This paper introduces a new class of orthogonal Shimura varieties over totally real fields, constructs special cycles on them, and proves the modularity of their generating series in cohomology.
Contribution
It develops a novel class of Shimura varieties, constructs associated special cycles, and establishes the modularity of their generating series, advancing understanding in arithmetic geometry.
Findings
01
Construction of new orthogonal Shimura varieties over totally real fields
02
Definition of special cycles on these varieties
03
Proof of modularity of Kudla's generating series in cohomology
Abstract
For a new class of Shimura varieties of orthogonal type over a totally real number field, we construct special cycles and show the the modularity of Kudla's generating series in the cohomology group.
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Full text
Generating series of a new class of orthogonal Shimura varieties
Department of Mathematics, UC Berkeley, Berkeley, CA 94709, USA
Abstract.
For a new class of Shimura varieties of orthogonal type over a totally real number field, we construct special cycles and show the the modularity of Kudla’s generating series in the cohomology group.
1. Introduction
For Hilbert modular surfaces, Hirzebruch and Zagier showed in [HZ] that certain generating series that have as coefficients the Hirzebruch-Zagier divisors are modular forms of weight 1. Further inspired by this work, Gross, Kohnen and Zagier showed in [GKZ] that a generating series that has Heegner divisors as coefficients is modular of weight 3/2. This approach is unified by Borcherds in [Bo], who showed more generally the modularity of generating series with Heegner divisor classes as coefficients in the Picard group over Q.
Kudla and Millson extended the results to Shimura varieties of orthogonal type over a totally real number field and showed the modularity in the cohomology group in [Ku1], based on work from [KM1], [KM2], [KM3]. This is further extended by Yuan, Zhang and Zhang in [YZZ1], who showed the modularity of the generating series in the Chow group.
In the current paper, inspired by the above work of Kudla and Millson, we construct special cycles on a different Shimura variety of orthogonal type over a totally real number field F and show the modularity of Kudla’s generating series in the cohomology group.
We consider the Shimura variety corresponding to the reductive group ResF/QG, where G=GSpin(V) is the GSpin group for V a quadratic space over a totally real number field F, [F:Q]=d. We choose V of signature (n,2) at e real places and signature (n+2,0) at the remaining d−e places. Kudla, Millson and Yuan, Zhang, Zhang have treated the case of e=1, while we allow e∈{1,…,d}.
If e>1, there is no simpler divisor case, which makes the analysis much harder. In particular, there is a very technical convergence issue that does not appear in the work of Kudla and Millson.
We present now the setting of the paper. For F be a totally real field with real embeddings σ1,…σd, let A=AF be the ring of adeles of F and let V be a quadratic space over F of signature (n,2) at the infinite places σ1,…,σe and of signature (n+2,0) elsewhere. Let G denote the reductive group GSpin(V) over F.
We define the hermitian symmetric domain D corresponding to G to be:
[TABLE]
where Di is the Hermitian symmetric domain of oriented negative definite 2−planes in Vσi=V⊗σiR.
Then (ResF/QG,D) is a Shimura datum and for any open compact subgroup K of G(Af), this gives us the complex Shimura variety:
[TABLE]
For i=1,…,e we let LDi be the complex line bundle corresponding to the points of Di. We also define the projections maps pi:D→Di and then the line bundles pi∗LDi∈Pic(D) descend to line bundles LK,i∈Pic(MK)⊗Q.
Let W be a totally positive subspace of V, meaning that Wσi=W⊗σiR is a positive subspace of Vσi=V⊗σiR for all places 1≤i≤d. We define VW=W⊥ to be the space of vectors in V that are orthogonal to W, GW=GSpin(VW) and DW=DW,1×⋯×DW,e the Hermitian symmetric domain associated to GW, where DW,i consists of the lines in Di perpendicular to W. We actually have the natural identifications:
[TABLE]
where ⟨⋅,⋅⟩ is the inner product corresponding to qi, the quadratic form on Vσi, that extends to Vσi(C) by C-linearity.
Then (ResF/QGW,DW) is a Shimura datum and we have a morphism (ResF/QGW,DW)→(ResF/QG,D) of Shimura data. For K⊂G(Af) an open compact subgroup and g∈G(Af), we can define the complex Shimura variety:
[TABLE]
Moreover, we have an injection of MgKg−1,W into MK given by:
[TABLE]
We define the cycle Z(W,g)K to be the image of the morphism above. Note that Z(W,g)K is represented by the subset DW×GW(Af)gK of D×G(Af).
Now let x=(x1,…,xr)∈V(F)r and let U(x):=SpanF{x1,…,xr} be a subspace of V. Then we define Kudla’s special cycles:
[TABLE]
Here c1 denotes the Chern class of a line bundle. We will also use the notation Gx:=GU(x), Dx:=DU(x), Vx:=VU(x). Note that if x=(x1,…,xr)∈V(F)r, we have Gx=Gx1∩⋯∩Gxr, as well as Dx=Dx1∩⋯∩Dxr.
Now we will define Kudla’s generating function. For any Schwartz-Bruhat functions ϕf∈S(Vr(Af))K and g′ in Sp2r(A), where Sp2r(A) is the metaplectic cover of the symplectic group Sp2r(A), we define the generating series:
[TABLE]
Here r is the Weil representation of Sp2r(A)×O(VAr), where T(x)=21(⟨xi,xj⟩)1≤i,j≤r∈Mr(F) is the intersection matrix of x, and WT(x) is the standard Whittaker function for T(x).
Note that when e=1, for gf=Id and a careful choice of g∞′ we recover the generating series presented by Yuan, Zhang and Zhang in [YZZ1].
The following is the main theorem of the paper:
Theorem 1.1**.**
Let ϕf∈S(Vr(Af))K be any Schwartz-Bruhat function invariant under K. Then the series [Z(g′,ϕf)] is an automorphic form, discrete of parallel weight 1+2n for g′∈Sp2r(A) and valued in H2er(MK,C).
By modularity here we mean that, for any linear function l:H2er(MK,C)→C, the generating series obtained by acting via l on the cohomology classes of the special cycles
[TABLE]
is absolutely convergent and an automorphic form with coefficients in C in the usual sense.
The case e=1 was proved by Kudla and Millson in [Ku1], based on work from [KM1], [KM2], [KM3]. Yuan, Zhang and Zhang proved further in [YZZ1] the modularity of Z(g′,ϕf) in the Chow group. One can further conjecture that for e>1 the series Z(g′,ϕf) is an automorphic form, discrete of weight 1+2n for g′∈Sp2r(A) valued in CHer(MK)C. This is out of reach at the moment, but one can expect to extend the methods of Borcherds (see [Bo]) to show the modularity in the Chow group.
We will present now the ideas of the proof. We prove the cases e>1 by extending the ideas of Kudla and Millson. For each cycle Z(x,g) we want to construct a Green current η(x,g) of Z(x,g) in MK(C). Via the isomorphism HdR2er(XK,C)≃H2er(n−1)BM(XK,C), where the former is deRham cohomology while the latter is Borel-Moore cohomology, we have the identification of cohomology classes:
[TABLE]
where ω(η(x,g)) is the Chern form corresponding to the Green current η(x,g).
Let x∈V(F)r such that U(x):=SpanF{x1,…,xr} is a totally positive definite k-subspace of V. Define
[TABLE]
such that x1′=xi1,…,xk′=xik with 1≤i1<⋯<ik≤r the smallest indices for which U(x′)=U(x).
