Counting Discrete, Level-$1 $, Quaternionic Automorphic

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arXiv:2106.09313v1 [math.NT] 17 Jun 2021 .Gop otiuigadRltdCntns11 9 of Endoscopy Constants Elliptic Related and Contributing 4.1. Groups Formula Hyperendoscopy 4. The 3.2. Notation Endoscopy of Side/Application 3.1. Geometric Series Discrete 3. Quaternionic 2.2. 2. Notation 1.4. Acknowledgements 1.3. Summary 1.2. Context 1.1. Introduction 1. ..Ro ytmof System Root 2.1. ..Edsoi osat n omlztos12 Transfers for Formulas Final Characters 5.3. Endoscopic Combinatorics 5.2. Root Transfers Endoscopic 5.1. Real Normalizations and Constants 5. Endoscopic 4.2. Date G ue1,2021. 18, June : ersnain nabtayrdciegop nta fj of instead groups discrete-at-in reductive about arbitrary information on exact representations computing in ested htti iauosyde o atrfrseiclytec the specifically M on for of matter series computations not discrete some does Using miraculously this “regular”. that being of ter in condition defined a are representations autmorphic quaternionic rep automorphic and forms form modular compact-at-infinity classical the of terms Jacquet-Langlands-sty in a prove them we way, level- the technique of On some spaces resentations. with of for dimensions together trace Ta¨ıbi compute this and to use Eichler-Selberg Renard, then We the forms. of modular analog an representations uoopi ersnain nteecpinlgroup modul exceptional the holomorphic GL on place representations of special automorphic representations the automorphic groups among other to eralize Abstract. ocp”tcnqe rmapeiu ok edvlpfrqua for develop we work, previous a from techniques doscopy” ONIGDSRT,LEVEL- DISCRETE, COUNTING 2 n utrincDsrt Series Discrete Quaternionic and ehp htti rjc evsa udn xml o anyo for example guiding a as serves project this that hope We h antcncldffiut sta h utrincdiscre quaternionic the that is difficulty technical main The UOOPI ERSNAIN ON REPRESENTATIONS AUTOMORPHIC utrincatmrhcrpeettosaeoeattempt one are representations automorphic Quaternionic G 2 G . 2 G 2 G AU DALAL RAHUL 2 c . Contents 1 2 ee esuyquaternionic study we Here, . 1 QUATERNIONIC , G s lsia ones. classical ust 2 so ontsatisfy not do of ms nt automorphic finity s fquaternionic of ase ersl describing result le sn “hyperen- Using . utrincrep- quaternionic 1 uafrclassical for mula eettoson resentations fChenevier, of s ny eshow we undy, rfrshave forms ar ternionic, esre that series te einter- ne G ogen- to 2 G 2 - 15 14 14 14 11 9 9 6 3 3 2 2 5 5 4 2 RAHUL DALAL

6. The H = SL2 SL2/ 1 term 15 6.1. Cohomological× Representations± of H(R) 16 6.2. Reduction to Modular Form Counts 17 6.3. Final Formula for SH 18 7. A Jacquet-Langlands-style result 18 7.1. First Form 18 7.2. In terms of Modular Forms 19 8. Counts of forms 20 c 8.1. Formula in terms of IG2 20 c 8.2. Computing IG2 21 8.3. Table of Counts 21 References 21

1. Introduction 1.1. Context. This work describes level-1, discrete, quaternionic automorphic rep- resentations on G . Let (k) be the set of such representations of weight k. For 2 Q1 each k > 2, we give a formula, (10), for 1(k) in terms of counts of automorphic |Q | c representations on the compact-at-infinity inner form G2 that were calculated by Chenevier and Renard in [CR15]. We also give a Jacquet-Langlands-style result (corollary 7.2.1) describing all elements of 1(k) in terms of certain automorphic c Q representations on G2 and certain pairs of classical modular forms. Quaternionic automorphic representations were developed as a way to general- ize to other groups the special place holomorphic modular forms have among au- tomorphic representations of GL2. Just like holomorphic modular forms, they are characterized by their infinite component being in a particular nice class of discrete series representations: the quaternionic discrete series of [GW96]. Just like modular forms they also have many unexpected applications and connections to other areas of math. For example, they have a nice theory of Fourier expansions with inter- esting arithmetic content—this was described for G2 in [GGS02] and generalized to all exceptional groups in [Pol20]. They also somehow appear in certain string theory computations involving black holes—see the end of chapter 15 in [FGKP18] for example. Quaternionic forms have been studied a lot by Pollack: see [Pol21] for an introductory article on them and [Pol18] for good exposition specifically on G2-quaternionic forms. We study discrete, quaternionic representations on G2 using the trace formula. Since quaternionic discrete series appear in L-packets with non-quaternionic mem- bers, this provides a great test case of the efficacy of the techniques in [Dal19] developed to split L-packets with the trace formula. More precisely, stabilizaiton lets us develop an “Eicher-Selberg”-style trace formula for quaternionic discrete se- ries. The counts of level one forms and Jacquet-Langlands-style results come from computations with this. The level-1 computation in particular also relies heavily on powerful shortcuts developed in [CR15] and [Ta¨ı17] to get exact counts of level-1 automorphic representations on classical groups through the invariant/stable trace formulas. Finally, as one technical point of interest, there is a particular miracle about quaternionic discrete series on G2 that crucially underpins this result. A priori, DISCRETE, QUATERNIONIC AUTOMORPHIC REPS. ON G2 3

[Dal19, Prop. 6.3.3] cannot be applied: such discrete series are not regular, imply- ing that there may not be a test function at infinity whose trace picks out exactly a quaternionic discrete series without also picking up some unwanted contributions from non-tempered representations. However, it turns out that specifically quater- nionic discrete series on G2 don’t get entangled in this way, even though other members of their L-packet do. The proof of this depends on results about Adams- Johnson packets for G2 that Mundy developed for studying Eisenstein cohomology in [Mun20]. The existence of this miracle suggests similar methods could be used to study other irregular discrete series at infinity through the simple trace formula. The methods here should be able to also compute averages of Hecke eigenvalues. We also hope that the computation here is an illuminating basic, starting exam- ple for people interested in doing explicit computations with discrete-at-infinity automorphic representations on general reductive groups instead of just classical ones.

1.2. Summary. We summarize the method of computation. Proposition 2.2.1 shows that traces against a pseudocoefficient of a quaternionic discrete series with weight k > 2 are 0 against all other unitary representations. This allows us to get a formula (2.2.2) for traces of finite-place test functions against the space of all quaternionic representations of weight k. Next, section 3 develops a general stabilized formula (2) for Igeom applied to test functions like ours. The combination of the results in §3 and formula (2.2.2) should be thought of as an analogue for quaternionic, G2-representations of the Eichler-Selberg trace formula for classical modular forms. We work out what this formula reduces to in the unramified case in section 4 using a computation of the endoscopy of G2 in section 4.1. Instead of using formula (2) directly, we compare c it applied to G2 to it applied to the compact real form G to construct a formula c 2 G2 G2 H for Ispec involving just Ispec- and Ispec-terms. Here, H is the endoscopic group SL2 SL2/ 1 of G2. c × ± G2 H Section 5 then tells us which exact Ispec- and Ispec-terms appear by computing endoscopic transfers at infinity. The difficult part of this computation is pinning down various signs coming from transfer factors. As a last piece of the puzzle, section 6 uses results about level-1 forms from [CR15] to reduce counts of forms on H to counts of classical modular forms. Section 7 uses all these formulas to characterize representations in k(1) with k> 2 in terms of automorphic representations on Gc and certain pairsQ of classical 2 c G2 modular forms. Finally, we substitute in values for the Ispec-terms from [CR15] and present a final table of dimensions: table 1, in section 8.

