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Theta correspondence and Arthur packets

Rui Chen and Jialiang Zou
Abstract.

In spirit of [GI18], we have established an Arthur’s multiplicity formula for even orthogonal or unitary groups with Witt index less than or equal to one. In that multiplicity formula, some local packets defined using the stable range theta lifts are involved. In this paper, we prove that at non-Archimedean places, the definition of the local packets involved in that multiplicity formula is independent of the choice of the dual-pairs used in their construction. Moreover, at those places where the groups are quasi-split, we prove that the local packets involved are the same as the local AA-packets defined by Arthur/ Mok.

1. Introduction

In this section we briefly explain our main motivation.

Let FF be a number field, 𝔸\mathbb{A} be the Adele ring of FF, and GG be a reductive group over FF. A central question in representation theory is to study the unitary representation L2(G(F)\G(𝔸))L^{2}(G(F)\backslash G(\mathbb{A})). By some classical works, this question is reduced to study the “discrete part” of L2(G(F)\G(𝔸))L^{2}(G(F)\backslash G(\mathbb{A})), which is usually denoted by Ldisc2(G)L_{disc}^{2}(G). When GG is a quasi-split classical group, this question is already very well-studied by Arthur [Art13] and Mok [Mok15]. Basically, they decomposed Ldisc2(G)L_{disc}^{2}(G) into some summands called “near equivalence classes”, and describe each of these summands using the so called “Arthur’s multiplicity formula”. For non quasi-split groups, Arthur has proposed some strategies to attack this question using the trace formula. For the case of inner forms of unitary groups, Kaletha-Mínguez-Shin-White have established some partial results in [KMSW14]. Also, for the case of certain inner forms of classical groups, Taïbi has proved the Arthur’s multiplicity formula for the near equivalence classes satisfying some conditions in [Taï19]. However, except these works, it seems that the general results for non quasi-split groups are not known.

On the other hand, the theta correspondence has provided a tool to “transfer” results between dual-pairs. In particular, one may “transfer” results for a quasi-split group to a possibly non quasi-split group using the theta correspondence. This idea has been used in many papers. In our previous paper [CZ21], we have established some results for non quasi-split even orthogonal or unitary groups. Now we briefly recall them.

1.1. Weak lift, multiplicity preservation and a multiplicity formula

We continue to let FF be a number field. Let (G,H)(G,H) be a reductive dual pair over FF in stable range and HH is the larger group, that is, the split rank of HH is greater than the dimension of the standard representation of GG (we shall make it more precisely later). In some early works of Howe [How82] and J-S. Li [Li97], they defined the so-called “low rank representations” of classical groups, and showed that theses representations can be characterized by the theta lift from some smaller groups. These works suggest the possibility to study the automorphic spectrum of GG in terms of HH, using the theta correspondence between (G,H)(G,H). This idea was first exploited by Gan-Ichino [GI18]. In their work, they put G=Mp(2n)G=Mp(2n), and H=SO(2r+1)H=SO(2r+1), such that r>2nr>2n. By computing some unramified theta lifts and partial LL-functions, they attached to each near equivalence class of GG an elliptic AA-parameter (i.e. showed the existence of the weak lift to GL(2n)GL(2n) through the standard representation of the dual group); they also observed that, for those automorphic representations π\pi of GG with tempered elliptic AA-parameters, any automorphic realization of π\pi must be cuspidal, which implies that

(1.1) mdisc(π)=mdisc(θabs(π)),m_{disc}(\pi)=m_{disc}\left(\theta^{abs}(\pi)\right),

where mdiscm_{disc} means the multiplicity in the automorphic discrete spectrum, and θabs(π)\theta^{abs}(\pi) means the abstract theta lift of π\pi to HH (i.e. restricted tensor product of the local theta lift at each local place). Combining this with some knowledge on the local theta lift, they proved the Arthur’s multiplicity formula for the tempered part of the automorphic discrete spectrum of Mp(2n)Mp(2n).

In our previous paper [CZ21], we put GG to be an even orthogonal or unitary group (not necessarily quasi-split), and HH be a symplectic or quasi-split unitary group according to GG. We established the same results as in [GI18]. Besides, we also observed that the multiplicity preservation (i.e. equality (1.1)) also holds if the Witt index of GG is less than or equal to one. Hence we obtained a description for the full automorphic discrete spectra of those even orthogonal or unitary groups, by “pulling back” the Arthur’s multiplicity formula for HH to GG through the theta lift. For each local place of FF, we defined the so-called “θ\theta-packets” of GG to be the theta lift of certain AA-packets of HH (see Section 2.5), and “glue” them together to get some global packets; we showed that the automorphic discrete spectrum of GG can be decomposed according to these global packets (see Theorem 8.13). We should emphasize here that, essentially our results in this paper are independent of the results in [CZ21]; we use [CZ21] only as one of the motivations for the results shown in this paper.

Notice that at each place of FF, the definition of the “θ\theta-packets” is purely local; also, although we assumed that the Witt index of GG is less or equal to one, the localization of GG at local places could be quite general. It makes sense to ask: are these “θ\theta-packets” dependent on the choice of HH? What are these “θ\theta-packets”? It turns out that, at least at non-Archimedean places, θ\theta-packets are independent of the choice of HH; moreover, at those places where our GG is quasi-split, we show that the θ\theta-packets are the same as the AA-packets defined by Arthur and Mok. These are the main results in this paper. Indeed, these questions are already asked in the study of local theta correspondence, known as the “Adams conjecture”.

1.2. Adams conjecture

Now let FF be a local field of characteristic 0. In his paper [Ada89] Section 4, Adams proposed the following conjecture, which describes the local theta lift in terms of AA-parameters:

Conjecture 1.1.

Let (G,H)(G,H) be a reductive dual pair, such that the dimension of the standard representation of GL\prescript{L}{}{G} is not greater than that of HL\prescript{L}{}{H}. Let ψ\psi be a local AA-parameter for GG. Then one can write down a local AA-parameter θ(ψ)\theta(\psi) for HH in terms of ψ\psi explicitly, such that

  1. (A)

    For an irreducible representation πΠψA(G)\pi\in\Pi_{\psi}^{A}(G), its theta lift θ(π)\theta(\pi) lies in the corresponding local AA-packet Πθ(ψ)A(H)\Pi_{\theta(\psi)}^{A}(H) if it is non-zero;

  2. (B)

    If we suppose further that (G,H)(G,H) is in the stable range, then the theta lift between (G,H)(G^{\prime},H) provides us a bijection

    θ:ΠψA(G)Πθ(ψ)A(H),\theta:\bigsqcup\Pi_{\psi}^{A}(G^{\prime})\longrightarrow\Pi_{\theta(\psi)}^{A}(H),

    where GG^{\prime} runs over all pure inner forms of GG.

Our results in this paper can be more or less regarded as a refined version of Conjecture 1.1 (B) here: we not only prove the bijection between packets as (multi) sets, we also show the consistency of “labelings”, i.e. the characters of component groups attached to the representations inside the packets. However, in our results, we use the terminology “θ\theta-packets” rather than “AA-packets”, due to two reasons:

  • for quasi-split groups, our results imply the two terminologies are the same, so there is no harm; but for non quasi-split groups, at present AA-packets (under the framework of Arthur, both locally and gloablly, cf. [Art13] Chapter 9, or [KMSW14] Chapter 1.6 and 1.7) are not avaliable, so we use θ\theta-packets for substitutions;

  • as explained in the last subsection, a motivation of studying this question is to obtain some results for non quasi-split groups from quasi-split groups via theta lifts; motivated by this purpose and taking the results of [CZ21] into account, it is natural to use the θ\theta-packets.

We should also mention to readers that Mœglin has done many wonderful works on Conjeture 1.1 in [Mœg11c], based on her explicit construction of local AA-packets for classical groups. Next we briefly recall her results.

1.3. Some results of Mœglin

For a classical group GG over some pp-adic field and a local AA-parameter ψ\psi of GG, Mœglin has construct a packet ΠψM(G)\Pi_{\psi}^{M}(G) consisting of irreducible unitary representations using the techniques of Jacquet modules. To be more precise, she defined a collection of unitary representations

π(ψ,t¯,η¯),\pi\left(\psi,\underline{t},\underline{\eta}\right),

where the parameter (t¯,η¯)(\underline{t},\underline{\eta}) runs over some set Σψ(G)\Sigma_{\psi}(G) (which can be writen down explicitly according to ψ\psi). These representations are either zero or irreducible, and the packet ΠψM(G)\Pi_{\psi}^{M}(G) is simply the collection of all non-zero guys. When GG is a symplectic group or quasi-split orthogonal group, it was proved in [Xu17a] that ΠψM(G)=ΠψA(G)\Pi_{\psi}^{M}(G)=\Pi_{\psi}^{A}(G). To distinguish various notions, we shall call the packet ΠψM(G)\Pi_{\psi}^{M}(G)MM-packet”.

Now, let (G,H)(G,H) be an orthogonal-symplectic dual pair such that the dimension of the standard representation of GL\prescript{L}{}{G} is not greater than that of HL\prescript{L}{}{H}, and ψ\psi be a local AA-parameter for the group GG. Then, for each (t¯,η¯)Σψ(G)(\underline{t},\underline{\eta})\in\Sigma_{\psi}(G), she constructed a pair (t¯~,η¯~)Σθ(ψ)(H)(\widetilde{\underline{t}},\widetilde{\underline{\eta}})\in\Sigma_{\theta(\psi)}(H), where θ(ψ)\theta(\psi) is the local AA-parameter for HH predicted by Conjecture 1.1. Under some technical assumptions on the local AA-parameter ψ\psi, she asserted that

θ(π(ψ,t¯,η¯))=π(θ(ψ),t¯~,η¯~)\theta\left(\pi\left(\psi,\underline{t},\underline{\eta}\right)\right)=\pi\left(\theta(\psi),\widetilde{\underline{t}},\widetilde{\underline{\eta}}\right)

if the LHS and the RHS are both non-zero (see [Mœg11c] 5.2 Théorème). She also showed some non-vanishing criterion for the representation π(ψ,t¯,η¯)\pi\left(\psi,\underline{t},\underline{\eta}\right) along the proof. Hence in some sense, she has proved Conjecture 1.1 (A) under her assumptions. Her method is purely local. To prove these results, she mastered the Kudla’s filtration and Jacquet modules very carefully. Moreover, she pointed out that Conjecture 1.1 (A) is generally not true by giving some counter-examples.

If we suppose further that (G,H)(G,H) is in the stable range, then Mœglin’s technical assumptions are automatically satisfied. From her results, one can easily check the following:

  • the assignment (t¯,η¯)(t¯~,η¯~)(\underline{t},\underline{\eta})\mapsto(\widetilde{\underline{t}},\widetilde{\underline{\eta}}) induces a bijection

    θ:Σψ(G)Σθ(ψ)(H),\theta:\bigsqcup\Sigma_{\psi}(G^{\prime})\longrightarrow\Sigma_{\theta(\psi)}(H),

    where GG^{\prime} runs over all pure inner forms of GG;

  • the representation π(ψ,t¯,η¯)\pi\left(\psi,\underline{t},\underline{\eta}\right) is non-zero if and only if π(θ(ψ),t¯~,η¯~)\pi\left(\theta(\psi),\widetilde{\underline{t}},\widetilde{\underline{\eta}}\right) is non-zero.

It follows that Conjecture 1.1 (B) holds (with “AA-packets” replaced by “MM-packets”).

However, we still want to look for an independent proof of Conjecture 1.1 (B), due to the following reasons:

  • As we have explained, one of the motivations of studying this question is to obtain some results for non quasi-split groups from quasi-split groups via theta lifts. Hence we want to look for an approach which is free of using results from non quasi-split groups.

  • Except for for the bijectivity, for our purpose, we also need to show the consistency of the “labelings”. To pass from Mœglin’s parametrization to that of Arthur, one still needs to do some computions following [Xu17a].

In the next subsection, we briefly describe the idea of our approach.

1.4. Idea of the proof

Our idea of the proof is very simple: we use global methods as much as possible. For quasi-split classical groups, the Arthur’s multiplicity formula implies that any localization of an irreducible unitary representation occuring in the automorphic discrete spectrum lies in a local AA-packet. One can image that, if the Arthur’s multiplicity formula has been established for all classical groups, then Conjecture 1.1 (B) should simply follows from the combination of some easy computations at unramified places and the Arthur’s multiplicity formula. From this point of view, many of our lemmas/ propositions in this paper indeed reduce to appropriately globalize a (local) representation. However, since the Arthur’s multiplicity formula for general non quasi-split groups has not been established yet, we still need to appeal to Mœglin’s explicit constructions of pp-adic local AA-packets to deal with some cases. But we should emphasize that our approach only rely on her results for quasi-split groups. As for the “labelings”, we shall use the intertwining relation to interpret the “labelings” of a local AA-packet as some representation-theoretical quantities. Then we can compute the “labelings” using the same techniques as in [GI16].

For Archimedean places, we also expect that Conjecture 1.1 (B) holds. Indeed, combining results in [Cos09] and [MR19], one can conclude that Conjecture 1.1 (B) holds for unitary dual-pairs when the AA-parameter ψ\psi is Adams-Johnson. We will not consider Archimedean places in this paper.

Now we give a summary of the layout of this paper. We formulate the main theorems in Section 2, taking the chance to recall some preliminaries. After doing some preparation work in Section 3 and recalling some results from other papers that we will use in Section 4, we prove our first result (independence of θ\theta-packets as sets on the choice of some data used in their construction) in Section 5, and we also prove some complementary results in Section 6. Then in Section 7 we recall the local intertwining relation by Arthur, and state an alternative version of it. Finally in Section 8, we prove the local intertwining relation for non quasi-split groups using some techniques developed by Gan-Ichino, and finish the proof of our main results; after that, we briefly summarize some expected and known properties of θ\theta-packets.

Acknowledgments

We would like to thank our supervisor Wee Teck Gan for many useful advices. We would also like to give a special thanks to Wen-Wei Li, Colette Mœglin, and Bin Xu for answering our naive questions. We thank Atsushi Ichino, Alberto Mínguez, and Lei Zhang for giving us many useful suggestions. We also thank Caihua Luo and Chuijia Wang for helpful discussions. The second author is supported by an MOE Graduate Research Scholarship.

2. Statement of main results

We first recall some notations from [CZ21]. Let FF be a local or global field, and EE be either FF or a quadratic field extension of FF. Let

c={the identity of Fif E=F;the non-trivial element in Gal(E/F)if [E:F]=2.c=\begin{cases}\textit{the identity of }F\quad&\textit{if }E=F;\\ \textit{the non-trivial element in }Gal(E/F)\quad&\textit{if }[E:F]=2.\end{cases}

In the case [E:F]=2[E:F]=2, we denote by ωE/F\omega_{E/F} the quadratic character of F×F^{\times} (or F×\𝔸×F^{\times}\backslash\mathbb{A}^{\times} if FF is global, and similarly in later paragraph) by class field theory, and we fix a trace zero element δE×\delta\in E^{\times}. Let V=V(n)V=V_{(n)} be a finite dimensional vector space over EE equipped with a non-degenerate Hermitian cc-sesquilinear form

,V:V×VE.\langle\cdot,\cdot\rangle_{V}:V\times V\longrightarrow E.

We consider the following three cases:

{Case OE=F and dimV=2n;Case U0[E:F]=2 and dimV=2n;Case U1[E:F]=2 and dimV=2n1.\begin{cases}\textit{Case $O$: }&\textit{$E=F$ and $\dim V=2n$};\\ \textit{Case $U_{0}$: }&\textit{$[E:F]=2$ and $\dim V=2n$};\\ \textit{Case $U_{1}$: }&\textit{$[E:F]=2$ and $\dim V=2n-1$}.\\ \end{cases}

where n0n\geq 0 is an integer (we require n1n\geq 1 in Case U1U_{1}). Sometimes when we want to deal with Case U0U_{0} and Case U1U_{1} at the same time, we shall simply write “Case UU”. Let G=G(V)G=G(V) be the group of elements gg in GL(V)GL(V) such that

gv,gwV=v,wVfor v,wV.\langle gv,gw\rangle_{V}=\langle v,w\rangle_{V}\quad\textit{for }v,w\in V.

If n=0n=0, we interpret GG as the trivial group. In Case OO, we let

χV:F××(orχV:F×\𝔸× if F is global )\chi_{V}:F^{\times}\longrightarrow\mathbb{C}^{\times}\quad\left(\textit{or}\quad\chi_{V}:F^{\times}\backslash\mathbb{A}^{\times}\longrightarrow\mathbb{C}\textit{ if $F$ is global }\right)

be the quadratic character associated to the discriminant of VV by class field theory. We set

ε0={1Case O;0Case U.\varepsilon_{0}=\begin{cases}1\quad&\textit{Case $O$};\\ 0\quad&\textit{Case $U$}.\end{cases}

All pure inner forms of G=G(V)G=G(V) arise in the form G=G(V)G^{\prime}=G(V^{\prime}) for some space VV^{\prime}. When FF is a local field, all these spaces VV^{\prime} are classified by some invariants. We briefly describe this classification.

When FF is non-Archimedean:

  • In Case OO, these VV^{\prime} are orthogonal spaces with the same dimension and discriminant as VV. There are exactly two of these spaces, distinguished by their (normalized) Hasse-Witt invariant ϵ(V)\epsilon(V) (cf. [Sch85] page 80–81). We shall denote by V+V^{+} the one with Hasse-Witt invariant +1+1, and by VV^{-} the one with Hasse-Witt invariant 1-1. Since V+V^{+} has the maximal possible Witt index, V+V^{+} must be isometric to

    V+V(d,c)+n1V^{+}\simeq V_{(d,c)}+\mathcal{H}^{n-1}

    for some d,cFd,c\in F, where

    V(d,c)=F[X]/(X2d)V_{(d,c)}=F[X]/(X^{2}-d)

    is an 22-dimensional vector space over FF equipped with the quadratic form

    a+bXc(a2b2d),a+bX\longmapsto c\cdot(a^{2}-b^{2}d),

    and \mathcal{H} is the (orthogonal) hyperbolic plane. We fix such a tuple (d,c)(d,c) and the isometry, and we shall say that V+V^{+} is of type (d,c)(d,c). Notice that the choice of the tuple (d,c)(d,c) is not unique.

  • In Case UU, these VV^{\prime} are Hermitian spaces with the same dimension as VV. There are also exactly two of these spaces, distinguished by their sign ϵ(V)=ωE/F(discV)\epsilon(V)=\omega_{E/F}(\operatorname{disc}V). We shall denote by V+V^{+} the one with sign +1+1, and by VV^{-} the one with sign 1-1.

When FF is real:

  • In this situation, such spaces VV^{\prime} are classified by their signatures (p,q)(p,q) (satisfying certain conditions). Similar to the non-Archimedean case, in Case OO, we shall denote by V+V^{+} the space with the same dimension, same discriminant as VV and with Hasse-Witt invariant +1+1, such that G(V+)G(V^{+}) is a quasi-split pure inner form of GG; and in Case UU, we shall denote by V+V^{+} the space with the same dimension as VV and with sign +1+1, such that G(V+)G(V^{+}) is a quasi-split pure inner form of GG.

When FF is complex:

  • There is only one such space up to isometry with given dimension, and we shall denote it by V+V^{+}.

When FF is a global field, the local-global principle for orthogonal or Hermitian spaces implies that, whenever we are given a collection of local spaces {Vv}v\{V^{\prime}_{v}\}_{v} for all places vv of FF, as long as these local spaces satisfy some “coherent” conditions, there will be a space VV^{\prime} over FF, such that the localization of VV^{\prime} at each place vv is isometry to VvV^{\prime}_{v} (see [Sch85] page 225 Theorem 6.10, or page 377 Theorem 6.9). Given VV and G=G(V)G=G(V), we let V+V^{+} be the space such that for each place vv of FF, Vv+V_{v}^{+} is (isometry to) the space we have defined in the local situations, i.e. (V+)v(Vv)+(V^{+})_{v}\simeq(V_{v})^{+}.

In all cases above, G=G(V+)G^{*}=G(V^{+}) is quasi-split, and we shall refer it as the quasi-split pure inner form of GG.

Convention 2.1.

In later proofs of our results, we will often use the Arthur’s multiplicity formula for quasi-split classical groups. When we say something like “VV is a space such that G=G(V)G=G(V) is quasi-split”, this should be understood as V=V+V=V^{+}, and GG is the quasi-split pure inner form of itself.

Let W=W(r)W=W_{(r)} be an

{2r-dimensionalCase O;(2r+1)-dimensionalCase U0;2r-dimensionalCase U1\begin{cases}2r\textit{-dimensional}\quad&\textit{Case $O$};\\ (2r+1)\textit{-dimensional}\quad&\textit{Case $U_{0}$};\\ 2r\textit{-dimensional}\quad&\textit{Case $U_{1}$}\\ \end{cases}

vector space over EE equipped with a non-degenerate skew-Hermitian cc-sesquilinear form

,W:W×WE,\langle\cdot,\cdot\rangle_{W}:W\times W\longrightarrow E,

such that WW is split (in Case U0U_{0} we require that the anisotropic kernel of WW is the 11-dimensional skew-Hermitian space represented by δ\delta). Let H=H(W)H=H(W) be the group of elements hh in GL(W)GL(W) such that

hv,hwW=v,wWfor v,wW.\langle hv,hw\rangle_{W}=\langle v,w\rangle_{W}\quad\textit{for }v,w\in W.

The pair (G,H)(G,H) is then an example of a reductive dual-pair. When FF is a local field, we fix a non-trivial additive character ψF\psi_{F} of FF, and pick up a pair of characters (χV,χW)(\chi_{V},\chi_{W}) of E×E^{\times} as follows

χV={the quadratic character associated to VCase O;a character of E× such that χV|F×=ωE/FdimVCase U.\chi_{V}=\begin{cases}\textit{the quadratic character associated to }V\quad&\textit{Case $O$};\\ \textit{a character of }E^{\times}\textit{ such that }\chi_{V}|_{F^{\times}}=\omega_{E/F}^{\dim V}\quad&\textit{Case $U$}.\end{cases}
χW={the trivial character of F×Case O;a character of E× such that χW|F×=ωE/FdimWCase U.\chi_{W}=\begin{cases}\textit{the trivial character of }F^{\times}\quad&\textit{Case $O$};\\ \textit{a character of }E^{\times}\textit{ such that }\chi_{W}|_{F^{\times}}=\omega_{E/F}^{\dim W}\quad&\textit{Case $U$}.\end{cases}

When FF is a global field, we fix a non-trivial additive character ψF\psi_{F} of F\𝔸F\backslash\mathbb{A}, and also characters (χV,χW)(\chi_{V},\chi_{W}) of E×\𝔸E×E^{\times}\backslash\mathbb{A}_{E}^{\times} similar to the local case. With respect to this tuple of auxiliary data (ψF,χV,χW)(\psi_{F},\chi_{V},\chi_{W}), one can consider the theta lift between (G,H)(G,H).

2.1. Theta lifts

Assume FF is local for a moment. With respect to the non-trivial additive character ψF\psi_{F} of FF and the auxliary data (χV,χW)(\chi_{V},\chi_{W}), one can define the Weil representation ω\omega of G×HG\times H. For any irreducible representation π\pi of GG, the maximal π\pi-isotypic quotient of ω\omega is of the form

πΘ(π)\pi\boxtimes\Theta(\pi)

for some smooth representation Θ(π)\Theta(\pi) of HH of finite length. Then by the Howe duality [How89], [Wal90], [GT16a], [GT16b], the maximal semi-simple quotient θ(π)\theta(\pi) of Θ(π)\Theta(\pi) is either zero or irreducible. Similarly, for any irreducible representation σ\sigma of HH, we can define Θ(σ)\Theta(\sigma) and θ(σ)\theta(\sigma).

Suppose next that FF is a number field. Fix a non-trivial additive character ψF\psi_{F} of F\𝔸F\backslash\mathbb{A}, and also characters (χV,χW)(\chi_{V},\chi_{W}). Let π=vπv\pi=\otimes_{v}\pi_{v} be an abstract irreducible representation of G(𝔸)G(\mathbb{A}) (i.e. a collection of local irreducible representations πv\pi_{v} of G(Fv)G(F_{v}) for all places vv of FF, such that πv\pi_{v} is unramified for almost all vv). At each place vv of FF, we can form the local theta lift θ(πv)\theta(\pi_{v}) with respect to (ψF,v,χV,v,χW,v)(\psi_{F,v},\chi_{V,v},\chi_{W,v}). Assume that they are all non-vanishing. Then θ(πv)\theta(\pi_{v}) is irreducible for all vv and is unramified for almost all vv. Hence we may define an abstract irreducible representation

θabs(π)=vθ(πv)\theta^{abs}(\pi)=\bigotimes_{v}\theta(\pi_{v})

of H(𝔸)H(\mathbb{A}). We call θabs(π)\theta^{abs}(\pi) the abstract theta lift of π\pi to H(𝔸)H(\mathbb{A}).

2.2. Unitary representations of low rank

The notion of rank for unitary representations was first introduced by Howe [How82] in the case of symplectic groups and was extended to the case of classical groups by J-S. Li [Li89a]. Following [Li89a], we say that an irreducible unitary representation of H=H(W(r))H=H\left(W_{(r)}\right) is of low rank if its rank is less than rr. Such representations are obtained by theta lifts as follows.

Let FF be a local field. Assume dimV<r\dim V<r. In particular, the reductive dual pair (G,H)(G,H) is in the stable range. Then for any irreducible representation π\pi of GG, its theta lift θ(π)\theta(\pi) to HH is non-vanishing. Moreover, if π\pi is unitary, then by [Li89b], so is θ(π)\theta(\pi). In [Li89a], J-S. Li showed that:

Theorem 2.2.

The theta lift provides a bijection

VIrrunitG(V)×{Characters of E1}{Irreducible unitary representations of H of rank dimV}.\begin{array}[]{c}\displaystyle{\bigsqcup_{V}}\operatorname{Irr}_{unit}G(V)\times\Big{\{}\textit{Characters of }E^{1}\Big{\}}\\ \Bigg{\updownarrow}\\ \Big{\{}\textit{Irreducible unitary representations of }H\textit{ of rank }\dim V\Big{\}}.\end{array}

where the disjoint union runs over all vector space VV over EE with fixed dimension, and equipped with a non-degenerate Hermitian cc-sesquilinear form (in Case OO we interpret E1E^{1} as the trivial group). The map sends a pair (π,χ)(\pi,\chi) in the first set to a representation θ(π)χ\theta(\pi)\otimes\chi of HH, where we regard χ\chi as a character of HH via the determinant map.

This result has a global analog. Let FF be a number field and σ=vσv\sigma=\otimes_{v}\sigma_{v} an irreducible unitary representation of H(𝔸)H(\mathbb{A}) which occurs as a subrepresentation of 𝒜(H)\mathcal{A}(H), where 𝒜(H)\mathcal{A}(H) is the space of automorphic forms of HH. Then, by [Li89b] and [Li97], we have:

Theorem 2.3.
  1. (1)

    The following are equivalent:

    • σ\sigma is of rank dimV\dim V;

    • σv\sigma_{v} is of rank dimV\dim V for all vv;

    • σv\sigma_{v} is of rank dimV\dim V for some vv.

  2. (2)

    Suppose that σ\sigma satisfies the above equivalent conditions. Then, there exists an unique G=G(V)G=G(V) together with an abstract representation π=vπv\pi=\otimes_{v}\pi_{v} of G(𝔸)G(\mathbb{A}), and an automorphic character χ\chi of E1(𝔸)E^{1}(\mathbb{A}), such that

    σθabs(π)χ.\sigma\simeq\theta^{abs}(\pi)\otimes\chi.

Finally, we recall another result of J-S. Li, which allows us to lift square-integrable automorphic representations of G(𝔸)G(\mathbb{A}) to H(𝔸)H(\mathbb{A}). For any irreducible representation π\pi of G(𝔸)G(\mathbb{A}), we define its multiplicities m(π)m(\pi) and mdisc(π)m_{disc}(\pi) by

m(π)\displaystyle m(\pi) =dimHomG(𝔸)(π,𝒜(G));\displaystyle=\dim\operatorname{Hom}_{G(\mathbb{A})}\big{(}\pi,\mathcal{A}(G)\big{)};
mdisc(π)\displaystyle m_{disc}(\pi) =dimHomG(𝔸)(π,𝒜2(G)),\displaystyle=\dim\operatorname{Hom}_{G(\mathbb{A})}\big{(}\pi,\mathcal{A}^{2}(G)\big{)},

where 𝒜2(G)=𝒜(G)Ldisc2(G)\mathcal{A}^{2}(G)=\mathcal{A}(G)\cap L^{2}_{disc}(G). Obviously, mdisc(π)m(π)m_{disc}(\pi)\leq m(\pi). Likewise, if σ\sigma is an irreducible representation of H(𝔸)H(\mathbb{A}), we have its multiplicities m(σ)m(\sigma) and mdisc(σ)m_{disc}(\sigma). By [Li97], we have

Theorem 2.4.

Assume that dimV<r\dim V<r. Let π\pi be an irreducible unitary representation of G(𝔸)G(\mathbb{A}) and θabs(π)\theta^{abs}(\pi) its abstract theta lift to H(𝔸)H(\mathbb{A}). Then we have

mdisc(π)mdisc(θabs(π))m(θabs(π))m(π).m_{disc}(\pi)\leq m_{disc}(\theta^{abs}(\pi))\leq m(\theta^{abs}(\pi))\leq m(\pi).

2.3. Local and global classifications

We briefly recall some terminologies and results from [Art13] (also [AG17]), [Mok15], and some other papers.

First let FF be a local field of characteristic 0. A local AA-parameter for the group GG is a homomorphism

ψ:LF×SL2()GL,\psi:L_{F}\times SL_{2}(\mathbb{C})\longrightarrow\prescript{L}{}{G},

where LFL_{F} is the Weil-Deligne group of FF. If there is no further explanations, we will assume that the image of the Weil group under a local AA-parameter is bounded by default. By composing this homomorphism with the standard representation of GL\prescript{L}{}{G}, we can regard a local AA-parameter as a (conjugate) self-dual representation of LE×SL2()L_{E}\times SL_{2}(\mathbb{C}) with certain parity. We denote by Ψ(G)\Psi(G) the set of local AA-parameters for GG. Following Arthur, we define

Sψ\displaystyle S_{\psi} =Cent(Imψ,G^),\displaystyle=Cent(\operatorname{Im}\psi,\widehat{G}),
𝒮ψ\displaystyle\mathcal{S}_{\psi} =π0(Sψ),\displaystyle=\pi_{0}(S_{\psi}),
𝒮ψ¯\displaystyle\overline{\mathcal{S}_{\psi}} =𝒮ψ/zψ,\displaystyle=\mathcal{S}_{\psi}/\langle z_{\psi}\rangle,

where zψz_{\psi} is the image of IG^-I\in\widehat{G} in 𝒮ψ\mathcal{S}_{\psi}. We shall call 𝒮ψ\mathcal{S}_{\psi} or 𝒮ψ¯\overline{\mathcal{S}_{\psi}} the component group associated to the local AA-parameter ψ\psi. If we write ψ\psi as

ψ=iIψmiψi,\psi=\sum_{i\in I_{\psi}}m_{i}\cdot\psi_{i},

where each ψi=ϕiSdi\psi_{i}=\phi_{i}\boxtimes S_{d_{i}} is an irreducible representation of LE×SL2()L_{E}\times SL_{2}(\mathbb{C}), and IψI_{\psi} is the index set of this summation, then as explicated in [GGP12] Section 8, 𝒮ψ\mathcal{S}_{\psi} has an explicit description in the form

𝒮ψ=iIψ(/2)ai,\mathcal{S}_{\psi}=\prod_{i\in I^{\prime}_{\psi}}\left(\mathbb{Z}/2\mathbb{Z}\right)a_{i},

where on the RHS, the product runs over the subset IψI^{\prime}_{\psi} of IψI_{\psi} containing all iIψi\in I_{\psi} such that ψi\psi_{i} is of the same parity as ψ\psi; each element in the canonical basis {ai}\{a_{i}\} of 𝒮ψ\mathcal{S}_{\psi} corresponds to such a ψi\psi_{i}. Under this identification, we have

zψ=iIψmiai,z_{\psi}=\sum_{i\in I^{\prime}_{\psi}}m_{i}\cdot a_{i},

and 𝒮ψ¯=𝒮ψ/zψ\overline{\mathcal{S}_{\psi}}=\mathcal{S}_{\psi}/\langle z_{\psi}\rangle; where again, the summation on the RHS runs over all ii such that ψi\psi_{i} is of the same parity as ψ\psi.

When V=V+V=V^{+}, i.e. G=GG=G^{*} is quasi-split, thanks to Arthur and Mok, we can talk about the local AA-packet ΠψA(G)\Pi_{\psi}^{A}(G^{*}) associated to the AA-parameter ψ\psi: this is a finite (multi) set of irreducible unitary representations of GG^{*}, together with a map to the Pontryagin dual of the component group

𝒥𝒲A:ΠψA(G)𝒮ψ¯^.\mathcal{J}^{A}_{\mathscr{W}}:\Pi_{\psi}^{A}(G^{*})\longrightarrow\widehat{\overline{\mathcal{S}_{\psi}}}.

This map depends on the choice of a Whittaker datum 𝒲\mathscr{W} of GG^{*}. The local AA-packet ΠψA(G)\Pi_{\psi}^{A}(G^{*}) can be also regarded as a representation of 𝒮ψ¯×G\overline{\mathcal{S}_{\psi}}\times G^{*} by setting

ΠψA(G)=π𝒥𝒲A(π)π,\Pi_{\psi}^{A}(G^{*})=\bigoplus_{\pi}\mathcal{J}^{A}_{\mathscr{W}}(\pi)\boxtimes\pi,

where the summation on the RHS runs over all irreducible unitary representations of GG^{*} in ΠψA(G)\Pi_{\psi}^{A}(G^{*}). Sometimes we shall adopt this point of view without any further explanation.

Similarly, one can define the local AA-parameter for the group HH, and for a local AA-parameter ψH\psi_{H} of HH, one can define and describe the component group 𝒮ψH¯\overline{\mathcal{S}_{\psi_{H}}} in the same manner. Again, according to Arthur and Mok’s works, we can talk about the local AA-packet ΠψHA(H)\Pi_{\psi_{H}}^{A}(H) associated to the AA-parameter ψH\psi_{H}, which can be regarded as a representation of 𝒮ψH¯×H\overline{\mathcal{S}_{\psi_{H}}}\times H by setting

ΠψHA(H)=σ𝒥𝒲A(σ)σ,\Pi_{\psi_{H}}^{A}(H)=\bigoplus_{\sigma}\mathcal{J}^{A}_{\mathscr{W}^{\prime}}(\sigma)\boxtimes\sigma,

where 𝒲\mathscr{W}^{\prime} is a Whittaker datum of HH, and the summation on the RHS runs over all irreducible unitary representations of HH in ΠψHA(H)\Pi_{\psi_{H}}^{A}(H).

