Pith. sign in

REVIEW 3 minor 1 cited by

An autonomous Lipschitz fast dynamo on the three-torus

T0 review · 0 major / 3 minor · reviewed 2026-08-04 · deepseek-v4-flash

Pith's one-line read This paper constructs one divergence-free, time-independent velocity field on the three-torus that amplifies magnetic fields at a rate bounded away from zero for every sufficiently small magnetic diffusivity.

desk verdict A substantial 67-page construction proving an autonomous Lipschitz fast dynamo on the flat three-torus, with honest limitations; deserves serious peer review. read the letter →

arxiv 2608.02586 v1 pith:X5TAVIZ5 submitted 2026-08-03 math.AP math-phmath.MPmath.SP

classification math.APmath-phmath.MPmath.SP MSC 76W0535P0547A1035B2537B40
keywords fastdynamokinematicinductionequationPonomarenkoLipschitzvelocitymagneticeigenmodeRieszprojectionmultiscaleconstructiontopologicalentropy
verification ladder T0 review T1 audit T2 compute T3 formal

The pith

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

The reading

The paper proves that the flat three-torus admits an autonomous Lipschitz fast dynamo: a single velocity field chosen before the diffusivity, with every sufficiently small positive diffusivity producing an exponentially growing magnetic eigenmode whose growth rate is uniformly positive. The field is divergence-free, time-independent, and even has zero topological entropy and no exponential particle stretching, so the growth comes from a multiscale spectral mechanism rather than chaotic advection. If true, this separates the Lipschitz regime from the classical smooth obstructions and shows that fast dynamo action on the flat torus does not require C^1 regularity.

What carries the argument

The argument is a multiscale assembly of copies of a local Ponomarenko-type screw flow. The local unstable spectral subspace, defined by a fixed Riesz contour around an unstable eigenvalue, is shown to persist under smoothing of the velocity jump via norm-resolvent perturbation estimates and to remain uniformly localized in space. Copies are placed at geometric scales ℓ_n with buffer regions of radius √ℓ_n so that every small ε matches one cell exactly after transverse rescaling; an added constant axial velocity in each cell shifts unwanted spectra in the imaginary direction. A parametrix glues the local resolvents to the torus operator, and a comparison of Riesz projections transfers the lo

What would settle it

Compute the dispersion relation for the smoothed screw profile with smoothing width h and check whether an eigenvalue with real part at least γ0 persists for all h ≤ h0 but disappears when h is comparable to the smallest cell scale ℓ_n used for a given ε; if such h can be fixed while ε tends to zero, the uniform lower bound would fail.

Watch

Extended reading notes

Core claim

The central claim is Theorem 1.3: there exists a real-valued divergence-free velocity u in W^{1,∞}(T^3; R^3) and constants ε0, γ0 > 0 such that for every 0 < ε ≤ ε0 the induction operator L_{ε,u} has an eigenvalue with real part at least γ0. For each ε there is a magnetic eigenmode V_ε = e^{2πi K_ε x3} b_ε(y) with K_ε ≠ 0, and the real initial field B_in = Re V_ε evolves under the induction equation with the exact L^2 norm law ||B_ε(t)||_2 = e^{t Re λ_ε} ||B_in||_2 for all t ≥ 0. The same velocity has particle flow with Lipschitz constants growing at most linearly, every time map has zero topological entropy, and the ideal induction group has zero exponential growth, so the resistive growth

Load-bearing premise

The construction depends on the local unstable spectral subspace surviving smoothing of the velocity jump and staying concentrated in one uniformly large disc; if either fails, the parametrix error bound cannot be made small and the global eigenvalue may not exist.

Editorial extensions

If this is right

  • If the construction is correct, the smooth autonomous fast-dynamo conjecture cannot be resolved by mollifying this example: the velocity is not C^1, and a fixed mollification changes precisely the cells matched to sufficiently small diffusivities.
  • The example bypasses the classical obstructions: zero topological entropy and zero ideal exponential growth do not rule out a fast dynamo once the velocity is merely Lipschitz.
  • For each diffusivity, the magnetic datum is real, divergence-free, and satisfies an exact exponential norm identity, so the growth is persistent in time rather than occurring only along a sequence of times.
  • The magnetic eigenmode has axial wave number of order ε^{-1/2} and H^1-based magnetic length of order √ε, matching the classical resistive scale associated with fast dynamo action.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

