2009/02/28 by Hernando Quevedo, Alberto Sanchez · 1 citation
Physics and Astronomy · #gr-qc
paper · pdf · doi:10.1103/physrevd.79.087504
Final version, published in Phys. Rev. D 79, 087504 (2009)
arxiv created 2009/10/22 · arxiv updated 2015/05/12
We study the properties of two-dimensional dilatonic black holes from the viewpoint of geometrothermodynamics. We show that the thermodynamic curvature of the equilibrium space vanishes only in the case of a flat spacetime, and it reproduces correctly the behavior of the thermodynamic interaction and phase transition structure of the corresponding black hole configurations.