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arXiv · 1609.07357

Rotating black holes with non-Abelian hair

Burkhard Kleihaus·Jutta Kunz·Francisco Navarro-Lerida
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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.

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Burkhard Kleihaus, Jutta Kunz, Francisco Navarro-Lerida. 2016-09-23. Rotating black holes with non-Abelian hair. https://doi.org/10.1088/0264-9381%2F33%2F23%2F234002

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