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Lecture 2 Wavelets on Groups

A matured mathematical theory looks like a tree. There is a solid trunk which supports all branches and leaves but could not be alive without them. In the case of group approach to wavelets the trunk of the theory is a construction of wavelets from a square integrable representation [38], [5, Chap. 8]. We begin from this trunk which is a model for many different generalisations and will continue with some smaller “generalising” branches later.

2.1 Wavelet Transform on Groups

Let G be a group with a left Haar measure dµ and let ρ be a unitary irreducible representation of a group G by operators ρg, gG in a Hilbert space H.

Definition 1 Let us fix a vector w0H. We call w0H a vacuum vector or a mother wavelet (other less-used names are ground state, fiducial vector, etc.). We will say that set of vectors wg=ρ(g) w0, gG form a family of coherent states (wavelets).
Exercise 2 If ρ is irreducible then wg, gG is a total set in H, i.e. the linear span of these vectors is dense in H.

The wavelet transform can be defined as a mapping from H to a space of functions over G via its representational coefficients (also known as matrix coefficients):

W: v ↦ v(g)= ⟨ ρ(g−1)v,w0  ⟩=  ⟨ v,ρ (g)w0  ⟩ = ⟨ v,wg  ⟩. (1)
Exercise 3 Show that the wavelet transform W is a continuous linear mapping and the image of a vector is a bounded continuous function on G. The liner space of all such images is denoted by W(G).
Exercise 4 Let a Hilbert space H has a basis ej, j∈ℤ and a unitary representation ρ of G=ℤ defined by ρ(k)ej=ej+k. Write a formula for wavelet transform with w0=e0 and characterise W(ℤ).

Proof.[Answer] v(n)=⟨ v,en ⟩.


Exercise 5 Let G be ax+b group and ρ is given by (cf. (3)):
[T(a,b)  f](x)= 
1
a
f


xb
a



,  (2)
in L2(ℝ). Show that
  1. The representation is reducible and describe its irreducible components.
  2. for w0(x)=1/2π i (x+i) coherent states are v(a,b)(x)=√a/2π i (x−(bia)).
  3. Wavelet transform is given by
          v(a,b)= 
    a
    2π i
     


    v(x)
    x−(b+ia)
    dx,
    which resembles the Cauchy integral formula.
  4. Give a characteristic of W(G).
  5. Write the wavelet transform for the same representation of the group ax+b and the Gaussian (or Gauss function)ex2/2 (see Fig. 2.1) as a mother wavelets.

Figure 2.1: The Gaussian function ex2/2.

Proposition 6 The wavelet transform W intertwines ρ and the left regular representation Λ (8) of G:
    W ρ(g) = Λ(g) W.

Proof. We have:

[W( ρ(g) v)] (h)=⟨ ρ(h−1) ρ(g) v , w0  ⟩ 
 =⟨ ρ((g−1h)−1) v , w0  ⟩ 
 =[Wv](g−1h)
 =[Λ(g) Wv] (h).


Corollary 7 The function space W(G) is invariant under the representation Λ of G.

Wavelet transform maps vectors of H to functions on G. We can consider a map in the opposite direction sends a function on G to a vector in H.

Definition 8 The inverse wavelet transform Mw0 associated with a vector w0H maps L1(G) to H and is given by the formula:
     
    Mw0:  L1(G) → H:  v(g) ↦ M  [v(g)] =
 


G
 v(g) wgdµ(g) 
 
  =
 


G
v(g) ρ(g) dµ(g) w0,  
(3)
where in the last formula the integral express an operator acting on vector w0.
Exercise 9 Write inverse wavelet transforms for Exercises 4 and 5.

Proof.[Answer]

  1. For Exercises 4: v=∑−∞ v(n) en.
  2. For Exercises 5:
          v(x) = 
    1
    2π i
     


    +2
    v(a,b)
    x−(bia)
    dadb
    a
    3
    2
     
    . 


Lemma 10 If the wavelet transform W and inverse wavelet transform M are defined by the same vector w0 then they are adjoint operators: W*=M.

Proof. We have:

    ⟨ Mv,wg  ⟩=
    ⟨ 
 


G
 v(g′) wgdµ(g′),wg  ⟩
 =
 


G
 v(g′) ⟨ wg,wg  ⟩ dµ(g′)
 =
 


G
 v(g′) 
⟨ wg,wg  ⟩
dµ(g′)
 =⟨  v,Wwg  ⟩,

where the scalar product in the first line is on H and in the last line is on L2(G). Now the result follows from the totality of coherent states wg in H.


