This paper constructs real analytic, canonical coordinates for the KdV equation near finite gap potentials, using pseudodifferential and paradifferential operators to facilitate stability analysis under perturbations.
Contribution
It introduces a novel coordinate system for KdV involving pseudodifferential operators, enabling normal form transformations and stability studies.
Findings
01
Coordinates are pseudodifferential operators with Fourier principal part.
02
Hamiltonian is in normal form up to order three.
03
Hamiltonian vector field admits paradifferential expansion.
Abstract
Near an arbitrary finite gap potential we construct real analytic, canonical coordinates for the KdV equation on the torus having the following two main properties: (1) up to a remainder term, which is smoothing to any given order, the coordinate transformation is a pseudodifferential operator of order 0 with principal part given by the Fourier transform and (2) the pullback of the KdV Hamiltonian is in normal form up to order three and the corresponding Hamiltonian vector field admits an expansion in terms of a paradifferential operator. Such coordinates are a key ingredient for studying the stability of finite gap solutions of the KdV equation under small, quasi-linear perturbations.
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Full text
Normal form coordinates for the KdV equation
having expansions in terms of pseudodifferential operators
Thomas Kappeler111Supported in part by the Swiss National Science Foundation. ,
Riccardo Montalto222Supported in part by the Swiss National Science Foundation.
Abstract.
Near an arbitrary finite gap potential we construct real analytic, canonical coordinates
for the KdV equation on the torus having the following two main properties: (1) up to a remainder term, which is smoothing to any given order,
the coordinate transformation is a pseudodifferential operator of order 0 with principal part given by the Fourier transform and
(2) the pullback of the KdV Hamiltonian is in normal form up to order three and
the corresponding Hamiltonian vector field admits an expansion in terms of a paradifferential operator.
Such coordinates are a key ingredient for studying the stability of finite gap solutions
of the KdV equation under small, quasi-linear perturbations.
Keywords: Normal form, KdV equation, finite gap potentials, pseudodifferential operators.
The goal of this paper is to construct canonical coordinates for the Korteweg-de Vries (KdV) equation on the circle
[TABLE]
taylored for studying the stability of finite gap solutions of (1.1), also referred to as periodic multisolitons, under quasi-linear perturbations.
To state our main results, we first need to make some preliminary considerations and introduce some notations. It is well known
that (1.1) is well-posed on the Sobolev spaces Hs={q∈HCs:q\mboxrealvalued} with s≥−1 (cf [17] and references therein) where
for any s∈R,
[TABLE]
Note that ∫01u(t,x)dx is a prime integral for equation (1.1). Without loss of generality, we restrict
our attention to the case where u has zero mean value (cf [13, Section 13]), i.e., we consider solutions u(t,x) of (1.1) in
H0s with s≥−1 where for any s∈R,
[TABLE]
It is well known that equation (1.1) can be written as a Hamiltonian PDE, ∂tu=∂x∇Hkdv(u)
where ∂x is the Gardner Poisson structure (with ∂x−1 being the corresponding symplectic structure)
and ∇Hkdv denotes the L2-gradient of the KdV Hamiltonian
[TABLE]
According to [13] (cf also [9]), there are canonical coordinates xn=xn(q), yn=yn(q), n≥1, defined on L02≡H00
so that when expressed in these coordinates, the KdV equation takes the form
[TABLE]
where ωnkdv denote the KdV frequencies.
To be more precise, introduce for any s∈R the sequence space
[TABLE]
and its real subspace h_{0}^{s}:=\big{\{}(w_{n})_{n\neq 0}\in h^{s}_{0,\mathbb{C}}:w_{-n}=\overline{w}_{n}\,\,\forall n\geq 1\big{\}}
and define the weighted complex coordinates z±n≡z±n(q),
[TABLE]
where ⋅≡+⋅ denotes the principal branch of the square root.
The results in [13] imply that the transformation, referred to as Birkhoff map,
[TABLE]
is canonical in the sense that
[TABLE]
whereas the brackets between all other coordinate functions vanish, and has the property that for any s∈Z≥0,
its restriction to H0s is a real analytic diffeomorphism with range h0s, Φkdv:H0s→h0s.
In terms of the coordinates zn(q),n=0, referred to as complex Birkhoff coordinates, the action variables
In(q) are defined by
[TABLE]
The sequences I(q)=(In(q))n≥1 fill out the whole positive quadrant ℓ+1,1 of ℓ1,1
where for any r≥0, the weighted ℓ1−space ℓ1,r is defined by
[TABLE]
A key feature of the Birkhoff map is that the KdV Hamiltonian, expressed in the coordinates zn,n=0,
[TABLE]
is in fact a function Hkdv of the actions I alone. More precisely,
Hkdv:ℓ+1,3→R is a real analytic map.
The KdV frequencies are then defined by ωnkdv:=∂InHkdv.
Finally, the differential
d0Φkdv:L02→h00 of Φkdv at q=0 is the Fourier transform F (cf [13, Theorem 9.8])
and hence d0Ψkdv the inverse Fourier transform F−1 where for any s∈Z,
[TABLE]
Let
[TABLE]
We denote by MS⊂L02 the manifold of S-gap potentials,
[TABLE]
and by MSo the open subset of MS, consisting of proper S-gap potentials,
[TABLE]
Note that MS is contained in ∩s≥0H0s and hence consists of C∞-smooth potentials
and that MSo can be parametrized by the action-angle coordinates
θS=(θk)k∈S+,IS=(Ik)k∈S+,
[TABLE]
where for any n=0, zn=zn(θS,IS) is given by
[TABLE]
Introduce for any s∈R
[TABLE]
as well as the maps, related to the Fourier transform,
[TABLE]
By a slight abuse of notation, we view MSo×h⊥s, s∈R, as a subset of h0s
and denote its elements by
[TABLE]
It is endowed by the standard Poisson bracket, given by
[TABLE]
whereas the brackets between all other coordinate functions vanish.
For any s∈R, we denote by x=(θS,IS,z⊥) elements in the tangent space Es
of MSo×h⊥s at any given point x∈MSo×h⊥s where Es is given by
[TABLE]
Furthermore, for any k≥1,∂x−k:HCs→H0,Cs+k is the bounded linear operator, defined by
[TABLE]
Finally, the standard inner products on L02 and on h00
are defined by
[TABLE]
Note that ⟨⋅,⋅⟩L02 and ⟨⋅,⋅⟩h00 extend as complex valued bilinear forms
to L0,C2 and respectively, h0,C0. In the sequel, restrictions of these inner products to various subspaces and extensions
as dual pairings will be denoted in the same way and the gradient of a functional F corresponding to these inner products by ∇F.
In more detail, for a C1−functional F:h00→C, one has
dF[z]=∑n=0zn∂znF=⟨∇F,z⟩
with the nth component of ∇F given by (∇F)n=∂z−nF.
Furthermore, for any given Banach spaces Y1,Y2, we denote by B(Y1,Y2) the space of bounded linear operators from Y1 to Y2, endowed with the operator norm.
Theorem 1.1**.**
Let S+⊆N be finite
and K be a subset of MSo of the form TS+×K1 where K1 is a compact subset of R>0S+.
Then there exists an open bounded neighbourhood V of K×{0} in MSo×h⊥0
and a canonical real analytic diffeomorphism
Ψ:V→Ψ(V)⊆L02,x=(θS,IS,z⊥)↦q
with the property that Ψ satisfies
[TABLE]
and is compatible in the sense explained below with the scale of Sobolev spaces H0s,s∈Z≥0, so that the following holds:
(AE1)
For any integer N≥1, Ψ admits an asymptotic expansion on V of the form
[TABLE]
where RN(θS,IS,0;Ψ)=0 and where
for any s∈Z≥0 and 1≤k≤N
[TABLE]
are real analytic maps satisfying the tame estimates of Theorem 1.2 below.
(AE2)
For any x∈V,
the transpose dΨ(x)t
(with respect to the standard inner products) of the differential
dΨ(x):E1→H01 is a bounded operator dΨ(x)t:H01→E1. For any q∈H01
and any integer N≥1, dΨ(x)t[q] admits an expansion of the form
[TABLE]
where for any s∈N and 1≤k≤N,
[TABLE]
[TABLE]
[TABLE]
are real analytic maps, satisfying the tame estimates of Theorem 1.2 below.
Furthermore, the coefficient a1(x;dΨt) satisfies
a1(x;dΨt)=−a1(x;Ψ).
(AE3)
The Hamiltonian H:=Hkdv∘Ψ:V∩(MSo×h⊥1)→R is in normal form up to order three. More precisely,
[TABLE]
where P:V∩(MSo×h⊥1)→R is real analytic and satisfies P(θS,IS,z⊥)=O(∥z⊥∥1∥z⊥∥02),
Ωnkdv:=2πn1ωnkdv,
n∈S+⊥, and ωnkdv denote the KdV frequencies introduced above. Furthermore for any integer N≥1,
there exists an integer σN≥N (loss of regularity) so that the gradient ∇P(θS,IS,z⊥) of P with components
∇θSP, ∇ISP, and ∇z⊥P admits an expansion of the form
[TABLE]
where for any integers s≥0 and 0≤k≤N,
[TABLE]
are real analytic and satisfy the tame estimates of Theorem 1.2 below.
Here Tak∇P denotes the operator of paramultiplication with ak∇P (cf Appendix E) and
the diffeomorphism Ψ:V→Ψ(V)⊂L02
being compatible with the scale of Sobolev spaces H0s, s∈Z≥0, means that for any s∈Z≥0,
\Psi\big{(}{\cal V}\cap({\cal M}_{S}^{o}\times h^{s}_{\bot})\big{)}\subseteq H^{s}_{0} and Ψ:V∩(MSo×h⊥s)→H0s
is a real analytic diffeomorphism onto its image.
In applications, it is of interest to know whether the coordinate transformation Ψ preserves the reversible structure, defined by the maps
Srev:L02→L02, (Srevq)(x):=q(−x), and
Srev:MSo×h⊥0→MSo×h⊥0 where
[TABLE]
Note that for any s∈Z≥0, Srev:H0s→H0s and Srev:MSo×h⊥s→MSo×h⊥s
are linear involutions and that without loss of generality, the neighbourhood V of Theorem 1.1 can
be chosen to be invariant under the map Srev, i.e., Srev(V)=V.
Addendum to Theorem 1.1The maps Ψ:V→L02, Ψkdv:h00→L02, and F−1:h00→L02 preserve
the reversible structure, i.e.,
[TABLE]
and so do the maps in the asymptotic expansions (AE1) (x∈V),
[TABLE]
and the ones in the asymptotic expansions (AE2) (x∈V∩(MSo×h⊥1), q∈H01),
[TABLE]
[TABLE]
Furthermore, the Hamiltonians Hkdv, H=Hkdv∘Ψ, and P are reversible, meaning that
[TABLE]
and the maps in the asymptotic expansion in (AE3) preserve the reversible structure,
[TABLE]
[TABLE]
Theorem 1.2 below states tame estimates for the map Ψ and the gradient ∇P of the remainder term P
in the expansion of H. In the sequel, we denote
elements in the tangent space Es:=RS+×RS+×h⊥s of V∩(MSo×h⊥s)
at any given point x=(θS,IS,z⊥) by x=(θS,IS,z⊥).
Throughout the paper, all the stated estimates for maps hold locally uniformly with respect to their arguments.
Theorem 1.2**.**
Let N,l∈N. Then
under the same assumptions as in Theorem 1.1, the following estimates hold:
(Est1)
For any x=(θS,IS,z⊥)∈V, 1≤k≤N, x1,…,xl∈E0, s∈Z≥0,
[TABLE]
Simlarly, for any \mathfrak{x}\in{\cal V}\cap\big{(}{\cal M}_{S}^{o}\times h^{s}_{\bot}\big{)}, x1,…,xl∈Es, s∈Z≥0,
[TABLE]
(Est2)
For any x=(θS,IS,z⊥)∈V∩(MSo×h⊥1), 1≤k≤N, x1,…,xl∈E1, s∈N,
[TABLE]
and
[TABLE]
Similarly, for any \mathfrak{x}\in{\cal V}\cap\big{(}{\cal M}_{S}^{o}\times h^{s}_{\bot}\big{)},
x1,…,xl∈Es, q∈H0s, s∈N,
[TABLE]
(Est3)
For any s∈Z≥0, \mathfrak{x}=(\theta_{S},I_{S},z_{\bot})\in{\cal V}\cap\big{(}{\cal M}_{S}^{o}\times h^{s+\sigma_{N}}_{\bot}\big{)}, ∥z⊥∥σN≤1, 1≤k≤N,
x1,…,xl∈Es+σN,
[TABLE]
For any s∈Z≥0, \mathfrak{x}\in{\cal V}\cap\big{(}{\cal M}_{S}^{o}\times h_{\bot}^{s\lor\sigma_{N}}\big{)} with ∥z⊥∥σN≤1,
x∈Es∨σN,
[TABLE]
and if in addition x1,…,xl∈Es∨σN, l≥2,
[TABLE]
Applications: The Birkhoff coordinates are well suited to study the initial value problem of (1.1) (cf e.g. [17], [11] and references therein)
and semilinear perturbations of (1.1) (cf e.g. [13], [19]). However, when equation (1.1) is expressed in Birkhoff coordinates,
various features of the KdV equation and its perturbations such as being partial differential equations, get lost.
On the other hand, due to the expansions (AE1)−(AE3), the coordinates of Theorem 1.1 allow
to preserve the essence of such features and in the form stated turn out to be well suited to study quasi-linear perturbations of the KdV equation.
Outline of the construction: In his pioneering work [19], Kuksin presents a general scheme for proving KAM-type theorems
for integrable PDEs in one space dimension such as the KdV or the sine-Gordon (sG) equations, which possess a Lax pair formulation
and admit finite dimensional integrable subsystems foliated by invariant tori. Expanding on work of Krichever [18], Kuksin considers bounded integrable subsystems of such a PDE
which admit action-angle coordinates. They are complemented by infinitely many coordinates
whose construction is based on a set of time periodic solutions, referred to as Floquet solutions of the PDE, obtained by linearizing
the PDE under consideration along a solution evolving in the integrable subsystem. It turns out that the resulting coordinate transformation
is typically not symplectic. Extending arguments of Moser and Weinstein to the given infinite dimensional setup (see [19], Lemma 1.4 and Section 1.7),
he constructs a second coordinate transformation so that the composition of the two transformations become symplectic. We follow Kuksin’s scheme of the proof
by constructing Ψ as the composition of ΨL∘ΨC of two transformations.
The ΨL is given by the Taylor expansion of Ψkdv of order one in the normal direction z⊥ around (θS,IS,0),
[TABLE]
The neighbourhood V of K×{0} is chosen sufficiently small so that by the inverse function theorem,
ΨL is a real analytic diffeomorphism onto its image.
Using that ΨL is given in terms of the Birkhoff map Ψkdv, we prove in a first step that ΨL admits an asymptotic expansion and tame estimates corresponding to the ones of Theorems 1.1, 1.2. In a second step we establish the corresponding results for the symplectic corrector ΨC.
The methods developed in this paper also apply to the defocusing NLS equation and can be used to provide corresponding asymptotic expansions
and estimates, thus complementing our previous work [12] on this equation.
Comments: In view of the definition of ΨL, the map Ψ=ΨL∘ΨC can be considered as a symplectic version of the Taylor expansion of Ψkdv of order 1
in normal directions at points of MSo×{0} and hence as a locally defined symplectic approximation of Ψkdv. Theorem 1.1 in particular says
that Ψ(θS,IS,z⊥)−F⊥−1[z⊥] maps V∩(MSo×h⊥s) into H0s+1 for any s≥0, i.e., that it is one-smoothing.
Such a property has previously been established for the Birkhoff map Ψkdv near [math] by Kuksin-Perelman [20], Theorem 0.2,
and proved to hold on the entire phase space by Kappeler-Schaad-Topalov [16]. Theorem 1.1 says that for the map Ψ, a much stronger property holds:
up to a remainder term which is (N+1)-smoothing, Ψ is a (nonlinear) pseudodifferential operator acting on F⊥−1(h⊥0).
Organization: The maps ΨL and ΨC are studied in Section 2 and respectively, Section 3.
The expansion of the KdV Hamiltonian in the new coordinates is treated in Section 4
and a summary of the proofs of Theorem 1.1 and Theorem 1.2 is given in Section 5.
In Appendix A –
Appendix D,
we present results needed for the analysis of the map ΨL in Section 2 and
in Appendix E we review material from the pseudodifferential and paradifferential calculus.
2 The map ΨL
In this section we define and study the map ΨL described in Section 1. First let us introduce some more notation. For S⊂Z finite as in (1.8),
denote by hS0⊂CS the subspace given by
[TABLE]
By a slight abuse of terminology, for any s∈Z, we identify h0s with hS0×h⊥s
and write (zS,z⊥) for z∈h0s.
According to the Addendum to Theorem A.1 at the end of Appendix A,
the space MS of S−gap potentials is viewed as a (real analytic) submanifold of the weighted Sobolev space H0w∗ and
the restriction of Φkdv to MS yields a real analytic diffeomorphism,
Φkdv∣MS:MS→hS0.
We endow
hS0 with the pull back of the standard Poisson
structure on h00 by the natural embedding hS0↪h00, where the standard Poisson structure is the one for which {zn,z−n}=2πin
for any n≥1 whereas the Poisson brackets among all the other coordinates vanish.
Consider the partially linearized inverse Birkhoff map
[TABLE]
where
d⊥Ψkdv(zS,0) denotes the Fréchet derivative of the map z⊥↦Ψkdv(zS,z⊥), evaluated at the point (zS,0).
By Theorem A.1, ΨL is a real analytic map.
Proposition 2.1**.**
The map ΨL has the following properties: (i) For any zS∈hS0,
[TABLE]
(ii) For any compact subset K⊆hS0 there exists an open neighbourhood V of K×{0} in h00≡hS0×h⊥0
so that for any integer s≥0, the restriction ΨL∣V∩h0s is a map V∩h0s→H0s
which is a real analytic diffeomorphism onto its image. The neighborhood V is chosen of the form VS×V⊥
where VS is an open, bounded neighborhood of K in hS0 and V⊥ is an open ball
in h⊥0 of sufficiently small radius, centered at zero.
