41 AD-A271 435 PL-TR-92-2325 CONVERGENCE OF THE HERMITE WAVELET EXPANSION G. v. H. Sandri Boston University College of Engineering and Center for Space Physics Boston, MA 02215 November 1992 Final Report 1 November 1988 - 31 October 1992 PHILLIPS $ BORATORY Approved for public release; distribution unlimited DTIC ELECTE OCT 2 2 1993 PHILLIPS LABORATORY Directorate of Geophysics 93 10 21 AIR FORCE SYSTEMS COMMAND HANSCOM AIR FORCE BASE, MA 01731-5000 93-25482 D UNIVERSITY OF MICHIGAN 3 9015 10495 5862 38115 "This technical report has been reviewed and is approved for publication" Arad ROBERT R. BELAND CONTRACT MANAGER Beland Donald & Bedo DONALD E. BEDO BRANCH CHIEF Roger Aiken sacul ROGER VAN TASSEL DIVISION DIRECTOR ناست This report has been reviewed by the ESD Public Affairs Office (PA) and is releasable to the National Technical Information Service (NTIS). Qualified requestors may obtain additional copies from the Defense Technical Information Center. All others should apply to the National Technical Information Service. If your address has changed, or if you wish to be removed from the mailing list, or if the addressee is no longer employed by your organization, please notify PL/TSI, Hanscom AFB, MA 01731-5000. This will assist us in maintaining a current mailing list. Do not return copies of this report unless contractual obligations or notices on a specific document requires that it be returned. REPORT DOCUMENTATION PAGE Public reporting burden for this collection of information is estimated to average 1 hour per response, including the time for reviewing instructions, searching existing data sources. gathering and maintaining the data needed and completing and reviewing the collection of information Send comments regarding this burden estimate or any other aspect of this collection of information, including suggestions for reducing this burden to Washington Headquarters Services. Directorate for information Operations and Reports, 1415 jetterson Davis Highway, Suite 1204, Arlington, VA 22202-4302, and to the Office of Management and Budget. Paperwork Reduction Project (0704-0188), Washington, DC 20503 1. AGENCY USE ONLY (Leave blank) 2. REPORT DATE 3. REPORT TYPE AND DATES COVERED Final. Nov. November 1992 4. TITLE AND SUBTITLE Convergence of the Hermite Wavelet Expansion 6. AUTHOR(S) G. v. H. Sandri 7. PERFORMING ORGANIZATION NAME(S) AND ADDRESS(ES) Boston University College of Engineering and Center for Space Physics Boston, MA 02215 9. SPONSORING/MONITORING AGENCY NAME(S) AND ADDRESS(ES) Phillips Laboratory Hanscom AFB, MA 01731-5000 Contract Manager: Robert Beland/GPOA 11. SUPPLEMENTARY NOTES 12a. DISTRIBUTION/AVAILABILITY STATEMENT Approved for public release; distribution unlimited. 13. ABSTRACT (Maximum 200 words) 14. SUBJECT TERMS Unclassified NSN 7540-01-280-5500 Form Approved OMB No. 0704-0188 OF ABSTRACT Unclassified 1, 1988 to Oct. 31, 1992 5. FUNDING NUMBERS TRAIL PE 61101F PR 7670 TA 15 WU AR Contract F19628-88-K- In this report we summarize the research carried out under this contract on the chaos dynamics anlysis of the free sheared atmosphere. Our approach is to expand the fluid equations into finite energy modes rather then in the conventional Fourier analysis. We prove rigorously that our expansion method has the re- quired convergence properties to ensure a satisfactory physical interpretation of the results. For the Taylor-Dyson atmosphere, our analysis, like the fourier analysis yields no unstable modes. 8. PERFORMING ORGANIZATION REPORT NUMBER Taylor-Dyson atmosphere, Hermite wavelet expansion. 