Rotating black holes with non-Abelian hair
High Energy Physics - Theory
2016-12-07 v1 General Relativity and Quantum Cosmology
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.
Keywords
Cite
@article{arxiv.1609.07357,
title = {Rotating black holes with non-Abelian hair},
author = {Burkhard Kleihaus and Jutta Kunz and Francisco Navarro-Lerida},
journal= {arXiv preprint arXiv:1609.07357},
year = {2016}
}
Comments
33 pages, 7 figures