Series Analysis and Schwartz Algebras of Spherical Convolutions on Semisimple Lie Groups
Olufemi O. Oyadare

TL;DR
This paper explores the harmonic analysis of spherical convolutions on semisimple Lie groups, focusing on the Harish-Chandra transform and Schwartz algebras, and clarifies the role of the Trombi-Varadarajan Theorem in this context.
Contribution
It provides exact descriptions of the Harish-Chandra transform of Schwartz functions and demonstrates how the Trombi-Varadarajan Theorem applies to spherical convolution transforms.
Findings
Explicit characterization of the Harish-Chandra transform for Schwartz functions
Connection established between spherical convolutions and $L^{p}$-Schwartz algebras
Proof of the role of Trombi-Varadarajan Theorem in harmonic analysis
Abstract
We give the exact contributions of Harish-Chandra transform, of Schwartz functions to the harmonic analysis of spherical convolutions and the corresponding Schwartz algebras on a connected semisimple Lie group (with finite center). One of our major results gives the proof of how the Trombi-Varadarajan Theorem enters into the spherical convolution transform of Schwartz functions.
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Taxonomy
TopicsAdvanced Algebra and Geometry · Mathematical Analysis and Transform Methods · Homotopy and Cohomology in Algebraic Topology
**Series Analysis and Schwartz Algebras of Spherical Convolutions on Semisimple Lie Groups.
**
**Olufemi O. Oyadare
**
Abstract. We give the exact contributions of Harish-Chandra transform, of Schwartz functions to the harmonic analysis of spherical convolutions and the corresponding Schwartz algebras on a connected semisimple Lie group (with finite center). One of our major results gives the proof of how the Trombi-Varadarajan Theorem enters into the spherical convolution transform of Schwartz functions.
Subject Classification:
Keywords: Harish-Chandra Transforms; Semisimple Lie groups; Harish-Chandra’s Schwartz algebras
** Introduction
**
Let be a connected semisimple Lie group with finite center, and denote the Harish-Chandra-type Schwartz spaces of functions on by , We know that for every such , and if is a maximal compact subgroup of such that represents the subspace of consisting of the bi-invariant functions, Trombi and Varadarajan ([]) have shown that the spherical Fourier transform is a linear topological isomorphism of onto the spaces ,
Obafemi Awolowo University, Ile-Ife, Nigeria.
E-mail: [email protected]
consisting of rapidly decreasing functions on certain sets of elementary spherical functions.
We show the existence of a hyper-function on both and (here named a spherical convolution) whose restriction to the group identity element, coincides with the spherical Fourier transforms, of Schwartz functions on and which affords us the opportunity of embarking on a more inclusive harmonic analysis on Indeed contains a more general Plancherel formula for the collection of these functions. As a function on its series expansion is in the present paper studied. We show that, aside from the fact that the spherical Fourier transforms, is the constant term of this series expansion, there is a region in where the spherical convolution is essentially Various algebras of these functions are thus studied and ultimately embedded in It is however clear that the results in and in the present paper may be extended to include what may be termed as the Harish-Chandra-type Schwartz spaces of Eisenstein Integrals on The author has recently used the idea of a spherical convolution to give an explicit computation of the image of under the Harish-Chandra transform, thus giving a concrete realization of the abstract results of Arthur, and showing the direct contribution of the Plancherel formula to Harish-Chandra transform on
The following is the breakdown of each of the remaining sections of the paper. contains the preliminaries to the research containing the structure theory, spherical functions and Schwartz algebras on while the series analysis of spherical convolutions on is the subject of The relationship existing among the Schwartz algebras of functions and those of spherical convolutions is considered in
** Preliminaries
**
For the connected semisimple Lie group with finite center, we denote its Lie algebra by whose Cartan decomposition is given as Denote by the Cartan involution on whose collection of fixed points is We also denote by the analytic subgroup of with Lie algebra is then a maximal compact subgroup of Choose a maximal abelian subspace of with algebraic dual and set For every put
[TABLE]
and call a restricted root of whenever
Denote by the open subset of where all restricted roots are and call its connected components the Weyl chambers. Let be one of the Weyl chambers, define the restricted root positive whenever it is positive on and denote by the set of all restricted positive roots. Members of which form a basis for and can not be written as a linear combination of other members of are called simple. We then have the Iwasawa decomposition , where is the analytic subgroup of corresponding to , and the polar decomposition with and denoting the closure of
