Compositio Math. 143 (2007) 201–221 doi:10.1112/S0010437X06002508
Matrix coefficients of cohomologically induced representations
Binyong Sun
Abstract We define integral formulas which produce certain matrix coefficients of cohomologically induced representations of real reductive groups. They are analogous to Harish-Chandra’s Eisenstein integrals for matrix coefficients of ordinary induced representations, and generalize Flensted-Jensen’s fundamental functions for discrete series.
1. Introduction
Let G be a connected real Lie group such that:
(i) the Lie algebra g0 of G is reductive; (ii) the connected Lie subgroup of G with Lie algebra [g0, g0] has a finite center. Such a G is called a connected real reductive group. Fix a maximal compact subgroup K of G, which is connected and unique up to conjugation. An elementary spherical function is a smooth function φ on G/K with the following three properties: (i) φ(1K)=1; (ii) φ is left K-invariant; (1) (iii) φ is a joint eigenfunction of D(G/K), where D(G/K)is the algebra of G-invariant differential operators on G/K. By using the Iwasawa decomposition G = NAK, Harish-Chandra found in [Har58] a pretty integral formula λ+ρ,H(kx) φλ(x)= e dk, x ∈ G, (2) K which produces elementary spherical functions on G,whereH is the map from G onto a0 =Lie(A) defined by
H(n exp(a)k)=a, n ∈ N,a ∈ a0,k ∈ K, ∗ and ρ ∈ a0 is half of the sum of positive roots (the positive system is the one that corresponds to N). Moreover, he proved that a function on G is elementary spherical if and only if it is of the ∗ form φλ for some λ ∈ a0 ⊗R C. Note that a function on G/K may be identified with a function on G which is right K-invariant. In terms of representation theory, elementary spherical functions can be expressed as matrix coefficients of irreducible spherical representations and its trivial K-type. In general, for an
Received 6 July 2005, accepted in final form 2 August 2006. 2000 Mathematics Subject Classification 22E46 (primary), 22E30 (secondary). Keywords: matrix coefficient, cohomological induction, bottom layer, real reductive group. This journal is c Foundation Compositio Mathematica 2007.
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admissible continuous representation π of G on a Hilbert space Vπ,andaK-type α, define
φπ,α(g)=pα ◦ π(g) ◦ jα,g∈ G,
where jα is the embedding of the α-isotypic component Vπ(α)intoVπ,andpα is the continuous linear projection from Vπ onto Vπ(α) defined by v, if v ∈ Vπ(α), pα(v)= 0, if v ∈ Vπ(β), for some K-type β = α.
It is clear that φπ,α is a real analytic function on G with values in EndC(Vπ(α)). When Vπ(α)has dimension 1, EndC(Vπ(α)) can be canonically identified with C, and therefore φπ,α is actually a complex valued function. If π is an irreducible spherical representation with the trivial K-type α0,
then Vπ(α0) has dimension 1, and the function φπ,α0 is an elementary spherical function. By the theory of spherical functions and spherical representations, all elementary spherical functions can
be expressed as φπ,α0 for some irreducible spherical representation π. In the sense of Vogan, α0 is the unique lowest K-type of every irreducible spherical representa- tion. Therefore, it is interesting to study φπ,α for a general irreducible admissible representation π and an arbitrary lowest K-type α of π. In particular, one may consider the following.
General Problem. Find an integral formula similar to (2)forφπ,α,whereπ is an arbitrary irreducible admissible representation, and α is an arbitrary lowest K-type of π.