Now we turn to the global classifications. Let FF be a number field. Two irreducible representations π=vπv\pi=\otimes_{v}\pi_{v} and π=vπv\pi^{\prime}=\otimes_{v}\pi^{\prime}_{v} of G(𝔸)G(\mathbb{A}) are said to be nearly equivalent if πv\pi_{v} and πv\pi^{\prime}_{v} are equivalent for almost all places vv of FF. The decomposition of automorphic discrete spectrum of GG into near equivalence classes will be expressed in terms of elliptic AA-parameters. Recall that an elliptic AA-parameter for GG is nothing but a formal finite sum

(2.1) ψ=iρiSdi,\psi=\sum_{i}\rho_{i}\boxtimes S_{d_{i}},

where

  • ρi\rho_{i} is an irreducible (conjugate) self-dual cuspidal automorphic representation of GLni(𝔸E)GL_{n_{i}}(\mathbb{A}_{E});

  • SdiS_{d_{i}} is the did_{i}-dimensional irreducible representation of SL2()SL_{2}(\mathbb{C});

  • inidi=dimV\sum_{i}n_{i}d_{i}=\dim V;

  • If did_{i} is odd, then ρi\rho_{i} is

    {orthogonalCase O;conjugate symplectic Case U0;conjugate orthogonal Case U1.\begin{cases}\textit{orthogonal}\quad&\textit{Case $O$};\\ \textit{conjugate symplectic }\quad&\textit{Case $U_{0}$};\\ \textit{conjugate orthogonal }\quad&\textit{Case $U_{1}$}.\end{cases}
  • If did_{i} is even, then ρi\rho_{i} is

    {symplecticCase O;conjugate orthogonal Case U0;conjugate symplectic Case U1.\begin{cases}\textit{symplectic}\quad&\textit{Case $O$};\\ \textit{conjugate orthogonal }\quad&\textit{Case $U_{0}$};\\ \textit{conjugate symplectic }\quad&\textit{Case $U_{1}$}.\end{cases}
  • If (ρi,di)=(ρj,dj)(\rho_{i},d_{i})=(\rho_{j},d_{j}), then i=ji=j;

  • In Case OO, if we denote the central character of ρi\rho_{i} by ωi\omega_{i}, then

    iωidi=χV.\prod_{i}\omega_{i}^{d_{i}}=\chi_{V}.

If further di=1d_{i}=1 for all ii, then we say that ψ\psi is generic. We denote the set of all elliptic AA-parameters by Ψell(G)\Psi_{ell}(G). For each place vv of FF, let

ψv:LFv×SL2()GvL\psi_{v}:L_{F_{v}}\times SL_{2}(\mathbb{C})\longrightarrow\prescript{L}{}{G_{v}}

be the localization of ψ\psi at vv. Here

LFv={the Weil group of Fvif v is Archimedean;the Weil-Deligne group of Fvif v is non-Archimedean,L_{F_{v}}=\begin{cases}\textit{the Weil group of }F_{v}\quad&\textit{if }v\textit{ is Archimedean};\\ \textit{the Weil-Deligne group of }F_{v}\quad&\textit{if }v\textit{ is non-Archimedean},\\ \end{cases}

and we use the local Langlands correspondence for the general linear groups. We associate to it an LL-parameter ϕψv:LFvGvL\phi_{\psi_{v}}:L_{F_{v}}\rightarrow\prescript{L}{}{G_{v}} by

ϕψv(w)=ψv(w,(|w|12|w|12)).\phi_{\psi_{v}}(w)=\psi_{v}\left(w,\left(\begin{array}[]{cc}{|w|^{\frac{1}{2}}}&{}\hfil\\ {}\hfil&{|w|^{-\frac{1}{2}}}\end{array}\right)\right).

We have

Theorem 2.5.

There exists a decomposition

Ldisc2(G)=ψΨell(G)Lψ2(G),L^{2}_{disc}(G)=\bigoplus_{\psi\in\Psi_{ell}(G)}L^{2}_{\psi}(G),

where Lψ2(G)L^{2}_{\psi}(G) is a full near equivalence class of irreducible representations π\pi in Ldisc2(G)L^{2}_{disc}(G) such that the LL-parameter of πv\pi_{v} is ϕψv\phi_{\psi_{v}} for almost all places vv of FF.

When G=GG=G^{*} is quasi-split, a further decomposition of each near equivalence class is avaliable, known as the Arthur’s multiplicity formula for GG^{*}. Fix a global Whittaker datum 𝒲\mathscr{W} of GG^{*}. Given an elliptic AA-parameter ψ\psi, we define the global packet ΠψA(G)\Pi_{\psi}^{A}(G^{*}) associated to ψ\psi as the restricted tensor product of the local AA-packets

ΠψA(G)\displaystyle\Pi_{\psi}^{A}(G^{*}) =vΠψvA(Gv)\displaystyle=\otimes^{\prime}_{v}\Pi_{\psi_{v}}^{A}(G^{*}_{v})
={π=vπv|πvΠψvA(Gv),πv unramified with the L-parameter ϕψv for almost all v}.\displaystyle=\{\pi=\otimes^{\prime}_{v}\pi_{v}~{}|~{}\pi_{v}\in\Pi_{\psi_{v}}^{A}(G^{*}_{v}),~{}\pi_{v}\textit{ unramified with the $L$-parameter $\phi_{\psi_{v}}$ for almost all }v\}.

We then have a map

𝒥𝒲A:ΠψA(G)\displaystyle\mathcal{J}_{\mathscr{W}}^{A}:\Pi_{\psi}^{A}(G^{*}) 𝒮ψ¯^,\displaystyle\longrightarrow\widehat{\overline{\mathcal{S}_{\psi}}},
π\displaystyle\pi 𝒥𝒲A(π),\displaystyle\longmapsto\mathcal{J}^{A}_{\mathscr{W}}(\pi),
𝒥𝒲A(π)(x)\displaystyle\mathcal{J}^{A}_{\mathscr{W}}(\pi)(x) v𝒥𝒲vA(πv)(xv),\displaystyle\coloneqq\prod_{v}\mathcal{J}_{\mathscr{W}_{v}}^{A}(\pi_{v})(x_{v}),

where x𝒮ψx\in\mathcal{S}_{\psi} and xvx_{v} is the localization of xx at vv. We can also define the so-called canonical sign character ϵψ𝒮ψ^\epsilon_{\psi}\in\widehat{\mathcal{S}_{\psi}} following [Art13] page 47, or [Mok15] page 29. We put

ΠψA(G,ϵψ)={πΠψA(G)|𝒥𝒲A(π)=ϵψ}.\Pi_{\psi}^{A}(G^{*},\epsilon_{\psi})=\left\{\pi\in\Pi_{\psi}^{A}(G^{*})~{}|~{}\mathcal{J}_{\mathscr{W}}^{A}(\pi)=\epsilon_{\psi}\right\}.

Then the main global Theorems in [Art13] and [Mok15] assert that

Theorem 2.6.

Let ψ\psi be an elliptic AA-parameter for GG^{*}. Then we have the decomposition

Lψ2(G)=πΠψA(G,ϵψ)π.L^{2}_{\psi}(G^{*})=\bigoplus_{\pi\in\Pi_{\psi}^{A}(G^{*},\epsilon_{\psi})}\pi.

Similarly, one can define the global AA-parameters for the group HH, and for a global elliptic AA-parameter ψH\psi_{H} of HH, one can define the associated global AA-packets by gluing local AA-packets in the same manner. Again, according to Arthur and Mok’s works, Theorem 2.5 and Theorem 2.6 also holds for HH.

2.4. Remarks on Whittaker data

Since the local or global classification of both GG^{*} and HH depend on the choices of Whittaker data on GG^{*} and HH, and the theta lift also depends on the choice of an additive character, we need to choose these data in a compatible way. We now briefly describe the way we choose these data.

Let FF be a local or global field. Firstly we fix a non-trivial additive character ψF\psi_{F} of FF (or F\𝔸F\backslash\mathbb{A} if FF is global). Next we fix an Whittaker datum 𝒲\mathscr{W} of GG^{*} as follows.

In Case OO, G=G(V+)G^{*}=G(V^{+}) is an even orthogonal groups. As explicated at the beginning of this section, we fix an isometry

V+V(d,c)+n1V^{+}\simeq V_{(d,c)}+\mathcal{H}^{n-1}

for some d,cFd,c\in F, where \mathcal{H} is the (orthogonal) hyperbolic plane. The images of 1,XF[X]1,X\in F[X] in V(d,c)V_{(d,c)} are denoted by e,ee,e^{\prime}, respectively. For 1kn11\leq k\leq n-1, we write the kk-th hyperbolic plane =Fvk+Fvk\mathcal{H}=Fv_{k}+Fv_{k}^{*} with

vk,vkV=vk,vkV=0andvk,vkV=1,\langle v_{k},v_{k}\rangle_{V}=\langle v_{k}^{*},v_{k}^{*}\rangle_{V}=0\quad\textit{and}\quad\langle v_{k},v_{k}^{*}\rangle_{V}=1,

and we set

Xk=Fv1++FvkandXk=Fv1++Fvk.X_{k}=Fv_{1}+\cdots+Fv_{k}\quad\textit{and}\quad X_{k}^{*}=Fv_{1}^{*}+\cdots+Fv_{k}^{*}.

We denote by B=TUB=TU the FF-rational Borel subgroup of GG^{*} stabilizing the complete flag

X1Xn1,X_{1}\subset\cdots\subset X_{n-1},

where TT is the FF-rational torus stabilizing the lines FviFv_{i} for 1kn11\leq k\leq n-1. We define a generic character μc\mu_{c} of UU by

μc(u)=ψF(uv2,v1V++uvn1,vn2V+ue,vn1V).\mu_{c}(u)=\psi_{F}(\langle uv_{2},v_{1}^{*}\rangle_{V}+\cdots+\langle uv_{n-1},v_{n-2}^{*}\rangle_{V}+\langle ue,v_{n-1}^{*}\rangle_{V}).

Let 𝒲=(U,μc)\mathscr{W}=(U,\mu_{c}). Note that in fact 𝒲\mathscr{W} does not depend on the choice of the additive character ψF\psi_{F}, but only depends on the constant cc we have picked up.

In Case U0U_{0}, G=G(V+)G^{*}=G(V^{+}) is an even unitary groups. Recall that we have fixed a trace zero element δE×\delta\in E^{\times}. Let V+V^{+} be the 2n2n-dimensional Hermitian space over EE such that G=U(V+)G^{*}=U(V^{+}). Since GG^{*} quasi-split, the Witt index of V+V^{+} is nn. We choose a basis {vi,vi|i=1,,n}\{v_{i},v_{i}^{*}~{}|~{}i=1,\cdots,n\} of V+V^{+} such that

vi,vjV=vi,vjV=0andvi,vjV=δi,j\langle v_{i},v_{j}\rangle_{V}=\langle v_{i}^{*},v_{j}^{*}\rangle_{V}=0\quad\textit{and}\quad\langle v_{i},v_{j}^{*}\rangle_{V}=\delta_{i,j}

for 1i,jn1\leq i,j\leq n. We set

Xk=Ev1++EvkandXk=Ev1++EvkX_{k}=Ev_{1}+\cdots+Ev_{k}\quad\textit{and}\quad X_{k}^{*}=Ev_{1}^{*}+\cdots+Ev_{k}^{*}

for 1i,jn1\leq i,j\leq n. We denote by B=TUB=TU the FF-rational Borel subgroup of GG^{*} stabilizing the complete flag

X1Xn,X_{1}\subset\cdots\subset X_{n},

where TT is the FF-rational torus stabilizing the lines EviEv_{i} for 1kn1\leq k\leq n. We define a generic character μ\mu of UU by

μ(u)=ψF(12TrE/F(δ(uv2,v1V++uvn,vn1V+uvn,vnV))).\mu(u)=\psi_{F}\Big{(}\frac{1}{2}\operatorname{Tr}_{E/F}\big{(}\delta\cdot(\langle uv_{2},v_{1}^{*}\rangle_{V}+\cdots+\langle uv_{n},v_{n-1}^{*}\rangle_{V}+\langle uv_{n}^{*},v_{n}^{*}\rangle_{V})\big{)}\Big{)}.

Let 𝒲=(U,μ)\mathscr{W}=(U,\mu).

In Case U1U_{1}, there is an unique Whittaker datum 𝒲\mathscr{W} of GG^{*}.

Finally we fix a Whittaker datum 𝒲\mathscr{W}^{\prime} of HH as follows.

In Case OO, WW is the 2r2r-dimensional symplectic space. We choose a basis {wi,wi|i=1,,r}\{w_{i},w_{i}^{*}~{}|~{}i=1,\cdots,r\} of WW such that

wi,wjW=wi,wjW=0andwi,wjW=δi,j\langle w_{i},w_{j}\rangle_{W}=\langle w_{i}^{*},w_{j}^{*}\rangle_{W}=0\quad\textit{and}\quad\langle w_{i},w_{j}^{*}\rangle_{W}=\delta_{i,j}

for 1i,jr1\leq i,j\leq r. We set

Yk=Fw1++FwkandYk=Fw1++FwkY_{k}=Fw_{1}+\cdots+Fw_{k}\quad\textit{and}\quad Y_{k}^{*}=Fw_{1}^{*}+\cdots+Fw_{k}^{*}

for 1i,jr1\leq i,j\leq r. We denote by B=TUB^{\prime}=T^{\prime}U^{\prime} the FF-rational Borel subgroup of HH stabilizing the complete flag

Y1Yr,Y_{1}\subset\cdots\subset Y_{r},

where TT^{\prime} is the FF-rational torus stabilizing the lines FwiFw_{i} for 1kr1\leq k\leq r. We define a generic character μc\mu^{\prime}_{c} of UU^{\prime} by

μc(u)=ψF(c(uw2,w1V++uwr,wr1V+uwr,wrV)),\mu^{\prime}_{c}(u)=\psi_{F}\Big{(}c\cdot\big{(}\langle uw_{2},w_{1}^{*}\rangle_{V}+\cdots+\langle uw_{r},w_{r-1}^{*}\rangle_{V}+\langle uw_{r}^{*},w_{r}^{*}\rangle_{V}\big{)}\Big{)},

where the constant cc is the one appearing in the isometry V+V(d,c)+n1V^{+}\simeq V_{(d,c)}+\mathcal{H}^{n-1} we have fixed. Let 𝒲=(U,μc)\mathscr{W}^{\prime}=(U^{\prime},\mu^{\prime}_{c}). In this case we also define another generic character μ1\mu^{\prime}_{1} of UU^{\prime} by

μ1(u)=ψF(uw2,w1V++uwr,wr1V+uwr,wrV),\mu^{\prime}_{1}(u)=\psi_{F}\Big{(}\langle uw_{2},w_{1}^{*}\rangle_{V}+\cdots+\langle uw_{r},w_{r-1}^{*}\rangle_{V}+\langle uw_{r}^{*},w_{r}^{*}\rangle_{V}\Big{)},

and let 𝒲1=(U,μ1)\mathscr{W}^{\prime}_{1}=(U^{\prime},\mu^{\prime}_{1}).

In Case U0U_{0}, WW is an (2r+1)(2r+1)-dimensional skew-Hermitian space. Hence there is an unique Whittaker datum 𝒲\mathscr{W}^{\prime} of HH.

In Case U1U_{1}, WW is an 2r2r-dimensional skew-Hermitian space. We choose a basis {wi,wi|i=1,,r}\{w_{i},w_{i}^{*}~{}|~{}i=1,\cdots,r\} of WW such that

wi,wjW=wi,wjW=0andwi,wjW=δi,j\langle w_{i},w_{j}\rangle_{W}=\langle w_{i}^{*},w_{j}^{*}\rangle_{W}=0\quad\textit{and}\quad\langle w_{i},w_{j}^{*}\rangle_{W}=\delta_{i,j}

for 1i,jr1\leq i,j\leq r. We set

Yk=Fw1++FwkandYk=Fw1++FwkY_{k}=Fw_{1}+\cdots+Fw_{k}\quad\textit{and}\quad Y_{k}^{*}=Fw_{1}^{*}+\cdots+Fw_{k}^{*}

for 1i,jr1\leq i,j\leq r. We denote by B=TUB^{\prime}=T^{\prime}U^{\prime} the FF-rational Borel subgroup of HH stabilizing the complete flag

Y1Yr,Y_{1}\subset\cdots\subset Y_{r},

where TT^{\prime} is the FF-rational torus stabilizing the lines FwiFw_{i} for 1kr1\leq k\leq r. We define a generic character μ\mu^{\prime} of UU^{\prime} by

μ(u)=ψF(12TrE/F(uw2,w1V++uwr,wr1V+uwr,wrV)).\mu^{\prime}(u)=\psi_{F}\Big{(}\frac{1}{2}\operatorname{Tr}_{E/F}\big{(}\langle uw_{2},w_{1}^{*}\rangle_{V}+\cdots+\langle uw_{r},w_{r-1}^{*}\rangle_{V}+\langle uw_{r}^{*},w_{r}^{*}\rangle_{V}\big{)}\Big{)}.

Let 𝒲=(U,μ)\mathscr{W}^{\prime}=(U^{\prime},\mu^{\prime}).

2.5. Theta packets

Now we recall the definition of the main object we want to study in this paper, the so-called “θ\theta-packet”, which is defined in [CZ21]. From now on, we let FF be a local field of characteristic 0. We fix Whittaker data 𝒲\mathscr{W} and 𝒲\mathscr{W}^{\prime} of the group GG^{*} and HH, depending on the additive character ψF\psi_{F}, as explicated in Section 2.4. Assume now dimV<r\dim V<r. Let ψ\psi be a local AA-parameter for GG, and

θ(ψ)=ψχW1χV+χVS2r2n+1\theta(\psi)=\psi\chi_{W}^{-1}\chi_{V}+\chi_{V}\boxtimes S_{2r-2n+1}

be a local AA-parameter for HH (sometimes we shall also write it as θr(ψ)\theta^{r}(\psi) to emphasize its dependence on the integer rr). There is an obvious map

𝒮ψ𝒮θ(ψ),\mathcal{S}_{\psi}\longrightarrow\mathcal{S}_{\theta(\psi)},

sending an element ai𝒮ψa_{i}\in\mathcal{S}_{\psi} corresponding to an irreducible constituent ψi\psi_{i} of ψ\psi, to the element ai𝒮θ(ψ)a^{\prime}_{i}\in\mathcal{S}_{\theta(\psi)} corresponding to the irreducible constituent ψiχW1χV\psi_{i}\chi_{W}^{-1}\chi_{V} of θ(ψ)\theta(\psi). We write the local AA-packet Πθ(ψ)A(H)\Pi_{\theta(\psi)}^{A}(H) as a representation of 𝒮θ(ψ)¯×H\overline{\mathcal{S}_{\theta(\psi)}}\times H

Πθ(ψ)A(H)=σ𝒥𝒲A(σ)σ,\Pi_{\theta(\psi)}^{A}(H)=\bigoplus_{\sigma}\mathcal{J}^{A}_{\mathscr{W}^{\prime}}(\sigma)\boxtimes\sigma,

as σ\sigma runs over all irreducible unitary representations of HH in Πθ(ψ)A(H)\Pi_{\theta(\psi)}^{A}(H). Then the θ\theta-packet of GG associated to the AA-parameter ψ\psi is defined as

Πψθ(G)=σ(𝒥𝒲A(σ)|𝒮ψ)θ(σ),\Pi_{\psi}^{\theta}(G)=\bigoplus_{\sigma}\left(\mathcal{J}^{A}_{\mathscr{W}^{\prime}}(\sigma)\Big{|}_{\mathcal{S}_{\psi}}\right)\boxtimes\theta(\sigma),

where θ(σ)\theta(\sigma) is the theta lift of σ\sigma to the group GG with respect to (ψF,χV,χW)(\psi_{F},\chi_{V},\chi_{W}), and we regard 𝒮ψ\mathcal{S}_{\psi} as a subgroup of 𝒮θ(ψ)\mathcal{S}_{\theta(\psi)} via the obvious map between them. Sometimes when we want to emphasize the possible dependence of Πψθ(G)\Pi_{\psi}^{\theta}(G) on the choice of H=H(W(r))H=H(W_{(r)}), we shall also use the notation Πψθ,r(G)\Pi_{\psi}^{\theta,r}(G). The θ\theta-packet Πψθ(G)\Pi_{\psi}^{\theta}(G) can be also regarded as a (multi) set of irreducible unitary representations of GG, together with a map

𝒥ψF:Πψθ(G)𝒮ψ^\mathcal{J}_{\psi_{F}}:\Pi_{\psi}^{\theta}(G)\longrightarrow\widehat{\mathcal{S}_{\psi}}

by sending θ(σ)\theta(\sigma) to 𝒥𝒲A(σ)|𝒮ψ\mathcal{J}^{A}_{\mathscr{W}^{\prime}}(\sigma)\Big{|}_{\mathcal{S}_{\psi}}.

Remark 2.7.

For those ψ\psi that do not have bounded image on the Weil group, but come from a localization of some global elliptic AA-parameter for an even orthogonal or unitary group, we can define the θ\theta-packet Πψθ(G)\Pi_{\psi}^{\theta}(G) in the same manner.

In this paper, we mainly consider the case that FF is non-Archimedean. Our main theorem in this paper is

Theorem 2.8.

Let FF be a non-Archimedean local field. For all local AA-parameter ψ\psi of G=G(V)G=G(V) (with bounded image on the Weil group), we have:

  1. (1)

    the definition of the packet Πψθ(G)\Pi_{\psi}^{\theta}(G) is indeed independent of the choice of H=H(W(r))H=H(W_{(r)}) with r>dimVr>\dim V;

  2. (2)

    if V=V+V=V^{+}, i.e. G=GG=G^{*} is quasi-split, then

    Πψθ(G)=ΠψA(G)\Pi_{\psi}^{\theta}(G)=\Pi_{\psi}^{A}(G)

    as representations of 𝒮ψ×G\mathcal{S}_{\psi}\times G^{*}.

Remark 2.9.

When FF is Archimedean, we also expect the same results hold. In the case that GG is a real unitary group and ψ\psi is Adams-Johnson, one can refer to [MR19] Théorème 1.1.

Along the way of proving this theorem, we also deduce some by-products. We shall summarize them in the last part of this paper.

3. Compatibility with parabolic inductions

In this section, we imitate [GI16] Section 8 to construct an equivariant map, and use this equivariant map to deduce some results in the context of the theta correspondence which will be used later.

3.1. A mixed model

We shall use a mixed model to do some computations. The same model is also used in [GI16] and [Ato18], so readers may also consult these two papers for details. For the convenience of readers, we briefly recall it. Suppose that we have

V=X+V0+XV=X+V_{0}+X^{*}

for some kk-dimensional totally isotropic subspace XX and XX^{*} of VV. Let n0=nkn_{0}=n-k, and r0=rkr_{0}=r-k. Then there is a maximal parabolic subgroup P=MPUPP=M_{P}U_{P} of GG stabilizing XX, where MPM_{P} is the Levi component of PP stabilizing XX^{*} and UPU_{P} is the unipotent radical of PP. We have

MP\displaystyle M_{P} ={mP(a)h0|aGL(X),h0G(V0)},\displaystyle=\{m_{P}(a)\cdot h_{0}~{}|~{}a\in GL(X),h_{0}\in G(V_{0})\},
UP\displaystyle U_{P} ={uP(b)uP(c)|bHom(V0,X),cHerm(X,X)},\displaystyle=\{u_{P}(b)\cdot u_{P}(c)~{}|~{}b\in\operatorname{Hom}(V_{0},X),c\in\operatorname{Herm}(X^{*},X)\},

where

mP(a)\displaystyle m_{P}(a) =(a1V0(a)1),\displaystyle=\left(\begin{array}[]{ccc}a&{}\hfil&{}\hfil\\ {}\hfil&1_{V_{0}}&{}\hfil\\ {}\hfil&{}\hfil&\left(a^{*}\right)^{-1}\end{array}\right),
uP(b)\displaystyle u_{P}(b) =(1Xb12bb1V0b1X),\displaystyle=\left(\begin{array}[]{ccc}1_{X}&b&-\frac{1}{2}bb^{*}\\ {}\hfil&1_{V_{0}}&-b^{*}\\ {}\hfil&{}\hfil&1_{X^{*}}\end{array}\right),
uP(c)\displaystyle u_{P}(c) =(1Xc1V01X),\displaystyle=\left(\begin{array}[]{ccc}{1_{X}}&{}\hfil&{c}\\ {}\hfil&{1_{V_{0}}}&{}\hfil\\ {}\hfil&{}\hfil&{1_{X^{*}}}\end{array}\right),

and

Herm(X,X)={cHom(X,X)|c=c}.\operatorname{Herm}(X^{*},X)=\{c\in\operatorname{Hom}(X^{*},X)~{}|~{}c^{*}=-c\}.

Here, the elements aGL(X)a^{*}\in GL(X^{*}), bHom(X,V0)b^{*}\in\operatorname{Hom}(X^{*},V_{0}), and cHom(X,X)c^{*}\in\operatorname{Hom}(X^{*},X) are the adjoints of aa, bb, and cc respectively, under the cc-Hermitian form on VV. Put

ρP=dimV0+kε02wP=(IX1V0IX1),\rho_{P}=\frac{\dim V_{0}+k-\varepsilon_{0}}{2}\quad w_{P}=\left(\begin{array}[]{ccc}{}\hfil&{}\hfil&-I_{X}\\ {}\hfil&1_{V_{0}}&{}\hfil\\ -I_{X}^{-1}&{}\hfil&\par{}\hfil\end{array}\right),

where we pick up IXIsom(X,X)I_{X}\in\operatorname{Isom}(X^{*},X) in an obvious way after choosing a basis of XX.

Similarly, suppose that we have

W=Y+W0+YW=Y+W_{0}+Y^{*}

for some kk-dimensional totally isotropic subspace YY and YY^{*} of WW. Then there is a maximal parabolic subgroup Q=MQUQQ=M_{Q}U_{Q} of GG stabilizing YY, where MQM_{Q} is the Levi component of QQ stabilizing YY^{*} and UQU_{Q} is the unipotent radical of QQ. For aGL(Y)a\in GL(Y), bHom(W0,Y)b\in\operatorname{Hom}(W_{0},Y) and cHerm(Y,Y)c\in\operatorname{Herm}(Y^{*},Y), we define elements mQ(a)MQm_{Q}(a)\in M_{Q} and uQ(b),uQ(c)UQu_{Q}(b),u_{Q}(c)\in U_{Q} as above. Put

ρQ=dimW0+k+ε02,wQ=(IY1W0IY1),\rho_{Q}=\frac{\dim W_{0}+k+\varepsilon_{0}}{2},\quad w_{Q}=\left(\begin{array}[]{ccc}{}\hfil&{}\hfil&-I_{Y}\\ {}\hfil&1_{W_{0}}&{}\hfil\\ I_{Y}^{-1}&{}\hfil&{}\hfil\end{array}\right),

where we pick up IYIsom(Y,Y)I_{Y}\in\operatorname{Isom}(Y^{*},Y) in an obvious way after choosing a basis of YY.

We write:

  • ω\omega for the Weil representation ωψF,V,W\omega_{\psi_{F},V,W} of G×HG\times H on a space 𝒮\mathscr{S};

  • ω0\omega_{0} for the Weil representation ωψF,V,W0\omega_{\psi_{F},V,W_{0}} of G0×HG_{0}\times H on a space 𝒮0\mathscr{S}_{0}, where G0=G(V0)G_{0}=G(V_{0});

  • ω00\omega_{00} for the Weil representation ωψF,V0,W0\omega_{\psi_{F},V_{0},W_{0}} of G0×H0G_{0}\times H_{0} on a space 𝒮00\mathscr{S}_{00}, where H0=H(W0)H_{0}=H(W_{0}).

We take a mixed model

𝒮=𝒮(WX)𝒮0\mathscr{S}=\mathscr{S}(W\otimes X^{*})\otimes\mathscr{S}_{0}

of ω\omega, where we regard 𝒮\mathscr{S} as a space of functions on WXW\otimes X^{*} with values in 𝒮0\mathscr{S}_{0}. Similarly, we take a mixed model

𝒮0=𝒮(YV0)𝒮00\mathscr{S}_{0}=\mathscr{S}(Y^{*}\otimes V_{0})\otimes\mathscr{S}_{00}

of ω0\omega_{0}, where we regard 𝒮0\mathscr{S}_{0} as a space of functions on YV0Y^{*}\otimes V_{0} with values in 𝒮00\mathscr{S}_{00}. Also, we write:

  • ρ0\rho_{0} for the Heisenberg representation of (WV0)\mathscr{H}(W\otimes V_{0}) on 𝒮0\mathscr{S}_{0} with central character ψF\psi_{F};

  • ρ00\rho_{00} for the Heisenberg representation of (W0V0)\mathscr{H}(W_{0}\otimes V_{0}) on 𝒮00\mathscr{S}_{00} with central character ψF\psi_{F}.

We can derive the following formulas for the Weil representations ω\omega and ω0\omega_{0}. For φ𝒮\varphi\in\mathscr{S} and xWXx\in W\otimes X^{*}, we have

(ω(h)φ)(x)\displaystyle(\omega(h)\varphi)(x) =ω0(h)φ(h1x),\displaystyle=\omega_{0}(h)\varphi(h^{-1}x), h\displaystyle h H,\displaystyle\in H,
(ω(g0)φ)(x)\displaystyle(\omega(g_{0})\varphi)(x) =ω0(g0)φ(x),\displaystyle=\omega_{0}(g_{0})\varphi(x), g0\displaystyle g_{0} G0,\displaystyle\in G_{0},
(ω(mP(a))φ)(x)\displaystyle(\omega(m_{P}(a))\varphi)(x) =χW(deta)|deta|dimW/2φ(ax),\displaystyle=\chi_{W}(\det a)|\det a|^{\dim W/2}\varphi(a^{*}x), a\displaystyle a GL(X),\displaystyle\in GL(X),
(ω(uP(b))φ)(x)\displaystyle(\omega(u_{P}(b))\varphi)(x) =ρ0((bx,0))φ(x),\displaystyle=\rho_{0}((b^{*}x,0))\varphi(x), b\displaystyle b Hom(V0,X),\displaystyle\in\operatorname{Hom}(V_{0},X),
(ω(uP(c))φ)(x)\displaystyle(\omega(u_{P}(c))\varphi)(x) =ψF(12cx,x)φ(x),\displaystyle=\psi_{F}(\frac{1}{2}\langle cx,x\rangle)\varphi(x), c\displaystyle c Herm(X,X),\displaystyle\in\operatorname{Herm}(X^{*},X),
(ω(wP)φ)(x)\displaystyle(\omega(w_{P})\varphi)(x) =γWkWXφ(IX1y)ψ(y,x)𝑑y,\displaystyle=\gamma_{W}^{-k}\int_{W\otimes X}\varphi(I_{X}^{-1}y)\psi(-\langle y,x\rangle)dy,

where γW\gamma_{W} is a certain constant. Also, for φ0𝒮0\varphi_{0}\in\mathscr{S}_{0} and xYV0x\in Y^{*}\otimes V_{0}, we have

(ω0(g0)φ0)(x)\displaystyle(\omega_{0}(g_{0})\varphi_{0})(x) =ω00(g0)φ0(g01x),\displaystyle=\omega_{00}(g_{0})\varphi_{0}(g_{0}^{-1}x), g0\displaystyle g_{0} G0,\displaystyle\in G_{0},
(ω0(h0)φ0)(x)\displaystyle(\omega_{0}(h_{0})\varphi_{0})(x) =ω00(h0)φ0(x),\displaystyle=\omega_{00}(h_{0})\varphi_{0}(x), h0\displaystyle h_{0} H0,\displaystyle\in H_{0},
(ω0(mQ(a))φ0)(x)\displaystyle(\omega_{0}(m_{Q}(a))\varphi_{0})(x) =χV(deta)|deta|dimV0/2φ0(ax),\displaystyle=\chi_{V}(\det a)|\det a|^{\dim V_{0}/2}\varphi_{0}(a^{*}x), a\displaystyle a GL(Y),\displaystyle\in GL(Y),
(ω0(uQ(b))φ0)(x)\displaystyle(\omega_{0}(u_{Q}(b))\varphi_{0})(x) =ρ00((bx,0))φ0(x),\displaystyle=\rho_{00}((b^{*}x,0))\varphi_{0}(x), b\displaystyle b Hom(W0,Y),\displaystyle\in\operatorname{Hom}(W_{0},Y),
(ω0(uQ(c))φ0)(x)\displaystyle(\omega_{0}(u_{Q}(c))\varphi_{0})(x) =ψF(12cx,x)φ0(x),\displaystyle=\psi_{F}(\frac{1}{2}\langle cx,x\rangle)\varphi_{0}(x), c\displaystyle c Herm(Y,Y),\displaystyle\in\operatorname{Herm}(Y^{*},Y),
(ω0(wQ)φ0)(x)\displaystyle(\omega_{0}(w_{Q})\varphi_{0})(x) =γVkYV0φ0(IY1y)ψ(y,x)𝑑y,\displaystyle=\gamma_{V}^{-k}\int_{Y\otimes V_{0}}\varphi_{0}(I_{Y}^{-1}y)\psi(-\langle y,x\rangle)dy,

where γV\gamma_{V} is a certain constant. Moreover, we have

(ρ0((y+y,0))φ0)(x)\displaystyle(\rho_{0}\left((y+y^{\prime},0)\right)\varphi_{0})(x) =ψ(x,y+12y,y)φ0(x+y),\displaystyle=\psi(\langle x,y\rangle+\frac{1}{2}\langle y^{\prime},y\rangle)\varphi_{0}(x+y^{\prime}), y\displaystyle y YV0,\displaystyle\in Y\otimes V_{0},
y\displaystyle y^{\prime} YV0,\displaystyle\in Y^{*}\otimes V_{0},
(ρ0((y0,0))φ0)(x)\displaystyle(\rho_{0}\left((y_{0},0)\right)\varphi_{0})(x) =ρ00((y0,0))φ0(x),\displaystyle=\rho_{00}\left((y_{0},0)\right)\varphi_{0}(x), y0\displaystyle y_{0} W0V0.\displaystyle\in W_{0}\otimes V_{0}.

3.2. An equivariant map

In this subsection we construct the explicit equivariant map. A non-vanishing result of this map will be important to us. The construction is roughly the same as [GI16] Section 8, except at one place we use the “small” theta lift whereas in Gan-Ichino’s paper they use the “big” theta lift.

