Geometrothermodynamics of black holes in Lorentz non-invariant massive gravity
General Relativity and Quantum Cosmology
2016-07-27 v1 High Energy Physics - Theory
Mathematical Physics
math.MP
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.
Keywords
Cite
@article{arxiv.1603.02259,
title = {Geometrothermodynamics of black holes in Lorentz non-invariant massive gravity},
author = {Alberto Sanchez},
journal= {arXiv preprint arXiv:1603.02259},
year = {2016}
}
Comments
16 latex pages, 8 figures