Volume 2013, Issue 1 909782
Research Article
Open Access

On the Spectral Asymptotics of Operators on Manifolds with Ends

Sandro Coriasco

Corresponding Author

Sandro Coriasco

Dipartimento di Matematica, Università degli Studi di Torino, V. C. Alberto, n. 10, I-10123 Torino, Italy dm.unito.it

Search for more papers by this author
Lidia Maniccia

Lidia Maniccia

Dipartimento di Matematica, Università degli Studi di Torino, V. C. Alberto, n. 10, I-10123 Torino, Italy dm.unito.it

Search for more papers by this author
First published: 11 April 2013
Citations: 8
Academic Editor: Changxing Miao

Abstract

We deal with the asymptotic behaviour, for λ → +, of the counting function NP(λ) of certain positive self-adjoint operators P with double order (m, μ), m, μ > 0, mμ , defined on a manifold with ends M. The structure of this class of noncompact manifolds allows to make use of calculi of pseudodifferential operators and Fourier integral operators associated with weighted symbols globally defined on n. By means of these tools, we improve known results concerning the remainder terms of the Weyl Formulae for NP(λ) and show how their behaviour depends on the ratio m/μ and the dimension of M.

1. Introduction

The aim of this paper is to study the asymptotic behaviour, for λ → +, of the counting function
()
where λ1λ2 ≤ ⋯ is the sequence of the eigenvalues, repeated according to their multiplicities, of a positive order, self-adjoint, classical, elliptic SG-pseudodifferential operator P on a manifold with ends. Explicitly, SG-pseudodifferential operators P = p(x, D) = Op(p) on n can be defined via the usual left-quantization
()
starting from symbols p(x, ξ) ∈ C(n × n) with the property that, for arbitrary multiindices α, β, there exist constants Cαβ ≥ 0 such that the estimates
()
hold for fixed m,   μ and all (x, ξ) ∈ n × n, where , yn. Symbols of this type belong to the class denoted by Sm,μ(n), and the corresponding operators constitute the class Lm,μ(n) = Op(Sm,μ(n)). In the sequel we will sometimes write Sm,μ and Lm,μ, respectively, fixing once and for all the dimension of the (noncompact) base manifold to n.
These classes of operators, introduced on n by Cordes [1] and Parenti [2], see also Melrose [3] and Shubin [4], form a graded algebra, that is, Lr,ρLm,μLr+m,ρ+μ. The remainder elements are operators with symbols in ; that is, those having kernel in 𝒮(2n), continuously mapping 𝒮(n) to 𝒮(n). An operator P = Op(p) ∈ Lm,μ and its symbol pSm,μ are called SG-elliptic if there exists R ≥ 0 such that p(x, ξ) is invertible for |x| + |ξ| ≥ R and
()
In such case we will usually write PELm,μ. Operators in Lm,μ act continuously from 𝒮(n) to itself and extend as continuous operators from 𝒮(n) to itself and from Hs,σ(n) to Hsm,σμ(n), where Hs,σ(n), s, σ, denotes the weighted Sobolev space
()
Continuous inclusions Hs,σ(n)↪Hr,ρ(n) hold when sr and σρ, compact when both inequalities are strict, and
()
An elliptic SG-operator PLm,μ admits a parametrix ELm,−μ such that
()
for suitable K1, K2L,− = Op(S,−), and it turns out to be a Fredholm operator. In 1987, Schrohe [5] introduced a class of noncompact manifolds, the so-called SG-manifolds, on which it is possible to transfer from n the whole SG-calculus. In short, these are manifolds which admit a finite atlas whose changes of coordinates behave like symbols of order (0,1) (see [5] for details and additional technical hypotheses). The manifolds with cylindrical ends are a special case of SG-manifolds, on which also the concept of SG-classical operator makes sense; moreover, the principal symbol of an SG-classical operator P on a manifold with cylindrical ends M, in this case a triple σ(P) = (σψ(P), σe(P), σψe(P)) = (pψ, pe, pψe), has an invariant meaning on M, see Egorov and Schulze [6], Maniccia and Panarese [7], Melrose [3], and Section 2. We indicate the subspaces of classical symbols and operators adding the subscript  cl  to the notation introduced above.

The literature concerning the study of the eigenvalue asymptotics of elliptic operators is vast and covers a number of different situations and operator classes, see, for example, the monograph by Ivrii [8]. Then, we only mention a few of the many existing papers and books on this deeply investigated subject, which are related to the case we consider here, either by the type of symbols and underlying spaces, or by the techniques which are used. We refer the reader to the corresponding reference lists for more complete informations. On compact manifolds, well-known results were proved by Hörmander [9] and Guillemin [10], see also the book by Kumano-go [11]. On the other hand, for operators globally defined on n, see Boggiatto et al. [12], Helffer [13], Hörmander [14], Mohammed [15], Nicola [16], and Shubin [4]. Many other situations have been considered, see the cited book by Ivrii. On manifolds with ends, Christiansen and Zworski [17] studied the Laplace-Beltrami operator associated with a scattering metric, while Maniccia and Panarese [7] applied the heat kernel method to study operators similar to those considered here.

Here we deal with the case of manifolds with ends for , positive and self-adjoint, such that m, μ > 0, mμ, focusing on the (invariant) meaning of the constants appearing in the corresponding Weyl formulae and on achieving a better estimate of the remainder term. Note that the situation we consider here is different from that of the Laplace-Beltrami operator investigated in [17], where continuous spectrum is present as well. In fact, in view of Theorem 14, spec(P) consists only of a sequence of real isolated eigenvalues {λj} with finite multiplicity.

As recalled above, a first result concerning the asymptotic behaviour of NP(λ) for operators including those considered in this paper was proved by Maniccia and Panarese in [7], giving, for λ → +,
()
Note that the constants C1, C2, above depend only on the principal symbol of P, which implies that they have an invariant meaning on the manifold M, see Sections 2 and 3. On the other hand, in view of the technique used there, the remainder terms appeared in the form o(λn/min {m,μ}) and o(λn/mlog λ) for mμ and m = μ, respectively. An improvement in this direction for operators on n had been achieved by Nicola [16], who, in the case m = μ, proved that
()
while, for mμ, showed that the remainder term has the form O(λ(n/min  {m,μ})−ε) for a suitable ε > 0. A further improvement of these results in the case m = μ has recently appeared in Battisti and Coriasco [18], where it has been shown that, for a suitable ε > 0,
()

Even the constant has an invariant meaning on M, and both and are explicitly computed in terms of trace operators defined on .

