arXiv · gr-qc/0110084
Horizon Properties of Einstein-Yang-Mills Black Hole
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 ``quasi-local uniqueness conjecture'', based on the horizon charges.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
B. Kleihaus, J. Kunz, A. Sood, M. Wirschins. 2001-10-19. Horizon Properties of Einstein-Yang-Mills Black Hole. https://doi.org/10.1103/physrevd.65.061502
Cite the original work for its findings. Save a collection to share your selection of sources.