1.3. Acknowledgements. This work was done under the support of NSF RTG grant DMS-1646385. I would like to thank Kimball Martin and Aaron Pollack for discussions at conferences that eventually led to the consideration of this problem. The key proposition 2.2.1 that made this problem solvable grew out of email conver- sations with Sam Mundy. Olivier Ta¨ıbi provided a great deal of help in pointing out many, many tricks and previous results I could use to keep computations reasonably simple and actually feasible. In particular, I am grateful for the suggestion to use “method 2” described in section 3.2.3 that he passed on from Ga¨etan Chenevier. Alexander Bertoloni-Meli again provided much help, this time teaching me things 4 RAHUL DALAL about transfer factors. The root system picture for G2 was heavily modified from an answer by user Heiko Oberdiek on TeX Stack Exchange.

1.4. Notation. Here is a list of notation used throughout: The group G2

G2 is the standard exceptional Chevalley group defined over Z. • c c G2 is the unique inner form of G2 over Q. Recall that (G2)R is the compact • real form. αi,ǫi, λi are particular roots and coroots of G2 defined in section 2.1. • s is the simple reflection associated to root or coroot λ. • λ ρ is half the sum of the positive roots of G2. • V is the finite dimensional representation of G of highest weight λ. • λ 2 K is a choice of maximal compact subgroup SU(2) SU(2)/ 1 of G2(R). • K∞ is the product of maximal compact subgroups ×G (Z ) over± all p. • 2 p Ω=ΩC is the Weyl group of G . • 2 ΩR is the Weyl group of K as a subset of Ω. • H will often refer to the specific endoscopic group SL2 SL2/ 1 of G2. • (1) is the set of discrete, quaternionic automorphic× representat± ions of • Qk G2 of weight k and level 1 (see section 2.2). General groups F G∞ = Res G(R) for G a reductive group over number field F . Since most • Q groups here are over Q, G∞ is usually G(R). S G , GS are more generally the standard upper- and lower-index notation • S for G(A ), G(AS )—leaving out the places in S or only including the places in S respectively. Ω(G) is the absolute Weyl group of G. • ΩR(G) is the subset of the Weyl group of G∞ with respect to an elliptic • maximal torus (if one exists) generated by elements of G∞. KG is a maximal compact subgroup of G∞. • ∞ KG for unramified G is the product of chosen hyperspecial subgroups at • all finite places. ρ is half the sum of the positive roots of G. • G [G(F )], [G(F )]ss, [G(F )]st, [G(F )]ell are the (semisimple, stable, elliptic) con- • jugacy classes of G(F ). Real test functions

ϕπ for π a discrete series representation of G∞ is the pseudocoefficient • defined in [CD90]. Πdisc(λ) is the discrete series L-packet corresponding to dominant weight • λ. η is the Euler-Poincar´efunction from [CD90] for Π (λ). We normalize • λ disc it to be the average of the pseudocoefficients for π Πdisc(λ) instead of their sum. ∈ Trace Formula

(G), disc(G) is the set of (discrete) automorphic representations on • ARG. AR ur(G) for G unramified is the space of unramified automorphic repre- • ARsentations of G. DISCRETE, QUATERNIONIC AUTOMORPHIC REPS. ON G2 5

Figure 1. Character lattice, roots, and choices of dominant cham- ber for G2

• • • • • •

2ǫ2 • • • • • • ρG2

• • α1 • •λ1 = ρK • • λ2 = β

• • • • • • 2ǫ1

• • • • • • α2

• • • • • •

mdisc(π),mcusp(π) are the multiplicities of automorphic representation π in • the discrete (cuspidal) subspace. G G G Ispec, Igeom, Idisc are the distributions from Arthur’s invariant trace formula • on G. SG = SG is the stable distribution defined in theorem 3.2.1. • geom Miscellaneous 1 is the indicator function of set S. • S k(1) is the set of normalized, classical, cuspidal eigenforms on GL2 of level •1 S and weight k.

2. G2 and Quaternionic Discrete Series

2.1. Root System of G2.

2.1.1. Roots. We use notation from [LS93] to specify the root system of G2. Let K be the maximal compact SU(2) SU(2)/ 1 of G (R). Choose a dominant × ± 2 chamber for K and the choice of simple roots of G2 consistent with this. Let β be the highest root with respect to this and note that it is long. We now give explicit coordinates. As a mnemonic convention, roots indexed 1 will be short and roots indexed 2 will be long. Figure 1 displays all the roots and shades our choices of dominant Weyl chambers with respect to both G2 and K. Compact roots at infinity are in red and non-compact in blue. 6 RAHUL DALAL

If the roots of the short and long SU2 are 2ǫ1 and 2ǫ2 respectively, then the simple roots of G2 are: (short) α = ǫ + ǫ , (long) α =3ǫ ǫ . 1 − 1 2 2 1 − 2 The other positive roots are:

(short) 2ǫ1 = α1 + α2, ǫ1 + ǫ2 =2α1 + α2,

(long) 2ǫ2 =3α1 + α2, 3ǫ1 + ǫ2 =3α2 +2α2. The fundamental weights are:

λ1 =2α1 + α2, λ2 =3α2 +2α2.

Of course β = λ2. The Weyl group is generated by simple reflections: 2ǫ ǫ + ǫ 2ǫ ǫ + ǫ s 1 = 1 2 , s 1 = 1 2 . α1 2ǫ 3ǫ ǫ α2 2ǫ −3ǫ + ǫ  2  1 − 2  2  1 2  Finally:

ρK = ǫ1 + ǫ2 =2α1 + α2,

ρG =4ǫ1 +2ǫ2 =5α1 +3α2.

2.1.2. Coroots. Coroots will follow the opposite mnemonic: coroots indexed 1 are long and coroots indexed 2 are short. ∗ Let T be a split maximal torus. Since G2 has trivial center, X (T ) is the root lattice: X∗(T )= aǫ + bǫ : a,b Z,a + b 2Z . { 1 2 ∈ ∈ } Let (δ1,δ2) be the dual basis to (2ǫ1, 2ǫ2): i.e. (δi,ǫj)=1/21i=j. Then:

X∗(T )= aδ + bδ : a,b Z,a + b 2Z . { 1 2 ∈ ∈ } Since ǫ1 and ǫ2 are perpendicular: ∨ (2ǫ1) =2δ1, ∨ (2ǫ2) =2δ2. More generally, the Weyl action gives: (α∨, 2ǫ )= 1, (α∨, 2ǫ )=3, 1 1 − 1 2 (α∨, 2ǫ )=1, (α∨, 2ǫ )= 1, 2 1 2 2 − so we get simple coroots: α∨ = δ +3δ , 1 − 1 2 α∨ = δ δ . 2 1 − 2 This reproduces that the coroot lattice is X∗(T ), implying that G2 is simply con- nected. For completeness: ∨ λ1 = δ1 +3δ2, ∨ λ2 = δ1 + δ2. 2.2. Quaternionic Discrete Series. DISCRETE, QUATERNIONIC AUTOMORPHIC REPS. ON G2 7

2.2.1. Description. Recall the notation from [Dal19, §2.2.1] to discuss discrete series. In particular, recall the two parametrizations of discrete series on G2(R): πG2 = πG2 λ,ω ω(λ+ρG2 ) for λ a dominant (but possibly irregular) weight of G2 and ω a Weyl-element that takes the ΩG2 dominant chamber to something ΩK -dominant—in other words, G2 1,sα1 , or sα2 . Note that πλ,ω has infinitesimal character λ + ρG2 . Recall that

