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Theta correspondence and simple factors in global Arthur parameters

Chenyan Wu chenyan.wu@unimelb.edu.au School of Mathematics and Statistics The University of Melbourne, Victoria 3010, Australia
Abstract.

By using results on poles of LL-functions and theta correspondence, we give a bound on bb for (χ,b)(\chi,b)-factors of the global Arthur parameter of a cuspidal automorphic representation π\pi of a classical group or a metaplectic group where χ\chi is a conjugate self-dual automorphic character and bb is an integer which is the dimension of an irreducible representation of SL2()\operatorname{\mathrm{SL}}_{2}(\mathbb{C}). We derive a more precise relation when π\pi lies in a generic global AA-packet.

Key words and phrases:
theta correspondence, Eisenstein series, LL-function, global Arthur packet
Corresponding author.

Introduction

Let FF be a number field and let 𝔸\mathbb{A} be its ring of adeles. Let π\pi be an irreducible cuspidal automorphic representation of a classical group GG defined over FF. We also treat the case of metaplectic groups in this work. However to avoid excessive notation, we focus on the case of the symplectic groups G=Sp(X)G=\operatorname{\mathrm{Sp}}(X) in this introduction where XX is a non-degenerate symplectic space over FF. By Arthur’s theory of endoscopy [2], π\pi belongs to a global AA-packet associated to an elliptic global AA-parameter, which is of the form

i=1r(τi,bi)\boxplus_{i=1}^{r}(\tau_{i},b_{i})

where τi\tau_{i} is an irreducible self-dual cuspidal automorphic representation of GLni(𝔸)\operatorname{\mathrm{GL}}_{n_{i}}(\mathbb{A}) and bib_{i} is a positive integer which represents the unique bib_{i}-dimensional irreducible representation of Arthur’s SL2()\operatorname{\mathrm{SL}}_{2}(\mathbb{C}). See Section 2, for more details.

In [17], Jiang proposed the (τ,b)(\tau,b)-theory. See, in particular, Principle 1.2 there. It is a conjecture that uses period integrals to link together automorphic representations in two global AA-packets whose global AA-parameters are “different” by a (τ,b)(\tau,b)-factor. We explain in more details. Let Πϕ\Pi_{\phi} denote the global AA-packet with elliptic global AA-parameter ϕ\phi. Let π\pi be an irreducible automorphic representation of G(𝔸)G(\mathbb{A}) and let σ\sigma be an irreducible automorphic representation of H(𝔸)H(\mathbb{A}), where HH is a factor of an endoscopic group of GG. Assume that π\pi (resp. σ\sigma) occurs in the discrete spectrum. Then it is expected that there exists some kernel function 𝒦\mathcal{K} depending on GG, HH and (τ,b)(\tau,b) only such that if π\pi and σ\sigma satisfy a Gan–Gross–Prasad type of criterion, namely, that the period integral

(0.1) H(F)\H(𝔸)G(F)\G(𝔸)𝒦(h,g)fσ(h)fπ(g)¯𝑑g𝑑h\int_{H(F)\operatorname{\backslash}H(\mathbb{A})}\int_{G(F)\operatorname{\backslash}G(\mathbb{A})}\mathcal{K}(h,g)f_{\sigma}(h)\overline{f_{\pi}(g)}dgdh

is non-vanishing for some choice of fσσf_{\sigma}\in\sigma and fππf_{\pi}\in\pi, then π\pi is in the global AA-packet Πϕ\Pi_{\phi} if and only if σ\sigma is in the global AA-packet Πϕ2\Pi_{\phi_{2}} with ϕ=(τ,b)ϕ2\phi=(\tau,b)\boxplus\phi_{2}. Then [17, Section 5] proceeds to construct certain kernel functions and then using them, defines endoscopy transfer (by integrating over H(F)\H(𝔸)H(F)\operatorname{\backslash}H(\mathbb{A}) only in (0.1)) and endoscopy descent (by integrating over G(F)\G(𝔸)G(F)\operatorname{\backslash}G(\mathbb{A}) only in (0.1)). It is not yet known if these are the kernel functions making the statements of Principle 1.2 in [17] hold. As the kernel functions come from Bessel coefficients or Fourier–Jacobi coefficients as in [7, Section 23], we see the non-vanishing of this period integral is analogous to condition (i) in the global Gan–Gross–Prasad Conjecture [7, Conjecture 24.1].

Jiang suggested in [17, Section 7] that if τ\tau is an automorphic character χ\chi, then the kernel function can be taken to be the theta kernel and endoscopy transfer and endoscopy descent are theta lifts. In this case, the span of

G(F)\G(𝔸)𝒦(h,g)fπ(g)¯𝑑g\displaystyle\int_{G(F)\operatorname{\backslash}G(\mathbb{A})}\mathcal{K}(h,g)\overline{f_{\pi}(g)}dg

as fπf_{\pi} runs over π\pi is the theta lift of π\pi. This is an automorphic representation of H(𝔸)H(\mathbb{A}). Lifting in the other direction is analogous. Assume that the theta lift of π\pi is non-zero. Write ϕπ\phi_{\pi} for the global AA-parameter of π\pi. Then [17, Principle 1.2] says that ϕπ\phi_{\pi} has a (χ,b)(\chi,b)-factor and that the global AA-parameter of the theta lift of π\pi from GG to HH should be ϕπ\phi_{\pi} with the (χ,b)(\chi,b)-factor removed. Here bb should be of appropriate size relative to GG and HH. Our work is one step in this direction.

One goal of this article is to expand on the (χ,b)(\chi,b)-theory and to present the results of [34], [10], [23], [46], [22], [48] for various cases in a uniform way. As different reductive dual pairs that occur in theta correspondence have their own peculiarities, the notation and techniques of these papers are adapted to the treatment of their own specific cases. We attempt to emphasise on the common traits of the results which are buried in lengthy and technical proofs in these papers.

After collecting the results on poles of LL-functions, poles of Eisenstein series and theta correspondence, we derive a bound for bb when bb is maximal among all factors of the global AA-parameter of π\pi. In addition, we derive an implication on global AA-packets. Of course, the heavy lifting was done by the papers mentioned above.

Theorem 0.1 (Corollary 5.3).

The global AA-packet attached to the elliptic global AA-parameter ϕ\phi cannot have a cuspidal member if ϕ\phi has a (χ,b)(\chi,b)-factor with

b>12dimFX+1,if G=Sp(X).b>\frac{1}{2}\dim_{F}X+1,\quad\text{if $G=\operatorname{\mathrm{Sp}}(X)$}.

Another way of phrasing this is that we have a bound on the size of bb that can occur in a factor of type (χ,)(\chi,*) in the global AA-parameter of a cuspidal automorphic representation. Thus our results have application in getting a Ramanujan bound, which measures the departure of the local components πv\pi_{v} from being tempered for all places vv of FF, for classical groups and metaplectic groups. This should follow by generalising the arguments in [18, Section 5] which treats the symplectic case. There they first established a bound for bb under some conditions on wave front sets. This enables them to control the contribution of GL1\operatorname{\mathrm{GL}}_{1}-factors in the global AA-parameter to the Ramanujan bound. Our result can supply this ingredient for classical groups and also metaplectic groups unconditionally. Then [18, Section 5] found a Ramanujan bound for π\pi by using the crucial results on the Ramanujan bound for GL2\operatorname{\mathrm{GL}}_{2} in [25] and [3].

We describe the idea of the proof of our result. First we relate the existence of a (τ,b)(\tau,b)-factor in the elliptic global AA-parameter of π\pi to the existence of poles of partial LL-functions LS(s,π×τ)L^{S}(s,\pi\times\tau^{\vee}). See Proposition 2.8. If the global AA-parameter of π\pi has a factor (τ,b)(\tau,b) where bb is maximal among all factors, we can show that the partial LL-function LS(s,π×τ)L^{S}(s,\pi\times\tau^{\vee}) has a pole at s=12(b+1)s=\frac{1}{2}(b+1). Thus studying the location of poles of LS(s,π×τ)L^{S}(s,\pi\times\tau^{\vee}) for τ\tau running through all self-dual cuspidal representations of GLn(𝔸F)\operatorname{\mathrm{GL}}_{n}(\mathbb{A}_{F}) can shed light on the size of bib_{i}’s that occur in the global AA-parameter of π\pi. Then we specialise to the case where τ\tau is a character χ\chi and consider LS(s,π×χ)L^{S}(s,\pi\times\chi^{\vee}) in what follows.

Next we relate the poles of LS(s,π×χ)L^{S}(s,\pi\times\chi^{\vee}) to the poles of Eisenstein series attached to the cuspidal datum χπ\chi\boxtimes\pi. See Section 3. In fact, in some cases, we use the non-vanishing of LS(s,π×χ)L^{S}(s,\pi\times\chi^{\vee}) at s=12s=\frac{1}{2} instead. See Proposition 3.1. Then we recall in Theorem 3.5 that the maximal positive pole of the Eisenstein series has a bound which is supplied by the study of global theta lifts. This is enough for showing Corollary 5.3, though we have a more precise result that the maximal positive pole corresponds to the invariant called the lowest occurrence index of π\pi with respect to χ\chi in Theorem 4.4. The lowest occurrence index is the minimum of the first occurrence indices over some Witt towers. For the precise definition see (4.2). We also have a less precise result (Theorem 4.1) relating the first occurrence index of π\pi with respect to certain quadratic spaces to possibly non-maximal and possibly negative poles of the Eisenstein series.

More precise results can be derived if we assume that π\pi has a generic global AA-parameter. This is because we have a more precise result relating poles or non-vanishing of values of the complete LL-functions to poles of the Eisenstein series supplied by [19]. Thus we get

Theorem 0.2 (Theorem 6.7).

Let π\pi be a cuspidal member in a generic global AA-packet of G(𝔸)=Sp(X)(𝔸)G(\mathbb{A})=\operatorname{\mathrm{Sp}}(X)(\mathbb{A}). Let χ\chi be a self-dual automorphic character of GL1(𝔸)\operatorname{\mathrm{GL}}_{1}(\mathbb{A}). Then the following are equivalent.

  1. (1)

    The global AA-parameter ϕπ\phi_{\pi} of π\pi has a (χ,1)(\chi,1)-factor.

  2. (2)

    The complete LL-function L(s,π×χ)L(s,\pi\times\chi^{\vee}) has a pole at s=1s=1.

  3. (3)

    The Eisenstein series E(g,fs)E(g,f_{s}) has a pole at s=1s=1 for some choice of section fs𝒜Q1(s,χπ)f_{s}\in\mathcal{A}^{Q_{1}}(s,\chi\boxtimes\pi).

  4. (4)

    The lowest occurrence index LOXχ(π)\operatorname{\mathrm{LO}}_{X}^{\chi}(\pi) is dimX\dim X.

Here Q1Q_{1} is a parabolic subgroup of Sp(X1)\operatorname{\mathrm{Sp}}(X_{1}) with Levi subgroup isomorphic to GL1×Sp(X)\operatorname{\mathrm{GL}}_{1}\times\operatorname{\mathrm{Sp}}(X), where X1X_{1} is the symplectic space formed from XX by adjoining a hyperbolic plane. Roughly speaking, 𝒜Q1(s,χπ)\mathcal{A}^{Q_{1}}(s,\chi\boxtimes\pi) is a space of automorphic forms on Sp(X1)\operatorname{\mathrm{Sp}}(X_{1}) induced from χ||sπ\chi|\ |^{s}\boxtimes\pi viewed as a representation of the parabolic subgroup Q1Q_{1}. We refer the reader to Section 3 for the precise definition of 𝒜Q1(s,χπ)\mathcal{A}^{Q_{1}}(s,\chi\boxtimes\pi). We note that the lowest occurrence index LOXχ(π)\operatorname{\mathrm{LO}}_{X}^{\chi}(\pi) is an invariant in the theory of theta correspondence related to the invariant called the first occurrence index. See Section 4 for their definitions. We also include a result (Theorem 6.3) that concerns the non-vanishing of L(s,π×χ)L(s,\pi\times\chi^{\vee}) at s=12s=\frac{1}{2} and the lowest occurrence index. We plan to improve this result in the future by studying a relation between non-vanishing of Bessel or Fourier–Jacobi periods and the lowest occurrence index.

We note that the LL-function L(s,π×χ)L(s,\pi\times\chi^{\vee}) has been well-studied and is intricately entwined with the study of theta correspondence, most prominently in the Rallis inner product formula which says that the inner product of two theta lifts is equal to the residue or value of L(s,π×χ)L(s,\pi\times\chi^{\vee}) at an appropriate point up to some ramified factors and some abelian LL-functions. We refer the reader to [49] which is a culmination of many previous results. See also the references in [49]. In our approach, the Eisenstein series E(g,fs)E(g,f_{s}), which is not of Siegel type, is the key link between L(s,π×χ)L(s,\pi\times\chi^{\vee}) and the theta lifts.

Now we describe the structure of this article. In Section 1, we set up some basic notation. In Section 2, we define elliptic global AA-parameters for classical groups and metaplectic groups and also the global AA-packet associated to an elliptic global AA-parameter. We show how poles of partial LL-functions detect (τ,b)(\tau,b)-factors in an elliptic global AA-parameter. In Section 3, we define Eisenstein series attached to the cuspidal datum χπ\chi\boxtimes\pi and recall some results on the possible locations of their maximal positive poles. In Section 4, we introduce two invariants of theta correspondence. They are the first occurrence index FOXY,χ(π)\operatorname{\mathrm{FO}}_{X}^{Y,\chi}(\pi) and the lowest occurrence index LOXχ(π)\operatorname{\mathrm{LO}}_{X}^{\chi}(\pi) of π\pi with respect to some data. We relate them to poles of Eisenstein series. Results in Sections 3 and 4 are not new. Our aim is to present the results in a uniform way for easier access. In Section 5, we show a bound for bb in (χ,b)(\chi,b)-factors of the global AA-parameter of π\pi. Finally in Section 6, we consider the case when π\pi has a generic global AA-parameter. We show that when L(s,π×χ)L(s,\pi\times\chi^{\vee}) has a pole at s=1s=1 (resp. L(s,π×χ)L(s,\pi\times\chi^{\vee}) is non-vanishing at s=12s=\frac{1}{2}), the lowest occurrence index is determined.