In this paper the remainder estimates in the case mμ are further improved. More precisely, we first consider the power Q = P1/max {m,μ} of P (see Maniccia et al. [19] for the properties of powers of SG-classical operators). Then, by studying the asymptotic behaviour in λ of the trace of the operator , ψλ(t) = ψ(t)eitλ, , defined via a Spectral Theorem and approximated in terms of Fourier Integral Operators, we prove the following.

Theorem 1. Let M be a manifold with ends of dimension n and let be a positive self-adjoint operator such that m, μ > 0, mμ, with domain Hm,μ(M)↪L2(M). Then, the following Weyl formulae hold for λ → +:

()
where ε1 = min {1/μ, n((1/m) − (1/μ))} and ε2 = min {1/m, n((1/μ) − (1/m))}.

The order of the remainder is then determined by the ratio of m and μ and the dimension of M, since
()

In particular, when max  {m, μ}/min  {m, μ} ≥ 2, the remainder is always O(λn/max  {m,μ}).

Examples include operators of Schrödinger type on M, that is, P = −Δg + V, Δg the Laplace-Beltrami operator in M associated with a suitable metric g, V a smooth potential that, in the local coordinates xUNn on the cylindrical end growths as 〈x〉 μ, with an appropriate μ > 0 related to g. Such examples will be discussed in detail, together with the sharpness of the results in Theorem 1, in the forthcoming paper [20], see also [21].

The key point in the proof of Theorem 1 is the study of the asymptotic behaviour for λ → + of integrals of the form
()
where a and φ satisfy certain growth conditions in x and ξ (see Section 3 for more details). The integrals I(λ) represent in fact the local expressions of the trace of , obtained through the so-called “geometric optic method,” specialised to the SG situation, see, for example, Coriasco [22, 23], Coriasco and Rodino [24]. To treat the integrals I(λ) we proceed similarly to Grigis and Sjöstrand [25], Helffer and Robert [26], see also Tamura [27].

The paper is organised as follows. Section 2 is devoted to recall the definition of SG-classical operators on a manifold with ends M. In Section 3 we show that the asymptotic behaviour of NP(λ), λ → +, for a positive self-adjoint operator , m, μ > 0, is related to the asymptotic behaviour of oscillatory integrals of the form I(λ). In Section 4 we conclude the proof of Theorem 1, investigating the behaviour of I(λ) for λ → +. Finally, some technical details are collected in the Appendix.

2. SG-Classical Operators on Manifolds with Ends

From now on, we will be concerned with the subclass of SG-operators given by those elements PLm,μ(n), (m, μ) ∈ 2, which are SG-classical, that is, P = Op(p) with . We begin recalling the basic definitions and results (see, e.g., [6, 19] for additional details and proofs).

Definition 2. (i) A symbol p(x, ξ) belongs to the class if there exist , i = 0,1, …, positively homogeneous functions of order mi with respect to the variable ξ, smooth with respect to the variable x, such that, for a 0-excision function ω,

()
(ii) A symbol p(x, ξ) belongs to the class if there exist , k = 0, …, positively homogeneous functions of order μk with respect to the variable x, smooth with respect to the variable ξ, such that, for a 0-excision function ω,
()

Definition 3. A symbol p(x, ξ) is SG-classical, and we write , if

(i) there exist such that for a 0-excision function ω, and

()
(ii) there exist such that for a 0-excision function ω, and
()
We set .

Remark 4. The definition could be extended in a natural way from operators acting between scalars to operators acting between (distributional sections of) vector bundles. One should then use matrix-valued symbols whose entries satisfy the estimates (3).

Note that the definition of SG-classical symbol implies a condition of compatibility for the terms of the expansions with respect to x and ξ. In fact, defining and on and , respectively, as

()
It is possibile to prove that
()

Moreover, the composition of two SG-classical operators is still classical. For the triple σ(P) = (σψ(P), σe(P), σψe(P)) = (pm, p·,μ, pm,μ) = (pψ, pe, pψe) is called the principal symbol of P. The three components are also called the ψ-, e- and ψe-principal symbol, respectively. This definition keeps the usual multiplicative behaviour, that is, for any , , (r, ρ), (s, σ) ∈ 2, σ(RS) = σ(S)σ(T), with component-wise product in the right-hand side. We also set

()
for a fixed 0-excision function ω. Theorem 5 allows to express the ellipticity of SG-classical operators in terms of their principal symbol.

Theorem 5. An operator is elliptic if and only if each element of the triple σ(P) is nonvanishing on its domain of definition.

As a consequence, denoting by {λj} the sequence of eigenvalues of P, ordered such that jkλjλk, with each eigenvalue repeated accordingly to its multiplicity, the counting function is well defined for a SG-classical elliptic self-adjoint operator P see, for example, [16, 18, 20, 21]. We now introduce the class of noncompact manifolds with which we will deal.

Definition 6. A manifold with a cylindrical end is a triple (M, X, [f]), where M = C𝒞 is a n-dimensional smooth manifold and

  • (i)

    is a smooth manifold, given by = (M0D) ∪ C with a n-dimensional smooth compact manifold without boundary M0, D a closed disc of M0, and CD a collar neighbourhood of D in M0;

  • (ii)

    𝒞 is a smooth manifold with boundary 𝒞 = X, with X diffeomorphic to D;

  • (iii)

    f : [δf, ) × 𝕊n−1𝒞, δf > 0, is a diffeomorphism, f({δf} × 𝕊n−1) = X and f({[δf, δf + εf)} × 𝕊n−1), εf > 0, is diffeomorphic to C;

  • (iv)

    the symbol ∐C means that we are gluing and 𝒞, through the identification of C and f({[δf, δf + εf)} × 𝕊n−1);

  • (v)

    the symbol [f] represents an equivalence class in the set of functions

    ()

where f ~ g if and only if there exists a diffeomorphism Θ ∈ Diff(𝕊n−1) such that
()
for all ρ ≥ max {δf, δg} and γ𝕊n−1.

We use the following notation:
  • (i)

    ;

  • (ii)

    𝒞τ = f([τ, ) × 𝕊n−1), where τδf. The equivalence condition (22) implies that 𝒞τ is well defined;

  • (iii)

    π : n∖{0} → (0, ) × 𝕊n−1 : xπ(x) = (|x | , x/|x|);

  • (iv)

    is a parametrisation of the end. Let us notice that, setting , the equivalence condition (22) implies

    ()

We also denote the restriction of fπ mapping onto by .