ω(λ + ρG2 ) is called the Harish-Chandra parameter of this discrete series. The quaternionic discrete series of weight k for k 2 lies in the L-packet ≥ Π ((k 2)β). disc − The members of this L-packet have Harish-Chandra parameters: (k 2)β + ρ , s ((k 2)β + ρ ), s ((k 2)β + ρ ). − G α1 − G α2 − G As in [GGS02], the quaternionic member is the one with minimal K-type λB =2kǫ2. We know that the discrete series π(ω, λ) has minimal K-type λ = ω(λ +2ρ ) 2ρ B G − K by [Kna01, Thm. 9.20]. Therefore the weight-k quaternionic discrete series πk is specifically π(s , (k 2)β)—computing, s fixes ρ so α2 − α2 K s (λ +2ρ ) 2ρ = s (λ +2ρ 2ρ )= s (λ +2β)= s (kβ)=2kǫ . α2 G − K α2 G − K α2 α2 2 This is the discrete series with Harish-Chandra parameter λ := s ((k 2)β + ρ ). k,H α2 − G 2.2.2. Their pseudocoefficients. Recall from [CD90] the notion of pseudocoefficients ϕπ for discrete series π. They satisfy: 1 σ = π

trσ(ϕπ)= 0 σ basic, σ = π  6 ? else for all unitary σ. Here a basic representation is a parabolic induction of a discrete series or limit of discrete series. Recall also the Euler-Poincar´efunctions ηλ that we normalize to be the average of pseudocoefficients over an L-packet. For a quick summary of properties of these functions in the notation used here, see [Dal19, §2.2.2]. Let ϕk be a pseudocoefficient for πk. A priori, πk is not a regular discrete series, so the trace against ϕk may be non-zero for certain non-tempered representations in addition to just πk. This could make it not work as a test function to pick out just automorphic representations π with π∞ = πk. However, this is miraculously not a problem for specifically quaternionic discrete series.

Proposition 2.2.1. Let k> 2. Then for any unitary representation ρ of G2(R):

1 ρ = πk trρ(ϕk)= . (0 else 8 RAHUL DALAL

Proof. By the same argument of Vogan described in [Dal19, lem. 6.3.1], the trace is 0 unless trρ(η(k−2)β ) = 0 for η(k−2)β the Euler-Poincar´efunction. This is only possible if ρ appears in6 an appropriate (g,K)-cohomology. By the main result of [VZ84], the only representations that do so are the packet Π ((k 2)β) and λ − something denoted Aq((k 2)β) for q corresponding to the Levi subgroup with roots α and Weyl group− Ω = s , 1 . This is because k > 2 implies that this ± 1 L { α1 } is the only Levi such that (k 2)β is fixed by ΩL. See also [LS93][lem. 2.2]. If ρ Π ((k 2)β) and tr− (ϕ ) = 0, then ρ = π by definition. It therefore ∈ λ − ρ k k suffices to exclude the case of Aq((k 2)β). We use that tr (ϕ ) is the − Aq((k−2)β) k coefficient of πk in the sum expansion ′ ′ Aq((k 2)β)= m(ρ )ρ − ′ ρ Xbasic in the Grothendieck group and will show that this coefficient is 0. By [Mun20][thm. 6.4.4], Aq is a Langlands quotient of a discrete series on a GL2 Levi. Let the corresponding parabolic induction be I. Since GL2 is a max- imal proper Levi and the infinitesimal character is regular, the other terms in the expansion need to be discrete series. There have to be two of these since trAq((k−2)β)(η(k−2)β ) = 2 (see [LS93][lem. 2.2] again). Call these ρ1 and ρ2 to make the expansion into− basics

Aq((k 2)β)= I ρ ρ . − − 1 − 2 The computation of the A-packet in [Mun20][thm. 6.4.4] shows that the charac- ter Aq((k 2)β) π = I ρ ρ π − − k − 1 − 2 − k is stable. By [She79][lem. 5.2], I is stable so ρ1 + ρ2 + πk also has to be. Then, [She79][lem. 5.1] further implies that ρ1 + ρ2 + πk is fully Weyl-invariant on an elliptic maximal torus. Examining Harish-Chandra’s character formula for discrete series, this is only possible if the three discrete series are exactly the three members Πdisc((k 2)β). In particular, πk = ρ1,ρ2 so we are done. Beware− that [Mun20] chooses dominant6 chambers for K and G in slightly differ- ent relative position, making the notation there a bit different.  Corollary 2.2.2. Let f ∞ be a compactly supported locally constant function on ∞ G2(A ) and k> 2. Then

∞ ∞ ∞ I (ϕ f )= m (π)δ ∞ tr (f ) spec k ⊗ disc π =πk π π∈ARXdisc(G2) ∞ ∞ = mcusp(π)δπ∞=πk trπ (f ). π∈ARXcusp(G2) Proof. The statement for discrete representations is the same argument as [Dal19, prop. 6.3.3] after we know proposition 2.2.1. Since π∞ = πk is necessarily discrete series for the non-zero terms, the main result of [Wal84] shows that mcusp(π) = mdisc(π).  We therefore have (1) (1) = I (ϕ 1 ) |Qk | spec k ⊗ K if we choose Gross’ canonical measure from [Gro97] at finite places. Note again that this heavily depends on the miracle of proposition 2.2.1 and a similar result does DISCRETE, QUATERNIONIC AUTOMORPHIC REPS. ON G2 9 not hold either for the other members of Πdisc((k 2)β) or for the Euler-Poincar´e function. −

3. Geometric Side/Application of Endoscopy 3.1. Notation. We will need to recall some extra notation related to general re- ductive group H over F : Ωc is the Weyl group generated by compact roots at infinity. • H d(H∞) is the size of the discrete series L-packets of H∞. Alternatively, • c d(H∞)= ΩH / ΩH . | | | | 1 1 k(H∞) is the size of the group K = ker(H (R,T ) H (R, G∞)) that • ell → appears in the theory of endoscopy for G∞.

q(H∞) = dim(H∞/K∞Z ∞ ) where K∞ is a maximal compact subgroup • H of H∞. ∗ H is the quasisplit inner form of H∞. • ∞ H¯∞ is the compact form. If H∞ has an elliptic maximal torus, this is inner. ∗ • q(H∞)−q(H∞) e(H∞) is the Kottwitz sign ( 1) . • − [H : M] = [H : M]F = dim(AM /AG), where A⋆ is the maximal F -split • torus in the center of ⋆. We call this the index of M in H. τ(H) is the Tamagawa number of H. • Mot is the Gross motive for H. • H L(MotH ) is the value of the corresponding L-function at 0 (or residue of • the pole). H H ι (γ)= ιF (γ) for γ H(F ) is the number of connected components of Hγ • that have an F -point.∈

3.2. The Hyperendoscopy Formula.

3.2.1. Preliminaries. We will use the hyperendoscopy formula of [Fer07] to compute I (ϕ f ∞). A priori, we need to apply the general case of [Dal19, Thm. 4.2.3] geom k ⊗ since G2 has endoscopy without simply connected derived subgroup. Let η be the Euler-Poincar´efunction for Π ((k 2)β). Let (G ) be the k disc − HEell 2 set of non-trivial hyperendoscopic paths for G2. Then, in the notation of [Dal19, §4],

˜ ˜ IG2 (ϕ f ∞)= IG2 (η f ∞)+ ι(G, )IH (((η ϕ ) f ∞)H), geom k ⊗ geom k ⊗ H geom k − k ⊗ H∈HEXell(G2) where the H˜ are choices of z-pair paths when they are needed.

