title: Asymptotically flat, stable black hole solutions in Einstein-Yang-Mills-Chern-Simons theory.
abstract: We construct finite mass, asymptotically flat black hole solutions in d=5 Einstein-Yang-Mills-Chern-Simons theory. Our results indicate the existence of a second order phase transition between Reissner-Nordström solutions and the non-Abelian black holes which generically are thermodynamically preferred. Some of the non-Abelian configurations are also stable under linear, spherically symmetric perturbations.
authors.affiliation: Physique-Mathématique, Université de Mons, Belgium.
authors.forename: Yves
authors.initials: Y
authors.lastname: Brihaye
authors.forename: Eugen
authors.initials: E
authors.lastname: Radu
authors.forename: D H
authors.initials: DH
authors.lastname: Tchrakian