Non-degenerate approximations fixing an unknotted orbit with , whose low-action orbits eventually have index : the orbit eventually bounds a disk-like global section
OpenHryniewiczCriterion.bounds_global_section_of_approx_of_eventually_czIndex_ge_threeLet be a strictly star-shaped level and let be a prime periodic orbit on that is unknotted with . Let be Hamiltonians such that
- every level is strictly star-shaped and every is non-degenerate;
- and at every point of ;
- in ;
- for every action bound there is such that for every periodic orbit on with has .
Then for all large , , viewed as a periodic orbit of (any with the same parametrization and period ), bounds a disk-like global surface of section for the flow on .
in means: for every and every compact , uniformly on . A Hamiltonian is non-degenerate when for every periodic orbit on (prime or not) and its linearized flow , the linearized return map on , written in the global frame as the matrix of linearizedXiPath, does not have as an eigenvalue. The action of a periodic orbit is , with the Liouville form (liouvilleForm). The Conley–Zehnder index is czIndexOfPath of the linearized flow on written in the global frame (linearizedXiPath), with its lower semicontinuous extension to degenerate orbits.
Hypothesis 4 controls only orbits of bounded action, so the levels are not assumed dynamically convex, and the limit level is not assumed dynamically convex or non-degenerate. In Hryniewicz's notation carries the non-degenerate contact form with , , on (his (29)). This is the step of his Section 3 that produces disk-like global sections for when is large.
import Definitions.Def_HryniewiczCriterion_ConleyZehnder import Definitions.Def_HryniewiczCriterion_GlobalSection import Definitions.Def_HryniewiczCriterion_SelfLinking open HryniewiczCriterion
theorem HryniewiczCriterion.bounds_global_section_of_approx_of_eventually_czIndex_ge_three (H : R4 → ℝ) (hS : IsStrictlyStarShapedLevel H)
(P : PeriodicOrbit H) (hP : P.IsPrime) (hu : IsUnknotted H P)
(hsl : HasSelfLinkingNumber H P (-1))
(Hs : ℕ → R4 → ℝ) (hSk : ∀ k, IsStrictlyStarShapedLevel (Hs k))
(hnd : (∀ k (R : PeriodicOrbit (Hs k)) (Y : ℝ → (R4 →L[ℝ] R4)), IsLinearizedFlow (Hs k) R.x Y →
∀ v : Fin 2 → ℝ, (linearizedXiPath (Hs k) R Y 1).mulVec v = v → v = 0))
(hjet : ∀ k, ∀ y ∈ P.image, Hs k y = H y ∧ fderiv ℝ (Hs k) y = fderiv ℝ H y)
(hconv : (∀ m : ℕ, ∀ K : Set R4, IsCompact K →
TendstoUniformlyOn (fun k => iteratedFDeriv ℝ m (Hs k)) (iteratedFDeriv ℝ m H) Filter.atTop K))
(hcz : ∀ A : ℝ, ∃ K : ℕ, ∀ k, K ≤ k → ∀ (R : PeriodicOrbit (Hs k)) (Y : ℝ → (R4 →L[ℝ] R4)),
IsLinearizedFlow (Hs k) R.x Y → (∫ t in (0 : ℝ)..R.T, liouvilleForm (R.x t) (deriv R.x t)) ≤ A →
3 ≤ czIndexOfPath (linearizedXiPath (Hs k) R Y)) :
∃ K : ℕ, ∀ k, K ≤ k → ∀ Pk : PeriodicOrbit (Hs k), Pk.x = P.x → Pk.T = P.T →
BoundsDiskLikeGlobalSection (Hs k) Pk := by sorry