  • The fixed-contour Riesz-projection transfer used here could serve as a template for transplanting local spectral instabilities into global operators in other settings, replacing fragile eigenvalue-tracking with subspace-tracking.
  • A natural numerical test is to truncate the velocity to finitely many cells and check whether the uniform lower bound γ0 appears as ε varies; the construction predicts the bound holds once enough cells are included.
  • If the mechanism generalizes to velocities that are C^{1-α} for small α, it would sharpen the boundary between the smooth obstructions and Lipschitz constructions; the paper's mechanism suggests the C^1 loss at the accumulation circle is essential.
  • The exact exponential norm identity for each real initial datum suggests that the construction may yield growth estimates for general initial data after averaging over axial phases, although the paper itself only claims the selected eigenmode.
Share X Bluesky LinkedIn Reddit HN

Editorial analysis

A structured set of objections, weighed in public.

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

Referee Report

0 major / 3 minor

Summary. The paper constructs a single real-valued, divergence-free, time-independent velocity field u ∈ W^{1,∞}(T^3; R^3) and positive constants ε0, γ0 such that, for every 0 < ε ≤ ε0, the kinematic induction operator L_{ε,u} has an eigenvalue with real part at least γ0, and a real divergence-free initial datum whose L² norm satisfies an exact exponential growth law with rate Re λ_ε ≥ γ0. The construction is multiscale: infinitely many rescaled copies of a compactly supported smooth helical/Ponomarenko-type local profile accumulate at a single circle, each cell carries an added axial velocity for spectral separation, and buffer annuli provide exponential resolvent decay. The proof first establishes a local unstable spectral subspace via an explicit Bessel-function dispersion calculation, proves its persistence under smoothing and variation of the diffusivity, then transfers it to the torus through a parametrix comparison and a non-zero Riesz projection argument. The same velocity is shown to have at most linear Lipschitz growth of the particle flow, zero topological entropy, and zero exponential growth for the ideal induction group, giving an ideal–resistive gap at Lipschitz regularity with the quantifier order of Arnold's Conjecture 1.2 but not its smoothness.

Significance. If correct, the theorem is a major step: it provides the first autonomous velocity field on the flat three-torus, at Lipschitz regularity, that is a fast dynamo for every sufficiently small diffusivity in the strong spectral sense — velocity and rate chosen before ε, eigenmode chosen per ε. It also shows that classical no-fast-dynamo results under smoothness or zero-topological-entropy hypotheses cannot be relaxed to W^{1,∞}. The paper is a rigorous analytic tour de force: the local dispersion root w0 = √3 + i with w0³ = 8i, the determinant identity D(κ) = κ⁻³ + O(κ⁻⁵), the h^{1/4} norm-resolvent convergence under smoothing, the exponential buffer decay, and the parametrix estimate (6.9) are all explicit and verifiable. The most delicate point — persistence and uniform spatial localization of the non-self-adjoint unstable spectral subspace — is addressed by Lemmas 2.5, 2.7, and 2.8, and I find the argument convincing. The paper honestly states its limitations (non-C¹ regularity, non-persistence under fixed-scale smoothing, no single datum for all ε), and the comparison with previous constructions clarifies the quantifier distinctions.

minor comments (3)
  1. [§5.3, Lemma 5.3] For the adjoint numerical-range estimate, the formal adjoint B† is displayed and the same bound is asserted 'after one enlargement.' It would ease verification to state explicitly the enlarged constant, e.g., Cnum' = Cnum + ∥G_m∥∞, and to note that the signs of the transport terms reverse but all magnitude bounds are unchanged.
  2. [§5.4, Lemma 5.7(b)] In the exterior exponential decay estimate, the test function η_out² e^{2Φ_out} \bar g is not compactly supported at infinity. Since Φ_out is bounded and Lipschitz and g ∈ H¹ outside D(p,R/4), this is admissible in the exterior weak formulation; a one-sentence approximation or truncation argument would make the justification self-contained.
  3. [§3.4, Proposition 3.2] The sentence 'every Lyapunov exponent is zero' is a bit compressed. Since it follows directly from the two-sided estimate Lip(Φ_t) + Lip(Φ_{-t}) ≤ C(1+|t|), a short chain — |v| ≤ C(1+|t|)|DΦ_t v| and |DΦ_t v| ≤ C(1+|t|)|v| — would make the step immediately transparent.

