Black hole holography and mean field evolution
Abstract
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.
- Authors:
-
- Brown Univ., Providence, RI (United States). Physics Dept.
- Univ. of Iceland, Reykjavik (Iceland). Science Inst.; Stockholm Univ. (Sweden). The Oskar Klein Centre for Cosmoparticle Physics, Dept. of Physics
- Publication Date:
- Research Org.:
- Brown Univ., Providence, RI (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC)
- OSTI Identifier:
- 1502066
- Grant/Contract Number:
- SC0010010
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Journal of High Energy Physics (Online)
- Additional Journal Information:
- Journal Name: Journal of High Energy Physics (Online); Journal Volume: 2018; Journal Issue: 1; Journal ID: ISSN 1029-8479
- Publisher:
- Springer Berlin
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; AdS-CFT Correspondence; Black Holes; Models of Quantum Gravity
Citation Formats
Lowe, David A., and Thorlacius, Larus. Black hole holography and mean field evolution. United States: N. p., 2018.
Web. doi:10.1007/jhep01(2018)049.
Lowe, David A., & Thorlacius, Larus. Black hole holography and mean field evolution. United States. https://doi.org/10.1007/jhep01(2018)049
Lowe, David A., and Thorlacius, Larus. Thu .
"Black hole holography and mean field evolution". United States. https://doi.org/10.1007/jhep01(2018)049. https://www.osti.gov/servlets/purl/1502066.
@article{osti_1502066,
title = {Black hole holography and mean field evolution},
author = {Lowe, David A. and Thorlacius, Larus},
abstractNote = {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.},
doi = {10.1007/jhep01(2018)049},
journal = {Journal of High Energy Physics (Online)},
number = 1,
volume = 2018,
place = {United States},
year = {Thu Jan 11 00:00:00 EST 2018},
month = {Thu Jan 11 00:00:00 EST 2018}
}
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Works referencing / citing this record:
Quantum out-of-equilibrium cosmology
journal, April 2019
- Choudhury, Sayantan; Mukherjee, Arkaprava; Chauhan, Prashali
- The European Physical Journal C, Vol. 79, Issue 4