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Quantum Gravity Partition Functions in Three Dimensions

Canonical reference. 100% of citing Pith papers cite this work as background.

15 Pith papers citing it
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abstract

We consider pure three-dimensional quantum gravity with a negative cosmological constant. The sum of known contributions to the partition function from classical geometries can be computed exactly, including quantum corrections. However, the result is not physically sensible, and if the model does exist, there are some additional contributions. One possibility is that the theory may have long strings and a continuous spectrum. Another possibility is that complex geometries need to be included, possibly leading to a holomorphically factorized partition function. We analyze the subleading corrections to the Bekenstein-Hawking entropy and show that these can be correctly reproduced in such a holomorphically factorized theory. We also consider the Hawking-Page phase transition between a thermal gas and a black hole and show that it is a phase transition of Lee-Yang type, associated with a condensation of zeros in the complex temperature plane. Finally, we analyze pure three-dimensional supergravity, with similar results.

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representative citing papers

A solvable model of 3d quantum gravity

hep-th · 2026-05-12 · unverdicted · novelty 7.0

A solvable 3d quantum gravity model is defined by summing Virasoro TQFT copies over all topologies, shown to be dual to a 2d CFT ensemble and to exhibit semiclassical features such as cured negative density of states and Hawking-Page transition in the large-c limit.

M\"obius randomness in the Hartle-Hawking state

hep-th · 2025-05-05 · unverdicted · novelty 7.0

The Hartle-Hawking state for toroidal quantum cosmologies is expressed in the Langlands decomposition as a sum over zeta zeros whose near-singularity dynamics follow the Hilbert-Pólya Hamiltonian and as a Möbius average of CFT partition functions.

On random matrix statistics of 3d gravity

hep-th · 2025-12-04 · unverdicted · novelty 6.0

3d gravity on Σ_{g,n} × I with EOW branes equals the Virasoro minimal string random matrix model, with exact match for g=0 n=2 and inner-product formulation for negative Euler characteristic.

Surgery and statistics in 3d gravity

hep-th · 2025-06-04 · unverdicted · novelty 6.0

Introduces RMT surgery to relate off-shell 3D gravity partition functions to CFT spectral statistics via Euclidean wormholes with four-punctured sphere and trumpet boundaries.

Inner Horizon Saddles and a Spectral KSW Criterion

hep-th · 2026-05-08 · unverdicted · novelty 6.0

Inner horizon saddles supply the semiclassical correction -exp(A_inner/4G) to near-extremal black-hole entropy and motivate a spectral KSW criterion for well-defined one-loop effects around complex gravitational saddles.

Spinning States and Unitarity in 3D Gravity

hep-th · 2026-04-16 · unverdicted · novelty 6.0

Spinning states scaled with central charge cancel negative densities in 3D gravity, reinterpreted as bulk defects or overspinning BTZ quotients of AdS3 that preserve the gap but exhibit causal pathologies.

Euclidean volume fluctuations in de Sitter quantum gravity

hep-th · 2026-04-28 · unverdicted · novelty 4.0 · 2 refs

From the de Sitter partition function in various approximations, the volume probability distribution concentrates around the classical value but shifts to favor smaller universes as quantum effects increase.

citing papers explorer

Showing 15 of 15 citing papers.

  • A solvable model of 3d quantum gravity hep-th · 2026-05-12 · unverdicted · none · ref 6 · internal anchor

    A solvable 3d quantum gravity model is defined by summing Virasoro TQFT copies over all topologies, shown to be dual to a 2d CFT ensemble and to exhibit semiclassical features such as cured negative density of states and Hawking-Page transition in the large-c limit.

  • Mind the crosscap: $\tau$-scaling in non-orientable gravity and time-reversal-invariant systems hep-th · 2025-09-24 · unverdicted · none · ref 11 · internal anchor

    Non-orientable topological gravity produces a resummed topological expansion whose late-time behavior matches the GOE universality class of random matrix theory for time-reversal invariant chaotic systems.

  • M\"obius randomness in the Hartle-Hawking state hep-th · 2025-05-05 · unverdicted · none · ref 49 · internal anchor

    The Hartle-Hawking state for toroidal quantum cosmologies is expressed in the Langlands decomposition as a sum over zeta zeros whose near-singularity dynamics follow the Hilbert-Pólya Hamiltonian and as a Möbius average of CFT partition functions.

