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arXiv · 1603.02259

Geometrothermodynamics of black holes in Lorentz non-invariant massive gravity

Alberto Sanchez
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Abstract

We analyze a static and spherically symmetric hairy black hole solution in non-invariant massive gravity. The formalism of geometrothermodynamics is used to describe the thermodynamic characteristics of this black hole in a Legendre invariant way. For a black hole in massive gravity, the geometry of the space of equilibrium states is computed showing that it contains information about the thermodynamic interaction, critical points and phase transitions structure.

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Alberto Sanchez. 2016-03-05. Geometrothermodynamics of black holes in Lorentz non-invariant massive gravity. https://doi.org/10.1103/physrevd.94.024037

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