The complex Liouville string: The gravitational path integral

We give a rigorous definition of sine dilaton gravity in terms of the worldsheet theory of the complex Liouville string [S. Collier et al., Phys. Rev. Lett. 134, 251602 (2025)]. The latter has a known exact solution that we leverage to explore the gravitational path integral of sine dilaton gravity – a quantum deformation of dS JT gravity that admits both AdS _2 <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:msub> <mml:mi/> <mml:mn>2</mml:mn> </mml:msub> </mml:math> and dS _2 <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:msub> <mml:mi/> <mml:mn>2</mml:mn> </mml:msub> </mml:math> vacua. We uncover that the gravitational path integral receives contributions from new saddles describing transitions between vacua in a third-quantized picture. We also discuss the sphere and disk partition function in this context and contrast our findings with other recent work on this theory.

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Publication Details

Journal
SciPost Physics
Published
2025-10-28
DOI
https://doi.org/10.21468/scipostphys.19.4.115
Citations
5
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
9.35
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article

The complex Liouville string: The gravitational path integral

Beatrix Mühlmann, Lorenz Eberhardt, Scott Collier
5 citations
SciPost Physics
Black Holes and Theoretical Physics
9.35
article

The complex Liouville string: The gravitational path integral

Beatrix Mühlmann, Lorenz Eberhardt, Scott Collier
article en
5 citations

Abstract

We give a rigorous definition of sine dilaton gravity in terms of the worldsheet theory of the complex Liouville string [S. Collier et al., Phys. Rev. Lett. 134, 251602 (2025)]. The latter has a known exact solution that we leverage to explore the gravitational path integral of sine dilaton gravity – a quantum deformation of dS JT gravity that admits both AdS _2 <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:msub> <mml:mi/> <mml:mn>2</mml:mn> </mml:msub> </mml:math> and dS _2 <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:msub> <mml:mi/> <mml:mn>2</mml:mn> </mml:msub> </mml:math> vacua. We uncover that the gravitational path integral receives contributions from new saddles describing transitions between vacua in a third-quantized picture. We also discuss the sphere and disk partition function in this context and contrast our findings with other recent work on this theory.

SciPost PhysicsVol. 19(4)
Delta Institute for Theoretical Physics (NL), Massachusetts Institute of Technology (US)
Openalex Percentile: Top 2%
Black Holes and Theoretical Physics
9.35
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