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Thin versus Thick Scrambling: Operational Reachability under the Maldacena–Shenker–Stanford Bound

Doug Doucette

Published Jul 25, 2026• 0 citations
Publisher

Abstract

This paper examines the mathematical relationship between the Maldacena–Shenker–Stanford (MSS) bound on the growth of chaos and the thin–thick chaos framework developed in recent work on coherent disorder and nonlinear stability. The MSS bound constrains the rate at which a regularized out-of-time-order correlator can deviate from its factorized value, yielding a universal speed limit on information scrambling in thermal quantum systems: the Lyapunov exponent satisfies λL≤2π/βλL≤2π/β, and the scrambling time is t∗=(β/2π)log⁡(1/ε)t∗=(β/2π)log(1/ε), where ε∼1/N2ε∼1/N2 is the microscopic initial amplitude. We introduce a thinness index Θ(t)Θ(t) constructed directly from the correlator deviation and show that, under the analyticity and boundedness hypotheses of the MSS argument, Θ(t)Θ(t) remains parametrically small until times of order the scrambling time. The same analytic strip that yields the Lyapunov bound therefore also controls the rate at which this particular thinness index can collapse. When the additional structural hypotheses of the Trojan Universality Class—spectral gap, two-mode normal form, and near-integrable remainder—are imposed, the prefactor of the exponential growth of Θ(t)Θ(t) is suppressed by a factor η(Δ)≤1η(Δ)≤1, delaying the onset of thickness by a logarithmic shift without altering the scrambling rate itself. The analysis reveals a conceptual distinction between scrambling, the microscopic spread of quantum information, and the transition to thick chaos, the operational crossing of a failure threshold in a chosen projection. For the correlator projection these coincide in time, but structural gaps can decouple them, allowing maximal-rate scrambling to coexist with prolonged operational thinness. Limitations include projection dependence, the restrictive nature of the Trojan criteria, and the absence of a general comparison theorem relating distinct thinness indices. The results are elementary consequences of the existing MSS hypotheses and do not modify the original bound.

