Phase transitions near black hole horizons
arXiv:hep-th/0505189 · doi:10.1088/0264-9381/22/23/013
Abstract
The Reissner-Nordstrom black hole in four dimensions can be made unstable without violating the dominant energy condition by introducing a real massive scalar with non-renormalizable interactions with the gauge field. New stable black hole solutions then exist with greater entropy for fixed mass and charge than the Reissner-Nordstrom solution. In these new solutions, the scalar condenses to a non-zero value near the horizon. Various generalizations of these hairy black holes are discussed, and an attempt is made to characterize when black hole hair can occur.
30 pages, 6 figures. v2: minor corrections, references added
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