Extremal black holes that are not extremal: maximal warm holes

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Abstract

We study a family of four-dimensional, asymptotically flat, charged black holes that develop (charged) scalar hair as one increases their charge at fixed mass. Surprisingly, the maximum charge for given mass is a nonsingular hairy black hole with nonzero Hawking temperature. The implications for Hawking evaporation are discussed.

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Dias, Ó. J. C., Horowitz, G. T., & Santos, J. E. (2022). Extremal black holes that are not extremal: maximal warm holes. Journal of High Energy Physics, 2022(1). https://doi.org/10.1007/JHEP01(2022)064

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