Acknowledgement

The author would like to thank Professor Dihua Jiang for suggesting the topic to her. The author would also like to thank the referee for reading the manuscript carefully and for informing her of some recent developments.

1. Notation

Let FF be a number field and let EE be either FF or a quadratic field extension of FF. Let ϱGal(E/F)\varrho\in\operatorname{\mathrm{Gal}}(E/F) be the trivial Galois element when E=FE=F and the non-trivial Galois element when EFE\neq F. When EFE\neq F, write εE/F\varepsilon_{E/F} for the quadratic character associated to E/FE/F via Class field theory. Let GG be an algebraic group over EE. We write RE/FG\operatorname{\mathrm{R}}_{E/F}G for the restriction of scalars of Weil. This is an algebraic group over FF.

Let ϵ\epsilon be either 11 or 1-1. By an ϵ\epsilon-skew Hermitian space, we mean an EE-vector space XX together with an FF-bilinear pairing

,X:X×XE\displaystyle\langle{\ },{\ }\rangle_{X}:X\times X\rightarrow E

such that

y,xX=ϵx,yXϱ,ax,by=ax,yXbϱ\langle{y},{x}\rangle_{X}=-\epsilon\langle{x},{y}\rangle_{X}^{\varrho},\quad\langle{ax},{by}\rangle=a\langle{x},{y}\rangle_{X}b^{\varrho}

for all a,bEa,b\in E and x,yXx,y\in X. We consider the linear transformations of XX to act from the right. We follow [49]’s notation closely and we intend to generalise the results here to the quaternionic unitary group case in our future work.

Let XX be an ϵ\epsilon-skew Hermitian space of finite dimension. Then the isometry group of XX is one of the following:

  1. (1)

    the symplectic group Sp(X)\operatorname{\mathrm{Sp}}(X) when E=FE=F and ϵ=1\epsilon=1;

  2. (2)

    the orthogonal group O(X)\mathrm{O}(X) when E=FE=F and ϵ=1\epsilon=-1;

  3. (3)

    the unitary group U(X)U(X) when EFE\neq F and ϵ=±1\epsilon=\pm 1.

We will also consider the metaplectic group. Let vv be a place of FF and let FvF_{v} denote the completion of FF at vv. Let 𝔸F\mathbb{A}_{F} (resp. 𝔸E\mathbb{A}_{E}) denote the ring of adeles of FF (resp. EE). Set 𝔸:=𝔸F\mathbb{A}:=\mathbb{A}_{F}. Write Mp(X)(Fv)\operatorname{\mathrm{Mp}}(X)(F_{v}) (resp. Mp(X)(𝔸F)\operatorname{\mathrm{Mp}}(X)(\mathbb{A}_{F})) for the metaplectic double cover of Sp(X)(Fv)\operatorname{\mathrm{Sp}}(X)(F_{v}) (resp. Sp(X)(𝔸F)\operatorname{\mathrm{Sp}}(X)(\mathbb{A}_{F})) defined by Weil [43]. We note that the functor Mp(X)\operatorname{\mathrm{Mp}}(X) is not representable by an algebraic group. We will also need the 1\mathbb{C}^{1}-extension Mp(X)(Fv)×μ21\operatorname{\mathrm{Mp}}(X)(F_{v})\times_{\mu_{2}}\mathbb{C}^{1} of Sp(X)(Fv)\operatorname{\mathrm{Sp}}(X)(F_{v}) and we denote it by Mp1(Fv)\operatorname{\mathrm{Mp}}^{\mathbb{C}^{1}}(F_{v}). Similarly we define Mp1(𝔸F)\operatorname{\mathrm{Mp}}^{\mathbb{C}^{1}}(\mathbb{A}_{F}).

Let ψ\psi be a non-trivial automorphic additive character of 𝔸F\mathbb{A}_{F} which will figure in the Weil representations as well as the global AA-parameters for Mp(X)\operatorname{\mathrm{Mp}}(X).

For an automorphic representation or admissible representation π\pi, we write π\pi^{\vee} for its contragredient.

2. Global Arthur Parameters

First we recall the definition of elliptic global Arthur parameters (AA-parameters) for classical groups as well as metaplectic groups. See [2] for the symplectic and the special orthogonal case and we adopt the formulation in [1] for the case of the (disconnected) orthogonal groups. For the unitary case, see [35, 26]. For the metaplectic case, see [9]. Then we focus on simple factors of global Arthur parameters and relate their presence to poles of partial LL-functions. This is a crude first step for detecting (τ,b)(\tau,b)-factors in an elliptic global AA-parameter according to the ‘(τ,b)(\tau,b)-theory’ proposed in [17].

Let 𝐆\mathbf{G} be U(X)\operatorname{\mathrm{U}}(X), O(X)\mathrm{O}(X), Sp(X)\operatorname{\mathrm{Sp}}(X) or Mp(X)\operatorname{\mathrm{Mp}}(X). Let dd denote the dimension of XX. Set 𝐆=SO(X)\mathbf{G}^{\circ}=\operatorname{\mathrm{SO}}(X) when 𝐆=O(X)\mathbf{G}=\mathrm{O}(X). Set 𝐆=𝐆\mathbf{G}^{\circ}=\mathbf{G} otherwise. Write 𝐆ˇ\check{\mathbf{G}} for the (complex) dual group of 𝐆\mathbf{G}^{\circ}. Then

𝐆ˇ={GLd(),if 𝐆=U(X);Spd1(),if 𝐆=O(X) and d is odd;SOd(),if 𝐆=O(X) and d is even;SOd+1(),if 𝐆=Sp(X);Spd(),if 𝐆=Mp(X).\check{\mathbf{G}}=\begin{cases}\operatorname{\mathrm{GL}}_{d}(\mathbb{C}),\quad&\text{if $\mathbf{G}=\operatorname{\mathrm{U}}(X)$};\\ \operatorname{\mathrm{Sp}}_{d-1}(\mathbb{C}),\quad&\text{if $\mathbf{G}=\mathrm{O}(X)$ and $d$ is odd};\\ \operatorname{\mathrm{SO}}_{d}(\mathbb{C}),\quad&\text{if $\mathbf{G}=\mathrm{O}(X)$ and $d$ is even};\\ \operatorname{\mathrm{SO}}_{d+1}(\mathbb{C}),\quad&\text{if $\mathbf{G}=\operatorname{\mathrm{Sp}}(X)$};\\ \operatorname{\mathrm{Sp}}_{d}(\mathbb{C}),\quad&\text{if $\mathbf{G}=\operatorname{\mathrm{Mp}}(X)$}.\end{cases}

An elliptic global AA-parameter for 𝐆\mathbf{G} is a finite formal sum of the form

ϕ=i=1r(τi,bi),for some positive integer r\phi=\boxplus_{i=1}^{r}(\tau_{i},b_{i}),\quad\text{for some positive integer $r$}

where

  1. (1)

    τi\tau_{i} is an irreducible conjugate self-dual cuspidal automorphic representation of GLni(𝔸E)\operatorname{\mathrm{GL}}_{n_{i}}(\mathbb{A}_{E});

  2. (2)

    bib_{i} is a positive integer which represents the unique bib_{i}-dimensional irreducible representation of Arthur’s SL2()\operatorname{\mathrm{SL}}_{2}(\mathbb{C})

such that

  • inibi=d𝐆ˇ\sum_{i}n_{i}b_{i}=d_{\check{\mathbf{G}}};

  • τi\tau_{i} is conjugate self-dual of parity (1)N𝐆ˇ+bi(-1)^{N_{\check{\mathbf{G}}}+b_{i}} (see Remark 2.3);

  • the factors (τi,bi)(\tau_{i},b_{i}) are pairwise distinct.

Here d𝐆ˇd_{\check{\mathbf{G}}} is the degree of the standard representation of 𝐆ˇ\check{\mathbf{G}} which, explicitly, is

d𝐆ˇ={dimX, if 𝐆=U(X);dimX1, if 𝐆=O(X) with dimX odd;dimX, if 𝐆=O(X) with dimX even;dimX+1, if 𝐆=Sp(X);dimX, if 𝐆=Mp(X)d_{\check{\mathbf{G}}}=\begin{cases}\dim X,&\text{ if $\mathbf{G}=\operatorname{\mathrm{U}}(X)$};\\ \dim X-1,&\text{ if $\mathbf{G}=\mathrm{O}(X)$ with $\dim X$ odd};\\ \dim X,&\text{ if $\mathbf{G}=\mathrm{O}(X)$ with $\dim X$ even};\\ \dim X+1,&\text{ if $\mathbf{G}=\operatorname{\mathrm{Sp}}(X)$};\\ \dim X,&\text{ if $\mathbf{G}=\operatorname{\mathrm{Mp}}(X)$}\end{cases}

and

N𝐆ˇ={dimXmod2, if 𝐆=U(X);0, if 𝐆=O(X) with dimX odd;1, if 𝐆=O(X) with dimX even;1, if 𝐆=Sp(X);0, if 𝐆=Mp(X).N_{\check{\mathbf{G}}}=\begin{cases}\dim X\mod 2,&\text{ if $\mathbf{G}=\operatorname{\mathrm{U}}(X)$};\\ 0,&\text{ if $\mathbf{G}=\mathrm{O}(X)$ with $\dim X$ odd};\\ 1,&\text{ if $\mathbf{G}=\mathrm{O}(X)$ with $\dim X$ even};\\ 1,&\text{ if $\mathbf{G}=\operatorname{\mathrm{Sp}}(X)$};\\ 0,&\text{ if $\mathbf{G}=\operatorname{\mathrm{Mp}}(X)$}.\end{cases}
Remark 2.1.

We adopt the notation in [17] and hence we write (τi,bi)(\tau_{i},b_{i}) rather than τiνbi\tau_{i}\boxtimes\nu_{b_{i}} as is more customary in the literature, so that the quantity bib_{i}, that we study, is more visible.

Remark 2.2.

In the unitary case, we basically spell out what Ψ2(U(N),ξ𝟏)\Psi_{2}(\operatorname{\mathrm{U}}(N),\xi_{\mathbf{1}}) in [35, Definition 2.4.7] is. We have discarded the second factor ψ~\tilde{\psi} as it is determined by ψN\psi^{N} and ξ𝟏\xi_{\mathbf{1}} in Mok’s notation.

Remark 2.3.
  1. (1)

    For 𝐆=U(X)\mathbf{G}=\operatorname{\mathrm{U}}(X), we say that τ\tau is conjugate self-dual of parity η\eta if the Asai LL-function L(s,τ,Asaiη)L(s,\tau,\mathrm{Asai}^{\eta}) has a pole at s=1s=1. If η=+1\eta=+1, we also say that τ\tau is conjugate orthogonal and if η=1\eta=-1, we also say that τ\tau is conjugate symplectic. The Asai representations come from the decomposition of the twisted tensor product representation of the LL-group. See [35, (2.2.9) and (2.5.9)] and [11].

  2. (2)

    For other cases, we mean self-dual when we write conjugate self-dual. We say that τ\tau is self-dual of parity +1+1 or orthogonal, if L(s,τ,Sym2)L(s,\tau,\operatorname{\mathrm{Sym}}^{2}) has a pole at s=1s=1; we say that τ\tau is self-dual of parity 1-1 or symplectic, if L(s,τ,2)L(s,\tau,\wedge^{2}) has a pole at s=1s=1.

  3. (3)

    The parity is uniquely determined for each irreducible conjugate self-dual cuspidal representation τ\tau.

Let Ψ2(𝐆)\Psi_{2}(\mathbf{G}) denote the set of elliptic global AA-parameters of 𝐆\mathbf{G}. Let ϕΨ2(𝐆)\phi\in\Psi_{2}(\mathbf{G}). Via the local Langlands conjecture (which is proved for the general linear groups), at every place vv of FF, we localise ϕ\phi to get an elliptic local AA-parameter,

ϕv:LFv×SL2()𝐆ˇWFv,\phi_{v}:L_{F_{v}}\times\operatorname{\mathrm{SL}}_{2}(\mathbb{C})\rightarrow\check{\mathbf{G}}\rtimes W_{F_{v}},

where WFvW_{F_{v}} is the Weil group of FvF_{v} and LFvL_{F_{v}} is WFvW_{F_{v}} if vv is archimedean and the Weil–Deligne group WFv×SL2()W_{F_{v}}\times\operatorname{\mathrm{SL}}_{2}(\mathbb{C}) if vv is non-archimedean. To ϕv\phi_{v} we associate the local LL-parameter φϕv:LFv𝐆ˇWFv\varphi_{\phi_{v}}:L_{F_{v}}\rightarrow\check{\mathbf{G}}\rtimes W_{F_{v}} given by

φϕv(w)=ϕv(w,(|w|12|w|12)).\varphi_{\phi_{v}}(w)=\phi_{v}(w,\begin{pmatrix}|w|^{\frac{1}{2}}&\\ &|w|^{-\frac{1}{2}}\end{pmatrix}).

