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REVIEW 4 major objections 3 minor 2 cited by

Pole-skipping organizes into Regge-like trajectories that carry the quantum Lyapunov exponent in generic chaotic systems, with stringy horizons staying sharp for each mode.

Reviewed by Pith at T0; open to challenge. T0 means a machine referee read the full paper against a public rubric. the ladder, T0–T4 →

T0 review · deepseek-v4-flash

2026-08-03 14:20 UTC pith:FN7VJO7R

load-bearing objection The Rindler spin-J pole-skipping formula is a real result, but the SYK-chain verification of the central conjecture fails arithmetically as written. the 4 major comments →

arxiv 2512.20700 v2 pith:FN7VJO7R submitted 2025-12-23 hep-th gr-qcquant-ph

Probing Stringy Horizons with Pole-Skipping in Non-Maximal Chaotic Systems

classification hep-th gr-qcquant-ph
keywords pole-skippingquantum chaosLyapunov exponentRegge trajectoriesRindler CFTSYK chainstringy horizonsholography
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved

The pith

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

This paper argues that pole-skipping—the special complex frequencies where lines of poles and zeros in a thermal retarded correlator intersect—is a universal feature of quantum chaotic systems, not just of maximally chaotic ones. In non-maximally chaotic systems, the pole-skipping points of few-body operators are claimed to organize into trajectories in the complex frequency–momentum plane, and the leading trajectory's intercept gives the quantum Lyapunov exponent. In holographic settings, these trajectories are identified with the Regge trajectories of stringy excitations around a black hole horizon, so each string mode sees a sharp horizon even though the summed string spectrum may look fuzzy. The paper demonstrates this in two solvable examples—a Rindler CFT and the large-q SYK chain—and conjectures that it holds for general finite-temperature stringy black holes.

Core claim

In a Rindler CFT (a CFT on R^{1,d-1} restricted to the Rindler wedge, equivalent to a thermal CFT on R × H^{d-1}), the retarded two-point function of a spin-J primary of dimension Δ has pole-skipping points at (ω,k)_p.s. = (i(J−2n−1−s), i(Δ−d/2−s)) for n≤J and (i(−n−1−s), i(Δ−d/2+n−J−s)) for n≥J, plus the k→−k reflected family. The highest point for each operator sits at i(J−1, Δ−d/2), exactly on that operator's Regge trajectory. Since Regge trajectories in the (J, Δ) plane can be reconstructed from these points, the leading trajectory—and hence the non-maximal Lyapunov exponent λ = j_leading(0)−1—is determined by the collective pole-skipping data. The paper argues the same organization hold

What carries the argument

Pole-skipping points are intersections of pole lines and zero lines of a retarded Green's function in the complex frequency–momentum plane. In the Rindler CFT, the explicit Fourier transform of the conformal two-point function—with the spin-J hypergeometric polynomial—yields the full pole-skipping lattice; in the SYK chain, the effective large-q action gives two universal families. The bridge is Regge trajectories: analytic continuation in spin of the dimensions of exchanged operators. The central identity is Eq. (4): the highest pole-skipping point of a spin-J operator equals i(J−1, Δ−d/2), placing it on the Regge trajectory, so the leading trajectory's intercept λ is read off from pole-ski

Load-bearing premise

The paper assumes that the pole-skipping–Regge-trajectory correspondence proven in the vacuum Rindler CFT, and illustrated in the large-q SYK chain, continues to hold for interacting finite-temperature theories dual to stringy black holes; Section III states no such bridge is currently available there and the transfer is made by conjecture, with the SYK universality claim deferred to a companion paper.

What would settle it

Compute the full pole-skipping spectrum of a finite-temperature, finite-coupling holographic theory (or any non-maximally chaotic model) beyond the Rindler and SYK examples, and check whether the highest pole-skipping points at imaginary Matsubara frequencies lie on a single leading curve whose intercept equals the independently computed Lyapunov exponent. If the highest points scatter without a common envelope, or the envelope intercept differs from λ, the central conjecture fails. For the SYK chain specifically, the companion paper's universality claim can be tested by computing pole-skippin

Watch this falsifier — get emailed when new claim-graph text bears on it.

