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 that is unknotted with sl(Pˉ)=−1. Then Pˉ is the binding of an open book decomposition of S with disk-like pages, adapted to the flow: every page is a disk-like global surface of section whose oriented boundary is Pˉ.
This strengthens the "if" direction of Hryniewicz's criterion from a single disk to a whole family of disk-like global sections that fill S∖Pˉ.
namespace HryniewiczCriterion
/-- Hryniewicz, Theorem 1.7, second sentence: a prime, unknotted periodic orbit with
`sl = -1` of a dynamically convex flow is the binding of an adapted open book
decomposition with disk-like pages. -/
theorem adapted_open_book_of_unknotted_selfLinking (H : R4 → ℝ)
(hS : IsStrictlyStarShapedLevel H) (hdc : IsDynamicallyConvex H)
(P : PeriodicOrbit H) (hP : P.IsPrime)
(hu : IsUnknotted H P) (hsl : HasSelfLinkingNumber H P (-1)) :
HasAdaptedDiskOpenBook H P := 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, second sentence
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What the Lean code literally says, in plain math · claude-opus-5-5
Binders and hypotheses. Let H:R4→R be any function, and assume:
(hS) the level Σ=H−1(1) is a strictly star-shaped level of H (H is C∞, each ray from the origin meets Σ exactly once, and DH(x)x>0 on Σ);
(hdc)H is dynamically convex (every periodic orbit, of every period, with every linearized flow, has index μ≥3; see below);
P is a periodic orbit of XH on Σ (a trajectory xP with a period TP>0);
(hP)P is prime: xP(t)=xP(0) for 0<t<TP;
(hu)P is unknotted: there is a C∞ map e:R2→R4, injective with injective derivative on the closed unit disk D, with e(D)⊆Σ and e(S1)=imP;
(hsl)P has self-linking number −1: there is ε0>0 such that for all 0<ε<ε0 the loops ℓP(s)=ν(xP(TPs)) and ℓPε(s)=ν(xP(TPs)+εξ1(xP(TPs))) have linking number −1 in the Gauss-integral sense defined below.
Conclusion.P has an adapted disk open book: there exists F:R×R2→R4, F(ϑ,u)=Fϑ(u), jointly C∞ and 1-periodic in ϑ, such that
every page Fϑ is a disk-like global section map for (H,P) (smooth disk embedding of D into Σ with boundary circle mapped onto imP, XH not tangent to the page at interior points, and every trajectory not starting on imP meets Fϑ(D) both after and before every time a);
Fϑ(cos2πt,sin2πt)=xP(TPt) for all ϑ,t;
ω0(∂u0Fϑ,∂u1Fϑ)>0 on the open disk D;
every point of Σ∖imP is F(ϑ,u) for exactly one (ϑ,u)∈[0,1)×D;
DF(ϑ,u) is injective for all ϑ∈R, u∈D.
Edge cases. The binding condition fixes the boundary parametrization of every page to t↦xP(TPt) with the given base point xP(0) and the given direction of c(t)=(cos2πt,sin2πt). The positivity condition fixes an orientation of each page relative to ω0. This is an implication only (no converse is stated).
Unfolded definitions used above
Throughout, R4 is the space of functions {0,1,2,3}→R (with the sup norm as its normed-space structure), points are written x=(x0,x1,x2,x3), and R2 (points u=(u0,u1)) is likewise {0,1}→R. DH(x) denotes the Fréchet derivative of H at x, which is by convention the zero map wherever H is not differentiable; similarly for every other derivative below. Divisions by 0 and inverses of 0 evaluate to 0.
Euclidean inner product and norm: ⟨x,y⟩=∑i=03xiyi, ∣x∣=⟨x,x⟩.
Partial derivatives ∂iH(x)=DH(x)ei (ei the i-th standard basis vector), and the Hamiltonian vector field
XH(x)=(−∂1H(x),∂0H(x),−∂3H(x),∂2H(x)).
Energy surface Σ={x∈R4:H(x)=1}.
Strictly star-shaped level (hypothesis hS): (i) H:R4→R is C∞ on all of R4; (ii) for every u=0 there is exactly one r>0 with H(ru)=1; (iii) for every x with H(x)=1, DH(x)x>0. (Consequence of (iii): H(0)=1, so 0∈/Σ, and XH=0 on Σ.)
Trajectory: a map y:R→R4 that is differentiable at every t∈R with y′(t)=XH(y(t)), and with H(y(t))=1 for all t∈R.
Periodic orbitP: a pair (xP,TP) consisting of a trajectory xP:R→R4 and a number TP>0 with xP(t+TP)=xP(t) for all t. TP is a period, not necessarily the minimal one; the same geometric orbit gives many different P (any time shift, any positive multiple of the minimal period). Its image is imP={xP(t):t∈R}.
Prime: xP(t)=xP(0) for all 0<t<TP (i.e. TP is the minimal period).