We take the currents defined by Kudla and Millson η0(xj′,τi) of Dxj,i in Di, where 1≤j≤k, 1≤i≤e. Taking further the ∗-product of the currents η0(xj′,τi) for 1≤i≤e, we get a Green current of Dx,i in Di:
[TABLE]
Taking the pullbacks via the projections pi:D→Di and taking the ∗-product, we obtain a Green current of Dx in D:
[TABLE]
Furthermore, we average the current η2(x′,g) on a lattice to get
[TABLE]
which is a Green current for G(F)(Dx×Gx(Af)gK/K) in D×G(Af)/K. Showing the convergence of the sum in the definition η3(x′,τ;g,h) represents the most technical part of the proof and it is treated in Section 3.7.
As η3(x′,τ;g,h) is invariant under the left action of G(F), η3(x′,τ;g,h) descends to a Green current η4(x′,τ;g,h) of Z(U(x),g)K in MK. Here G(F)(τ,h)K∈MK.
Taking the Chern forms, the ∗-product turns into wedge product and the averages, as well as the pullbacks are preserved. ω0(xj′,τi) is the Chern form of η0(xj′,τi) that is defined by Kudla and Millson in [Ku1], based on work from [KM1], [KM2], [KM3]. Furthermore, we have
[TABLE]
[TABLE]
are the Chern forms of η1(x′,τi) and η2(x′,τ) respectively, and
[TABLE]
is the Chern form of the Green current η3(x′,τ;g,h). Finally, ω3(x′,τ;g,h) descends to ω4(x′,τ;g,h) corresponding to the divisor Z(U(x),g)K in MK and is the Chern form of η4(x′,τ;g,h).
We defined above ω2,ω3 and ω4 for x′∈V(F)k with dimU(x′)=k. We actually can extend the definitions of ω2,ω3 and ω4 for x∈V(F)r when dimU(x)<r as well. For x∈V(F)r, if dimU(x)=k, we have the equality of cohomology classes [Z(U(x),g)]=[ω4(x′,τ;g,h)] in H2ek(MK,C) and we can actually show further that we also have:
[TABLE]
in H2er(MK,C).
Plugging in [ω4(x,τ;g,h)] for the cohomology class of [Z(x,g)], we take the the pullback p∗ of the natural projection map p:D×G(Af)/K→MK and unwind the sums. Then we get:
[TABLE]
It is enough to show that (1) is an automorphic form with values in H2er(D×G(Af)/K,C). We show this using the properties of the Kudla-Millson form on the weight of each individual ω0(x,τi), as we can rewrite (1) as:
[TABLE]
and the RHS is a theta function of weight (n+2)/2 with values in H2er(D×G(Af)/K,C), thus it is automorphic.
Acknowledgements. The authors would like to thank Xinyi Yuan for suggesting the problem and for very helpful discussions and insights regarding the problem. We would also like to thank the anonymous reviewer for detailed feedback. ER would also like to thank Max Planck Institute in Bonn for their hospitality, as well as to the IAS of Tsinghua University where part of the paper was written.
2. Background
2.1. Complex Geometry
We will recall now some background from complex geometry (see for example [CG], [GH]).
Let X be a connected compact complex manifold of dimension m. Suppose Y is a closed compact complex submanifold of codimension d. Then Y has no boundary and is thus a 2(m−d) chain in X. We can take the class of Y to be [Y]∈H2(m−d)(X,C).
Note that we have the perfect pairing:
[TABLE]
given by (Y,η)→∫Yη. Thus H2(m−d)(X,C)≃HdR2(m−d)(X,C)∨. We also have the perfect pairing:
[TABLE]
given by (η,ω)→∫Xη∧ω. Thus HdR2(m−d)(X,C)∨≃HdR2d(X,C). We can compose these isomorphisms to get:
[TABLE]
For X non-compact, we similarly can take the isomorphism:
[TABLE]
where the first group is the Borel-Moore homology, which allows infinite linear combinations of simplexes, while the second group is the deRham cohomology with compact support, which uses closed differential forms with compact support.
Now for Y a closed submanifold of X, in light of the above isomorphisms, a closed 2d-form ω on X in HdR2d(X,C) represents the class [Y] in H2(m−d)(X,C) (respectively H2(m−d)BM(X,C) when X non-compact), if and only if
[TABLE]
for any closed 2(m−d) form η on X.
If X is not connected, we restrict the above to each of the connected components.
2.2. Green currents and Chern forms
We recall some background on Green currents, following mainly [GS].
Let X be a quasi-projective complex manifold of dimension m. We define Ap,q(X) and Acp,q(X) to be the spaces of (p,q)-differential forms, and, respectively, (p,q)-differential forms with compact support. Let Dp,q(X)=Acp,q(X)∗ be the space of functionals that are continuous in the sense of deRham [DR]. That is, for a sequence {ωr}∈Ap,q(X) with support contained in a compact set K⊂X and for T∈Dp,q(X), we must have T(ωr)→0 if ωr→0, meaning that the coefficients of ωr and finitely many of their derivatives tend uniformly to [math].
We also recall the differential operators:
[TABLE]
2.2.1. Currents.
We define Dp,q:=Dm−p,m−q the space of (p,q)-currents. Then we have an inclusion Ap,q(X)→Dp,q(X) given by ω→[ω], where we define the current
[TABLE]
for any α∈Acm−p,m−q(X).
For Y⊂X a closed complex submanifold of dimension p, let ι:Y↪X be the natural inclusion and we also define a current δY∈Dp,p(X) by:
[TABLE]
for any α∈Acm−p,m−p.
Definition 2.1**.**
A Green current for a codimension p analytic subvariety Y⊂X is a current g∈Dp−1,p−1(X) such that
[TABLE]
for some smooth form ωY∈Ap,p(X).
This means for η∈Acm−p,m−p, we have:
[TABLE]
It implies that for a closed form with compact support η the LHS equals [math], and thus ∫XωY∧η=∫Yη. Thus for g a Green current of Y in X, we have as cohomology classes in the isomorphism (3):
[TABLE]
2.2.2. Green functions and Green forms.
One natural way to obtain Green currents is from Green functions. For Y⊂X a closed compact submanifold of codimension 1, a Green function of Y is a smooth function
[TABLE]
which has a logarithmic singularity along Y. This means that for any pair (U,fU) with U⊂X open and fU:U→C a holomorphic function such that Y∩U is defined by fU=0, then the function
[TABLE]
extends uniquely to a smooth function on U.
This definition can be extended for Y⊂X a closed complex submanifold of codimension p of X. We can define smooth forms gY∈Ap−1,p−1(X) of logarithmic type along Y such that the current [gY]∈Dp−1,p−1 given as in (4) by:
[TABLE]
is a Green current. We call such smooth forms Green forms of Y in X. We will occasionally abuse notation and use gY for both the Green form and the Green current corresponding to gY.
2.2.3. Chern forms.
Now let g be a Green function of Y⊂X, for Y a divisor on X. For U⊂X let fU=0 be the local defining equation of U∩Y. We define locally:
[TABLE]
By gluing together all ωU we get a differentiable form ωY over X. We call this the Chern form associated to the Green function g. In general for Y of codimension p in X, for a Green form gY of Y in X we call ωY the Chern form corresponding to gY.
