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Theorem 1.7 (necessity): a binding of a disk-like global section is unknotted with sl⁡=−1\operatorname{sl}=-1sl=−1

Proved
HryniewiczCriterion.unknotted_selfLinking_of_bounds_global_section

by Mazecto · Oct 5, 2026 · Mathlib 0df444a (Lean v4.33.1)

contact-geometrydynamical-systemssymplectic-geometry

Let S=H−1(1)⊂R4S=H^{-1}(1)\subset\mathbb{R}^4S=H−1(1)⊂R4 be a strictly star-shaped energy surface whose flow is dynamically convex. Let Pˉ\bar PPˉ be a prime periodic orbit on SSS. If Pˉ\bar PPˉ bounds a disk-like global surface of section, then

Pˉ is unknottedandsl⁡(Pˉ)=−1.\bar P\ \text{is unknotted}\quad\text{and}\quad \operatorname{sl}(\bar P)=-1.Pˉ is unknottedandsl(Pˉ)=−1.

This is the "only if" half of Hryniewicz's criterion. Unknottedness is immediate from the spanning disk. The value of the self-linking number comes from the transversality of the disk to the flow.

Preamble
import Definitions.Def_HryniewiczCriterion_ConleyZehnder
import Definitions.Def_HryniewiczCriterion_GlobalSection
import Definitions.Def_HryniewiczCriterion_SelfLinking
Formal statement
namespace HryniewiczCriterion

/-- Hryniewicz, Theorem 1.7, "only if" direction: a prime periodic orbit of a
dynamically convex flow that bounds a disk-like global surface of section is unknotted
and has self-linking number `-1`. -/
theorem unknotted_selfLinking_of_bounds_global_section (H : R4 → ℝ)
    (hS : IsStrictlyStarShapedLevel H) (hdc : IsDynamicallyConvex H)
    (P : PeriodicOrbit H) (hP : P.IsPrime)
    (hD : BoundsDiskLikeGlobalSection H P) :
    IsUnknotted H P ∧ HasSelfLinkingNumber H P (-1) := by sorry

end HryniewiczCriterion
Source
Hryniewicz, Systems of global surfaces of section for dynamically convex Reeb flows on the 3-sphere, J. Symplectic Geom. 12 (2014) 791-862, https://arxiv.org/abs/1105.2077, Theorem 1.7, p. 3 (only-if direction; proof outline p. 4, via Proposition 2.1 of Hryniewicz, Trans. AMS 364 (2012), https://arxiv.org/abs/0812.4076)
Read-back

What the Lean code literally says, in plain math · claude-opus-5-5

Read-back. Let H:R4→RH : \mathbb{R}^4 \to \mathbb{R}H:R4→R be any function; coordinates are x=(x0,…,x3)x = (x_0,\dots,x_3)x=(x0​,…,x3​), DH(x)DH(x)DH(x) is the Fréchet derivative (taken to be 000 where not differentiable), Σ={H=1}\Sigma = \{H = 1\}Σ={H=1}, and

XH(x)=(−∂1H(x), ∂0H(x), −∂3H(x), ∂2H(x)),∂iH(x)=DH(x)ei.X_H(x) = \bigl(-\partial_1 H(x),\ \partial_0 H(x),\ -\partial_3 H(x),\ \partial_2 H(x)\bigr),\quad \partial_iH(x) = DH(x)e_i .XH​(x)=(−∂1​H(x), ∂0​H(x), −∂3​H(x), ∂2​H(x)),∂i​H(x)=DH(x)ei​.

A trajectory is y:R→R4y : \mathbb{R}\to\mathbb{R}^4y:R→R4 with y′(t)=XH(y(t))y'(t) = X_H(y(t))y′(t)=XH​(y(t)) and H(y(t))=1H(y(t)) = 1H(y(t))=1 for all ttt. A periodic orbit is a trajectory xxx with a real T>0T>0T>0 and x(t+T)=x(t)x(t+T) = x(t)x(t+T)=x(t) for all ttt (TTT not necessarily minimal).

