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Bounding the Space of Holographic CFTs with Chaos

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

6 Pith papers citing it
abstract

Thermal states of quantum systems with many degrees of freedom are subject to a bound on the rate of onset of chaos, including a bound on the Lyapunov exponent, $\lambda_L\leq 2\pi /\beta$. We harness this bound to constrain the space of putative holographic CFTs and their would-be dual theories of AdS gravity. First, by studying out-of-time-order four-point functions, we discuss how $\lambda_L=2\pi/\beta$ in ordinary two-dimensional holographic CFTs is related to properties of the OPE at strong coupling. We then rule out the existence of unitary, sparse two-dimensional CFTs with large central charge and a set of higher spin currents of bounded spin; this implies the inconsistency of weakly coupled AdS$_3$ higher spin gravities without infinite towers of gauge fields, such as the $SL(N)$ theories. This fits naturally with the structure of higher-dimensional gravity, where finite towers of higher spin fields lead to acausality. On the other hand, unitary CFTs with classical $W_{\infty}[\lambda]$ symmetry, dual to 3D Vasiliev or hs[$\lambda$] higher spin gravities, do not violate the chaos bound, instead exhibiting no chaos: $\lambda_L=0$. Independently, we show that such theories violate unitarity for $|\lambda|>2$. These results encourage a tensionless string theory interpretation of the 3D Vasiliev theory. We also perform some CFT calculations of chaos in Rindler space in various dimensions.

citation-role summary

background 2 method 1

citation-polarity summary

years

2026 3 2025 3

verdicts

UNVERDICTED 6

representative citing papers

Entanglement Revivals and Scrambling for Evaporating Black Holes

hep-th · 2026-04-29 · unverdicted · novelty 7.0 · 2 refs

Increasing black hole scrambling time in JT and RST evaporating geometries suppresses and eliminates late-time entanglement revivals in 2d CFT mutual information for disjoint intervals, interpolating between quasiparticle and maximal scrambling regimes.

Searching for emergent spacetime in spin glasses

hep-th · 2025-10-23 · unverdicted · novelty 6.0

Spectral functions of SYK, p-spin, and SU(M) Heisenberg models show exponential tails in spin-glass phases and quasiparticle families in spin-liquid phases, with a proof that exponential decay blocks detection of bulk causal structure.

Quantum chaos and the holographic principle

quant-ph · 2026-04-14 · unverdicted · novelty 1.0

A review of the chaos-assisted holographic correspondence linking the SYK model to 2D JT gravity, including the need for string theory corrections at fine quantum scales.

citing papers explorer

Showing 6 of 6 citing papers.

  • Entanglement Revivals and Scrambling for Evaporating Black Holes hep-th · 2026-04-29 · unverdicted · none · ref 17 · 2 links · internal anchor

    Increasing black hole scrambling time in JT and RST evaporating geometries suppresses and eliminates late-time entanglement revivals in 2d CFT mutual information for disjoint intervals, interpolating between quasiparticle and maximal scrambling regimes.

  • Probing Evaporating Black Holes with Modular Flow in SYK hep-th · 2025-12-03 · unverdicted · none · ref 43 · internal anchor

    Modular flow in SYK models coupled to a bath reveals singularities allowing reconstruction of bulk flow past the horizon in two-sided AdS2 black holes.

  • Violation of Universal Operator Growth Hypothesis in $\mathcal{W}_3$Conformal Field Theories hep-th · 2025-06-02 · unverdicted · none · ref 23 · internal anchor

    In W3 CFTs, Lanczos coefficients b_N grow as N^2 for generalized Liouvillian with W generators, violating the universal linear growth bound and causing divergent Krylov complexity, with the same quadratic growth in the SL(3,R) subalgebra.

  • Butterflies in $\textrm{T}\overline{\textrm{T}}$ deformed anomalous CFT$_2$ hep-th · 2026-05-12 · unverdicted · none · ref 83 · internal anchor

    In TTbar-deformed anomalous CFT2 the chaos bound stays saturated while butterfly velocity depends nontrivially on deformation strength and anomaly, with a Hagedorn regime where the chaotic response turns complex.

  • Searching for emergent spacetime in spin glasses hep-th · 2025-10-23 · unverdicted · none · ref 62 · internal anchor

    Spectral functions of SYK, p-spin, and SU(M) Heisenberg models show exponential tails in spin-glass phases and quasiparticle families in spin-liquid phases, with a proof that exponential decay blocks detection of bulk causal structure.

  • Quantum chaos and the holographic principle quant-ph · 2026-04-14 · unverdicted · none · ref 114

    A review of the chaos-assisted holographic correspondence linking the SYK model to 2D JT gravity, including the need for string theory corrections at fine quantum scales.