Let Ldisc2(𝐆)L^{2}_{\mathrm{disc}}(\mathbf{G}) denote the discrete part of L2(𝐆(F)\𝐆(𝔸F))L^{2}(\mathbf{G}(F)\operatorname{\backslash}\mathbf{G}(\mathbb{A}_{F})) when 𝐆Mp(X)\mathbf{G}\neq\operatorname{\mathrm{Mp}}(X) and the genuine discrete part of L2(Sp(F)\Mp(𝔸F))L^{2}(\operatorname{\mathrm{Sp}}(F)\operatorname{\backslash}\operatorname{\mathrm{Mp}}(\mathbb{A}_{F})) for 𝐆=Mp(X)\mathbf{G}=\operatorname{\mathrm{Mp}}(X). Define the full near equivalence class Lϕ,ψ2(𝐆)L^{2}_{\phi,\psi}(\mathbf{G}) attached to the elliptic global AA-parameter ϕ\phi to be the Hilbert direct sum of all irreducible automorphic representations σ\sigma occurring in Ldisc2(𝐆)L^{2}_{\mathrm{disc}}(\mathbf{G}) such that for almost all vv, the local LL-parameter of σv\sigma_{v} is φϕv\varphi_{\phi_{v}}. We remark that in the Mp(X)\operatorname{\mathrm{Mp}}(X)-case, the parametrisation of σv\sigma_{v} is relative to ψv\psi_{v} since the local LL-parameter of σv\sigma_{v} is attached via the Shimura–Waldspurger correspondence which depends on ψv\psi_{v}. This is the only case in this article where Lϕ,ψ2(𝐆)L^{2}_{\phi,\psi}(\mathbf{G}) depends on ψ\psi.

Let 𝒜2(𝐆)\mathcal{A}_{2}(\mathbf{G}) denote the dense subspace consisting of automorphic forms in Ldisc2(𝐆)L^{2}_{\mathrm{disc}}(\mathbf{G}). Similarly define 𝒜2,ϕ,ψ(𝐆)\mathcal{A}_{2,\phi,\psi}(\mathbf{G}) to be the dense subspace of Lϕ,ψ2(𝐆)L^{2}_{\phi,\psi}(\mathbf{G}) consisting of automorphic forms. Then we have a crude form of Arthur’s multiplicity formula which decomposes the L2L^{2}-discrete spectrum into near equivalence classes indexed by Ψ2(𝐆)\Psi_{2}(\mathbf{G}).

Theorem 2.4.

We have the orthogonal decompositions

Ldisc2(𝐆)=^ϕΨ2(𝐆)Lϕ,ψ2(𝐆)and𝒜2(𝐆)=ϕΨ2(𝐆)𝒜2,ϕ,ψ(𝐆).\displaystyle L^{2}_{\mathrm{disc}}(\mathbf{G})=\hat{\oplus}_{\phi\in\Psi_{2}(\mathbf{G})}L^{2}_{\phi,\psi}(\mathbf{G})\quad\text{and}\quad\mathcal{A}_{2}(\mathbf{G})=\oplus_{\phi\in\Psi_{2}(\mathbf{G})}\mathcal{A}_{2,\phi,\psi}(\mathbf{G}).
Remark 2.5.

This crude form of Arthur’s multiplicity formula has been proved for Sp(X)\operatorname{\mathrm{Sp}}(X) and quasi-split O(X)\mathrm{O}(X) by Arthur [2], for U(X)\operatorname{\mathrm{U}}(X) by [35] and [26] and for Mp(X)\operatorname{\mathrm{Mp}}(X) by [9]. This is also proved for non-quasi-split even orthogonal (and also unitary groups) in [6] and for non-quasi-split odd orthogonal groups in [16]. Thus for all cases needed in this paper, Theorem 2.4 is known.

We have some further remarks on the orthogonal and unitary cases.

Remark 2.6.

Arthur’s statements use SO(X)\operatorname{\mathrm{SO}}(X) rather than O(X)\mathrm{O}(X) and he needs to account for the outer automorphism of SO(X)\operatorname{\mathrm{SO}}(X) when dimX\dim X is even. See the paragraph below [2, Thm. 1.5.2]. The formulation for quasi-split even O(X)\mathrm{O}(X) is due to Atobe and Gan [1, Thm. 7.1(1)]. For odd O(X)\mathrm{O}(X), which is isomorphic to SO(X)×μ2\operatorname{\mathrm{SO}}(X)\times\mu_{2}, the reformulation of Arthur’s result is easy. Let TT be a finite set of places of FF. Assume that it has even cardinality. Let sgnT\operatorname{\mathrm{sgn}}_{T} be the automorphic character of μ2(𝔸F)\mu_{2}(\mathbb{A}_{F}) which is equal to the sign character at places in TT and the trivial character at places outside TT. These give all the automorphic characters of μ2(𝔸F)\mu_{2}(\mathbb{A}_{F}). Then every irreducible automorphic representation π\pi of O(X)(𝔸F)\mathrm{O}(X)(\mathbb{A}_{F}) is of the form π0sgnT\pi_{0}\boxtimes\operatorname{\mathrm{sgn}}_{T} for some irreducible automorphic representation π0\pi_{0} of SO(X)(𝔸F)\operatorname{\mathrm{SO}}(X)(\mathbb{A}_{F}) and some finite set TT of places of even cardinality. A near equivalence class of O(X)(𝔸F)\mathrm{O}(X)(\mathbb{A}_{F}) then consists of all irreducible automorphic representations π0sgnT\pi_{0}\boxtimes\operatorname{\mathrm{sgn}}_{T} for π0\pi_{0} running over a near equivalence class of SO(X)(𝔸F)\operatorname{\mathrm{SO}}(X)(\mathbb{A}_{F}) and sgnT\operatorname{\mathrm{sgn}}_{T} running over all automorphic characters of μ2(𝔸F)\mu_{2}(\mathbb{A}_{F}).

Remark 2.7.

For the U(X)\operatorname{\mathrm{U}}(X) case, the global AA-parameter depends on the choice of a sign and a conjugate self-dual character which determine an embedding of the LL-group of U(X)\operatorname{\mathrm{U}}(X) to the LL-group of RE/FGLd\operatorname{\mathrm{R}_{E/F}\operatorname{\mathrm{GL}}}_{d} where we recall that d:=dimXd:=\dim X. We refer the reader to [35, Sec. 2.1], in particular (2.1.9) there, for details. In this work, we choose the +1+1 sign and the trivial character, which, in Mok’s notation, means κ=1\kappa=1 and χκ=𝟏\chi_{\kappa}=\mathbf{1}. Then this corresponds to the standard base change of U(X)\operatorname{\mathrm{U}}(X) to RE/FGLd\operatorname{\mathrm{R}_{E/F}\operatorname{\mathrm{GL}}}_{d}. We note that the LL-functions we use below are such that

Lv(s,πv×τv)=Lv(s,BC(πv)τv),L_{v}(s,\pi_{v}\times\tau_{v})=L_{v}(s,\operatorname{\mathrm{BC}}(\pi_{v})\otimes\tau_{v}),

for all places vv, automorphic representations π\pi of 𝐆(𝔸F)\mathbf{G}(\mathbb{A}_{F}) and τ\tau of RE/FGLa(𝔸F)\operatorname{\mathrm{R}_{E/F}\operatorname{\mathrm{GL}}}_{a}(\mathbb{A}_{F}) where BC\operatorname{\mathrm{BC}} denotes the standard base change.

By Theorem 2.4, we get

Proposition 2.8.

Let π\pi be an irreducible automorphic representation of 𝐆(𝔸F)\mathbf{G}(\mathbb{A}_{F}) that occurs in 𝒜2,ϕ,ψ(𝐆)\mathcal{A}_{2,\phi,\psi}(\mathbf{G}). Then

  1. (1)

    if ϕ\phi has a (τ,b)(\tau,b)-factor with bb maximal among all factors, then the partial LL-function LS(s,π×τ)L^{S}(s,\pi\times\tau^{\vee}) has a pole at s=b+12s=\frac{b+1}{2} and this is its maximal pole;

  2. (2)

    if the partial LL-function LS(s,π×τ)L^{S}(s,\pi\times\tau^{\vee}) has a pole at s=b+12s=\frac{b^{\prime}+1}{2}, then ϕ\phi has a (τ,b)(\tau,b)-factor with bbb\geq b^{\prime}.

Remark 2.9.

In the Mp(X)\operatorname{\mathrm{Mp}}(X) case, the LL-function depends on ψ\psi, but we suppress it from notation here.

Proof.

First we collect some properties of the Rankin–Selberg LL-functions for GLm×GLn\operatorname{\mathrm{GL}}_{m}\times\operatorname{\mathrm{GL}}_{n}. By the Rankin–Selberg method, for an irreducible unitary cuspidal automorphic representation τ\tau, LS(s,τ×τ)L^{S}(s,\tau\times\tau^{\vee}) has a simple pole at s=1s=1 and is non-zero holomorphic for Re(s)1\operatorname{\mathrm{Re}}(s)\geq 1 and s1s\neq 1; for irreducible unitary cuspidal automorphic representations τ\tau and τ\tau^{\prime} such that τ≇τ\tau\not\cong\tau^{\prime}, LS(s,τ×τ)L^{S}(s,\tau\times\tau^{\prime\vee}) is non-zero holomorphic for Re(s)1\operatorname{\mathrm{Re}}(s)\geq 1. These results can be found in Cogdell’s notes [5] which collect the results from [20, 21, 38, 39].

Assume that ϕ=i=1r(τi,bi)\phi=\boxplus_{i=1}^{r}(\tau_{i},b_{i}). Then

LS(s,π×τ)=i=1rj=0bi1LS(sbi12+j,τi×τ),L^{S}(s,\pi\times\tau^{\vee})=\prod_{i=1}^{r}\prod_{j=0}^{b_{i}-1}L^{S}(s-\frac{b_{i}-1}{2}+j,\tau_{i}\times\tau^{\vee}),

where SS is a finite set of places of FF outside of which all data are unramified.

Assume that ϕ\phi has a (τ,b)(\tau,b)-factor with bb maximal among all factors, then by the properties of the Rankin–Selberg LL-functions, we see that LS(s,π×τ)L^{S}(s,\pi\times\tau^{\vee}) has a pole at s=b+12s=\frac{b+1}{2} and it is maximal.

Next assume that the partial LL-function LS(s,π×τ)L^{S}(s,\pi\times\tau^{\vee}) has a pole at s=b+12s=\frac{b^{\prime}+1}{2}. If ϕ\phi has no (τ,c)(\tau,c)-factor for any c>0c\in\mathbb{Z}_{>0}, then LS(s,π×τ)L^{S}(s,\pi\times\tau^{\vee}) is holomorphic for all ss\in\mathbb{C} and we get a contradiction. Thus ϕ\phi has a (τ,b)(\tau,b)-factor. We take bb maximal among all factors of the form (τ,)(\tau,*) in ϕ\phi. As bb may not be maximal among all simple factors of ϕ\phi, we can only conclude that LS(s,π×τ)L^{S}(s,\pi\times\tau^{\vee}) is holomorphic for Re(s)>b+12\operatorname{\mathrm{Re}}(s)>\frac{b+1}{2}. Thus bbb^{\prime}\leq b. ∎

Given an irreducible cuspidal automorphic representation π\pi, write ϕπ\phi_{\pi} for the global AA-parameter of π\pi. By studying poles of LS(s,π×τ)L^{S}(s,\pi\times\tau^{\vee}) for varying τ\tau’s, we can detect the existence of (τ,b)(\tau,b)-factors with maximal bb in ϕπ\phi_{\pi}. We would also like to construct an irreducible cuspidal automorphic representation with global AA-parameter ϕπ(τ,b)\phi_{\pi}\boxminus(\tau,b) which means removing the (τ,b)(\tau,b)-factor from ϕπ\phi_{\pi} if ϕπ\phi_{\pi} has a (τ,b)(\tau,b)-factor. Doing this recursively, we will be able to compute the global AA-parameter of a given irreducible cuspidal automorphic representation. In reverse, the construction should produce concrete examples of cuspidal automorphic representations in a given global AA-packet with an elliptic global AA-parameter. This will be investigated in our future work.

In this article, we focus our attention on the study of poles of LS(s,π×τ)L^{S}(s,\pi\times\tau^{\vee}) where τ\tau is a conjugate self-dual irreducible cuspidal automorphic representation of RE/FGL1(𝔸)\operatorname{\mathrm{R}_{E/F}\operatorname{\mathrm{GL}}}_{1}(\mathbb{A}). Now we write χ\chi for τ\tau to emphasise that we are considering the case of twisting by characters. This case has been well-studied and it is known that the poles of LS(s,π×χ)L^{S}(s,\pi\times\chi^{\vee}) are intricately related to invariants of theta correspondence via the Rallis inner product formula which relates the inner product of two theta lifts to a residue or a value of the LL-function. We refer the readers to [27, 45, 12, 49] for details. One of the key steps is the regularised Siegel–Weil formula which relates a theta integral to a residue or a value of a Siegel Eisenstein series. Our work considers an Eisenstein series which is not of Siegel type, but which is closely related to L(s,π×χ)L(s,\pi\times\chi^{\vee}).

3. Eisenstein series attached to χπ\chi\boxtimes\pi

In this section we deviate slightly from the notation in Section 2. We use G(X)G(X) to denote one of Sp(X)\operatorname{\mathrm{Sp}}(X), O(X)\mathrm{O}(X) and U(X)\operatorname{\mathrm{U}}(X). We let 𝐆(X)\mathbf{G}(X) be a cover group of G(X)G(X), which means 𝐆(X)=Sp(X)\mathbf{G}(X)=\operatorname{\mathrm{Sp}}(X) or Mp(X)\operatorname{\mathrm{Mp}}(X) if G(X)=Sp(X)G(X)=\operatorname{\mathrm{Sp}}(X), 𝐆(X)=O(X)\mathbf{G}(X)=\mathrm{O}(X) if G(X)=O(X)G(X)=\mathrm{O}(X) and 𝐆(X)=U(X)\mathbf{G}(X)=\operatorname{\mathrm{U}}(X) if G(X)=U(X)G(X)=\operatorname{\mathrm{U}}(X). We adopt similar notation to that in [36]. We define Eisenstein series on a larger group of the same type as 𝐆(X)\mathbf{G}(X) and collect some results on their maximal positive poles.