Notation: D,D˚,S1⊂R2D, \mathring D, S^1 \subset \mathbb{R}^2D,D˚,S1⊂R2 are the closed unit disk, open unit disk and unit circle; ⟨a,b⟩=∑iaibi\langle a,b\rangle = \sum_i a_ib_i⟨a,b⟩=∑i​ai​bi​, ∣a∣=⟨a,a⟩|a| = \sqrt{\langle a,a\rangle}∣a∣=⟨a,a⟩​; ω0(u,v)=u0v1−u1v0+u2v3−u3v2\omega_0(u,v) = u_0v_1 - u_1v_0 + u_2v_3 - u_3v_2ω0​(u,v)=u0​v1​−u1​v0​+u2​v3​−u3​v2​; λx(v)=12(x0v1−x1v0+x2v3−x3v2)\lambda_x(v) = \tfrac12(x_0v_1 - x_1v_0 + x_2v_3 - x_3v_2)λx​(v)=21​(x0​v1​−x1​v0​+x2​v3​−x3​v2​); Q1x=(−x2,x3,x0,−x1)Q_1x = (-x_2, x_3, x_0, -x_1)Q1​x=(−x2​,x3​,x0​,−x1​), Q2x=(x3,x2,−x1,−x0)Q_2x = (x_3, x_2, -x_1, -x_0)Q2​x=(x3​,x2​,−x1​,−x0​);

ξ1(x)=∣x∣−1(Q2x−DH(x)Q2xDH(x)xx),ξ2(x)=∣x∣−1(Q1x−DH(x)Q1xDH(x)xx).\xi_1(x) = |x|^{-1}\Bigl(Q_2x - \tfrac{DH(x)Q_2x}{DH(x)x}x\Bigr),\qquad \xi_2(x) = |x|^{-1}\Bigl(Q_1x - \tfrac{DH(x)Q_1x}{DH(x)x}x\Bigr).ξ1​(x)=∣x∣−1(Q2​x−DH(x)xDH(x)Q2​x​x),ξ2​(x)=∣x∣−1(Q1​x−DH(x)xDH(x)Q1​x​x).

Division by 000 and 0−10^{-1}0−1 evaluate to 000.

Hypotheses.

  • hShShS (strictly star-shaped level): HHH is C∞C^\inftyC∞ on R4\mathbb{R}^4R4; for every u≠0u \neq 0u=0 there is exactly one r>0r > 0r>0 with H(ru)=1H(ru) = 1H(ru)=1; and DH(x) x>0DH(x)\,x > 0DH(x)x>0 for every x∈Σx \in \Sigmax∈Σ.
  • hdchdchdc (dynamically convex): for every periodic orbit (x,T)(x, T)(x,T) of HHH (of any, not necessarily minimal, period) and every Y:R→L(R4,R4)Y : \mathbb{R}\to \mathrm{L}(\mathbb{R}^4,\mathbb{R}^4)Y:R→L(R4,R4) with Y(0)=idY(0) = \mathrm{id}Y(0)=id and Y′(t)=DXH(x(t))∘Y(t)Y'(t) = DX_H(x(t))\circ Y(t)Y′(t)=DXH​(x(t))∘Y(t) for all ttt, the integer μ(M)≥3\mu(M) \ge 3μ(M)≥3, where M(τ)M(\tau)M(τ) is the 2×22\times22×2 matrix
M(τ)ij=[cx(Tτ)(πx(Tτ)(Y(Tτ) ξj(x(0))))]i,πx(v)=v−λx(v)λx(XH(x))XH(x),cx(v)=(ω0(v,ξ2(x)), ω0(ξ1(x),v)),M(\tau)_{ij} = \Bigl[c_{x(T\tau)}\bigl(\pi_{x(T\tau)}(Y(T\tau)\,\xi_j(x(0)))\bigr)\Bigr]_i,\quad \pi_x(v) = v - \tfrac{\lambda_x(v)}{\lambda_x(X_H(x))}X_H(x),\quad c_x(v) = \bigl(\omega_0(v,\xi_2(x)),\ \omega_0(\xi_1(x),v)\bigr),M(τ)ij​=[cx(Tτ)​(πx(Tτ)​(Y(Tτ)ξj​(x(0))))]i​,πx​(v)=v−λx​(XH​(x))λx​(v)​XH​(x),cx​(v)=(ω0​(v,ξ2​(x)), ω0​(ξ1​(x),v)),