First of all we need to fix Haar measures on various groups. For this part, we simply follow [Ato18] Section 6.3 in Case OO, and [GI16] Section 7.2 in Case UU. We shall identify GL(X)GL(X) with GLk(F)GL_{k}(F) using a basis {vi}i\{v_{i}\}_{i} for XX, and similarly identify GL(Y)GL(Y) with GLk(F)GL_{k}(F) using a basis {wi}i\{w_{i}\}_{i} for YY. We write {vi}i\{v_{i}^{*}\}_{i} and {wi}i\{w_{i}^{*}\}_{i} for the dual basis for XX^{*} and YY^{*} respectively. Then we can define an isomorphism i:GL(X)GL(Y)i:GL(X)\rightarrow GL(Y) via these identifications. Put

e\displaystyle e =w1v1++wkvkYX,\displaystyle=w_{1}\otimes v_{1}^{*}+\cdots+w_{k}\otimes v_{k}^{*}\in Y\otimes X^{*},
e\displaystyle e^{*} =w1v1++wkvkYX.\displaystyle=w_{1}^{*}\otimes v_{1}+\cdots+w_{k}^{*}\otimes v_{k}\in Y^{*}\otimes X.

Then i(a)ce=aei(a)^{c}e=a^{*}e and (i(a)c)e=ae\left(i(a)^{c}\right)^{*}e^{*}=ae^{*} for aGL(X)a\in GL(X).

For φ𝒮=𝒮(WX)𝒮0\varphi\in\mathscr{S}=\mathscr{S}(W\otimes X^{*})\otimes\mathscr{S}_{0}, we define functions 𝔣(φ)\mathfrak{f}(\varphi), 𝔣^(φ)\hat{\mathfrak{f}}(\varphi) on G×HG\times H with values in 𝒮0\mathscr{S}_{0} by

𝔣(φ)(g,h)\displaystyle\mathfrak{f}(\varphi)(g,h) =(ω(g,h)φ)(e00),\displaystyle=(\omega(g,h)\varphi)\left(\begin{matrix}e\\ 0\\ 0\end{matrix}\right),
𝔣^(φ)(g,h)\displaystyle\hat{\mathfrak{f}}(\varphi)(g,h) =YX(ω(g,h)φ)(x00)ψ(x,e)𝑑x\displaystyle=\int_{Y\otimes X^{*}}(\omega(g,h)\varphi)\left(\begin{matrix}x\\ 0\\ 0\end{matrix}\right)\psi(\langle x,e^{*}\rangle)dx

for gGg\in G and hHh\in H. Here we write an element in WXW\otimes X^{*} as a block matrix relative to the decomposition WX=YXW0XYXW\otimes X^{*}=Y\otimes X^{*}\oplus W_{0}\otimes X^{*}\oplus Y^{*}\otimes X^{*}. We also define functions f(φ)f(\varphi), f^(φ)\hat{f}(\varphi) on G×HG\times H with values in 𝒮00\mathscr{S}_{00} by

f(φ)(g,h)\displaystyle f(\varphi)(g,h) =ev(𝔣(φ)(g,h)),\displaystyle=ev(\mathfrak{f}(\varphi)(g,h)),
f^(φ)(g,h)\displaystyle\hat{f}(\varphi)(g,h) =ev(𝔣^(φ)(g,h)).\displaystyle=ev(\hat{\mathfrak{f}}(\varphi)(g,h)).

Here ev:𝒮0=𝒮(YV0)𝒮00𝒮00ev:\mathscr{S}_{0}=\mathscr{S}(Y^{*}\otimes V_{0})\otimes\mathscr{S}_{00}\rightarrow\mathscr{S}_{00} is the evaluation at 0YV00\in Y^{*}\otimes V_{0}. If f=f(φ)f=f(\varphi) or f^(φ)\hat{f}(\varphi), then

f(ug,uh)\displaystyle f(ug,u^{\prime}h) =f(g,h),\displaystyle=f(g,h), u\displaystyle u UP,\displaystyle\in U_{P},
u\displaystyle u^{\prime} UQ,\displaystyle\in U_{Q},
f(g0g,h0h)\displaystyle f(g_{0}g,h_{0}h) =ω00(g0,h0)f(g,h),\displaystyle=\omega_{00}(g_{0},h_{0})f(g,h), g0\displaystyle g_{0} G0,\displaystyle\in G_{0},
h0\displaystyle h_{0} H0,\displaystyle\in H_{0},
f(mP(a)g,mQ(i(a)c)h)\displaystyle f(m_{P}(a)g,m_{Q}(i(a)^{c})h) =(χVcχW)(deta)|deta|ρP+ρQf(g,h),\displaystyle=(\chi_{V}^{c}\chi_{W})(\det a)|\det a|^{\rho_{P}+\rho_{Q}}f(g,h), a\displaystyle a GL(X).\displaystyle\in GL(X).

Let τ\tau be an irreducible unitary representation of GLk(E)GL_{k}(E) on a space 𝒱τ\mathscr{V}_{\tau}. We may regard τ\tau as a representation of GL(X)GL(X) or GL(Y)GL(Y) via the above identifications. Let π0\pi_{0} and σ0\sigma_{0} be irreducible unitary representations of G0G_{0} and H0H_{0} on spaces 𝒱π0\mathscr{V}_{\pi_{0}} and 𝒱σ0\mathscr{V}_{\sigma_{0}} respectively. Fix non-zero invariant non-degenerate bilinear forms ,\langle\cdot,\cdot\rangle on 𝒱τ×𝒱τ\mathscr{V}_{\tau}\times\mathscr{V}_{\tau^{\vee}}, 𝒱π0×𝒱π0\mathscr{V}_{\pi_{0}}\times\mathscr{V}_{{\pi_{0}}^{\vee}}, and 𝒱σ0×𝒱σ0\mathscr{V}_{\sigma_{0}}\times\mathscr{V}_{{\sigma_{0}}^{\vee}}. Let

,:(𝒱τ𝒱σ0)×𝒱τ𝒱σ0\langle\cdot,\cdot\rangle:(\mathscr{V}_{\tau}\otimes\mathscr{V}_{{\sigma_{0}}^{\vee}})\times\mathscr{V}_{\tau^{\vee}}\longrightarrow\mathscr{V}_{{\sigma_{0}}^{\vee}}

be the induced map. Assume that

σ0=θψF,V0,W0(π0).\sigma_{0}=\theta_{\psi_{F},V_{0},W_{0}}(\pi_{0}).

We fix a non-zero G0×H0G_{0}\times H_{0}-equivariant map

𝒯00:ω00σ0π0.\mathcal{T}_{00}:\omega_{00}\otimes\sigma_{0}^{\vee}\longrightarrow\pi_{0}.

For φ𝒮\varphi\in\mathscr{S}, ΦsIndQH(τscχVcσ0)\varPhi_{s}\in\operatorname{Ind}_{Q}^{H}(\tau_{s}^{c}\chi_{V}^{c}\boxtimes\sigma_{0}^{\vee}), gGg\in G, vˇ𝒱τ\check{v}\in\mathscr{V}_{\tau^{\vee}}, and vˇ0𝒱π0\check{v}_{0}\in\mathscr{V}_{\pi_{0}^{\vee}}, put

𝒯s(φ\displaystyle\langle\mathcal{T}_{s}(\varphi Φs)(g),vˇvˇ0\displaystyle\otimes\varPhi_{s})(g),\check{v}\otimes\check{v}_{0}\rangle
=L(ss0,τ)1×UQH0\H𝒯00(f^(φ)(g,h)Φs(h),vˇ),vˇ0𝑑h,\displaystyle=L\left(s-s_{0},\tau\right)^{-1}\times\int_{U_{Q}H_{0}\backslash H}\langle\mathcal{T}_{00}(\hat{f}(\varphi)(g,h)\otimes\langle\varPhi_{s}(h),\check{v}\rangle),\check{v}_{0}\rangle dh,

where we set

s0=rn,s_{0}=r-n,

and L(s,τ)L(s,\tau) is the standard LL-factor of τ\tau. Similar to [GI16], one can show that

Proposition 3.1.
  1. (1)

    The integral is absolutely convergent when (s)0\Re(s)\gg 0 and admits a holomorphic continuation to \mathbb{C}. Hence we obtain a G×HG\times H-equivariant map

    𝒯s:ωIndQH(τscχVcσ0)IndPG(τsχWπ0).\mathcal{T}_{s}:\omega\otimes\operatorname{Ind}_{Q}^{H}\left(\tau_{s}^{c}\chi_{V}^{c}\boxtimes\sigma_{0}^{\vee}\right)\longrightarrow\operatorname{Ind}_{P}^{G}\left(\tau_{s}\chi_{W}\boxtimes\pi_{0}\right).
  2. (2)

    When (s)0\Re(s)\ll 0, we have

    𝒯s(φ\displaystyle\langle\mathcal{T}_{s}(\varphi Φs)(h),vˇvˇ0\displaystyle\otimes\varPhi_{s})(h),\check{v}\otimes\check{v}_{0}\rangle
    =L(ss0,τ)1γ(ss0,τ,ψF)1\displaystyle=L\left(s-s_{0},\tau\right)^{-1}\cdot\gamma\left(s-s_{0},\tau,\psi_{F}\right)^{-1}
    ×UQH0\H𝒯00(f(φ)(g,h)Φs(h),vˇ),vˇ0dh.\displaystyle\times\int_{U_{Q}H_{0}\backslash H}\langle\mathcal{T}_{00}({f}(\varphi)(g,h)\otimes\langle\varPhi_{s}(h),\check{v}\rangle),\check{v}_{0}\rangle dh.
  3. (3)

    Let Nτ>0N_{\tau}>0 be a positive real number such that L(s,τ)L(s,\tau) has no zeros or poles outside the stripe

    Nτ<(s)<Nτ.-N_{\tau}<\Re(s)<N_{\tau}.

    Assume that r>Nτ+nr>N_{\tau}+n. Let ΦIndQH(τscχVcσ0)\varPhi\in\operatorname{Ind}_{Q}^{H}\left(\tau_{s}^{c}\chi_{V}^{c}\boxtimes\sigma_{0}^{\vee}\right). If Φ0\varPhi\neq 0, then there exists φ𝒮\varphi\in\mathscr{S} such that

    𝒯0(φΦ)0.\mathcal{T}_{0}(\varphi\otimes\varPhi)\neq 0.
Proof.

The proofs of the first two statements are totally the same as [GI16] Lemma 8.1 and Lemma 8.2. As for the proof of the last statement, it is also similar to Lemma 8.3 in Gan-Ichino’s paper; the only difference is that, we use the condition on rr to avoid the zeros or poles of the LL-function L(s,τ)L\left(s,\tau\right), whereas they use the tempered condition on the representations. ∎

Remark 3.2.

If we assume that τ\tau is an irreducble unitary representation of GLk(E)GL_{k}(E) of Arthur type, say, corresponding to a local AA-parameter

ψτ=iρiSaiSbi,\psi_{\tau}=\sum_{i}\rho_{i}\boxtimes S_{a_{i}}\boxtimes S_{b_{i}},

where ρi\rho_{i} is an irreducible representation of the Weil group WEW_{E} (with bounded image), SaiS_{a_{i}} is the aia_{i}-dimensional irreducible representation of the Weil-Deligne SL2SL_{2}, and SbiS_{b_{i}} is the bib_{i}-dimensional irreducible representation of the Arthur SL2SL_{2}. Then we have

L(s,τ)\displaystyle L(s,\tau) =L(s,ψτ)\displaystyle=L(s,\psi_{\tau})
=ij=1biL(s+ai12+bi+12j,ρi).\displaystyle=\prod_{i}\prod_{j=1}^{b_{i}}L\left(s+\frac{a_{i}-1}{2}+\frac{b_{i}+1}{2}-j,\rho_{i}\right).

It is easy to see that in this case, we can take a positive number NτN_{\tau} satisfying our requirements, such that

Nτ<k.N_{\tau}<k.

Moreover, from the above expression one can also see that the LL-function L(s,τ)L(s,\tau) has a pole at some real number if and only if there exists some ii, such that ρi=𝟙\rho_{i}=\mathbbm{1}.

Similarly, we can construct a backward G×HG\times H equivariant map

𝒯s:ωIndPG(τscχWcπ0)IndQH(τsχVσ0)\mathcal{T}^{\prime}_{s}:\omega\otimes\operatorname{Ind}_{P}^{G}\left(\tau_{s}^{c}\chi_{W}^{c}\boxtimes\pi_{0}^{\vee}\right)\longrightarrow\operatorname{Ind}_{Q}^{H}\left(\tau_{s}\chi_{V}\boxtimes\sigma_{0}\right)

and show some similar statements as the previous proposition. In summary, we have:

Corollary 3.3.

Let Nτ>0N_{\tau}>0 be a positive real number such that L(s,τ)L(s,\tau) has no zeros or poles outside the stripe

Nτ<(s)<Nτ.-N_{\tau}<\Re(s)<N_{\tau}.

Assume that r>Nτ+nr>N_{\tau}+n. Then the theta lift defines a bijection

JH(IndPG(τχWπ0))JH(IndQH(τχVσ0)).JH\left(\operatorname{Ind}_{P}^{G}\left(\tau\chi_{W}\boxtimes\pi_{0}\right)\right)\longleftrightarrow JH\left(\operatorname{Ind}_{Q}^{H}\left(\tau\chi_{V}\boxtimes\sigma_{0}\right)\right).

Here, we use JHJH to denote “The multi-set of irreducible constituents”.

Proof.

Let

𝒯0:ωIndQH(τcχVcσ0)IndPG(τχWπ0)\mathcal{T}_{0}:\omega\otimes\operatorname{Ind}_{Q}^{H}\left(\tau^{c}\chi_{V}^{c}\boxtimes\sigma_{0}^{\vee}\right)\longrightarrow\operatorname{Ind}_{P}^{G}\left(\tau\chi_{W}\boxtimes\pi_{0}\right)

be the G×HG\times H-equivariant map we constructed in Proposition 3.1, and

𝒯0:ωIndPG(τcχWcπ0)IndQH(τχVσ0)\mathcal{T}_{0}^{*}:\omega\otimes\operatorname{Ind}_{P}^{G}\left(\tau^{c}\chi_{W}^{c}\boxtimes\pi_{0}^{\vee}\right)\longrightarrow\operatorname{Ind}_{Q}^{H}\left(\tau\chi_{V}\boxtimes\sigma_{0}\right)

be the adjoint map associated to 𝒯0\mathcal{T}_{0}, defined by

𝒯0(φΦ),Ψ=𝒯0(φΨ),Φ,\left\langle\mathcal{T}_{0}^{*}\left(\varphi\otimes\varPhi^{\vee}\right),\varPsi^{\vee}\right\rangle=\left\langle\mathcal{T}_{0}\left(\varphi\otimes\varPsi^{\vee}\right),\varPhi^{\vee}\right\rangle,

where φ𝒮\varphi\in\mathscr{S},

ΦIndPG(τcχWcπ0)(IndPG(τχWπ0)),\varPhi^{\vee}\in\operatorname{Ind}_{P}^{G}\left(\tau^{c}\chi_{W}^{c}\boxtimes\pi_{0}^{\vee}\right)\simeq\left(\operatorname{Ind}_{P}^{G}\left(\tau\chi_{W}\boxtimes\pi_{0}\right)\right)^{\vee},

and

ΨIndQH(τcχVcσ0)(IndQH(τχVσ0)).\varPsi^{\vee}\in\operatorname{Ind}_{Q}^{H}\left(\tau^{c}\chi_{V}^{c}\boxtimes\sigma_{0}^{\vee}\right)\simeq\left(\operatorname{Ind}_{Q}^{H}\left(\tau\chi_{V}\boxtimes\sigma_{0}\right)\right)^{\vee}.

By Proposition 3.1, the map 𝒯0\mathcal{T}_{0}^{*} is surjective. Hence for any irreducible constituent σ\sigma of IndQH(τχVσ0)\operatorname{Ind}_{Q}^{H}\left(\tau\chi_{V}\boxtimes\sigma_{0}\right), we deduce that its theta lift π\pi to the group GG is an irreducible constituent of IndPG(τχWπ0)\operatorname{Ind}_{P}^{G}\left(\tau\chi_{W}\boxtimes\pi_{0}\right). Moreover, if we denote by

mQ(σ)=dimHomH(σ,IndQH(τχVσ0)),m_{Q}(\sigma)=\dim\operatorname{Hom}_{H}\left(\sigma,\operatorname{Ind}_{Q}^{H}\left(\tau\chi_{V}\boxtimes\sigma_{0}\right)\right),

and

mP(π)=dimHomG(π,IndPG(τχWπ0)),m_{P}(\pi)=\dim\operatorname{Hom}_{G}\left(\pi,\operatorname{Ind}_{P}^{G}\left(\tau\chi_{W}\boxtimes\pi_{0}\right)\right),

then the surjectivity also implies that

mQ(σ)mP(π).m_{Q}(\sigma)\leq m_{P}(\pi).

Similarly, use the backward G×HG\times H-equivariant map

𝒯0:ωIndPG(τcχWcπ0)IndQH(τχVσ0),\mathcal{T}^{\prime}_{0}:\omega\otimes\operatorname{Ind}_{P}^{G}\left(\tau^{c}\chi_{W}^{c}\boxtimes\pi_{0}^{\vee}\right)\longrightarrow\operatorname{Ind}_{Q}^{H}\left(\tau\chi_{V}\boxtimes\sigma_{0}\right),

we can prove a reverse inequality. This completes the proof. ∎

4. Preparations

In this section we recall some basic facts we shall need in later proofs.

4.1. Explicit construction of Arthur packets à la Mœglin

We first recall some results due to Mœglin in [Mœg11b]. Readers may also consult the paper [Xu17a]. We emphasize that our proof of Theorem 2.8 relies on these results.

In this subsection, we temporarily let G=G(W)G=G(W) be either an even orthogonal, or a symplectic, or an unitary group; i.e. WW is an orthogonal, or symplectic, or Hermitian space, and GG is the isometry group of WW. Assume that GG is quasi-split. We fix a Whittaker datum 𝒲\mathscr{W} of GG. Let ψ\psi be a local AA-parameter for GG. Recall that a local AA-parameter can be regarded as a formal sum

ψ=iρiSaiSbi\psi=\sum_{i}\rho_{i}\boxtimes S_{a_{i}}\boxtimes S_{b_{i}}

satisfies certain properties; where ρi\rho_{i} is an irreducible representation of the Weil group WEW_{E} (with bounded image), SaiS_{a_{i}} is the aia_{i}-dimensional irreducible representation of the Weil-Deligne SL2SL_{2}, and SbiS_{b_{i}} is the bib_{i}-dimensional irreducible representation of the Arthur SL2SL_{2}.

Definition 4.1.
  1. (1)

    ψ\psi is said to be of good parity, if for every ii, ρiSaiSbi\rho_{i}\boxtimes S_{a_{i}}\boxtimes S_{b_{i}} is (conjugate) self-dual and of the same parity with ψ\psi;

  2. (2)

    ψ\psi is said to have discrete diagonal restriction (“DDR” for short), if the pull-back of ψ\psi along the diagonal map

    Δ:WE×SL2()\displaystyle\Delta:W_{E}\times SL_{2}(\mathbb{C}) WE×SL2()×SL2(),\displaystyle\longrightarrow W_{E}\times SL_{2}(\mathbb{C})\times SL_{2}(\mathbb{C}),
    (w,x)\displaystyle(w,x) (w,x,x),\displaystyle\longmapsto(w,x,x),

    denoted by ψd\psi_{d}, is a discrete LL-parameter for GG;

  3. (3)

    ψ\psi is said to be elementary, if it has DDR, and for every ii, either aia_{i} or bib_{i} is 11.

For ψΨ(G)\psi\in\Psi(G) and η𝒮ψ¯^\eta\in\widehat{\overline{\mathcal{S}_{\psi}}}, Mœglin constructed a finite-length semi-simple smooth representation πM(ψ,η)\pi_{M}(\psi,\eta) of GG. She showed that ΠψA(G)\Pi_{\psi}^{A}(G) consists of πM(ψ,η)\pi_{M}(\psi,\eta) for all η𝒮ψ¯^\eta\in\widehat{\overline{\mathcal{S}_{\psi}}}, and by studying their properties she was able to conclude that (cf. [Xu17a] Theorem 8.9):

Theorem 4.2.

ΠψA(G)\Pi_{\psi}^{A}(G) is multiplicity-free. Moreover, there exist a character ηψM/A𝒮ψ¯^\eta_{\psi}^{M/A}\in\widehat{\overline{\mathcal{S}_{\psi}}}, such that for any η𝒮ψ¯^\eta\in\widehat{\overline{\mathcal{S}_{\psi}}},

πM(ψ,η)=πA(ψ,ηηψM/A).\pi_{M}(\psi,\eta)=\pi_{A}(\psi,\eta\cdot\eta_{\psi}^{M/A}).

Here πA(ψ,η)\pi_{A}(\psi,\eta) is Arthur’s parametrization.

Remark 4.3.

Notice that both Mœglin’s and Arthur’s parametrizations of local AA-packets depend on the choice of Whittaker datum!

There are several steps in Mœglin’s explicit construction. The starting point is the elementary AA-parameters, whose associated AA-packets are constructed by using some generalized Aubert involutions. Two facts about the local AA-packets of elementary type are remarkable to us. The first one is about supercuspidal representations. Recall we have the following parametrization of supercuspidal representations of GG, which is also due to Mœglin (cf. [Mœg11b] Théorème 1.5.1, or [Xu17b] Theorem 3.3).

Theorem 4.4.

Under the local Langlands correspondence for GG established by Arthur/ Mok, the irreducible supercuspidal representations of GG are parametrized by ϕΦ2(G)\phi\in\Phi_{2}(G) and η𝒮ϕ¯^\eta\in\widehat{\overline{\mathcal{S}_{\phi}}}, satisfying the following properties

  1. (1)

    (Chain condition) if ρSaϕ\rho\boxtimes S_{a}\subset\phi, then ρSa2ϕ\rho\boxtimes S_{a-2}\subset\phi as long as a2>0a-2>0;

  2. (2)

    (Alternating condition) if ρSa,ρSa2ϕ\rho\boxtimes S_{a},\rho\boxtimes S_{a-2}\subset\phi, then

    η(xρ,a)η(xρ,a2)=1,\eta(x_{\rho,a})\cdot\eta(x_{\rho,a-2})=-1,

    where xρ,ax_{\rho,a} is the element in 𝒮ϕ\mathcal{S}_{\phi} which corresponds to ρSa\rho\boxtimes S_{a};

  3. (3)

    (Initial condition) if ρS2ϕ\rho\boxtimes S_{2}\subset\phi, then η(xρ,2)=1\eta(x_{\rho,2})=-1.

According to Mœglin’s construction, we have (cf. [Xu17a] Definition 6.3)

Lemma 4.5.

Assume that ψΨ(G)\psi\in\Psi(G) is elementary, and η𝒮ψ¯^\eta\in\widehat{\overline{\mathcal{S}_{\psi}}}. If (ψd,η)(\psi_{d},\eta) is a pair parametrizing a supercuspidal representation (i.e. satisfies conditions listed in the previous theorem, here we identify 𝒮ψ\mathcal{S}_{\psi} and 𝒮ψd\mathcal{S}_{\psi_{d}} in the obvious way), then

πM(ψ,η)=πA(ψd,η)\pi_{M}(\psi,\eta)=\pi_{A}(\psi_{d},\eta)

is supercuspidal.

The second remarkable fact is (cf. [Xu17a] Theorem 6.1)

Lemma 4.6.

Assume that ψΨ(G)\psi\in\Psi(G) is elementary. Then the map

𝒥𝒲A:ΠψA(G)𝒮ψ¯^\mathcal{J}_{\mathscr{W}}^{A}:\Pi_{\psi}^{A}(G)\longrightarrow\widehat{\overline{\mathcal{S}_{\psi}}}

is a bijection.

The next step is to construct AA-packets in the DDR case based on the elementary case by taking certain socles. Having the DDR case at hand, the AA-packets in the good parity case can be constructed based on the DDR case, by taking a sequence of partial Jacquet modules. To be more precise, we briefly describe this procedure.

Let ψ\psi be a local AA-parameter for GG which is of good parity, we write

ψ=iψi,\psi=\sum_{i}\psi_{i},

where the ψi=ρiSaiSbi\psi_{i}=\rho_{i}\boxtimes S_{a_{i}}\boxtimes S_{b_{i}} occuring in this sum are not necessarily distinct one from each other. We denote by IψI_{\psi} the index set of this summation. For each iIψi\in I_{\psi}, put

ζi={+1if aibi;1if ai<bi.\zeta_{i}=\begin{cases}+1\quad&\textit{if }a_{i}\geq b_{i};\\ -1\quad&\textit{if }a_{i}<b_{i}.\end{cases}

Let ρ\rho be an irreducible (conjugate) self-dual representation of WEW_{E}, we set

Iψ,ρ={iIψ|ρiρ}.I_{\psi,\rho}=\left\{i\in I_{\psi}~{}\big{|}~{}\rho_{i}\simeq\rho\right\}.
Definition 4.7.
  1. (1)

    A total order >ψ,ρ>_{\psi,\rho} on Iψ,ρI_{\psi,\rho} is said to be an admissible order on Iψ,ρI_{\psi,\rho} if it satisfies the following condition:

    For i,jIψ,ρ, if ai+bi>aj+bj|aibi|>|ajbj|, and ζi=ζj, then i>ψ,ρj.\quad\bullet~{}\textit{For $i,j\in I_{\psi,\rho}$, if $a_{i}+b_{i}>a_{j}+b_{j}$, $|a_{i}-b_{i}|>|a_{j}-b_{j}|$, and $\zeta_{i}=\zeta_{j}$, then $i>_{\psi,\rho}j$.}

    A partial order >ψ>_{\psi} on IψI_{\psi} is said to be an admissible order on IψI_{\psi} if its restriction to Iψ,ρI_{\psi,\rho} is an admissible order on Iψ,ρI_{\psi,\rho} for any irreducible (conjugate) self-dual representation ρ\rho of WEW_{E}.

  2. (2)

    Let WW^{\gg} be a space in the Witt tower containing WW, and G=G(W)G_{\gg}=G(W^{\gg}). We say that a local AA-parameter ψ\psi_{\gg} for GG_{\gg} dominates ψ\psi with respect to the admissible order >ψ>_{\psi}, if

    ψ=iρiSaiSbi,\psi_{\gg}=\sum_{i}\rho_{i}\boxtimes S_{a^{\prime}_{i}}\boxtimes S_{b^{\prime}_{i}},

    where the summation runs over iIψi\in I_{\psi}, such that for each iIψi\in I_{\psi}, we have

    (ai,bi)={(ai+2ti,bi)if ζi=+1;(ai,bi+2ti)if ζi=1\left(a^{\prime}_{i},b^{\prime}_{i}\right)=\begin{cases}\left(a_{i}+2t_{i},b_{i}\right)\quad&\textit{if }\zeta_{i}=+1;\\ \left(a_{i},b_{i}+2t_{i}\right)\quad&\textit{if }\zeta_{i}=-1\end{cases}

    for some non-negative integer tit_{i}, and >ψ>_{\psi} is also an admissible order for ψ\psi_{\gg}.

Remark 4.8.
  1. (1)

    For any ψΨ(G)\psi\in\Psi(G) of good parity, there exists at least one admissible order >ψ>_{\psi} on IψI_{\psi}. Moreover, if ψ\psi has DDR, then there is an admissible order >ψ>_{\psi} on IψI_{\psi}, such that for any i,jIψ,ρi,j\in I_{\psi,\rho}, we have i>ψji>_{\psi}j if and only if ai+bi>aj+bja_{i}+b_{i}>a_{j}+b_{j}. Admissible orders satisfying this condition are called “natural order”.

  2. (2)

    For any ψΨ(G)\psi\in\Psi(G) of good parity, let >ψ>_{\psi} be an admissible order on IψI_{\psi}. Then there exists a group GG_{\gg}, together with a local AA-parameter ψ\psi_{\gg}, such that

    • ψ\psi_{\gg} has DDR;

    • ψ\psi_{\gg} dominates ψ\psi with respect to the admissible order >ψ>_{\psi};

    • >ψ>_{\psi} is a natural order for ψ\psi_{\gg}.

Now, given ψΨ(G)\psi\in\Psi(G) of good parity, let >ψ>_{\psi} be an admissible order on IψI_{\psi}, and ψ\psi_{\gg} a local AA-parameter has DDR for some group GG_{\gg}, such that ψ\psi_{\gg} dominates ψ\psi with respect to the admissible order >ψ>_{\psi}. We have the following deep theorem due to Mœglin (cf. [Mœg10] Proposition 2.8.1, or [Xu17a] Proposition 8.5):

Theorem 4.9.
  1. (1)

    For πΠψA(G)\pi_{\gg}\in\Pi_{\psi_{\gg}}^{A}(G_{\gg}), let

    π=iIψJacXiπ,\pi=\circ_{i\in I_{\psi}}Jac_{X_{i}^{\gg}}\pi_{\gg},

    where the composition is taken in the decreasing order with respect to >ψ>_{\psi}, and the symbol JacXiJac_{X_{i}^{\gg}} means applying partial Jacquet module Jacρi||xJac_{\rho_{i}|\cdot|^{x}} (cf. [Xu17a] page 897) consecutively for xx ranging over the generalized segment

    Xi=(aibi2aibi2+ζi(ai+bi21)ζiai+bi2ζi)X_{i}^{\gg}=\left(\begin{array}[]{ccc}\frac{a^{\prime}_{i}-b^{\prime}_{i}}{2}&\cdots&\frac{a_{i}-b_{i}}{2}+\zeta_{i}\\ \vdots&{}\hfil&\vdots\\ \left(\frac{a^{\prime}_{i}+b^{\prime}_{i}}{2}-1\right)\zeta_{i}&\cdots&\frac{a_{i}+b_{i}}{2}\zeta_{i}\end{array}\right)

    from top to bottom and from left to right, i.e.

    JacXi=(Jacρi||ai+bi2ζiJacρi||aibi2+ζi)(Jacρi||ai+bi2ζiζiJacρi||aibi2).Jac_{X_{i}^{\gg}}=\left(Jac_{\rho_{i}|\cdot|^{\frac{a_{i}+b_{i}}{2}\zeta_{i}}}\circ\cdots\circ Jac_{\rho_{i}|\cdot|^{\frac{a_{i}-b_{i}}{2}+\zeta_{i}}}\right)\circ\cdots\circ\left(Jac_{\rho_{i}|\cdot|^{\frac{a^{\prime}_{i}+b^{\prime}_{i}}{2}\zeta_{i}-\zeta_{i}}}\circ\cdots\circ Jac_{\rho_{i}|\cdot|^{\frac{a^{\prime}_{i}-b^{\prime}_{i}}{2}}}\right).

    Then π\pi is either zero or irreducible.

  2. (2)

    As a set, the local AA-packet of GG associated to the AA-parameter ψ\psi is

    ΠψA(G)={π=iIψJacXiπ|πΠψA(G)}\{0}.\Pi_{\psi}^{A}(G)=\left\{\pi=\circ_{i\in I_{\psi}}Jac_{X_{i}^{\gg}}\pi_{\gg}~{}\big{|}~{}\pi_{\gg}\in\Pi_{\psi_{\gg}}^{A}(G_{\gg})\right\}\Big{\backslash}\left\{0\right\}.

    The definition of ΠψA(G)\Pi_{\psi}^{A}(G) is indeed independent of the choice of GG_{\gg} and ψ\psi_{\gg}, as well as the admissible order >ψ>_{\psi}.

Finally the AA-packet associated to a general ψ\psi can be constructed from the good parity case by using parabolic inductions. For this part, readers may also consult [Art13] Proposition 2.4.3, or [Mok15] Proposition 3.4.4.

4.2. Globalizations

Since in our later proofs we heavily use global methods, in this subsection, we collect some results on globalizing local data.

Lemma 4.10.

Let (F˙,E˙)(\dot{F},\dot{E}) be a pair of number fields, and uu is a place of F˙\dot{F}, such that (F˙u,E˙u)(F,E)(\dot{F}_{u},\dot{E}_{u})\simeq(F,E). We require that F˙\dot{F} has enough real places in the case E˙=F˙\dot{E}=\dot{F}. Let SS be a finite set of non-Archimedean places of F˙\dot{F} not containing uu. Let mm be a positive integer. Fix κ=±1\kappa=\pm 1. For each place vS{u}v\in S\cup\{u\}, let ϕv\phi_{v} be a discrete mm-dimensional (conjugate) self-dual representation of LE˙vL_{\dot{E}_{v}} with parity κ\kappa. Then there exists an irreducible cuspidal automorphic representation ϕ˙\dot{\phi} of GLm(𝔸E˙)GL_{m}(\mathbb{A}_{\dot{E}}), such that the following conditions hold:

  1. (1)

    ϕ˙\dot{\phi} is (conjugate) self-dual with parity κ\kappa;

  2. (2)

    for each place vS{u}v\in S\cup\{u\}, ϕ˙v=ϕv\dot{\phi}_{v}=\phi_{v}.

Proof.

In Case OO, this is follows from [Art13] Lemma 6.2.2. In Case UU, this follows from [Shi12] Theorem 5.13. (In Case UU, readers may also consult [GI16] Section 6.4; if F˙\dot{F} has enough real places different from uu, then this also follows from [Mok15] Lemma 7.2.3.) ∎

Remark 4.11.

Indeed, from the proof of this lemma, we can also allow SS to contain one Archimedean place.

As an application of this lemma, we deduce:

Corollary 4.12.

Assume that ψ\psi is a local AA-parameter of good parity for GG. Then, for any irreducible unitary representation π\pi in ΠψA(G)\Pi_{\psi}^{A}(G), there exist a tuple of data (F˙,E˙,G˙,π˙,ψ˙,u)(\dot{F},\dot{E},\dot{G},\dot{\pi},\dot{\psi},u), where

  • F˙\dot{F} is a number field, and E˙\dot{E} is either F˙\dot{F} itself or a quadratic extension of F˙\dot{F}, according to the case at hand;

  • G˙\dot{G} a quasi-split even orthogonal or symplectic or unitary group over F˙\dot{F}, according to the group GG; in the case that G˙\dot{G} is an unitary group, E˙\dot{E} is the splitting field of G˙\dot{G};

  • π˙\dot{\pi} is an automorphic representation occuring in the automorphic discrete spectrum of G˙\dot{G}, and ψ˙\dot{\psi} is the elliptic AA-parameter associated to π˙\dot{\pi};

  • uu is a finite place of F˙\dot{F}.

such that the following condition holds

(F˙u,E˙u,G˙u,π˙u,ψ˙u)(F,E,G,π,ψ).(\dot{F}_{u},\dot{E}_{u},\dot{G}_{u},\dot{\pi}_{u},\dot{\psi}_{u})\simeq(F,E,G,\pi,\psi).
Proof.

