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Flat Information Geometries in Black Hole Thermodynamics

1 Pith paper cite this work. Polarity classification is still indexing.

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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.

fields

hep-lat 1

years

2019 1

verdicts

REJECT 1

representative citing papers

A Fluctuation Theory of Topological Susceptibility

hep-lat · 2019-08-09 · reject · novelty 3.0

The claim that ChPT topological susceptibility fluctuations are always non-interacting relies on a determinant that the paper's own equations show to be nonzero, and the slab sub-volume analysis contains further algebraic errors.

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  • A Fluctuation Theory of Topological Susceptibility hep-lat · 2019-08-09 · reject · none · ref 53 · internal anchor

    The claim that ChPT topological susceptibility fluctuations are always non-interacting relies on a determinant that the paper's own equations show to be nonzero, and the slab sub-volume analysis contains further algebraic errors.