A family of J-holomorphic maps through an embedded fast plane
OpenFiniteEnergyPlane.exists_jHolomorphic_family_of_fastPlaneLet be a strictly star-shaped level with a compatible complex structure on the contact planes, and let be a periodic Reeb orbit. Assume the Conley–Zehnder index of is at least (P.IsCZAtLeast 3; may be degenerate), and let be an embedded fast finite-energy plane asymptotic to at .
Then there is such that every eigenvalue of the asymptotic operator below has winding number at most and every eigenvalue above has winding number at least , in the global frame of , and for every integer there are and a map with such that:
- for every , the map is smooth, avoids , is -holomorphic and asymptotic to at (
IsNondegenerateEnd), and is smooth; - for every there is with for all ;
- for every there is such that for every some has ;
- for every , the identity forces , and ;
- for every there is such that is -close to in the sense of
IsCylCloseTofor all .
Role. This is the existence part of the family of fast planes through in Hryniewicz (Trans. AMS 2012), Lemma 6.10.
Formalization Note. The symplectization is , with , = aCoord H y and = proj H y. Winding numbers are HasEigenWind; is the cylindrical weight for . Clause 3 measures the -derivative modulo the tangent plane of the member, relative to , which is the -invariant size in the symplectization. Clause 2 compares with the image of , not with a parametrization.
import Definitions.Def_FiniteEnergyPlane_CylClose
namespace FiniteEnergyPlane
open MeasureTheory Metric Filter Topology
open scoped ContDiff ENNReal Real
/-- A family of `J̃`-holomorphic maps through an embedded fast plane. Let `u` be an embedded fast
finite-energy plane asymptotic to `P` at `∞`, where the Conley–Zehnder index of `P` is at least `3`.
Then there is `δ < 0` 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`, and for every `l ≥ 1` there are
`r > 0` and a `C^l` map `g : ℂ × (-r, r) → V 1` with `g(·, 0) = u` such that for every `t`: `g(·, t)`
is smooth, avoids `0`, is `J̃`-holomorphic and asymptotic to `P` at `∞`; `∂ₜg(·, t)` is smooth; the
distance from `proj (g(z, t))` to the image of `P` is at most `C (1 + ‖z‖)^{δ/2π}`; some `Δ` has
`‖Dg(z, t)(Δ, 1)‖ ≤ C (1 + ‖z‖)^{δ/2π} ‖g(z, t)‖`; and at `z = 0`,
`Dg(0, t)(Δ, δt) + λ • g(0, t) = 0` forces `Δ = 0`, `δt = 0`, `λ = 0`. Moreover `g(·, t)` tends to
`u` in the sense of `IsCylCloseTo` as `t → 0`. -/
theorem exists_jHolomorphic_family_of_fastPlane (H : V 1 → ℝ) (hH : IsStrictlyStarShapedLevel H)
(J : V 1 → V 1 →L[ℝ] V 1) (hJ : IsCompatibleXiStructure H J)
(P : ReebOrbit H) (hcz : P.IsCZAtLeast 3) (u : ℂ → V 1)
(hu : IsFastPlane H J u) (huP : IsNondegenerateEnd H u cylInf P 1)
(hue : IsEmbeddedPlane u) (l : ℕ) (hl : 1 ≤ l) :
∃ δ < 0, (∀ (μ : ℝ) (k : ℤ), HasEigenWind J P μ k → (μ < δ ∧ k ≤ 1) ∨ (δ < μ ∧ 2 ≤ k)) ∧
∃ r > 0, ∃ g : ℂ × ℝ → V 1, ContDiffOn ℝ l g (Set.univ ×ˢ Set.Ioo (-r) r) ∧
(∀ z, g (z, 0) = u z) ∧
(∀ t ∈ Set.Ioo (-r) r,
ContDiff ℝ ∞ (fun z => g (z, t)) ∧ (∀ z, g (z, t) ≠ 0) ∧
JHolomorphic.IsJHolomorphicOn (Jtilde H J) Set.univ (fun z => g (z, t)) ∧
ContDiff ℝ ∞ (fun z => fderiv ℝ g (z, t) (0, 1)) ∧
IsNondegenerateEnd H (fun z => g (z, t)) cylInf P 1 ∧
(∃ C : ℝ, ∀ z, infDist (proj H (g (z, t))) (Set.range P.x) ≤
C * (1 + ‖z‖) ^ (δ / (2 * π))) ∧
(∃ C : ℝ, ∀ z, ∃ Δ : ℂ, ‖fderiv ℝ g (z, t) (Δ, 1)‖ ≤
C * (1 + ‖z‖) ^ (δ / (2 * π)) * ‖g (z, t)‖) ∧
∀ (Δ : ℂ) (δt lam : ℝ), fderiv ℝ g (0, t) (Δ, δt) + lam • g (0, t) = 0 →
Δ = 0 ∧ δt = 0 ∧ lam = 0) ∧
∀ ε > 0, ∃ r' ∈ Set.Ioc 0 r, ∀ t ∈ Set.Ioo (-r') r',
IsCylCloseTo H ε (fun z => g (z, t)) u := by
sorry
end FiniteEnergyPlane