First we choose a pair of number fields (F˙,E˙)(\dot{F},\dot{E}), together with two places uu and ww of F˙\dot{F}, satisfy the following properties:

  1. (1)

    (F˙u,E˙u)(F,E)(\dot{F}_{u},\dot{E}_{u})\simeq(F,E);

  2. (2)

    if GG is an even orthogonal or symplectic group, then F˙\dot{F} has enough real places, and F˙w\dot{F}_{w} is a finite extension of 2\mathbb{Q}_{2} with a sufficiently big residue field (this condition guarantees we will have enough irreducible orthogonal representations of WF˙wW_{\dot{F}_{w}}; see [CZ21] Appendix B);

  3. (2)(2^{\prime})

    if GG is an unitary group, then F˙w\dot{F}_{w} is a finite extension of p\mathbb{Q}_{p} for some p2p\neq 2 with a sufficiently big residue field, and E˙w\dot{E}_{w} is a ramified quadratic field extension of F˙w\dot{F}_{w} (this condition guarantees we will have enough irreducible conjugate self-dual representations of WE˙wW_{\dot{E}_{w}}, with any given parity; see [CZ21] Appendix C).

Let S={w}S=\{w\}. We write

ψ=iϕiSdi\psi=\sum_{i}\phi_{i}\boxtimes S_{d_{i}}

for some (not necessarily distinct) nin_{i}-dimensional irreducible (conjugate) self-dual representations of LE×SL2L_{E}\times SL_{2}. For each ii, we pick up an irreducible (conjugate) self-dual representations ρw,i\rho_{w,i} of WE˙wW_{\dot{E}_{w}}, with the same dimension and parity of ϕi\phi_{i}. Apply the Lemma 4.10, we can globalize ϕi\phi_{i} to an irreducible (conjugate) self-dual cuspidal representation ϕ˙i\dot{\phi}_{i} of GLni(𝔸E˙)GL_{n_{i}}(\mathbb{A}_{\dot{E}}) with the same parity as ϕi\phi_{i}, such that

  1. (1)

    (ϕ˙i)u=ϕi(\dot{\phi}_{i})_{u}=\phi_{i};

  2. (2)

    (ϕ˙i)w=ρw,iS1(\dot{\phi}_{i})_{w}=\rho_{w,i}\boxtimes S_{1}.

We require that when iii\neq i^{\prime}, ρw,i≄ρw,i\rho_{w,i}\not\simeq\rho_{w,i^{\prime}}. Let

ψ˙={i(ϕ˙iω˙)Sdiif G is symplectic;iϕ˙iSdiif G is even orthogonal or unitary,\dot{\psi}=\begin{cases}\sum_{i}\left(\dot{\phi}_{i}\cdot\dot{\omega}\right)\boxtimes S_{d_{i}}&\textit{if $G$ is symplectic};\\ \sum_{i}\dot{\phi}_{i}\boxtimes S_{d_{i}}\quad&\textit{if $G$ is even orthogonal or unitary},\end{cases}

where

ω˙=iω˙idi,\dot{\omega}=\prod_{i}\dot{\omega}_{i}^{d_{i}},

and ω˙i\dot{\omega}_{i} is the central character of ϕ˙i\dot{\phi}_{i}. If GG is a symplectic group, then ψ˙\dot{\psi} is already an elliptic AA-parameter for some symplectic group G˙\dot{G} over F˙\dot{F}. If GG is an even orthogonal or unitary group, since ψ˙\dot{\psi} is (conjugate) self-dual with the same parity as ψ\psi, at each place vv of F˙\dot{F} we can pick up a cc-Hermitian space VvV_{v}, such that G(Vv)G(V_{v}) is quasi-split, and ψ˙v\dot{\psi}_{v} is a local AA-parameter for the group G(Vv)G(V_{v}). It follows from the local-global principle for orthogonal or unitary groups that the collection {Vv}v\{V_{v}\}_{v} indeed form a cc-Hermitian space V˙\dot{V} over E˙\dot{E}. In this case we put G˙=G(V˙)\dot{G}=G(\dot{V}). Then G˙\dot{G} is quasi-split, and ψ˙\dot{\psi} is an elliptic AA-parameter for G˙\dot{G}. Notice that

ψ˙w=iρw,iS1Sdi\dot{\psi}_{w}=\sum_{i}\rho_{w,i}\boxtimes S_{1}\boxtimes S_{d_{i}}

is elementary, and the localization map

ιw:𝒮ψ˙𝒮ψ˙w\iota_{w}:\mathcal{S}_{\dot{\psi}}\longrightarrow\mathcal{S}_{\dot{\psi}_{w}}

is an isomorphism.

Next we define an irreducible representation π˙\dot{\pi} as follows:

  • at a place v{u,w}v\notin\{u,w\}, if G˙v\dot{G}_{v} and ψ˙v\dot{\psi}_{v} are both unramified, then π˙v\dot{\pi}_{v} is the unramified representation of G˙v\dot{G}_{v} with LL-parameter ϕψ˙v\phi_{\dot{\psi}_{v}}; otherwise, let π˙v\dot{\pi}_{v} be an arbitrarily given representation of G˙v\dot{G}_{v} lying in the AA-packet Πψ˙vA(G˙v)\Pi_{\dot{\psi}_{v}}^{A}(\dot{G}_{v});

  • at the place uu, π˙u=π\dot{\pi}_{u}=\pi;

  • at the place ww, π˙w=πA(ψ˙w,ηw)\dot{\pi}_{w}=\pi_{A}\left(\dot{\psi}_{w},\eta_{w}\right), where ηw\eta_{w} is the character of 𝒮ψ˙w\mathcal{S}_{\dot{\psi}_{w}}, determined by the formula

    vηv=ϵψ˙,\prod_{v}\eta_{v}=\epsilon_{\dot{\psi}},

    where ηv=𝒥𝒲A(π˙v)\eta_{v}=\mathcal{J}_{\mathscr{W}}^{A}(\dot{\pi}_{v}), and ϵψ˙\epsilon_{\dot{\psi}} is the canonical sign character associated to ψ˙\dot{\psi}. It follows from Lemma 4.6 that π˙w0\dot{\pi}_{w}\neq 0.

Then, according to the Arthur’s multiplicity formula for G˙\dot{G}, π˙\dot{\pi} is an irreducible subrepresentation of Lψ˙2(G˙)L^{2}_{\dot{\psi}}(\dot{G}). One can easily check that the tuple of data (F˙,E˙,G˙,π˙,ψ˙,u)(\dot{F},\dot{E},\dot{G},\dot{\pi},\dot{\psi},u) satisfies all our requirements. ∎

5. Comparison of packets from different level as sets

From now we let FF be a non-Archimedean local field of characteristic 0. In this section, we shall prove that as a set, the definition of the θ\theta-packets (see Section 2.5) is independent of the choice of H=H(W(r))H=H(W_{(r)}). The word “level” in the title of this section refers to the integer rr, i.e. the “level” in the Witt tower.

5.1. First properties

Before we start to prove, we develop some first properties of Πψθ(G)\Pi_{\psi}^{\theta}(G).

Lemma 5.1.

Πψθ(G)\Pi_{\psi}^{\theta}(G) is multiplicity-free. Hence we can regard Πψθ(G)\Pi_{\psi}^{\theta}(G) as a subset of Irrunit(G)\operatorname{Irr}_{unit}(G).

Proof.

This is simply follows from the Howe duality and that Πθ(ψ)A(H)\Pi_{\theta(\psi)}^{A}(H) is multiplicity-free. ∎

Consider the theta lift between (G,H)(G,H) for all pure inner form GG of GG^{*} simultaneously, we get

Proposition 5.2.

Suppose ψ\psi is a local AA-parameter of good parity for GG^{*}. Then the theta lift provide us a bijection of sets

θ:Πθ(ψ)A(H)Πψθ(G),\theta:\Pi_{\theta(\psi)}^{A}(H)\longrightarrow\bigsqcup\Pi_{\psi}^{\theta}(G),

where the disjoint union on the RHS of the arrow runs over all pure inner forms GG of GG^{*}.

Proof.

First we construct this map, i.e. we need to show that, for any irreducible representation σΠθ(ψ)A(H)\sigma\in\Pi_{\theta(\psi)}^{A}(H), there is a pure inner form GG of GG^{*}, such that the theta lift of σ\sigma to GG is non-zero. Applying Lemma 4.10, we globalize the tuple of local data (F,E,V+,W,ψ,ψF,χV,χW)(F,E,V^{+},W,\psi,\psi_{F},\chi_{V},\chi_{W}) to a tuple global data

(F˙,E˙,V˙+,W˙,ψ˙,ψF˙,χV˙,χW˙),(\dot{F},\dot{E},\dot{V}^{+},\dot{W},\dot{\psi},\psi_{\dot{F}},\chi_{\dot{V}},\chi_{\dot{W}}),

where

  • F˙\dot{F} is a number field, and E˙\dot{E} is either F˙\dot{F} itself or a quadratic extension of F˙\dot{F}, according the cases;

  • V˙+\dot{V}^{+} is a cc-Hermitian space over E˙\dot{E} so that G˙=G(V˙+)\dot{G}^{*}=G(\dot{V}^{+}) is quasi-split;

  • W˙\dot{W} is the split cc-skew-Hermitian space over E˙\dot{E}, in particular H˙=H(W˙)\dot{H}=H(\dot{W}) is also quasi-split;

  • ψ˙\dot{\psi} is an elliptic AA-parameter of G˙\dot{G}^{*};

  • (ψF˙,χV˙,χW˙)(\psi_{\dot{F}},\chi_{\dot{V}},\chi_{\dot{W}}) is a tuple of auxiliary data allow us to define the theta lift between (G˙,H˙)(\dot{G}^{*},\dot{H});

together with two places uu and ww of F˙\dot{F}, such that

  1. (1)

    (F˙u,E˙u,V˙u+,W˙u,ψ˙u,ψF˙u,χV˙u,χW˙u)(F,E,V+,W,ψ,ψF,χV,χW)(\dot{F}_{u},\dot{E}_{u},\dot{V}^{+}_{u},\dot{W}_{u},\dot{\psi}_{u},\psi_{\dot{F}_{u}},\chi_{\dot{V}_{u}},\chi_{\dot{W}_{u}})\simeq(F,E,V^{+},W,\psi,\psi_{F},\chi_{V},\chi_{W});

  2. (2)

    at the place ww, ψ˙w\dot{\psi}_{w} is elementary, and the localization map

    ιw:𝒮ψ˙𝒮ψ˙w\iota_{w}:\mathcal{S}_{\dot{\psi}}\longrightarrow\mathcal{S}_{\dot{\psi}_{w}}

    is an isomorphism.

For any irreducible unitary representation σΠθ(ψ)A(H)\sigma\in\Pi_{\theta(\psi)}^{A}(H), similar to the proof of Corollary 4.12, by using the Arthur’s multiplicity formula for H˙\dot{H}, we may globalize σ\sigma to an irreducible subrepresentation σ˙\dot{\sigma} of Lθ(ψ˙)2(H˙)L^{2}_{\theta(\dot{\psi})}(\dot{H}), where

θ(ψ˙)=ψ˙χW˙1χV˙+χV˙S2r2n+1\theta(\dot{\psi})=\dot{\psi}\chi_{\dot{W}}^{-1}\chi_{\dot{V}}+\chi_{\dot{V}}\boxtimes S_{2r-2n+1}

is an elliptic AA-parameter for the group H˙\dot{H}. It then follows from J-S. Li’s work on low rank representations (Theorem 2.3) that σ˙\dot{\sigma} is of rank dimV\dim V, and so is σ\sigma. Indeed, J-S. Li’s results also assert that there exists a pure inner form G˙\dot{G} of G˙\dot{G}^{*}, together with an automorphic representation π˙\dot{\pi} of G˙\dot{G}, such that σ˙\dot{\sigma} is the theta lift of π˙\dot{\pi}. We set

σπ˙u.\sigma\longmapsto\dot{\pi}_{u}.

This gives us the desired map. Notice that π˙u\dot{\pi}_{u} is nothing but the theta lift of σ\sigma to G˙u\dot{G}_{u}. Hence by the conservation relation [SZ15], this map is well-defined and independent of the globalization. The injectivity of this map then follows from the Howe duality principle, and the surjectivity simply follows from the definition of the θ\theta-packets. ∎

Let V~=Vk\widetilde{V}=V\oplus\mathcal{H}^{k}, where \mathcal{H} is the cc-Hermitian hyperbolic plane. We can decompose V~\widetilde{V} as

V~=X+V+X,\widetilde{V}=X+V+X^{*},

where XX and XX^{*} are kk-dimensional totally isotropic subspaces of V~\widetilde{V} such that XXkX\oplus X^{*}\simeq\mathcal{H}^{k} and orthogonal to VV. Let PP be the maximal parabolic subgroup of G~=G(V~)\widetilde{G}=G(\widetilde{V}) stabilizing XX and MM be its Levi component stabilizing XX^{*}, so that

MGL(X)×G.M\simeq GL(X)\times G.

For an irreducible unitary representation τ\tau of GLk(E)GL_{k}(E) of Arthur type corresponding to an AA-parameter ψτ\psi_{\tau}, we consider the induced representation

IndPG~(τχWΠψθ(G)).\operatorname{Ind}_{P}^{\widetilde{G}}\Big{(}\tau\chi_{W}\boxtimes\Pi_{\psi}^{\theta}(G)\Big{)}.
Lemma 5.3.

Assume that r>dimV+kr>\dim V+k. Then

IndPG~(τχWΠψθ(G))\operatorname{Ind}_{P}^{\widetilde{G}}\Big{(}\tau\chi_{W}\boxtimes\Pi_{\psi}^{\theta}(G)\Big{)}

is semi-simple and multiplicity-free as a representation of G~\widetilde{G}.

Proof.

The semi-simplicity simply follows from the unitaricity. We now prove the multiplicity-freeness. Let Nτ>0N_{\tau}>0 be a positive number such that L(s,τ)L(s,\tau) has no zeros or poles outside the stripe

Nτ<(s)<Nτ.-N_{\tau}<\Re(s)<N_{\tau}.

Since τ\tau is of Arthur type, we may take Nτ<kN_{\tau}<k. Hence all the requirements in Corollary 3.3 are satisfied. Let W~=Wk\widetilde{W}=W\oplus\mathcal{H}^{\prime k}, where \mathcal{H}^{\prime} is the cc-skew-Hermitian hyperbolic plane. We can decompose W~\widetilde{W} as

W~=Y+W+Y,\widetilde{W}=Y+W+Y^{*},

where YY and YY^{*} are kk-dimensional totally isotropic subspaces of W~\widetilde{W} such that YYkY\oplus Y^{*}\simeq\mathcal{H}^{\prime k} and orthogonal to WW. Let QQ be the maximal parabolic subgroup of H~=H(W~)\widetilde{H}=H(\widetilde{W}) stabilizing YY and NN be its Levi component stabilizing YY^{*}, so that

NGL(Y)×H.N\simeq GL(Y)\times H.

By Corollary 3.3, for each πΠψθ(G)\pi\in\Pi_{\psi}^{\theta}(G), the theta lift between G~×H~\widetilde{G}\times\widetilde{H} defines a bijection

JH(IndPG~(τχWπ))JH(IndQH~(τχVσ)),JH\left(\operatorname{Ind}_{P}^{\widetilde{G}}\left(\tau\chi_{W}\boxtimes\pi\right)\right)\longleftrightarrow JH\left(\operatorname{Ind}_{Q}^{\widetilde{H}}\left(\tau\chi_{V}\boxtimes\sigma\right)\right),

where σ\sigma is the (small) theta lift of π\pi to HH. By the construction, σΠθ(ψ)A(H)\sigma\in\Pi_{\theta(\psi)}^{A}(H). Add up all πΠψθ(G)\pi\in\Pi_{\psi}^{\theta}(G) together, we obtain an injection

JH(IndPG~(τχWΠψθ(G)))JH(IndQH~(τχVΠθ(ψ)A(H))).JH\left(\operatorname{Ind}_{P}^{\widetilde{G}}\left(\tau\chi_{W}\boxtimes\Pi_{\psi}^{\theta}(G)\right)\right)\longrightarrow JH\left(\operatorname{Ind}_{Q}^{\widetilde{H}}\left(\tau\chi_{V}\boxtimes\Pi_{\theta(\psi)}^{A}(H)\right)\right).

Hence in order to show the multiplicity-freeness of the LHS, it is sufficient to show the RHS is multiplicity-free. Let

ψ~=ψτχW+ψ+(ψτχW),\widetilde{\psi}=\psi_{\tau}\chi_{W}+\psi+\left(\psi_{\tau}\chi_{W}\right)^{\vee},

and

θ(ψ~)=ψτχV+θ(ψ)+(ψτχV).\theta(\widetilde{\psi})=\psi_{\tau}\chi_{V}+\theta(\psi)+(\psi_{\tau}\chi_{V})^{\vee}.

Then according to [Art13] Proposition 2.4.3 (or [Mok15] Proposition 3.4.4), we have

IndQH~(τχVΠθ(ψ)A(H))=Πθ(ψ~)A(H~)\operatorname{Ind}_{Q}^{\widetilde{H}}\Big{(}\tau\chi_{V}\boxtimes\Pi_{\theta(\psi)}^{A}(H)\Big{)}=\Pi_{\theta(\widetilde{\psi})}^{A}(\widetilde{H})

as representations of H~\widetilde{H}. By Theorem 4.2, as a representation of H~\widetilde{H}, Πθ(ψ~)A(H~)\Pi_{\theta(\widetilde{\psi})}^{A}(\widetilde{H}) is multiplicity-free. Therefore IndPG~(τχWΠψθ(G))\operatorname{Ind}_{P}^{\widetilde{G}}\Big{(}\tau\chi_{W}\boxtimes\Pi_{\psi}^{\theta}(G)\Big{)} is also multiplicity-free. ∎

Under the hypothesis of Lemma 5.3, we deduce

Corollary 5.4.

Suppose ψ\psi is a local AA-parameter of good parity for GG^{*}, and all requirements in Lemma 5.3 are satisfied. We retain the notations in the proof of Lemma 5.3. Then

Πψ~θ,r+k(G~)=IndPG~(τχWΠψθ,r(G))\Pi_{\widetilde{\psi}}^{\theta,r+k}(\widetilde{G})=\operatorname{Ind}_{P}^{\widetilde{G}}\Big{(}\tau\chi_{W}\boxtimes\Pi_{\psi}^{\theta,r}(G)\Big{)}

as representations of G~\widetilde{G}. In particular, Proposition 5.2 also holds for general AA-parameters.

Proof.

This is a simple combination of the Corollary 3.3, Proposition 5.2 and the proof of the Lemma 5.3. ∎

Now we specialize to the case that G=GG=G^{*} is quasi-split.

Proposition 5.5.

Suppose ψ\psi is a local AA-parameter of good parity for GG^{*}. Then as subsets of Irrunit(G)\operatorname{Irr}_{unit}(G^{*}), we have

ΠψA(G)Πψθ(G).\Pi_{\psi}^{A}(G^{*})\subset\Pi_{\psi}^{\theta}(G^{*}).
Proof.

First we apply Lemma 4.12 to the irreducible unitary representation πΠψA(G)\pi\in\Pi_{\psi}^{A}(G^{*}). We obtain a tuple of global data (F˙,E˙,G˙,π˙,ψ˙,u)(\dot{F},\dot{E},\dot{G},\dot{\pi},\dot{\psi},u). We also globalize the tuple of local auxiliary data (ψF,χV,χW)(\psi_{F},\chi_{V},\chi_{W}) in the definition of the local theta lift to a global tuple (ψF˙,χV˙,χW˙)(\psi_{\dot{F}},\chi_{\dot{V}},\chi_{\dot{W}}). Let W˙\dot{W} be the split cc-skew-Hermitian space over E˙\dot{E} with the same dimension as WW. Put H˙=H(W˙)\dot{H}=H(\dot{W}). Consider the abstract theta lift σ˙=θabs(π˙)\dot{\sigma}=\theta^{abs}(\dot{\pi}) of π˙\dot{\pi} to H˙\dot{H}. Since mdisc(π˙)1m_{disc}(\dot{\pi})\geq 1, we deduce from J-S. Li’s inequality that mdisc(σ˙)1m_{disc}(\dot{\sigma})\geq 1. Hence, Arthur/ Mok has attached an elliptic AA-parameter ψ˙H\dot{\psi}_{H} to σ˙\dot{\sigma}.

We claim that ψ˙H\dot{\psi}_{H} is of the form ψ˙H=θ(ψ˙)\dot{\psi}_{H}=\theta(\dot{\psi}), where

θ(ψ˙)=ψ˙χW˙1χV˙+χV˙S2r2n+1.\theta(\dot{\psi})=\dot{\psi}\chi_{\dot{W}}^{-1}\chi_{\dot{V}}+\chi_{\dot{V}}\boxtimes S_{2r-2n+1}.

In fact, for almost all place vv of F˙\dot{F}, the LL-parameter of π˙v\dot{\pi}_{v} is ϕψ˙v\phi_{\dot{\psi}_{v}}; hence by the local theta correspondence for unramified representations, for almost all place vv of F˙\dot{F}, the LL-parameter of σ˙v\dot{\sigma}_{v} is

(5.1) ϕψ˙vχW˙,v1χV˙,v+(j=nrrn||j)χV˙,v.\phi_{\dot{\psi}_{v}}\chi_{\dot{W},v}^{-1}\chi_{\dot{V},v}+\left(\bigoplus_{j=n-r}^{r-n}|\cdot|^{j}\right)\chi_{\dot{V},v}.

It then follows that ψ˙H=θ(ψ˙)\dot{\psi}_{H}=\theta(\dot{\psi}). Therefore by the Arthur’s multiplicity formula for H˙\dot{H}, the localization of σ˙\dot{\sigma} at the place uu lies in the local AA-packet Πψ˙H,uA(H˙u)\Pi_{\dot{\psi}_{H,u}}^{A}(\dot{H}_{u}), i.e. we have

σΠθ(ψ)A(H),\sigma\in\Pi_{\theta(\psi)}^{A}(H),

which is equivalent to say that πΠψθ(G)\pi\in\Pi_{\psi}^{\theta}(G^{*}). ∎

Remark 5.6.

If we assume the same multiplicity-freeness result Theorem 4.2 hold for the Archimedean places, then we can show that this lemma is also true for Archimedean places.

5.2. A special class of parameters

In this subsection we deal with a special class of local AA-parameters. Let ψΨ(G)\psi\in\Psi(G) be a local AA-parameter. Suppose that the following hypothesis is satisfied:

Hypothesis 5.7.

There is a tuple of data (F˙,E˙,V˙+,ψ˙,u,w1,w2)(\dot{F},\dot{E},\dot{V}^{+},\dot{\psi},u,w_{1},w_{2}), where:

  • F˙\dot{F} is a number field, and E˙\dot{E} is either F˙\dot{F} itself or a quadratic extension of F˙\dot{F}, according to the cases at hand;

  • V˙+\dot{V}^{+} is a cc-Hermitian space over E˙\dot{E} so that G˙=G(V˙+)\dot{G}^{*}=G(\dot{V}^{+}) is quasi-split;

  • ψ˙\dot{\psi} is an elliptic AA-parameter of G˙\dot{G}^{*};

  • u,w1,w2u,w_{1},w_{2} are finite places of F˙\dot{F};

such that the following conditions hold:

  1. (1)

    (F˙u,E˙u,V˙u+,ψ˙u)(F,E,V+,ψ)(\dot{F}_{u},\dot{E}_{u},\dot{V}^{+}_{u},\dot{\psi}_{u})\simeq(F,E,V^{+},\psi);

  2. (2)

    ψ˙w1\dot{\psi}_{w_{1}} is elementary, and there exists ηw1𝒮ψ˙w1¯^\eta_{w_{1}}\in\widehat{\overline{\mathcal{S}_{\dot{\psi}_{w_{1}}}}}, such that πA(ψ˙w1,ηw1)\pi_{A}(\dot{\psi}_{w_{1}},\eta_{w_{1}}) is supercuspidal;

  3. (3)

    ψ˙w2\dot{\psi}_{w_{2}} is elementary, and the localization map

    ιw2:𝒮ψ˙𝒮ψ˙w2\iota_{w_{2}}:\mathcal{S}_{\dot{\psi}}\longrightarrow\mathcal{S}_{\dot{\psi}_{w_{2}}}

    is an isomorphism.

Let rr be any integer greater than dimV\dim V. Let W=W(r)W=W_{(r)}, and

θ(ψ)=ψχW1χV+χVS2r2n+1\theta(\psi)=\psi\chi_{W}^{-1}\chi_{V}+\chi_{V}\boxtimes S_{2r-2n+1}

be a local AA-parameter for H=H(W(r))H=H(W_{(r)}).

Proposition 5.8.

Suppose that the local AA-parameter ψ\psi satisfies the Hypothesis 5.7. Let π\pi be an irreducible unitary representation of GG, such that its small theta lift σ=θ(π)\sigma=\theta(\pi) to HH lies in the local AA-packet Πθ(ψ)A(H)\Pi_{\theta(\psi)}^{A}(H). Then there is a pair of data (G˙,π˙)(\dot{G},\dot{\pi}), where

  • G˙\dot{G} is a pure inner form of G˙\dot{G}^{*} over F˙\dot{F};

  • π˙\dot{\pi} is an automorphic representation occuring in the automorphic discrete spectrum of G˙\dot{G} with the elliptic AA-parameter ψ˙\dot{\psi};

such that π˙v=π\dot{\pi}_{v}=\pi. Moreover, if G=GG=G^{*} is quasi-split, we can take G˙=G˙\dot{G}=\dot{G}^{*}. Hence in this case, we have

πΠψA(G).\pi\in\Pi_{\psi}^{A}(G^{*}).
Proof.

We globalize the tuple of local auxiliary data (ψF,χV,χW)(\psi_{F},\chi_{V},\chi_{W}) in the definition of the local theta lift to a global tuple (ψF˙,χV˙,χW˙)(\psi_{\dot{F}},\chi_{\dot{V}},\chi_{\dot{W}}). Let W˙=W˙(r)\dot{W}=\dot{W}_{(r)} be the split cc-skew-Hermitian space over E˙\dot{E} with the same dimension as W=W(r)W=W_{(r)}. Put H˙=H(W˙)\dot{H}=H(\dot{W}). Let SS be a finite set of places of F˙\dot{F}, including uu, w1w_{1}, w2w_{2}, and all Archimedean places, such that for all vSv\notin S, the dual-pair G˙×H˙\dot{G}\times\dot{H}, the auxiliary data (ψF˙v,χV˙v,χW˙v)(\psi_{\dot{F}_{v}},\chi_{\dot{V}_{v}},\chi_{\dot{W}_{v}}), and the local AA-parameter ψ˙v\dot{\psi}_{v} are all unramified. We construct an automorphic representation σ˙\dot{\sigma} occuring in the automorphic discrete spectrum of H˙\dot{H} with elliptic AA-parameter

θ(ψ˙)=ψ˙χW˙1χV˙+χV˙S2r2n+1\theta(\dot{\psi})=\dot{\psi}\chi_{\dot{W}}^{-1}\chi_{\dot{V}}+\chi_{\dot{V}}\boxtimes S_{2r-2n+1}

as follows:

  • at a place vSv\notin S, σ˙v\dot{\sigma}_{v} is the unramified representation of H˙v\dot{H}_{v} with LL-parameter ϕθ(ψ˙v)\phi_{\theta(\dot{\psi}_{v})}; then, by the theta lift for unramified representations, it is clear that σ˙v=θ(πv)\dot{\sigma}_{v}=\theta(\pi_{v}), where πv\pi_{v} is the unramified representation of G˙v\dot{G}^{*}_{v} with LL-parameter ϕψ˙v\phi_{\dot{\psi}_{v}};

  • at a place vS\{u,w1,w2}v\in S\backslash\{u,w_{1},w_{2}\}, let πv\pi_{v} be an arbitrarily given representation of G˙v\dot{G}^{*}_{v} lying in the AA-packet Πψ˙vA(G˙v)\Pi_{\dot{\psi}_{v}}^{A}(\dot{G}^{*}_{v}), and σ˙v=θ(πv)\dot{\sigma}_{v}=\theta(\pi_{v}) is the theta lift of πv\pi_{v} to the group H˙v\dot{H}_{v}; similar to the proof of Proposition 5.5, one can show that σ˙vΠθ(ψ˙v)A(H˙v)\dot{\sigma}_{v}\in\Pi_{\theta(\dot{\psi}_{v})}^{A}(\dot{H}_{v}) by using some global arguments;

  • at the place uu, σ˙u=σ\dot{\sigma}_{u}=\sigma, which lies in Πθ(ψ˙u)A(H˙u)\Pi_{\theta(\dot{\psi}_{u})}^{A}(\dot{H}_{u}) by our assumptions;

  • at the place w1w_{1}, σ˙w1=θ(πA(ψ˙w1,ηw1))\dot{\sigma}_{w_{1}}=\theta\left(\pi_{A}(\dot{\psi}_{w_{1}},\eta_{w_{1}})\right), which lies in Πθ(ψ˙w1)A(H˙w1)\Pi_{\theta(\dot{\psi}_{w_{1}})}^{A}(\dot{H}_{w_{1}}) by Proposition 5.5;

  • at the place w2w_{2}, σ˙w2=πA(θ(ψ˙w2),ηw2)\dot{\sigma}_{w_{2}}=\pi_{A}\left(\theta(\dot{\psi}_{w_{2}}),\eta_{w_{2}}\right), where ηw2\eta_{w_{2}} is the character of 𝒮ψ˙w2\mathcal{S}_{\dot{\psi}_{w_{2}}}, determined by the formula

    vηv=ϵθ(ψ˙),\prod_{v}\eta_{v}=\epsilon_{\theta(\dot{\psi})},

    where ηv=𝒥𝒲A(σ˙v)\eta_{v}=\mathcal{J}_{\mathscr{W}^{\prime}}^{A}(\dot{\sigma}_{v}), and ϵθ(ψ˙)\epsilon_{\theta(\dot{\psi})} is the canonical sign character associated to θ(ψ˙)\theta(\dot{\psi}). It follows from Lemma 4.6 that σ˙w20\dot{\sigma}_{w_{2}}\neq 0.

Then, according to the Arthur’s multiplicity formula for H˙\dot{H}, σ˙\dot{\sigma} is an irreducible subrepresentation of Lθ(ψ˙)2(H˙)L^{2}_{\theta(\dot{\psi})}(\dot{H}). By J-S. Li’s work on low rank representations (Theorem 2.3), there is an unique pure inner form G˙\dot{G} of G˙\dot{G}^{*} and an automorphic representation π˙\dot{\pi} of G˙\dot{G}, such that

σ˙=θabs(π˙).\dot{\sigma}=\theta^{abs}(\dot{\pi}).

Also, by our construction, π˙w1=πA(ψ˙w1,ηw1)\dot{\pi}_{w_{1}}=\pi_{A}(\dot{\psi}_{w_{1}},\eta_{w_{1}}) is supercuspidal. This forces any automorphic realization of π˙\dot{\pi} to be cuspidal. Hence π˙\dot{\pi} lies in the automorphic discrete spectrum of G˙\dot{G}, with elliptic AA-parameter ψ˙\dot{\psi}.
 
When G=GG=G^{*} is quasi-split, by the uniqueness of G˙\dot{G} (see Theorem 2.3) and the local-global principle for even orthogonal or unitary groups, it is easy to see that G˙=G˙\dot{G}=\dot{G}^{*}. Hence by Arthur’s multiplicity formula for G˙\dot{G}^{*}, the localization of π˙\dot{\pi} at the place uu will lie in the local AA-packet Πψ˙uA(G˙u)\Pi_{\dot{\psi}_{u}}^{A}(\dot{G}^{*}_{u}), i.e.

πΠψA(G).\pi\in\Pi_{\psi}^{A}(G^{*}).

This completes the proof. ∎

As a corollary of this proposition, we deduce

Corollary 5.9.

Suppose that the AA-parameter ψ\psi satisfies Hypothesis 5.7. Then

  1. (1)

    as a set, the definition of the packet Πψθ(G)\Pi_{\psi}^{\theta}(G) is indeed independent of the choice of H=H(W(r))H=H(W_{(r)});

  2. (2)

    if G=GG=G^{*} is quasi-split, then

    Πψθ(G)=ΠψA(G)\Pi_{\psi}^{\theta}(G^{*})=\Pi_{\psi}^{A}(G^{*})

    as sets.

Proof.

Firstly we globalize the tuple of local auxiliary data (ψF,χV,χW)(\psi_{F},\chi_{V},\chi_{W}) in the definition of the local theta lift to a global tuple (ψF˙,χV˙,χW˙)(\psi_{\dot{F}},\chi_{\dot{V}},\chi_{\dot{W}}). For any positive integer r>dimVr^{\prime}>\dim V, let W˙=W˙(r)\dot{W}=\dot{W}_{(r^{\prime})} be the split cc-skew-Hermitian space over E˙\dot{E} with the same dimension as W=W(r)W=W_{(r^{\prime})}. Put H˙r=H(W˙(r))\dot{H}^{r^{\prime}}=H\left(\dot{W}_{(r^{\prime})}\right).

For an irreducible unitary representation πΠψθ,r(G)\pi\in\Pi_{\psi}^{\theta,r}(G), we have proved that we can globalize it to a cuspidal representation π˙\dot{\pi} of G˙\dot{G}, with elliptic AA-parameter ψ˙\dot{\psi}. Similar to the proof of Proposition 5.5, one can easily see that the abstract theta lift σ˙r=θabs(π˙)\dot{\sigma}^{r^{\prime}}=\theta^{abs}(\dot{\pi}) of π˙\dot{\pi} to H˙r\dot{H}^{r^{\prime}} occurs in the automorphic discrete spectrum of H˙r\dot{H}^{r^{\prime}}, with elliptic AA-parameter

θr(ψ˙)=ψ˙χW˙1χV˙+χV˙S2r2n+1.\theta^{r^{\prime}}(\dot{\psi})=\dot{\psi}\chi_{\dot{W}}^{-1}\chi_{\dot{V}}+\chi_{\dot{V}}\boxtimes S_{2r^{\prime}-2n+1}.

