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Proceedings of the National Academy of Sciences of the United States of America logoLink to Proceedings of the National Academy of Sciences of the United States of America
. 1997 Oct 14;94(21):11133–11137. doi: 10.1073/pnas.94.21.11133

Zeta functions and Eisenstein series on classical groups

Goro Shimura 1
PMCID: PMC34506  PMID: 11607757

Abstract

We construct an Euler product from the Hecke eigenvalues of an automorphic form on a classical group and prove its analytic continuation to the whole complex plane when the group is a unitary group over a CM field and the eigenform is holomorphic. We also prove analytic continuation of an Eisenstein series on another unitary group, containing the group just mentioned defined with such an eigenform. As an application of our methods, we prove an explicit class number formula for a totally definite hermitian form over a CM field.

Section 1.

Given a reductive algebraic group G over an algebraic number field, we denote by GA, Ga, and Gh its adelization, the archimedean factor of GA, and the nonarchimedean factor of GA. We take an open subgroup D of GA of the form D = D0Ga with a compact subgroup D0 such that D0Ga is maximal compact in Ga. Choosing a specific type of representation of D0Ga, we can define automorphic forms on GA as usual. For simplicity we consider here the forms invariant under D0Gh. Each Hecke operator is given by DτD, with τ in a subset 𝔛 of GA, which is a semigroup containing D and the localizations of G for almost all nonarchimedean primes. Taking an automorphic form f such that f|DτD = λ(τ)f with a complex number λ(τ) for every τ ∈ 𝔛 and a Hecke ideal character χ of F, we put

graphic file with name M1.gif 1.1

where ν0(τ) is the denominator ideal of τ and N0(τ)) is its norm. Now our first main result is that if G is symplectic, orthogonal, or unitary, then

graphic file with name M2.gif 1.2

where Λ(s, χ) is an explicitly determined product of L-functions depending on χ, Wp is a polynomial determined for each vh whose constant term is 1, and p runs over all the prime ideals of the basic number field. This is a purely algebraic result concerning only nonarchimedean primes.

Let Z(s, f, χ) denote the right-hand side of Eq. 1.2. As our second main result, we obtain a product 𝔊(s) of gamma factors such that 𝔊Z can be continued to the whole s-plane as a meromorphic function with finitely many poles, when G is a unitary group of an arbitrary signature distribution over a CM field, and f corresponds to holomorphic forms.

Now these problems are closely connected with the theory of Eisenstein series E on a group G′ in which G is embedded. To describe the series, let ℨ′ denote the symmetric space on which G′ acts. Then the series as a function of (z, s) ∈ ℨ′ × C can be given (in the classical style) in the form

graphic file with name M3.gif 1.3

where Γ is a congruence subgroup of G′, and P is a parabolic subgroup of G′ which is a semidirect product of a unipotent group and G × GLm with some m. The adelized version of δ will be explicitly described in Section 5. Now our third main result is that there exists an explicit product 𝔊′ of gamma factors and an explicit product Λ′ of L-functions such that 𝔊′(s)Λ′(s)Z(s, f, χ)E(z, s; f, χ) can be continued to the whole s-plane as a meromorphic function with finitely many poles.

Though the above results concern holomorphic forms, our method is applicable to the unitary group of a totally definite hermitian form over a CM field. In this case, we can give an explicit class number formula for such a hermitian form, which is the fourth main result of this paper.

Section 2.

For an associative ring R with identity element, we denote by R× the group of all its invertible elements and by Rnm the R-module of all m × n matrices with entries in R. To indicate that a union X = ∪iI Yi is disjoint, we write X = ⊔iI Yi.

Let K be an associative ring with identity element and an involution ρ. For a matrix x with entries in K, we put x* = txρ, and = (x*)−1 if x is square and invertible. Given a finitely generated left K-module V, we denote by GL(V) the group of all K-linear automorphisms of V. We let GL(V) act on V on the right; namely we denote by wα the image of wV under α ∈ GL(V). Given ɛ = ±1, by an ɛ-hermitian form on V, we understand a biadditive map ϕ:V × VK such that ϕ(x, y)ρ = ɛϕ(y, x) and ϕ(ax, by) = aϕ(x, y)bρ for every a, bK. Assuming that ϕ is nondegenerate, we put