Proposition 11 The inverse wavelet transform M intertwines the representation Λ (8) on L2(G) and ρ on H:
    M Λ(g) = ρ(g) M.

Proof. We have:

    M [Λ(g)v(h)]=M [ v(g−1h)] 
 =
 


G
 v(g−1h)     wh  dµ(h)
 =
 


G
 v(h′) wghdµ(h′)
 =
ρ(g) 
 


G
v(h′) whdµ(h′)
 =ρ(g) M [v(h′)],

where h′=g−1h.


Corollary 12 The image M(L1(G))⊂ H of subspace under the inverse wavelet transform M is invariant under the representation ρ.

An important particular case of such an invariant subspace is Gårding space.

Definition 13 Let C0(G) be the space of infinitely differentiable functions with compact supports. Then for the given representation in H the Gårding space G()⊂ H is the image of C0(G) under the inverse wavelet transform with all possible reconstruction vectors:
    G()={Mw φ  ∣  w∈ H, φ∈C0(G)}.
Corollary 14 The Gårding space is invariant under the derived representation d.

The following proposition explain the usage of the name “inverse” (not “adjoint” as it could be expected from Lemma 10) for M.

Theorem 15 The operator
P= MW: H → H (4)
maps H into its linear subspace for which w0 is cyclic. Particularly if ρ is an irreducible representation then P is cI for some constant c depending from w0 and w0.

Proof. It follows from Propositions 6 and 11 that operator MW: HH intertwines ρ with itself. Then Corollaries 7 and 12 imply that the image MW is a ρ-invariant subspace of H containing w0. From irreducibility of ρ by Schur’s Lemma [159, § 8.2] one concludes that MW=cI on C for a constant c∈ℂ.


Remark 16 From Exercises 4 and 9 it follows that irreducibility of ρ is not necessary for MW=cI, it is sufficient that w0 and w0 are cyclic only.

We have similarly

Theorem 17 Operator WM is up to a complex multiplier a projection of L1(G) to W(G).

2.2 Square Integrable Representations

So far our consideration of wavelets was mainly algebraic. Usually in analysis we wish that the wavelet transform can preserve an analytic structure, e.g. values of scalar product in Hilbert spaces. This accomplished if a representation ρ possesses the following property.

Definition 18 [159, § 9.3] Let a group G with a left Haar measure dµ have a unitary representation ρ: GL(H). A vector wH is called admissible vector if the function ŵ(g)=⟨ ρ(g)w,w is non-void and square integrable on G with respect to dµ:
0<c2=
 


G
 ⟨ ρ(g)w,w  ⟩ ⟨ w,ρ(g)w  ⟩  dµ(g) < ∞. (5)
If an admissible vector exists then ρ is a square integrable representation.

Square integrable representations of groups have many interesting properties (see [85, § 14] for unimodular groups and [87], [5, Chap. 8] for not unimodular generalisation) which are crucial in the construction of wavelets. For example, for a square integrable representation all functions ⟨ ρ(g)v1,v2 ⟩ with an admissible vector v1 and any v2H are square integrable on G; such representation belong to dicrete series; etc.

Exercise 19 Show that
  1. Admissible vectors form a linear space.
  2. For an irreducible ρ the set of admissible vectors is dense in H or empty.

Proof.[Hint] The set of all admissible vectors is an ρ-invariant subspace of H.


Exercise 20
  1. Find a condition for a vector to be admissible for the representation (2) (and therefore the representation is square integrable).
  2. Show that w0(x)=1/2π i (x+i) is admissible for ax+b group.
  3. Show that the Gaussian ex2 is not admissible for ax+b group.

For an admissible vector w we take its normalisation w0=||w||/c w to obtain:

 


G

⟨ ρ(g)w0,w0  ⟩ 
2  dµ(g)= ⎪⎪
⎪⎪
w0⎪⎪
⎪⎪
2. (6)

Such a w0 as a vacuum state produces many useful properties.

