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Black hole holography and mean field evolution
Stockholm University, Faculty of Science, Department of Physics. Stockholm University, Faculty of Science, The Oskar Klein Centre for Cosmo Particle Physics (OKC). University of Iceland, Iceland.
Number of Authors: 22018 (English)In: Journal of High Energy Physics (JHEP), ISSN 1126-6708, E-ISSN 1029-8479, no 1, article id 049Article in journal (Refereed) Published
Abstract [en]

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.

Place, publisher, year, edition, pages
2018. no 1, article id 049
Keywords [en]
AdS-CFT Correspondence, Black Holes, Models of Quantum Gravity
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:su:diva-152532DOI: 10.1007/JHEP01(2018)049ISI: 000422669000004OAI: oai:DiVA.org:su-152532DiVA, id: diva2:1184372
Available from: 2018-02-21 Created: 2018-02-21 Last updated: 2018-02-21Bibliographically approved

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Thorlacius, Larus
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