The smoothness of convolutions of orbital measures on complex Grassmannian symmetric spaces
Sanjiv Kumar Gupta, Kathryn E. Hare

TL;DR
This paper proves that convolutions of orbital measures on complex Grassmannian symmetric spaces become smooth in the sense of belonging to L^2 space after a small number of convolutions, extending known results to these spaces.
Contribution
It establishes the L^2 property for convolutions of orbital measures on all complex Grassmannian symmetric spaces, a case not previously covered.
Findings
Convolution powers of orbital measures are in L^2 for all complex Grassmannian symmetric spaces.
For a dense set of points, the second or third convolution of orbital measures is in L^2.
The results extend the understanding of measure smoothness in symmetric spaces.
Abstract
It is well known that if is any irreducible symmetric space and is a continuous orbital measure supported on the double coset then the convolution product, is absolutely continuous for some suitably large . The minimal value of is known in some symmetric spaces and in the special case of groups or rank one symmetric spaces it has even been shown that belongs to the smaller space for some . Here we prove that this property holds for all the compact, complex Grassmanian symmetric spaces, . Moreover, for the orbital measures at a dense set of points , we prove that (or if ).
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Taxonomy
TopicsAdvanced Algebra and Geometry · Analytic and geometric function theory · Geometric Analysis and Curvature Flows
The smoothness of convolutions of
orbital measures on complex Grassmannian symmetric spaces
Sanjiv Kumar Gupta
Dept. of Mathematics and Statistics
Sultan Qaboos University
P.O.Box 36 Al Khodh 123
Sultanate of Oman
and
Kathryn E. Hare
Dept. of Pure Mathematics
University of Waterloo
Waterloo, Ont., Canada
N2L 3G1
Abstract.
It is well known that if is any irreducible symmetric space and is a continuous orbital measure supported on the double coset then the convolution product, is absolutely continuous for some suitably large . The minimal value of is known in some symmetric spaces and in the special case of groups or rank one symmetric spaces it has even been shown that belongs to the smaller space for some . Here we prove that this property holds for all the compact, complex Grassmanian symmetric spaces, . Moreover, for the orbital measures at a dense set of points , we prove that (or if ).
Key words and phrases:
orbital measure, spherical functions, complex Grassmannian symmetric space, absolute continuity
2000 Mathematics Subject Classification:
Primary 43A90, 43A85; Secondary 58C35, 33C50
This research is supported in part by NSERC 2016-03719 and by Sultan Qaboos University. The authors thank Acadia University for their hospitality when this research was done.
This paper is in final form and no version of it will be submitted for publication elsewhere.
1.
Introduction
Suppose is a Lie group with Cartan involution and is the compact subgroup of fixed by . In a now classical paper, [19], Ragozin proved that if the symmetric space, is irreducible, then any convolution product of continuous, -bi-invariant measures on is absolutely continuous with respect to the Haar measure on . In the case that is a non-compact group, Ragozin’s result was significantly improved by Graczyk and Sawyer in [5] who showed that convolutions would suffice. The building blocks for all -bi-invariant measures on are the so-called orbital measures, supported on the double cosets, . Building on the work of Graczyk and Sawyer in [5]-[8], the authors in [11] improved this result by characterizing the convolution products of orbital measures that are absolutely continuous, for any classical, non-compact symmetric space.
For the compact symmetric spaces for compact, the authors in [12] proved that any convolution product of continuous, -bi-invariant measures is absolutely continuous. Any compact Lie group, can be regarded as a compact symmetric space, namely with . The –bi-invariant, orbital measures are the -invariant measures supported on the conjugacy classes of the group. In this special case, it is known that belongs to the (smaller) space if and only if is absolutely continuous (equivalently, belongs to ). Moreover, the minimal exponent, such that has even been determined for each ; see [10, 14, 20]. This dichotomy was shown to be false in the compact symmetric space , although it is still true that for all continuous orbital measures in any rank one symmetric space; see [2], [13]. These results were all found by studying the decay properties of characters or spherical functions.