Proposition 21 If both wavelet transform W and inverse wavelet transform M for an irreducible square integrable representation ρ are defined by the same admissible vector w0 then the following three statements are equivalent:
  1. w0 satisfy (6);
  2. MW=I;
  3. for any vectors v1, v2H:
    ⟨ v1,v2  ⟩=
     


    G
     v1(g) 
    v2(g)
      dµ(g). (7)

Proof. We already knew that MW=cI for a constant c∈ ℂ. Then (6) exactly says that c=1. Because W and M are adjoint operators it follows from MW=I on H that:

    ⟨ v1,v2  ⟩= ⟨ MWv1,v2  ⟩= ⟨ Wv1,M*v2  ⟩=⟨ Wv1,Wv2  ⟩,

which is exactly the isometry of W  (7). Finally condition (6) is a partticular case of general isometry of W for vector w0.


Exercise 22 Write the isometry conditions (7) for wavelet transforms for and ax+b groups (Exercises 4 and 5).

Wavelets from square integrable representation closely related to the following notion:

Definition 23 A reproducing kernel on a set X with a measure is a function K(x,y) such that:
     
      K(x,x) > 0,   ∀ x∈ X,(8)
    K(x,y) =
K(y,x)
,  
(9)
    K(x,z) =
 


X
K(x,y)K(y,z) dy.  
(10)
Proposition 24 The image W(G) of the wavelet transform W has a reproducing kernel K(g,g′)=⟨ wg,wg. The reproducing formula is in fact a convolution:
     
    v(g′) =
 


G
K(g′,g) v(g) dµ(g)
 
  =
 


G
 ŵ0(g−1g′) v(g) dµ(g)  
(11)
with a wavelet transform of the vacuum vector ŵ0(g)= ⟨ w0,ρ(g)w0.

Proof. Again we have a simple application of the previous formulas:

     
    v(g′) = ⟨ ρ(g−1)v,w0  ⟩    
 =
 


G
 ⟨ ρ(h−1) ρ(g−1) v,w0  ⟩  
⟨ ρ(h−1)  w0,w0  ⟩
dµ(h)  
(12)
 =
 


G
 ⟨ ρ((gh)−1) v,w0  ⟩  ⟨ ρ(h)  w0,w0  ⟩ dµ(h)   
 
 =
 


G
 v (gh)  ŵ0(h−1)   dµ(h)  
 
  =
 


G
 v(g)  ŵ0(g−1g′) dµ(g), 
 

where transformation (12) is due to  (7).


Exercise 25 Write reproducing kernels for wavelet transforms for and ax+b groups (Exercises 4 and 5.
Exercise* 26 Operator (11) of convolution with ŵ0 is an orthogonal projection of L2(G) onto W(G).

Proof.[Hint] Use that an left invariant subspace of L2(G) is in fact an right ideal in convolution algebra, see Lemma 36.


Remark 27 To possess a reproducing kernel—is a well-known property of spaces of analytic functions. The space W(G) shares also another important property of analytic functions: it belongs to a kernel of a certain first order differential operator with Clifford coefficients (the Dirac operator) and a second order operator with scalar coefficients (the Laplace operator) [15, 172, 170, 223], which we will consider that later too.

We consider only fundamentals of the wavelet construction here. There are much results which can be stated in an abstract level. To avoid repetition we will formulate it later on together with an interesting examples of applications.

The construction of wavelets from square integrable representations is general and straightforward. However we can not use it everywhere we may wish:

  1. Some important representations are not square integrable.
  2. Some groups, e.g. ℍn, do not have square representations at all.
  3. Even if representation is square integrable, some important vacuum vectors are not admissible, e.g. the Gaussian ex2 in 3.
  4. Sometimes we are interested in Banach spaces, while unitary square integrable representations are acting only on Hilbert spaces.

To be vivid the trunk of the wavelets theory should split into several branches adopted to particular cases and we describe some of them in the next lectures.

2.3 Fundamentals of Wavelets on Homogeneous Spaces

Let G be a group and H be its closed normal subgroup. Let X=G/H be the corresponding homogeneous space with a left invariant measure dµ. Let s: XG be a Borel section in the principal bundle of the natural projection p: GG/H. Let ρ be a continuous representation of a group G by invertible unitary operators ρ(g), gG in a Hilbert space H.

