Read-back: FiniteEnergyPlane.one_le_windInf_of_plane
Setting. Here V=R4 with coordinates (v0,v1,v2,v3), and
j0(v)=(−v1,v0,−v3,v2),ω0(u,v)=⟨j0u,v⟩=u0v1−u1v0+u2v3−u3v2,λx(v)=21ω0(x,v).
The gradient of H is taken coordinatewise, XH(x)=j0(∇H(x)), and the Reeb field is R(x)=λx(XH(x))−1XH(x). If λx(XH(x))=0, the inverse is 0 by convention, so R(x)=0. The energy surface is S={H=1}. The contact plane condition "v∈ξx" means λx(v)=0 and dHx(v)=0.
Data and hypotheses. Let:
- H:R4→R be strictly star-shaped: H is C∞; for every u=0 there is exactly one r>0 with H(ru)=1; and dHx(x)>0 whenever H(x)=1.
- J:R4→L(R4,R4) be a compatible ξ-structure: J is C∞, and for every x∈S and every v,w∈ξx we have Jxv∈ξx, JxJxv=−v, ω0(v,Jxv)>0 if v=0, and ω0(Jxv,Jxw)=ω0(v,w). Nothing is required of Jx off ξx or for x∈/S.
- u:C→R4 be a finite-energy curve on all of C. This means:
- u is C∞ on C and u(z)=0 for every z;
- u is J~-holomorphic at every z: u is differentiable there and ∂su+J~(u)∂tu=0, where ∂s and ∂t are the derivatives in the directions 1 and i;
- E(u)<∞, with E and J~ as defined below.
- P be a Reeb orbit of H: a map x:R→R4 and a number T>0 with x(τ)∈S, x′(τ)=R(x(τ)) and x(τ+T)=x(τ) for all τ. The period T need not be minimal, and P is not assumed prime or nondegenerate.
- u have a "nondegenerate end" at ∞ asymptotic to P with sign ε=1; see "Ends" below.
Auxiliary notions.
- σ(y) is a chosen r>0 with H(ry)=1 if such an r exists, and σ(y)=1 otherwise. For y=0 this r is unique. For y=0 with H(0)=1, it is an arbitrary positive choice.
- proj(y)=σ(y)y and a(y)=−21logσ(y).
- J~(y) is defined as follows. Put x=proj(y), r=σ(y), α(v)=rdHx(v)/(2dHx(x)), β(v)=rλx(v) and w(v)=v−α(v)2y−β(v)r−1R(x). Then
J~(y)v=α(v)r−1R(x)−β(v)2y+Jx(w(v)).
- Write au=a∘u and wu=proj∘u. Then
E(u)=φsup∫Cmax(0, φ′(au)(∂sauλwu(∂twu)−∂tauλwu(∂swu))+φ(au)ω0(∂swu,∂twu))dz.
The supremum runs over C∞ monotone φ:R→[0,1]. The integral is a lower Lebesgue integral with values in [0,∞], so the integrand is the positive part of the density.
Ends. Let e(s,t)=e2πse2πit and W(s,t)=proj(u(e(s,t))). The condition "nondegenerate end at ∞ asymptotic to P with ε=1" means that there are d,c,b∈R with b>0 such that, uniformly in t∈R as s→+∞,
a(u(e(s,t)))−Ts−d→0andebs(W(s,t)−x(Tt+c))→0.
This condition is only exponential uniform convergence of the end. It says nothing about the linearized return map of P.
Winding. A function f:R→C has loop winding k∈Z if all of the following hold:
- f is continuous and 1-periodic, and never zero;
- there is a continuous θ:R→R with f(t)=∣f(t)∣eiθ(t) for all t;
- θ(1)−θ(0)=2πk.
The ξ-coordinate map ξC(x,v)∈C is
ξC(x,v)=ω0(v,f2(x))+iω0(f1(x),v),
with frames
f1(x)=∣x∣−1(Q2x−dHx(x)dHx(Q2x)x),f2(x)=∣x∣−1(Q1x−dHx(x)dHx(Q1x)x),
where Q1x=(−x2,x3,x0,−x1) and Q2x=(x3,x2,−x1,−x0). As usual, ∣x∣ is the Euclidean norm, and division by 0 gives 0.
The Reeb-removing map is πξ(x,v)=v−λx(v)R(x).
"u has winding k at ∞" means: there is s0 such that for every s≥s0, the loop
t↦ξC(W(s,t), πξ(W(s,t), ∂sW(s,t)))
has loop winding k. Here ∂sW is the Fréchet derivative of W on R2 applied to (1,0), which is 0 by convention wherever W is not differentiable.
Conclusion. Under all these hypotheses, there is an integer k with
k≥1
such that u has winding k at ∞ in the sense just described.
Confirmed by the moderator at approval.