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Scanning Tunneling Macroscopy, Black Holes, and AdS/CFT Bulk Locality

High Energy Physics - Theory · Submitted 16 Mar 2014

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim Our results demonstrate that, if there is a black hole of any size in the bulk, then sub-AdS bulk locality is no longer well-encoded in boundary data in terms of local CFT operators.

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arXiv ID1403.3943 (version 2)
Pith IDD7E7VXN7, Pith's permanent record of this paper and its review
CitationSoo-Jong Rey, Vladimir Rosenhaus. "Scanning Tunneling Macroscopy, Black Holes, and AdS/CFT Bulk Locality." arXiv:1403.3943 (2014). https://pith.science/paper/D7E7VXN7
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Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 6,863 input tokens, $0.0003 reported.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.73 · human participants 0.01 · controlled comparison 0.07 · randomized assignment 0.01 · states quantitative result 0.72 · compares with prior results 0.19 · mentions code or data availability 0.01.

The abstract, sentence by sentence

arXiv listing abstract v2. Results and the main claim are underlined; .

We establish resolution bounds on reconstructing a bulk field from boundary data on a timelike hypersurface. If the bulk only supports propagating modes, reconstruction is complete. If the bulk also supports evanescent modes, local reconstruction is not achievable unless one has exponential precision in knowledge of the boundary data. Without exponential precision, for a Minkowski bulk, one can reconstruct a spatially coarse-grained bulk field, but only out to a depth set by the coarse-graining scale. For an asymptotically AdS bulk, reconstruction is limited to a spatial coarse-graining proper distance set by the AdS scale. AdS black holes admit evanescent modes. We study the resolution bound in the large AdS black hole background and provide a dual CFT interpretation. Our results demonstrate that, if there is a black hole of any size in the bulk, then sub-AdS bulk locality is no longer well-encoded in boundary data in terms of local CFT operators. Specifically, in order to probe the bulk on sub-AdS scales using only boundary data in terms of local operators, one must either have such data to exponential precision or make further assumptions about the bulk state.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 We establish resolution bounds on reconstructing a bulk field from boundary data on a timelike hypersurface. contribution 0.92 0.93 0.11 asserted 1.00
s1 If the bulk only supports propagating modes, reconstruction is complete. result 1.00 0.71 0.05 asserted 1.00
s2 If the bulk also supports evanescent modes, local reconstruction is not achievable unless one has exponential precision in knowledge of the boundary data. result 0.99 0.68 0.17 asserted 0.99
s3 Without exponential precision, for a Minkowski bulk, one can reconstruct a spatially coarse-grained bulk field, but only out to a depth set by the coarse-graining scale. result 0.99 0.77 0.06 asserted 0.72
s4 For an asymptotically AdS bulk, reconstruction is limited to a spatial coarse-graining proper distance set by the AdS scale. result 0.99 0.76 0.09 asserted 1.00
s5 AdS black holes admit evanescent modes. background 0.66 0.26 0.03 asserted 1.00
s6 We study the resolution bound in the large AdS black hole background and provide a dual CFT interpretation. contribution 1.00 0.93 0.06 asserted 0.84
s7 Our results demonstrate that, if there is a black hole of any size in the bulk, then sub-AdS bulk locality is no longer well-encoded in boundary data in terms of local CFT operators. result 0.57 0.85 0.86 asserted 1.00
s8 Specifically, in order to probe the bulk on sub-AdS scales using only boundary data in terms of local operators, one must either have such data to exponential precision or make further assumptions about the bulk state. result 0.53 0.77 0.39 asserted 0.98

What kind of paper the classifier reports this is: theoretical result 1.00 · evidence from proof or derivation 0.98.

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Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

The paper
Original abstract

We establish resolution bounds on reconstructing a bulk field from boundary data on a timelike hypersurface. If the bulk only supports propagating modes, reconstruction is complete. If the bulk also supports evanescent modes, local reconstruction is not achievable unless one has exponential precision in knowledge of the boundary data. Without exponential precision, for a Minkowski bulk, one can reconstruct a spatially coarse-grained bulk field, but only out to a depth set by the coarse-graining scale. For an asymptotically AdS bulk, reconstruction is limited to a spatial coarse-graining proper distance set by the AdS scale. AdS black holes admit evanescent modes. We study the resolution bound in the large AdS black hole background and provide a dual CFT interpretation. Our results demonstrate that, if there is a black hole of any size in the bulk, then sub-AdS bulk locality is no longer well-encoded in boundary data in terms of local CFT operators. Specifically, in order to probe the bulk on sub-AdS scales using only boundary data in terms of local operators, one must either have such data to exponential precision or make further assumptions about the bulk state.

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References
How the literature uses it

21 arXiv papers cite this in 39 sentences

Each citing sentence is taken from the citing paper's LaTeX source and typed by Pith's classifier. A label appears at probability 0.8 or more (0.95 for support), a contest at 0.7 or more; the quoted words are the citing authors'. How each label was checked · JSON

Papers citing it · 28 sentences without a confident label

Contests it 1 paper
  • It was immediately realized, however, that in fact this expression for $K$ is not well-defined [ref] (see also [ref] ); the reason is that from Stirling's formula it is straightforward to see that at large $λ$ we have |N_ωλ|^2∼e^-π√(λ).

    Bulk Locality and Quantum Error Correction in AdS/CFT · More details on AdS-Rindler reconstruction · contest 0.83

Uses its method or tool 1 paper
  • Following [ref] we consider a minimally coupled scalar field $Φ$ on a static spherically symmetric geometry described by the line element [equation] The Klein-Gordon equation in this background can be solved by separation of variables, $Φ(t,Ω,r)=e^-iωtY(Ω)ϕ(r)$, and with $d$ denoting the spatial dimension, the radial equation takes the form [equation] which is conveniently rewritten by replacing $ϕ(r)=u(r)/r^d-1/2$ and using “tortoise” coordinates, $r_*=r/f$: [equation] where the effective potential $V$ is given by [equation] The advantage of these coordinates is that we recognise the form of the radial time-independent Schrödinger equation, and can invoke our intuition about its solutions.

    Quenched coupling, entangled equilibria, and correlated composite operators: a tale of two O(N) models · Effective potential for scalar waves around black holes · 0.91

Compares with it 3 papers
Cites it as support 1 paper
Cites it as background 4 papers
  • Wave propagation in an AdS black hole background in standard gravity theory includes so called evanescent modes with an exponential fall-off towards the boundary whose existence is tied to the event horizon in the bulk spacetime geometry [ref] .

    Black holes from large N singlet models · Evanescent modes · 0.93

  • We also give some relevant properties of this spacetime such as the presence of “evanescent” modes [ref] whose CFT reconstruction will be of particular interest.

    Thermofield Duality for Higher Spin Rindler Gravity · Introduction · 0.88

  • For example, there has been some debate in the literature on highly spacelike modes [ref] where the ratio of value of the mode function near the horizon to its value at the boundary can vary exponentially with temperature.

    Comments on the Necessity and Implications of State-Dependence in the Black Hole Interior · A state-independent mini-superspace bulk-boundary map outside the horizon · 0.83

What it cites · 12 sentences without a confident label

Cites as background 13 papers

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