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1. Thus and from the graphs of F(X) and of the straight line with negative slope g(X) — —mX, the required inequalities (23) follows. • X telle que tp\(p(K) = tp'1. La formule G(y) = (p(F(tp(y))) definit une fonction multivoque compacte s.c.s. et acyclique de / " dans lui-meme. D'apres le resultat cite d'Eilenberg et Montgomery, G a un point fixe yg, et il est facile de voir que X une fonction multivoque compacte s.c.s. et acyclique. Le lemme 1 nous fournit une X verifiant les conditions du lemme 2. Soit 0, done G est aussi acyclique. Puisque Z appartient a A, (U(Z), T') est un retracte absolu. Le theoreme de point fixe mentionne dans l'introduction montre que G a un point fixe ZQ. Alors z0 appartient a Z, done tp(z0) = (f(zo) € 0 there exists a neighborhood U C B of this point such that \ip(t) - v{i/)\ < e 71 0 be an arbitrary number, KE{UQ) be the ball of radius e around UQ in the space H™+n. A pseudosolution of the problem (1), (2) is defined to be a the function ue e H™+n minimizing the estimation error 0 is a weighted coefficients, 7172 ^ 0. If 71 or 72 is equal to zero then we erase respectively addend and equate respectively norm to zero. For instance, 71 denotes that we minimize the functional \\lu — V?l|2_i/2 o n the set of solutions of system Lu = f in the ball K6{UQ). This problem is studied in the paper [9] for the PDE with constant coefficients at the case / = 0. In contrast to the problem (1), (2) this problem not always has pseudosolutions. The other nonlocal problem, in particular, multipoint and also the nonlocal problem in other scales of functional spaces can be studied in the same way. References 1. A.A. Dezin, General questions of the boundary value problems theory. Nauka, Moscow, 1980 (in Russian). 2. B.Yo. Ptashnyk, Several ill-posed boundary value problems for PDE. Naukova dumka, Kyiv, 1984 (in Russian). 3. V.S. Il'kiv, Multipoint nonlocal boundary value problem for PDE, Diff. uravneniya (Diff. equations) 23 (3) (1987) 487-492. 4. E.A. Grebennikov, Yu.A. Rjabov, Resonances and small denominators in celestial mechanics. Nauka, Moscow, 1978 (in Russian). 5. V.S. Il'kiv, Nonlocal boundary value problem for normal anizotropic systems of partial equations with constant coefficients, Visnyk of the Lviv University. Series Mechanics and Mathematics (1999) (54) 84-95 (in Ukrainian). 6. V.S. Il'kiv, Nonlocal boundary value problem for systems of partial equations in anizotropic spaces, Nonlinear boundary value problems 11 (2001) 57-64 (in Ukrainian). 7. Yu.P. Pytiev, Mathematical methods of experiment interpretation. Vysshaja shcola, Moscow, 1989 (in Russian). 8. V.V. Vojevodin, Yu.A. Kuznjecov, Matrices and calculations. Nauka, Moscow, 1984 (in Russian). 9. V.S. Il'kiv, Investigation of nonlocal boundary value problem for normal partial differential equation by means of minimization method in Sobolev spaces, Mathematychni studii 11 (1999) 167-176 (in Ukrainian). G T^{Ma) for every y> G X, n € N. Analogously one can prove that \in9 G 2?(Ma) for every g € V(T) C X',n£ N. Then from (3) and (4) we get for every ^ 6 l , j £ D(T), and n G N, / <^XTn -Tg-Magdm +), then ip £ V(MOi.P+) and P+MOiiP+¥ (R(A)), . Then Vt G Z a;(i) = ^ /02?r x^e1** dip and SS(^) = e i v x ( » . Thus the spectrum of 3 is the circle {elv : 0 < u{ t ) of U~g <j>u(t) = Eexp(i(T,J7 -$)) = Eexp(i([/*T, ^ ) ) = 0, J^(f) = J^(vr) = 0, e G (0; ^ ) . Then the function |J($,a;)| — 1 = — evsin(i/xi) satisfies the conditions (6), (7) (see, for instance, [4]). This means that the mapping $ preserves the measure of all unit balls and all balls with radius r £ An. Repeating the arguments from the proof of Theorem 2 we conclude that $ is one-to-one mapping. Besides, since | J ( $ , x ) | is not identically unit there exists a ball B e l " such that m($(B)) ^ m(B). This completes the proof of Theorem 3. References 1. 2. 3. 4. 0. Note that even in the case of Banach space E the condition (6) is weaker than the classical Cartan's condition (see [3]) requiring the operator x *-> g(x,-) be an isomorphism of the spaces E and E*. Proposition 11. If a quadratic form
56
Jamel Ben Amara
Corollary 12. The eigenvalues An satisfy the asymptotic An = ( — ) +o(n 4 ), \ 7/
as n —> oo,
(24)
where 7 = / ( - J) Jo \P
dt.
Proof. This follows from Theorem 11 and the asymptotic (e.g; see [9], Chap. 2) Pn=(—) [l + O(-)l, V7 / L nJ
as
n->oo.
(25)
D We shall now examine the relation between An and pn more carefully. The graphs of F and g might suggest that (An — p n - i ) —»• 0, as n —> oo, but this is not true as shown in the following result. Theorem 13. Let m > 0 and let p, ,r be positive and belong to Wf [0,1]. Then An-pn_ixn2,
as ra —> oo.
(26)
Proof. Let G(X) = (F(X))'1. Since F(A) is meromorphic, then by (23), G is C 1 on /„ = [pn-i, An] (G has no poles in In). Thus we obtain G(Xn) - G{pn.x)
= (An - p n _i)G'(A n )
(27)
for some A s / „ . From (19) and (24), it follows that the left side of (27) is of order n~ 4 . We study now the behaviour of G'(A) for A G In and large n. From (18) and (22) we obtain
G'(X) = rory\x,X)dx ([(py"(x,\)y-qy'(x,X)]lx^)2 From (23) it follows that {(py"(x, A))' - qy'(x, X)}\x=7r ^ 0 for A e / „ , hence G' is a bounded function on / „ . Let {yi{x,X)Y^z\ be a system of fundamental solutions of Equation (1.1) satisfying the asymptotics (e.g., see [9], Chap 2) wx
yi(x)=e"
' [l
+ O^-1)},
as H->oo
and y\k\x) = (r/p^^w,)^^[l + O(p-% k G {1,2,3}, 4 4 where /i = A, Wi = 1 and X = ^{r/pY^dt. Without loss of generality, we can suppose that the solution y(x, X) of Problem (6) satisfies j/"(0) = 1. Using the above asymptotics we obtain
y{x,X) = [(cos/JT - coshMX) -
c o s
^ + c o s h ^ ( s i n / ,x - 8inh/xX)][l + O(M" 1 )] sin //7 - sinh ^7 = ( c o s p X - s i n p ^ f l + O^" 1 )] (29)
Fourth Order Spectral Problem
57
as \n| —» oo, where the constant 7 is denned in Corollary 13. Moreover, u
"t
wv
it
\M
3 / l + cosh/rycos/^A
_:
[(py (x,A)) - W ( * , A ) ] | x = i r = „ ( — ^ — , - ^ - J [1 + O(M 3
1
=/i cos/i7[l + 0(/i" )],
X
)]
(3())
as |//| —» 00.
From (29), (30), a simple calculation gives G'(Xn) x Mn6x
n
~6'
as
Therefore, from (27) the required result follows.
« —*• 00. •
R e m a r k 14. In the case m < 0, the interlacing property (23) of the eigenvalues slightly changes, while the asymptotics of Xn obtained for m > 0 remains valid. More deep studies of this and of the indefinite case will be done in a separate work.
The author thanks A.A.Vladimirov of the Moscow State University, for many helpful discussions. The author also thanks the referee for useful comments. References 1. M. J. Ahn, Quart. Appl. Math. 39 (1) (1981) 109-117. 2. T.Ya. Azizov, I. S. Iokhvidov, Linear operators in spaces with indefinite metric. John Wieley, Chichester, 1989. 3. J.A. Ben Amara, A.A.Shkalikov, A Sturm-Liouville Problem With Physical and Spectral Parameters in Boundary Conditions, Mathem. Notes 66 (2) (1999) 163-172. 4. P.A. Binding, P. J. Browne, K. Seddighi, Sturm-Liouville problems with eigenparameter dependent boundary conditions, Proc. Edinburgh Math. Soc. 37 (1993), 57-72. 5. L. Collatz, Eigenwertaufgaben mit Technischen Anwendungen. Akademishe Verlag, Leipzig, 1963. 6. C.T. Fulton, Two-point boudary value problems with eigenvalue parameter contained in the boundary conditions, Proc. Soc. Edinburgh Sect. A 77 (1977) 393-308. 7. F.P. Gantmaher, M. G. Krein, Oscillating matrices and kernels and small oscillation of mechanic systems. Moscow 1957. 8. W. Leighton, Z. Nehari, On the oscillation of solutions of self-adjoint linear differential equations of the fourth order, Trans. Amer. Math. Soc. 98 (1958) 325-377. 9. M.A. Naimark, Linear differential operators. Ungar, New York, 167. 10. F. Roseau, Theory of vibration in mechanicals systems. Springer-Verlag 1983.
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Jamel Ben Amara
11. A.A. Shkalikov, Boundary value problems for ordinary differential equations with parameter in the boundary conditions, J. Soviet Math. 33 (1986) 1311— 1342. 12. A.A. Shkalikov, Operator pencils arising in elasticity and hydrodynamics: Instability index formula, in the book "Operator theory: Advances and Applications", Vol. 87 258-285, Birkhaiiser Verlag, 1996. 13. S.P. Timoshenko, Strength and vibrations of structural members. Collection of paper (E. I. Grigolyuk, editor) in Russian, Nauka, Moscow, 1975. 14. A.G. Kostyuchenko, A.A. Shkalikov, On the theory of self-adjoint quadratic operator pencils, Math. Bull. Moscow State Univ. 38 (1983) 44-58. 15. J. Walter, Regular eigenvalue problems with eigenvalue parameter in the boundary conditions, Math. Z. 133 (1973) 301-312.
Functional Analysis and its Applications V. Kadets and W. Zelazko © 2004 Elsevier B.V. All rights reserved
59
Extending Operators into C^ Spaces Under a Twisted Light Felix Cabello Sanchez, Jesus M. F. Castillo, Yolanda Moreno Departamento de Matematicas, Universidad de Extremadura 06071 Badajoz, Spain
David T. Yost Department of Mathematics, King Saud University P.O. Box 2455, Riyadh 11451, Saudi Arabia
Abstract We present a homological approach to the problem of extending operators which take values in C(K) or C^ spaces. In this way we obtain unified simpler proofs of results of Lindenstrauss-Pelczynski and Johnson-Zippin. Key words: Extension of linear operators, operator ideals, Banach spaces 2000 MSC: 46B20, 47L20
Introduction and preliminaries The classical problem of extension of linear operators is: when can a given operator Y —> B from a subspace Y of a Banach space X be extended to an operator Email addresses: f [email protected] (Felix Cabello Sanchez), castilloSunex.es (Jesiis M. F. Castillo), ymorenoOunex.es (Yolanda Moreno), dthoyost8ksu.edu.sa (David T. Yost). 1 FCS, JMFC and YM where supported in part by the DGICYT project BFM 2001-0813. DTY'sde Extremadura and partly by KSU Research Centre Project Number Math/1420/25.
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Felix Cabello et al.
X —> B7 Equivalently, when is the restriction operator 2(X, B) —* £(Y, B) surjective? Linear continuous operators cannot, as a rule, be extended; but it is possible in many interesting situations. For instance, when either i) Y is complemented in X; or ii) B is injective; or iii) the operator is 2-summing (regardless of the spaces involved; see [10, Theorem 4.15]). We see that there are three variables involved here: the pair Y —> X, the space B, and the class of operators 21 we want to extend; and, accordingly, there are three different extension problems depending on which two of these three elements are chosen as the data. Our main concern will be generalizations of ii) due to Lindenstrauss-Pelczynski and Johnson-Zippin. The fact that an injective Banach space has to be an /^-space attracts one's attention to /^-spaces. The fact that the identity operator CQ —>• CQ cannot be extended to l^ sets the limits of what can be done: in general, even C(K)-valned operators cannot be extended. The problem admits an algebraic formulation and treatment, and this is precisely the point of view and the language we adopt in this paper. For general information about £oc-spaces, see [10, Chapter 3] or [2]. In section 3 we assume from the reader familiarity with the basic theory of exact sequences and extensions; in section 4, only, we moreover assume familiarity with the theory of quasi and zero-linear mappings. All this background can be found in [1] or [8]. Here is a brief description. A short exact sequence (also called an extension of Z by Y) is a diagram 0
> Y — — > X -^—*
Z
• 0
(!)
composed of Banach spaces and operators in which the kernel of each arrow coincides with the image of the preceding one. Two exact sequences 0 —* Yi —> Xi —> Zi —> 0 (i = 1,2) are said to be isomorphically equivalent if there exist isomorphisms a,/?,7 making the diagram 0
> Yx
a
l
> Xx
4
> Zx
>0
7
1
0 > Y2 > X2 > Z2 >0 commutative. This notion was introduced in [5,9] and clearly generalizes the older notion of equivalent sequences (where it is assumed that Y2 = Y\, Z2 = Zx and a and 7 are the identity). An exact sequence (1) is said to split if it is equivalent to the trivial sequence 0 —> Y —> Y © Z —> Z —> 0; a common shorthand for this is Ext(Z, Y) = 0. There is a correspondence between exact sequences of Banach spaces (1) and the so-called zero-linear maps, which are homogeneous maps F : Z —> Y satisfying an estimate ||F (X)ILi xi) ~ Z)ILi F (xi)\\ — ^-F X) llx*ll f° r s o m e constant Ap, each n e N and all Xi G Z. With these tools let us return to the extension problem and consider it in full generality, replacing £ by other operator ideals. Since it is well known that given a
Extending Operators into £oc Spaces Under a Twisted Light
61
surjective operator ideal 21 (see [8, §2.5]), an exact sequence (1) and a fixed Banach space B the induced sequence
o
> X(Z,B)
*' ) 2i(x,B)
'* > a(y,B)
>o
(2)
is exact u p t o 2l(X, f?), the extension problem consists in deciding whether the whole diagram (2) is exact. If so, we shall say that the functor 2l(-,B) is exact at (1). A functor is called exact (see [8]) when it is exact at every exact sequence. For instance, the functor £(•, B) is exact if and only if the space B is injective.
A brief reminder of extension results When 21 = 8., the ideal of compact operators, an affirmative answer to the extension problem characterizes jC^-spaces. Precisely: Proposition 1 (Lindenstrauss [15]). A Banach space B is an Cx space if and only if the functor £(•, B) is exact. Proof. Let B be an iZoo-space and let T : Y —> B be a finite rank operator. Since T(Y) is A-isomorphic to a subspace of some f^-space, the operator T admits a finite rank extension r : X —> B with ||r|| < A||T||. But £x spaces have the (bounded) approximation property and so the finite rank operators are dense in &(Y, B). Thus, the restriction &(X, B) —> &(Y,B) is almost open and therefore (open and) surjective. To prove the converse just observe that the canonical inclusion S : B —> B** extends to any superspace X by: A(x)(b*) = limu(A£;a;)(6*), where E denotes a typical finite dimensional subspace of B, il is an ultrafilter refining the Frechet filter on the directed set of all such subspaces, and A# is an extension (with norm at most A) to X of the restriction of 5 to E. It follows easily that B** is A-complemented in X**, and by a well known characterization of £oo-spaces, that is all that we need.
•
The choice 21 = 2U, the ideal of weakly compact operators, was first published by Bourgain and Delbaen [3, Theorem 2.4]. Their real contribution was to give examples of spaces showing that the following result is not vacuous. Proposition 2. A Banach space B is an C^ space with the Schur property if and only if the functor 2U(-, B) is exact. The proof is as before taking into account that weakly compact operators into a Schur space are compact (only if); to get the if part, take a weakly null sequence in B. The sequence is contained in the image of some reflexive space; when extended to all the C(-KT)-space this weakly compact operator should be completely continuous.
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Felix Cabello et al.
Straeuli considered in [19, 3.1] the extension problem for different operator ideals. We quote: Proposition 3. Let 21 be an idempotent operator ideal with A C 21 C 9t, where *H denotes the Rosenthal operators. Then the functor 2l(-, B) is exact if and only if B is an £ oc -space such that 2l(-, B) = &(-,B) The extension problem for the choices 21 = 8. or 21 = 2U but fixing the exact sequence was solved by Fakhoury [11, Theoreme 3.1]: Proposition 4. The functors &(-,B) —or W(-,B)— are exact at (1) if and only if the dual sequence 0 —> Z* —> X* —> Y* —> 0 splits.
One then says that (1) locally splits or that Y is locally complemented in X. (Other authors use different terminologies.) Returning to the general problem, there are two distinguished situations in which C(ii')-valued operators extend: the Lindenstrauss-Pelczynski theorem [16] for subspaces of CQ and the Johnson-Zippin theorem [12] for weakly* closed subspaces of
Proposition 5 (Lindenstrauss-Pelczyriski). Every C(K)-v&lued operator defined on a subspace of CQ can be extended to all of CQTheir proof is of Hahn-Banach style, showing that if H C CQ, T : H —> C(K) is an operator, e > 0 and p £ H, then there exists an extension Tp : H +\p] —> C(K) with norm ||TP|| < ||T|| + s. Therefore, an operator T : H —> C(K) defined on a subspace H of CQ can, for every e > 0, be extended to an operator r : Co —> C(K) with ||T|| < (1 + e)||T||. An equal norm extension (i.e., s = 0) cannot be achieved as an example of Johnson and Zippin [13] shows. In this same paper Johnson and Zippin extend the validity of the extension result to subspaces of CQ(T) using a different approach, which we will discuss now, that allows one to circumvent the e in the original proof. Given an inclusion i : Y —> X, Lindenstrauss [15] approached the extension problem for C(K)-v&lued operators in different ways, one of them being the existence of a certain selection for the dual quotient map i*. This was precisely formulated by Zippin in [20]. There, Y is said to be A-almost complemented in X if each operator T : Y —> C{K) extends to X with norm at most A||T||: Lemma 1. Let i : Y —> X be an isomorphic embedding. Then Y is A-almost complemented in Xif and only if there exists a weakly* continuous function u> : Bally* —> A BallX* such that i*ui = id. (We shall call such a function a selector for i*.)
Extending Operators into Cx Spaces Under a Twisted Light
63
Proof. As usual, we identify K with the carrier space of C(K). If a weakly* continuous selector u : BallY* —> ABallX* exists for i* then r(x)(k) = u(T*k)(x) defines an operator r : X —> C(K) with ||T|| < A||T|| and such that r(i(y))(k) = u(T*k)(iy) = i*u(T*k){y) = T*k(y) = Ty(k). Conversely, if every C(-Ff)-valued operator admits such an extension then consider the canonical operator <5 : Y —> C(Ball Y*, weak*) and let D be its extension to X with norm at most A. The weakly* continuous selector for i* is ui(y*)(x) = D(x)(y*), since u{y*)(i(y)) = D{i(y))(y*) = y*{y). • Let us say that (1) A-almost splits if Y is A-almost complemented in X through i. Observe that the notions of almost split and locally split sequences are independent. On one hand, the sequence
0
> X —*—>• C(BallX*)
> C(BaRX*)/d(X)
>0
almost splits, as follows from the existence of the weakly* continuous selector BallX* —> BallC(BallX*)* for 6* given by D(x*)(f) = f(x*). Since \\D{x*)\\ = \\x* |J the sequence 1-almost splits. This sequence locally splits if and only if X is an £ oc -space since in that case X** would be complemented in C(BallX*)**. On the other hand, the sequence 0 —> X —> X** —> H(X) —> 0 locally splits, while it does not almost split when X is a non-injective C(-ff)-space. With the aid of this approach Zippin obtained in [21,22] different proofs for the Lindenstrauss-Pelczyriski theorem. At the end of the paper [21] Zippin poses three questions, one of which connects with the nature of the Ext functor: When does an exact sequence 0 — • E —> l\ —> Z —> 0 almost split? By, e.g. [7, Theorem 1.1], this is the same as asking: When is Ext(Z, C(K)) = 0? We will use this equivalence several times in the sequel. A substantial answer to this problem was obtained by Johnson and Zippin in [12]. (A partial converse to this in [14] shows that the hypothesis on the subspace cannot be weakened much.) Proposition 6 (Johnson-Zippin). Every C^-valued operator defined on a
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Felix Cabello et al.
The Lindenstrauss-Pelczyriski theorem We reformulate Proposition 5. Theorem 1. Every exact sequence 0 —> H —> CQ —> CQ/H —> 0 almost splits. Proof. The first ingredient of our proof is a decomposition result of Johnson, Rosenthal and Zippin (see [18, Theorems l.g.2 and 2.d.l]) asserting that every subspace H of CQ admits an exact sequence 0 —> co(An) —> H —> co(Bn) —> 0 in which An and Bn are finite dimensional spaces. Crossing the new sequence with the starting one and completing the diagram we get 0 0
I I
i I
co{An) =
0
>
0
> co(Bn)
co{An)
H
>
I
c0
I > co/co(An)
> co/H
>0
I > co/H
• 0
W
I
I
0 0 To control the vertical sequence centered at CQ we use a theorem of Lindenstrauss and Rosenthal [17] which implies that any such sequence is isomorphically equivalent to a sequence 0 > co(An) — = - ^ co(C ( n ) ) > co(e™M/An) > 0, where K is defined by K,((an)n) = (jra(«n))n, for suitable (1 + e)-into isomorphisms j n : An —> £™ . The Bartle-Graves selection principle (we use the stronger version appearing in [1, Proposition 1.19 (ii)]) yields a continuous selector uin : Ball A^ —> (1 + e) B a l l ^ for fn. Putting together all these maps, we obtain a selector LJ : Ball(£i(^;)) —> (1 + e)Ball(£1(e™in))) for K* defined by w ( « ) n ) = (w n (a^)) n . This selector turns out to be weakly* continuous since its domain is metrizable and a bounded sequence in a space £i(Fn) with Fn finite-dimensional is weakly* null if and only if the norms of its projections into Fn are convergent to 0. In conclusion, every exact sequence 0 —> co(An) —> CQ —> Q —> 0 almost-splits. We just finish the proof with a kind of 3-space property for the extension of operators. (Actually, one should be a bit more careful because the LindenstraussRosenthal result used above only gives an isomorphically equivalent sequence; we leave the reader to worry about these details.)
Extending Operators into Cx Spaces Under a Twisted Light
65
Proposition 7. If the functor £(•, 4>) is exact at the sequences 0 —> A —>• X —> X/A —> 0 and 0 —> Y/A —> X/A —> X/Y —• 0 then it is also exact at 0 —> Y —> X —> X/Y —> 0. Proof. This can be seen by drawing homology sequences but this time it is easier to go back to basics. So let T € £(Y, 6) be any operator. By our first assumption, T\A admits an extension S : X —> 4- Since S — T vanishes on A: its restriction to Y factorizes as RQ where Q : Y —> Y/A is the quotient map and R £ £(Y/A, £). Our second assumption guarantees that R has an extension (for which we use the same symbol) in £(X/A, 4k). Then x — i > Sx — R(x + A) is the required extension of T. D Our homological approach has some advantages and, of course, some disadvantages. The worst of these is the absence of a good estimate for the norm of the extension: we obtain (1 + e)-for subspaces of CQ of the form co(An) but the estimate for general subspaces blows up during the last part of the proof. This is precisely the benefit of Zippin's careful work [22]: he obtains 1 + e. The advantages, on the other hand, are clear: our proof is clean and, as we shall see, by duality it provides a proof for the Johnson-Zippin theorem. We close this section with an example showing that the hypotheses of the Lindenstrauss-Pelczynski theorem are optimal, in the sense that C^-fQ-spaces cannot be replaced by arbitrary £oc-spaces. Since we will refer to the following construction of Bourgain and Pisier [4] later on, we quote it at this stage. Proposition 8. Any separable Banach space Y can be embedded in a separable £oo space ^^(Y) such that CX{Y)/Y has the Schur property. Example. Let 0 —> H —> CQ —> Q —> 0 be an exact sequence with Q ^ CQ. Then there is an operator from H into an £ oo -space that cannot be extended to CQ. Proof. Let 0 —> H —> Coo(H) —> S —> 0 be the corresponding Bourgain-Pisier sequence. Pushing out and completing the diagram [8] we obtain
0
>
0
0
i
i
H
>
I 0
> CX(H)
1 S I 0
= =
c0
> co/H
I
II
> PO
• co/H
1 PO/co 1 0
>0
>0
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Felix Cabello et al.
Now, if the inclusion H —> COO(H) extends to CQ then the lower row splits and PO = £X(H) © CQ/H. However, the middle vertical sequence certainly splits by Sobczyk's theorem, so that PO = c0 © S. Therefore CX(H) © co/H = c0 © S thus making Co/H a complemented subspace of CQ © 5. Since 5 is Schur, it is totally incomparable with CQ and thus by the Edelstein-Wojtasczyk theorem (see [18, Theorem 2.C.13]) CQ/H decomposes as A © B where A is a complemented subspace of CQ and B a complemented subspace of S. Since Co/H is a subspace of Co then B has to be finite dimensional, and therefore CQ/H = CQ, which we assumed not to happen. •
The Johnson-Zippin theorem We reformulate Proposition 6 via almost splitting sequences; of course the extension result is also valid for £oc-valued operators and not only for C(i^)-valued ones. Theorem 2. Let H be a subspace of CQ. Every exact sequence 0 —> H1- —> lx —> H* —> 0 almost splits. Proof. First of all, a fundamental difference from other extension results is our access to the tool which we mentioned earlier: a sequence 0 —> W —> l\ —> X —>0 almost splits if and only if Ext{X, C{K)) = 0 for all C(K)-spaces. Thus the result asserts that whenever H is a subspace of CQ then Fxt(H*, C(K)) = 0 for all C(-£Q-spaces. Now, entering into the proof, since every subspace H of CQ admits a decomposition 0 —> Co(An) —> H —> co(Bn) —> 0, every dual H* of a subspace of Co admits a decomposition 0 —> ii(B^) —> H* —> ii(A^) —> 0. The property Ext(-, 4) = 0 is a 3-space property (e.g. [7, Corollary 1.2]), so it is enough to prove that Ext(^(F n ), £oo) = 0. Every exact sequence 0 —> C^ —> X —> Z —> 0 locally splits, so there is a constant C such that every exact sequence 0 —*• £oc —> Xp —> F —> 0 with F finite dimensional splits and there exists a projection Xp —> C^ with norm at most C (see [6]); i.e., Ext(F,£oo) = 0 uniformly on F. So, Ext(£i(.F n ), £-,<,)) = nExt( J F n ,£ o o ) = 0. D An estimate of the norm of the extension can be obtained through a non-linear argument: Lemma 2. Let 0 —> Y —> X —• F —> 0 be an exact sequence with F finitedimensional. For every e > 0 there exists a homogeneous lifting g : F —> X for n with finite-dimensional range, and ||g(x)|| < (1 +e)||a;|| for all x 6 F. If furthermore Y is an £00^ space then there is a projection P : X —> Y with norm ||P|| < A + 2 + e.
Extending Operators into Cx Spaces Under a Twisted Light
67
Proof. Let A be a finite (symmetric) subset of the unit sphere of F whose convex hull contains the ball of radius 1 — e. For each a G A choose a point g(a) G a + Y with ||g(«)!l < 1 + e, and put g(0) = 0. Any x £ F with norm 1 — e is a finite convex combination of elements of A; define g(x) as the corresponding convex combination from g(A). Extending g to all of F by homogeneity gives us a selection for the quotient mapping with finite dimensional range. It also satisfies the inequality ||g(x)|| < (1 + e)(l — e)"1!!^!! for all x G F, which is near enough. Now suppose that Y is an £OC,A space. Let £ : F —> X be any linear lifting for the quotient mapping, and define fi : F —> Y by Cl(z) = £(z) — g(z). This is a zero-linear map with constant An < 1 + e. Since Q(F) is finite dimensional, it is contained in some finite-dimensional subspace E of Y which is within BanachMazur distance A of a finite dimensional P^, space. Now we apply the so-called nonlinear Hahn-Banach Theorem [5, Lemma 1] coordinatewise to obtain a linear mapping L : F —> Y satisfying the inequality \\L(z) — ^(z)ll ^ M\z\\The operator {£ — L) o IT : X —> X is a projection with kernel Y (one has ((£ — L) o TT)2 = (£ — L) o TT since TT O L = 0 and TT O £ = id) and verifies, for any x, | | ( ^ - L ) 7 n r | | < \\£irx - nirx\\ + \\n-rrx - Lirx\\ < (1 + e + X)\\wx\\. Hence id — (£ — L)ir is the desired projection onto V with norm < 2 + A + e.
•
Since C(.ftf)-spaces are jC^A-spaces for every A > 1, the decomposition technique of the previous section gives us an estimate of 3 + e for the norm of a projection in an exact sequence 0 —> C(K) —> X —> H* —> 0 when H is a subspace of Co(FjJ). This is the same estimate that Johnson and Zippin obtain in [12], although our proof is considerably simpler. However, under the additional assumption that E has the approximation property, they were able to obtain the stronger conclusion that the extension operator T could be chosen so that ||T|| < (1 +e)||T||. They ask if this estimate could be true without the approximation property; this remains unknown.
Further results and open problems Let's begin this section with another especially interesting example of almost splitting obtained by Zippin in [20,21]: Proposition 9. Every sequence 0 —> W —^-> £p —> £P/W —> 0 (with 1 < p < oo) almost-splits. Since the proof does not explicitly appear in the literature, let us present here a sketch: the dual space £*p = £p* is strictly convex, so there exists a unique Hahn-Banach extension operator u : W* —> lp*. We show that its restriction u) : Ball W* —> Ball £p- is weak*-to-weak* continuous. The map u) is the composition of three maps
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W
— ^
lp
where Jp and Jw are the support mappings (also called the duality maps). Since Jp(x) = ||x|| 2 ~ p |x| p ~ 1 sgn x, it is clear that Jp is weakly sequentially continuous, as is the inclusion i. The support mapping Jjy is just Jp o i. Its restriction to Ball W endowed with the weak topology is a continuous map from a compact space to a Hausdorff space, hence a homeomorphism; this makes its inverse weakly continuous. In general, however, the extension of operators on a reflexive subspace is not to be expected. Suppose for example that a sequence 0 —> Y —> X —> Z —> 0 does not locally split (as will be the case when Y is complemented in its bidual but not in X). Then there exists, by Proposition 4 and the well known factorization of weakly compact operators, an operator T : Y —> R into some reflexive space R that cannot be extended to X. This gives rise to the question of what happens when R is embedded into some C(K) space. Does the resulting composition Y —• R —> C{K) extend to XI In particular Question 1. Does every sequence 0 —> £2 —> C[0,1] —• C[0, l]/^2 —> 0 almost split? We remark that, in general, £oo-valued operators cannot be extended: consider the diagram
o
> e2 —!-^
c[o,i]
• c[o,i]/e2
> o
0
> £2 - ^ - ^
£00(^2)
>
> 0
S
in which £00(^2) is the Bourgain-Pisier space associated to £2 (Proposition 8). Since S is Schur, £00(^2) does not contain CQ and therefore any possible extension J : C(K) —> £00(^2) of j would be weakly compact, hence completely continuous (by the Dunford-Pettis property of C(K)- spaces) and therefore J o j could not be the identity on £2A simpler argument (using the fact that every operator ^ —> C[0,1] is weakly compact) shows that if X is a separable non-Schur space, then no sequence 0 —> X —> 4c —• £^/X —>0 almost-splits. The notion of almost-complementation puts all C(-ftT)-spaces at the same level. We could, however, try to distinguish between different C(ii")-spaces regarding extension properties of operators into them. As a token that such finer classification is possible, we consider the sequence 0 —> WT —• £\ —* T —> 0 where T denotes Tsirelson's space. Since Tsirelson's space emphatically fails the Schur property, it follows from [7,14] that this sequence admits operators WT —• C[0,1] which do not extend to £1, yet every operator WT —> C(utu) does extend to £\. This suggests Question 2. Given a fixed compact space K, characterize the sequences 0 —> Y —> £1 —> Z —> 0 such that all operators Y —> C(K) extend to £\.
Extending Operators into Coc Spaces Under a Twisted Light
69
The problem of distinguishing between C(K) and /loo-spaces pervades the paper, so another natural question is: Question 3. If Ext(Z, C(K)) = 0 for every compact K, does Ext(Z, Cx) = 0 for all £oc-spaces? And, more generally and not only for subspaces of £\, Question 4. Let H be the class of all subspaces of CQ, and let C^Ti) be the class of all £oo spaces with the property that every operator T : H —> L from H e 7i into L G CociJ-i) can be extended to CQ. Characterize the class Coo(7i). The same question for the class of subspaces of £p, of subspaces of Lp, and for Hilbert subspaces of C[0,1] does not lack interest. Or difficulty: although many Banach spaces (e.g. complemented subspaces of C(K) spaces) belong to these classes, any characterization seems to be quite elusive. Now let 0 —> £2 —• £00(^2) —> S —> 0 be a Bourgain-Pisier sequence. If if is a subspace of CQ then £(H,£2) = 8.{H, £2) and also £(H, S) = &(H, S) since S is a Schur space. It is not hard to verify that £(H, 4) = R{H, 4) is a 3-space property (see [8, §6.1 and §6.7]). In particular £(H, £oo(4)) = &(H, Cx{£2)) and thus, by Proposition 1, operators H —• £00(^2) extend to CQ. Since £00(^2) does not contain CQ (another 3-space property, see [8]) it cannot be a complemented subspace of a C(K)-space.
References 1.
Y. Benyamini and J. Lindenstrauss, Geometric nonlinear functional analysis, Vol. 1, Amer. Math. Soc, Providence (1999). 2. J. Bourgain, New classes of £ p -spaces. Lecture Notes in Math. 889 Springer, Berlin-New York, 1981. 3. J. Bourgain and F. Delbaen, A class of special £oo-spaces, Ada Math. 145 (1980) 155-176. 4. J. Bourgain and G. Pisier, A construction of £oo-spaces and related Banach spaces, Bol. Soc. Bras. Mat. 14 (1983) 109-123. 5. F. Cabello Sanchez and J.M.F. Castillo, Duality and twisted sums of Banach spaces, J. Fund. Anal. 175 (2000) 1-16. 6. F. Cabello Sanchez and J.M.F. Castillo, Uniform boundedness and twisted sums of Banach spaces, Houston J. Math, to appear. 7. F. Cabello Sanchez, J.M.F. Castillo, N.J. Kalton and D. Yost, Twisted sums with C(i^)-spaces, Trans. Amer. Math. Soc. to appear. 8. J.M.F. Castillo and M. Gonzalez, Three Space Problems in Banach Space Theory, Lecture Notes in Math. 1667 Springer, New York-Berlin, 1977. 9. J.M.F. Castillo and Y. Moreno, On isomorphically equivalent extensions of quasi-Banach spaces, in Recent Progress in Functional Analysis, (K.D. Bierstedt, J. Bonet, M. Maestre, J. Schmets (eds.)), North-Holland Math. Studies 187 (2000) 263-272. 10. J. Diestel, H. Jarchow and A. Tonge, Absolutely summing operators. Cambridge Studies in Advanced Mathematics, 43 Cambridge University Press, 1995.
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11. H. Fakhoury, Selections lineaires associees au theoreme de Hahn-Banach, J. Functional Analysis 11 (1972) 436-452. 12. W.B. Johnson and M. Zippin, Extension of operators from weak*-closed subspaces of l\ into C(K) spaces, Studia Math. 117 (1995) 43-55. 13. W.B. Johnson and M. Zippin, Extension of operators from subspaces of CQ(T) into C(K) spaces, Proc. Amer. Math. Soc. 107 (1989) 751-754. 14. N. J. Kalton, On subspaces of CQ and extension of operators into C(fsT)-spaces, Quart. J. Math, (Oxford) 52 (2001) 313-328. 15. J. Lindenstrauss, On the extension of compact operators, Memoirs of the AMS 48 (1964). 16. J. Lindenstrauss and A. Pelczyriski, Contributions to the theory of the classical Banach spaces, J. Fund. Anal. 8 (1971) 225-249. 17. J. Lindenstrauss and H.P. Rosenthal, Automorphisms in CQ,£I and m, Israel J. Math. 7 (1967) 227-239. 18. J. Lindenstrauss and L. Tzafriri, Classical Banach spaces, Springer-Verlag. Berlin-Heidelberg-New York, 1977. 19. E. Straeuli, On Hahn-Banach extension for certain operator ideals, Arch. Math. (Basel) 47 (1986) 49-54. 20. M. Zippin, The embedding of Banach spaces into spaces with structure, Illinois J. Math. 34 (1990) 586-606. 21. M. Zippin, A global approach to certain operator extension problems, in Springer Lecture Notes in Math. 1470 (1990) 78-84. 22. M. Zippin, Applications of Michael's continuous selection theorem to operator extension problems, Proc. Amer. Math. Soc. 127 (1999) 1371-1378.
Functional Analysis and its Applications V. Kadets and W. Zelazko © 2004 Elsevier B.V. All rights reserved
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Un theoreme de point fixe pour les fonctions multivoques acycliques Robert Cauty Universite Paris 6, UFR 920, Boite courrier 172, 4, place Jussieu, 75252 Paris Cedex 05
Abstract We prove that equiconnected spaces have the fixed point property for multivalued u.s.c. acyclic compact mappings. Key words: points fixes, fonctions multivoques acycliques 2000 MSC: 54H25, 54C60, 55M20
1. Introduction Soit / = [0,1]. Un espace topologique X est dit uniformement contractile, ou UC, s'il existe une fonction continue A : I x I x / ^ I verifiant, quels que soient x, y dans X et t dans / , X(x,y,0) = x, \{x,x,t) = x
\{x,y,l)=y
S'il est necessaire de fixer la fonction A verifiant ces conditions, nous parlerons de 1'espaceUC (X,A). La classe des espaces UC est vaste. Elle contient les sous-ensembles convexes des espaces topologiques, les groupes contractiles et les retractes de tels espaces. En particulier, tout retracte absolu est UC. Email address: cautySmath.jussieu.fr (Robert Cauty).