Consider the localizations of π˙\dot{\pi} and σ˙r\dot{\sigma}^{r^{\prime}} at the place uu, it follows that πΠψθ,r(G)\pi\in\Pi_{\psi}^{\theta,r^{\prime}}(G), i.e. Πψθ,r(G)Πψθ,r(G)\Pi_{\psi}^{\theta,r}(G)\subset\Pi_{\psi}^{\theta,r^{\prime}}(G). Symmetrically, we also have the reverse containment. Hence

Πψθ,r(G)=Πψθ,r(G).\Pi_{\psi}^{\theta,r}(G)=\Pi_{\psi}^{\theta,r^{\prime}}(G).

The second statement is a tautology of Proposition 5.8. ∎

5.3. Sharp construction

In this subsection we describe a key construction for our later proof. This construction allows us to “embed” any AA-parameter of good parity as a “sub AA-parameter” which satisfies the Hypothesis 5.7.

Lemma 5.10.

For any local AA-parameter ψΨ(G)\psi\in\Psi(G^{*}) of good parity, there exists a tuple of data (F˙,E˙,V˙,ψ˙,u,w1,w2)(\dot{F},\dot{E},\dot{V}^{\sharp},\dot{\psi}^{\sharp},u,w_{1},w_{2}), where:

  • F˙\dot{F} is a number field, and E˙\dot{E} is either F˙\dot{F} itself or a quadratic extension of F˙\dot{F}, according to the cases at hand;

  • V˙\dot{V}^{\sharp} is a cc-Hermitian space over E˙\dot{E} so that G˙=G(V˙)\dot{G}^{\sharp}=G(\dot{V}^{\sharp}) is quasi-split;

  • ψ˙\dot{\psi}^{\sharp} is an elliptic AA-parameter of G˙\dot{G}^{\sharp};

  • u,w1,w2u,w_{1},w_{2} are finite places of F˙\dot{F};

such that the following conditions hold:

  1. (1)

    (F˙u,E˙u)(F,E)(\dot{F}_{u},\dot{E}_{u})\simeq(F,E);

  2. (2)

    dimV˙\dim\dot{V}^{\sharp} is bounded by some constant which only depends on dimV\dim V but not on ψ\psi;

  3. (3)

    V˙u=V+k\dot{V}^{\sharp}_{u}=V^{+}\oplus\mathcal{H}^{k} for some integer kk, where \mathcal{H} is the cc-Hermitian hyperplane;

  4. (4)

    ψ˙u=ψτ+ψ+(ψτc)\dot{\psi}^{\sharp}_{u}=\psi_{\tau}+\psi+\left(\psi_{\tau}^{c}\right)^{\vee}, where ψτ\psi_{\tau} is a sum of tempered irreducible (conjugate) self-dual representations of the Weil group WEW_{E} (regarded as representations of LE×SL2L_{E}\times SL_{2} which is trivial on Weil-Deligne and Arthur SL2SL_{2}) with the same parity as ψ\psi;

  5. (5)

    ψ˙w1\dot{\psi}^{\sharp}_{w_{1}} is elementary, and there exists ηw1𝒮ψ˙w1¯^\eta_{w_{1}}\in\widehat{\overline{\mathcal{S}_{\dot{\psi}^{\sharp}_{w_{1}}}}}, such that πA(ψ˙w1,ηw1)\pi_{A}(\dot{\psi}^{\sharp}_{w_{1}},\eta_{w_{1}}) is supercuspidal;

  6. (6)

    ψ˙w2\dot{\psi}^{\sharp}_{w_{2}} is elementary, and the localization map

    ιw2:𝒮ψ˙𝒮ψ˙w2\iota_{w_{2}}:\mathcal{S}_{\dot{\psi}^{\sharp}}\longrightarrow\mathcal{S}_{\dot{\psi}^{\sharp}_{w_{2}}}

    is an isomorphism.

In short, the tuple of data (F˙,E˙,V˙,ψ˙,u,w1,w2)(\dot{F},\dot{E},\dot{V}^{\sharp},\dot{\psi}^{\sharp},u,w_{1},w_{2}) satisfies Hypothesis 5.7, and with ψ˙u\dot{\psi}^{\sharp}_{u} related with ψ\psi as in the condition 44.

Proof.

First we choose a pair of number fields (F˙,E˙)(\dot{F},\dot{E}), together with three places uu, w1w_{1}, and w2w_{2} of F˙\dot{F}, satisfying the following properties:

  1. (1)

    (F˙u,E˙u)(F,E)(\dot{F}_{u},\dot{E}_{u})\simeq(F,E), and (F˙w1,E˙w1)(F˙w2,E˙w2)(\dot{F}_{w_{1}},\dot{E}_{w_{1}})\simeq(\dot{F}_{w_{2}},\dot{E}_{w_{2}});

  2. (2)

    if we are in Case OO, then F˙\dot{F} has enough real places, and F˙wi\dot{F}_{w_{i}} is a finite extension of 2\mathbb{Q}_{2} with a sufficiently big residue field (this condition guarantees we will have enough irreducible orthogonal representations of WF˙wiW_{\dot{F}_{w_{i}}}; see [CZ21] Appendix B);

  3. (2)(2^{\prime})

    if we are in Case UU, then F˙wi\dot{F}_{w_{i}} is a finite extension of p\mathbb{Q}_{p} for some p2p\neq 2 with a sufficiently big residue field, and E˙wi\dot{E}_{w_{i}} is a ramified quadratic field extension of F˙wi\dot{F}_{w_{i}} (this condition guarantees we will have enough irreducible conjugate self-dual representations of WE˙wiW_{\dot{E}_{w_{i}}}, with any given parity; see [CZ21] Appendix C).

We write the local AA-parameter ψ\psi as a sum

ψ=iψi,\psi=\sum_{i}\psi_{i},

where each ψi=ρiSaiSbi\psi_{i}=\rho_{i}\boxtimes S_{a_{i}}\boxtimes S_{b_{i}} is a (conjugate) self-dual irreducible representation of LE×SL2L_{E}\times SL_{2}, with the same parity as ψ\psi. For every ii and every positive integer jj such that bi2j>0b_{i}-2j>0, let ni,j=dimρiai(bi2j)n_{i,j}=\dim\rho_{i}\cdot a_{i}\cdot(b_{i}-2j). We define an ni,jn_{i,j}-dimensional discrete (conjugate) self-dual representation ϕi,j\phi_{i,j} of LEL_{E} with the same parity as ψi\psi_{i} as follows:

  • -

    Suppose we are in the Case OO, we take:

    • \bullet

      if ni,jn_{i,j} is even, then we arbitrarily pick up an ni,jn_{i,j}-dimensional irreducible orthogonal representation of the Weil group of EE, say ρi,j\rho_{i,j}, and let ϕi,j=ρi,jS1\phi_{i,j}=\rho_{i,j}\boxtimes S_{1} be a discrete orthogonal representation of LEL_{E};

    • \bullet

      if ni,jn_{i,j} is odd, then we arbitrarily pick up an (ni,j1)(n_{i,j}-1)-dimensional irreducible orthogonal representation of the Weil group of EE, say ρi,j\rho_{i,j}, and a quadratic character of the Weil group of EE, say χi,j\chi_{i,j}, and let ϕi,j=ρi,jS1+χi,jS1\phi_{i,j}=\rho_{i,j}\boxtimes S_{1}+\chi_{i,j}\boxtimes S_{1} be a discrete orthogonal representation of LEL_{E}.

  • -

    Suppose we are in the Case UU, we take:

    • \bullet

      for 1ξni,j1\leq\xi\leq n_{i,j}, we arbitrarily pick up conjugate self-dual characters χi,jξ\chi_{i,j}^{\xi} with the same parity as ψ\psi, and we require that they are distinct one from each other; let

      ϕi,j=ξχi,jξS1\phi_{i,j}=\sum_{\xi}\chi_{i,j}^{\xi}\boxtimes S_{1}

      be a discrete conjugate self-dual representation of LEL_{E} with the same parity as ψ\psi.

Put ψi,j=ϕi,jS1\psi_{i,j}=\phi_{i,j}\boxtimes S_{1} a representation of LE×SL2L_{E}\times SL_{2}. Let χ\chi be a (conjugate) self-dual representation of the Weil group of EE, with the same parity as ψ\psi, and

ψ=χ+i((jψi,j)+ψi+(j(ψi,jc)))+(χc),\psi^{\sharp}=\chi+\sum_{i}\left(\bigg{(}\sum_{j}\psi_{i,j}\bigg{)}+\psi_{i}+\bigg{(}\sum_{j}\left(\psi_{i,j}^{c}\right)^{\vee}\bigg{)}\right)+\left(\chi^{c}\right)^{\vee},

which is also of good parity. Now we apply Lemma 4.10 to globalize each ψi\psi_{i}, ψi,j\psi_{i,j}, (ψi,jc)\left(\psi_{i,j}^{c}\right)^{\vee}, χ\chi and χ\chi^{\vee}.

  • For each ψi=ρiSaiSbi\psi_{i}=\rho_{i}\boxtimes S_{a_{i}}\boxtimes S_{b_{i}}, we globalize ρiSai\rho_{i}\boxtimes S_{a_{i}} to a (conjugate) self-dual cuspidal representation ϕ˙i\dot{\phi}_{i} of GLni(E˙)GL_{n_{i}}(\dot{E}), where ni=dimρiain_{i}=\dim\rho_{i}\cdot a_{i}, which is of the same parity as ρiSai\rho_{i}\boxtimes S_{a_{i}}, such that its localizations at places w1w_{1} and w2w_{2} are isomorphic, and supercuspidal. For w{w1,w2}w\in\{w_{1},w_{2}\}, we use ϕw,i=ρw,iS1\phi_{w,i}=\rho_{w,i}\boxtimes S_{1} to denote the LL-parameter of this supercuspidal representation. We also require that when iii\neq i^{\prime}, ρw,i≄ρw,i\rho_{w,i}\not\simeq\rho_{w,i^{\prime}}. Let ψ˙i=ϕi˙Sbi\dot{\psi}_{i}=\dot{\phi_{i}}\boxtimes S_{b_{i}}.

  • For each ψi,j=ϕi,jS1\psi_{i,j}=\phi_{i,j}\boxtimes S_{1}, we globalize ϕi,j\phi_{i,j} to a (conjugate) self-dual cuspidal representation ϕ˙i,j\dot{\phi}_{i,j} of GLni,j(E˙)GL_{n_{i,j}}(\dot{E}), which is of the same parity as ϕi,j\phi_{i,j}, such that the localizations at places w1w_{1} and w2w_{2} are isomorphic, and correspond to the LL-parameter ρw,iSbi2j\rho_{w,i}\boxtimes S_{b_{i}-2j}. Let ψ˙i,j=ϕ˙i,jS1\dot{\psi}_{i,j}=\dot{\phi}_{i,j}\boxtimes S_{1}.

  • For each (ψi,jc)=(ϕi,jc)S1\left(\psi_{i,j}^{c}\right)^{\vee}=\left(\phi_{i,j}^{c}\right)^{\vee}\boxtimes S_{1}, we globalize (ϕi,jc)\left(\phi_{i,j}^{c}\right)^{\vee} to a (conjugate) self-dual cuspidal representation ϕ˙i,j\dot{\phi}_{i,j}^{\dagger} of GLni,j(E˙)GL_{n_{i,j}}(\dot{E}), which is of the same parity as (ϕi,jc)\left(\phi_{i,j}^{c}\right)^{\vee}, such that the localizations at places w1w_{1} and w2w_{2} are isomorphic, and supercuspidal. We use ϕw,i,j=ρw,i,jS1\phi_{w,i,j}^{\dagger}=\rho_{w,i,j}^{\dagger}\boxtimes S_{1} to denote the LL-parameter of this supercuspidal representation. We also require that all ρw,i\rho_{w,i} and ρw,i,j\rho_{w,i,j}^{\dagger} are distinct one from each other. Let ψ˙i,j=ϕ˙i,jS1\dot{\psi}_{i,j}^{\dagger}=\dot{\phi}_{i,j}^{\dagger}\boxtimes S_{1}. Notice that ψ˙i,j≄(ψ˙i,jc)\dot{\psi}_{i,j}^{\dagger}\not\simeq\left(\dot{\psi}_{i,j}^{c}\right)^{\vee}!

  • For χ\chi, we globalize it to a (conjugate) self-dual character χ˙\dot{\chi} of GL1(E˙)GL_{1}({\dot{E}}), which is of the same parity as χ\chi, such that the localizations at places w1w_{1} and w2w_{2} are isomorphic. We use χw\chi_{w} to denote the localization at w1w_{1} (or w2w_{2}). We also require that χw\chi_{w} is distinct from all ρw,i\rho_{w,i} and ρw,i,j\rho_{w,i,j}^{\dagger}.

  • For (χc)\left(\chi^{c}\right)^{\vee}, we globalize it to a (conjugate) self-dual character χ˙\dot{\chi}^{\dagger} of GL1(E˙)GL_{1}({\dot{E}}), which is of the same parity as (χc)\left(\chi^{c}\right)^{\vee}, such that the localizations at places w1w_{1} and w2w_{2} are isomorphic. We use χw\chi_{w}^{\dagger} to denote the localization at w1w_{1} (or w2w_{2}). We also require that χw\chi_{w}^{\dagger} is distinct from χw\chi_{w} and all ρw,i\rho_{w,i} and all ρw,i,j\rho_{w,i,j}^{\dagger}.

Let

ψ˙=χ˙+i((jψ˙i,j)+ψ˙i+(jψ˙i,j))+χ˙.\dot{\psi}^{\sharp}=\dot{\chi}+\sum_{i}\left(\bigg{(}\sum_{j}\dot{\psi}_{i,j}\bigg{)}+\dot{\psi}_{i}+\bigg{(}\sum_{j}\dot{\psi}_{i,j}^{\dagger}\bigg{)}\right)+\dot{\chi}^{\dagger}.

Since ψ˙\dot{\psi}^{\sharp} is (conjugate) self-dual with the same parity as ψ\psi, similar to the proof of Corollary 4.12, one can show that there exists a cc-Hermitian space V˙\dot{V}^{\sharp}, such that G˙=G(V˙)\dot{G}^{\sharp}=G(\dot{V}^{\sharp}) is quasi-split, and ψ˙\dot{\psi}^{\sharp} is an elliptic AA-parameter for G˙\dot{G}^{\sharp}.

Finally we check that the tuple of data (F˙,E˙,V˙,ψ˙,u,w1,w2)(\dot{F},\dot{E},\dot{V}^{\sharp},\dot{\psi}^{\sharp},u,w_{1},w_{2}) we have constructed satisfies all our requirements. Indeed, except for the condition 55, all other requirements follow from the construction directly. As for the condition 55, notice that

ψ˙w1\displaystyle\dot{\psi}_{w_{1}}^{\sharp} =i(ρw,iS1Sbi+jρw,iSbi2jS1)\displaystyle=\sum_{i}\left(\rho_{w,i}\boxtimes S_{1}\boxtimes S_{b_{i}}+\sum_{j}\rho_{w,i}\boxtimes S_{b_{i}-2j}\boxtimes S_{1}\right)
+i,jρw,i,jS1S1+χwS1S1+χwS1S1\displaystyle+\sum_{i,j}\rho_{w,i,j}^{\dagger}\boxtimes S_{1}\boxtimes S_{1}+\chi_{w}\boxtimes S_{1}\boxtimes S_{1}+\chi_{w}^{\dagger}\boxtimes S_{1}\boxtimes S_{1}

is elementary and ψ˙w1,d\dot{\psi}_{w_{1},d}^{\sharp} satisfies the chain condition. Hence by Theorem 4.4, we may define a character ηw1𝒮ψ˙w1¯^\eta^{\prime}_{w_{1}}\in\widehat{\overline{\mathcal{S}_{\dot{\psi}^{\sharp}_{w_{1}}}}} satisfying the alternating condition and initial condition, so that πM(ψ˙w1,ηw1)\pi_{M}(\dot{\psi}_{w_{1}}^{\sharp},\eta^{\prime}_{w_{1}}) is supercuspidal (χ˙\dot{\chi} and χ˙\dot{\chi}^{\dagger} here guarantee that we can pick ηw1\eta^{\prime}_{w_{1}} in 𝒮ψ˙w1¯^\widehat{\overline{\mathcal{S}_{\dot{\psi}^{\sharp}_{w_{1}}}}}, rather than just 𝒮ψ˙w1^\widehat{{\mathcal{S}_{\dot{\psi}^{\sharp}_{w_{1}}}}}). Let

ηw1=ηw1(ηψ˙w1M/A)1.\eta_{w_{1}}=\eta^{\prime}_{w_{1}}\cdot\left(\eta_{\dot{\psi}_{w_{1}}^{\sharp}}^{M/A}\right)^{-1}.

Then πA(ψ˙w1,ηw1)=πM(ψ˙w1,ηw1)\pi_{A}(\dot{\psi}_{w_{1}}^{\sharp},\eta_{w_{1}})=\pi_{M}(\dot{\psi}_{w_{1}}^{\sharp},\eta^{\prime}_{w_{1}}) is supercuspidal, as we required. ∎

Now, for G=G(Vϵ)G=G(V^{\epsilon}), where ϵ{±1}\epsilon\in\{\pm 1\}, we let V,ϵ=VϵkV^{\sharp,\epsilon}=V^{\epsilon}\oplus\mathcal{H}^{k}, and G=G(V,ϵ)G^{\sharp}=G(V^{\sharp,\epsilon}). Let PP^{\sharp} be a maximal parabolic subgroup of GG^{\sharp} with Levi component

MGLk(E)×G,M^{\sharp}\simeq GL_{k}(E)\times G,

and τ\tau be the irreducible unitary representation of GLk(E)GL_{k}(E) with AA-parameter ψτ\psi_{\tau}.

Corollary 5.11.

Assume that r>dimV+kr>\dim V+k. Then we have

Πψθ(G)=IndPG(τΠψθ,r(G))\Pi_{\psi^{\sharp}}^{\theta}\left(G^{\sharp}\right)=\operatorname{Ind}_{P^{\sharp}}^{G^{\sharp}}\Big{(}\tau\boxtimes\Pi_{\psi}^{\theta,r}(G)\Big{)}

as representations of GG^{\sharp}, where the LHS is independent of the choice of rr. In particular, if G=GG=G^{*} is quasi-split, then as sets, we have

Πψθ,r(G)=ΠψA(G).\Pi_{\psi}^{\theta,r}(G^{*})=\Pi_{\psi}^{A}(G^{*}).
Proof.

The first statement simply follows from Corollary 5.4, Corollary 5.9, and our “sharp construction” in this subsection. For the second statement, recall that Lemma 5.5 already asserts that ΠψA(G)Πψθ,r(G)\Pi_{\psi}^{A}(G^{*})\subset\Pi_{\psi}^{\theta,r}(G^{*}), it remains to show reverse containment. But this is easy. By Corollary 5.9, when G=GG=G^{*} is quasi-split, we have

Πψθ(G)=ΠψA(G)\Pi_{\psi^{\sharp}}^{\theta}\left(G^{\sharp}\right)=\Pi_{\psi^{\sharp}}^{A}\left(G^{\sharp}\right)

as representations of GG^{\sharp}. On the other hand, we also have

ΠψA(G)=IndPG(τΠψA(G)).\Pi_{\psi^{\sharp}}^{A}\left(G^{\sharp}\right)=\operatorname{Ind}_{P^{\sharp}}^{G^{\sharp}}\Big{(}\tau\boxtimes\Pi_{\psi}^{A}(G)\Big{)}.

Compare this equality with the equality in the first statement, we get

IndPG(τΠψθ,r(G))=IndPG(τΠψA(G)).\operatorname{Ind}_{P^{\sharp}}^{G^{\sharp}}\Big{(}\tau\boxtimes\Pi_{\psi}^{\theta,r}(G)\Big{)}=\operatorname{Ind}_{P^{\sharp}}^{G^{\sharp}}\Big{(}\tau\boxtimes\Pi_{\psi}^{A}(G)\Big{)}.

Hence we have no choice but

Πψθ,r(G)=ΠψA(G).\Pi_{\psi}^{\theta,r}(G^{*})=\Pi_{\psi}^{A}(G^{*}).

5.4. Descent along the Witt tower

In the previous subsection, given a local AA-parameter ψ\psi of good parity for the group GG, we have constructed another local AA-parameter ψ\psi^{\sharp} for some larger group GG^{\sharp}. By using this construction, we have proved that some parabolic induction of the θ\theta-packet Πψθ(G)\Pi_{\psi}^{\theta}(G) is indeed independent of the choice of rr (as a set). In this subsection, we shall prove that the θ\theta-packet Πψθ(G)\Pi_{\psi}^{\theta}(G) itself is independent of the choice of rr (as a set). To achieve this, we use some techniques of the Jacquet modules. The method we are using here is similar to that in [Mœg11c] Section 5.2.

We retain the notations and assumptions from the last subsection. So ψ\psi is a local AA-parameter of good parity for GG^{*}. Let

𝒰={πIrrunit(G)|HomM(τπ,s.s.JacPΠψθ(G))0},\mathcal{U}=\left\{\pi\in\operatorname{Irr}_{unit}\left(G\right)~{}\big{|}~{}\operatorname{Hom}_{M^{\sharp}}\left(\tau\boxtimes\pi,s.s.Jac_{P^{\sharp}}\Pi_{\psi^{\sharp}}^{\theta}\left(G^{\sharp}\right)\right)\neq 0\right\},

where s.s.JacPs.s.Jac_{P^{\sharp}} means taking the semi-simplification of the Jacquet-module along the parabolic PP^{\sharp}. Obviously 𝒰\mathcal{U} is a finite subset of Irrunit(G)\operatorname{Irr}_{unit}\left(G\right). Moreover, it follows from Corollary 5.11 that for rr sufficiently large, we have

Πψθ,r(G)𝒰.\Pi_{\psi}^{\theta,r}(G)\subset\mathcal{U}.
Lemma 5.12.

Fix a positive integer r0>dimVr_{0}>\dim V. Then, for rr sufficiently large, we have

Πψθ,r(G)Πψθ,r0(G).\Pi_{\psi}^{\theta,r}(G)\subset\Pi_{\psi}^{\theta,r_{0}}(G).
Proof.

To distinguish notations, for an irreducible representation π\pi of GG, we shall use σr=θr(π)\sigma^{r}=\theta^{r}(\pi) to denote the theta lift of π\pi to the group Hr=H(W(r))H^{r}=H(W_{(r)}). Since 𝒰\mathcal{U} is a finite subset of Irrunit(G)\operatorname{Irr}_{unit}\left(G\right), according to [GT16a] Proposition 3.2, there is a positive integer NuN_{u}, such that for all r>r0+Nur>r_{0}+N_{u}, and all π𝒰\pi\in\mathcal{U}, σr\sigma^{r} is a subrepresentation of

IndQr,r0Hr(χV||nrχV||nr01σr0),\operatorname{Ind}_{Q^{r,r_{0}}}^{H^{r}}\left(\chi_{V}|\cdot|^{n-r}\boxtimes\cdots\boxtimes\chi_{V}|\cdot|^{n-r_{0}-1}\boxtimes\sigma^{r_{0}}\right),

where Qr,r0Q^{r,r_{0}} is a parabolic subgroup with Levi component GL1(E)××GL1(E)×Hr0GL_{1}(E)\times\cdots\times GL_{1}(E)\times H^{r_{0}}.

Next we choose a tuple of data

(>ψ,ψ,V,r1),\left(>_{\psi},\psi_{\gg},V^{\gg},r_{1}\right),

where

  • >ψ>_{\psi} is an admissible order on IψI_{\psi};

  • ψ\psi_{\gg} is a local AA-parameter has DDR for the group G=G(V)G_{\gg}=G(V^{\gg}), with VV^{\gg} a space in the Witt tower containing VV; for any cc-skew-Hermitian space WW, we shall also let WW^{\gg} be the space in the Witt tower containing WW, such that

    dimWdimV=dimWdimV;\dim W^{\gg}-\dim V^{\gg}=\dim W-\dim V;
  • r1>max{r0,dimV}r_{1}>\max\left\{r_{0},\dim V^{\gg}\right\} is a positive integer;

such that the following conditions holds:

  1. (1)

    for any rr0r\geq r_{0}, >ψ>_{\psi} can be uniquely extended to an admissible order >ψ,r>_{\psi,r} on the index set of θr(ψ)\theta^{r}(\psi)

    Iθr(ψ)=Iψ{ir},I_{\theta^{r}(\psi)}=I_{\psi}\sqcup\left\{i^{r}\right\},

    such that iri^{r} is the unique maximal element under the partial order >ψ,r>_{\psi,r}; here iri^{r} is the element in the index set Iθr(ψ)I_{\theta^{r}(\psi)} corresponding to the irreducible constituent χVS2r2n+1\chi_{V}\boxtimes S_{2r-2n+1};

  2. (2)

    for any r>r1r>r_{1}, the local AA-parameter

    θr(ψ)=ψχW1χV+χVS2r2n+1\theta^{r}(\psi_{\gg})=\psi_{\gg}\chi_{W}^{-1}\chi_{V}+\chi_{V}\boxtimes S_{2r-2n+1}

    for the group Hr=H((W(r)))H_{\gg}^{r}=H\left(\left(W_{(r)}\right)^{\gg}\right) has DDR, and dominates θr(ψ)\theta^{r}(\psi) with respect to the admissible order >ψ,r>_{\psi,r}; in particular, θr(ψ)\theta^{r}(\psi_{\gg}) will also dominate θr0(ψ)\theta^{r_{0}}(\psi) with respect to the admissible order >ψ,r0>_{\psi,r_{0}}.

Now assume that r>max{dimV+k,r0+Nu,r1}r>\max\left\{\dim V+k,r_{0}+N_{u},r_{1}\right\}. For any irreducible unitary representation πΠψθ,r(G)\pi\in\Pi_{\psi}^{\theta,r}(G), it is sufficient to prove that its theta lift σr0\sigma^{r_{0}} to the group Hr0H^{r_{0}} lies in the local AA-packet Πθr0(ψ)A(Hr0)\Pi_{\theta^{r_{0}}(\psi)}^{A}\left(H^{r_{0}}\right). We consider the theta lift σr\sigma^{r} of π\pi to the group HrH^{r}. By the definition of the θ\theta-packet, σr\sigma^{r} lies in the local AA-packet Πθr(ψ)A(Hr)\Pi_{\theta^{r}(\psi)}^{A}\left(H^{r}\right). According to Theorem 4.9, there exists some σΠθr(ψ)A(Hr)\sigma_{\gg}\in\Pi_{\theta^{r}(\psi_{\gg})}^{A}\left(H^{r}_{\gg}\right), such that

σr=iIψJacXiσ,\sigma^{r}=\circ_{i\in I_{\psi}}Jac_{X_{i}^{\gg}}\sigma_{\gg},

where we identify IψI_{\psi} with a subset of Iθr(ψ)I_{\theta^{r}(\psi)} in the obvious way, and each XiX_{i}^{\gg} is some generalized segment. Since θr(ψ)\theta^{r}(\psi_{\gg}) also dominants θr0(ψ)\theta^{r_{0}}(\psi) with respect to the admissible order >ψ,r0>_{\psi,r_{0}}, again by Theorem 4.9, the representation

JacXir0σr=JacXir0(iIψJacXiσ)Jac_{X_{i^{r_{0}}}^{\gg}}\sigma^{r}=Jac_{X_{i^{r_{0}}}^{\gg}}\circ\left(\circ_{i\in I_{\psi}}Jac_{X_{i}^{\gg}}\sigma_{\gg}\right)

is either zero or irreducible and lies in the AA-packet Πθr0(ψ)A(Hr0)\Pi_{\theta^{r_{0}}(\psi)}^{A}\left(H^{r_{0}}\right), where the generalized segment Xir0X_{i^{r_{0}}}^{\gg} is

Xir0=(nrnr01).X_{i^{r_{0}}}^{\gg}=\Big{(}\begin{array}[]{ccc}n-r&\cdots&n-r_{0}-1\end{array}\Big{)}.

On the other hand, since σr\sigma^{r} is a subrepresentation of

IndQr,r0Hr(χV||nrχV||nr01σr0),\operatorname{Ind}_{Q^{r,r_{0}}}^{H^{r}}\left(\chi_{V}|\cdot|^{n-r}\boxtimes\cdots\boxtimes\chi_{V}|\cdot|^{n-r_{0}-1}\boxtimes\sigma^{r_{0}}\right),

it follows that

JacXir0σrσr0Jac_{X_{i^{r_{0}}}^{\gg}}\sigma^{r}\simeq\sigma^{r_{0}}

is non-zero and hence lies in the local AA-packet Πθr0(ψ)A(Hr0)\Pi_{\theta^{r_{0}}(\psi)}^{A}\left(H^{r_{0}}\right). This completes the proof. ∎

Corollary 5.13.

Let ψ\psi be a local AA-parameter for GG^{*}. Then as a set, the θ\theta-packet Πψθ(G)\Pi_{\psi}^{\theta}\left(G\right) is indeed independent of the choice of H=H(W(r))H=H\left(W_{(r)}\right). Moreover, if G=GG=G^{*} is quasi-split, then as sets, we have

Πψθ(G)=ΠψA(G).\Pi_{\psi}^{\theta}(G^{*})=\Pi_{\psi}^{A}(G^{*}).
Proof.

We first assume that ψ\psi is of good parity. In this case, it suffices to prove that as sets, we have

Πψθ,r(G)=Πψθ,r0(G)\Pi_{\psi}^{\theta,r}(G)=\Pi_{\psi}^{\theta,r_{0}}(G)

in the previous lemma. We consider all pure inner forms of GG^{*} simultaneously: it then follows from the previous lemma that

|Πψθ,r(G)||Πψθ,r0(G)|,\Big{|}\bigsqcup\Pi_{\psi}^{\theta,r}\left(G\right)\Big{|}\leq\Big{|}\bigsqcup\Pi_{\psi}^{\theta,r_{0}}\left(G\right)\Big{|},

where the disjoint unions on both sides run over all pure inner forms GG of GG^{*}. On the other hand, we deduce from Proposition 5.2 that

|Πψθ,r(G)|=|Πθr(ψ)A(Hr)|and|Πψθ,r0(G)|=|Πθr0(ψ)A(Hr0)|.\Big{|}\bigsqcup\Pi_{\psi}^{\theta,r}\left(G\right)\Big{|}=\Big{|}\Pi_{\theta^{r}(\psi)}^{A}(H^{r})\Big{|}\quad\textit{and}\quad\Big{|}\bigsqcup\Pi_{\psi}^{\theta,r_{0}}\left(G\right)\Big{|}=\Big{|}\Pi_{\theta^{r_{0}}(\psi)}^{A}(H^{r_{0}})\Big{|}.

Also, as explicated in the proof of the previous lemma, Theorem 4.9 asserts that Πθr0(ψ)A(Hr0)\Pi_{\theta^{r_{0}}(\psi)}^{A}(H^{r_{0}}) can be obtained from Πθr(ψ)A(Hr)\Pi_{\theta^{r}(\psi)}^{A}(H^{r}) by taking some partial Jacquet modules. To be more precise, we have

Πθr0(ψ)A(Hr0)={σ0=JacXir0σ|σΠθr(ψ)A(Hr)}\{0},\Pi_{\theta^{r_{0}}(\psi)}^{A}(H^{r_{0}})=\left\{\sigma_{0}=Jac_{X_{i^{r_{0}}}^{\gg}}\sigma~{}\big{|}~{}\sigma\in\Pi_{\theta^{r}(\psi)}^{A}(H^{r})\right\}\Big{\backslash}\left\{0\right\},

where the generalized segment Xir0X_{i^{r_{0}}}^{\gg} is the same that in the previous lemma. It follows that

|Πθr(ψ)A(Hr)||Πθr0(ψ)A(Hr0)|.\Big{|}\Pi_{\theta^{r}(\psi)}^{A}(H^{r})\Big{|}\geq\Big{|}\Pi_{\theta^{r_{0}}(\psi)}^{A}(H^{r_{0}})\Big{|}.

Hence there is no other choice that we must have

Πψθ,r(G)=Πψθ,r0(G)\Pi_{\psi}^{\theta,r}(G)=\Pi_{\psi}^{\theta,r_{0}}(G)

as subsets of Irrunit(G)\operatorname{Irr}_{unit}\left(G\right). This completes the proof in the good parity case.

The general case then easily follows from the good parity case and Corollary 5.4. ∎

6. Independency on the auxiliary data

We have already proved that, as subsets of Irrunit(G)\operatorname{Irr}_{unit}\left(G\right), the definition of the θ\theta-packets is independent of the choice of H=H(W(r))H=H\left(W_{(r)}\right). But this is not the only choice we have made: recall that in the definition of the theta lift between (G,H)(G,H), we also need to choose a tuple of auxiliary data (ψF,χV,χW)(\psi_{F},\chi_{V},\chi_{W}). In fact as subsets of Irrunit(G)\operatorname{Irr}_{unit}\left(G\right), the definition of the θ\theta-packets is also independent of the choice of these data, though maybe this fact is not so apparent. In this section we shall investigate this independency.

6.1. Similitude group action vs. Adjoint group action

In this subsection we consider two actions on the group HH, one is by the similitude group, and another one is by the adjoint group.

Recall that WW is a cc-skew-Hermitian space over EE, and H=H(W)H=H(W) is the isometry group associated to WW. Let H=H(W)H^{\sim}=H^{\sim}(W) be the group of elements hh in GL(W)GL(W) such that

hv,hwW=λhv,wWfor v,wW,\langle hv,hw\rangle_{W}=\lambda_{h}\cdot\langle v,w\rangle_{W}\quad\textit{for }v,w\in W,

where λhE×\lambda_{h}\in E^{\times} is some constant, called the scale of hh. We shall call HH^{\sim} the similitude group associated to WW. Let ZHZ_{H} be the center of HH, we also have another group

Had,/F=H/F/ZH,/F,H_{ad,/F}=H_{/F}\big{/}Z_{H,/F},

which we shall call it the adjoint group of HH. Here we use the subscript “/F~{}_{/F}” to emphasize that the groups are regarded as algebraic groups over FF. Denote by HadH_{ad} the FF-points of Had,/FH_{ad,/F}. There is a commutative diagram of algebraic groups

1ZH,/FH/FHad,/F11ResE/F𝔾mH/FHad,/F1.\setcounter{MaxMatrixCols}{11}\begin{CD}1@>{}>{}>Z_{H,/F}@>{}>{}>H_{/F}@>{}>{}>H_{ad,/F}@>{}>{}>1\\ @V{}V{}V@V{}V{}V\Big{\|}\\ 1@>{}>{}>Res_{E/F}\mathbb{G}_{m}@>{}>{}>H^{\sim}_{/F}@>{}>{}>H_{ad,/F}@>{}>{}>1\end{CD}\quad.

