DISCRETE AND CONTINUOUS doi:10.3934/dcds.2020359 DYNAMICAL SYSTEMS Volume 41, Number 5, May 2021 pp. 2205–2225
QUANTITATIVE OPPENHEIM CONJECTURE FOR S-ARITHMETIC QUADRATIC FORMS OF RANK 3 AND 4
Jiyoung Han Research Institute of Mathematics, Seoul National University GwanAkRo 1, Gwanak-Gu Seoul, 08826, South Korea
(Communicated by Zhiren Wang)
Abstract. The celebrated result of Eskin, Margulis and Mozes [8] and Dani and Margulis [7] on quantitative Oppenheim conjecture says that for irrational quadratic forms q of rank at least 5, the number of integral vectors v such that q(v) is in a given bounded interval is asymptotically equal to the volume of the set of real vectors v such that q(v) is in the same interval. In rank 3 or 4, there are exceptional quadratic forms which fail to satisfy the quantitative Oppenheim conjecture. Even in those cases, one can say that two asymptotic limits coincide for almost all quadratic forms([8, Theorem 2.4]). In this paper, we extend this result to the S-arithmetic version.
1. Introduction.
History. The Oppenheim conjecture, proved by Margulis [17], says that the image set q(Zn) of integral vectors of an isotropic irrational quadratic form q of rank at least 3 is dense in the real line (See [19] for the original statement of Oppenheim conjecture). Let (a, b) be a bounded interval and let Ω ⊂ Rn be a convex set containing the n origin. For any T ∈ R>0, define T Ω = {v ∈ R : v/T ∈ Ω}. Dani and Margulis [7] and Eskin, Margulis and Mozes [8] established a quantitative version of Oppenheim conjecture: for a quadratic form q, let V(a,b),Ω(T ) be the volume of the region −1 −1 T Ω ∩ q (a, b) and N(a,b),Ω(T ) be the number of integral vectors in T Ω ∩ q (a, b). They found that if an irrational isotropic quadratic form q is of rank greater than or equal to 4 and is not a split form, then V(a,b),Ω(T ) approximates N(a,b),Ω(T ) as T goes to infinity. Moreover, in this case, the image set q(Zn) is equidistributed in the real line. Their works heavily rely on the dynamical properties of orbits of a certain se- misimple Lie group, generated by its unipotent one-parameter subgroups, on the associated homogeneous space.
2020 Mathematics Subject Classification. Primary: 22F30, 22E45, 20F65; Secondary: 20E08, 37P55. Key words and phrases. Quantitative Oppenheim conjecture, S-arithmetic space, action of quadratic form-preserving groups, low-dimensional p-adic symmetric space, Euclidean building. This paper is supported by the Samsung Science and Technology Foundation under project No. SSTF-BA1601-03 and the National Research Foundation of Korea(NRF) grant funded by the Korea government under project No. 0409-20200150.
2205 2206 JIYOUNG HAN
The S-arithmetic space is one of the optimal candidates for a generalization of n n their work, since it has a lattice ZS which is similar to the integral lattice Z in Rn. Borel and Prasad [5] generalized Margulis’ theorem to the S-arithmetic version and the author, Lim and Mallahi-Karai [13] proved the quantitative version of S- arithmetic Oppenheim conjecture. See also [29] and [15] for flows on S-arithmetic symmetric spaces. Ratner [21] generalized her measure rigidity of unipotent sub- groups in the real case to the Cartesian product of real and p-adic spaces.
