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• W3100974887 startingPage "5121" @default.
• W3100974887 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." @default.
• W3100974887 created "2020-11-23" @default.
• W3100974887 creator A5084570424 @default.
• W3100974887 date "2005-11-22" @default.
• W3100974887 modified "2023-10-01" @default.
• W3100974887 title "Phase transitions near black hole horizons" @default.
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• W3100974887 doi "https://doi.org/10.1088/0264-9381/22/23/013" @default.
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