Let π\pi be an irreducible cuspidal automorphic representation of 𝐆(X)(𝔸)\mathbf{G}(X)(\mathbb{A}). We always assume that π\pi is genuine when 𝐆(X)=Mp(X)\mathbf{G}(X)=\operatorname{\mathrm{Mp}}(X). Let χ\chi be a conjugate self-dual automorphic character of RE/FGL1(𝔸)=𝔸E×\operatorname{\mathrm{R}}_{E/F}\operatorname{\mathrm{GL}}_{1}(\mathbb{A})=\mathbb{A}_{E}^{\times}. When EFE\neq F, we define

(3.1) ϵχ={0,if χ|𝔸F×=𝟙;1,if χ|𝔸F×=εE/F.\epsilon_{\chi}=\begin{cases}0,&\quad\text{if $\chi|_{\mathbb{A}_{F}^{\times}}=\mathds{1}$};\\ 1,&\quad\text{if $\chi|_{\mathbb{A}_{F}^{\times}}=\varepsilon_{E/F}$}.\end{cases}

Let aa be a positive integer. Let XaX_{a} be the ϵ\epsilon-skew Hermitian space over EE that is formed from XX by adjoining aa-copies of the hyperbolic plane. More precisely, let a+\ell_{a}^{+} (resp. a\ell_{a}^{-}) be a totally isotropic aa-dimensional EE-vector space spanned by e1+,,ea+e_{1}^{+},\ldots,e_{a}^{+} (resp. e1,,eae_{1}^{-},\ldots,e_{a}^{-}) such that ei+,ej=δij\langle{e_{i}^{+}},{e_{j}^{-}}\rangle=\delta_{ij} where δij\delta_{ij} is the Kronecker symbol. Then Xa=a+XaX_{a}=\ell_{a}^{+}\oplus X\oplus\ell_{a}^{-} with XX orthogonal to a+a\ell_{a}^{+}\oplus\ell_{a}^{-}.

Let G(Xa)G(X_{a}) be the isometry group of XaX_{a}. Let QaQ_{a} be the parabolic subgroup of G(Xa)G(X_{a}) that stabilises a\ell_{a}^{-}. Write Qa=MaNaQ_{a}=M_{a}N_{a} in the Levi decomposition with NaN_{a} being the unipotent radical and MaM_{a} the standard Levi subgroup. We have an isomorphism

m:RE/FGLa×G(X)Ma.m:\operatorname{\mathrm{R}_{E/F}\operatorname{\mathrm{GL}}}_{a}\times G(X)\rightarrow M_{a}.

where we identify RE/FGLa\operatorname{\mathrm{R}_{E/F}\operatorname{\mathrm{GL}}}_{a} with RE/FGL(a+)\operatorname{\mathrm{R}_{E/F}\operatorname{\mathrm{GL}}}(\ell_{a}^{+}). Let ρQa\rho_{Q_{a}} be the half sum of the positive roots in NaN_{a}, which can be viewed as an element in 𝔞Ma:=Rat(Ma)\mathfrak{a}_{M_{a}}^{*}:=\operatorname{\mathrm{Rat}}(M_{a})\otimes_{\mathbb{Z}}\mathbb{R} where Rat(Ma)\operatorname{\mathrm{Rat}}(M_{a}) is the group of rational characters of MaM_{a}. We note that as QaQ_{a} is a maximal parabolic subgroup, 𝔞Ma\mathfrak{a}_{M_{a}}^{*} is one-dimensional. Via the Shahidi normalisation [41], we identify 𝔞Ma\mathfrak{a}_{M_{a}}^{*} with \mathbb{R} and thus may regard ρQa\rho_{Q_{a}} as the real number

12(dimEX+a),\displaystyle\frac{1}{2}(\dim_{E}X+a),\quad if G(Xa) is unitary;\displaystyle\text{if $G(X_{a})$ is unitary};
12(dimEX+a1),\displaystyle\frac{1}{2}(\dim_{E}X+a-1),\quad if G(Xa) is orthogonal;\displaystyle\text{if $G(X_{a})$ is orthogonal};
12(dimEX+a+1),\displaystyle\frac{1}{2}(\dim_{E}X+a+1),\quad if G(Xa) is symplectic.\displaystyle\text{if $G(X_{a})$ is symplectic}.

Let Ka,vK_{a,v} be a good maximal compact subgroup of G(Xa)(Fv)G(X_{a})(F_{v}) in the sense that the Iwasawa decomposition holds and set Ka=vKa,vK_{a}=\prod_{v}K_{a,v}.

Let 𝒜Qa(s,χπ)\mathcal{A}^{Q_{a}}(s,\chi\boxtimes\pi) denote the space of \mathbb{C}-valued smooth functions ff on Na(𝔸)Ma(F)\G(Xa)(𝔸)N_{a}(\mathbb{A})M_{a}(F)\operatorname{\backslash}G(X_{a})(\mathbb{A}) such that

  1. (1)

    ff is right KaK_{a}-finite;

  2. (2)

    for any xRE/FGLa(𝔸)x\in\operatorname{\mathrm{R}_{E/F}\operatorname{\mathrm{GL}}}_{a}(\mathbb{A}) and gG(Xa)(𝔸)g\in G(X_{a})(\mathbb{A}) we have

    f(m(x,I)g)=χ(det(x))|det(x)|𝔸Es+ρQaf(g);f(m(x,I)g)=\chi(\det(x))|\det(x)|_{\mathbb{A}_{E}}^{s+\rho_{Q_{a}}}f(g);
  3. (3)

    for any fixed kKak\in K_{a}, the function hf(m(I,h)k)h\mapsto f(m(I,h)k) on G(X)(𝔸)G(X)(\mathbb{A}) is in the space of π\pi.

Now let 𝐆(X)=Mp(X)\mathbf{G}(X)=\operatorname{\mathrm{Mp}}(X). This case depends on ψ\psi. Let GL~1(Fv)\widetilde{\operatorname{\mathrm{GL}}}_{1}(F_{v}) be the double cover of GL1(Fv)\operatorname{\mathrm{GL}}_{1}(F_{v}) defined as follows. As a set it is GL1(Fv)×μ2\operatorname{\mathrm{GL}}_{1}(F_{v})\times\mu_{2} and the multiplication is given by

(g1,ζ1)(g2,ζ2)=(g1g2,ζ1ζ2(g1,g2)Fv)(g_{1},\zeta_{1})(g_{2},\zeta_{2})=(g_{1}g_{2},\zeta_{1}\zeta_{2}(g_{1},g_{2})_{F_{v}})

which has a Hilbert symbol twist when multiplying the μ2\mu_{2}-part. Analogously we define the double cover GL~1(𝔸)\widetilde{\operatorname{\mathrm{GL}}}_{1}(\mathbb{A}) of GL1(𝔸)\operatorname{\mathrm{GL}}_{1}(\mathbb{A}). Let χψ,v\chi_{\psi,v} denote the genuine character of GL~1(Fv)\widetilde{\operatorname{\mathrm{GL}}}_{1}(F_{v}) defined by

χψ,v((g,ζ))=ζγv(g,ψ12,v)1\chi_{\psi,v}((g,\zeta))=\zeta\gamma_{v}(g,\psi_{\frac{1}{2},v})^{-1}

where γv(,ψ12,v)\gamma_{v}(\cdot,\psi_{\frac{1}{2},v}) is a 44-th root of unity defined via the Weil index. It is the same one as in [8, page 521] except that we have put in the subscripts vv. Then

χψ((g,ζ))=ζvγv(gv,ψ12,v)1\chi_{\psi}((g,\zeta))=\zeta\prod_{v}\gamma_{v}(g_{v},\psi_{\frac{1}{2},v})^{-1}

is a genuine automorphic character of GL~1(𝔸)\widetilde{\operatorname{\mathrm{GL}}}_{1}(\mathbb{A}). Let K~a\widetilde{K}_{a} denote the preimage of KaK_{a} under the projection Mp(Xa)(𝔸)Sp(Xa)(𝔸)\operatorname{\mathrm{Mp}}(X_{a})(\mathbb{A})\rightarrow\operatorname{\mathrm{Sp}}(X_{a})(\mathbb{A}). We will also use ~\widetilde{\ } to denote the preimages of other subgroups of Sp(Xa)(𝔸)\operatorname{\mathrm{Sp}}(X_{a})(\mathbb{A}). Let m~\widetilde{m} be the isomorphism

GL~a(𝔸)×μ2𝐆(X)(𝔸)M~a(𝔸)\widetilde{\operatorname{\mathrm{GL}}}_{a}(\mathbb{A})\times_{\mu_{2}}\mathbf{G}(X)(\mathbb{A})\rightarrow\widetilde{M}_{a}(\mathbb{A})

that lifts m:GLa(𝔸)×G(X)(𝔸)Ma(𝔸)m:\operatorname{\mathrm{GL}}_{a}(\mathbb{A})\times G(X)(\mathbb{A})\rightarrow M_{a}(\mathbb{A}). Let det~\widetilde{\det} be the homomorphism

GL~a(𝔸)\displaystyle\widetilde{\operatorname{\mathrm{GL}}}_{a}(\mathbb{A}) GL~1(𝔸)\displaystyle\rightarrow\widetilde{\operatorname{\mathrm{GL}}}_{1}(\mathbb{A})
(x,ζ)\displaystyle(x,\zeta) (det(x),ζ).\displaystyle\mapsto(\det(x),\zeta).

We keep writing det\det for the non-genuine homomorphism

GL~a(𝔸)\displaystyle\widetilde{\operatorname{\mathrm{GL}}}_{a}(\mathbb{A}) GL1(𝔸)\displaystyle\rightarrow\operatorname{\mathrm{GL}}_{1}(\mathbb{A})
(x,ζ)\displaystyle(x,\zeta) det(x).\displaystyle\mapsto\det(x).

Given a non-genuine representation τ\tau of GL~a(𝔸)\widetilde{\operatorname{\mathrm{GL}}}_{a}(\mathbb{A}), we can twist it by χψdet~\chi_{\psi}\circ\widetilde{\det} to get a genuine representation which we denote by τχψ\tau\chi_{\psi}.

We remark that there are canonical embeddings of Na(𝔸)N_{a}(\mathbb{A}) and Sp(Xa)(F)\operatorname{\mathrm{Sp}}(X_{a})(F) to Mp(Xa)(𝔸)\operatorname{\mathrm{Mp}}(X_{a})(\mathbb{A}), so we may regard them as subgroups of 𝐆(Xa)(𝔸)\mathbf{G}(X_{a})(\mathbb{A}). Let 𝒜ψQa(s,χπ)\mathcal{A}^{Q_{a}}_{\psi}(s,\chi\boxtimes\pi) denote the space of \mathbb{C}-valued smooth functions ff on Na(𝔸)Ma(F)\𝐆(Xa)(𝔸)N_{a}(\mathbb{A})M_{a}(F)\operatorname{\backslash}\mathbf{G}(X_{a})(\mathbb{A}) such that

  1. (1)

    ff is right K~a\widetilde{K}_{a}-finite;

  2. (2)

    for any xGL~a(𝔸)x\in\widetilde{\operatorname{\mathrm{GL}}}_{a}(\mathbb{A}) and g𝐆(Xa)(𝔸)g\in\mathbf{G}(X_{a})(\mathbb{A}) we have

    f(m~(x,I)g)=χχψ(det~(x))|det(x)|𝔸Es+ρQaf(g);f(\widetilde{m}(x,I)g)=\chi\chi_{\psi}(\widetilde{\det}(x))|\det(x)|_{\mathbb{A}_{E}}^{s+\rho_{Q_{a}}}f(g);
  3. (3)

    for any fixed kK~ak\in\widetilde{K}_{a}, the function hf(m~(I,h)k)h\mapsto f(\widetilde{m}(I,h)k) on 𝐆(X)(𝔸)\mathbf{G}(X)(\mathbb{A}) is in the space of π\pi.

To unify notation, we will also write 𝒜ψQa(s,χπ)\mathcal{A}^{Q_{a}}_{\psi}(s,\chi\boxtimes\pi) for 𝒜Qa(s,χπ)\mathcal{A}^{Q_{a}}(s,\chi\boxtimes\pi) in the non-metaplectic case. It should be clear from the context whether we are treating the Sp(X)\operatorname{\mathrm{Sp}}(X) case or the Mp(X)\operatorname{\mathrm{Mp}}(X) case.

Now return to the general case, so 𝐆(X)\mathbf{G}(X) is one of Sp(X)\operatorname{\mathrm{Sp}}(X), O(X)\mathrm{O}(X), U(X)\operatorname{\mathrm{U}}(X) and Mp(X)\operatorname{\mathrm{Mp}}(X). Let fsf_{s} be a holomorphic section of 𝒜ψQa(s,χπ)\mathcal{A}^{Q_{a}}_{\psi}(s,\chi\boxtimes\pi). We associate to it the Eisenstein series

EψQa(g,fs):=γQa(F)\G(Xa)(F)fs(γg).E_{\psi}^{Q_{a}}(g,f_{s}):=\sum_{\gamma\in Q_{a}(F)\operatorname{\backslash}G(X_{a})(F)}f_{s}(\gamma g).

Note that the series is over γQa(F)\Sp(Xa)(F)\gamma\in Q_{a}(F)\operatorname{\backslash}\operatorname{\mathrm{Sp}}(X_{a})(F) when 𝐆(X)=Mp(X)\mathbf{G}(X)=\operatorname{\mathrm{Mp}}(X). By Langlands’ theory of Eisenstein series [36, IV.1], this series is absolutely convergent for Re(s)>ρQa\operatorname{\mathrm{Re}}(s)>\rho_{Q_{a}}, has meromorphic continuation to the whole ss-plane, its poles lie on root hyperplanes and there are only finitely many poles in the positive Weyl chamber. By our identification of 𝔞Ma\mathfrak{a}_{M_{a}}^{*} with \mathbb{R} and the fact that χ\chi is conjugate self-dual, the statements on poles mean that the poles are all real and that there are finitely many poles in the half plane Re(s)>0\operatorname{\mathrm{Re}}(s)>0.

