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Thermal states are vital: Entanglement Wedge Reconstruction from Operator-Pushing
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abstract
We give a general construction of a setup that verifies bulk reconstruction, conservation of relative entropies, and equality of modular flows between the bulk and the boundary, for infinite-dimensional systems with operator-pushing. In our setup, a bulk-to-boundary map is defined at the level of the $C^*$-algebras of state-independent observables. We then show that if the boundary dynamics allow for the existence of a KMS state, physically relevant Hilbert spaces and von Neumann algebras can be constructed directly from our framework. Our construction should be seen as a state-dependent construction of the other side of a wormhole and clarifies the meaning of black hole reconstruction claims such as the Papadodimas-Raju proposal. As an illustration, we apply our result to construct a wormhole based on the HaPPY code, which satisfies all properties of entanglement wedge reconstruction.
Forward citations
Cited by 2 Pith papers
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Observing Spacetime
An asymptotic observer can check a proposed quantum gravity microstate with a probe tuned to the state's creating operator, because extra wormhole saddles make the response O(1) larger than any generic probe.
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Algebraic approach to spacetime bulk reconstruction
Complementary recovery in holographic codes is shown to be equivalent to preservation of Connes cocycle flow, and this holds for AdS Klein-Gordon fields in boundary diamonds and bulk wedges.
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