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A moving mirror in AdS space as a toy model for holographic thermalization

High Energy Physics - Theory · Submitted 28 Jan 2011

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

The authors' main claim We test our method on two sample trajectories for the mirror, and find that the singularity structure of the two-point functions is in agreement with geometric optics.

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arXiv ID1101.5505 (version 2)
Pith IDCAADWWMB, Pith's permanent record of this paper and its review
CitationJohanna Erdmenger, Shu Lin, Thanh Hai Ngo. "A moving mirror in AdS space as a toy model for holographic thermalization." arXiv:1101.5505 (2011). https://pith.science/paper/CAADWWMB
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What the abstract itself states, as probabilities: claims first 0.04 · states limitation 0.36 · human participants 0.01 · controlled comparison 0.04 · randomized assignment 0.01 · states quantitative result 0.05 · compares with prior results 0.28 · mentions code or data availability 0.02.

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

It is expected that thermalization may be described within gauge/gravity duality by considering time-dependent configurations on the gravity side of the correspondence, for instance a gravitational collapse of a matter configuration in Anti-de Sitter space. As a step towards the ambitious goal of describing such a configuration, we investigate a simple time-dependent toy model in which a mirror moves in the radial direction of Anti-de Sitter space. For this configuration, we establish a procedure for calculating two-point functions of scalar fluctuations, based on a WKB approximation. We test our method on two sample trajectories for the mirror, and find that the singularity structure of the two-point functions is in agreement with geometric optics.

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 It is expected that thermalization may be described within gauge/gravity duality by considering time-dependent configurations on the gravity side of the correspondence, for instance a gravitational collapse of a matter configuration in Anti-de Sitter space. background 1.00 0.04 0.04 hedged possibility 1.00
s1 As a step towards the ambitious goal of describing such a configuration, we investigate a simple time-dependent toy model in which a mirror moves in the radial direction of Anti-de Sitter space. contribution 0.82 0.86 0.05 asserted 0.88
s2 For this configuration, we establish a procedure for calculating two-point functions of scalar fluctuations, based on a WKB approximation. method 0.98 0.96 0.06 asserted 1.00
s3 We test our method on two sample trajectories for the mirror, and find that the singularity structure of the two-point functions is in agreement with geometric optics. result 1.00 0.97 0.43 asserted 1.00

What kind of paper the classifier reports this is: theoretical result 0.61 · evidence from proof or derivation 0.95.

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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

It is expected that thermalization may be described within gauge/gravity duality by considering time-dependent configurations on the gravity side of the correspondence, for instance a gravitational collapse of a matter configuration in Anti-de Sitter space. As a step towards the ambitious goal of describing such a configuration, we investigate a simple time-dependent toy model in which a mirror moves in the radial direction of Anti-de Sitter space. For this configuration, we establish a procedure for calculating two-point functions of scalar fluctuations, based on a WKB approximation. We test our method on two sample trajectories for the mirror, and find that the singularity structure of the two-point functions is in agreement with geometric optics.

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References
How the literature uses it

10 arXiv papers cite this in 21 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 · 12 sentences without a confident label

Builds on it 1 paper
Uses its method or tool 1 paper
  • Similar to the appendix of [ref] , we have: G_LO(t<t')=A_1/at'^-d+1/2\(t/u_0\)^d-1/2 e^iπb(d-1)/2a\(2iπ/a\)^cΦ(e^2iπb/a,-c,d-1/4), with $a=lnu_0+1/u_0-1, b=lnt/t'+lnu_0-1/u_0, c=d+1/2$. $Φ$ is the Lerch transcendent function.

    Time singularities of correlators from Dirichlet conditions in AdS/CFT · Explicit evaluations of the correlators: scaling trajectory · 0.97

Cites it as background 6 papers
  • First, we will analyze the non-equilibrium evolution and equilibration of the spectral density, $ρ(Q)$, which has been studied in non-equilibrium contexts by several groups [ref] .

    Heavy ions and string theory · Non-equilibrium two-point functions · 0.93

  • Much effort is devoted to such problems in connection with, for example, application of the AdS/CFT correspondence to QCD physics like that in the RHIC experiment, or to nonequilibrium phenomena in condensed matter physics and fluid dynamics [ref] .

    Hawking temperature for near-equilibrium black holes · Introduction · 0.93

  • The effect of a dynamical boundary condition has also been studied in the background of a moving mirror [ref] .

    Holographic Thermalization · Thermalization scenarios · 0.92

What it cites · 20 sentences without a confident label

Builds on 4 papers
Uses the method or tool of 3 papers
  • We will follow [ref] for the computation of the two point correlator[Note a subtlety involved in this procedure is elaborated in [ref] , but this does not affect our result for the massless scalar.].

    Anti De Sitter Space And Holography · Derivation of the correlator · 1.00

  • We will follow [ref] for the computation of the two point correlator[Note a subtlety involved in this procedure is elaborated in [ref] , but this does not affect our result for the massless scalar.].

    Correlation functions in the CFT(d)/AdS(d+1) correpondence · Derivation of the correlator · 1.00

  • We focus on the UV part of the correlator following the work by Amado and Hoyos [ref] .

    AdS black holes as reflecting cavities · Different limits of the correlator · 0.89

Compares with 4 papers
  • It should be stressed that while the authors of [ref] use a static mirror in $$ which introduces an explicit scale to the boundary CFT, our mirror moves in such a way that scale invariance of the boundary CFT is still preserved.

    AdS black holes as reflecting cavities · Different limits of the correlator · 0.92

  • Finally, let us compare our results for two-point functions of a massless scalar field with light-like separation to previous discussions of space-like separation, for instance those of [ref] .

    Holographic Evolution of Entanglement Entropy · Conclusion · 1.00

  • Finally, let us compare our results for two-point functions of a massless scalar field with light-like separation to previous discussions of space-like separation, for instance those of [ref] .

    AdS Dynamics from Conformal Field Theory · Conclusion · 1.00

Cites as background 19 papers

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