17. SECURITY CLASSIFICATION 18. SECURITY CLASSIFICATION 19. SECURITY CLASSIFICATION OF REPORT OF THIS PAGE Unclassified 10. SPONSORING/MONITORING AGENCY REPORT NUMBER PL-TR-92-2325 12b. DISTRIBUTION CODE 0017 15. NUMBER OF PAGES 38 16. FRICE CODE 20. LIMITATION OF ABSTRACT SAR Standard Form 298 (Rev 2-89) Prescribed by Ali Std 259-18 240 2 INTRODUCTION 2. MATHEMATICAL FRAMEWORK 1. ત 3. 4. 5. DEFINITIONS AND NOTATION CHARACTERIZATION OF HYPERDISTRIBUTIONS CLASSES D({M}) AND THE DIFFUSION GROUP 6. SUMMARY AND CONCLUSIONS References iii Accesion For NTIS CRASI DTIC TAS Chama ced J By CATON Distributor! Cist Avarieti |A-11 CONTENTS 500 Dedes Avid and or Special 1 2 ~ ~ 7 11 21 22 332323 31 3 כי 1 Introduction In this contract we have first investigated a phenomenological approach to a chaos dynamical analysis at the free sheered atmosphere. We have then turned to a theoretical phase in which we have developed a novel expansion of the equations for the free sheared atmosphere which hinge on properties of hermite polynomials and the gaussian function. In this final scientific report we give the conditions for the basic expansions used during our analysis to converge. More specifically, the necessary and sufficient conditions are given for the quasianalytic function classes D({M}) and the corresponding classes of distributions D'({M}) to be invariant with respect to the complex-time diffusion group ∞ zk 82k U₁ = Σ Uz k=0 x k! Əx²k' ≈ Є R¹, z Є C. In addition, the properties of hyperdistributions moments r = Σ ακδία) (4) k=0 are studied. It is shown that hyperdistributions are characterized by the behavior of their µk(T) = г(x*). We conclude that expansions based on hermite polynomials multipied by a gaussian have a proper limiting behaviour. The objective to give complete mathematical foundations for our analysis has been accomplished. 1 1 2 Mathematical Framework Many physical processes have diffusive character: the spreading of smoke in air, the behav- ior of the temperature in a material body, and the vorticity in a fluid flow are examples illustrating this feature. The engineer's notion of blurring and filtering have similar nature. The one-dimensional diffusion processes are governed by the heat equation JV(x,t) _ 0²¥(x,t) at 8x2 In order to determine the behavior of the physical quantity V under consideration, provided its initial value Y(x, 0) = x(x), x Є R¹, is given, we have to solve the Cauchy problem (1) (2) for the heat equation. It is well-known that the solution of the Cauchy problem (1) - (2) with appropriately chosen initial condition is given by Poisson's formula 4(x,t) = √√A= √1. P(3) e- (=x)" dy, 1 4πt JV(x,t) at ≈ Є R',t > 0. - g²y(x,t), მუ2 (3) The following interpretation of formula (3) is possible. We get the solution (x, t) as a result of filtering the given data y through a Gassian filter of width √t. Suppose we would like to reverse the process of filtering. This is important, for example, when we are concerned with the problem of reconstructing sharp images from degraded pictures. It is clear that the inverse filtering is described by the inverse heat equation (1) ≈ € R¹,t > 0. ≈ € R¹, t > 0. (2) (4) 2 It is possible to incorporate the heat equation (1), the inverse heat equation (4), and the Schrödinger equation OV (z, t), 0² V (z, t), = at მე2 which describes the one-dimensional motion of a free particle in quantum mechanics, into the so-called complex-time diffusion equation JY(x, z) __ Ə²Y(x, z) Əz მუ2 Consider now the following formal semi-group of operators U₁ = ∞ tk 82k Σ k=0 U₁ = e', (the diffusion semi-group). It can be easily seen [6] that the formula ¥(x,t) = U₁y(x), ≈ Є R¹‚t > 0 defines the formal solution of the Cauchy problem (1) – (2). - Using the Taylor expansion of the function etu, u € R¹ in (6), we can represent {U₁} as a semi-group of differential operators of infinite order k! Ox²k' , = Σ k=0 x Є R¹‚t Є R¹. მ2k k! Jx²k' ≈ Є R¹, z