We give the setup for any positive integer aa, though we will only need a=1a=1 in the statements of our results. However the proofs require ‘going up the Witt tower’ to 𝐆(Xa)\mathbf{G}(X_{a}) for aa large enough. Since we plan to prove analogous results for quaternionic unitary groups in the future, we keep the setup for general aa.

There is a relation between poles of LL-functions and the Eisenstein series.

Proposition 3.1.
  1. (1)

    Assume that the partial LL-function LψS(s,π×χ)L^{S}_{\psi}(s,\pi\times\chi^{\vee}) has its rightmost positive pole at s=s0s=s_{0}. Then EψQ1(g,fs)E_{\psi}^{Q_{1}}(g,f_{s}) has a pole at s=s0s=s_{0}.

  2. (2)

    Assume that the partial LL-function LψS(s,π×χ)L^{S}_{\psi}(s,\pi\times\chi^{\vee}) is non-vanishing at s=12s=\frac{1}{2} and is holomorphic for Re(s)>12\operatorname{\mathrm{Re}}(s)>\frac{1}{2}. Assume that

    𝐆(X)=U(X) with dimXϵχ(mod2);\displaystyle\text{$\mathbf{G}(X)=\operatorname{\mathrm{U}}(X)$ with $\dim X\equiv\epsilon_{\chi}\pmod{2}$};
    𝐆(X)=O(X) with dimX odd;\displaystyle\text{$\mathbf{G}(X)=\mathrm{O}(X)$ with $\dim X$ odd};
    𝐆(X)=Mp(X).\displaystyle\text{$\mathbf{G}(X)=\operatorname{\mathrm{Mp}}(X)$}.

    Then EψQ1(g,fs)E_{\psi}^{Q_{1}}(g,f_{s}) has a pole at s=12s=\frac{1}{2}.

Remark 3.2.

This is [23, Proposition 2.2] in the symplectic case, [46, Proposition 3.2] in the metaplectic case, [22, Proposition 2.2] in the unitary case and [34, Remarque 2] and [22, Proposition 2.2] in the orthogonal case.

Remark 3.3.

The allowed 𝐆(X)\mathbf{G}(X)’s in item (2) are those for which we have theta dichotomy and epsilon dichotomy (in the local non-archimedean setting). See [8, Corollary 9.2, Theorem 11.1].

Remark 3.4.

When π\pi is a cuspidal member in a generic global AA-packet of 𝐆(X)(𝔸)\mathbf{G}(X)(\mathbb{A}), there is a more precise result. See Theorem 6.3 which was proved in [19] and strengthened in [24].

We summarise the results on the maximal positive pole of EψQ1(g,fs)E_{\psi}^{Q_{1}}(g,f_{s}) from [10, Theorem 3.1], [22, Theorem 3.1], [23, Theorem 2,8] and [46, Theorem 4.2].

Theorem 3.5.

The maximal positive pole of EψQ1(g,fs)E_{\psi}^{Q_{1}}(g,f_{s}) is of the form

(3.2) s={12(dimX+1(2j+ϵχ)),if 𝐆(X)=U(X);12(dimX2j),if 𝐆(X)=O(X);12(dimX+22j),if 𝐆(X)=Sp(X);12(dimX+2(2j+1)),if 𝐆(X)=Mp(X)s=\begin{cases}\frac{1}{2}(\dim X+1-(2j+\epsilon_{\chi})),&\quad\text{if $\mathbf{G}(X)=\operatorname{\mathrm{U}}(X)$};\\ \frac{1}{2}(\dim X-2j),&\quad\text{if $\mathbf{G}(X)=\mathrm{O}(X)$};\\ \frac{1}{2}(\dim X+2-2j),&\quad\text{if $\mathbf{G}(X)=\operatorname{\mathrm{Sp}}(X)$};\\ \frac{1}{2}(\dim X+2-(2j+1)),&\quad\text{if $\mathbf{G}(X)=\operatorname{\mathrm{Mp}}(X)$}\end{cases}

where jj\in\mathbb{Z} such that

(3.3) {rX2j+ϵχ<dimX+1,if 𝐆(X)=U(X);rX2j<dimX,if 𝐆(X)=O(X);rX2j<dimX+2,if 𝐆(X)=Sp(X);rX2j+1<dimX+2,if 𝐆(X)=Mp(X)\begin{cases}r_{X}\leq 2j+\epsilon_{\chi}<\dim X+1,&\quad\text{if $\mathbf{G}(X)=\operatorname{\mathrm{U}}(X)$};\\ r_{X}\leq 2j<\dim X,&\quad\text{if $\mathbf{G}(X)=\mathrm{O}(X)$};\\ r_{X}\leq 2j<\dim X+2,&\quad\text{if $\mathbf{G}(X)=\operatorname{\mathrm{Sp}}(X)$};\\ r_{X}\leq 2j+1<\dim X+2,&\quad\text{if $\mathbf{G}(X)=\operatorname{\mathrm{Mp}}(X)$}\end{cases}

where rXr_{X} denotes the Witt index of XX.

Remark 3.6.

The middle quantities in the inequalities of (3.3) are, in fact, the lowest occurrence index of π\pi in the global theta lift which depends on χ\chi and ψ\psi. (See Theorem 4.4.) In some cases, the lowest occurrence index turns out to be independent of ψ\psi.

Remark 3.7.

To derive the inequalities rXr_{X}\leq..., we already need to make use of properties of the global theta correspondence. The other parts of the statements can be derived by relating our Eisenstein series to Siegel Eisenstein series whose poles are completely known. We note that via the Siegel–Weil formula, Siegel Eisenstein series are related to global theta correspondence.

4. Theta correspondence

We keep the notation of Section 3. First we define the theta lifts and the two invariants called the first occurrence index and the lowest occurrence index. Then we relate the invariants to poles of our Eisenstein series.

Recall that we have taken an ϵ\epsilon-skew Hermitian space XX over EE. Let YY be an ϵ\epsilon-Hermitian space equipped with the form ,Y\langle{\ },{\ }\rangle_{Y}. We note that ,Y\langle{\ },{\ }\rangle_{Y} is an FF-bilinear pairing

,Y:Y×YE\displaystyle\langle{\ },{\ }\rangle_{Y}:Y\times Y\rightarrow E

such that

y2,y1Y=ϵy1,y2Yϱ,y1a,y2bY=aϱy1,y2Yb\langle{y_{2}},{y_{1}}\rangle_{Y}=\epsilon\langle{y_{1}},{y_{2}}\rangle_{Y}^{\varrho},\quad\langle{y_{1}a},{y_{2}b}\rangle_{Y}=a^{\varrho}\langle{y_{1}},{y_{2}}\rangle_{Y}b

for all a,bEa,b\in E and y1,y2Yy_{1},y_{2}\in Y. Let G(Y)G(Y) be its isometry group. We note that G(X)G(X) acts on XX from the right while G(Y)G(Y) acts on YY from the left. Let WW be the vector space RE/F(YEX)\operatorname{\mathrm{R}}_{E/F}(Y\otimes_{E}X) over FF and equip it with the symplectic form

,W:W×WF\displaystyle\langle{\ },{\ }\rangle_{W}:W\times W\rightarrow F

given by

y1x1,y2x2W=trE/F(y1,y2Yx1,x2Xϱ).\displaystyle\langle{y_{1}\otimes x_{1}},{y_{2}\otimes x_{2}}\rangle_{W}=\operatorname{\mathrm{tr}}_{E/F}(\langle{y_{1}},{y_{2}}\rangle_{Y}\langle{x_{1}},{x_{2}}\rangle_{X}^{\varrho}).

With this set-up, G(X)G(X) and G(Y)G(Y) form a reductive dual pair inside Sp(W)\operatorname{\mathrm{Sp}}(W). Let W=W+WW=W^{+}\oplus W^{-} be a polarisation of WW. Let Mp1(W)(Fv)\operatorname{\mathrm{Mp}}^{\mathbb{C}^{1}}(W)(F_{v}) be the 1\mathbb{C}^{1}-metaplectic extension of Sp(W)(Fv)\operatorname{\mathrm{Sp}}(W)(F_{v}). Let ωv\omega_{v} denote the Weil representation of Mp1(W)(Fv)\operatorname{\mathrm{Mp}}^{\mathbb{C}^{1}}(W)(F_{v}) realised on the space of Schwartz functions 𝒮(W+(Fv))\mathcal{S}(W^{+}(F_{v})). The Weil representation depends on the additive character ψv\psi_{v}, but we suppress it from notation. When vv is archimedean, we actually take the Fock model [15] rather than the full Schwartz space and it is a (𝔰𝔭(W)(Fv),K~Sp(W),v)(\mathfrak{sp}(W)(F_{v}),\widetilde{K}_{\operatorname{\mathrm{Sp}}(W),v})-module but we abuse language and call it a representation of Mp1(W)(Fv)\operatorname{\mathrm{Mp}}^{\mathbb{C}^{1}}(W)(F_{v}). When neither G(X)G(X) or G(Y)G(Y) is an odd orthogonal group, by [29] there exists a homomorphism

G(X)(Fv)×G(Y)(Fv)Mp1(W)(Fv)G(X)(F_{v})\times G(Y)(F_{v})\rightarrow\operatorname{\mathrm{Mp}}^{\mathbb{C}^{1}}(W)(F_{v})

that lifts the obvious map G(X)(Fv)×G(Y)(Fv)Sp(W)(Fv)G(X)(F_{v})\times G(Y)(F_{v})\rightarrow\operatorname{\mathrm{Sp}}(W)(F_{v}). In this case, set 𝐆(X)=G(X)\mathbf{G}(X)=G(X) (resp. 𝐆(Y)=G(Y)\mathbf{G}(Y)=G(Y)). When G(X)G(X) is an odd orthogonal group, we take 𝐆(Y)(Fv)\mathbf{G}(Y)(F_{v}) to be the metaplectic double cover of G(Y)(Fv)G(Y)(F_{v}) and set 𝐆(X)=G(X)\mathbf{G}(X)=G(X). Then by [29] there exists a homomorphism

G(X)(Fv)×𝐆(Y)(Fv)Mp1(W)(Fv)G(X)(F_{v})\times\mathbf{G}(Y)(F_{v})\rightarrow\operatorname{\mathrm{Mp}}^{\mathbb{C}^{1}}(W)(F_{v})

that lifts G(X)(Fv)×G(Y)(Fv)Sp(W)(Fv)G(X)(F_{v})\times G(Y)(F_{v})\rightarrow\operatorname{\mathrm{Sp}}(W)(F_{v}). The case is analogous when G(Y)G(Y) is an odd orthogonal group. In any case, we get a homomorphism

ιv:𝐆(X)(Fv)×𝐆(Y)(Fv)Mp1(Fv).\iota_{v}:\mathbf{G}(X)(F_{v})\times\mathbf{G}(Y)(F_{v})\rightarrow\operatorname{\mathrm{Mp}}^{\mathbb{C}^{1}}(F_{v}).

It should be clear from the context when 𝐆(X)\mathbf{G}(X) (resp. 𝐆(Y)\mathbf{G}(Y)) refers to a cover group and when it is not truly a cover. In the unitary case, there are many choices of ιv\iota_{v}. Once we fix χ\chi and an additional character χ2\chi_{2}, then ιv\iota_{v} is fixed. This is worked out in great details in [14, Section 1]. Our (χ,χ2)(\chi,\chi_{2}) matches (χ1,χ2)(\chi_{1},\chi_{2}) in [14, (0.2)]. We note that YY should be compatible with χ\chi and χ\chi determines the embedding of G(X)(𝔸)G(X)(\mathbb{A}) into Mp1(𝔸)\operatorname{\mathrm{Mp}}^{\mathbb{C}^{1}}(\mathbb{A}) whereas XX should be compatible with χ2\chi_{2} and χ2\chi_{2} determines the embedding of G(Y)(𝔸)G(Y)(\mathbb{A}) into Mp1(𝔸)\operatorname{\mathrm{Mp}}^{\mathbb{C}^{1}}(\mathbb{A}). By ‘compatible’, we mean ϵχdimY(mod2)\epsilon_{\chi}\equiv\dim Y\pmod{2} (resp. ϵχ2dimX(mod2)\epsilon_{\chi_{2}}\equiv\dim X\pmod{2}). See [29] for more details. We pull back ωv\omega_{v} to 𝐆(X)(Fv)×𝐆(Y)(Fv)\mathbf{G}(X)(F_{v})\times\mathbf{G}(Y)(F_{v}) via ιv\iota_{v} and still denote the representation by ωv\omega_{v}.

Denote by ι\iota the adelic analogue of ιv\iota_{v}. We also have the (global) Weil representation ω\omega of Mp1(𝔸)\operatorname{\mathrm{Mp}}^{\mathbb{C}^{1}}(\mathbb{A}) on the Schwartz space 𝒮(W+(𝔸))\mathcal{S}(W^{+}(\mathbb{A})) and its pullback via ι\iota to 𝐆(X)(𝔸)×𝐆(Y)(𝔸)\mathbf{G}(X)(\mathbb{A})\times\mathbf{G}(Y)(\mathbb{A}).

Then we can define the theta function which will be used as a kernel function. Let

θX,Y(g,h,Φ):=wW+(F)ω(ι(g,h))Φ(w)\theta_{X,Y}(g,h,\Phi):=\sum_{w\in W^{+}(F)}\omega(\iota(g,h))\Phi(w)

for g𝐆(X)(𝔸)g\in\mathbf{G}(X)(\mathbb{A}), h𝐆(Y)(𝔸)h\in\mathbf{G}(Y)(\mathbb{A}) and Φ𝒮(W+(𝔸))\Phi\in\mathcal{S}(W^{+}(\mathbb{A})). It is absolutely convergent and is an automorphic form on 𝐆(X)(𝔸)×𝐆(Y)(𝔸)\mathbf{G}(X)(\mathbb{A})\times\mathbf{G}(Y)(\mathbb{A}). For fπf\in\pi, set

θXY(f,Φ):=[𝐆(X)]f(g)¯θX,Y(g,h,Φ)𝑑g.\theta_{X}^{Y}(f,\Phi):=\int_{[\mathbf{G}(X)]}\overline{f(g)}\theta_{X,Y}(g,h,\Phi)dg.

