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Wormholes and entanglement in holography

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arxiv 1405.4817 v1 pith:NVPY4WMJ submitted 2014-05-19 hep-th

classification hep-th
keywords dualentangledentanglementgravityholographyarguebasiccausally
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In this essay, we consider highly entangled states in theories with a gravity dual, where the entangled degrees of freedom are causally disconnected from each other. Using the basic rules of holography, we argue that there is a non-traversable wormhole in the gravity dual whose geometry encodes the pattern of the entanglement.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Nonlocal Nonstabilizerness from Holographic Schwinger Pair Production

    hep-th 2026-05 unverdicted novelty 6.0 of 10

    In holographic Schwinger pair production, the excess capacity of entanglement is √λ(d−2)/(d−1)³ — positive for d>2, zero for d=2 — so the produced pair carries nonlocal magic for d>2.

  2. Signature change as phase transition in holography

    hep-th 2025-05 conditional novelty 4.0 of 10

    Entangled holographic states below the Hawking-Page temperature stay classically connected through Euclidean spacetime regions, extending ER-EPR to cases where Lorentzian wormholes are unstable.

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