Set-up and notation. Consider a finite set Sf = {p1, . . . , ps} of odd primes and let S = {∞} ∪ Sf . We refer to an element of S as a place. For each place p ∈ S, denote by Qp the completion field of Q with respect to the p-adic norm. If p = ∞, Q the norm k · k∞ is the usual Euclidean norm and Q∞ = R. Define QS = p∈S Qp, the Cartesian product of Qp’s (p ∈ S). In this paper, we will use the product notations only for the Cartesian product. Since each Qp has the normed topology, let us assign the product topology of these normed topologies to QS. Let ∆ : Q ,→ QS be the embedding given as ∆(z) = (z, . . . , z) ∈ QS, z ∈ Q. Define
n1 ns ZS = {mp1 ··· ps : m, n1, . . . , ns ∈ Z} ⊂ Q. It is well-known that the quotient /∆( ) ' / × Q is compact, where QS ZS R Z p∈Sf Zp Zp = {z ∈ Qp : |z|p ≤ 1}, so that ∆(ZS) is a uniform lattice subgroup of QS. For simplicity, we will use the notations Q and ZS instead of ∆(Q) and ∆(ZS), respectively. n Let us define an S-lattice Λ in QS as a free ZS-module of rank n. An S-quadratic form qS is an S-tuple of quadratic forms qp defined over Qp (p ∈ S). We only consider the cases when all of qp have the same rank, and in this case, we define the rank of qS as the rank of qp. We call qS nondegenerate (isotropic, respectively) if every qp in qS is nondegenerate (isotropic, respectively). We say that qS is rational if there is a single rational quadratic form q such that qS = (λpq)p∈S, where λp ∈ Qp − {0} and qS is irrational if it is not rational. n Q n n One can regard a Q-module QS as the product p∈S Qp of vector spaces Qp n (p ∈ S). Let us denote an element of QS by v = (vp)p∈S, where vp is a vector in n Qp for each p ∈ S. We refer to the p-adic norm kvkp as the p-adic norm kvpkp of a n vector vp ∈ Qp . Define the map σ : S → {1, −1} by −1 if p < ∞, σ(p) = 1 if p = ∞. σ σ n We will use the notation v/kvkp := (vp/kvpkp )p∈S for an element of QS consisting of unit vectors in each place p ∈ S. n For p ∈ S, we fix a star-shaped convex set Ωp on Qp centered at the origin defined as n σ Ωp = v ∈ Qp : kvkp < ρp(v/kvkp ) , n Q where ρp is a positive function on the set of unit vectors in Qp and let Ω = p∈S Ωp. If p < ∞, we further assume that ρp is (Zp − pZp)-invariant: for any u ∈ Zp − pZp n n and for any unit vector vp ∈ Zp − pZp ,
ρp(uvp) = ρ(vp).
Let Ip ⊂ Qp be a bounded convex set of the form (a, b), where a, b ∈ R, if p = ∞, b and a+p Zp, where a ∈ Qp and b ∈ Z, if p < ∞. We call Ip a p-adic interval. Define S-ARITHMETIC QUANTITATIVE OPPENHEIM FOR LOW RANK 2207 an S-interval I = Q I . Denote by T = (T ) ∈ × Q (pZ ∪ {0}), S p∈S p p p∈S R≥0 p∈Sf m the S-tuple of radius parameters Tp, p ∈ S, where pZ = {p : m ∈ Z}. Consider Q TΩ = p∈S TpΩp the dilation of Ω by T.
Main statement. We are interested in the number N(T) = N(qS, Ω, IS)(T) of n elements v in ZS ∩TΩ such that qS(v) ∈ IS. Let µ be the product of Haar measures µp on Qp, p ∈ S. We assume that µ∞ is the usual Lebesgue measure on R and µp(Zp) = 1 when p < ∞. Let V(T) = V(qS, Ω, IS)(T) be the volume of the set n n {v ∈ TΩ: qS(v) ∈ IS} with respect to µ on QS. Recall that a quadratic form of rank 4 is split if it is equivalent to x1x4 − x2x3. In [13], when an isotropic irrational quadratic form qS is of rank n ≥ 4 and does not contain a split form, then as T → ∞, N(T) approximates V(T). Here, we say that T → ∞ if Tp → ∞ for all p ∈ S. Moreover, it is possible to estimate V(T) in terms of I and T ([13, Proposition 1.2]). As a result, there is a constant λ > 0 S qS ,Ω such that as T goes to infinity, N(T) ∼ λ µ(I )|T|n−2, qS ,Ω S Q where |T| = p∈S Tp ([13, Theorem 1.5]). Although [13] provides a precise condition of quadratic forms for which the quan- titative Oppenheim conjecture holds, for the case of rank 4, the condition that qS does not contain any split form, forces us to exclude substantial numbers of compo- s s s nents (3 × 7 − 2 × 6 among 3 × 7 , where s = #Sf ) in the space of nondegenerate n isotropic quadratic forms in QS. Note that each of the components can be identified 0 0 with the quotient space SO(qS)\SLn(QS), for some qS. In fact, there are quadratic forms for which N(T) fails to approximate V(T), when qS is of rank 3, or qS is of rank 4 and contains a split form. For instance, there is an irrational quadratic form 1−ε qS of rank 3 and a sequence (Tj) for a given ε > 0 so that N(Tj) ≥ |Tj|(log |Tj|) (See[8, Theorem 2.2] and [13, Lemma 9.2]). Our main theorem shows that quadratic forms for which N(T) approximates V(T) are generic in those excluded components, hence in the whole space of non- degenerate isotropic quadratic forms. In the case of rank 3, Theorem 1.1 is entirely a new result. Here, the term generic is with respect to the following measure: since one can 0 identify each component of the space of quadratic forms with SO(qS) \ SLn(QS), 0 where qS = (qp)p∈S is taken to be associated with the discriminant of each qp, one can assign an SLn(QS)-invariant measure on this space.