We derive from this diagram that

HadH/E×H_{ad}\simeq H^{\sim}\big{/}E^{\times}

as abstract groups. Recall that HH^{\sim} acts on the group HH by conjugation. The adjoint group HadH_{ad} also has an action on the group HH, which can be described as follows. Let h¯Had\overline{h}\in H_{ad}, and h~H/F(F¯)\widetilde{h}\in H_{/F}(\overline{F}) be a lift of h¯\overline{h}, where F¯\overline{F} is the algebraic closure of FF. Then for xHx\in H, the action of h¯\overline{h} on xx is

h¯.x=h~xh~1.\overline{h}.x=\widetilde{h}\cdot x\cdot\widetilde{h}^{-1}.

These actions induce the actions of HH^{\sim} and HadH_{ad} on representations/ functions/ distributions of HH.

Lemma 6.1.

The conjugation action of HH^{\sim} on the group HH factor through HadH_{ad}, i.e. for any hHh\in H^{\sim}, and xHx\in H, we have

h.x=h¯.x,h.x=\overline{h}.x,

where h¯\overline{h} is the image of hh in HadH_{ad}.

Proof.

This is trivial. ∎

Notice that in our cases, the derived group of HH is simply-connected. Hence the stable conjugacy in HH is just the same as the H/F(F¯)H_{/F}(\overline{F})-conjugacy. We have

Lemma 6.2.

The action of HadH_{ad} on irreducible representations of HH preserves the local AA-packets of HH.

Proof.

Let ψH\psi_{H} be a local AA-parameter for HH. Recall that Arthur/ Mok have attached a stable distribution SΘψHS\Theta_{\psi_{H}} to ψH\psi_{H}, which is a linear combination of characters of irreducible unitary representations in the AA-packet ΠψHA(H)\Pi_{\psi_{H}}^{A}(H)

SΘψH=σΠψHA(H)𝒥𝒲A(σ)(sψH)Θσ,S\Theta_{\psi_{H}}=\sum_{\sigma\in\Pi_{\psi_{H}}^{A}(H)}\mathcal{J}^{A}_{\mathscr{W}^{\prime}}(\sigma)(s_{\psi_{H}})\cdot\Theta_{\sigma},

where sψHs_{\psi_{H}} is certain element in the component group, and Θσ\Theta_{\sigma} is the character of σ\sigma. Since SΘψHS\Theta_{\psi_{H}} is stable, the action of HadH_{ad} preserves this distribution. Let h¯Had\overline{h}\in H_{ad}, we obtain

σΠψHA(H)𝒥𝒲A(σ)(sψH)Θσ=σΠψHA(H)𝒥𝒲A(σ)(sψH)Θσh¯.\sum_{\sigma\in\Pi_{\psi_{H}}^{A}(H)}\mathcal{J}^{A}_{\mathscr{W}^{\prime}}(\sigma)(s_{\psi_{H}})\cdot\Theta_{\sigma}=\sum_{\sigma\in\Pi_{\psi_{H}}^{A}(H)}\mathcal{J}^{A}_{\mathscr{W}^{\prime}}(\sigma)(s_{\psi_{H}})\cdot\Theta_{{}^{\overline{h}}\sigma}.

By the linear independency of the characters, we can conclude that the lemma holds. ∎

6.2. Even orthogonal case: the scaling property

Now we prove the independence of θ\theta-packets (as sets) on the auxiliary data (ψF,χV,χW)(\psi_{F},\chi_{V},\chi_{W}) in Case OO. In this case, the pair of characters (χV,χW)(\chi_{V},\chi_{W}) is fixed, so we only need to consider the changes of the additive character ψF\psi_{F}.

Let ψ\psi be a local AA-parameter for GG. In this subsection, to emphasize the possible dependence of the θ\theta-packets on the choice of ψF\psi_{F}, we shall write Πψθ(G)\Pi_{\psi}^{\theta}(G) as Πψθ,ψF(G)\Pi_{\psi}^{\theta,\psi_{F}}(G). Let aF×a\in F^{\times}, and ψF,a=ψF(a)\psi_{F,a}=\psi_{F}(a\cdot~{}) be another additive character of FF. Recall that we have the well-known scaling property of the theta lift (cf. [Kud96] II Corollary 6.2 and IV Proposition 1.9)

θψF,a(π)=θψFδa(π)\theta_{\psi_{F,a}}(\pi)=~{}^{\delta_{a}}\theta_{\psi_{F}}(\pi)

for any irreducible smooth representation π\pi of GG, where θψF(π)\theta_{\psi_{F}}(\pi) means the theta lift of π\pi to the group HH with respect to the additive character ψF\psi_{F}, and δa\delta_{a} is an element in the similitude HH^{\sim} with scale aa. We rewrite the θ\theta-packet Πψθ,ψF(G)\Pi_{\psi}^{\theta,\psi_{F}}(G) as

Πψθ,ψF(G)={πIrrunit(G)|θψF(π)Πθ(ψ)A(H)}.\Pi_{\psi}^{\theta,\psi_{F}}(G)=\left\{\pi\in\operatorname{Irr}_{unit}(G)~{}\big{|}~{}\theta_{\psi_{F}}(\pi)\in\Pi_{\theta(\psi)}^{A}(H)\right\}.

Let δ¯a\overline{\delta}_{a} be the image of δa\delta_{a} in HadH_{ad}. Then, for any πΠψθ,ψF(G)\pi\in\Pi_{\psi}^{\theta,\psi_{F}}(G), according to Lemma 6.1 and Lemma 6.2, we have

θψF,a(π)=θψFδ¯a(π)\theta_{\psi_{F,a}}(\pi)=~{}^{\overline{\delta}_{a}}\theta_{\psi_{F}}(\pi)

also lies in the AA-packet Πθ(ψ)A(H)\Pi_{\theta(\psi)}^{A}(H). It follows that

Πψθ,ψF(G)Πψθ,ψF,a(G).\Pi_{\psi}^{\theta,\psi_{F}}(G)\subset\Pi_{\psi}^{\theta,\psi_{F,a}}(G).

Similarly, we also have the reverse containment. This implies that as a set of irreducible unitary representations, Πψθ,ψF(G)\Pi_{\psi}^{\theta,\psi_{F}}(G) is in fact not dependent on the choice of ψF\psi_{F}.

6.3. Unitary case: inputs from Archimedean places

Now we prove the independence of θ\theta-packets (as sets) on the auxiliary data (ψF,χV,χW)(\psi_{F},\chi_{V},\chi_{W}) in Case UU. In this case, we have the flexibility of choosing the pair of characters (χV,χW)(\chi_{V},\chi_{W}). Hence the scaling property is not sufficient for us to prove the independence. We shall use another approach.

The idea is the same as that of Section 5.2, i.e. trying to use the global method. Let ψ\psi be a local AA-parameter of good parity for the group GG. Applying Lemma 4.10, one can easily construct a tuple of data (F˙,E˙,V˙,ψ˙,u,w)(\dot{F},\dot{E},\dot{V},\dot{\psi},u,w), where:

  • F˙\dot{F} is a number field, and E˙\dot{E} is a quadratic field extension of F˙\dot{F};

  • V˙+\dot{V}^{+} is a cc-Hermitian space over E˙\dot{E} so that G˙=G(V˙+)\dot{G}^{*}=G(\dot{V}^{+}) is quasi-split;

  • ψ˙\dot{\psi} is an elliptic AA-parameter of G˙\dot{G};

  • u,wu,w are finite places of F˙\dot{F};

such that the following conditions hold:

  1. (1)

    (F˙u,E˙u,V˙u+,ψ˙u)(F,E,V+,ψ)(\dot{F}_{u},\dot{E}_{u},\dot{V}^{+}_{u},\dot{\psi}_{u})\simeq(F,E,V^{+},\psi);

  2. (2)

    F˙\dot{F} has at least one real place, and E˙\dot{E} is not split at this place;

  3. (3)

    ψ˙w\dot{\psi}_{w} is elementary, and the localization map

    ιw:𝒮ψ˙𝒮ψ˙w\iota_{w}:\mathcal{S}_{\dot{\psi}}\longrightarrow\mathcal{S}_{\dot{\psi}_{w}}

    is an isomorphism.

Indeed, as stated in Remark 4.11, we can further impose some requirements on one more Archimedean place. Let ww_{\infty} be a real place of F˙\dot{F}, such that E˙\dot{E} is not split at ww_{\infty}. We require that

  1. (4)(4)

    ψ˙w\dot{\psi}_{w_{\infty}} is of good parity, and (ψ˙w)d\left(\dot{\psi}_{w_{\infty}}\right)_{d} is a square-integrable LL-parameter for G˙w\dot{G}_{w_{\infty}}; here (ψ˙w)d\left(\dot{\psi}_{w_{\infty}}\right)_{d} is a dimV\dim V-dimensional representation of LL_{\mathbb{C}} defined by

    (ψ˙w)d(z)=ψ˙w(z,((z/z¯)1/2(z/z¯)1/2))\left(\dot{\psi}_{w_{\infty}}\right)_{d}(z)=\dot{\psi}_{w_{\infty}}\left(z,\left(\begin{array}[]{cc}\left(z/\bar{z}\right)^{1/2}&\\ &\left(z/\bar{z}\right)^{-1/2}\end{array}\right)\right)

We shall need the following remarkable fact:

Lemma 6.3.

Let VwV_{w_{\infty}} be an anisotropic Hermitian space over \mathbb{C} of the same dimension as VV, and let Gw=G(Vw)G_{w_{\infty}}=G(V_{w_{\infty}}) be the compact unitary group associated to it. Let WwW_{w_{\infty}} be the split skew Hermitian space over \mathbb{C} of the same dimension as WW (as explicated at the begining of Section 2), and let Hw=H(Ww)H_{w_{\infty}}=H(W_{w_{\infty}}). Then we have

Πψ˙wθ(Gw)=Π(ψ˙w)dL(Gw).\Pi_{\dot{\psi}_{w_{\infty}}}^{\theta}\left(G_{w_{\infty}}\right)=\Pi_{\left(\dot{\psi}_{w_{\infty}}\right)_{d}}^{L}\left(G_{w_{\infty}}\right).

In particular, Πψ˙wθ(Gw)\Pi_{\dot{\psi}_{w_{\infty}}}^{\theta}\left(G_{w_{\infty}}\right) is non-empty.

Proof.

By [MR19] Théorème 1.1, if we replace the terminology “AA-packets” by “AJAJ-packets” (i.e. Adams-Johnson packets), then Conjecture 1.1 (B) holds for real unitary groups. On the other hand, by [Cos09] Corollary 3.8, we have

Πθ(ψ˙w)AJ(Hw)=Πθ(ψ˙w)A(Hw).\Pi_{\theta(\dot{\psi}_{w_{\infty}})}^{AJ}\left(H_{w_{\infty}}\right)=\Pi_{\theta(\dot{\psi}_{w_{\infty}})}^{A}\left(H_{w_{\infty}}\right).

It follows that

Πψ˙wθ(Gw)=Πψ˙wAJ(Gw)=Π(ψ˙w)dL(Gw).\Pi_{\dot{\psi}_{w_{\infty}}}^{\theta}\left(G_{w_{\infty}}\right)=\Pi_{\dot{\psi}_{w_{\infty}}}^{AJ}\left(G_{w_{\infty}}\right)=\Pi_{\left(\dot{\psi}_{w_{\infty}}\right)_{d}}^{L}\left(G_{w_{\infty}}\right).

Let πΠψθ(G)\pi\in\Pi_{\psi}^{\theta}(G). We now try to globalize π\pi to a discrete automorphic representation of some unitary group over F˙\dot{F}, with AA-parameter ψ˙\dot{\psi}. Firstly we globalize the tuple of local auxiliary data (ψF,χV,χW)(\psi_{F},\chi_{V},\chi_{W}) in the definition of the local theta lift to a global tuple (ψF˙,χV˙,χW˙)(\psi_{\dot{F}},\chi_{\dot{V}},\chi_{\dot{W}}). Let W˙=W˙(r)\dot{W}=\dot{W}_{(r)} be the split skew-Hermitian space over E˙\dot{E} with the same dimension as W=W(r)W=W_{(r)}. Put H˙=H(W˙)\dot{H}=H(\dot{W}). Similar to the proof of Proposition 5.8, applying the Arthur’s multiplicity formula for H˙\dot{H}, we may construct a discrete automorphic representation σ˙\dot{\sigma} of H˙\dot{H} with elliptic AA-parameter

θ(ψ˙)=ψ˙χW˙1χV˙+χV˙S2r2n+1,\theta(\dot{\psi})=\dot{\psi}\chi_{\dot{W}}^{-1}\chi_{\dot{V}}+\chi_{\dot{V}}\boxtimes S_{2r-2n+1},

such that:

  1. (1)

    at the place uu, σ˙u=θ(π)\dot{\sigma}_{u}=\theta(\pi);

  2. (2)

    at the place ww_{\infty}, σ˙w=θ(πw)\dot{\sigma}_{w_{\infty}}=\theta\left(\pi_{w_{\infty}}\right) for the unique πwΠ(ψ˙w)dL(Gw)\pi_{w_{\infty}}\in\Pi_{\left(\dot{\psi}_{w_{\infty}}\right)_{d}}^{L}\left(G_{w_{\infty}}\right).

By J-S. Li’s work on low rank representations (Theorem 2.3), there is an pure inner form G˙\dot{G} of G˙\dot{G}^{*} and an automorphic representation π˙\dot{\pi} of G˙\dot{G}, such that

σ˙=θabs(π˙).\dot{\sigma}=\theta^{abs}(\dot{\pi}).

Also, by our construction, G˙w=Gw\dot{G}_{w_{\infty}}=G_{w_{\infty}} is compact. This forces any automorphic realization of π˙\dot{\pi} to be cuspidal. Hence π˙\dot{\pi} lies in the automorphic discrete spectrum of G˙\dot{G}.

So now, we have successfully globalize the local triple (G,ψ,π)(G,\psi,\pi) to a global triple (G˙,ψ˙,π˙)(\dot{G},\dot{\psi},\dot{\pi}). The same argument as Corollary 5.9 implies that for any tuple of auxiliary data (ψF,χV,χW)(\psi^{\prime}_{F},\chi^{\prime}_{V},\chi^{\prime}_{W}), π\pi will also lie in the θ\theta-packet defined with respect to (ψF,χV,χW)(\psi^{\prime}_{F},\chi^{\prime}_{V},\chi^{\prime}_{W}). It follows that the definition of the θ\theta-packets is independent of the choice of (ψF,χV,χW)(\psi_{F},\chi_{V},\chi_{W}).

Remark 6.4.

The argument in this subsection can be used to prove Corollary 5.13 in Case UU as well. Indeed, this would simplify our proof in Case UU.

7. Local intertwining relation

To investigate the “labeling” of irreducible unitary representations inside a local AA-packet for quasi-split classical groups, i.e. the characters of the component group attached to each element inside the packet, we need the so-called “local intertwining relation”. However, the original version of local intertwining relation formulated by Arthur is not so convenient for our applications, we shall formulate an alternative version of it, in the spirit of the one formulated in [GI16] [AG17]. To distinguish these two versions, we shall write Arthur’s version “LIR-A” for abbreviation, and write Gan-Ichino’s version “LIR-B” for abbreviation.

In this section we retain the notations of Section 3.

7.1. Local intertwining operators

We first briefly recall the definition of the (normalized) intertwining operators, for both quasi-split and non quasi-split groups.

Recall that we have

V=X+V0+XV=X+V_{0}+X^{*}

for some kk-dimensional totally isotropic subspace XX and XX^{*} of VV. Let n0=nkn_{0}=n-k, and r0=rkr_{0}=r-k. We have a maximal parabolic subgroup P=MPUPP=M_{P}U_{P} of GG stabilizing XX, where MPM_{P} is the Levi component of PP stabilizing XX^{*} and UPU_{P} is the unipotent radical of PP. Let τ\tau be an irreducible unitary representation of GL(X)GL(X) on a space 𝒱τ\mathscr{V}_{\tau} with central character ωτ\omega_{\tau}. Suppose that τ\tau is of Arthur type, and corresponds to an irreducible AA-parameter ψτ\psi_{\tau}. Let ψ0\psi_{0} be a local AA-parameter for G0G_{0}, and π0\pi_{0} an irreducible unitary representation in the packet Πψ0θ(G0)\Pi_{\psi_{0}}^{\theta}(G_{0}). We consider the induced representation

IndPG(τsπ0)\operatorname{Ind}_{P}^{G}\left(\tau_{s}\boxtimes\pi_{0}\right)

of GG. Let APA_{P} be the split component of the center of MPM_{P} and W(MP)=NG(AP)/MPW(M_{P})=N_{G}(A_{P})/M_{P} be the relative Weyl group for MPM_{P}. Noting that W(MP)/2W(M_{P})\simeq\mathbb{Z}/2\mathbb{Z}, we denote by ww the non-trivial element in W(MP)W(M_{P}). For any representative w~G\widetilde{w}\in G of ww, we define an unnormalized intertwining operator

(w~,τsπ0):IndPG(τsπ0)IndPG(w(τsπ0))\mathcal{M}(\widetilde{w},\tau_{s}\boxtimes\pi_{0}):\operatorname{Ind}_{P}^{G}(\tau_{s}\boxtimes\pi_{0})\longrightarrow\operatorname{Ind}_{P}^{G}\left(w(\tau_{s}\boxtimes\pi_{0})\right)

by (the meromorphic continuation of) the integral

(w~,τsπ0)Φs(g)=UPΦs(w~1ug)𝑑u,\mathcal{M}(\widetilde{w},\tau_{s}\boxtimes\pi_{0})\varPhi_{s}(g)=\int_{U_{P}}\varPhi_{s}(\widetilde{w}^{-1}ug)du,

where the Haar measures on various groups are fixed as in Section 3.

Having fixed an additive character ψF\psi_{F}, as explicated in Section 2.4, we can define a Whittaker datum 𝒲ψF=𝒲\mathscr{W}_{\psi_{F}}=\mathscr{W} of GG^{*}. To normailze this operator with respect to the Whittaker datum 𝒲ψF\mathscr{W}_{\psi_{F}}, we need to choose the following data appropriately:

  • a representative w~\widetilde{w};

  • a normalizing factor r(w,τsπ0)r(w,\tau_{s}\boxtimes\pi_{0});

  • an intertwining isomorphism 𝒜w\mathcal{A}_{w}.

For the representative, we take w~G\widetilde{w}\in G defined by

w~=wPmP((1)nκVJ)(1V0)k,\widetilde{w}=w_{P}\cdot m_{P}\left((-1)^{n^{\prime}}\cdot\kappa_{V}\cdot J\right)\cdot(-1_{V_{0}})^{k},

where wPw_{P} is as in Section 3, n=[dimV/2]n^{\prime}=[\dim V/2], and

κV={cCase O;δCase U0;1Case U1,\kappa_{V}=\begin{cases}c\quad&\textit{Case $O$};\\ -\delta\quad&\textit{Case $U_{0}$};\\ -1\quad&\textit{Case $U_{1}$},\end{cases}

where the constant cc in Case OO and the constant δ\delta in Case U0U_{0} arise in the choice of Whittaker datum 𝒲ψF\mathscr{W}_{\psi_{F}}; and

J=((1)k111)GLk(E).J=\left(\begin{array}[]{cccc}{}\hfil&{}\hfil&{}\hfil&(-1)^{k-1}\\ {}\hfil&{}\hfil&\iddots&{}\hfil\\ {}\hfil&-1&{}\hfil&{}\hfil\\ 1&{}\hfil&{}\hfil&\par{}\hfil\end{array}\right)\in GL_{k}(E).

Here, we have identified GL(X)GL(X) with GLk(E)GL_{k}(E) by choosing a basis of XX. In [GI16] Section 7.3, it was shown that the representative defined above coincides with the representative defined in [Mok15] when we are in Case UU and ϵ(V)=1\epsilon(V)=1.

Next we define the normalizing factor r(w,τsσ0)r(w,\tau_{s}\boxtimes\sigma_{0}). Put

λ(w,ψF)={λ(E/F,ψF)kCase O, here E is the splitting field of V+;λ(E/F,ψF)(k1)k/2Case U0;λ(E/F,ψF)(k+1)k/2Case U1.\lambda(w,\psi_{F})=\begin{cases}\lambda(E^{\prime}/F,\psi_{F})^{k}\quad&\textit{Case $O$, here $E^{\prime}$ is the splitting field of $V^{+}$};\\ \lambda(E/F,\psi_{F})^{(k-1)k/2}\quad&\textit{Case $U_{0}$};\\ \lambda(E/F,\psi_{F})^{(k+1)k/2}\quad&\textit{Case $U_{1}$}.\end{cases}

where λ(E/F,ψF)\lambda(E^{\prime}/F,\psi_{F}) or λ(E/F,ψF)\lambda(E/F,\psi_{F}) is the Langlands λ\lambda-factor. Let ϕτ\phi_{\tau} and ϕ0\phi_{0} be the LL-parameters associated to the AA-parameter ψτ\psi_{\tau} and ψ0\psi_{0} respectively. We set

r(w,τsπ0)=λ(w,ψF)γ(s,ϕτϕ0,ψE)1γ(2s,Rϕτ,ψF)1,r(w,\tau_{s}\boxtimes\pi_{0})=\lambda(w,\psi_{F})\cdot\gamma\left(s,\phi_{\tau}\otimes\phi_{0}^{\vee},\psi_{E}\right)^{-1}\cdot\gamma\left(2s,R\circ\phi_{\tau},\psi_{F}\right)^{-1},

and the normalized intertwining operator

(w,τsπ0)|κV|kρPr(w,τsπ0)1(w~,τsπ0);\mathcal{R}(w,\tau_{s}\boxtimes\pi_{0})\coloneqq|\kappa_{V}|^{k\rho_{P}}\cdot r(w,\tau_{s}\boxtimes\pi_{0})^{-1}\cdot\mathcal{M}(\widetilde{w},\tau_{s}\boxtimes\pi_{0});

where

R={2Case O;AsCase U0;As+Case U1.R=\begin{cases}\bigwedge^{2}\quad&\textit{Case $O$};\\ As^{-}\quad&\textit{Case $U_{0}$};\\ As^{+}\quad&\textit{Case $U_{1}$}.\end{cases}
Lemma 7.1.

The normalized intertwining operator (w,τsπ0)\mathcal{R}(w,\tau_{s}\boxtimes\pi_{0}) is holomorphic at s=0s=0.

At least when G=GG=G^{*} is quasi-split, this should follow from [Art13] Proposition 2.3.1 in Case OO, or [Mok15] Proposition 3.3.1 in Case UU. We shall prove this lemma in the next section for GG is non quasi-split.

Finally we define the intertwining isomorphism. Assume that w(τπ0)τπ0w(\tau\boxtimes\pi_{0})\simeq\tau\boxtimes\pi_{0}, which is equivalent to (τc)τ\left(\tau^{c}\right)^{\vee}\simeq\tau. We may take the unique isomorphism

𝒜w:𝒱τ𝒱π0𝒱τ𝒱π0\mathcal{A}_{w}:\mathscr{V}_{\tau}\otimes\mathscr{V}_{\pi_{0}}\longrightarrow\mathscr{V}_{\tau}\otimes\mathscr{V}_{\pi_{0}}

such that:

  • 𝒜w(w(τπ0))(m)=(τπ0)(m)𝒜w\mathcal{A}_{w}\circ(w(\tau\boxtimes\pi_{0}))(m)=(\tau\boxtimes\pi_{0})(m)\circ\mathcal{A}_{w} for all mMPm\in M_{P};

  • 𝒜w=𝒜w1𝒱π0\mathcal{A}_{w}=\mathcal{A}_{w}^{\prime}\otimes 1_{\mathscr{V}_{\pi_{0}}} with an isomorphism

    𝒜w:𝒱τ𝒱τ\mathcal{A}_{w}^{\prime}:\mathscr{V}_{\tau}\longrightarrow\mathscr{V}_{\tau}

    as described in [Art13] Section 2.2, or [Mok15] Section 3.2.

Note that 𝒜w2=1𝒱τ𝒱π0\mathcal{A}_{w}^{2}=1_{\mathscr{V}_{\tau}\otimes\mathscr{V}_{\pi_{0}}}. We define a self-intertwining operator

R(w,τπ0):IndPG(τπ0)IndPG(τπ0)R(w,\tau\boxtimes\pi_{0}):\operatorname{Ind}_{P}^{G}(\tau\boxtimes\pi_{0})\longrightarrow\operatorname{Ind}_{P}^{G}(\tau\boxtimes\pi_{0})

by

R(w,τσ0)Φ(g)=𝒜w((w,τσ0)Φ(g)).R(w,\tau\boxtimes\sigma_{0})\varPhi(g)=\mathcal{A}_{w}(\mathcal{R}(w,\tau\boxtimes\sigma_{0})\varPhi(g)).

We shall also use the notation R(w,τπ0,ψF)R(w,\tau\boxtimes\pi_{0},\psi_{F}) if we want to emphasize the dependence of R(w,τπ0)R(w,\tau\boxtimes\pi_{0}) on the additive character ψF\psi_{F}.

Similarly, we can define the intertwining operator for HH, with respect to a Whittaker datum 𝒲ψF\mathscr{W}_{\psi_{F}} of HH, where

𝒲ψF={𝒲1Case O;𝒲Case U.\mathscr{W}_{\psi_{F}}=\begin{cases}\mathscr{W}^{\prime}_{1}\quad&\textit{Case $O$};\\ \mathscr{W}^{\prime}\quad&\textit{Case $U$}.\end{cases}

We put

w~=wQmQ((1)rκWJ)(1W0)k,\widetilde{w}=w_{Q}\cdot m_{Q}\left((-1)^{r^{\prime}}\cdot\kappa_{W}\cdot J\right)\cdot(-1_{W_{0}})^{k},

where wQw_{Q} is as in Section 3, r=[dimW/2]r^{\prime}=[\dim W/2], and

κW={1Case O;δCase U0;1Case U1,\kappa_{W}=\begin{cases}1\quad&\textit{Case $O$};\\ -\delta\quad&\textit{Case $U_{0}$};\\ 1\quad&\textit{Case $U_{1}$},\end{cases}

Let σ0\sigma_{0} be an irreducible unitary representation of H0H_{0} lies in some local AA-packet Πψ0A(H0)\Pi_{\psi^{\prime}_{0}}^{A}(H_{0}). We denote the LL-parameters associated to the AA-parameter ψ\psi^{\prime} by ϕ0\phi^{\prime}_{0}. We set

r(w,τsσ0)=λ(w,ψF)γ(s,ϕτ(ϕ0),ψE)1γ(2s,Rϕτ,ψF)1,r(w,\tau_{s}\boxtimes\sigma_{0})=\lambda(w,\psi_{F})\cdot\gamma\left(s,\phi_{\tau}\otimes\left(\phi^{\prime}_{0}\right)^{\vee},\psi_{E}\right)^{-1}\cdot\gamma(2s,R\circ\phi_{\tau},\psi_{F})^{-1},

where

λ(w,ψF)={1Case O;λ(E/F,ψF)(k+1)k/2Case U0;λ(E/F,ψF)(k1)k/2Case U1,\lambda(w,\psi_{F})=\begin{cases}1\quad&\textit{Case $O$};\\ \lambda(E/F,\psi_{F})^{(k+1)k/2}\quad&\textit{Case $U_{0}$};\\ \lambda(E/F,\psi_{F})^{(k-1)k/2}\quad&\textit{Case $U_{1}$},\end{cases}

and

R={2Case O;As+Case U0;AsCase U1.R=\begin{cases}\bigwedge^{2}\quad&\textit{Case $O$};\\ As^{+}\quad&\textit{Case $U_{0}$};\\ As^{-}\quad&\textit{Case $U_{1}$}.\end{cases}

Put

(w,τsσ0)|κW|kρQr(w,τsσ0)1(w~,τsσ0),\mathcal{R}(w,\tau_{s}\boxtimes\sigma_{0})\coloneqq|\kappa_{W}|^{k\rho_{Q}}\cdot r(w,\tau_{s}\boxtimes\sigma_{0})^{-1}\cdot\mathcal{M}(\widetilde{w},\tau_{s}\boxtimes\sigma_{0}),

it follows from Arthur and Mok’s work that this normalized intertwining operator is holomorphic at s=0s=0. Assume that w(τσ0)τσ0w(\tau\boxtimes\sigma_{0})\simeq\tau\boxtimes\sigma_{0}, we take an isomorphism 𝒜w\mathcal{A}_{w} similarly, and define the self-intertwining operator R(w,τσ0)R(w,\tau\boxtimes\sigma_{0}) by

R(w,τσ0)Φ(h)=𝒜w((w,τsσ0)Φ(h))R(w,\tau\boxtimes\sigma_{0})\varPhi(h)=\mathcal{A}_{w}\left(\mathcal{R}(w,\tau_{s}\boxtimes\sigma_{0})\varPhi(h)\right)

for ΦIndQH(τσ0)\varPhi\in\operatorname{Ind}_{Q}^{H}\left(\tau\boxtimes\sigma_{0}\right), and hHh\in H.

7.2. Local intertwining relation: an alternative version

Now we can state the desired version of the local intertwining relation, which gives us a chance to interpret the “labeling” of a local AA-packet as some representation-theoretical quantities. For the original version of the local intertwining relation, one can refer to [Art13] Proposition 2.4.3 (Case OO), [Mok15] Proposition 3.4.4, and also [KMSW14] Chapter 2 (Case UU).

Theorem 7.2 (LIR-B for quasi-split groups).

Suppose that G=GG=G^{*} is quasi-split. Let π\pi be an irreducible constituent of IndPG(τπ0)\operatorname{Ind}_{P}^{G}(\tau\boxtimes\pi_{0}). Then:

  1. (1)

    π\pi is in the local AA-packet ΠψA(G)\Pi_{\psi}^{A}(G), where

    ψ=ψτ+ψ0+(ψτc);\psi=\psi_{\tau}+\psi_{0}+\left(\psi_{\tau}^{c}\right)^{\vee};
  2. (2)

    if we regard 𝒮ψ0\mathcal{S}_{\psi_{0}} as a subgroup of 𝒮ψ\mathcal{S}_{\psi} via the natural embedding, then

    𝒥𝒲ψFA(π)|𝒮ψ0=𝒥𝒲ψFA(π0);\mathcal{J}^{A}_{\mathscr{W}_{\psi_{F}}}(\pi)\Big{|}_{\mathcal{S}_{\psi_{0}}}=\mathcal{J}^{A}_{\mathscr{W}_{\psi_{F}}}(\pi_{0});
  3. (3)

    if we further assume that ψτ\psi_{\tau} is (conjugate) self-dual with the same parity as ψ\psi, then the restriction of the normalized intertwining operator R(w,τπ0,ψF)R(w,\tau\boxtimes\pi_{0},\psi_{F}) to π\pi is the scalar multiplication by

    R(w,τπ0)|π=𝒥𝒲ψFA(π)(aτ),R(w,\tau\boxtimes\pi_{0})\Big{|}_{\pi}=\mathcal{J}^{A}_{\mathscr{W}_{\psi_{F}}}(\pi)(a_{\tau}),

    where aτa_{\tau} is the element in 𝒮ψ\mathcal{S}_{\psi} corresponding to ψτ\psi_{\tau}.

Similar results also hold for the group HH.

Proof.

The first and second claims directly follow from [Art13] Proposition 2.4.3 in Case OO, and [Mok15] Proposition 3.4.4 in Case UU. We show the last claim. Indeed, this proof is almost the same as that of [Ato17] Theorem 2.4. In that paper, Atobe proved this LIR-B in the tempered case. We shall use some notations occuring in [Art13] diagram (2.4.3) or in [Mok15] diagram (3.4.2) without explanations.

Since ψτ\psi_{\tau} and ψ0\psi_{0} are (conjugate) self-dual representations (with appropriate parity), there are non-degenerated bilinear forms Bτ(,)B_{\tau}\left(\cdot,\cdot\right) and BV0(,)B_{V_{0}}\left(\cdot,\cdot\right) on k\mathbb{C}^{k} and N0\mathbb{C}^{N_{0}} respectively, where N0N_{0} is the dimension of the standard representation of G^0\widehat{G}_{0}, such that they are preserved by ψτ\psi_{\tau} and ψ0\psi_{0}, in the sense that for all wLE×SL2w\in L_{E}\times SL_{2}, we have

Bτ(ψτ(w)v,ψτc(w)v)=Bτ(v,v)for all v,vk,B_{\tau}\left(\psi_{\tau}(w)v,\psi_{\tau}^{c}(w)v^{\prime}\right)=B_{\tau}\left(v,v^{\prime}\right)\quad\textit{for all }v,v^{\prime}\in\mathbb{C}^{k},

and

BV0(ψ0(w)v,ψ0c(w)v)=BV0(v,v)for all v,vN0.B_{V_{0}}\left(\psi_{0}(w)v,\psi_{0}^{c}(w)v^{\prime}\right)=B_{V_{0}}\left(v,v^{\prime}\right)\quad\textit{for all }v,v^{\prime}\in\mathbb{C}^{N_{0}}.

Let AτA_{\tau} and A0A_{0} be two matrices represent these two forms respectively. We regard G^\widehat{G} as the cc-isometry group with respect to the biliner form represented by the matrix diag(Aτ,A0,Aτ)diag(A_{\tau},A_{0},-A_{\tau}). Let {e1,,ek,e1,,eN0,e1′′,,ek′′}\{e^{\prime}_{1},\cdots,e^{\prime}_{k},e_{1},\cdots,e_{N_{0}},e^{\prime\prime}_{1},\cdots,e^{\prime\prime}_{k}\} be the canonical basis of V^=N\widehat{V}=\mathbb{C}^{N}, where N=N0+2kN=N_{0}+2k. Then M^P\widehat{M}_{P} can be realized as the Levi subgroup of G^\widehat{G} stabilizing two isotropic subspaces

X^=Span{ei+ei′′|i=1,,k}andX^=Span{eiei′′|i=1,,k}.\widehat{X}=Span\{e^{\prime}_{i}+e^{\prime\prime}_{i}~{}|~{}i=1,\cdots,k\}\quad\textit{and}\quad\widehat{X}^{*}=Span\{e^{\prime}_{i}-e^{\prime\prime}_{i}~{}|~{}i=1,\cdots,k\}.

Note that the image of ψ\psi stabilizes these two subspaces, so we can also regard G^0\widehat{G}_{0} as the cc-isometry group with respect to the bilinear form represent by the matrix A0A_{0} on V^0=Span{e1,,eN0}\widehat{V}_{0}=Span\{e_{1},\cdots,e_{N_{0}}\}. Via these identifications, we have M^PGL(X^)×G^0\widehat{M}_{P}\simeq GL(\widehat{X})\times\widehat{G}_{0}.

