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Limits of normalized fast planes keep the asymptotic orbit at ∞\infty∞

Proved
FiniteEnergyPlane.isNondegenerateEnd_cylInf_of_tendstoCInftyLocOn

by Mazecto · Nov 4, 2026 · Mathlib 0df444a (Lean v4.33.1)

compactnesspseudoholomorphic-curvesreeb-dynamicssymplectization

Let P=(x,T)P=(x,T)P=(x,T) be a periodic Reeb orbit on a strictly star-shaped level S⊂R4S\subset\mathbb{R}^4S⊂R4 such that every periodic orbit of period at most TTT is nondegenerate, and let 0<γ0<\gamma0<γ be smaller than every such period and every difference of two distinct such periods. Let uku_kuk​ be a sequence in the set Θ(K,P)\Theta(K,P)Θ(K,P) of fast finite-energy planes asymptotic to PPP at ∞\infty∞ with uk(0)∈Ku_k(0)\in Kuk​(0)∈K and dλd\lambdadλ-energy γ\gammaγ outside the closed unit disk. Suppose a sequence of radial rescalings of the uku_kuk​ converges in Cloc∞(C∖Γ)C^\infty_{\mathrm{loc}}(\mathbb{C}\setminus\Gamma)Cloc∞​(C∖Γ), with Γ\GammaΓ a finite subset of the closed unit disk, to a finite-energy J~\tilde JJ~-holomorphic curve www on C∖Γ\mathbb{C}\setminus\GammaC∖Γ. Then www has a nondegenerate positive puncture at ∞\infty∞ over PPP, and the action of www on circles of radius ρ\rhoρ tends to TTT as ρ→∞\rho\to\inftyρ→∞.

This identifies the behaviour at ∞\infty∞ of every limit of such a sequence.

Formalization Note R4∖{0}≅R×S\mathbb{R}^4\setminus\{0\}\cong\mathbb{R}\times SR4∖{0}≅R×S is V 1 \ {0}, with aaa = aCoord H and pr\mathrm{pr}pr = proj H; Θ\ThetaΘ = fastPlaneSet H J P K γ. The rescaling is (Real.exp (-(2 * a_k 2))) • u_k; the end is IsNondegenerateEnd H w cylInf P 1, and the action is loopAction H w (ccwLoop ρ).

Preamble
import Definitions.Def_FiniteEnergyPlane_Compactness
Formal statement
namespace FiniteEnergyPlane

open MeasureTheory Metric Filter Topology
open scoped ContDiff ENNReal Real

/-- Let `P` and `γ` be as in `exists_loop_near_orbit_of_mem_fastPlaneSet`, let `uₖ` be a sequence in
`fastPlaneSet H J P K γ`, and suppose the shifted planes `e^{-2aₖ(2)} • uₖ` converge in
`C^∞_loc(ℂ \ Γ)` to a finite-energy `J̃`-holomorphic curve `w` on `ℂ \ Γ`, with `Γ` a finite subset
of the closed unit disk. Then `w` has a nondegenerate positive puncture at `∞` over the same orbit
`P`, and the actions `∫_{|z| = ρ} w*λ` tend to `P.T` as `ρ → ∞`. -/
theorem isNondegenerateEnd_cylInf_of_tendstoCInftyLocOn (H : V 1 → ℝ)
    (hH : IsStrictlyStarShapedLevel H) (J : V 1 → V 1 →L[ℝ] V 1) (hJ : IsCompatibleXiStructure H J)
    (P : ReebOrbit H) (hnd : ∀ Q : ReebOrbit H, Q.T ≤ P.T → Q.IsNondegenerate)
    (γ : ℝ) (hγ : 0 < γ) (hγ₁ : ∀ Q : ReebOrbit H, Q.T ≤ P.T → γ < Q.T)
    (hγ₂ : ∀ Q₁ Q₂ : ReebOrbit H, Q₁.T ≤ P.T → Q₂.T ≤ P.T → Q₁.T ≠ Q₂.T → γ < |Q₁.T - Q₂.T|)
    (K : Set (V 1)) (u : ℕ → ℂ → V 1) (hu : ∀ k, u k ∈ fastPlaneSet H J P K γ)
    (Γ : Finset ℂ) (hΓ : ∀ z ∈ Γ, ‖z‖ ≤ 1) (w : ℂ → V 1) (hw : IsFiniteEnergyCurve H J (↑Γ)ᶜ w)
    (hconv : JHolomorphic.TendstoCInftyLocOn
      (fun k z => Real.exp (-(2 * aCoord H (u k 2))) • u k z) w (↑Γ)ᶜ) :
    IsNondegenerateEnd H w cylInf P 1 ∧
      Tendsto (fun ρ : ℝ => loopAction H w (ccwLoop ρ)) atTop (𝓝 P.T) := by
  sorry

end FiniteEnergyPlane
Source
U. Hryniewicz, Trans. AMS 364 (2012), arXiv:0812.4076, Section 4 (Lemma 4.17 and its proof)

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