Two fixed linear maps Q1(x)=(−x2,x3,x0,−x1) and Q2(x)=(x3,x2,−x1,−x0), and the frame vectors
Given a path of real 2×2 matrices φ:R→M2(R) and s∈R, an angle lift from s is a function θ:R→R, continuous on [0,1], with θ(0)=s, such that for every t∈[0,1] there is r>0 with φ(t)ρ(s)=rρ(θ(t)). (No continuity or invertibility of φ is assumed; if φ(t)ρ(s)=0 for some t∈[0,1], no lift from s exists.)
Winding set W(φ)={2πθ(1)−s:s∈[0,2π],θ an angle lift of φ from s}⊆R.
Index: let a=infW(φ), b=supW(φ) (each set to 0 if W(φ) is empty or unbounded on that side), and k=⌈b⌉ (least integer ≥b). Then
μ(φ)={2(k−1)2k−1if a≤k−1,otherwise.
In particular, if W(φ)=∅ then a=b=0, k=0 and μ(φ)=−1.
A linearized flow along a curve x:R→R4 is a map Y:R→L(R4,R4) (continuous linear maps) with Y(0)=Id and, for every t∈R, Y differentiable at t with Y′(t)=DXH(x(t))∘Y(t), where DXH is the Fréchet derivative of the vector field XH.
Projection along XH: πx(v)=v−λx(XH(x))λx(v)XH(x).
H is dynamically convex means: for every periodic orbit P (any period TP, so including all multiple covers and time shifts) and every linearized flow Y along xP, μ(ΦP,Y)≥3. (If for some P no linearized flow exists, the condition is vacuous for that P.)
Disks and global sections.
D={u:u02+u12≤1}, D={u:u02+u12<1}, S1={u:u02+u12=1}, and c(t)=(cos2πt,sin2πt).
Smooth disk embeddinge:R2→R4: e is C∞ on all of R2, injective on D, and De(u) is injective for every u∈D.
Disk-like global section map for (H,P): a map e:R2→R4 such that
e is a smooth disk embedding;
e(D)⊆Σ;
e(S1)=imP (set equality);
for every u∈D (open disk), XH(e(u))∈/rangeDe(u);
for every trajectory y with y(0)∈/imP and every a∈R, there exist t>a with y(t)∈e(D) and t′<a with y(t′)∈e(D) (the hitting set is the image of the closed disk).
No orientation condition is imposed.
P bounds a disk-like global section: some disk-like global section map for (H,P) exists.
P is unknotted: there is a smooth disk embedding e with e(D)⊆Σ and e(S1)=imP (conditions 1–3 above only).
Adapted disk open book for (H,P): a map F:R×R2→R4, F(ϑ,u)=Fϑ(u), such that
F is jointly C∞;
Fϑ+1=Fϑ for all ϑ;
every page Fϑ is a disk-like global section map for (H,P);
(binding) Fϑ(c(t))=xP(TPt) for all ϑ,t∈R;
(positivity) for all ϑ and u∈D, ω0(∂u0Fϑ(u),∂u1Fϑ(u))>0;
(fibration) every y∈Σ∖imP equals F(ϑ,u) for exactly one pair (ϑ,u) with ϑ∈[0,1), u∈D;
(regularity) for all ϑ∈R and u∈D, the derivative DF(ϑ,u):R×R2→R4 is injective.
"P has an adapted disk open book" means such an F exists. (Since each page is injective on D, the binding condition forces t↦xP(TPt) to be injective on [0,1), i.e. P prime.)
Linking and self-linking.
ν(x)=x/∣x∣ (with ν(0)=0).
For N∈R4, the map σN(y)=1−⟨y,N⟩y−⟨y,N⟩N (equal to 0 when ⟨y,N⟩=1), with values in R4.
volN(a,b,c)=det of the 4×4 matrix with rows −N,a,b,c.
Gauss integral of two curves γ1,γ2:R→R4 with respect to N: writing α(s)=σN(γ1(s)), β(t)=σN(γ2(t)),
where derivatives are 0 at non-differentiability points, the integrand is 0 where α(s)=β(t), and an interval integral of a non-integrable function is 0.
γ1,γ2 have linking number n∈Z: (a) there exists N with ∣N∣=1 such that γ1(s)=N and γ2(s)=N for all s∈R; and (b) for everyN with ∣N∣=1 avoiding both curves on all of R in that sense, GN(γ1,γ2)=n. (Avoidance is required over all s∈R; the integral uses only [0,1]. The curves are not required to be closed or smooth.)
Orbit loop ℓP(s)=ν(xP(TPs)); push-off loop ℓPε(s)=ν(xP(TPs)+εξ1(xP(TPs))). Over s∈[0,1] these traverse the period TP, which is the minimal period only if P is prime.
P has self-linking number n: there is ε0>0 such that for every ε∈(0,ε0), the curves ℓP,ℓPε have linking number n (in the sense above).
P links Q nontrivially: there is an integer n=0 such that ℓP,ℓQ have linking number n.
Confirmed by the moderator at approval.