3.2.2. Telescoping. Next, an unpublished result of Kottwitz summarized in [Mor10, ∞ §5.4] and proved by other methods in [Pen19] stabilizes Igeom(ϕ f ) when ϕ satisfies a technical property of being stable-cuspidal (as all terms on⊗ the right side above can be taken to be).

∞ Theorem 3.2.1. Let ϕ be stable cuspidal on G2(R) and f a test function on G(A∞). Then

˜ ˜ IG2 (ϕ f ∞)= ι(G, H)SH ((ϕ f ∞)H ), geom ⊗ geom ⊗ H∈EXell(G2) 10 RAHUL DALAL where (G ) is the set of elliptic endoscopic groups for G and the H˜ are z- Eell 2 2 extensions if necessary. The transfers (ϕ f ∞)H˜ depend on choices of measures for G and H. ⊗ The Sgeom terms are defined by their values on Euler-Poincar´efunctions:

H ∞ [H:M] ΩM,F Sgeom(ηλ f )= ( 1) | |τ(M) ⊗ cusp − ΩH,F M∈LX (H) | | ¯ M −1 e(Mγ,∞) k(M∞) H ∞ ∞ ι (γ) ΦM (γ, λ)SOγ ((f )M ), × | | vol(M¯ /A ¯ ) k(H∞) ∞ γ,∞ Mγ ,∞ γ∈[M(XQ)]st,ell choosing Tamagawa globally measure on all centralizers. The volume on M¯ γ,∞ is transferred from that on Mγ,∞ in the standard way for inner forms so that the entire term doesn’t depend on a choice of measure at infinity. There’s an alternating sign in the hyperendoscopy formula: if is a hyperendo- scopic path, then ι(G, )ι( ,H) = ι(G, ( ,H)) for H any endoscopicH group of . Here, ( ,H) represents− H theH concatenationH and is overloaded to also refer to Hthe last groupH in . H In particular,H substituting in the stabilization telescopes the hyperendoscopy formula. 3.2.3. Final Geometric Formulas and Method of Computation. The final telescoped formula is: ˜ ˜ (2) IG2 (ϕ f ∞)= SG2 (η f ∞)+ ι(G, H)SH ((ϕ f ∞)H ). geom k ⊗ geom k ⊗ geom k ⊗ H∈Eell(G2) HX=6 G2 We recall: τ(G) ι(G, H)= Λ(H, ,s,η) −1 , | H | τ(H) where Λ(H, ,s,η) is the image in Out(H) of the automorphisms of the endoscopic quadruple. H There are two possible methods to proceedb here. We will be using method 2 and mention method 1 in case it is useful for anyone attempting a similar computation on another group. Method 1: We can try calculate the Sgeom terms directly from their formula. We will need to choose Euler-Poincar´emeasure at M¯ γ times canonical measure for the orbital integrals (canonical measure is the same for all inner forms). This adds an extra factor of L(MotMγ ) d(M¯ ∞) γ, rank(M ∞) e(M¯ γ,∞)2 γ, by [ST16, lem. 6.2]. Since d(H∞) = 1 and volEP (H∞/AH∞ ) =1 for H compact, this expands the terms in (2) as:

H ∞ [H:M] ΩM,F k(M∞) Sgeom(ηλ f )= ( 1) | | τ(M) ⊗ cusp − ΩH,F k(H∞) M∈LX (H)  | |    2− rank(Mγ,∞)ΦH (γ, λ) L(Mot ) ιM (γ) −1SO∞((f ∞) ) , × M Mγ | | γ M γ∈[M(Q)] ∞ Xst,ell  DISCRETE, QUATERNIONIC AUTOMORPHIC REPS. ON G2 11 where the stable orbital integrals are now computed using canonical measure on centralizers. The hardest terms here are the stable orbital integrals, the L-values, and the ∞ ∞ characters Φ. Note that since we are using f = 1K∞ , the constant terms (f )M are also indicator functions of hyperspecials. The L-values may be computed as products of values of Artin L-functions by explicitly describing the motives from [Gro97]. The terms Φ can be reduced to linear combinations traces of γ against finite dimensional representations of G2 by the algorithm on [Art89, pg. 273]. These can of be computed by the Weyl character formula and its extension to irregular elements stated in, for example, [CR15, prop. 2.3]. The stable orbital integrals unfortunately cause far more difficulty. They are computed and listed in a table on [GP05, pg. 159]. First, they are interpreted as c orbital integrals on compact-at-infinity G2. The spectral side of the trace formula c on G2 is then possible to compute, allowing the orbital integrals to be solved for once the coefficients in terms of L-values are known. Even using the previous work of [GP05], this method is horrendously compli- cated. Method 2: Fortunately, there is a much simpler way to compute our desired count. Recalling c G2 c that I is known from [CR15], we can compare the expansions (2) for G2 and G2. c The term for SG2 a appears in the expansion for IG2 and can therefore be solved for and substituted in the expansion for IG2 . In total we get a formula c IG2 = IG2 + corrections, where the corrections are in terms of SH for smaller endoscopic H. In the next section we will see that there aren’t actually that many H appearing. Finally, section 6 will show that the terms for these H are easily computed through another trick. Method 2 also gives in section 7 a Jacquet-Langlands-style result c comparing quaternionic representations on G2 to representations on G2.

4. Groups Contributing and Related Constants

4.1. Elliptic Endoscopy of G2. The elliptic endoscopic groups of G2 are G2, PGL3, SO4, and potentially some tori. This is stated in a thesis [Alt13] but not fully explained, so we work out the computation here for reader convenience. We use notational conventions for endoscopy as in [Dal19, §3]. By inspecting the root data, the conjugacy classes of centralizers H of a semisim- ple element in G G (C) are: 2 ≃ 2 G2 itself, b • SL fromb the long roots, • 3 SL2 SL2/ 1 from a short and long root that are orthogonal, • GL ×from a{± short} root, • 2 GL2 from a long root, • G2 . • m We compute the possible endoscopic pairs (s,ρ) for each possibility. Recall that, since G is split, ρ is a map from a Galois group to Out(H) Ω . 2 ∩ G2 Since G2 has trivial center, the cohomology condition on s is always satisfied so we don’t bother checking it. Trivial center further gives thatb the isomorphism class 12 RAHUL DALAL of the pair cannot change with s. Therefore the only thing that depends on s is whether we can exhibit one that is Galois invariant when ρ is non-trivial. For each pair we will also compute the automorphism group Λ that comes up in the formula for ι(G, H). G2: Then ρ is trivial. This gives the trivial endoscopic group G2. Since only the trivial element of Out(H) can be realized in ΩG2 , Λ = 1. SL3: There are two possibilitiesb for ρ: trivial or sending a quadratic Galois element to the outer automorphism of SL : (δ ,δ ) (δ , δ ) (fixing a long root). We are 3 1 2 7→ 1 − 2 forced to choose s so that without loss of generality (δ1 + δ2)(s) = (δ1 δ2)(s)= ζ3 ◦ − (two short roots of G2 at 120 ). This is preserved by only the trivial ρ.

