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3D near-de Sitter gravity and the soft mode of DSSYK

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5 Pith papers citing it
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abstract

We present a dual gravity interpretation of the complex reparametrization mode $\psi(u)$ that governs the soft dynamics of double-scaled SYK in the presence of a time-dependent Maldacena-Qi coupling. We find that the dual gravity system takes the form of 2+1-dimensional Einstein-de Sitter gravity with an energy distribution localized on a dS$_2$ slice within dS$_3$. The effective SYK equations of motion take the form of the Israel junction conditions across the dS$_2$ slice. We study the 1D effective action of the SYK soft mode and show that it coincides with the effective action derived from 3D Einstein-de Sitter gravity with conformal boundary conditions on $\mathscr{I}^\pm$. The boundary conditions split $\mathscr{I}^\pm$ into two hyperbolic $k=-1$ slices, and the holographic screen is placed at the intersection. We adapt the Gibbons-Hawking calculation of the Schwarzschild-de Sitter entropy to the case with $k=-1$ boundary conditions and find that it reproduces the semiclassical DSSYK entropy. The boundary-to-boundary Green functions in 3D de Sitter are equal to the square of DSSYK two-point functions. We give an alternative holographic interpretation of our results in terms of 3D AdS gravity with two time directions.

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hep-th 5

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2026 5

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representative citing papers

Generalized Free Fields in de Sitter from 1D CFT

hep-th · 2026-05-04 · unverdicted · novelty 7.0

Pairs of large-N 1D CFTs encode generalized free fields on a timelike geodesic in de Sitter space via large-N factorization, 1D conformal symmetry, and split representations of dS Green 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.

Undulating Conformal Boundaries in 3D Gravity

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

Inhomogeneous torus boundaries in 3D gravity are thermodynamically favourable for AdS in the range 2 < K |Λ|^{-1/2} < 3/√2 and support macroscopic entropy for all Λ.

Baby Universe in a Coupled SYK Model

hep-th · 2026-05-06 · unverdicted · novelty 6.0

A saddle point in the coupled SYK model yields a bulk geometry with a baby universe whose chord-diagram Hilbert space state is entangled with the exterior, giving evidence that closed universes can carry nontrivial quantum information.

citing papers explorer

Showing 5 of 5 citing papers.

  • Generalized Free Fields in de Sitter from 1D CFT hep-th · 2026-05-04 · unverdicted · none · ref 34 · internal anchor

    Pairs of large-N 1D CFTs encode generalized free fields on a timelike geodesic in de Sitter space via large-N factorization, 1D conformal symmetry, and split representations of dS Green functions.

  • An observer's quantization of 3d de Sitter hep-th · 2026-06-24 · unverdicted · none · ref 49 · 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.

  • Undulating Conformal Boundaries in 3D Gravity hep-th · 2026-05-08 · unverdicted · none · ref 25 · internal anchor

    Inhomogeneous torus boundaries in 3D gravity are thermodynamically favourable for AdS in the range 2 < K |Λ|^{-1/2} < 3/√2 and support macroscopic entropy for all Λ.

  • Baby Universe in a Coupled SYK Model hep-th · 2026-05-06 · unverdicted · none · ref 12 · internal anchor

    A saddle point in the coupled SYK model yields a bulk geometry with a baby universe whose chord-diagram Hilbert space state is entangled with the exterior, giving evidence that closed universes can carry nontrivial quantum information.

  • q-Askey Deformations of Double-Scaled SYK hep-th · 2026-05-13 · unreviewed · ref 34 · 2 links · internal anchor