The couple is called the exit chart. If is such that the subset is a finite atlas for and , then M, with the atlas 𝒜, is a SG-manifold (see [4]). An atlas 𝒜 of such kind is called admissible. From now on, we restrict the choice of atlases on M to the class of admissible ones. We introduce the following spaces, endowed with their natural topologies,
()

Definition 7. The set consists of all the symbols which fulfill (3) for only. Moreover, the symbol a belongs to the subset if it admits expansions in asymptotic sums of homogeneous symbols with respect to x and ξ as in Definitions 2 and 3, where the remainders are now given by SG-symbols of the required order on .

Note that, since is conical, the definition of homogeneous and classical symbol on makes sense. Moreover, the elements of the asymptotic expansions of the classical symbols can be extended by homogeneity to smooth functions on n∖{0}, which will be denoted by the same symbols. It is a fact that, given an admissible atlas on M, there exists a partition of unity {θi} and a set of smooth functions {χi} which are compatible with the SG-structure of M, that is,

  • (i)

    supp θi ⊂ Ωi, supp χi ⊂ Ωi, χiθi = θi, i = 1, …, N;

  • (ii)

    and for all .

Moreover, θN and χN can be chosen so that and are homogeneous of degree 0 on Uδ. We denote by u* the composition of u : ψii) ⊂ n with the coordinate patches ψi, and by v* the composition of v : ΩiM with , i = 1, …, N. It is now possible to give the definition of SG-pseudodifferential operator on M.

Definition 8. Let M be a manifold with a cylindrical end. A linear operator is an SG-pseudodifferential operator of order (m, μ) on M, and we write PLm,μ(M), if, for any admissible atlas on M with exit chart (ΩN, ψN):

  • (1)

    for all i = 1, …, N − 1 and any , there exist symbols pi(x, ξ) ∈ Sm(ψii)) such that

    ()

  • (2)

    for any θN, χN of the type described above, there exists a symbol such that

    ()

  • (3)

    KP, the Schwartz kernel of P, is such that

    ()
    where Δ is the diagonal of M × M and with any conical neighbourhood V of the diagonal of .

The most important local symbol of P is pN. Our definition of SG-classical operator on M differs slightly from the one in [7].

Definition 9. Let PLm,μ(M). P is an SG-classical operator on M, and we write , if and the operator P, restricted to the manifold , is classical in the usual sense.

The usual homogeneous principal symbol pψ of an SG-classical operator is of course well defined as a smooth function on T*M. In order to give an invariant definition of the principal symbols homogeneous in x of an operator , the subbundle was introduced. The notions of ellipticity can be extended to operators on M as well.

Definition 10. Let and let us fix an exit map fπ. We can define local objects pmj,μi, p·,μi as

()

Definition 11. An operator is elliptic, and we write , if the principal part of satisfies the SG-ellipticity conditions on and the operator P, restricted to the manifold , is elliptic in the usual sense.

Proposition 12. The properties PLm,μ(M) and , as well as the notion of SG-ellipticity, do not depend on the (admissible) atlas on M. Moreover, the local functions pe and pψe give rise to invariantly defined elements of and , respectively.

Then, with any , it is associated an invariantly defined principal symbol in three components σ(P) = (pψ, pe, pψe). Finally, through local symbols given by , j = 1, …, N − 1, and , s, σ, we get a SG-elliptic operator and introduce the (invariantly defined) weighted Sobolev spaces Hs,σ(M) as
()

The properties of the spaces Hs,σ(n) extend to Hs,σ(M) without any change, as well as the continuity of the linear mappings P : Hs,σ(M) → Hsm,σμ(M) induced by PLm,μ(M), mentioned in Section 1.

3. Spectral Asymptotics for SG-Classical Elliptic Self-Adjoint Operators on Manifolds with Ends

In this section we illustrate the procedure to prove Theorem 1, similar to [13, 25, 27]. The result will follow from the Trace formula (39), (41), the asymptotic behaviour (42), and the Tauberian Theorem 19. The remaining technical points, in particular the proof of the asymptotic behaviour of the integrals appearing in (41), are described in Section 4 and in the Appendix.

Let the operator be considered as an unbounded operator P : 𝒮(M) ⊂ H0,0(M) = L2(M) → L2(M). The following proposition can be proved by reducing to the local situation and using continuity and ellipticity of P, its parametrix, and the density of 𝒮(M) in the Hs,σ(M) spaces.

Proposition 13. Every , considered as an unbounded operator P : 𝒮(M) ⊂ L2(M) → L2(M), admits a unique closed extension, still denoted by P, whose domain is 𝒟(P) = Hm,μ(M).

From now on, when we write we always mean its unique closed extension, defined in Proposition 13. As standard, we denote by ϱ(P) the resolvent set of P, that is, the set of all λ such that λIP maps Hm,μ(M) bijectively onto L2(M). The spectrum of P is then spec(P) = ϱ(P). The next theorem was proved in [7].

Theorem 14 (Spectral theorem). Let be regarded as a closed unbounded operator on L2(M) with dense domain Hm,μ(M). Assume also that m,   μ > 0 and P* = P. Then

  • (i)

    (λIP) −1 is a compact operator on L2(M) for every λϱ(P). More precisely, (λIP) −1 is an extension by continuity from 𝒮(M) or a restriction from 𝒮(M) of an operator in .

  • (ii)

    spec (P) consists of a sequence of real isolated eigenvalues {λj} with finite multiplicity, clustering at infinity; the orthonormal system of eigenfunctions {ej} j≥1 is complete in L2(M) = H0,0(M). Moreover, ej𝒮(M) for all j.

Given a positive self-adjoint operator , m, μ > 0,  μm, we can assume, without loss of generality (considering, if necessary, P + c in place of P, with c a suitably large constant), 1 ≤ λ1λ2…. Define the counting function NP(λ), λ, as
()

Clearly, NP is nondecreasing, continuous from the right and supported in [0, +). If we set Q = P1/l, l = max {m, μ} (see [19] for the definition of the powers of P), Q turns out to be a SG-classical elliptic self-adjoint operator with . We denote by {ηj} the sequence of eigenvalues of Q, which satisfy . We can then, as above, consider NQ(η). It is a fact that NQ(η) = O(ηn/l), see [7].