Circularity Check

0 steps flagged · score 0.0 of 10

No significant circularity: the derivation chain is self-contained and the central claim is not fitted or self-referential.

full rationale

The paper's load-bearing chain does not reduce to its own inputs. The local instability is an actual spectral computation: the dispersion relation (2.7), D(κ)=κ^{-3}+O(κ^{-5}), is solved with Rouché's theorem to produce an eigenvalue λ_N with Re λ_N ≥ N²/2; this is a derived output, not a fitted target. The persistence of the unstable Riesz projection under smoothing (Lemma 2.5) is obtained from the quantitative norm-resolvent bound (2.15), which follows from explicit form perturbation estimates, not from an assumption that the desired spectral point exists. The scaling identity (4.3), U_n^{-1} A^{(n)}_{ε,n} U_n = L_{δ_n} - iτ, is an exact algebraic conjugation that transfers the already-proved local spectral statement to the matching cell; the added term -iτ is purely imaginary and leaves all real parts unchanged. The global gluing argument is constructive: buffer decay estimates (5.10)-(5.11), the error bound (6.9), and the Riesz projection comparison (6.14) show that the full torus operator inherits a non-zero spectral projection, with the growth constant γ0 = g* read off from the fixed contour G. No parameter is fitted to a predicted quantity, no 'prediction' is defined in terms of the claimed result, and there is no self-citation chain: the paper is single-authored and its main external supports are classical Ponomarenko/Gilbert analyses plus standard perturbation theory, none of which is used to assume the target theorem. The honest limitations stated in the paper (non-C^1 regularity, openness of the smooth case, fixed-scale smoothing not preserving the mechanism) do not indicate circularity. Therefore no circular step is present.

Assumptions & free parameters 7 free parameters · 6 assumptions · 0 invented entities

Everything the central claim rests on is either standard spectral theory and Bessel analysis, the physically standard kinematic dynamo model, or the author's own construction parameters, which are existential knobs chosen subject to explicit inequalities rather than fitted data. The hand-chosen constants are Omega, U (local design), h (smoothing), q, q-bar (scale ratios), J (truncation), tau (axial shift amplitude), K0 (initial index), and alpha = 1/2 (buffer exponent, explicitly non-essential). No invented physical entities or new forces/fields are introduced. The eigenvalue and growth rate are solved, not prescribed.