If this is right

  • Pole-skipping can be used to extract the quantum Lyapunov exponent in systems that do not saturate the chaos bound, where the energy-density pole-skipping point alone carries no information about λ.
  • The full set of pole-skipping points over all operators encodes the Regge data of the theory; individual operators' pole-skipping points are fragments of this global structure.
  • The stringy horizon remains sharp for each bulk string mode: every higher-spin field has a well-defined pole-skipping point tied to a horizon symmetry, while the non-maximal Lyapunov exponent emerges only from the collective sum of all modes.
  • In the SYK chain, the leading pole-skipping trajectory reproduces the momentum-dependent Lyapunov exponent, giving a concrete non-conformal, non-spin example of the proposed organization.
  • Composite-operator correlators (time-ordered four-point functions) can reveal universal pole-skipping data without knowing the operator spectrum in advance.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • If the conjecture generalizes, pole-skipping could serve as a practical probe of quantum chaos in numerical simulations: scanning a retarded correlator's pole-zero crossings in the complex plane is often easier than direct OTOC measurement.
  • The paper's picture suggests 'horizon fuzziness' is an observable-dependent statement: single-string-mode probes see a sharp horizon and its symmetries; fuzziness appears only in sums over the Hagedorn tower. That distinction might be testable in toy stringy models by comparing single-mode versus summed correlators.
  • One might test the proposal in other solvable non-maximally chaotic models, e.g., SYK-like chains with different coupling patterns or low-dimensional non-conformal field theories, by checking whether upper envelopes of pole-skipping families always match independently computed Lyapunov exponents.
  • The exceptional pole-skipping points found in the composite-operator analysis of the Rindler CFT (off the Matsubara frequencies) may correspond to nonlocal intermediate operators; understanding them could sharpen the correspondence between pole-skipping and Regge trajectories.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit.

Referee Report

4 major / 3 minor

Summary. Using Rindler CFT and the large-q SYK chain as examples, the paper argues that pole-skipping points of few-body operators in non-maximally chaotic systems form trajectories in the complex (omega,k) plane, and that the leading trajectory encodes the quantum Lyapunov exponent. In Rindler CFT it derives Eq. (3) for a spin-J primary, whose highest pole-skipping point (4) lies at i(J-1, Delta-d/2), on the operator's Regge trajectory, leading to the relation lambda = j_leading(0)-1 in Eq. (7). The paper then conjectures that in stringy black holes these trajectories coincide with Regge trajectories of bulk string excitations and that the horizon remains sharp for each mode. The same trajectory picture is claimed to be verified in the large-q SYK chain, where a leading trajectory (10) is asserted to be saturated by pole-skipping points.

Significance. The Rindler calculation is substantial, analytically explicit, and internally coherent; if correct, it provides a rare solvable handle on higher-spin pole-skipping and a clean conformal-field-theory derivation of the Regge/Lyapunov dictionary. The proposed reinterpretation of pole-skipping as tracking individual stringy modes is thought-provoking. However, the paper's only explicit non-conformal test of conjecture 1 is marred by an arithmetic inconsistency, and the completeness of the SYK pole-skipping set is delegated to an unpublished companion. These issues must be resolved before the broad claims can be accepted.

