Stable black hole solutions with non-Abelian fields
Nov, 2011Citations per year
Abstract: (arXiv)
We construct finite mass, asymptotically flat black hole solutions in d=4 Einstein-Yang-Mills theory augmented with higher order curvature terms of the gauge field. They possess non-Abelian hair in addition to Coulomb electric charge, and, below some non-zero critical temperature, they are thermodynamically preferred over the Reissner-Nordstrom solution. Our results indicate the existence of hairy non-Abelian black holes which are stable under linear, spherically symmetric perturbations.Note:
- 8 pages, 3 figures
- 04.20.-q
- 04.70.-s
- 11.10.-z
- black hole: nonabelian
- black hole: stability
- curvature: higher-order
- black hole: charge
- symmetry: rotation
- black hole: hair
- perturbation: linear
References(16)
Figures(3)