graphic file with name M4.gif 2.1

Given (V, ϕ) and (W, ψ), we can define an ɛ-hermitian form ϕ ⊕ ψ on VW by

graphic file with name M5.gif
graphic file with name M6.gif 2.2

We then write (VW, ϕ ⊕ ψ) = (V, ϕ) ⊕ (W, ψ). If both ϕ and ψ are nondegenerate, we can view Gϕ × Gψ as a subgroup of Gϕ⊕ψ. The element (α, β) of Gϕ × Gψ viewed as an element of Gϕ⊕ψ will be denoted by α × β or by (α, β). Given a positive integer r, we put Hr = IrIr, Ir = Ir = Kr1 and

graphic file with name M7.gif 2.3

We shall always use Hr, Ir, Ir, and ηr in this sense. We understand that H0 = {0} and η0 = 0.

Hereafter we fix V and a nondegenerate ϕ on V, assuming that K is a division ring whose characteristic is different from 2. Let J be a K-submodule of V which is totally ϕ-isotropic, by which we mean that ϕ(J, J) = 0. Then we can find a decomposition (V, ϕ) = (Z, ζ) ⊕ (H, η) and an isomorphism f of (H, η) onto (Hr, ηr) such that f(J) = Ir. In this setting, we define the parabolic subgroup Inline graphic of Gϕ relative to J by

graphic file with name M9.gif 2.4

and define homomorphisms Inline graphicGζ and Inline graphicGL(J) such that zα − zπζϕ (α) ∈ J and wα = wλJϕ(α) if zZ, wJ, and α ∈ Inline graphic

Taking a fixed nonnegative integer m, we put

graphic file with name M13.gif 2.5

We can naturally view Gψ × Gϕ as a subgroup of Gω. Since W = VHm, we can put X = VHmV with the first summand V in W, and write every element of X in the form (u, h, v) with (u, h) ∈ VHm = W and vV. Put

graphic file with name M14.gif

Observing that U is totally ω-isotropic, we can define Inline graphic

Proposition 1. Let λ(ϕ) be the maximum dimension of totally ϕ-isotropic K-submodules of V. Then

graphic file with name M16.gif 2.6

has exactly λ(ϕ) orbits. Moreover,

graphic file with name M17.gif 2.7

with ξ running over Gϕ and β over Inline graphicGψ, where H = Hmand I = Im.

In fact, we can give an explicit set of representatives {τe}e=1λ(ϕ) for Eq. 2.6 and also an explicit set of representatives for PUω/PUωτe[Gψ × Gϕ] in the same manner as in Eq. 2.7. This proposition plays an essential role in the analysis of our Eisenstein series E(z, s; f, χ).

Section 3.

In this section, K is a locally compact field of characteristic 0 with respect to a discrete valuation. Our aim is to establish the Euler factor Wp of Eq. 1.2. We denote by r and q the valuation ring and its maximal ideal; we put q = [r:q] and |x| = q−ν if xK and x ∈ πν r× with ν ∈ Z. We assume that K has an automorphism ρ such that ρ2 = 1, and put F = {xK | xρ = x}, g = F ∩ r, and d−1 = {xK | TrK/F (xr) ⊂ g} if KF. We consider (V, ϕ) as in Section 2 with V = Kn1 and ϕ defined by ϕ(x, y) = xϕy* for x, yV with a matrix ϕ of the form

graphic file with name M19.gif 3.1

where t = n − 2r. We assume that θ is anisotropic and also that

graphic file with name M20.gif 3.2a
graphic file with name M21.gif 3.2b

Thus our group Gϕ is orthogonal, symplectic, or unitary. The element δ of Eq. 3.2b can be obtained by putting δ = uuρ with u such that r = g[u]. We include the case rt = 0 in our discussion. If t = 0, we simply ignore θ; this is always so if K = F and ɛ = −1. We have ϕ = θ if r = 0.

Denoting by {ei} the standard basis of Kn1, we put

graphic file with name M22.gif
graphic file with name M23.gif
graphic file with name M24.gif

Then Gϕ = PJϕC. We choose {er+i}i=1t so that N = ∑i=1trer+i. Then we can find an element λ of rtt such that

graphic file with name M25.gif 3.3

Put

graphic file with name M26.gif 3.4

We can write every element of PJϕ in the form

graphic file with name M27.gif
graphic file with name M28.gif 3.5

If t = 0, we simply ignore b, e, and f, so that ξ = [Inline graphicInline graphic]; we have ξ = e if r = 0.