major comments (4)
  1. [IV, Eqs. (8)-(10)] Equation (8) and the saturation claim around Eq. (9) are inconsistent. For odd n, (8) gives h = n/lambda0 + 3/2 + 2k, so the upper bound in (9) is lambda0(h-1) = n + lambda0(1/2 + 2k) > n = Im(omega). For even n, h = n/lambda0 + 5/2 + 2k, so lambda0(h-2) = n + lambda0(1/2 + 2k) > n. Thus no point of family (8) saturates the bounds, contradicting the statement that each upper bound is saturated by infinitely many pole-skipping points. Consequently the identification of (10) as an envelope actually populated by pole-skipping points is unsupported. In addition, the n=1, k=0 point has h = 1/lambda0 + 3/2, which cannot equal h(0)=2 for lambda0 <= 1, so the claimed relation to the standard pole-skipping point (1) is not evident. Unless Eq. (8) or Eq. (9) contains a typo, the only explicit verification of conjecture 1 fails as written.
  2. [IV, around Eq. (11) and Ref. [42]] The identification of families (8) and (11) as the complete universal set of pole-skipping points for bilinear operators of the SYK chain is essential for the leading-trajectory claim, since other families could change the upper envelope. This completeness is stated to be proved in the unpublished companion [42]. The reader cannot check this load-bearing point from the present manuscript. The authors should either include the argument or clearly mark the completeness as a conjecture rather than a proved input.
  3. [II and S-I.B] The derivation of Eq. (3) deliberately keeps only zero lines coming from individual gamma functions and discards 'sporadic' pole-skipping points arising from linear combinations of terms, with the statement that these are non-universal. No systematic criterion is given for this separation. Since the conclusion that pole-skipping data reconstruct Regge trajectories is a statement about the full retarded correlator, the treatment of these extra points should be made precise. Otherwise the trajectory claim applies only to a hand-picked subset of pole-skipping points, which weakens the claimed universality.
  4. [III] The passage from the Rindler vacuum result to a finite-temperature, finite-coupling CFT on R x S^{d-1} is made by conjecture; the text explicitly states that the Regge bridge 'does not appear to be available' and then conjectures that items 1-4 apply to a stringy black hole horizon. The central assertion about generic non-maximally chaotic systems therefore rests on an unproven assumption. The paper should either soften the language or supply a concrete test, such as a near-horizon computation for a higher-spin string field or a finite-temperature conformal-block analysis, to make the conjectural step more controlled.
minor comments (3)
  1. [IV, Eq. (8)] The notation '(-)^n /2' is ambiguous. It should be written as (-1)^n/2, and the resulting odd/even expressions for h should be displayed explicitly to avoid the confusion that arises in the saturation check.
  2. [FIG. 2] The figure caption states that the blue and yellow curves are the two bounds in (9) and shows the pole-skipping points together with those curves. If, as the arithmetic in the main text indicates, no point saturates the bounds, the figure should be redrawn or annotated to make the actual relation between the points and the curves clear.
  3. [IV, text below Eq. (10)] The statement that the special point n=1, k=0 corresponds to the pole-skipping point (1) 'related to the maximal Lyapunov exponent' requires a derivation. From Eq. (8) this point has h = 1/lambda0 + 3/2, and it is not immediate how this maps to the energy-density pole-skipping point, especially since lambda0 < 1.

Circularity Check

2 steps flagged

SYK 'leading trajectory' recovers λ0 by construction, and the claimed universality of the pole-skipping families is deferred to an unpublished self-citation; the Rindler derivation itself is independent.

specific steps
  1. self definitional [Section IV, Eqs. (8)-(10)]
    "(ω, h(p))p.s. = (in, n/λ0 + 1 + (−)n/2 + 2k+ 1) (8) ... We thus identify the first line of (9) as giving the leading trajectory jleading(p) = (h(p)−1)λ0 + 1, which indeed recovers the Lyapunov exponent with jleading(0)−1 = λ0 (h(0) = 2). The large-qSYK chain thus verifies beautifully the conjecture 1."

    The 'leading trajectory' (10) is literally the first line of (9), an inequality obtained by algebra from (8), and (8) already contains λ0 as an explicit parameter. Substituting h(0)=2 into (10) gives jleading(0)-1=λ0 by definition, so 'recovering/extracting the Lyapunov exponent' is a rearrangement of the input, not an independent prediction. Moreover, by the paper's own formula no point of (8) saturates (9): for odd n, λ0(h-1)=n+λ0(1/2+2k)>n, and for even n, λ0(h-2)=n+λ0(1/2+2k)>n. Thus the claimed saturation is not realized, and the curve (10) is imposed using the already-known λ0 from (S72) rather than being an envelope of actual pole-skipping points.

  2. uniqueness imported from authors [Section IV, paragraph before Eq. (8)]
    "In [42], we show that the two families identified in [26] (shown in FIG. 2 and described below) are the only ones that are universal and independent of the specific choice of composite operator. They can therefore be identified with the full universal set of pole-skipping points associated with bilinear operators."