(iii) For any z=(zS,z⊥)∈V and z=(z^S,z^⊥)∈hS0×h⊥0,
[TABLE]
where the linear map dΨL(zS,0)=dΨkdv(zS,0)
is canonical and d_{S}\big{(}d_{\bot}\Psi^{kdv}(z_{S},0)[z_{\bot}]\big{)} denotes the Fréchet derivative
of the map
[TABLE]
Proof.
(i) The stated formulas follow from the definition of ΨL in a straightforward way. (ii) In view of Theorem A.1,
the claimed statements can be proved by using the same arguments as in the proof of the corresponding results for the defocusing NLS equation in [12, Proposition 3.1].
Item (iii) is proved in a straightforward way.
∎
In a next step we want to analyze d⊥Ψkdv(zS,0) further. Consider the Hamiltonian vector fields ∂x∇qz±n, n≥1,
corresponding to the Hamiltonians given by the complex Birkhoff coordinates z±n.
Since Φkdv is canonical in the sense that {zn,z−n}=2πin for any n=0
whereas the brackets among all the other coordinates vanish, it follows that for any q∈L02 and n≥1,
[TABLE]
where Xz±n are the constant vector fields on h0,C0 given by
[TABLE]
and e(n),e(−n) are the standard basis elements in the sequence space h0,C0,
[TABLE]
(Here we extended dqΦkdv:L02→h00 as a C-linear map L0,C2→h0,C0). Hence for any n≥1,
[TABLE]
It then follows from [13, Theorem 9.5, 9.7] and the formulas (B.5), (B.6)
for the functions Hn, Gn together with their properties stated in Proposition B.1
that for any q∈MS and n∈S+⊥
[TABLE]
and similarly
[TABLE]
where βn=∑ℓ∈S+βℓn (cf [13, Theorem 8.5]) and ξn=8In/γn (cf [13, Theorem 7.3]).
Since q∈MS and n∈S+⊥ one has γn(q)=0 and the factor ξn(q) is obtained by a limiting argument. By a slight abuse of terminology,
we denote this limit also by 8In(q)/γn2(q).
The formulas (2.5) - (2.6) allow to express ∂x∇qz±n in terms of the Floquet solutions
fn(x)≡fn(x,q) as follows (cf Appendix B for notations).
At q=0, nπξn=1, βn=0, Δ¨(τn)m˙2(τn)=−1 and
f±n(x)=e±πinx for any n≥1, confirming that (d0Φkdv)−1[e(±n)]=e±2πinx (cf [13]).
For any given q∈MS and n∈S+⊥, introduce the functions W±n(x)≡W±n(x,q) given by
[TABLE]
We record that for any n∈S+⊥, W−n=Wn since f−n=fn.
Combining Proposition 2.1 and Proposition 2.2
one obtains the following formula for the map ΨL:
Corollary 2.1**.**
For any z=(zS,z⊥)∈V, one has
d⊥Ψkdv(zS,0)[z⊥]=Ψ1(zS)[z⊥] where
[TABLE]
Note that Ψ1(zS)[z⊥]=ΨL(z)−q is linear in z⊥.
Since q∈MS is a finite gap potential, it is C∞-smooth and so is Wn(x,q). Next we want to show that ΨL(z) admits an expansion of the type stated in Theorem 1.1.
Recall from the Addendum to Theorem A.1 at the end of Appendix A that for any q∈MS, Vq,S∗ denotes a neighborhood of q,
consisting of complex valued S−gap potentials in the weighted Sobolev space H0,Cw∗ so that the restriction of Φkdv to Vq,S∗
is a real analytic diffeomorphism onto its image Φkdv(Vq,S∗)⊂hS,C0.
Combining Theorem C.1 and Lemma C.4 - Lemma C.6
of Appendix C and using that
[TABLE]
one obtains the following
Theorem 2.1**.**
(i) Let q∈MS and N∈N. Then for any p∈Vq,S∗,
Wn(x)≡Wn(x,p), n∈S⊥, has an expansion as ∣n∣→∞ of the form
[TABLE]
where for any s∈Z≥0,
Wkae:Vq,S∗→HCs, p↦Wkae(⋅,p), k≥1, are real analytic and
RNWn:Vq,S∗→HCs,p↦RNWn(⋅,p), n∈S⊥,
are analytic and satisfy for any j≥0,
[TABLE]
The constants CN,j can be chosen locally uniformly for p∈Vq,S∗.
By a slight abuse of terminology, in the sequel, we will view Wkae(⋅,q) and RNWn(⋅,q) as functions of zS,
[TABLE]
(ii) For any zS∈hS0,
the linear operator Ψ1(zS), given by
[TABLE]
has the property that for any s∈Z≥0, its restriction to h⊥s is a bounded linear operator h⊥s→H0s.
Furthermore, up to a remainder, the operator Ψ1(zS):h⊥0→L02 is a pseudodifferential operator of order [math].
More precisely, Ψ1(zS) has an expansion to any order N≥1 of the form
[TABLE]
where
[TABLE]
For any s≥0, the restriction of RN(zS;Ψ1) to h⊥s defines a bounded linear operator h⊥s→Hs+N+1 and the map
[TABLE]
is real analytic. Corresponding properties hold for the map ΨL:V→L02, defined
in Proposition 2.1,
[TABLE]
where
[TABLE]
Remark 2.2**.**
*(i) Note that the pseudodifferential operator \big{(}\text{Id}+\sum_{k=1}^{N}a_{k}(z_{S};\Psi_{1})\partial_{x}^{-k}\big{)}\circ{\cal F}_{\bot}^{-1}
defines a bounded linear operator h⊥s→Hs for any s∈R whereas the remainder RN(zS;Ψ1)
defines a bounded linear operator h⊥s→Hs+N+1 for any s≥−N−1.
(ii) Whenever possible, we will use similar notation for the coefficients of the expansion of the various quantities such as Ψ1(zS).
If the coefficients are operators, we use the upper case letter A
and write Ak for the kth coefficient, whereas when they are functions (or operators, defined as the multiplication by a function),
we use the lower case letter a and write ak for the k’th coefficient. The quantity, which is expanded, is indicated
as an argument of Ak and ak.
(iii) The fact that up to a remainder term, ΨL(zS,⋅) is given by the pseudodifferential operator of order 0,
(Id+∑k=1Nak(zS;Ψ1)∂x−k)∘F⊥−1,
acting on the scale of Hilbert spaces h⊥s, s∈Z≥0, is at the heart of this paper.
The result shows that the differential of the Birkhoff map z↦Ψkdv(z) at a finite gap potential, has distinctive features.*
A straightforward application of Theorem 2.1(ii)
yields an expansion of the transpose operator Ψ1(zS)t of Ψ1(zS).
Since F⊥−1 is the restriction of the inverse of the Fourier transform to h⊥0,
the transpose F⊥−t:=(F⊥−1)t of F⊥−1 with respect to the standard inner products in L02 and h⊥0
is given by the Fourier transform, i.e., for any q∈L02,
[TABLE]
Corollary 2.2**.**
For any zS∈hS0, q=Ψkdv(zS,0), and N∈N,
Ψ1(zS)t:L2→h⊥0,q↦(⟨W−n(⋅,q),q⟩)n∈S⊥
has an expansion of the form
[TABLE]
where for any s≥0, the coefficients hS0→Hs, zS↦ak(zS;Ψ1t), k≥1, and the remainder
hS0→B(Hs,h⊥s+N+1), zS↦RN(zS;Ψ1t), are real analytic.
Furthermore, ak(zS;Ψ1t)=−ak(zS;Ψ1).
Corresponding properties hold for the map
[TABLE]
For any z∈V,N∈N, dΨL(z)t has an expansion of the form
[TABLE]
where ak(z;dΨLt)=ak(zS;Ψ1t) and where for any integer s≥0,V∩h0s→B(L2,h0s+N+1),z↦RN(z;dΨLt)
is real analytic.
Remark 2.3**.**
Again we record that the pseudodifferential operator {\cal F}_{\bot}\circ\big{(}\text{Id}+\sum_{k=1}^{N}a_{k}(z_{S};\Psi_{1}^{t})\partial_{x}^{-k}\big{)}
defines a bounded linear operator Hs→h⊥s for any s∈R whereas the remainder RN(zS;Ψ1t)
defines a bounded linear operator Hs→h⊥s+N+1 for any s≥−N−1.
Proof.
By Theorem 2.1(ii),
Ψ1(zS)=F⊥−1+∑k=1Nak(zS;Ψ1)∂x−kF⊥−1+RN(zS;Ψ1) where for any z⊥∈h⊥0,
[TABLE]
Note that the functions ak(zS;Ψ1)(x), k≥1, are real valued.
Taking into account that F⊥−t=F⊥ and (∂x−k)t=(−1)k∂x−k, the expansion of the transpose Ψ1(zS)t of Ψ1(zS) then reads
(RN(zS;Ψ1))t:Hs→h⊥s+N+1 is bounded, and
the map hS0→B(Hs,h⊥s+N+1), zS↦RN(zS;Ψ1t), is real analytic.
Since by Lemma E.2 and the notation introduced there,
[TABLE]
one sees that Ψ1(zS)t admits an expansion of the form,
[TABLE]
where ak(zS;Ψ1t), k≥1, and RN(zS;Ψ1t) satisfy the claimed properties. Since
[TABLE]
the claimed properties of dΨL(z)t follow from the ones of Ψ1(zS)t.
∎
Using results of Appendix D and Appendix C, one obtains the following properties of the functions Wn, n∈S⊥, and the map ΨL
with regard to the reversible structure, introduced in Section 1.
Addendum to Theorem 2.1(i) For any zS∈hS0, q=Ψkdv(zS,0) satisfies Srevq=Ψkdv(Srev(zS,0))
and for any n∈S⊥, x∈R,
Wn(x,Srevq)=W−n(−x,q) as well as ( k≥1, N≥1)
[TABLE]
(ii)
For any z=(zS,z⊥)∈hS0×h⊥0 and x∈R,
[TABLE]
As a consequence,
for any z∈V, x∈R
[TABLE]
(iii) For any zS∈hS0 and q∈L02, one has
Ψ1(SrevzS)t[Srevq]=Srev(Ψ1(zS)t[q]). As a consequence,
for any k≥1 and N≥1,
[TABLE]
Proof of Addendum to Theorem 2.1
(i) By the Addendum to Theorem C.1, we know that for any q∈MS and n∈S+⊥, f±n(x,Srevq)=f∓n(−x,q).
Furthermore, one has ξn(Srevq)=ξn(q), Δ(λ,Srevq)=Δ(λ,q),m2(λ,Srevq)=m2(λ,q) (Lemma D.1) and βn(Srevq)=−βn(q) (Corollary D.1).
In view of the definition (2.7) of W±n it then follows that W±n(x,Srevq)=W∓n(−x,q)
and in turn, comparing the expansion (2.9) of W±n(x,Srevq) with the one of W∓n(−x,q),
one obtains the identities (2.13). (ii) By (i) one has for any zS∈hS0 and q=Ψkdv(zS,0),
[TABLE]
as well as Wkae(x,SrevzS)=(−1)kWkae(−x,zS) and
({\cal R}_{N}(\mathcal{S}_{rev}z_{S};\,\Psi_{1})[\mathcal{S}_{rev}z_{\bot}])(x)=\big{(}{\cal R}_{N}(z_{S};\Psi_{1})[z_{\bot}]\big{)}(-x).
By (2.10), the claimed identities (2.14) then follow.
(iii) Recall that for any zS∈hS0, q∈L02, one has Ψ1(zS)t[q]=(⟨W−n(⋅,q),q⟩)n∈S⊥.
It then follows from item (i) that
[TABLE]
Comparing the expansion (2.11) for \mathcal{S}_{rev}\big{(}\Psi_{1}(\mathcal{S}_{rev}z_{S})^{t}[\widehat{q}]\big{)} with the one for Ψ1(zS)t[Srevq]
and taking into account that Srev∘F⊥=F⊥∘Srev and ∂x∘Srev=−Srev∘∂x one sees that for any k≥1,
[TABLE]
In the remaining part of this section we describe the pull back ΨL∗ΛG of the symplectic form ΛG by the map ΨL, defined in Proposition 2.1,
where ΛG, defined by the Gardner Poisson structure, is given by
[TABLE]
Note that ΛG=dλG where the one form λG, defined on L02, is given by
[TABLE]
To compute the pull back of ΛG by ΨL, note that for any z=(zS,z⊥)∈V=VS×V⊥,
the derivative dΨL(z), when written in 1×2 matrix form, is given by (cf (2.8))
[TABLE]
For any z=(zS,z⊥),w=(wS,w⊥)∈h00 one has
[TABLE]
Since by construction, dΨL(zS,0):h00→L02 is symplectic, one has
[TABLE]
where Λ is the symplectic form on h00,
[TABLE]
and J−1 denotes the inverse of the diagonal operator, acting on the scale of Hilbert spaces h0s,s∈R,
[TABLE]
Note that Λ=dλ where λ is the one form on h00,
[TABLE]
Altogether we have that
[TABLE]
where
the operator L(z):hS0×h⊥0→hS0×h⊥0 has the form
[TABLE]
with LSS(z):hS0→hS0, LS⊥(z):h⊥0→hS0, and L⊥S:hS0→h⊥0 given by
[TABLE]
For any z=(zS,z⊥)∈V, the operators L(z),LSS(z),LS⊥(z), and L⊥S(z) are bounded.
In the sequel, we will often write the operators (2.22) in the following way
[TABLE]
where q=Ψkdv(zS,0).
The operators LSS(z), LS⊥(z), and L⊥S(z) satisfy the following properties.
Lemma 2.1**.**
(i)* The maps*
[TABLE]
are real analytic. Furthermore, the following estimates hold: for any z=(zS,z⊥)∈V, zS∈hS0,
and z1,…,zl∈h00, l≥1 ,
[TABLE]
and if in addition, z⊥∈h⊥0,
[TABLE]
(ii)*
For any z=(zS,z⊥)∈V,
L⊥S(z) has an expansion of arbitrary order N≥2,*
[TABLE]
where for any s≥0, k≥1, the maps
[TABLE]
are real analytic. In particular, the operator L⊥S(z) is two smooothing. More precisely, for any s≥0,
[TABLE]
is real analytic.
The coefficients Ak(zS;L⊥S) are independent of z⊥ and satisfy for any s≥0,zS∈VS,zS∈hS0,z1,…,zl∈h00, l≥1, the following estimates
[TABLE]
Furthermore, for any s∈Z≥0, z=(zS,z⊥)∈V∩h0s, zS∈hS0, and
z1,…,zl∈h0s, l≥1, RN(z;L⊥S)[zS] satisfies
∥RN(z;L⊥S)[zS]∥s+N+1≲s,N∥zS∥∥z⊥∥s and
[TABLE]
(iii) As a consequence, for any integer s≥0, the map V∩h0s→B(h00,h0s+2),z↦L(z) is real analytic. Furthermore,
for any z=(zS,z⊥)∈V∩h0s and z∈h00, it satisfies the estimates
[TABLE]
and if in addition z1,…,zl∈h0s, l≥1, one has
[TABLE]
for some constants C(s;L)≥1, C(s,l;L)≥1.
Remark 2.4**.**
Recall that by Remark 2.2(i), ∂x−1Ψ1(zS):h⊥−1→H00
is a bounded linear operator for any z∈V. Since ∂znΨ1(zS)[z⊥]∈H00 for any n∈S, it then follows that
LS⊥(z):h⊥−1→hS0
and in turn L(z):h0−1→h00 are bounded linear operators. Estimates, corresponding to the ones for LS⊥(z) and L(z)
of Lemma 2.1, continue to hold, when these operators are extended to h⊥−1 and, respectively, h0−1.
Proof.
The lemma follows in a straightforward way by using the properties of the maps Ψ1(zS) and Ψ1(zS)t
(cf Lemma 2.2) and the expansion of the composition ∂x−n∘a∂x−k (cf Lemma E.2 in Appendix E).
∎
Finally, we discuss the properties of the symplectic forms ΛG, Λ, and ΨL∗ΛG with respect to
the reversible structures introduced in Section 1.
First note that for any u,v∈L02,
[TABLE]
and similarly, for any z,w∈h00,
[TABLE]
By the Addendum to Theorem 2.1, the pullback Srev∗ΨL∗ΛG can then be computed as
In this section we construct the symplectic corrector ΨC. Our approach is based on a well known method of Moser and Weinstein,
implemented for an infinite dimensional setup in [19] (cf also [12]).
We begin by briefly outlining the construction. At the end of Section 2, we introduce the symplectic forms Λ
and ΨL∗ΛG. They are defined on V=VS×V⊥ and are related as follows (z∈V,z,w∈h00)
[TABLE]
where L(z) is the operator defined by (2.21). Our candidate for ΨC is ΨX0,1 where X≡X(τ,z)
is a non-autonomous vector field, defined for z∈V and 0≤τ≤1,
so that (ΨX0,1)∗(ΨL∗ΛG)=Λ.
The flow ΨXτ0,τ, corresponding to the vector field X, is required to be well defined on a neighborhood V′ (cf Lemma 3.4) for 0≤τ0,τ≤1
and to satisfy the standard normalization conditions ΨXτ0,τ0(z)=z for any z∈V′ and 0≤τ0≤1.
To find X with the desired properties, introduce the one parameter family of two forms,
[TABLE]
Note that Λ0=Λ, Λ1=ΨL∗ΛG, and (ΨX0,0)∗Λ0=Λ0.
The desired identity (ΨX0,1)∗Λ1=Λ0 then follows if one can show that (ΨX0,τ)∗Λτ
is independent of τ, that is, \partial_{\tau}\big{(}(\Psi_{X}^{0,\tau})^{*}\Lambda_{\tau}\big{)}=0. By Cartan’s identity,
[TABLE]
Hence we need to choose the vector field X(τ,z) in such a way that
[TABLE]
where for any 0≤τ≤1 and z∈V, the operator Lτ(z):h00→h00 is defined by
[TABLE]
and where J−1 is the inverse of the diagonal operator J, defined by (2.18).