2.2.4. Star product.
Another natural way to get Green currents is by taking their ∗-product. For Y,Z closed irreducible subvarieties of a smooth variety X such that Y and Z intersect properly, let gY,gZ Green forms of Y and Z, respectively. Then the ∗-product [gY]∗[gZ] is defined by Gillet and Soulé in [GS] to be:
[TABLE]
where [ωY]∧gZ(η)=∫Xη∧ωY∧gZ and [gY]∧δZ=π∗[π∗gY], where π:Z→X is the embedding map. For the definition of pushforwards of currents see [GS]. We can also define similarly the ∗-product [gY]∗GZ for gY a Green form of Y and GZ a Green current for Z (see [GS]).
Moreover, from [SABK] (Theorem 4, page 50), when Y and Z have the Serre intersection multiplicity 1, then [gY]∗[gZ] is a Green current for Y∩Z and we have:
[TABLE]
2.2.5. Pullback.
Also from [SABK] (3.2, page 50) for Z an irreducible smooth projective complex variety such that f:Z→X is a map with f−1(Y)=Z, then if gY is a Green form of logarithmic type along Y, f∗gY is a Green form of logarithmic type along f−1(Y). We define the pullback of currents f∗[gY]:=[f∗gY] and, when the components of f−1(Y) have Serre intersection multiplicity 1, the current f∗[gY] satisfies:
[TABLE]
3. Construction of Green currents and Chern forms
In this section we will construct a Green current of Z(U,g)K in MK for U a totally positive subspace of V(F).
3.1. The Shimura Variety
Recall σ1,…,σd are the embeddings of F into R and let (V,q) be a quadratic space such that Vσi=V⊗σiR, has signature (n,2) for 1≤i≤e and signature (n+2,0) otherwise. V has the inner product given by ⟨x,y⟩=q(x+y)−q(x)−q(y). This can be naturally extended to Vσi at each place σi for 1≤i≤d, and we denote by qi the quadratic form corresponding to this inner product.
We defined in the introduction the Hermitian symmetric domain
[TABLE]
where Di consists of all the oriented negative definite planes in Vσi. We can actually write explicitly the definition of Di as:
[TABLE]
where ⟨⋅,⋅⟩ is the inner product corresponding to qi that extends to Vσi(C) by C-linearity, and v↦vˉ is the involution on Vσi(C)=Vσi⊗RC induced by complex conjugation on C.
We now recall the definition of GSpin(V). Let (V,q) be a quadratic space over F and C(V,q)=(⊕kV⊗k)/I be the Clifford algebra of (V,q), where we are taking the quotient by the ideal I={q(v)−v⊗v∣v∈V}.
Then C(V,q) has dimension 2dim(V) and we have a Z-grading on T(V)=⨁kV⊗k. The map V→V, v→−v naturally extends to an algebra automorphism α:C(V,q)→C(V,q). Then there is a natural Z/2Z-grading on C(V,q) given by C(V,q)=C0(V,q)⊕C1(V,q), where
[TABLE]
We naturally have V⊂C1(V,q). Then we can define the GSpin group of V:
[TABLE]
We denote by G=GSpin(V) and note that G acts on V by conjugation. The group ResF/QG is reductive over Q and the pair (ResF/QG,D) is a Shimura datum. For K⊂G(AF) an open compact subgroup, this gives us the complex Shimura variety:
[TABLE]
For more details on the Shimura variety MK see [Sh].
We also define the complex line bundle LDi to be the restriction to Di of the tautological complex line bundle on P(Vσi(C)). Then for the projection maps pi:D→Di, we get the line bundles pi∗LDi∈Pic(D), which further descend to the line bundles LK,i∈Pic(MK)⊗Q over MK, defined to be:
[TABLE]
3.2. Green functions of Dx,i in Di
We first recall how to construct a Green function of Dx,i in Di, where
[TABLE]
Let τ∈Di. It corresponds to a negative definite 2−plane W in Vσi and we can write any x∈Vσi as x=xτ+xτ⊥ where xτ∈W and xτ⊥∈W⊥.
We define:
[TABLE]
Note that this implies R(x,τ)=0 if and only if τ∈Dx,i. For x=0 and qi(x)<0, then Dx,i is empty, and the statement that R(x,τ)=0 if and only if τ∈Dx,i is void, thus still true.
In terms of an orthogonal basis we can write τ=α+β−1 with α,β∈Vσi such that ⟨α,β⟩=0 and ⟨α,α⟩=⟨β,β⟩<0. Then τ corresponds to the negative oriented plane Wτ=Rα+Rβ⊂V(R), and we have:
[TABLE]
Another important property that we use is R(gx,gτ)=R(x,τ). This is easily seen in the definition above as the inner product is invariant under the action of g.
Moreover, we show below that −log(R(x,τ)) is a Green function for Dx,i in Di:
Lemma 3.1**.**
For fixed x∈V, x=0, and τ∈Di\Dx,i, the function −log(R(x,τ)) is a Green function for Dx,i in Di.
Proof: Recall the line bundle LDi is the restriction to Di of the tautological complex line bundle on P(Vσi(C)). It has the fiber Lτ=τC⊂Vσi(C) and we have a map:
[TABLE]
This defines an element sx(τ)∈Lτ∨. As τ varies, we get a map
[TABLE]
Then sx is a holomorphic section of the line bundle LDi∨. This section has a hermitian metric
[TABLE]
where v∈Lτ is any nonzero vector. In terms of an orthogonal basis we can write v=α+β−1 such that ⟨α,β⟩=0 and ⟨α,α⟩=⟨β,β⟩<0. Then
[TABLE]
and also xτ=⟨α,α⟩⟨x,α⟩α+⟨β,β⟩⟨x,β⟩β.
Computing directly gives us R(x,τ)=2∥sx(τ)∥2. It follows by a theorem of Poincaré-Lelong (see Theorem 2, p. 41 in [SABK]) that −log(R(x,τ)) is a Green function for Dx,i in Di.
For x∈V(F) and τ∈Di, we have the Green function defined by Kudla and Millson (see [Ku1]):
[TABLE]
where f(t)=−Ei(−t)=∫t∞xe−xdx is the exponential integral. Note that f(t)=−log(t)−γ−∫0txe−x−1dx, where γ is the Euler-Mascheroni constant. The function f(t) is smooth on (0,∞), f(t)+log(t) is infinitely differentiable on [0,∞), and f(t) decays rapidly as t→∞, thus using Lemma 3.1 we easily see that η(x,τ) is a Green function of Dx,i in Di.
Furthermore, Kudla and Millson have constructed explicitly the Chern form φKM(1)(x,τ) of η(x,τ). We recall its definition and properties in the following section.
Note that we can consider η(x,τ) as a restriction to Di of the Green function f(2π∥sx(v)∥2)=f(2π∣⟨v,v⟩∣∣⟨x,v⟩∣2) of Px(Vσi(C)):={v∈Px(Vσi(C)):⟨v,x⟩=0} inside P(Vσi(C)). Then the theory of Section 2.2, in particular the definition of the ∗-product, hold by restricting to Di.
3.3. The Kudla-Millson form φKM
We will now recall some results from Kudla (see [Ku1]), based on previous work of Kudla and Millson (see [KM1], [KM2] and [KM3]). Our goal is to present explicitly the construction of the form φKM(1).
