Information Preservation and Weather Forecasting for Black Holes
By S. Hawking. 2014
181 citations recorded by the source corpus.
It has been suggested [1] that the resolution of the information paradox for evaporating black holes is that the holes are surrounded by firewalls, bolts of outgoing radiation that would destroy any infalling observer. Such firewalls would break the CPT invariance of quantum gravity and seem to be ruled out on other grounds. A different resolution of the paradox is proposed, namely that gravitational collapse produces apparent horizons but no event horizons behind which information is lost. This proposal is supported by ADS-CFT and is the only resolution of the paradox compatible with CPT. The collapse to form a black hole will in general be chaotic and the dual CFT on the boundary of ADS will be turbulent. Thus, like weather forecasting on Earth, information will effectively be lost, although there would be no loss of unitarity.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics
View Paper: https://www.semanticscholar.org/paper/d545549ee1b64d234d61b2345330083f7fd849fa
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In Astronomy and Astrophysics
- Valeri P. Frolov
- Hal M. Haggard
- Carlo Rovelli
- Alejandro Perez
- B. Dittrich
- Matt Visser
- Alex Simpson
- D. Marolf
In Nuclear and High Energy Physics
- Valeri P. Frolov
- Hal M. Haggard
- Carlo Rovelli
- Alejandro Perez
- B. Dittrich
- Giovanni Amelino-Camelia
- Matt Visser
- L. Freidel
In Statistical and Nonlinear Physics
- Hal M. Haggard
- Valeri P. Frolov
- Carlo Rovelli
- Alejandro Perez
- B. Dittrich
- T. Thiemann
- L. Modesto
- D. Oriti
Citations in the corpus
- Information loss problem and a ‘black hole’ model with a closed apparent horizon (2014, background): “Hawking in his recent paper [14] proposed to solve the information loss puzzle by assuming that in the gravitational collapse an apparent is formed but the event horizon does not exists.”
- Quantum-gravity effects outside the horizon spark black to white hole tunneling (2014, background): “This suggests that we can search for the metric of a bouncing star by gluing a collapsing region with its time reversal, where the star is expanding [20].”
- Introduction to holographic superconductor models (2015, unknown): “, evolves in a unitary fashion [52, 53].”