DOI
10.5281/zenodo.21543041

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This paper examines the mathematical relationship between the Maldacena–Shenker–Stanford (MSS) bound on the growth of chaos and the thin–thick chaos framework developed in recent work on coherent disorder and nonlinear stability. The MSS bound constrains the rate at which a regularized out-of-time-order correlator can deviate from its factorized value, yielding a universal speed limit on information scrambling in thermal quantum systems: the Lyapunov exponent satisfies λL≤2π/βλL≤2π/β, and the scrambling time is t∗=(β/2π)log⁡(1/ε)t∗=(β/2π)log(1/ε), where ε∼1/N2ε∼1/N2 is the microscopic initial amplitude. We introduce a thinness index Θ(t)Θ(t) constructed directly from the correlator deviation and show that, under the analyticity and boundedness hypotheses of the MSS argument, Θ(t)Θ(t) remains parametrically small until times of order the scrambling time. The same analytic strip that yields the Lyapunov bound therefore also controls the rate at which this particular thinness index can collapse. When the additional structural hypotheses of the Trojan Universality Class—spectral gap, two-mode normal form, and near-integrable remainder—are imposed, the prefactor of the exponential growth of Θ(t)Θ(t) is suppressed by a factor η(Δ)≤1η(Δ)≤1, delaying the onset of thickness by a logarithmic shift without altering the scrambling rate itself. The analysis reveals a conceptual distinction between scrambling, the microscopic spread of quantum information, and the transition to thick chaos, the operational crossing of a failure threshold in a chosen projection. For the correlator projection these coincide in time, but structural gaps can decouple them, allowing maximal-rate scrambling to coexist with prolonged operational thinness. Limitations include projection dependence, the restrictive nature of the Trojan criteria, and the absence of a general comparison theorem relating distinct thinness indices. The results are elementary consequences of the existing MSS hypotheses and do not modify the original bound.
This paper investigates whether gravitational dynamics can be classified into distinct universality classes based on the architecture of chaos, rather than viewing black holes as a monolithic category. The authors build on the Maldacena-Shenker-Stanford (MSS) chaos bound, which establishes that black holes saturate the universal limit on information scrambling, making them maximally chaotic with a quantum Lyapunov exponent λ_L = 2πT. The paper proposes a fundamental reclassification. The Thick Chaos Universality Class comprises systems that saturate the MSS bound—these are the familiar black holes of Einstein gravity with dense, continuous spectra and immediate, complete transport of local instabilities. Their scrambling time is short: t_* ~ β log S. The Thin Chaos Universality Class is a mathematically coherent but hypothetical regime, defined by the structural conditions of the Trojan Universality Class (TUC): two dominant oscillatory modes, a persistent spectral gap Δ > 0, and near-integrability. In this class, the spectral gap suppresses transport, confining local instability and preventing it from acquiring operational reach. The central mathematical result is that the Thouless time—the timescale on which chaos becomes effective—scales exponentially with the spectral gap in the Thin Chaos Class: t_Th ~ (1/Δ)exp[(Δ/ε)^α], where ε is the perturbation strength. This establishes a rigorous distinction between the two classes: Thick Chaos has a short Thouless time; Thin Chaos delays chaos for exponentially long periods. The transition between classes occurs when Δ/ε ~ 1, marking the collapse of spectral protection—a genuine phase transition rather than a smooth interpolation. The paper translates these gravitational conditions into holographic terms: a CFT with a spectral gap and large Thouless time would be the signature of the Thin Chaos Class. The authors are transparent that the Thin Chaos Class may not be realized in nature. The results are theoretical and conditional on TUC assumptions, but they provide a precise mathematical language for describing what a non-maximal black hole would look like—a work of theoretical cartography that illuminates why maximal chaos is the rule by defining the mathematically possible exception.
Abstract Chaos, in quantum systems, can be diagnosed by certain out-of-time-order correlators (OTOCs) that obey the chaos bound of Maldacena, Shenker, and Stanford (MSS). We begin by deriving a dispersion relation for this class of OTOCs, implying that they must satisfy many more constraints beyond the MSS bound. Motivated by this observation, we perform a systematic analysis obtaining an infinite set of constraints on the OTOC. This infinite set includes the MSS bound as the leading constraint. In addition, it also contains subleading bounds that are highly constraining, especially when the MSS bound is saturated by the leading term. These new bounds, among other things, imply that the MSS bound cannot be exactly saturated over any duration of time, however short. Furthermore, we derive a sharp bound on the Lyapunov exponent λ2 ≤ 6πβ \frac{6\pi }{\beta } β6π​ 6 π β of the subleading correction to maximal chaos.
Out-of-Time-Ordered Commutators (OTOCs), representing a key diagnostic for scrambling as a facet of short-time quantum chaos, have attracted wide-ranging interest, from many-body physics to quantum gravity. By means of a suitable form of the Wigner-Moyal expansion, and invoking ensemble equivalence in statistical physics, we provide a consistent approach to the growth rate of the OTOC for many-body systems with chaotic classical limit where both the classical Lyapunov exponent and the quantum nature of the density of states enter. Applying this construction to quantized high-dimensional hyperbolic motion, i.e., a quantum chaotic system that exhibits gravity-like correlation functions in the late-time regime, we compute the OTOC growth rate ΛΛΛ as a function of the number of degrees of freedom, fff, and inverse temperature, βββ. We show that the scaled growth rate, Λ/fΛ/fΛ/f, can be described by a universal function of fβf βfβ and displays a cross-over from classical to quantum behavior as we increase fff and/or lower the temperature. In the deep quantum regime of infinite fff, we find maximally fast scrambling in the sense of the Maldacena-Shenker-Stanford bound on chaos. This elucidates the non-perturbative mechanism underlying the saturation of the bound via quantum contributions to the mean density of states, and it provides further support for this dynamical system as a dual to two-dimensional quantum gravity. In this way, we present first evidence of maximally fast scrambling in a quantum chaotic system with a well-defined classical Hamiltonian limit, without invoking any external mechanism such as (disorder) averaging.
PROBING THE MSS BOUND AND SCRAMBLING DYNAMICS IN A MINIMAL 3-QUBIT SYSTEM ABSTRACT:This study investigates the fundamental limits of quantum chaos—the Maldacena-Shenker-Stanford (MSS) bound—using a minimal 3-qubit non-integrable system[cite: 82, 87]. By prioritizing measurement precision (16,384 shots) over system size on the IBM Quantum Torino processor, I resolve the complete "scrambling life-cycle," including the chaotic burst and the finite-size recurrence of quantum complexity[cite: 89, 91]. The extracted intrinsic Lyapunov exponent (1.30 +/- 0.05) satisfies the MSS bound in the infinite-temperature limit[cite: 90]. These results demonstrate that minimal quantum hardware can probe deep holographic principles and provide a high-precision benchmark for quantum gravity simulations[cite: 92]. KEY SCIENTIFIC ADVANCES:- Intrinsic Lyapunov Extraction: Utilized non-linear data collapse and bootstrap analysis to isolate the scrambling rate from finite-size effects[cite: 138, 140].- Observation of Unitary Recurrence: Resolved the late-time revival of information fidelity at t=3, a hallmark of unitary dynamics in finite Hilbert spaces[cite: 131, 132].- MSS Bound Verification: Defined an effective scrambling temperature scale to confirm adherence to the universal chaos bound[cite: 147, 148]. REPOSITORY CONTENTS:1. Manuscript & SI: Complete text and detailed quantum circuit sequences.2. Raw Experimental Data: Execution counts (shots) from the IBM Quantum Torino processor[cite: 64, 118].3. Analysis Scripts: Python scripts for data collapse fitting and Lyapunov exponent extraction[cite: 64, 139]. NOTE:This work serves as the foundational technical benchmark for larger-scale holographic simulations on NISQ devices[cite: 160].
Quantum scrambling often gives rise to short-time exponential growth in out-of-time-ordered correlators. The scrambling rate over an isolated saddle point at finite temperature is shown here to be reduced by a hierarchy of quenching processes. Two of these appear in the classical limit, where escape from the neighborhood of the saddle reduces the rate by a factor of two, and thermal fluctuations around the saddle reduce it further; a third process can be explained semiclassically as arising from quantum thermal fluctuations around the saddle, which are also responsible for imposing the Maldacena-Shenker-Stanford bound.
Quantum scrambling often gives rise to short-time exponential growth in out-of-time-ordered correlators (OTOCs). The scrambling rate over an isolated saddle point at finite temperature is shown here to be reduced by a hierarchy of quenching processes. Two of these appear in the classical limit, where escape from the neighbourhood of the saddle reduces the rate by a factor of two, and thermal fluctuations around the saddle reduce it further; a third process can be explained semiclassically as arising from quantum thermal fluctuations around the saddle, which are also responsible for imposing the Maldacena-Shenker-Stanford bound.