Let ψMP=(ψτ,ψ0)\psi_{M_{P}}=(\psi_{\tau},\psi_{0}) be a local AA-parameter for MPM_{P}, and πMP=τπ0\pi_{M_{P}}=\tau\boxtimes\pi_{0} be an irreducible unitary representation lies in ΠψMPA(MP)\Pi_{\psi_{M_{P}}}^{A}(M_{P}). Let 𝒰G^\mathscr{U}\in\widehat{G} be the element which acts on {e1,,ek,e1,,eN0}\{e^{\prime}_{1},\cdots,e^{\prime}_{k},e_{1},\cdots,e_{N_{0}}\} by 11 and on {e1′′,,ek′′}\{e^{\prime\prime}_{1},\cdots,e^{\prime\prime}_{k}\} by 1-1. Then 𝒰Norm(AM^P,Sψ)\mathscr{U}\in Norm\left(A_{\widehat{M}_{P}},S_{\psi}\right). We write uu for the image of 𝒰\mathscr{U} in 𝔑ψ(G,MP)\mathfrak{N}_{\psi}(G,M_{P}). One can easily check the following

  • the image of uu in Wψ(G,MP)W(MP)W_{\psi}(G,M_{P})\subset W(M_{P}) is the unique non-trivial element ww;

  • the image of uu in 𝒮ψ(G,MP)𝒮ψ\mathcal{S}_{\psi}(G,M_{P})\subset\mathcal{S}_{\psi} is aτa_{\tau};

  • as endomorphisms of IndPG(πMP)\operatorname{Ind}_{P}^{G}\left(\pi_{M_{P}}\right), RP(wu,π~MP,ψMP)=R(w,τπ0)R_{P}(w_{u},\widetilde{\pi}_{M_{P}},\psi_{M_{P}})=R(w,\tau\boxtimes\pi_{0}).

By applying the endoscopic character identity ([Art13] Theorem 2.2.1 in Case OO or [Mok15] Theorem 3.2.1 in Case UU) and the original local intertwining relation ([Art13] Theoerem 2.4.1 in Case OO or [Mok15] Theorem 3.4.3 in Case UU) to uu, we obtain

(7.1) πΠψA(G)𝒥𝒲ψFA(π)(aτ)Θπ(f)=π0Πψ0A(G0)u~,τπ0~Tr(R(w,τπ0)IndPG(τπ0,f))\sum_{\pi\in\Pi_{\psi}^{A}(G)}\mathcal{J}^{A}_{\mathscr{W}_{\psi_{F}}}(\pi)(a_{\tau})\cdot\Theta_{\pi}(f)=\sum_{\pi_{0}\in\Pi_{\psi_{0}}^{A}(G_{0})}\langle\widetilde{u},\widetilde{\tau\boxtimes\pi_{0}}\rangle\operatorname{Tr}\left(R(w,\tau\boxtimes\pi_{0})\operatorname{Ind}_{P}^{G}(\tau\boxtimes\pi_{0},f)\right)

for any f(G)f\in\mathcal{H}(G). The constant u~,τπ0~\langle\widetilde{u},\widetilde{\tau\boxtimes\pi_{0}}\rangle can be computed as follows (see [Mok15] bottom of page 62 in Case UU): the restriction map

Norm(AM^P,Sψ)G^0,𝒰𝒰|V0Norm\left(A_{\widehat{M}_{P}},S_{\psi}\right)\longrightarrow\widehat{G}_{0},\quad\mathscr{U}^{\prime}\longmapsto\mathscr{U}^{\prime}\Big{|}_{V_{0}}

induces a section

𝔰:𝔑ψ(G,MP)𝒮ψ0\mathfrak{s}:\mathfrak{N}_{\psi}(G,M_{P})\longrightarrow\mathcal{S}_{\psi_{0}}

then we have

u~,τπ0~=𝒥𝒲ψFA(π0)(𝔰(u))\langle\widetilde{u},\widetilde{\tau\boxtimes\pi_{0}}\rangle=\mathcal{J}^{A}_{\mathscr{W}_{\psi_{F}}}(\pi_{0})\left(\mathfrak{s}(u)\right)

By the definition of 𝒰\mathscr{U} and uu we have 𝔰(u)=1\mathfrak{s}(u)=1, thus u~,τπ0~=1\langle\widetilde{u},\widetilde{\tau\boxtimes\pi_{0}}\rangle=1. Then equation (7.1) together Mœglin’s multiplicity-freeness result Theorem 4.2 will imply that

πΠψA(G)𝒥𝒲ψFA(π)(aτ)Θπ(f)=π0Πψ0A(G0)πIndPG(τπ0)Tr(R(w,τπ0)π(f))\sum_{\pi\in\Pi_{\psi}^{A}(G)}\mathcal{J}^{A}_{\mathscr{W}_{\psi_{F}}}(\pi)(a_{\tau})\cdot\Theta_{\pi}(f)=\sum_{\pi_{0}\in\Pi_{\psi_{0}}^{A}(G_{0})}\sum_{\pi\subset\operatorname{Ind}_{P}^{G}(\tau\boxtimes\pi_{0})}\operatorname{Tr}(R(w,\tau\boxtimes\pi_{0})\pi(f))

for any f(G)f\in\mathcal{H}(G). Therefore by Schur’s Lemma and linear independence of characters, we have

R(w,τπ0)|π=𝒥𝒲ψFA(π)(aτ).R(w,\tau\boxtimes\pi_{0})\Big{|}_{\pi}=\mathcal{J}^{A}_{\mathscr{W}_{\psi_{F}}}(\pi)(a_{\tau}).

There is also an anolog for θ\theta-packets.

Theorem 7.3 (LIR-B for θ\theta-packets).

Suppose that G=G(Vϵ)G=G(V^{\epsilon}) is an even orthogonal or unitary group as in Section 3 (which is not necessarily quasi-split). Let π\pi be an irreducible constituent of IndPG(τπ0)\operatorname{Ind}_{P}^{G}(\tau\boxtimes\pi_{0}). Then:

  1. (1)

    π\pi is in the local θ\theta-packet Πψθ(G)\Pi_{\psi}^{\theta}(G), where

    ψ=ψτ+ψ0+(ψτc);\psi=\psi_{\tau}+\psi_{0}+\left(\psi_{\tau}^{c}\right)^{\vee};
  2. (2)

    if we regard 𝒮ψ0\mathcal{S}_{\psi_{0}} as a subgroup of 𝒮ψ\mathcal{S}_{\psi} via the natural embedding, then

    𝒥ψF(π)|𝒮ψ0=𝒥ψF(π0);\mathcal{J}_{\psi_{F}}(\pi)\Big{|}_{\mathcal{S}_{\psi_{0}}}=\mathcal{J}_{\psi_{F}}(\pi_{0});
  3. (3)

    if we further assume that ψτ\psi_{\tau} is (conjugate) self-dual with the same parity as ψ\psi, then the restriction of the normalized intertwining operator R(w,τπ0,ψF)R(w,\tau\boxtimes\pi_{0},\psi_{F}) to π\pi is the scalar multiplication by

    R(w,τπ0)|π=ϵk𝒥ψF(π)(aτ),R(w,\tau\boxtimes\pi_{0})\Big{|}_{\pi}=\epsilon^{k}\cdot\mathcal{J}_{\psi_{F}}(\pi)(a_{\tau}),

    where aτa_{\tau} is the element in 𝒮ψ\mathcal{S}_{\psi} which corresponds to ψτ\psi_{\tau}.

We shall devote to proving this theorem in the next section. Combining this theorem with Corollary 5.13 and Theorem 7.2, we deduce

Corollary 7.4.

Theorem 2.8 holds.

Proof.

In Corollary 5.13 we have proved that as sets, θ\theta-packets are independent of the choice of H=H(W(r))H=H\left(W_{(r)}\right). It remains to show that the “labeling” is also independent of the choice of H=H(W(r))H=H\left(W_{(r)}\right). Let G=G(Vϵ)G=G(V^{\epsilon}), ψ\psi be a local AA-parameter for GG, and π\pi be an irreducible unitary representation in the packet Πψθ(G)\Pi_{\psi}^{\theta}(G). We shall prove that 𝒥ψF(π)\mathcal{J}_{\psi_{F}}(\pi) is also independent of the choice of HH.

Let ψτi\psi_{\tau_{i}} be any irreducible (conjugate) self-dual subrepresentation of ψ\psi, and also with the same parity as ψ\psi. Then ψτi\psi_{\tau_{i}} correponds to an irreducible unitary representation τi\tau_{i} of GLd(E)GL_{d}(E), for some ddimVd\leq\dim V. Let V~=V+d\widetilde{V}=V+\mathcal{H}^{d}, where \mathcal{H} is the (cc-Hermitian) hyperbolic plane. We can decompose V~\widetilde{V} as following

V~=Xτi+V+Xτi,\widetilde{V}=X_{\tau_{i}}+V+X_{\tau_{i}}^{*},

where XτiX_{\tau_{i}} and XτiX_{\tau_{i}}^{*} are dd-dimensional totally isotropic subspaces of V~\widetilde{V} such that XτiXτidX_{\tau_{i}}\oplus X_{\tau_{i}}^{*}\simeq\mathcal{H}^{d} and orthogonal to VV. Let P~\widetilde{P} be the maximal parabolic subgroup of G~=G(V~)\widetilde{G}=G(\widetilde{V}) stabilizing XτiX_{\tau_{i}} and L~\widetilde{L} be its Levi component stabilizing XτiX_{\tau_{i}}^{*}, so that

L~GL(Xτi)×G.\widetilde{L}\simeq GL(X_{\tau_{i}})\times G.

We consider the induced representation IndP~G~(τiπ)\operatorname{Ind}_{\widetilde{P}}^{\widetilde{G}}(\tau_{i}\boxtimes\pi). Let π~\widetilde{\pi} be any irreducible constituent of IndP~G~(τiπ)\operatorname{Ind}_{\widetilde{P}}^{\widetilde{G}}(\tau_{i}\boxtimes\pi). By Theorem 7.3, we know that it lies in the θ\theta-packet Πψ~θ(G~)\Pi_{\widetilde{\psi}}^{\theta}(\widetilde{G}), with

ψ~=ψτi+ψ+(ψτic);\widetilde{\psi}=\psi_{\tau_{i}}+\psi+\left(\psi_{\tau_{i}}^{c}\right)^{\vee};

also the “labeling” of π~\widetilde{\pi} is related to the “labeling” of π\pi by

𝒥ψF(π~)|𝒮ψ=𝒥ψF(π),\mathcal{J}_{\psi_{F}}(\widetilde{\pi})\Big{|}_{\mathcal{S}_{\psi}}=\mathcal{J}_{\psi_{F}}(\pi),

where we use the natural map 𝒮ψ𝒮ψ~\mathcal{S}_{\psi}\simeq\mathcal{S}_{\widetilde{\psi}} to identify 𝒮ψ\mathcal{S}_{\psi} with 𝒮ψ~\mathcal{S}_{\widetilde{\psi}}. Let R(w,τiπ)R(w,\tau_{i}\boxtimes\pi) be the normalized intertwining operator defined in Section 7.1. Then Theorem 7.3 also asserts that

𝒥ψF(π~)(aτi)=ϵdR(w,τiπ)|π~,\mathcal{J}_{\psi_{F}}(\widetilde{\pi})(a_{\tau_{i}})=\epsilon^{d}\cdot R(w,\tau_{i}\boxtimes\pi)\big{|}_{\widetilde{\pi}},

where aτia_{\tau_{i}} is the element in 𝒮ψ\mathcal{S}_{\psi} corresponding to ψτi\psi_{\tau_{i}}. Since ψτi\psi_{\tau_{i}} is arbitrary, and ϵdR(w,τiπ)|π~\epsilon^{d}\cdot R(w,\tau_{i}\boxtimes\pi)\big{|}_{\widetilde{\pi}} is obviously independent of the choice of HH, it follows that 𝒥ψF(π)\mathcal{J}_{\psi_{F}}(\pi) is also independent of the choice of HH.

When ϵ=+1\epsilon=+1, G=GG=G^{*} is quasi-split, we have also proved in Corollary 5.13 that as sets, θ\theta-packets and AA-packets coincide. In this case by Theorem 7.2 we also have

𝒥𝒲ψFA(π~)|𝒮ψ=𝒥𝒲ψFA(π),\mathcal{J}^{A}_{\mathscr{W}_{\psi_{F}}}(\widetilde{\pi})\Big{|}_{\mathcal{S}_{\psi}}=\mathcal{J}^{A}_{\mathscr{W}_{\psi_{F}}}(\pi),

and

𝒥𝒲ψFA(π~)(aτi)=R(w,τiπ)|π~.\mathcal{J}^{A}_{\mathscr{W}_{\psi_{F}}}(\widetilde{\pi})(a_{\tau_{i}})=R(w,\tau_{i}\boxtimes\pi)\big{|}_{\widetilde{\pi}}.

These equalities imply that

𝒥ψF(π)=𝒥𝒲ψFA(π).\mathcal{J}_{\psi_{F}}(\pi)=\mathcal{J}^{A}_{\mathscr{W}_{\psi_{F}}}(\pi).

This completes the proof. ∎

7.3. Changes of Whittaker data

As an application of the LIR-B, we prove a formula which concerns the behavior of the “labeling” in a local AA-packet for HH with respect to changes of Whittaker data.

In this subsection, we shall temporarily use ψ\psi to denote a local AA-parameter for HH. Let σ\sigma be an irreducible unitary representation in ΠψA(H)\Pi_{\psi}^{A}(H). Let 𝒲ψF\mathscr{W}_{\psi_{F}} and 𝒲ψF,c\mathscr{W}_{\psi_{F,c}} be the two Whittaker data of HH, associated to the additive character ψF\psi_{F} and ψF,c\psi_{F,c} respectively, where cF×c\in F^{\times}.

Lemma 7.5.

Let η=𝒥𝒲ψFA(σ)\eta=\mathcal{J}^{A}_{\mathscr{W}_{\psi_{F}}}(\sigma) and η=𝒥𝒲ψF,cA(σ)\eta^{\prime}=\mathcal{J}^{A}_{\mathscr{W}_{\psi_{F,c}}}(\sigma). Then we have

η=ηηψ,c,\eta^{\prime}=\eta\cdot\eta_{\psi,c},

where ηψ,c\eta_{\psi,c} is the character of 𝒮ψ\mathcal{S}_{\psi} defined by

ηψ,c(ai)=det(ψi)(c),\eta_{\psi,c}(a_{i})=\det(\psi_{i})(c),

for the element aia_{i} in 𝒮ψ\mathcal{S}_{\psi} which corresponds to an irreducible constituent ψi\psi_{i} of ψ\psi.

Proof.

Similar to the proof of Corollary 7.4, given G,ψ,πG,\psi,\pi and ψτi\psi_{\tau_{i}}, we define V~,G~,P~,L~\widetilde{V},\widetilde{G},\widetilde{P},\widetilde{L} and π~\widetilde{\pi}. Then we have

η(aτi)=R(w,τiπ,ψF)|π~,\eta(a_{\tau_{i}})=R(w,\tau_{i}\boxtimes\pi,\psi_{F})\big{|}_{\widetilde{\pi}},

and also

η(aτi)=R(w,τiπ,ψF,c)|π~.\eta^{\prime}(a_{\tau_{i}})=R(w,\tau_{i}\boxtimes\pi,\psi_{F,c})\big{|}_{\widetilde{\pi}}.

From the definition of (normalized) local intertwining operators, one can easily show that

R(w,τiπ,ψF,c)=R(w,τiπ,ψF)ωτi(c).R(w,\tau_{i}\boxtimes\pi,\psi_{F,c})=R(w,\tau_{i}\boxtimes\pi,\psi_{F})\cdot\omega_{\tau_{i}}(c).

Hence we have

η(aτi)=η(aτi)det(ψτi)(c).\eta^{\prime}(a_{\tau_{i}})=\eta(a_{\tau_{i}})\cdot\det(\psi_{\tau_{i}})(c).

Since ψτi\psi_{\tau_{i}} is arbitrary, we conclude that

η=ηηψ,c.\eta^{\prime}=\eta\cdot\eta_{\psi,c}.

This completes the proof. ∎

From the proof of this lemma one can see that certainly an analog of this lemma will also hold for the group GG. We omit the details here.

8. Completion of the proof

In this section we prove Lemma 7.1 and Theorem 7.3. These results will complete our proof of Theorem 2.8.

8.1. A diagram

We retain the notations in the last section. Having fixed irreducible unitary representations τ\tau, π0\pi_{0}, and σ0\sigma_{0}, we shall write

(w~P,s)\displaystyle\mathcal{R}({\widetilde{w}}_{P},s) =(w~P,τsχWπ0),\displaystyle=\mathcal{R}({\widetilde{w}}_{P},\tau_{s}\chi_{W}\boxtimes\pi_{0}),
(w~Q,s)\displaystyle\mathcal{R}({\widetilde{w}}_{Q},s) =(w~Q,τscχVcσ0)\displaystyle=\mathcal{R}\left({\widetilde{w}}_{Q},\tau^{c}_{s}\chi^{c}_{V}\boxtimes\sigma_{0}^{\vee}\right)

for the normalized intertwining operators. Recall that in Section 3, we have constructed a G×HG\times H-equivariant map

𝒯s:ωIndQH(τscχVcσ0)IndPG(τsχWπ0),\mathcal{T}_{s}:\omega\otimes\operatorname{Ind}_{Q}^{H}\left(\tau_{s}^{c}\chi_{V}^{c}\boxtimes\sigma_{0}^{\vee}\right)\longrightarrow\operatorname{Ind}_{P}^{G}\left(\tau_{s}\chi_{W}\boxtimes\pi_{0}\right),

where σ0=θψF,V0,W0(π0)\sigma_{0}=\theta_{\psi_{F},V_{0},W_{0}}(\pi_{0}). By the Howe duality, the diagram

(8.1) ωIndQH(τscχVcσ0)𝒯sIndPG(τsχWπ0)1(w~Q,s)(w~P,s)ωIndQH(wP(τscχVcσ0))𝒯sIndPG(wQ(τsχWπ0))\begin{CD}\omega\otimes\operatorname{Ind}_{Q}^{H}\left(\tau^{c}_{s}\chi^{c}_{V}\boxtimes\sigma_{0}^{\vee}\right)@>{\mathcal{T}_{s}}>{}>\operatorname{Ind}_{P}^{G}\left(\tau_{s}\chi_{W}\boxtimes\pi_{0}\right)\\ @V{1\otimes\mathcal{R}({\widetilde{w}}_{Q},s)}V{}V@V{}V{\mathcal{R}({\widetilde{w}}_{P},s)}V\\ \omega\otimes\operatorname{Ind}_{Q}^{H}\left(w_{P}\left(\tau^{c}_{s}\chi^{c}_{V}\boxtimes\sigma_{0}^{\vee}\right)\right)@>{\mathcal{T}_{-s}}>{}>\operatorname{Ind}_{P}^{G}\left(w_{Q}\left(\tau_{s}\chi_{W}\boxtimes\pi_{0}\right)\right)\end{CD}

commutes up to a scalar. This scalar can be computed explicitly as follows. Recall that τΠψτA(GLk(E))\tau\in\Pi_{\psi_{\tau}}^{A}\left(GL_{k}(E)\right), π0Πψ0θ(G0)\pi_{0}\in\Pi_{\psi_{0}}^{\theta}(G_{0}), and σ0Πθ(ψ0)A(H)\sigma_{0}\in\Pi_{\theta(\psi_{0})}^{A}(H) respectively, where

θ(ψ0)=ψ0χW1χV+χVS2r2n+1.\theta(\psi_{0})=\psi_{0}\chi_{W}^{-1}\chi_{V}+\chi_{V}\boxtimes S_{2r-2n+1}.

Let ϕτ\phi_{\tau}, ϕ0\phi_{0}, and ϕ0\phi^{\prime}_{0} be the LL-parameter associated to ψτ\psi_{\tau}, ψ0\psi_{0}, and θ(ψ0)\theta(\psi_{0}) respectively. Then

Proposition 8.1.

For φ𝒮\varphi\in\mathscr{S} and ΦsIndQH(τscχVcσ0)\varPhi_{s}\in\operatorname{Ind}_{Q}^{H}(\tau_{s}^{c}\chi^{c}_{V}\boxtimes\sigma_{0}^{\vee}), we have

(w~P,τsχWπ0)𝒯s(φΦs)=αβ(s)𝒯s(φ(w~Q,τscχVcσ0)Φs),\mathcal{R}(\widetilde{w}_{P},\tau_{s}\chi_{W}\boxtimes\pi_{0})\mathcal{T}_{s}(\varphi\otimes\varPhi_{s})=\alpha\cdot\beta(s)\cdot\mathcal{T}_{-s}\left(\varphi\otimes\mathcal{R}\left(\widetilde{w}_{Q},\tau^{c}_{s}\chi^{c}_{V}\boxtimes\sigma_{0}^{\vee}\right)\varPhi_{s}\right),

where

α={γVkχV(1)kωτ((1)rn+1c1)λ(w~P,ψF)1Case O;[γW1γVχW((1)n1κV1)χV((1)r1κW1)(χWdimVχVdimW)(δ)]k×ωτ((1)n+r1κWcκV1)λ(w~Q,ψF)λ(w~P,ψF)1Case U,\alpha=\begin{cases}\gamma_{V}^{k}\cdot\chi_{V}\left(-1\right)^{k}\cdot\omega_{\tau}\left((-1)^{r-n+1}\cdot c^{-1}\right)\cdot\lambda\left(\widetilde{w}_{P},\psi_{F}\right)^{-1}\quad&\textit{Case $O$};\\ ~{}\\ \left[\gamma_{W}^{-1}\cdot\gamma_{V}\cdot\chi_{W}\left((-1)^{n^{\prime}-1}\cdot\kappa_{V}^{-1}\right)\cdot\chi_{V}\left((-1)^{r^{\prime}-1}\cdot\kappa_{W}^{-1}\right)\cdot(\chi_{W}^{-\dim V}\chi_{V}^{\dim W})(\delta)\right]^{k}\\ \quad\times\omega_{\tau}\left((-1)^{n^{\prime}+r^{\prime}-1}\cdot\kappa_{W}^{c}\kappa_{V}^{-1}\right)\cdot\lambda(\widetilde{w}_{Q},\psi_{F})\cdot\lambda(\widetilde{w}_{P},\psi_{F})^{-1}\quad&\textit{Case $U$},\end{cases}

and

β(s)=\displaystyle\beta(s)= L(ss0,ϕτ)1L(ss0,(ϕτc))\displaystyle L\left(s-s_{0},\phi_{\tau}\right)^{-1}\cdot L\left(-s-s_{0},\left(\phi_{\tau}^{c}\right)^{\vee}\right)
×γ(ss0,(ϕτc),ψE)|κWκV1|ks\displaystyle\times\gamma\left(-s-s_{0},\left(\phi_{\tau}^{c}\right)^{\vee},\psi_{E}\right)\cdot|\kappa_{W}\kappa_{V}^{-1}|^{ks}
×γ(s,ϕτcχVcϕ0,ψE)1γ(s,ϕτχWϕ0,ψE).\displaystyle\times\gamma\left(s,\phi_{\tau}^{c}\chi_{V}^{c}\otimes\phi^{\prime}_{0},\psi_{E}\right)^{-1}\cdot\gamma\left(s,\phi_{\tau}\chi_{W}\otimes\phi_{0}^{\vee},\psi_{E}\right).
Proof.

Similar to [GI16] Proposition 8.4 and Corollary 8.5. ∎

Lemma 8.2.

The function β(s)\beta(s) is holomorphic at s=0s=0.

Proof.

Indeed, by the assumption that r>dimVr>\dim V, we have s0>ks_{0}>k. As τ\tau is of Arthur type, it follows from Remark 3.2 that L(ss0,ϕτ)1L\left(s-s_{0},\phi_{\tau}\right)^{-1}, L(ss0,(ϕτc))L\left(-s-s_{0},\left(\phi_{\tau}^{c}\right)^{\vee}\right), and γ(ss0,(ϕτc),ψE)\gamma\left(-s-s_{0},\left(\phi_{\tau}^{c}\right)^{\vee},\psi_{E}\right) should be holomorphic at s=0s=0. On the other hand, from the definitions one can easily see that

ϕ0=ϕ0χW1χV+χV(i=nrrn||i);\phi^{\prime}_{0}=\phi_{0}\chi_{W}^{-1}\chi_{V}+\chi_{V}\cdot\left(\bigoplus_{i=n-r}^{r-n}|\cdot|^{i}\right);

hence

(8.2) γ(s,ϕτcχVcϕ0,ψE)1γ(s,ϕτχWϕ0,ψE)=j=nrrnγ(s+j,ϕτ,ψE)1.\gamma\left(s,\phi_{\tau}^{c}\chi_{V}^{c}\otimes\phi^{\prime}_{0},\psi_{E}\right)^{-1}\cdot\gamma\left(s,\phi_{\tau}\chi_{W}\otimes\phi_{0}^{\vee},\psi_{E}\right)=\prod_{j=n-r}^{r-n}\gamma\left(s+j,\phi_{\tau},\psi_{E}\right)^{-1}.

If we write the AA-parameter ψτ\psi_{\tau} as

ψτ=iρiSaiSbi,\psi_{\tau}=\sum_{i}\rho_{i}\boxtimes S_{a_{i}}\boxtimes S_{b_{i}},

and let τi\tau_{i} be the irreducible unitary representation of some general linear group corresponding to the AA-parameter ρiSaiSbi\rho_{i}\boxtimes S_{a_{i}}\boxtimes S_{b_{i}}, then the RHS of equality (8.2) can be written as

j=nrrnγ(s+j,ϕτ,ψE)1=ij=nrrnγ(s+j,τi,ψE)1.\prod_{j=n-r}^{r-n}\gamma\left(s+j,\phi_{\tau},\psi_{E}\right)^{-1}=\prod_{i}\prod_{j=n-r}^{r-n}\gamma\left(s+j,\tau_{i},\psi_{E}\right)^{-1}.

Again, as explicated in Remark 3.2, if ρi≄𝟙\rho_{i}\not\simeq\mathbbm{1}, then

j=nrrnγ(s+j,τi,ψE)1\prod_{j=n-r}^{r-n}\gamma\left(s+j,\tau_{i},\psi_{E}\right)^{-1}

is holomorphic at s=0s=0; otherwise if ρi=𝟙\rho_{i}=\mathbbm{1}, then τiτi\tau_{i}\simeq\tau_{i}^{\vee}, and it follows from the functional equation that

j=nrrnγ(s+j,τi,ψE)1=γ(ss0,τi,ψE)1j=1rn(γ(s+j,τi,ψE)γ(s+1j,τi,ψE))1\prod_{j=n-r}^{r-n}\gamma\left(s+j,\tau_{i},\psi_{E}\right)^{-1}=\gamma\left(s-s_{0},\tau_{i},\psi_{E}\right)^{-1}\cdot\prod_{j=1}^{r-n}\Big{(}\gamma\left(s+j,\tau_{i},\psi_{E}\right)\cdot\gamma\left(s+1-j,\tau_{i}^{\vee},\psi_{E}\right)\Big{)}^{-1}

is also holomorphic at s=0s=0. Thus we can conclude that the function β(s)\beta(s) is holomorphic at s=0s=0. ∎

We deduce from diagram (8.1) that:

Corollary 8.3.

The normalized intertwining operator (w~P,τsχWπ0)\mathcal{R}({\widetilde{w}}_{P},\tau_{s}\chi_{W}\boxtimes\pi_{0}) is holomorphic at s=0s=0.

Proof.

Since τ\tau is of Arthur type, when r>dimVr>\dim V, the requirements in Proposition 3.1 and Corollary 3.3 are automatically satisfied. It follows that the equivariant map 𝒯s\mathcal{T}_{s} is surjective at s=0s=0. This fact allows us to “approximate” any holomorphic section of IndPG(τsχWπ0)\operatorname{Ind}_{P}^{G}\left(\tau_{s}\chi_{W}\boxtimes\pi_{0}\right) by images of 𝒯s\mathcal{T}_{s} at s=0s=0.

Let Φs\varPhi_{s} be a holomorphic section of IndPG(τsχWπ0)\operatorname{Ind}_{P}^{G}\left(\tau_{s}\chi_{W}\boxtimes\pi_{0}\right). Since 𝒯s\mathcal{T}_{s} is surjective at s=0s=0, we may take φ0𝒮\varphi_{0}\in\mathscr{S} and Ψ(0)IndQH(τcχVcσ0)\varPsi^{(0)}\in\operatorname{Ind}_{Q}^{H}\left(\tau^{c}\chi^{c}_{V}\boxtimes\sigma_{0}^{\vee}\right), such that

𝒯0(φ0Ψ(0))=Φ0.\mathcal{T}_{0}\left(\varphi_{0}\otimes\varPsi^{(0)}\right)=\varPhi_{0}.

We extend Ψ(0)\varPsi^{(0)} to a holomorphic section Ψs(0)\varPsi_{s}^{(0)} of IndQH(τscχVcσ0)\operatorname{Ind}_{Q}^{H}\left(\tau^{c}_{s}\chi^{c}_{V}\boxtimes\sigma_{0}^{\vee}\right). Then we have

Φs=𝒯s(φ0Ψs(0))+sΦs(1),\varPhi_{s}=\mathcal{T}_{s}\left(\varphi_{0}\otimes\varPsi_{s}^{(0)}\right)+s\cdot\varPhi_{s}^{(1)},

where

Φs(1)=s1(Φs𝒯s(φ0Ψs(0)))\varPhi_{s}^{(1)}=s^{-1}\cdot\bigg{(}\varPhi_{s}-\mathcal{T}_{s}\left(\varphi_{0}\otimes\varPsi_{s}^{(0)}\right)\bigg{)}

is again a holomorphic section of IndPG(τsχWπ0)\operatorname{Ind}_{P}^{G}\left(\tau_{s}\chi_{W}\boxtimes\pi_{0}\right). Repeat this procedure, for any positive integer kk, we obtain an expansion

Φs=0i<ksi𝒯s(φiΨs(i))+skΦs(k)\varPhi_{s}=\sum_{0\leq i<k}s^{i}\cdot\mathcal{T}_{s}\left(\varphi_{i}\otimes\varPsi_{s}^{(i)}\right)+s^{k}\cdot\varPhi_{s}^{(k)}

for some φi𝒮\varphi_{i}\in\mathscr{S}, Ψs(i)\varPsi_{s}^{(i)} holomorphic sections of IndQH(τscχVcσ0)\operatorname{Ind}_{Q}^{H}\left(\tau^{c}_{s}\chi^{c}_{V}\boxtimes\sigma_{0}^{\vee}\right), and another holomorphic section Φs(k)\varPhi_{s}^{(k)} of IndPG(τsχWπ0)\operatorname{Ind}_{P}^{G}\left(\tau_{s}\chi_{W}\boxtimes\pi_{0}\right). Hence

(w~P,τsχWπ0)Φs\displaystyle\mathcal{R}\left({\widetilde{w}}_{P},\tau_{s}\chi_{W}\boxtimes\pi_{0}\right)\varPhi_{s} =(w~P,τsχWπ0)(0i<ksi𝒯s(φiΨs(i)))+sk(w~P,τsχWπ0)Φs(k)\displaystyle=\mathcal{R}\left({\widetilde{w}}_{P},\tau_{s}\chi_{W}\boxtimes\pi_{0}\right)\left(\sum_{0\leq i<k}s^{i}\cdot\mathcal{T}_{s}\left(\varphi_{i}\otimes\varPsi_{s}^{(i)}\right)\right)+s^{k}\cdot\mathcal{R}\left({\widetilde{w}}_{P},\tau_{s}\chi_{W}\boxtimes\pi_{0}\right)\varPhi_{s}^{(k)}
=αβ(s)(0i<ksi𝒯s(φi(w~Q,τscχVcσ0)Ψs(i)))\displaystyle=\alpha\cdot\beta(s)\cdot\left(\sum_{0\leq i<k}s^{i}\cdot\mathcal{T}_{-s}\left(\varphi_{i}\otimes\mathcal{R}\left(\widetilde{w}_{Q},\tau^{c}_{s}\chi^{c}_{V}\boxtimes\sigma_{0}^{\vee}\right)\varPsi_{s}^{(i)}\right)\right)
+sk(w~P,τsχWπ0)Φs(k),\displaystyle\qquad\qquad+s^{k}\cdot\mathcal{R}\left({\widetilde{w}}_{P},\tau_{s}\chi_{W}\boxtimes\pi_{0}\right)\varPhi_{s}^{(k)},

where the second equality follows from the diagram (8.1). Since β(s)\beta(s), 𝒯s\mathcal{T}_{-s}, and (w~Q,τscχVcσ0)\mathcal{R}\left(\widetilde{w}_{Q},\tau^{c}_{s}\chi^{c}_{V}\boxtimes\sigma_{0}^{\vee}\right) are all holomorphic at s=0s=0, we know that the first term in the last equality is holomorphic at s=0s=0. On the other hand, since we already know that (w~P,τsχWπ0)\mathcal{R}\left({\widetilde{w}}_{P},\tau_{s}\chi_{W}\boxtimes\pi_{0}\right) is meromorphic, we may take the positive integer kk to be sufficiently large, such that

sk(w~P,τsχWπ0)s^{k}\cdot\mathcal{R}\left({\widetilde{w}}_{P},\tau_{s}\chi_{W}\boxtimes\pi_{0}\right)

is holomorphic at s=0s=0; then the second term in the last equality is also holomorphic at s=0s=0. It follows that (w~P,τsχWπ0)Φs\mathcal{R}\left({\widetilde{w}}_{P},\tau_{s}\chi_{W}\boxtimes\pi_{0}\right)\varPhi_{s} is holomorphic at s=0s=0. ∎

This corollary implies that Lemma 7.1 holds.

8.2. Contragredient and Arthur packets

To compute the “labeling” of θ\theta-packets using the diagram (8.1), we also need to know the behavior of AA-parameters and characters of component groups under taking contragredient. In this subsection, we prove such a formula for the group HH.

Proposition 8.4.

Let ψH\psi_{H} be a local AA-parameter for HH, and σΠψHA(H)\sigma\in\Pi_{\psi_{H}}^{A}(H) an irreducible unitary representation. Then

  1. (1)

    σ\sigma^{\vee} lie in the AA-packet ΠψHA(H)\Pi_{\psi_{H}^{\vee}}^{A}(H);

  2. (2)

    let ησ\eta_{\sigma} be the character of 𝒮ψH\mathcal{S}_{\psi_{H}} associated to σ\sigma, and ησ\eta_{\sigma^{\vee}} be the character of 𝒮ψH\mathcal{S}_{\psi_{H}^{\vee}} associated to σ\sigma^{\vee}, both with respective to the Whittaker datum 𝒲ψF\mathscr{W}_{\psi_{F}} of HH associated to the additive character ψF\psi_{F}, we have

    ησ=ησν,\eta_{\sigma^{\vee}}=\eta_{\sigma}\cdot\nu,

    where we use the obvious isomorphism between 𝒮ψH\mathcal{S}_{\psi_{H}} and 𝒮ψH\mathcal{S}_{\psi_{H}^{\vee}} to identify them, and the character ν\nu of 𝒮ψH\mathcal{S}_{\psi_{H}} is defined by

    ν(ai)=det(ψH,i)(1)\nu(a_{i})=\det(\psi_{H,i})(-1)

    for the element aia_{i} in 𝒮ψH\mathcal{S}_{\psi_{H}} which corresponds to an irreducible constituent ψH,i\psi_{H,i} of ψH\psi_{H}.