In a next step we want to rewrite ΛL(z) as the differential of a properly chosen one form. First note that
since ΛG=dλG (cf (2.15)) and Λ=dλ (cf (2.19)),
the two form ΛL is closed, ΛL=d(λ1−λ0) where λ1:=ΨL∗λG and λ0:=λ.
Furthermore, by Lemma 2.1, L(zS,0)=0 and hence ΛL(zS,0)=0 for any zS∈VS.
It then follows by the Poincaré Lemma (cf e.g. [12, Appendix 1]) that dλL=ΛL where
[TABLE]
Since LS⊥(zS,tz⊥)=tLS⊥(zS,z⊥) (cf (2.23)) one is then led to
Arguing as in the proof of [12, Lemma 4.1] one can show that after shrinking the ball V⊥, if needed,
Lτ(z) is invertible for any 0≤τ≤1 and z∈V. In view of Lemma 2.1,
the following version of [12, Lemma 4.1] holds:
Lemma 3.1**.**
After shrinking the ball V⊥⊂h⊥0 in V=VS×V⊥, if needed,
for any s≥0,z∈V∩h0s, and τ∈[0,1], the operator
Lτ(z):h0s→h0s is invertible with inverse Lτ(z)−1:h0s→h0s given by the Neumann series,
[TABLE]
Furthermore, for any s≥0, the map
[TABLE]
is real analytic and the following estimates hold: for any z∈V∩h0s, 0≤τ≤1,
z,z1,…,zl∈h0s, l≥1,
[TABLE]
[TABLE]
Note that by (3.4) and (2.23), E(z) and hence λL(z) are quadratic expressions in z⊥.
Applying Lemma 2.1 to E(z), one obtains the following estimates:
Lemma 3.2**.**
The map V→hS0×h⊥0, z↦E(z)=(ES(z),0) is real analytic. Furthermore, for any
z∈V, z1,…,zl∈h00, l≥1, one has
[TABLE]
Since Lτ(z) is invertible (cf Lemma 3.1), equation (3.5) can be solved for X(τ,z),
[TABLE]
Note that by Lemma 3.2, JE(z) is C∞−smooth.
Hence it follows from Lemma 3.1 that
for any integer s≥0,z∈V∩h0s
[TABLE]
Lemma 3.1 and Lemma 3.2 then lead to the following results (cf Lemma [12, 4.3]).
Lemma 3.3**.**
For any s≥0, the non-autonomous vector field
[TABLE]
is real analytic and the following estimates hold: for any z∈V∩h0s,0≤τ≤1, z∈h0s,
[TABLE]
and for any z1,…,zl∈h0s, l≥2,
[TABLE]
By a standard contraction argument, there exists an open neighborhood VS′⊂VS of K⊂hS0 and a ball V⊥′⊂V⊥, centered at [math],
so that for any τ,τ0∈[0,1], the flow map ΨXτ0,τ of the non-autonomous differential equation ∂τz=X(τ,z)
is well defined on V′:=VS′×V⊥′ and
[TABLE]
is real analytic. Arguing as in the proof of [12, Lemma 4.4] one shows that ΨXτ0,τ−id
is one smoothing. More precisely, the following holds.
Lemma 3.4**.**
Shrinking the ball V⊥′⊂h⊥0 in V′=VS′×V⊥′, if needed, it follows that
for any s≥0, τ0,τ∈[0,1], the map
ΨXτ0,τ−id:V′∩h0s→h0s+1 is real analytic and for any z∈V′∩h0s, 0≤τ0,τ≤1,
z∈h0s,
[TABLE]
and for any z1,…,zl∈h0s, l≥2,
[TABLE]
Our aim is to derive expansions for the flow maps ΨXτ0,τ(z).
To this end we derive such expansions for Lτ(z)−1 and in turn for the vector field X(τ,z).
Recall that Lτ(z)−1 is given by the Neumann series (3.6) and hence we
first derive an expansion for the operators (JL(z))n.
It is convenient to introduce the projections
[TABLE]
and the maps
[TABLE]
Furthermore, let JS:=πSJπS, J⊥:=π⊥Jπ⊥. Then
JS−1=πSJ−1πS, J⊥−1=π⊥J−1π⊥, or, more explicitly,
[TABLE]
Lemma 3.5**.**
For any n≥1, z=(zS,z⊥)∈V,
(JL(z))n has an expansion of arbitrary order N≥1,
[TABLE]
where for any integers s≥0, 1≤k≤N, the maps
[TABLE]
[TABLE]
are real analytic. For any z=(zS,z⊥)∈V, z=(zS,z⊥)∈h00,
AkS(z;(JL)n)[zS] and Ak⊥(z;(JL)n)[z⊥] satisfy the estimates
[TABLE]
whereas for any integer s≥0, z=(zS,z⊥)∈V∩h0s, z∈h00
[TABLE]
for some constants C(k),C0(N)≥1.
Furthermore, the following estimates hold for the derivatives of these maps: for k,l≥1, there exists a constant C(k,l)≥1,
so that for any zS∈VS, zS∈hS0, z⊥∈h⊥0, z1,…,zl∈h00,
[TABLE]
[TABLE]
Finally, there exist constants C0(N,l)≥1, l≥1, so that for any z∈V∩h0s, z∈h00, z1,…,zl∈h0s,
[TABLE]
We refer to Remark 2.2 where we comment on the notation introduced for the coefficients in such expansions.
Furthermore, we recall that V⊥ denotes the open ball in h⊥0, centered at 0, whose radius is smaller than one and downscaled according to our needs.
Proof.
We begin by proving the claimed statements for n=1. By (2.21), the operator L(z), z∈V, can be written as
[TABLE]
Using that J⊥∘F⊥=F⊥∘∂x, it then follows from Lemma 2.1 that
[TABLE]
where AkS(zS;JL) and RN(z;JL) are obtained from
Ak(zS;L⊥S) and RN(z;L⊥S), given by Lemma 2.1,
in a straightforward way. It then follows that for any s≥0 and 1≤k≤N, the maps
[TABLE]
are real analytic and that RN(z;JL) is of the form
[TABLE]
For any integer s≥0, zS∈VS, zS∈hS0,
z1,…,zl∈h00, l≥1, one has
[TABLE]
Furthermore, for any integer s≥0, z=(zS,z⊥)∈V∩h0s,z∈h00,
z1,…,zl∈h0s, l≥1, the remainder term satisfies
∥RN(z;JL)[z]∥s+N+1≲s,N∥z⊥∥s∥z∥0 and
[TABLE]
To prove the claimed statements for n+1, n≥1, write (JL(z))n+1=JL(z)(JL(z))n.
By the expansion (3.13) it follows that
(JL(z))n+1 is of the form
[TABLE]
where AkS(z)≡AkS(z;(JL)n+1), Ak⊥(z)≡Ak⊥(z;(JL)n+1),
and RN(z)≡RN(z;(JL)n+1) are given by
[TABLE]
It then follows that these maps are real analytic as claimed in the statement of the lemma. Furthermore, for any s≥0, z=(zS,z⊥)∈V,zS∈hS0
one has by (3.14)
[TABLE]
where
C0:=C(0;L) is given by (2.25).
Similarly, again by (3.14), for any z=(zS,z⊥)∈V, z⊥∈h⊥0 one has
[TABLE]
whereas for any s≥0,z=(zS,z⊥)∈V∩h0s,z=(zS,z⊥)∈h00
[TABLE]
Next we estimate the derivatives of AkS(z;(JL)n+1)[zS].
For any s≥0, zS∈VS, zS∈hS0, z1,…,zl∈h00, l≥1,
the estimate of \|d^{l}\big{(}{\cal A}_{k}^{S}(z;(J\mathcal{L})^{n+1})[\widehat{z}_{S}]\big{)}[\widehat{z}_{1},\ldots,\widehat{z}_{l}]\|_{s} is obtained from the estimates of
Note that we introduced the element wl−m to indicate that in \|d^{m}\big{(}{\cal A}_{k}^{S}(z;J\mathcal{L})[\widehat{w}_{l-m}]\big{)}[\widehat{z}_{1},\ldots,\widehat{z}_{m}]\|_{s}
the derivative dm does not act on wl−m.
Increasing the constant C0 and/or decreasing the radius of the ball V⊥ depending on the size of l
it follows from (2.25) - (2.26) that
[TABLE]
Combining these estimates implies that
[TABLE]
In the same way one shows that for any s≥0, zS∈VS, z⊥∈h⊥0, z1,…,zl∈h00, l≥1,
[TABLE]
Finally, the claimed estimate for ∥dl(RN(z;(JL)n)[z])[z1,…,zl]∥s+N+1
where s≥0, z∈V∩h0s, z∈h00, z1,…,zl∈h0s, l≥1,
follows from the estimates of
Increasing the constant C0 and/or decreasing the radius of the ball V⊥ depending on the size of l,
it follows from (2.25) - (2.26) that
[TABLE]
Combining these estimates yields the claimed estimate for ∥dl(RN(z;(JL)n)[z])[z1,…,zl]∥s+N+1,
with constants chosen appropriately.
∎
Recall that V⊥ denotes the open ball in h⊥0, centered at 0, whose radius is smaller than one and downscaled at several instances in the course of our analysis.
Lemma 3.6**.**
For any N≥1,X(τ,z)=−Lτ(z)−1[JE(z)] (0≤τ≤1, z∈V) has an expansion of the form
[TABLE]
where for any s≥0 and k≥1, the maps
[TABLE]
are real analytic. Furthermore, for any 0≤τ≤1, z∈V, z∈h00,
[TABLE]
and for any z1,…,zl∈h00, l≥2,
[TABLE]
For any z∈V∩h0s, 0≤τ≤1, z∈h0s, the remainder term RN(τ,z;X) satisfies
[TABLE]
[TABLE]
whereas for any z1,…,zl∈h0s, l≥2,
[TABLE]
Proof.
By the Neumann series expansion, one has for any z∈V, 0≤τ≤1,
[TABLE]
Since JE(z)=(JSES(z),0), Lemma 3.5 yields that for any n≥1,
[TABLE]
where
[TABLE]
[TABLE]
By applying the estimates of Lemma 3.2 and Lemma 3.5, one gets for any s≥0, z∈V, 0≤τ≤1,
Shrinking the radius of the ball V⊥, if needed, one can assume that C(k)∥z⊥∥0<1, C0(N)∥z⊥∥0<1 for any
1≤k≤N, z⊥∈V⊥.
The expansion (3.17), the analyticity statement,
and the claimed estimates for ∥ak(τ,z;X)∥s and ∥RN(τ,z;X)∥s+N+1
then follow from the estimates (3.19), (3.20), and Lemma 3.2, Lemma 3.5.
The estimates for the derivatives of ak(τ,z;X) and RN(τ,z;X) follow by similar arguments.
Indeed, it follows from Lemma 3.5
that for any for 1≤k≤N, z∈V, 0≤τ≤1, z∈h00,
[TABLE]
Using that by Lemma 3.2, ∥JSES(z)∥≲∥z⊥∥02 and ∥d(JSES(z))[z]∥0≲∥z⊥∥0∥z∥0
one then concludes from Lemma 3.5
[TABLE]
and
[TABLE]
In view of the definition (3.21) of ak(τ,z;X) one then obtains the claimed estimate
∥dak(τ,z;X)[z]∥s≲s,k∥z⊥∥0∥z∥0.
The estimates for ∥dlak(τ,z;X)[z1,…,zl]∥s
with l≥2 are derived in a similar fashion.
Finally let us consider the estimates of the derivatives of the remainder term.
For any n≥1, z∈V∩h0s, 0≤τ≤1, z∈h0s,
it follows from Lemma 3.5 and the product rule that
[TABLE]
Using again that by Lemma 3.2, ∥JE(z)∥0≲∥z⊥∥02 and ∥dJE(z)[z]∥0≲∥z⊥∥0∥z∥0
and taking into account the definition (3.21) of RN(τ,z;X) one sees that
[TABLE]
yielding the claimed estimate for ∥dRN(τ,z;X)[z]∥s+N+1. The ones for ∥dlRN(τ,z;X)[z1,…,zl]∥s+N+1
with l≥2 are derived in a similar fashion.
∎
After these preliminary considerations we can now state the main result of this section, saying that for any τ0,τ∈[0,1],
the flow map ΨXτ0,τ, defined on V′ and with values in V, admits an expansion,
referred to as parametrix for the solution of the initial value problem of ∂τz=X(τ,z).
Theorem 3.1**.**
(i) For any τ0,τ∈[0,1], N∈N, and z=(zS,z⊥)∈V′,
[TABLE]
where for any τ0,τ∈[0,1], 1≤k≤N, and s≥0, the maps
[TABLE]
are real analytic. Furthermore, for any z∈V′, z∈h00,
[TABLE]
and for any z1,…,zl∈h00, l≥2,
[TABLE]
The remainder term satisfies the following estimates: for any z∈V′∩h0s, z∈h0s
[TABLE]
and for any z1,…,zl∈h0s, l≥2,
[TABLE]
(ii) In particular, the statements of item (i) hold for ΨC:=ΨX0,1:V′→ΨX0,1(V′), referred to as symplectic corrector,
and ΨX1,0:V′→ΨX1,0(V′),
which by a slight abuse of terminology with respect to its domain of definition we refer to as the inverse of ΨC and denote by ΨC−1.
The expansion of the map ΨC is then written as (z∈V′)
[TABLE]
where
[TABLE]
Similarly, the expansion for the inverse ΨC−1(z), z∈V′, is written as
[TABLE]
where
[TABLE]
Proof.
Clearly, item (ii) is a direct consequence of (i). Since the proof of item (i) is quite lengthy, we divide it up into several steps.
First note that the flow map Ψτ0,τ≡ΨXτ0,τ is a bounded nonlinear operator acting on V′∩h0s, s≥0, satisfying the integral equation
[TABLE]
Using the latter equation, the coefficients ak(z;Ψτ0,τ), k≥1, and the remainder term RN(z;ΨXτ0,τ) of the parametrix (3.22)
are determined inductively.
By (3.17), one obtains for any 0≤τ0,t≤1,z∈V′,
[TABLE]
Expansion of ∂x−kF⊥−1[π⊥Ψτ0,t(z)], 1≤k≤N: To find candidates for the coeffcients ak(z;ΨXτ0,τ)
we argue formally and substitute the expansion (3.22)
into the expression ∂x−kF⊥−1[π⊥Ψτ0,t(z)] yielding
[TABLE]
where
[TABLE]
Using Lemma E.2(i) and the notation established there, one has
[TABLE]
where
[TABLE]
By Lemma E.2, for any z∈V′∩h0s, s≥0, 0≤t,τ0≤1, 1≤j≤N
Changing in the double sum ∑j=1N−k∑i=0N−k−j the index i of summation to n:=i+j and then interchanging the order of summation, one obtains
[TABLE]
implying that ∂x−kF⊥−1[π⊥Ψτ0,t(z)] equals
[TABLE]
Expansion of ∑k=1Nak(t,Ψτ0,t(z);X)∂x−kF⊥−1[π⊥Ψτ0,t(z)]:
To simplify notation, introduce
[TABLE]
and then substitute (3.30) into ∑k=1Nak(t,Ψτ0,t(z);X)∂x−kF⊥−1[π⊥Ψτ0,t(z)] to get
[TABLE]
Changing the index of summation n to l:=k+n and then interchanging the sum with respect to k and l and in turn with respect to k and j,
the triple sum in (3.32) becomes
[TABLE]
Expansion of X(t,Ψτ0,t(z)):
Writing k for l and n for k, the expansion (3.24) of X(t,Ψτ0,t(z)) takes the form
[TABLE]
where
[TABLE]
and
[TABLE]
Definition and estimates of ak(z;Ψτ0,t), 1≤k≤N:
The fact that for any given 1≤k≤N, the coefficient bk(t,z;τ0) only depends on the unknown coefficients aj(z;Ψτ0,t) with 1≤j≤k−1, but not on ak(z;Ψτ0,t)
allows to determine ak(z;Ψτ0,t) recursively by using equation (3.23). Indeed,
substituting (3.34) for X(t,Ψτ0,t(z)) into equation (3.23) and combining it with (3.22),
leads, up to remainder terms, to the equations
[TABLE]
and for any 2≤k≤N,
[TABLE]
We then define for any z∈V′,0≤τ0,τ≤1,
[TABLE]
and for any k≥2,ak(z;Ψτ0,τ):=∫τ0τ(ak(t,z;τ0)+bk(t,z;τ0))dt, or more explicitly,
[TABLE]
To prove the claimed estimates for ak(z;Ψτ0,τ), we first estimate ak(t,z;τ0). Recall that by (3.31),
ak(t,z;τ0)=ak(t,Ψτ0,t(z);X).
By Lemma 3.6 and Lemma 3.4 one has
for any 0≤τ0,t≤1, z∈V′, and s≥0,
[TABLE]
It then follows from the definition of a1(z;Ψτ0,τ) that for any s≥0,
[TABLE]
To prove corresponding estimates for ak(z;Ψτ0,τ) with 2≤k≤N, we argue by induction.
Assume that
for any 1≤j≤k−1 and s≥0,
[TABLE]
By the estimate (3.38), the definition (3.37) of ak(z;Ψτ0,τ),
and the interpolation Lemma E.3,
one then concludes that the estimate (3.39) is also satisfied for j=k.
Using the analyticity properties established for ak(τ,z;τ0) and Ψτ0,τ(z), one verifies the ones stated for the coefficients ak(z;Ψτ0,τ).
Estimates of the derivatives of ak(z;Ψτ0,τ):
By Lemma 3.6, Lemma 3.4 and the chain rule one has
for any 0≤τ0,t≤1, z∈V′, z∈h00, s≥0,
[TABLE]
and if in addition, z1,…,zl∈h00, l≥2,
[TABLE]
By the definition of a1(z;Ψτ0,τ), (3.40) and (3.41)
yield the claimed estimate for ∥dla1(z;Ψτ0,τ)[z1,…,zl]∥s for any l≥1.
To prove corresponding estimates for the derivatives of ak(z;Ψτ0,τ) with 2≤k≤N, we again argue by induction.
Assume that for any 1≤j≤k−1 and s≥0,
[TABLE]
By the definition (3.37) of ak(z;Ψτ0,τ), the estimate (3.40) and the product rule it then follows that
(3.42) also holds for j=k.