From now on we focus on the case μ > m > 0. The case m > μ > 0 can be treated in a completely similar way, exchanging the role of x and ξ. So we can start from a closed positive self-adjoint operator with domain 𝒟(Q) = Hm,1(M), m ∈ (0,1). For uHm,1(M), t, we set
()
and the series converges in the L2(M) norm (cf., e.g., [25]). Clearly, for all t, U(t) is a unitary operator such that
()
Moreover, if uHkm,k(M) for some k, U(t)uCk(, H0,0(M))∩⋯∩C0(, Hkm,k(M)) and, for uHm,1(M), we have DtU(t)uQU(t)u = 0, U(0)u = u, which implies that v(t, x) = U(t)u(x) is a solution of the Cauchy problem
()
Let us fix ψ𝒮(). We can then define the operator either by using the formula
()
or by means of the vector-valued integral (∫ψ(t)U(t)dt)u = ∫ψ(t)U(t)udt, uH0,0(M). Indeed, there exists N0 such that , so the definition makes sense and gives an operator in (L2(M)) with norm bounded by . The following lemma, whose proof can be found in the Appendix, is an analog on M of Proposition  1.10.11 in [13].

Lemma 15. is an operator with kernel .

Clearly, we then have
()

By the analysis in [2224, 28] (see also [29]), the above Cauchy problem (33) can solve modulo 𝒮(M) by means of a smooth family of operators V(t), defined for t ∈ (−T, T), T > 0 suitably small, in the sense that (DtQ)∘V is a family of smoothing operators and V(0) is the identity on 𝒮(M). More explicitly, the following theorem holds (see the Appendix for some details concerning the extension to the manifold M of the results on n proved in [2224, 28]).

Theorem 16. Define , where θk and χk are as in Definition 8, with χkθk = θk, k = 1, …, N, while the Ak(t) are SG FIOs which, in the local coordinate open set Uk = ψkk) and with v𝒮(n), are given by

()

Each Ak(t) solves a local Cauchy problem (DtQk)∘AkC((−T, T), L,−(n)), Ak(0) = I, with Qk = Op(qk) and local (complete) symbol of Q associated with {θk}, {χk}, with phase and amplitude functions such that

()
Then, V(t) satisfies
()
and UVC((−T, T), L,−(M)).

Remark 17. Trivially, for k = 1, …, N − 1, qk and ak can be considered SG-classical, since, in those cases, they actually have order − with respect to x, by the fact that qk(x, ξ) vanishes for x outside a compact set.

Remark 18. Notation like bC((−T, T), Sr,ρ(n)), BC((−T, T), Lr,ρ(M)), and similar, in Theorem 16 and in the sequel, also mean that the seminorms of the involved elements in the corresponding spaces (induced, in the mentioned cases, by (3)), are uniformly bounded with respect to t ∈ (−T, T).

If we write ψλ(t) = ψ(t)eitλ in place of ψ(t), for a chosen , the trace formula (35) becomes
()
Let us denote the kernel of UV by r(t; x, y) ∈ C((−T, T), 𝒮(M × M)). Then, the distribution kernel of is
()
where the local coordinates in the right-hand side depend on k and, to simplify the notation, we have omitted the corresponding coordinate maps. By the choices of ψ, θk and χk we obtain
()
Let , T > 0, be such that ψ(0) = 1 and , (e.g., set with a suitable ). By the analysis of the asymptotic behaviour of the integrals appearing in (41), described in Section 4, we finally obtain
()
with n* = min {n, (n/m) − 1}. The following Tauberian theorem is a slight modification of Theorem  4.2.5 of [13] (see the Appendix).

Theorem 19. Assume that

  • (i)

    is an even function satisfying ψ(0) = 1, , ;

  • (ii)

    NQ(λ) is a nondecreasing function, supported in [0, +), continuous from the right, with polynomial growth at infinity and isolated discontinuity points of first kind {ηj}, j, such that ηj → +;

  • (iii)

    there exists d0 ≥ 0 such that

    ()

with m ∈ (0,1), n* = min {n, (n/m) − 1}.

Then

()

Remark 20. The previous statement can be modified as follows: with ψ, NQ, and m as in Theorem 19, when

()
with m ∈ (0,1), then NQ(λ) = (d0/2π)λn/m + O(λ(n/m)−1) + O(λn), for λ → +.

4. Proof of Theorem 1

In view of Theorem 19 and Remark 20, to complete the proof of Theorem 1 we need to show that (42) holds. To this aim, as explained previously, this section will be devoted to studying the asymptotic behaviour for |λ | →+ of
()
where , ψ(0) = 1, aC((−T, T),  S0,0(n)), a(0; x, ξ) = 1, and
()
such that
  • (i)

    tφ(t; x, ξ) = q(x, dxφ(t; x, ξ)), φ(0; x, ξ) = xξ;

  • (ii)

    C−1ξ〉≤〈dxφ(t; x, ξ)〉≤Cξ〉, for a suitable constant C > 1;

  • (iii)

    , 0 < m < 1, SG-elliptic.

Since q−1(x, ξ) ∈ O(〈x〉 −1ξ〉 m) for |x | +|ξ | ≥ R > 0, it is not restrictive to assume that this estimate holds on the whole phase space, so that, for a certain constant A > 1,
()

Remark 21. The assumption on q−1 above amounts, at most, to modifying q by adding and subtracting a compactly supported symbol, that is, an element of S,−(n). The corresponding solutions φ and a of the eikonal and transport equations, respectively, would then change, at most, by an element of C((−T, T), S,−(n)), see [23, 24, 28]. It is immediate, by integration by parts with respect to t, that an integral as (46) is O(|λ|) for aC((−T, T), S,−(n)). Then, the modified q obviously keeps the same sign everywhere.

For two functions f, g, defined on a common subset X of and depending on parameters , we will write fg or f(x, y)≺g(x, y) to mean that there exists a suitable constant c > 0 such that |f(x, y)| ≤ c | g(x, y)| for all (x, y) ∈ X × Y. The notation f ~ g or f(x, y) ~ g(x, y) means that both fg and gf hold.

Remark 22. The ellipticity of q yields, for λ < 0,

()
which, by integration by parts, implies I(λ) = O(|λ|) when λ → −.

From now on any asymptotic estimate is to be meant for λ → +.

We will make use of a partition of unity on the phase space. The supports of its elements will depend on suitably large positive constants k1, k2 > 1. We also assume, as it is possible, λλ0, again with an appropriate λ0 ≫ 1. As we will see below, the values of k1, k2, and λ0 depend only on q and its associated seminorms.

Proposition 23. Let H1 be any function in such that supp H1⊆[(2k1) −1, 2k1], 0 ≤ H1 ≤ 1 and H1 ≡ 1 on , where k1 > 1 is a suitably chosen, large positive constant. Then

()

Proof. Write

()
and observe that, by A−1x〉〈ξmq(x, ξ) ≤ Ax〉〈ξm, x, ξn, we find
()
()

Thus, if k1 > 2AC we have |tΦ(t; x, ξ; λ)| ~ λ + 〈x〉〈ξ〉 m on the support of 1 − H1(〈x〉〈ξ〉 m/λ), and the assertion follows integrating by parts with respect to t in the first integral of (51).