Theorem 1.1. For almost all isotropic quadratic forms qS of rank 3 or 4, as T → ∞, N(q , Ω, I )(T) ∼ λ µ(I )|T|n−2, S S qS ,Ω S where n = rank(q ) and λ is a constant depending on the quadratic form q S qS ,Ω S and the convex set Ω described above. For the case of real quadratic forms of signature (2, 2), Eskin, Margulis and Mozes provided an example of a quadratic form such that Na,b,Ω(T ) does not approximate to Va,b,Ω(T ) and found a necessary condition of quadratic forms (called EWAS) that two quantities asymptotically coincide [9]. On the generic quadratic forms and their Oppenheim conjecture-type problems, there is a work of Bourgain [6] for real diagonal quadratic forms using the analytic number-theoretical method. Ghosh and Kelmer [11] showed another version of 2208 JIYOUNG HAN the quantitative version of Oppenheim problem for real generic ternary quadratic forms and Ghosh, Gorodnik and Nevo [10] extended this result for more general setting, such as for generic characteristic polynomial maps. Recently, there have been effective results about the bound of the error terms N(a,b),Ω(T ) − V(a,b),Ω(T ) for almost all real quadratic forms of rank at least 3 by Athreya and Margulis [2], for almost all real homogeneous forms of even degree and of rank at least 3 by Kelmer and Yu [14], and for almost all systems of a homogeneous polynomial of even degree and a linear map with the certain condition by Bandi, Ghosh and the author [3]. For a pair of a quadratic form q and a linear form L of Rn, Gorodnik [12] com- puted the density of {(q(v),L(v)) : v ∈ P(Zn)} ⊆ R2 under the certain assumption and Lazar [16] generalized his result for the S-arithmetic setting. Sargent computed the density of M({v ∈ Zn : q(v) = a}) ⊆ R, where q is a rational quadratic form and M is a linear map [23]. In [24], he showed the quantitative version of his result.
Strategy and organization. The proof of the main theorem is provided in Section 4, by showing that V(T) approximates N(T) almost surely, using an equidistribution theorem (Proposition2) in one hand and the fact that V(T) is asymptotically n−2 proportional to the measure of IS and |T| on the other hand (Proposition4). Note that functions we consider in Section 4 are unbounded and non-compactly supported so that the general type of equidistribution theorems are not applicable.
In Section 3, we will introduce an αS-function, defined on SLn(QS)/SLn(ZS), to modify an equidistribution theorem for those functions. The function αS gives an upper bound to functions we want to consider (so-called Schmidt’s lemma), hence enables us to ignore the cusp parts of such functions, in almost all cases. We will prove Proposition2 by using Howe-Moore theorem (Theorem 3.2) and Borel-Cantelli lemma. We also need to compute the measures of some given subsets of a maximal compact subgroup of SO(qS), which are associated with Cartan (also known as KAK) decomposition. For this, in Section 2, we first review the well- known properties of symmetric spaces given by (products of) real hyperbolic spaces, and then explain how one can extend these properties to “the p-adic symmetric spaces”, which are Bruhat-Tits Euclidean buildings in our case.