Special cases of this General Problem have been extensively studied over the years. Harish- Chandra defined in [Har75](or[Kna86, Wal92]) the Eisenstein integral which represents φπ,α when π is a parabolically induced representation. In [Fle80a], Flensted-Jensen solved the problem when π is a discrete series representation. Li and Wallach obtained a formula when π is a lowest weight unitary representation [Li90]. Harris and Li gave formulas for some very special cases of cohomologically induced representations [HL98]. Some lower rank group cases have been explicitly calculated by mathematical physicists. It is important to point out that Flensted-Jensen also attempted to give a solution of the General Problem [Fle80b]. His formulas produce functions with good properties. However, he has to consider the convergence problem since his formulas involve integrations over non-compact groups. In order to attack the convergence problem, he has to assume that the parameters in his formulas must be sufficiently regular.
The objective of this paper is to give an integral formula for φπ,α when π is a cohomologically induced representation and α is in the bottom layer (we describe cohomological inductions and bottom layers in detail in § 5). One of the good features of our formulas is that the integrations involved in our formulas are over compact groups. Hence, we do not have to deal with the convergence issue. In what follows, we explain precisely why our formulas are enough for a solution to the General Problem.
Let g be the complexification of g0. It is known that the function φπ,α depends only on α and the underlying (g,K)-module of π. Therefore, it makes sense to write φM,α for a finitely generated admissible (g,K)-module M (every M has at least one globalization π). Fix a Cartan involution θ on G such that the fixed point group Gθ = K. Recall that a parabolic subalgebra q of g is called a θ-stable parabolic if θ(q)=q, and q ∩ ¯q is a Levi factor of q, 202
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where ‘¯’ is the complex conjugation relative to the real form g0. Assume that α is a lowest K-type of an irreducible (g,K)-module M. It is automatic that α has multiplicity 1 in M. Vogan associated to α a θ-stable parabolic q (depending on some fixed positive system). Define G = normalizer of q in G. Then G is a quasisplit connected real reductive group. Write g =Lie(G ) ⊗R C and K = K ∩ G . Let α be the K-type which is q-associated to α (Definition 3.1). Then α is fine with respect to G in the sense of Vogan. By [SV98, Theorem 2.9], or [Vog81, Theorems 6.5.10 and 6.5.12], there is a (g,K)-module P in the non-unitary principal series such that: (i) α occurs in P (automatically has multiplicity 1); RS (ii) α is in the bottom layer of XG, occurring with multiplicity 1, where XG = q (P )isa cohomologically induced standard (g,K)-module (this is automatic from condition (i), see the comments after Definition 5.4);
(iii) M is isomorphic to the unique irreducible subquotient of XG containing the K-type α.
From the third condition above we know that φM,α can be canonically identified with φXG,α.Itis also known that φP ,α can be expressed in terms of the parameters of principal series by Harish- Chandra’s Eisenstein integral. Therefore, if we can express φXG,α in terms of φP ,α ,wegivea solution to the general problem. In this paper, we define an integral (Definition 3.2) which is analogous to Harish-Chandra’s Eisenstein integral and does express φXG,α in terms of φP ,α (Theorem 6.3). It generalizes Flensed- Jensen’s fundamental functions for discrete series [Fle80a]. The crucial point is that we use the Langlands decomposition which is more general than the Iwasawa decomposition which was used by Flensted-Jensen [Fle80b]. A direct application of the formulas is to show certain positivity properties which are essential in the study of discrete spectra of theta correspondences [HL98, Li90, Li97]. For example, we find that φπ,α(x) is a positive definite operator when π is an irreducible unitary representation with non-zero cohomology, α is the unique lowest K-type, and x ∈ exp(p0), where p0 ⊂ g0 is the −1eigenspace of θ. In the next section, we recall Flensted-Jensen duality which relates functions on G to functions on a Riemannian symmetric space. In § 3, we introduce the integral and prove that the integral behaves well under the translations of K.In§ 4, we prove that the integral behaves well under the actions of U(g)K .In§ 5, we recall cohomological inductions and bottom layers, and study the actions of U(g)K on bottom layers. The results of §§ 3, 4,and5 imply that both our integral and φM,α have three properties which are similar to those of (1), where M is a cohomologically induced module and α is in the bottom layer. In § 6, we use the uniqueness of functions with these properties to get the equality between our integral and φM,α, and give two interesting examples.
