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Thermodynamic stability of asymptotically anti-de Sitter rotating black holes in higher dimensions
2014
Classical and quantum gravity
Conditions for thermodynamic stability of asymptotically anti-de Sitter rotating black holes in D-dimensions are determined. Local thermodynamic stability requires not only positivity conditions on the specific heat and the moment of inertia tensor but it is also necessary that the adiabatic compressibility be positive. It is shown that, in the absence of a cosmological constant, neither rotation nor charge is sufficient to ensure full local thermodynamic stability of a black hole.
doi:10.1088/0264-9381/31/16/165011
fatcat:7kbtj4gyajcwjiyb2ddg2zklsu