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AdS black holes, the bulk-boundary dictionary, and smearing functions

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arxiv 1304.6821 v2 pith:R5TZNSIV submitted 2013-04-25 hep-th gr-qc

classification hep-thgr-qc
keywords boundarybulkmodesarguebarrierblackbulk-boundarydictionary
verification ladder T0 review T1 audit T2 compute T3 formal
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In Lorentzian AdS/CFT there exists a mapping between local bulk operators and nonlocal CFT operators. In global AdS this mapping can be found through use of bulk equations of motion and allows the nonlocal CFT operator to be expressed as a local operator smeared over a range of positions and times. We argue that such a construction is not possible if there are bulk normal modes with exponentially small near boundary imprint. We show that the AdS-Schwarzschild background is such a case, with the horizon introducing modes with angular momentum much larger than frequency, causing them to be trapped by the centrifugal barrier. More generally, we argue that any barrier in the radial effective potential which prevents null geodesics from reaching the boundary will lead to modes with vanishingly small near boundary imprint, thereby obstructing the existence of a smearing function. While one may have thought the bulk-boundary dictionary for low curvature regions, such as the exterior of a black hole, should be as in empty AdS, our results demonstrate otherwise.

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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. Boundary-to-bulk maps for AdS causal wedges and RG flow

    hep-th 2019-08 conditional novelty 7.0 of 10

    Robin-boundary-condition HKLL smearing functions with spacelike support are constructed in AdS causal wedges and used to map the double-trace-deformed CFT Wightman function to the bulk Robin Wightman function.

  2. Complexity measures in holographic cascading theories with multiscale dynamics

    hep-th 2026-08 accept novelty 6.0 of 10

    In holographic B8 gauge theories, complexity growth flattens near a walking conformal regime, while Krylov oscillation periods track the infrared scale and persist in screened, non-confining phases.

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