Remark 24. We actually choose k1 > 4AC > 2AC, since this will be needed in the proof of Proposition 28; see also Section C in the Appendix.

Let us now pick such that 0 ≤ H2(υ) ≤ 1, H2(υ) = 1 for |υ | ≤ k2 and H2(υ) = 0 for |υ | ≥ 2k2, where k2 > 1 is a constant which we will choose big enough (see below). We can then write

()

In what follows, we will systematically use the notation Sr,ρ = Sr,ρ(y, η), yk, ηl, to generally denote functions depending smoothly on y and η and satisfying SG-type estimates of order r, ρ in y, η. In a similar fashion, will stand for some function of the same kind which, additionally, depends smoothly on t ∈ (−T, T), and, for all s+, satisfies SG-type estimates of order r, ρ in y, η, uniformly with respect to t ∈ (−T, T).

To estimate I1(λ), we will apply the stationary phase theorem. We begin by rewriting the integral I1(λ), using the fact that φ is solution of the eikonal equation associated with q and that q is a classical SG-symbol. Note that then , since

()

In view of the Taylor expansion of φ at t = 0, recalling the property q(x, ξ) = ω(x)qe(x, ξ) + Sm,0(x, ξ), ω a fixed 0-excision function, we have, for some 0 < δ1 < 1,

()
where the subscript e denotes the x-homogeneous (exit) principal parts of the involved symbols, which are all SG-classical and real-valued, see [28].

Observe that |x | ~ λ on the support of the integrand in I1(λ), so that we can, in fact, assume ω(x) ≡ 1 there. Indeed, recalling that, by definition, ωC(n), ω(υ) ≡ 0 for |υ | ≤ B, ω(υ) ≡ 1 for |υ | ≥ 2B, with a fixed constant B > 0, it is enough to observe that
()
which of course implies 〈x〉~|x|, provided that λ0λ is large enough. Moreover, by the ellipticity of q, writing x = |x | ς, ς𝕊n−1, with the constant A > 1 of (48),
()
taking the limit for |x | →+. Then, setting x = λζς, ζ ∈ [0, +), ς𝕊n−1, λλ0 ≫ 1, in I1(λ), by homogeneity and the previous remarks, we can write
()
and find, in view of the compactness of the support of the integrand (see the proof of Proposition 25 below) and the hypotheses
()
with X = (t, ζ), Y = (ς, ξ). We can now prove the following.

Proposition 25. Choosing the constants k1, λ0 > 1 large enough and T > 0 suitably small, one has, for any k2 > 1 and for a certain sequence cj, j = 0,1, …,

()
that is, I1(λ) = c0λn−1 + O(λn−2), with
()

Proof. It is easy to see that, on the support of U1, the phase function F1(X, Y) admits a unique, nondegenerate, stationary point X0 = X0(Y) = (0, qe(ς, ξ) −1), that is, for all Y such that (X, Y) ∈ supp U1, provided that T > 0 is chosen suitably small (see, e.g., [25, page 136]), and the Hessian equals −qe(ς, ξ) 2 < 0. Moreover, the amplitude function

()
is compactly supported with respect to the variables X and Y and satisfies, for all ,
()
for all X, Y, λλ0. In fact,
  • (1)

    , ς𝕊n−1, supp [H2(|ξ|)]⊆{ξ  :  |ξ| ≤ 2k2}, and

    ()
    where λ0 > 2k1〈2k2〉 m;

  • (2)

    all the factors appearing in the expression of U1 are uniformly bounded, together with all their X-derivatives, for XSX = supp ψ × [ζ0, ζ1], YSY = 𝕊n−1 × {ξ:|ξ | ≤ 2k2}, and λλ0.

Of course, (2) trivially holds for the cutoff functions ψ(t) and H2(|ξ|), and for the factor ζn−1. Since , on SX × SY we have, for all and λλ0 > 1,

()

Moreover, since is actually in on SX × SY, the same holds for exp (iG1), by an application of the Faà di Bruno formula for the derivatives of compositions of functions, so also this factor fulfills the desired estimates. Finally, another straightforward computation shows that, for all γ2+ and λλ0 > 1,

()
on SX × SY.  The proposition is then a consequence of the stationary phase theorem (see [30, Proposition  1.2.4], [31, Theorem  7.7.6]), applied to the integral with respect to X = (t, ζ). In particular, the leading term is given by λn/(2π)n−1 times the integral with respect to Y of , that is
()
recalling that ψ(0) = 1, a(0; x, ξ) = 1 for all x, ξn.

Indeed, having chosen k1 > 2A, λ0 > 2k1〈2k2〉 m, (58) implies

()
uniformly for ς𝕊n−1, ξ ∈ supp [H2(|ξ|)], λλ0. This concludes the proof.

Let us now consider I2(λ). We follow a procedure close to that used in the proof of Theorem  7.7.6 of [31]. However, since here we lack the compactness of the support of the amplitude with respect to x, we need explicit estimates to show that all the involved integrals are convergent, so we give the argument in full detail in what follows.

We initially proceed as in the analysis of I1(λ) mentioned previously. In view of the presence of the factor 1 − H2(|ξ|) in the integrand, we can now assume |ξ | ≥ k2 > max {B, 1}, B > 0 the radius of the smallest ball in n including supp (1 − ω), so that q(x, ξ) = ω(ξ)qψ(x, ξ) + Sm−1,1(x, ξ) = qψ(x, ξ) + Sm−1,1(x, ξ). Then, with some 0 < δ2 < 1,
()
Setting ξ = (λζ) 1/mς, ζ ∈ [0, +), ς𝕊n−1, λλ0, we can rewrite I2(λ) as
()
X = (t, ζ), Y = (ς, x), where we have set
()
On the support of U2, we have
()
so that
()

For any fixed Y𝕊n−1 × n, we then have X belonging to a compact set, uniformly with respect to λλ0, say supp ψ × [c−1x〉 −1, cx〉 −1], for a suitable c > 1.

Remark 26. Incidentally, we observe that a rough estimate of λn/mI2(λ) is

()
An even less precise result would be the bound λn/m, using the convergence of the integral with respect to x in the whole n, given by −(n/m) + n < 0.

The next lemma is immediate, and we omit the proof.

Lemma 27. for any ζ ∈ [0, +), xn, ς𝕊n−1, λλ0, m ∈ (0,1), and, for all ,

()

The main result of this section is as follows.

