Asymptotically Flat, Stable Black Hole Solutions in Einstein-Yang-Mills-Chern-Simons Theory
Journal Article
·
· Physical Review Letters
- Physique-Mathematique, Universite de Mons, Mons (Belgium)
- School of Theoretical Physics-DIAS, 10 Burlington Road, Dublin 4 (Ireland)
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-Nordstroem 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.
- OSTI ID:
- 21532307
- Journal Information:
- Physical Review Letters, Vol. 106, Issue 7; Other Information: DOI: 10.1103/PhysRevLett.106.071101; (c) 2011 American Institute of Physics; ISSN 0031-9007
- Country of Publication:
- United States
- Language:
- English
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