    The SYK verification of conjecture 1 depends on (8) and (11) being the complete universal set of pole-skipping points for bilinear operators. That uniqueness claim is not derived here but delegated to [42], an unpublished companion by the same authors. No external or machine-checkable support is given. If another family of pole-skipping points existed, the 'leading trajectory' (10) need not be the actual leading curve, so the central SYK test would be unsupported. This is a load-bearing self-citation rather than an independent mathematical fact.

full rationale

The Rindler-CFT part is not circular: Eq. (3)/(4) is obtained in S-I by Fourier-transforming the conformal two-point function (2), with no Lyapunov data as input, and Eq. (7) is standard conformal Regge theory supported by external references. The independent content of the paper rests there. The SYK chain section, however, contains a circular 'verification': Eq. (8) already contains λ0 as a parameter, and Eq. (10) is just the first line of (9), an algebraic inequality derived from (8). Therefore jleading(0)-1=λ0 follows by substitution (h(0)=2), so 'extracting the Lyapunov exponent from the TOC' is a rearrangement of the input. There is also an arithmetic tension, noted in the step above, that no point of (8) saturates (9), making the assignment of (10) as the envelope even more clearly an a priori choice using the known λ0. Finally, the universality of the two families (8),(11) is delegated to the authors' unpublished companion [42]; this self-citation is load-bearing for the SYK test. Since the central Rindler result is independent and the stringy-horizon generalization is explicitly conjectural, the circularity is partial rather than total: the claimed SYK verification reduces by construction, while the Rindler/Regge bridge retains independent content.

Axiom & Free-Parameter Ledger

0 free parameters · 6 axioms · 0 invented entities

The Rindler computation uses only conformal kinematics and standard pole/zero analysis; no parameter is fitted. In the SYK section, λ0 and η are physical model parameters from [26], not ad hoc fits. The conjectural extensions to stringy black holes and the unpublished universality claim in [42] are the main additional inputs. No new particles, forces, dimensions, or conserved quantities are postulated.

axioms (6)
  • domain assumption Lyapunov exponent of Rindler CFT is given by λ = j_leading(0) − 1 (Eq. 7), where j_leading is the analytic continuation of the leading Regge trajectory.
    Invoked in Section II after Eq. (4) to connect pole-skipping points to the Lyapunov exponent; standard conformal Regge theory, not re-derived here.
  • domain assumption Rindler wedge vacuum of a CFT is equivalent to a thermal state on R×H^{d−1} at inverse temperature β=2π.
    Used throughout Section II to treat vacuum two-point functions as thermal correlators and to define pole-skipping; standard Unruh/Rindler correspondence.
  • ad hoc to paper In the large-q SYK chain, the pole-skipping families (8) and (11) from [26] are the universal pole-skipping points of bilinear operators.
    Section IV and S-II: universality is deferred to the authors' unpublished companion [42]; without it, the SYK trajectory extraction lacks support.
  • ad hoc to paper The results for the Rindler CFT extend to a stringy black hole horizon: each bulk stringy field has pole-skipping at (4) and the set reconstructs bulk Regge trajectories.
    Section III states this as a conjecture ('we conjecture that the statements in items 1-4 above apply to a stringy black hole horizon as well'), not a derivation.
  • domain assumption Regge limit of CFT four-point functions maps to high-energy AdS scattering across the Rindler horizon; stringy Regge trajectories determine the non-maximal Lyapunov exponent.
    Section III, items 1-4 and surrounding text; relies on cited literature (e.g. [34,35,38]).
  • domain assumption The two-point function of a composite operator (S30) has pole-skipping points that reduce to those of the intermediate operators exchanged in the four-point function, up to ad hoc contributions.
    Section S-II A; this is the bridge used to extract universal pole-skipping data for bilinear operators in the SYK chain.

pith-pipeline@v1.3.0-alltime-deepseek · 28655 in / 21318 out tokens · 190034 ms · 2026-08-03T14:20:18.622242+00:00 · methodology

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read the original abstract

In this paper, we study pole-skipping in non-maximally quantum chaotic systems. Using Rindler conformal field theories and the large-$q$ SYK chain as illustrative examples, we argue that the pole-skipping points of few-body operators organize into trajectories in the complex frequency-momentum plane, with the leading trajectory encoding the quantum Lyapunov exponent. We further propose that these trajectories admit a natural interpretation as Regge trajectories of stringy excitations in a dual stringy black hole geometry. From this perspective, pole-skipping for an individual operator can be viewed as tracking the stringy horizon through the response of a single excitation. Our results suggest that pole-skipping reflects intrinsic properties of quantum chaotic systems and may be deeply connected to the structure of horizons in the stringy regime.

Figures

Figures reproduced from arXiv: 2512.20700 by Hong Liu, Ping Gao.