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Pour tout compact K et tout entier n > 0, nous notons Hn(K,Q) le n-eme groupe de cohomologie de Cech de K a coefficients rationnels (cohomologie reduite si n = 0). Le compact K est dit acyclique si Hn(K, Q) = 0 pour tout n > 0. Soient X, Y des espaces separes. Une fonction multivoque compacte de X dans Y est une fonction faisant correspondre a tout element x de X un sous-ensemble compact non vide F(x) de V et telle que \Jx£X F(x) s °it contenu dans un compact de Y. Une telle fonction est dite semi-continue superieurement, ou s.c.s., si, pour tout point x de X et tout voisinage U de F{x) dans Y, il existe un voisinage V de x tel que F(y) C £/ pour tout y &V. Elle est dite acyclique si le compact F{x) est acyclique pour tout i £ l Si F est une fonction multivoque de X dans lui-meme, un point XQ de X est un point fixe de F si XQ £ F(XO). II est connu que si X est un retracte absolu, alors toute fonction multivoque compacte s.c.s. et acyclique F de X dans lui-meme a un point fixe. Lorsque X est compact, c'est un cas particulier d'un theoreme d'Eilenberg et Montgomery [4], et le cas general se ramene au cas compact comme suit. Soit K un compact de X contenant Lbex -^( x )i e^ s °it
/ et verifiant g(Xx(x,y,t)) = X(g(x),g(y),t) quels que soient x, y et t. Soit Y un espace UC, et soit F une fonction multivoque compacte s.c.s. et acyclique de Y dans lui-meme. Fixons un sous-ensemble compact X de Y contenant U 6 y F(y). La propriete universelle de notre foncteur nous permet de trouver une fonction continue r de U(X) dans Y telle que r(x) = x pour tout x G X. La formule G(x) = F(r(x)) definit alors une fonction multivoque compacte s.c.s. et acyclique de U(X) dans X. Si XQ est un point fixe de G, il appartient a X et, comme r(xo) = XQ, c'est aussi un point fixe de F. La demonstration est done ramenee a la verification du cas particulier suivant: Proposition. Pour tout compact X, toute fonction multivoque compacte s.c.s. et acyclique de U(X) dans X a un point fixe.
Points fixes des fonctions multivoques
73
La demonstration de cette proposition se fera en deux etapes. Nous la prouverons d'abord pour les compacts metrisables en utilisant l'existence d'un compact Z et d'une fonction continue
2. Le cas metrisable Si le compact X est metrisable, nous notons T(X) l'ensemble des topologies metrisables r sur U(X) qui sont moins fines que la topologie libre et telles que
Xx : {U(X),T)
x (U(X),T)
x I -> (U(X),T)
soit continue.
Lemme 1. Soit X un compact metrisable, et soit F une fonction multivoque compacte de U(X) dans X. Si F est s.c.s., il existe r £ 1~(X) telle que F soit r-s.c.s.. Demonstration. Soit B = {Bi}^L0 une base denombrable de X stable par reunion finie. Pour i > 0, soit Vt = {x € U(X) \ F(x) C Bz}. Pour tout compact K de X et tout voisinage U de K dans X, il existe i tel que K C Bi C U, done F sera r-s.c.s. si tous les Vi sont r-ouverts. Puisque F est s.c.s., V* est ouvert. Puisque U(X) est parfaitement normal, il existe une fonction continue c^ : U(X) —> I telle que a ^ Q O , 1]) = Vi. Definissons a : U(X) -*• I" p a r a(x) = (ao(x), ax(x),...). Puisque a est continue, le lemme 2 de [3] montre l'existence d'une topologie r € T{X) telle que a soit r-continue. Cette topologie a la propriete souhaitee. Soit A la classe des compacts X tels que (U(X), T) soit un retracte absolu quelle que soit r G T(X). Un compact iC est de forme triviale s'il est non vide et si toute fonction continue de K dans un retracte absolu de voisinage est homotope a une fonction constante; en particulier, un compact de forme triviale est acyclique. Le lemme suivant est prouve dans [2]. Lemme 2. Soit X un compact metrisable. II existe un compact metrisable Z et une fonction continue
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Robert Cauty
topologie r £ T(X) telle que F soit r-s.c.s. Fixons un compact Z et une fonction continue
3. Resultats auxiliaires Un systeme projectif d'espaces topologiques sur un ensemble ordonne filtrant A sera note S = (Xa,pP,,A) (les Xa sont des espaces topologiques et, pour a < (3, p^ : Xp —» Xa est continue). Nous notons lim§ la limite projective de ce systeme et pa la projection de limS dans Xa. Si B est un sous-ensemble filtrant de A, nous notons S\B = (Xa,p^,B) le systeme obtenu en restreignant l'ensemble des indices a B. Si B est cofinal dans A, nous identifions naturellement lim(S|B) a limS. Un systeme projectif § = {Xa,p^, A) est appele un w-systeme projectif s'il verifie les conditions suivantes: (a) Tout sous-ensemble denombrable totalement ordonne de A a une borne superieure. (b) Pour tout sous-ensemble totalement ordonne B de A admettant une borne superieure /3, la fonction lim^gep^ : Xp —> lim(S|B) est un homeomorphisme. (c) Chaque Xa a une base denombrable. II est connu que tout compact X est la limite d'un w-systeme projectif (Xa,p^, A) tel que les projections pa : X —> Xa soient surjectives (voir la demonstration de la proposition 3.2.17 de [6]). Un sous-ensemble B d'un ensemble filtrant A est dit ferme si, pour tout sousensemble totalement ordonne C de B admettant une borne superieure dans A, cette borne superieure appartient a B. Si § = (Xa,p^,A) est un w-systeme projectif et si B est un sous-ensemble cofinal et ferme de A, alors S\B est aussi un w-systeme projectif. Soient (Xa,p^,A) et (Ya,q^,A) deux o;-systemes projectifs de compacts de limites X et Y respectivement, et soit F une fonction multivoque compacte s.c.s. et acyclique de X dans Y. Supposons les projections pa surjectives. Nous pouvons alors, pour tout a £ A, definir une fonction multivoque compacte Fa : Xa —> Ya par la formule
Fa(x) = qa(F(p-1(x))).
Points fixes des fonctions multivoques
75
Etant composee des fonctions s.c.s. qa, F et p " 1 , Fa est s.c.s.. Pour ce qui est de son acyclicite, nous avons le resultat suivant: Lemme 3. L'ensemble B des a G A tels que Fa soit acyclique est cofinal et ferine dans A. Demonstration. Soit M un sous-ensemble totalement ordonne de A admettant une borne superieure fi. Pour a < j3, nous avons p'^1(x) C Pal{Pa(x))' d'ou Qa(F/3(x)) ^ Fa(Pa(x)) P o u r tout x G Xp. Par consequent, pour tout x G X^, nous avons un systeme projectif (FQ(p£(ar)),g£\F0(p^{x)),M) et q^F^x)) C Fa(p£{x)) pour tout a G M. Affirmation 1. Pour tout x G XM, les fonctions q^F^x) : F)1(x) —> F a (p^(x)) representent F^(x) comme limite du systeme projectif (Fa(p£(x)),q%\Fp(pp(x)),M). En effet, d'apres (b), la limite de ce systeme projectif est un sous-ensemble de Yp. Puisque q£(F^(x)) C Fa(p£(x)) pour tout a G M, FM(x) est contenu dans cette limite. Si y G 1^ n'appartient pas a ^(a;), il y a, d'apres (b), un a G M tel que 1a(y) 4- 1a(Fn(x))- Puisque F^ est s.c.s., l'ensemble V des z G XM tels que F^(z) C ^M \ (ia)~1 (ia(y)) e s t u n voisinage de x. II existe done (3 £ M avec cc < /3 et un voisinage W de p£(z) dans Xp tels que (p^)" 1 !^) C F. Alors ( p ^ ) " 1 ^ ^ ^ ) ) C F , d'ou
Fetyix)) = q0(F(p/(p$(x)))) = q0{F{p-\{P^)-\P^x))))) C q0{F{p-\V))) = $q»(F(p-\V))) = q^F^V)) C q^ \ (qZrHqtty))) C Yp \ (gf)" 1 ^^)), ce qui entraine que g^(y) n'appaxtient pas a Fp(p^(x)) puisqu'il est contenu dans (
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Robert Cauty
tif (Fai(p^i(x)),qa3i\Fa:j(p".(x))>^o) et le choix des a; garantit que les fonctions +1 x q"l \Fai+1(Pai+1( )) de ce systeme induisent des homomorphismes triviaux en cohomologie de Cech. La continuite de la cohomologie de Cech entraine alors que Hn(Fa(x), Q) = 0 pour tout n > 0 et tout x € Xa, done a appartient a B. Pour simplifier les notations dans la demonstration de l'affirmation 2, nous ferons les conventions suivantes. Pour j3 < 7 dans A, K C Yp et e G Hn(K, Q), nous notons (^)- 1 (e)(resp.^ 1 (e))l'imagedeedansff' l ((g^)- 1 (^),Q)(resp.jy™(g^ 1 (^),Q)) par rhomomorphisme induit par la fonction de K dans {q^)~l{K) (resp. q^l(K)) induite par gl (resp. qp). Pour L C K, nous noterons e|L l'image de e dans Hn(L, Q) par rhomomorphisme induit par l'inclusion de L dans K. Fixons une base denombrable O = {Oi}^Z1 de la topologie de Yao stable par reunion finie. Pour i > 1, soit Ui = {x G Xao \ Fao(x) C O,}. Puisque FQ,0 est s.c.s., Ui est ouvert, done est cr-compact puisque le compact Xao est metrisable. Soit Ui = Uj*Li Kli o u ^ / es * compact. Pour tout compact metrisable Z, Hn(Z, Q) est denombrable pour tout n > 0, done nous pouvons trouver une partition N = Ufci -^i de Pensemble des entiers et, pour tout i, une surjection k 1—> e^ de ATj sur
Ur=o^n(^,Q)Soit (i,j,k) un triplet d'entiers tel que k appartienne a Ni, et soit n tel que efc s Hn(Oi,Q). Nous allons montrer qu'il existe /? = f3(i,j,k) > 0.$ tel que, pour tout x € (Pao)~1(-ft'i'), (9ao)~1(efc)l^/3(x) = ^- Pour cela, remarquons d'abord que l'argument utilise pour prouver l'affirmation 1 montre aussi que, pour tout x G X, Fix) est la limite du systeme projectif (Fa(pa(x)),qP\Fp(pp(x)),A). Soit x € Pao(K-i); nous avons done Fao(pao(x)) C Oi- Puisque F{x) est acyclique, la continuite de la cohomologie de Cech entraine l'existence d'un (3X > ao tel que (
(1)
Les ouverts p~p~l(Wx) recouvrent le compact p^{Kl), done il existe Xi,... ,xs tels que p^(K{) C U ' = I Pjlr (w*r)- Fixons /? = /3(z,j, fc) tel que (3 > /3Xr pour 1 < r < s. Soit x € (PQ O )~ 1 (-?^/)- II existe x' £ X tel que pp(x') = x et 1 < r < s tel que i ' e P^ p (Wx P ). Alors p ^ J x ) = ppxr(x') e Wxr et ^ ^ ( ^ ( x ) ) C i ^ r ( * & > ) ) , d'ou, d'apres (1),
Puisque A est filtrant, la condition (a) entraine l'existence d'un a\ € A tel que /3(*>j\k) < Qi pour tout triplet d'indices (i,j,k) tel que k € TV;. Soit x G X a i et soit e G iJ ra (FQ, o (p"j(x)),Q). Puisque C est stable par reunion finie, tout voisinage de Fao(p%i(x)) dans Yao contient la fermeture d'un Ot contenant Fao(p2l(x)). La continuite de la cohomologie de Cech entraine done l'existence d'un i tel que Oi contienne -FQo(p™j(x)) et d'un element e' G Hn(O~,Q) tel que e = e'|F Qo (p"j(x)).
Points fixes des fonctions multivoques
77
II existe j tel que p"l(x) £ K\ et un k 6 AT* tel que e' = e^. L'image de e dans /f™(FQ1(a;),Q) par Fhomomorphisme induit par q^l\Fai{x)) est done egale a ( C ) " 1 ^ ) ! ^ ! ^ ) - S o i t 0 = ^(*.J. fc )- N o u s a v o n s Qo < P < «i et ^ ( F Q l ( z ) ) C ^(^(x)),d'ou = (^1)-1(0)|JFai(x)=0, et TafErmation 2 en resulte. Pour a < P et n > 1, nous notons p^n (resp. pa,n) l e prolongement naturel de p^ (resp. pQ) a Un(Xp) (resp. !7n(X)) ( p ^ = pf et p Q]1 = p Q ). Pour m < n, nous avons pf,m = p^jE/mpi^) (resp. p O i m = p Q , n |£/ m (A»). Puisque le foncteur Un commute aux limites projectives et preserve la surjectivite des fonctions, (Un(Xa),p^n,A) est un w-systeme projectif de limite Un(X) et les projections p QiK sont surjectives si les pa le sont. Soit F une fonction multivoque compacte s.c.s. de U(X) dans Y. Supposons les projections pa surjectives. Alors, pour a £ A et n > 1, la formule
FS{x) = qa(F(p-jn(x))) definit une fonction multivoque compacte s.c.s. de Un(Xa) dans Ya. Notant Uo(Xa) = 0, nous definissons alors une fonction multivoque Ga de U(Xa) dans Ya en posant
Ga{x) = F£(x)
si x G Un(Xa) \ Un-i{Xa), n > 1.
Lemme 4. L'ensemble des a & A tels que G a soit s.c.s. est cofinal dans A. Demonstration. Etant donne ao £ A, nous allons construire une suite croissante {a n }^L 0 d'elements de A et, pour tout n > 1, une base denombrable £>n = {-B^jga de Yan stable par reunion finie, de fagon que la condition suivante soit verifiee:
(*) Pour tout m
Um(Xan)\Um-i{Xan)
et tout i > 1, si Garl(paZ*n (x)) C SJj, alors il existe un voisinage V de x dans ^n(* Q n + 1 ) tel que qZ+1 (F^+l(y)) C Sj, pour tout yeV. Puisque Uo(XaQ) = 0, nous pouvons prendre a.\ = «o et pour Si n'importe quelle base denombrable stable par reunion finie de Yai. Soit n > 1 et supposons an et 23n construits. Pour l < m < n e t i > l , soit W(m,i) = {x G t/ m (X a n ) \ !7 m _i(X Qn )|G Qn (x) C Bln}. Puisque G Q n |U m {X a n )\U m -i{X a n ) = F™n\Um{Xan)\ Um-i(Xan) est s.c.s., W(m,i) est ouvert dans Um(Xan) \ Um-i(Xarl), done est acompact. Soit W(m,i) = U j l i K3m t, ou les K3m i sont compacts. Soit Oi = {x G C/n(X) | gari(.F(x)) c -B^}. Puisque F est s.c.s., Oi est ouvert dans Un(X). Puisque G a . ( i ) = -F™ (x) pour x G Um(XaJ \ Um-i(XaJ, la definition de F™n entraine que le compact p~^ niK^ t) \ Oi est disjoint de Um(X), done il existe (3 = f3(m, i,j) > a tel que
PsAPalJK^i)
\ Oi) n um{x0) = 0.
(2)
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Robert Cauty
La condition (a) entraine l'existence d'un an+\ G A tel que an+\ > /3(m,i,j) quels que soient m, % et j . Soient m < n et x G Um(Xan+1) \ Um-i(Xan+l) tel que pa: + 1 (x) G [ / m ( X t t J \ Um-i(Xari). Si G Qn (p£;#(a:)) C #i, il existe j tel que PaZ~tn{x) € K3mi. Soit /3 = P(m,i,j). Puisque x appartient a Um(Xan+1), P^ {x) appartient a Um(Xg) et (2) entraine P£n(x)
c P}l{{pin,nr\Kltl)
n Um(X0)) c Ot.
II existe done un voisinage V de pa^x (x) dans Un(Xp) tel que p^^(V) C Oi- Pour 2/ € ( P ^ 1 ) " 1 ^ ) -
nous
avons
c gan(F(p^n(V))) c (fcJFfOO) c B ; , done la condition (*) est verifiee. Prenons pour Bn+i n'importe quelle base denombrable de Yan+1 stable par reunion finie. Pour prouver le lemme, il suffit, puisque «o etait arbitraire, de montrer que si a est la borne superieure de la suite {an}^L0, alors Ga est s.c.s. et, comme U(Xa) est la limite inductive de la suite croissante de compacts {Uk(Xa)}, il suffit pour cela de montrer que Ga\Uk(Xa) est s.c.s. pour tout k > 1. Fixons un entier k > 1, et soit x £ Uk(Xa). Soit m < k tel que x G Um(Xa) \ Um-i(Xa). Puisque Um-i(Xa) est ferme dans Uk{Xa), (b) entraine l'existence d'un n 0 > k tel que p^no,k(x) e Um(Xano) \ Um-i(Xano). Alors, pour n0 < n, nous avons ft^x) G Um(XaJ \ Um-!{XaJ, done G Qn (p2 nifc (x)) = ^ ( a : ) et G a ( i ) = F^*(a;). L'affirmation 1 s'applique a la fonction F™ et montre que Ga(x) est la limite du systeme projectif (G Qn (p^ n fe(x)),3°;|GQr{p^>A.(x)),n > n 0 ), done si M est un voisinage de Ga(x) dans Ya, il existe n > no et un voisinage N de G an (p2 n , fc (^)) dans Yan tel que GQ(x) C (q"n,k)~H^) C M. Puisque la base S n de Y"arl est stable par reunion finie, il existe i tel que G Qn (p^ k(x)) ^ ^n ^ -^rPuisque m < k < n et que P^ n + 1 ^(a;) appartient a Um(Xan+1), il existe d'apres (*) un voisinage V de p^n+uk(x) dans C/ n (^a n+1 ) tel que gS" +1 (^« n+1 (y)) C -B^ pour tout y dans V. Alors (p° fc)^1(^) ^ Uk(Xa) est un voisinage de x dans C/fc(XQ) et si y appartient a ce voisinage, alors
Ga(y) c F2{y) c ( ^ J - 1 ^ ^ ^ ^ , * ^ ) ) ) . d'ou
&n(Ga(y)) = C + 1 °C +1 (Ga(y)) c C+1(^n+1(PaB+1,it(y))) c B\ puisque p^n
l k
G V. Par consequent
Ga(y) c ( C ) " 1 ^ ) c (gSJ-1 W c M, ce qui montre que Ga\Uk{Xa)
est bien s.c.s. et acheve de prouver le lemme.
Points fixes des fonctions multivoques
79
4. Le cas general Soit X un compact, et soit F : U(X) —* X une fonction multivoque compacte s.c.s. et acyclique. Representons X comme limite d'un w-systeme projectif (Xa,p^,A) de compacts tels que les projections pa soient surjectives. Alors Un(X) est la limite de 1'w-systeme projectif (Un(X),p^n,A) et, pour a £ A, nous definissons une fonction multivoque compacte s.c.s. .F™ : Un(Xa) —> Xa par FZ(x)=pa(F(p^n(x))), et une fonction multivoque compacte Ga : U(Xa) —+ Xa par Ga(x) = F%{x) si x G J7n(Xa) \ t/ n _i(X a ), n > 1. Le lemme 3 entraine que l'ensemble An des a E A tels que F£ soit acyclique est cofinal et ferme dans A. D'apres la proposition 3.1.1 de [6], Ax = H^Li ^n est cofinal et ferme dans A. D'apres le lemme 4, l'ensemble B des a € Ax tels que G a soit s.c.s. est cofinal dans Ax, done dans A. Si a; S £?, alors GQ est une fonction multivoque compacte s.c.s. et acyclique de /7(XQ) dans Xa. Puisque Xa est metrisable, l'ensemble Pa des points fixes de Ga est non vide pour tout a G B et, comme Ga est s.c.s., P a est ferme dans U(Xa). Evidemment, Pa est contenu dans Xa. Soient a < /3 dans B et x S P/3. Puisque x appartient a JC^, nous avons Gp{x) = F^(x) done, puique p0al = pPa et paA = pa, Ga(p0a(x)) =FlM{x)) =
=pa{F{p-l^a{x)))^pa{F{p-0\x)))
P0aP0(F(pe1(x)))=pe(G0(x))BpP(x),
ce qui montre que p^(P^) C Pa. Nous obtenons done un systeme projectif de compacts (Pa,p^\P/3,B). Comme ces compacts sont non vides, leur limite P n'est pas vide, et est contenue dans la limite du systeme projectif {Xa,p^,B), qui est egale a X puisque B est cofinal dans A. Si y appartient a P, alors, en raisonnant comme dans la demonstration de l'affirmation 1, on constate que F(y) est la limite du systeme projectif {F^(pa{y)),p^\F^(pp(y)),B), et comme pa(y) appartient a Fa(Pa(y)) = Ga(pa(y)) pour tout a € B, nous avons y 6 F(y), done y est un point fixe de F et la proposition est prouvee. References 1. R. Cauty, Solution du probleme de point fixe de Schauder, Fund. Math. 170 (2001) 231-246. 2. R. Cauty, Le probleme de Schauder; correction et complement, Prepublication. 3. R. Cauty, Le theoreme de point fixe de Lefschetz-Hopf pour les compacts ULC, Prepublication. 4. S. Eilenberg and D. Montgomery, Fixed point theorems for multivalued transformations, Amer. J. Math. 68 (1946) 214-222.
80
Robert Cauty
5. S. Eilenberg and N. Steenrod, Foundations of algebraic topology. Princeton University Press, Princeton, 1952. 6. V.V. Fedorchuk et A. Chigogidze, Retractes absolus et varietes de dimension infinie. Nauka, Moscou, 1992 (en Russe). 7. E.H. Spanier, Algebraic topology. Me Graw Hill, New York, 1996.
Functional Analysis and its Applications V. Kadets and W. Zelazko © 2004 Elsevier B.V. All rights reserved
81
Almost Periodic Mappings to Complex Manifolds Sergej Favorov and Natalia Parfyonova Karazin Kharkiv National University, Department of Mechanics and Mathematics, Kharkiv, Ukraine Key words: Almost periodic holomorphic mappings, meromorphic functions 2000 MSC: 32A20 A continuous mapping F of a tube TK = {z = x + iy : x £ Rm, y G K C ]Rm} to a metric space X is almost periodic if the family {F(z + i)}tgRm of shifts along Mm is a relatively compact set with respect to the topology of the uniform convergence
onTK. Further, let X be a complex manifold, and F be a holomorphic mapping of a tube TQ = {z = x + iy : x e Mm, y e 0 } , with the convex open base fl C Mm, to X. We will say that F is almost periodic if the restriction of i71 to each tube TK, with the compact base K C O, is almost periodic. For X = C we obtain the well-known class of holomorphic almost periodic functions; for X = Cq the corresponding class was being studied in [3], [7], [8]; for X = CP, we get the class of meromorphic almost periodic functions that was being studied in [4], [10], [5]; the class of holomorphic almost periodic curves, corresponding to the case X = CP 9 , was being studied in [6]. The following theorem is well known: Theorem B (H. Bohr [2]). If a holomorphic bounded function on a strip is almost periodic on some straight line in this strip, then this function is almost periodic on the whole strip. This theorem was extended to holomorphic functions on a tube domain in [11]; besides usual uniform metric, various integral metric were being studied there. The direct generalization of Theorem B to complex manifold is not valid: Email address: [email protected] (Natalia Parfyonova).
82
Sergej Favorov, Natalia Parfyonova
Example. Let f(z) be the quotient of two periodic functions sin y/2z and sin z. It is clear that the restriction of f(z) to any straight line {z = x + iyo : x G R}, yo ^ 0, is almost periodic on this line. Besides, f(z) is bounded as a mapping to compact manifold CP. Nevertheless, zeros and poles of f(z) are not separated on the axis z = x e l , therefore f(z) is not almost periodic on any substrip containing the real axis ( see [4]). In order to give the right version of Theorem B, we need the following proposition. Proposition. If K is compact subset ofM.m, then an almost periodic mapping F of TK to a metric space X is uniformly continuous and F(TK) is a relatively compact subset of X.
Proof. Let
teRm.
It is easy to prove that ip(t) is an almost periodic function on R m , therefore the function
for each t,t' € UnW . Using the obvious inequality V{t-t)<\
+
t))<e.
Therefore the function F(T,
y) =
lim x—>T,
F(x + iy)
xGM™
is well-defined and continuously maps the compact set B x K to X. Since F(x, y) = F(x + iy) for x € M.m, we obtain all the statements of our proposition. Note that a bounded holomorphic function on a tube domain is uniformly continuous on every subtube with the compact base, but bounded holomorphic mappings, in general, have not this property. It motivates the following result is natural. Theorem. Let F be a holomorphic mapping of TQ to a complex manifold X such that for every compact subset K C il the mapping F is uniformly continuous on TK and F(TK) is a relatively compact subset of X. If the restriction of F(z) to some hyperplane Rm +iy' is almost periodic, then F(z) is an almost periodic mapping of Tn to X. Corollary. Let F be a holomorphic mapping form TQ to a compact complex manifold X such that F is uniformly continuous on TK for every compact set K C f2. If
Almost Periodic Mappings to Complex Manifolds
83
the restriction of F(z) to some hyperplane R m + iy' is almost periodic, then F(z) is an almost periodic mapping ofTn to X. Proof the Theorem. Take an arbitrary sequence {£„} C R m . Since the function F(z) is uniformly continuous, the family {F(z + tn} is equicontinuous on each compact set S C Tn. Further, it follows from the condition of the Theorem that the union of all the images of S under mappings of this family is contained compact subset of X. Therefore, passing on to a subsequence if necessary, we may assume that the sequence {F(z + tn)} converges to a holomorphic mapping G(z) uniformly on every compact subset of TQ. It easy to see that the mapping G(z) is bounded and uniformly continuous on every tube TK with the compact base K C ft. Let us prove that this convergence is uniform on every TK • Assume the contrary. Then we get d(F(zn+tn),G{zn))>eo>0
(1)
for some sequence zn = xn + iyn € TK1, where K' is some compact subset of f2. Replacing sequence by a subsequence if necessary, we may assume that the mappings G(xn + z) converge to a holomorphic mapping H(z), and the mappings F(z+xn+tn) converge to a holomorphic mapping H(z) uniformly on every compact subsets of Tfi. We may also assume that yn —> yo £ K' • Using (1) we get \H(iyo)-H(iyo))\>eo. Since the mapping F(x + iyl) of R m to X is almost periodic, we may assume that a subsequence of the mappings F{x + tn + iy') converges to G(x + iy') uniformly in x £ R m . Therefore the sequences of mappings F(x+xn+tn+iy') and G(x+xn+iy') have the same limit, i. e., H{x + iy') = H(x + iy') for all i e R m . Since H(z), H(z) are holomorphic mappings, we get H(x+iy') = H(x+iy') on TQ. This contradiction proves the Theorem. References 1. Ch. Berg, Introduction to the almost periodic functions of Bohr, Proceedings of a symposium held in Copenhagen, April 24-25 (1987), 15-24. 2. H. Bohr, Ueber analytische fastperiodische Funktionen, Math. Ann. 103 (1930) 1-14. 3. S.Ju. Favorov, A.Ju. Rashkovskii, L.I. Ronkin, Almost periodic divisors in a strip, Journal D'analyse Mathematique 74 (1998) 325-345. 4. N.D. Parfyonova, S.Yu. Favorov, Meromorphic almost periodic functions, Mathematychni Studii 13 (2000) 190-198. 5. N.D. Parfyonova, Meromorphic almost periodic functions and their continuous extension on the Bohr's compact, Vestnik Kharkovskogo Universiteta 542 (2002) 73-84. (In Russian). 6. N.D. Parfyonova, Holomorphic almost periodic mappings into complex manifolds, Mat. Fiz. Anal. Geom. 9 (2002) 294-305. (In Russian).
84
Sergej Favorov, Natalia Parfyonova
7. A.Yu. Rashkovskii, Monge-Ampere operators and Jessen functions of holomorphic almost periodic mappings. Mat. Fiz. Anal. Geom. 5 (1998) 274296. 8. A.Yu. Rashkovskii, Flows associated with holomorphic almost periodic functions, Mat. Fiz. Anal. Geom. 2 (2) (1995) 150-169. 9. L.I. Ronkin, Jessens' theorems for holomorphic almost periodic functions in tube domains, Sib. Math. J. 28 (3) (1987) 199-204. (In Russian). 10. F. Sunyer i Balaguer, Una nova generalitzacio de les functions gairebeperiodiques, Inst.d'Estudis Catalans, Arxius de la seccio de ciencies XVII, 1949, 3-46. 11. O.I. Udodova, Holomorphic almost periodic functions in tube donains,. Vestnik Kharkovskogo Universiteta 542 (2002) 96-105.
Functional Analysis and its Applications V. Kadets and W. Zelazko © 2004 Elsevier B.V. All rights reserved
85
Some new differential equations of the first-order in the spaces M(l,3) x R(u) and M(l,4) x R(u) with given symmetry groups Vasyl Fedorchuk a and Volodymyr Fedorchuk b a
Pedagogical Academy, Institute of Mathematics, 2 Podchorazych Street, 30-084, Krakow, Poland; Pidstryhach Institute of Applied Problems of Mechanics and Mathematics of NAS of Ukraine, 3b Naukova Street, 79-601, Lviv, Ukraine; b Ivan Franko Lviv National University, 1 Universytetska Street, Lviv, 79000, Ukraine
Abstract We present some new first-order differential equations invariant under continuous subgroups of the generalized Poincare group P(l,4) and defined in the spaces M(l,3)xR{u) and Af(l,4) x i?(u). Key words: Lie groups, Lie algebras, subgroup structure, differential invariants, differential equations 2000 MSC: 58J70, 35A30, 59D19
1. Introduction The mathematical modeling of various natural processes very often requires that some symmetry properties of the processes considered be taken into account. This leads to mathematical models with non-trivial symmetry groups. In many cases this type of models can be expressed in the form of (linear or nonlinear) differential equations with non-trivial symmetry properties in the spaces of different dimensions. It is well known that among equations, important for theoretical and mathematical physics, there are also ones which have nontrivial symmetry groups. For example, in the space M ( l , 3) x R(u) we have the Eikonal equation, the Euler-Lagrange-
86
Vasyl Fedorchuk, Volodymyr Fedorchuk
Born-Infeld equation and homogeneous and inhomogeneous Monge-Ampere equations. In the space M(l,4) x R(u) we have the linear and nonlinear wave equations and Dirac equation. Here, and in what follows, R(u) is the number axis of the dependent variable u. These equations are invariant under the generalized Poincare group P(l,4) (see, for example, [7, 11-16]). The group P(l,4) is the group of rotations and translations of the five-dimensional Minkowski space M(l, 4). This group has many applications in theoretical and mathematical physics [7, 11, 16]. The group P(l,4) has many subgroups used in theoretical physics [3-6, 9]. Among these subgroups there are the Poincare group P(l,3) and the extended Galilei group G(l,3) (see also [10]). Thus, the results obtained with the help of the subgroup structure of the group P ( l , 4) will be useful in relativistic and nonrelativistic physics. Therefore, it is important from the physical and mathematical points of view that we are able to construct, in the spaces M(l,3) x R(u) and M(l, 4) x R(u), new differential equations invariant under continuous subgroups of the generalized Poincare group P(l,4). The papers [1,2] are devoted to the construction of the first-order differential equations invariant under splitting subgroups of the group P(l,4), defined in the spaces M(l,3) x R(u) and M(l,4) x R(u). In the present paper we continue to study this type of equations. We concentrate our attention on the first-order differential equations invariant under continuous subgroups of the group P(l,4), defined in the spaces M(l,3)xR(u) and M ( l , 4 ) x R(u). We give the number of all first-order differential equations of a certain form (in these spaces) which are invariant under splitting subgroups of the group P ( l , 4) as well as some new obtained equations. Recently, we have constructed the first-order differential equations (in the spaces M(l,3) x R(u) and M(l,4) x R(u) ) which are invariant under non-splitting subgroups of the group P(l,4) for the majority of these subgroups. Our paper is organized as follows. In the first section we introduce some notation and results concerning the Lie algebra of the group P(l,4) which we use in the following. Sections 3 and 4 present our main results.
2. The Lie algebra of the group P ( l , 4) and its non-conjugate subalgebras The Lie algebra of the group P(l,4) is given by the 15 basis elements M^v = -Mvii (fj,,v = 0,1,2,3,4) and P^ (fj, = 0,1,2,3,4), which satisfy the commutation relations
[/*, P'v] = 0,
[Mlv, Pi] = g^P'v -
9vaPl,
[ M ^ , M'pa] = gpPM'va + gvaM'w - g^M'^
-
g^M'vp,
Some new differential equations with given symmetry groups
87
where g00 = - 0 n = -322 = -333 = ~344 = 1, g^ = 0, if fj, ^ v. Here, and in what follows, M'^ = iM^v. Below, we will use the following basis elements: G = M'i0,
Li = A^2)
Pa = M'Aa~M'a0, X0 = \(P^-Pi),
L2 = -M'3l,
Ca = M'ia + M^0,
Xk = P'k
(k= 1,2,3),
L3 = M21, (a = 1,2,3), XA = \ ( i * + Pi).
For the study of the subgroup structure of the group P(l, 4) we used the method proposed in [20]. Continuous subgroups of the group P(l,4) have been described in [3-6, 9]. From the results obtained (see also [10]) it follows, in particular, that the Lie algebra of the group P(l,4) contains as subalgebras the Lie algebra of the Poincare group P(l,3) and the Lie algebra of the extended Galilei group G(l,3).
3. The first-order differential equations in the space iW(l,3) X R(u) The group P(l, 4) acts on M(l, 3) x R(u) (i.e. on the Cartesian product of the four-dimensional Minkowski space (of the independent variables xo,xi,X2,X3) and the number axis of the dependent variable u). The group P(l,4) usually acts on M(l, 3) x R(u) as a group generated by translations and rotations of this space. Let X=
^i(x,u)—+r,{x,u)i=0
be one of the basis infinitesimal operators. The first prolongation of X has the form
where w» = ^ , i = 0,1,2,3. Now, a function J{x,u^) is a first-order differential invariant if X (1) - J(x,w(1)) = 0. Here u^ = (U,UQ,UI, «2,«3) is an element of the first prolongation R(u)^\ The results obtained in [12-14] enable us to use the subgroup structure [3-6, 9] of the generalized Poincare group P(l,4) in order to construct the first-order differential equations invariant under continuous subgroups of the group P(l,4), defined in the space M(l,3) x R(u). Let us consider the following representation of the Lie algebra of the group P(l,4):
88
Vasyl Fedorchuk, Volodymyr Fedorchuk
P'-A P i=
'
P'--A-
P'--A-
~~L' M'lu/ = -(xllP'u-xl/P'll),x4
P'--A-
= u.
More details about this representation can be found in [12-15]. The considered equations can be written in the following form (see, for example [17-19,21]): F(J1,J2,...,Jt) = 0, (1) where F is an arbitrary smooth function of its arguments, {Ji, J2,..., Jt] is a functional basis of the first-order differential invariants of continuous subgroups of the group P ( l , 4 ) . In the construction of the differential equations with non-trivial symmetry groups it has turned out that different non-conjugate subalgebras can have the same functional basis of the first-order differential invariants. Consequently, there is no oneto-one correspondence between non-conjugate subalgebras of the Lie algebra of the group P(l,4) and corresponding differential equations. Definition 1. We call two subalgebras L1 and L2 of the Lie algebra of the group P(l, 4) equivalent if they have the same functional basis of the first-order differential invariants. It is possible to prove that the relation of equivalence of subalgebras L1 and I? given by Definition 1 is the set-theoretical equivalence relation. With respect to this equivalence relation, all non-conjugate subalgebras of the Lie algebra of the group P ( l , 4 ) split into classes of equivalent subalgebras. Each two different classes have different functional bases of the first-order differential invariants. Definition 2. We call two classes of the first-order differential equations of the form (1) equivalent if functional bases corresponding to them belong to the equivalent subalgebras. First, we give the results obtained with the help of the splitting subgroups of the group P(l,4). One of the results in this section can be formulated as follows. Proposition 1. In the space M ( l , 3) x R(u), there exist 242 non-equivalent classes of the first-order differential equations of the form (1) which are invariant under the splitting subgroups of the group P(l,4). This proposition has been proved with use of: - the list of the splitting subalgebras of the Lie algebra of the group P(l,4) [8]; - the general ranks of the matrices which contain coordinates of the basis elements of the subalgebras of the considered Lie algebra; - theorem on the number of invariants of the Lie group of point transformations (see, for example, [18, 19]).
Some new differential equations with given symmetry groups
89
The differential first-order equations in the space M(l,3) x R(u) which are invariant under splitting subgroups of the group P(l,4) are constructed. Some of the results obtained have been presented in [ 2 ]. Since we cannot present all the results obtained here, in this section we only give some of the new results which cannot be found in [ 2 ]. Below, for some splitting subgroups of the group P ( l , 4), we write the basis elements of its Lie algebras and corresponding arguments J i , J2,..., Jt of the function F. 1.
J2=x2,
J
6 = ^ , J7 = ^ , 2. (G, P3), Jl=XU
J2=X2,
J4 = (xl-u2)l/2,
h=x3, J
8 = ;^r±i,
J5 =
(xo+u)2^j,
uM = ^ , /i = 0, 1, 2, 3;
J3 = (xg - x\ - M2)1/2,
Ji=^^Ui,
3. (G, L3, X4>, J1=X3,
J 2 = (X2+X2)V2,
J 3=
f t S f
^ ,
J 4=
( x o + U
)(^,
4. (G, P ^ , X 4 ), Jl=X3, T _
^2 = f^fW3,
u%-u\-u\-\
J 3 = X 1 + ^±f« 1 ,
J4=a.2
+
2a±HU2)
.
5. {L3 + 6G, P l 5 P2, P3, Xu X2, Xi, 6 > 0 ) , ^1 = x 3 + ^ « 3 , J2 = («§ - «? - « | - u§ - l) ( ^ ± f ) 2 ; 6. (G, P l 5 P 2 ) P 3 ) X i , X2, X3, X4),
J^iul-ul-ul-ul-l)^)2 ; 7. (Li, L 2 , L 3 , P i , P 2 , P 3 , X i , X 2 , X 3 , X 4 ), Jl = a;o+ M,
j 2= "i + ^;t?i" 0 + 1 ) ;
8. (G, L i , L2; L%, Pi, P2, P3, X\, X2, X3, X4),
Jx = {ul-ul-ul-ul-l){^)2
.
