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Black hole entanglement and quantum error correction

Author(s): Verlinde, Erik; Verlinde, Herman L.

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Abstract: It was recently argued in [1] that black hole complementarity strains the basic rules of quantum information theory, such as monogamy of entanglement. Motivated by this argument, we develop a practical framework for describing black hole evaporation via unitary time evolution, based on a holographic perspective in which all black hole degrees of freedom live on the stretched horizon. We model the horizon as a unitary quantum system with finite entropy, and do not postulate that the horizon geometry is smooth. We then show that, with mild assumptions, one can reconstruct local effective field theory observables that probe the black hole interior, and relative to which the state near the horizon looks like a local Minkowski vacuum. There construction makes use of the formalism of quantum error correcting codes, and works for black hole states who seen tanglement entropy does not yet saturate the Bekenstein-Hawking bound. Our general framework clarifies the black hole final state proposal, and allows a quantitative study of the transition into the “firewall” regime of maximally mixed black hole states.
Publication Date: 17-Oct-2013
Electronic Publication Date: 17-Oct-2013
Citation: Verlinde, Erik, Verlinde, Herman L. (2013). Black hole entanglement and quantum error correction. JOURNAL OF HIGH ENERGY PHYSICS, doi:10.1007/JHEP10(2013)107
DOI: doi:10.1007/JHEP10(2013)107
ISSN: 1029-8479
Type of Material: Journal Article
Version: Final published version. This is an open access article.

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