Abstract
We consider static axially symmetric Einstein-Yang-Mills black holes in the isolated horizon formalism. The mass of these hairy black holes is related to the mass of the corresponding particle-like solutions by the horizon mass. The hairy black holes violate the “quasilocal uniqueness conjecture,” based on the horizon charges.
- Received 19 October 2001
DOI:https://doi.org/10.1103/PhysRevD.65.061502
©2002 American Physical Society