If we set , and and call them the centralizer and normalizer of in respectively, then (see , p. ); (i) and are compact and have the same Lie algebra and (ii) the factor is a finite group called the Weyl group. acts on as a group of linear transformations by the requirement
[TABLE]
, , , the complexification of . We then have the Bruhat decomposition
[TABLE]
where is a closed subgroup of and is the representative of (i.e., ). The Weyl group invariant members of a space shall be denoted by the superscript w while represents the cardinality of
Some of the most important functions on are the spherical functions which we now discuss as follows. A non-zero continuous function on shall be called a (zonal) spherical function whenever : , , and for every where This leads to the existence of a homomorphism given as . This definition is equivalent to the satisfaction of the functional relation
[TABLE]
It has been shown by Harish-Chandra [] that spherical functions on can be parametrized by members of Indeed every spherical function on is of the form
[TABLE]
where and that iff for some Some of the well-known properties of spherical functions are while Also if is the Casimir operator on then
[TABLE]
where and for elements , This differential equation may be written simply as where is the well-known Harish-Chandra homomorphism. The elements , are uniquely defined by the requirement that and for every ([], Theorem ). Clearly
Due to a hint dropped by Dixmier in his discussion of some functional calculus, it is necessary to recall the notion of a ‘positive-definite’ function and then discuss the situation for positive-definite spherical functions. We call a continuous function (algebraically) positive-definite whenever, for all in and all in we have
[TABLE]
It can be shown that and for every implying that the space of all positive-definite spherical functions on is a subset of the space of all bounded spherical functions on
We know, by the Helgason-Johnson theorem (), that
[TABLE]
where is the convex hull of in Defining the involution of as , it follows that for every , and if , then and are Weyl group conjugate, leading to a realization of as a subset of becomes a locally compact Hausdorff space when endowed with the weak topology as a subset of .
Let
[TABLE]
be denoted as and define as
[TABLE]
for every where is a norm on the finite-dimensional space These two functions are spherical functions on and there exist numbers such that
[TABLE]
Also there exists such that ( p. ). For each define to be the set consisting of functions in for which
[TABLE]
where the universal enveloping algebra of and We call the Schwartz space on for each and note that is the well-known (see ) Harish-Chandra space of rapidly decreasing functions on The inclusions
[TABLE]
hold and with dense images. It also follows that whenever Each is closed under involution and the convolution, Indeed is a Frchet algebra ( p. ). We endow with the relative topology as a subset of
We shall say a function on satisfies a general strong inequality if for any there is a constant such that
[TABLE]
We observe that if then, using the fact that and such a function satisfies
[TABLE]
showing that a function on which satisfies a general strong inequality satisfies in particular a strong inequality (in the classical sense of Harish-Chandra, ). Members of are those functions on for which satisfies the strong inequality, for all We may then define to be those functions on for which satisfies the general strong inequality, for all and a fixed It is clear that and that which contains may be given an inductive limit topology. The seminorms defining this topology will be explicitly given in
For any measurable function on we define the spherical Fourier transform as
[TABLE]
It is known (see ) that for we have:
on whenever (or ) is right - (or left-) -invariant; 2.
; hence on and, if we define then 3.
on
We shall denote the spherical Fourier transform of by and refer to it as the Harish-Chandra transforms of Its major properties are well-known and may be found in It should be noted that
That is, the Harish-Chandra transforms of is the restriction of the function
[TABLE]
on to the identity element. It is therefore worthwhile to explore in some details for all in order to put its behaviour at (as the Harish-Chandra transforms of ) in a proper and larger perspective.
The beauty of studying the entirety of the function for which we shall explore in this paper, is that it could be viewed as a transformation in six () different ways; As
[TABLE]
and
[TABLE]
(from where the Plancherel formula for the space of functions has recently been computed in ) both of which are maps on or as
[TABLE]
(which, at led Harish-Chandra to the consideration of ) and
[TABLE]
both of which are maps on or as
[TABLE]
and
[TABLE]
both of which are maps on Hence the function may rightly be called an hyper-function on whose major contribution to harmonic analysis would be to absorb other known functions of the subject and put their results in proper perspectives, as we shall establish here for the *Harish-Chandra transform.