For this section we will use the notation VR for a quadratic space over R with signature (n,2), G=GSpin(VR) and D the space of oriented negative 2−planes in VR. We fix a point z0∈D and let K=Stab(z0) be its stabilizer in GSpin(VR). Then
[TABLE]
Let g0=Lie(G) be the Lie algebra of G and k0=Lie(K) be the Lie algebra of K. We denote the complexifications of these lie algebras by g and k, respectively. We also can identify the Lie subalgebra p0⊂g0 given by
[TABLE]
Moreover, we can give p0 a complex structure using J=(0−110)∈GL2(R) acting as multiplication on the right. We denote by p+ and p− the ±i eigenspaces of p. Then we have a Harish-Chandra decomposition
[TABLE]
Moreover for the space of differential forms of type (a,b) on D we have an isomorphism:
[TABLE]
where on the RHS we have the wedge product ⋀a,b(p∗)=⋀ap+∗∧⋀bp−∗ for p+∗,p−∗ the dual spaces of p+ and p−, respectively.
Recall that Sp2m(R) is the metaplectic cover of Sp2m(R), and let K′ be the preimage under the projection map Sp2m(R)→Sp2m(R) of the compact subgroup:
[TABLE]
where U(m) is the unitary group. The group K′ has a character det1/2 whose square descends to the determinant character of U(m).
Then Kudla and Millson constructed a Schwartz form
[TABLE]
where S(VRm) is the Schwartz space over VRm, and by invariance under G we mean:
[TABLE]
We present their result below:
Theorem**.**
There exists an element φKM∘,(m)(x,τ)∈(S(VRm)⊗Ωm,m(D))G with the following properties:
(1)
For k′∈K′ such that ι(k′)=(A−BBA) under the natural map ι:Sp2m(R)→Sp2m(R), then we have:
[TABLE]
2. (2)
dφKM∘,(m)=0* i.e. for any x∈VRm, the form φKM∘,(m)(x,⋅) is a closed (m,m)-form on D which is Gx-invariant.*
We define below φKM∘,(m) explicitly following [Ku1]. The form φKM(m),∘ is denoted by φ(m) in [Ku1]. First we will construct φKM∘,(1).
Note that we have an isomorphism
[TABLE]
given by evaluating at z0. Recall that we identified the Lie algebra \displaystyle\mathfrak{p}_{0}=\big{\{}\left(\begin{smallmatrix}0&B\\
B^{T}&0\end{smallmatrix}\right):B\in M_{n\times 2}(\mathbb{R})\big{\}}\simeq M_{n\times 2}(\mathbb{R}). Then we have the differential forms ωi,j∈Ω1(D)=Ω1,0(D)⊕Ω0,1(D), 1≤i≤n, 1≤j≤2, defined by the function ωi,j∈p0∗, ωi,j:p0≃Mn×2(R)→R given by the map u=(ust)1≤s≤n,1≤t≤2→uij.
We first define for x=(x(1),…,x(n+2))∈VR the form φKM(1)(x) that is also G-invariant:
[TABLE]
We further define φKM∘,(1)(x) to be φKM∘,(1)(x)=e−2πqz0(x)φKM(1)(x), and finally, for x=(x1,…,xm)∈Vm we define:
[TABLE]
as well as φKM∘,(m)(x)=e−2πi=1∑mqz0(xi)φKM(m)(x).
Recall the Green function η(x,τ)=f(2πR(x,τ)), where x∈V(F) and τ∈Di. It has the important property ([Ku2], Proposition 4.10):
[TABLE]
where φKM(1)∈(S(V)⊗Ω1,1(Di))K is the Schwartz form defined above. This implies that φKM(1)(x,τ) is the Chern form corresponding to the Green function η(x,τ).
Note that (12) is mentioned in [Ku3], Theorem 4.10 for F=Q, but holds in general for F with a fixed real place σi for which Vσi has signature (n,2).
3.4. Averaging of Green currents and their Chern forms
Now let x=(x1,…,xr)∈V(F)r such that U(x)=SpanF{x1,…,xr} is a totally positive k-subspace of V(F), k≤r. Our goal is to construct a Green current of Z(U(x),g) in MK and its corresponding Chern form.
We define x′=(x1′,…,xk′) such that x1′=xi1,…,xk′=xik and U(x′)=U(x). To make this uniquely defined, we pick the smallest indices (i1,…,ik) for which this happens. Note further that as U(x)=U(x′), we also have Dx=Dx′, Vx=Vx′ and Gx=Gx′.
For τi∈Di and xj′∈V(F) for 1≤j≤r, 1≤i≤e, we define as in (9):
[TABLE]
that is a Green function of Dxj′,i in Di.
We can further fix z0,i∈Di for 1≤i≤e and we define the Kudla-Millson forms φKM(1)(xj′,τi)∈(S(V)⊗Ω(Di)(1,1))G for τi∈Di, xj′∈S(V), as in Section 3.3, that satisfy the equation:
[TABLE]
As x1′,…,xk′ are linearly independent, the submanifolds Dxj′,i intersect properly inside Di and thus we can take the ∗-product of the Green functions fi(xj′,τi) for 1≤j≤k. Denote
[TABLE]
Then, from (7), this is a Green current for Dx,i=Dx′,i=DU(x′),i=j=1⋂kDxj′,i in Di for 1≤i≤e.
As the star product turns into wedge product when we take the Chern forms (see (7)), the Chern form associated to η1(xj,τ) is going to be:
[TABLE]
Note that ω1(x′,τi)=φKM(k)(x′,τi) and thus from the definition (6) of the star product, η1 satisfies the equation:
[TABLE]
Let pi:D→Di be the natural projections as before. Then, from (8), pi∗η1(x,τi) is a Green function of pi∗Dx,i in D and the form pi∗φKM,i(k)(x′,τi) satisfies:
[TABLE]
By taking the ∗-product, we define for τ=(τ1,…,τe)∈D∖Dx:
[TABLE]
This is a Green current of Dx in D. This follows from (8), as the divisors pi∗Dx,i have Serre’s intersection multiplicity 1 in D. The Chern form of η2(x′,τ) is going to be:
[TABLE]
and it satisfies:
[TABLE]
We further take for (τ,h)∈D×G(Af) the average of Green currents:
[TABLE]
Note that this can be rewritten as
[TABLE]
where Γh=Gx(F)∖G(F)∩Gx(Af)gKh−1 is a lattice in G(F). It is clear from the average that η3 has a singularity along G(F)(Dx×Gx(Af)gK/K) in D×G(Af)/K. However, note that it is not obvious that this function converges. We are actually going to prove in Section 3.7 the following proposition:
Proposition 3.2**.**
Let x∈V(F)k such that U(x) is a totally positive k-subspace of V(F). Then the defining sum of η3(x,τ;g,h) is absolutely convergent and η3(x,τ;g,h) is a Green current of G(F)(Dx×Gx(Af)gK/K) in D×G(Af)/K.
This implies that η3(x′,τ;g,h) is a Green current of G(F)(Dx×Gx(Af)gK/K) in D×G(Af)/K. To get the Chern form we apply ddc locally and glue all the local forms using again [SABK], Theorem 4, page 50. This is possible due to the discussion at the end of the proof of Proposition 3.2 in Section 3.7.
Then η3 has the Chern form:
[TABLE]
where Γh=Gx′(F)∖G(F)∩Gx′(Af)gKh−1 as before.