The estimates for ∥dlak(z;Ψτ0,τ)[z1,…,zl]∥s
with l≥2 are derived in a similar fashion.
Definition and estimate of RN(z;Ψτ0,τ): The remainder term RN(z;Ψτ0,τ)
is defined so that the identity (3.22) holds,
[TABLE]
where ak(z;ΨXτ0,τ) are given by (3.37).
By (3.23) and the expansion (3.34) of X,
RN(z;Ψτ0,τ) satisfies
We estimate the two components πS∫τ0τRN(4)(t,z;τ0)dt and π⊥∫τ0τRN(4)(t,z;τ0)dt
of ∫τ0τRN(4)(t,z;τ0)dt separately.
By (3.43)
[TABLE]
and
[TABLE]
By Lemma 3.6 and Lemma 3.4, for any z∈V′, 0≤τ0,t≤1,
[TABLE]
implying that
[TABLE]
By the definition (3.29) of RN,k(3)(t,z;τ0), one has
[TABLE]
Furthermore, by the definition (3.26) of RN,k(1)(t,z;τ0), the term ∫τ0τak(t,z;τ0)RN,k(1)(t,z;τ0)dt equals
[TABLE]
Altogether, one concludes that π⊥RN(z;Ψτ0,τ) satisfies the integral equation
[TABLE]
where
[TABLE]
By the estimates (3.28) of RN,k,j(2)(t,z;τ0),
the ones of ak(τ,z;X) and RN(τ,z;X) given by Lemma 3.6,
the estimates of Ψτ0,t(z), given by Lemma 3.4, and the ones of ak(z;Ψτ0,τ), given by (3.39),
and using the interpolation Lemma E.3, one obtains for any s≥0,
[TABLE]
Note that ∑k=1Nak(t,z;τ0)∂x−k is a pseudodifferential operator of order −1 where by (3.38)
the coefficients ak(t,z;τ0) satisfy ∥ak(t,z;τ0)∥s≲s,k∥z⊥∥02.
Hence for any z∈V′∩h0s, 0≤τ0,τ≤1,
[TABLE]
By Gronwall’s inequality and since V⊥′ is a ball of sufficiently small radius, the integral equation (3.46) yields that for any s≥0,
[TABLE]
The estimates (3.44), (3.48) imply the claimed estimate of RN(z;Ψτ0,τ).
The stated analyticity property of RN(z;ΨXτ0,τ) then follows from the already established analyticity properties of
ΨXτ0,τ(z), ak(τ,z;τ0), and ak(z;Ψτ0,τ) (cf e.g. [7, Theorem A.5]).
Estimates of the derivatives of RN(z;Ψτ0,τ): The estimates of the derivatives of RN(z;Ψτ0,τ) can be obtained in a similar way
as the ones for RN(z;Ψτ0,τ). Indeed, for any s≥0, z∈V′∩h0s, 0≤τ0,τ≤1, z∈h0s,
one has
[TABLE]
Again, we estimate
\pi_{S}\big{(}d{\cal R}_{N}(z;\Psi^{\tau_{0},\tau})[\widehat{z}]\big{)}=\int_{\tau_{0}}^{\tau}\,\pi_{S}\big{(}d\big{(}{\cal R}_{N}(t,\Psi^{\tau_{0},t}(z);X)\big{)}[\widehat{z}]\big{)}\,dt
and \pi_{\bot}\big{(}d{\cal R}_{N}(z;\Psi^{\tau_{0},\tau})[\widehat{z}]\big{)}
separately. By Lemma 3.6, Lemma 3.4, and the chain rule, one has
[TABLE]
whereas by (3.46),
\pi_{\bot}\big{(}d{\cal R}_{N}(z;\Psi^{\tau_{0},\tau})[\widehat{z}]\big{)}
satisfies
[TABLE]
with BN(1)(τ,z;τ0)[z] given by
[TABLE]
Since
[TABLE]
we conclude from (3.50) by Gronwall’s inequality that
[TABLE]
The estimates (3.49) and (3.51)
imply the claimed estimate for dRN(z;Ψτ0,τ)[z].
In a similar fashion, one derives the estimates for ∥dlRN(z;Ψτ0,τ)[z1,…,zl]∥s+N+1
with z1,…,zl∈h0s, l≥2.
∎
It turns out that the flow maps ΨXτ0,τ and hence the symplectic corrector ΨC and its inverse ΨC−1
preserve the reversible structures, introduced in Section 1, acts on. To state the result in more detail, note that without loss of generality, we may assume that the neighborhood
V′=VS′×V⊥′ (cf Lemma 3.4) is invariant under the map Srev.
Addendum to Theorem 3.1(i) For any 0≤τ0,τ≤1,
ΨXτ0,τ∘Srev=Srev∘ΨXτ0,τ on V′
and for any z∈V′, x∈R, N∈N, and 1≤k≤N,
[TABLE]
(ii) As a consequence, ΨC and ΨC−1 are invariant under Srev on V′,
[TABLE]
and for any z∈V′, x∈R, N∈N, and 1≤k≤N,
[TABLE]
Proof of Addendum to Theorem 3.1 Clearly, item (ii) is a direct consequence of item (i).
By the Addendum to Lemma 2.1, the operator L(z), introduced in (2.20),
satisfies L(Srevz)∘Srev=−Srev∘L(z) on V.
It implies that for any z∈V,
E(Srevz)=−SrevE(z) where E(z) has been introduced in (3.4).
Altogether we then conclude that the vector field X(τ,z), introduced in (3.7), satisfies
[TABLE]
and hence by the uniqueness of the initial value problem of ∂τz=X(τ,z), the solution map satisfies
[TABLE]
The claimed identities for ak(z;ΨXτ0,τ) and RN(z;ΨXτ0,τ)
then follow from the expansion (3.22).
□
We now discuss two applications of Theorem 3.1. The first one concerns the expansion
of the transpose dΨX0,τ(z)t of the differential dΨX0,τ(z) which will be used in Section 4
in the proof of Lemma 4.10. Recall that for any z∈V′, and z, w∈h00
[TABLE]
and that the flow ΨX0,τ satisfies \partial_{\tau}\big{(}(\Psi^{0,\tau}_{X})^{*}\Lambda_{\tau}\big{)}=0 and hence (ΨX0,τ)∗Λτ=Λ0.
By the definition of the pullback this means that for any z∈V′,0≤τ≤1,z, w∈h00,
[TABLE]
Using that dΨX0,τ(z)−1=dΨXτ,0(ΨX0,τ(z)) one obtains the following formula for dΨX0,τ(z)t,
[TABLE]
Note that dΨXτ,0(ΨX0,τ(z)) and Lτ(ΨX0,τ(z))−1 are bounded linear operators on h00,
implying that dΨX0,τ(z)t is one on h01, and that these operators and their derivatives depend continuously on 0≤τ≤1.
Corollary 3.1**.**
For any 0≤τ≤1, z∈V′, the transpose dΨX0,τ(z)t
(with respect to the standard inner product) of the differential
dΨX0,τ(z) is a bounded linear operator dΨX0,τ(z)t:h01→h01 and for any N∈N and z∈h01,
dΨX0,τ(z)t[z] admits an expansion of the form
[TABLE]
where for any integer s≥0 and 1≤k≤N,
[TABLE]
[TABLE]
are real analytic maps. Furthermore, for any z∈V′, 1≤k≤N, z1,…,zl∈h00, l≥2,
[TABLE]
[TABLE]
and for any z∈V′, z∈h01, z1,…,zl∈h00, l≥1,
[TABLE]
The remainder RN(z;(dΨX0,τ)t) satisfies for any z∈V′∩h0s, z∈h0s+1, and z1,…,zl∈h0s, l∈N,
[TABLE]
[TABLE]
Remark 3.1**.**
Corollary 3.1 holds in particular for dΨC(z)t=dΨX0,1(z)t.
Proof.
The starting point is the formula (3.53) for dΨX0,τ(z)t.
Note that ∥Jz∥s≲s∥z∥s+1 and ∥J−1z∥s+1≲s∥z∥s.
Hence it suffices to derive corresponding estimates for the operator
dΨXτ,0(ΨX0,τ(z))Lτ(ΨX0,τ(z))−1.
By Theorem 3.1, for any w∈h00, dΨXτ,0(w)[w] admits an expansion of the form
[TABLE]
where in the situation at hand
[TABLE]
By writing \mathcal{L}_{1}(w)^{-1}=\big{(}\text{Id}+J\mathcal{L}(w)\big{)}^{-1} as a Neumann series, its asymptotic expansion is then obtained
from Lemma 3.5 (cf also proof of Theorem 3.1).
Combining these results, one obtains the corresponding asymptotic expansion of dΨXτ,0(ΨX0,τ(z))Lτ(ΨX0,τ(z))−1.
The claimed estimate then follow from Lemma 3.5 and Theorem 3.1.
∎
As a second application of Theorem 3.1, we compute the Taylor expansion of the symplectic corrector ΨC(zS,z⊥) in z⊥ at [math].
This expansion will be needed in the subsequent section to show that the KdV Hamiltonian, when expressed in the new coordinates
provided by the map ΨL∘ΨC, is in Birkhoff normal
form up to order three. Note that by Theorem 3.1, for any zS∈VS′,z⊥∈h⊥0, 1≤k≤N,
[TABLE]
Hence the Taylor expansion of RN(z;ΨC) in z⊥ of order three at [math] reads
[TABLE]
with the Taylor remainder term RN,3(z;ΨC) given by
[TABLE]
whereas for any 1≤k≤N, {\cal F}_{\bot}\big{(}a_{k}(z;\Psi_{C})\partial_{x}^{-k}{\cal F}_{\bot}^{-1}[z_{\bot}]\big{)} vanishes in z⊥ at [math] up to order two.
Furthermore, according to Corollary 3.1, for any (zS,0)∈V′, RN((zS,0);dΨCt)=0 and hence for any
z∈h01, the Taylor expansion of RN(z;dΨCt)[z] of order 2 in z⊥ around [math] reads
[TABLE]
where RN,2(z;dΨCt)[z] denotes the Taylor remainder term of order 2.
Corollary 3.2**.**
(i)* For any integer N≥1, the Taylor expansion of the symplectic corrector ΨC(zS,z⊥) in z⊥ around [math] reads*
[TABLE]
where ΨC,3(z)≡ΨC,N,3(z) is given by
[TABLE]
For any s≥0, the map V′∩h0s→h0s+N+1, z↦RN,2(z;ΨC) is real analytic
and the following estimates hold: for any z∈V′∩h0s, z∈h0s,
[TABLE]
and, if in addition z1,…,zl∈h0s, l≥2,
[TABLE]
Similarly, for any s≥0, the map V′∩h0s→h0s+N+1, z↦RN,3(z;ΨC) is real analytic
and the following estimates hold: for any z∈V′∩h0s, z1,z2∈h0s,
[TABLE]
[TABLE]
and if in addition z1,…,zl∈h0s, l≥3,
[TABLE]
(ii)* For any integer N≥1 and z∈h01, the Taylor expansion of dΨC(zS,z⊥)t[z] in z⊥ around [math] is given by*
[TABLE]
where ΨC,1t(z)=RN,1(z;dΨCt) (cf (3.56)) and ΨC,2t(z)[z] has an expansion of the form
[TABLE]
with ak(z;dΨCt), Ak(z;dΨCt) given as in Corollary 3.1,
and RN,2(z;dΨCt)[z] given by (3.56).
For any i=1,2, s≥0,
[TABLE]
is a real analytic maps. Furthermore, for any z∈V′∩h0s, z∈h0s+1,
[TABLE]
and if in addition z1,…,zl∈h0s, l∈N,
[TABLE]
and for any z∈V′∩h0s, z∈h0s+1,z1∈h0s,
[TABLE]
[TABLE]
and if in addition z2,…,zl∈h0s, l≥2,
[TABLE]
[TABLE]
Proof.
(i) The claimed properties of RN,2(z;ΨC) follow directly from Theorem 3.1. In view of the formula (3.55)
the same is true for the ones of RN,3(z;ΨC).
Item (ii) is a direct consequence of Corollary 3.1.
∎
4 The KdV Hamiltonian in new coordinates
In this section we provide an expansion of the transformed KdV Hamiltonian H=Hkdv∘Ψ
where the map Ψ=ΨL∘ΨC is the composition of ΨL (cf Section 2) with the symplectic corrector ΨC (cf Section 3)
and Hkdv is the KdV Hamiltonian given by
[TABLE]
First we need to make some preliminary considerations. Recall that
for any finite subset S+⊂N, the Birkhoff map Ψkdv establishes a one to one correspondance between MS
and the set MS of S−gap potentials
where S=S+∪(−S+).
For any S−gap potential q, the corresponding KdV actions I=(IS,I⊥), defined in terms of the Birkhoff coordinates Φkdv(q), satisfy I⊥=0.
Denote by Ω⊥(IS)≡Ω⊥kdv(IS) and ΩS(IS)≡ΩSkdv(IS) the diagonal linear operators defined by
[TABLE]
[TABLE]
where for any n≥1,
[TABLE]
and ωn(I)≡ωnkdv(I) is the nth KdV frequency, viewed as a function of the actions.
By Lemma C.7, one has:
Lemma 4.1**.**
For any finite gap potential q∈MS, n≥1, and N≥1 one has
[TABLE]
where Ω2kae(IS)=ω2k−1ae(IS,0), R2NΩn(IS)=R2Nωn(IS,0)
and ω2k−1ae(IS,0), R2Nωn(IS,0) are given by Lemma C.7.
Assume that q(t) is a solution of the KdV equation (1.1) in MS with
z(t):=Φkdv(q(t))∈V for any t. Note that z(t) is of the form (zS(t),0),
the actions I=(In)n≥1 of q(t) are independent of t, and I=(IS,0)
where IS=(2πn1zn(0)z−n(0))n∈S+. Furthermore,
∂tzS(t)=JSΩS(IS)[zS(t)], or in more detail, for any n∈S,
[TABLE]
Denote by q(t) the solution of the equation, obtained by linearizing the KdV equation along q(t),
[TABLE]
We need to investigate ∂xd∇Hkdv(q(t))[q(t)] further.
If q(0) is of the form dΨL(zS(0),0)[0,z⊥(0)] (=Ψ1(zS(0))[z⊥(0)] ) with z⊥(0)∈h⊥3,
then by (2.2) (definition of ΨL)
and (2.3) (formula of the differential dΨL),
z⊥(t), defined by q(t)=Ψ1(zS(t))[z⊥(t)], solves the equation
[TABLE]
or more explicitly, for any n∈S+⊥,
[TABLE]
By differentiating q(t)=Ψ1(zS(t))[z⊥(t)] with respect to t, one gets
[TABLE]
Comparing (4.6) and (4.7)
and using that ∂tzS(t)=JSΩS(IS)[zS(t)], one gets
[TABLE]
Now apply Ψ1(zS(t))−1 to both sides of the latter equality yielding
[TABLE]
Since Ψ1(zS) is symplectic one has Ψ1(zS)t∂x−1Ψ1(zS)=J⊥−1 or
Ψ1(zS)−1∂x=J⊥Ψ1(zS)t,
implying that
[TABLE]
The latter identity implies that for any zS∈VS, IS=(2πn1znz−n)n∈S+, q=Ψkdv(zS,0), z⊥∈h⊥3,
[TABLE]
where G(zS):h⊥0→h⊥0 is given by
[TABLE]
In the next lemma we record an expansion for the operator G(zS).
Lemma 4.2**.**
For any integer N≥1, the operator G(zS):h⊥0→h⊥0 admits an expansion of the form
[TABLE]
where for any 1≤k≤N,s≥0,
the maps
[TABLE]
are real analytic.
Proof.
In view of the definition (4.12) of G,
the lemma follows from item (ii) of Theorem 2.1 (expansion of Ψ1(zS))
and Lemma E.2.
∎
After this preliminary discussion, we can now study the transformed Hamiltonian Hkdv∘Ψ where Ψ=ΨL∘ΨC.
We split the analysis into two parts. First we expand H(1):=Hkdv∘ΨL and then we analyze H(2)=H(1)∘ΨC.
Expansion of H(1):=Hkdv∘ΨL
To expand Hkdv∘ΨL, it is useful to write Hkdv(u) as Hkdv(u)=H2kdv(u)+H3kdv(u) where
[TABLE]
The L2−gradient ∇Hkdv of Hkdv and its derivative are then given by
[TABLE]
Let zS∈VS, q=Ψkdv(zS,0).
The Taylor expansion of Hkdv(q+v) around q in direction
v=Ψ1(zS)[z⊥]
with z⊥∈V⊥∩h⊥1 reads
[TABLE]
Since v=dΨkdv(zS,0)[0,z⊥] one has
⟨∇Hkdv(q),v⟩=∂y∣y=0Hkdv(Ψkdv(zS,yz⊥)).
Recall that Hkdv=Hkdv∘Ψkdv is a function of the actions alone and In=2πn1znz−n, n≥1.
It implies that
[TABLE]
and hence ⟨∇Hkdv(q),v⟩=0.
Since ΨL(z)=q+Ψ1(zS)[z⊥] one then gets
Since Ψ1(zS)td∇Hkdv(q)Ψ1(zS) and Ω⊥kdv(IS) are symmetric,
so is the operator G(zS).
In summary,
[TABLE]
where for any z=(zS,z⊥)∈V∩h01,
[TABLE]
Note that HSkdv(z)=HSkdv(ΠSz) where
ΠS:hS0×h⊥0→hS0×h⊥0 denotes the projection, given by
(zS,z⊥)↦(zS,0) (cf (3.9)).
We record that P2(1)(z) is quadratic and P3(1)(z) cubic in z⊥ where the superscript (1) refers to the Hamiltonian H(1).
Recall from (E.3) that for any a∈H1, the paraproduct Tau of the function a with u∈L2
with respect to the cut-off function χ is defined as (Tau)(x)=∑k,n∈Zχ(k,n)akunei2π(k+n)x
with un, n∈Z, denoting the Fourier coefficients of u.