Note that we write [𝐆(X)][\mathbf{G}(X)] for G(X)(F)\G(X)(𝔸)G(X)(F)\operatorname{\backslash}G(X)(\mathbb{A}) when 𝐆(X)\mathbf{G}(X) is not metaplectic and G(X)(F)\𝐆(X)(𝔸)G(X)(F)\operatorname{\backslash}\mathbf{G}(X)(\mathbb{A}) or more explicitly Sp(X)(F)\Mp(X)(𝔸)\operatorname{\mathrm{Sp}}(X)(F)\operatorname{\backslash}\operatorname{\mathrm{Mp}}(X)(\mathbb{A}) when 𝐆(X)\mathbf{G}(X) is metaplectic. This is an automorphic form on 𝐆(Y)(𝔸)\mathbf{G}(Y)(\mathbb{A}). It depends on χ\chi and χ2\chi_{2} in the unitary case and when we want to emphasise the dependency, we will write θX,χ2Y,χ(f,Φ)\theta_{X,\chi_{2}}^{Y,\chi}(f,\Phi). Let ΘXY(π)\Theta_{X}^{Y}(\pi) denote the space of functions spanned by θXY(f,Φ)\theta_{X}^{Y}(f,\Phi)’s and let ΘX,,χ2Y,χ(π)\Theta_{X,,\chi_{2}}^{Y,\chi}(\pi) denote the space of functions spanned by θX,χ2Y,χ(f,Φ)\theta_{X,\chi_{2}}^{Y,\chi}(f,\Phi)’s in the unitary case.

From now on assume that YY is anisotropic (possibly zero), so that it sits at the bottom of its Witt tower. Define YrY_{r} to be the ϵ\epsilon-Hermitian space formed by adjoining rr-copies of the hyperbolic plane to YY. These YrY_{r}’s form the Witt tower of YY. By the tower property [37, 44], if the theta lift to 𝐆(Yr)\mathbf{G}(Y_{r}) is non-zero then the theta lift to 𝐆(Yr)\mathbf{G}(Y_{r^{\prime}}) is also non-zero for all rrr^{\prime}\geq r.

Define the first occurrence index of π\pi in the Witt tower of YY to be

(4.1) FOXY,χ(π):={min{dimYr|ΘX,χ2Yr,χ(π)0},if 𝐆(X)=U(X);min{dimYr|ΘXYr(π(χυ))0},if 𝐆(X)=O(X);min{dimYr|ΘXYr(π)0},if 𝐆(X)=Sp(X) or Mp(X).\operatorname{\mathrm{FO}}_{X}^{Y,\chi}(\pi):=\begin{cases}\min\left\{\dim Y_{r}\middle|\Theta_{X,\chi_{2}}^{Y_{r},\chi}(\pi)\neq 0\right\},\quad&\text{if $\mathbf{G}(X)=\operatorname{\mathrm{U}}(X)$};\\ \min\left\{\dim Y_{r}\middle|\Theta_{X}^{Y_{r}}(\pi\otimes(\chi\circ\upsilon))\neq 0\right\},\quad&\text{if $\mathbf{G}(X)=\mathrm{O}(X)$};\\ \min\left\{\dim Y_{r}\middle|\Theta_{X}^{Y_{r}}(\pi)\neq 0\right\},\quad&\text{if $\mathbf{G}(X)=\operatorname{\mathrm{Sp}}(X)$ or $\operatorname{\mathrm{Mp}}(X)$}.\end{cases}

Note that it depends on χ\chi but not on χ2\chi_{2} in the unitary case as changing χ2\chi_{2} to another compatible one produces only a character twist on ΘX,χ2Yr,χ(π)\Theta_{X,\chi_{2}}^{Y_{r},\chi}(\pi). For more details, see [48, (1-1)]. In the orthogonal case, we twist π\pi by χυ\chi\circ\upsilon where υ\upsilon denotes the spinor norm. If 𝐆(X)=Sp(X)\mathbf{G}(X)=\operatorname{\mathrm{Sp}}(X) or Mp(X)\operatorname{\mathrm{Mp}}(X), we require that χY=χ\chi_{Y}=\chi where χY\chi_{Y} is the quadratic automorphic character of GL1(𝔸)\operatorname{\mathrm{GL}}_{1}(\mathbb{A}) associated to YY given by

χY(g)=(g,(1)dimY(dimY1)/2det,Y),\chi_{Y}(g)=(g,(-1)^{\dim Y(\dim Y-1)/2}\det\langle{\ },{\ }\rangle_{Y}),

where (,)(\ ,\ ) is the Hilbert symbol.

Define the lowest occurrence index to be

(4.2) LOXχ(π):=min{FOXY,χ(π)|Y is compatible with χ},\operatorname{\mathrm{LO}}_{X}^{\chi}(\pi):=\min\left\{\operatorname{\mathrm{FO}}_{X}^{Y,\chi}(\pi)\middle|\ \text{$Y$ is compatible with $\chi$}\right\},

when 𝐆(X)=U(X),Sp(X)\mathbf{G}(X)=\operatorname{\mathrm{U}}(X),\operatorname{\mathrm{Sp}}(X) or Mp(X)\operatorname{\mathrm{Mp}}(X). Here compatibility means that

dimYϵχ(mod2),\displaystyle\dim Y\equiv\epsilon_{\chi}\pmod{2}, if 𝐆(X)=U(X);\displaystyle\text{ if }\mathbf{G}(X)=\operatorname{\mathrm{U}}(X);
(4.3) χY=χ,\displaystyle\chi_{Y}=\chi, if 𝐆(X)=Sp(X) or Mp(X).\displaystyle\text{ if }\mathbf{G}(X)=\operatorname{\mathrm{Sp}}(X)\text{ or }\operatorname{\mathrm{Mp}}(X).

Define the lowest occurrence index to be

(4.4) LOXχ(π):=min{FOXY,χ(πsgnT)|T a set of even number of places of F},\operatorname{\mathrm{LO}}_{X}^{\chi}(\pi):=\min\left\{\operatorname{\mathrm{FO}}_{X}^{Y,\chi}(\pi\otimes\operatorname{\mathrm{sgn}}_{T})\middle|\ \text{$T$ a set of even number of places of $F$}\right\},

when 𝐆(X)=O(X)\mathbf{G}(X)=\mathrm{O}(X).

We have the following relations of the first occurrence (resp. the lowest occurrence) and the poles (resp. the maximal positive pole) of the Eisenstein series. See [23, Corollary 3.9, Theorem 3.10] for the symplectic case, [46, Corollary 6.3, Theorem 6.4] for the metaplectic case, [22, Corollary 3.5, Corollary 3.7] for the unitary case and [10, Theorem 5.1, Theorem 1.3] for the orthogonal case.

Theorem 4.1.

Let π\pi be an irreducible cuspidal automorphic representation of 𝐆(X)(𝔸)\mathbf{G}(X)(\mathbb{A}). Let χ\chi be a conjugate self-dual automorphic character of RE/FGL1(𝔸)\operatorname{\mathrm{R}}_{E/F}\operatorname{\mathrm{GL}}_{1}(\mathbb{A}). Let YY be an anisotropic ϵ\epsilon-Hermitian space that is compatible with χ\chi in the sense of (4.3). Assume that FOXY,χ(π)=dimY+2r\operatorname{\mathrm{FO}}_{X}^{Y,\chi}(\pi)=\dim Y+2r. Set

(4.5) s0={12(dimX+1(dimY+2r)),if 𝐆(X)=U(X);12(dimX(dimY+2r)),if 𝐆(X)=O(X);12(dimX+2(dimY+2r)),if 𝐆(X)=Sp(X) or Mp(X).s_{0}=\begin{cases}\frac{1}{2}(\dim X+1-(\dim Y+2r)),\quad&\text{if $\mathbf{G}(X)=\operatorname{\mathrm{U}}(X)$};\\ \frac{1}{2}(\dim X-(\dim Y+2r)),\quad&\text{if $\mathbf{G}(X)=\mathrm{O}(X)$};\\ \frac{1}{2}(\dim X+2-(\dim Y+2r)),\quad&\text{if $\mathbf{G}(X)=\operatorname{\mathrm{Sp}}(X)$ or $\operatorname{\mathrm{Mp}}(X)$}.\end{cases}

Assume that s00s_{0}\neq 0. If 𝐆(X)=O(X)\mathbf{G}(X)=\mathrm{O}(X) and s0<0s_{0}<0, further assume that 12dimX<r<dimX2\frac{1}{2}\dim X<r<\dim X-2. Then s=s0s=s_{0} is a pole of the Eisenstein series EψQ1(g,fs)E_{\psi}^{Q_{1}}(g,f_{s}) for some choice of fs𝒜ψQ1(s,χπ)f_{s}\in\mathcal{A}_{\psi}^{Q_{1}}(s,\chi\boxtimes\pi).

Remark 4.2.

Using the notation from Section 2. The quantity s0s_{0} in (4.5) can be written uniformly as

12(d𝐆(X)d𝐆(Yr)+1).\frac{1}{2}(d_{\mathbf{G}(X)^{\vee}}-d_{\mathbf{G}(Y_{r})^{\vee}}+1).
Remark 4.3.

Note that we always have rdimXr\leq\dim X. The extra condition when 𝐆(X)=O(X)\mathbf{G}(X)=\mathrm{O}(X) is to avoid treating period integrals over the orthogonal groups of split binary quadratic forms, as our methods cannot deal with the technicality. Theorem 4.1 allows negative s0s_{0}. It is possible to detect non-maximal poles and negative poles of the Eisenstein series by the first occurrence indices.

Theorem 4.4.

Let π\pi be an irreducible cuspidal automorphic representation of 𝐆(X)(𝔸)\mathbf{G}(X)(\mathbb{A}). Let χ\chi be a conjugate self-dual automorphic character of RE/FGL1(𝔸)\operatorname{\mathrm{R}}_{E/F}\operatorname{\mathrm{GL}}_{1}(\mathbb{A}). Then the maximal positive pole of EψQ1(g,fs)E_{\psi}^{Q_{1}}(g,f_{s}) for fsf_{s} running over 𝒜ψQ1(s,χπ)\mathcal{A}_{\psi}^{Q_{1}}(s,\chi\boxtimes\pi) is at s=s0s=s_{0}\in\mathbb{R} if and only if

(4.6) LOXχ(π)={dimX+12s0,if 𝐆(X)=U(X);dimX2s0,if 𝐆(X)=O(X);dimX+22s0,if 𝐆(X)=Sp(X) or Mp(X).\operatorname{\mathrm{LO}}_{X}^{\chi}(\pi)=\begin{cases}\dim X+1-2s_{0},\quad&\text{if $\mathbf{G}(X)=\operatorname{\mathrm{U}}(X)$};\\ \dim X-2s_{0},\quad&\text{if $\mathbf{G}(X)=\mathrm{O}(X)$};\\ \dim X+2-2s_{0},\quad&\text{if $\mathbf{G}(X)=\operatorname{\mathrm{Sp}}(X)$ or $\operatorname{\mathrm{Mp}}(X)$}.\end{cases}
Remark 4.5.

Theorem 4.4 does not allow negative s0s_{0}.

In Remark 3.7, we mentioned that the part rXr_{X}\leq... in Theorem 3.5 is proved by using theta correspondence. What we used is that we always have LOXχ(π)rX\operatorname{\mathrm{LO}}_{X}^{\chi}(\pi)\geq r_{X} by the stable range condition [37, Theorem I.2.1].

5. Application to Global Arthur Packets

We have derived relations among (χ,b)(\chi,b)-factors of global AA-parameters, poles of partial LL-functions, poles of Eisenstein series and lowest occurrence indices of global theta lifts. Combining these, we have the following implication on global AA-packets.

Theorem 5.1.

Let π\pi be an irreducible cuspidal automorphic representation of 𝐆(X)(𝔸)\mathbf{G}(X)(\mathbb{A}). Let ϕπ\phi_{\pi} be its global AA-parameter. Let χ\chi be a conjugate self-dual automorphic character of RE/FGL1(𝔸)\operatorname{\mathrm{R}}_{E/F}\operatorname{\mathrm{GL}}_{1}(\mathbb{A}). Assume that ϕπ\phi_{\pi} has a (χ,b)(\chi,b)-factor for some positive integer bb. Then

(5.1) b{dimXrX,if 𝐆(X)=U(X);dimXrX1,if 𝐆(X)=O(X);dimXrX+1=12dimX+1,if 𝐆(X)=Sp(X) or Mp(X).b\leq\begin{cases}\dim X-r_{X},&\quad\text{if $\mathbf{G}(X)=\operatorname{\mathrm{U}}(X)$};\\ \dim X-r_{X}-1,&\quad\text{if $\mathbf{G}(X)=\mathrm{O}(X)$};\\ \dim X-r_{X}+1=\frac{1}{2}\dim X+1,&\quad\text{if $\mathbf{G}(X)=\operatorname{\mathrm{Sp}}(X)$ or $\operatorname{\mathrm{Mp}}(X)$}.\end{cases}

where rXr_{X} denotes the Witt index of XX.

Proof.

