triplet, while in the presence of a complex Higgs doublet the black holes carry sphaleron hair. The inclusion of a dilaton allows for Smarr type mass formulae.
33 pages, 7 figures
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Cited by in corpus (6)
- Static spherically symmetric Einstein-Yang-Mills-dilaton black hole and its thermodynamics
- Finite-action solutions of Yang-Mills equations on de Sitter dS and anti-de Sitter AdS spaces
- Static dilatonic black hole with nonlinear Maxwell and Yang-Mills fields of power-law type
- Compact Objects in Alternative Gravities
- High precision numerical sequences of rotating hairy black holes
- Non-Abelian black holes in conformal gravity