Proposition 28. If k1, k2, λ0 > 1 are chosen large enough, one has

()
Explicitly,
()

We will prove Proposition 28 through various intermediate steps. First of all, arguing as in the proof of (58), exchanging the role of x and ξ, we note that, for all xn, ς𝕊n−1,
()
(x, ς) ∈ n × 𝕊n−1. We now study
()
X = (t, ζ) ∈ SX = supp ψ × [c−1x〉 −1, cx〉 −1], Y = (ς, x) ∈ SY = 𝕊n−1 × n, λλ0, where we have used Lemma 27. By the symbolic calculus, remembering that on supp U2, we can rewrite the expressions mentioned previously as
()
It is clear that ζ ~ 〈x−1 implies ζS−1,1(x, (λζ)1/m) = S−1,0(x, (λζ)1/m)  and , so that we finally have
()
We now prove that, modulo an O(|λ|) term, we can consider an amplitude such that, on its support, the ration ζ/ζ0 is very close to 1. To this aim, take such that 0 ≤ H3(υ) ≤ 1, H3(υ) = 1 for |υ | ≤ (3/2)ε and H3(υ) = 0 for |υ | ≥ 2ε, with an arbitrarily fixed, small enough ε ∈ (0, 1/2), and set
()

Proposition 29. With the choices of T, k1, λ0, for any ε ∈ (0, 1/2), one can find k2 > 1 large enough such that J1(λ) = O(λ).

Proof. Since 0 < m < 1, in view of (3), (74), and (79), we can choose k2 > 1 so large that, for an arbitrarily fixed ε ∈ (0, 1/2), for any λλ0, ζ ∈ (0, +) satisfying |ξ | = (λζ) 1/mk2,

()
()
uniformly with respect to (X, Y) ∈ SX × SY⊇supp U2(·; λ). Then, F2 is nonstationary on supp V1, since there we have |(ζ/ζ0) − 1| ≥ (3/2)ε, while
()
which implies tF2(X, Y; λ)≻1. Observing that, on supp V1, , as well as , the assertion follows by repeated integrations by parts with respect to t, using the operator
()
and recalling Remark 26.

Proposition 30. With the choices of ε, T > 0, k1, k2, λ0 > 1, one can assume, modulo an O(λn−1) term, that the integral with respect to x in J2(λ) is extended to the set {xn : 〈x〉≤ϰλ}, with

()

Proof. Indeed if , we can split J2(λ) into the sum

()
since the inequality is true when k2 is sufficiently large.

Observing that, on suppU2,

()
switching back to the original variables, the first integral in (88) can be treated as I1(λ), and gives, in view of Proposition 25, an O(λn−1) term, as stated.

Now we can show that F2(X, Y; λ) admits a unique, nondegenerate stationary point belonging to supp V2 for 〈x〉 ≤ ϰλ. Under the same hypotheses, lies in a circular neighbourhood of X0 = (0, ζ0) = (0, qψ(x,ς)−1) of arbitrarily small radius.

Proposition 31. With ε ∈ (0, 1/2), T > 0, k1,   k2,   λ0 > 1 fixed previously, vanishes on supp V2 only for , that is, for all Y such that (X, Y; λ) ∈ supp V2. Moreover,

()
holds on supp V2.

Proof. We have to solve

()
(X, Y; λ) ∈ supp V2. By (79) and (84a) and (84b), with the choices of ε, T > 0, k1, k2, λ0, the coefficient of t in the second equation does not vanish at any point of supp V2. Then t = 0, and ζ must satisfy
()
Since, by the choice of k2, |ζG(ζ; Y; λ)| ≤ k0 < 1, uniformly with respect to Y𝕊n−1 × {xn : 〈x〉≤ϰλ}, λλ0, G has a unique fixed point , smoothly depending on the parameters; see the Appendix for more details. Since
()
we can assume that and the choices of the other parameters imply, on supp V2,
()
So we have proved that, on supp V2,
()

By (3), (92), and , (X, Y) ∈ SX × SY⊇supp V2(·; λ), we also find

()
uniformly with respect to λλ0. The proof is complete.

Remark 32. The choice of k2 depends only on the properties of q and on the values of k1 and ε; that is, we first fix k1 > 4AC > 2AC > 2 and ε ∈ (0, 1/2), then T > 0 small enough as explained at the beginning of the proof of Proposition 25, then k2 > 1 as explained in the proofs of Propositions 29 and 31, then, finally, .

The next lemma says that the presence in the amplitude of factors which vanish at implies the gain of negative powers of λ.

Lemma 33. Assume , |α | > 0,

()
W is smooth, Wk(X, Y; λ)≺〈xk, k+, and has a SG-behaviour as the factors appearing in the expression of V2. Then
()
where has the same SG-behaviour, support and x-order of V2, including the powers of ζ.

Proof. By arguments similar to those used in the proof of Proposition 29, on supp W

()
Assume that the first condition in (97) holds. Under the hypotheses, if α1 > 0, we can first insert in the left-hand side of (98), where Lζ = Dζ/λζF2(X, Y; λ), and integrate by parts α1 times. Similarly, if α2 > 0, we subsequently use , Lt = Dt/λtF2(X, Y; λ), and integrate by parts α2 times. The assertion then follows, remembering that ζ-derivatives of W produce either an additional ζ−1 factor or a lowering of the exponent of , and that on supp W. The proof in the case that the second condition in (97) holds is the same, using first Lζ and then Lt.

Proof of Proposition 28. Define,

()
and, for s ∈ [0,1],
()
Remembering that , , 𝒬 is the Taylor polynomial of degree two of F2 at , so that 𝒢 vanishes of order 3 at . Obviously, 0(X, Y; λ) = 𝒬(X, Y; λ) and 1(X, Y; λ) = F2(X, Y; λ). Write
()
, and consider the Taylor expansion of 𝒥τ(s) of order 2𝒩 − 1, 𝒩 > 1, so that
()

Since

()
Remark 26 and Lemma 33 imply that , , s ∈ [0,1]. Indeed, it is easy to see, by direct computation, that 𝒢 can be bounded by linear combinations of expressions of the form
()
with Wk, k+, having the required properties. Then, the bound of 𝒢2𝒩 will always contain a term of the type , which corresponds to the (minimum) value |α| = 3𝒩 in (97).