We consider the Hecke algebra ℜ(E, GLr(K)) consisting of all formal finite sums ∑cxExE with cxQ and xGLr(K), with the law of multiplication defined as in ref. 1. Taking r indeterminates t1, … , tr, we define a Q-linear map

graphic file with name M31.gif 3.6

as follows; given ExE with xGLr(K), we can put ExE = ⊔y Ey with upper triangular y whose diagonal entries are πe1, … , πer with eiZ. Then we put

graphic file with name M32.gif 3.7

Next we consider the Hecke algebra ℜ(C, Gϕ) consisting of all formal finite sums ∑cτCτC with cτQ and τ ∈ Gϕ. We then define a Q-linear map

graphic file with name M33.gif 3.8

as follows; given CτC with τ ∈ Gϕ, we can put CτC = ⊔ξ Cξ with ξ ∈ P of form Eq. 3.5. We then put

graphic file with name M34.gif 3.9

where ω0 is given by Eq. 3.6 and dξ is the d-block in Eq. 3.5. We can prove that this is well defined and gives a ring-injection.

Given xKnm, we denote by ν0(x) the ideal of r which is the inverse of the product of all the elementary divisor ideals of x not contained in r; we put then ν(x) = [r:ν0(x)]. We call x primitive if rank(x) = Min(m, n) and all the elementary divisor ideals of x are r.

Proposition 2. Given ξ as in Eq. 3.5, suppose that both e and (δθ)−1 (e − 1) have coefficients in r if t > 0. Let a = g−1 h with primitive [g h] ∈ r2rr and gb = j−1k with primitive [j k] ∈ rr+tr. Then

graphic file with name M35.gif

where we take j = 1r if t = 0.

We now define a formal Dirichlet series 𝔗 by

graphic file with name M36.gif 3.10

This is a formal version of the Euler factor of Eq. 1.2 at a fixed nonarchimedean prime.

Theorem 1. Suppose that δϕ ∈ GLn(r); put p = [g:gq]. (Thus p = q if K = F.) Then

graphic file with name M37.gif
graphic file with name M38.gif
graphic file with name M39.gif
graphic file with name M40.gif

Here θi = 1 if i is even; when i is odd, θi is −1 or 0 according as d = r or d ≠ r.

This can be proved in the same manner as in ref. 2 by means of Proposition 2.

Since we are going to take localizations of a global unitary group, we have to consider Gϕ = G(V, ϕ) of Eq. 2.1 with V = Kn1, K = F × F, and ρ defined by (x, y)ρ = (y, x), where F is a locally compact field of characteristic 0 with respect to a discrete valuation. Let g and p be the valution ring of F and its maximal ideal; put r = g × g and p = [g:p]. We consider ℜ(C, Gϕ) with C = GϕGLn(r). Then the projection map pr of GLn(K) onto GLn(F) gives an isomorphism η:ℜ(C, Gϕ) → ℜ(E1, GLn(F)), where E1 = GLn(g). To be explicit, we have η(C(x, tx−1)C) = E1xE1. Let ω1 denote the map of Eq. 3.6 defined with n, E1, and F in place of r, E, and K. Putting ω = ω1 ○ η, we obtain a ring-injection

graphic file with name M41.gif 3.11

For z = (x, y) ∈ Knn with x, yFnn put ν1(z) = ν(x) and ν2(z) = ν(y), where ν is defined with respect to g instead of r. We then put

graphic file with name M42.gif 3.12

Then we obtain

graphic file with name M43.gif 3.13

Section 4.

We now take a totally imaginary quadratic extension K of a totally real algebraic number field F of finite degree. We denote by a (resp. h) the set of archimedean (resp. nonarchimedean) primes of F; further we denote by g (resp. r) the maximal order of F (resp. K). Let V be a vector space over K of dimension n. We take a K-valued nondegenerate ɛ-hermitian form ϕ on V with ɛ = 1 with respect to the Galois involution of K over F, and define Gϕ as in Section 2. For every vah and an object X, we denote by Xv its localization at v. For vh not splitting in K and for va, we take a decomposition

graphic file with name M44.gif 4.1

with anisotropic θ′v and a nonnegative integer rv. Put tv = dim(Tv). Then n = 2rv + tv. If n is odd, then tv = 1 for every vh. If n is even, then tv = 0 for almost all vh and tv = 2 for the remaining vh. If n is odd, by replacing ϕ by cϕ with a suitable cF, we may assume that ϕ is represented by a matrix whose determinant times (−1)(n−1)/2 belongs to NK/F(K).