In [1], Al-Hashami and Anchouche studied the analogous problem for the compact, complex Grassmannian symmetric spaces where and . They proved that for the dense set of ‘regular’ points , for a choice of which is much smaller than ; see (4.2). They did this by using the Berezin-Karpelevich formula for the spherical functions and obtaining rates of decay for these functions at the regular elements. Using these estimates and the Sobolev embedding theorem, they also proved that for regular elements and suitably large choices of depending on .
In this note, we find estimates on the rates of decay for the spherical functions at all points , these being the points which give rise to the continuous orbital measures . Obtaining such estimates at non-regular points is quite delicate for then the singularities of the spherical functions must be understood. With these estimates we are able to prove that for all whenever
[TABLE]
For the special case of the regular elements we show that if and otherwise. This significantly improves the work in [1] as their exponent was unbounded in . We also show that for all for suitable .
Although smaller than our minimal exponent is typically much larger than . It would be interesting to know what the sharp exponent is for the problem and whether the dichotomy holds.
2. Notation and Preliminaries
2.1. Orbital measures and their smoothness
Suppose is an irreducible symmetric space, where is a compact Lie group with Cartan involution and . Denote its non-compact dual space by and suppose the Lie algebra of is . We fix the Cartan decomposition and the maximal abelian subspace of as in [15]. We identify the Lie algebra of with the subspace of the complexified Lie algebra and let . Always . For any the set is called a double coset and has Haar measure zero.
Definition 1**.**
Given any we define the orbital measure on , with support by
[TABLE]
for all continuous functions .
This probability measure is -bi-invariant. It is continuous (meaning as a measure on ) precisely when and is purely singular with respect to Haar measure.
In [19], Ragozin essentially proved the following geometric characterization.
Proposition 1**.**
Let , . Then is absolutely continuous if and only if the product of double cosets has non-empty interior in . Moreover, if and then is absolutely continuous.
Ragozin used geometric methods to show that has non-empty interior for if for all . Notice that if then and hence has Haar measure zero. Thus is purely singular to Haar measure for all . Ragozin’s geometric characterization was verified using algebraic methods by the authors in [11] when they improved upon his result, showing that suffices. This exponent is close to sharp as there are continuous orbital measures (in some compact symmetric spaces) with singular; [10].
A measure is absolutely continuous with respect to Haar measure if and only if its density function (or Radon Nikodym derivative) belongs to . If the density function belongs to the properly smaller space (or to we will write (resp., Ragozin’s geometric approach is not helpful in studying the problem of determining if . Instead, a harmonic analysis approach has been taken: estimates are made on the rate of decay of the Fourier transform of the measure and then the Peter Weyl theorem is invoked. This approach has been applied very successfully when the symmetric space is a compact group or a rank one compact symmetric space, and is the approach we will take in this paper to study the problem for the complex Grassmannian symmetric spaces.
2.2. The symmetric space
For the remainder of this paper we will focus on the case of the complex Grassmannian symmetric space, , where , and . This compact symmetric space has rank and dimension . The non-compact dual space is the symmetric space where has Lie algebra . With Cartan decomposition , we can take as the maximal abelian subspace the matrices of the form
[TABLE]
where are anti-diagonal matrices, with and respectively, on the anti-diagonal. As above, we let . We can identify by .
The restricted roots and the highest spherical weights will be very important in our work. The positive restricted roots can be taken to be
[TABLE]
(where are the usual basis vectors for with multiplicities , (so these are not present if ) and . The restricted roots act on in the natural way. We also view the roots as acting on by the (well defined) rule . The reader is referred to [15] for further background information.
It is well known that the normalizer, is characterized by the property that if and only if for all restricted roots .
An element or is said to be** regular** if for each restricted root thus is regular precisely when for all and for all . Such elements are dense in or respectively. When is regular, is absolutely continuous (whatever the compact symmetric space); [9].
The highest spherical weights are given by
[TABLE]
We denote the spherical function corresponding to by . Put
[TABLE]
so that . We denote the normalized Jacobi polynomials by
[TABLE]
According to the Berezin-Karpelevich formula (see [3] or [4])
[TABLE]
where
[TABLE]
and the quotient should be understood in the limiting sense if some . Of course, this situation occurs precisely if some mod .