2. Flensted-Jensen duality
2.1 Complexifications of groups
We denote by HC the universal complexification of a Lie group H.LetuH : H → HC be the canonical homomorphism, and ¯ : HC → HC be the anti-holomorphic automorphism on HC which is identity on uH (H). Recall that the universal complexification map uH is defined by the following property [Hoc66]: if H is a complex Lie group and φ : H → H is a Lie group homomorphism, then there is a unique holomorphic homomorphism φ : HC → H such that 203
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the following diagram commutes. uH / H BB HC BB Bφ BB φ B H When A is a connected real analytic manifold, B is a connected complex manifold, and c : A → B is a real analytic map, we call c a complexification map if its differential is a complexification of a real vector space everywhere. The following are well known: (i) every Lie group has a unique universal complexification; (ii) the universal complexification of a connected Lie group is connected;
(iii) if H is a connected real reductive group, then uH is a complexification map and has a finite kernel;
(iv) if H is compact, then uH is injective and HC is a reductive complex group.
2.2 Flensted-Jensen duality for groups Recall from § 1 that θ is a Cartan involution on G such that K is its fixed point group. The involution θ induces a Lie algebra involution θ : g → g.Let
g0 = k0 + p0 and g = k + p be the usual decompositions corresponding to θ.Write θ¯ = θ ◦ ¯=¯◦ θ : g → g.
The involution θ : G → G also induces a holomorphic involution θ : GC → GC. Still write
θ¯ = θ ◦ ¯=¯◦ θ : GC → GC.
Let U be the fixed points of θ¯ in GC.NotethatU is connected, and it is a maximal compact subgroup of GC when G has a compact center. We have a commutative diagram
pK G/K −−−−→ G vG uG (3)
pU GC/U −−−−→ GC
where vG is the map induced by uG, pK is defined by −1 pK(xK)=xθ(x ),x∈ G,
and pU is defined by −1 pU (xU)=xθ¯(x ),x∈ GC.
Note that both uG and pU are complexification maps. Fix a finite-dimensional continuous representation τ of K × K on V, and still denote by τ the holomorphic extension of the representation to KC × KC. We have a smooth representation T of G × G on C∞(G; V) defined by −1 (Tg,hφ)(x)=φ(g xh) for all g, h, x ∈ G, φ ∈ C∞(G; V). By taking its differential, we get a representation T of U(g)⊗U(g) ∞ ∞ on C (G; V). We also have a smooth representation T of GC on C (GC/U; V)by −1 (Tgψ)(x)=ψ(g x) 204
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∞ for all g ∈ GC, x ∈ GC/U, ψ ∈ C (GC/U; V). Again by taking its differential and using the complexification g → g × g, X → (X, θ¯(X)), ∞ we get a representation T of U(g) ⊗ U(g)onC (GC/U; V). Define three spaces of τ-spherical functions by ∞ ∞ −1 C (G; τ)={φ ∈ C (G; V) | φ(k1xk2 )=τ(k1,k2)φ(x),k1,k2 ∈ K, x ∈ G};(4) ∞ ∞ C (GC/U; τ)={φ ∈ C (GC/U; V) | φ(kx)=τ(k, k¯)φ(x),k∈ KC,x∈ GC/U};(5) C∞(G/K; τ)={φ ∈ C∞(G/K; V) | φ(kx)=τ(k, k)φ(x),k∈ K, x ∈ G/K}. (6) ω ω ω The spaces C (G; τ), C (GC/U; τ)andC (G/K; τ) are defined similarly, here the superscript ‘ω’ ω ω stands for real analytic functions. Note that both C (G; τ)andC(GC/U; τ) are stable under K TU(g)K ⊗U(g)K ,whereU(g) is as usual the K-fixed vectors in U(g) under the adjoint action. The following is essentially [Fle80a, Theorem 7.1]. We omit its proof.