Є C. t>0 t> 0. (5) If we put a complex number z EC instead of t in (7), we obtain the complex-time diffusion group of operators (6) zЄ C. (7) (8) The group {U₂} provides a formal solution of the complex-time diffusion equation (5). More- over, it is a formal analytic continuation of the semi-group (7). We use the word "formal” in 3 considerations above, because we have not yet defined the domain of the operators U, given by (8). Suppose {M} is a sequence of positive numbers. Define a function class D({M}) on R¹ by the following formula D({M₁}) = {y € C∞(R¹) : |p(*) (x)| ≤ Ah*Mk, k ≥ 0, ≈ € R¹}, where positive constants A and h depend on y. These classes are important in making the formal considerations above precise. Perhaps, Hadamard [4], [5] was one of the first who understood the importance of classes, defined by given upper bounds for the successive derivatives of functions, in dealing with the Cauchy problem for the heat equation. Hadamard posed in [4] the problem of characterizing those classes D({M}), for which every function ↳ € D({M}) can be uniquely determined by the sequence (*)(xo), k ≥ 0 for any given a € R¹. Such classes D({M}) are called the quasianalytic classes. Hadamard's problem has been solved by Denjoy and Carleman (see Section 2 below, where we formulate the Denjoy-Carleman Theorem). - The classes D({M}) have become useful tools in complex analysis [8], [10] – [11], in the theory of distributions [2], [13], and in the theory of differential operators of infinite order [1]. The simple example of their usefulness in the Cauchy problem for the heat equation is given by the following. For an appropriately chosen class D({M}), the functions ∞0 tk 82k p(x) U₁y(x) = Σ k! 8x2k k=0 are defined for every function y Є D({M₁}) and U₁y(x) = V(x,t), t> 0 x Є R¹, t > 0, 4 where is given by (3). An important contribution to the application of the quasianalytic classes in the theory of partial differential equations is due to Gelfand and Shilov [2], [3]. They contributed sub- stantially to the theory of distributions over quasianalytic classes and to the uniqueness and well-posedness problems for the heat equation with complex diffusion coefficient a, namely JY(x,t) Ə²y(x,t) at მუ2 =a ≈ € R¹, a Є C. Gelfland and Shilov found in [2] the classes of generalized distributions which provide solu- tions to these problems. They wrote in [2]: "Applications of these spaces to the Cauchy problem in Vol. 3 will illustrate the well-known statement of Hadamard's on the relation between uniqueness theo- rems in the Cauchy problem on the one hand, and the theory of quasianalytic functions and the general theory of functions of a complex variable, on the other." One of the problems we consider in this work is to characterize those classes D({Mk}), which are invariant with respect to the complex-time diffusion group (8), which means that U₂(D({M₁})) C D({Mk}), We answer this question in Section 5. The U-invariance of D({M}) implies that we can diffuse, anti-diffuse, disperse, and anti-disperse¹, staying in the same class. It is easy to see that the operator U, in (8) is a convolution operator, defined by the formula zЄ C. U₂y = y *г₂, ¹Dispersion and anti-dispersion correspond to the Schrödinger equation for the free particle. 