Distinguishing Black Hole Microstates using Holevo Information
arXiv:1808.02873 · doi:10.1103/PhysRevLett.121.251603
Abstract
We use the Holevo information in a two-dimensional conformal field theory (CFT) with a large central charge to distinguish microstates from the underlying thermal state. Holographically, the CFT microstates of a thermal state are dual to black hole microstate geometries in three-dimensional anti-de Sitter space. It was found recently that the holographic Holevo information shows plateau behaviors at both short and long interval regions. This indicates that the black hole microstates are indistinguishable from the thermal state by measuring over a small region, and perfectly distinguishable over a region with its size comparable to the whole system. In this letter, we demonstrate that the plateaus are lifted by including the corrections from both the vacuum and non-vacuum conformal families of CFT in either the canonical ensemble or microcanonical ensemble thermal state. Our results imply that the aforementioned indistinguishability and distinguishability of black hole microstate geometries from the underlying black hole are spoiled by higher order Newton constant corrections of quantum gravity.
arXiv commentV1, 5+7 pages, 3 figures; V2, discussions on numbers of primary and descendant states refined; V3, 5+7 page, 1+2 figures, references added, published version
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- Revealing quantum operator scrambling via measuring Holevo information on digital quantum simulators
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- Subsystem fidelity in two-dimensional conformal field theories
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