Thermal states in Anti-de Sitter space-time and the role of time-like infinity
arXiv:gr-qc/9402009 · doi:10.1103/PhysRevD.50.5148
Abstract
The grand-canonical thermodynamic potential for Bose and Fermi fields in anti-de Sitter space-time is introduced and a Mellin complex representation is given. This is used to investigate the high temperature properties of the thermal state at finite charge. The time-like nature of spatial infinity is shown to act as a boundary, and changes the free energy of the field in thermal equilibrium.
8, Latex, UTF 317
Cited by in corpus (4)
- Thermodynamical properties of hairy black holes in n spacetimes dimensions
- Finite temperature current densities and Bose-Einstein condensation in topologically nontrivial spaces
- Bose-Einstein condensation as symmetry breaking in compact curved spacetimes
- Interaction of Low - Energy Induced Gravity with Quantized Matter -- II. Temperature effects