Proof.

Since the local AA-packets for general AA-parameters can be constructed using the parabolic induction from the good parity case, without loss of generality, we may assume that ψH\psi_{H} is of good parity.

Indeed, if σ\sigma lies in the LL-packet ΠϕψHL(H)\Pi_{\phi_{\psi_{H}}}^{L}(H) inside ΠψHA(H)\Pi_{\psi_{H}}^{A}(H), then the desired conclusions were already proved by Kaletha in [Kal13]. Hence in particular, if ψH=ϕH\psi_{H}=\phi_{H} is a square-integrable LL-parameter (regarded as an AA-parameter trivial on Arthur SL2SL_{2}) for HH, then this proposition holds for ψH\psi_{H}. We shall prove the good parity case based on this.

We first assume that ψH\psi_{H} is an elementary AA-parameter for HH, and is trivial on Weil-Deligne SL2SL_{2}. Then we have

ψH=ϕ^H\psi_{H}=\widehat{\phi}_{H}

for some square-integrable LL-parameter ϕH\phi_{H} for HH, where we use ϕ^H\widehat{\phi}_{H} to denote the Aubert involution of ϕH\phi_{H}. Since the Aubert involution commutes with taking contragredient (see [Aub95] Théorème 1.7), it follows from the compatibilities of AA-packets and the Aubert involution that the proposition also holds for these ψH\psi_{H}.

Next we appeal to the global method to prove this proposition for any ψH\psi_{H} of good parity. Let σ\sigma be an irreducible unitary representation in ΠψHA(H)\Pi_{\psi_{H}}^{A}(H). Similar to the proof of Corollary 4.12, we may construct a tuple of data (F˙,E˙,H˙,ψ˙H,u1,u2,w)(\dot{F},\dot{E},\dot{H},\dot{\psi}_{H},u_{1},u_{2},w), where

  • F˙\dot{F} is a number field, and E˙\dot{E} is either F˙\dot{F} itself or a quadratic extension of F˙\dot{F}, according the cases;

  • H˙\dot{H} a symplectic or quasi-split unitary group over F˙\dot{F}, according to the group HH; in the case that H˙\dot{H} is an unitary group, E˙\dot{E} is the splitting field of H˙\dot{H};

  • ψ˙H\dot{\psi}_{H} is an elliptic AA-parameter for H˙\dot{H};

  • u1u_{1}, u2u_{2}, and ww are finite places of F˙\dot{F}.

such that the following conditions hold:

  1. (1)

    (F˙u1,E˙u1,H˙u1,ψ˙H,u1)(F˙u2,E˙u2,H˙u2,ψ˙H,u2)(F,E,H,ψH)(\dot{F}_{u_{1}},\dot{E}_{u_{1}},\dot{H}_{u_{1}},\dot{\psi}_{H,u_{1}})\simeq(\dot{F}_{u_{2}},\dot{E}_{u_{2}},\dot{H}_{u_{2}},\dot{\psi}_{H,u_{2}})\simeq(F,E,H,\psi_{H});

  2. (2)

    if we are in the Case UU, then E˙w/F˙w\dot{E}_{w}/\dot{F}_{w} is a quadratic field extension;

  3. (3)

    the localization maps 𝒮ψ˙H𝒮ψ˙H,u1\mathcal{S}_{\dot{\psi}_{H}}\longrightarrow\mathcal{S}_{\dot{\psi}_{H,u_{1}}} and 𝒮ψ˙H𝒮ψ˙H,u2\mathcal{S}_{\dot{\psi}_{H}}\longrightarrow\mathcal{S}_{\dot{\psi}_{H,u_{2}}} agree, and they are surjections;

  4. (4)

    ψ˙H,w\dot{\psi}_{H,w} is elementary, and is trivial on the Weil-Deligne SL2SL_{2}; moreover, the localization map 𝒮ψ˙𝒮ψ˙w\mathcal{S}_{\dot{\psi}}\longrightarrow\mathcal{S}_{\dot{\psi}_{w}} is an isomorphism.

Let SS be a finite set of places of F˙\dot{F}, include u1u_{1}, u2u_{2}, ww, and all Archimedean places, such that for all vSv\notin S, the group H˙v\dot{H}_{v}, and the local AA-parameter ψ˙H,v\dot{\psi}_{H,v} are both unramified. We construct an automorphic representation σ˙\dot{\sigma} which occurs in the automorphic discrete spectrum of H˙\dot{H} with elliptic AA-parameter ψ˙H\dot{\psi}_{H} as follows:

  • at a place vSv\notin S, σ˙v\dot{\sigma}_{v} is the unramified representation of H˙v\dot{H}_{v} with LL-parameter ϕψ˙H,v\phi_{\dot{\psi}_{H,v}};

  • at a place vS\{u1,u2,w}v\in S\backslash\{u_{1},u_{2},w\}, let σ˙v\dot{\sigma}_{v} be an arbitrarily given representation of H˙v\dot{H}_{v} lies in the AA-packet Πψ˙H,vA(H˙v)\Pi_{\dot{\psi}_{H,v}}^{A}(\dot{H}_{v});

  • at the places u1u_{1} and u2u_{2}, σ˙u1=σ˙u2=σ\dot{\sigma}_{u_{1}}=\dot{\sigma}_{u_{2}}=\sigma;

  • at the place ww, σ˙w\dot{\sigma}_{w} lies in the AA-packet Πψ˙H,wA(H)\Pi_{\dot{\psi}_{H,w}}^{A}(H), corresponds to the character ησw\eta_{\sigma_{w}} of 𝒮ψ˙H,w\mathcal{S}_{\dot{\psi}_{H,w}}, determined by the formula

    vηv=ϵψ˙H,\prod_{v}\eta_{v}=\epsilon_{\dot{\psi}_{H}},

    where ηv=𝒥𝒲ψFA(σ˙v)\eta_{v}=\mathcal{J}_{\mathscr{W}_{\psi_{F}}}^{A}(\dot{\sigma}_{v}), and ϵψ˙H\epsilon_{\dot{\psi}_{H}} is the canonical sign character associated to ψ˙H\dot{\psi}_{H}. It follows from Lemma 4.6 that σ˙w0\dot{\sigma}_{w}\neq 0.

Then, according to the Arthur’s multiplicity formula for H˙\dot{H}, σ˙\dot{\sigma} is an irreducible subrepresentation of Lψ˙H2(H˙)L^{2}_{\dot{\psi}_{H}}(\dot{H}). Consider the contragredient σ˙\dot{\sigma}^{\vee} of σ˙\dot{\sigma}. It is not hard to see that σ˙\dot{\sigma}^{\vee} also occurs in the automorphic discrete spectrum of H˙\dot{H}, with elliptic AA-parameter ψ˙H\dot{\psi}_{H}^{\vee}. Indeed, any realization 𝒱\mathcal{V} of σ˙\dot{\sigma} in 𝒜2(H˙)\mathcal{A}^{2}(\dot{H}) gives a realization

𝒱¯={f¯|f𝒱}\overline{\mathcal{V}}=\left\{\overline{f}~{}\big{|}~{}f\in\mathcal{V}\right\}

of σ˙\dot{\sigma}^{\vee} in 𝒜2(H˙)\mathcal{A}^{2}(\dot{H}), where f¯\overline{f} means the complex conjugate of the function ff. By the Arthur’s multiplicity formula for H˙\dot{H}, localizing at the place u1u_{1}, we obtain

σΠψHA(H).\sigma^{\vee}\in\Pi_{\psi_{H}^{\vee}}^{A}(H).

Let ϵψ˙H\epsilon_{\dot{\psi}_{H}^{\vee}} be the canonical sign character associated to ψ˙H{\dot{\psi}_{H}^{\vee}}. If we identify 𝒮ψ˙H\mathcal{S}_{\dot{\psi}_{H}} and 𝒮ψ˙H\mathcal{S}_{\dot{\psi}_{H}^{\vee}} in the obvious way, then

ϵψ˙H=ϵψ˙H.\epsilon_{\dot{\psi}_{H}}=\epsilon_{\dot{\psi}_{H}^{\vee}}.

Indeed, if HH is a symplectic group, this is obvious; if HH is an unitary group, this follows from the fact that the epsilon factor is invariant under the Galois conjugation. Then comparing Arthur’s multiplicity formula for σ˙\dot{\sigma} and σ˙\dot{\sigma}^{\vee}, we get

(8.3) vS\{u1,u2,w}ησv=vS\{u1,u2,w}ησvνv\prod_{v\in S\backslash\{u_{1},u_{2},w\}}\eta_{\sigma_{v}^{\vee}}=\prod_{v\in S\backslash\{u_{1},u_{2},w\}}\eta_{\sigma_{v}}\cdot\nu_{v}

as characters of 𝒮ψ˙H\mathcal{S}_{\dot{\psi}_{H}}. Here we use the fact that the proposition holds for ψ˙H,w\dot{\psi}_{H,w} and places outside SS.

Now we construct another automorphic representation σ˙\dot{\sigma}^{\prime} occuring in the automorphic discrete spectrum of H˙\dot{H} with elliptic AA-parameter ψ˙H\dot{\psi}_{H} as following:

  • at a place v{u2,w}v\notin\{u_{2},w\}, σv=σv\sigma^{\prime}_{v}=\sigma_{v};

  • at the place u2u_{2}, let σ˙u2\dot{\sigma}^{\prime}_{u_{2}} be an irreducible unitary representation in the LL-packet ΠϕψHL(H)\Pi_{\phi_{\psi_{H}}}^{L}(H);

  • at the place ww, σ˙w\dot{\sigma}^{\prime}_{w} lies in the AA-packet Πψ˙H,wA(H)\Pi_{\dot{\psi}_{H,w}}^{A}(H), corresponds to the character ησw\eta_{\sigma^{\prime}_{w}} of 𝒮ψ˙H,w\mathcal{S}_{\dot{\psi}_{H,w}}, which is determined by the formula

    vηv=ϵψ˙H,\prod_{v}\eta^{\prime}_{v}=\epsilon_{\dot{\psi}_{H}},

    where ηv=𝒥𝒲ψFA(σ˙v)\eta^{\prime}_{v}=\mathcal{J}_{\mathscr{W}_{\psi_{F}}}^{A}(\dot{\sigma}^{\prime}_{v}). It follows from Lemma 4.6 that σ˙w0\dot{\sigma}^{\prime}_{w}\neq 0.

Then, according to the Arthur’s multiplicity formula for H˙\dot{H}, σ˙\dot{\sigma}^{\prime} is an irreducible subrepresentation of Lψ˙H2(H˙)L^{2}_{\dot{\psi}_{H}}(\dot{H}). Again, comparing the Arthur’s multiplicity formula for σ˙\dot{\sigma}^{\prime} and its contragredient, we get

(8.4) vS\{u2,w}ησv=vS\{u2,w}ησvνv\prod_{v\in S\backslash\{u_{2},w\}}\eta_{\sigma_{v}^{\vee}}=\prod_{v\in S\backslash\{u_{2},w\}}\eta_{\sigma_{v}}\cdot\nu_{v}

as characters of 𝒮ψ˙H\mathcal{S}_{\dot{\psi}_{H}}. Combining these two equalities (8.3) and (8.4), we obtain the desired formula for ησ\eta_{\sigma^{\vee}}. This completes the proof. ∎

8.3. Calculation of the labeling

Finally we are now able to calculate the actions of normalized intertwining operators on induced representations of GG explicitly.

Proposition 8.5.

Let G=G(Vϵ)G=G(V^{\epsilon}) be an even orthogonal or unitary group, and

ψ=ψτ+ψ0+(ψτc),\psi=\psi_{\tau}+\psi_{0}+\left(\psi_{\tau}^{c}\right)^{\vee},

with ψτ\psi_{\tau} and ψ0\psi_{0} as in the setting of this section. Let π\pi be an irreducible constituent of IndPG(τχWπ0)\operatorname{Ind}_{P}^{G}(\tau\chi_{W}\boxtimes\pi_{0}). Assume that ψτ\psi_{\tau} is (conjugate) orthogonal. Then the restriction of the normalized intertwining operator R(w,τχWπ0,ψF)R(w,\tau\chi_{W}\boxtimes\pi_{0},\psi_{F}) to π\pi is the scalar multiplication by

R(w,τχWπ0)|π=ϵk𝒥ψF(π)(aτ),R(w,\tau\chi_{W}\boxtimes\pi_{0})\Big{|}_{\pi}=\epsilon^{k}\cdot\mathcal{J}_{\psi_{F}}(\pi)(a_{\tau}),

where aτa_{\tau} is the element in 𝒮ψ\mathcal{S}_{\psi} corresponding to ψτχW\psi_{\tau}\chi_{W}.

Proof.

Since τ\tau is of Arthur type, when r>dimVr>\dim V, the requirements in Proposition 3.1 and Corollary 3.3 are automatically satisfied. It follows that the equivariant map

𝒯s:ωIndQH(τscχVcσ0)IndPG(τsχWπ0)\mathcal{T}_{s}:\omega\otimes\operatorname{Ind}_{Q}^{H}\left(\tau_{s}^{c}\chi_{V}^{c}\boxtimes\sigma_{0}^{\vee}\right)\longrightarrow\operatorname{Ind}_{P}^{G}\left(\tau_{s}\chi_{W}\boxtimes\pi_{0}\right)

is surjective at s=0s=0. Moreover, by Lemma 5.3 and Theorem 4.2, the induced representations IndPG(τχWπ0)\operatorname{Ind}_{P}^{G}\left(\tau\chi_{W}\boxtimes\pi_{0}\right) and IndQH(τcχVcσ0)\operatorname{Ind}_{Q}^{H}\left(\tau^{c}\chi_{V}^{c}\boxtimes\sigma_{0}^{\vee}\right) are semi-simple and multiplicity-free. Therefore we can restrict the diagram (8.1) to

ωσ𝒯0π1R(w,τcχVcσ0,ψF)R(w,τχWπ0,ψF)ωσ𝒯0π,\begin{CD}\omega\otimes\sigma^{\vee}@>{\mathcal{T}_{0}}>{}>\pi\\ @V{1\otimes R(w,\tau^{c}\chi^{c}_{V}\boxtimes\sigma_{0},\psi_{F})}V{}V@V{}V{R(w,\tau\chi_{W}\boxtimes\pi_{0},\psi_{F})}V\\ \omega\otimes\sigma^{\vee}@>{\mathcal{T}_{0}}>{}>\pi\end{CD},

where σ\sigma is the theta lift of π\pi to HH. Applying Proposition 8.1 to this sub-diagram, we deduce

(8.5) R(w,τχWπ0,ψF)|π\displaystyle R(w,\tau\chi_{W}\boxtimes\pi_{0},\psi_{F})\Big{|}_{\pi} =αβ(0)R(w,τcχVcσ0,ψF)|σ\displaystyle=\alpha\cdot\beta(0)\cdot R(w,\tau^{c}\chi^{c}_{V}\boxtimes\sigma_{0},\psi_{F})\Big{|}_{\sigma^{\vee}}
=αβ(0)𝒥𝒲ψFA(σ)(aτ),\displaystyle=\alpha\cdot\beta(0)\cdot\mathcal{J}^{A}_{\mathscr{W}_{\psi_{F}}}(\sigma^{\vee})(a^{\prime}_{\tau}),

here aτa^{\prime}_{\tau} is the element in 𝒮θ(ψ)\mathcal{S}_{\theta(\psi)^{\vee}} corresponds to ψτcχVc\psi_{\tau}^{c}\chi_{V}^{c}. Let ϕτ\phi_{\tau}, ϕ0\phi_{0}, and ϕ0\phi^{\prime}_{0} be the LL-parameter associated to ψτ\psi_{\tau}, ψ0\psi_{0}, and θ(ψ0)\theta(\psi_{0}) respectively. Then we have

ϕ0=ϕ0χW1χV+χV(i=nrrn||i),\phi^{\prime}_{0}=\phi_{0}\chi_{W}^{-1}\chi_{V}+\chi_{V}\cdot\left(\bigoplus_{i=n-r}^{r-n}|\cdot|^{i}\right),

where nn is a integer which depends on the group GG (see the begining of Section 2). It follows that

β(0)\displaystyle\beta(0) =i=nr+1rnγ(i,ϕτ,ψE)1\displaystyle=\prod_{i=n-r+1}^{r-n}\gamma\left(i,\phi_{\tau},\psi_{E}\right)^{-1}
=ωτ(1)nr.\displaystyle=\omega_{\tau}(-1)^{n-r}.

Here we use the functional equation

γ(s,τ,ψE)γ(1s,τ,ψE)=ωτ(1).\gamma(s,\tau,\psi_{E})\cdot\gamma(1-s,\tau^{\vee},\psi_{E})=\omega_{\tau}(-1).

Now we calculate case by case.

Case OO: In this case, the Whittaker datum 𝒲\mathscr{W}^{\prime} of HH is the Whittaker datum associated to the additive character ψF,c\psi_{F,c} (recall that we have fixed d,cF×d,c\in F^{\times} such that V+V^{+} is of type (d,c)(d,c)). Also, we have

γVλ(E/F,ψF)1=ϵχV(c)\gamma_{V}\cdot\lambda\left(E^{\prime}/F,\psi_{F}\right)^{-1}=\epsilon\cdot\chi_{V}(c)

and

γW=1.\gamma_{W}=1.

Substitute these into the equality (8.5), we obtain

R(w,τχWπ0,ψF)|π\displaystyle R(w,\tau\chi_{W}\boxtimes\pi_{0},\psi_{F})\Big{|}_{\pi} =ϵkωτ(c)χV(c)k𝒥𝒲ψFA(σ)(aτ)\displaystyle=\epsilon^{k}\cdot\omega_{\tau}(-c)\cdot\chi_{V}(-c)^{k}\cdot\mathcal{J}^{A}_{\mathscr{W}_{\psi_{F}}}(\sigma^{\vee})(a^{\prime}_{\tau})
=ϵkωτ(c)χV(c)k𝒥𝒲ψFA(σ)(aτ)\displaystyle=\epsilon^{k}\cdot\omega_{\tau}(c)\cdot\chi_{V}(c)^{k}\cdot\mathcal{J}^{A}_{\mathscr{W}_{\psi_{F}}}(\sigma)(a_{\tau}) (by Proposition 8.4)
=ϵk𝒥𝒲A(σ)(aτ)\displaystyle=\epsilon^{k}\cdot\mathcal{J}^{A}_{\mathscr{W}^{\prime}}(\sigma)(a_{\tau}) (change Whittaker data)
=ϵk𝒥ψF(π)(aτ).\displaystyle=\epsilon^{k}\cdot\mathcal{J}_{\psi_{F}}(\pi)(a_{\tau}). (by our construction of 𝒥ψF)\displaystyle\textit{(by our construction of }\mathcal{J}_{\psi_{F}}\textit{)}

Hence the proposition holds in this case.

Case U0U_{0}: In this case, the Whittaker datum 𝒲\mathscr{W}^{\prime} of HH is just the Whittaker datum associated to the additive character ψF\psi_{F}. Also, we have

γV=ϵ\gamma_{V}=\epsilon

and

γWλ(E/F,ψF)1=χW(δ)1.\gamma_{W}\cdot\lambda\left(E/F,\psi_{F}\right)^{-1}=\chi_{W}(\delta)^{-1}.

Substitute these into the equality (8.5), we obtain

R(w,τχWπ0,ψF)|π\displaystyle R(w,\tau\chi_{W}\boxtimes\pi_{0},\psi_{F})\Big{|}_{\pi} =ϵk𝒥𝒲A(σ)(aτ)\displaystyle=\epsilon^{k}\cdot\mathcal{J}^{A}_{\mathscr{W}^{\prime}}(\sigma^{\vee})(a^{\prime}_{\tau})
=ϵk𝒥𝒲A(σ)(aτ)\displaystyle=\epsilon^{k}\cdot\mathcal{J}^{A}_{\mathscr{W}^{\prime}}(\sigma)(a_{\tau}) (by Proposition 8.4)
=ϵk𝒥ψF(π)(aτ).\displaystyle=\epsilon^{k}\cdot\mathcal{J}_{\psi_{F}}(\pi)(a_{\tau}). (by our construction of 𝒥ψF)\displaystyle\textit{(by our construction of }\mathcal{J}_{\psi_{F}}\textit{)}

Hence the proposition holds in this case.

Case U1U_{1}: In this case, the Whittaker datum 𝒲\mathscr{W}^{\prime} of HH is just the Whittaker datum associated to the additive character ψF\psi_{F}. Also, we have

γVλ(E/F,ψF)1=ϵ\gamma_{V}\cdot\lambda\left(E/F,\psi_{F}\right)^{-1}=\epsilon

and

γW=χW(δ)1.\gamma_{W}=\chi_{W}(\delta)^{-1}.

Substitute these into the equality (8.5), we obtain

R(w,τχWπ0,ψF)|π\displaystyle R(w,\tau\chi_{W}\boxtimes\pi_{0},\psi_{F})\Big{|}_{\pi} =ϵkωτ(1)χV(1)k𝒥𝒲A(σ)(aτ)\displaystyle=\epsilon^{k}\cdot\omega_{\tau}(-1)\cdot\chi_{V}(-1)^{k}\cdot\mathcal{J}^{A}_{\mathscr{W}^{\prime}}(\sigma^{\vee})(a^{\prime}_{\tau})
=ϵk𝒥𝒲A(σ)(aτ)\displaystyle=\epsilon^{k}\cdot\mathcal{J}^{A}_{\mathscr{W}^{\prime}}(\sigma)(a_{\tau}) (by Proposition 8.4)
=ϵk𝒥ψF(π)(aτ).\displaystyle=\epsilon^{k}\cdot\mathcal{J}_{\psi_{F}}(\pi)(a_{\tau}). (by our construction of 𝒥ψF)\displaystyle\textit{(by our construction of }\mathcal{J}_{\psi_{F}}\textit{)}

Hence the proposition holds in this case.

Corollary 8.6.

Theorem 7.3 holds.

Proof.

The first two statements follows from the construction of the θ\theta-packets and LIR-B for HH Theorem 7.2. The last statement follows from Proposition 8.5. ∎

So now, we have finished proving our main theorems.

8.4. Summary

To make things more clear, in this subsection, we shall briefly summarize some expected and known results for θ\theta-packets.

First we let FF be a local field of characteristic 0, and G=G(V)G=G(V) be an even orthogonal or unitary group over FF. Let ψ\psi be a local AA-parameter for GG with bounded image on the Weil group. Then, after choosing a symplectic or quasi-split unitary group HH over FF with sufficiently big split rank, and also a tuple of auxiliary data (ψF,χV,χW)(\psi_{F},\chi_{V},\chi_{W}) as in Section 2, one can define the θ\theta-packet Πψθ(G)\Pi_{\psi}^{\theta}(G) by using the theta lift between (G,H)(G,H) with respect to (ψF,χV,χW)(\psi_{F},\chi_{V},\chi_{W}). It is a (multi) set of irreducible unitary representations of GG, equipped with a map

𝒥ψF:Πψθ(G)𝒮ψ^\mathcal{J}_{\psi_{F}}:\Pi_{\psi}^{\theta}(G)\longrightarrow\widehat{\mathcal{S}_{\psi}}

to the Pontryagin dual of the component group 𝒮ψ\mathcal{S}_{\psi}. It can be also regarded as a representation of 𝒮ψ×G\mathcal{S}_{\psi}\times G as explicated in Section 2.5. Let ΠψM(G)\Pi_{\psi}^{M}(G) be the local packet contructed by Mœglin in [Mœg11b]. We have:

Theorem 8.7.

When FF is non-Archimedean, the θ\theta-packet Πψθ(G)\Pi_{\psi}^{\theta}(G) has the following properties:

  1. (1)

    as a representation of 𝒮ψ×G\mathcal{S}_{\psi}\times G, it is independent of the choice of HH; moreover, if G=GG=G^{*} is quasi-split, we have

    Πψθ(G)=ΠψA(G)\Pi_{\psi}^{\theta}(G^{*})=\Pi_{\psi}^{A}(G^{*})

    as representations of 𝒮ψ×G\mathcal{S}_{\psi}\times G^{*};

  2. (2)

    as a representation of GG, it is independent of the choice of auxiliary data (ψF,χV,χW)(\psi_{F},\chi_{V},\chi_{W}); moreover, it is multiplicity-free;

  3. (3)

    it coincides with ΠψM(G)\Pi_{\psi}^{M}(G) (as sets); in particular, it contains the LL-packet ΠϕψL(G)\Pi_{\phi_{\psi}}^{L}(G) as a subset;

  4. (4)

    it satisfies LIR-B, as stated in Theorem 7.3.

Proof.

The 11st statement is provided by Theorem 2.8; the 22nd statement is provided by Section 6; the 33rd statement is provided by [Mœg11c], and the last statement is just Theorem 7.3. ∎

We remark that, except for the 33rd statement, the proofs of all other properties in this theorem do not rely on the construction of ΠψM(G)\Pi_{\psi}^{M}(G) for non quasi-split GG. We expect the following conjecture holds:

Conjecture 8.8.

Similar results as stated in Theorem 8.7 also hold when FF is real or complex.

From the main body of this paper, we also conclude that:

Theorem 8.9.

When FF is non-Archimedean, there is a commutative diagram

(8.6) Πθ(ψ)A(H)𝒥𝒲A𝒮θ(ψ)¯^θΠψθ(G)𝒥ψF𝒮ψ^\begin{CD}\Pi^{A}_{\theta(\psi)}(H)@>{\mathcal{J}^{A}_{\mathscr{W}^{\prime}}}>{}>\widehat{\overline{\mathcal{S}_{\theta(\psi)}}}\\ @V{}V{\theta}V@V{}V{\ell^{*}}V\\ \bigsqcup\Pi_{\psi}^{\theta}(G)@>{\mathcal{J}_{\psi_{F}}}>{}>\widehat{\mathcal{S}_{\psi}}\end{CD}

where the disjoint union runs over all pure inner forms of GG^{*}, the arrow θ\theta is a bijection given by the theta lift, and the arrow \ell^{*} is the pull-back of the natural map

:𝒮ψ𝒮θ(ψ).\ell:\mathcal{S}_{\psi}\longrightarrow\mathcal{S}_{\theta(\psi)}.
Proof.

This is the combination of Theorem 2.8 and Corollary 5.4. ∎

This can be more or less regarded as a refined version of Conjecture 1.1 (B).

For our global purpose, we also need to treat those AA-parameter of GG with non-bounded image on the Weil group, since the Ramanujan conjecture is not proved yet. Let ψ\psi be a local AA-parameter of GG with non-bounded image on the Weil group, but we assume that ψ\psi is a localization of some global elliptic AA-parameter for an even orthogonal or unitary group. We write

ψ=(ψτ1||s1++ψτr||sr)+ψ0+((ψτ1||s1++ψτr||sr)c),\psi=(\psi_{\tau_{1}}|\cdot|^{s_{1}}+\cdots+\psi_{\tau_{r}}|\cdot|^{s_{r}})+\psi_{0}+\left((\psi_{\tau_{1}}|\cdot|^{s_{1}}+\cdots+\psi_{\tau_{r}}|\cdot|^{s_{r}})^{c}\right)^{\vee},

where

  • for i=1,,ri=1,\cdots,r, ψτi\psi_{\tau_{i}} is an irreducible representation of LE×SL2L_{E}\times SL_{2} with bounded image on the Weil group, which corresponds to an irreducible unitary representation τi\tau_{i} of GLki(E)GL_{k_{i}}(E), and sis_{i} is a real number such that

    s1sr>0;s_{1}\geq\cdots\geq s_{r}>0;
  • ψ0\psi_{0} is a local AA-parameter for some smaller group G0=G(V0)G_{0}=G(V_{0}), where V0V_{0} is the space in the Witt tower containing VV with appropriate dimension (if there is no such V0V_{0}, it follows from the induction principle of the theta lift [Kud86] and Theorem 8.6 that the θ\theta-packet Πψθ(G)\Pi_{\psi}^{\theta}(G) is empty).

So we have a natural isomorphism 𝒮ψ0𝒮ψ\mathcal{S}_{\psi_{0}}\simeq\mathcal{S}_{\psi}. There is a parabolic subgroup of GG, say PP, with Levi component MM, so that

MGLk1(E)××GLkr(E)×G0.M\simeq GL_{k_{1}}(E)\times\cdots\times GL_{k_{r}}(E)\times G_{0}.

For any irreducible unitary representation π0Πψ0θ(G0)\pi_{0}\in\Pi_{\psi_{0}}^{\theta}(G_{0}), we denote by I(π0)I(\pi_{0}) the parabolic induction

IndPG(τ1|det|s1τr|det|srπ0).\operatorname{Ind}_{P}^{G}\left(\tau_{1}|\det|^{s_{1}}\boxtimes\cdots\boxtimes\tau_{r}|\det|^{s_{r}}\boxtimes\pi_{0}\right).

We expect the following conjecture holds:

Conjecture 8.10.

The induced representation I(π0)I(\pi_{0}) is irreducible for any π0Πψ0θ(G0)\pi_{0}\in\Pi_{\psi_{0}}^{\theta}(G_{0}). Moreover, if

I(π0)I(π0)I(\pi_{0})\simeq I(\pi^{\prime}_{0})

for some π0,π0Πψ0θ(G0)\pi_{0},\pi^{\prime}_{0}\in\Pi_{\psi_{0}}^{\theta}(G_{0}), then we have π0π0\pi_{0}\simeq\pi^{\prime}_{0}.

About this conjecture, we have:

Proposition 8.11.
  1. (1)

    Conjecture 8.10 holds in the following cases:

    • if the AA-parameter ψ\psi is trivial on the Arthur SL2SL_{2};

    • if G=GG=G^{*} is quasi-split, and FF is non-Archimedean.

    Similar results also hold for the group HH.

  2. (2)

    When FF is non-Archimedean, in general, for any irreducible unitary representation πΠψθ(G)\pi\in\Pi_{\psi}^{\theta}(G), there exists an unique π0Πψ0θ(G0)\pi_{0}\in\Pi_{\psi_{0}}^{\theta}(G_{0}), such that π\pi is a sub-quotient of I(π0)I(\pi_{0}), and

    𝒥ψF(π)=𝒥ψF(π0),\mathcal{J}_{\psi_{F}}(\pi)=\mathcal{J}_{\psi_{F}}(\pi_{0}),

    where we use the natural isomorphism between 𝒮ψ\mathcal{S}_{\psi} and 𝒮ψ0\mathcal{S}_{\psi_{0}} to identify them. Moreover, the map

    Πψθ(G)\displaystyle\Pi_{\psi}^{\theta}(G) Πψ0θ(G0),\displaystyle\longrightarrow\Pi_{\psi_{0}}^{\theta}(G_{0}),
    π\displaystyle\pi π0\displaystyle\longmapsto\pi_{0}

    is a bijection.

Proof.

The two cases in 11st statement follows from [CZ21] Section 6 and [Mœg11a] Proposition 5.1 respectively, and the 22nd statement follows from the combination of the 11st statement (for HH), the induction principle of the theta lift [Kud86], and Theorem 8.6. ∎

Finally we turn to the global properties of θ\theta-packets. Now let FF be a number field, and fix an additive character ψF\psi_{F}. Let GG be an even orthogonal or unitary group over FF. Given an elliptic AA-parameter ψ\psi for GG, we define the global packet Πψθ(G)\Pi_{\psi}^{\theta}(G) associated to ψ\psi as the restricted tensor product of the local θ\theta-packets

Πψθ(G)\displaystyle\Pi_{\psi}^{\theta}(G) =vΠψvθ(Gv)\displaystyle=\otimes^{\prime}_{v}\Pi_{\psi_{v}}^{\theta}(G_{v})
={π=vπv|πvΠψvθ(Gv),πv unramified with the L-parameter ϕψv for almost all v}.\displaystyle=\{\pi=\otimes^{\prime}_{v}\pi_{v}~{}|~{}\pi_{v}\in\Pi_{\psi_{v}}^{\theta}(G_{v}),~{}\pi_{v}\textit{ unramified with the $L$-parameter $\phi_{\psi_{v}}$ for almost all }v\}.

We then have a map

𝒥ψF:Πψθ(G)\displaystyle\mathcal{J}_{\psi_{F}}:\Pi_{\psi}^{\theta}(G) 𝒮ψ^,\displaystyle\longrightarrow\widehat{{\mathcal{S}_{\psi}}},
π\displaystyle\pi 𝒥ψF(π),\displaystyle\longmapsto\mathcal{J}_{\psi_{F}}(\pi),
𝒥ψF(π)(x)\displaystyle\mathcal{J}_{\psi_{F}}(\pi)(x) v𝒥ψFv(πv)(xv),\displaystyle\coloneqq\prod_{v}\mathcal{J}_{\psi_{F_{v}}}(\pi_{v})(x_{v}),

where x𝒮ψx\in\mathcal{S}_{\psi} and xvx_{v} is the localization of xx at vv. Let ϵψ𝒮ψ^\epsilon_{\psi}\in\widehat{\mathcal{S}_{\psi}} be the canonical sign character associated to ψ\psi. We put

Πψθ(G,ϵψ)={πΠψθ(G)|𝒥ψF(π)=ϵψ}.\Pi_{\psi}^{\theta}(G,\epsilon_{\psi})=\left\{\pi\in\Pi_{\psi}^{\theta}(G)~{}|~{}\mathcal{J}_{\psi_{F}}(\pi)=\epsilon_{\psi}\right\}.

The following conjecture is the ultimate goal of our series of works:

Conjecture 8.12.

Let ψ\psi be an elliptic AA-parameter for GG. Then we have the decomposition

Lψ2(G)=πΠψθ(G,ϵψ)π.L^{2}_{\psi}(G)=\bigoplus_{\pi\in\Pi_{\psi}^{\theta}(G,\epsilon_{\psi})}\pi.

In our previous paper [CZ21], we have proved that

Theorem 8.13.

Conjecture 8.12 holds if the Witt index of GG is less than or equal to one.

The author hopes that one day in the future, he can have a chance to prove Conjecture 8.12 in full generality.

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