Now, we present results obtained with the help of the non-splitting subgroups of the group P ( l , 4 ) . We have constructed classes of the first-order differential equations (in the space M(l,3) x R(u) ) which are invariant under non-splitting subgroups of the group P(l, 4) for the majority of these subgroups. These classes of equations can be written in the form (1), where {J\, J2,..., Jt} is a functional basis of the first-order
90
Vasyl Fedorchuk, Volodymyr Fedorchuk
differential invariants of the non-splitting subgroups of the group P ( l , 4 ) . Here, we only write some of the new results obtained. Below, for some non-splitting subgroups of the group P ( l , 4), we give the basis elements of their respective Lie algebras and corresponding arguments J\, J2,..., Jt of the function F. 1. (L3 - XA, P3), J2 = {x\ + xl)1/2,
Ji=xo+u, T J i
X3 ~
1
XQ+U
U3
" " " Uo + 1 '
T 5
J3 = x\ - x\ - u2 + (XQ + u) arctan ^ ,
X1V.2—X2U1 ~
^7 = ^ +^ , «^^ 2. {G + a3X3, Pu P2, a 3 < 0 ) , «^i = ^3 — c-3 l n ( x 0 + u),
J5 = x2 + (x0 + w)^tr,
J __ U1+U2 6
Iltll+I2tl2'
)
~ ~ (uo + 1 ) 2 '
/ x = 0,l,2)3; — W2)1/2,
J 2 = (XQ —X\—X\
^=
^
3
;
3. (G + a3X3, L3, Pi, P2, a 3 < 0 ) ,
J^Cxg-xf-xl-ti2)1^,
J2= ( x o + W ) - ^ T , / \2 / \2 J3 = x3 - a3 ln(a;o + u), J4 = [Xi + f^y«iJ + ^2 + ^ f i ^ J ,
J5 = "3-y- 1 ;
4. (L 3 , P x + X 2 , p 2 - X L P 3 + /i 3 X 3 , X4>, Ji=x o + u,
J2=x3 + (x0 + u ) ^
I
- ^ ,
Jz = (xi + ^ x + ^ f « i ) 2 + (x2 - - ^ + ^ ± f « 2 ) 2 , T _ u2,+ul+ul+2(u0 + l) . ~ («o + l) 2 ' 5. (G + aX3, L3, Plt P2, P3, X4, a<0), J4
J1 = (.0+ ,) 2 ("i + t + 0 ^"° + 2 -l) ; J2=(xi
+ ^ui)2+(x2
+^ u
2
) \
Jz = x3 - aln(x0 + u) + (x0 + M ) ^ J ; 6. (G + aX3, Pu P 2 , P 3 , Jd, X2, X4, a < 0), Ji = aln(x o +w) - (a;o + w ) ^ T -a; 3 ,
J2 = ( M 2 - U 2 - U l - u 2 - l ) g ^ ; 7. (Li + i(P! + Ci), L2 + \{P2+ C2), L3 + i(P 3 + C3),
Some new differential equations with given symmetry groups Li -\(P* T J
l
+ C3) + a{X0 + X4), Xlt
91
X2, X3, Xo - X4, b< 0),
_ ul+ul+ul + l -
<
•
4. The first-order differential equations in the space JVf(l,4) X R(u) In this section we present some of the new results concerning the first-order differential equations in the space M(l,4) x R(u). The group P(l,4) acts on M(l,4) x R(u) (i.e. on the Cartesian product of the five-dimensional Minkowski space (of the independent variables xo,X\,X2,X3,X4) and the number axis of the dependent variable u). The group P(l, 4) usually acts on M(l, 4) as a group generated by translations and rotations of this space, and it acts trivially on R(u) in this specific case. Let i=o ° l be one of the basis infinitesimal operators. It generates the action
gt(x,u(x)) = (gtx,u(x)) = (y,u(g-ty)), where gt — exptX G P(l,4), x G M(l,4), y = gtx. From this, one obtains the first prolongation of X in the form
i = 0
Now, a function J(x,u^)
ux
j=0
ua
i
U L
t
- J
is a first-order differential invariant if J ( X , M ( 1 ) ) = 0.
X^-
Here u^ = (U,UQ,U\, 112,113,114) is an element of the first prolongation R(u)(lh Let us consider the following representation of the Lie algebra of the group P(l,4): P'-
d
P>-
OX0
P' —
d
9
P>-
OXi
M'
—
P'-
OX2
(v
P'
T
9
OX3
P'\
The equations in the space M(l, 4) x R(u) which are invariant under continuous subgroups of the group P(l,4) can also be written in the form (1). First, we also give the results which are based on splitting subgroups of the group P(l,4). One of the results obtained can be formulated as follows.
92
Vasyl Fedorchuk, Volodymyr Fedorchuk
Proposition 2. In the space M(l,4) x R(u), there exist 243 non-equivalent firstorder differential equations of the form (1) which are invariant under the splitting subgroups of the group P ( l , 4 ) . The proof of Proposition 2 has been obtained in analogous manner as the proof of Proposition 1. The first-order differential equations in the space M(l,4) x R(u) which are invariant under splitting subgroups of the group P(l,4) are constructed. Some of the results obtained have been presented in [1]. In this section we only give some of the new results which cannot be found in Below, for some splitting subgroups of the group -P(l, 4), we also write the basis elements of their respective Lie algebras and corresponding arguments Ji, J2,..., Jt of the function F. 1. (P3 + C3 + 2L3), Ji=x0, J5 = u,
Ji = X1X4 - 3:22:3, Je = x\u
J 8 = «o, JQ = U\+ 2. (L3, X 0 + X 4 ) ,
V%,
h = {x\ + x | ) 1 / 2 ,
J4 =
(xl+xl)1/2,
Jt = £31*4 — X4U3,
JIO
= u\ + u\,
Ji=x3,
J2 = x4,
J3-{x\-\-xl)l/2,
J6 = M0,
h = «3,
^8 = "4,
uM = ^ - , n = 0, 1, 2, 3, 4; J4-u,
JQ = U\+UI
J5 = xiu2 - x2ui,
;
3- (G, L3, Xt), J2 = ( x ? + x | ) 1 / 2 ,
^1=^3,
J5 = (xo + x^iuo+u^), 4. ( L i , I/2, L3,
XQ
J3=w,
J6 = u3;
J 4 = X1U1 + X2U2 + X3M3, 5. (G, L 3 ) P i , P 2 ) X 4 ) ,
J1=X3,
J7 = ul-u\i
-x2ui, J% = u\ + u\;
— X4),
J2 = (xj +x\+ xl)1/2,
Ji = x0,
J 4 = xiu2
J2=M,
J 3 = u,
J 5 = M0,
J& = «4,
J7 = M2 + M | + M§ ;
J3 = f^ft,
• / 4 = ( ^ l + S ^ « l ) 2 + (x2 + f ^ W 2 ) 2 ,
J5=«3,
2
J6 = M§ - M - u\ - u\ ; 6. (G, P3) L3) X 1; X2, X4), ^=U.
J
2= ^ t ,
J3 = ^ t x 3 + M 3 ,
J 4 =M 2 +M 2 ,
J5 = M§ - u\ - u\ ; 7- (Pi, P2, P3, X\, X2, X3, X4), Ji = x0 + x4, J 2 = u, J 3 = u0 - M4, 8. (I/ 3 , Pi, P2, P3, X i , X2, X3, X4),
J 4 = Wg - u\ - u\ - u\ - u\ ;
Some new differential equations with given symmetry groups Jl = X0 + X 4 ,
J 2 = U,
9. (L1 + l(P1+C1),
^4 = UQ —ul -
J3 = Mo - «4i
L2 + l(P2+C2),
93
U
2 ~ U3 ~ Ul !
L3 + \(P3 + C3),
L3 — 2(^3 + C3), .Xo, Xi, X2, X3, X4), Jl = U, J2 = Uo, J3 = u\ + lt| + W3 + «4 • Here, we also present some of the new results concerning the non-splitting subgroups of the group P(l,4). For the majority of non-splitting subgroups, the first-order differential equations in the space M(l,4) x R(u) which are invariant under these subgroups are found. These equations can also be written in the form (1), where {Ji, J2, •••, ./*} is a functional basis of the first-order differential invariants of the non-splitting subgroups of the group P(l,4). Now, we only write some of the new results obtained. Below, for some non-splitting subgroups of the group -P(l, 4), we give the basis elements of their respective Lie algebras and corresponding arguments Ji,J2,...,Jt of the function F.
1. (L3,
P3+X0),
J^Orf+z!) 1 / 2 ,
J2 =
(x0+x4)2-2x3,
J3 = 2(xo + x 4 ) 3 - 6x3(2:0 + £4) + 3(x0 — x 4 ), J5=X1U2-X2Ui,
J6=Xo+X4 + ^ ^ ,
J8=uf+ul, J9 = ul~ul-u\, 2. (G + a3X3, P x , P2, a 3 < 0 ) , Ji = x 3 - a 3 ln(x 0 +X4),
J2 =
J 4 = u, J7=U0-U4,
Uf, = ^ - , (XQ - X\
-
/i = 0,1,2,3,4;
X\ - X | ) 1 / 2 ,
J 3 = M,
J7 = u3, J8 = u§ - u\ - u\ - u\ ; 3. (G + a3X3, L3, P1; P2, a 3 <0), J1 = ( x g - x ? - x | - x l ) 1 / 2 , J2 = w, J3 = ^ ^ , J4 = X3-a3ln(xo + x4),
J5 = («i + n ^ )
J6 = U3, J7 = «o - u\ ~ U2 ~ ul ! 4.
J2=U,
J3=X3+
X
^^71"3,
^4 = ( S J X ! + M l ) 2 + ( f ^ X 2 + M2)2 , ^5 = "0 - «4,
^6 = «0 - «1 - U2 ~ U3 ~ U4 ;
5. (G + aX3, L3, Pu P2, P3, X 4 , a < 0 ) ,
+(M2+ X
2
^^) ,
94
Vasyl Fedorchuk, Volodymyr Fedorchuk Ji = x3 -a ln(u0 - Ui) + ^z^u3, 6. {L3 + bG + kX3, P u P 2 , P 3 , X
Ji = u, 9
J2 = f ^ , 9
9
u
J 5 = w§ - u\- u\- u\X2, XA, b > 0 , k < 0 ) ,
J3 = 6a;3 - k\n{x0 + x4) + 9
u\ ;
fef^us,
9
^4 = ^0 "" Ul ~ U2 ~ U3 ~ UX 5
7. (L1 + I(p 1 + Ci), L2 + \(P2+C2), L3 + \(P3 + C3), L3 - \{P3 + C3) + a(X0 + Xi), Xu X2, X3, Xo - X4, a < 0), Ji = u,
J2 = u0.
J3 — ul + u2+u3 + ul .
Since the Lie algebra of the group P(l,4) contains, as subalgebras, the Lie algebra of the Poincare group P(l, 3) and the Lie algebra of the extended Galilei group G(l,3) [10], the results obtained can be used in relativistic and nonrelativistic physics.
References 1.
2.
3. 4. 5. 6.
7.
8.
9.
Fedorchuk V.I., Differential equations of the first-order in the space M ( l , 4) x R(u) with nontrivial symmetry groups, Proc. of the Institute of Mathematics of NAS of Ukraine 36 (2001) 283-292. Fedorchuk V.I., On Differential Equations of First- and Second-Order in the Space M(l,3) x R(u) with Nontrivial Symmetry Groups, Proc. of the Fourth Internat. Conf. Symmetry in Nonlinear Mathematical Physics (9-15 July 2001, Kyiv, Ukraine), Proceedings of Institute of Mathematics of NAS of Ukraine, Kyiv, 43, Part 1, 145-148. Fedorchuk V.M., Continuous subgroups of the inhomogeneous de Sitter group P ( l , 4 ) , Preprint, Inst. Matemat. Acad. Nauk Ukr. SSR N 78.18, 1978. Fedorchuk V.M., Nonsplitting subalgebras of the Lie algebra of the generalized Poincare group P ( l , 4 ) , Ukr. Mat. Zh. 33 (5) (1981) 696-700. Fedorchuk V.M., Splitting subalgebras of the Lie algebra of the generalized Poincare group P ( l , 4 ) , Ukr. Mat. Zh. 31 (6) (1979) 717-722. Fedorchuk V.M. and Fushchych W.I., On subgroups of the generalized Poincare group, in Proceedings of the International Seminar on Group Theoretical Methods in Physics, Moscow, Nauka, V. 1, 1980, 61-66. Fushchych W.I., Representations of full inhomogeneous de Sitter group and equations in five-dimensional approach. I, Teoret. i mat. fizika 4 (3) (1970) 360-367. Fushchych W., Barannyk L. and Barannyk A., Subgroup analysis of the Galilei and Poincare groups and reductions of nonlinear equations. Kiev, Naukova Dumka, 1991. Fushchich W.I., Barannik A.F., Barannik L.F. and Fedorchuk V.M., Continuous subgroups of the Poincare group P ( l , 4 ) , J. Phys. A: Math. Gen. 18 (4) (1985) 2893-2899.
Some new differential equations with given symmetry groups
95
10. Fushchich W.I. and Nikitin A.G., Reduction of the representations of the generalized Poincare algebra by the Galilei algebra, J. Phys.A: Math, and Gen. 13 (7) (1980) 2319-2330. 11. Fushchych W.I. and Nikitin A.G., Symmetries of Equations of Quantum Mechanics. Allerton Press Inc., New York, 1994. 12. Fushchych W.I. and Serov N.I., On some exact solutions of the multidimensional nonlinear Euler-Lagrange equation, Dokl. Akad. Nauk SSSR 278 (4) (1984) 847-851. 13. Fushchych W.I. and Serov N.I., The symmetry and some exact solutions of the multidimensional Monge-Ampere equation, Dokl. Akad. Nauk SSSR 283 (3) (1983) 543-546. 14. Fushchych W.I. and Shtelen W.M., The symmetry and some exact solutions of the relativistic Eikonal equation, Lett. Nuovo Cim. 34 (16) (1982) 498-502. 15. Fushchych W.I., Shtelen W.M. and Serov N.I., Symmetry Analysis and Exact Solutions of Equations of Nonlinear Mathematical Physics. Dordrecht, Kluver Academic Publishers, 1993. 16. Kadyshevsky V.G., New approach to theory electromagnetic interactions, Fizika elementar. chastitz. i atomn. yadra 11 (1) (1980) 5-39. 17. Lie S., Uber Differentialinvarianten, Math. Ann. 24 (1) (1884) 52-89. 18. Olver P.J., Applications of Lie Groups to Differential Equations. SpringerVerlag, New York, 1986. 19. Ovsiannikov L.V., Group Analysis of Differential Equations. Academic Press, New York, 1982. 20. Patera J., Winternitz P. and Zassenhaus H., Continuous subgroups of the fundamental groups of physics. I. General method and the Poincare group, J. Math. Phys. 16 (8) (1975) 1597-1614. 21. Tresse A., Sur les invariants differentiels des groupes continus de transformations, Ada math. 18 (1894) 1-88.
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Functional Analysis and its Applications V, Kadets and W. Zelazko © 2004 Elsevier B.V. All rights reserved
97
Inverse Spectral Problems for Sturm-Liouville Operators with Singular Potentials, II. Reconstruction by Two Spectra* Rostyslav O. Hryniv a b and Yaroslav V. Mykytyuk b a
Institute for Applied Problems of Mechanics and Mathematics, 3b Naukova st., 79601 Lviv, Ukraine b Lviv National University, 1 Universytetska st., 79602 Lviv, Ukraine
Abstract We solve the inverse spectral problem of recovering the singular potentials q £ VF2"~1(0,1) of Sturm-Liouville operators by two spectra. The reconstruction algorithm is presented and necessary and sufficient conditions on two sequences to be spectral data for Sturm-Liouville operators under consideration are given. Key words: Inverse spectral problems, Sturm-Liouville operators, singular potentials 2000 MSC: 34A55, 34B24, 34L05, 34L20
1. Introduction Suppose that q is a real-valued distribution from the space W f1 (0,1). A SturmLiouville operator T in a Hilbert space Ti := £2(0,1) corresponding formally to the differential expression * The work was partially supported by Ukrainian Foundation for Basic Research DFFD under grant No. 01.07/00172. Ft. H. acknowledges support of the Alexander von Humboldt Foundation. Email addresses: rhrynivaiapmm.lviv.ua (Rostyslav O. Hryniv), yamykytyukayahoo.com (Yaroslav V. Mykytyuk).
98
Rostyslav 0. Hryniv, Yaroslav V. Mykytyuk
can be defined as follows [18]. We take a distributional primitive a G 7i of q, put la{u) := —(u' — au)' — av!
for absolutely continuous functions u whose quasi-derivative u'1! := u' — au is again absolutely continuous, and then set
Tu := la{u) for suitable u (see Section 2 for rigorous definitions). When considered on this natural domain subject to the boundary conditions ull](0)-Hu(0)
= 0, u[1](l) + hu(l)=0,
H,h GRU{oo},
(1.2)
the operator T = T(cr, H, h) becomes [17,18] selfadjoint, bounded below, and possesses a simple discrete spectrum accumulating at +oo. (If H = oo or h = oo, then the corresponding boundary condition is understood as a Dirichlet one.) We observe that among the singular potentials included in this scheme there are, e.g., the Dirac <5-potentials and Coulomb 1/x-like potentials that have been widely used in quantum mechanics to model particle interactions of various types (see, e.g., [1,2]). It is also well known that singular potentials of this kind usually do not produce a single Sturm-Liouville operator. Still for many reasons T(a, H, h) can be regarded as a natural operator associated with differential expression (1.1) and boundary conditions (1.2). For instance, la(u) = —u" + qu in the sense of distributions and hence for regular (i.e., locally integrable) potentials q the above definition of T(cr, H, h) coincides with the classical one. Also T(a, H, h) depends continuously in the uniform resolvent sense on a G 7i, which allows us to regard T(a, H, h) for singular q = a' as a limit of regular Sturm-Liouville operators. Sturm-Liouville and Schrodinger operators with distributional potentials from the space W% (0,1) and W^~unif(R) respectively have been shown to possess many properties similar to those for operators with regular potentials, see, e.g., [9,10,17,18]. In particular, just as in the regular case, the potential q = a' and boundary conditions (1.2) of the Sturm-Liouville operator T(a,H,h) can be recovered via the corresponding spectral data, the sequences of eigenvalues and so-called norming constants [11]. The main aim of the present paper is to treat the following inverse spectral problem. Suppose that {A^} is the spectrum of the operator T(a, H, hi) and {/J^} is the spectrum of the operator T(a, H, ft^) with h,2 / h\. Is it possible to recover a, H, hi, and /12 from the two given spectra? More generally, the task is to find necessary and sufficient conditions for two sequences (A^) and (fi^) so that they could serve as spectra of Sturm-Liouville operators on (0,1) with some potential q — a' e W/2~1(0,1) and boundary conditions (1.2) for two different values of h and, then, to present an algorithm recovering these two operators (i.e., an algorithm determining a and the boundary conditions). For the case of a regular (i.e., locally integrable) potential q the above problem was treated by LEVITAN AND GASYMOV [14,15] when h\ and h2 are finite and by
Reconstruction by two spectra
99
MARCHENKO [16, Ch. 3.4] when one of hi,h2 is infinite. Earlier, BORG [4] proved that two such spectra determine the regular potential uniquely. Observe that T(a + h',H - ti, h + h') = T(cr, H, h) for any h' G C, so that it is impossible to recover a, H, hi, and hi uniquely; however, we shall show that the potential q = a' and the very operators T(a, H, hi) and T(a, H, h2) are determined uniquely by the two spectra. The reconstruction procedure consists in reduction of the problem to recovering the potential q = a' and the boundary conditions based on the spectrum and the sequence of so-called norming constants. The latter problem has been completely solved in our paper [11], and this allows us to give a complete description of the set of spectral data and to develop a reconstruction algorithm for the inverse spectral problem under consideration. The organization of the paper is as follows. In the next two sections we restrict ourselves to the case where H = oo and h\,h2 G R. In Section 2 refined eigenvalue asymptotics is found and some other necessary conditions on spectral data are established. These results are then used in Section 3 to determine the set of norming constants and completely solve the inverse spectral problem. The case where one of hi and h2 is infinite is treated in Section 4, and in Section 5 we comment on the changes to be made if H is finite. Finally, Appendix A contains some facts about Riesz bases of sines and cosines in L2{Q, 1) that are frequently used throughout the paper.
2. Spectral asymptotics In this section (and until Section 4) we shall consider the case of the Dirichlet boundary condition at the point x = 0 and the boundary conditions of the third type at the point x = 1 (i. e., the case where H = oo and hi,h,2 G K). We start with the precise definition of the Sturm-Liouville operators under consideration. Suppose that q is a real-valued distribution from the class Wr2~1(0,1) and a G Ti is any of its real-valued distributional primitives. For h £ R we denote by Ta^h = T(a, oo, h) the operator in Ti given by Ta}hu = la(u):=-{u[1]
)'-
and the boundary conditions M(0)=0,
uw(l) + hu(l) = 0 ,
ftel
(we recall that «W stands for the quasi-derivative v! — cru of «). More precisely, the domain of X^/, equals £ ( 2 ^ ) = {w G ^ [ 0 , 1 ] | «[1] G WftO.l], / »
G W,
u(0) = 0, u[1](l) + hu{l) = 0}. It follows from [18] that so defined Ta>h is a selfadjoint operator with simple discrete spectrum accumulating at +oo. The results of [19] also imply that the eigenvalues A^ of To-./i) when ordered increasingly, obey the asymptotic relation \ n = 7r(n—l/2)+An
100
Rostyslav 0. Hryniv, Yaroslav V. Mykytyuk
with an ^-sequence (An). However, we shall need a more precise form of An, and shall derive it next. To start with, we introduce an operator Ta defined by Tau = la(u) on the domain 2>(Tff) = {u G Wl[0,1] | v,W G Wl[0,1], la(u) G H, /(0) = 0}. In other words, Ta is a one-dimensional extension of Ta^ discarding the boundary condition at the point x = 1. We invoke now the following results of [12] on the operator Ta. Just as in the classical situation with regular potential q the operators T±a turn out to be similar to the potential-free operator To; the similarity is performed by the transformation operators I + K^r, where K^r are integral Volterra operators of Hilbert-Schmidt class given by K±u{x)= / k±(x,t)u(t)dt. Jo It follows that any function u from ©(X^) has the form u = (I + K^)v for some function v G 5D(To) (i.e., for some v G W|[0,1] satisfying the boundary condition v(0) = 0) and that Ta(I + K+)v = ~(I + K+)v". Moreover, there exists a HilbertSchmidt kernel ra(x,t) such that
[(I + K+)vf\x)
= [(I + K-)v']{x) + f ra(x, t)v{t) dt Jo
for every v G Q{T0). Also, for every fixed x G [0,1] the functions kf(x,-) and ra{x, •) belong to 7i. Due to the above similarity of Ta and To, for any nonzero A G C the function
fx u(x, A) := sin Ax + / fc£(x,t) sin Xt dt
Jo is an eigenfunction of the operator Ta corresponding to the eigenvalue A2 G C If in addition u(x, A) satisfies the boundary condition u^(l) + hu(l) = 0, then u(x, A) is also an eigenfunction of the operator Ta^ corresponding to the eigenvalue A2. Therefore the nonzero spectrum of Ta^ consists of the squared nonzero A-solutions of the equation fi
c o s A + / ka(l,t)cos\t Jo
1
dt+-
,i
Ai0 h
ra(l,t) h
sin At At f
+ - s i n A + - / fc+(l,<)sinAt A A Jo
d< = 0.
Recall that the operator Ta^ is bounded below and hence after addition to q a suitable constant Ta^ becomes positive. Therefore without loss of generality we may assume that all solutions of equation (2.1) are real and nonzero. Observe also that due to the symmetry we may consider only the positive zeros. The asymptotics of these zeros is given in the following theorem.
Reconstruction by two spectra
101
Theorem 2 . 1 . Suppose that a € H and h € M are such that the operator X^/j is positive and denote by Af < Af < •• • the eigenvalues of Ta^- Then the numbers Xn satisfy the relation Xn = n(n - 1/2) + — + Sn(h) + -yn, in which the sequences (<5n(/i))n=1 and (yn)n°=i belong to £\ and ^2 respectively with 7 n independent of ft. Proof. Recall that Xn —>• 00 as n —> 00 and that the functions fc^(l,i) and r CT (l,i) belong to 7i. Therefore (2.1) and the Riemann lemma imply that
cosAn = - / k-(l,t)cos\ntdt Jo
+ 0{l/Xn) = o(l)
as n —> 00. By the standard Rouche-type arguments (see details, e.g., in [16, Ch. 1.3]) we conclude that Xn = n(n — 1/2) + An with An —> 0 as n —> cc. As a result (see Appendix A), the system {sinXnx} turns out to be a Riesz basis of Tt and the sequences (cn)^°=1 and (c'n)'£L1 with
cn:= f k+{l,t)sinXntdt, Jo
c'n:= [ ra{l, t) sinXnt dt Jo
belong to £2- Relation (2.1) now implies that
sinAn = ( - i r + 1 f1 k~(l,t)cosXnt dt + h°-^ Jo
+ (_i)n+iftc" + <
Xn
=
Xn
where 7n:=(-l)n+1 f Jo
fc-(l,t)cos7r(n-l/2)tdt,
S'n := ( - l ) n + 1 I jfc~(l,f)[cosAni - cos7r(n - 1/2)*] dt, Jo hc C „ __ fecOsAw h Un + l n+ 'n n
'~~
\ An
-rrn Tin
^
'
(2.2)
\ An
Next we observe that the systems {cos7r(n — l/2)t}^L1 and {cos Xnt}^=1 form Riesz bases of Ti, so that (7,,) and (S'n) belong to £2- It follows that (sin An) € £2 and therefore (An) € £2- Lemma A.2 now implies that the numbers S'n form an £\sequence, and simple arguments justify the same statement about 5'^. Thus we have shown that ~ h s i n A n = 7 n + — +8'n + 8Z with the sequences (7ra) from £2 and (5'n) and (<5^) from £\. Applying arcsin to both parts of this equality, we arrive at
102
Rostyslav
0. Hryniv,
Yaroslav V.
~ h K = In H
Mykytyuk
r
1" On
with some £i-sequence (5n), and t h e theorem is proved.
•
It was shown in [11] that any sequence (A 2 ) of pairwise distinct positive numbers satisfying t h e relation Xn = ir(n—l/2)+\n with an ^-sequence (A n ) is the spectrum of some Sturm-Liouville operator Ta
y±
dx\u)
a
j
\u)
and hence u enjoys the standard uniqueness properties of solutions to first order differential systems with regular (i.e. locally integrable) coefficients. The numbers An and \xn are then solutions of the equations v^{\,X) + hiu(l,X) = 0 and u [11 (l, A) + h2u(l, A) = 0 respectively. We introduce a continuous function 9(x, X) through cot#(:r,A) = u^/u. After differentiating both sides of this identity in x and using (2.3) we get -^-22 = sin 8
2 uz
A = - cot<9 + <7
2
-A,
or 9' = X sin2 9 + (cos 9 + a sin 9)2. It follows from [3, Ch. 8.4] or [7, proof of Theorem XI.3.1] that the function 9(1, A) is strictly increasing in A; hence solutions of the equations cot#(l,A) = —hi and cot 9(1, A) = —/12 interlace, and the proof is complete. •
The next restriction concerns asymptotics of Xn and jj,n.
Reconstruction by two spectra
103
Lemma 2.3. Suppose that (A^) and ()in) are spectra of Sturm-Liouville operators Ta,h! and Tath2 with real-valued a 6 H and hi,h2 G R- Then there exists an ^2-sequence {vn) such that hi -h2 K-Vn
=
vn 1
irn
•
(2-4)
n
Proof. Put An := An - 7r(n — 1/2) and Jin := fin - ir(n - 1/2) so that An - fin = An —Jin- Recall that sinA n - sin/In = ^ — - + S'n(hi) - S'n(h2) + 5'^hi) - %(h2) with the quantities 6'n(h),8£(h) of (2.2). Relation
S'n(hi) - S'n(h2) = ( - l ) n + 1 / ^-(l.^IcosA,,* - cos^t] dt Jo
and Lemma A.2 show that 5'n(hi) -5'n(h2) = (An —/xn)t£ for some ^-sequence (v'n). Also there exists an ^-sequence (i/£) such that S'^hi) — ^'(Z^) = v'^/n. Finally, using the relations sin Ara - sin jun = (An - Jin) cos ?„, where vn are points between An and Jin (so that (1 — cos? n ) is an ^-sequence), and combining the above relations we arrive at (An -/x n )(cos i / n - i / n ) = ——
h—,
which implies (2.4).
D
Corollary 2.4. Under the above assumptions, lim n ^ oc (A^ — /i^) = 2(/i! — hi)-
3. Reduction to the inverse spectral problem by one spectrum and norming constants Suppose that a € H. is real-valued and that {A^} and {/^} are eigenvalues of the operators Ta^ and Tath2 respectively introduced in the previous section. We shall show how the problem of recovering a, hi, and h2 based on these spectra can be reduced to the problem of recovering a and hi based on the spectrum {An} of T^j^ and the so-called norming constants {an} defined below. This latter problem for the class of Sturm-Liouville operators with singular potentials from W^~l(0,1) is completely solved in [11]; see also [13,16] for the regular case of integrable potentials. Denote by U\{x, A) and u2(x, A) solutions of the equation la(u) = \2u satisfying the terminal conditions Ui(l,A) = u 2 (l,A) = 1 and w^(l,A) = —hj, j = 1,2.
104
Rostyslav O. Hryniv, Yaroslav V. Mykytyuk
Then Ui(x,Xn) are the eigenfunctions of the operator X^/jj corresponding to the eigenvalues X\, and we put f1
an:=2
Jo
\ux(x,\n)\2
dx.
Our next aim is to show that an can be expressed in terms of the spectra {A2.,//2.} only. Set $j(A) := Uj(0, A), j = 1,2; then zeros of <J?i and $2 are precisely the numbers ±A n and ±fin respectively. We show that $1 and $2 uniquely determine an and are uniquely determined by their zeros. Lemma 3.1. The norming constants an satisfy the following equality: a
n =
7 ft a v An *2(,AnJ
(3-1)
Proof. The proof is rather standard and the details can be found, e.g., in [13], so we shall only sketch its main points here. Put m(A) := -$ 2 (A)/$i(A); then the function /(x, A) := u2{x, A) +m(X)ui(x, A) for all A G C such that A2 is not in the spectrum of TG)hx satisfies the equation lo-(f) = A 2 / and the boundary condition /(0,A) = 0. In other words, f(x, A) is an eigenfunction of the operator TCT corresponding to the eigenvalue A2. Since u\ (x, An) is an eigenfunction of the operator Ta corresponding to the eigenvalue A2, we have
(A2-A2) / Jo
f(x,X)u1(x,Xn)dx=(Taf,u1)-(f,Taul) = - / W ( l , A M M ) + / ( I , A)«W(l,An) =
h2-h1.
On the other hand, ( A 2 - A 2 ) / /(x,A) U l (x,A n )dx = (A 2 -A 2 ) / Jo Jo 2
u2(x,X)Ul(x:Xn)dx
- (A - ^ ) f ^ j jj 1 Ul(a:, A)Ul(x, An) dx,
and after combining the two relations and letting A —> Xn we arrive at _h1-h2
D
The following statement has appeared in many variants in numerous sources, but we include its proof here for the sake of completeness.
Reconstruction by two spectra
105
Lemma 3.2. In order that a function /(A) admit the representation /(A) = c o s A + / g(t) cos Xtdt Jo with an Ti-function g, it is necessary and sufficient that
(3.2)
where /^ := ir(k — 1/2) + /& and (fk) is an ^-sequence. Proof. Necessity. The function / of (3.2) is an even entire function of order 1, and the standard Rouche-type arguments (see the analysis of Section 2) show that zeros ±/fc of / have the asymptotics fk = n(k — 1/2) + fk with (fk) € £2- On the other hand, up to a scalar factor C, the function / is recovered from its zeros as
W>-<#-j?)-*n;F$f$i.
(">
where f
fc=l
k
To determine Ci, we observe that, in view of (3.2), lim^^oo f(iv)/ that -
[
(7r2(A._1/2)2_A2)
™x=n
U(fc-i/2)»
;
cos iv = 1 and
(3 5)
-
fc—1
comparing now (3.4) and (3.5), we conclude that C\ = 1 and the necessity is justified. Sufficiency. Suppose now that / has a representation of the form (3.3), in which fk = ir(k — 1/2) + fk with (fk) £ (-2- We assume first that the zeros fk are pairwise distinct. Then due to the asymptotics of fk the system (cos /fcx)^_1 is a Riesz basis of Ti (see Lemma A.I) and the numbers Ck := — cos fk = (—l)fc sin fk define an £2sequence. Therefore there exists a unique function g £ 7i with Fourier coefficients Ck in the Riesz basis (cos fkx)kxLl. Now the function 1
/(A):=cosA+ /f g(x)cos\x dx (3-6) Jo is an even entire function of order 1 and has zeros at the points ±/fc. It follows that / and / differ by a scalar factor, which as before is shown to equal 1. Due to the asymptotics of the zeros fk only finitely many of them can repeat. If, e.g., fn = fn+i = • • • = fn+p-i is a zero of the function / of multiplicity p = p(n), then we include to the above system the functions cosfnx, x s i n / n x , ••• , xp~1 sin(7rp/2 — fnx). After this modification has been done for every multiple root, we again get a Riesz basis of Ti and can find a function g G Ti with Fourier
106
Rostyslav 0. Hryniv, Yaroslav V. Mykytyuk
coefficients c n := - c o s / n , c n + i = - s i n / n , - - - , cn+p(n) := - sin(7rp(n)/2 - fnx). Then ± / n becomes a zero of the function / in (3.6) of multiplicity p(n), and the proof is completed as above. • Lemma 3.3. The following equalities hold:
$1(\) = l[n-2(k-l/2)-2(\l-\2), $2(A) = n^ 2 (^-l/2)- 2 (^-A 2 ). Proof. We recall [12] that the function u\ has a representation via a transformation operator connected with the point x = 1 of the form Mi (x, A) = cos A(l - x) + / k(x, t) cos A(l - t) dt, Jx
which implies that $1(A) = cosA+ / k\ (t) cos At dt, Jo where k\{t) := fc(0,1 — t) is a function from H. The claim now follows from Lemma 3.2. The representation for $2 is derived analogously, and the lemma is proved. • Now, given two spectra (A2) and (/^) of two Sturm-Liouville operators Ta^,x and To-^2 respectively, with unknown a € H and h\,hi € R, we proceed as follows. First, we identify hi — hi as lim n ^ oo (A^ — Ai21)/2 (see Corollary 2.4), then construct the functions $1 and $2 of (3.7) and determine the norming coefficients (an) via (3.1). The spectral data {(A^), (ctn)} determine a and hi up to an additive constant by means of the algorithm of [11]. This gives the required function a and two numbers h\ and hi up to an additive constant, and the reconstruction is complete. The second part of the inverse spectral problem is to identify those pairs of sequences (A^) and (/x^) that are spectra of Sturm-Liouville operators T,,^ and Tafo for some real-valued a € 7i and some real hi, /12, hi ^ hi- We established in Theorem 2.1 and Lemmata 2.2 and 2.3 the necessary conditions on the two spectra; it turns out that these conditions are sufficient as well. Namely, the following statement holds true. Theorem 3.4. Suppose that sequences (A^) and (fi^) of positive pairwise distinct numbers satisfy the following assumptions: (i) the sequences (A£) and {n2n) interlace; (ii) An = ?r(n — 1/2) + An and fj,n = 7r(n — 1/2) + Jin with some ^-sequences (Ara) and (£„); (iii) there exist a real number h and an ^-sequence (vn) such that Xn — ixn = _h_ •Kn
1 VJO, n '
Reconstruction by two spectra
107
Then there exist a function a £ Tt and two real numbers h\ and h2 such that (An) and (/zn) are the spectra of the Sturm-Liouville operators Ta^x and T^/^ respectively. Moreover, the operators Ta ^ and TCT ^2 are recovered uniquely. In order to prove the theorem we have to show first that the numbers an constructed for the two sequences through formula (3.1), with the functions $ i , $ 2 of (3.7) and hi — hi := h with h of item (3), are positive and obey the asymptotics an = 1 + a n for some ^-sequence (an). Then the algorithm of [11] uses (An) and (an) to determine a (unique up to an additive constant) function a 6 Ti and hi € R such that {An} is the spectrum of the Sturm-Liouville operator T^hx and an are the corresponding norming constants. The second and final step is to verify that {/«„} is the spectrum of the Sturm-Liouville operator Ta^i with hi := hi —h, where h is the number of item (3). These two steps are performed in the following two lemmata. Lemma 3.5. Assume (l)-(3) of Theorem 3.4. Then the numbers an constructed via relation (3.1) with <3>1; <3>2 of (3.7) and hi - h2 := h with h of item (3) are all positive and obey the asymptotics an = 1 + an, where (an) is an ^-sequence. Proof. By Lemma 3.2 there exist H-functions / i , fa such that the functions $ j , j = 1, 2, of (3.7) admit the representation $ j (A) = cos A + / fj (t) cos At dt. Jo It follows that $ i (An) = - sin An - / tfi (t) sin Ant dt Jo
= ( - l ) " c o s A n - / iA(t) sin A n tdt = (-1)" + An, Jo where ( A n ) ^ ! £ £2, and by similar arguments $ 2 (A n ) = (An - ^n)*'2(/*n) + O(\Xn = (An-Mn)[(-l)n+An]
Mn|
2
)
for some ^2-sequence (/in). Next, assumptions (2) and (3) easily imply the relation h —rr
r = 1 + !/„,
^nV^n ~ A*nj
for some ^-sequence (i>n). Therefore the numbers = Qn
obey the required asymptotics.
