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Loop Space Hamiltonians And Field Theory Of Non-Critical Strings

High Energy Physics - Theory · Submitted 14 Dec 1993

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

The authors' main claim We demonstrate how collective field theory with its loop space interactions generates a field theory of non-critical strings.

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arXiv IDhep-th/9312118 (version 2)
Pith IDFXAJ3T2A, Pith's permanent record of this paper and its review
CitationA. Jevicki, J. Rodrigues. "Loop Space Hamiltonians And Field Theory Of Non-Critical Strings." arXiv:hep-th/9312118 (1993). https://pith.science/paper/FXAJ3T2A
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Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 2,844 input tokens, $0.0001 reported.

What the abstract itself states, as probabilities: claims first 0.04 · 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 0.51 · mentions code or data availability 0.01.

The abstract, sentence by sentence

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

We consider the loop space representation of multi-matrix models. Explaining the origin of a time variable through stochastic quantization we make contact with recent proposals of Ishibashi and Kawai. We demonstrate how collective field theory with its loop space interactions generates a field theory of non-critical strings.

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 consider the loop space representation of multi-matrix models. contribution 0.70 0.68 0.06 asserted 0.70
s1 Explaining the origin of a time variable through stochastic quantization we make contact with recent proposals of Ishibashi and Kawai. contribution 0.53 0.82 0.07 asserted 0.98
s2 We demonstrate how collective field theory with its loop space interactions generates a field theory of non-critical strings. result 0.60 0.91 0.76 asserted 1.00

What kind of paper the classifier reports this is: theoretical result 0.99 · evidence from proof or derivation 0.94.

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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 consider the loop space representation of multi-matrix models. Explaining the origin of a time variable through stochastic quantization we make contact with recent proposals of Ishibashi and Kawai. We demonstrate how collective field theory with its loop space interactions generates a field theory of non-critical strings.

Human review
References
How the literature uses it

10 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 · 6 sentences without a confident label

Uses its method or tool 2 papers
  • A straight forward way to determine this Jacobian [ref] is by requiring that the Schwinger-Dyson equations derived in the original $ϕ^a(x^μ)$ variables agree with those derived using the $σ(x_1^μ,x_2^μ)$ variables[The set of gauge invariant variables that defines the collective field must be chosen large enough that the invariants appearing in the Schwinger-Dyson equations all belong to the set.].

    Gravitational dynamics from collective field theory · Collective Field Theory · 0.87

  • Therefore it is quite easy to develop the Fokker-Planck formalism [ref] for string fields using which we can compute the off-shell amplitudes $A_g,n^I_1⋯I_n$.

    Strebel differentials and string field theory · The Fokker-Planck formalism · 0.84

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Cites it as background 2 papers

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