5 where T, is the Green's function for equation (5), namely Σ = 8 (2k) k=0 r₁ = The symbol do in (9) denotes the Dirac's delta function at 0. The formal series, invloving all the derivatives of the delta-function, namely r = Σax(*), k=0 r₁ = I' are called hyperdistributions. They are highly singular objects and Schwartz's theory of distributions (see [9], [14], [2]) does not include them. The most appropriate theory, which involves hyperdistributions, is that of the distributions over the classes D({M}) (see [2], [3], [13]). In this theory the functions y € D({M}) are considered as test functions and the distributions are defined as bounded linear functionals on the class D({M₁}), equipped with appropriate topology. In [13] the formal series (10) were considered as distributions over non-quasianalysitc classes D({Mk}) (see [13], p. 51). Hyperdistributions are of much use in image processing (see [6], [7]). They have been used for deblurring and compressing of images. This is easy to understand if we recall that a hyperdistribution (9) =(-1)* (24), (−t)k (11) k! k=0 is the Green's function for the inverse heat equation and thus we may reconstruct sharp images from damaged ones by convolving them with hyperdistributions (11). This paper is organized as follows: In Section 3 the necessary definitions and known re- sults are gathered. Section 4 is concerned with the structure of hyperdistributions. We prove (see Theorems 3 and 4) that, roughly speaking, the hyperdistributions are distributions over classes D({M}), which have moments of all orders, and their moments should satisfy special (10) t> 0 6 conditions. In Section 5 we give a characterization of the U₂-invariant classes D({M}) and the U, invariant classes of distributions D'({M}) (see Theorems 5 and 6). As the corollary of Theorem 5 we get the following result. The quasianalytic classes D({k}), 0 ≤ y < 1, are U-invariant, while the class D({**/2}) is not (see Corollaries 2 and 3). 3 Definitions and Notation Definition 1 (see [8],[11],[12]). Suppose {M} is a sequence of positive numbers. We say that an infinitely differentiable function & on the real line belongs to the class D({Mx}) if there exist positive constants A, and ho, depending on 4, such that the following estimates hold for the successive derivatives (*) of the function 4, |ø(k) (x)| ≤ A¢h*Mk, x Є R¹. Definition 2 (see [8],[11],[12]). The class D({M}) is called quasianalytic if $ € D({Mx}), $(k) (x0) = 0 for some xo € R¹ and all k ≥ 0 ⇒ ☀ = 0, while all the classes D({M}), which does not satisfy the quasianalyticity condition (12) are called non-quasianalytic. (12) It is easy to see that classes D({M}) are linear and dilation-invariant. The quasianalytic classes D({M}) cannot contain functions with compact support. Definition 3 (see [13]). In this definition we equip the class D({M}) with the locally conver topology. First we consider linear subclasses, Dm({Mx}) = {$ € D({Mx}) : |ø(*)(x)| ≤ Аøm*Μk, k≥ 0}, m ≥ 1 7 of D({Mk}). Each of the classes D({M₁}) is a Banach space with the norm defined by 10(*)(x)| Pm (4) = sup sup зER¹ k≥⁰ M⭑m* It is clear that D({i} = UDm({Mx}). We equip D({M}) with the inductivet topology with respect to the family of its subspaces Dm({Mx}), m ≥ 1 (see [12] for the definition of the inductive limit). Definition 4 (see [13]). The space D'({M}) of all bounded linear functionals on the locally compact space D({M}), equipped with the strong topology (see [12]), will be called the space of distributions over the class D({M₁}). It is not difficult to prove that every band-limited function & Є L²(R¹) belongs to the class D({M}) with M = 1, k ≥ 0. The tand-limitedness means that the support of the Fourier transform of 4 is bounded. One more example is given by the Gaussian ☀(x) = e−r² which belongs to the class D({k*/2}). In the book by Mandelbrojt [11] (see p. 89) there are examples of functions & € D({M}), which do not belong to any proper subclass D({M}) of D({M}). Our next goal is to introduce new classes Ď({M}), which contain D({M}) and all the polynomials. Definition 5 For given sequence {M} consider a class Ď{{x}} of infinitely differentiable functions on the real line such that there exists a constant ho, depending only on 4, and for every finite interval IC R¹ there exists a constant A1,, depending on! and 4, for which |ø(k) (x)| ≤ A1,øht, M½, ≈ € I, k ≥ 0. 