'
h ^(An) A n * 2 (A n )
108
Rostyslav 0. Hryniv, Yaroslav V. Mykytyuk
Finally, the interlacing property of the two sequences implies that all an are of the same sign, and thus are all positive in view of the asymptotics established. The proof is complete. • With the above-stated properties of the sequences (An) and (an) we can employ the result of [11] that guarantees existence of a unique Sturm-Liouville operator Ta,h\ with a real-valued function a G Ti and a real number hi such that {A^} coincides with the spectrum of Ta^x and an are the corresponding norming constants. Now we put hi :— h\ — h with h of assumption (3) and expect {/i2} to be the spectrum of Tajl2. Lemma 3.6. The spectrum of the Sturm-Liouville operator Ta^ a € Ti. and hi € R coincides with (/i^).
with the above
Proof. Denote by V\{x,X) a solution of the equation la(v) = X2v satisfying the boundary conditions v(l) = 1, ^E1!(1) = —h\. Then V\(x, Xn) is an eigenfunction of the operator Ta^ corresponding to the eigenvalue Ara, and by construction
2/ 1 |, 1 (x,A n )| 2 d, = a n : = A | i M with the functions $i,3>2 of (3.7). Denote by (f^) the spectrum of T^h2 and put oc
* 2 (A):=n^ 2 (fc-l/2)- 2 (^-A 2 ). fc=i
By Lemma 3.1 we have h $;(Ara) Ctn = T— ~
,
An $ 2 (A n ) whence $2(^71) = ^2(Ara) for all n £ N . Lemma 3.2 implies that f1 $2(A) - $ 2 (A) = / f(t) cos At At Jo for some f £H. Equality $ 2 (A n ) = $2(Ara) means that the function / is orthogonal to cos Xnt, n e N. Since the system {cos Xnt} forms a Riesz basis of Ti, we get / = 0 and \&2 = ^2- Thus vn = /in, and the lemma is proved. •
4. Reconstruction by Dirichlet and Dirichlet-Neumann spectra The analysis of the previous two sections does not cover the case where one of hi, hi is infinite. In this case the other number may be taken 0 without loss of generality (recall that TCT;/j = Ta+h,o), i-e., the boundary conditions under considerations become Dirichlet and Dirichlet-Neumann ones.
Reconstruction by two spectra
109
Suppose therefore that a £ Ti is real valued and that (A^) and (/z^) are spectra of the operators TCTjo and TCTjOO respectively; without loss of generality we assume that An and \in are positive and strictly increase with n. The reconstruction procedure remains the same as before; namely, we use the two spectra to determine a sequence of norming constants (an) and then recover a by the spectral data {(A^), (an)}. Denote by «-(•, A) and u+(-, A) solutions of the equation lau = Xu satisfying the initial conditions «-(0, A) = 0, u_ (0, A) = A and the terminal conditions u+(l, A) = 1, U+ (1, A) = 0 respectively. Then u+(-, An) is an eigenfunction of the operator TCT>o corresponding to the eigenvalue A^ and /•i
an:=2
Jo
\u+{x,Xn)\2 dx
is the corresponding norming constant. We also put ^i(A) := w+(0, A) and \&2(A) := «_(1,A); then zeros of the functions $ i and ^2 are numbers ±A n and ±/i n respectively. As earlier, the function ^1 is uniquely determined by its zeros through formula (3.7). Observe that the Dirichlet eigenvalues /ij; have asymptotics different from that of A^, so that \&2 requires slight modification of formula (3.7). We first investigate the asymptotics of //„. Theorem 4.1 ([12,17]). Suppose that a e Ti and {fJ%}, n G N, is the spectrum of the operator T(T)0O. Then the numbers \xn satisfy the relation /i n = ?rn + Jin, in which the sequence {jxn) belongs to £2Proof. The solution w_ can be represented by means of the transformation operator [12] as U-(x, A) = sin Ax + J^ k£(x,t) sinXt dt, where k£ is the kernel of the transformation operator. Therefore the numbers ±fj,n are zeros of the function * 2 ( A ) : = s i n A + / /c+(l,i) sin Ai di, (4.1) Jo which is entire of order 1. Since the function A;+(l, •) belongs to H. [12], the required asymptotics of \xn is derived in a standard way (cf. [16] and Section 2). • The function \&2 is determined by its its zeros in the following way. Lemma 4.2. The following equality holds:
*2(A) = A [ I x - 2 r V t - A 2 ) .
(4.2)
The proof is completely analogous to that of Lemma 3.2 and is left to the reader. Now we show how the norming constants an are expressed via \&i and \&2-
110
Rostyslav 0. Hryniv, Yaroslav V. Mykytyuk
Lemma 4.3. The norming constants satisfy the following equality:
Proof, (cf. [5]) The Green's function G(x,y, A2) of the operator TCTj0 (i- e., the kernel of the resovlent (Tafi — A 2 )" 1 ) equals
m
2
^2^ _ ^
2
G(x,y,A j - 2 ^ A - A2
u+(x,Xn)u+(y,Xn) a
'
On the other hand, we have ,2)
r( [X V
''
=
'
1 (u-(x,\)u+(y,\), W(X)'\u+(x,X)u.(y,X),
0<x
where W(X) := u+(x,X)u_ (x,X) — U-(x,X)u+ (x,X) is the Wronskian of u+ and «_. The value of W(X) is independent of x G [0,1]; in particular, taking i = 0we find that W(X) = Xu+(0, A) = A*i(A). Now we take x = y = 1 in the above expressions and find that v^ ^A
2
2 -A
1 2
a
n
* 2 (A) A*! (A)"
Comparing the residues at the poles A = An, we derive formula (4.3), and the lemma is proved. • Now the reconstruction procedure is completed as follows: we determine the sequence of norming constants (an) as explained above and find a unique operator T<jfi with spectrum (A2) and norming constants (an), see [11]. This gives the function a G 7i and thus the operator T(Tj00. Now we would like to give an explicit description of the set of all possible spectra of the operators Tao and Tat00 when a real-valued function a runs through Ti, i. e., to give the necessary and sufficient conditions on two sequences (A2) and (/LJ2) to be the spectra of X^o and Ta>oo with a real-valued a G 7i. Necessary conditions are that the eigenvalues A2 and p?n should interlace and obey the asymptotics described in Theorems 2.1 and 4.1; we shall show that these conditions are in fact sufficient as well. Theorem 4.4. Suppose that sequences (A2) and (/i2) of positive pairwise distinct numbers satisfy the following assumptions: (i) the sequences (A2) and (/z2) interlace: 0 < X\ < \i\ < A| < . . . ; (ii) An = ?r(n — 1/2) + An and /zn = irn + Jin with some ^-sequences (An) and
(fin)Then there exist a unique function a G Ti. such that (A2) and (/x^) are the spectra of the Sturm-Liouville operators Ta^ and Ta
Reconstruction by two spectra
111
The main ingredients of the proof of this theorem are the same as for Theorem 3.4: first, we construct functions >J/i and ^2 by their zeros and define the sequence (a n ) as explained in Lemma 4.3; then we prove that an are all positive and have the required asymptotics an = 1 + an for some ^-sequence (an). Using now the reconstruction algorithm of [11], we find a unique function a £ TL such that the corresponding Sturm-Liouville operator T^o with potential q = a' € H possesses the spectral data {(A^), ( a n ) } . Finally, we prove that (/z^) is the spectrum of the operator TaiOO with a just found, and the reconstruction procedure is complete.
5. The case of the Neumann boundary condition at x — 0 The analysis of the previous sections can easily be modified to cover the case H = 0, i.e., the Neumann boundary condition uM(0) = 0. As before, we use the two spectra to determine the sequence of norming constants and then apply the reconstruction procedure of [11] to find the corresponding Sturm-Liouville operators. Also the necessary and sufficient conditions on the two spectra can be established. We formulate the corresponding results in the following two theorems. Theorem 5.1. Suppose that sequences (A^) and (//^) of positive pairwise distinct numbers satisfy the following assumptions: (i) the sequences (A^) and (/i£) interlace; (ii) An = 7r(n - 1) + An and \in = 7r(n -1) + Jln with some £2-sequences (An) and G"n); (iii) there exist a real number h and an ^-sequence (yn) such that Xn — fJ,n = •nn '
n '
Then there exist a unique function a £ 7i and real constants h\,hi such that (A^) and (/i^) are the spectra of the Sturm-Liouville operators X^o,^ and TaQ^2 respectively. Conversely, the spectra (A^) and (//^) of Sturm-Liouville operators TCT]o,hi and Ta,o,h2 with cr eH and hi, h2 G M satisfy assumptions (l)-(3). For the case where one of hi, hi is infinite (say, hi = 00) the asymptotics of the corresponding spectrum is different; also assumption (3) becomes meaningless and should be omitted. Theorem 5.2. Suppose that sequences (A^) and (/i^) of positive pairwise distinct numbers satisfy the following assumptions: (i) the sequences (A^) and ((jfy interlace; (ii) \ n = 7r(n — 1) + An and fj,n — ?r(n - 1/2) + jun with some £2-sequences (An) and (/!„). Then there exist a unique function a € H and a real constant hi such that (A^) and (/x^) are the spectra of the Sturm-Liouville operators T^o,^ and TCTjo,oo respectively.
112
Rostyslav 0. Hryniv, Yaroslav V. Mykytyuk
Conversely, the spectra (An) and {fi\) of Sturm-Liouville operators T^o,^ and Ta,o,oa with a S H and h\ £ M. satisfy assumptions (1) and (2).
Appendix Appendix A. Riesz bases In this appendix we gather some well known facts about Riesz bases of sines and cosines (see, e.g., [6,8] and the references therein for a detailed exposition of this topic). Recall that a sequence (e n )f° in a Hilbert space % is a Riesz basis if and only if any element e £ TC has a unique expansion e = X)^Li cnen with (c n ) € ii- If (e n ) is a Riesz basis, then in the above expansion the Fourier coefficients cn are given by cn = (e, e'n), where {e'n)^° is a system biorthogonal to (e n ), i.e., a system which satisfies the equalities (ek,e'n) = Skn for all k,n G N. Moreover, the biorthogonal system (e'n) is a Riesz basis of TL as long as (en) is, in which case for any e € H also the expansion e = XXei e «) e n takes place. In particular, if (e n ) is a Riesz basis, then for any e G TL the sequence (c^) with c'n := (e,era) belongs to £2. Proposition A.I ([8]). Suppose that /^/. —> 0 as fc —> 00 and that the sequence Trfc + /Ufc is strictly increasing. Then each of the following systems forms a Riesz basis of 1/2(0,1): (a) {sin(ivkx +/j,kx)}%Li, (b) {sin{Tr[k - l/2}x + fikx)}^=1; (c) {cos(nkx + nkx)}^=0; (d) {cos(n[k + l/2]x + nkx)}%LQ. Lemma A.2. Suppose that (An) and (fin) are two sequences of real numbers such that lim |An - 7r(n - 1/2)1 = lim \un - 7r(n - 1/2)1 = 0. n—>oo
L
'
n—>oo
L
J
and assume that / € W. Then there exists an ^-sequence (vn) such that /
f(t)[cOS\nt
- COS flnt] dt = (An - / i n ) ^ + 0(1 An - MnH
as n —> 00. Proof. Using the relation cosAn£ — cos fint = —2sin[(An - fxn)t/2] sin[(An + jjLn)t/2], we find that
Reconstruction by two spectra
113
f1 / f(t)[cos\nt Jo
— cosfint] dt = - 2 f f(t) sin[(An - tin)t/2] sin[(An + fin)t/2] dt Jo = -(A n - fin) / tf(t) sin[(An + /i n )t/2] dt + O{\\n Jo
fin\3).
We put vn := —/ 0 i/(t)sin[(A n + /zn)£/2] dt and observe that the sequence (un) belongs to £2 since the system {sin[(An + /j,n)t/2]} is Riesz basic in H (at least for all n large enough) and the function tf(t) belongs to H. D
References 1. S. Albeverio, F. Gesztesy, R. H0egh-Krohn, and H. Holden, Solvable Models in Quantum Mechanics. Springer-Verlag, New York-Berlin-Heidelberg-LondonParis-Tokyo, 1988. 2. S. Albeverio and P. Kurasov, Singular Perturbations of Differential Operators. Solvable Schrodinger Type Operators. Cambridge University Press, Cambridge, 2000. 3. F. V. Atkinson, Discrete and Continuous Boundary Problems. Academic Press, New York-London, 1964. 4. G. Borg, Eine Umkehrung der Sturm-Liouvilleschen Eigenwertaufgabe, Ada Math. 78 (1) (1946) 1-96. 5. F. Gesztesy and B. Simon, On the determination of a potential from three spectra, in Differential operators and spectral theory, 85-92, Amer. Math. Soc. Transl. Ser. 2, 189, Amer. Math. Soc, Providence, RI, 1999. 6. I. Gohberg and M. Krein, Introduction to the Theory of Linear Non-selfadjoint Operators in Hilbert Space. Nauka Publ., Moscow, 1965 (in Russian); Engl. transl.: Amer. Math. Soc. Transl. Math. Monographs, vol. 18, Amer. Math. Soc, Providence, RI, 1969. 7. P. Hartman, Ordinary Differential Equations. John Wiley&Sons, New York, 1964. 8. X. He and H. Volkmer, Riesz bases of solutions of Sturm-Liouville equations, J. Fourier Anal. Appl. 7 (3) (2001) 297-307. 9. R. O. Hryniv and Ya. V. Mykytyuk, ID Schrodinger operators with singular periodic potentials, Meth. Fund. Anal. Topol. 7 (4) (2001) 31-42. 10. R. O. Hryniv and Ya. V. Mykytyuk, ID Schrodinger operators with singular Gordon potentials, Meth. Fund. Anal. Topol. 8 (1) (2002) 36-48. 11. R. O. Hryniv and Ya. V. Mykytyuk, Inverse spectral problems for SturmLiouville operators with singular potentials, Inverse Probl. 19 (2003) 665-684. 12. R. O. Hryniv and Ya. V. Mykytyuk, Transformation operators for SturmLiouville operators with singular potentials, Math. Phys. Anal. Geom. (2003), to appear.
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13. B. M. Levitan, Inverse Sturm-Liouville Problems. Nauka Publ., Moscow, 1984 (in Russian); Engl. transl.: VNU Science Press, Utrecht, 1987. 14. B. M. Levitan, On determination of a Sturm-Liouville differential equation by two spectra, Izv. AN SSSR, Ser. Math. 28 (1) (1964) 63-78. 15. B. M. Levitan and M. G. Gasymov, Determination of a differential equation by two spectra, Uspekhi Mat. Nauk 19 (2) (1964) 3-63. 16. V. A. Marchenko, Sturm-Liouville Operators and Their Applications. Naukova Dumka Publ., Kiev, 1977 (in Russian); Engl. transl.: Birkhauser Verlag, Basel, 1986. 17. A. M. Savchuk, On eigenvalues and eigenfunctions of Sturm-Liouville operators with singular potentials, Matem. Zametki (Math. Notes) 69 (2) (2001) 277-285. 18. A. M. Savchuk and A. A. Shkalikov, Sturm-Liouville operators with singular potentials, Matem. Zametki (Math. Notes) 66 (6) (1999) 897-912. 19. A. M. Savchuk and A. A. Shkalikov, The Sturm-Liouville operators with distributional potential, Trudy Mosk. Matem Ob-va (Trans. Moscow Math. Soc.) 64 (2003) 159-212.
Functional Analysis and its Applications V. Kadets and W. Zelazko © 2004 Elsevier B.V. All rights reserved
115
Incorrect Nonlocal Boundary Value Problem for Partial Differential Equations Volodymyr Il'kiv Lviv Polytechnic National University, Bandery str. 12, Lviv, Ukraine
Abstract The existence and uniqueness conditions of the pseudosolutions of a nonlocal twopoint boundary value problem for a system of PDE with continuous coefficients in Sobolev spaces are studying. Key words: Nonlocal boundary value problem, PDE, pseudosolutions, lagrangian function, small denominators 2000 MSC: 35G05, 35G15 The nonlocal boundary value problems for PDE, generally, are incorrect in the Hadamar sense. For example, the problem with two-point nonlocal conditions with respect to one selected variable in the Sobolev space scale has no solution or has a non unique solution [1-3]. Incorrectness of this problem can be explain by a null (nonuniqueness of solution) or arbitrary closely to null (nonuniqueness of solution) quantities which in the last case enter as multipliers into denominators of terms of Fourier series which represent a formal solution of the problem. For this reason these type of quantities will be called the small denominators, and the problem of their lower estimation was known since the XVIII century in the problem of celestial mechanics as the problem of small denominators [4]. By using the metrical approach to the problem of small denominators the nonlocal problem solvability in the Sobolev space scales [2, 5] for almost all coefficients in differential quantity of this problem has been established. This is true in particular for a such problem. Email address: [email protected] (Volodymyr Il'kiv).
116
Volodymyr Il'kiv
Let Q = [0, T] x dp be a cylindrical domain, where Q.p a p-dimensional torus, (t,x) G Q, x = (x\,... ,xp). In the domain Q we consider the following problem with nonlocal boundary conditions in time variable t for the canonical system of m partial n order differential equations
lu = y[BOl{D)%Z^\
where Lj(t,D)
°^
-
+BTJD)^J
I Qtn-3 s
= Yl LjS(t)D ,
^
"
I Qfn-j
)=V,
(2)
I
\ )
*,
LjS(t) are complex m-matrix coefficients contin-
M<j
= J2 lQjSDs, hj(D) = J2 hjSDs, kjs, hjs are nm x m kl with the inner product uous on [0,T],
ZOJ(-D)
fcezp
(ft,5), = (27r)P^fc2«r(fc)M*), fc€ZP
where g(x) =
XI d{k)e%(*k<x\ k = (/ci,... ,kp), (k,x) = fciXi + • • • + kpxp, % =
Jl + kj + • • • + fc^ a n d * denotes the Hermitian conjugate of matrix. We use the notation Hq for vector-function spaces of arbitrary dimension so that (h,g)g = (h>i,gi)q + (^2,52)9 for vector-functions h = col(/ii,/i2) and g = col (31,32) of the same dimension. We denote by iT™, 9 G M, n G N, the completion of the space, of infinitely differentiable finite sums v(t,x) = J2v(t,k)el(h>x^ by the norm, generated by the k
inner product T
{v w) n =
> *
TJ
^{WW),-^-
0 J=o
The spaces i? ? and if™ form the scales of spaces with respect to index q G R. If a vector-function
Incorrect Nonlocal Boundary Value Problem
117
F(Di,... ,DP) we shall mean the operator acting on the vector-function h(x) = Y, 'h{k)ei{-k'x"> e Hq by the rule fcez»
F(k)h{k)ei(k'x).
F(D)h(x) = J2 keif
By operations on these operators F(D) we mean the same operations on F(k) for k € Zp, in particular, the conjugate operator F*(D) is defined by the Hermitian conjugate matrix F* (k) and the scalar operator D is defined by the number sequence k, k £ Zp. A pseudoresolution of the problem (1), (2) will be found in the space H™+n, where q € R is the some fixed number. The operators L : H™+n —> Hq and I : Hq+n —•> Hq-1/2 are continuous, so that we may take the right-hand sides / and
Ru=\\Lu-n\fl on the set Ke(uo), namely
KE(HQ)
=
+ \\lu-
R(u). If
UQ =
0 then a pseudosolution
«eKe(u0)
with the minimal norm will be called the normal pseudosolution; if UQ ^ 0 then the ito-normal pseudosolution be called the pseudosolution minimizing \\v — Wo||9+n,n on the set of pseudosolutions of the problem (1), (2). Let u e Hf+n. Then g = Lu & H°, Cj = d^1u{0,x)/dp-1 e Hq+n_j+1/2, j = l , . . . , n , and C = C{x) = c o l ( C i , . . . ,Cn) G Hq+n_1/2 x ••• x Hq+1/2; the function u may be written as the solution of the Cauchy problem Lu = g,
dj~1u/dtj~l\t=o
= Cj, j = 1,... ,n, in the form u = FUU — FU\C + Fu2g, where t
= E{t,D)j£-l(TjD)g{T,x)dT, E(t,D) is the noro mal (on t = 0) fundamental system of solutions of the system (1), £(t,D) = col (E(t,D),dE{t,D)/dt,... ,dn-1E(t,D)/dtn~1), £~1{T,D) is a matrix formed l by the last m column of the matrix £~ (r, D). Similarly we obtain the following relations H°3Lu = FLU = FL1C + FL2g, Ful = E(t,D),
(Fu2g){t,x)
Hq 3 b-l'2lu H°BVu
= FtU = FnC + Fl2 g,
= col (Dnu, Dn-ldu/dt,...,
dnu/dtn)
where FL1 = 0, FL2 = Im, Fn = lo(D) + h(D)£(T,
= FVU = FVIC + FV2 g, D),
T 1
Fl2g = lT(D)£(T,D)j£- (T,D)g(T,-)dT, o
FV1 = col (Z,A)£(t,D),
118
Vo lodymyr II 'kiv t
(FV2 g){t, x) = col {Z, A)£(t, D) J £~1(T, D)g{r, x) dr + col (0, g{t, x)), o 2 Z = diag ( / > , . . . , D ,5), A= A(t,D)=(Ln(t,D),...,L1(t,D)), lo(D)=D-^2(lOn(D),...
,loi(D)), lT{D)=D-l'2{lTn(D),..
.,hi(D)).
The estimate error R(u) = TZ{U) can be represented in the form TZ(U) = \\FLU - f\\l0 + \\FiU -
< e}.
(3)
The problem (3) is a convex conditional minimization problem [7] in the space if ° norm on the linear set of elements col (FL,FI)U — £. For solving this problem we, can use the Lagrange multiplier method. Consider now the Lagrange function CU(U) = R(u) + u{\\u - u o l l ^ - e2) = = U{U) + LO(\\FVU - Vixoll^ - s2) = \\FU - ry||^0 - UJE2, where F — col (FL, F[, S/LOFV), r\ = col (^, ^/UJVUQ), LO > 0 is a Lagrange multiplier, saddle points of which (C/E, u>e) [7] will determine the solutions Ue of the problem (3). By the Kuhn-Tucker theorem [7] the saddle point (C/£, u>s) satisfies the following conditions: CUe(U£) = min{£Ue(C/) : LUU e H^+n}, (4) Lje(\\FvUs-Vuo\\lo-e2) = 0, \\FvUs-Vuo\\lo<e2. Let F* denote the conjugate operator to operator F, then r7-1*
/ TJ*
TTT*
/~,TP*\
(5)
( FL1 Fl\ V^Fvi ) L l
11
V
VI
and the operator F*F = F£FL + FfFi + cuFyFy is the positive definite operator since \\FU\\lo = {F*FU,U)qfi > u>\\FvU\\l0 = w||u||? +n , n > 0 for an arbitrary function 0 ^ u = LUU G H™+n. We construct the projector PF = F(F*F)~1F* onto the range of F to make the lower estimation of Lagrange function Cu{U) and find its minimal value for an arbitrary u> > 0. We obtain CU(U) = \\FU - PpvWlo + ||(7 - PF)V\\l0
- ue2.
The components of operator F* have the following form *ii=0,
F*L2 = Im,
F;i=l*o(D)+£*(T,D)l*T(D),
1
Fl*2=T£- *(t,D)£*(T,D)l*T(D), T
Kiv = ^
I£*(T,D)(Z,A*(T,D))v(r,-)dT, o
(6)
Incorrect Nonlocal Boundary Value Problem
119
T
1
(F^2v)(t,x) = £- *(t,D)J£*(T,D)(Z,A*(T,D))v(T,x)dT+(O,Im)v(t,x). t
Since FU - PFr] = F{U - {F*F)~1F*7j), from the formula (16) we obtain romCu{U) = Cu(Uu)ior ii
—F U
JJ — (F*F)~1 F*n
(7)
The function uu is a unique function that minimizes the Lagrangion function CU{U), in particular COJ{UU) < C^Fy^Vuo)
= R(u0) < oo.
(8)
Using formula (7) we also have uu =uo + FuFy1(G*G)~1G*£o
= u+ +coui,
(9)
where G = col (FL, Ft)Fy \ ^o = ? - col (Lu 0 , D"1/2Zw0) = £ - GVu0, G+ = lim (G*G + LO)~1G* = lim G{G*G + UJ)~1 is a pseudoinverse operator [7, 8] ofG. U " ° Theorem 1. If e < e0 = \\go\\2q+n,n, go = FuFylG+£,0 = u+ FuFylG+GVu0, then a pseudosolution of the problem (1), (2) exists, is unique, has the form uE = uUc = u0 + FuFy\G*G
+ to^G^o
= u+ + LUEU1E,
(10)
where uie is a solution of the algebraic equation \\uu — UQ\\ = e, uu = FUF~\G*G
+ LOE)-\VUO
- G+0, £
and is not the solution of the problem (1), (2), R(u ) > 0. If e > e$ then a pseudoresolution exists, generally, is not unique and has the form ue =u++ FuFy\l
- G+G)Q = uo + go + FuFy\l
- G+G)(Q - Vu0),
(11)
where Q is an arbitrary vector-function in space H® that satisfies the inequality \\(I— G+G){Q — Vwo)||^o —£2 ~£oi there exists a unique uo-normal pseudosolution ue = uo+go and a unique normal pseudosolution ue = u++/3FuFyl(I—G+G)Vuo, where (3 > 0 is some constant. If £ = GG+£, then pseudosolutions (11) are the solutions of the problem (1), (2); if the inverse operator G'1 exists, then the pseudoresolution (11) is unique and is the solution of the problem (1), (2). Proof. From (4) and (5) we find the saddle point of the Lagrangian function. The function UE = Uulc determined in (7) satisfies condition (4) for all value coe > 0. Choose u!e so that condition (5) is valid. Consider the function \\uu — uo||?,o = il-FVL^ — V«o||g,o = ||(G*G + u)~1G*t;o\\q,o which is continuous and strictly decreasing to zero as u> —> +oo; moreover, lim uu = UQ, lim « u = UQ + go, u—>+oo
uj—»+0
^o = IM| g +n,n may be a number if g0 G H£+n or e0 = +oo if g0 £ H"+n. For this
120
Volodymyr Il'kiv
reason when e < £o the equation \\uu — UQ\\ = e has a unique solution u> = u>£ and Ue = UUs. Relation (10) follows from (9) at the change us by a>£. The estimation error R(u) at the pseudosolution ue is
R(u°) = ||(7 - GG+)Z\\2g,0 + "1\\{G*G + u^fa
- (I - GG+)t)\\lo-
If R{uE) = 0, then (/ - GG+)£ = 0 and £0 = (I - GG+)£, namely £0 = 0 and 0 = ||G+£o||<2,o = So < £ that contradicts the condition 0 < e < SQ. Consequently, R(uE) > 0 namely any pseudosolution of the problem (1), (2) is its solution. When £ > EQ, the equation ||uw — ito||<j+ra,n = e has no solution and the condition (5) satisfies only at LU£ = 0. Then C0(U) = R(u) = \\GFVU - £\\2qfi and
£o(U) = R{u) = \\G(FVU-G+O\\l0 + \\(I-GG+)£\\lo > IIU-GG + )t\\lo- (12) If U£ = Fy^G+t) + Fyl{I - G+G)Q then for all vector-functions Q £ H° the minimum CQ{UE) = \\{I — GG+)^\\^0 vanishes. Choose among vector-functions Q satisfying condition (5) which means that for functions uE = FUUE = u0 + g0 + FuFy\l 2
- G+G)(Q - Vu0)
(13)
t h e inequality \\u* - uo\\ q+n,n = \\gO\\ q+n,n + \\(I - G+G)(Q - Vuo)\\lo < s 2 is satisfied, this implies the condition on vector-functions Q. For any pseudosolution (13) u£ ^ Uo + go we have the inequality e2 > \\us — u o\\2q+n,n > llffo||^+n,n = 4 = II(«o + 9o) - Uo||g+n,n hence uE = UQ+ g0 is the uo-normal pseudosolution. Compute the minimal value of the norm ||w £ || g+nin for the set of the functions (13) satisfying condition \\ue — uo\\q+n,n < £ to construct a normal pseudosolution. The Lagrangian function of this conditional minimization problem ||w£||^+n n + r2(||u£ — «o||^ +n n — £2) satisfies inequality
\\u%+ntn +
2
m\ns-uo\\2q+n^-e2)>
> ( T ^ ^ I K 7 - G+G)Vuo\\lo + \\G+Z\?qfl + n(e2 - e2), so that when (/ - G+G)Q = n\\{I - G+G)Vuo\\lo/(l + ft), namely ue = u0 + l go - FuFy (I - G+G)Vuo/(l + ft) it transformed into equality. If a = \\(I G+G)Vuo\\qfi — \Je2 — £g > 0, then ft = ft£ = a/\Js2 — e\ determines the Lagrangion multiplier with the help of which me construct the desired normal pseudosolution ue = u+ + %==FuFy\l - G+G)Vu0. 2 a + A / £ - £g If a < 0 then normal pseudosolution us — u+ corresponds to zero Lagrangian multiplier. Putting j3 = max(0,1 — \Je2 — SQ)/\\(I — G+G)Vuo\\q,o w e obtain the desired normal pseudosolution. An equality R(u£) = 0 results from (12), when £ = GG+t;, namely pseudosolutions (13) have been the solutions of the problem (1), (2). If operator G" 1 exists, then G+G = I, G~l = Fv{co\{FL, Fi))'1 and formula (12) and (13) imply that ue = uo + go = u+ = .FM(col (FL, Fi))~l£ is an unique solution of the problem (1), (2). The theorem is proved.
Incorrect Nonlocal Boundary Value Problem
121
The theorem results that the condition e < oo is a necessary condition of the existence of the solution of the problem (1), (2) in the space H™+n. The case e = oo indicates that this problem has small denominators and shows that the solution of this problem can exist only in the spaces of smaller smoothness and does not exist in the space H™+n. We note that other pseudosolutions may be obtained by using the minimization the weighted estimation error of the problem (1), (2), in particular one may examine the minimization problem of functional ||Lu — /||^ + r l n / 7 i + \\lu —
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Functional Analysis and its Applications V. Kadets and W. Zelazko © 2004 Elsevier B.V. All rights reserved
123
Singular Integral Operators with Flip and Unbounded Coefficients on Rearrangement-Invariant Spaces Alexei Karlovich a l a
Departamento de Matematica, Instituto Superior Tecnico, Av. Rovisco Pais 1, 1049-001 Lisboa, Portugal
Abstract We We obtain Fredholm criteria for singular integral operators of the form P++MbP_+MuUP-, where P± are the Riesz projections, U is the flip operator, and Mb, Mu are operators of multiplication by functions b, u, respectively, on a reflexive rearrangementinvariant space with nontrivial Boyd indices over the unit circle. We assume a priori that Mb is bounded, but Mu may be unbounded. The function u belongs to a class of, in general, unbounded functions that relates to the Douglas algebra H°° + C• Key words: Rearrangement-invariant space, Boyd indices, Douglas algebra H°° + C, outer function, Fredholmness, singular integral operator with flip 2000 MSC: 47A53, 46J15, 47B38, 48B60, 46B42
1. Introduction Let T be the unit circle equipped with the normalized Lebesgue measure m and let X := X(T,m) be a rearrangement-invariant space (for the definition and basic properties, see [1]). Rearrangement-invariant spaces are wide generalizations 1 The author is partially supported by F.C.T. (Portugal) grants POCTI/ 34222/MAT/2000 and PRAXIS/XXI/BPD/22006/99.
124
Alexei Karlovich
of Lebesgue spaces LP := L P (T, TO), 1 < p < oo, as well as Orlicz and Lorentz spaces. The domain of a linear operator T from X to X is denoted by T>(T). The set of all closed (bounded) linear operators from X to X is denoted by C(X) (respectively, B(X)). We shall denote by / the identity operator on X and by Ma the operator of multiplication by a measurable (not necessarily bounded) function a on T. The flip operator is defined by (U
:=t
(
The Cauchy singular integral of a function ip G L 1 is given by
(5^)(i) := lp.«. JT^z{dT
(t£T).
We will always assume that the rearrangement-invariant space X is reflexive and the Boyd indices a\,Px of X (see [3]) are nontrivial, i.e., ax,Px & (0,1). Lemma 1.1. (a) S, U G B{X) and U2 =I,S2 (b) Ma G B{X) if and only if a G L°°.
= I, SU = -US;
Proof, (a) Since S,U € B(LP) for p G (l,oo), by Boyd's interpolation theorem [3], S,U G B(X) whenever X has nontrivial Boyd indices. The equality U2 = I is obvious. The equality S2 = I is proved in [7, Lemma 6.5]. The equality SU = —US is proved similarly. Part (b) is proved in [10, Theorem 1]. • Put P+ := (I + S)/2 and P_ := (/ - S)/2. From Lemma l.l(a) it follows that Pl = P+,
P2=P-,
U2 = I,
P+U = UP-,
P-U = UP+.
(1)
For a linear operator T from X to X, we shall use the notation
R{T)
:=P++TP_.
Following [9], we study Fredholmness of singular integral operators with flip of the form R(A), where A := Mb + MUU, b G L°°, but the function u may be unbounded. We refer to [8, Ch. 3-4] for properties of operators in C(X) and to [2, Ch. 1], [5, Ch. 4] for the definition and properties of (bounded) Fredholm operators on Banach spaces. The paper is organized as follows. In Section 2, we prove that R(A) is closed whenever b G L 00 and u is measurable and a.e. finite. Further we study the invertibility of two auxiliary operators. In Section 3, we define the class A of, in general, unbounded functions u such that logw G L1 and uOl.~ belongs to the Douglas algebra H°° + C. Here u := max{l, \u\} and O1,~ is the outer function generated by 1/u. Then we prove the relative compactness of the Hankel operator P_MUP+ with respect to the operator MUP+ assuming u G A. By using this key result, we obtain Fredholm criteria for the operator R(A), where b G L°° and u G A.
Singular Integral Operators on Rearrangement-Invariant Spaces
125
2. Auxiliary results 2.1. Closedness of R{A) Lemma 2.1. If a is a measurable a.e. finite function on T, then Ma G C(X). Proof. The idea of the proof is borrowed from [4, Ch. 3, Theorem 9.2]. Clearly,
D(Ma) = {f e X : atpeX}. For each n G N, let Tn := {t G T : \a(t)\ < n}. Then OC
T n C T n + i,
| J Tn = T \ T^,
where T^ := {t G T : a(t) = oo}.
(2)
n=l
For every ip £ X and n G N, put
\fn\ < M,
Wn\ =
WXTM
neN.
Hence, by the lattice property (see [1, Ch. 1, Definition 1.1]), fn and a
G(f) = (f,g):=
f
fgdm,
Jt where / G X,g G X' and ||G|| X * = ||
JT
Hence, the operators Ma and Ma are adjoint to each other. Let us show that any other adjoint to Ma is a restriction of M-^. Assume T is an adjoint to Ma, that is, (Matp,g) = {
= (y>,xrn{Tg - M^g)} = 0.
Therefore, Tg = M-^g a.e. on T n for every g G V(T) and every n G N. Since w(Too) = 0) taking into account (2), we deduce that Tg = M-^g a.e. on T for every g G V(T). Thus, T is a restriction of M^, and M^ is the adjoint to Ma.
126
Alexei Karlovich
By [1, Ch. 1, Corollary 4.4], (X1)* = X" = X. In view of just proved, M« is densely defined in X' and (Ma)* = M= = Ma. Since Ma is densely defined in X1, its adjoint Ma is closed in X (see [8, Ch. 3, Section 5.4]). • L e m m a 2.2. If b g L°° and u is a measurable a.e. finite function on T, then R(A),MuP+eC(X). Proof. By Lemma 1.1, Mb,U,P-,P+ € B(X). Lemma 2.1 gives Mu € C(X). By using [8, Ch. 3, Section 5.2, Problems 5.6-5.7], we subsequently conclude that the operators MUU, MUP+, Mb + MUU, (Mb + MUU)P-, P+ + (Mb + MJJ)P- are closed. • If T g C(X), then its domain T>(T) becomes a Banach space with respect to the graph norm
\\f\\v(T):=\\f\\x
+ \\Tf\\x
(see, e.g., [8, Ch. 4, Section 1.1, Remark 1.4]). Hence, from Lemma 2.2 it follows that T>(R(A)) equipped with the graph norm is a Banach space. L e m m a 2.3. If b € L°° and u is a measurable a.e. finite function on T, then T>(R(A)) = V(MUUP-)
= V(P±MUUP-)
= UV(MUP+).
(5)
Proof. By Lemma 1.1, the operators P± and R(Mb) are bounded on X. Therefore, using the representation R(A) = R(Mb) + MUUP-,
(6)
we can easily obtain the equalities V(R(A)) = V(MUUP-) = V(P±MUUP-). equality V(R(A)) = UV(MUP+) is proved as in [9, Lemma 2.3]. •
The
2.2. Invertibility of some auxiliary operators Lemma 2.4. If b g L°° and u is a measurable a.e. finite function on T, then / - P+MUUP- : V(R(A)) -+ V(R(A)) is a bounded and continuously invertible operator. Its inverse is / +
(7) P+MUUP-.
The proof is straightforward. Consider the usual Hardy spaces Hp, 1 < p < oo, over T (see, e.g., [6]). For a nonnegative function $ with log
T
-^- log $ ( T ) dm{T)] , z G D := {C £ C : |C| < 1}- Z J It is analytic in D and has the crucial property that |O$| = $ a.e. on T. Moreover, 0 $ G H1 if and only if $ G L1 (see, e.g., [6, p. 62]). For a measurable function u on T, put u := max{l, \u\}. \JT T
Singular Integral Operators on Rearrangement-Invariant Spaces
127
Proposition 2.5. (a) If logw G L 1 , then O1/~ G H°°. (b) If logu G L \ F G tf\ and CKF G Z,1, then £>~F G ZZ1. (c) If logu G L1 and
= MOiLP+f,
P_MoaP+
(8)
Proof, (a) Obviously, logu G L1 if and only if log(l/w) G Z,1. Hence, O 1 ,~ is well defined whenever log u G L1. From the definition of u it follows that 1/u G L 00 C L 1 . Hence, O1/~ G L°° n iJ 1 = Zf °°. Part (a) is proved. (b) Obviously, O~O,,~ = 1. (9) Therefore, O~F = F/O, .— T h e denominator is in H1, in view of Part (a). By the '
u
i
1/u
\
'
/
j
assumption, the numerator is in H1 and the fraction is in L1. Hence, the fraction is in H1, due to [6, Ch. 5, Exercise 5, p. 75]. Part (b) is proved. (c) Hip e V(MUP+), then MuP+ip G X and P+
a.e. on T.
Then \MOilP+
(11)
is bounded and continuously invertible. Its inverse is R(UMOM) : V(R(A)) -> X.
