Rotating black holes with non-Abelian hair
Burkhard KleihausInstitut für Physik, Universität Oldenburg, 26111 Oldenburg, GermanyJutta KunzInstitut für Physik, Universität Oldenburg, 26111 Oldenburg, GermanyFrancisco Navarro-LéridaDept. de Física Atómica, Molecular y Nuclear, Ciencias Físicas Universidad Complutense de Madrid, E-28040 Madrid, Spain
2016en
ABI
Annotatsiya
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.
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