Lemma 4.3**.**
For any integer N≥1, there exists an integer σN≥N (loss of regularity) so that on V∩h0σN,
the L2−gradient ∇P3(1) of P3(1) admits the asymptotic expansion of the form
[TABLE]
where for any s≥0, 1≤k≤N, the maps
[TABLE]
are real analytic. Furthermore, for any z∈V∩h0s+σN with ∥z∥σN≤1,
∥ak(z;∇P3(1))∥s≲s,N∥z⊥∥s+σN
and if in addition z1,…,zl∈h0s+σN, l≥1,
[TABLE]
Similarly, for any z∈V∩h0s∨σN with ∥z∥σN≤1, z∈h0s∨σN,
∥RN(z;∇P3(1))∥s+N+1≲s,N∥z⊥∥s∨σN∥z⊥∥σN and
[TABLE]
and if in addition z1,…,zl∈h0s∨σN, l≥2, then
[TABLE]
Proof.
By a straightforward calculation, one has
∇⊥P3(1)(z)=3Ψ1(zS)t(Ψ1(zS)[z⊥])2.
By the Bony decomposition given in Lemma E.1(ii),
[TABLE]
The expansion (4.18) and the stated estimates follow from Theorem 2.1(ii),
Corollary 2.2, and Lemmata E.1, E.2, E.3.
∎
Expansion of H(2):=H(1)∘ΨC
To compute the expansion of H(2)(z)=H(1)(ΨC(z)) on V′∩h01,
we study the composition of each of the terms in (4.16) with the symplectic corrector ΨC separately.
Recall that ΨC is defined on V′ and takes values in V.
Term HSkdv:
By Corollary 3.2, ΨC(z) has a Taylor expansion in z⊥ around [math] of the form
[TABLE]
where RN,2(z;ΨC) is the term of order two, given by RN,2(z;ΨC)=21d⊥2RN((zS,0);ΨC)[z⊥,z⊥] (cf (3.54)),
and ΨC,3(z) is given by (3.57)
[TABLE]
with RN,3(z;ΨC) denoting the Taylor remainder term (3.55).
Since HSkdv(z)=HSkdv(ΠSz) (cf (4.17)),
the Taylor expansion of HSkdv(ΨC(z))=HSkdv(z+Ψ~C(z)) reads
[TABLE]
where P3(2a)(z) is the Taylor remainder term of order three, given by
[TABLE]
and πS:hS0×h⊥0→hS0 denotes the map given by z=(zS,z⊥)↦zS (cf (3.10)).
Since πSΨC,3(z)=πSRN,3(z;ΨC) and πSΨ~C(z)=πSRN(z;ΨC),
one has
[TABLE]
In the next lemma we show that ∇P3(2a)(z) is in h0s+N+1 for any z∈V′∩h0s.
Lemma 4.4**.**
The Hamiltonian P3(2a):V′→R is real analytic and for any integers s≥0, N≥1,
the map V′∩h0s→h0s+N+1, z↦∇P3(2a)(z) is real analytic.
Furthermore, for any z∈V′∩h0s, and
z∈h0s,
[TABLE]
and if in addition z1,…,zl∈h0s, l≥2,
[TABLE]
Proof.
We begin by analyzing the first term
⟨∇SHSkdv(z),πSΨC,3(z)⟩ on the right hand side of (4).
It is given by the finite sum ∑n∈Shn(z) where
[TABLE]
and (en)n∈S denotes the standard basis of hS0.
The derivative of hn in direction z∈h00 then reads
[TABLE]
implying that
[TABLE]
By
Corollary 3.2, for any s≥0,
V′∩h0s→h0s+N+1, z↦∇hn(z) is real analytic and satisfies the estimates
∥∇hn(z)∥s+N+1≲s,N∥z⊥∥s∥z⊥∥0.
The estimates for the higher order derivatives of hn, n∈S, are obtained by differentiating the expression for ∇hn(z)
and using the estimates of
Corollary 3.2.
In order to analyze the second term on the right hand side of (4)
it suffices to study the functions hn,k(z), n,k∈S, given by
[TABLE]
where 0≤y≤1. Clearly, hn,k(z;y) depends continuously on y as do all the derivatives with respect to the variable z.
Since HSkdv(z+yΨ~C(z)) only depends on πS(z+yΨ~C(z))
one sees that
[TABLE]
implying that
[TABLE]
By Corollary 3.2, for any s≥0,
the map V′∩h0s→h0s+N+1, z↦∇hn,k(z;y) is real analytic and satisfies the estimate
∥∇hn,k(z;y)∥s+N+1≲s,N∥z⊥∥s∥z⊥∥02.
The estimates for the higher order derivatives are obtained by differentiating ∇hn,k
and applying again Corollary 3.2.
∎
Term HΩ(z):=21⟨Ω⊥(IS)[z⊥],z⊥⟩:
According to (4.3), the operator Ω⊥(IS) reads
For any integer N≥2, the operator Ω⊥(0)(IS) admits the expansion
[TABLE]
where for any 2≤k≤N and s≥0, the maps
[TABLE]
are real analytic.
To analyze HΩ(ΨC(z)), we write the quadratic form \big{\langle}\Omega_{\bot}(I_{S})[z_{\bot}],\,z_{\bot}\big{\rangle}, z⊥∈h01, as a sum
[TABLE]
and consider ⟨D⊥2[z⊥],z⊥⟩ and ⟨Ω⊥(0)(IS)[z⊥],z⊥⟩ separately.
When substituting for z⊥ in \big{\langle}D_{\bot}^{2}[z_{\bot}],z_{\bot}\big{\rangle}
the expression π⊥ΨC(z)=z⊥+π⊥Ψ~C(z), one gets
[TABLE]
where the map π⊥ is defined in (3.10). With a view towards the expansion of Hkdv∘Ψ, stated in Theorem 1.1,
we treat the difference
[TABLE]
as part of the error term P3(z). It needs special care since the two terms
[TABLE]
could have the property that the associated Hamiltonian vector field is unbounded.
We write
[TABLE]
and note that by the mean value theorem,
[TABLE]
where for τ∈[0,1], z∈V, PΩ(τ,z) is defined by
[TABLE]
In a first step we analyze PΩ(τ,z). One has
[TABLE]
Since HΩ=21⟨Ω⊥(IS)[z⊥],z⊥⟩
and Ω⊥(IS)=D⊥2+Ω⊥(0)(IS) one has
[TABLE]
Concerning the term 21⟨Ω⊥(IS)z⊥,π⊥X(τ,z)⟩ in (4.30), recall that
X(τ,z)=−Lτ(z)−1[JE(z)] (cf (3.7)),
Lτ(z)=Id+τJL(z) (cf (3.2))
and hence
[TABLE]
Since E(z)=(ES(z),0) and Jt=−J, the term \big{\langle}\Omega_{\bot}(I_{S})z_{\bot},\,\pi_{\bot}{X}(\tau,z)\big{\rangle}
becomes
[TABLE]
By (2.21) the component L⊥⊥(z) of L(z) vanishes, implying that
π⊥L(z)X(τ,z)=L⊥S(z)πSX(τ,z). Substituting the latter expression into (4.33)
and using that L⊥S(z)t=−LS⊥(z) since L(z) is skew adjoint (cf (2.20))
then leads to
Since Ω⊥(IS)=D⊥2+Ω⊥(0)(IS) and J⊥D⊥2=iD⊥3 we need
to analyze Ψ1(zS)iD⊥3. By Remark 2.2,
Ψ1(zS)iD⊥3 is a bounded linear operator h⊥s→H0s−3 for any s≥0.
Lemma 4.6**.**
For any integer N≥0, the operator T(zS):=Ψ1(zS)iD⊥3−F⊥−1iD⊥3F⊥Ψ1(zS) admits the expansion
[TABLE]
where for any s≥0, −1≤k≤N, the maps
[TABLE]
are real analytic. A similar statement holds for the transpose T(zS)t of T(zS).
Proof.
First note that the expression obtained from Ψ1(zS)iD⊥3−F⊥−1iD⊥3F⊥Ψ1(zS)
by replacing Ψ1(zS) by its highest order part F⊥−1 (cf Theorem 2.1),
vanishes. Since the order of the commutator of two scalar
pseudodifferential operators of order one is again of order one, it follows that
the operator T(zS) is of order 1, meaning that
the expansion of T(zS) is of the form as stated.
Taking into account that iD⊥3=−F⊥∂x3F⊥−1,
the claimed statements follow from Theorem 2.1 (expansion of Ψ1(zS))
and Corollary 2.2 (expansion of Ψ1(zS)t).
∎
Taking into account that J⊥Ω⊥(IS)=iD⊥3+J⊥Ω⊥(0)(IS),
the operator ∂x−1Ψ1(zS)J⊥Ω⊥(IS),
appearing in formula (4.35) reads
[TABLE]
By the definition of T(zS) and using that ∂x−1F⊥−1iD⊥3=−∂x2F⊥−1 , one then gets
[TABLE]
Altogether we thus have shown that the nth component \big{\langle}\partial_{x}^{-1}\Psi_{1}(z_{S})[J_{\bot}\Omega_{\bot}(I_{S})z_{\bot}]\,,\,\partial_{z_{n}}\Psi_{1}(z_{S})[z_{\bot}]\big{\rangle}, n∈S,
of LS⊥(z)[J⊥Ω⊥(IS)z⊥]
is given by
[TABLE]
where for any zS∈VS, the operator T1,n(zS) is given by
[TABLE]
Since (∂znΨ1(zS))t is one smoothing (cf Corollary 2.2) and
∂x−1T(zS) is of order zero (cf Lemma 4.6), one sees that
T1,n(zS) maps h⊥0 into h⊥1. More precisely, the following result holds.
Lemma 4.7**.**
For any n∈S and N∈N, the operator T1,n(zS), defined by (4.37) for zS∈VS, admits the expansion
[TABLE]
where for any s≥0, 1≤k≤N, the maps
[TABLE]
are real analytic.
Proof.
The claimed statements follow from Corollary 2.2, Lemmata 4.5, 4.6,
and Lemma E.2.
∎
We now turn our attention to the term -\big{\langle}\partial_{x}^{2}\Psi_{1}(z_{S})[z_{\bot}]\,,\,\partial_{z_{n}}\Psi_{1}(z_{S})[z_{\bot}]\big{\rangle}
in (4.36).
By (4.13)
[TABLE]
Hence using that −∂x2=d∇Hkdv(q)−6q one obtains for any n∈S
we conclude that -\big{\langle}\partial_{x}^{2}\Psi_{1}(z_{S})[z_{\bot}]\,,\,\partial_{z_{n}}\Psi_{1}(z_{S})[z_{\bot}]\big{\rangle} equals
[TABLE]
Using again that for any n∈S,
∂znΩ⊥(IS)=∂znΩ⊥(0)(IS),
one thus obtains
[TABLE]
where
[TABLE]
Lemma 4.8**.**
For any n∈S and any integer N≥0, the operator T2,n(zS):h⊥0→h⊥0, defined by (4.40) for zS∈VS, admits the expansion
[TABLE]
where for any s≥0, 0≤k≤N, the maps
[TABLE]
are real analytic.
A similar statement holds for the transpose T2,n(zS)t of the operator T2,n(zS).
Proof.
The lemma follows by Lemmata 2.2, 4.2, 4.5, and Lemma E.2.
∎
By (4.29) –
(4.31),
(4.34) –
(4.36),
and (4.40)
the Hamiltonian PΩ(τ,z), defined in (4.29), is given by
[TABLE]
where for any j∈S, zS∈VS, and 0≤τ≤1, the operator T3,j(τ,zS):h⊥0→h⊥0 is defined by
[TABLE]
The Hamiltonian PΩ(τ,z) has the following properties.
Lemma 4.9**.**
For any 0≤τ≤1 and any integer N≥0, the Hamiltonian PΩ(τ,⋅):V→R is real analytic and ∇PΩ(τ,z) admits the expansion
[TABLE]
where for any s≥0, 0≤k≤N, the maps
[TABLE]
are real analytic.
Furthermore, for any 0≤τ≤1, z∈V, z∈h00
[TABLE]
and if in addition, z1,…,zl∈h00, l≥2,
[TABLE]
Similarly, for any 0≤τ≤1, z∈V∩h0s, z1,z2∈h0s,
[TABLE]
[TABLE]
and if in addition z1,…,zl∈h0s, l≥3,
[TABLE]
Proof.
One has ∇SPΩ(τ,z)=(∂z−nPΩ(τ,z))n∈S with
[TABLE]
whereas ∇⊥PΩ(τ,z) can be computed to be
[TABLE]
The claimed statements then follow by Lemmata 3.6, 4.5, 4.7, 4.8.
∎
We are now ready to analyze the gradient of the Hamiltonian P3(2b)(z):=∫01PΩ(τ,ΨX0,τ(z))dτ (cf (4.28)).
Lemma 4.10**.**
The Hamiltonian P3(2b):V′→R is real analytic and for any integer N≥0, its gradient ∇P3(2b)(z) admits the expansion
[TABLE]
where for any s≥0, 0≤k≤N, the maps
[TABLE]
are real analytic. Furthermore, the following estimates hold: for any z∈V′, z∈h00,
[TABLE]
and if in addition z1,…,zl∈h00,l≥2, then
∥dlak(z;∇P3(2b))[z1,…,zl]∥s≲s,l∏j=1l∥zj∥0.
Similarly, for any z∈V′∩h0s, z1,z2∈h0s,
[TABLE]
[TABLE]
and if in addition z1,…,zl∈h0s,l≥2, then
[TABLE]
Proof.
By a straightforward computation, one has for any z∈V′,
[TABLE]
The claimed statements then follow by applying Corollary 3.1 (expansion of dΨX0,τ(z)t),
Lemma 4.9 (expansion of ∇PΩ(τ,z)),
Theorem 3.1 (expansion of ΨX0,τ(z)), and Lemma E.2.
∎
Terms P2(1), P3(1): Recall that the Hamiltonians P2(1) and P3(1) were introduced in (4.17). We write
[TABLE]
where by the mean value theorem
[TABLE]
The Hamiltonian P3(2c)(ΨC(z)) has the following properties.
Lemma 4.11**.**
The Hamiltonian P3(2c):V′∩h01→R is real analytic and for any integer N≥0 its gradient ∇P3(2c)(z) admits the expansion
[TABLE]
with the property that there exists an integer σN≥N (loss of regularity) such that for any s≥0, 0≤k≤N, the maps
[TABLE]
are real analytic. Furthermore, for any s≥0,z∈V′∩h0s+σN with ∥z∥σN≤1, z1,…,zl∈h0s+σN, l≥1,
[TABLE]
Similarly, for any s≥0,z∈V′∩h0s∨σN with ∥z∥σN≤1, z∈h0s∨σN,
[TABLE]
and if in addition z1,…,zl∈h0s∨σN, l≥2,
[TABLE]
Proof.
The lemma follows by differentiating the Hamiltonian P3(2c), defined in (4.43) and then applying Corollary 3.2,
Lemmata 4.2, 4.3 and using Lemmata E.1, E.2.
∎
By (4.16), (4.22), (4.27), (4.43) it follows that
for z=(zS,z⊥)∈V′, the Hamiltonian
H(2)(z) is given by
Note that P2(2) is quadratic with respect to z⊥, whereas P3(2)
is a remainder term of order three in z⊥.
Being quadratic with respect to z⊥, P2(2) can be written as
[TABLE]
The following vanishing lemma is due to Kuksin [19]. Since our setup is different from the one in [19],
we include its proof for the convenience of the reader.
Lemma 4.12**.**
The Hamiltonian P2(2) vanishes on V′.
Proof.
In view of (4.47), it suffices to prove that for any zS∈VS′, the operator d⊥∇⊥P2(2)(zS,0) vanishes.
We establish that d⊥∇⊥P2(2)(zS,0)=0 by studying the linearization of ∂tw=J∇H(2)(w) along an arbitrary
solution w(t) of the form w(t)=(wS(t),0).
First we need to make some preliminary considerations.
Let t↦q(t)∈MS be a solution of the KdV equation ∂tq=∂x∇Hkdv(q)
and denote by t↦z(t):=(zS(t),0) the corresponding solution in Birkhoff coordinates, defined by q(t)=Ψkdv(z(t)).
It satisfies ∂tz(t)=JΩ(IS)[z(t)].
Furthermore, let q(t) be the solution of the equation, obtained by linearizing the KdV equation along q(t),
[TABLE]
with initial data q0:=dΨkdv(zS(0),0)[0,z⊥0] and z⊥0∈h⊥3.
Similarly, denote by z(t) the solution of the equation, obtained by linearizing ∂tz=JΩ(IS)[z]
along the solution z(t) with initial data z0=(0,z⊥0),
∂tz(t)=Jd∇Hkdv(z(t))[z(t)].
Since ∂tz(t)=JΩ(IS)[z(t)] one concludes that
[TABLE]
and since Ψkdv is symplectic and Hkdv=Hkdv∘Ψkdv, one has
q(t)=dΨkdv(zS(t),0)[z(t)].
Recall that for any zS∈VS′, ΨL(zS,0)=Ψkdv(zS,0) (cf definition (2.2) of ΨL)
and ΨC(zS,0)=(zS,0)
(cf Corollary 3.2),
implying that Ψ(zS,0)=Ψkdv(zS,0) and hence q(t)=Ψ(zS(t),0) for any t.
Since Ψ:V′→H00 is symplectic and H(2)=Hkdv∘Ψ,
one sees that z(t)=(zS(t),0) is also a solution of the equation
∂tw=J∇H(2)(w).
With these preliminary considerations made, we are now ready to prove that d⊥∇⊥P2(2)(zS,0) vanishes.
To this end consider the solution w(t) of the equation obtained by linearizing ∂tw=J∇H(2)(w) along the solution z(t)=(zS(t),0)
with initial data w0=(0,z⊥0). Again using that the map Ψ is symplectic and H(2)=Hkdv∘Ψ,
it follows that dΨ(z(t))[w(t)] solves the linearized KdV equation. Since dΨ(z(0))=dΨkdv(z(0)) and w0=z0,
one then concludes from the uniqueness of the initial value problem that dΨ(z(t))[w(t)]=dΨkdv(z(t))[z(t)] and hence
w(t)=z(t) for any t. It means that z(t) satisfies also the linear equation
[TABLE]
In view of the expansion (4.44) of H(2) one then obtains
[TABLE]
Comparing the latter identity with (4.48) one concludes that in particular,
d⊥∇⊥P2(zS(0),0)=0. Since the initial data zS(0)∈VS′ can be chosen arbitrarily,
we thus have d⊥∇⊥P2(zS,0)=0 for any zS∈VS′ as claimed.