For any gG there is a unique decomposition of the form g=s(x)h, hH, x=p(g)∈ X. We will define r: GH: r(g)=h=(s(p(g)))−1g from the previous equality. Then there is a geometric action of G on XX defined as follows

g: x ↦ g−1 · x = p (g−1s(x)).
Example 28 As a subgroup H we select now the center of n consisting of elements (t,0). Of course X=G/H isomorphic to n and mapping s: ℂnG simply is defined as s(z)=(0,z). The Haar measure on n coincides with the standard Lebesgue measure on 2n+1 [321, § 1.1] thus the invariant measure on X also coincides with the Lebesgue measure on n. Note also that composition law p(g· s(z)) reduces to Euclidean shifts on n. We also find p((s(z1))−1· s(z2))=z2z1 and r((s(z1))−1· s(z2))= 1/2 ℑ z1z2.

Let ρ: GL(V) be a unitary representation of the group G by operators in a Hilbert space V.

Definition 29 Let G, H, X=G/H, s: XG, ρ: GL(V) be as above. We say that w0H is a vacuum vector if it satisfies to the following two conditions:
     
   ρ(h) w0  = χ(h) w0,    χ(h) ∈ ℂ,  for all  h∈ H;(13)
  
 


X

⟨ w0,ρ(s(x))w0  ⟩ 
2dx  = ⎪⎪
⎪⎪
w0⎪⎪
⎪⎪
2.  
(14)
We will say that set of vectors wx=ρ(x) w0, xX form a family of coherent states.

Note that mapping h → χ(h) from (13) defines a character of the subgroup H. The condition (14) can be easily achieved by a renormalisation w0 as soon as we sure that the integral in the left hand side is finite and non-zero.

Convention 30 In that follow we will usually write xX and x−1X instead of s(x)∈ G and s(x)−1G correspondingly. The right meaning of “x” can be easily found from the context (whether an element of X or G is expected there).
Example 31 As a “vacuum vector” we will select the original vacuum vector of quantum mechanics—the Gauss function w0(q)=eq2/2 (see Figure 2.1), which belongs to all L2(ℝn). Its transformations are defined as follow:
    wg(q)=[ρ(s,z)w0](q)=
e
i(2s
2
xq+xy)
 
e
(q− 
2
y)
2/2
 
 =
e2is−(x2+y2)/2e
((x+iy)2q2)/2−
2
i(x+iy)q
 
 =
e2iszz/2e
(z2q2)/2−
2
izq
 
.
Particularly (t,0) w0](q)=e−2itw0(q), i.e., it really is a vacuum vector in the sense of our definition with respect to H.
Exercise 32 Check the square integrability condition  (14) for w0(q)=eq2/2.

The wavelet transform (similarly to [eq:wavelet-transform]the group case) can be defined as a mapping from V to a space of bounded continuous functions over G via representational coefficients

  v ↦ v(g)= ⟨ ρ(g−1)v,w0  ⟩=  ⟨ v,ρ (g)w0  ⟩.

Due to (13) such functions have simple transformation properties along H-orbits:

  v(gh)=⟨ v,ρ (gh)w0  ⟩
 =⟨ v,ρ (g) ρ(h)w0  ⟩
 =⟨ v,ρ (g) χ(h)w0  ⟩
 =χ(h)⟨ v,ρ (g) w0  ⟩
 =χ(h)v(g),        where   g∈ G, h∈ H.

Thus the wavelet transform is completely defined by its values indexed by points of X=G/H. Therefore we prefer to consider so called induced wavelet transform.

Remark 33 In the earlier papers [170], [173] we use name reduced wavelet transform since it produces functions on a homogeneous space rather than the entire group. From now on we prefer the name induced wavelet transform due to its explicit connection with induced representations.
Definition 34 The induced wavelet transform W from a Hilbert space H to a space of function W(X) on a homogeneous space X=G/H defined by a representation ρ of G on H, a vacuum vector w0 is given by the formula
W: H → W(X): v ↦ v(x)=  [Wv] (x)=⟨ ρ(x−1) v,w0  ⟩= ⟨ v,ρ(x)w0  ⟩. (15)
Example 35 The transformation (15) with the kernel (0,z) w0](q) is an embedding L2(ℝn) → L2(ℂn) and is given by the formula
     