If bb is not maximal among all factors (τ,b)(\tau,b) appearing in ϕπ\phi_{\pi}, then b<12d𝐆(X)b<\frac{1}{2}d_{\mathbf{G}(X)^{\vee}}. Then it is clear that bb satisfies (5.1). Now we assume that bb is maximal among all factors appearing in ϕπ\phi_{\pi}. By Prop. 2.8, LS(s,π×χ1)L^{S}(s,\pi\times\chi^{-1}) has its rightmost pole at s=12(b+1)s=\frac{1}{2}(b+1). Then by Prop. 3.1, EψQ1(g,fs)E_{\psi}^{Q_{1}}(g,f_{s}) has a pole at s=12(b+1)s=\frac{1}{2}(b+1) for some choice of fsf_{s}. Assume that s=12(b1+1)s=\frac{1}{2}(b_{1}+1) is the rightmost pole of the Eisenstein series with b1bb_{1}\geq b. By Thm. 3.5,

12(b1+1){12(dimX+1rX),if 𝐆(X)=U(X);12(dimXrX),if 𝐆(X)=O(X);12(dimX+2rX),if 𝐆(X)=Sp(X) or Mp(X).\frac{1}{2}(b_{1}+1)\leq\begin{cases}\frac{1}{2}(\dim X+1-r_{X}),&\quad\text{if $\mathbf{G}(X)=\operatorname{\mathrm{U}}(X)$};\\ \frac{1}{2}(\dim X-r_{X}),&\quad\text{if $\mathbf{G}(X)=\mathrm{O}(X)$};\\ \frac{1}{2}(\dim X+2-r_{X}),&\quad\text{if $\mathbf{G}(X)=\operatorname{\mathrm{Sp}}(X)$ or $\operatorname{\mathrm{Mp}}(X)$}.\end{cases}

or in other words, b1b_{1} is less than or equal to the quantity on the RHS of (5.1). Using the fact that bb1b\leq b_{1}, we get the desired bound for bb. ∎

Remark 5.2.

Our result generalises [18, Theorem 3.1] for symplectic groups to classical groups and metaplectic groups. In addition, we do not require the assumption on the wave front set in [18, Theorem 3.1]. This type of result has been used in [18, Section 5] to find a Ramanujan bound which measures the departure of the local components of a cuspidal π\pi from being tempered.

The metaplectic case has been treated in [47, Theorem 0.1], though the proof is not written down explicitly. Here we supply the detailed arguments for all classical groups and metaplectic groups uniformly.

The corollary below follows immediately from the theorem.

Corollary 5.3.

The global AA-packet Πϕ\Pi_{\phi} attached to the elliptic global AA-parameter ϕ\phi cannot have a cuspidal member if ϕ\phi has a (χ,b)(\chi,b)-factor with

b>{dimEXrX,if 𝐆(X)=U(X);dimFXrX1,if 𝐆(X)=O(X);dimXrX+1=12dimX+1,if 𝐆(X)=Sp(X) or Mp(X).b>\begin{cases}\dim_{E}X-r_{X},&\quad\text{if $\mathbf{G}(X)=\operatorname{\mathrm{U}}(X)$};\\ \dim_{F}X-r_{X}-1,&\quad\text{if $\mathbf{G}(X)=\mathrm{O}(X)$};\\ \dim X-r_{X}+1=\frac{1}{2}\dim X+1,&\quad\text{if $\mathbf{G}(X)=\operatorname{\mathrm{Sp}}(X)$ or $\operatorname{\mathrm{Mp}}(X)$}.\end{cases}

6. Generic Global AA-packets

Following the terminology of [2], we say that an elliptic global AA-parameter is generic if it is of the form ϕ=i=1r(τi,1)\phi=\boxplus_{i=1}^{r}(\tau_{i},1) and we say a global AA-packet is generic if its global AA-parameter is generic. Assume that π\pi is a cuspidal member in a generic global AA-packet. Then our results can be made more precise. We note that our results for Mp(X)\operatorname{\mathrm{Mp}}(X) are conditional on results on normalised intertwining operators. See Assumption 6.1 and Remark 6.2.

First assume that G(X)G(X) is quasi-split and that π\pi is globally generic. We explain what we mean by globally generic. We use the same set-up as in [40, Section 3]. Let BB be a Borel subgroup of G(X)G(X). Let NN denote its unipotent radical and let TT be a fixed choice of Levi subgroup of BB. Of course, in this case TT is a maximal torus of G(X)G(X). We require that TT is maximally split. Let F¯\bar{F} denote an algebraic closure of FF. Let Δ\Delta denote the set of simple roots of T(F¯)T(\bar{F}) in N(F¯)N(\bar{F}). Let {Xα}αΔ\{X_{\alpha}\}_{\alpha\in\Delta} be a Gal(F¯/F)\operatorname{\mathrm{Gal}}(\bar{F}/F)-invariant set of root vectors. Recall that ψ\psi is a fixed non-trivial automorphic character of 𝔸F\mathbb{A}_{F} which is used in the definitions of the Weil representation and the global AA-packets for Mp(X)\operatorname{\mathrm{Mp}}(X). It gives rise to generic characters of N(𝔸)N(\mathbb{A}). We use the one defined as follows. For each place vv of FF, we define a character ψN,v\psi_{N,v} of N(Fv)N(F_{v}). Write an element of N(Fv)N(F_{v}) as αΔexp(xαXα)\prod_{\alpha\in\Delta}\exp(x_{\alpha}X_{\alpha}) for xαF¯vx_{\alpha}\in\bar{F}_{v} such that σxα=xσα\sigma x_{\alpha}=x_{\sigma\alpha} with σGal(F¯/F)\sigma\in\operatorname{\mathrm{Gal}}(\bar{F}/F). Set

ψN,v(αΔexp(xαXα))=ψv(αΔxα).\displaystyle\psi_{N,v}(\prod_{\alpha\in\Delta}\exp(x_{\alpha}X_{\alpha}))=\psi_{v}(\sum_{\alpha\in\Delta}x_{\alpha}).

Let ψN=vψN,v\psi_{N}=\otimes_{v}\psi_{N,v}. In the Mp(X)\operatorname{\mathrm{Mp}}(X) case, we view N(𝔸)N(\mathbb{A}) as a subgroup of Mp(X)(𝔸)\operatorname{\mathrm{Mp}}(X)(\mathbb{A}) via the canonical splitting. We require that π\pi is globally generic with respect to the generic character ψN\psi_{N} of N(𝔸)N(\mathbb{A}). Thus the notion of global genericity depends on the choice of the generic automorphic character of N(𝔸)N(\mathbb{A}). However by [4, Appendix A], the choice has no effect on the LL-factors, the ε\varepsilon-factors and the global AA-parameter for π\pi in the case of 𝐆(X)=Sp(X),O(X),U(X)\mathbf{G}(X)=\operatorname{\mathrm{Sp}}(X),\mathrm{O}(X),\operatorname{\mathrm{U}}(X). The case of Mp(X)\operatorname{\mathrm{Mp}}(X) is highly dependent on the choice.

When π\pi is globally generic, b=1b=1 for every factor (τ,b)(\tau,b) in the global AA-parameter ϕπ\phi_{\pi}. This is because the Langlands functorial lift of π\pi is an isobaric sum of conjugate self-dual cuspidal representations of some RE/FGLn(𝔸)\operatorname{\mathrm{R}_{E/F}\operatorname{\mathrm{GL}}}_{n}(\mathbb{A}). See Theorem 11.2 of [13].

By [19], there is a more precise relation on the poles of LL-functions and the poles of Eisenstein series. The set of possible poles of the normalised Eisenstein series is determined by the complete LL-function L(s,π×χ)L(s,\pi\times\chi^{\vee}). From the assumption that π\pi is globally generic, in the right half plane, L(s,π×χ)L(s,\pi\times\chi^{\vee}) has at most a simple pole at s=1s=1. In fact we only need [19, Proposition 4.1] rather than the full strength of [19, Theorem 1.2] which allows the induction datum to be a Speh representation on the general linear group factor of the Levi. By [24, Theorem 5.1], [19, Proposition 4.1] can be strengthened to include the case where π\pi is a cuspidal member in a generic global AA-packet of 𝐆(X)(𝔸)\mathbf{G}(X)(\mathbb{A}) where 𝐆(X)=Sp(X),O(X),U(X)\mathbf{G}(X)=\operatorname{\mathrm{Sp}}(X),\mathrm{O}(X),\operatorname{\mathrm{U}}(X) does not have to be quasi-split. We rephrase [19, Proposition 4.1] in our context as Theorem 6.3.

First we set up some notation and outline the method for extending [19, Proposition 4.1] to the case of Mp(X)\operatorname{\mathrm{Mp}}(X). Let

(6.1) ρ+:={Asaiη, where η=(1)dimX+1,if 𝐆(X)=U(X),2,if 𝐆(X)=O(X) with dimX odd or if 𝐆(X)=Mp(X);Sym2,if 𝐆(X)=O(X) with dimX even or if 𝐆(X)=Sp(X)\rho^{+}:=\begin{cases}\mathrm{Asai}^{\eta}\text{, where $\eta=(-1)^{\dim X+1}$},\quad&\begin{array}[]{l}\text{if $\mathbf{G}(X)=\operatorname{\mathrm{U}}(X)$,}\end{array}\\ \wedge^{2},\quad&\begin{array}[]{l}\text{if $\mathbf{G}(X)=\mathrm{O}(X)$ with $\dim X$ odd}\\ \text{ or if $\mathbf{G}(X)=\operatorname{\mathrm{Mp}}(X)$};\end{array}\\ \operatorname{\mathrm{Sym}}^{2},\quad&\begin{array}[]{l}\text{if $\mathbf{G}(X)=\mathrm{O}(X)$ with $\dim X$ even}\\ \text{ or if $\mathbf{G}(X)=\operatorname{\mathrm{Sp}}(X)$}\end{array}\end{cases}

and

(6.2) ρ:={Asaiη, where η=(1)dimX+1,if 𝐆(X)=U(X),Sym2,if 𝐆(X)=O(X) with dimX odd or if 𝐆(X)=Mp(X);2,if 𝐆(X)=O(X) with dimX even or if 𝐆(X)=Sp(X).\rho^{-}:=\begin{cases}\mathrm{Asai}^{-\eta}\text{, where $\eta=(-1)^{\dim X+1}$},\quad&\begin{array}[]{l}\text{if $\mathbf{G}(X)=\operatorname{\mathrm{U}}(X)$,}\end{array}\\ \operatorname{\mathrm{Sym}}^{2},\quad&\begin{array}[]{l}\text{if $\mathbf{G}(X)=\mathrm{O}(X)$ with $\dim X$ odd}\\ \text{ or if $\mathbf{G}(X)=\operatorname{\mathrm{Mp}}(X)$};\end{array}\\ \wedge^{2},\quad&\begin{array}[]{l}\text{if $\mathbf{G}(X)=\mathrm{O}(X)$ with $\dim X$ even}\\ \text{ or if $\mathbf{G}(X)=\operatorname{\mathrm{Sp}}(X)$}.\end{array}\end{cases}

The results of [19] do not cover the metaplectic case, but the method should generalise without difficulty. We explain the strategy. First the poles of the Eisenstein series are related to those of the intertwining operators

M(w0,τ||sπ):IndQa(𝔸)𝐆(Xa)(𝔸)(τ||sπ)IndQa(𝔸)𝐆(X1)(𝔸)(τ||sπ)M(w_{0},\tau|\ |^{s}\boxtimes\pi):\operatorname{\mathrm{Ind}}_{Q_{a}(\mathbb{A})}^{\mathbf{G}(X_{a})(\mathbb{A})}(\tau|\ |^{s}\boxtimes\pi)\rightarrow\operatorname{\mathrm{Ind}}_{Q_{a}(\mathbb{A})}^{\mathbf{G}(X_{1})(\mathbb{A})}(\tau|\ |^{-s}\boxtimes\pi)

where τ\tau is a conjugate self-dual cuspidal automorphic representation of GLa(𝔸E)\operatorname{\mathrm{GL}}_{a}(\mathbb{A}_{E}) and w0w_{0} is the longest Weyl element in Qa\G(Xa)/QaQ_{a}\operatorname{\backslash}G(X_{a})/Q_{a}. Then define the normalised intertwining operator

N(w0,τ||sπ):=\displaystyle N(w_{0},\tau|\ |^{s}\boxtimes\pi):= L(s,π×τ)L(2s,τ,ρ)L(s+1,π×τ)L(2s+1,τ,ρ)ε(s,π×τ)ε(2s,τ,ρ)\displaystyle\frac{L(s,\pi\times\tau^{\vee})L(2s,\tau,\rho^{-})}{L(s+1,\pi\times\tau^{\vee})L(2s+1,\tau,\rho^{-})\varepsilon(s,\pi\times\tau^{\vee})\varepsilon(2s,\tau,\rho^{-})}
(6.3) M(w0,τ||sπ).\displaystyle\quad\cdot M(w_{0},\tau|\ |^{s}\boxtimes\pi).

The proof of [19, Proposition 4.1] relies on the key result that the normalised intertwining operator is holomorphic and non-zero for Res12\operatorname{\mathrm{Re}}s\geq\frac{1}{2}. Then it boils down to finding the poles of the normalising factors or equivalently

L(s,π×τ)L(2s,τ,ρ)L(s+1,π×τ)L(2s+1,τ,ρ).\displaystyle\frac{L(s,\pi\times\tau^{\vee})L(2s,\tau,\rho^{-})}{L(s+1,\pi\times\tau^{\vee})L(2s+1,\tau,\rho^{-})}.

Once we have the key result available, we expect to have a version of [19, Proposition 4.1] for the metaplectic groups. Note that our ρ±\rho^{\pm} defined in (6.1) and (6.2) is different from the ρ\rho and ρ\rho^{-} in [19].

Then by using an inductive formula, we expect to be able to prove [19, Theorem 1.2] as well. We hope to supply the details in a future work.

