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Correlators in Timelike Bulk Liouville Theory
High Energy Physics - Theory · Submitted 25 Mar 2003
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim The expression agrees exactly with the minisuperspace result for the closed string pair-production rate (which diverges at finite time).
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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The abstract, sentence by sentence
Liouville theory with a negative norm boson and no screening charge corresponds to an exact classical solution of closed bosonic string theory describing time-dependent bulk tachyon condensation. A simple expression for the two point function is proposed based on renormalization/analytic continuation of the known results for the ordinary (positive-norm) Liouville theory. The expression agrees exactly with the minisuperspace result for the closed string pair-production rate (which diverges at finite time). Puzzles concerning the three-point function are presented and discussed.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | Liouville theory with a negative norm boson and no screening charge corresponds to an exact classical solution of closed bosonic string theory describing time-dependent bulk tachyon condensation. | background 0.68 | 0.22 | 0.25 | asserted 1.00 |
| s1 | A simple expression for the two point function is proposed based on renormalization/analytic continuation of the known results for the ordinary (positive-norm) Liouville theory. | contribution 0.58 | 0.86 | 0.15 | asserted 0.44 |
| s2 | The expression agrees exactly with the minisuperspace result for the closed string pair-production rate (which diverges at finite time). | result 0.99 | 0.80 | 0.33 | asserted 1.00 |
| s3 | Puzzles concerning the three-point function are presented and discussed. | contribution 0.49 | 0.80 | 0.04 | unclear 0.53 |
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The paper
Original abstract
Liouville theory with a negative norm boson and no screening charge corresponds to an exact classical solution of closed bosonic string theory describing time-dependent bulk tachyon condensation. A simple expression for the two point function is proposed based on renormalization/analytic continuation of the known results for the ordinary (positive-norm) Liouville theory. The expression agrees exactly with the minisuperspace result for the closed string pair-production rate (which diverges at finite time). Puzzles concerning the three-point function are presented and discussed.
Human review
References
How the literature uses it
17 arXiv papers cite this in 27 sentences
Papers citing it · 17 sentences without a confident label
Contests it 1 paper
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Earlier works [ref] missed these possibilities by working directly with wave functions analytically continued from the spacelike theory.
Quantum Gravity from Timelike Liouville theory · Comments on the minisuperspace approximation · contest 0.81
Compares with it 1 paper
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This result makes a sharp contrast with the open and closed string creation in the rolling tachyon backgrounds [ref] , where the string creation rate diverges.
Decaying D-branes and Moving Mirrors · D-brane Interpretation and Moving Mirror · 1.00
Cites it as support 1 paper
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If one attempts to define it via the analytic continuation of the Euclidean Liouville with $ϕ=iX^0$ and $β$ purely imaginary then one can show that it does not satisfy all axioms of CFT [ref] (certain 3-pt functions do not reduce to 2-pt functions upon insertion of the identity operator as one of the 3 operators).
A Short Review of Time Dependent Solutions and Space-like Singularities in String Theory · Tachyon condensation · 0.99
Cites it as background 6 papers
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Consider string theory cosmological backgrounds based on worldsheet CFTs of the form (see e.g. [ref] [ref] [ref] [ref] [ref] [ref] [ref] [ref] [ref] ): [equation] A nice feature of such models is that the combined central charge of the two $SL(2,R)/U(1)$ factors is independent of $|k|$, and so this can be taken to be an independent, varying parameter.
A Wave-function for Stringy Universes · Liouville type models · 0.96
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The status of the Liouville theory with imaginary Liouville exponent, or time-like signature Liouville theory, which can be obtained after a further rotation of the field space $ϕ→iT$ to make the action real, is not as well-established as in the usual space-like case (see e.g. [ref] [ref] [ref] [ref] [ref] ).
Eternal Inflation with Liouville Cosmology · Universe as holographic Liouville theory · 0.99
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Moreover, the kinetic term for the Weyl compensator is negative or `timelike', so the Weyl compensator is related to the Liouville field by a subtle analytic continuation which is not yet fully understood in the quantum theory [ref] .
Quantum Cosmology Near Two Dimensions · Introduction · 0.83
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