A family of holomorphic maps through an embedded fast plane, for a given decay rate
OpenFiniteEnergyPlane.exists_jHolomorphic_family_of_windowLet be strictly star-shaped, a compatible complex structure on , and the induced almost complex structure on the symplectization . Let be a periodic Reeb orbit with and let be an embedded fast finite-energy plane asymptotic to at . Let be a number that is not an eigenvalue of the asymptotic operator , such that every eigenvalue of below has winding number at most and every eigenvalue above has winding number at least .
Then for every there are and a map , of class on , with , such that for every :
- is smooth, avoids , is -holomorphic and asymptotic to at ;
- there is with for all ;
- there is such that for every some satisfies .
Moreover implies , , , and for every there is such that is -close to in the sense of IsCylCloseTo for all .
The statement produces a one-parameter family of holomorphic maps through a fast plane, transverse to the translation direction at one point, with controlled decay at the puncture; it is the existence part of the local structure of the space of fast planes near .
Formalization Note: the plane is a map u : ℂ → V 1 with V 1 = ℝ⁴; proj H is the radial projection to ; IsNondegenerateEnd H u cylInf P 1 is asymptotic convergence to at with sign ; HasEigenWind J P μ k says is an eigenvalue of all of whose eigenvectors have winding ; fderiv ℝ g (z, t) (Δ, 1) is .
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, for a given rate `δ`. Let `u`
be an embedded fast finite-energy plane asymptotic to `P` at `∞`, where the Conley–Zehnder index of
`P` is at least `3`, and let `δ < 0` be a number that is not an eigenvalue of `A_P`, 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`. Then 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 `∞`; the distance from `proj (g(z, t))` to the
image of `P` is at most `C (1 + ‖z‖)^{δ/2π}`; and some `Δ` has
`‖Dg(z, t)(Δ, 1)‖ ≤ C (1 + ‖z‖)^{δ/2π} ‖g(z, t)‖`. At `(z, t) = (0, 0)`,
`Dg(0, 0)(Δ, δt) + λ • g(0, 0) = 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_window (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) (δ : ℝ) (hδ : δ < 0) (hδe : ∀ v, ¬ IsAsymptoticEigen J P δ v)
(hwin : ∀ (μ : ℝ) (k : ℤ), HasEigenWind J P μ k → (μ < δ ∧ k ≤ 1) ∨ (δ < μ ∧ 2 ≤ k))
(l : ℕ) (hl : 1 ≤ l) :
∃ 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)) ∧
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, 0) (Δ, δt) + lam • g (0, 0) = 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