Theorem 2.1. We have the following.
(i) The pull backs of pK and vG in the diagram (3) induce canonical isomorphisms of vector spaces: ∞ ∼ ∞ ∼ ∞ C (G; τ) = C (G/K; τ) = C (GC/U; τ). (ii) The above identifications induce linear isomorphisms ω ∼ ω ∼ ω C (G; τ) = C (G/K; τ) = C (GC/U; τ). (iii) The identification ω ∼ ω C (G; τ) = C (GC/U; τ) respects the actions of U(g)K ⊗ U(g)K .
3. The integral
3.1 The definition As in § 1, q is a θ-stable parabolic, G is the normalizer of q in G, g =Lie(G ) ⊗R C and K = K ∩ G . It is known that G is a connected real reductive group and K is a maximal compact subgroup of it. The involution θ stabilizes G and induces a holomorphic involution of GC, which is also denoted by θ.Let θ¯ = θ ◦ ¯=¯◦ θ as before. Denote by U the fixed points of θ¯ in GC.Letn be the nilpotent radical of q ∩ [g, g]. Then q = g ⊕ n.
Denote by N the connected complex subgroup of GC with Lie algebra n.Denoteby jC : GC → GC the complexification of the embedding j : G → G. The Langlands decomposition GC = NjC(GC)U 205
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enables us to define a real analytic map Hq : GC/U → GC/U (7) njC(g)U → gU for all n ∈ N and g ∈ GC. The following conventions will be used freely: if H is a Lie group, c is a complex subspace of a complex Lie algebra, and H acts on c by certain adjoint action, then δc is the non-unitary character on H defined by
δc(x)=Det(Ad(x)|c). If σ is a continuous finite-dimensional representation of a Lie group H, then its differential and its holomorphic extension to HC are still denoted by σ.Notethat
δc(X)=Tr(ad(X)|c),X∈ Lie(H) ⊗R C. (8) Define + ¯ −1 ∈ δn (xU )=δn(xθ(x )),xU GC/U . (9) + It is not difficult to see that δn has positive values everywhere. However, this fact plays no roll in this paper.
Definition 3.1. (i) If σ is a finite-dimensional continuous representation of K on W , define a representation σ of K on W = {v ∈ W | σ(n ∩ k)v =0} (10) by σ (k)v = δn¯∩p(k)σ(k)v, k ∈ K ,v ∈ W . (11) Then σ is called the representation q-associated to σ. (ii) If τ is a finite-dimensional continuous representation of K × K on V, define a representation τ of K × K on V = {v ∈ V | τ(X, Y )v =0forallX ∈ n ∩ k,Y ∈ n¯ ∩ k}. (12) by τ (k, l)v = δn¯∩p(k)δn∩p(l)τ(k, l)v, k, l ∈ K ,v∈ V . (13) Then τ is called the representation q × q¯-associated to τ.
Now let τ be the representation q × q¯-associated to τ as in the second part of the definition. ∞ ∞ We define C (GC/U ; τ ) in the same way as that of C (GC/U; τ)in(5). We also use similar notation for other spaces. Now we have enough preparations to define our integral.
Definition 3.2. For any ∞ φ ∈ C (GC/U ; τ ), define the integral −1 −1 + ∈ Eq(φ : x)= τ(k ,k )(δn φ)(Hq(kx)) dk, x GC/U. (14) K As usual, we use normalized Haar measures on compact groups for integration. Our integral is very similar to Harish-Chandra’s Eisenstein integral for a real parabolic subgroup. The remainder of this section is used to establish one of the main results in this paper. ∞ ∞ Theorem 3.3. We have Eq(φ) ∈ C (GC/U; τ) for all φ ∈ C (GC/U ; τ ).
