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.
Hartle and S.W .Hawking, Wave function of the universe, Phys
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Signature change as phase transition in holography
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.