Black holes, entanglement and random matrices
- 28 August 2014
- journal article
- Published by IOP Publishing in Classical and Quantum Gravity
- Vol. 31 (18) , 185009
Abstract
We provide evidence that strong quantum entanglement between Hilbert spaces does not generically create semiclassical wormholes between the corresponding geometric regions in the context of the AdS/CFT correspondence. We propose a description of low-energy gravity probes as random operators on the space of black hole states. We use this description to compute correlators between the entangled systems, and argue that a wormhole can only exist if correlations are large. Conversely, we also argue that large correlations can exist in the manifest absence of a Lorentzian wormhole. Thus the strength of the entanglement cannot generically diagnose spacetime connectedness, without information on the spectral properties of the probing operators. Our random matrix picture of probes also provides suggestive insights into the problem of ‘seeing behind a horizon’.Keywords
All Related Versions
This publication has 30 references indexed in Scilit:
- Holographic holes in higher dimensionsJournal of High Energy Physics, 2014
- Bulk curves from boundary data in holographyPhysical Review D, 2014
- Black holes and the butterfly effectJournal of High Energy Physics, 2014
- Gauge-Gravity Duality and the Black Hole InteriorPhysical Review Letters, 2013
- Cool horizons for entangled black holesFortschritte der Physik, 2013
- BUILDING UP SPACE–TIME WITH QUANTUM ENTANGLEMENTInternational Journal of Modern Physics D, 2010
- Building up spacetime with quantum entanglementGeneral Relativity and Gravitation, 2010
- Holographic Derivation of Entanglement Entropy from the anti–de Sitter Space/Conformal Field Theory CorrespondencePhysical Review Letters, 2006
- THE LIBRARY OF BABELInternational Journal of Modern Physics D, 2005
- Holographic particle detectionPhysical Review D, 2000