In order to know the image of the spherical Fourier transform when restricted to we need the following spaces that are central to the statement of the well-known result of Trombi and Varadarajan []. Let be the closed convex hull of the (finite) set in , i.e.,
[TABLE]
where we recall that, for every
Now for each set Each is convex in and
[TABLE]
([], Lemma ). Let us define and, for each let be the space of all -valued functions such that is defined and holomorphic on and for each holomorphic differential operator with polynomial coefficients we have
The space is converted to a Frchet algebra by equipping it with the topology generated by the collection, of seminorms given by It is known that above extends to a continuous function on all of ([], pp. ). An appropriate subalgebra of for our purpose is the closed subalgebra consisting of -invariant elements of , The following (known as the Trombi-Varadarajan Theorem) is the major result of Let and set Then the spherical Fourier transform is a linear topological algebra isomorphism of onto That is, the topological algebra is an isomorphic copy or a realization of
In order to find other isomorphic copies or realizations of under the more inclusive general transformation map
[TABLE]
we shall now introduce a more general algebra, of valued functions on which, when restricted to coincides with The form of this new algebra is suggested by Theorem Set and let be the collection of all valued functions () such that
is holomorphic in the variable analytic in and spherical on
and for every holomorphic differential operator with polynomial coefficients and every left-invariant differential operator on and
the restriction of to (or to for some zero neighbourhood in as will later be seen in Theorem ) is (a non-zero constant multiple of) the Harish-Chandra transform,
It may be shown, in exact manner as for above, that the space is converted to a Frchet algebra by equipping it with the topology generated by the collection, of seminorms given by
[TABLE]
An appropriate subalgebra of for our purpose is the closed subalgebra consisting of -invariant elements of , By the time Theorem is established it will be clear that for every in some zero neighbourhood in In particular,
** Series Analysis of Spherical Convolutions
**
Let and we recall from the definition of spherical convolutions, on corresponding to the pair as
[TABLE]
We already know that where is the identity element of and This relation between a function on at the identity element and another function on suggests we study the full contribution of the Harish-Chandra transforms, of to the properties of and to seek other functions on which have not been known in the harmonic analysis of but still contribute to a deeper understanding of the structure of
In order to explore the nature of this idea we consider opening up the spherical convolutions via its *Taylor’s series expansion.
Lemma 3.1. Let be a neighbourhood of origin in and be sufficiently small in (say ). Then
[TABLE]
where for every we set
Proof. The proof follows from a direct application of Taylor’s series expansion,
At and the formula in the Lemma becomes
[TABLE]
[TABLE]
This observation leads quickly to the following result which gives the exact contribution of the Harish-Chandra transforms to the study of spherical convolutions.
Lemma 3.2. *The Harish-Chandra transforms, is the constant term in the (Taylor’s) series expansion of spherical convolutions, around for every
It may be deduced, from the expansion leading to the proof Lemma that the only time the remaining terms in after the (non-zero) constant term could vanish is when the differential operator That is, when It therefore follows that the well-known (Harish-Chandra) harmonic analysis on has always been that of the consideration of the map at only which is the origin of or which corresponds to the identity point of Hence, since the constant term, of corresponds indeed to the consideration of the constant term in the asymptotic expansion of (zonal) spherical functions, it also follows that other terms in the expansion of may be needed to completely understand
The expression for therefore suggests that a full harmonic analysis of may be attained from a close study of the remaining contributions of the transform of given as
[TABLE]
for all and sufficiently small values of in the same manner that its constant term,
[TABLE]
had been considered.
However before considering the transformational properties of spherical convolutions we note the following lemmas which lead to a more inclusive view of the Trombi-Varadarajan Theorem and prepares the ground for its generalization.
Lemma 3.3. Let be a neighbourhood of origin in and be sufficiently small in (say ). Then
[TABLE]
for every
Proof. We note here that
[TABLE]
[TABLE]
Hence
[TABLE]
The particular case of setting and in Lemma introduces the Harish-Chandra transforms, into the analysis of this series, proving the following.
Lemma 3.4. Let be a neighbourhood of origin in and Then the spherical convolution function, is a non-zero constant multiple of the Harish-Chandra transforms, on
Proof. Set and into Lemma to have
[TABLE]
with
Let us denote the non-zero constant in Lemma above by The following theorem is a consequence of normalizing the spherical convolutions in Lemma
Theorem 3.5. (Trombi-Varadarajan Theorem for Spherical Convolutions) *Let set and Set for Then the spherical convolution transforms is a linear topological algebra isomorphism of onto
We recover the Trombi-Varadarajan Theorem for Harish-Chandra transforms by setting in Theorem Indeed, Theorem above says that every (and not just ) gives a topological algebra isomorphism between and However if for any neighborhood of zero in Trombi-Varadarajan Theorem may not be appropriate and it may be necessary to seek a more general realization of under the map f\mapsto l_{1}(\lambda):=s_{\lambda,f}(x),\;\mbox{for any x\in G}. Before considering another major result of this paper, giving the fine structure of spherical convolution functions, we state a result on the finiteness of a central integral usually used in the estimation of many other integrals of harmonic analysis on semisimple Lie groups.
To this end we define, for every the function as
[TABLE]
We observe here that
[TABLE]
which is a constant whose proof of finiteness may be found in This constant is crucial to all harmonic analysis of and, in particular, to the embedding of in It is therefore important to understand the nature of for all in order to employ it in a more inclusive harmonic analysis on We consider the nature of this integral in the following.
