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The asymptotic dynamics of three-dimensional Einstein gravity with a negative cosmological constant

6 Pith papers cite this work. Polarity classification is still indexing.

6 Pith papers citing it
abstract

Liouville theory is shown to describe the asymptotic dynamics of three-dimensional Einstein gravity with a negative cosmological constant. This is because (i) Chern-Simons theory with a gauge group $SL(2,R) \times SL(2,R)$ on a space-time with a cylindrical boundary is equivalent to the non-chiral $SL(2,R)$ WZW model; and (ii) the anti-de Sitter boundary conditions implement the constraints that reduce the WZW model to the Liouville theory.

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hep-th 6

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2026 5 2025 1

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UNVERDICTED 6

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The Super Virasoro Minimal String from 3d Supergravity

hep-th · 2026-04-28 · unverdicted · novelty 8.0

The super Virasoro minimal string arises from quantizing 3d supergravity, with 0A+ and 0B+ dual to the bosonic minimal string matrix integral, 0B- to one with inverse square root singularity, and 0A- having vanishing non-trivial perturbative amplitudes.

Timelike Liouville theory and AdS$_3$ gravity at finite cutoff

hep-th · 2025-08-05 · unverdicted · novelty 6.0

Proposes that AdS3 gravity at finite cutoff is dual to a CFT2 coupled to timelike Liouville theory deformed by a marginal operator, with checks via semiclassical partition functions and EOM matching.

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  • Timelike Liouville theory and AdS$_3$ gravity at finite cutoff hep-th · 2025-08-05 · unverdicted · none · ref 72 · internal anchor

    Proposes that AdS3 gravity at finite cutoff is dual to a CFT2 coupled to timelike Liouville theory deformed by a marginal operator, with checks via semiclassical partition functions and EOM matching.