∎
In summary, we have proved the following results on the Hamiltonian H(2)=Hkdv∘Ψ.
Theorem 4.1**.**
The Hamiltonian H(2):V′∩h01→R has an expansion of the form
[TABLE]
where Ω⊥(IS) is given by (4.3) and the remainder term P3(2), defined by (4.45),
satisfies the following:
P3(2):V′∩h01→R is real analytic and for any integer N≥1, its gradient ∇P3(2)(z) admits the asymptotic expansion
[TABLE]
with the property that there there exists an integer σN≥N (loss of regularity) so that for any s≥0, 0≤k≤N, the maps
[TABLE]
are real analytic and satisfy the following estimates: for any s≥0,z∈V′∩h0s+σN with ∥z∥σN≤1,
z1,…,zl∈h0s+σN, l≥1,
[TABLE]
Similarly, for any s≥1, z∈V′∩h0s∨σN with ∥z⊥∥σN≤1, z∈h0s∨σN,
[TABLE]
and if in addition z1,…,zl∈h0s∨σN, l≥2,
[TABLE]
Proof.
The identity (4.49) folllows from formula (4.44) and Lemma 4.12.
The claimed asymptotic expansion of the gradient of P3(2) and its properties follow from
Lemmata 4.4, 4.10, 4.11 and Lemma E.1.
∎
5 Summary of the proofs of Theorem 1.1 and Theorem 1.2
In this section we summarize the proofs of Theorem 1.1, of its addendum, and of Theorem 1.2.
First recall that in view of the envisioned applications, these theorems are formulated in terms of action angle coordinates on the submanifold MSo of proper S−gap potentials.
Denote by Ξ the map relating action angle variables and complex Birkhoff coordinates,
[TABLE]
Clearly, Ξ is symplectic and, for any s≥0, the map Ξ:TS+×R>0S+×h⊥s→hS0×h⊥s, is real analytic.
Furthermore, in view of the definition (1.9), the map Ξ preserves the reversible structure.
Hence the claimed results for the map ΨL∘ΨC∘Ξ follow from the corresponding ones for the map ΨL∘ΨC.
In what follows we summarize the proofs of the results for ΨL∘ΨC corresponding to the ones claimed for ΨL∘ΨC∘Ξ.
Proof of Theorem 1.1. By a slight abuse of notation, the map Ψ of Theorem 1.1 is
defined to be the composition ΨL∘ΨC.
By (3.8), it is defined on the neighborhood V′=VS′×V⊥′
where VS′ is a bounded neighborhood of any given compact subset K⊂hS0 and V⊥′ is a ball in h⊥0
of radius smaller than 1, centered at [math]. The expansion of Ψ, corresponding to the one of (AE1),
follows from the expansion for the map ΨL, provided by Theorem 2.1
and the one for the map ΨC, provided by Theorem 3.1.
The expansion of the transpose dΨ(z)t of the derivative dΨ(z), corresponding to the one of (AE2),
follows from the fact that Ψ:V′→L02 is symplectic, meaning that
for any z∈V′, the operator dΨ(z)t:H01→h01 satisfies dΨ(z)t=J−1(dΨ(z))−1∂x.
The expansion of Ψ(z) in (AE1) then leads to an expansion
of dΨ(z) and in turn of (dΨ(z))−1 and hence of dΨ(z)t. In addition, the identity dΨ(z)t=J−1(dΨ(z))−1∂x
implies that the coefficient a1(z;dΨt) in the expansion of dΨt satisfies a1(z;dΨt)=−a1(z;Ψ).
The expansion of the Hamiltonian H(2) and of the remainder term P3(2),
corresponding to the one in (AE3), are provided in Theorem 4.1.
□
Proof of Addendum to Theorem 1.1. Clearly, the Fourier transform F and its inverse preserve
the reversible structure and by Proposition D.1, so do the Birkhoff map Φkdv and its inverse Ψkdv.
Furthermore, by the Addendum to Theorem 2.1, and the Addendum to Theorem 3.1
also the maps ΨL and ΨC and hence ΨL∘ΨC preserve the reversible structure, as do the coefficients and the remainder terms
in their expansions as well as the transpose of their derivatives.
Clearly, the KdV Hamiltonian Hkdv is reversible and therefore so is H(2)=Hkdv∘Ψ.
By (4.49) one then concludes that also the remainder P3(2) is reversible.
□
Proof of Theorem 1.2. The estimates of the coefficients and the remainder in the expansion of Ψ=ΨL∘ΨC, corresponding to the ones of (Est1),
follow from the estimates of the coefficients and the remainder in the expansion of the map ΨL, provided by Theorem 2.1,
and the ones of the coefficients and the remainder in the expansion of the map ΨC, provided by Theorem 3.1.
The estimates of the coefficients and the remainder in the expansion of dΨ(z)t, corresponding to the one of (Est2),
follow from the fact that Ψ:V′→L02 is symplectic, meaning that for any z∈V′,
dΨ(z)t:H01→h01 satisfies dΨ(z)t=J−1(dΨ(z))−1∂x
and the estimates (Est1) of the coefficients and the remainder in the expansion of Ψ(z) which lead to corresponding estimates
of the coefficients and the remainder in the expansion of dΨ(z) and in turn of (dΨ(z))−1.
The estimates of the remainder term P3(2) in the expansion of the Hamiltonian H(2)=Hkdv∘Ψ, corresponding to (Est3),
are provided by Theorem 4.1.
□
Appendix A Birkhoff map
In this appendix we review the Birkhoff map and properties of it, relevant for our purposes. We refer to [13] and [9], [14], [16] for more details
in these matters.
There exists an open neighborhood W of L02 in L0,C2 and a real analytic map
[TABLE]
with Φkdv(0)=0 so that the following holds:
(B0)
For any n∈N, the complex Birkhoff coordinates zn(q),z−n(q) are related to the Birkhoff coordinates xn(q),yn(q) as introduced in **[13]**
by the formulas (1.4) .
(B1)
For any s∈Z≥0, the restriction of Φkdv to H0s gives rise to a map Φkdv:H0s→h0s which is a bi-analytic diffeomorphism.
(B2)
The map Φkdv is canonical, meaning that on W, {zn,z−n}=i2πn for any n∈N and the brackets between all other coordinate functions vanish.
(B3)
The Hamiltonian Hkdv∘(Φkdv)−1, defined on h01, only depends on the actions (In)n∈N(cf (1.5)).
More precisely, it can be viewed as a real analytic map Hkdv on a complex neighborhood of the positive quadrant ℓ+1,3 in ℓ1,3(N,C)(cf (1.6)).
(B4)
The differential d0Φkdv of Φkdv at [math] is the
Fourier transform F(cf (1.7)).
(B5)
The nonlinear part of the Birkhoff map, Akdv:=Φkdv−F, and the one of its inverse, Bkdv:=(Φkdv)−1−F−1,
are one smoothing. More precisely, for any s∈N,
Akdv:H0s→h0s+1 and Bkdv:h0s→H0s+1 are real analytic.
*The inverse of Φkdv is denoted by Ψkdv.
*
To continue we first need to introduce some more notations and review properties of the Schrödinger operator −∂x2+q.
For any s∈Z≥0, denote by HCs[0,1]≡Hs([0,1],C) the Sobolev space of functions
f:[0,1]→C with the property that for any 0≤j≤s, the distributional derivative ∂xjf is in LC2[0,1]≡L2([0,1],C).
Similarly, H0,Cs≡H0s(T,C) denotes the Sobolev space of functions q:T→C in Hs(T,C) with ∫01q(x)dx=0.
For any q∈L0,C2≡H0,C0 and λ∈C, we denote by yj(x,λ)≡yj(x,λ,q), j=1,2, the fundamental solutions
of −y′′+qy=λy. These are the solutions satisfying the initial conditions y1(0,λ)=1, y1′(0,λ)=0 and
y2(0,λ)=0, y2′(0,λ)=1. It is well known that for any s∈Z≥0 and 1≤j≤2, the map
[TABLE]
is analytic (cf [24]).
For q in L0,C2, the Schrödinger operator −∂x2+q, considered on the interval [0,2] with periodic boundary conditions, has a discrete spectrum.
It consists of a sequence of complex numbers
bounded from below. We list them lexicographically and with algebraic multiplicities, i.e.,
λ0+⪯λ1−⪯λ1+⪯λ2−⪯… where λn±≡λn±(q) (cf [13]).
They are referred to as periodic eigenvalues of q and satisfy the asymptotic estimates λn+,λn−=n2π2+ℓn2,
valid uniformly on bounded subsets of L0,C2 (cf [13]).
For real valued q, the periodic eigenvalues are real and come in isolated pairs, meaning that
λ0+<λ1−≤λ1+<λ2−≤λ2+<….
We remark that for any given finite subset S+⊆N, the manifold MS of S-gap potentials defined in the introduction, coincides with the set
\big{\{}q\in L^{2}_{0}:\lambda_{n}^{-}(q)=\lambda_{n}^{+}(q)\,\,\forall\,n\in S_{+}^{\bot}\big{\}}.
By shrinking the neigbourhood W of
Theorem A.1, if needed, one can ensure that for any q∈W, the closed intervals
[TABLE]
are disjoint from each other. By a slight abuse of terminology, we refer to the closed interval Gn, n≥1, as the n’th gap and to γn≡γn(q)
as the n’th gap length, γn:=λn+−λn− and denote by τn≡τn(q) the middle point of Gn, τn=(λn++λn−)/2.
Due to the asymptotic behaviour of the periodic eigenvalues, (Gn)n≥1 admit mutually disjoint neighbourhoods
Un⊆C, n≥1, with Gn⊆Un, referred to as isolating neighbourhoods.
They can be chosen locally independently of q (cf [13]).
Denote by F(λ)≡F(λ,q) the Floquet matrix
[TABLE]
and introduce the discriminant Δ(λ)≡Δ(λ,q):=Tr(F(λ,q)), its derivative Δ˙(λ)≡Δ˙(λ,q):=∂λΔ(λ,q),
and the anti-discriminant δ(λ)≡δ(λ,q)=m1(λ,q)−m2′(λ,q).
The functions mj(λ)≡mj(λ,q) and
mj′(λ)≡mj′(λ,q)
are analytic on C×L0,C2. The entire functions Δ2(λ)−4 and Δ˙(λ) have product representations
(see [13, Proposition B.10, Proposition B.13])
[TABLE]
where πn=nπ for any n≥1 and where the zeroes λ˙n≡λ˙n(q) satisfy the asymptotic estimate λ˙n=n2π2+ℓn2.
We also need to consider the operator −∂x2+q on [0,1] with Dirichlet and Neumann boundary conditions. For any q in L0,C2,
the corresponding spectra are again discrete, consisting of sequences of complex numbers, bounded from below.
They are referred to as Dirichlet and respectively, Neumann eigenvalues of q. We list them lexicographically and with their algebraic multiplicities
μ1⪯μ2⪯μ3⪯… and ν0⪯ν1⪯ν2⪯… .
The μn≡μn(q) and νn≡νn(q) satisfy the asymptotics μn,νn=n2π2+ℓn2, valid uniformly on bounded subsets of L0,C2.
For real valued q, the Dirichlet and the Neumann eigenvalues are real and satisfy
[TABLE]
By shrinking the neighbourhood W of Theorem A.1, if needed, one can assure that for any q∈W there exist isolating neighbourhoods
(Un)n≥1 so that for any n≥1, μn,νn,τn,λ˙n∈Un, whereas λ0+ and ν0 are not contained in any of the Un’s (cf [13]). Isolating neighbourhoods with this additional property
can also be chosen locally independently of q. Note that for q∈W, the Dirichlet und Neumann eigenvalues are all simple and are analytic functions on W.
Similarly, τn and λ˙n, n∈N, are analytic on W. In addition,
m2(λ) and m1′(λ) admit the product representations (cf [13, Proposition B.6])
[TABLE]
Let S+⊂N be finite and set S=S+∪(−S+). For any s∈Z≥0, we identify h0s with hS0×h⊥s and h0,Cs with CS×h⊥,Cs.
The manifold MS of S−gap potentials is given by Ψkdv(hS0×{0}). By item (B1) of Theorem A.1 it then follows that MS⊂∩s≥0H0s.
Actually, potentials in MS are real analytic functions.
For our purposes, it is useful to consider the Hilbert spaces H0,Cw:={q∈L0,C2:∥q∥w≡∥(qn)n=0∥w<∞} and
h0,Cw:={(zn)n=0∈ℓ0,C2:∥(zn)n=0∥w<∞}
where
[TABLE]
The weight w=(wn)n∈Z is referred to as Gevrey weight and the Hilbert space H0,Cw as weighted Sobolev space. Functions in H0,Cw are Gevrey smooth.
Correspondingly, we define the real Hilbert spaces H0w:={q∈H0,Cw:q\mboxrealvalued} and h0w:={(zn)n=0∈h0,Cw:z−n=zn∀n≥1}.
To fix ideas we will only consider the Gevrey weight with parameters r=0,a=1, and σ=1/2 und denote it by w∗, but any other choice of a Gevrey weight would also be possible.
Note that MS⊂H0w∗ and that H0,Cw∗ naturally embeds into H0,Cs for any s∈Z≥0.
According to [14, Addendum 1 to Theorem 5], we have the following
Addendum to Theorem A.1 *The restriction of Φkdv to H0w∗ gives rise to a map Φkdv:H0w∗→h0w∗
which is a bi-analytic diffeomorphism. In particular, for any q∈MS, there exists a neighborhood Vq∗ of q in H0,Cw∗∩W and a neighborhood
Vz(q)∗ of z(q)=Φkdv(q) in h0,Cw∗ so that the restriction of Φkdv to Vq∗ gives rise to a real analytic diffeomorphism
Φkdv:Vq∗→Vz(q)∗. The neighborhood Vz(q)∗ can be chosen to be of the form VzS(q)∗×V0,⊥∗
where VzS(q)∗ is a neighborhood of zS(q)=(zn(q))n∈S in CS and V0,⊥∗ is a ball in h⊥,Cw, centered at [math]
with radius depending on q.
We denote the set Ψkdv(VzS(q)∗×{0}) by Vq,S∗. It consists of complex valued S−gap potentials near q. *
Appendix B Floquet solutions
In this appendix we obtain formulas for Floquet solutions f±n(x,q), n∈S+⊥, for potentials q in MS
which will be used in Proposition 2.2 of Section 2 to relate these solutions to
the differentials of the complex Birkhoff coordinates z±n(q).
The resulting formulas are a key ingredient for proving the asymptotic expansion of the map ΨL (cf Section 2).
Without further reference, we will use the notations estabished in Appendix A.
We begin by recalling the notion of Floquet solutions of −y′′+qy=λy for any given q∈L02 and λ∈R.
The eigenvalues κ±(λ)≡κ±(λ,q) of the Floquet matrix F(λ) (cf (A.1)) are given by the roots of {\rm det}\big{(}F(\lambda)-\kappa{\rm Id}_{2\times 2}\big{)}=\kappa^{2}-\Delta(\lambda)\kappa+1.
For λ in (\lambda_{0}^{+},\infty)\setminus\big{(}\bigcup_{n\geq 1}[\lambda_{n}^{-},\lambda_{n}^{+}]\big{)} one has
κ±(λ)=2Δ(λ)∓21cΔ2(λ)−4∈C
where cΔ2(λ)−4 denotes the canonical root determined by
{\rm sign}\big{(}\sqrt[c]{\Delta^{2}(\lambda)-4}\big{)}=-{\rm i} for λ0+<λ<λ1− (cf [13, definition (6.10)]).
For \lambda\in(\lambda_{0}^{+},\infty)\setminus\big{(}\bigcup_{n\geq 1}[\lambda_{n}^{-},\lambda_{n}^{+}]\big{)},
m2(λ)=0 (λ is not a Dirichlet eigenvalue), m1′(λ)=0 (λ is not a Neumann eigenvalue)
and (1,a+(λ))∈C2 is an eigenvector of F(λ) corresponding to the eigenvalue κ+(λ)
[TABLE]
where a+(λ)≡a+(λ,q) is given by
[TABLE]
Similarly, (1,a−(λ))∈C2, a−(λ)≡a−(λ,q),
is an eigenvector of F(λ) corresponding to the eigenvalue κ−(λ),
[TABLE]
If λn+ is a double periodic eigenvalue, one has λn−=λn+=τn and F(τn)=(−1)nId2×2.
By de l’Hospital’s rule, the formulas in (B.1) - (B.2) admit limits at such eigenvalues.
Recall that S+⊆N is finite, S+⊥=N∖S+ and S=S+∪(−S+).
We denote by ˙ the derivative with respect to λ.
Lemma B.1**.**
For any q∈MS and n∈S+⊥, the following holds:
(i)* (−1)nm˙2(τn)>0, (−1)n+1Δ¨(τn)>0.*
(ii)* The limit a±n≡a±n(q):=limλ→τna±(λ,q) exists and*
[TABLE]
(iii)* One has m1˙′(τn)=0 and*
[TABLE]
Remark B.1**.**
Recall that for any given q∈MS, Vq,S∗ is the set of S−gap potentials, introduced at the end of Appendix A.
By shrinking W of Theorem A.1, if needed, the expressions in the formulas for a±n, n∈S+⊥, of item (ii) and (iii) of Lemma B.1
are well defined, real analytic functions on Vq,S∗ and the formulas for a±n continue to hold for any potential in Vq,S∗ (cf Appendix A).
Proof.
(i) For any q∈MS and n∈S+⊥, τn=μn, m1(τn)=(−1)n, m2′(τn)=(−1)n, and
m˙2(μn)=(−1)n∫01y2(x,μn)2dx
(cf [13, Proposition B.4]). Since τn is a nondegenerate critical point of Δ, one has Δ˙(τn)=0 and Δ¨(τn)=0.
Furthermore, one has Δ(τn)=(−1)n2 and (−1)n+1Δ¨(τn)>0.