8 Definition 6 We introduce the locally convex topology of the class Ď({M}) in the following way. Consider linear subspaces Ďm({Mx}) = {Þ € Ď({Mk}) : P1,m(4) = sup sup <∞, ICR¹}. (13) The family of semi-norms P1,m generates the Frechet space topology on D({M}). It is clear that 10(*)(x)| El k>0 mk Mk Ď({Mk}) = ||Ďm({Mk}). m We equip D({Mk}) with the inductive limit topology with respect to the family of its linear subspaces {Ďm({M})}, m ≥ 1 (see [12] for the definition of the inductive limit). are called the moments of г. Suppose I is a bounded linear functional on the space Ď({M}). The next definition introduces the moments of such functionals. Definition 7 For the functional г as above, the numbers µk(T) = T(x^), k≥0 (14) It is clear that D({Mx}) ℃ Ď({Mx}). Thus, every bounded linear functional г on Ď({M}) belongs to the space D'({Mk}). Definition 8 The space Ď'({M}) of all bounded linear functionals on the locally conver space D({M}), equipped with the strong topology (see [12]), will be called the space of dis- tributions over the class D{{M}), which have moments. 9 The quasianalyticity property of the class D({M}) depends on the behavior of the Ostrovski function k≥0 Mk (see [8]). For every sequence {M}, the new sequence {M}, defined by T(r) = sup (15) is called the convex logarithmic regularization of the sequence {M}. The sequence {ln Mx} is the largest convex sequence, minorizing the sequence {ln M}. If the initial sequence {Mk} is logarithmically convex, namely if M² ≤ Mk−1 Mk+1, k ≥ 1, 2. then M = Mk, K≥ 0. The main result in the theory of quasianalytic classes is called the Denjoy-Carleman theorem (see [8]). 3. Theorem 1 (Denjoy-Carleman) The following conditions are equivalent: 1. The class D({M}) is quasianalytic. 4. - In M = sup(k ln r — ln T(r)), r>0 ∞ ln T(r) 1+2 %°° ! M8 r>0 k=0 k=0 M Mkti Σ(Mk)−¹/* dr = ∞. ∞. = ∞. 10 The following theorem reduces the case of the general classes D({M}) to the case of classes with logarithmically convex defining sequences. Theorem 2 (Cartan-Gorny) (see [8]) For every positive sequence {M} we have D({M}) = D({M}). As we have already mentioned in the introduction, the formal infinite series, F = Σ αιδία) Ž k=0 will be called hyperdistributions. We have (formally) the following formula for the moments (14) of г: µk(T) = (−1)^k!ak, k≥0 and the following moment representation for r: r = √ (− 1)^ k! k=0 4 In section 4 formulas (16) and (17) will be given exact meaning. -HA(T)S(A) Characterization of hyperdistributions The first result in this section provides conditions for a hyperdistribution r = Σ a₁d (*) k=0 to be a distribution, belonging to the class Ď'({MÂ}). (16) (17) (18) 11 Theorem 3 Suppose a hyperdistribution (18) and a sequence {M} are given. If Σ|ax|Mxh* < ∞ for every h > 0, then г € Ď'({Mx}) and is true for г. k=0 (20) Remark 1 Theorem 1 shows that for a given sequence {M} all hyperdistributions (18), satisfying condition (19), have moments µ(г) of all orders. Moreover, ak = (−1)*µk(T)(k!)−¹, k≥0. 1. for every h> 0 and the moment representation formula r = √ (−1) ^ k=0 2. k=0 lux(I) Minh cao k! Then the following result holds. k! Hk (I)ε(*) We now formulate the main result of this section. It will be shown that for some sequences {M} the inverse to Theorem 3 holds. The restriction for sequences {M} will be as follows: there exists a positive function p(h), h≥ 0 and a positive sequence {} such that Σμπτη 200 n=0 Mn+mh"
0, n > 0, h> họ.
(19)
(21)
(22)
12
Theorem 4 Suppose a sequence {M} satisfies the conditions above. Then every distribu-
tion г € Ď¹({Mx}) is a hyperdistribution (18), for which (20), (21), and (22) hold.
