Global and Local Thermodynamics of the Rotating GaussBonnet BTZ Black Hole
Abstract
The aim of this paper is to study the local and the global thermodynamic properties of the 3dimensional rotating GaussBonnet BTZ black hole. We are interested in deriving the conditions for local and global thermodynamic stability of the solution in a given ensemble of state quantities. It is wellknown that determining the local thermodynamic stability requires the calculation of the specific heats of the system. We identify the regions of stability for every physical specific heat together with the existing Davies curves. In addition to the local analysis, we generalize the notion of global thermodynamic stability from the standard thermodynamics to describe the global equilibrium of black holes. Here, we apply a proper Legendre transformation of the energy or the entropy to find the natural thermodynamic potential for the given ensemble of macro parameters. The global stability analysis is now conducted on the properties of the new thermodynamic potential. The advantage of this method is that it allows one to chose different potentials, corresponding to different constraints to which the system may be subjected. Finally, we find it natural to impose global thermodynamic stability only where local one exists for the given black hole solution.
 Publication:

arXiv eprints
 Pub Date:
 October 2021
 arXiv:
 arXiv:2110.05166
 Bibcode:
 2021arXiv211005166D
 Keywords:

 General Relativity and Quantum Cosmology;
 High Energy Physics  Theory
 EPrint:
 21 pages, 7 figures