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3.2 An integral formula In this subsection, we establish an integral formula which is crucial for the proof of Theorem 3.3. The formula is a stronger version of [KV95, Corollary 11.40]. We formulate it in full generality, although we only need to apply it to the complex group KC, since the proof of the general case in no more difficult than that of the special case. The notation of this subsection is not used in other parts of this paper. Let G be a real reductive Lie group (which the reader may assume to be connected), and θ be a Cartan involution on G.Letq0 be a parabolic subalgebra of g0 =Lie(G). We introduce the following notation: • K is the maximal compact subgroup of G corresponding to θ; • g0 = k0 + p0 is the Cartan decomposition corresponding to θ; • Q is the normalizer of q0 in G; • L = Q ∩ θ(Q); • Q = LN is the Levi decomposition; • q0 = l0 + n0 is the corresponding Levi decomposition at the Lie algebra level; • l0 = l0 ∩ p0; • δ : L → R× is the homomorphism defined by the absolute value of the determinant of the adjoint representation of L on n0. By Langlands decomposition, the map N × l × K → G, 0 (15) (n, X, k) → n exp(X)k is a real analytic diffeomorphism. We define two maps κ : G → K and I : G → L by κ(nak)=k, I(nak)=a a for all n ∈ N, a ∈ exp(l0), k ∈ K.Ifa ∈ G, we define a map κ : K → K by κa(k)=κ(ka).
Proposition 3.4. If f is a continuous function on K, a ∈ G,then f(κa(k)) dk = f(k)δ(I(ka−1)) dk. K K The proof of Proposition 3.4 follows from Lemma 3.5–3.8 given in the remainder of this subsection.
−1 Lemma 3.5. The maps κa and κa are inverse to each other. Hence, κa is an analytic diffeomorphism. Proof. Let k ∈ K and ka = n1s1k1,wheren1 ∈ N,s1 ∈ exp(l0), and k1 ∈ K.Thenwehave −1 −1 −1 −1 −1 −1 k1a = s1 n1 k =(s1 n1 s1)s1 k. Hence, a−1 a a−1 −1 κ κ (k)=κ (k1)=κ(k1a )=k. −1 Change a to a−1,wegetκaκa (k)=k.
If a ∈ G,wedenotebyTa the right translation of a on Q\G.WegiveQ\G the unique K-invariant measure with total mass 1. 207
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Lemma 3.6. If k ∈ K, then the Jacobian of Ta at Qk is
JTa (Qk)=δ(I(ka)).
This should be known. We give a proof for the sake of completeness.
Proof. Let ka = nsκ(ka), where n ∈ N and s = I(ka). We have the following commutative diagram.
Q\G −−−−Ta→ Q\G Tk−1 Tκ(ka)−1
Q\G −−−−Tns→ Q\G
Since Tk−1 and Tκ(ka)−1 preserve the measure,
JTa (Qk)=JTns (Q1).
The right-hand side is the absolute value of the determinant of the tangent map dTns|Q at the point Q. We have another commutative diagram.
Ad(ns)−1 G −−−−−−→ G
Q\G −−−−Tns→ Q\G By taking the tangent map at the identity, we get the following diagram.
Ad(ns)−1 g0 −−−−−−→ g0
dTns|Q1 g0/q0 −−−−−→ g0/q0 Hence,
JTa (Qk)=JTns (Q1) = |Det(dTns|Q1)| | | Det(Ad(ns)−1 ) 1 = | | | = −1 = δ(s). Det(Ad(ns)−1 q0 ) δ(s )
a For any a ∈ G,letJa be the Jacobian of κ .
Lemma 3.7. The Jacobian Ja is left K ∩ Q invariant.
Proof. For any k ∈ K,weuseLk to denote the left translation on K by k. The lemma comes from the fact that if k ∈ K ∩ Q, then the following diagram commutes. a K −−−−κ → K Lk Lk
a K −−−−κ → K We omit the easy proof of this fact.
