The enriched phase structure of black branes in canonical ensemble
Abstract
It is found that a necessary completion of phase structure of D-dimensional charged black p-brane (p > 0) in a cavity requires two additional thermodynamical phases, the so-called "bubble of nothing" and/or the extremal brane, in canonical ensemble. This finding resolves the puzzle about the missing phases which are needed for the underlying phase diagram when d = D - p - 3 ≤ 2 and gives a new (bubble) phase which can become globally stable when d > 2. An analog of Hawking-Page transition is also found among other new phase transitions, giving a complete phase structure in this setup.
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