This gives endoscopic group PGL3. Here, Out(H) is realized in ΩG2 and com- mutes with ρ so Λ b= 2. | | SL SL / 1 : b 2 × 2 {± } No outer automorphisms can be realized through conjugation in G2 so ρ is trivial. This gives endoscopic group SL SL / 1 . Since Out(H) Ω is trivial, Λ = 1. 2 × 2 {± } ∩ G2 Short GL2: b Without loss of generality assume the short root is 2δb2. To be elliptic ρ needs to send a quadratic Galois element to the outer automorphism (δ1,δ2) ( δ1,δ2) of GL . To have the right centralizer, 2δ (s) = α for some α = 1 and7→ 2δ (−s) = 1. 2 1 6 2 However, then (δ1 + δ2)(s)= √α which can’t be equal to it’s inverse. Therefore s can’t invariant under ρ. In total,± there are no such elliptic endoscopic groups. Long GL2: This is the same as the previous case and gives no elliptic endoscopy. 2 Gm:

Here ρ send Galois elements to any element of ΩG2 . Elliptic means the action can have no invariants except zero in X∗(T ). To find which ρ have an invariant, regular s, we look through the possible images of Galois: conjugacy classes of subgroups of D12 that don’t fix any line.

C2: generated by α α: Then an invariant s needs to evaluate on all • roots to 1 which is7→ impossible. − − C3: Then three short roots in an orbit need to evaluate to the same value on • −1 s. The other three short roots evaluate to the square, so we need α1(s) = 2 α1(s) = α1(s)= ζ3, which means that long roots evaluate to 1, which is impossible.⇒ D4: impossible since C2 is. • D : impossible since C is • 6 3 C6: impossible since C2, C3 are. • D : impossible since C , C are. • 12 2 3 Therefore none are elliptic endoscopic groups. If a group contributes to the stabilization applied to our test function, then by the fundamental lemma, it needs to be unramified away from infinity. By formulas for transfers of pseudocoefficients (see [Dal19, lem. 5.6.1]), it needs to have an elliptic maximal torus at infinity. The only groups contributing are therefore the G and the SL SL / 1 . 2 2 × 2 {± } 4.2. Endoscopic Constants and Normalizations. DISCRETE, QUATERNIONIC AUTOMORPHIC REPS. ON G2 13

4.2.1. The ι. Let H = SL SL / 1 and let Gc be the unique non-split inner 2 × 2 ± 2 form of G2 over Q which is compact at infinity. Then, τ(G) 1 ι(Gc ,H)= ι(G ,H)= Λ(H, ,s,η) −1 =1 , 2 2 | H | τ(H) · 2 c ι(G2, G2)=1, 1 1 by Kottwitz’s formula for Tamagawa numbers (note that ker (Q,ZH ) = ker (Q, 1 )= 1). {± } 4.2.2. The transfer factors. We also need to fix transfer factors at all places to compute transfers. The computations in [Ta¨ı17] demonstrate how to do so explic- itly. First, they can be chosen consistently by fixing a global Whittaker datum. The corresponding local Whittaker datum determine the local transfer factors as in [KS99]. Since G2 is defined over Z, we can choose a global datum that is unram- ified/admissible at all finite places with respect to the G2(Zp) as in [Hal93, §7], so we can use the fundamental lemma at all finite places. All we will need to know about the Archimedean Whittaker datum for G2 is which element of Π ((k 2)β) it makes Whittaker-generic. This will have to disc − be π(k−2)β,1 since our choice of dominant Weyl chamber has all simple roots non- compact and is the only possible such choice up to ΩK (see the discussion before lemma 4.2.1 in [Ta¨ı17]. In fact, there is only one possible conjugacy class of Whit- taker datum at infinity by considerations explained there). 4.2.3. The stabilizations. We fix canonical measure at finite places so that the fun- H 1 ∞ 1 ∞ damental lemma directly gives K = KH . Recall that EP-functions and pseu- G2 docoefficients are defined depending on measure so we don’t need to fix measure at infinity. Then, (2) gives

G2 (3) I (ϕπ (s ,(k−2)β) 1K∞ ) G2 α2 ⊗ G2

G2 G2 1 H H = S (η 1K∞ )+ S ((ϕπ (s ,(k−2)β)) 1K∞ ). (k−2)β ⊗ G2 2 G2 α2 ⊗ H A simple case of the discrete transfer formula in [Lab11, §IV.3] computes that c G2 G G2 c c (η ) 2 = η (note that ΩR(G ) ΩC(G ) is trivial so κ is too), so (k−2)β (k−2)β 2 \ 2 c c c G G2 G G2 1 H G2 H I 2 (η 1 ∞ )= S 2 (η 1 ∞ )+ S ((η ) 1 ∞ ). (k−2)β K c (k−2)β KG (k−2)β KH ⊗ G2 ⊗ 2 2 ⊗ Since type A1 A1 has no non-trivial centralizer of full semisimple rank, all elliptic endoscopy of SL× SL / 1 is non-split. Therefore, it is ramified at some prime, 2 × 2 ± 1 ∞ H H so the transfers of KH vanish, implying that S = I on our test functions. Substituting one stabilization into another finally gives:

c c G G G2 (4) I 2 (ϕ 1 ∞ )= I 2 (η 1 ∞ ) πG2 (sα2 ,(k−2)β) KG (k−2)β K c ⊗ 2 ⊗ G2 c 1 H G2 H 1 H H I ((η ) 1K∞ )+ I ((ϕπ (s ,(k−2)β)) 1K∞ ) − 2 (k−2)β ⊗ H 2 G2 α2 ⊗ H under canonical measure at finite places. This is our realization of method 2. There are three steps remaining to get counts: (1) Compute the transfers of EP-functions to H. 14 RAHUL DALAL

H (2) Write the resulting I (ηλ 1KH ) terms in terms of counts of level-1, clas- sical modular forms. ⊗ c (3) Look up values for the G2-term from [CR15].

5. Real Endoscopic Transfers

Let H again be the one endoscopic group we care about: SL2 SL2/ 1 . We c × {± } want to compute (ϕ )H and (ηG2 )H . By our choice of transfer πG2 (sα2 ,(k−2)β) (k−2)β factors, we may do so by the formulas in [Lab11, §IV.3]. As a choice for computation that doesn’t affect the final result, we realize the ∗ roots of H as 2ǫ1 and 2ǫ2. Orient X (T ) by setting the 1st quadrant in ǫ1 and ǫ2 to be dominant. The Weyl elements Ω(G, H) that send the G-dominant chamber to an H-dominant one are 1,s ,s . { α1 α2 } ∗ 5.1. Root Combinatorics. Since ρG ρH X (T ), [Lab11, §IV.3] gives the transfer of the pseudocoefficient of the quaternionic− ∈ discrete series to H: (5) (ϕ )H = πG2 (sα2 ,(k−2)β) H −1 H H −1 H H κ (sα2 )η(k−2)β+ρ −ρ κ (sα1 sα2 )ηs ((k−2)β+ρ )−ρ ηs ((k−2)β+ρ )−ρ G H − α1 G H − α2 G H for some signs κ. We compute that ρH = ǫ1 + ǫ2. Then (k 2)β + ρ ρ = (k 2)(3ǫ + ǫ )+(3ǫ + ǫ)=3(k 1)ǫ + (k 1)ǫ . − G − H − 1 2 1 − 1 − 2 In addition,

sα1 ρG =5ǫ1 + ǫ2, sα1 β = β,

sα2 ρG = ǫ1 +3ǫ2, sα2 β =2ǫ2, so s ((k 2)β + ρ ) ρ = (k 2)(3ǫ + ǫ )+(4ǫ )=(3k 2)ǫ + (k 2)ǫ α1 − G − H − 1 2 1 − 1 − 2 and s ((k 2)β + ρ ) ρ = (k 2)(2ǫ )+(2ǫ )=2(k 1)ǫ . α2 − G − H − 2 2 − 2 5.2. Endoscopic Characters. It remains to compute the κ terms in 5. These signs depend in a very complicated way on the realization of H and the exact trans- fer factors chosen. They can be pinned down most easily by looking at endoscopic character identities. Let ψH be a (discrete in our case) L-parameter for H(R) and ψG the composition :with LH ֒ LG . The we have an identity of traces over L-packets → 2 SΘ (f H )= ϕ , π Θ (f), ψH h H i π π∈Π XψG H where f is a transfer of f,Θπ is the Harish-Chandra character, SΘψH is the stable character corresponding to the L-packet, ΠϕG is the L-packet corresponding to the L-parameter, and ϕH , π is a particular pairing depending on transfer factors. See [Kal16, §1] for an expositionh i of how this works in general. If π on G2 is discrete series, Labesse’s formula tells us:

G2 H H (ϕπ ) = ǫ(λ, π)ηλ Xλ DISCRETE, QUATERNIONIC AUTOMORPHIC REPS. ON G2 15 for some signs ǫ and weights λ. Let ψλ be the L-parameter corresponding to weight-λ discrete series on H. Plugging this formula into the character identity for ψλ gives that ψλ is required to push forward to the parameter for π and that ǫ(λ, π)= ψ , π . h λ i The only fact we need now is that ǫ(λ, π) = ψλ, π = 1 whenever π is the Whittaker-generic member of its L-packet. Therefore,h ini Labesse’s formula for the generic member π1,(k−2)β,

H H H H (ϕπ (1,(k−2)β)) = η + κ (sα1 ) sgn(sα1 )η G2 (k−2)β+ρG−ρH sα1 ((k−2)β+ρG)−ρH H H + κ (sα2 ) sgn(sα2 )η , sα2 ((k−2)β+ρG)−ρH all the coefficients need to be 1. The allows to solve κH (s )= κH (s )= 1 α1 α2 − for our choice of transfer factors. Right-ΩR-invariance of κ then also gives that κH (s s )= 1. α1 α2 − 5.3. Final Formulas for Transfers. Therefore, our final transfer is

H H H H (6) (ϕπ (s ,(k−2)β)) = η + η η . G2 α2 − 3(k−1)ǫ1+(k−1)ǫ2 (3k−2)ǫ1+(k−2)ǫ2 − 2(k−1)ǫ2 c c c Transfers from G2 are easier. Here, ΩR(G2) ΩC(G2) is trivial so the average value of κ is 1. Averaging Labesse’s formula as in\ [Dal19, cor. 5.1.5] therefore gives:

c (7) (ηG2 )H = ηH ηH ηH . (k−2)β 3(k−1)ǫ1+(k−1)ǫ2 − (3k−2)ǫ1+(k−2)ǫ2 − 2(k−1)ǫ2

6. The H = SL SL / 1 term 2 × 2 ± Here we compute the terms IH (η 1 ) for Euler-Poincar´efunctions η . Any λ ⊗ KH λ λ = aǫ1 + bǫ2 is a weight of H if a + b is even. Note first that

H H H ∞ H I (η 1 )= tr ∞ (η ) tr (1 )= tr ∞ (η ), λ ⊗ KH π λ π KH π λ π∈ARdisc(H) π∈ARdisc(H) X π unram.X by Arthur’s simple trace formula and using our choice of canonical measure at finite places. To move forward, we need to understand automorphic reps on H by relating them to other groups. Consider the sequence 1 1 SL SL H 1. →± → 2 × 2 → → It induces on local or global F : 1 1 SL SL (F ) H(F ) F ×/(F ×)2 1, →± → 2 × 2 → → → 1 × × 2 1 using that H (F, 1) = F /(F ) and H (F, SL2) = 1 for the F we care about (the R case of the± second equality comes from the determinant exact sequence on ′ GL2). Let HF be the image of SL2 SL2(F ). × ′ As noted in a similar analysis for SL2 in [LL79], unitary irreducibles for HF induce to semisimple representations of H(F ). 16 RAHUL DALAL

6.1. Cohomological Representations of H(R). Next, we recall that the infinite trace measures an Euler characteristic against (h,KH,∞)-cohomology: H ∗ tr ∞ (η )= χ(H (h,K ∞, π∞ V )), π λ H, ⊗ λ where h is the Lie algebra of H(R) and Vλ is the finite dimensional representation of weight λ. Using the definition from [BW00, §5.1],

0 ∗ ∗ 0 KH,∞/K ∞ H (h,K ∞, π∞ V )= H (h,K , π∞ V ) H, , H, ⊗ λ H,∞ ⊗ λ ′ it suffices to consider the π∞ whose restrictions to H∞ contain a component that is cohomological when pulled back to [SL2 SL2](R). By Frobenius reciprocity and semisimplicity of inductions, these are exactly× the irreducible constituents of H∞ ′ ′ ′ ′ IndH∞ π for π cohomological of H∞. ′ ′ ′(h) Next, H∞ is index 2. Pick h H∞ H∞ and let π be the representation γ π′(h−1γh). Define character∈ − 7→ ′ χ : H∞ H∞/H = 1. 7→ ∞ ± ′ ′ There are two cases for H∞-cohomological π : ′ ′(h) H∞ ′ H∞ H∞ ′ ′ ′(h) (1) π = π : then Ind ′ π is irreducible, and Res ′ Ind ′ π = π π . 6 H∞ H∞ H∞ ⊕ ′ ′(h) H∞ ′ (2) π = π : then Ind ′ π = V (V χ) for some irreducible V . Only one H∞ ⊕ ⊗ of these factors will have a subspace fixed by KH,∞ so only one of them will H∞ H∞ ′ ′ ′ have fixed chains and therefore be cohomological. Also, ResH∞ IndH∞ π = π′ π′. ⊕ Recalling a standard result, the cohomological representations of SL2(R) with respect to λ are:

A discrete series L-packet πλ,1, πλ,s (where ΩSL2 = 1,s ), • The trivial representation 1 if λ = 0. { } • SL2 By the K¨unneth rule, cohomological representations of SL2 SL2(R) are exactly products of those on SL (R). Those of H′ are exactly the SL× SL (R) ones that 2 ∞ 2 × 2 are trivial on 1—in other words, with λ = aǫ1 + bǫ2 and a + b even. Consider such± λ. There are three cases of inductions to consider to compute ′ the cohomological representations of H. Note that conjugation by h H∞ H ∈ − ∞ switches both factors to the other member of their SL2-L-packet if they are discrete series and otherwise fixes the trivial representation. a,b = 0: We look at the inductions of products of discrete series. This • is case6 (1) so the 4 products pair up in sums that are 2 members of an H H L-packet. These are of course πλ,1 and πλ,s where s is a length-1 element of ΩH : H π ′ = (π ⊠ π ) (π ⊠ π ), λ,1|H∞ aǫ1,1 bǫ2,1 ⊕ aǫ1,s bǫ2,s H π ′ = (π ⊠ π ) (π ⊠ π ). λ,s|H∞ aǫ1,1 bǫ2,s ⊕ aǫ1,s bǫ2,1 Without loss of generality, a =0,b = 0: We also need to consider inductions • ⊠ 6 H of 1 πbǫ2,⋆. This is case (1) and both induce to a single irreducible σλ : H σ ′ = (1 ⊠ π ) (1 ⊠ π ). λ |H∞ bǫ2,1 ⊕ bǫ2,s a = b = 0: In addition to both the above, we need to consider the induction • ⊠ of 1SL2 1SL2 . This is case (2). This trivial representation induces to

1 ∞ χ on H∞. The cohomological piece is 1 ∞ . H ⊕ H DISCRETE, QUATERNIONIC AUTOMORPHIC REPS. ON G2 17