As η3 is invariant under the action of G(F), it descends to a Green current via the projection map p:D×G(Af)/K→MK to:
[TABLE]
where (τ,h) represent the class G(F)(τ,h)K in MK. The Green current condition (5) is also preserved under the projection map, and the singularity is given by exactly the cycle Z(U(x),g)K inside the Shimura variety MK. Thus we get:
Proposition 3.3**.**
For x′ defined as above, η4(x′,τ;g,h) is a Green current of Z(U(x),g)K in MK.
Note that ω3(x′,τ;g,h) descends as well to the Chern form ω4(x′,τ;g,h) of η4(x′,τ;g,h). Moreover, the Chern form ω3(x′,τ;g,h) is the pullback under the projection map p:D×G(Af)/K→MK of ω4(x′,τ):
[TABLE]
3.5. Extending notation
In the previous section we have defined the Chern forms ω2,ω3,ω4 for x′=(x1′,…,xk′) with the coordinates x1′,…,xk′ linearly independent. We want to extend the definition to x=(x1,…,xk) in V(F)k when the coordinates x1,…,xk are linearly dependent over F.
In order to do that, we take ω1(x,τi)=φKM(k)(x,τi), ω2(x,τ)=p1∗ω1(x,τ1)∧⋯∧pe∗ω1(x,τe), and
[TABLE]
We will show in Section 3.7 in Proposition 3.9 that ω3 is well-defined.
Also note that for U a totally positive k-dimensional subspace of V(F) we can pick any y=(y1,…,yk) such that U(y)=U and η4(y,τ;g,h) is going to be a Green current of Z(U,g) in MK with its corresponding Chern form ω4(y,τ;g,h).
We can actually extend the definition of η2,η3,ω2,ω3 for v∈GLk(F∞) when x=(x1,…,xk)∈V(F)k such that U(x) is a totally positive k-plane inside of V. We define:
[TABLE]
where vi=σi(v)∈GLk(R) for 1≤i≤e. Note that Gvix=Gx and Dvix,i=Dx,i for all 1≤i≤e and η2(vx,τ) is a Green form of Dx in D.
We define further:
[TABLE]
where η3(vx,τ;g,h) is a Green form of G(F)(Dx×Gx(Af)gK/K) in D×G(Af)/K. The proof of convergence is similar to the one for η3(x,τ;g,h).
The Chern forms of η2(vx,τ) and η3(vx,τ) are going to be, respectively:
[TABLE]
[TABLE]
The Propositions 3.2 and 3.9 extend as well for η3(vx,τ;g,h) and ω3(vx,τ;g,h), thus they are well defined. As they are invariant under the action of G(F), η3 and ω3 further descend to the Green current η4(vx,τ;g,h) of Z(U(x),g) in MK that has the corresponding Chern form ω4(vx,τ;g,h).
Moreover, we extend the notation of ω2,ω3 for x=(x1,…,xk) with dimU(x)≤k by taking:
[TABLE]
[TABLE]
Propositions 3.9 extends as well, making ω3 well-defined in general.
3.6. Chern forms for x=0
Recall that we defined in Section 3.1 the line bundles LK,i∈Pic(MK,i)⊗Q. For x=0, we claim that we can still define ωi for 1≤i≤4 and the same relationships hold as in Section 3.4. Moreover, we are going to have:
[TABLE]
We define the Chern form ω1(0,τi)=(−1)rφKM(r)(0,τi). Here recall φKM(1)(0,τi)=−2π1j=1∑nωj,1∧ωj,2(τi) and φKM(r)(0,τi)=⋀rφKM(1)(0,τi) as defined in Section 3.3.
We actually have:
Lemma 3.4**.**
φKM(1)(0,τi)=−c1(LDi∨), for 1≤i≤e.
This is Corollary 4.12 in [Ku3]. Kudla considers F=Q, but the result is unchanged for a totally real number field F with a fixed embedding σi into R such that Vσi has signature (n,2).
Thus from the lemma above we have ω1(0,τi)=(−1)rc1(LDi∨)r. Then as before we define ω2(0,τ)=p1∗ω1(0,τ1)∧⋯∧pe∗ω1(0,τe). Note that ω2(0,τ)=(−1)rep1∗c1(LD1∨)r∧⋯∧pe∗c1(LDe∨)r. Furthermore, as G0=G, when we average over Γh=G0(F)∖(G(F)∩G0(Af)gKh−1) we get:
[TABLE]
Moreover, we have as before ω3(0,τ)=p∗ω4(0,τ), and thus
[TABLE]
where c1(LK∨):=c1(LK,1∨)…c1(LK,e∨). Finally, note that ω4(0,τ) is exactly the cycle Z(0,g)K in MK.
3.7. Convergence of η3(x,τ;g,h) and ω3(x,τ;g,h)
Now we are ready to show the convergence of η3(x,τ;g,h). More precisely, we are going to prove Proposition 3.2.
Before we continue, we mention two short lemmas that tell us about the behavior of R(x,τ) when τ varies in a compact set in Di and x varies in a lattice.
The first lemma tells us that the quadratic forms qτ bound each other:
Lemma 3.5**.**
Let Ki⊂Di be a compact set. Fix τ0∈Ki. Then there exist c,d>0 such that
[TABLE]
for all τ∈Ki.
Proof: Let τ∈Ki and x∈V, x=0. Consider the function ψ:Ki×{x∈V∣qτ0(x)=1}→R, ψ(τ,x)=qτ(x). Since qτ0 is positive definite, the set of vectors of norm 1 is a sphere and thus compact. Hence the domain is compact and thus the image is compact, and thus bounded. Since x=0, it must also be bounded away from [math]. Thus we can find constants c,d such that:
[TABLE]
and cqτ0(x)≤qτ(x)≤dqτ0(x) as desired.
The second lemma tells us how R(x,τ) increases when x varies in a lattice:
Lemma 3.6**.**
For a compact set K0⊂D and a lattice Γ⊂G(F), there are only finitely many γ∈Γ such that R(γ−1x,τi)≤N for any τ=(τ1,…,τe)∈K0. More precisely, if dimV=n+2, we have at most O(Nn/2+1) such γ∈Γ.
Proof: Fix some τ0∈K0∩Di. If for y∈Γx we have R(y,τi)=2qτi(y)−a<N, then from the previous lemma this implies that there exists c>0 such that qτ0(y)<ca+2N.
Thus y lies in a n+2 dimensional sphere in V of radius ca+2N. The result follows.
Now we want to compute the summands of:
[TABLE]
where Γh=Gx(F)∖G(F)∩Gx(Af)gKh−1. Recall η1(x,τi)=η0(x1,τi)∗⋯∗η0(xk,τi), where η0(x,τi)=f(2πR(x,τi)).
We compute first the general formula for the ∗-product of N Green currents:
Lemma 3.7**.**
Let f1,…,fN Green forms for the cycles Y1,…,YN inside X, chosen such that the star product [f1]∗⋯∗[fN] is well-defined. Let φ1,…,φN be their corresponding Chern forms. Then we have the ∗-product of N-terms:
[TABLE]
Proof: We denote δi,j=δi∧δi+1⋯∧δj, φi,j=φi∧⋯∧φj for i≤j and we take δi,j=φi,j=1 for i>j. We show the result by induction. For n=2, we have [f1]∗[f2]=f1∧δ2+φ1∧f2. Assume the result is true for n. Then we have:
[TABLE]
By definition, we have
[TABLE]
[TABLE]
This is exactly k=1∑n+1φ1,k−1∧[fk]∧δk+1,n+1 which finishes the proof.