free parameters (7)
  • Local design constants Omega = 16 N^3, U = -16 N^2 (N = 2 pi k*) = Omega = 128 pi^3 k*^3, U = -64 pi^2 k*^2
    Chosen in Section 2.2 so the dispersion relation D(kappa) = -i/(8 N^3) has a right-half-plane root with lambda_N/N^2 -> 1 + 2 sqrt(3) i. Hand-designed for the ansatz, then rigorously verified by Rouché's theorem; not fitted to data.
  • Smoothing width h = 0 < h <= h0, existential
    The velocity jump at r = 1 is smoothed over width h; the proof only needs ||v_h - V0||_{L4} = O(h^{1/4}) and any sufficiently small h works (Lemma 2.5).
  • Geometric ratios q, q-bar = 1 < q < q-bar < sqrt(delta+/delta-)
    Required in Section 3.2 for overlap of the diffusivity intervals I_n (equation (3.1)). Existence-level choices, fixed before J, tau, K0.
  • Truncation index J = J in N with M theta_J < min{1/4, g*/8}
    Fixed in Proposition 5.2 to make the small-cell tail energetically negligible; chosen before tau and K0, as stated in the parameter order.
  • Axial shift parameter tau = tau c_q >= 2 C_num + 2 sup_{zeta in G} |Im zeta| + 1 (5.7)
    The added axial velocities a_n = tau/(2 pi K_n) translate each cell's spectrum by -i tau; tau is chosen large to achieve spectral separation (Lemma 5.4). This is the main hand-tuned knob, chosen after C_num is bounded independently of n, epsilon.
  • Initial Fourier index K0 = large enough for (3.4), (3.8), (6.11), (6.16)
    The final existential parameter; enlarging K0 shrinks cells and buffers and makes the parametrix error small. Explicitly ordered last in Section 6.
  • Buffer exponent alpha = 1/2 = R_n = l_n^alpha with alpha = 1/2
    Acknowledged as not essential in Remark 6.4: any 0 < alpha < 1 satisfies the sufficient conditions (6.13). The choice is made for symmetry of estimates.
assumptions (6)
  • standard math Standard spectral theory for non-self-adjoint operators: closed sectorial forms and the representation theorem, analytic Fredholm theory, Riesz projections and their norm-resolvent stability (Kato, Gohberg-Goldberg-Kaashoek).
    Invoked throughout Section 2 (form domains, essential spectrum (-infinity, -N^2], eigenvalue isolation, persisting Riesz rank) and in Lemma 1.1.
  • standard math Analytic semigroup theory with spectral mapping for compact semigroups and subadditivity of semigroup growth (Engel-Nagel).
    Lemma 1.1 and Appendix A: gamma(u,epsilon) = sup Re spec(L_{epsilon,u}) and immediate compactness of e^{tL} for t > 0.
  • standard math Bessel function asymptotics with uniform sector estimates (DLMF sections 10.25, 10.28, 10.40).
    The dispersion relation D(kappa) = kappa^{-3} + O(kappa^{-5}) and the large-N root w0 = sqrt(3)+i in Lemma 2.1.
  • standard math Sobolev embedding H^1(T^2) into L^4, Ladyzhenskaya inequality, elliptic regularity for Delta_perp - N^2 with N != 0.
    Used in the tail estimate (Lemma 5.1), resolvent bounds (Lemma 2.6, Proposition 5.2), and regularity steps.
  • domain assumption Kinematic dynamo model: the induction equation (1.1) with prescribed divergence-free velocity in W^{1,infinity}; L^2_sigma topology; fast/slow dynamo defined by the liminf of sustained spectral growth (Vainshtein-Zel'dovich).
    The physical and mathematical problem definition, Section 1.1. Growth is measured in operator norm on the solenoidal subspace.
  • domain assumption Cauchy-Lipschitz theory and the Cauchy formula for W^{1,infinity} flows (Ambrosio-Crippa): ideal induction as pushforward by D Phi_t, formulas (3.18)-(3.19).
    Proposition 3.2 and Corollary 3.3 require u in W^{1,infinity}, div u = 0, and the flow-level Cauchy formula.

how reviews work

0 comments
Cite this review

Pith. "Pith review of An autonomous Lipschitz fast dynamo on the three-torus." pith.science (2026). https://pith.science/paper/X5TAVIZ5

@misc{pith2026260802586,
  author       = {Pith},
  title        = {Pith review of: An autonomous Lipschitz fast dynamo on the three-torus},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/X5TAVIZ5}},
  note         = {Machine review of arXiv:2608.02586}
}
abstract

We construct a single real-valued, divergence-free, time-independent velocity field $u\in\mathrm{W}^{1,\infty}(\mathbb{T}^3;\mathbb{R}^3) $ that is a fast dynamo for the kinematic induction equation on the flat three-torus. For every sufficiently small positive magnetic diffusivity, the corresponding induction operator has an eigenvalue whose real part is bounded below by a positive constant independent of the diffusivity. For each such diffusivity, there is a non-zero real-valued, divergence-free solution of the induction equation whose $\mathrm{L}^2 $-norm obeys an exact exponential growth law with a uniformly positive rate. For the same velocity field, the particle flow and its inverse have Lipschitz constants growing at most linearly in time, every time map has zero topological entropy, and the ideal induction group has zero exponential growth rate in operator norm. The velocity is differentiable everywhere and smooth away from a single circle, but is not $\mathrm{C}^1 $.

Figures

Figures reproduced from arXiv: 2608.02586 by the authors.

Figure 1
Figure 1. Schematic transverse geometry, not drawn to scale. In the model, the discs D(pn, Rn) shrink and accumulate at p∞; in T 3 , the corresponding accumulation set is the axial circle {p∞} × T. In each cell, the local-flow core has scale ℓn. The added axial velocity equals ane3 throughout D(pn, 3Rn/4), including the local-flow core and the surrounding constant-coefficient buffer, and is smoothly cut off before the boundar… view at source ↗

Discussion (0). Sign in to comment.

Forward citations

Cited by 1 Pith paper

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

  1. Exponential growth and decay in the ideal induction equation

    math.AP 2026-08 conditional novelty 8.0 of 10

    A piecewise-affine, time-periodic shear flow on the 3-torus is a universal ideal dynamo: every non-zero divergence-free L^p initial field grows exponentially for large shear amplitude.