  • Dimensional reduction of AdS3 Chern-Simons gravity: Schwarzian and affine boundary theories hep-th · 2026-05-14 · unverdicted · none · ref 29 · internal anchor

    Symmetry reduction of 3D AdS Chern-Simons gravity on toroidal boundary yields two inequivalent 1D boundary theories: standard Schwarzian and affine-deformed Schwarzian with Kac-Moody extensions.

  • How to tame your (black hole) saddles: Lessons from the Lorentzian Gravitational Path Integral hep-th · 2026-03-25 · accept · none · ref 55 · internal anchor

    A Lorentzian path integral contour for charged AdS black holes selects a finite subset of complex saddles via Picard-Lefschetz theory, ensuring the semiclassical sum converges at finite β.

  • On random matrix statistics of 3d gravity hep-th · 2025-12-04 · unverdicted · none · ref 60 · internal anchor

    3d gravity on Σ_{g,n} × I with EOW branes equals the Virasoro minimal string random matrix model, with exact match for g=0 n=2 and inner-product formulation for negative Euler characteristic.

  • Surgery and statistics in 3d gravity hep-th · 2025-06-04 · unverdicted · none · ref 26 · internal anchor

    Introduces RMT surgery to relate off-shell 3D gravity partition functions to CFT spectral statistics via Euclidean wormholes with four-punctured sphere and trumpet boundaries.

  • AdS3 axion wormholes as stable contributions to the Euclidean gravitational path integral hep-th · 2025-04-15 · unverdicted · none · ref 31 · internal anchor

    The paper shows that Euclidean axion wormholes remain regular and stable in AdS3 for any mouth radius to AdS radius ratio and across topologies, with computable actions that can be included in the 3D gravitational path integral.

  • Inner Horizon Saddles and a Spectral KSW Criterion hep-th · 2026-05-08 · unverdicted · none · ref 80

    Inner horizon saddles supply the semiclassical correction -exp(A_inner/4G) to near-extremal black-hole entropy and motivate a spectral KSW criterion for well-defined one-loop effects around complex gravitational saddles.

  • Spinning States and Unitarity in 3D Gravity hep-th · 2026-04-16 · unverdicted · none · ref 15

    Spinning states scaled with central charge cancel negative densities in 3D gravity, reinterpreted as bulk defects or overspinning BTZ quotients of AdS3 that preserve the gap but exhibit causal pathologies.

  • Finite cutoff JT gravity: Baby universes, Matrix dual, and (Krylov) Complexity hep-th · 2025-02-18 · unverdicted · none · ref 6 · internal anchor

    Finite cutoff in JT gravity causes faster ERB-length saturation, deformation-dependent baby-universe emission only under Lorentzian evolution, and possible one-cut universality corrections in the matrix dual.

  • Algebraic Realisation of the Zamolodchikov Metric in Narain Theories hep-th · 2024-12-18 · unverdicted · none · ref 53 · internal anchor

    The Zamolodchikov metric in Narain CFTs is realized using the Cartan matrix K_g and its inverse from finite-dimensional Lie algebras g.

  • The many facets of a hyperbolic tetrahedron: open and closed triangulations of 3d gravity hep-th · 2026-04-10 · unverdicted · none · ref 19

    Open Virasoro TQFT computes 3d gravity path integrals on compact regions using threshold-dependent boundary conditions and yields an open-closed duality relating Conformal Turaev-Viro theory to the diagonal sector of two Virasoro TQFT copies.

  • Euclidean volume fluctuations in de Sitter quantum gravity hep-th · 2026-04-28 · unverdicted · none · ref 17 · 2 links

    From the de Sitter partition function in various approximations, the volume probability distribution concentrates around the classical value but shifts to favor smaller universes as quantum effects increase.

  • Lecture notes on strings in AdS$_3$ from the worldsheet and the AdS$_3$/CFT$_2$ duality hep-th · 2026-01-10 · unverdicted · none · ref 224 · internal anchor

    Lecture notes deliver a self-contained pedagogical overview of worldsheet strings in AdS3 with NSNS flux, summarizing 25 years of results with emphasis on spectrally flowed correlation functions.