We want to apply the above lemma to each of the ∗-products summands in (17) that define η3:
[TABLE]
Denote fi=pi∗η0 and φi=pi∗ω0. Then we get the terms:
[TABLE]
where all the terms before fi are the smooth forms φ and all the terms following fi are the operators δ.
Proof of Proposition 3.2: To show the convergence of η3, we need to show that for μ a smooth form with compact support, the integral ∫Xη3∧μ converges, where X=D×G(Af)/K. Note that we can cover the compact support supp(μ) of μ by finitely many open sets and in each of them we can write μ in local coordinates as a linear combination of smooth functions that are bounded inside supp(μ).
Thus it is enough to show that the form η3 converges to a smooth form on compacts.
for τ inside a compact set K0⊂D, where the average is taken over y=(y1,…,yk)∈Γhx. For the terms containing at least one δ, the terms
[TABLE]
are nonzero only for τe∈Dγ−1xk,e. However, this implies R(γ−1xk,τe)=0 and this only happens for finitely many γ∈Γ when τe∈K0 inside a compact from Lemma 3.6.
Thus the sum:
[TABLE]
is finite. This leaves the last term:
[TABLE]
which we treat below in Lemma 3.8. We show that the sum F2(x,τ) converges uniformly on compacts to a smooth form. This finishes the proof of the convergence in Proposition 3.2.
Note that F1(x,τ) is a finite sum of forms, while F2(x,τ) is the average of wedge products of smooth forms which converges to a smooth form.
To check the Green current condition (5) is met by η3(x,τ;g,h), again it is enough to check the condition on compact sets. Note first that τi∈Dyi only for finitely many y∈Γhx when τ is inside a compact set K0. For τi∈Dyi then we have a finite sum of terms η2 that satisfy the Green current condition (5): ddcη2(y,τ)+δDy,τ=[ω2(y,τ)]. For all the other terms, we do not have singularities, and as γ∈Γh∑η2(γ−1x,τ) and all its derivatives converge to a smooth form, we can just take ddc to get
[TABLE]
giving us the condition (5) for η3. Moreover, note that its Chern form is:
As promised, we show the convergence of F2(x,τ) below:
Lemma 3.8**.**
The average
[TABLE]
converges uniformly on compacts to a smooth form.
Proof: Let K0 be a compact. We are free to discard finitely many terms from our average of the star product without affecting the convergence, so we discard the terms for which fe(yk,τe)=0 on K0. For y=(y(1),i,…,y(n+2),i) coordinates determined by the point z0,i in Dy,i, we recall the explicit definition of φi(y,τi)=pi∗φKM(y,τi) that we presented in Section 3.3:
[TABLE]
Thus, in the average, all the terms are of the form:
[TABLE]
The forms pi∗ωs,1i,pi∗ωs,2i are smooth on K0 and the values of the smooth functions representing them in local coordinates are bounded inside a compact. As they are independent of y, the convergence of F2(x,τ) reduces to the convergence of:
[TABLE]
Here P(y)=i=1∏ej=1(i,j)=(e,k)∏k1,≤s,t≤n∑f=0∑1(yj(s),iyj(t),i)f is a polynomial of degree 2k(e−1).
Similarly, for computing the derivatives of F2(x,z) we are reduced to computing averages of the wedge products
[TABLE]
[TABLE]
We will break the proof in two main steps below:
**Step 1: ** We claim that it is enough to show that the sums:
[TABLE]
converge for any integers Re,k,Se,k≥0.
In order to show this, let us compute first the partial derivatives in τi of the terms φ(yj,τi) with (j,i)=(k,e). We get:
[TABLE]
where f∈{0,1} and 1≤s,t≤n. Since pi∗ωs,2i∧pi∗ωt,2i are smooth forms on compacts, the terms ∂Rτi∂Sτi∂pi∗ωs,1i∧pi∗ωt,2i(τi) are smooth as well. Then the problem reduces to showing that the coefficients:
[TABLE]
converge on compacts.
We can discard finitely many terms for which we have R(yj,τi)≤1 for any pair (i,j) with 1≤i≤e and 1≤j≤k. Then we can bound
[TABLE]
And thus we can further bound ∣P(y)∣≤Ci=1∏ej=1(i,j)=(e,k)∏k(qi(xj)+R(yj,z0,i))n2. By discarding finitely many terms from the lattice, we can bound e−2πR(yj,τi)R(yj,z0,i)m≤1, for any 1≤m≤n2 and then
[TABLE]
which is a constant. Thus we need to show that the sums:
[TABLE]
converge for any integers Re,k,Se,k≥0, as claimed in (19).
Step 2: Now we show the convergence of (19), in two parts.
(1)
First we show the case of y∈Γhx∑fe(yk,τe). We have fe(yk,τe)≤R(yk,τe)e−2πR(yk,τ)≤e−2πR(yk,τe) for R(yk,τe)≥1, which happens for all except finitely many yk’s from Lemma 3.6. Furthermore, also from Lemma 3.6, since there are at most O(z2n+2) vectors yk in our sum with z≤R(yk,τe)≤z+1, we are reduced to the convergence of
[TABLE]
which converges using the integral test.
2. (2)
Now we show the convergence of (19) for the partial derivatives in τe for the term fe(yk,τe). Note first that we can compute the derivatives:
[TABLE]
[TABLE]
We get in general terms of the form:
[TABLE]
where the above is a finite sum, Pi(∂R,yk) are polynomials in ∂aiτe∂biτe∂R(yk,τe), and the constants ci,di are integers that satisfy di≥1,and di>ci≥0. This can be easily shown by induction.
Excluding the terms for which R(yk,τe)≤1, note that if we fix a basis (e1,…,en+2) for Vσe, we have:
[TABLE]
thus we can further bound:
[TABLE]
where Ma,b is the upper bound of the values ∂aτe∂bτe∂R(ej,τe) for 1≤j≤n+2 and τe in our compact.
As di>ci, for R(yk,τe)≥1, we have (2πR(yk,τe))die−2πciR(yk,τe)<1 and using the above bound we have more generally:
[TABLE]
where Q~ is a polynomial in R(yk,z0,e). Let D be the degree of Q~ and let Q0(x):=∑∣an∣xn if Q:=∑anxn.
Similarly as before, we have at most O(z2n+2) values yk such that z≤R(yk,τe)≤z+1 for τe inside a compact, and the above convergence is equivalent to the convergence of
[TABLE]
which converges by the integral test.
Now we are also going to show:
Proposition 3.9**.**
For x=(x1,…,xk)∈V(F)k, the form
[TABLE]
converges.
Proof: Note that the above statement follows for dimU(x)=k from the proof of Proposition 3.2. For the general case the proof is similar to that
of Lemma 3.8. Using the notation from Lemma 3.8, we can write:
[TABLE]
Using the definition of φi(yj,τi):
[TABLE]
the terms pi∗ωs,1i∧pi∗ωt,1i are independent of y, and we are reduced to the convergence of the coefficients:
[TABLE]
where P(y)=i=1∏ej=1∏k1≤s,t≤n∑f=0∑1(yj(s),iyj(t),i)f. As in Lemma 3.8, we can bound:
[TABLE]
Moreover, for (i,j)=(e,k), by discarding finitely many terms from the lattice we have R(yk,τe) large enough and we can bound e−2πR(yj,τi)R(yj,z0,i)m≤1, for any 1≤m≤n2. Thus the convergence reduces to showing that
[TABLE]
converges, or equivalently that any of the terms:
[TABLE]
converge for 1≤m≤n2. Again we have at most O(z2n+2) values yk such that z≤R(yk,τe)≤z+1 for τe inside a compact, thus the above reduces to the convergence of:
[TABLE]
which converges by the integral test. This finishes our proof.