(12)
Proof. The idea of the proof is borrowed from the proof of [9, Lemma 2.6]. If logu G L1, then u is a measurable and a.e. finite function. Hence, by Lemma 2.2, R(A) is closed. Therefore, T>{R{A)) is a Banach space with respect to the graph norm. By Proposition 2.5(a), Olf~ G Zf°°. Then MOl/z,R(UMOl/M) G B(X). By using (1), (6), and Ol/~ G H°°, we get for
= R(Mb)R(UMOl/M)
+ MuMOl/MP-
(13)
Since b G L°°, we have R(M(,) G B(X), in view of Lemma 1.1. On the other hand, from properties of outer functions and the definition of u we get \uO1 ,~\ = \u\/u < 1 a.e. on T. Therefore, by the lattice property (see [1, Ch. 1, Definition 1.1]), ||MuMOl/a||B(x)
(14)
128
Alexei Karlovich
Thus, from (13) and (14) we deduce that the operator (11) is bounded and lmR{UMOiruU)dV{R{A)).
(15)
V{R{A)) c lmR(UMOirJJ).
(16)
Let us show that Assume that / G V{R(A)) C X. By Lemma 2.3, Uf G V{MUP+). Proposition 2.5(c) and (1), we get P+ UMoz UP- / = 0, Put ip := P+f + UMoJJP-f. R(UMOl/.U)
Therefore, by
P- UMOii UP- f = UMO~U UP-f.
(17)
Then from (1), (9), and (17) we obtain = P+f + UMOl/M2MoMP-f
= f.
Hence, (16) holds and
R(UMOl/.U)R(UMo.U)f = / ,
f£V(R(A)).
(18)
Analogously to (18), by using Proposition 2.5(a), one can show that R(UMozU)R(UMOl/iiU)
=
(19)
Equalities (18) and (19) imply that the operator (11) is invertible and its inverse is given by (12). Moreover, we have shown that the operator (11) is bounded (and, therefore, it is closed) and its image coincides with the range space (see (15) and (16)). From above and the closed graph theorem (see, e.g., [8, Ch. 3, Section 5.4, Problem 5.21]) it follows that the operator (12) is bounded. •
3. Fredholm theory 3.1. Relative compactness of Hankel operators By analogy with [9] define the class A := < u is measurable :
logu £ L1,
uOl/~€
Lemma 3.1. If u G A, then the operator P_MUP+ respect to the operator MUP+.
H°° + c\.
is relatively compact with
Proof. This lemma is proved by analogy with [9, Lemma 2.1]. Since P_ is bounded on X, we have V(MUP+) = V(P-MUP+). Let {ifn} C T>(MUP+) be a bounded sequence in X such that the sequence {MuP+(pn} is also bounded in X. Since P+ is bounded on X, the sequence {P+
Singular Integral Operators on Rearrangement-Invariant Spaces
129
for some constant C > 0 and all n € N. Thus, {ipn} is bounded in X. Taking into account (8) and (9), we obtain P-MuP+
= P_MuOl/sP+^n.
(20)
Since u £ A, we have u O ^ - G ff°° + C. By [2, Theorem 2.54], the operator P^-Muo1/^P+ is compact on L p for every p £ (l,oo). Hence, by [11, Corollary 1], it is compact on X. This means that, for the bounded sequence {i>n} C X, the corresponding sequence {P-Muo1/-P+t()n} contains a convergent subsequence. From (20) we deduce that the sequence {P-MuP-^
(21)
R(MbUMOl/M)
(22)
:X->X
are bounded; (b) the operator (21) is Fredholm if and only if the operator (22) is Fredholm. If one of these operators is Fredholm, then their indices coincide. Proof. This statement is proved similarly to [9, Lemma 2.7]. By analogy with (18) one can prove that R{MbUMOl/JJ)R{UMoJJ)y
= R{Mb)
(23)
(a) By Proposition 2.5(a), M O l / _ £ B(X). Due to Lemma 1.1, Mb e B{X). Thus, the operator (22) is bounded. On the other hand, by Lemma 2.6, the operator R{UMOJJ)
: T>(R(A)) -> X
(24)
is also bounded. From above and (23) we infer that the operator (21) is bounded too. Part (a) is proved. (b) By Lemma 2.6, the operator (24) is invertible. Therefore, by [5, Ch. 4, Theorem 6.1], from (23) we conclude that the operators (21) and (22) are Fredholm only simultaneously and their indices coincide. • Lemma 3.3. If 6 £ L°° and u £ A, then the operator R(A) : V(R{A)) -» X
(25)
is Fredholm if and only if the operator (21) is Fredholm. If one of these operators is Fredholm, then their indices coincide.
130
Alexei Karlovich
Proof. This statement is proved by analogy with [9, Lemmas 2.4 and 2.5]. By Lemma 3.1, the operator P-MUP+ is relatively compact with respect to the operator MUP+. From this fact and the definition of relative compactness (see [8, Ch. 4, Section 1.3]) one can easily obtain that the operator P_MUUP- = P-MUP+U is relatively compact with respect to the operator MUP+U = MUUP^.. Due to Lemma 1.1, R{Mt>) is bounded on X. Therefore, it is not difficult to prove that the operator P^MUUP~ is relatively compact with respect to the operator R(A) = R(Mb) + MUUP_. Hence, the operator P_MUUP- is also relatively bounded with respect to the operator R(A) (see [8, Ch. 4, Section 1.3]). Thus, the operator P_MUUP- : T>(R(A)) —• X becomes bounded and compact (see [8, Ch. 4, Section 1.1, Remark 1.4 and Section 1.3, Remark 1.12]). By [5, Ch. 4, Theorem 6.3], the operator (25) is Fredholm if and only if the operator R(A) - P-MUUP- : V(R{A)) -> X
(26)
is Fredholm and the indices of (25) and (26) coincide. From (1), (5), and (6) we get for any
(R{A) - P-MUUP~)(I
- P+MuUP-)
(27)
In view of Lemma 2.4, the operator (7) is bounded and continuously invertible. From above and (27) it follows that the operator (26) (and thus, the operator (25)) is Fredholm if and only if the operator (21) is Fredholm. In that case the indices of the operators (25), (26), and (21) coincide (see [5, Ch. 4, Theorem 6.1]). • Now we are in a position to prove the main result of this paper. Theorem 3.4. If b G L°° and u G A, then the operator (25) is Fredholm if and only if u G L°° and the operator R(Mb) : X ^ X
(28)
is Fredholm. If one of these operators is Fredholm, then their indices coincide. Proof. The proof is developed by analogy with [9, Theorem 2.8]. Necessity. By Lemma 3.2(a), the operator (21) is bounded. If the operator (25) is Fredholm, then the operator (21) is Fredholm, due to Lemma 3.3. Therefore, by Lemma 3.2, the operator (22) is bounded and Fredholm. Hence, by [7, Theorem 6.8], essmi\b(t)O1/Z(l/t)\>0. Then 0 < e s s i n f O,,~(l/t)
= essinf (l/u(t))
= (esssupw(£))
The latter condition is obviously equivalent to u G L°°. Therefore, u G L°°. In this case R(A) is bounded on X. Thus, V{R(A)) = X. So, the operator (28) is Fredholm. The necessity part is proved. Sufficiency. Assume that u G L°° and the operator (28) is Fredholm. Then the first condition guarantees that R(A) G B{X), and so, V(R(A)) = X. This means
Singular Integral Operators on Rearrangement-Invariant Spaces that the operator (28) coincide with the operator (25) is Fredholm and its index coincide with the Theorem 3.4 generalizes [9, Theorem 2.8]. It Lp, 1 < p < oo, because the class A is essentially
131
(21). By Lemma 3.3, the operator index of the operator (28). • is new even for Lebesgue spaces wider than the class
QC+ := {/ is measurable : logu € Ll, uOx/~ G (H°° + C) f) (H55 + C ) } , which was considered in [9]. References 1. C. Bennett, R. Sharpley, Interpolation of Operators, Pure and Applied Mathematics 129 Academic Press, Inc., Boston, MA, 1988. 2. A. Bottcher, B. Silbermann, Analysis of Toeplitz Operators, Springer-Verlag, Berlin, 1990. 3. D. W. Boyd, Indices of function spaces and their relationship to interpolation, Canad. J. Math. 21 (1969), 1245-1254. 4. D. E. Edmunds, W. D. Evans, Spectral Theory and Differential Operators, Oxford Mathematical Monographs. Oxford Science Publications. The Clarendon Press, Oxford University Press, New York, 1987. 5. I. Gohberg, N. Krupnik, One-dimensional Linear Singular Integral Equations, Vol. 1. Operator Theory: Advances and Applications, 53. Birkhauser Verlag, Basel, Boston, Berlin, 1992. Russian original: Shtiintsa, Kishinev, 1973. 6. K. Hoffman, Banach Spaces of Analytic Functions, Dover Publications, Inc., New York, 1962. 7. A. Karlovich, Singular integral operators with piecewise continuous coefficients in reflexive rearrangement-invariant spaces, Integral Equations and Operator Theory 32 (1998) 436-481. 8. T. Kato, Perturbation theory for linear operators, Springer-Verlag, Berlin, 1995. 9. V. G. Kravchenko, A. B. Lebre, G. S. Litvinchuk, F. S. Teixeira, Fredholm theory for a class of singular integral operators with Carleman shift and unbounded coefficients, Math. Nachr. 172 (1995) 199-210. 10. L. Maligranda, L.-E. Persson, Generalized duality of some Banach function spaces, Nederl. Akad. Wetensch. Indag. Math. 51 (1989) 323-338. 11. R. Sharpley, Interpolation theorems for compact operators, Indiana Univ. Math. J. 22 (1972/73) 965-984.
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Spectrum as the Support of Functional Calculus Vladimir V. Kisil 1 School of Mathematics, University of Leeds, Leeds LS2 9JT, UK
Abstract We investigate the new definition of analytic functional calculus in the terms of representation theory o/SL(2,R). We avoid any usage of its algebraic homomorphism property and replace it by the demand to be an intertwining operator. The related notion of spectrum and spectral mapping theorem are given. The construction is illustrated by a simple example of calculus and spectrum of non-normal nxn matrix. Key words: Functional calculus, spectrum, intertwining operator, spectral mapping theorem, jet spaces 2000 MSC: 47A60, 46H30
0. Introduction United in the trinity functional calculus, spectrum, and spectral mapping theorem play the exceptional role in functional analysis and could not be substituted by anything else. All traditional definitions of functional calculus are covered by the following rigid template based on algebra homomorphism property: Definition 1. An functional calculus for an element a € 21 is a continuous linear mapping ^> : ^4 —> 2t such that 1
On leave from Odessa University.
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Vladimir V. Kisil
(i) $ is a unital algebra homomorphism $(/•) = $ ( / ) • $(5)(ii) There is an initialisation condition:
(1)
However the power of the classic spectral theory rapidly decreases if we move beyond the study of one normal operator (e.g. for quasinilpotent ones) and is virtually nil if we consider several non-commuting ones. Sometimes these severe limitations are seen to be irresistible and alternative constructions, i.e. model theory [10], were developed. Yet the spectral theory can be revived from a fresh start. While three components—functional calculus, spectrum, and spectral mapping theorem—are highly interdependent in various ways we will nevertheless arrange them as follows: (i) Functional calculus is an original notion defined in some independent terms; (ii) Spectrum (or spectral decomposition) is derived from previously defined functional calculus as its support (in some appropriate sense); (iii) Spectral mapping theorem then should drop out naturally in the form (1) or some its variation. Thus the entire scheme depends from the notion of the functional calculus and our ability to escape limitations of Definition 1. The first known to the present author definition of functional calculus not linked to algebra homomorphism property was the Weyl functional calculus denned by an integral formula [1]. Then its intertwining property with afHne transformations of Euclidean space was proved as a theorem. However it seems to be the only "non-homomorphism" calculus for decades. The different approach to whole range of calculi was given in [4] and developed in [7] in terms of intertwining operators for group representations. It was initially targeted for several non-commuting operators because no non-trivial algebra homomorphism with a commutative algebra of function is possible in this case. However
Spectrum as the Support of Functional Calculus
135
it emerged later that the new definition is a useful replacement for classical one across all range of problems. In the present note we will support the last claim by consideration of the simple known problem: characterization a n x n matrix up to similarity. Even that "freshman" question could be only sorted out by the classical spectral theory for a small set of diagonalisable matrices. Our solution in terms of new spectrum will be full and thus unavoidably coincides with one given by the Jordan normal form of matrix. Other more difficult questions are the subject of ongoing research.
1. Another Approach to Analytic Functional Calculus Anything called "functional calculus" uses properties of functions to model properties of operators. Thus changing our viewpoint on functions we could get another approach to operators. We start from the following observation reflected in the almost any textbook on complex analysis: Proposition 4. Analytic function theory in the unit disk D is a manifestation of the mock discrete series representation p\ o/SL(2,K): Pi(g) • f(z) ~ —^-r
^ r ) . a-0z f (\a-(3zj
a P \_p ~ a)J e SL(2,K).
where (
(2)
The representation (2) is unitary irreducible when acts on the Hardy space H2. Consequently we have one more reason to abolish the template Definition 1: H2 is not an algebra. Instead we replace the homomorphism property by a symmetric covariance: Definition 5. An analytic functional calculus for an element a £ 21 and an 21module M is a continuous linear mapping <& : .4(0) —> A(O, M) such that (i) $ is an intertwining operator $Pi = Pa* between two representations of the SL(2, R) group p\ (2) and pa defined bellow in (9). (ii) There is an initialisation condition: $[VQ] = m for VQ(Z) = 1 and m G M, where M is a left 2l-module. Note that our functional calculus released form the homomorphism condition can take value in any left 2t-module M, which however could be 21 itself if suitable. This add much flexibility to our construction. The earliest functional calculus, which is not an algebraic homomorphism, was the Weyl functional calculus and was defined just by an integral formula as an oper-
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Vladimir V. Kisil
ator valued distribution [1]. In that paper (joint) spectrum was defined as support of the Weyl calculus, i.e. as the set of point where this operator valued distribution does not vanish. We also define the spectrum as a support of functional calculus, but due to our Definition 5 it will means the set of non-vanishing intertwining operators with primary subrepresentations. Definition 6. A corresponding spectrum of a G 21 is the support of the functional calculus <£, i.e. the collection of intertwining operators of pa with prime representations [3, § 8.3]. More variations of functional calculi are obtained from other groups and their representations [4,7].
2. Background in Complex Analysis from SL(2,R) Group To understand the functional calculus from Definition 5 we need first to realise the function theory from Proposition 4, see [5,6,8,9] for more details. Elements of SL(2, R) could be represented by 2 x 2-matrices with complex entries such that:
,-(a\
9-=f
a
i . W-itf-..
\-/3 a)
\-0aJ
There are other realisations of SL(2,R) which may be more suitable under other circumstances, e.g. in the upper half-plane. We may identify the unit disk D with the left coset T\SL(2, R) for the unit circle T through the important decomposition SL(2,R) ~ T x B with K = T—the only compact subgroup of SL(2, M.):
where u> = arga,
u=
flct~l,
\u\ < 1.
Each element g £ SL(2,R) acts by the linear-fractional transformation (the Mobius map) on D and T H2(T) as follows: -i g
:z^
*Z~P —,
a-(3z
x. where
-i g
("
~P\
=
.
\_p aJ
,A^ (4)
Spectrum as the Support of Functional Calculus
137
In the decomposition (3) the first matrix on the right hand side acts by transformation (4) as an orthogonal rotation of T and D; and the second one—by transitive family of maps of the unit disk onto itself. The standard linearization procedure [3, § 7.1] leads from Mobius transformations (4) to the unitary representation p\ irreducible on the Hardy space:
*G0 • /(*) - ~ \ f (^l)
where ^ = [& A .
(5)
Mobius transformations provide a natural family of intertwining operators for p\ coming from inner automorphisms of SL(2,K) (will be used later). We choose [7,8] K-invariant function vo(z) E 1 to be a vacuum vector. Thus the associated coherent states v{g, z) = pi(g)vo(z) = (u-
z)~l
are completely determined by the point on the unit disk u = (3a~x. The family of coherent states considered as a function of both u and z is obviously the Cauchy kernel [5]. The wavelet transform [5,7] W : L 2 (T) -> H2(B) : f{z) i-> Wf(g) = (/, vg) is the Cauchy integral:
yVf
^ = hff^zdz-
(6)
T
Other classical objects of complex analysis (the Cauchy-Riemann equation, the Taylor series, the Bergman space, etc.) can be also obtained [5,8] from representation pi but are not used and considered here.
3. Representations of SL(2,K) in Banach Algebras A simple but important observation is that the Mobius transformations (4) can be easily extended to any Banach algebra. Let 21 be a Banach algebra with the unit e, an element a £ 21 with ||a|| < 1 be fixed, then g:a^g-a
= (aa-Pe){ae-(3a)-\
5
GSL(2,M)
(7)
is a well defined SL(2,R) action on a subset A = {g-a \ g G SL(2,M)} C 21, i.e. A is a SL(2,]R)-homogeneous space. Let us define the resolvent function R(g,a) : A —> 21 by the familiar formula R(g, a) — (ae — (3a)~l then fli(fli, a)i*i(s 2 , s r ' a ) =
fli(fli(fe,a).
(8)
The last identity is well known in representation theory [3, § 13.2(10)] and is a key ingredient of induced representations. Thus we can again linearise (7) (cf. (5)) in the space of continuous functions C(A,M) with values in a left 2t-module M, e.g.M = 21:
138
Vladimir V. Kisil Pa(gi) •• f(g~X • a) i-> R{gi1g~1,a)f(g^1g~1
• a)
(9)
For any m £ M we can again define a if-invariant vacuum vector as fm(c;~1 • a) = m ® v$(g~l -a) S C(A, Af). It generates the associated with vm family of coherent states vm(u,a) = (we — a)~1m, where u £ ED. The wavelet transform defined by the same common formula based on coherent states (cf. (6)):
Wmf(g) = {f,Pa(g)Vm), is a version of Cauchy integral, which maps L2(A) to C(SL(2,R),M). It is closely related (but not identical!) to the Riesz-Dunford functional calculus: the traditional functional calculus is given by the case: $:/>->• W m /(0)
for M = 21 and m = e.
The both conditions—the intertwining property and initial value—required by Definition 5 easily follows from our construction.
4. Jet Bundles and Prolongations of px Spectrum was defined in 6 as the support of our functional calculus. To elaborate its meaning we need the notion of a prolongation of representations introduced by 5. Lie, see [11,12] for a detailed exposition. Definition 7. [12, Chap. 4] Two holomorphic functions have nth order contact in a point if their value and their first n derivatives agree at that point, in other words their Taylor expansions are the same in first n + 1 terms. A point (z,«(")) = (z,u,ui,...,«„) of the jet space J" ~ D x C n is the equivalence class of holomorphic functions having nth contact at the point z with the polynomial: . . (w — z)n (w — z) PnM=Unj - - + • • • + Ml 1 , ' + U. n! 1!
, . 10
For a fixed n each holomorphic function / : D —> C has nth prolongation (or n-je£)Jn/:B-^C™ + 1 :
U(z) = (f(z),f'(z),...JinHz)). The graph r l
(11)
of j n / is a submanifold of JT" which is section of the jet bundle over
ED with a fibre C n + 1 . We also introduce a notation Jn for the map Jn : f' <-* T^J1' of a holomorphic / to the graph Tj1 of its n-jet j n / ( z ) (11).
Spectrum as the Support of Functional Calculus
139
One can prolong any map of functions ip : f(z) H-» [tpf](z) to a map ip^ of n-jets by the formula ^n\jnf) = Jn^f)-
(12)
For example such a prolongation p™ of the representation p\ of the group SL(2,R) in H2{p) (as any other representation of a Lie group [12]) will be again a representation of SL(2,R). Equivalently we can say that Jn intertwines pi and pj : JnPi(g) = p[n)(g)Jn
for all g G SL(2,R).
Of course, the representation p™ is not irreducible: any jet subspace Jfc, 0 < k < n is p]™ -invariant subspace of JJn. However the representations p^ are primary [3, § 8.3] in the sense that they are not sums of two subrepresentations. The following statement explains why jet spaces appeared in our study of functional calculus. Proposition 8. Let matrix a be a Jordan block of a length k with the eigenvalue A = 0, and m be its root vector of order k, i.e. ak~1m ^ akm = 0. Then the restriction of pa on the subspace generated by vm is equivalent to the representation PI
5. Spectrum and the Jordan Normal Form of a Matrix Now we are prepared to describe a spectrum of a matrix. Since the functional calculus is an intertwining operator its support is a decomposition into intertwining operators with prime representations (we could not expect generally that these prime subrepresentations are irreducible). Recall the transitive on D group of inner automorphisms of SL(2,R), which can send any A G D to 0 and are actually parametrised by such a A. This group extends Proposition 8 to the complete characterisation of pa for matrices. Proposition 9. Representation pa is equivalent to a direct sum of the prolongations p\ of p\ in the kth jet space Jfc intertwined with inner automorphisms. Consequently the spectrum of a (defined via the functional calculus $ = Wm) labelled exactly by n pairs of numbers (Aj, ki), A; £ D, i;, 6 Z + , 1 < i < n some of whom could coincide. Obviously this spectral theory is a fancy restatement of the Jordan normal form of matrices. Example 10. Let Jfc (A) denote the Jordan block of the length k for the eigenvalue A. On the Fig. 1 there are two pictures of the spectrum for the matrix
140
Vladimir V. Kisil
Fig. 1. Classical spectrum (a) of a matrix vs. the new version (b) with its mapping (c).
a = J 3 (Ai) © J 4 (A2) © Jx (A3) © J 2 (A 4 ), where
Ai = ^e-/ 4 ,
A2 = ^
6
,
A3 = j^e"^ 4 , A4 = jje"-/ 3 .
Part (a) represents the conventional two-dimensional image of the spectrum, i.e. eigenvalues of a, and (b) describes spectrum spa arising from the wavelet construction. The first image did not allow to distinguish a from many other essentially different matrices, e.g. the diagonal matrix diag(Ai, A2, A3, A 4 ), which even have a different dimensionality. At the same time the Fig. l(b) completely characterise a up to a similarity. Note that each point of spa on Fig. l(b) corresponds to a particular root vector, which spans a primary subrepresentation.
6. Spectral Mapping Theorem As was mentioned in the Introduction a resonable spectrum should be linked to the corresponding functional calculus by an appropriate spectral mapping theorem. The new version of spectrum is based on prolongation of pi into jet spaces (see Section 4). Naturally a correct version of spectral mapping theorem should also operate in jet spaces. Let 4> : ID —> D be a holomorphic map, let us define its action on functions [4>*f](z) = f((j>(z)). According to the general formula (12) we can define the prolongation <j)* onto the jet space J n . Its associated action Pi4>* = 4>* Pi o n the pairs (A, k) is given by the formula:
^*>=(*(^d^]).
<13>
where degA <j> denotes the degree of zero of the function >(z) — 0(A) at the point z = X and [x] denotes the integer part of x.
Spectrum as the Support of Functional Calculus
141
Theorem 11 (Spectral mapping). Let 4> be a holomorphic mapping <j): D —*• D and its prolonged action 4>i defined by (13), then sp
The explicit expression of (13) for 4>i , which involves derivatives of <j> upto nth order, is known, see for example [2, Thm. 6.2.25], but was not recognised before as form of spectral mapping. Example 12. Let us continue with Example 10. Let
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Generalized Normality in Topological Products and Related Structures 1 Anatoli P. Kombarov and Andrew N. Yakivchik* Faculty of Mechanics and Mathematics, Moscow State University, Moscow 119992, Russia
Abstract We survey recent progress in generalizing the results that provide necessary conditions for (hereditary) normality of topological products, hyperspaces, function spaces and other structures (these results include the well-known theorems by Katetov, Zenor, Noble, Tamano, Keesling-Velichko) to the case where the normality is replaced with a more general property. Key words: Topological product, Exponential space, Function space, Normal functor, Weak normality, 5-normality, 'P-normality, Subnormality 2000 MSC: 54B10, 54B20, 54C35, 54D15
Introduction The property of normality of a topological space, being, unlike weaker separation axioms up to Tychonoff's T 3 i , neither productive nor hereditary, is involved in a plenty of remarkable results: a fairly strong and important topological property is often implied by the normality of some topological products, their subspaces, or other structures (hyperspaces etc.); they are recalled in the sequel. * Corresponding author. Email addresses: kombarovSmech.math.rnsu.su (Anatoli P. Kombarov), anyak9mech.math.msu.su (Andrew N. Yakivchik). 1 The work was supported by Russian Foundation for Basic Research.
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Anatoli P. Kombarov, Andrew N. Yakivchik
The problem that we will discuss here is: What happens to these results when normality is replaced with a more general property? It is worth to note that there are different ways of generalizing the property of normality, particularly because of its dual nature: indeed, equivalently any two disjoint closed sets are separated by putting them into disjoint open sets, and by mapping them into 0 and 1 by a continuous real-valued function (by virtue of the well-known Urysohn lemma). One can consider the following ways to generalize the normality: (i) relax the requirement on the separating function (weak normality), (ii) restrict the class of closed sets to be separated (5-normality, V-normality), (iii) allow the separating sets to be more general than the open ones (subnormality). Below we recollect some recent results in this trend obtained within the last few years. Some open problems are pointed out. Most of the special topological notions relevant to our subject are recalled in course of the paper and indexed at the end. For the explanation of other terms not defined here, see [6] or [18].
1. Weak normality Throughout this section, all spaces are assumed to be Tychonoff. Definition 1 ([1]). Let V be a class of spaces (resp. Z be a space). A space X is weakly normal over the class V (resp. over Z) if for any two closed sets A,B C X such that A (1 B = 0 there exists a continuous mapping f:X —> Y = f(X) G V (resp. f-.X^-Z) such that f{A) n f(B) = 0. By default, V is the class of separable metric spaces (resp. Z = R"). The concept of weak normality was introduced by A.V. Arhangel'skii in connection with the theory of cleavable spaces. A space is cleavable (over V, over Z) if arbitrary disjoint sets A, B are taken to disjoint sets in R" (in Y € V, in Z)]. The (standard) cleavability of a space X has an important application in functional analysis; it is equivalent to the possibility of pointwise approximation of an arbitrary real-valued function on X by a countable family of continuous functions, see [2]. By the Urysohn lemma, every normal space is weakly normal (over M). Also, cleavable spaces are evidently (hereditarily) weakly normal. Remark 2. Weak normality is preserved neither by discrete sums (of more than c spaces, see [33]) nor by perfect mappings.
Generalized Normality in Topological Products
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1.1. Tamano's theorem on X x 0X Tamano's theorem of 1960 (from [29]) says: A space X is paracompact iff the product X x (3X (X x bX for some/every compactification bX of X) is normal. A.N. Yakivchik proved [33] that this result holds true when the normality is relaxed to the weak normality (even over the class of metrizable spaces). Theorem 3. For a space X and its (arbitrary) compactification bX, if X x bX is weakly normal over the class of all metrizable spaces then X is paracompact. Recall that the Hewitt-Nachbin number q{X) does not exceed r if the remainder f3X \ X is the union of G r -sets in f3X; thus, q(X) < LO means the realcompactness oiX. Theorem 4 ([33]). Let X be a pseudocompact space andbX be its compactification. If X x bX is weakly normal over W then q(X) < r. The last theorem lets one easily find a space XT of weight r + which is not weakly normal over RT; namely, XT = r + x ( r + + l). Another result resembling Tamano's theorem was found by Y. Yajima [32] who characterized the Lindelofness of a space X as follows: Theorem 5. A space X is Lindelof iff the subspace (X x 0X) U (j3X x X) of {(3X)2 is normal. Problem 6. Is it possible to characterize Lindelof property by weak normality? 1.2. Morita's P-spaces K. Morita (1964) proved that, for a space X, the following are equivalent [21]: (i) X x M is normal for any metrizable space M; (ii) X is a normal P-space. We now recall Morita's definition of P-spaces. Definition 7 ([21]). A space X is called a P-space iff for any family of open sets GSo...sk C GSo...SkSk+1 C X, Si e S, there exist closed sets FSo..,Sk t h a t X = \Jkeuj GSo...Sk implies X = \Jk&ui FSo...Sk.
C GSo...Sk such
It is also appropriate to recollect two covering properties which are of special importance for studying normality and its generalizations. Definition 8. A space X is countably paracompact (resp. countably metacompact)
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Anatoli P. Kombarov, Andrew N. Yakivchik
if every countable open cover of X has a locally finite (resp. point-finite) open refinement. An equivalent formulation of the countable paracompactness of a space X is that every countable open cover {Gi}i&LJ of X has a closed refinement {Fi}iEuj where Fi c Gi. Hence, every normal P-space is countably paracompact. Problem 9. Suppose that X x M is weakly normal for every metrizable space M. Is it true that X is a P-space? Such a space X may appear to be neither normal nor countably paracompact, as shown by the following Example 10 ([33]). Let X = ((CJI + 1) x (u + 1)) \ {(wi,w)} be the Tychonoff plank. Then X x P is weakly normal for every first countable paracompact space P . 1.3. Products with the unit interval and Dowker spaces In 1951, C.H. Dowker [5] proved that, for a space X, the following are equivalent: (i) X is normal and countably paracompact; (ii) X x [0; 1] is normal; (iii) X x (u> + 1) is normal. Recall that a space X which is normal but not countably paracompact (hence X x [0; 1] fails to be normal) is called a Dowker space. For a survey of Dowker spaces see, e.g., [26]. Dowker's result cannot be verbally extended to the weak normality. It can easily be observed that for every weakly normal space X and every countable space K the product I x i f i s weakly normal. However, there is still a hope to accomplish this without clause (iii), i.e., for the products with a closed interval. Problem 11. If a space X is (weakly) normal, is then the product X x [0; 1] weakly normal? A good positive approximation to this problem was found by P. Szeptycki in 1995. The following two results are contained in [28]. Theorem 12. If X is weakly normal and countably metacompact then X x [0; 1] is weakly normal. Theorem 13. If Y = Ylieu^i ~^~ •*•) w^h the box product topology (M.E. Rudin's Dowker space, 1971, [25]) then Y x [0; 1] is weakly normal.
Generalized Normality in Topological Products
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1.4. Large powers N. Noble's theorem of 1971 [22] affirms that the normality is not multiplicative "in large": If X is a space and XT is normal for any cardinal T (for some r >
max{aJi,w(X)}) then X is compact. A.P. Kombarov [13] carried over this result to the weak normality. Theorem 14. If XT is weakly normal for any cardinal r (for some cardinal r > max{wi, w(X)}) then X is compact. The proof is based on the facts that, firstly, the space uf1 (A.H. Stone's example) is not weakly normal and, secondly, every countably compact weakly normal space is normal. 1.5. Hyperspaces For a space X, by exp(X) we mean the hyperspace of non-empty closed subsets of X endowed with the Vietoris topology. If X is a space such that exp(X) is normal, then X is compact. This result was proved by J. Keesling (under CH, [12]) and N.V. Velichko (in ZFC, [31]). It is known [10] that if exp(X) is normal then X is countably compact. Hence, the next theorem, due to Kombarov [14], is a strengthening of Velichko's theorem: Theorem 15. / / exp(X) is weakly normal and X is countably compact then X is compact. Actually, in Theorem 15 [Theorem 14] one needs weak normality of exp(X) over the class of all normal spaces where any countably compact subspace are closed (particular cases are metrizable spaces, normal sequential spaces) [and all points are Gg\. Nevertheless, the requirement of countable compactness of X in Theorem 15 cannot be omitted: obviously, exp(w) is weakly normal because it admits a one-toone continuous mapping onto the Cantor set D".
2. Other generalized normality properties All spaces considered from now on are Hausdorff. 2.1. S-normality Recall that a (necessarily closed) subset F of a space X is a regular Gs-set if it is the intersection of the closures of countably many open neighborhoods of F in X.
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Anatoli P. Kombarov, Andrew N. Yakivchik
Definition 16 (J. Mack [20]). A space X is 5-normal if for any two disjoint closed sets A,BcX where A is a regular G^-set, there exist disjoint open neighborhoods. Every countably paracompact space is <5-normal. Moreover, a space X is countably paracompact iff X x [0; 1] is 5-normal [20]. C. Good and I.J. Tree in [8] proved that there exist: 1) a (5-normal Moore space which is not countably paracompact; 2) a (5-normal space which is not countably metacompact.
2.2. V-normality
Definition 17 (A.P. Kombarov, 2000, [16]). Let V be a class of spaces. A space X is V-normal iff any two disjoint closed subsets one of which belongs to V have disjoint open neighborhoods. The property of P-normality becomes more general as V is taken narrower. If V is the class of all countable spaces, this property is the pseudonormality introduced by C.W. Proctor (1970, [24]). Compact-normality is equivalent to regularity. Every Tychonoff (5-normal space is Lindelof-normal, and hence a-compact-normal, pseudonormal.
2.3. Subnormality This is a generalized normality property introduced by T.R. Kramer in 1973 [17]. Definition 18. A space is subnormal if every two its disjoint closed subsets are contained in disjoint G<;-sets. Evidently, subnormality generalizes both normality and perfectness. Similar to the latter and unlike the former, it is inherited by countable unions of closed subsets. In 1998 Yajima [32] obtained the following generalization of Dowker's theorem: Theorem 19. A space X is countably subparacompact (or, equivalently, subnormal and countably metacompact) iff X x [0; 1] is subnormal. Recall that a space X is called countably subparacompact [17] if every countable open cover of X has a countable closed refinement.
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3. Hereditary generalized normality 3.1. Theorems by Katetov and Zenor and hereditary S-normality First, let us recall these two classical theorems: If X x Y is hereditarily normal then either every countable subset in X is closed or Y is perfectly normal (M. Katetov, 1948, [11]). If X x Y is hereditarily countably paracompact then either every countable discrete subset in X is closed or Y is perfectly normal (P. Zenor, 1971, [35]). In 1999, Kombarov [15] proved the following theorem, which is a common generalization of these results. Theorem 20. If X x Y is hereditarily S-normal then either all countable subsets in X are closed or Y is perfectly normal. In the same paper of 1948, M. Katetov [11] proved that if the cube X3 of a compact space X is hereditarily normal then X is metrizable. For the hereditary normality of the square X2, this was an open problem very famous and long-standing since, but finally its independence on ZFC has been proven. Counterexamples had been found under MA + -.CH (P. Nyikos, 1977, [23]) and in CH (G. Gruenhage and P. Nyikos, 1993, [9]); and only recently P. Larson and S. Todorcevic [19], using forcing techniques, proved the consistency of the affirmative solution. Some analogous results for hereditary 5-normality of products were published by Kombarov in 1999-2000. Theorem 21 ([15]). If X is a countably compact space and X3 is hereditarily S-normal then X is metrizable (and compact). Problem 22. Is a compact space X metrizable if X 3 is hereditarily pseudonormal? Theorem 23 ([16]). (MA + -.CH) If X is a countably compact space and X2 is hereditarily 5-normal then X is compact. The latter is deduced from Theorem 20 and the fact that a countably compact perfect regular space is compact under MA + -iCH. 3.2. Fa -6-normality We say that a space X has property Fa-V if every FCT-subset of X has V. Fcr-5-normality is a simultaneous generalization of normality and F^-countable paracompactness. Zenor's theorem of 1976 (see [36]) claims: If X x Y is i^-countably paracompact then either all countable discrete subsets of X are closed or Y is normal. It has
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been generalized as follows:
Theorem 24 (A.P. Kombarov, 1999, [15]). IfXxY
is Fa-8-normal then either
all countable subsets of X are closed or Y is normal and countably paracompact. This also yields the following generalization of the Keesling-Velichko theorem: Theorem 25 ([15]). If exp(X) is Fa-S-normal then the space X is compact. Note that S-normality does not suffice here, because exp(wi) is S-normal. Another application of Theorem 24 concerns spaces CP(X) of continuous realvalued functions in the topology of pointwise convergence (i.e., inherited from Tychonoff product topology of M.x). V.V. Tkachuk proved in [30] that if CP(X) is i^-countably paracompact then it is normal. Theorem 26 ([15]). If CP(X) is Fa-8-normal then it is normal. And, there is another generalization of Noble's theorem: Theorem 27 ([15]). If XT is Fa-5-normal for every cardinal r (for some r > max{tjJi,w(X)}) then X is compact. 3.3. Katetov's theorems and hereditary subnormality For hereditary subnormality of finite products, Yakivchik obtained the following results [34]: Theorem 28. Let r be an uncountable cardinal. If the product X x Y is hereditarily subnormal then either every subspace of X of cardinality < T has countable pseudocharacter or every closed subset ofY is a GT-set. Example 29. For any space P of cardinality u>i with at most one non-isolated point (in particular, for the compact space P = A{u){)), every finite power Pk is hereditarily subnormal. Problem 30. Let X be a compact space such that X2 (X 3 , Xk for finite k) is hereditarily subnormal. Is it then true that w(X) < a>i? That x(X) < LO\1 It can be observed that a compact space X such that X2 is hereditarily subnormal cannot have two different uncountable regular cardinals as local characters at points in closed subspaces of X.
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Problem 30 has quite recently got almost complete affirmative solution. T. Banakh proved [3] the following result (we formulate its particular case). Theorem (i) if X2 of X (ii) if X3
31. For a compact space X: is hereditarily subnormal then the hereditary Lindelof number hl(X) does not exceed ui\, and hence x(^0 < w i / is hereditarily subnormal then either X is perfectly normal or w{X) <
(Hi) if X4 is hereditarily subnormal then w(X) < u)\. It remains unknown whether the hereditary subnormality of X 3 for compact X implies the inequality w(X) < u>i. Theorem 32. Suppose that P is a regular space and P = Q U D where Q is an Fa-discrete space (i.e., the union of countably many discrete closed subspaces) and D is discrete expandable in P (i.e., there exists a discrete family {Vy}y££, of open subsets of P where Vy 3 y). Then the product X x P of a space X with P is hereditarily normal in each of the following cases: 1) X is hereditarily Lindelof; 2) X is metrizable. Problem 33. Is Theorem 32 true when X is hereditarily paracompact and perfectly normal? 3.4. Hyperspaces A well-known result of M.M. Choban (1971, see [4]) says: If exp(X) is hereditarily normal then X is a metrizable compact space. Some analog of this theorem happens to be true for the case of hereditary weak normality: Theorem 34 (A.P. K o m b a r o v , 1997, [13]). If X is a countably compact space and exp(X) is hereditarily weakly normal then X is a perfectly normal hereditarily separable compact space. Hence, if X is countably compact and exp(exp(X)) or exp(X x X) is hereditarily weakly normal then X is a metrizable compact space. Problem 35. Is a compact space X metrizable, if exp(X) is hereditarily weakly normal? Theorem 36 (A.P. Kombarov, 2000, [16]). (MA + -.CH) //exp(X) is hereditarily Lindelof-normal then X is a metrizable compact space.