(ii) It is well known that F(λ) is real analytic in λ (cf Appendix A). Expanding m1(λ) and m2(λ) at τn, n∈S+⊥ , one has
[TABLE]
and
\Delta(\lambda)=(-1)^{n}2+\frac{\ddot{\Delta}(\tau_{n})}{2}(\lambda-\tau_{n})^{2}+O\big{(}(\lambda-\tau_{n})^{3}\big{)}\,.
It follows that for λn−1+<λ<λn+1−,
[TABLE]
(where we set cΔ2(τn)−4=0).
Combining these asymptotic estimates, the claimed formula (B.3) then follows from (B.1) - (B.2).
(iii) Since τn is a Neumann eigenvalue and Neumann eigenvalues are simple, it follows that m˙1′(τn)=0.
Expanding m1′(λ), m2′(λ) at τn one gets
For q∈MS and n∈S+⊥, we define the Floquet solutions f±n(x)≡f±n(x,q) at τn by
[TABLE]
By Lemma B.1 and Remark B.1 they are welldefined for any potential in Vq,S∗.
Furthermore, consider the normalized solutions Hn(x)≡Hn(x,q) and Gn(x)≡Gn(x,q) of −y′′+qy=τny,
[TABLE]
[TABLE]
One then has Gn(0)=0 and
[TABLE]
Note that for any q∈MS, f−n(x,q)=fn(x,q), and
Hn(x,q) and Gn(x,q) are the normalized real and respectively imaginary parts of fn(x,q).
In addition, they satisfy Hn(0,q)>0 and Gn′(0,q)>0 by the formulas above.
Hence given q∈MS, by shrinking Vq,S∗, if needed, we can assume that ReHn(0)>0 and ReGn′(0)>0 on Vq,S∗
for any n∈S+⊥.
Proposition B.1**.**
*For any q∈MS and n∈S+⊥ the following holds:
(i) For any s∈Z≥0, Hn(⋅,p), Gn(⋅,p), and f±n(⋅,p) are
analytic maps in p∈Vq,S∗ with values in HCs[0,1].
(ii) For any p∈Vq,S∗, the Floquet solutions*
[TABLE]
have the property that Hn,Gn are the unique solutions of −y′′+py=τny,
satisfying the following normalization conditions: (ii1)∫01Hn(x)Gn(x)dx=0 and
[TABLE]
Proof.
(i) Since for any s∈Z≥0, H0,Cw∗ embeds into the Sobolev space H0,Cs the claimed analyticity statements follow from the results
recorded in Appendix A.
(ii) Clearly, the statement on uniqueness follows from the uniqueness of the initial value problem for −y′′+qy=τny.
Hence it remains to prove that Gn and Hn satisfy items (ii1) - (ii3). In view of item (i), it suffices to verify these normalisation conditions on MS.
By [24], Theorem 6, page 21, one has
[TABLE]
[TABLE]
To prove (ii1) it is to show that J:=∫01(Refn(x))y2(x,τn)dx=0. By (B.5)-(B.9),
[TABLE]
Since Δ˙(τn)=0 and at the same time Δ˙(τn)=m˙1(τn)+m˙2′(τn)
one concludes that J=0.
(ii2) By the definition of Gn, one has Gn(0)=0 and Gn′(0)>0.
To see that ∫01Gn(x)2dx=1, note that
[TABLE]
implying that ∫01Gn(x)2dx=1.
(ii3) Since Refn(0)=y1(0,τn)=1, one has Hn(0)>0 whereas
By the definition (B.5), it is therefore to show that
[TABLE]
This latter identity follows by combining the two formulas for an, given in Lemma B.1.
∎
Appendix C Asymptotic expansions
The main purpose of this appendix is to provide for any S−gap potential q an asymptotic expansion of the Floquet solutions f±n(x)≡f±n(x,q)
as n→∞. These expansions are a key ingredient for proving the asymptotic expansion of the map ΨL, stated in
Theorem 2.1 in Section 2.
At the end of this appendix we provide an asymptotic expansion for the KdV frequencies for S−gap potentials, needed for the expansion of the KdV Hamiltonian
in the new coordinates.
Throughout this appendix, if not mentioned otherwise,
we assume that q∈MS where S=S+∪(−S+) and S+⊂N is a finite subset.
Furthermore, Vq,S∗ is the neighborhood of q, introduced at the end of Appendix A.
If not mentioned otherwise,
μ denotes the principal branch +μ of the square root, defined for μ∈C∖(−∞,0].
Recall that for any p∈Vq,S∗, one has ∫01p(x)dx=0 and
[TABLE]
where yj(x,λ), j=1,2, denote the fundamental solutions of
−y′′+py=λy, a±n are the complex numbers given by (B.3), and
τn=(λn++λn−)/2. Note that if p is real valued, then
[TABLE]
Theorem C.1**.**
Let q∈MS and N∈Z≥0. Then for any p∈Vq,S∗, the Floquet solutions fn, n∈S⊥,
have an expansion as ∣n∣→∞ of the form
[TABLE]
where for any s≥0, the coefficients Vq,S∗→HCs, p↦fkae(⋅,p), k≥1, are real analytic and
the remainder Vq,S∗→HCs, p↦RNfn(⋅,p), is analytic.
In addition, for any given j≥0,
[TABLE]
where the constant CN,j≥1 can be chosen locally uniformly for p in Vq,S∗.
To prove Theorem C.1, we first need to establish some auxiliary results.
Lemma C.1**.**
For any q∈MS and any integers N,M≥0, the following holds: for any p∈Vq,S∗ and ν∈C∖{0}, there exist solutions yN,M(x,ν)≡yN,M(x,ν,p)
of −y′′+py=ν2y of the form
[TABLE]
The functions ykae(x)≡ykae(x,p), k≥1, are defined inductively by
[TABLE]
and for any s∈Z≥0, the maps Vq,S∗→HCs[0,1], p↦ykae(⋅,p), are real analytic.
The remainder y~N,M(x,ν,p) satisfies y~N,M(0,ν,p)=0, ∂xy~N,M(0,ν,p)=∑k=1M(2iν)k∂xyN+kae(0,p)
and has the property that for any s∈Z≥0, (C∖{0})×Vq,S∗→HCs[0,1], (ν,p)↦y~N,M(⋅,ν,p)
is analytic. Furthermore, if ν∈R∖{0} and p is real valued then yN,M(x,−ν,p)=yN,M(x,ν,p).
In addition, for any given c>0, the remainder y~N,M(⋅,ν,p) satisfies
[TABLE]
where the constant CN,M can be chosen locally uniformly in p∈Vq,S∗.
Remark C.1**.**
By (C.5), for any k≥1 and s≥k−1,
the map ykae:H0,Cs→HCs−k+2[0,1],q↦ykae(⋅,q) is real analytic.
Writing Q(x):=∫0xq(t)dt, the formulas for y1ae,y2ae, and y3ae read as follows:
[TABLE]
[TABLE]
Proof.
For any p∈Vq,S∗ and ν=0, the solutions yN,M(x,ν)≡yN,M(x,ν,p) of −y′′+py=ν2y are obtained from solutions of the form
[TABLE]
with an appropriate choice of N1. Solutions of the form (C.7) were studied in [21, Chapter 1, Section 4]. Here for any k≥1,
ykae(x)≡ykae(x,p) is defined by (C.5)
and yN1(x,ν)≡yN1(x,ν,p) is the unique solution of the inhomogeneous ODE
[TABLE]
satisfying the initial conditions
[TABLE]
Clearly, for any s≥0 and k≥1, the maps Vq,S∗→HCs[0,1], p↦ykae(⋅,p), are real analytic.
Arguing as in [13, Chapter 1], one sees that for any s≥0, the map (C∖{0})×Vq,S∗→HCs[0,1], (ν,p)↦y~N1(⋅,ν,p)
is analytic. Furthermore, note that yN1(0,ν)=0 and ∂xyN1(0,ν)=iν+∑k=1N1(2iν)k∂xykae(0).
It then follows that for any ν=0,yN1(x,ν) is a solution of −y′′+py=ν2y. Indeed
[TABLE]
Hence by (C.5) and (C.8), \big{(}-\partial_{x}^{2}+p-\nu^{2}\big{)}y_{N_{1}}=0.
The solution yN,M(x,ν) is then defined as follows
[TABLE]
Since by the definition (C.5), ykae(0)=0 for any k≥1 and by (C.9), yN+M(0,ν)=0
one concludes that yN,M(0,ν)=0. Furthermore, since by (C.9) ∂xyN+M(0,ν)=0, one has
[TABLE]
and by the arguments above, for any s≥0, the map (C∖{0})×Vq,S∗→HCs[0,1], (ν,p)↦y~N,M(⋅,ν,p) is analytic.
Furthermore, if ν∈R∖{0} and p is real valued then
[TABLE]
Since yN,M(0,±ν)=1 and yN,M(0,ν) and yN,M(0,−ν) both solve −y′′+py=ν2y
it follows by the uniqueness of the initial value problem that yN,M(⋅,−ν)=yN,M(⋅,ν).
It remains to show the estimate (C.6). Note that for any p∈Vq,S∗, the terms (2iν)k−1yN+kae(x), 1≤k≤M,
satisfy an estimate of the type (C.6). Hence it suffices to show that
[TABLE]
for some constant CN,M>0.
By (C.8), (C.9), yN+M solves the initial value problem
[TABLE]
By the method of the variation of the constants it is given by
[TABLE]
where
K(x,t,ν2)=y1(x,ν2)y2(t,ν2)−y1(t,ν2)y2(x,ν2), satisfying the estimates (cf [13, Chapter 1])
[TABLE]
[TABLE]
for some constant C>0. It then follows from (C.12) and (C.5) that
sup0≤x≤1∣Imν∣≤c,∣ν∣≥1∣yN+M(x,ν)∣≤C.
Since K(x,x,ν2)=0 one has that
[TABLE]
implying that
sup0≤x≤1∣Imν∣≤c,∣ν∣≥1∣ν∣∣∂xyN+M(x,ν)∣≤C.
Using equation (C.11) one gets
[TABLE]
yielding
sup0≤x≤1∣Imν∣≤c,∣ν∣≥1∣ν∣2∣∂x2yN+M(x,ν)∣≤C.
By taking derivatives of (C.13), one then concludes that there exists a constant CN,M>0 so that for any 0≤j≤M,
sup0≤x≤1∣Imν∣≤c,∣ν∣≥1∣ν∣j∣∂xjyN+M(x,ν)∣≤CN,M.
Going through the arguments of the proof one concludes that the constant CN,M can be chosen locally uniformly for p∈Vq,S∗.
∎
Let q∈MS and N,M≥0. Then for any p∈Vq,S∗ and ν=0 with ∣ν∣ sufficiently large, the solutions yN,M(x,ν) and yN,M(x,−ν) of
−y′′+py=ν2y, considered in Lemma C.1,
are linearly independent. Indeed by Lemma C.1, for any ν=0,
[TABLE]
implying that the Wronskian of yN,M(⋅,−ν) and yN,M(⋅,ν) equals
[TABLE]
Hence there exists νb≥1 so that
[TABLE]
The bound νb can be chosen locally uniformly in p∈Vq,S∗. It then follows that for ∣ν∣≥νb, y1(x,ν2), y2(x,ν2) are linear combinations
of yN,M(x,ν) and yN,M(x,−ν),
[TABLE]
[TABLE]
and
[TABLE]
[TABLE]
We note that βN,M(−ν)=−βN,M(ν) and for ∣ν∣ sufficiently large, αN,M(ν)≃21 and βN,M(ν)≃2iν1.
Furthermore, in case p is real valued and ν∈R with ∣ν∣≥νb, one has
[TABLE]
implying that βN,M(ν) is purely imaginary.
Finally, to prove Theorem C.1, the following two additional results are needed.
It is well know that τn=(λn++λn−)/2 admits an asymptotic expansion as n→∞ (cf e.g. [15, Theorem 1.3]).
More precisely, we have the following
Lemma C.2**.**
Let q∈MS and N∈Z≥0. Then for any p∈Vq,S∗, τn(p),n∈S+⊥, has an expansion of the form
[TABLE]
where Vq,S∗→C, p↦τ2kae(p), k≥1, and Vq,S∗→C, p↦R2Nτn(p)
are real analytic.
As a consequence, choosing n0≥mS:=1+\mboxmax{n∈S} so that Re(τn(p))>0 for any n≥n0, it follows that
2iτn(p), n≥n0, admits an expansion of the form
[TABLE]
where Vq,S∗→C, p↦τ2kae(p), k≥2, and Vq,S∗→C, p↦R2Nτn(p)
are real analytic.
In addition, the remainders R2Nτn(p) and R2Nτn(p) satisfy
[TABLE]
where the constants CN>0 and n0>mS can be chosen locally uniformly for p∈Vq,S∗.
Proof.
The functions τ2kae(q), k≥2, are given by polynomial expressions of integrals of densities, involving q and its derivatives up to order 2k (cf [15])
and are real analytic maps, H0,Ck→C,q↦τ2kae(q). Since τn is real analytic on Vq,S∗ so is
[TABLE]
The claimed bounds for R2Nτn(p) were established in [15].
In view of the asymptotics of τn(p), one finds n0≥mS with the claimed properties and then obtains the coefficients τ2kae(p)
from the expansion of τn(p) in a recursive way and concludes that they are real analytic. Since τn(p) is real analytic
one again concludes that the remainder term R2Nτn(p) is real analytic as well and deduces the claimed bounds.
∎
The second result concerns the asymptotic expansion of the coefficients an, defined in (B.3).
Lemma C.3**.**
Let q∈MS and N∈Z≥0. Then for any p∈Vq,S∗, an(p), n∈S⊥, has an expansion of the form
[TABLE]
where Vq,S∗→C, p↦akae(p), k≥0, are real analytic and Vq,S∗→C, p↦RNan(p) is analytic.
In addition, the remainders RNan(p) satisfy
[TABLE]
where the constant CN>0 can be chosen locally uniformly for p∈Vq,S∗.
Proof.
To start with, we compute the leading term in the expansion of an. Recall that by (B.3),
[TABLE]
By (B.8) - (B.9), for any n∈S+⊥,
m˙1(τn)=(−1)n∫01y1(t,τn)y2(t,τn)dt and
m˙2(τn)=(−1)n∫01y2(x,τn)2dx,
yielding
[TABLE]
Since \sqrt{\tau_{n}}=n\pi\big{(}1+O(\frac{1}{n^{4}})\big{)} (Lemma C.2) and hence y1(t,τn)=cos(nπt)+O(n1) and
y2(t,τn)=nπsin(nπt)+O(n21) (cf [24, Chapter 1]) one has
[TABLE]
To analyze the quotient −m˙2(τn)Δ¨(τn) we use the product representation
of Δ˙(λ) and m2(λ) (cf Appendix A),
[TABLE]
Since for n∈S+⊥, λn+=λ˙n=μn=τn,
[TABLE]
and one concludes that
[TABLE]
Altogether we thus have proved that for any n∈S+⊥,
[TABLE]
Expressing y1(t,τn) and y2(t,τn) in terms of yN,M(x,±τn) (cf (C.15), (C.17)),
one obtains an expansion of the form (C.21) where the coefficients akae can be explicitly computed by using the expansion of yN,M(x,ν),
obtained in Lemma C.1 and the one of τn of Lemma C.2.
It follows that for any k≥0, the map Vq,S∗→C, p↦akae(p) is analytic. In case p is real valued one has
a−n=an (cf definition (B.3) of a±n). By an inductive argument it then follows from the expansion
of an+a−n that for any k≥0, the coefficient akae is real valued.
With regard to the remainder term, since for any n∈S⊥,an is analytic on
Vq,S∗ (cf Remark B.1) one sees that RNan is analytic on Vq,S∗.
The claimed estimates are obtained from the corresponding estimates of Lemma C.1 and Lemma C.2.
∎
Proof of Theorem C.1. Let q∈MS and N≥0. To prove that for p∈Vq,S∗,
fn(x,p) has an expansion of the form (C.2) we first note that since y1(x,τn)=cos(nπx)+O(n1), y2(x,τn)=nπ1sin(nπx)+O(n21),
and a±n=inπ+O(1), one has f±n(x)=e±iπnx+O(n1). To obtain the expansion as claimed,
we want to apply Lemma C.1.
Choose M≥0 (arbitrarily large) and n0≥mS (cf Lemma C.2) so that Reτn>0 and in addition
∣τn∣≥νb for any n≥n0 where νb≥1 is given by (C.14).
We then substitute the formulas (C.15) and (C.17) with ν2=τn
into the expression (C.1) for f±n(x)≡f±n(x,p) to get for n≥n0
[TABLE]
Using the expansions of τn (Lemma C.2), a±n (Lemma C.3),
and yN,M(x,ν) (Lemma C.1) one gets an expansion of fn, ∣n∣≥n0, of the form (C.2)
where the coefficients fkae, k≥1,
and the remainder RNfn can be explicitly computed. One verifies that for any s≥0 and k≥1,
fkae:Vq,S∗→HCs[0,1] is analytic.
Furthermore, by choosing M sufficiently large and using
the estimates of the lemmas referred to above, one obtains the claimed estimate (C.3) of RNfn for any ∣n∣≥n0.
Note that at this point, we only know that fkae(⋅,p) is an element in HCs[0,1] for any s≥0.
But since e−iπnxfn(x) is one periodic in x, it follows by induction that for any k≥1, fkae(x) is one periodic in x as well.
Since in case p is real valued, e−iπnxfn(x)=eiπnxf−n(x)
one reads off from the expansions of e−iπnxfn(x) and eiπnxf−n(x) that fkae, k≥1, are real valued.
Altogether this shows that for any s≥0 and k≥1, fkae:Vq,S∗→HCs is real analytic.
For n∈S⊥ with ∣n∣<n0, we define RNfn(x) by
[TABLE]
We then conclude that for any n∈S⊥, RNfn(x) is one periodic in x. Furthermore,
since for any n∈S⊥ and s≥0, e−iπnxfn:Vq,S∗→HCs is analytic (cf (C.1)) it follows that
RNfn:Vq,S∗→HCs is analytic as well.
