Critical Phenomena of Born-Infeld-de Sitter Black Holes in Cavities
read the original abstract
We examine the thermodynamic behaviour of charged, asymptotically de Sitter black holes embedded in a finite-radius isothermal cavity, with a Born-Infeld gauge field replacing the ordinary Maxwell field. We find that the non-linearities of Born-Infeld theory lead to the presence of reentrant phase transitions in the canonical ensemble, whose existence and character are determined by the maximal electric field strength of the theory. We also examine the phase structure in the grand canonical ensemble, and demonstrate the presence of a new reentrant phase transition from radiation, to an intermediate size black hole, and back to radiation.
This paper has not been read by Pith yet.
Forward citations
Cited by 1 Pith paper
-
Critical Inter-Horizon Thermal Dynamics on the Lukewarm Reissner-Nordstr\"om-de Sitter Manifold
Lukewarm RNdS black holes are promoted to a critical inter-horizon thermal manifold where a linearized mode's relaxation time diverges at ρ_* ≈ 0.4354.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.