Next we allow G(X)G(X) to be non-quasi-split. We assume that π\pi is a cuspidal member in a generic global AA-packet of 𝐆(X)\mathbf{G}(X). Then by [24, Theorem 5.1], (6) is holomorphic and non-zero for Res12\operatorname{\mathrm{Re}}s\geq\frac{1}{2} when 𝐆(X)=Sp(X),O(X),U(X)\mathbf{G}(X)=\operatorname{\mathrm{Sp}}(X),\mathrm{O}(X),\operatorname{\mathrm{U}}(X). Then the proof of [19, Proposition 4.1] goes through verbatim for such π\pi. The proof of [24, Theorem 5.1] does not generalise readily to the case of Mp(X)\operatorname{\mathrm{Mp}}(X) as the relevant results for Mp(X)\operatorname{\mathrm{Mp}}(X) are not available.

Thus we make an assumption on the normalised intertwining operator:

Assumption 6.1.

The normalised intertwining operator N(w0,χ||sπ)N(w_{0},\chi|\ |^{s}\boxtimes\pi) is holomorphic and non-zero for Res12\operatorname{\mathrm{Re}}s\geq\frac{1}{2}.

Remark 6.2.

This is shown to be true by [24, Theorem 5.1] when π\pi is a cuspidal member in a generic global AA-packet of 𝐆(X)(𝔸)\mathbf{G}(X)(\mathbb{A}) for 𝐆(X)=Sp(X),O(X),U(X)\mathbf{G}(X)=\operatorname{\mathrm{Sp}}(X),\mathrm{O}(X),\operatorname{\mathrm{U}}(X). Thus this is only a condition when 𝐆(X)=Mp(X)\mathbf{G}(X)=\operatorname{\mathrm{Mp}}(X).

Theorem 6.3.

Assume Assumption 6.1. Let π\pi be a cuspidal member in a generic global AA-packet of 𝐆(X)(𝔸)\mathbf{G}(X)(\mathbb{A}). Let χ\chi be a conjugate self-dual automorphic character of RE/FGL1(𝔸)\operatorname{\mathrm{R}}_{E/F}\operatorname{\mathrm{GL}}_{1}(\mathbb{A}).

  1. (1)

    Assume 𝐆(X)=U(X)\mathbf{G}(X)=\operatorname{\mathrm{U}}(X) with ϵχdimX(mod2)\epsilon_{\chi}\not\equiv\dim X\pmod{2}, O(X)\mathrm{O}(X) with dimX\dim X even or Sp(X)\operatorname{\mathrm{Sp}}(X). Then L(s,π×χ)L(s,\pi\times\chi^{\vee}) has a pole at s=1s=1 if and only if EQ1(g,fs)E^{Q_{1}}(g,f_{s}) has a pole at s=1s=1 and it is its maximal pole.

  2. (2)

    Assume 𝐆(X)=U(X)\mathbf{G}(X)=\operatorname{\mathrm{U}}(X) with ϵχdimX(mod2)\epsilon_{\chi}\equiv\dim X\pmod{2}, O(X)\mathrm{O}(X) with dimX\dim X odd or Mp(X)\operatorname{\mathrm{Mp}}(X). Then L(s,π×χ)L(s,\pi\times\chi^{\vee}) is non-vanishing at s=12s=\frac{1}{2} if and only if EψQ1(g,fs)E_{\psi}^{Q_{1}}(g,f_{s}) has a pole at s=12s=\frac{1}{2} and it is its maximal pole.

Remark 6.4.

The result of [19] involves normalised Eisenstein series, but the normalisation has no impact on the positive poles. The following remarks use the notation in [19]. We only need the case b=1b=1 in [19] which is Proposition 4.1 there. Furthermore we only apply it in the case where τ\tau is a character. The condition that L(s,τ,ρ)L(s,\tau,\rho) has a pole at s=1s=1 is automatically satisfied by the requirement on our χ\chi that it is conjugate self-dual of parity (1)N𝐆(X)+1(-1)^{N_{\mathbf{G}(X)^{\vee}}+1}. See Section 2, especially Remark 2.3.

The global AA-parameter ϕπ\phi_{\pi} can possibly have a (χ,1)(\chi,1)-factor only when χ\chi satisfies the condition that L(s,χ,ρ+)L(s,\chi,\rho^{+}) has a pole at s=1s=1. Due to the parity condition on factors of an elliptic global AA-parameter, in some cases, ϕπ\phi_{\pi} cannot have a (χ,1)(\chi,1)-factor.

Combining with our result (Theorem 4.4) on poles of Eisenstein series and lowest occurrence indices with Theorem 6.3 which gives a precise relation between poles of the complete LL-function and those of the Eisenstein series, we get

Theorem 6.5.

Assume Assumption 6.1. Let π\pi be a cuspidal member in a generic global AA-packet of 𝐆(X)(𝔸)\mathbf{G}(X)(\mathbb{A}). Let χ\chi be a conjugate self-dual automorphic character of RE/FGL1(𝔸)\operatorname{\mathrm{R}}_{E/F}\operatorname{\mathrm{GL}}_{1}(\mathbb{A}). In each of the following statements, we consider only those 𝐆(X)\mathbf{G}(X)’s that are listed.

  1. (1)

    Assume that L(s,π×χ)L(s,\pi\times\chi^{\vee}) has a pole at s=1s=1. Then

    LOXχ(π)={dimX1,if 𝐆(X)=U(X) and ϵχdimX(mod2);dimX2,if 𝐆(X)=O(X) with dimX even;dimX,if 𝐆(X)=Sp(X).\operatorname{\mathrm{LO}}_{X}^{\chi}(\pi)=\begin{cases}\dim X-1,\quad&\text{if $\mathbf{G}(X)=\operatorname{\mathrm{U}}(X)$ and $\epsilon_{\chi}\not\equiv\dim X\pmod{2}$};\\ \dim X-2,\quad&\text{if $\mathbf{G}(X)=\mathrm{O}(X)$ with $\dim X$ even};\\ \dim X,\quad&\text{if $\mathbf{G}(X)=\operatorname{\mathrm{Sp}}(X)$}.\end{cases}
  2. (2)

    Assume that L(s,π×χ)L(s,\pi\times\chi^{\vee}) does not have a pole at s=1s=1. Then

    LOXχ(π){dimX+1,if 𝐆(X)=U(X) and ϵχdimX(mod2);dimX,if 𝐆(X)=O(X) with dimX even;dimX+2,if 𝐆(X)=Sp(X).\operatorname{\mathrm{LO}}_{X}^{\chi}(\pi)\geq\begin{cases}\dim X+1,\quad&\text{if $\mathbf{G}(X)=\operatorname{\mathrm{U}}(X)$ and $\epsilon_{\chi}\not\equiv\dim X\pmod{2}$};\\ \dim X,\quad&\text{if $\mathbf{G}(X)=\mathrm{O}(X)$ with $\dim X$ even};\\ \dim X+2,\quad&\text{if $\mathbf{G}(X)=\operatorname{\mathrm{Sp}}(X)$}.\end{cases}
  3. (3)

    Assume L(12,π×χ)0L(\frac{1}{2},\pi\times\chi^{\vee})\neq 0. Then

    LOXχ(π)={dimX,if 𝐆(X)=U(X) and ϵχdimX(mod2);dimX1,if 𝐆(X)=O(X) with dimX odd;dimX+1,if 𝐆(X)=Mp(X).\operatorname{\mathrm{LO}}_{X}^{\chi}(\pi)=\begin{cases}\dim X,\quad&\text{if $\mathbf{G}(X)=\operatorname{\mathrm{U}}(X)$ and $\epsilon_{\chi}\equiv\dim X\pmod{2}$};\\ \dim X-1,\quad&\text{if $\mathbf{G}(X)=\mathrm{O}(X)$ with $\dim X$ odd};\\ \dim X+1,\quad&\text{if $\mathbf{G}(X)=\operatorname{\mathrm{Mp}}(X)$}.\end{cases}
  4. (4)

    Assume L(12,π×χ)=0L(\frac{1}{2},\pi\times\chi^{\vee})=0. Then

    LOXχ(π){dimX+2,if 𝐆(X)=U(X) and ϵχdimX(mod2);dimX+1,if 𝐆(X)=O(X) with dimX odd;dimX+3,if 𝐆(X)=Mp(X).\operatorname{\mathrm{LO}}_{X}^{\chi}(\pi)\geq\begin{cases}\dim X+2,\quad&\text{if $\mathbf{G}(X)=\operatorname{\mathrm{U}}(X)$ and $\epsilon_{\chi}\equiv\dim X\pmod{2}$};\\ \dim X+1,\quad&\text{if $\mathbf{G}(X)=\mathrm{O}(X)$ with $\dim X$ odd};\\ \dim X+3,\quad&\text{if $\mathbf{G}(X)=\operatorname{\mathrm{Mp}}(X)$}.\end{cases}
Remark 6.6.

By the conservation relation for local theta correspondence [42], there always exists an ϵ\epsilon-Hermitian space Z[v]Z_{[v]} over EvE_{v} of dimension given by the RHS of the equalities in items (1), (3) such that the local theta lift of πv\pi_{v} to 𝐆(Z[v])\mathbf{G}(Z_{[v]}) is non-vanishing. Thus in the case of items (2), (4) and 𝐆(X)O(X)\mathbf{G}(X)\neq\mathrm{O}(X), the collection {Z[v]}v\{Z_{[v]}\}_{v} for vv running over all places of FF is always incoherent, i.e., there does not exist an ϵ\epsilon-Hermitian space ZZ over EE such that the localisation ZvZ_{v} is isomorphic to Z[v]Z_{[v]} for all vv. In the case of items (2), (4) and 𝐆(X)=O(X)\mathbf{G}(X)=\mathrm{O}(X), we have a non-trivial theta lift of πv(χvυv)(η[v]det)\pi_{v}\otimes(\chi_{v}\circ\upsilon_{v})\otimes(\eta_{[v]}\circ\det) to 𝐆(Z[v])\mathbf{G}(Z_{[v]}) for η[v]\eta_{[v]} being the trivial character or the sign character for each place vv of FF, but the collection {η[v]}v\{\eta_{[v]}\}_{v} is incoherent, i.e., there does not exist an automorphic character η\eta of 𝔸F×\mathbb{A}_{F}^{\times} such that the localisation ηv\eta_{v} is equal to η[v]\eta_{[v]} for all vv. See the definitions of first occurrence (4.1) and lowest occurrence (4.4) for O(X)\mathrm{O}(X) for why we have a (χvυv)(\chi_{v}\circ\upsilon_{v})-twist. We also note that when π\pi is an irreducible cuspidal automorphic representation and L(12,π×χ)=0L(\frac{1}{2},\pi\times\chi^{\vee})=0, it is conjectured that there is an arithmetic version of the Rallis inner product formula which says that the conjectural Beilinson–Bloch height pairing of arithmetic theta lifts (which are cycles on Shimura varieties constructed from an incoherent collection of ϵ\epsilon-Hermitian spaces) gives the derivative L(12,π×χ)L^{\prime}(\frac{1}{2},\pi\times\chi^{\vee}) up to some ramified factors and some abelian LL-functions. The low rank cases have been proved in [28] and [30, 31]. More recently, the cases of unitary groups of higher rank have been proved in [32] and [33], conditional on hypothesis of the modularity of Kudla’s generating functions of special cycles.

In terms of ‘(χ,b)(\chi,b)’-factors, we have

Theorem 6.7.

Let 𝐆(X)=U(X)\mathbf{G}(X)=\operatorname{\mathrm{U}}(X) with ϵχdimX(mod2)\epsilon_{\chi}\not\equiv\dim X\pmod{2}, 𝐆(X)=O(X)\mathbf{G}(X)=\mathrm{O}(X) with dimX\dim X even or 𝐆(X)=Sp(X)\mathbf{G}(X)=\operatorname{\mathrm{Sp}}(X). Let π\pi be a cuspidal member in a generic global AA-packet of 𝐆(X)(𝔸)\mathbf{G}(X)(\mathbb{A}). Let χ\chi be a conjugate self-dual automorphic character of RE/FGL1(𝔸)\operatorname{\mathrm{R}}_{E/F}\operatorname{\mathrm{GL}}_{1}(\mathbb{A}). Then the following are equivalent.

  1. (1)

    The global AA-parameter ϕ\phi of π\pi has a (χ,1)(\chi,1)-factor.

  2. (2)

    The complete LL-function L(s,π×χ)L(s,\pi\times\chi^{\vee}) has a pole at s=1s=1 (and this is its maximal pole).

  3. (3)

    The Eisenstein series EQ1(g,fs)E^{Q_{1}}(g,f_{s}) has a pole at s=1s=1 for some choice of fs𝒜Q1(s,χπ)f_{s}\in\mathcal{A}^{Q_{1}}(s,\chi\boxtimes\pi) (and this is its maximal pole).

  4. (4)

    The lowest occurrence index LOXχ(π)\operatorname{\mathrm{LO}}_{X}^{\chi}(\pi) is

    {dimX1,if 𝐆(X)=U(X);dimX2,if 𝐆(X)=O(X);dimX,if 𝐆(X)=Sp(X).\begin{cases}\dim X-1,\quad&\text{if $\mathbf{G}(X)=\operatorname{\mathrm{U}}(X)$};\\ \dim X-2,\quad&\text{if $\mathbf{G}(X)=\mathrm{O}(X)$};\\ \dim X,\quad&\text{if $\mathbf{G}(X)=\operatorname{\mathrm{Sp}}(X)$}.\end{cases}
Remark 6.8.

The statements that the poles are maximal are automatic since π\pi lies in a generic global AA-packet. We note that when 𝐆(X)=U(X)\mathbf{G}(X)=\operatorname{\mathrm{U}}(X) with ϵχdimX(mod2)\epsilon_{\chi}\equiv\dim X\pmod{2}, 𝐆(X)=O(X)\mathbf{G}(X)=\mathrm{O}(X) with dimX\dim X odd or 𝐆(X)=Mp(X)\mathbf{G}(X)=\operatorname{\mathrm{Mp}}(X), ϕπ\phi_{\pi} cannot have a (χ,1)(\chi,1)-factor as the parity condition is not satisfied.

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