    f(z)=⟨ fs(z)f0  ⟩   
 =
πn/4
 


n
f(q)  ezz/2e
− (z2+q2)/2+
2
zq
 
dq   
 
 =
ezz/2πn/4
 


n
f(q) e
− (z2+q2)/2+
2
zq
 
dq .
(16)
Then f(g) belongs to L2( ℂn , dg) or its preferably to say that function f(z)=ezz/2f(t0,z) belongs to space L2( ℂn , e− | z |2 dg) because f(z) is analytic in z. Such functions form the Segal-Bargmann space F2( ℂn, e− | z |2 dg) of functions [17, 301], which are analytic by z and square-integrable with respect to the Gaussian measure Gauss measure e− | z |2dz. We use notation W for the mapping v ↦ v(z)=ezz/2Wv. Analyticity of f(z) is equivalent to the condition ( ∂ / ∂zj + 1/2 zj I ) f(z)=0. The integral in (16) is the well-known Segal-Bargmann transform [17, 301].
Exercise 36 Check that w0(z)=1 for the vacuum vector w0(q)=eq2/2.

There is a natural representation of G in W(X). It can be obtained if we first lift functions from X to G, apply the left regular representation Λ and then pul them back to X. The result defines a representation λ(g): W(X) → W(X) as follow

[λ(g) f] (x) = χ(r(g−1· x)) f(g−1· x). (17)

We recall that χ(h) is a character of H defined in (13) by the vacuum vector w0. Of course, for the case of trivial H={e} (17) becomes the left regular representation Λ(g) of G.

Proposition 37 The induced wavelet transform W intertwines ρ and the representation λ (17) on W(X):
  W ρ(g) = λ(g) W.

Proof. We have with obvious adjustments in comparison with Proposition 6:

[W( ρ(g) v)] (x)=⟨  ρ(g) v , ρ(x)w0  ⟩ 
 =⟨  v , ρ(g−1s(x))w0  ⟩ 
 =⟨  v , ρ(s(g−1· x)) ρ(r(g−1· x)) w0  ⟩ 
 =⟨  v , ρ(s(g−1· x))χ(r(g−1· x)) w0  ⟩ 
 =χ(r(g−1· x))⟨  v , ρ(s(g−1· x)) w0  ⟩ 
 =χ(r(g−1· x)) [Wv] (g−1x) 
 =λ(g) [Wv] (x).


Corollary 38 The function space W(X) is invariant under the representation λ of G.
Example 39 Integral transformation (16) intertwines the Schrödinger representation (4) with the following realisation of representation (17):
     
    λ(s,z) f(u) = f0(z−1· u)  χ(s+r(z−1· u))   
  = f0(uz)eis+iℑ(zu)  (18)
Exercise 40
  1. Using relation W=e−| z |2/2W derive from above that W intertwines the Schrödinger representation with the following:
          λ(s,z) f(u) = f0(uz) e
    2iszu
    z
    2/2
     
     .
  2. Show that infinitesimal generators of representation λ are:
          ∂λ(s,0,0)=iI,   ∂λ(0,x,0)=−∂uuI,   ∂λ(0,0,y)=i(−∂z+zI)

We again introduce a transform adjoint to W.

Definition 41 The inverse wavelet transform M from W(X) to H is given by the formula:
     
    M:  W(X) → H: v(x) ↦ M  [v(x)] =
 


X
 v(x) wxdµ(x) 
 
  =
 


X
 v(x) ρ(x) dµ(x) w0.  
(19)
Proposition 42 The inverse wavelet transform M intertwines the representation λ on W(X) and ρ on H:
    M λ(g) = ρ(g) M.

Proof. We have:

    M [λ(g)v(x)]=M [ χ(r(g−1· x)) v(g−1· x)] 
 =
 


X
 χ(r(g−1· x)) v(g−1· x)  wx  dµ(x)
 =
χ(r(g−1· x)) 
 


X
 v(x′) wg· xdµ(x′)
 =
ρg
 


X
 v(x′) wxdµ(x′)
 =ρgM [v(x′)],

where x′=g−1 · x.


Corollary 43 The image M(W(X))⊂ H of subspace W(X) under the inverse wavelet transform M is invariant under the representation ρ.
Example 44 Inverse transformation to (16) is given by a realisation of (19):
     
    f(q) =
 


 ℂn
 f(z) fs(z)(q) dz
 
  =
 


 ℂn
 f(x,y) e
iy(x
2
y)
 
e
(q
2
y)
2/2
 
  dxdy 
(20)
  =
 


n
 f(z) e
− (z2+q2)/2+
2
zq
 
   e
− 
z
2
 
  dz.  
 