Reference graph

Works this paper leans on

51 extracted references · 25 canonical work pages · cited by 1 Pith paper

  1. [1]

    Ambrosio and G

    L. Ambrosio and G. Crippa,Continuity equations and ODE flows with non-smooth velocity, Proc. Roy. Soc. Edinburgh Sect. A144(2014), no. 6, 1191–1244, doi:10.1017/S0308210513000085

  2. [2]

    Armstrong and V

    S. Armstrong and V. Vicol,Anomalous diffusion by fractal homogenization, Ann. PDE11(2025), no. 1, Paper No. 2, doi:10.1007/s40818-024-00189-6

  3. [3]

    V. I. Arnold,Arnold’s Problems, Springer–Verlag, Berlin, and PHASIS, Moscow, 2004, Problem 1994– 28, doi:10.1007/b138219

  4. [4]

    V. I. Arnold and B. A. Khesin,Topological Methods in Hydrodynamics, Applied Mathematical Sciences, vol. 125, Springer, 1998, doi:10.1007/b97593

  5. [5]

    V. I. Arnol’d, Ya. B. Zel’dovich, A. A. Ruzmaikin and D. D. Sokolov,A magnetic field in a stationary flow with stretching in Riemannian space, Sov. Phys. JETP54(1981), no. 6, 1083–1086, English translation

  6. [6]

    P. H. Baxendale and B. L. Rozovskii,Kinematic dynamo and intermittence in a turbulent flow, Geophys. Astrophys. Fluid Dyn.73(1993), no. 1–4, 33–60, doi:10.1080/03091929308203618

  7. [7]

    B. J. Bayly and S. Childress,Construction of fast dynamos using unsteady flows and maps in three dimensions, Geophys. Astrophys. Fluid Dyn.44(1988), no. 1–4, 211–240, doi:10.1080/03091928808208887

  8. [8]

    B¨ ogli,Schr¨ odinger operator with non-zero accumulation points of complex eigenvalues, Comm

    S. B¨ ogli,Schr¨ odinger operator with non-zero accumulation points of complex eigenvalues, Comm. Math. Phys.352(2017), no. 2, 629–639, doi:10.1007/s00220-016-2806-5

Show all 51 references
  1. [9]

    Bowen,Entropy for group endomorphisms and homogeneous spaces, Trans

    R. Bowen,Entropy for group endomorphisms and homogeneous spaces, Trans. Amer. Math. Soc. 153(1971), 401–414, doi:10.1090/S0002-9947-1971-0274707-X

  2. [10]

    Chicone and Y

    C. Chicone and Y. Latushkin,The geodesic flow generates a fast dynamo: an elementary proof, Proc. Amer. Math. Soc.125(1997), no. 11, 3391–3396, doi:10.1090/S0002-9939-97-04187-7

  3. [11]

    Chicone, Y

    C. Chicone, Y. Latushkin and S. Montgomery-Smith,The spectrum of the kinematic dynamo operator for an ideally conducting fluid, Comm. Math. Phys.173(1995), no. 2, 379–400, doi:10.1007/BF02101239

  4. [12]

    Childress,New solutions of the kinematic dynamo problem, J

    S. Childress,New solutions of the kinematic dynamo problem, J. Math. Phys.11(1970), no. 10, 3063–3076, doi:10.1063/1.1665095

  5. [13]

    Childress and A

    S. Childress and A. D. Gilbert,Stretch, Twist, Fold: The Fast Dynamo, Lecture Notes in Physics Monographs, vol. 37, Springer, 1995, doi:10.1007/978-3-540-44778-8

  6. [14]

    Coti Zelati and V

    M. Coti Zelati and V. Navarro-Fern´ andez,Three-dimensional exponential mixing and ideal kinematic dynamo with randomized ABC flows, J. Dynam. Differential Equations (2026), doi:10.1007/s10884- 026-10483-5

  7. [15]

    Coti Zelati, M

    M. Coti Zelati, M. Sorella and D. Villringer,Alpha-unstable flows and the fast dynamo problem, arXiv:2504.00855v1, 2025

  8. [16]

    Coti Zelati, M

    M. Coti Zelati, M. Sorella and D. Villringer,A fast dynamo on the three-torus, arXiv:2603.09861v2, 2026

  9. [17]