4. Modularity of Z(g′,ϕ)
We recall now the definition of the standard Whittaker function. Recall from Section 3.3 that we defined Sp2r(R) to be the metaplectic cover of Sp2r(R), K′ the preimage under the projection map Sp2r(R)→Sp2r(R) of the compact subgroup {(A−BBA),A+iB∈U(r)}, where U(r) is the unitary group. We also defined the character det1/2 on K′ whose square descends to the determinant character of U(r).
For (V+,q+) a quadratic space over R of signature (n+2,0), let φ+∘(x+)∈S(V+r) be the standard Gaussian:
[TABLE]
where 21(x,x)+=21((xi,xj))1≤i,j≤r is the intersection matrix of x=(x1,…,xr)∈V+r for the inner product (⋅,⋅) given by q+ on V+.
Then for x∈V+r and β=21(x,x)+ with β in Symr(R), the group of symmetric r×r matrices, we define the βth ”holomorphic” Whittaker function:
[TABLE]
where g∈Sp2r(R) and r is the Weil representation of Sp2r(R)×O(Vr).
Using the Iwasawa decomposition of Sp2r(R), we can write each g in the form:
[TABLE]
and we have:
[TABLE]
where τ=u+(v⋅vT)−1 is an element of Hr, the Siegel upper half-space of genus r (see [YZZ1] for a reference).
We can extend this definition for F∞. For g′=(gj′)1≤j≤d∈Sp2r(F∞)=σj:F↪R∏Sp2r(Rσj), we take:
[TABLE]
Moreover, by writing each gj′=(10uj1)(vj00(vjT)−1)kj′ using the Iwasawa decomposition and taking τj=uj+i(vj⋅vjT) as above, we get:
[TABLE]
Recall from the Introduction that we defined T(x)=21(⟨xi,xj⟩)1≤i,j≤r to be the intersection matrix in Mr(F). Note that for 1≤i≤e the intersection matrix T(x) is different from the intersection matrix 21(x,x)+ above, for which the inner product (⋅,⋅) is positive-definite.
We extend the definition of Wβ to σj(β)∈/Symr(R) for some σj, 1≤j≤e, by taking Wβ(g∞′)=0.
For g′∈Sp2r(A), ϕ∈(S(VAr))K, we defined in the introduction Kudla’s generating series:
[TABLE]
We will show:
Theorem 4.1**.**
The function Z(g′,ϕ) is an automorphic form parallel of weight 1+n/2 for g′∈Sp2r(A), ϕ∈S(VAr) with values in H2er(MK,C).
Recall that in H2er(MK,C) we have [Z(x,g)]=[ω4(x′,τ;g,h)∧((−1)ec1(LK∨))r−k] as cohomology classes, where c1(LK∨)=c1(LK,1∨)…c1(LK,e∨). We are actually going to show in Section 4.1 that [Z(x,g)]=[ω4(x,τ;g,h)] and we will replace in the sum (20) the cohomology class of the special cycle Z(x,g) with the cohomology class of ω4(x,τ;g,h). We are going to show first the following expansion of the pullback of [Z(g′,ϕ)] to D×G(Af)/K:
Lemma 4.2**.**
The pullback of the cohomology class [Z(g′,ϕ)] to D×G(Af)/K is the cohomology class:
[TABLE]
where p:D×G(Af)/K→MK is the natural projection map and gi′=(10ui1)(vi00(viT)−1)ki′ is the Iwasawa decomposition of gi′=σi(g′) for 1≤i≤d.
We claim that this will imply Theorem 4.1. We will first discuss the pullback of cohomology classes in Section 4.1 and we will show Lemma 4.2 and Theorem 4.1 at the end of the section.
4.1. Cohomology classes
First we would like to understand better how we take the pullback of the cohomology classes [ω3(x,τ;g,h)] to H2er(D×G(Af)/K,C).
Note that for x∈V(F)r with U(x) a totally positive k-subspace of V, and g∈G(Af), we have the equality of cohomology classes [Z(U(x),g)]=[ω4(x′,g)] in H2ek(MK,C) and we can take the pullback [ω3(x′,g)] to H2ek(D×G(Af)/K,C). The pullback of (−1)ec1(LK∨) to H2(D×G(Af)/K,C) is ω3(0,τ).
We are actually going to show that the pullbacks of the Kudla cycles Z(U(x),g)c1(LK∨)r−k can be represented by the cohomology class of [ω3(x,g)] in H2er(D×G(Af)/K,C) in the lemma below:
Lemma 4.3**.**
In H2er(D×G(Af)/K,C) we have the equality of cohomology classes:
[TABLE]
To show this, we first recall from [Ku1], Lemma 7.3, how the pullback acts on the Kudla-Millson form φKM(k). For 1≤i≤e, recall that (Vσi,qi) is a quadratic space of signature (n,2).
Lemma 4.4**.**
Let U⊂Vσi be a positive k-plane. For y∈U, let φ+∘∈S(Uk) be the standard Gaussian φ+∘(y)=e−πqi(y).
Let ιU:DU,i→Di be the natural injection. Then under the pullback ιU∗:Ωk(Di)→Ωk(DU,i) of differential forms, we have:
[TABLE]
where φKM,VU(k),∘∈(S(Uk)⊗Ωk,k(DU,i))K is the Kudla-Millson form for the vector space Vi,U=⟨U⟩⊥ and Hermitian symmetric domain DU,i.
For x∈V(F)r such that U(x) is a totally positive k-subspace of V we defined x′=(xi1,…,xik). Let x′′=(xj1,…,xjr−k) consist of the remaining components of x.
Just for this section, we will use the notation ωi(m)(x,τ) for i=2,3 when x=(x1,…,xm)∈Vm. Using the above lemma, we are first going to show:
Lemma 4.5**.**
With the above notation, the pullback of ω3(r−k)(x′′,τ;g,h) to DU×GU(Af)gK/K via the inclusion map ι:DU×GU(Af)gK/K→D×G(Af)/K equals:
[TABLE]
Proof: From the definition of φKM(r),∘ we can write:
[TABLE]
Then from Lemma 4.4, for ιU:DU,i→Di the natural embedding, we have iU∗φKM(r−k),∘(x′′)=(φ+∘⊗φKM,VU,i(r−k),∘)(x′′)=φ+∘(x′′)φKM,VU,i(r−k)(0), as x′′∈Ur−k. Note that this implies:
[TABLE]
We first want to pullback everything to D, via the projection maps pi:D→Di. We have the maps ιU:DU↪D, pi:D→Di. Recall that
[TABLE]
and we can further define the embedding ιU,i:DU,i↪Di and the projection map pU,i:DU→DU,i. It is easy to see that ιU,i∘pU,i=pi∘ιU as maps from DU to Di, thus we also have the equality of pullbacks of differentials Ωr−k(Di)→Ωr−k(DU):
[TABLE]
Then we get the equality:
[TABLE]
From (23), we have the RHS equal to pU,i∗φKM,VU,i(r−k)(0,τi). Applying the same steps also for φKM(r−k)(0), we get:
[TABLE]
Thus we have:
[TABLE]
Note that we can further take the wedge product of ιU∗pi∗φKM(r−k)(x,τi) for 1≤i≤e to get
[TABLE]
and using (24) this gives us ιU∗(ω2(r−k)(0,τ)). Note that this implies:
[TABLE]
Finally, we are interested in the pullback of ω3(r−k)(x′′,τ;g,h) to DU×GU(Af)gK/K via the inclusion map ι:DU×GU(Af)gK/K→D×G(Af)/K. We have:
[TABLE]
and using the pullback above for the RHS we get
[TABLE]
which equals ι∗ω3(r−k)(0,τ;g,h). Thus we have ι∗ω3(r−k)(x′′,τ;g,h)=ι∗ω3(r−k)(0,τ;g,h), which is the result of the lemma.
