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Higher Spin Realization of the dS/CFT Correspondence

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19 Pith papers citing it
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abstract

We conjecture that Vasiliev's theory of higher spin gravity in four-dimensional de Sitter space (dS) is holographically dual to a three-dimensional conformal field theory (CFT) living on the spacelike boundary of dS at future timelike infinity. The CFT is the Euclidean Sp(N) vector model with anticommuting scalars. The free CFT flows under a double-trace deformation to an interacting CFT in the IR. We argue that both CFTs are dual to Vasiliev dS gravity but with different future boundary conditions on the bulk scalar field. Our analysis rests heavily on analytic continuations of bulk and boundary correlators in the proposed duality relating the O(N) model with Vasiliev gravity in AdS.

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representative citing papers

Replica wormholes and the black hole interior

hep-th · 2019-11-27 · conditional · novelty 9.0

Replica wormhole geometries justify the replica trick computation of the Page curve in holographic black hole models and support entanglement wedge reconstruction via the Petz map.

Worldline Higher Spin Gravity

hep-th · 2026-05-27 · unverdicted · novelty 8.0

A worldline path integral model for higher-spin gravity in AdS4 is constructed using twistor actions and double-line vertices, reproducing boundary correlators of free boson and fermion vector models.

dS$^4$ Metamorphosis

hep-th · 2026-02-23 · conditional · novelty 7.0

Higher spin gravity path integral on S^4 glues to an Sp(N) or superconformal S^3 boundary theory, giving leading contribution 2^N with one-loop cancellations.

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.

An observer's quantization of 3d de Sitter

hep-th · 2026-06-24 · unverdicted · novelty 6.0

Proposes an SL(2,Z) sum of Kerr-lens geometries in 3d dS gravity whose spectral density is computed via crosscap amplitudes in CLS ⊗ CLS, matching semi-classical predictions and reducing in a simple case to GΣ ⊗ GΣ on the observer worldline.

Exact and Finite de Sitter QFT from CFT

hep-th · 2026-06-23 · unverdicted · novelty 6.0

Constructs exact finite de Sitter QFT from CFT data using moduli space of oriented balls and Casimir completion of operators.

No boundary density matrix in elliptic de Sitter dS/$\mathbb{Z}_2$

hep-th · 2025-11-30 · unverdicted · novelty 6.0

The Euclidean path integral on elliptic de Sitter defines a no-boundary density matrix whose entropies reduce to vertex operator correlators on non-orientable surfaces, with a one-dimensional global Hilbert space but nontrivial observer Fock spaces.

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.

CFT Dual for Timelike Geodesic in Lorentzian dS

hep-th · 2026-06-27 · unverdicted · novelty 5.0

Analytic continuation produces a PT-invariant CFT state reproducing the Bunch-Davies Wightman function for dS, but entanglement entropy captures only real central charge, motivating a timelike geodesic-integrated dual for OPE block correlators and conformal defects from dS/CFT symmetry.

3d QFT IR divergences as UV divergences in 4d Holographic Cosmology

hep-th · 2026-05-15 · unverdicted · novelty 4.0

In a 3d toy model for holographic cosmology, a mass term preserving generalized conformal structure permits 2-loop computations that indicate possible IR finiteness beyond perturbation theory, corresponding to UV finiteness without singularities in the 4d dual.

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.

Dark energy from string theory: an introductory review

hep-th · 2026-03-26 · unverdicted · novelty 2.0

String theory imposes constraints on dark energy but permits various construction attempts for de Sitter vacua and single-field exponential quintessence models despite obstructions.

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Showing 5 of 5 citing papers after filters.

  • Horizon Edge Partition Functions in $\Lambda>0$ Quantum Gravity hep-th · 2026-03-21 · unverdicted · none · ref 90 · internal anchor

    Horizon edge mode spectra in de Sitter and Nariai spacetimes exhibit universal shift symmetries that produce novel symmetry breaking in one-loop partition functions.

  • An observer's quantization of 3d de Sitter hep-th · 2026-06-24 · unverdicted · none · ref 30 · internal anchor

    Proposes an SL(2,Z) sum of Kerr-lens geometries in 3d dS gravity whose spectral density is computed via crosscap amplitudes in CLS ⊗ CLS, matching semi-classical predictions and reducing in a simple case to GΣ ⊗ GΣ on the observer worldline.

  • Deforming the Double-Scaled SYK & Reaching the Stretched Horizon From Finite Cutoff Holography hep-th · 2026-02-05 · unverdicted · none · ref 232 · internal anchor

    Deformations of the double-scaled SYK model via finite-cutoff holography produce Krylov complexity as wormhole length and realize Susskind's stretched horizon proposal through targeted T² deformations in the high-energy spectrum.

  • On bulk reconstruction in Lorentzian AdS and its flat space limit hep-th · 2026-05-15 · unverdicted · none · ref 14 · internal anchor

    Constructs bulk scalar field representations in Lorentzian AdS4 from boundary primaries via time-ordered propagators and derives their flat-space limits to plane-wave or Carrollian bases.

  • Dark energy from string theory: an introductory review hep-th · 2026-03-26 · unverdicted · none · ref 125 · internal anchor

    String theory imposes constraints on dark energy but permits various construction attempts for de Sitter vacua and single-field exponential quintessence models despite obstructions.