Lemma 3.8. We have Ja(k)=δ(I(ka)) for all k ∈ K.
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→ \ → \ Proof. Let π be the map K Q G, k Qk. By the above lemma, there is a function Ja on Q G such that J ◦ π = Ja. For all continuous function f on Q\G,wehave a f(Ta(x))Ja(x) dx = f(Ta(π(k)))Ja(π(k)) dk Q\G K a a = f((π(κ (k))))Ja(k) dk (Ta ◦ π = π ◦ κ ) K = f(π(k)) dk K = f(x) dx Q\G
= f(Ta(x))JTa (x) dx. Q\G Hence, Ja = JTa .WeconcludetheproofbyLemma3.6.
Proof of Proposition 3.4. We have a a a−1 f(κ (k)) dk = f(κ (κ (k)))Ja−1 (k) dk K K = f(k)δ(I(ka−1)) dk. K
3.3AproofofTheorem3.3 We now return to the notation of § 3.1. We apply the results obtained in the last subsection to the group KC.Letk0 be the Lie algebra of K .LetNc be the connected subgroup of KC with Lie algebra n ∩ k. Now the parabolic subgroup is NcKC.Themap(15)inthiscaseis √ Nc × −1k0 × K → KC, (n, X, k) → n exp(X)k. a × Define κ : KC → K, I : KC → KC, κ : K → K, a ∈ KC,andδ : KC → R as in the last subsection. Lemma 3.9. We have a −1 −1 a Hq(kax)=(I(κ (k)a )) Hq(κ (k)x) for all k ∈ K, a ∈ KC and x ∈ GC/U. √ Proof. Write ka = n a k ,wheren ∈ Nc, a ∈ exp( −1k0), k ∈ K .Then κa(k)a−1 = ka−1 = a−1n−1k =(a−1n−1a)a−1k. Therefore, I(κa(k)a−1)=a−1. As Hq is GC-equivariant and N-invariant, we have a −1 −1 a a a (I(κ (k)a )) Hq(κ (k)x)=a Hq(κ (k)x)=Hq(a κ (k)x) −1 = Hq(a k x)=Hq(n kax)=Hq(kax). | Define a representation τ KC of KC on V by | ¯ τ KC (k)=τ(k, k), 209
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and a representation τ|K of K on V by
τ|K (k)=τ(k, k). Lemma 3.10. We have + ¯ | + (δn φ)(kx)=δn∩k(k)δn¯∩k(k)τ KC (k)(δn φ)(x) ∞ for all k ∈ KC, x ∈ GC/U ,andφ ∈ C (GC/U ; τ ). Proof. + + δn φ(kx)=δn (kx)φ(kx) ¯−1 + ¯ = δn(k)δn(k )δn (x)τ (k, k)φ(x)by(9) ¯−1 ¯ + ¯ = δn(k)δn(k )δn¯∩p(k)δn∩p(k)δn (x)τ(k, k)φ(x)by(13) ¯ | + = δn∩k(k)δn¯∩k(k)τ KC (k)(δn φ)(x). We omit the proof of the following elementary lemma.
Lemma 3.11. We have −1 ¯ δ(k )δn∩k(k)δn¯∩k(k)=1 for all k ∈ KC.