We take and fix an element κ of K such that κρ = −κ and iκvϕv has signature (rv + tv, rv) for every va. Then G(iκvϕv) modulo a maximal compact subgroup is a hermitian symmetric space which we denote by ℨvϕ. We take a suitable point iv of ℨvϕ which plays the role of “origin” of the space. If rv = 0, we understand that ℨvϕ consists of a single point iv. We put ℨϕ = ∏vavϕ. To simplify our notation, for xKA× or x ∈ (C×)a, aZa, and c ∈ (C×)a, we put

graphic file with name M45.gif 4.2

For ξ ∈ Gvϕ and w ∈ ℨvϕ, we define ξw ∈ ℨvϕ in a natural way and define also a scalar factor of automorphy jξ(w) so that det(ξ)rvjξ(w)n is the jacobian of ξ. Given k, ν ∈ Za, z ∈ ℨϕ, and α ∈ GAϕ, we put

graphic file with name M46.gif 4.3

Then, for a function f:ℨϕC, we define fkα:ℨϕC by

graphic file with name M47.gif 4.4

Now, given a congruence subgroup Γ of Gϕ, we denote by 𝔐kϕ(Γ) the vector space of all holomorphic functions f on ℨϕ which satisfy fkγ = f for every γ ∈ Γ and also the cusp condition if Gϕ is of the elliptic modular type. We then denote by 𝔖kϕ(Γ) the set of all cusp forms belonging to 𝔐kϕ(Γ). Further, we denote by 𝔐kϕ resp. 𝔖kϕ the union of 𝔐kϕ(Γ) resp. 𝔖kϕ(Γ) for all congruence subgroups Γ of G. If ϕ is anisotropic, we understand that 𝔖0,νϕ = C.

Let D be an open subgroup of GAϕ such that DGhϕ is compact. We then denote by 𝔖kϕ(D) the set of all functions f: GAϕC satisfying the following conditions:

graphic file with name M48.gif 4.5

for every  p ∈ Ghϕ there exists an element fp ∈ 𝔖kϕ such that

graphic file with name M49.gif 4.6

We now take D in a special form. We take a maximal r-lattice M in V whose norm is g in the sense of ref. 3 (p. 375) and put

graphic file with name M50.gif 4.7
graphic file with name M51.gif 4.8
graphic file with name M52.gif 4.9

where d is the different of K relative to F and c is a fixed integral g-ideal. Clearly is an r-lattice in V containing M, and we easily see that Dϕ is an open subgroup of GAϕ. We assume that

graphic file with name M53.gif 4.10

Define a subgroup 𝔛 of GAϕ by

graphic file with name M54.gif 4.11

We then consider the algebra ℜ(D, 𝔛) consisting of all the finite linear combinations of DτD with τ ∈ 𝔛 and define its action on 𝔖kϕ (D) as follows. Given τ ∈ 𝔛 and f ∈ 𝔖kϕ(D), take a finite subset Y of Ghϕ so that DτD = ⊔η∈YDη and define f|DτD:GAϕC by

graphic file with name M55.gif 4.12

These operators form a commutative ring of normal operators on 𝔖kϕ(D).

For xGAϕ, we define an ideal ν0(x) of r by

graphic file with name M56.gif 4.13

where ν0(xv) is defined as in Section 3 with respect to an rv-basis of Mv. Clearly ν0(x) depends only on CxC.

Let f be an element of 𝔖kϕ(D) that is a common eigenfunction of all the DτD with τ ∈ 𝔛, and let f|DτD = λ(τ)f with λ(τ) ∈ C. Given a Hecke ideal character χ of K such that |χ| = 1, define a Dirichlet series 𝔗(s, f, χ) by

graphic file with name M57.gif 4.14

where χ* is the ideal character associated with χ and N(a) is the norm of an ideal a. Denote by χ1 the restriction of χ to FA×, and by θ the Hecke character of F corresponding to the quadratic extension K/F. For any Hecke character ξ of F, put

graphic file with name M58.gif 4.15

From Theorem 1 and Eq. 3.13, we see that

graphic file with name M59.gif
graphic file with name M60.gif 4.16

with a polynomial Wq of degree n whose constant term is 1, where q runs over all the prime ideals of K prime to c. Let Z(s, f, χ) denote the function of Eq. 4.16. Put

graphic file with name M61.gif 4.17

Theorem 2. Suppose that χa(b) = bμ|b|iκ−μ with μ ∈ Zaand κ ∈ Rasuch thatva κv = 0. Put m = k + 2ν − μ and

graphic file with name M62.gif

with γv defined by

graphic file with name M63.gif
graphic file with name M64.gif
graphic file with name M65.gif
graphic file with name M66.gif
graphic file with name M67.gif

Then ℜ(s, f, χ) can be continued to the whole s-plane as a meromorphic function with finitely many poles, which are all simple. It is entire if χ1 ≠ θν for ν = 0, 1.