Going through the arguments of the proof one sees that the estimate (C.3) holds for any n∈S⊥ and that the constant CN,j in
(C.3) can be chosen locally uniformly for p∈Vq,S∗. □
The next result states how the map Srev, defined in Section 1,
acts on the functions fn(x,q) and how on the coefficients and the remainder of its expansion.
Proof of Addendum to Theorem C.1. Let q∈MS and n∈S+⊥. By Lemma D.1, one knows that
τn(Srev(q))=τn(q) and
[TABLE]
where τn≡τn(q).
Recall that a±n is given by a±n=−m˙2(τn)m˙1(τn)±i(−1)nm˙2(τn)(−1)n+1Δ¨(τn)/2.
Note that again by Lemma D.1, one has
[TABLE]
Since Δ˙(τn,q)=0 and hence m˙2′(τn,q)=−m˙1(τn,q) it then follows that m˙1(τn,Srevq)=−m˙1(τn,q).
Combining all these identities one concludes that a±n(Srevq)=−a∓n(q) and hence by (C.26)
[TABLE]
as claimed. Considering the expansions of the latter identities one obtains (C.25). □
To obtain the asymptotic expansion for ΨL, presented in Section 2,
we need to establish such an expansion for each of the factors appearing in the definition (2.7) of W±n(q) for a finite gap potential q.
First we consider the factor ξn which compares the square root of the n’th action
with the n’th gap length. For any q∈W (cf Theorem A.1) with γn(q)=0, it is given by 8In(q)/γn2(q).
In case γn(q)=0, it can be computed by a limiting argument. By a slight abuse of terminology,
we denote this limit also by 8In(q)/γn2(q).
Lemma C.4**.**
Let q∈MS and N∈Z≥0. Then for any p∈Vq,S∗,
ξn(q):=8In(q)/γn2(q), n∈S+⊥, has an expansion of the form
[TABLE]
where Vq,S∗→C, p↦ξ2kae(p), k≥1, and Vq,S∗→C, p↦R2Nξn(p),
are real analytic.
In addition, the remainders R2Nξn(p) satisfy
[TABLE]
where the constant CN>0 can be chosen locally uniformly for p∈Vq,S∗.
Proof.
Let q∈MS and N∈Z≥0.
Following the proof of [13, Theorem 7.3], for any p∈Vq,S∗ and n∈S+⊥, 8In(p)/γn2(p) can be computed
by considering a sequence of Sn-gap potentials (pj)j≥1 in W (cf Theorem A.1) with γn(pj)>0 so that pj→p as j→∞
where Sn:=S∪{−n,n}.
One then obtains in the limit the formula 8In(p)/γn2(p)=χ(τn(p),p) where χ(λ)≡χ(λ,p) is given by
λ−λ01∏k∈S+(λk+−λ)(λk−−λ)λ−λ˙k, implying that
for n≥n0 with n0≥mS chosen so that Re(τn(p))>0 for any n≥n0 (cf Lemma C.2)
[TABLE]
Combining (C.28)
with the expansion of τn (cf Lemma C.2) then
yields the expansion
[TABLE]
where Vq,S∗→C, p↦ξ2kae(p), k≥1, are real analytic and supn∈S+⊥∣R2Nξn(p)∣ is bounded.
For n∈S+⊥ with n<n0, R2Nξn(p) is defined by (2\pi{\rm i}n)^{2N+2}\big{(}\sqrt{n\pi}\xi_{n}(p)-1-\sum_{k=1}^{N}\frac{\xi_{2k}^{ae}(p)}{(2\pi{\rm i}n)^{2k}}\big{)}.
Since for any n∈S+⊥, nπξn is real analytic on Vq,S∗ , so is RNξn(p).
Going through the arguments of the proof one sees that the constant CN in (C.27) can be chosen locally uniformly for p∈Vq,S∗.
∎
Next we prove an expansion for the factor m˙2(τn(q),q)/Δ¨(τn(q),q) in (2.7) for q∈MS.
More precisely, we show the following
Lemma C.5**.**
Let q∈MS and N∈Z≥0. Then for any p∈Vq,S∗,
dn(p):=−m˙2(τn(p),p)/Δ¨(τn(p),p), n∈S+⊥,
has an expansion of the form
[TABLE]
where Vq,S∗→C, p↦d2kae(p), k≥1, and Vq,S∗→C, p↦R2Ndn(p),
are real analytic.
In addition, the remainders R2Ndn(p) satisfy
[TABLE]
where the constant CN>0 can be chosen locally uniformly for p∈Vq,S∗.
Proof.
Let q∈MS and N∈Z≥0 be given.
For any p∈Vq,S∗, m2(λ)≡m2(λ,p) admits the product representation (cf Appendix A)
m2(λ)=∏k≥1π2k2μk−λ
where (μk)k≥1 denote the Dirichlet eigenvalues of the operator −∂x2+p, listed in lexicograpic order. By (A.2), Δ˙(λ) also admits such a representation,
Δ˙(λ)=−∏k≥1π2k2λ˙k−λ with (λ˙k)k≥1 being listed in lexicographic order.
Since (μk)k≥1,(λ˙k)k≥1 are simple
[TABLE]
For any n∈S+⊥, one has μn=λ˙n=τn and hence one concludes that for n sufficiently large so that Reτn>0,
[TABLE]
Combining this with the results of τn (Lemma C.2) then yields the expansion of the stated form.
Going through the arguments of the proof one concludes that d2kae, k≥1, and R2Ndn have the claimed properties.
∎
It remains to prove that the factors e±iβn(q), appearing in the definition (2.7) of W±n(x,q),
admit an expansion as well. Clearly, it suffices to prove such an expansion for βn(q).
Recall that for any q∈MS and n∈S+⊥, βn(q) is given by
βn(q)=∑ℓ∈S+βℓn(q) ([13, Theorem 8.5]) and by [13, page 70],
[TABLE]
where δ(λ)≡δ(λ,q) denotes the anti-discriminant. Here we used that for any ℓ∈S+⊥∖{n}, one has μℓ=λℓ−
and hence βℓn(q)=0. Furthermore recall that by [13, Theorem 8.1] ψn(λ,q) is an entire function of λ.
Lemma C.6**.**
Let q∈MS and N∈Z≥0. After shrinking Vq,S∗, if needed, it follows that for any p∈Vq,S∗,
βn(p), n∈S+⊥, admits an expansion of the form
[TABLE]
where Vq,S∗→C, p↦β2kae(p), k≥1, and Vq,S∗→C, p↦R2Nβn(p),
are real analytic.
In addition, the remainders R2Nβn(p) satisfy
[TABLE]
where the constant CN>0 can be chosen locally uniformly for p∈Vq,S∗.
Proof.
Let p∈Vq,S∗ and n∈S+⊥. Since p is an S−gap potential, it follows from [13, Theorem 8.5] that the quotient of ψn(λ)≡ψn(λ,p)
with Δ2(λ)−4≡Δ2(λ,p)−4 is of the form
[TABLE]
where up to a sign, the complex numbers sjn≡sjn(p), 0≤j≤M−1, are the symmetric functions of the roots σℓn, ℓ∈S+,
of ψn(λ), M=∣S∣, and R(λ)≡R(λ,p) is given by
[TABLE]
Here we used that for any k=n with λk+=λk−, the eigenvalue λk+ is also a root of ψn(λ)
and we listed the roots σℓn, ℓ∈S+, in lexicographic order. Without loss of generality
we thus may assume in the sequel that λℓ+=λℓ− for any ℓ∈S+. It then follows that for any ℓ∈S+,
[TABLE]
Using Lemma C.2, one concludes that τn−λn2π2=1+O(n21) and shows in a straightforward way that τn−λn2π2
and hence the integrals ∫λℓ−μℓ∗Rλjτn−λn2π2dλ admit an expansion
in (2πin)2k1, k≥0, with coefficients and remainder having properties as stated.
It thus remains to show that for any 0≤j≤M−1, sjn also admits such an expansion.
By the uniqueness statement of [13, Proposition D.7] (and after shrinking Vq,S∗, if needed,) it follows that (sjn)0≤j≤M−1
is the unique solution of the following inhomogeneous, linear M×M system
[TABLE]
It then follows that det(En)=0 where En≡En(p) denotes the M×M matrix with coefficients
[TABLE]
Therefore,
[TABLE]
Using once again the expansion of τn of Lemma C.2 one shows that sjn, 0≤j≤M−1, admit an expansion
in (2πin)2k1, k≥0, with coefficients and remainder having properties as stated. As an aside, we remark that by
[13, Proposition D.7], limn→∞σℓn=λ˙ℓ, ℓ∈S+, and hence limn→∞sjn=sj
for any 0≤j≤M−1 where up to signs, (sj)0≤j≤M−1 are the symmetric polynomials of λ˙ℓ,ℓ∈S+.
One then concludes that σℓn=λ˙ℓ+O(n21), ℓ∈S+, and in turn sjn=sj+O(n21), 0≤j≤M−1.
∎
We finish this appendix by proving an expansion of the KdV frequencies ωn≡ωnkdv (cf Section 1) at finite gap potentials.
Using the Birkhoff map, we view them as functions of the potential, which by a slight abuse of notation, we denote also by ωn.
Lemma C.7**.**
Let q∈MS and N∈Z≥0. Then for any p∈Vq,S∗, the KdV frequencies ωn(p), n∈S+⊥,
have an expansion of the form
[TABLE]
where Vq,S∗→C, p↦ω2k−1ae(p), k≥1, and Vq,S∗→C, p↦R2Nωn(p),
are real analytic.
In addition, the remainders R2Nωn(p) satisfy
[TABLE]
where the constant CN>0 can be chosen locally uniformly for p∈Vq,S∗.
Proof.
Let q∈MS and N∈Z≥0 be given.
The basic ingredient into our proof of (C.30) are formulas of the frequencies
in terms of periods of an Abelian differential of the second kind on the hyperelliptic Riemann surface Σp,
associated to the periodic spectrum of Lp=−∂x2+p (see [5], [6], [8], [17], [22]).
We follow [17, Section 2] and note that the arguments made there extend to complex valued potentials: for any p∈Vq,S∗, denote by Σp the compact Riemann surface
associated to the simple periodic eigenvalues of p,
[TABLE]
where J≡J(p):={j∈S+:λj+(p)=λj−(p)}. The variable z∈C around the point z=0 gives a complex chart in a neighborhood of the
branch point ∞∈Σp via the substitution λ=−z21. By construction, this chart is defined uniquely up to a change of sign
of the variable z, z↦−z, and is referred to as standard chart. Then Σp admits an Abelian differential Ω4
of the second kind, uniquely determined by the following properties: (i) Ω4 is holomorphic on Σp∖{∞};
(ii) near ∞, Ω4 is of the form
[TABLE]
in the appropriate standard chart; (iii) ∫ajΩ4=0 for any j∈J
where aj are the smooth cycles around the gap [λj−,λj+] defined in [17, Section 2].
The differential Ω4 is of the form
[TABLE]
where M:=∣J(p)∣ and the coefficients c1,…,cM+1 are real analytic functions on Vq,S∗. Then by [17, formula (2.19)],
[TABLE]
where bn, n≥1, are the cycles as defined in [17, Section 2]. Let
mS:=1+max{k∈S}. Then for any n≥mS, λn−=λn+=τn.
It then follows from the definition of the cycles bn that for any n≥mS
[TABLE]
with the appropriate choice of the root in the denominator of Ω4.
The abelian integral ∫τmSλΩ4 has an expansion as λ→∞ of the form
[TABLE]
and hence as n→∞
[TABLE]
In view of the formula [17, (2.20)] of Ω4, the coefficients b∗,b∗∗,b0,b1,… are real analytic functions on Vq,S∗.
Furthermore, it is well known
(cf e.g. [16, Proposition 8.1]) that since ∫01p(x)dx=0
[TABLE]
Combining (C.32) - (C.34)
with the results on τn and τn of Lemma C.2
one obtains an expansion of ωn, n≥mS, of the form (C.30)
where ω2k−1ae:Vq,S∗→C, k≥1, and R2Nωn:Vq,S∗→C, n≥mS, are real analytic
and R2Nωn:Vq,S∗→C, n≥mS, have the claimed bounds.
For n∈S+⊥ with n<mS, one defines R2Nωn by (C.30) and
since ωn are real analytic on Vq,S∗, one then concludes that R2Nωn, n∈S+⊥,
are real analytic on Vq,S∗ and satisfy the claimed bounds.
∎
Appendix D Reversibility structure
In this appendix we prove that the Birkhoff map Φkdv and hence also its inverse Ψkdv preserve the reversible structure,
defined by the maps
[TABLE]
Proposition D.1**.**
One has
[TABLE]
As a consequence, Srev∘Ψkdv=Ψkdv∘Srev and by the chain rule, for any q∈L02(T) and w∈h00
[TABLE]
First we establish some preliminary results. Recall that yj(x,q)≡yj(x,λ,q), j=1,2, denote the fundamental solutions of −y′′+qy=λy,
Δ(λ)≡Δ(λ,q) the discriminant, and δ(λ)≡δ(λ,q) the anti-discriminant,
[TABLE]
In a straightforward way, one verifies the following
Lemma D.1**.**
For any q∈L02, λ∈C, x∈R,
[TABLE]
or alternatively,
[TABLE]
The latter identities imply that
[TABLE]
An immediate consequence of the first identity in (D.1) is that
For any q∈L02, the action variables In≡In(q), n≥1, are defined by contour integrals (cf. [13, p 64]),
[TABLE]
Furthermore the normalizing factor ξn≡ξn(q), defined for q∈L02 with γn(q)>0 by ξn=8In/γn2,
extends analytically to L02 (cf [13, Theorem 7.3]). By [13, Theorem 8.5], βn=∑k=nβkn is well defined on L02
where βkn≡βkn(q) is given by (cf [13, p 70])
[TABLE]
with the sign of Δ2(λ)−4 determined by ∗Δ(μk)−4=δ(μk). On the other hand, ηn≡ηn(q) and θn≡θn(q)
are well defined modul 2π on L02∖Zn by
[TABLE]
where Z_{n}=\big{\{}q\in L^{2}_{0}:\gamma_{n}(q)=0\big{\}}.
One then concludes from (D.1), (D.2), (D.3) that the following holds.
Corollary D.1**.**
For any q∈L02 and n≥1,
[TABLE]
Furthermore on L02∖Zn, θn(Srevq)=−θn(q) modulo 2π.
With these preparations made we now prove Proposition D.1.
Proof of Proposition D.1. For any n≥1 and q∈L02∖Zn, the complex Birkhoff coordinates zn(q),z−n(q) are given by
zn(q)=nπIn(q)e−iθn(q), z−n(q)=nπIn(q)eiθn(q), whereas for q∈Zn, zn(q)=0 and z−n(q)=0.
Hence it follows from Corollary D.1 that zn(Srevq)=z−n(q) and z−n(Srevq)=zn(q) for any n≥1. This proves that Φkdv∘Srev=Srev∘Φkdv.
□
Appendix E Properties of pseudodifferential and paradifferential calculus
In this appendix we collect some well known facts about pseudodifferential and paradifferential calculus on the torus. We refer to [23] for further details.
Let χ∈C∞(R2,R) be an admissible cut-off function. It means that χ is an even function
and that there exist
0<ε1<ε2<1 so that for any (ϑ,η)∈R2 and α,β∈Z≥0,
[TABLE]
[TABLE]
For any a∈H1, the paraproduct Tau of the function a with u∈L2 (with respect to the cut-off function χ) is defined as
[TABLE]
where we recall that un, n∈Z, denote the Fourier coefficients of u, un=∫01u(x)e−2πinxdx.
Note that since a, u, and χ are real valued and χ is even, Tau is real valued as well.
Given any s,s′∈Z, we denote by B(Hs,Hs′) the Banach space of all bounded linear operators
Hs→Hs′, endowed with the operator norm ∥⋅∥B(Hs,Hs′).
In case s=s′, we also write B(Hs) instead of B(Hs,Hs). Given any linear operator A∈B(Hs,Hs′),
we denote by At the transpose of A with respect to the L2−inner product. It is an element in B((Hs′)∗,(Hs)∗)
where (Hs)∗ denotes the dual of Hs.
Lemma E.1**.**
(i)* For any s∈Z≥0 and a∈H1, the linear operator Ta:u↦Tau is in B(Hs). Furthermore
the linear map H1→B(Hs),a↦Ta, is bounded, ∥Ta∥B(Hs)≲s∥a∥1.*
(ii)* Let a∈Hs1,b∈Hs2 and s1,s2∈Z≥1. Then*
[TABLE]
where the bilinear map R(B):Hs1×Hs2→Hs1+s2−1, (a,b)↦R(B)(a,b), is continuous
and satisfies the estimate
[TABLE]
(iii)* Let a∈Hρ with ρ∈Z≥2. Then for any s≥0, Tat−Ta∈B(Hs,Hs+ρ−1) and*
[TABLE]
(iv)* Let a,b∈Hρ with ρ∈Z≥1. Then for any s≥0, T_{a}\circ T_{b}-T_{ab}\in{\cal B}\big{(}H^{s},H^{s+\rho-1}\big{)} and*
[TABLE]
Lemma E.2**.**
(i)* Let k,j∈Z≥0 and a∈C∞(T). Then for any s∈Z≥0 and N∈N with N≥k+j, the composition
∂x−k∘a∂x−j is a bounded linear operator Hs→Hs+k+j which admits an expansion of the form*
[TABLE]
where Ci(k,j), 1≤i≤N−k−j, are constants depending on k,j and the remainder RN,k,jψdo(a) is a bounded linear operator
Hs→Hs+N+1,
satisfying the estimate
[TABLE]
(ii)* Let k,j∈Z≥0 and N≥k+j. There exists a constant σN>N−k−j+1 such that for any a∈HσN
and any s∈Z≥0, the composition ∂x−k∘Ta∘∂x−j is a bounded linear operator
Hs→Hs+k+j which admits an expansion of the form*
[TABLE]
where Ci(k,j), 1≤i≤N−k−j, are constants depending on k,j and for any s≥0, the remainder RN,k,j(B)(a)
is a bounded linear operator Hs→Hs+N+1, satisfying the estimate
[TABLE]
Finally, we record the following well known tame estimates of products of functions in Sobolev spaces.
Lemma E.3**.**
For any s∈Z≥1,
[TABLE]
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