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• W3102007228 abstract "The Hessian of either the entropy or the energy function can be regarded as a metric on a Gibbs surface. For two parameter families of asymptotically flat black holes in arbitrary dimension one or the other of these metrics are flat, and the state space is a flat wedge. The mathematical reason for this is traced back to the scale invariance of the Einstein-Maxwell equations. The picture of state space that we obtain makes some properties such as the occurence of divergent specific heats transparent." @default.
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• W3102007228 date "2006-06-21" @default.
• W3102007228 modified "2023-09-27" @default.
• W3102007228 title "Flat Information Geometries in Black Hole Thermodynamics" @default.
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• W3102007228 doi "https://doi.org/10.1007/s10714-006-0306-1" @default.
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