and for a matrix path φ\varphiφ: W(φ)W(\varphi)W(φ) is the set of (θ(1)−s)/(2π)(\theta(1)-s)/(2\pi)(θ(1)−s)/(2π) over s∈[0,2π]s \in [0,2\pi]s∈[0,2π] and θ\thetaθ continuous on [0,1][0,1][0,1] with θ(0)=s\theta(0)=sθ(0)=s and φ(t)(cos⁡s,sin⁡s)∈R>0 (cos⁡θ(t),sin⁡θ(t))\varphi(t)(\cos s,\sin s) \in \mathbb{R}_{>0}\,(\cos\theta(t),\sin\theta(t))φ(t)(coss,sins)∈R>0​(cosθ(t),sinθ(t)) for t∈[0,1]t\in[0,1]t∈[0,1]; a=inf⁡Wa = \inf Wa=infW, b=sup⁡Wb = \sup Wb=supW (both 000 if WWW is empty or unbounded on that side); μ(φ)=2(⌈b⌉−1)\mu(\varphi) = 2(\lceil b\rceil - 1)μ(φ)=2(⌈b⌉−1) if a≤⌈b⌉−1a \le \lceil b\rceil - 1a≤⌈b⌉−1, else 2⌈b⌉−12\lceil b\rceil - 12⌈b⌉−1.

  • PPP: a periodic orbit (x,T)(x, T)(x,T) of HHH.
  • hPhPhP (prime): x(t)≠x(0)x(t) \neq x(0)x(t)=x(0) for all 0<t<T0 < t < T0<t<T.
  • hDhDhD (bounds a disk-like global section): there is e:R2→R4e : \mathbb{R}^2 \to \mathbb{R}^4e:R2→R4 such that: eee is C∞C^\inftyC∞, injective on DDD, with De(u)De(u)De(u) injective for every u∈Du\in Du∈D; e(D)⊆Σe(D) \subseteq \Sigmae(D)⊆Σ; e(S1)=x(R)e(S^1) = x(\mathbb{R})e(S1)=x(R); XH(e(u))∉range⁡De(u)X_H(e(u)) \notin \operatorname{range} De(u)XH​(e(u))∈/rangeDe(u) for every u∈D˚u \in \mathring Du∈D˚; and every trajectory yyy with y(0)∉x(R)y(0) \notin x(\mathbb{R})y(0)∈/x(R) satisfies, for every a∈Ra\in\mathbb{R}a∈R, y(t)∈e(D)y(t)\in e(D)y(t)∈e(D) for some t>at > at>a and y(t′)∈e(D)y(t')\in e(D)y(t′)∈e(D) for some t′<at' < at′<a.

Conclusion (a conjunction of two statements).

  1. Unknotted: there is e:R2→R4e : \mathbb{R}^2\to\mathbb{R}^4e:R2→R4 that is C∞C^\inftyC∞, injective on DDD, with De(u)De(u)De(u) injective for u∈Du\in Du∈D, with e(D)⊆Σe(D)\subseteq\Sigmae(D)⊆Σ and e(S1)=x(R)e(S^1) = x(\mathbb{R})e(S1)=x(R). (These are exactly the first three conditions already contained in hDhDhD.)
  2. Self-linking number −1-1−1: there is ε0>0\varepsilon_0 > 0ε0​>0 such that for every ε\varepsilonε with 0<ε<ε00 < \varepsilon < \varepsilon_00<ε<ε0​, the linking number of the two loops
γ1(s)=x(Ts)∣x(Ts)∣,γ2ε(s)=x(Ts)+ε ξ1(x(Ts))∣x(Ts)+ε ξ1(x(Ts))∣(s∈R)\gamma_1(s) = \frac{x(Ts)}{|x(Ts)|}, \qquad \gamma_2^\varepsilon(s) = \frac{x(Ts) + \varepsilon\,\xi_1(x(Ts))}{|x(Ts) + \varepsilon\,\xi_1(x(Ts))|} \qquad (s\in\mathbb{R})γ1​(s)=∣x(Ts)∣x(Ts)​,γ2ε​(s)=∣x(Ts)+εξ1​(x(Ts))∣x(Ts)+εξ1​(x(Ts))​(s∈R)

