Asymptotically Flat, Stable Black Hole Solutions in Einstein–Yang-Mills–Chern-Simons Theory

Brihaye, Yves and Radu, Eugen and Tchrakian, D. H. (2010) Asymptotically Flat, Stable Black Hole Solutions in Einstein–Yang-Mills–Chern-Simons Theory. Physical Review Letters, 106 (7). ISSN 0031-9007

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Official URL: http://doi.org/10.1103/PhysRevLett.106.071101

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. In addition a solution in closed form describing an extremal black hole with non-Abelian hair is found for a special value of the Chern-Simons coupling constant.

Item Type: Article
Divisions: School of Theoretical Physics > Preprints
Date Deposited: 05 Oct 2017 19:25
Last Modified: 26 Jul 2018 10:04
URI: http://dair.dias.ie/id/eprint/265

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