The transformation  (20) intertwines the representations (18) and the Schrödinger representation (4) of the Heisenberg group.

The following proposition explain the usage of the name for M.

Theorem 45 The operator
P= MW: H → H (21)
is a projection of H to its linear subspace for which w0 is cyclic. Particularly if ρ is an irreducible representation then the inverse wavelet transform M is a left inverse operator on H for the wavelet transform W:
  MW=I.

Proof. It follows from Propositions 37 and 42 that operator MW: HH intertwines ρ with itself. Then Corollaries 38 and 43 imply that the image MW is a ρ-invariant subspace of H containing w0. Because of MWw0=w0 we conclude that MW is a projection.

From irreducibility of ρ by Schur’s Lemma [159, § 8.2] one concludes that MW=cI on H for a constant c∈ℂ. Particularly

MWw0= 
 


X
 ⟨ ρ(x−1)w0,w0  ⟩  ρ(x)  w0dµ(x)=cw0.

From the condition (14) it follows that ⟨ cw0,w0 ⟩=⟨ MW w0,w0 ⟩=⟨ w0,w0 ⟩ and therefore c=1.


We have similar

Theorem 46 Operator WM is a projection of L1(X) to W(X).
Corollary 47 In the space W(X) the strong convergence implies point-wise convergence.

Proof. From the definition of the wavelet transform:

    
f(x) 
=
⟨ f,ρ(x)w0  ⟩ 
⎪⎪
⎪⎪
f⎪⎪
⎪⎪
⎪⎪
⎪⎪
w0⎪⎪
⎪⎪
.

Since the wavelet transform is an isometry we conclude that | f(x) |≤ c||f|| for c=||w0||, which implies the assertion about two types of convergence.


Example 48 The corresponding operator for the Segal-Bargmann space P (21) is an identity operator L2(ℝn) → L2(ℝn) and (21) gives an integral presentation of the Dirac delta.

While the orthoprojection L2( ℂn, e− | z |2 dg) → F2( ℂn, e− | z |2 dg) is of a separate interest and is a principal ingredient in Berezin quantization [35, 67]. We can easy find its kernel from (24). Indeed, f0(z)=e − | z |2 , then the kernel is

    K(z,w)=f0(z−1· w) χ(r(z−1· w))
 =f0(wz)eiℑ(zw)
 =
exp


1
2
(− 
wz
2 +wzzw)


 =
exp


1
2
(− 
z
2− 
w
2)  +wz


.

To receive the reproducing kernel for functions f(z)=e| z |2 f(z) in the Segal-Bargmann space we should multiply K(z,w) by e(−| z |2+ | w |2)/2 which gives the standard reproducing kernel = exp(− | z |2 +wz) [17, (1.10)].

We denote by W*: W*(X) → H and M*: HW*(X) the adjoint (in the standard sense) operators to W and M respectively.

Corollary 49 We have the following identity:
⟨ Wv , M*l  ⟩W(X)  = ⟨ v,l  ⟩H,     ∀ v, l∈ H,  (22)
or equivalently
 


X
 ⟨ ρ(x−1) v,w0  ⟩  ⟨ ρ(x) w0,l  ⟩  dµ(x)  = ⟨ v,l  ⟩. (23)

Proof. We show the equality in the first form (23) (but we will apply it often in the second one):

    ⟨ Wv , M*l  ⟩W(X)  = ⟨ MWv ,l  ⟩H =⟨ v,l  ⟩H.


Corollary 50 The space W(X) has the reproducing formula
v(y)=
 


X
 v(x)    b0(x−1· y) dµ(x), (24)
where b0(y)=[Ww0] (y) is the wavelet transform of the vacuum vector w0.

Proof. Again we have a simple application of the previous formulas:

     
    v(y) = ⟨ ρ(y−1)v,w0  ⟩    
 =
 


X
 ⟨ ρ(x−1) ρ(y−1) v,w0  ⟩  ⟨ ρ(x)  w0,w0  ⟩ dµ(x)  
(25)
 =
 


X
 ⟨ ρ(s(y· x)−1) v,w0  ⟩  ⟨ ρ(x)  w0,w0  ⟩ dµ(x)   
 
 =
 


X
 v (y· x)  b0(x−1)   dµ(x)  
 
  =
 


X
 v(x)  b0(x−1y) dµ(x), 
 

where transformation (25) is due to (23).


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Last modified: October 28, 2024.
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