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A close J-holomorphic plane approaching the orbit at a window rate is fast

Proved
FiniteEnergyPlane.isFastPlane_of_infDist_le

by Mazecto · Nov 6, 2026 · Mathlib 0df444a (Lean v4.33.1)

pseudoholomorphic-curvessymplectic-geometry

Let S=H−1(1)⊂R4S = H^{-1}(1) \subset \mathbb{R}^4S=H−1(1)⊂R4 be a strictly star-shaped level with a compatible complex structure JJJ on the contact planes, and let PPP be a periodic Reeb orbit. Let uuu be a fast finite-energy plane asymptotic to PPP at ∞\infty∞, and let δ<0\delta < 0δ<0 be such that every eigenvalue of the asymptotic operator APA_PAP​ below δ\deltaδ has winding number at most 111 and every eigenvalue above δ\deltaδ has winding number at least 222, in the global frame of ξ\xiξ.

Let f:C→V1f : \mathbb{C} \to V_1f:C→V1​ be smooth, avoid 000, be J~\tilde JJ~-holomorphic and asymptotic to PPP at ∞\infty∞ (IsNondegenerateEnd), and be ε\varepsilonε-close to uuu in the sense of IsCylCloseTo for some ε\varepsilonε. If dist⁡(proj⁡f(z),P(R))≤C(1+∣z∣)δ/2π\operatorname{dist}(\operatorname{proj} f(z), P(\mathbb{R})) \le C (1 + |z|)^{\delta / 2\pi}dist(projf(z),P(R))≤C(1+∣z∣)δ/2π for all zzz, then fff is a fast finite-energy plane (IsFastPlane).

Role. It identifies the members of a family of J~\tilde JJ~-holomorphic maps near a fast plane as fast planes, as in Hryniewicz (Trans. AMS 2012), Lemma 6.18. In particular, finiteness of the energy of fff is part of the conclusion.

Formalization Note. The symplectization R×S\mathbb{R} \times SR×S is V1∖{0}V_1 \setminus \{0\}V1​∖{0}, with y=e2axy = e^{2a} xy=e2ax, aaa = aCoord H y and xxx = proj H y. Winding numbers are HasEigenWind; (1+∣z∣)δ/2π(1 + |z|)^{\delta/2\pi}(1+∣z∣)δ/2π is the cylindrical weight eδse^{\delta s}eδs for ∣z∣=e2πs|z| = e^{2\pi s}∣z∣=e2πs. PPP may be degenerate, and ε\varepsilonε need not be small.

Preamble
import Definitions.Def_FiniteEnergyPlane_CylClose
Formal statement
namespace FiniteEnergyPlane

open MeasureTheory Metric Filter Topology
open scoped ContDiff ENNReal Real

/-- A `J̃`-holomorphic plane close to a fast plane that approaches the orbit at a window rate is
fast. Let `u` be a fast finite-energy plane asymptotic to `P` at `∞`, and let `δ < 0` be such that
every eigenvalue of `A_P` below `δ` has winding number at most `1` and every eigenvalue above `δ`
has winding number at least `2`. Let `f : ℂ → V 1` be smooth, avoid `0`, be `J̃`-holomorphic and
asymptotic to `P` at `∞`, be `ε`-close to `u` in the sense of `IsCylCloseTo` for some `ε`, and have
distance from `proj (f z)` to the image of `P` at most `C (1 + ‖z‖)^{δ/2π}`. Then `f` is a fast
finite-energy plane. -/
theorem isFastPlane_of_infDist_le (H : V 1 → ℝ) (hH : IsStrictlyStarShapedLevel H)
    (J : V 1 → V 1 →L[ℝ] V 1) (hJ : IsCompatibleXiStructure H J)
    (P : ReebOrbit H) (u : ℂ → V 1)
    (hu : IsFastPlane H J u) (huP : IsNondegenerateEnd H u cylInf P 1)
    (δ : ℝ) (hδ : δ < 0)
    (hwin : ∀ (μ : ℝ) (k : ℤ), HasEigenWind J P μ k → (μ < δ ∧ k ≤ 1) ∨ (δ < μ ∧ 2 ≤ k))
    (ε : ℝ) (f : ℂ → V 1) (hf : ContDiff ℝ ∞ f) (hf0 : ∀ z, f z ≠ 0)
    (hfJ : JHolomorphic.IsJHolomorphicOn (Jtilde H J) Set.univ f)
    (hfP : IsNondegenerateEnd H f cylInf P 1) (hclose : IsCylCloseTo H ε f u)
    (C : ℝ) (hrate : ∀ z, infDist (proj H (f z)) (Set.range P.x) ≤
      C * (1 + ‖z‖) ^ (δ / (2 * π))) :
    IsFastPlane H J f := by
  sorry

end FiniteEnergyPlane
Source
U. Hryniewicz, Fast finite-energy planes in symplectizations and applications, Trans. AMS 364 (2012), arXiv:0812.4076, Lemma 6.10 and Lemma 6.20

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