We can give an explicitly defined finite set of points in which the possible poles of ℜ belong. Notice that pv and qv are polynomials; in particular, pv = 1 if 0 ≤ mvkv and qv = 1 if |μv − 2νv| ≥ n − 1.

The results of the above type and also of the type of Theorem 3 below were obtained in refs. 2, 4, and 5 for the forms on the symplectic and metaplectic groups over a totally real number field. The Euler product of type Z, its analytic continuation, and its relationship with the Fourier coefficients of f have been obtained by Oh (6) for the group Gϕ as above when ϕ = ηr.

Section 5.

We now put (W, ψ) = (V, ϕ) ⊕ (Hm, ηm) as in Eq. 2.5 with (V, ϕ) of Section 4 and m ≥ 0. Writing simply I = Im, we can consider the parabolic subgroup PIψ of Gψ. We put Pψ = PIψ for simplicity, λ0(α) = det(λIψ(p)) for pPψ, and

graphic file with name M68.gif 5.1

with M of Section 4 and the standard basis {ɛi, ɛm+n+i}i=1m of Hm. We can define the space ℨψ and its origin iψ in the same manner as for Gϕ. We then put

graphic file with name M69.gif 5.2
graphic file with name M70.gif 5.3

Here ev is the element of End(Vv) defined for xv by wxvwev ∈ (Hm)v for wVv. We define an R-valued function h on GAψ by

graphic file with name M71.gif 5.4

Taking f ∈ 𝔖kϕ(Dϕ) and χ as in Section 4, we define μ:GAψC as follows: μ(x) = 0 if xPAψDψ; if x = pw with pPAψ and wDψC0ψ, then we put

graphic file with name M72.gif 5.5

where χc = ∏v|c χv. Then we define E(x, s) for xGAψ and sC by

graphic file with name M73.gif
graphic file with name M74.gif 5.6

This is meaningful if χa(b) = bk+2ν|b|iκ−k−2ν with κ ∈ Ra, ∑va κv = 0, and the conductor of χ divides c. We take such a χ in the following theorem. The series of Eq. 5.6 is the adelized version of a collection of several series of the type in Eq. 1.3.

Theorem 3. Define γv as in Theorem 2 with m = 0. Put

graphic file with name M75.gif
graphic file with name M76.gif

Then the product

graphic file with name M77.gif
graphic file with name M78.gif

can be continued to the whole s-plane as a meromorphic function with finitely many poles, which are all simple.

We can give an explicitly defined finite set of points in which the possible poles of the above product belong.

Section 6.

Let G be an arbitrary reductive algebraic group over Q. Given an open subgroup U of GA containing Ga and such that UGh is compact, we put Ua = aUa−1 and Γa = GUa for every aGA. We assume that Ga acts on a symmetric space 𝔚, and we let G act on 𝔚 via its projection to Ga. We also assume that Γa/𝔚 has finite measure, written vol(Γa/𝔚), with respect to a fixed Ga-invariant measure on 𝔚. Taking a complete set of representatives 𝔅 for G/GA/U, we put

graphic file with name M79.gif 6.1

where T is the set of elements of G which act trivially on 𝔚, and we assume that [ΓaT:1] is finite. Clearly σ(U) does not depend on the choice of 𝔅. We call σ(G, U) the mass of G with respect to U. If Ga is compact, we take 𝔚 to be a single point of measure 1 on which Ga acts trivially. Then we have

graphic file with name M80.gif 6.2

We can show that σ(U′) = [U:U′]σ(U′) if U′ is a subgroup of U. If strong approximation holds for the semisimple factor of G, then it often happens that both [ΓaT:1] and vol(Γa/𝔚) depend only on U, so that

graphic file with name M81.gif 6.3

If Ga is compact and U is sufficiently small, then Γa = {1} for every a, in which case we have σ(U) = #(G/GA/U). If U is the stabilizer of a lattice L in a vector space on which G acts, then #(G/GA/U) is the number of classes in the genus of L. Therefore, σ(U) may be viewed as a refined version of the class number in this sense.