Remark 2 The conditions 1)-2) above and the similar conditions in Section 4 are useful
in problems, which we consider in this paper. The conditions 1)-2) imply, on the one hand,
the differentiability condition for the classes D({Mk}), namely
Mk+1 ≤ c* Mk
with some c > 0. This condition is necessary and sufficient for the differentiation invariance
of the class D({M}) (see [13], p. 57). On the other hand, conditions 1)-2) above imply
h* Mk(k!)−¹ → 0
as k → ∞ for each h>0. Condition (23) guarantees the convergence of Taylor series
= = 6)(0) = ,
φ(2) = Σ ¿(³) (0)µ³¸ þ€ Ď{{Mk})
j!
j=0
everywhere on the real line.
remainder of the series in (24). Similarly, all the Taylor series
This can be shown by estimating the Lagrange form of the
85 (k) (x) = £ ¤(³+k) (0) µ³, k ≥0, ¢ € Ď({Mk})
j!
j=0
converge uniformly on all subintervals of R¹.
(23)
г(Ø) = (-1)*a*(*)(0).
k=0
(24)
Proof of Theorem 3. If a hyperdistribution (18) is given and if a function belongs to
the class Ď({M}), then (19) implies the absolute convergence of the series
(25)
13
Moreover, if I is any interval, for which 0 € I, we have
|T(0)| ≤ P1,m(4) Σ|ax|m* Mk, m≥1,
k=0
where the semi-norms PI,m are defined in (13).
It follows from (26) that the functional I is bounded on the space Ďm({M}), m ≥ 1.
Hence, it is bounded on the inductive limit Ď({M}) of the spaces Ďm({Mk}),m ≥ 1 (see
[12] for the properties of the inductive limits).
Formula (20) follows easily from the definition of the moments.
Theorem 3 is proved.
Proof of Theorem 4. We will need the following lemma.
Lemma 1 Suppose conditions 1)-2) hold for a sequence {M}. Then the Taylor series (24)
of a function & € Ď({M}) converges to & in the topology of the space Ď({Mx}).
Proof. Consider a sequence of remainders of the Taylor series of p, namely
$(m)(0)
m!
Φ;(x) = Σ
m=j
x", j≥0.
By Remark 2, the sequence ; tends to 0 as j→ ∞ uniformly on every interval. Moreover,
we may differentiate k-times under the summation sign (see (25) in Remark 2).
Differentiating k times, we get
(514) (2) = {
m
¿(m+k) (0) x²
Σm=0+)(0)
Σm-j-k
(26)
m!
otherwise
if kj
(27)
It follows from the properties of inductive limits (see [12]) that Lemma 1 will be proved
if we show that there exists p > 1 such that þ; € Ďp({Mx}) for j ≥ jo and
Pl,p(øj) → 0
(28)
14
as j→ ∞o for every interval I.
From (13) and (27) we get for ≈ € I, k ≥ j/2
Bm
|ø(*) (z)| ≤ Σ [ø(m+k)(0)| |x|″ < Alights
||=| ≤ Aight Mm+kh™ B™
m!
m=0
Using 1) and 2), we obtain
|ø(*)(x)| ≤ A1‚¢h*p(ho)*+¹ Mk Σ TmBm ≤ Ã1,h™ Mx,, k≥ j/2, ≈ € I. (29)
m=0
In the case k 0, n ≥ 0, h> họ.
η
c) There exist two positive functions M and p on [0,∞) such that
M(k) = Mk, k≥0
holds for all > 1, μ ≥ 1, and h> ho.
h“M(µλ)¹¹ ≤ p(h)(µ − 1)AM(A)¹
-
(60)
(61)
(62)
21
Proof. We begin by showing that if there exists a positive function p such that
Man+mh" ho,
then assertion a) holds.