′ Grothendieck group relations stay true restricted to H∞ so we can compute traces against ηλ. Recall that in SL2(R): 1 = I π π , − 0,1 − 0,s where I is some non-cohomological parabolically induced representation. First, by our normalization H H tr H (η )=tr H (η )=1/2. πλ,1 λ πλ,s λ ′ Next, working in H∞: 1 ⊠ π = (I π π ) ⊠ π = I ⊠ π π ⊠ π π ⊠ π , λ,⋆ − 0,1 − 0,s λ,⋆ λ,⋆ − 0,1 λ,⋆ − 0,s λ,⋆ so σH = 1 ⊠ π + 1 ⊠ π = I ⊠ (π + π ) πH πH , λ λ,1 λ,s λ,1 λ,s − 0+λ,1 − 0+λ,s implying H trσH (ηλ )= 1. λ − Finally

1 ⊠ 1 = (I π π ) ⊠ (I π π ) − 0,1 − 0,s − 0,1 − 0,s = I ⊠ I I ⊠ (π + π ) (π + π ) ⊠ I + πH + πH , − 0,1 0,s − 0,1 0,s 0+0,1 0+0,s so H tr1(ηλ )=1. In total, our H-term becomes a count

w(π∞), π∈ARXdisc,ur(H) where w is a weight

0 π∞ not cohomological H H 1/2 π∞ one of the πλ,∗ w (π∞)= H .  1 π∞ one of the σ ∗ − λ, 1 π∞ trivial  Call the cohomological cases type I, II, and III in order.

6.2. Reduction to Modular Form Counts. We now recall a result from [CR15]. ′ ′ ′ ′∞ Consider central isogeny G G of algebraic groups over Z. If π = π∞ π is an unramified, discrete automorphic→ representation of G′, let R(π′) be the⊗ set of ∞ unitary, admissible representations π = π∞ π of G(A) that satisfy: ⊗ π∞ is unramified with Satake parameters induced from those of π′∞ through • G′ G. → ′ ′ π∞ is a constituent of the restriction of π through G(R) G (R). • ∞ → b b ′ ′ Note that the size of R(π ) is the number of constituents of the restriction of π∞.

Theorem 6.2.1 ([CR15, cor. 4.10]). Assume that all π disc,ur(G) have mul- ′ ′ ∈ AR ′ ′ tiplicity one. Then the same holds for G and the R(π ) with π disc,ur(G ) partition (G). ∈ AR ARdisc,ur 18 RAHUL DALAL

Make similar definitions of type I, II, and III for representations of [SL SL ](R) 2 × 2 and [GL2 GL2](R). Since type I and II on H decompose into two constituents in SL SL ×and type III decomposes into 1, our count becomes π (SL 2 × 2 ∈ ARdisc,ur 2 × SL2) weighted by

1/4 π∞ type I SL2×SL2 w (π∞)= 1/2 π∞ type II . − 1 π∞ type III Each π (SL SL ) lifts to a rep of SL SL G2 . This group ∈ ARdisc,ur 2 × 2  2 × 2 × m is further isogenous to GL2 GL2 so we apply the theorem again. Type I on GL GL decomposes into 4× constituents on SL SL G2 , type II into 2, and 2 × 2 2 × 2 × m type III into 1. Therefore, we get a count of π disc,ur(GL2 GL2) weighted by ∈ AR ×

1 π∞ type I GL2×GL2 w (π∞)= 1 π∞ type II . − 1 π∞ type III Let (1) be the set of normalized, level-1, weight-k cuspidal eigenforms. If k  λ = aǫS+ bǫ , then type I representations on GL GL correspond to pairs in 1 2 2 × 2 Sa+2(1) Sb+2(1). Type II is a single form times the trivial representation and Type I is× only the trivial representation.

6.3. Final Formula for SH . Therefore, if S = (1) , k |Sk | we get: (8) IH (ηH 1 ) = (S 1 )(S 1 ), aǫ1+bǫ2 ⊗ KH a+2 − a=0 b+2 − b=0 using canonical measure at finite places. By a classical formula ([DS05, Thm. 3.5.2] for example), 0 a +2=2or a + 2 odd a+2 Sa+2 = 1 a +2 2 (mod 12) . ⌊ 12 ⌋− ≡  a+2 else ⌊ 12 ⌋  7. A Jacquet-Langlands-style result 7.1. First Form. Generalizing (4) slightly and substituting in (6) and (7) gives:

c ∞ c G ∞ ∞ (9) IG2 (ϕ f )= IG2 (η 2 f ) IH (ηH (f )H ) πk ⊗ (k−2)β ⊗ − (3k−3)ǫ1 +(k−1)ǫ2 ⊗ + IH (ηH (f ∞)H ). (3k−2)ǫ1+(k−2)ǫ2 ⊗ ∞ c ∞ ∞ for any unramified function f (we use here that (G2) = (G2) ). This will let c us describe the set k(1) for k > 2 in terms of certain representations of G2 and H. Q ∞ ∞ Choose π = πk π k(1). Since π is unramified, it can be described by a sequence of Satake⊗ parameters:∈ Q for each prime p, a semisimple conjugacy class ∞ cp(π ) [G2]ss (note that G2 is split so we don’t need to worry about the full Langlands∈ dual and see [ST16, §3.2] for full background). c DISCRETE, QUATERNIONIC AUTOMORPHIC REPS. ON G2 19

The endoscopic datum for H also gives an embedding H ֒ G2 (noting again that everything is split) whose image contains a chosen maximal→ torus and therefore induces a map b c G2 ։ TH :[H]ss [G2]ss.

The fibers of this map are ΩG2 -orbits of conjugacy classes in H and have size 3 at G2-regular elements. b c ∞ ∞ Proposition 7.1.1. Let k > 2 and π an unramified representation of (G2) . Then

c 1 mG2 (π π∞)= mG2 (V π∞) SH (π∞, (3k 3)ǫ + (k 1)ǫ ) disc k ⊗ disc (k−2)β ⊗ − 2| − 1 − 2 | 1 + SH (π∞, (3k 2)ǫ + (k 2)ǫ ) . 2| − 1 − 2 | c Recall here that Vλ is the finite dimensional representation of G2 with highest weight H ∞ ∞ λ. Also, S (π , λ) is the set of π∞ π1 disc(H) such that: H ⊗ ∈ AR π∞ Π (λ), • ∈ disc For all p, c (π∞) (T G2 )−1(c (π∞)). • p 1 ∈ H p Proof. This is a standard Jacquet-Langlands-style argument. Through the Sa- take isomorphism, each f can be thought of as a function [G ] C through p 2 ss → fp(cp(π)) = trπp (fp). It is in fact a Weyl-invariant regular function on a maximal torus in G2. The full version of the fundamental lemma (seec the introduction to [Hal95] for example) shows that

c H G2 fp (cp)= fp(TH (cp)) for all cp H. ∈ ∞ G2 ∞ ∞ There are only finitely many sequences cp(π1 ) and TH (cp(π1 )) for π1 the unramified finiteb component of an automorphic representation either:

of G2 with infinite part πk, • of Gc with infinite part V , • 2 (k−2)β or of H with infinite part in Π ((3k 3)ǫ + (k 1)ǫ ) or Π ((3k • disc − 1 − 2 disc − 2)ǫ1 + (k 2)ǫ2). − ∞ ∞ Therefore we can choose an f that is 0 on all of these sequences cp(π1 ) except 1 ∞ on exactly the sequence cp(π ) (this reduces to finding Weyl-invariant polynomials on (C×)2 that take specified values on certain Weyl orbits). The result follows from ∞ H  plugging this f into (9) and noting that mdisc(π) is always 0 or 1. 7.2. In terms of Modular Forms. We can use the argument from section 6.2 to reduce the H-multiplicity terms to GL2-multiplicty ones. Since we already got multiplicity 1 from comparing H to SL SL there, it will end up being more 2 × 2 convenient here to compare H to PGL2 PGL2. First, we have a map on conjugacy classes× T H :[PGL\PGL ] ։ [H] . PGL2×PGL2 2 × 2 ss ss Since the first group is SL2 SL2(C), the fibers of this map are of the form c, c for some c [SL SL (C)]× . Composing then gives mapb { − } ∈ 2 × 2 ss G2 \ T :[PGL2 PGL2]ss ։ [G2]ss. PGL2×PGL2 × c 20 RAHUL DALAL