Figure 1
Figure 1. Figure 1: FIG. 1. The overlay of Regge trajectories and the pole [PITH_FULL_IMAGE:figures/full_fig_p003_1.png] view at source ↗
Figure 2
Figure 2. Figure 2: FIG. 2. The pole-skipping points of the large [PITH_FULL_IMAGE:figures/full_fig_p005_2.png] view at source ↗

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Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. High-Order Pole-Skipping in Near-Extremal Holography

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    In near-extremal holographic black holes, the n-th order pole-skipping momentum with mode index q becomes order-independent as T→0: k²_{n,q} → −m²h(r_h) + ½q(q−1)h(r_h)f″(r_h), with q identified as the AdS2 IR conform...

  2. Probing bulk geometry via pole skipping: from static to rotating spacetimes

    gr-qc 2026-04 unverdicted novelty 7.0

    Pole-skipping data encodes enough information to reconstruct the full metric of 3D rotating black holes and the radial functions of 4D separable rotating black holes, with Einstein equations becoming algebraic constra...

Reference graph

Works this paper leans on

66 extracted references · 43 linked inside Pith · cited by 2 Pith papers

  1. [1]

    The highest pole-skipping points for eachJlies on the (ℑω,ℑk) plane at (ω, k)(highest) p.s. = i(J−1,∆−d/2).(4) For the stress tensor, withJ= 2 and ∆ =d, equa- tion (4) can be related to (1), corresponding to the theory onR 1,d−1 at finite temperature, where vB = 1/(d−1) by a shiftk→k+i(d/2−1) [26, 31]

  2. [2]

    All these pole-skipping points lie at the Matsubara frequencies (recallβ= 2πhere), ω= 2πi(J−n)/βwithn= 1,2,3,· · ·,(5) which agrees with the results of [18] for bulk higher- spin fields in AdS black holes. 4

  3. [3]

    ForJ= 1 andJ= 2, the first group contains one and three rows of pole-skipping points respec- tively, which are consistent with previous works [30, 31]

    For eachJ, writingω= imwithm≤J−1, we find that it is natural to separate the pole-skipping points for each operator into two families based on the numberN m of pole-skipping points for eachm Nm = ( 2 J−1−m 2 + 2−(J−1)≤m≤J−1 2|m|m≤ −J .(6) The second group was motivated from the result of a scalar operator in holographic systems [19] where the number of po...

  4. [4]

    field-dependent Lyapunov exponent

    From the conformal partial wave analysis, in the stringy regime, each higher-spin field still con- tributes individually to AdS Regge scattering with an exponentλ J =J−1. This “field-dependent Lyapunov exponent” is still captured by the high- est pole-skipping point of the field

  5. [5]

    The highest pole-skipping points of bulk stringy fields collectively trace out the Regge trajectories ofbulkstring excitations

  6. [6]

    In semiclassical gravity, it has been argued that for J= 2 (metric perturbations), the highest pole-skipping point (4) can be attributed to certain horizon symme- tries [12]

    The full analytic Regge trajectories of the bulk string theory can be reconstructed from the pole- skipping points via analytic continuation, includ- ing in particular the leading trajectoryj leading(µ)— which corresponds to the highest curve in the (ℑk,ℑω) plane—together with the associated non- maximal Lyapunov exponentλ. In semiclassical gravity, it ha...

  7. [7]

    descendants

    The horizon symmetries underlying pole-skipping persist into the stringy regime for each individual bulk field. At strong coupling, where the bulk dynamics is de- scribed by classical gravity—including both Einstein and higher-derivative theories—there is strong evidence that the pole-skipping frequenciesω= 2πi(J−n) β , n= 1,2,· · · for each bulk field de...

  8. [8]

    In a general non-maximally chaotic theory at a fi- nite temperature, the highest pole-skipping points at imaginary Matsubara frequencies align along certain trajectories, among which there is a leading trajectoryℑω=λ(k), whose interceptλ(0) gives the Lyapunov exponent

  9. [9]

    string-type

    For systems with a bulk stringy dual, the trajecto- ries of pole-skipping points correspond to the Regge trajectories of stringy excitations in the associated black hole geometry. This picture—that in the stringy regime, at leading or- der in theg s expansion (the free-string limit), the hori- zon remains sharp for each individual higher-spin bulk stringy...

