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arXiv · 1011.1624

Asymptotically flat, stable black hole solutions in Einstein--Yang-Mills--Chern-Simons theory

Yves Brihaye·Eugen Radu·D. H. Tchrakian
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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-Nordstrom 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.

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Yves Brihaye, Eugen Radu, D. H. Tchrakian. 2010-11-07. Asymptotically flat, stable black hole solutions in Einstein--Yang-Mills--Chern-Simons theory. https://doi.org/10.1103/physrevlett.106.071101

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