Each term , k = 0, …, 2𝒩 − 1, has the quadratic phase function 𝒬, which of course also satisfies

()
Then, denoting by Γ the Taylor expansion of 𝒢 at of order 3𝒩, we observe that 𝒢k − Γk can be bounded by polynomial expressions in of the kind appearing in the right-hand side of (97), with |α | = 𝒩 + k (cf. the proof of Theorem 7.7.5 in [31]). Setting
()
Lemma 33 implies
()

We now apply the stationary phase method to and prove that

()
which is a consequence of
()
with M evaluated with τ−1 in place of λ. Recalling (95), it follows that the inverse matrix M−1 satisfies, on supp V2,
()
in view of the ellipticity of the involved symbols. Then, the operators Lj,k,Y,τ, j, k+, do not increase the x-order of the resulting function with respect to that of their arguments, (iλΓ) kV2, which is the same of V2, uniformly with respect to τ. The proof of (110) then follows by Theorem 7.6.1, the proof of Lemma 7.7.3 and formula (7.6.7) in [31]; see also [26, 32]. Indeed, by the mentioned results,
()
since 〈x〉≺λ on supp V2. It is then enough to sum all the expansions of , k = 0, …, 2𝒩 − 1, and sort the terms by decreasing exponents of λ (as in the proof of Theorem 7.7.5 in [31]) to obtain (109) with the usual expression
()
so that, in particular,
()
for any j+, . We can then integrate 𝒥τ(1) and its asymptotic expansions with respect to Y𝕊n−1 × {xn : 〈x〉 ≤ ϰλ} and find
()
Recall that ψ(0) = 1 and a(0, x, ξ) = 1, for all x, ξn. Moreover, for , the factors H1, H2, and H3 are identically equal to 1 (see the Appendix). Then, the coefficient of the leading term in (115) is given by
()
with M evaluated in . We say that
()
To confirm this, first note that , λ → +, for any (Y; λ) belonging to the support of the integrand, see the Appendix. Moreover, the integrand is uniformly bounded by the summable function 〈xn/m, and its support is included in the set S. Then, recalling (95) and setting ,
()

The second integral is always O(λn−(n/m)), since qψ(x, ς) ~ 〈x〉 implies

()

The first integral can be estimated as follows. Since

()
by the properties of (see the appendix) we find
()
since . By (95), we similarly have , so that
()
If n > 1/(1 − m)⇔n − 1 − ((n − 1)/m) < −1, n, m ∈ (0,1), the integral in R1 is convergent for λ → + and R1 = O(λ−1/m). In this case, R1 contributes an O(λ(n/m)−1−(1/m)) term to the expansion of I2(λ), which is of lower order than the O(λ(n/m)−2) term, which is one of the remainders appearing in (77). On the other hand, if n < 1/(1 − m), the integral in R1 is divergent, and R1 itself is O(λn−(n/m)), since, trivially
()
Finally, if n = 1/(1 − m), R1 is O(λ−1/mln λ), by
()
and again contributes a term of lower order than the remainder O(λ(n/m)−2). Similar conclusions can be obtained for the subsequent terms of the expansion of J2(λ).

The proof is complete, combining the contributions of the remainders like R with the other terms in the expansion of J2(λ), and remembering that

()

Remark 34. The same conclusions concerning the behaviour of R1 in the final step of the proof of Proposition 28 could have been obtained studying the Taylor expansion of the extension of , τ = λ−1, to the interval , similarly to [32].

Proof of Theorem 1. The statement for μ > m follows by the arguments in Section 3 and Propositions 23, 25 and 28, summing up the contribution of the local symbol on the exit chart to the contributions of the remaining local symbols, which gives the desired multiple of the integral of on the cosphere bundle as coefficient of the leading term λn/m. The remainder has then order equal to the maximum between (n/m) − 1 and n, as claimed. The proof for μ < m is the same, by exchanging step by step the role of x and ξ.

Acknowledgments

The authors wish to thank U. Battisti, L. Rodino, and E. Schrohe for useful discussions and hints. Thanks are also due to N. Batavia. The first author was partially supported by the PRIN Project “Operatori Pseudo-Differenziali ed Analisi Tempo-Frequenza” (Director of the national project: G. Zampieri; local supervisor at Università di Torino: L. Rodino). The first author also gratefully acknowledges the support by the Institut für Analysis, Fakultät für Mathematik und Physik, Gottfried Wilhelm Leibniz Universität Hannover, during his stay as Visiting Scientist in the Academic Year 2011/2012, where this paper was partly developed and completed.

    Appendix

    For the sake of completeness, here we illustrate some details of the proof of Theorem 1, which we skipped in the previous sections. They concern, in particular, formula (41), which expresses the relation between and the oscillatory integrals examined in Section 4. We mainly focus on the aspects which are specific for the manifolds with ends.

    We also show more precisely how the constants k1, k2, λ are involved in the solution of (92) via the fixed point theorem, completing the proof of Proposition 31.

    A. Solution of Cauchy Problems and SG Fourier Integral Operators

    Using the so-called “geometric optics method”, specialised to che pseudodifferential calculus we use (see [2224, 28, 29, 33]), the Cauchy problem (33) can be solved modulo 𝒮(M) by means of an operator family V(t), defined for t in a suitable interval (−T, T), T > 0: V(t) induces continuous maps
    ()
    ()
    ()
    First of all, we recall that the partition of unity {θk} and the family of functions {χk} of Definition 8 can be chosen so that and are SG-symbols of order (0,0) on Uk, extendable to symbols of the same class defined on n (see [5]).

    Remark A.1. (1) The complete symbol of Q depends, in general, on the choice of the admissible atlas, of {θk} and of {χk}. Anyway, if is another complete symbol of Q, for an admissible cutoff function κ supported in .

    (2) The solution of (33) in the SG-classical case and the properties of φk and ak in (37) were investigated in [28] (see also [33, Section 4]). In particular, it turns out that , Tk > 0. According to ([23, page 101]), for every SG phase functions φ of the type involved in the definition of V(t) we also have, for all xn,

    ()
    with a constant C > 0 not depending on t, x, ξ. The function Φt,ξ(x) : = ∇ξφ(t, x, ξ) turns out to be a (SG-) diffeomorphism, smoothly depending on the parameters t and ξ (see [22]).

    Before proving Theorem 16, we state a technical lemma, whose proof is immediate and henceforth omitted.

    Lemma A.2. Let Un be an open set and define Uδ : = ⋃xUB(x, δx〉) for arbitrary δ > 0. Assume θ, χC(n) such that supp θUδ/5, supp χUδ and . Then, for any diffeomorphism Φt,ξ, smoothly depending on t ∈ (−T, T), ξn, and such that for all  t, x, ξ  |Φt,ξ(x) − x| ≤ C|t|〈x〉 with a constant C > 0 independent of t, x, ξ,

    ()
    for any multi-index α and x, ξn.

