A Study of Phase Transition in Black Hole Thermodynamics
arXiv:1104.3723 · doi:10.1007/s10509-010-0488-6
Abstract
This paper deals with five-dimensional black hole solutions in (a) Einstein-Maxwell-Gauss-Bonnet theory with a cosmological constant and (b)Einstein-Yang-Mills-Gauss-Bonnet theory for spherically symmetric space time. In both the cases the possibility of phase transition is examined and it is analyzed whether the phase transition is a Hawking-Page type phase transition or not.
16 figures
References in corpus (8)
- Thermodynamics of Spacetime: The Einstein Equation of State
- Temperature, Energy, and Heat Capacity of Asymptotically Anti-De Sitter Black Holes
- Geometry of black hole thermodynamics
- Thin-shell wormholes in Einstein-Maxwell theory with a Gauss-Bonnet term
- 5D-Black Hole Solution in Einstein-Yang-Mills-Gauss-Bonnet Theory
- Thermodynamics of Schwarzschild-de Sitter black hole: thermal stability of Nariai black hole
- The geometry of the higher dimensional black hole thermodynamics in Einstein-Gauss-Bonnet theory
- Black holes in the Einstein -Gauss-Bonnet theory and the geometry of their thermodynamics-II