equals −1-1−1, in the following sense:

  • (a) there exists N∈R4N\in\mathbb{R}^4N∈R4 with ∣N∣=1|N| = 1∣N∣=1 such that γ1(s)≠N\gamma_1(s)\neq Nγ1​(s)=N and γ2ε(s)≠N\gamma_2^\varepsilon(s)\neq Nγ2ε​(s)=N for all s∈Rs\in\mathbb{R}s∈R; and
  • (b) for every such NNN (unit, avoided by both loops for all sss), LkN(γ1,γ2ε)=−1\mathrm{Lk}_N(\gamma_1,\gamma_2^\varepsilon) = -1LkN​(γ1​,γ2ε​)=−1, where, with σN(y)=(1−⟨y,N⟩)−1(y−⟨y,N⟩N)\sigma_N(y) = (1 - \langle y,N\rangle)^{-1}\bigl(y - \langle y,N\rangle N\bigr)σN​(y)=(1−⟨y,N⟩)−1(y−⟨y,N⟩N) and VN(a,b,c)=det⁡V_N(a,b,c) = \detVN​(a,b,c)=det of the 4×44\times44×4 matrix with rows −N,a,b,c-N, a, b, c−N,a,b,c,
LkN(γ1,γ2)=14π∫01 ⁣ ⁣∫01VN(ddsσN(γ1(s)), ddtσN(γ2(t)), σN(γ1(s))−σN(γ2(t)))∣σN(γ1(s))−σN(γ2(t))∣3 dt ds.\mathrm{Lk}_N(\gamma_1,\gamma_2) = \frac{1}{4\pi}\int_0^1\!\!\int_0^1 \frac{V_N\Bigl(\tfrac{d}{ds}\sigma_N(\gamma_1(s)),\ \tfrac{d}{dt}\sigma_N(\gamma_2(t)),\ \sigma_N(\gamma_1(s)) - \sigma_N(\gamma_2(t))\Bigr)}{\bigl|\sigma_N(\gamma_1(s)) - \sigma_N(\gamma_2(t))\bigr|^3}\,dt\,ds .LkN​(γ1​,γ2​)=4π1​∫01​∫01​​σN​(γ1​(s))−σN​(γ2​(t))​3VN​(dsd​σN​(γ1​(s)), dtd​σN​(γ2​(t)), σN​(γ1​(s))−σN​(γ2​(t)))​dtds.

Edge cases and conventions. The push-off direction is the specific vector field ξ1\xi_1ξ1​ (built from Q2Q_2Q2​). In LkN\mathrm{Lk}_NLkN​: a derivative at a non-differentiable point is 000; the inner and outer integrals are 000 if their integrands are not integrable; a zero denominator makes the integrand 000; γ1\gamma_1γ1​, γ2ε\gamma_2^\varepsilonγ2ε​ evaluate to 000 where the vector being normalized is 000. Condition (b) ranges over all admissible unit NNN, and (a) asserts at least one exists. The first conjunct follows directly from the data in hDhDhD. Hypothesis hShShS(3) excludes 000 from Σ\SigmaΣ, so ∣x(Ts)∣>0|x(Ts)| > 0∣x(Ts)∣>0.

Human review
  • Endorsed by Shuze Chen · Oct 6, 2026

    Confirmed by the moderator at approval.

  • Endorsed by Mazecto · Oct 6, 2026

    Confirmed by the mission captain (proposal self-audit).

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