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Holography and String Dynamics in Time-dependent Backgrounds

High Energy Physics - Theory · Submitted 19 Aug 2002

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

The authors' main claim This provides a concrete example of holography in a cosmological setting.

how it is stated · asserted 1.00 read the record →

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arXiv IDhep-th/0208126 (version 2)
Pith IDOWVKYGJG, Pith's permanent record of this paper and its review
CitationAkikazu Hashimoto, Savdeep Sethi. "Holography and String Dynamics in Time-dependent Backgrounds." arXiv:hep-th/0208126 (2002). https://pith.science/paper/OWVKYGJG
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The compiled record

The paper's own sentences, arranged. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.

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Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 3,438 input tokens, $0.0001 reported.

What the abstract itself states, as probabilities: claims first 0.05 · states limitation 0.05 · human participants 0.01 · controlled comparison 0.01 · randomized assignment 0.01 · states quantitative result 0.03 · compares with prior results 0.05 · mentions code or data availability 0.02.

The abstract, sentence by sentence

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

We study the dynamics of D-branes in a smooth time-dependent background. The theory on the branes is a time-dependent non-commutative field theory. We find the metric and fluxes that determine the dual holographic closed string theory. This provides a concrete example of holography in a cosmological setting.

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 study the dynamics of D-branes in a smooth time-dependent background. contribution 0.98 0.90 0.05 asserted 0.94
s1 The theory on the branes is a time-dependent non-commutative field theory. result 0.50 0.22 0.09 asserted 1.00
s2 We find the metric and fluxes that determine the dual holographic closed string theory. result 0.72 0.95 0.21 asserted 1.00
s3 This provides a concrete example of holography in a cosmological setting. interpretation 1.00 0.64 0.52 asserted 1.00

What kind of paper the classifier reports this is: theoretical result 1.00 · evidence from proof or derivation 0.99.

What was examined, and what was not

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not examined
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  • P abstract
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  • S sections
  • T body sentences
  • C citations
  • R cross-paper relations

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 study the dynamics of D-branes in a smooth time-dependent background. The theory on the branes is a time-dependent non-commutative field theory. We find the metric and fluxes that determine the dual holographic closed string theory. This provides a concrete example of holography in a cosmological setting.

Human review
References
How the literature uses it

6 arXiv papers cite this in 11 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 · 8 sentences without a confident label

Builds on it 1 paper
Cites it as support 1 paper
Cites it as background 1 paper
  • Melvin twists, in a context of D-branes and their near horizon limits, can be used to formulate wide variety of exotic field theories, including non-commutative gauge theories [ref] , NCOS theories [ref] , dipole theories [ref] , and $β$ deformed superconformal theories [ref] .

    Microscopic Formulation of Puff Field Theory · Introduction · 0.81

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