    Cuenin,Schr¨ odinger operators with complex sparse potentials, Comm

    J.-C. Cuenin,Schr¨ odinger operators with complex sparse potentials, Comm. Math. Phys.392(2022), no. 3, 951–992, doi:10.1007/s00220-022-04358-1

  10. [18]

    Datchev and A

    K. Datchev and A. Vasy,Gluing semiclassical resolvent estimates via propagation of singularities, Int. Math. Res. Not. IMRN (2012), no. 23, 5409–5443, doi:10.1093/imrn/rnr255

  11. [19]

    Del Nin, D

    G. Del Nin, D. Faraco, S. Lindberg and F. Mengual,Turbulent dynamos on bounded domains and their generalization to the geometric transport equation, arXiv:2605.20451v1, 2026

  12. [20]

    R. J. DiPerna and P.-L. Lions,Ordinary differential equations, transport theory and Sobolev spaces, Invent. Math.98(1989), no. 3, 511–547, doi:10.1007/BF01393835

  13. [21]

    Engel and R

    K.-J. Engel and R. Nagel,One-Parameter Semigroups for Linear Evolution Equations, Graduate Texts in Mathematics, vol. 194, Springer, 2000, doi:10.1007/b97696. 66 LUKAS NIEBEL

  14. [22]

    Friedlander and M

    S. Friedlander and M. M. Vishik,Dynamo theory, vorticity generation, and exponential stretching, Chaos1(1991), no. 2, 198–205, doi:10.1063/1.165829

  15. [23]

    Galitski, M

    V. Galitski, M. Kargarian and S. Syzranov,Dynamo effect and turbulence in hydrodynamic Weyl metals, Phys. Rev. Lett.121(2018), no. 17, Paper No. 176603, doi:10.1103/PhysRevLett.121.176603

  16. [24]

    G´ erard-Varet and F

    D. G´ erard-Varet and F. Rousset,Shear layer solutions of incompressible MHD and dynamo effect, Ann. Inst. H. Poincar´ e C Anal. Non Lin´ eaire24(2007), no. 5, 677–710, doi:10.1016/j.anihpc.2006.04.005

  17. [25]

    A. D. Gilbert,Fast dynamo action in the Ponomarenko dynamo, Geophys. Astrophys. Fluid Dyn. 44(1988), no. 1–4, 241–258, doi:10.1080/03091928808208888

  18. [26]

    Gohberg, S

    I. Gohberg, S. Goldberg and M. A. Kaashoek,Classes of Linear Operators, Vol. I, Operator Theory: Advances and Applications, vol. 49, Birkh¨ auser, Basel, 1990, doi:10.1007/978-3-0348-7509-7

  19. [27]

    Helffer and J

    B. Helffer and J. Sj¨ ostrand,Multiple wells in the semi-classical limit I, Comm. Partial Differential Equations9(1984), no. 4, 337–408, doi:10.1080/03605308408820335

  20. [28]

    Jiang and W

    N. Jiang and W. Zhang,Quenched correlation decay for random splittings of some prototypical 3D flows including the ABC flow, arXiv:2504.14564v1, 2025

  21. [29]

    Kato,Perturbation Theory for Linear Operators, Classics in Mathematics, Springer, 1995, doi:10.1007/978-3-642-66282-9

    T. Kato,Perturbation Theory for Linear Operators, Classics in Mathematics, Springer, 1995, doi:10.1007/978-3-642-66282-9

  22. [30]

    Katok and B

    A. Katok and B. Hasselblatt,Introduction to the Modern Theory of Dynamical Systems, Encyclopedia of Mathematics and its Applications, vol. 54, Cambridge University Press, Cambridge, 1995, doi:10.1017/CBO9780511809187

  23. [31]

    A. P. Kazantsev,Enhancement of a magnetic field by a conducting fluid, Sov. Phys. JETP26(1968), no. 5, 1031–1034, English translation

  24. [32]

    Klapper and L

    I. Klapper and L. S. Young,Rigorous bounds on the fast dynamo growth rate involving topological entropy, Comm. Math. Phys.173(1995), no. 3, 623–646, doi:10.1007/BF02101659

  25. [33]

    Lions and E

    J.-L. Lions and E. Magenes,Non-Homogeneous Boundary Value Problems and Applications, vol. I, Grundlehren der mathematischen Wissenschaften, vol. 181, Springer, 1972, doi:10.1007/978-3-642- 65161-8

