On the many saddle points description of quantum black holes
arXiv:1307.6238 · doi:10.1016/j.physletb.2014.04.030
Abstract
Considering two dimensional gravity coupled to a CFT, we show that a semiclassical black hole can be described in terms of two Liouville theories matched at the horizon. The black hole exterior corresponds to a space-like while the interior to a time-like Liouville theory. This matching automatically implies that a semiclassical black hole has an infinite entropy. The path integral description of the time-like Liouville theory (the Black Hole interior) is studied and it is found that the correlation functions of the coupled CFT-gravity system are dominated by two (complex) saddle points, even in the semiclassical limit. We argue that this system can be interpreted as two interacting Bose-Einstein condensates constructed out of two degenerate quantum states. In AdS/CFT context, the same system is mapped into two interacting strings intersecting inside a three-dimensional BTZ black hole. Finally, we discuss why, beyond the semiclassical approximation, we expect no firewalls appearing in our system.
11 pages, RevTeX; v2 clarifications and references added
References in corpus (6)
Cited by in corpus (7)
- Excluding Black Hole Firewalls with Extreme Cosmic Censorship
- On Information Loss in AdS/CFT
- Liouville Quantum Gravity
- Liouville mode in Gauge/Gravity Duality
- Firewalls as artefacts of inconsistent truncations of quantum geometries
- Retrieving black hole information from the main Lorentzian saddle point
- Remnants in two-dimensional quantum gravity