  10. [10]

    Bohigas, M.J

    O. Bohigas, M.J. Giannoni and C. Schmit, Characterization of chaotic quantum spectra and universality of level fluctuation laws,Physical Review Letters52(1984) 1

  11. [11]

    Srednicki,Chaos and quantum thermalization,Phys

    M. Srednicki,Chaos and quantum thermalization,Phys. Rev. E50(1994) 888 [chao-dyn/9403051]

  12. [12]

    Shenker and D

    S.H. Shenker and D. Stanford,Black holes and the butterfly effect,JHEP03(2014) 067 [1306.0622]

  13. [13]

    Shenker and D

    S.H. Shenker and D. Stanford,Multiple Shocks,JHEP 12(2014) 046 [1312.3296]

  14. [14]

    Roberts, D

    D.A. Roberts, D. Stanford and L. Susskind,Localized shocks,JHEP03(2015) 051 [1409.8180]

  15. [15]

    Shenker and D

    S.H. Shenker and D. Stanford,Stringy effects in scrambling,JHEP05(2015) 132 [1412.6087]

  16. [16]

    Kitaev,Hidden correlations in the Hawking radiation and thermal noise,talk at KITP(2015)

    A. Kitaev,Hidden correlations in the Hawking radiation and thermal noise,talk at KITP(2015)

  17. [17]

    Roberts and D

    D.A. Roberts and D. Stanford,Two-dimensional conformal field theory and the butterfly effect,Phys. Rev. Lett.115(2015) 131603 [1412.5123]

  18. [18]

    Grozdanov, K

    S. Grozdanov, K. Schalm and V. Scopelliti,Black hole scrambling from hydrodynamics,Phys. Rev. Lett.120 (2018) 231601 [1710.00921]

  19. [19]

    Blake, H

    M. Blake, H. Lee and H. Liu,A quantum hydrodynamical description for scrambling and many-body chaos,JHEP10(2018) 127 [1801.00010]

  20. [20]

    Blake, R.A

    M. Blake, R.A. Davison, S. Grozdanov and H. Liu, Many-body chaos and energy dynamics in holography, JHEP10(2018) 035 [1809.01169]

  21. [21]

    Knysh, H

    M. Knysh, H. Liu and N. Pinzani-Fokeeva,New horizon symmetries, hydrodynamics, and quantum chaos,JHEP 09(2024) 162 [2405.17559]

  22. [22]

    Blake and H

    M.A. Blake and H. Liu,On systems of maximal quantum chaos,J. High Energy Phys.2021(2021) 229 7 [arXiv:2102.11294 [hep-th]]

  23. [23]

    Grozdanov,On the connection between hydrodynamics and quantum chaos in holographic theories with stringy corrections,JHEP01(2019) 048 [1811.09641]

    S. Grozdanov,On the connection between hydrodynamics and quantum chaos in holographic theories with stringy corrections,JHEP01(2019) 048 [1811.09641]

  24. [24]

    Natsuume and T

    M. Natsuume and T. Okamura,Nonuniqueness of Green ’s functions at special points,JHEP12(2019) 139 [1905.12015]

  25. [25]

    Wu,Higher curvature corrections to pole-skipping, JHEP12(2019) 140 [1909.10223]

    X. Wu,Higher curvature corrections to pole-skipping, JHEP12(2019) 140 [1909.10223]

  26. [26]

    Baishya and K

    B. Baishya and K. Nayek,Probing pole-skipping through scalar Gauss-Bonnet coupling,Nucl. Phys. B1001 (2024) 116521 [2301.03984]

  27. [27]

    Wang and Z.-Y

    D. Wang and Z.-Y. Wang,Pole Skipping in Holographic Theories with Bosonic Fields,Phys. Rev. Lett.129 (2022) 231603 [2208.01047]

  28. [28]

    Blake, R.A

    M. Blake, R.A. Davison and D. Vegh,Horizon constraints on holographic Green ’s functions,JHEP01 (2020) 077 [1904.12883]

  29. [29]

    Y. Ahn, V. Jahnke, H.-S. Jeong and K.-Y. Kim, Scrambling in Hyperbolic Black Holes: shock waves and pole-skipping,JHEP10(2019) 257 [1907.08030]

  30. [30]

    Blake and R.A

    M. Blake and R.A. Davison,Chaos and pole-skipping in rotating black holes,JHEP01(2022) 013 [2111.11093]

  31. [31]

