Critical Black Holes in a Large Charge Limit
arXiv:1705.01154 · doi:10.1142/S0217732318501754
Abstract
The extended thermodynamics of Reissner-Nordström charged black holes in D-dimensional anti-de Sitter spacetime has a phase structure in the (T,p) plane that includes a line of first order phase transitions ending in a second order transition point. For each D>=4, properties of the critical black hole at that point are explored, motivated by the observation that in D=4 its neighbourhood plays a core role in defining a very special class of heat engines that asymptote to Carnot efficiency in the large charge limit. This new limit provides a model of a novel low-temperature thermodynamic system. The double limit of approaching the horizon while sending q large at an appropriate rate yields a fully decoupled D-dimensional Rindler spacetime with zero cosmological constant.
4 pages, 1 figure
References in corpus (3)
Cited by in corpus (8)
- Novel relations in massive gravity at Hawking-Page transition
- Photon orbits and phase transition for Non-Linear charged Anti-de Sitter black holes
- Topology and phase transition for EPYM AdS black hole in thermal potential
- Restricted phase space thermodynamics of Einstein-power-Yang-Mills AdS black hole
- Dynamic Property of Phase Transition for Non-Linear Charged Anti-de Sitter black holes
- Nonlinearity effect on Joule-Thomson expansion of Einstein-power-Yang-Mills AdS black hole
- Critical Heat Engines in Massive Gravity
- Phase transition of non-linear charged Anti-de Sitter black holes