Lemma 3.6. Let Then there exist such that
[TABLE]
Proof. We already know that Also
[TABLE]
It follows therefore that
[TABLE]
The last integral in the above inequality is finite if we embark on its computation via the polar decomposition, of
Theorem 3.7. Let be a neighbourhood of origin in where is a measurable function on which satisfies the general strong inequality. The integral defining the spherical convolution function, is absolutely and uniformly convergent for all Moreover the transforms of with is a continuous function on If is such that then
[TABLE]
Proof. We recall that Hence
[TABLE]
Continuity follows from the use of the Lebesgue’s dominated convergence theorem
The following well-known result on the foundational properties of the Harish-Chandra transforms, now follows from the general outlook given by Theorem
Corollary 3.8. Let be a measurable function on which satisfies the strong inequality. The integral defining the Harish-Chandra transforms,
[TABLE]
is absolutely and uniformly convergent for all and is continuous on If is such that then
[TABLE]
Proof. Set in Theorem to have the first results. The inequality follows if we set and observe that
We now consider the image of under the full spherical convolution map, f\mapsto l_{1}(\lambda):=s_{\lambda,f}(x),\;\mbox{for any x\in G}. In order to discuss this we have two options. One of the options is to introduce wave-packet that will still have its domain as while using an appropriate Plancherel measure on This option has been explored in where the Plancherel measure, on for the spherical convolution function (when viewed as a function on ) was defined to absorb the group variable, The results therein suggest that the image of under the full spherical convolution map is indeed possible.
The second option is to retain the spherical Bochner measure, on (a subset of) and define the wave-packet as a map on the Frchet algebra This will reflect the nature of the full spherical convolution map as a transform of members of whose arguments are (generally) taken from (and not just from as in the first option).
To this end recall the Frchet algebra let and set
[TABLE]
where is a zero neighbourhood in It is clear that is also a zero neighbourhood in and that for all It follows, from Theorem that for every We then have the following.
Lemma 3.9. *For every and we have that for some
We now employ these remarks to define a map from to as follows. Let and be the Harish-Chandra function defined on We associate to every the function on defined as
[TABLE]
It should be noted here that
[TABLE]
[TABLE]
[TABLE]
which is due to the invarianve of and that
[TABLE]
being a property inherited from and
The (extra) requirement of being spherical on placed on members of may at first be seen as a restriction, when compared to the requirements on members of It however turns out that this extra requirement is what is needed to assure us of the generalization of the classical wave-packets (of Trombi-Varadarajan) on to all of This is established as follows.
Lemma 3.10. *Let and be as defined above. Then, for every the map is the classical wave-packet of
Proof. We observe that, with
[TABLE]
for some Here we have employed the spherical property of on in the second equality and Lemma in the third equality
The above Lemma shows that the definition and properties of the map is consistent with the relationship (in Lemma ) existing between spherical convolutions, and the Harish-Chandra transfroms, Hence in order to extend Trombi-Varadarajan Theorem (which gives the image of the algebra under ) to all (under the spherical convolution tranform), it will be necessary to show that is the wave-packet of for all According to Lemma this needs only be done for those in with for any neighbourhood, of zero in We however give a self-contained discussion of these results, the first of which is given below.
Theorem 3.11. * for every
In order to finish the establishment of this Theorem we need some lemmas which give appropriate background for it. Indeed we derive an appropriate bound for where and is well-chosen, and the appropriate collection of seminorms are also in place. These will be considered in a forthcoming paper on Trombi-Varadarajan Theorem via the eigenfunction expansion of spherical convolution, which includes the extension of Theorem to all
** Algebras of Spherical Convolutions
**
We now consider the various algebras of spherical convolutions that have emanated in the course of this research and their relationship with the Harish-Chandra Schwartz algebra, on as well as its distinguished commutative subalgebra, of (elementary) spherical functions.
Define and set for all It is clear that is contained in We may therefore topologize by giving it the relative topology from the topology defined on by the seminorms,
Lemma 4.1. The inclusions
[TABLE]
*are all proper
Theorem 4.2. * is a closed subalgebra of *
Proof. We recall that where for some However
[TABLE]
[TABLE]
[TABLE]
[TABLE]
Hence
It may be recalled that members of are exactly those functions on whose left and right derivatives satisfy the strong inequality. In the light of this observation we define as exactly those functions on whose left and right derivatives satisfy the general strong inequality, for each Explicitly we set as
[TABLE]
A collection of seminorms on each of may be given by
[TABLE]
It is however clear that so that
Theorem 4.3. The natural inclusion has a dense image.
Proof. It is known that the natural inclusion of in has a dense image, The result therefore follows if we recall that, as sets of functions,
[TABLE]
where the second inclusion holds from the fact that
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[2.]
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