An elementary, but useful, observation is that
[TABLE]
3. Decay of Spherical Functions
The objective of this section is to obtain estimates on the decay of the spherical functions. We will find estimates that hold for all and better estimates for the regular elements.
Theorem 1**.**
Suppose is a highest spherical weight and .
(i) If then
[TABLE]
where is a constant that depends on and , but not .
(ii) If is regular, then there is a constant such that
[TABLE]
Remark 1**.**
Note that when is regular, for any . This is very significant as it means we do not have the complication of having to understand through the limiting process. In [1], the decay in was studied for this special case.111The authors do not make this assumption explicit in the statement of their theorem, but the properties of a regular element are used in their proof. They obtained the bound,
[TABLE]
In our proof, the constants which appear may vary from one occurrence to another, but will always be independent of . We will frequently write as shorthand for . When we say for functions defined on , we mean there are constants such that for all
We begin by collecting useful facts about Jacobi polynomials.
Lemma 1**.**
The following are well known facts about Jacobi polynomials:
(i)
(ii) when
*(iii) so *
(iv) for all
(v) if
We will first prove part (ii) of the Theorem, the special case when is regular.
Proof.
[of Theorem(ii)] Assume is regular. Then for any and that means for any . Furthermore, and that implies for any . This latter fact ensures that
[TABLE]
Consequently, formula (2.1) implies
[TABLE]
as claimed.
For general we must consider the possibility that the formula (2.1) for has to be understood through the limiting process. The next several lemmas will help with this. The proof of the first lemma also introduces a reduction technique that will be frequently used throughout the remainder of the proof of the theorem.
Lemma 2**.**
Fix and suppose there is an index such that for any . Then
[TABLE]
Proof.
First, suppose . In this case,
[TABLE]
where from Lemma 1(iii) we see that is a matrix with entries bounded independent of the choice of . As it follows that
[TABLE]
as we desired to show.
Now assume . Expand the determinant in (2.1) along column to obtain
[TABLE]
Assume the maximum occurs at index . Then
[TABLE]
where
[TABLE]
and
[TABLE]
(with understood in the limiting sense if some
As when , applying property (2.2) gives
[TABLE]
since
In order to bound we will use a reduction argument. Consider the symmetric space where and the spherical representation where are the standard basis vectors for and
[TABLE]
This choice is made so that satisfies the conditions for and for . Let belong to for (here the notation means the element is not present) and for . Notice that for any
[TABLE]
so since all spherical functions are bounded by . Thus
[TABLE]
Lemma 3**.**
Suppose (upon a suitable reordering of coefficients, if necessary) where each with for all if , for all and . Then
[TABLE]
Proof.
We will give the details for but it will be clear how the method generalizes. Thus assume where for for , and .
A basic property of the determinant is that
[TABLE]
where the sum is over all choices, of indices, say is the determinant of the matrix , is the determinant of the submatrix of formed by the remaining rows and columns (the remaining columns being columns ), and is a suitable choice of . This gives the bound
[TABLE]
where
[TABLE]
[TABLE]
and
[TABLE]
(As usual, should be understood in the limiting sense.)
Since
[TABLE]
it follows that
[TABLE]
As whenever and , we see that
[TABLE]
Similar to the previous lemma, and are, up to a constant, the modulus of spherical functions on Grassmanian symmetric spaces of rank and respectively. Indeed, on where is identified with and and similarly for . Hence both are bounded and therefore has the claimed bound.
Lemma 4**.**
Suppose where for all but . Then
[TABLE]
Proof.
Here we must understand as
[TABLE]
where are distinct and not equal to . According to [17] (see also [16, Lemma 4.1]), this limit is equal to
[TABLE]
where and means the derivative of . Applying Lemma 1(v) repeatedly, we see that
[TABLE]
where we recall that if . So the main task is to bound
[TABLE]
Using the permutation method for taking derivatives, one can easily see this determinant is bounded in modulus by
[TABLE]
where the maximum is taken over all permutations of .
If all , this expression is clearly bounded (independently of the choice ), so assume otherwise, say
[TABLE]
for some . Put if all .
Now, implies and thus . Since Lemma 1(ii) together with this observation yields the bound
[TABLE]
for these . Moreover, for these .