Suppose (63) is true and let € D({M}). Then
121k
2 + |ø (2k+j) ( x) | ≤ Ash³
k=0
Applying (63) with h = 2h2|z|, we get
and
It follows from (64) and (65) that
[U₁6(x)]() =
M2k+i h2* |z|* < 2−*p(2h3|z|)i+¹Mj.
2k
k!
Σ — +
k=0
k=0
121* 2k
k!
-h2 M2k+j⋅
$(2k+j) (x),
(63)
(64)
(65)
[[U₂6(x)](i)| ≤ c₂‚øh²¿Mj, z€ C, j≥ 0,
which proves that (63) implies a). Using Cartan-Gorny Theorem (see Theorem 2 in Section
3, we conclude that a) follows from b).
Remark 3 Analyzing the previous part ot the proof of Theorem 3, we see that condition
(63) implies not only the validity of inclusion a), but also the continuity of the operators U,,
z> 0 on D({M}). Since the topologies of the classes D({M}) and D({M}) coincide (see
the proof of Cartan-Gorny Theorem in [8]), the validity of condition b) in Theorem 3 implies
the continuity of U, on the class D({Mx}).
22
The next step consists in proving that a) implies b). Appealing again to Cartan-Gorny
Theorem, we see that condition a) is equivalent to the condition
U₂(D({M})) CD({M}), z E C.
Therefore, we should prove that b) follows from (66).
The sequence {M} is logarithmically convex and hence convex. Without loss of gener-
ality we may suppose that M increases and that M₁ = 1. It is easy to see that for such
{M} there always exists a smooth logarithmically convex increasing function M on [0,∞),
for which
and
M(k) = Mk, k≥0
Denote
lim
818
(68)
Now consider the following continuous version of the Ostrovski function (see Section 3)
(69)
In M(u)
น
T₁(r) = sup
W,(u)
=
ru
M(u)'
you
M(u)'
Since V(0) = 1 and equality (68) is true, we have
∞.
T > 0.
u > 0, r > 1.
W,(0) = 1, lim.—∞ W‚(u) = 0.
Therefore, the continuous function W, attains its maximum on [0,∞).
Denote
(66)
P(u) = ln M(u)
น
Since M is logarithmically convex, the function P increases.
(67)
23
It is easy to see that the point u。 = u。(r), at which the maximal value of W, is attained,
satisfies
Thus
It is clear that
where
u。(r) = P−¹(lnr).
P(u。(T)) = ln r.
T₁(r) =
go40 (r)
M(uo(T))'
(71)
After these prelimimary considerations we proceed with the proof of the implication
a) ⇒ b).
Suppose (66) holds. Define a function by
φ(z) = Σ
Σ
k=1
Differentiating formally, we obtain
COS(T(k)x)
k² T₁(T(k))'
From (67) and (69) it is clear that
r > 1.
T(k) = eP(k), k ≥ 1.
(73)
Let us show that the series in (72) and all the m-times termwise differentiated series
converge absolutely.
|ø(m) (x)| ≤ Σ k²T₁(7(k))*
T(k)m
x Є R¹,
T₁(T(k)) >
T(k)n
M
for every k and n. Applying (75) with n = m to (74), we get
(70)
|ø(m) (x)| ≤ MmΣk-², m≥0,
k=1
(72)
(74)
(75)
24
which means that $ € D({M₁}).
Using (66), we obtain
U_h(4) € D({M}),
and recalling the definition of the class D({M}), we get
k=0
with some positive function p.
It is clear that
(−h)* $(2k+j) (0)| ≤ chp(h)³M,, j≥0
k!
$(2k+m) (0) = 0
for every odd integer m. In the case of the even integer m = 2j we get from (70), (71), and
(73) that
T(m)2k+2j
ø (2k+2;) (0) = (− 1)k+; † T(m) 2k+2;
m²T₁(T(m))
Σ
m=1
It follows from (76) that
242
k=
MmT(m) 2k+2j
m²τ(m)m
=1
=(−1)k+iMmT (m)²k+2j
m²r(m)m
m=1