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Problem 37. Does Theorem 36 hold in ZFC? 3.5. Normal functors For the definition of a normal functor (of degree n) and a survey of covariant functors, see [27]. M. Katetov's theorem on the cube was extended in 1989 by V.V. Fedorchuk [7] as follows: Theorem 38. If X is a compact space and T{X) is hereditarily normal where T is a normal functor of degree > 3 then X is metrizable. In 2000, the analogous result for the countably paracompact case was proved similarly by T.F. Zhuraev [37]: Theorem 39. If X is a compact space and J~(X) is hereditarily countably paracompact where T is a normal functor of degree > 3 then X is metrizable. A simultaneous generalization of the two previous results has been recently obtained by A.P. Kombarov: Theorem 40. Let X be a compact space and T be a normal functor of degree > 3. If J-{X) is hereditarily a-compact-normal then X is metrizable. Problem 41. In the last theorem, is it enough to assume that !F{X) is hereditarily pseudonormal? If exp 3 (X) is hereditarily tr-compact-normal and X is compact then X is metrizable. It does not suffice to consider countably compact X, because exp3(wi) is (even) hereditarily Lindelof-normal. 3.6. Hereditarily weakly normal products X x Y The results below have visual (rather than logical) relevance to Katetov's theorem. Theorem 42 (A.N. Yakivchik, 1997, [33]). Let r be an infinite cardinal. If X xY is hereditarily weakly normal over the class of all spaces with pseudocharacter < r then either every subset of X with cardinality < r is closed or every compact subspace of X has tightness < r. Theorem 43 ([33]). If X x T+ is hereditarily weakly normal over the class of all
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spaces with pseudoweight < T then every subset of X with cardinality < r is closed. References 1. A.V. Arhangel'skii, Divisibility and cleavability of spaces, in: Recent Developments of General Topology and its Applications. International Conference in memory of Felix Hausdorff, Math. Res. 67 (Akademie-Verlag, Berlin, 1992) 13-26. 2. A.V. Arhangel'skii, D.B. Shakhmatov, On pointwise approximation of arbitrary functions by countable families of continuous functions, Trudy Semin. Petrovskogo 13 (1988) 206-227 (in Russian). 3. T. Banakh, On topological spaces with hereditary subnormal product, preprint. 4. M.M. Choban, Note sur topologie exponentielle, Fund. Math. 171 (1971) 27-41. 5. C.H. Dowker, On countably paracompact spaces, Canad. J. Math. 3 (1951) 219-224. 6. R. Engelking, General Topology. Heldermann-Verlag, Berlin, 1989. 7. V.V. Fedorchuk, On Katetov's theorem on the cube, Moscow Univ. Math. Bull. 44 (4) (1989) 102-106. 8. C. Good and I.J. Tree, On 5-normality, Topology Appl. 56 (1994) 117-127. 9. G. Gruenhage and P. Nyikos,, Normality in X2 for compact X, Trans. Amer. Math. Soc. 340 (1993) 563-586. 10. V.M. Ivanova, On the theory of spaces of subsets, Dokl. Akad. Nauk SSSR 101 (1955) 601-603 (in Russian). 11. M. Katetov, Complete normality of Cartesian products, Fund. Math. 35 (1948) 271-274. 12. J. Keesling, On the equivalence of normality and compactness in hyperspaces, Pacific J. Math. 33 (1970) 657-667. 13. A.P. Kombarov, Weak normality of subsets of exp(X), Topology Appl. 76 (1997) 157-160. 14. A.P. Kombarov, Weak normality of 2X and XT, Fund. Prikl. Mat. 4 (1) (1998) 135-140 (in Russian). 15. A.P. Kombarov, On i^-^-normality and hereditary <5-normality, Topology Appl. 91 (1999) 221-226. 16. A.P. Kombarov, On Lindelof-normal spaces, Topology Appl. 107 (2000) 117122. 17. T.R. Kramer, A note on countably subparacompact spaces, Pacific J. Math. 46 (1973) 209-213. 18. K. Kunen and J.E. Vaughan, eds., Handbook of Set-Theoretic Topology. NorthHolland, Amsterdam, 1984. 19. P. Larson and S. Todorcevic, Katetov's problem, Trans. Amer. Math. Soc. 354 (2002) 1783-1791 (electronic). 20. J. Mack, Countable paracompactness and weak normality properties, Trans. Amer. Math. Soc. 148 (1970) 265-272. 21. K. Morita, Products of normal spaces with metric spaces, Math. Ann. 154 (1964) 365-382.
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22. N. Noble, Products with closed projections II, Trans. Amer. Math. Soc. 160 (1971) 169-183. 23. P. Nyikos, A compact nonmetrisable space P such that P2 is completely normal, Topology Proc. 2 (1977) 359-363. 24. C.W. Proctor, A separable pseudonormal nonmetrizable Moore space, Bull. Acad. Polon. Sci. 18 (1970) 179-181. 25. M.E. Rudin, A normal space X for which X x I is not normal, Fund. Math. 73 (1971) 179-186. 26. M.E. Rudin, Dowker spaces, in: K. Kunen and J.E. Vaughan, eds., Handbook of Set-Theoretic Topology (North-Holland, Amsterdam, 1984) 761-780. 27. E.V. Shchepin, Functors and uncountable powers of compacta, Soviet Math. Surveys 36 (3) (1981) 1-71. 28. P.J. Szeptycki, Weak normality in Dowker spaces, Topology Proc. 20 (1995) 289-296. 29. H. Tamano, On paracompactness, Pacific J. Math. 10 (1960) 1043-1047. 30. V.V. Tkachuk, Methods in the theory of cardinal invariants and the theory of mappings in application to function spaces, Siberian Math. J. 32 (1991) 93-107. 31. N.V. Velichko, On a space of closed subsets, Siberian Math. J. 16 (1975) 484486. 32. Y. Yajima, Analogous results to two classical characterizations of covering properties by products, Topology Appl. 84 (1998) 3-7. 33. A.N. Yakivchik, Weakly normal topological spaces and products, Topology Appl. 76 (1997) 193-201. 34. A.N. Yakivchik, Subnormality in subspaces of products, Topology Appl. 107 (2000) 197-205. 35. P. Zenor, Countable paracompactness in product spaces, Proc. Amer. Math. Soc. 30 (1971) 199-201. 36. P. Zenor, Countable paracompactness of FCT-sets, Proc. Amer. Math. Soc. 55 (1976) 201-202. 37. T.F. Zhuraev, Normal functors and the metrizability of compact Hausdorff spaces, Moscow Univ. Math. Bull. 55 (4) (2000) 6-9.
Functional Analysis and its Applications V. Kadets and W. Zelazko © 2004 Elsevier B.V. All rights reserved
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Nonstandard Universe based on Internal Set Theory Taras Kudryk a , Wladyslav Lyantse a and Vitor Neves b a
b
Lviv National University, 1 Universytetska st., 79602 Lviv, Ukraine Department of Mathematics, University of Aveiro, 3810-193 Aveiro, Portugal
Abstract This paper is an invitation to look what occurs when tools of Robinson's and Nelson's Nonstandard Analysis act simultaneously. For instance, in this case we have several kinds of infinitesimals in our disposal. Key words: Standard, internal, external, shadow, infinitesimal, galaxy, hull, Loeb measure 2000 MSC: 03H05, 46S20
1. Preliminaries We suppose that the reader is familiar with NSA (the Nonstandard Analysis of Robinson, see [9] or [2]) and 1ST (the Internal Set Theory of Nelson, see [6] or [4], or [5]). Multiple standardness was studied by E. Gordon and Y. Peraire in a series of interesting papers (see, for instance [3], [7], [8]). Note that none new definition of standardness is introduced in this article. You can see also the following papers [10], [11], or the book [12] discussing similar topics. To avoid misunderstandings let us fix notation and terminology. We determine the standard Mathematics as based on the ZFC (Zermelo-Fraenkel with Choice) set theory, but as the background of the whole Mathematics we accept Email addresses: tkudrykfifranko.lviv.ua (Taras Kudryk), wlancSlitech.lviv.ua (Wladyslav Lyantse), [email protected] (Vitor Neves).
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the Internal Set Theory (which includes the ZFC axiomes). Thus "to be standard" means "to be uniquely determined by tools of ZFC (without the predicate st = " to be standard" and related with st axioms of Idealization, Standardization and Transfer) and standard data". This is a recurrent definition with the empty set 0 as the beginning. We realize our considerations in some fixed model of set theory. The uniqueness of interpretation allows do not differ a symbol (name of an entity) and the entity itself. We emphasize that the 1ST recognizes internal sets only (i.e. such that are elements of standard sets). Since x G {x} and {x} is standard, whenever x is so, each standard item is internal. Write "si(x)" for "x is standard". A predicate of the ZFC-language without occurence of st(-) is called internal, whereas one which contains st(-) is called external. The subset construction B — {x G A : p(x)} in our 1ST Mathematics is allowed for A and p internal only. Nevertheless one uses the following denotation: st E := {x G E : st(x)}; stE (the collection of standard elements of the set E) is not a genuine set, but an "external" set. One uses stE to write formulas, for instance, "x G stE", "stE = stF, which mean respectively "x G E A st(x)", "(\/x)(st(x) => x G E <*=> x € F)", and so on. An internal predicate without occurence of nonstandard constants is said to be standard. (Obviously, standard predicates belong to the ZFC-language.) For a standard predicate p the Nelson's transfer principle holds: 3 j ; p(i) => 3 st x p(i),
V st ij)(i)=>Vxp(x);
(1-1)
understand "Bcc" as "for some internal x" and "Vx" as "for any internal x". An essential corollary of (1.1) is the following: st(E) A E ^ 0 => stE ± 0.
(1.2)
Notice also an essential corollary of the Nelson's idealization principle: st(E) A cardS > card N^E\stE st
^ 0.
(1.3)
st
The presence of nontrivial parts E and E \ E according to (1.2) and (1.3) is an important feature of the Internal Set Theory. Now a few words about the construction of the Robinson's Nonstandard Universe W and the Transfer Map *. Initial data for these are as follows: S - the set of individuals, 0, - the set of indices, T - a fixed free ultrafilter on 0,. We accept the following 1.1 Main assumption. The initial data S, 0, T are standard (in the sense of 1ST). Besides, in order that W and * be nontrivial we assume that cardO > cardS1 > cardN. Recall that the standard universe 5 is the superstructure S := \Jn€N Sn,
S0:=S,
V n G N Sn+l := Sn U 2 s ".
To each "block" Sn of S there corresponds a set *Sn defined by the conditions (i) each function / G S% determines an element / G *Sn, (ii) let h, h G S*?, then fx = f2 iff h =r f2 (i.e., {w G Q : A H = /2(w)} G 7),
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(iii) let / G ( 2 s " ) n , then / is the set of g G *Sn such that g e? f (i.e., {UJ G 0. :
g(u) G f(u)} S .F), (iv) for f € S$ f = {g E Sg : g =jr f} and *S 0 is the set of all such / . The nonstandard universe W is defined as the bounded ultrapower:
W:=S"/F = Unm*Sn. The transfer map * transforms S into W as follows: if E G Sn and n > 1, then *E := {/ G *S n _i : / £? E}; ii E £ So = S, then *E = / where / G *S 0 and / =jr E. *E is said to be the star-version of E G S. 1.2 Remark. On account of injectivity of the map * one can identify each individual with its star-version: VsGSo *S = S (1.4) But for n > 0 the restriction of * to Sn \ So is not surjective. That is why an E G S\S cannot be identified with its star-version *E. 1.3 Remark. It may well happen for two individuals that each one is an element of the other. (Recall that all items in Internal Set Theory are sets.) It is necessary to keep in mind that after identification (1.4) for s,t G S the formula s G t is meaningless. Indeed, both *s and *t are classes of functions, which excludes the relation *s G *t. Let a be an assertion of the ZFC-language which states something about E G S. Denote by *a the assertion obtained from a by the replacement of E by *E. Then the Robinson's transfer theorem holds: a <^=>* a.
(1.5)
For instance, for E G S \S define!? := {*x : x £ E}; ~E is the pointwise image of E by the map *. Theorem (1.5) implies that WE G S \ S~E C *E, but *E \"E ^ 0 -^=> cardi? > cardN. In the framework of NSAU is a counterpart of stE of 1ST. An essential corollary of assumption 1.1 is the following statement: 1.4 Proposition. The superstructure S, the ultrapower W, the transfer map * are standard (in the sense of 1ST). If E G s t ( 5 \ S), then *E and'E are standard. For instance, *Sn is standard for each n G st N. Notice that for n G N \ s t N Sn and *Sn are internal. 1.5 Warning. The terminology in Robinson's NSA is somewhat different, namely an E G W is said to be standard iff it is the star-version of some F G S. To avoid misunderstandings, we call an E G W such that E = *F, for some F G S, R-standard (standard in the sense of Robinson).
2. Numbers Let us look what numbers are available in the universe W constructed within 1ST. As usually, by N, Z, Q, R, C we denote standard sets of natural, integer, rational,
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real and complex numbers respectively. Their star-versions *N, . . . , *C are called respectively sets of hypernatural, . . . , hypercomplex numbers. For convenience assume that C c S . This implies st
CcC=Cc'C;
and similarly for N, . . . , K. Notice that (in our terminology) *N,..., *C are standard and s t N,..., st C are strictly external. Begin with naturals and hypernaturals. Consider each n G N as a (finite) ordinal, i.e. a transitive set, totally ordered by the membership relation G. So for n G N we have n := {0,... ,n — 1}. Since N C 5, in view of remark 1.3 this cannot be transferred to *N. But it can be used that the restriction of G to N is identical to the ordinary inequality relation <. Temporararily denote the last by X. We have X G S, therefore the star-version * I really exists. Because I c f t x N c S x S , X C *X and * I n (N x N) = X. These relation allow to denote X and *X by the unique usual symbol <. Since (N, <) is a linearly ordered set, by the transfer theorem (1.5) (*N, <) is also so. But (*N, <) is not totally ordered (though (N, <) is a totally ordered set). The cause is that for E G S \ S the star-version of 2E is not 2* £ , but *{2E) = 2'E n W. This involves that some sets A c *N can be simultaneously internal and R-external. For instance, the set *N \ N is standard, nonempty and does not contain a minimal number. Even for n G * N \ N the nonempty internal set {k G *N \ N : k < n} lacks the minimum. Call a number n G N \ s t N infinite, and a number n G *N \ N R-infinite (Robinson's infinite). Of course, if p is R-infinite, then Vn G N n < p. The main purpose of natural numbers is to be values of the measure card. Let E be some internal set and n G N. We write caidE = n iff there exists a bijection / G En (i.e. d o m / = n = {0, ...,n — 1}, i m / = E). By restricting the map card to S\S, we get card G S. Thus there exists a star-version "card G W; *card as well as card are standard. The domain of *card is W \*S. 2.1 Proposition. There exists a standard R-infinite hypernatural number. Proof. Since N and *N are standard, *N \ N is so. Because *N \ N ^ 0, by (1.1) (*N\N) ^ 0 .>
st
2.2 Remark. A standard n G *N \ N can be demonstrated explicitly. For / , g G N n define / =? g = {u) G fi : f(w) = g(uo)} G T. Then each / G N n uniquely determines a hypernatural number / , namely the equivalence class / := {g G N n : g =? / } . If / is essentially unbounded, i.e., (Vn G N) ({to Gil: f{u>) > n } e f ) , then / G *N \ N and / is standard whenever / Gst(Nn). > 2.3 Remark. A standard hypernatural number can be even greater than an Rinfinite one. Indeed, let n,p G s t ( * N \ N ) and n < p. If the set {x G *N : n < x < p} is infinite, for instance with p = n 2 , by Nelson's theorem (1.3) it contains nonstandard elements. It is easy to demonstrate such elements explicitly. Standard hypernaturals entirely fill in some galaxies.
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It is also interesting to mention the existence of e x t r a infinite hypernaturals, i.e. the existence of p G *N such that V n £ st (*N) n < p. This follows from the Idealization principle: VstflnX3y VxGX (xG*NAyG*NAx<2/)^ => 3yVxG s t (*N) (ye
*NAx
Pass to the reals and hyperreals. The arithmetical operations, the order and their star-versions are denoted identically by +, •, <. For x, y G *K define x « y = V n € s t N \x - y\ < - , I := {x G M : x ss 0}, (2.1) In x~y = VneN \x - y\ < -n , *I := {x G *R : x ~ 0}, (2.2) 1 st x « y = Vn G (*N)|x - yl < - , e I : = { i e * R : i « 0}. n Elements of I and *I (»I is not a star-version of I) are called respectively infinitesimals and R-infinitesimals, and ones of e I extra infinitesimals. *I is standard in the sense of 1ST whereas I and e I are strictly external. In view of the standard archimedean principle, we have Vx,yGR. x~y=>x = y.
(2.3)
Of course, V i e J Vy G I \» I |a;| < \y\. For x G *R define x|
F := {x G E : |z| < oo},
x| <* oo = 3n G N \x\ < n,
»F := {x G *E : |x[ <* oo},
st
x| < oo = 3 n G (*N) |x| < n, e¥ := {x G *R : |x| < oo}. Elements of the strictly external sets F ande F respectively are called finite and e x t r a finite. The set *F is standard and its elements are called R-finite. »F (F) is a subring of the ordered field *M (M) and *I (I) is an ideal of the ordered ring *F (F). Similarly for e I ande F. Permanence principles do not reach the sets of extra infinitesimals and extra finite numbers. It is known that for each x G F there exists a unique y Gs t R such that x « y. This y is called the shadow of x and denoted by °x. Also to each x G »F there corresponds a unique j / e R such that x ~ y. This y is called the R-shadow of x and denoted by °x. Thus, VXGF
°X G stM, X W °X,
VXG*F
°XGR, X ~ ° X .
(2.4)
2.4 Proposition. Let x G *K and \x\
Proof. If x G *R and |x|
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2.5 Remark. If x £ *M. and |x|
°x := [a;] +* (x - [x]).
(2.6)
st
Notice that *R = *Z + *[0,1[, Vx G *R °x G *Z + [0,1[, ° i « i , ° i e * Z + [0,1[, °x ~ x. The map x — i > °x is strictly external and x — i > °x is standard. 2.7 Proposition. (External) sets *R/ « and *Z + st[0,1[ are ordered additive groups. The extended shadow map is an isomorphism of theirs, i.e. Vx,y £ *R Vn G *Z °(x + n) = °x + n, °(x + y) = °x + °y, x < y => °x < °j/. Proof. Let x = m + £, where m £ *Z, ^ € *[0,1[. Then by (2.6) °x = m + °£. For n £ *1 we have [x + n] = TO + n. Therefore °(x + n) = m + n + °£, i.e. the first equality holds. Using it it is quite easy to prove the rest. >
2.8 Warning. In general °(xy) ^ °x°y. 2.9 Remark. By usual means one can form the set of standard hyperrationals from the set of R-infinite hypernaturals which is even more rich than Q but that is not the same that *Q.
3. Metric spaces In the sequel {X, d) will denote a standard metric space such that X is infinite and C U X C S. From this assumption it follows (see (1.4)) that stX C X = 'X C *X. *X and *d as well as X and d are standard. We write d instead of *d, because d C *d. For xi,x? £ *X define (see (2.1), (2.2)) x\ « xi = d(x\,X2) ~ 0, x\ ~ X2 = rf(xi,X2) ~ 0, xi « X2 = d(xi,X2) ~ 0. Notice that (2.3) implies Wxx,x2£X
x\ ~ x2 =>• xi = X2-
(3.1)
3.1 Remaric. We cannot consider (*X,d) as a metric space, because values of d on *X x *X are hyperreals. Nevertheless *X is a standard topological space with the topology *r which is the star-version of the topology r induced by the distance d on X. {*X, d) is said to be a hypermetric space. 3.2 Definition. For any x £ *X form equivalency classes h(x) := {£ £ X : £ « x}, */i(x) := {$ G *X : £ ~ x}, e /i(z) = {^ G *X : ^ « x}. The sets ft(x) and th(x) are called respectively the halo and the R-halo of x. eh(x) is the extra halo.
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3.3 Remark. Of course, the map *X 9 I H */I(X) G 2*x is standard. Therefore, if x G st(*X), then the R-halo *h(x) is standard. But for x G *X \ X it is possible that h(x) = 0. Notice that from (3.1) it follows that */i(x) n X = {x} whenever xeX. 3.4 Definition. Denote by X the quotient of *X relative to ~: X := *X/ ~ = {x : x G *X, x = *h(x)}. For Xi,x2 G X, £i G Xi, £2 € x2 put d(xi,x 2 ) := °d(£i>£2); here ° is the R-shadow map (see (2.6)). (The independence of d(xi, x2) from £i G Xi, £2 £ %2 follows from (3.1).) 3.5 Proposition. The function d is an almost distance, i.e. it has properties of a genuine distance except that its values are reals modulo *N. Proof, is an immediate check-up. Warning. The quotient X/ « cannot be formed in the framework of 1ST although it has a clear naive sense. 3.6 Remark. The almost distance d defines on X a standard separable topology f: a set E G 2X is f-open iff for each x G X there exists a real r > 0 (at least infinitesimal) such that for f G X the inequality d(£, x) < r implies £ G £. The standard topological space (X, r) is called the ns-hull of (X, cf). 3.7 Definition. Let / G *(XX) = W fl *X*X and x G *X. The function / is said to be R-continuous at the point x iff VfG*X
Z ~ x => f(0 Z f(x).
(3.2)
(Notice that it is well known that an R-standard function / is continuous at a R-standard point x G *X iff it is R-continuous at this point.) Let / G *(XX) be R-continuous at each point x G *X. For x G *X and ( 6 i : = »/i(x) put
/(*) :=nO-
(3-3)
It is clear that (3.3) determines / as a map X into X. This map is called the ns-hull of/. 3.8 Proposition. The ns-hull f of an R-continuous function f G *{XX) is continuous in respect to the topology f. Proof. Let £ be a positive real. For x G *X consider the set Exe of positive reals S such that d(x,0 < 5 implies d(f(£),f(x)) < s, i.e. from °d(£, x) < 5 it follows that 0 d(f(O> f(x)) < £- For (3.2) the set Ex^£ contains each positive R-infmitesimal 5. By R-overspill it contains some positive real S. > Consider another variant of continuity. Let (X,d), (Y,d) be standard metric spaces such that C U X U Y C 5. For a function / G Yx we have / C */, that is why we write / instead of */.
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3.9 Proposition. Suppose that f G si(Yx) VZ,£G*X
and
£ « x =• / ( 0
~ /(x).
(3.4)
Then f is constant on each connected component of X. Proof. For a fixed x0 G s t X denote £ := {£ G X : /(£) = /(x 0 )}. Then £ is standard and closed. If x,£ G X and £ « x then by (3.1) and (3.4) /(£) = /(x). Therefore for each x G st i? h(x) C iJ, hence £ is open. > 3.10 P r o p o s i t i o n . Let f G W n * y * x , x G * X . Suppose that V I G ' I ^ ~ I 4 /(£) ~ / ( x ) - TV&en / is continuous at the point x in the usual sense, i.e. for each positive real e there exists a positive real 8 such that for any £ G *X the inequality d(£,x) < S implies d(f(£),f(x)) < e. Proof. For a real e > 0 put E := {r G *R : r > 0 and d(£,x) < r => d(f(£),f(x)) < e}. By the principle of internal definition E G W. Since {r G *I : r > 0} C E, by the R-overspill .E contains a ball of the space *X with center x and radius 6 *> 0. >
4. Galaxies Define some more equivalencies on *X. For x\, X2 G *X put x i ~ X2 s d[x\, X2)
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X2- Then for any two R-galaxies Gi, Q2 their ns-hulls (Qi,d), (&2,d) are isometric metric spaces.
Proof. Let Q\ = *G(a?i), Q2 = *G{x2) and let / be an isometric map X on X such that f(xi) = X2- Since / C */, we write / instead of */. For the NSA-transfer principle (1.5) / is an isometry *X on *X. Therefore / is R-continuous, hence has the ns-hull/. For arbitrary &,& G *X we have d(/(6),/fe)) = M/(£i), /(&)) = °d(^i,^2), whence V 6 , 6 G**
d(/(|i),/(6)) = d(|i,£ 2 ).
(4-1)
In particular, the restriction of / to an arbitrary ns-hull Q is an isometric map G on ^. Let £ € &, then by (4.1)^2,,/(£» = d(/>i),/(I)) = d(*i,O, i-e. d(x2,f(O) e K. We see that V£ G & /(£) € S2- Evidently f~l exists and is an isometric map Q2 on Q\. > 4.6 Corollary. For a standard normed space X and points xi,a;2 G X put V ^ £ l /(£) = ^ + X2 — x\. The shift / is an isometry X onto X such that /(xi) = X2 • Therefore the ns-hulls Q\, Q2 of arbitrary galaxies Q\, Q2 of the space X are isometric. Thus it is sufficient to investigate the principal galaxy Q = *G(x), x G X, only. >
5. A standard R-infinite-dimensional Hilbert space Let rn be a fixed standard R-infinite number: TO G st (*N\N). Denote by CTO the linear space of complex valued functions x defined on TO = {0,1,... ,TO — 1}. Arithmetical operations in C m are defined pointwise. 5.1 Definition. A function x G C m is said to be integrable iff for any real e > 0 there exists a finite set A C m (obviously, "e is real" means "e G R", and "A is finite" means "cardA G N") such that for arbitrary finite E\:E2 C m we have Ac£in£2=> |V
jx(i)|-V
\x(t)\ <e.
(5.1)
The subspace of integrable functions x G C m is denoted by i\ (m) or shortly by l\. 5.2 Remark. For a; G C m put suppx := {t £ m : x(t) 7^ 0}. The support suppa; of x G i\ is enumerable: Va; G l\ cardsuppx < cardN. Indeed, if cardsuppa; > cardN, then there exists a real e > 0 such that card { t e r n : \x{t)\ > e} > cardN. Thus x does not satisfy condition (5.1). > 5.3 Definition. For x G i\ by J x denote the sum of the absolutely convergent series £ t 6 s u p p x z(£). 5.4 Remark. If x G £1, then for any real e > 0 there is a finite set A C m such that for any finite set E C m A C -E =>• | / x — X^eB^Wl < £- Notice that the
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integral J x is a linear positive functional on £\, bounded relative to the norm
Nli:=J>l=£tesuppxl*(*)l5.5 Definition. By £2(m) or shortly by £2 we denote the space of square integrable functions x G C m with the inner product
{x\y):= J xy = YJt<mx{t)W)-
(5-2)
5.6 Remark. £2 is a standard nonseparable (complete) Hilbert space. The Kronecker deltas (Ss)S£m form an orthonormal basis of £2: Vx G £2 x = ^2s&mx(s)Ss. There is a natural standard decomposition of £2 as an orthogonal sum of its separable subspaces. At first let us decompose m. 5.7 Definition. The restriction of the equivalence *~ to m := { 0 , 1 , . . . , m — 1} determines the quotient set [i := m/ *~. For each ml G \i put ^(m1) = {x G £2 '• suppa; C m'}. 5.8 Proposition. For each m' G /x £2(1^') is a closed separable (i.e. £2{m') has orthonormal bases of cardinality cardN, for instance (5 s ) s6m ' / ) subspace of £2 and
e2=l2(m) = ®m,eite2(m').
Proof. For v G m let mv denote the equivalence class mv := {t G m : t *~ v). Observe that rriQ = N, m m _ i = (m —1) —N and for v G m\(moUm m _i) vnv = v+Z. This proves our assertion. >
6. Shift on £2(m) Denote by 3 the shift operator defined on £2(Z) by Vx G £2{1) Vt G Z 3a;(i) = x(i + 1). Notice that 3 is unitary. For x G ^ ( Z ) and 0 <
{
x(t+l) for t < m-1, x(0)
for t = m - 1.
(6.1)
6.1 Proposition. TTie operator 2) is unitarily equivalent to a (nonenumerable) orthogonal sum of copies 3 m ' , rn' £ fi = m/ *~, 0/ i/ie operator 3 •' 2J ~ © m ' g m 3m' • 7n particular, the spectrum ofty is purely continuous and fills in the circle {e%v : 0 < ip < 2TT} with the multiplicity card/x.
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Proof. Let TO' G /J, \ (TOO U m m _ i ) . Then the subspace ^{m') of £2^) is invariant under 2). Denote 2J' = Z)\e2(m>) and for v G TO', t 6 Z, x £ ^2(Z) put 3"a;(t) = x(t + i'). Then 3 " is a unitary map ^2(Z) —> ^2(?ro') which transforms 3 in 2)':
3^3 = qj'3". Now let TO" = TOO U mm_\ and let 2J" = %)t2(m")- The map t H> m - 1 + t transforms Z_ := {t e Z : £ < 0} onto m m _ i . Observe that mo = N. Therefore the operator 3o : = I^2(m0) + 3 m ~ : is a unitary map £2(Z) —*• ^ 2 (m") which transforms 3 in 2J": 3o3 = 2)"3o- Because 2J = (©2)') © 2J", our assertion is proven. > 6.2 Remark. Another point of view on the shift 2) defined by (6.1) is natural, too. Consider £2{m) as a Hilbert space (not over C but) over the field *C of hypercomplex numbers. Now the sum in (x\y) = ^2t€m x(t)y(t) (see (5.2)) is simply the starversion of the sum of a finite set of summands. Under this treatment 2) is also standard, unitary and its spectrum consists of eigenvalues po, • • • ,pm-i which are roots of the equation pm = 1. The normed eigenfunction x which corresponds to the eigenvalue p is the following: \/t € m x(t) = -i=/9*-
7. Shift and Loeb measure Consider another approach to the same subject. Let as before m G s t ( * N \ N ) . Denote by £ the normed counting measure defined on the R-finite algebra 2lo =
W n2m by VA e $[0 £A = ±(*caid)A; notice that IA G *Q and Im = 1. To
the R-finite measure space (m,2t 0 ,^) there corresponds the standard Loeb measure space (m, 21, C). The starting condition is 2t0 C 21; V ,4 G 2t0 £ A = *£A. The cr-algebra 21 and the cr-additive measure C are obtained by the usual standard procedure of extension. The relation between C— and £— integrals is as follows. A function £ £W D (*C) m is said to be S-integrable iff Jm |£| d£ := ± Y,t&m If (*)l < * oo and for n e *N \ N m E|€(t)|>n IfWI ~ °- A Unction ^ G #• n (*C) m is said to be a lifting for a function x G (*C) m iff x(t) = °£(t) C-a.e. It is proven that a function x G (*C) m is (^-measurable and) £-integrable iff it has an S-integrable lifting. If it is so, then After this introduction denote by H the Hilbert space 1/2(^,21, C) with the scalar product Vx, y G H (x\y) = fmx(t)y(t) C(dt). If £ and r] are square Sintegrable liftings for x and y, then (x\y) = °(f |»7), where (^77) = ^ E t 6 mf( i ) r ?( i )Now define the shift 2J on H by Vx G H W G (m - 1) 2)x(t) = x(t + 1); this is meaningless for t = TO — 1, but never mind: the Loeb measure of an one-point set is: £{t} = ° ^ = 0 . Moreover, because C is cr-additive, we have £N = C(m — N) = C(t + Z) = 0. Besides, define on the linear space if0 = W fl (*C)m the shift 2J0 by Vt G (TO - 1) 2Jo£(O = £(< + 1) and 2J0f (m - 1) = 4(0). Let ^ G Ho be a lifting for x G if. Then 2J0^ is a lifting for 2Jx, i.e. 2Jx(i) = °2J0£(i) £-a.e. We see that
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V x G H 2J:r G H. Because 2)o is a unitary map of Ho relative to scalar product (6.1), 2) is a unitary map H —> H. Denote *cr := {p G *C : pm = 1},
a:={reC:
\r\ = 1}.
7.1 Proposition. The circle a is the spectrum of the shift 2J in H = L2(rn,Qi,£). For p G »<7 denote V£ G TO x p (£) := °(p*). TTien a:p is an eigenfunction
of 2)
corresponding to the eigenvalue r = c'p. The family (x p ) pe>(T is complete in H. Proof. The set »
Functional Analysis and its Applications V. Kadets and W. Zelazko © 2004 Elsevier B.V. All rights reserved
167
The Beurling Theorem for Entire Functions of Finite Order Konstantin G. Malyutin Deparment of the mathematics, Ukrainian Academy of Banking, Sumy, Ukraine
Nazim Sadyk Department of mathematics, Istanbul state university, Turkey
Abstract We extend the result of Beurling on the closure in Hp of the linear manifold F(z) • {polynomials of z} to the classes of entire functions of finite order. Key words: Beurling theorem, entire functions of finite order 2000 MSC: 30D20, 30D55 The following theorem (for p = 2 proven by Beurling, the general case was considered by T. Srinivasan and J.K. Wang [4]) is well known. Beurling theorem. Let F = IFQF 6 Hp, p > 0, where Ip is the inner function of F. Then the closure in Hp of the linear manifold F(z) • {polynomials of z} is IF • Hp.
In this paper we generalize the Beurling theorem to the classes of entire functions of finite order. Denote by E the set of all entire functions on the complex plane C. For real constants p > 0, a > 0, we define the Banach space £ £ : = { / : / € E, ||/|| Pi<7 = sup \f(z)\exp(-o-\z\>>) < w} zee and set E^ = [J Eap. The set E^ is a linear locally convex space with the topology CT>0
of inductive limit. The sequence of entire functions {/„} converges in the space E^ Email address: kgmSacademy.sumy.ua (Konstantin G. Malyutin).
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Konstantin G. Malyutin, Nazim Sadyk
as n —> oo to a function / if and only if {/„} converges to a function / uniformly on every compact subset of C and there exists K > 0 such that |/ n (^)| < exp(K\z\p) for all z e C . The space E^° is a topological algebra with respect to the product of the functions. Linear continuous functional I on the space E^ is such that oo
oo
fc=O fc=0 l
l k
where lim k- 'P\ck\ /
= 0 [2].
k —*oc
Lemma. Let f =£ E^°. Then there exists a sequence of polynomials Pn{z) such that Pn(z) converge in E^° as n —> oo to f. OC
Proof. Let f(z) = J2 hzk. Then we set fc=0 n
^hzk.
Pn(z) = k=0
oo
Let I be a linear continuous functional on E°f. Then l(f—Pn) =
J2 ctbk converge k=n+l
as n —> oo to zero. Let / be any entire function, let {an} be the set of all zeros of the function / , and let J/(z) be canonical product of the set {an} (if the set {an} is empty then If(z) = 1) [3]. We shall say that Ij(z) is the interior factor for / . The function Qf(z) = f(z)/I/(z) is called the exterior factor of / .
Theorem. Let f = IfQf G E™. Then the closure in £^° of the linear manifold f(z) • {polynomials of z) is If • E^°. Proof, a) IfE™ includes this closure. Let g G E™, and let {Pn{z)} be the sequence of polynomials such that fPn converge in £p° as n —> oo to g. Let ak be a zero of the function f(z). Since fPn converges to g uniformly on every compact set, the f(a,k)Pn(ak) converges as n —+ oo to giflk)- Since we have f{ak)Pn(ak) = 0 for all k = 1,2,..., g(a,k) = 0, k = 1, 2,..., follows then. We just prove G := g/Ij G E^°. The following argument we shall call "standard argument". Let C(£,p) be a disc of radius p about £. Let {C(£n,pn)} be a sequence of discs. The number L = lim sup - ^ pn ^ ° ° r\U\
is called the upper density of the set (J C(£,n,pn) [3]. n-l
(1)
The Beurling Theorem for Entire Functions of Finite Order
169
If / e ££° then for all s > 0 there exists Ke > 0 such that \n\f(reie)\>-K£r", for all re%6 £ CE, where Ce is a set of upper density e and Ks is the constant dependent on e [1]. Thus, there exists a set C£ of upper density e such that \n\G(reie)\ < KErp
(2)
for all reie £ CE. Let z = re10 & Ce and let pn be the radius of the disc centered at £„, denoted C(£n,Pn), such that z e C(£n,pn). It follows from (1) that pn < j^r. By the maximum modulus principle the relation (2) is true (probably with other constant) for all z e C . b) The closure of f(z) • {polynomials of z] includes If • £^°. It is equivalent to prove that the linear manifold Qj(z) • {polynomials of z) is dense set in E^°. Really, if g G E^ and fPn —>• g in E^° then g = If G as in a). We prove that G belongs to the closure in E^° of the manifold Qf{z) • {polynomials of z}. There exists K > 0 such that \f(z)Pn(z)\ < exp[ff 1 r p ] for all z = re10. By "standard argument", we find K\ > 0 such that
|Q/(z)P n (*)|<exp[Jir 1 r'']. By Stieltyes-Vitali theorem, the sequence {QfPn} converges uniformly on every compact set, it is clear to the function G and G G £^°. Let g be any function of E™. Then g/Gf € ££°. Let {Pn(z)} be the sequence of polynomials converges in E^ to g(z). Then QjPn convergent to Q/g. Acknowledgements. The authors would like to thank the Referee for pointing out mistakes in earlier versions of the paper. References
1. A.F. Grishin, Continuity and asymptotic continuity of subharmonic functions, Mat. Fix., Anal, Geom. 1 (1994) 193-215 (Russian). 2. A.F. Leontyev, Generalization of series of exponents. Nauka, Moscow, 1981 (Russian). 3. B.Ya. Levin, Distribution of zeros of entire functions. GITTL, Moscow, 1956 (Russian). Revised English transl.: Amer. Math. Soc, Providence, Rh. I., 1980. 4. T. Srinivasan, J.K. Wang, On closed ideals of analytic functions, Proc. Amer. Math. Soc. 16 (1965) 49-52.
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Dvoretzky's Theorem by Gaussian Method Ivan Matsak a and Anatolij Plichkob a
Kyiv State University of Technology and Design, 2 Str. Nemirovich-Danchenko, Kyiv 04011 Ukraine b Institute of Mathematics, Cracow University of Technology, Cracow, Poland
Abstract A complete proof of the Dvoretzky theorem, accessible to graduate students, is given. Key words: Dvoretzky theorem, Gaussian random variables, Gaussian measures 2000 MSC: 46B20, 46B09, 28C20, 46G12 In this note we give a complete proof of the well known Dvoretzky theorem on the almost spherical (or rather ellipsoidal) sections of convex bodies. Our proof follows Pisier [18],[19]. It is accessible to graduate students. In the references we list papers containing other proofs of Dvoretzky's theorem.