  26. [34]

    H. K. Moffatt,Magnetic Field Generation in Electrically Conducting Fluids, Cambridge University Press, 1978

  27. [35]

    H. K. Moffatt and M. R. E. Proctor,Topological constraints associated with fast dynamo action, J. Fluid Mech.154(1985), 493–507, doi:10.1017/S002211208500163X

  28. [36]

    S. A. Molchanov, A. A. Ruzmaikin and D. D. Sokoloff,A dynamo theorem, Geophys. Astrophys. Fluid Dyn.30(1984), 241–259, doi:10.1080/03091928408222852

  29. [37]

    Navarro-Fern´ andez and D

    V. Navarro-Fern´ andez and D. Villringer,Spectral instability in the smooth Ponomarenko dynamo, arXiv:2509.19201v1, 2025

  30. [38]

    NIST Digital Library of Mathematical Functions,Bessel functions,https://dlmf.nist.gov/10

  31. [39]

    V. I. Oseledets,Fast dynamo problem for a smooth map on a two-torus, Geophys. Astrophys. Fluid Dyn.73(1993), no. 1–4, 133–145, doi:10.1080/03091929308203625

  32. [40]

    Y. B. Ponomarenko,Theory of the hydromagnetic generator, J. Appl. Mech. Tech. Phys.14(1973), 775–778, doi:10.1007/BF00853190

  33. [41]

    F. A. Pramy, B. D. Mestel and A. D. Gilbert,A computer-assisted proof of dynamo growth in the stretch-fold-shear map, Dynamical Systems38(2023), no. 1, 102–120, doi:10.1080/14689367.2022.2139224

  34. [42]

    G. O. Roberts,Spatially periodic dynamos, Philos. Trans. Roy. Soc. London Ser. A266(1970), no. 1179, 535–558, doi:10.1098/rsta.1970.0011

  35. [43]

    Rowan,A subsequentially fast dynamo onT 3, arXiv:2505.23936v1, 2025

    K. Rowan,A subsequentially fast dynamo onT 3, arXiv:2505.23936v1, 2025

  36. [44]

    A. A. Ruzmaikin, D. D. Sokoloff and A. M. Shukurov,Hydromagnetic screw dynamo, J. Fluid Mech. 197(1988), 39–56, doi:10.1017/S0022112088003167

  37. [45]

    Sorella and D

    M. Sorella and D. Villringer,A limsup fast dynamo onT 3, arXiv:2511.23024v2, 2025

  38. [46]

    A. M. Soward,Fast dynamo action in a steady flow, J. Fluid Mech.180(1987), 267–295, doi:10.1017/S0022112087001800

  39. [47]

    A. M. Soward,An asymptotic solution of a fast dynamo in a two-dimensional pulsed flow, Geophys. Astrophys. Fluid Dyn.73(1993), no. 1–4, 179–215, doi:10.1080/03091929308203628

  40. [48]

    S. I. Vainshtein and Ya. B. Zel’dovich,Origin of magnetic fields in astrophysics (turbulent “dynamo” mechanisms), Sov. Phys. Usp.15(1972), no. 2, 159–172, doi:10.1070/PU1972v015n02ABEH004960. A F AST DYNAMO ON THE THREE-TORUS 67

  41. [49]

    M. M. Vishik,Magnetic field generation by the motion of a highly conducting fluid, Geophys. Astrophys. Fluid Dyn.48(1989), nos. 1–3, 151–167, doi:10.1080/03091928908219531

  42. [50]

    Walters,An Introduction to Ergodic Theory, Graduate Texts in Mathematics, vol

    P. Walters,An Introduction to Ergodic Theory, Graduate Texts in Mathematics, vol. 79, Springer– Verlag, New York, 1982, doi:10.1007/978-1-4612-5775-2

  43. [51]

    Ya. B. Zel’dovich, A. A. Ruzmaikin, S. A. Molchanov and D. D. Sokoloff,Kinematic dynamo problem in a linear velocity field, J. Fluid Mech.144(1984), 1–11, doi:10.1017/S0022112084001488. (Lukas Niebel)ETH Z ¨urich, Department of Mathematics, R¨amistrasse 101, 8092 Z¨urich, Swit...

Pith tools

Reviewed August 4, 2026 · model on record in the stance chip above.