arXiv · 1012.3256
Black hole phase transitions via Bragg-Williams
Abstract
We argue that a convenient way to analyze instabilities of black holes in AdS space is via Bragg-Williams construction of a free energy function. Starting with a pedagogical review of this construction in condensed matter systems and also its implementation to Hawking-Page transition, we study instabilities associated with hairy black holes and also with the $R$-charged black holes. For the hairy black holes, an analysis of thermal quench is presented.
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Souvik Banerjee, Sayan K. Chakrabarti, Sudipta Mukherji, Binata Panda. 2010-12-15. Black hole phase transitions via Bragg-Williams. https://doi.org/10.1142/s0217751x11053845
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