    We remark that, since a manifold with ends is, in particular, a SG-manifold, the charts (Ωk, ψk), and the functions {θk}, {χk} can be chosen such that
    • (i)

      for a fixed δ > 0, each coordinate open set Uk = ψkk), k = 1, …, N, contains an open subset Wk such that ;

    • (ii)

      the supports of θk and χk, k = 1, …, N, satisfy hypotheses as the supports of θ and χ in Lemma A.2 (see, e.g., Section 3 of [5] for the construction of functions with the required properties).

    In fact, this is relevant only for k = N.

    Proof of Theorem 16. We will write RS when RSL,−(M) and when the functions are smooth, nonnegative, supported in Ωk, satisfy and are SG-symbols of order (0,0) on Uk = ψkk). Obviously, RL,−(M) implies RVC((−T, T), L,−(M)). To simplify notation, in the following computations we will not distinguish between the functions χk, θk, and so forth, and their local representations.

    V(t) obviously satisfies (A.3). To prove (A.2), choose functions ζk, υk supported in Ωk such that θkζkχkυk. Then and, for all k = 1, …, N, QχkυkQkχk (see [1], Section 4.4; cf. also [11]), so that

    ()
    That the first term in the sum (A.6) is smoothing comes from the SG symbolic calculus in n and the observations above, since sym([Qk, χk]ζk) ~ 0. The same property holds for each k in the second term, provided , Tk > 0 small enough. In fact, by Theorems 7 and 8 of [22], (1 − ζk)Vk(t)θk is a SG FIO with the same phase function φk and amplitude wk such that
    ()
    with suitable SG-symbols bjα defined in terms of φk and ak. By Remark A.1 and Lemma A.2, wk ~ 0 for |t| small enough. The proof that V(t) satisfies (A.2) is completed once we set T = min {T1, …, TN}. The last part of the theorem can be proved as in [25], Proposition 12.3, since, setting W(t)≔U(−t)V(t), it is easy to see DtW(t) ≡ 0, so that W(0) = IW(t) ≡ IV(t) ≡ U(t), with smooth dependence on t, as claimed.

    B. Trace Formula and Asymptotics for

    Proof of Lemma 15. Consider first the finite sum

    ()
    and reduce to the local situation (cf. Schrohe [5]), via the SG-compatible partition of unity {θl} subordinate to the atlas 𝒜, by
    ()
    ()
    Then, by ek𝒮(M) and the fact that is supported and at most of polynomial growth in Ur, it turns out that we can extend (θrek) * and (θsek) * to elements of 𝒮(n). By an argument similar to the proof of Proposition 1.10.11 in [13] (or by direct estimates of the involved seminorms, as in [25]), in 𝒮(n × n) when J → +, with kernel of . This proves that is an operator with kernel .

    The proof of Theorem 19 is essentially the one in [25], while the proof of Lemma B.1 comes from [13]. We include both of them here for convenience of the reader.

    Proof of Theorem 19. Setting and integrating (42) in (−, λ), we obtain

    ()
    Now, observe that
    ()
    where H(τ) is the Heaviside function. Bringing the series under the integral sign, we can write
    ()
    since . In view of the monotonicity of N and next Lemma B.1 (cf. Lemma 4.2.8 of [13]), for λ ≥ 1
    ()
    We can then conclude that R(λ) = O(λn/m−1), λ ≥ 1, since , and this, together with (B.4) and (B.6), completes the proof.

    Lemma B.1. Under the hypotheses of Theorem 19, there exists a constant C > 0 such that for any K ≥ 0 and any λ

    ()

    Proof. Let and [−K0, K0] such that for all t ∈ [−K0, K0]. Then, trivially,

    ()

    Let us now prove that

    ()
    Indeed, this is clear for and , suitably large, in view of hypothesis (iii). For , choose a constant C1 so large that . This shows that, for all λ,
    ()

    For arbitrary K > 0 there exists l such that (l − 1)K0K < lK0. We write

    ()

    By (B.11), the last sum can be estimated by

    ()
    as claimed.

    C. The Solution of the Equation ζ = G(ζ; Y; λ)

    We know that A−1x〉 −1ζ0(ς, x) = qψ(x, ς) −1Ax〉 −1, , and that k1 > 4AC > 2AC > 2. Moreover, k2 > 1 is chosen so large that, in particular, on supp U2⊃supp V2, the absolute value of the ζ-derivative of G is less than k0 ≤ 1, uniformly with respect to , λλ0, (X, Y; λ) ∈ supp V2. We want to show that once k1 is fixed, the choice of such a suitably large k2 > 1 allows to make G a contraction on the compact set Ix = [A−1(1 − (ε/2))〈x−1, A(1 + (ε/2))〈x−1] ⊂ [c−1x−1, cx−1], uniformly with respect to (ς, x), λλ0, provided 〈x〉≤ϰλ, ϰ = (1 − (ε/2))[A(2k2) m] −1. This gives the existence and unicity of such that is the unique stationary point of F2(X; Y; λ), with respect to X, which belongs to the support of V2(X; Y; λ) for 〈x〉≤ϰλ.

    First of all, the presence of the factors and H2((λζ) 1/m) in the expression of U2 implies and
    ()
    Since k1 > 4AC > 2AC, clearly Ix ⊂ [c−1x〉 −1, cx〉 −1]. With an arbitrarily chosen ε ∈ (0, 1/2), take k2 > max {B, 1} such that implies |S−1,0(x, (λζ) 1/m)| ≤ ε/2 and |ζ0ζ−1S−1,0(x, (λζ) 1/m)| ≤ k0 < 1, which is possible, in view of (3) and of the fact that ζ0ζ−1 is bounded on supp V2. Fix λλ0 > 2k1〈2k2〉 m and 〈x〉≤ϰλ. Then, on supp  V2,
    ()
    Since |ζG(ζ; Y; λ)| = |ζ0ζ−1S−1,0(x, (λζ)1/m)| ≤ k0 < 1, for all ζIx, 〈x〉 ≤ ϰλ, we have proved that for any choice of , λλ0 as above, G(·; Y; λ) has a unique fixed point in , solution of ζ = G(ζ; Y; λ).
    By well-known corollaries of the fixed point theorem for strict contractions on compact subsets of metric spaces, we of course have that depends smoothly on Y and λ. Moreover, since for all , λλ0, obviously and
    ()
    pointwise for any (ς, x). Moreover, by the choices of k1, k2, and ε,
    ()
    These imply, for any ς𝕊n−1, xn, λλ0 such that 〈x〉≤ϰλ,
    ()
    Of course, by the choice of H3, for , λλ0,
    ()

      The full text of this article hosted at iucr.org is unavailable due to technical difficulties.