    Grozdanov and M

    S. Grozdanov and M. Vrbica,Pole-skipping of gravitational waves in the backgrounds of four-dimensional massive black holes,Eur. Phys. J. C 83(2023) 1103 [2303.15921]

  32. [32]

    S. Ning, D. Wang and Z.-Y. Wang,Pole skipping in holographic theories with gauge and fermionic fields, JHEP12(2023) 084 [2308.08191]

  33. [33]

    Y. Ahn, V. Jahnke, H.-S. Jeong, C.-W. Ji, K.-Y. Kim and M. Nishida,On pole-skipping with gauge-invariant variables in holographic axion theories,JHEP06(2024) 020 [2402.12951]

  34. [34]

    W.Z. Chua, T. Hartman and W.W. Weng,Replica manifolds, pole skipping, and the butterfly effect, 2504.08139

  35. [35]

    C. Choi, M. Mezei and G. S´ arosi,Pole skipping away from maximal chaos,2010.08558

  36. [36]

    Gu, X.-L

    Y. Gu, X.-L. Qi and D. Stanford,Local criticality, diffusion and chaos in generalized Sachdev-Ye-Kitaev models,JHEP05(2017) 125 [1609.07832]

  37. [37]

    Perlmutter,Bounding the space of holographic cfts with chaos,JHEP10(2016) 069 [arXiv:1602.08272 [hep-th]]

    E. Perlmutter,Bounding the space of holographic cfts with chaos,JHEP10(2016) 069 [arXiv:1602.08272 [hep-th]]

  38. [38]

    Mezei and G

    M. Mezei and G. S´ arosi,Chaos in the butterfly cone, JHEP01(2020) 186 [1908.03574]

  39. [39]

    Y. Ahn, V. Jahnke, H.-S. Jeong, K.-Y. Kim, K.-S. Lee and M. Nishida,Pole-skipping of scalar and vector fields in hyperbolic space: conformal blocks and holography, JHEP09(2020) 111 [2006.00974]

  40. [40]

    Haehl, W

    F.M. Haehl, W. Reeves and M. Rozali, Reparametrization modes, shadow operators, and quantum chaos in higher-dimensional CFTs,JHEP11 (2019) 102 [1909.05847]

  41. [41]

    Homrich, D

    A. Homrich, D. Simmons-Duffin and P. Vieira, Multitwist Trajectories and Decoupling Zeros in Conformal Field Theory,Phys. Rev. Lett.134(2025) 011602 [2211.13754]

  42. [42]

    Henriksson, P

    J. Henriksson, P. Kravchuk and B. Oertel,Missing local operators, zeros, and twist-4 trajectories,JHEP07 (2024) 248 [2312.09283]

  43. [43]

    Penedones,Writing cft correlation functions as ads scattering amplitudes,J

    J. Penedones,Writing cft correlation functions as ads scattering amplitudes,J. High Energy Phys.03(2011) 025 [arXiv:1011.1485 [hep-th]]

  44. [44]

    Costa, V

    M.S. Costa, V. Goncalves and J. Penedones,Conformal Regge theory,JHEP12(2012) 091 [1209.4355]

  45. [45]

    Caron-Huot,Analyticity in Spin in Conformal Theories,JHEP09(2017) 078 [1703.00278]

    S. Caron-Huot,Analyticity in Spin in Conformal Theories,JHEP09(2017) 078 [1703.00278]

  46. [46]

    D. Li, D. Meltzer and D. Poland,Conformal bootstrap in the regge limit,J. High Energy Phys.02(2018) 093 [arXiv:1703.03430 [hep-th]]

  47. [47]

    Brower, J

    R.C. Brower, J. Polchinski, M.J. Strassler and C.-I. Tan,The Pomeron and gauge/string duality, JHEP12(2007) 005 [hep-th/0603115]

  48. [48]

    Khemani, D.A

    V. Khemani, D.A. Huse and A. Nahum, Velocity-dependent Lyapunov exponents in many-body quantum, semiclassical, and classical chaos,Phys. Rev. B98(2018) 144304 [1803.05902]

  49. [49]

    Gesteau and H

    E. Gesteau and H. Liu,Toward stringy horizons, 2408.12642

  50. [50]

    Herderschee and J

    A. Herderschee and J. Kudler-Flam,Stringy algebras, stretched horizons, and quantum-connected wormholes, 2510.01556

  51. [51]