Note that using (23) and (14) one can actually show that
[TABLE]
as cohomology classes in H2r(Di,C).
Moreover, using (25) and (16), one can further show that
[TABLE]
as cohomology classes in H2r(D,C).
The proof of Lemma 4.3 below is based on the same principle.
Proof of Lemma 4.3: To show the equality of cohomology classes, we need to show that for a closed (l−r,l−r)-form μ with compact support, where l is the complex dimension of D×G(Af)/K, we have:
[TABLE]
From (5), for a closed form μ, as μ∧ω3(r−k) is a closed (l−k,l−k)-form we have:
[TABLE]
From (21), we have ι∗(μ∧ω3(r−k)(x′′))=ι∗(μ∧ω3(r−k)(0)), thus we get above:
Combining the two equations (27) and (28) we get (26).
Remarks on ω3(vx) and ω4(vx). We follow up with some remarks regarding ω3(vx,τ;g,h) and ω4(vx,τ;g,h) when v∈GLr(F∞) and x∈V(F)r with U(x) totally positive definite k-subspace of V(F). We have defined them in Section 3.5. Lemma 4.3 extends easily for ω3(vx,τ;g,h) and ω4(vx,τ;g,h) and we have as cohomology classes in H2er(D×G(Af)/K,C):
[TABLE]
As actually ω3((vx)′) represents the same cohomology class as the preimages of Z(U(vx),g) in D×G(Af)/K, and as Z(U(x),g)=Z(U(vx),g), we have:
Lemma 4.6**.**
(i)
As cohomology classes in H2er(D×G(Af)/K,C), we have:
[TABLE]
2. (ii)
Noting that (29) descends to MK, we also have as cohomology classes in H2er(MK,C):
[TABLE]
Proof of modularity: We will finish below the proofs of Lemma 4.2 and Theorem 4.1.
Proof of Lemma 4.2: The pullback to D×G(Af)/K of ω4(x′,τ) is ω3(x′,τ) and ω3(0,τ) is the pullback of (−1)erc1r(LK∨)=Z(0,g). Then in (20) we can write:
[TABLE]
Furthermore, from Corollary 4.3 we have [ω3(x′,g;τ,h)∧ω3(r−k)(0,τ)]=[ω3(x,τ;g,h)] as classes in H2er(D×G(Af)/K,C). From (29) we also have the equality of cohomology classes [ω3(x,τ;g,h)]=[ω3(vx,τ;g,h)]. Thus we get:
[TABLE]
By plugging in the definition ω3(vx,τ;g,h)=γ∈Gx(F)∖G(F)∑ω2(vx,γτ)1Gx(Af)gK(γh), we get the cohomology class p∗[Z(g′,ϕ)] equal to the cohomology class of:
[TABLE]
We will unwind the sum below to get the result of the lemma. We interchange the summations to get:
[TABLE]
Note that 1Gx(Af)gK(γh)=0 iff γh∈Gx(Af)gK, or equivalently if g∈Gx(Af)γhK, and since we are summing for g∈Gx(Af)∖G(Af)/K, we can replace g by γh everywhere and get:
[TABLE]
Since the action of G(Af) on ϕ is given by r(gf′,γh)ϕf(x)=r(gf′)ϕf(h−1γ−1x) and ω2(vx,γτ)=ω2(γ−1vx,τ)=ω2(v(γ−1x),τ), then we have:
[TABLE]
which gives us the result of the lemma.
Proof of Theorem 4.1: We would like to rewrite the sum of Lemma 4.2:
[TABLE]
and first show that this sum is automorphic with values in H2er(D×G(Af)/K,C).
We recall the Iwasawa decomoposition of g′=(gi′)1≤i≤d∈Sp2r(F∞) to be gi′=(10ui1)(vi00(viT)−1)ki′, where vi∈GLr(Rσi)+, ki′∈Ki′.
Recall that we have, for 1≤i≤e, ω1(x,τi)=φKM(r)(x,τi) and ω2(x,τ)=p1∗ω1(x,τ1)∧⋯∧pe∗ω1(x,τe). From the property (1) of the Theorem of Kudla and Millson we presented in Section 3.3, we have
[TABLE]
where φKM(r),∘(x,τi)=e−2πtrσi(T(x))φKM(x,τi). Using the Weil representation this easily extends to:
[TABLE]
We take the pullback to D via the projection maps pi:D→Di. We denote φi(x,τi)=pi∗φKM(r)(x,τi) and φi∘(x,τi)=e−2πtrσi(T(x))φi(x,τi) and thus we also have:
[TABLE]
Note that on the RHS we got Wσi(T(x))(gi′)φi(vix,τi), thus:
[TABLE]
Furthermore, as we can rewrite
[TABLE]
[TABLE]
we get:
[TABLE]
where ϕ∘(x,τ)=φ1∘(x,τ1)∧⋯∧φe∘(x,τe)i=e+1∏dφ0,i(x). Recall that for i≥e+1, WT(σi(x))(gi)=r(gi)φ0,i(x). Here φ0,i(x)=e−πtrT(σi(x)) is the standard Gaussian, as (Vσi,qi) is positive definite for i≥e+1.
and this is a theta function of weight (n+2)/2 with values in the cohomology group H2er(D×G(Af)/K,C). This means that for any linear functional l:H2er(D×G(Af)/K,C)→C acting on the cohomology part of ϕ∘(x,τ), the generating series:
[TABLE]
is a theta function of weight (n+2)/2. Note that this series is obtained by unwinding:
[TABLE]
Denote
[TABLE]
For the the natural projection p:D×G(Af)/K→MK, recall the pullback p∗:Ω2er(MK)→Ω2er(D×G(Af)/K), which further descends to the cohomology groups p∗:HdR2er(MK)→HdR2er(D×G(Af)/K) and the map is an injection.
We denote by SC2er(MK) the subspace of HdR2er(MK) generated by the classes [ω4(x,g)] and by SC2er(D×G(Af)/K) the subspace of HdR2er(MK) generated by the classes [ω3(x,g)].
Then the above pullback map restricts to p∗:SC2er(MK)→SC2er(D×G(Af)/K) and it is an injection.
Then for any linear functional l of SC2er(MK), we can just define the linear functional l on SC2er(D×G(Af)/K) given by l(p∗[ω])=l([ω]), and thus l(Z0(g′,ϕ))=l([Z(g′,ϕ)]) is automorphic. Thus [Z(g′,ϕ)] is a theta function valued in H2er(MK).
We can also easily check the weight of the theta function by computing r(k′)ϕ∘(x,τ)=r(k1′)φ1∘(x,τ1)∧⋯∧r(ke′)φe∘(x,τe)i=e+1∏dr(ki′)ϕ0,i(x) which gives us the factor det(ki′)2n+2 at each place i.
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