This allows us to define SPGL2×PGL2 (π∞, λ) analogous to SH (π∞, λ) for all λ = aǫ1 + bǫ2 with both a and b even. For indexing purposes, set it to be empty when a and b aren’t even. H ∞ Formula (8) gives us that S (π ,aǫ1 + bǫ2) = also when a and b aren’t ∅ PGL2×PGL2 both even. In addition, the restriction of discrete series πλ to H(R) H has as components the entire L-packet Πdisc(λ). Therefore, theorem 6.2.1 shows H ′ ′ PGL2×PGL2 ∞ H ∞ that the RPGL2×PGL2 (π ) for π S (π , λ) partition S (π , λ). Since H ∈ RPGL2×PGL2 is two-to-one, this gives SH (π∞, λ) =2 SPGL2×PGL2 (π∞, λ) . | | | | Finally, PGL2 is a quotient of GL2 by a central torus with trivial Galois coho- mology, so automorphic representations on PGL2 are just those on GL2 with all components having trivial central character. Recalling injection , [(ι : [SL SL (C)] ֒ [GL GL (C 2 × 2 ss → 2 × 2 ss this gives: ∞ ∞ Corollary 7.2.1. Let k> 2 and π an unramified representation of (G2) . Then

Gc mG2 (π π∞)= m 2 (V π∞) SGL2×GL2 (π∞, (3k 3)ǫ + (k 1)ǫ ) disc k ⊗ disc (k−2)β ⊗ − | − 1 − 2 | + SGL2×GL2 (π∞, (3k 2)ǫ + (k 2)ǫ ) . | − 1 − 2 | c Recall here that Vλ is the finite dimensional representation of G2 with highest weight GL ×GL2 ∞ ∞ λ. Also, S 2 (π , λ) is the set of π∞ π (GL GL ) such that: ⊗ 1 ∈ ARdisc 2 × 2 GL2×GL2 π∞ is the discrete series πλ , • ∞ ′ ′ G2 −1 ∞ For all p, cp(π ) = ι(c ) for some c (T ) (cp(π )). Here ι • 1 p p ∈ PGL2×PGL2 . [(is the map [SL SL (C)] ֒ [GL GL (C 2 × 2 ss → 2 × 2 ss Of course, since all infinite terms in sight are discrete series, we may again replace the mdisc by mcusp using [Wal84]. GL2×GL2 ∞ Note of course that S (π ,aǫ1 + bǫ2)= unless both a and b are even. Therefore, we can interpret this as, for k> 2: ∅

If k is even: k(1) is the corresponding set of representations transferred • c Q from G2 in addition to representations transferred from pairs of cuspidal eigenforms in − (1) − (1). S3k 2 × Sk 2 If k is odd: k(1) is the corresponding set of representations transferred • c Q from G2 except for representations that are also transferred from pairs of cuspidal eigenforms in − (1) − (1). S3k 3 × Sk 1 Results for level > 1 would be a lot more complicated since formula (4) would have many further hyperendoscopic terms and the comparison to GL2 GL2 would not work as nicely. ×

8. Counts of forms c 8.1. Formula in terms of IG2 . To get counts instead of a list, combining formulas (1),(9), and (8) gives that

c Gc G2 2 ∞ k(1) = I (ηλ 1K c ) (S3k−1 13k−3=0)(Sk+1 1k−1=0) |Q | ⊗ G2 − − − + (S 1 − )(S 1 − ). 3k − 3k 2=0 k − k 2=0 DISCRETE, QUATERNIONIC AUTOMORPHIC REPS. ON G2 21

This finally becomes, for k> 2:

c G2 ∞ (10) k(1) = I (ηλ 1K c ) |Q | ⊗ G2 k k 1 k 2 (mod 12) ⌊ 4 ⌋ ⌊ 12 ⌋− ≡ k k k 0, 4, 6, 8, 10 (mod 12) ⌊ 4 ⌋⌊12 ⌋  ≡  3k−1 k+1 +  12 1 12 1 k 1 (mod 12) . − ⌊ ⌋− ⌊ ⌋− ≡  3k−1 1 k+1 k 5, 9 (mod 12) − ⌊ 12 ⌋− ⌊ 12 ⌋  ≡ 3k−1 k+1 k 3, 7, 11 (mod 12)  12 12  −⌊ ⌋⌊ ⌋ ≡ c c G2 c G2 8.2. Computing I . The group G2(R) is compact so the I term takes a very simple form: L2(Gc (Q) Gc(A)) decomposes as a direct sum of automorphic repre- 2 \ 2 sentations and the EP-functions ηλ are just scaled matrix coefficients of the finite- c dimensional representations Vλ with highest weight λ on G2(R). Therefore c G2 ∞ ∞ ∞ I (ηλ 1K c )= 1π∞=Vλ trπ (1K c ), ⊗ G2 G2 ∈AR c π X(G2) c which is just counting the number of unramifed automorphic reps of G2 that have infinite component Vλ. ∞ By standard results on unramified representations, taking K c invariants sends G2 each such π to a linearly independent copy of Vλ that together span the Vλ-isotypic component of 2 c c ∞ 2 c c 2 c L (G (Q) G (A)/K c )= L (G (Z) G (R)) L (G (R)). 2 \ 2 G2 2 \ 2 ⊆ 2 2 c ⊕ dim Vλ By Peter-Weyl, L (G2(R)) has Vλ-isotypic component Vλ . In fact, this com- ponent for both the left- and right-actions is the same subspace. Therefore the c Z number of copies of V L2(Gc (Z) Gc (R)) is dim V G2( ) by a dimension count. λ ⊆ 2 \ 2 λ Summarizing:   c Gc(Z) G2 ∞ 2 (11) I (ηλ 1K c ) = dim Vλ . ⊗ G2 A PARI/GP 2.5.0 program in the online appendix to [CR15] computes this for all λ by pairing the trace character of V Z with the trivial character. λ|G2( ) 8.3. Table of Counts. Table 1 gives values of k(1) for k = 3 to 52 produced by formula (10) and [CR15]’s table for formula|Q (11). The| lowest-weight example is bolded, although this work does not rule out the existence of an example with weight 2 or weight 1 (as defined by [Pol20, §1.1]). .

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Table 1. Counts of discrete, quaternionic automorphic represen- tations of level 1 on G2.

k (1) k (1) k (1) k (1) k (1) |Qk | |Qk | |Qk | |Qk | |Qk | 3 0 13 5 23 76 33 478 43 1792 4 0 14 13 24 126 34 610 44 2112 5 0 15 8 25 121 35 637 45 2250 6 1 16 23 26 175 36 807 46 2619 7 0 17 17 27 173 37 849 47 2790 8 2 18 37 28 248 38 1037 48 3233 9 1 19 30 29 250 39 1097 49 3447 10 4 20 56 30 341 40 1332 50 3938 11 1 21 50 31 349 41 1412 51 4201 12 9 22 83 32 460 42 1686 52 4780

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