    Gao and H

    P. Gao and H. Liu,Quantum chaos in largeqSYK chain,to appear

  52. [52]

    Lin and D

    H.W. Lin and D. Stanford,A symmetry algebra in double-scaled SYK,SciPost Phys.15(2023) 234 [2307.15725]

  53. [53]

    Ohya,Intertwining operator in thermal CFT d,Int

    S. Ohya,Intertwining operator in thermal CFT d,Int. J. Mod. Phys. A32(2017) 1750006 [1611.00763]

  54. [54]

    Dolan and H

    F.A. Dolan and H. Osborn,Conformal Partial Waves: Further Mathematical Results,1108.6194

  55. [55]

    Kravchuk and D

    P. Kravchuk and D. Simmons-Duffin,Light-ray operators in conformal field theory,JHEP11(2018) 102 [1805.00098]

  56. [56]

    Karateev, P

    D. Karateev, P. Kravchuk and D. Simmons-Duffin, Harmonic Analysis and Mean Field Theory,JHEP10 (2019) 217 [1809.05111]

  57. [57]

    Gadde,In search of conformal theories,1702.07362

    A. Gadde,In search of conformal theories,1702.07362

  58. [58]

    Sommerfeld,Partial differential equations in physics, vol

    A. Sommerfeld,Partial differential equations in physics, vol. 1, Academic press (1949)

  59. [59]

    momentum-space

    G.N. Watson,The diffraction of electric waves by the earth,Proceedings of the Royal Society of London. Series A, Containing Papers of a Mathematical and Physical Character95(1918) 83. 8 Supplementary Materials S-I. POLE-SKIPPING OF A SPINJOPERA TOR A. Mode expansion on hyperbolic space for a single block The Minkowski coordinatesx= (t, y, ⃗ x⊥) and the Ri...

  60. [60]

    Exotic case:µ= i(a 1j(µ) +a 2d+a 3)

  61. [61]

    Chiralp ±-case:µ= i(a 1j(µ) +a 2d+a 3 + ia4p±)

  62. [62]

    wherea i are all rational constants

    Frequency case:µ= i(a 2d+a 3 + ia4ω). wherea i are all rational constants. We number the 8 gamma functions in the numerator of (S51) from 1 to 8 (i.e. 1 is for Γ(−J+ i(t+s)) and 8 is for Γ( iµ−J+1−ip + 2 + it)), and Table S1 summarizes which three choices correspond to each case. We will explore the corresponding pole-skipping points of these four cases r...

  63. [63]

    Depending on whethera 1 = 0 or not, this equation could have simple solution or nontrivial solution that depending on the trajectoryj(µ)

    Exotic case In the exotic case,µis not a function ofp ± but fixed by a nontrivial equation. Depending on whethera 1 = 0 or not, this equation could have simple solution or nontrivial solution that depending on the trajectoryj(µ). Denote this solution asµ ∗ and we will fix a pointj(µ ∗) on the trajectory accordingly. For a generic local operator in a gener...

  64. [64]

    Chiral case Since the two chiralp ±-cases are related to each other by reflectionk→ −k, we only need to analyze thep −-case. As shown in Table S1, there are 12 choices for thep −-case, where in each case the remaining 5 gamma functions are in the following two types Γ(a0 + ia2p− + ia3p+),Γ(a 0 +a 1j(µ) + ia2p− + ia3p+) (S56) wherea i are constants. The fi...

  65. [65]

    The result of solvingp − is given in Table S7, where there are two additional choices but both potential pole lines are canceled due to (S53)

    Frequency case For the frequency case, asµis a function ofω= (p − +p +)/2, we can solve eitherp −,p + orj(µ(ω)) at the pole of the remaining 5 gamma functions. The result of solvingp − is given in Table S7, where there are two additional choices but both potential pole lines are canceled due to (S53). Solvingp + orj(µ(ω)) neither leads to new choices

  66. [66]

    They could be either higher or lower than the trajectory

    Relative location of the exceptional pole-skipping points to a Regge trajectory Here we just give an example of the exceptional pole-skipping points to show that its relative location on the (ℑω,ℑk) plane to a trajectory is model-dependent. They could be either higher or lower than the trajectory. Take #1§b1 in Table S3. On the pole line,µis a function of...