1. Gaussian random variables Let £ be a real valued random variable (r.v.) on a probability space (Q,B,P). Put E£ := Jn £(w)dP. If £ > 0, then E£ = /0°° P{£ > t}dt = / 0 °°(l - P{£ < t})dt [6], 15.6. Definition 1. An r.v. g with a distribution function P{g
1 = -7=
/"*
u2 exp(—-)du , t e R ,
is called a standard Gaussian r.v. Its characteristic function is (see f.e. [3], 17.2) t2 4>{t) := Eexp(ii5) = exp(- —) . Email addresses: inforl8valtek.kiev.ua (Ivan Matsak), aplichko3kspu.kr.ua (Anatolij Plichko).
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Ivan Matsak, Anatolij Plichko
Proposition 1. Let (,)" be independent standard Gaussian r.v. and X ^ a | = 1Then "Y^\aj9j *sa standard Gaussian r.v. as well. Proof. Let us find the characteristic function of r.v. Yliaj9j- As ^s known ([3], 15.12), the characteristic function of a sum of independent r.v. equals to the product of the characteristic functions of summands. So n
n
Eexp(it^2aj9j) = J^Eexp(itojgj) = j=i
i n
a2t2
IIexP(—1~)
=ex
t2
n
t2
P(-y^ a ?) = e x p ("^")
i.e we obtain the characteristic function of standard Gaussian r.v. However, the distribution of an r.v. is uniquely determined by its characteristic function [3], 10.3. Hence, Y^i aj9j i s a standard Gaussian r.v. • Proposition 2. There exists a constant c > 0 such that for any independent standard Gaussian r.v. (gj)™ Emax|aj| > c(lnn) 1/2 . Proof. By definition, /•oo
E max \gj | = / [1 - P{max \gA < t\]dt = i
f°[l-(P{M <*})"]<** =
Jo /•OO
/ [1 - (1 - P{|ff| > i])n)dt > (for any a > 0) > Jo f [ l - (1 - P{| 5 | > t})n]dt > a[l - (1 - P{\g\ > a})"]. Now t2
/~2~ f°°
P{\g\ > a} = yj- J
eM~\)dt>
Take a = (Inn) 1 / 2 . Then for sufficiently large n [2
((Inn)1/2 + 1)2
ft
mnN
1
P{|,| > a} > yj- ex P (-iL_^__± ) > ^_ e x p ( _ _ ) > _ .
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Theorem by Gaussian Method
173
Hence, for some c > 0 E m a x | 5 i | > ( l n n ) 1 / 2 ^ - (1 - - ) " ] > ( I n n ) 1 / 2 •{!--) j
n
e
> c- ( l n n ) 1 / 2
for sufficiently large n . •
2. Standard Gaussian random vectors and Gaussian measures A random vector ~~g = (<7j)™ with independent standard Gaussian components gj we call a standard Gaussian random vector. Theorem 1. Let g be a standard Gaussian random vector and let U be an orthogonal matrix in M n . Then U~g is a standard Gaussian random vector as well. Proof. Let
=
M?) = 0(7) = exp(-i f>?) . But the distribution of a random vector is uniquely determined by its characteristic function ([3], 10.6). Therefore, U( g ) is a standard Gaussian random vector. • Definition 2. A measure 7(^4) := ~P{g 6 A} {A C K is Borel) is called a Gaussian measure (generated by a standard Gaussian r.v. g). Of course, different standard Gaussian r.v. generate the same Gaussian measure A Gaussian random vector ~~g generates a Gaussian measure 7n(^4) = P{lf £ ^4} in K n . The fundamental property of Gaussian measure is its invariance under rotations. More exactly, Theorem 1 implies Corollary. Let a Gaussian random vector g generate a Gaussian measure "/n and let U be an orthogonal matrix in W1 . Then U~g generates the same measure j n .
Lemma 1. J*R exp(ai)c?7(t) = exp ^- .
Proof.
174
Ivan Matsak, Anatolij Plichko 2 f f i t / exp(at)d-y{t) = / exp(at)—= exp(- — )dt =
1 -/=
f /
ex
,a2-{t-a)2,J P( 7,
2
, 1 / , i2w a2 ) * = exp( — )-== / e x p ( - - ) d t = exp— . D ta
Proposition 3. Let~f = (h,...,
/„) € R n . T/ien
/" exp(7,7}rf7n(T) = exp(J||7|J2)Proof. Let 7 = (
e x P ( 7 , ? ) d 7 n ( T ) = /" exp(V M)d7 n ("t > ) =
^R"
JR"
' ^
(by the Fubini theorem) = = TT / exp(fltl)d/y(ti) i JTS.
=
(by Lemma 1) = f[exp{±f?) = exp(|||7||l) . •
3. Some mathematical analysis Definition 3. A vector function x(6) = {x\(8),... ,xn(6)) from R to R™ is said to be differentiable in a point 9 if there are usual derivatives x[ (9),..., x'n(9). A vector function x'{6) = (x[(6),... ,x'n(0)) is called a derivative of x{9). A mapping F(x) from R™ to R is called differentiable in a point x if there exist a linear functional (denote it by F'(x) and its using to y e R n by (F'(x),y)) such that F(y) - F(x) = (F'(x), y-x)+
o(\\y - x\\)
i£\\y-x\\^0. Proposition 4. Let a vector function x(9) be differentiable in a point 6 and let a map F : R n —> R be differentiable in x(S). Then the usual function F(x(9)) is differentiable in 9, moreover [F(x(9))}' =
{F'(x(8)),x'(9)).
Proof. Indeed, F(x(ti)) - F(x(9)) = (F'(x(9)), x{0) - x{0)) + o(\\x{0) - x(6)\\) Now, divide by 1? — 9 and pass to limit. •
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175
Proposition 5. Let $(£) be a convex measurable scalar function and let f(x) be an integrable function on a measurable space (A,T,,fj,). Then *[ / f(x)dfi] < - ^ l *\n(A) • f{x)]d» . JA V\A) J A Proof. Let, first, / be a simple function taking values ti on sets Ai. Then
To finish the proof one can use a passage to limit. • Recall also the Markov (or Chebyshev) inequality fA f(x)dfi > t • fj,{x : f(x) > t} which (in the case of strictly increasing function Phi) we can write in the form tx{x : f{x) >t} = fi{x : 0>(f(x)) > $(t)} <
JA
)}
^
** .
(1)
4. Sobolev inequality T h e o r e m 2 . ("Sobolev inequality"). Let F :Rn —> K be a differ-entiable map and let $ be a convex measurable function in M.. Then f *[F(x)-
[
F(y)dln(y)]dln(x)<
f
f
<S>£{F'(x),y)]dln(y)dln(x)
.
Proof. For fixed elements x,y eRn and 9 G [0, f ] put x(9) = x • sin 0 + y • cos 9. Then, by Proposition 4, F(x) - F(y) = F(x£))z
- F(x(0)) = [' [F(x(9))]'d9 = [ * {F'(x(9)),x'(9))d9 . Jo Jo
This equality and Proposition 5 give $[F(x) - F{y)\ = $>l[2(F'(x(9)),x'(9))d9} Jo
< - [' *£(F'(x(9)),x'(9)}]d9 2 K Jo
.
Integrating the last inequality over x and y we obtain / f
f
- r
I
$[F(x) - F(y)]dln{y)dln{x)
<
$£(F'(x(9)),x'(9)}]d9dln(y)dln(x).
(2)
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Ivan Matsak, Anatolij Plichko
Now observe that x'(9) = x cos 9 — y sin 9 , that for every fixed 9 the map (x, y) —> (x(9),x'(9)) is a rotation in R n x M.n an that (this is the crucial point) j n x 7 n is invariant with respect to this map. Thus the right-hand side of (2) is equal to
/
/
^(F'(xly)}dln(y)dln(x).
(3)
By Proposition 5, /
$[F(x)- I F(y)dln(y)]dln(x) < [
f $[F(x) - F(y)}dln(y)dln(x) . (4)
From (4),(2) and (3) we get the theorem. •
5. Gaussian random elements in normed spaces. Second weak moment Definition 4. We say that X is a standard Gaussian random element (r.e.) in a normed space E if there are linearly independent elements (ej)™ in E and independent scalar standard Gaussian r.v. (5*)™ such that X = J2™ 9iei • Definition 4 is connected with the definition of standard Gaussian random vector (Section 2) in the following way. Consider a map T : R n —> E : n
T(ai,...,an)
= ^2atet
.
(5)
1
This map generates a standard random vector Kn.
T~1X(LJ)
= (gi(ui),... ,gn(ui)) in
Proposition 6. Let (X^)™ be independent identically distributed standard Gaussian r.e. in a normed space E and let Y2T at = -'•• Then J ] " a^X^ is a standard Gaussian r. e. with the same distribution as X^.
Proof. Let Xk = £"=1 9kiet. Then m
m
22 akXk = ^ 1
fc=i
n
n
m
a
k ^2 gkiei = ^£2(^2 ak9ki)ei • i=i
j=i fc=i
Since (gki)k,i all are independent and (by Proposition 1) for every i , SfcLi afc5fci is a standard Gaussian r.v., hence ^ZfeLi ak^k is a standard Gaussian r.e. with the same distribution as Xk. • Definition 5. The second weak moment of r.e. X in a normed space E is, by definition, a = a(X) := sup (E/2(X))1/2 . ll/ll=i,/e£* Proposition 7. Let X = Y^i 9iei be a standard Gaussian r.e. in a normed space E and let T be defined by (5). Then a = ||T||.
Dvoretzky's Theorem by Gaussian Method
177
Proof. Obviously, without restriction of generality, one can suppose lin(ei)™ = E. Let (fi) be the biorthogonal to (e») functional. Then for / G E* we have / = Y,i Cifi and a= sup ( E < X > e i , f > / 2 ) 2 ) 1 / 2 = sup (E(]T> Cl ) 2 ) 1/2 = 11/11=1 i i II/II=I V
c 1/2 r C2E 1/2 SU SU T T D sup ( J 2 & = P ( E ' ) = P ii */n = II *II = II II • ii/n=i i ii/n=i i i[/n=i 6. Tail behavior (the concentration of measure phenomenon)
Theorem 3. (Maurey-Pisier; [19], Theorem 4.7). Let X = YX 9iei Gaussian r.e. in a normed space E. Then for any t > 0
be a
P{|!|X|| - E||X||| >t}< 2 e x p ( - ^ ) . Proof. Let T be the operator of Section 5. Then (6) is equivalent to r ot2 n e R : HITill - / \\Tx\\dJn\ >t}< 2 e x p ( - ~ ) . ln{x
standard (6)
(7)
Put F(x) = \\Tx\\ and suppose temporary that || • || is differentiable. Since for any x, y e R" li^O-i^UIITtx-^II^IITIHIz-ylb, Il-^'(a;)l|2 < o" for every i e R " (recall, a = \\T\\ !). Thus, by Proposition 3, for any Ael
I exp[^(F'(x),y)}d^(y) = exp[J A ^ F ' t o H l ] < e X p[^) 2 a 2 ] . (8) Taking in Theorem 2 $(<) = exp(Ai), we get /
exP[A{F(x) - / f
f
F(y)dln(y)}]dln(x)
<
eM^{F'(x),y)}dln(y)dln(x)<
(by (8)) < /
(9)
exp[|(^) 2 ]d 7 n (x) = . 1 . \TCO~,
2
I
exp[-(^-)2] • Using the Markov inequality (1), taking there $(t) = exp(Ai) , f(x) = F(x) — / R n F{y)drin{y) and fj, = in{x), we get from (9) ln{x
: F(x) - JF{y)dln{y)
> t} < e x p [ i ( ^ ) 2 - At] .
178
Ivan Matsak, Anatolij Plichko
Putting A = T~\2 we obtain ln{x
: F(x) - J F{y)dln{y) > t} < e x p [ - ^ ^ ] .
Clearly, the same inequality holds for —F, so we finally obtain (7), and hence (6), for differentiable norms. To finish the proof, observe that in the finite dimensional space lin(ej)™ one can approximate any norm by differentiable one as exact as need. • Remark. The estimation (6) is an important result in theory of Banach valued Gaussian r.e. It demonstrates that the distribution of \\X\\ is concentrated near E||X|| as dense as the distribution of Gaussian r.v. a • g near 0. In a somewhat different form: P{|||X[|-m||X||l>i}<2(l-$(^)),
(10)
(where mj[X|| is the median of \\X\\ and $(£) is the distribution function of g), the concentration phenomenon is presented in books Ledoux-Talagrand ([14], 3.1) and Lifshits ([15], Chapt.12). In fact, the concentration phenomenon in the form (10) was contained as far as in Borell [2] and Sudakov-Tsirelson [21]. In connection with Theorem 3, note also papers Fernique [7], Landau-Shepp [13] and Skorokhod [20], where for the first time were established exponential integrability of the norm for Gaussian r.e., and Yurinskii [24], where for the first time was proposed the martingale approach to estimations of probabilities of large deviations for the norm of sums of independent r.e. in Banach spaces.
7. Levy's inequality Recall that an r.e. X in a normed space E is called symmetric if P{X G ^4} = P{X G -.4} for any Borel set A C E. Theorem 4. (Levy's inequality; [11], II.3). Let (Xj)™ be symmetric independent r.e. in a normed space E and S = Y^i Xi • Then for every t > 0
2P{||5|| >0>P{max||Xi|| > t} . i
Proof. Put r = r(w) = min{i : ||Xi|| > t}. Then P{||S||>t}>£p{||S||>t,T = i}. Now since (Xi,...
,Xn) and (—X\,...,
-Xi-\,Xi,
—Xi+\,...,
(11) —Xn) are identically
distributed and r depends on {||Xj||}™ only, we have P{||5|| > t , r =i} = P { \ \ X i - i y > t , r = i},
Dvoretzky's
Theorem by Gaussian Method
179
where Ri = S — Xi. This equality and (11) imply 2 P { | | 5 | | >t}> £ P { | | S | |
> t
,
T=
i} + P { | | * -IU\\>t,T
= i}.
(12)
By triangle inequality
2HJM < ||X4 + Ri\\ + | | * -Ri\\ = \\S\\ + | | * - Ri\\ . Hence P{||5|| >t,T = i} + P { | | * - iJiH > t , T = i} > P{||5|| > t \ / | | * -Ri\\>t,T P { 2 | | * | | >2t,r
= i}> P{\\S\\ + | | * - i?i|| > 2 t , r = i} >
= i} = P { | | * | | > t , r = i} = P { r = i} .
This inequality and (12) imply n
2P{||5|| > t } > V p { T = i}=P{max||*|| > t} . D ^—' i=l
i
Corollary There exists c > 0 sitcft t/ioi for any normed space E and any standard Gaussian r.e. X = ^ " ^ e , in E E\\X\\ >c-min||ei|| -(lnn) 1 / 2 . Proof. Evidently, standard Gaussian r.e. are symmetric. Hence one can use Levy's inequality taking S = X and * = giCi. We have for any t 2P{\\X\\ > t} >P{ma.x\\giel\\
> t} .
^
Integrating over t we receive E||X|| > -EmaxllfteiH > - min || ei || • E m a x ^ l > Z
^
Z i
i
(Proposition 2) > c • min ||ej|| • (Inn) 1 ' 2 . D i
8. Dvoretzky-Rogers t h e o r e m T h e o r e m 5. (Dvoretzky-Rogers, [5]). Let || • || be a norm on MN and let D be the ellipsoid of maximal volume inscribed in the unit ||-||-6an B. Then there exists a basis (ei)f, orthonormal with respect to D, such that 1 > ||ej|| > 2~(~N~1^(-N~^ , i = 1,...,N-1 . Proof. We choose the basis (ei) inductively in the following way. Let ei be a vector in D with maximal norm (clearly ||ei|| = 1). Given e i , . . . ,e,, choose e^+i in Dt~\ (e\,..., ei)1- with maximal possible norm (_!_ is the orthogonal complement with respect to D).
180
Ivan Matsak, Anatolij Plichko
Then for any x € lin(e»,..., ejv) n D
INI < INI •
(13)
Now consider the ellipsoid V*" 1 ^ 2
N
TN a2
i=i
Of course, this ellipsoid depends on i and scalars a and b which we shall choose late on. If X)j=i ajej ^ ^ then Y^L~ a,jej € aD and thus || 2 i ~ ajej\\ < a- I n the same wa
y' II Y!j=ia3ei\\ ^ & a n d tnus > by ( 13 ): II YH ajej\\ < Hei\\Choosing a = 1/2 , 6 = l/(2||ei||), we get that U C B. On the other hand
so necessarily 1
1
2^'(2||ei||)^-1 or He,!! > 2-( JV " 1 )/( JV - 1 ). • Corollary 1. Let E be an N-dimensional normed space and N = [y]. Then there exist {ei)i C E such that ||ej|| > | and for any (a^ C K
IIE«^II<(E«?)1/2i
(14)
i
Corollary 2. For even/ N-dimensional normed space E there exists a sub space E C E of dimension N = [y] and E-valued standard Gaussian r.e. X with E||X|| = 1 and cr2(X) < c/lnN, where c > 0 is an absolute constant. Proof. Let X = ^2i 9iei where (gi) are independent Gaussian r.v. and (e^) are from Corollary 1. Then, by (14),
a(X) := sup ^f(X)Y'2 111/1 = 1
= sup (f> 2 (e 8 )) 1 / 2 = sup || V V e J 1 / 2 < 1 . 111/1 = 1 ~l
l|o||2 = l
On the other hand, by Corollary of Theorem 4 E||X|| > ci(lnTV)1/2 > c 2 (lniV) 1/2 . Now put X = X/E||X|| . •
9. Two geometric lemmas
~y
Dvoretzky's Theorem by Gaussian Method
181
Lemma 2. Let || • || be any norm on R n with unit ball B and unit sphere S. Let 8 > 0. There is a 5-net A C S with cardinality cardA < (1 + ~)n . o
(15)
Proof. Let A be a maximal subset of S such that \\a — b\\ > 8 for all a, b G A , a ^ b. Clearly, by maximality, A is a <5-net of S. To majorize c&idA we note that balls a + f-B , a G A are disjoint and included into (1 + |)£?. Therefore £
vol(a + | f i ) < vol((l + ^)B) = (1 + |)»volB ;
hence cardA • (^)"voLB < (1 + ^)™volB . This inequality implies (15). • Lemma 3. For each e > 0 there is a 5 = S(e) , 0 < S < 1, «n£/i ifte following property. Let || • || fee an arbitrary norm on W1 with the unit sphere S. Let A be a 8-net in S and let X\,..., xn be elements of a normed space E . If for every a= (ai,...,an) GA n
1-6 < \\^2akxk\\
then for every a G S n
( 1 + e ) " 1 < |l^a f c xfc|| < 1 + e;. I
Proof. There is a 0 in A such that \\a — a°\\ < 8 hence a — a0 + \\a' with |Ai| < 8 and a' G S. Continuing this process we obtain a = a0 + Xia1 + X2a2 + • • • with aj G A and |Aj| < Sj. It follows that
HEa fc x fe ||<^^||f:4^ll<^. 1
j>0
fe=l
Similarly ii V -
IV^ o \\}_,akxk\\ I I>^ I \\^4x k\\
ii
6(1 + 6) ^ , - ^—^ > l - 6. - -8(1f +- 8)f = y -1-38y .
Hence, if 8 > 0 is chosen small enough so t h a t 1-35 1 ~i T - T~,— 1 —6 1+ e
and
, 1+ 8 1 ^i 1 < 1 + £ > 1 —8
we obtain the announced result. Note that one can find a suitable 8 depending only on £ (and independent on n). •
182
Ivan Matsak, Anatolij Plichko
10. Dvoretzky's theorem Theorem 6. (Dvoretzky). For each e > 0, there is a number r\ = jj(e) > 0 with the following property. Every normed space E of dimension N contains a subspace of dimension n = [ryln JV] which is (1 + s) 2 — isomorphic to V^. Let us present first the idea of proof. We take independent copies X\,..., Xn of r.e. X from Corollary 2 of Dvoretzky-Rogers theorem, n sa lniV, which is determined on a probability space (fi,S, P ) . Let Cl(n,e) be the set of all ui in Q. such that for every a = (ai,... ,an) in the unit sphere S of Euclidean space R n
(l +
1
n
e)- <\\Y/^Xl(u;)\\
We will show that P{fi(n, e)} > 0 provided that n is not too large and precisely provided n < r]/a2. This clearly yields Theorem 6. Now the Proof. Let E be the subspace and X be an r.e. from Corollary 2 of Theorem 5. Let X\,... ,Xn be independent copies of X (n we choose late on). Then for any a = ( a i , . . . ,an) in S the r.e. J^i ak^k has the same distribution as X (Proposition 6). Thus we have E|| X)"akXk\\ = 1. Therefore, by Theorem 3, for any S > 0 2r ! > 2
™
Fi2
P{||| ^> fc X fe |( - 1| ><&} < 2 e x p ( - ^ ) < 2 e x p ( - - ) . Let A be as in Lemmas 2 and 3 with ||a|| = ||a||2- Then preceding inequality implies P{3aG.4: ||| 5]a fc X fc || - 1| > 6} < 2(card^)exp(
-) <
l
(by Lemma 2) < 2 ( 1 + .In.
2exp(— exp
.
52.
2n S2 exp( -) < o o~z .In <52. n
T)
^) = 2exp
(16)
-) .
Now let 8 = S(e) be the function of e, given by Lemma 3. Let we choose n so that
Then the probability (16) is not greater than 2exp(—^j-). Clearly, we can always assume that a is small enough (say a < (5/2), otherwise there is nothing to prove. Hence we can assume that the right side of (16) < 1. We than obtain that with positive probability, for every a G A
\\\J2akXk(u)\\-l\<6
Dvoretzky's Theorem by Gaussian Method
183
i.e. n
1-6
< ||^OfeX f c (w)|| < 1 + 5 . i
By Lemma 3 (recall, we choose S = 6(e)\), we conclude that with positive probability for all a £ S n
(l + er^U^afcXfcMU^l + e. I
Therefore, there exists UIQ £ fl such that for Xk = Xk(uJo) and for every a G 5 n
1
(l + e)-
By homogenity of the norm it means that lin(:Efc)™ is (1 + e)2-isomorphic to Zj • To satisfy (17) put S3 (recall, a2 < c/lniV, by Corollary 2 of Theorem 5). • Acknowledgement. The first version of this note was written when the second author visited Politecnico di Milano. He express his thanks to P.Terenzi for hospitality and valuable remarks. The authors also express they thanks to M.Ostrovskii for valuable references.
References 1. Y. Benyamini and J. Lindenstrauss, Geometric Nonlinear Functional Analysis. V.I, Colloq. Publ. Amer. Math. Soc, Rhode Island, 2000. 2. C. Borell, The Brunn-Minkowski inequality in Gauss space , Invent. Math. 30 (1975) 207-216. 3. H. Cramer, Mathematical Methods of Statistics. Princeton Univ. Press, N.J., 1946. 4. A. Dvoretzky, Some results on convex bodies and Banach spaces. Proc. Int. Symp. on Linear Spaces, Jerusalem, 1961, 123-160. 5. A. Dvoretzky and C.A. Rogers, Absolute and unconditional convergence in normed linear spaces, Proc. Nat. Acad. Sci. USA 36 (1950) 192-197. 6. W. Feller, An Introduction to Probability Theory and its Applications. V.II, John Wiley and Sons, New York, 1966. 7. K. Fernique, Integrabilite des vecteurs gaussiens, C.R. Acad. Sci. Paris, ser. A 270 (1970) 1698-1699. 8. T. Figiel, A short proof of Dvoretzky's theorem on almost spherical sections, Compositio Math., 33 (1976), 297-301. 9. T. Figiel, J. Lindenstrauss and V.D. Milman, The dimension of almost spherical sections of convex bodies, Ada Math. 139 (1977) 53-94.
184
Ivan Matsak, Anatolij Plichko
10. Y. Gordon, On Dvoretzky's theorem and extensions of Slepian's lemma, Israel Semin. Geom. Aspects Fund. Anal, Technion preprint series No. MT-636 (1983) (4) II.l.l-H.1.25. 11. J.P. Kahane, Some Random Series of Functions. D.C. Heath and Co, Lexington, 1968. 12. J.L. Krivine, Sous-espaces de dimension finie des espaces de Banach reticules, Ann. of Math. 104 (1) (1976) 1-29. 13. H.J. Landau and L.A. Shepp, On the supremum of a Gaussian process, Sankhya 32 (1970) 369-378. 14. M. Ledoux and M. Talagrand, Probability in Banach Spaces. Isoperimetry and Processes. Springer, Berlin, 1991. 15. M.A. Lifshits, Gaussian Random Functions. TViMS, Kyiv, 1995 (Russian). 16. V.D. Milman, New proof of the theorem of Dvoretzky on sections of convex bodies, Funkts. Anal. Prilozh. 5 (5) (1971) 28-37 (Russian). 17. V.D. Milman and G. Schechtman, Asymptotic theory of finite dimensional normed spaces. Lect. Notes in Math. 1200 (1986). 18. G. Pisier, Probabilistic methods in the geometry of Banach spaces, Lecture Notes in Math., 1206 (1986) 167-241. 19. G. Pisier, The Wolume of Convex Bodies and Banach Space Geonetry. Cambridge Univ. Press, Cambridge e.a., 1989. 20. A.V. Skorokhod, A note on Gaussian measures in a Banach space, Teor. Veroyatn. Prim. 15 (1970) 519-520 (Russian). 21. V.N. Sudakov and B.S. Tsirel'son, Extremal properties of half-spaces for spherically invariant measures, Zap. Nauch. Sem. L.O.M.I. 41 (1974) 14-24 (Russian). 22. A. Szankowski, On Dvoretzky's theorem on almost spherical sections of convex bodies, Israel J. Math. 17 (1974) 325-338. 23. L. Tzafriri, On Banach spaces with unconditional bases, Israel J. Math. 17 (1974) 84-93. 24. V.V. Yurinskii, Exponential bounds for large deviations, Teor. Veroyatn. Prim. 19 (1974) 152-153 (Russian).
Functional Analysis and its Applications V. Kadets and W. Zelazko © 2004 Elsevier B.V. All rights reserved
185
On the Inverse Problem of Scattering Theory for a Differential Operator of the Second Order Khanlar R. Mamedov, Hamza Menken Mersin University-Turkey
Abstract Direct and inverse problem of scattering theory (IPST) are investigated for the differential equation -y" + q(x)y = X2y on half line containing a spectral parameter in the boundary condition y'(0) + (a0 + iaiX + a2X2)y(0) = 0. Key words: Sturm-Liouville operator, inverse problem of scattering theory, scattering function, scattering data 2000 MSC: 34B24, 34A55
1. Introduction Consider the Sturm-Liouville equation on the half line -y" + q(x)y = X2y (0 < x < oo)
(1)
with the spectral parameter dependent boundary condition y'(O) + (a o + iaiA + a2A2)2/(O) = O. Email addresses: hanlarSaport .ru;[email protected] (Khanlar R. Mamedov,), hmenkenSmersin.edu.tr (Hamza Menken ).
(2)
186
Khanlar R. Mamedov,, Hamza Menken
Here q(x) is real-valued function satisfying the condition
/ (l + x)\q{x)\dx
(3)
and ao, ai, a.2 are real numbers with a\ > 0, a.i > 0. In this paper, we study the inverse problems of scattering theory (IPST) for the boundary problem of (1), (2). Before we discuss our problem we shall recall some works which has the spectral parameter dependent boundary condition. The boundary problems with spectral parameter dependent boundary condition for second order ( or higher order) of differential equations are interesting with their applications, and we refer to [4], [13], [14]. The many spectral properties of such this boundary problems were investigated with different methods by the many authors. About this subject it was given more informations and references in [18], and also in [17]-[5]. The other interesting problem with spectral parameter dependent boundary condition for equation (1) is the inverse problems of spectral analysis, so that it is the construction of the differential operator associated the equation (1) with respect to some spectral characteristics (to two spectres, spectral function, scattering data, etc. ). In finite interval and half line, this problem with spectral parameter dependent boundary condition were investigated with different methods in [l]-[6]. In [16], on the half line the inverse problem was investigated with respect to spectral function for the boundary problem -y" + q(x)y = Ay, y(0) = 8(\)y'(0) where 9(X) is an arbitrary analytic function whose imaginary part is non-negative and q(x) is a real-valued function. Similar problem was investigated in [6] in case
fc=l
A f c
"A
where the numbers a, 6, Afc, pk (k = 1, 2,...) are real coefficients and pu > 0. Also, in the similar cases, on the finite interval too, it is obtained results with respect to two spectres and spectral function, and now the problem on half line that we study is about the inverse problem of scattering theory. In [11],[12] it was considered the boundary problem without any spectral parameter in the boundary condition -y" + q{x)y = X2y,
(0 < x < oo)
(4)
2/(0) - 0 (5) where q{x) is a real valued function satisfying the condition (3), and the inverse problem of scattering theory of the boundary problem (4), (5) was solved. That the boundary value problem (4), (5) has bounded solutions u(X,x) for —oo < A < oo and A = iXk {k = 1, n), moreover, as x —> oo u(X, x) = e'iXkX - S(X)eiXx + o(l), ( - oo < A < oo)
On the Inverse Problem of Scattering Theory for a Differential Operator 187 and
u(i\k,x) = mke-iXkX(l
+ o(l)), (k = l^n),
respectively. Thus, the collection {S(A) (—00 < A < 00); A&; mt {k = l,n) } provides a complete description of the behavior at infinity of all radial wave functions. The collection of quantity {S(A) (—00 < A < 00); A&; m,k (k = l,n) } that specify the behavior all radial wave functions u(X, x) at infinity, will be referred to as scattering data of the boundary value problem (4), (5). In terms of the scattering data, the potential q(x) is recover uniquely (see [17], p. 217). In [8], the inverse problem of scattering theory of the boundary problem -y" + q(x)y = X2y, (0 < x < 00) y'(0) = %(0) was solved where h is any real number. Similar problems for the boundary problem (1), (2) they are considered in [9] and in this paper. The some properties of scattering data were investigated in [10]. According to [12], for any A from closed upper-half plane, the equation (1) has a solution e(A, x) described by e(A,z)=elAx+ /
K(x,t)eiXtdt
(6)
Jx
and for the kernel function K(x, t) the inequality
\K(x,t)\ < ^(^)ex P |a 1 (x) - < n ( ^ ) } holds where
a{x) = I
\q{t)\dt, 0^)=
Jx
I
a(t)dt.
Jx
Moreover,
K{x,x) = -J
q{t)dt.
The solution e(A, x) is an analytic function of A in the upper half plane Im A > 0 and is continuous on the real line. The following estimates hold through the half plane Im A > 0,
\e(X,x)-eiXx\ < L^-cnix+^expi-lmXx
+ o-jix)}
(7)
and \e'(X,x) -iXeiXx\
< a(x)exp {-Im Xx + 0\{x)}
(8)
for real A ^ 0, the functions e(X,x) and e(—X,x) form a fundamental system of solutions of the equation (1) and their Wronskian is equal to 2iA :
W{e(X,x),e(-X,x)}
= e'{X,x)e(-X,x) - e{X,x)e'(-X,x) = 2iX.
(9)
188 2.
Khanlar R. Mamedov,, Hamza Menken Main Results
Let u>(x, A) be a solution of the equation (1) satisfying the initial-value conditions ui(X, 0) = 1,
u>'(\, 0) = - ( a 0 + iaiX + a2X2).
Theorem 1. The identity ——-— 2i\u{\,x) e'(A,O) + (ao + iaiA + Qf2A2)e(O,A)
=
^ ^ y _ v '
5(A)e(A y K
'
x) ' '
(10) '
v
holds for all A ^ 0, where = 1 j
e'(X, 0) + (q 0 + faiA + a2A2)e(A, 0) e'(A,O) + (ao + iaiA + a2A2)e(A,O)
and 5(A) = 5(-A). Proof. Since two function e(—X,x) and e(A,x) form a fundamental system of solutions to equation (1) for all A ^ 0, we can write LO(X, A) = ci(X)e(X,x) +c 2 (A)e(A,x) where m C l ( j
_ e'(A, 0) + (a 0 + iaiX + ct2A2)e(A, 0) ~ -2iX
and ... C2(A) =
e'(A,O) + (a o + iaiA + a2A2)e(A,O) 2iA •
Then, w(a. A) =
i U 0 ) + (ao+ ia,A+ a a A » ) ^ 0 ) e ( A > ^ + —2zA 2 | e'(A,0) + (Qo + ia 1 A + Q 2 A )e(A,0)--—2?A
Let £(A, 0) = e^A, 0) + (a 0 + ioc\X + a2A2)e(A, 0). Since q(x) is real, it follows that e(-A,0) = e(A,0), and hence that £(A,0) ^ 0 for all real A ^ 0. To prove this we assume that there is a non-zero Ao G (—00,00) such that E(X0,0) = e'(A0,0) + (a 0 + i^X + a 2 A 2 )e(A 0 ,0) = 0 or e'(A0,0) = - ( a o + i a i A + a 2 A 2 )e(A 0 ,0). From the formula (9) we get e'(A0,0)e(Ao,0) - e(A0,0)e'(A0,0) = 2iXo or -2iaiA 0 |e(A 0 ,0)| 2 = 2iA0.
On the Inverse Problem of Scattering Theory for a Differential Operator 189 Since a\ > 0 we have a construction, hence we have that E(X, 0) ^ 0 for all real A ^ 0. According to the formula (11) we obtain „ , , 2iA^A'^ ^ ^ = J(X^) - S(X)e(X,x) y y J y e'(A,0) + (ao+iQiA + a 2 A 2 )e(A,0) ' ' ' ; where 1
, '
=
e'(A, 0) + (q 0 + jaiX + a2A2)e(A, 0) e'(A,0) + (ao + iaiA + a2A2)e(A,0)
and £(A,0) = e'(-A, 0) + (a 0 - «*i A + a 2 A 2 )e(-A, 0) = E(-X, 0),
5(A) = 5FA). This proves the theorem. • T h e o r e m 2. The function E(X, 0) may have only a finite number of zeros on the half plane Im A > 0, they are all simple and lie on the imaginary. Proof. From the proof of Theorem 1, since -E(A, 0 ) ^ 0 for all real A ^ 0, the point A = 0 is the possible real zero of the function E(X,0). Since the function E(X, 0) is analytic in the upper half plane Im A > 0 we have that the zeros of E(X, 0) are at most countable. Now to show that the set of the zeros of E(X, 0) is bounded we assume, by way of contradiction, that this set is bounded, so that there exist the numbers A& such that these numbers satisfy the relation E(Xk, 0) = 0 for Im A& > 0 and |Afc| —> oo or e'(Afc,0) = -(ao + ia\X + a2A2)e(Afc,0). From the relation (8) and last statement we have that lim e(Afc,0) = 0 as \Xk\ —• oo. On the other hand, k—»oc
according to (7) it follows that lim e(Afc, 0) = 0. This contradiction shows that the k—>oc
set {A*;} is bounded. Hence, the zeros of the function E(X, 0) is bounded and is form at most countable set having 0 the only possible limit point. In [9], it was shown that the zeros of the function E(X,0) are simple and are purely imaginary. Now we shall prove that the function E(X,0) has finitely many zeros in the half plane Im A > 0. This is obvious if -E(0,0) =/= 0, because under this assumption, the set of zeros cannot have limit points. To verify that the number of zeros of E(X, 0) is finite in the general case too, we show that the distance between neighboring zeros is bounded away from zero. We let 5 denote the infimum of the distances between two neighboring zeros of .E(A, 0), and show next that S > 0. Otherwise, we could exhibit a sequence of zeros, iiXk \ and {iXk} of the zeros the function E(X,0), such that lim (Afc - Afc) = 0, Afc > Afc > 0, and maxA^ < M. Then it follows from estimate (9) that, for A large fc enough, the inequality e(iX,x) > \e~Xx holds uniformly with respect to x G [A, oo) and A £ [0, oo) whence
190
Khanlar R. Mamedov,, Hamza Menken oc _
/
e-2AM
e{i\k,x)e{iXk,x)dx >
g M
.
(12)
A
On the other hand, according to the formula (11) in [9] we have oc
0 = (Afc - Afc) / e(iXk, x)e(iXk, x)dx + a 2 ((A fc - Afc) • o
•e(iXk, 0)e(iAfc, 0) + axe{iXk, 0)e{iXk, 0).
(13)
Letting k —> oo, we get a 1 |e(iA fc ,0)| 2 = 0. This relation gives a contradiction if a.\ > 0. If ot\ = 0, from the formula (13) we write oc
0 = / e(i\k, x)e(iXk,x)dx o
+ e(iXk,0)e(iXk, 0) =
A
= o
A
e(iXk,x) \e(i\k,x) - e(iXk,x)\ dx + / e(iXk,x)e{iXk,x)dx + o oc
+ / e(iXk, x)e(iXk, x)dx +
e(iXk,0)e(iXk,0).
A
Taking limit as k —> oo, we get oo
0 > lim
k^ooJ A
e(iXk,x)e(iXk,x)dx.
But this contradict with the inequality (12). Thus, the assumption is not true, so that 5 > 0. Thus the function E(X,0) has finitely many zeros. This completes the proof. • Theorem 3. The function 1 — S(X) is the Fourier transform of a function Fs(x) of the form FS(X) = FP(X)+FP(X), where Fg(x) sup
Fs2\x)
£
L\(—oo,oo),
whereas Fg (x)
< oo.
— oc
Proof. From the formula (6) it follows that oo
fK(O,t)eiXtdt,
e(A,0) = l + o
6
L2{—oo,oo) and
On the Inverse Problem of Scattering Theory for a Differential Operator 191 oo
e'(A, 0) = iX - K(0,0) + I"Kx{0, t)eiXtdt. o We shall use the following notations for shortly: <po(X) = a0 + iaiX + a2X2 - q0;
go = K(0,0);
Ki(t)=Kx{0,t)+aoK(0,t);
K2(t) = axK{Q, t) + a2Kt(0,t);
K3(t)=aiK(O,t)-a2Kt{O,t) and oo
^(-A) = IK^ty^dt,
j = 1,2,3.
o Then we have _ s(x)
1
2iA(l + a2q0) + Xx(-A) + zAJf2(-A) - K^X) - iXK3(X)
=
<po{X)+iX{l +
a2qo)+K1(-X)+iXK2(-X)
Every one of the functions ~
iX(l + a2q0)
fl(X)
=
7TT
Vo(X) ~ MX)
~
£!(-A)+a£2(-A) 7^-T
, 72 (A) =
,
fo{X) K1(X) + iXK3(X) =
MV
•
is the Fourier transformation of a summable function. Hence we have 1-S(A)=
where
^ 1 + K(-X) _ _ _ _ /(A)=2/ 1 (A) + / 2 (A)-/ 3 (A), ^ ( - A ) = /1(A) + / 2 (A).