a Proof of Theorem 3.3. Let a ∈ KC and x ∈ GC/U.Writek = κ (k). Then Lemma 3.9 implies | −1 + Eq(φ : ax)= τ K (k )(δn φ)(Hq(kax)) dk K | a−1 −1 + −1 −1 = τ K ((κ (k )) )(δn φ)((I(k a )) (Hq(k x))) dk. K
Now by using Proposition 3.4,wehave −1 | a−1 −1 + −1 −1 Eq(φ : ax)= δ(I(ka ))τ K ((κ (k)) )(δn φ)((I(ka )) Hq(kx)) dk. K −1 Write I =(I(ka−1))−1 and k =(κa (k))−1 for simplicity. By Lemma 3.10,wehave −1 | ¯ | + Eq(φ : ax)= δ(I )τ K (k )δn∩k(I )δn¯∩k(I )τ KC (I )(δn φ)(Hq(kx)) dk K −1 ¯ | + = (δ(I )δn∩k(I )δn¯∩k(I ))τ KC (k I )(δn φ)(Hq(kx)) dk. K −1 ∈ | Note that k I = ak n for some n Nc,andNc fix the values of φ under the action τ KC . Therefore, Lemma 3.11 implies | −1 + | Eq(φ : ax)= τ KC (ak )(δn φ)(Hq(kx)) dk = τ KC (a)Eq(φ : x). K
4. Differential equations satisfied by the integral 4.1 The differential equations We recall the generalized Harish-Chandra homomorphism ξ :U(g)K → U(g)K from [Vog79, § 3]. 210
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By the Poincar´e–Birkhoff–Witt theorem, U(g)=U(g) ⊕ (n U(g)+U(g)n¯). It is known that U(g)K ⊂ U(g)K ⊕ (n U(g) ∩ U(g)n¯). Denote the projection to the first factor by ξ˜ :U(g)K → U(g)K . It is also known that ξ˜ is an algebra homomorphism. Let ηq :U(g ) → U(g ) be the algebra homomorphism such that
ηq(X)=X + δn(X) (16) for all X ∈ g.Notethat
δn(X)=Tr(ad(X)|n), which is twice the shift in the definition of Harish-Chandra homomorphism. It is easy to see that K ηq maps U(g ) onto itself. The map ξ is now defined by K K ξ = ηq ◦ ξ˜ :U(g) → U(g ) . Recall that there is an anti-automorphism ∨ :U(g) → U(g) which maps X to −X for all X ∈ g. It preserves both U(g)K and U(g)K .IfA, B are two subalgebras of U(g) which are stable under ∨,andifη : A → B is any algebra homomorphism, then denote by η∨ : A → B the algebra homomorphism such that the diagram η A −−−−→ B ∨ ∨
η∨ A −−−−→ B commutes. Let V, τ, V and τ be as in § 3.1. Recall that we have an action T of U(g) ⊗ U(g)on ∞ ∞ ∞ C (GC/U; V)andC (G; V). Denote by T the analogous action of U(g )⊗U(g )onC (GC/U ; V ) and C∞(G; V). Recall that ∞ TU(g)K ⊗U(g)K stabilizes C (GC/U; τ), and, similarly, ∞ TU(g )K ⊗U(g )K stabilizes C (GC/U ; τ ). The main result of this section is the following theorem.
K K ∞ Theorem 4.1. For all X ⊗ Y ∈ U(g) ⊗ U(g) and φ ∈ C (GC/U ; τ ), TX⊗Y Eq(φ)=Eq(Tξ∨(X)⊗ξ(Y )φ).
4.2 Proof of Theorem 4.1 Note that we also have U(g)K ⊂ U(g)K ⊕ (n¯ U(g) ∩ U(g)n). The projection to the first factor is just the algebra homomorphism ξ˜∨ :U(g)K → U(g)K .
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K K ∞ Lemma 4.2. Let X ⊗ Y ∈ U(g) ⊗ U(g) and f ∈ C (GC/U; V).Iff is N-invariant, then
TX⊗Y f = Tξ˜∨(X)⊗ξ˜(Y )f. Proof. Let X = X + X, Y = Y + Y ,whereX = ξ˜∨(X), X ∈ U(g)n, Y = ξ˜(Y ), Y ∈ U(g)n¯. Note that under the complexification 1 × θ¯ : g → g × g, v → (v,θ¯(v)),
the Lie algebra of N has a complexification n×n¯. Therefore, the N invariance of f implies Tn×n¯f =0, i.e. Tn⊗1+1⊗n¯f =0.Sowehave