Coming back to the unitary group Gϕ of Section 4, we can prove the following theorem.

Theorem 4. Suppose that Gaϕ is compact. Let M be a g-maximal lattice in V of norm g and let d be the different of K relative to F. Define an open subgroup D of GAϕ by Eq. 4.9 with an integral ideal c. If n is odd, assume that ϕ is represented by a matrix whose determinant times (−1)(n−1)/2 belongs to NK/F(K); if n is even, assume that c is divisible by the product e of all prime ideals for which tv = 2. Then

graphic file with name M82.gif
graphic file with name M83.gif

where d = [F:Q], DF is the discriminant of F, and A = 1 or A = N(e)nN(d)n/2 according as n is odd or even.

If n is odd, we can also consider σ(D′) for

graphic file with name M84.gif 6.4

with an arbitrary integral ideal c. Then σ(D′) = 2−τσ(D), where τ is the number of primes in F ramified in K.

Section 7.

Let us now sketch the proof of the above theorems. The full details will be given in ref. 7. We first take 𝔅 ⊂ Inline graphic so that Inline graphic = ⊔b∈𝔅GϕbDϕ. Given E(x, s) as in Eq. 5.6, for each qGhψ we can define a function Eq(z, s) of (z, s) ∈ ℨψ × C by

graphic file with name M87.gif 7.1

The principle is the same as in Eq. 4.6, and so it is sufficient to prove the assertion of Theorem 3 with Eq(z, s) in place of E(x, s). In particular, we can take q to be q = b × 12m with b ∈ 𝔅. Define (X, ω) as in Eq. 2.5. Then there is an isomorphism of (X, ω) to (Hm+n, ηm+n) which maps PUω of Proposition 1 to the standard parabolic subgroup P of Gm+n). Therefore, we can identify ℨω with the space ha with

graphic file with name M88.gif 7.2

We can also define an Eisenstein series E′(x, s; χ) for xGAω and sC, which is defined by Eq. 5.6 with (Gm+n)A, P, 1) in place of (GAψ, Pψ, f). Taking E′ and (q, a) ∈ Ghω (with a ∈ 𝔅) in place of E(x, s) and q, we can define a function Eq,a(z, s) of (z, s) ∈ ha × C in the same manner as in Eq. 7.1. There is also an injection ι of ℨψ × ℨϕ into ha compatible with the embedding Gψ × GϕGm+n). We put then

graphic file with name M89.gif 7.3

for every function g on ha, where δ(w, z) is a natural factor of automorphy associated with the embedding ι. Take a Hecke eigenform f as in Section 4 and define fa by the principle of Eq. 4.6. Then, employing Proposition 1, we can prove

graphic file with name M90.gif
graphic file with name M91.gif 7.4

where q = b × 12m, A is a certain gamma factor, and Φa = Γa/ℨϕ. The computation is similar to, but more involved than, that of ref. 4 (Section 4). Since the analytic nature of Eq,a can be seen from the results of ref. 8, we can derive Theorem 3 from Eq. 7.4.

Take m = 0. Then ψ = ϕ and Eq(z, s) = fb(z). Then the analytic nature of 𝔗 (s, f, χ), and consequently that of Z(s, f, χ), can be derived from Eq. 7.4. However, here we have to assume that χa(b) = bk+2ν|b|iκ−k−2ν with κ ∈ Ra, ∑va κv = 0, and the conductor of χ divides c. The latter condition on c is a minor matter, but the condition on χa is essential. To obtain Z(s, f, χ) with an arbitrary χ, we have to replace Eq,a by 𝔇E"q,a, where E" is a series of type E′ with 2ν − μ in place of k and 𝔇 is a certain differential operator on ha.

As for Theorem 4, we take again ψ = ϕ and observe that a constant function can be taken as f if Gaϕ is compact. The space ℨϕ consists of a single point. The integral on the right-hand side of Eq. 7.4 is merely the value (Eq,a)°(z, w; s). We can compute its residue at s = n explicitly. Comparing it with the residue on the left-hand side, we obtain Theorem 4 when c satisfies Eq. 4.10. If n is odd, we can remove this condition by computing a group index of type [U:U′].

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