Hawking-Page phase transition, Page curve and islands in black holes
arXiv:2107.05218
Abstract
We study the Page curve and the effect of the Hawking-Page phase transition in the Vaidya model of evaporating BTZ black holes, both with and without islands. The phase transition can occur before, at, or after the Page time. When it occurs before the Page time, the information release does not require an island yet still reproduces the Page curve. From the first law of entanglement, the entanglement temperature changes from negative to positive, diverging at the Page time. Thus, the information deposition phase corresponds to a negative temperature, and the release phase to a positive temperature. If the Hawking-Page phase transition takes place, all black hole information is released at once via a quantum jump. We speculate that first-order phase transitions universally affect black hole information, providing an alternative escape mechanism independent of Hawking radiation.
References in corpus (10)
- Holographic Derivation of Entanglement Entropy from AdS/CFT
- Entanglement Entropy and Quantum Field Theory
- P-V criticality of charged AdS black holes
- Information in Black Hole Radiation
- The cosmological constant and the black hole equation of state
- Phases of R-charged Black Holes, Spinning Branes and Strongly Coupled Gauge Theories
- Thermodynamical Property of Entanglement Entropy for Excited States
- Holographic entanglement plateaux
- RG flow of entanglement entropy to thermal entropy
- Holographic entanglement entropy and generalized entanglement temperature