Since always is uniformly bounded over (with constant depending on it follows that the terms
[TABLE]
are uniformly bounded when . Consequently, the expression in (3.2) for any fixed is bounded by
[TABLE]
where does not depend on the choice of .
Since the terms are strictly increasing, this is maximized with the permutation that maps to . Hence
[TABLE]
Recalling the formula (3.1), we have
[TABLE]
When (all ), this simplifies to which is even smaller than the valued stated in the lemma. Otherwise, and for , thus
[TABLE]
We immediately deduce that is bounded as stated in the lemma.
Lemma 5**.**
Suppose where for all . Then
[TABLE]
Remark 2**.**
We note that when for such .
Proof.
Similar arguments to the previous proof show that
[TABLE]
In this situation, bounding the determinant by a multiple of the largest term in the sum that arises from the permutation method for calculating the determinant will not give us a good enough estimate. We will actually directly compute the determinant, instead. As before, we have
[TABLE]
From Lemma 1(i),
[TABLE]
thus we need to evaluate the determinant of the matrix whose entry is given by
[TABLE]
In other words, we want to find
[TABLE]
where and for
[TABLE]
Put and and consider the multi-variable polynomial
[TABLE]
Our desire is to compute at with . Notice that if some coordinates for then the matrix has two identical rows and therefore . Thus the polynomial divides . Since both and are degree polynomials, it must be that there is a constant such that for all ,
[TABLE]
In particular,
[TABLE]
Hence,
[TABLE]
We are now ready to complete the proof of the theorem for arbitrary .
Proof.
[of Theorem (i)] Let with .
First, suppose there is a pair such that . In this case, . Lemmas 2 or 3 (depending on the situation) show that for such is bounded in modulus by .
So we can assume that for every either or (or both). If there is some such that then this will be true for all . Then for all restricted roots and that contradicts the assumption that .
If some then the same is true for all and then for all . In the case that , as the positive restricted roots are only of the form and , we again have for all , giving a contradiction. If Lemma 5 gives the bound
[TABLE]
Otherwise we must have for any , but for all and then Lemma 4 says that when and
[TABLE]
for . That completes the proof.
4. and other smoothness results
With these decay estimates we can determine when convolution powers of orbital measures have square integrable density functions.
Theorem 2**.**
Let .
(i) Then provided if or if .
(ii) If is regular, then when and when .
Proof.
We will use the Weyl character formula, which in this setting tells that
[TABLE]
c.f., [2]. As we already have estimates on the rate of decay of the spherical functions, the key additional idea needed to prove this result is a bound on the growth in the degree of as a function of . This uses the Weyl degree formula which states
[TABLE]
where is half the sum of the positive roots. Here
[TABLE]
so
[TABLE]
Thus (a) if (and there are such roots, each with multiplicity ;
(b) if ;
(c) (with multiplicity for the roots and multiplicity for the roots ).
Consequently,
[TABLE]
Thus if Theorem 1(i) and the degree formula (4.1) tells us that
[TABLE]
Since when , it follows that
[TABLE]
This sum is clearly finite if for all (equivalently, ) and (i.e., ), as we desired to show.
Similar reasoning using the other formula from Theorem 1(i) for the case or the formula from part (ii) in the regular case, gives the other statements.
Remark 3**.**
We remark that the conclusion for regular is sharp since is singular. Previously, it was shown in [1] that when is regular if
[TABLE]
In [1], conditions are given under which the density function of belongs to . This is done by noting that if is the Sobolev space of functions in with derivatives up to order in then the Sobolev embedding theorem [18, Theorem 1.2.1], implies that if then . Moreover, the norm can be computed as
[TABLE]
where is the Casmir constant, . They deduce that for when is regular.
With our better estimates on the decay of the spherical functions, we can obtain the following stronger results.
Proposition 2**.**
(i) For any if if and if .
(ii) If is regular, then if .
The proof involves the same types of calculations as in the proof of the theorem above.
Remark 4**.**
It would be interesting to know if these results are sharp and also to determine for each the minimal exponent such that (or
The reference list from the paper itself. Each links out to its DOI / PubMed record.
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