Black hole holography and mean field evolution
Holographic theories representing black holes are expected to exhibit quantum chaos. We argue if the laws of quantum mechanics are expected to hold for observers inside such black holes, then such holographic theories must have a mean field approximation valid for typical black hole states, and for...
Published in: | Journal of High Energy Physics |
---|---|
Main Authors: | , |
Other Authors: | , , , , , |
Format: | Article in Journal/Newspaper |
Language: | English |
Published: |
Springer Nature
2018
|
Subjects: | |
Online Access: | https://hdl.handle.net/20.500.11815/677 https://doi.org/10.1007/jhep01(2018)049 |
Summary: | Holographic theories representing black holes are expected to exhibit quantum chaos. We argue if the laws of quantum mechanics are expected to hold for observers inside such black holes, then such holographic theories must have a mean field approximation valid for typical black hole states, and for timescales approaching the scrambling time. Using simple spin models as examples, we examine the predictions of such an approach for observers inside black holes, and more speculatively inside cosmological horizons. This research was supported in part by DOE grant de-sc0010010, Icelandic Research Fund grant 163422-052, the University of Iceland Research Fund, and the Swedish Research Council under contract 621-2014-5838. Peer Reviewed |
---|