We can rewrite the formula (14) as form
1 - 5(A) = /(A) [{l + (1 - MAiV-^t-A)}' 1 - l] + +/(A)-/(A)| ^ 1—-\ (15) T-[ l + |l-/i(AiV- 1 ) J ft:(-A)| 1 + AX-A)J where 1, h(X)=
2-|A|, 0,
* / |A| < 1 if 1 < A < 2 if
|A| > 2
192
Khanlar R. Mamedov,, Hamza Menken
is the Fourier transform of the function h(x) € Li(—00,00). Also, h(\N~l) Fourier transform of the function h^ix) = Nh(xN), and i\imJ\f(x)-hN*f(x)\\Li=O
is the
(16)
for all f(x) G Li(—00, 00), where h^ * f(x) is the convolution of functions hpf(x) and f(x) from L\{—00, 00). Note that the convolution h^* fix) of functions h^ix) and f(x) from Li( —00, 00) is denned as h^ * fix) = f hff(x — t)f(t)dt.
In general,
— oc
recall that the Fourier transform of the convolution 00
/ * g(x) = J f{x- t)g{t)dt —00
of two functions from L\{—00, 00) equals the product /(A)g(A) of their Fourier transforms, and the norm of the convolution does not exceed the product of norms:
II/^IIL^II/IILJMI^Consequently, if ||/|| L l < 1, then the series
-f(x) + f*f(x)-f*f*f(x)
+ ...
converges in the metric of L\{—00,00), its sum belongs to this space and its Fourier transform is equal to
-/(A) + {/(A} 2 - {/(A} 3 +... = {1 + /(A}" 1 - 1 . We conclude, from (16) and the previous argument that for N large enough, the function 1 + < 1 - h{\N~l) \ / ( - A ) - 1 is the Fourier transform of function from Li(—00, 00). It follows that the sum of the first two terms in the right-hand side of (15) is also the Fourier transform of a summable function Fg (x). Finally, since hiXN'1) = 0 for |Aj > 2N, the third term in the same formula vanishes for |A| > 2N and is bounded. As such, it is the Fourier transform of a bounded function Fg (x) S Li{—00, 00), and the theorem is proved. • Using the identity (10), Theorem 2 and Theorem 3, as in [9], we obtain GelfandLevitan-Marcenko's basic equation which has important role in the solution of IPST /•OC
F[x + y)+ K(x, y)+
K{x, t)F(t + y)dt = 0, (x < y < 00) Jx
where
Fix) = Y,™2ke-XkX + — / k=\
(1 -
Si\)yXxdx
J
-°D
and "the norming constants" are
m-k> = T \eix,i\k)\2dx+ai\la2Xk JO
|e(Q,iAfc)|2.
l
*k
On the Inverse Problem of Scattering Theory for a Differential Operator 193 The collection {S'(A) (—00 < A < 00); A&; rrik {k = l,n) } which is defined as above is defined as the scattering data of the boundary problem (1), (2). Theorems on uniquely construction of the boundary problem (1), (2) with respect to the scattering data are given in [9].
References 1. P. A. Binding, P. J. Browne, B. A. Watson, Inverse spectral problems for SturmLiouville equations with eigenparameter dependent boundary conditions, J. London Math. Soc. 2 (62) (2000) 161-182. 2. P. A. Binding, P. J. Browne, B. A. Watson, Sturm-Liouville problems with boundary conditions rationally dependent on the eigenparameter I, Proc. Edinburg Math. Soc. 45 (2002) 631-645. 3. P. A. Binding, P. J. Browne, B. A. Watson, Sturm-Liouville problems with boundary conditions rationally dependent on the eigenparameter II, Journal of Comp. and Appl. Math. 148 (2002) 147-168. 4. C. T Fulton, Singular eigenvalue problems with eigenvalue-parameter contained in the boundary conditions, Proc. Soc. Edinburgh Sec. A 87 (1980) 1-34. 5. N. Y. Kapustin, E. I. Moiseev, A remark on the convergence problem for spectral expansions corresponding to classical problem with a spectral parameter in the boundary condition, Diff. Equations 37 (12) (2001) 1677-1683. 6. V. I. Kopilov, Levitan-Gasymov inverse spectral theorem for Sturm-Liouville problem with a spectral parameter in the boundary condition, Functional Analysis, Linear Spaces. Ulyanovsk (1983) 73-82. 7. N. B. Kerimov, Kh. R. Mamedov, On a boundary value problem with a spectral parameter in the boundary conditions, Sib. Math. J. 40 (2) (1999) 281-290; translation from Sib. Mat. Zh. 40 (2) (1999) 325-335. 8. B. M. Levitan, The inverse scattering problem of quantum theory, Math. Notes 17 (4) (1975) 611-624. 9. Kh. R. Mamedov, Uniqueness of solution of the inverse problem of scattering theory with a spectral parameter in the boundary condition, Math. Notes 74 (1) (2003). 10. Kh. R. Mamedov, H. Menken, Levinson's type formula for boundary problem with a spectral parameter in the boundary condition, Ukr. Math. J. (to appear). 11. V. A. Marchenko, Reconstruction of the potential energy from the phases of the scattered waves, Dokl. Akad. Nauk SSSR 104 (5) (1955) 695-698. 12. V. A Marchenko, Strum-Liouville Operators and Applications. Birkhauser Verlag (1986). 13. A. G. Megrabov, Inverse problems of scattering for planar waves with free boundary or dependent non-homogeneous surface, Proc. Geom. Math. Problems 4, Novosibirsk (1979). 14. S. V. Meleshko, Yu. V. Pokornyj, On a vibrational boundary value problem, Diff. Uravn. 23 (8) (1987) 1466-1467.
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Khanlar R. Mamedov,, Hamza Menken
15. V. N. Pivovarchik, Direct and inverse three-point Sturm-Liouville problem with parameter-dependent boundary conditions, Asymptotic Anal. 26 (2001) 219238. 16. E. A Pocheykina-Fedotova, On the inverse problem of boundary problem for second order differential equation on the half line, Izv. Vuzov 17 (1972) 75-84. 17. E. M. Russakovskii, The matrix Sturm-Liouville problem with spectral parameter in the boundary conditions, Algebraic and operator aspects, Trans. Moscow. Math. Soc. 57 (1996) 159-184. 18. A. A. Shkalikov, Boundary problems for ordinary differential equations with parameter in the boundary conditions, J. Soviet. Math. 33 (1986) 1311-1342.
Functional Analysis and its Applications V. Kadets and W. Zelazko © 2004 Elsevier B.V. All rights reserved
195
On the Automorphisms and Multipliers Related to Generalized Integration Operators Swietlana Minczewa-Kamiriska a institute of Mathematics, University of Rzeszow, Rejtana 16 A, 35-310 Rzeszow, Poland
Abstract We give necessary and sufficient conditions for multipliers of a convolution of the generalized integration operator to be topological automorphisms in the space of continuous functions. Moreover, an equivalent form of the conditions is found in terms of cyclic elements of the considered integration operator. Key words: Generalized integration operator, convolution of generalized integration operator, commutant, multiplier, cyclic element. 2000 MSC: 45D05, 45E10, 45P05, 46E15
1. Introduction Due to the Titchmarsh theorem, the convolutional algebra of continuous functions on the positive half-line has no divisor of zero which makes it possible to construct the field of the convolution quotients, called Mikusiriski operators, the objects interesting both for their mathematical elegance and numerous applications (see [8]). Though the Titchmarsh theorem is not true on the whole real line, the space of continuous functions (on an arbitrary interval A containing 0, bounded or not) remains an annihilators-free convolutional algebra with respect to the Duhamel convolution and there is an interesting interplay between the Duhamel convolution, the multipliers (in the sense of Larsen [6]) and continuous automorphisms of this algebra commuting with the Volterra integration operator (see [2] and [9]).
196
Swietlana Minczewa-Kaminska
Together with a general notion of the Dimovski convolution introduced in [1], embracing the Duhamel convolution as a particular case, it appeared a problem of mutual relations between this notion, the generalized integration operator and the multipliers of this convolution in various classes of functions. Several papers (see e.g. [2], [9], [3]) were devoted to a study of many aspects of this problem. In this paper, we are interested in giving a convolutional representation of multipliers of the Dimovski convolution in the space C(A) of continuous functions on A. The main result (Theorem 12) is a characterization of the topological automorphisms on C(A) among multipliers of the Dimovski convolution. We also give (see Theorem 14) necessary and sufficient conditions for continuous functions to be cyclic elements of the generalized integration operator in C(A). We begin with some general definitions. Let X be a linear space over the field C of complex numbers and let L: X —> X be a linear operator. A bilinear, commutative and associative operation ©: X x X —> X is said to be a convolution of the linear
operator L if L(x®y) = {Lx)®y,
x,y G X
and the pair (X, ©) is called a convolutional algebra. The convolutional algebra (X, ©) is annihilators-free if x ® y = 0 for all x G X implies y = 0. An element d of (X, ©) is a divisor of zero of the convolution © if d ^ 0 and d ® a = 0 for a certain a E l , f l / 0 . A linear operator L: X ^ I i s said to be a convolutional operator if there exists an r G X such that Lx = r © x,
x G X,
(1)
where © is a convolution of L. Definition 1. A linear operator M : X —> X is said to be a multiplier of the convolutional algebra (X, ©) if M(x ®y) = (Mx) © y for all x, y G X. Due to [7], the multipliers of annihilators-free convolutional algebra (X, ©) are linear operators on X and form a commutative ring. By [6], if a linear topological space X has the closed graph theorem property, the convolutional algebra (X, ©) is annihilators-free and the convolution © is separately continuous, then every multiplier of (X, ©) is a continuous operator. Definition 2. An operator A: X —» X, where X is a linear topological space, is called a topological automorphism of X if it is a linear operator and a homeomorphism on X. Let XD be a subspace of a linear space X and let D : XQ —> X be a linear operator. A linear operator R : X —> Xp is said to be a right inverse of D, if DRx = x for each x G X. According to Dimovski [1], if a convolutional operator L given by (1) is a right inverse operator of D, then each multiplier M of the convolutional algebra (X, ©) has the form
On the Automorphisms and Multipliers Mx = D(m ® x),
where m := Mr.
197 (2)
In this paper we will assume that X = C(A), where A is an arbitrary (finite, infinite, closed, open, or half-open) interval containing zero, i.e. X is a Banach space in case A is a compact interval and is a Frechet space in case A is a noncompact interval.
2. Dimovski convolutions in C(A) We will study the right inverse operator of the differentiation D = d/dt with a given boundary value condition, i.e. the operator L = L$ which assigns to each / € C(A) the solution y = Lf of the boundary value problem y' = f,
$(?/) = 0,
where $ is a nonzero linear continuous functional on C(A). By [1, p. 69], a linear continuous operator R : C(A) —> C(A) is a right inverse of the differentiation D = d/dt iff it admits a representation of the form t
Rf(t)= J f(T)dT + T(f) 0
with a continuous linear functional T on C(A). Consequently, the operator L$ is represented in the form:
L*f(t) = Jf{T)dT-$ljf(T)dT\,
(3)
under the condition that the restriction of $ to C rl (A) is I — L$>D (necessary for $ to be so-called defining projector of L$ - see [1, p. 40-41]). The linear continuous operator L$ given by (3) will be called the generalized integration operator. By the Dimovski convolution, we mean the operation *: C(A) x C(A) —> C(A) defined for a given nonzero linear continuous functional $ on C(A) and f,g& C(A) by the formula:
(ftg)(t):=^x{Px{f,g)},
(4)
where the symbol $ x means that $ acts on x only and t
Ix(f,g):=Jf(x + t-T)g(T)dT.
(5)
X
In [1, p. 62], Dimovski introduced the above convolution * and proved that * is a bilinear, commutative, associative and separately continuous operation on C(A)
198
Swietlana Minczewa-Kamiriska
and the algebra (C(A), * ) is annihilators-free. One can prove that * is a convolution of the generalized integration operator L$ given by (3). Example 3 . If <&(/) = /(0), the generalized integration operator L$ given by (3) coincides with the Volterra integration operator I given for / G C(A) by t
lf(t):= Jf(T)dT 0
and the Dimovski convolution * in C(A) coincides with the Duhamel convolution * defined for f,g £ C(A) by t
(f*9)(t):= Jf(t-T)g(r)dT.
(6)
o All multipliers of the Duhamel convolution in C(A) and all automorphisms among them are described in [2]. Example 4. In case $ = E, where E(f) ~ ^(/(0) + / ( l ) ) and [0,1] C A, the generalized integration operator L$, called in this case the Euler integration operator, is of the form l
t l
LEf{t) = J f{T)dr- -J o
f{r)dT o
and the convolution * in C(A) is given by l
v t
iS*m = \ Jf(t-T)g(r)dT-Jf(l+t-r)g(T)dT . Lo
t
Example 5. In case $ = B, where B(f) := JQ / ( r ) dr and [0,1] C A, the generalized integration operator L
t
LBf(t) = J f(r) dr - J(1 - T)f(r) dr 0
0
and the convolution * in C(A) is of the form
On the Automorphisms and Multipliers
if*9)(t) = jljf(x 0
199
+ t~T)g(r)dr[dx.
[x
)
3. Multipliers of Dimovski convolution Let us normalize <3? £ (C(A))', $ 7^ 0, by imposing on $ the condition ${1} = 1.
(7)
Then operator L$ defined in (3) is a convolutional operator of the form L*f = {1} * / ,
/ e C(A),
where {1} denotes the constant function on A. By the Riesz-Markov theorem (see [5], Theorem 4.10.1), $ has a compact support, i.e. there are a compact interval [a,0\ C A and a function ui of bounded variation on [a, /3] such that 0
*(f)=Jf(x)du(x). a
The case where a; is a jump-function is described in [3]. We will assume further on that u> £ AC[a,0\ and v := to' € BV[a,/3]. In this case (see [9], p. 50) there exists a * e (C(A))', * 7^ 0, such that
*(/) = ** I / /W dr I = W)> / eC(A)-
(8)
Then the convolution * given by (4) maps C(A) x C(A) in C (A) and the derivative of the convolution (/ * g) defined in (4) is of the form
(f*gy(t)=f(tMg)+9m(f) -*{l}(/*fl)W+*x{4(/.ff)}.
(9)
where * is the Duhamel convolution defined by (6) and I\. is given by (5) (see [1, p. 67]). Lemma 6. ([1, p. 75]) The operation * : C(A) x C(A) -> C(A) given by
(f*9)(t) := f(tWg)+9m(f)
- *{1}(/ * g)(t) + * s {£(/)5)}
(10)
is a convolution of the generalized integration operator of the form L*/ = //-*(/ 2 /)
(11)
200
Swietlana Minczewa-Kamirlska
with \I/ £ (C(A))'. The operator L* is a convolutional operator of the form L * / = r* f with r := 1{1} — \I/(Z2{1}) and (C(A), *) is a convolutional algebra with a unit, i.e.{l}if = fforfeC(A). Now we will characterize all multipliers of the convolution * defined by (4) with $ of the form (8).
Theorem 7. A linear continuous operator M : C(A) —> C(A) is a multiplier of £/ie Dimovski convolution * given by (4) with $ of the form (8) iff
Mf(t) = f(tMm)+m(tWf) -tt{l}(m * / ) ( « ) + ^ { I ^ m , / ) } ,
(12)
where m := M{\] £ C(A). Proof. It is clear that every operator M of the form (12) satisfies the identity M(f
* g) = (Mf) * g for / , g £ C(A). On the other hand, if M is a multiplier of
the convolution * of the form (4), then equations (2) and (9) imply (12).
•
Corollary 8. A linear continuous operator M: C(A) —> C(A) is a multiplier of i/ie convolution * wii/i $ given by (8) iff Mf = mi f where m := Af{l} G C'(A) and * is defined by (10). Lemma 9. If the multiplier M of the convolution * , given by (12) with * £ (C(A))', satisfies the condition ^>(lm) = 0, i/ten
*(ZM/) = 0,
/ £ C(A).
(13)
Proof. It follows from the assumptions that
*(ZM/) = - * t * x J /" m(r) dr /" /(a) da I +tttttx{h(t,i ) } ,
lo
o
J
"|
x
where t
h(t,x) =
rt+x-T
17I(T) o
rt+i-T
I f(a)da dr — I m{r) j f(a)da L t-r Jo LX-T
dr.
Since h(t,x) = —h(x,t), the assertion follows from the Fubini theorem.
•
On the Automorphisms and Multipliers
201
Define the operator T, for / £ C(A), by Tf(t) := m ( i ) $ ( / ) - M>{l}(m * /)(*) + * s {^(m, / ) } .
(14)
Lemma 10. Let A be a compact interval. Then T, given by (14) with m £ C(A), is a compact operator in the space C(A). Proof. The assertion follows due to the Arzela-Ascoli theorem, applied to each of the addends in the representation (14) of the operator T (see [9]). • From Lemma 10 one can easily conclude the following assertion: Corollary 11. Every operator T of the form (14) with m £ C(A) is compact in C(A) also in case A is a noncompact interval. Theorem 12. A multiplier M of the convolutional algebra (C(A), * ) with $ given by (8) is a topological automorphism on C{A) iff the following conditions hold: (a) (b)
M{1} is not a divisor of zero of the convolution * ; *(Zm) ^ 0, where m := M{1}.
Proof. Due to Lemma 2 in [2], it suffices to show that conditions (a) and (6) are necessary and sufficient for M of the form (12) to be invertibile. Assume that M is a one-to-one linear mapping and condition (a) is not fulfilled, i.e. M{1} * / = 0 for some non-zero function / £ C(A). But then the operator M defined in (12) is not injective, contrary to the assumption. If (b) does not hold, then (13) follows by Lemma 9, which contradicts (7) and so the surjectivity of the operator M. Assume (a) and (b). By (a), (9) and (7), it follows that M is an injection. To prove that M is a surjection consider the equation m*f = g.
(15)
Since M is an injection and T given by (14) is compact, equation (15) has a unique solution / for a given g £ C(A), according to (b) and the Fredholm alternative. •
4. Cyclic elements of L in C(A) In this part, we suppose that $ e (C(A))' is of the form (8) with * £ (C(A))' and denote, for simplicity, the generalized integration operator L$ by L. We will use the convolution * to characterize explicitly the cyclic elements (in C(A)) of the operator L. We start from a general definition:
202
Swietlana Minczewa-Kamiriska
Definition 13. For an arbitrary linear continuous operator S on C(A), a function k € C(A) is said to be a cyclic element of the operator 5 if the span of {Snk}%'=1 is dense in C(A). Theorem 14. A function k G C(A) is a cyclic element of the operator L in the space C(A) i/f k is not a divisor of zero of the convolution * and *5>(lk) ^ 0. Proof. First assume that k is a cyclic element of L and a divisor of zero of the convolution * . Then there exists a j € C(A), g ^ 0 such that k * g = 0. Hence L(k t g) = 0 and so (Lnfc) * g = 0 for all n e No := N|J{0}. Consequently, / * g = 0 for every / G C(A), but this contradicts the identity Lg = {1} * g. Let now k be a cyclic element of L and >3>(£fc) = 0. Let An be the Appell polynomials, i.e. An(t) := £ n { l } for t & (—00,00) and n € No- Since Lfc = {1} * k, we have Ln+ k = An(t) * k for n e No or, due to formula (9),
Lnk(t) = An(t)$(k) + k(t)$(An) -*{l}(^ n *fc)(i) + * x {/*(A n ,fc)}
(16)
for t G (—00,00). This is an equation analogous to (12). By Lemma 9, the condition ty(Ik) = 0 implies $(Lnfc) = 0 for n = No- Therefore, {1} cannot be approximated by means of linear combinations of Lnk, in view of (7). This proves the necessity of the condition ^f(lk) ^ 0. Let now k € C(A) satisfy the condition ty(lk) j^ 0 and be not a divisor of zero of the convolution * . We will show that A; is a cyclic element of L in C(A). Fix / e C(A). We look for a function g £ C(A) such that /(*) = $ ( % ( t ) + *(*)$() - *{l}(fc * g)(t) +
.
(17)
The operator T, given by
Tg(t) := k(t)$(g) - *{l}(fc * g)(t) + <SX {ll(k,g)} , is of the form (14). By Lemma 10 and Corrolary 11, the operator T is compact. Since ^(lk) =£ 0, equation (17) is a Fredholm integral equation of the second kind. But k is not a divisor of zero of the convolution * , so the function g = 0 is the unique solution of the homogeneous equation k* g = 0, which guarantees the existence of a unique solution g of (17). Let {gn}^Lo be a sequence of polynomials converging almost uniformly to g in C(A), which can be represented in the form gn = Y^j=o ajn-^j f° r « £ No, where Aj are the Appell polynomials. Let fn := ^ n _ 0 a^nlJk. By (16), we can write
fn(t) = $(k)gn(t) + k(t)$[gn(t)) - *{l}(k * gn)(t) + * x {/*(fc, gn)} . Hence the sequence {fn}^Lo converges almost uniformly to the function / in C(A), due to (17). Therefore, k is a cyclic element of L in C(A). •
On the Automorphisms and Multipliers
203
The above characterization allows us to reformulate Theorem 12 as follows: Theorem 15. A multiplier M of the convolutional algebra (C(A), * ) with $ defined in (8) is a topological automorphism on the space C(A) iff the function m := M{1} € C(A) is a cyclic element of the operator L. References 1. I. Dimovski, Convolutional Calculus ( Kluwer Acad. Publ., Dordrecht, 1990). 2. I. Dimovski, S. Mincheva, Automorphisms of C which commutes with the integral operator, Integral Transforms and Special Functions 4 (1996) 69-76. 3. I. Dimovski, A. Kamiriski, S. Mincheva, The commutant of an integration operator with multipoint functional, Fractional Calculus & Applied Analysis 4 (2001) 245-254. 4. I. Dimovski, S. Grozdev, Bernoulli operational calculus, in: Mathematics and Education in Mathematics, (Sofia, 1980) 30-36 (in Bulgarian). 5. R. Edwards, Functional Analysis. Theory and Applications. Holt, Rinehart and Winston, New York, 1965. 6. R. Larsen, An Introduction to the Theory of Multipliers. Springer-Verlag, Berlin, 1972. 7. L. Mate, Multiplier operators and quotiend algebra, Bull. Acad. Polon. Sciences, Ser. Math. Astr. et Phys. 13 (1972) 523-526. 8. J. Mikusinski, Operational Calculus, vol. I—II, PWN-Pergamon Press, Warszawa, 1983, 1987. 9. S. Mincheva, Automorphisms commuting with integration operators in some functional spaces, Institute of Mathematics and Informatics, Bulgarian Academy of Sciences (Sofia, 2000) 1-151 (Ph.D. Dissertation; in Bulgarian).
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Functional Analysis and its Applications V. Kadets and W. Zelazko © 2004 Elsevier B.V. All rights reserved
205
On Some Classes of Mappings Preserving of Measure Oksana A. Ochakovskaya Institute of Applied Mathematics and Mechanics NAS Ukraine, Donetsk, Ukraine
Abstract Main result in the present paper contains the conditions which give that certain oneto-one mapping is a measure-preserving transformation. Some of these conditions can not be relaxed. Key words: Measure-preserving transformations, ergodic theory 2000 MSC: 28D05
1. Introduction Measure-preserving transformations plays an important role in ergodic theory and related questions (see, for instance, [1], [2] and the bibliography therein). In the present paper we study such transformations acting from W1 into R™. Throughout, we assume that n > 2. Denote by Cfe(]Rn,Kn) the collection of all Ck - mappings from Rn into Rn. For
r > 0, y G Rn we set Br(y) = {x&Rn : \x-y\ < r}, Sr{y) = {x G Rn : \x-y\ = r}, where | • j is the Euclidean norm in R n . We write m(G) for Lebesgue measure of the set G C W1. Let / * g be a convolution of functions / and g. Denote by XG the characteristic function of the set G C R™. For r > 0 let Vr(M.n) be a collection of all functions / £ C(Wn) with zero integrals over each ball with radius r. We set also A n = {t > 0 : t = | , where J%(a) = J%{/3) = 0, j3 ± 0}, where Jv is the Bessel function of order v. Let En = {x G Rn : xn > 0}.
206
Oksana A. Ochakovskaya
2. Main results Theorem 1. Assume that the injective map F G C 1 (M ra ,R n ) satisfies the following conditions: a)m{F(Bl{y))) = m{Bl{y)) for all y&Rn; b) there exist a positive numbers Mq, q = 1, 2,... such that
f ; ( m f M*) ' = 00
(1)
and
J
\m(F(Br(y)))-m(Br(y))\(l
+ \y1\ + ... + \yn_1\)'>dy1...dyn_1<Mqea^
(2)
R"-i
/or some a > 0 and all yn G R1, g € N. TTien m(F(G)) = m(G) for each Lebesgue measurable set G C K™. Theorem 2. for every r > 0, a > 0 and every a sequence {Mq}q*Ll of positive numbers such that °° / A""1 > inf Mq9 ) < oo (3) i/iere eiisis a one-to-one mapping F € C1(En, En) with positive Jacobian such that m{F(Bx(y))) = m(B1{y)) for all B1(y) C En and f \m{F(Br{y)))-m(Br(y))\{l
+ \y1\ + ... + \yn-1\)idy1...dyn-l
<Mqe~a^
(4)
R»-l
for all yn > r, q € N. Moreover m(F(B)) ^ m(B) for some ball B C En. Theorem 3. For each r G Ara there exists an one-to-one mapping $ £ C°°(]Rra,]Rn) wii/i positive Jacobian such that m($(Bi(y))) = m(B\(y)) and m($(Br(y))) = m(Br(y)) for all y e I " . Besides, m(${B)) ^ m(B) for some ball B C W1.
3. Proofs To prove the main results we require the following auxiliary statements: 1) Let f G Vr(Mn) and assume that there exist a positive numbers Mq,q = 1,2,... satisfying (1) such that the following inequality holds
J \f(Xl,...,xn)\(l
+ \Xl\ + ... + \xn-1\)«dx1...dxn^1
for some a > 0 and all xn G R 1 , q G N. Then / = 0.
<Mqea^
(5)
On Some Classes of Mappings Preserving of Measure
207
2) For every a > 0 and every a sequence {Mq}qxLl of positive numbers satisfying (3) there exists a real-valued function fa £ Vr(Rn) nC°°(R n ) such that
J l/afo, ...,z n )|(l + |*i| + ... + \xn.l\)"dx1...dxn.1
< Mqe'ax-
for all xn > 0, q G N. Besides, the function S^f- is nonzero and bounded in En. The proof of this statement can be obtained by repeating the arguments from the paper [3]. We proceed now to the proof of the main results. Proof of Theorem 1. Using the formula m(F(G)) = J \J(F, x)\dx, where J(F, x) G
is the Jacobian of mapping F, we can rewrite the condition a) in Theorem 1 as / (\J(F, x) - 1) dx = 0 for all y eRn
(6)
Bi(y)
Besides
m(F(Br(y)))-m(Br(y))=
J
(| J(F,x)\ - l)dx = v *XBr = 0,
(7)
BAy)
where v(x) = \J(F,x)\ - 1. Thus the function / = v * XBT satisfies the condition (5). Hence, / = 0 on W1. Taking into account that r ^ A n , by two-radii theorem (see, [4]) we obtain that v = 0. This means that m(F(G)) = m(G) for every Lebesgue measurable set G C W1. The proof of Theorem 1 is now complete. Proof of Theorem 2. Let a > 0, r > 0 and assume that the sequence {Mq}^L1 M ear satisfies (3). Then the sequence M'q = -2— also satisfies (3). We set (2 -|- r)Q(n — l)q
ip(x) = fa(x) where fa is a function in Lemma for the sequence M'. Then —— < C for all x s En. We consider the mapping F(x) = (Fi(x),...,Fn(x))
\
n™/2rn~l
OX\
= (x± +
-\
——, x 2 ,..., x n ), where N > max < C, —-—-r— >. Then we have •^ I 1 V"2 ) J We now claim that F is one-to-one mapping. Let x,x' € En such that x =fi x'. If (x2,—,xn) ^ (x'2i..-,x'n) we see that F{x) / F(x'). Otherwise, (x 2 ,...,x n ) = (x 2 , •••,x'n) and X\ ^ I'J. In this case the F(x) ^ F(x') since the function F\(x) = xi H
!-T— is increasing with respect to variable xi. Indeed, from the definition of dFi 1 dip N we have the inequality —— = 1 + —: 7:— > 0. This yields that F is one-to-one. dxi N dxi We now prove the condition b). Setting sq(x) = (1 + |xi| + ... + |x ra _i|) 9 for x = (xi, ...,x n ) £ IRra, we obtain
208
Oksana A. Ochakovskaya f \m(F(Br{y)))
- m(Br(y))\sq(y)dy1...dyn_1
=
R"
J Jf~g^dx
= J
sq{y)dy1...dyn-1.
Using Green's theorem we estimate the left part of last equality by the expression
•jj /
I
/ \if(yi'--,yn-i,yn+Xn)\sq(y-x)dy1...dyn-1\ 1
Sr(0) V K " where da(x) is the surface element of sphere Sr(0). Further, for x € 5 r (0) and y £ R™"1 we have
sq(y-x)<(n-l)"(2
da(x)
(9)
/
+ ry8q(y)
Then (9) can be estimated by the expression
^ ( n - l ) ? ( 2 + r)« J ( J
\
5 r ( 0 ) R™-1
•sg{y)dy1...dyn-i)d*(x) < Mqe~a^+X^
<
Mqea^e~a^
Bearing in mind that
P. Billingsley, Ergodic Theory and Information. John Wiley and Sons, New York, 1965. I.P.Kornfeld, J.G. Sinay, S.V. Fomin, Ergodic theory. Nauka, Moskow, 1980. (In Russian). O.A. Ochakovskaya, Functions with zero integrals over balls with fixed radius, Mathematical Physics, Analysis, Geometry 10 (3) (2002) 43-51. V.V. Volchkov, A definite version of the local two-radii theorem, Math. Sb. 186 (6) (1995) 15-34; English transl. in Sbornik Math. 186 (1995).
Functional Analysis and its Applications V. Kadets and W. Zelazko © 2004 Elsevier B.V. All rights reserved
209
Extreme Problems and Scales of the Operator Spaces Igor V. Orlov Taurida National V. Vernadsky University, Simferopol, Ukraine
Abstract The repeated compact-normal differentiability of the Euler-Lagrange functional is proved. The sufficient extreme conditions for such a functional in the case of one and two variables are obtained. Key words: Euler-Lagrange functional, locally convex space, inductive scale of spaces, extreme problems, nuclear space, normal derivative, compact extremum 2000 MSC: 58C20, 46T20, 46A03
Introduction The extreme problems for integral functional play an important role in the modern nonlinear analysis and its application. Diverse methods are employed for the investigation of these problems (see, e.g. [1-3]). One of the fundamental difficulties arising in these questions is absence, with the exception of trivial cases [16], the second strong derivative for general integral functionals. The other aspect of the problem above is that extremae of such functionals are seek, as a rule, on some compact set. These cases exclude application of the classical Frechet extreme conditions and enclose the investigation in the framework of the (in any case generalized) variational calculus. In the present work, on the contrary, the notion of strong differentiability is rather weakened. As a result, the modified Frechet extreme conditions are extended to the extremae of integral functionals on compact sets. The obtained results are new both in the general case of integrand function taking values in locally convex space (LCS) and in the classical scalar or Banach case.
210
Igor V. Orlov
The work consists of two sections. In the first section the extreme theory for the normally differentiable and if-differentiable functions in LCS is constructed. The normal differentiability and the repeated if-differentiability of Euler-Lagrange functional are proved. It allowed to obtain the sufficient if-extreme conditions for such a functional. In the second section the sufficient extreme and if-extreme conditions for the two variables functions in the products of the nuclear spaces are obtained. It allowed to obtain the sufficient if-extreme conditions for two variables Euler-Lagrange functional.
1. .K"-extremae of the integral functionals As it was shown by I.V.Skrypnik [1], the integral functionals of the classical Euler-Lagrange functional type 6
$(j/) = J f(x,y(x),y'(x))dx
(1)
a
are not, in general, twice Frechet differentiable. It is shown by M.Z.Zgurovsky and V.S.Melnik that the derivatives of such functionals are T-differentiable (see [19,7]). We'll show that the functional (1) satisfies a much more strong requirement of the repeated if-differentiability, even in the case of mapping y(-) into LCS. It allows us to apply the classical extreme conditions in terms of ii'-derivatives for investigation of the compact extremae (or, iiT-extremae, def. 17) for such a functional. The introduced below notion of normal and (further) compact - normal differentiability (or, X-differentiability) is jointly connected to decompositions of the operator spaces into the inductive scales of LCS. In what follows, E, Ei,F, F^ are LCS with the corresponding defining systems of semi-norms {|| • \\t}teT, {\\ • I k k e i o {|| • || s } s e5, {|| • || Sj }^es 3 -, inductively ordered in ascending order of the semi-norms; (E; F) is a space of the linear continuous operators acting from E to F; (Ei,E2',F) is a space of the bilinear continuous operators acting from E\ x E2 to F. Definition 1. Let A G (E;F). Assume, for any s G S, nA(S)
= {t£T
: \\A\\'t := sup ||Ar|| s < + 0 0 } .
The multivalued mapping UA '• S —> ray(T), here ray(T) is the set of rays in T, is called the normal index, or n-index of the operator A; the quantities ||A||| are called the co-norms. The main properties and examples of normal indices are considered in [8,9].
Extreme Problems and Scales of the Operator Spaces
211
Definition 2. Let J\f = Af{E; F) be set of the normal indices of operators from (E; F). Put, for every n G M, (E; F)n = {A G (E; F) : nA^n}. Provide the every (E; F)n with the projective topology rn relative to the defining systems of semi-norms {|| • ||t}ten(s)>s £ S. The inductive scale of LCS {ETF):={((E;F)n,rn)}neM
(2)
is called the normal decomposition of the space (E; F). An information about inductive scales of LCS see in [17,4]. Note that the scales under consideration below are more general than the classical interpolational scales and the S.G.Krein-Yu.I.Petunin scales [5,6]. By analogy with the decomposition (2), one can introduce the normal indices and decompositions into the inductive scales of LCS for the space of linear continuous operators, acting from Ei to {E^F):
(Ei;(E2;F)], and for the space of bilinear continuous operators, acting from E\ x E2 to F : (EX,E2-F).
Proposition 3. (The canonical isomorphism of normal indices for the linear and bilinear operators [10]). The canonical relation B{hi,h,2) = {Ahi)li2 between the linear operators A : E\ —» {E2\ F) and bilinear operators B : Ei x E2 —• F generates an isomorphism of the corresponding normal indices. In addition, the corresponding spaces of scales {E\; (E2; F)) and ((E\,E2\F) are isometrically isomorphic; that allows to say about an isometric isomorphism of the normal decompositions: (E^iE^F))
- (EltE2;F).
(3)
Definition 4. Let a mapping if : E —> F be defined in some zero neighborhood of E. Say that ip{h) = o(h) if Vs € S3t e T : (||¥>(/0||7l|ft||t) ~> ° a« h -> °Definition 5. A mapping / : E —> F defined in some neighborhood of x G E is called normally differentiable at the point x if Af(x,h) = Axh +
212
Igor V. Orlov
proposed above is well known in infinite-dimensional differential calculus. This approach is closed to the names of D.H.Hyers, H.R.Fisher, S.Lang, E.Binz and a number of other mathematicians (see, e.g., survey [1]). The distinction of our approach is consideration of the first normal derived mapping as a mapping from E to the scale (E;F).As the result, beginning with the continuous differentiability the proposed approach essentially differs from the abovementioned one and leads to some new applications. At first, let formulate the "normal form" of the mean value theorem [9].
Proposition 6 (Normal form of the mean value theorem). Let E and F are real LCS, [a; b] C E,D be finite or countable subset of [a; b], f : [a; b) —> F. If f is continuous on [a;b] and normally differentiable on [a;b]\D, here n/(x) =4 n G N for x G [a; b]\D, then for all s £ S and t G n{s): \\f{b)-f{a)\\s^
sup
||/'(x)||M|6-a||t.
(4)
xe[a;fa]\D
A typical situation for which the upper bound (4) is applicable, is the continuous normal differentiability, that is the continuity of the mapping f':E—> (E;F). Definition 7. Let a mapping / : E —> F be continuously normally differentiate at a point x £ E. Then the derived mapping f : E —> (E; F) can be considered at some neighborhood of x as the mapping to some LCS (E;F)n, n G J\f. If / ' : E —> (E; F)n is normally differentiable at a point x then we'll say that / is twice normally differentiable at the point x; moreover f"(x) := (f')'(x). Analogously, one can defined the normal derivatives f^(x), k > 2. Note that by virtue of the canonical isomorphism (3), f"{x) can be considered as a bilinear continuous operator. So, / " : E —> (E,E; F), in addition the corresponding co-norms coincide: \\f"(x)\\%> = ||/"(x)||f lt2 . Definition 8. Say that a mapping r : E —> F defined in some zero neighborhood in E is the small mapping of the order k (k = 0,1,2,...), or r(h) = o((/i)fe), if \/seS
BtGT:
lim(||rW||7(||ft|| t ) f e )=0.
Theorem 9 (Taylor's formula in the asymptotic form). If a mapping f : E —> F is m times normally differentiable at a point x G E then m
f{x + h) = Y,
{k)
T]f
{x){h)k + o((h)n).
(5)
The proof see in [13]. Let introduce now a notion of the positive definite quadratic form in LCS [12].
Extreme Problems and Scales of the Operator Spaces
213
Definition 10. Let ip be a continuous quadratic form in LCS E generated by a bilinear form g on E2. The form ip is called nondegenerate if
inf "f',5>0 Mtj^o
(6)
|[z||tl
for some t\, £2 £ ng. If
= 0)
=> (an = 0).
Theorem 12. (Condition of positive definiteness, [12]). If ip 2> 0 on LCS E then there exist such index t s T and constant Ct > 0 that