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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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The abstract, sentence by sentence
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
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| 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 |
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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.
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References
How the literature uses it
10 arXiv papers cite this in 11 sentences
Papers citing it · 6 sentences without a confident label
Uses its method or tool 2 papers
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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
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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
Compares with it 1 paper
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This formulation is reminiscent of an analogous formulation for Euclidean quantum gravity defined through DT [ref] .
Causal random geometry from stochastic quantization · Conclusion · 0.99
Cites it as background 2 papers
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The relation between the string field theory of DT and the matrix model was also discussed in [ref] .
Dynamical Triangulations for 2D Pure Gravity and Topological Recursion · Introduction · 0.91
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Large $N$ multi-matrix problems are at the center of many theories of current interest, involving membranes [ref] , reduced super Yang-Mills theories [ref] , field theory of critical and noncritical strings [ref] , phase transitions and black holes [ref] , and M-atrix theory [ref] .
Large N Optimization for multi-matrix systems · Introduction · 0.99
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