Cool horizons for entangled black holes
2013/06/03 by Juan Maldacena, J. Maldacena, Leonard Susskind +1 · 2 voices · 1,258 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Black hole (networking) #Cosmology and Gravitation Theories #Firewall (physics) #General relativity #Hawking radiation #Noncommutative and Quantum Gravity Theories #Quantum entanglement #Theory of relativity #hep-th
paper · pdf · doi:10.1002/prop.201300020
published in Fortschritte der Physik 61(9), 781-811 (Wiley) · 48 pages, 23 figures. v2: references added
arxiv published 2013/06/03 · arxiv created 2013/07/11 · openalex publication_date 2013/08/01 · arxiv updated 2015/06/16 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Abstract
Abstract General relativity contains solutions in which two distant black holes are connected through the interior via a wormhole, or Einstein‐Rosen bridge. These solutions can be interpreted as maximally entangled states of two black holes that form a complex EPR pair. We suggest that similar bridges might be present for more general entangled states. In the case of entangled black holes one can formulate versions of the AMPS(S) paradoxes and resolve them. This suggests possible resolutions of the firewall paradoxes for more general situations.
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