Let S=H−1(1)⊂R4 be a strictly star-shaped energy surface whose flow is dynamically convex. Let Pˉ be a prime periodic orbit on S. If Pˉ bounds a disk-like global surface of section, then
Pˉis 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.
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→R be any function; coordinates are x=(x0,…,x3), DH(x) is the Fréchet derivative (taken to be 0 where not differentiable), Σ={H=1}, and
A trajectory is y:R→R4 with y′(t)=XH(y(t)) and H(y(t))=1 for all t. A periodic orbit is a trajectory x with a real T>0 and x(t+T)=x(t) for all t (T not necessarily minimal).
Notation: D,D˚,S1⊂R2 are the closed unit disk, open unit disk and unit circle; ⟨a,b⟩=∑iaibi, ∣a∣=⟨a,a⟩; ω0(u,v)=u0v1−u1v0+u2v3−u3v2; λx(v)=21(x0v1−x1v0+x2v3−x3v2); Q1x=(−x2,x3,x0,−x1), Q2x=(x3,x2,−x1,−x0);
hS (strictly star-shaped level):H is C∞ on R4; for every u=0 there is exactly one r>0 with H(ru)=1; and DH(x)x>0 for every x∈Σ.
hdc (dynamically convex): for every periodic orbit (x,T) of H (of any, not necessarily minimal, period) and every Y:R→L(R4,R4) with Y(0)=id and Y′(t)=DXH(x(t))∘Y(t) for all t, the integer μ(M)≥3, where M(τ) is the 2×2 matrix
and for a matrix path φ: W(φ) is the set of (θ(1)−s)/(2π) over s∈[0,2π] and θ continuous on [0,1] with θ(0)=s and φ(t)(coss,sins)∈R>0(cosθ(t),sinθ(t)) for t∈[0,1]; a=infW, b=supW (both 0 if W is empty or unbounded on that side); μ(φ)=2(⌈b⌉−1) if a≤⌈b⌉−1, else 2⌈b⌉−1.
P: a periodic orbit (x,T) of H.
hP (prime):x(t)=x(0) for all 0<t<T.
hD (bounds a disk-like global section): there is e:R2→R4 such that: e is C∞, injective on D, with De(u) injective for every u∈D; e(D)⊆Σ; e(S1)=x(R); XH(e(u))∈/rangeDe(u) for every u∈D˚; and every trajectory y with y(0)∈/x(R) satisfies, for every a∈R, y(t)∈e(D) for some t>a and y(t′)∈e(D) for some t′<a.
Conclusion (a conjunction of two statements).
Unknotted: there is e:R2→R4 that is C∞, injective on D, with De(u) injective for u∈D, with e(D)⊆Σ and e(S1)=x(R). (These are exactly the first three conditions already contained in hD.)
Self-linking number −1: there is ε0>0 such that for every ε with 0<ε<ε0, the linking number of the two loops
(a) there exists N∈R4 with ∣N∣=1 such that γ1(s)=N and γ2ε(s)=N for all s∈R; and
(b) for every such N (unit, avoided by both loops for all s), LkN(γ1,γ2ε)=−1, where, with σN(y)=(1−⟨y,N⟩)−1(y−⟨y,N⟩N) and VN(a,b,c)=det of the 4×4 matrix with rows −N,a,b,c,
Edge cases and conventions. The push-off direction is the specific vector field ξ1 (built from Q2). In LkN: a derivative at a non-differentiable point is 0; the inner and outer integrals are 0 if their integrands are not integrable; a zero denominator makes the integrand 0; γ1, γ2ε evaluate to 0 where the vector being normalized is 0. Condition (b) ranges over all admissible unit N, and (a) asserts at least one exists. The first conjunct follows directly from the data in hD. Hypothesis hS(3) excludes 0 from Σ, so ∣x(Ts)∣>0.
Confirmed by the moderator at approval.