2. Symmetric spaces. Let us denote by G an S-arithmetic group of the form Q G = p∈S Gp, where Gp is a semisimple Lie group defined over Qp (p ∈ S). An element of G is g = (gp)p∈S = (g∞, g1, . . . , gs), where gi ∈ Gp . In most cases, G is Q i SLn(QS) := p∈S SLn(Qp), n ≥ 3. Consider the lattice subgroup Γ = SLn(ZS) of G and the symmetric space G/Γ, which can be embedded in the space of unimodular n S-lattices in QS. The Haar measure µG on G is the product of Haar measures µp on Gp. We will use the same notation µG for the normalized G-invariant measure on G/Γ. 0 When we refer to qS, which we will call a standard quadratic form, it is an S-tuple of quadratic forms consisting of: 2 q∞(x1, x2, x3) = 2x1x3 + x2, 0 2 if rank(qS) = 3; qp(x1, x2, x3) = 2x1x3 + a1x , 2 (1) 2 2 q∞(x1, x2, x3, x4) = 2x1x4 + a1x2 + a2x3, 0 2 2 if rank(qS) = 4, qp(x1, x2, x3, x4) = 2x1x4 + a1x2 + a2x3, where a1, a2 ∈ {±1} if p = ∞ and a1, a2 ∈ {±1, ±u0, ±p, ±pu0} if p < ∞. Here u0 is some fixed square-free integer in Qp (See [26, Section 4.2]). S-ARITHMETIC QUANTITATIVE OPPENHEIM FOR LOW RANK 2209
0 0 In SO(qS), we fix a maximal compact subgroup K of SO(qS)
Y 0 Y 0 K = K∞ × Kp = SO(q∞) ∩ SO(n) × SO(qp) ∩ SLn(Zp) p∈Sf p∈Sf with the measure m = Q m , where m is the normalized Haar measure on K p∈Sf p p p (p ∈ S). We also fix a diagonal subgroup Y A = a = a : t = (t , t , . . . , t ) ∈ × pZ × · · · × pZ , (2) t tpi ∞ 1 s R≥0 1 s p∈S
−t∞ t∞ tp −tp where at∞ = diag(e , 1,..., 1, e ) and atp = diag(p , 1,..., 1, p )(p ∈ Sf ). These groups K and A will be heavily used throughout the paper. We assume that T and t have the relation
t∞ tp T∞ = e and Tp = p , ∀p ∈ Sf ,
unless otherwise specified. Also we briefly denote by Ti or ti instead of Tpi or tpi respectively. In this section, we take G∞ = SLn(R) and Gp = GLn(Qp), p < ∞, where n = 3 or 4. Corresponding maximal compact subgroups are Kˆ∞ = SO(n) and ˆ Kp = GLn(Zp), respectively.
3 0 2.1. The 3-dimensional hyperbolic space H . Let q∞ be a standard isotropic 0 quadratic form of rank n, n = 3, 4. The special orthogonal subgroup H∞ = SO(q∞) is one of the well-known linear groups SO(2, 1), SO(3, 1) and SO(2, 2). Let us examine the symmetric space K∞ \ H∞ and set a right invariant metric which is invariant by right multiplication. 3 3 Case i) H∞ = SO(3, 1). Set H to be the 3-dimensional hyperbolic space H = {z + ti : z = x + yj ∈ C and t ∈ R>0 }. The group SO(3, 1) is locally isomor- + 3 phic to PSL2(C), which is the group Isom (H ) of orientation-preserving isome- 3 3 tries of H . Here, the (P)SL2(C)-action on H is given by Mobius transformation, a b az + b .z = . Notice that entries of elements in SL ( ) are of the form c d cz + d n C x + yj. Since the stabilizer of the point i in PSL2(C) is the maximal compact subgroup PSU(2), we may identify the symmetric space K∞ \SO(3, 1), which is isomorphic to 3 PSU(2)\PSL2(C), with the hyperbolic space H . Let p : SO(3, 1) → K∞\SO(3, 1) ' 3 H be the projection given by p(g) = g.i. Define the metric d∞ of K∞ \ SO(3, 1) by
3 d∞(g1, g2) = d∞(K∞g1,K∞g2) := dH (p(g1), p(g2)).
Case ii) H∞ = SO(2, 1). Consider the identification
2 K∞ \ SO(2, 1) ' PSO(2) \ PSL2(R) ' H = {x + ti : x ∈ R and t ∈ R>0 }.
Let us use the notation p for the projection SO(2, 1) → H2 as well. We define the metric d∞ of K∞ \ SO(2, 1) by
2 d∞(g1, g2) := dH (p(g1), p(g2)). 2210 JIYOUNG HAN
Case iii) H∞ = SO(2, 2). In the case of H∞ = SO(2, 2), consider the isomorphism 4 between real vector spaces R and M2(R) given by x y (x, y, z, w) 7→ . z w
x y The split form xw − yz of 4 corresponds to the determinant of in R z w M2(R). Moreover, there is the local isomorphism from SL2(R)×SL2(R) to SO(2, 2), which is induced by the action x y x y (g , g ). = g gt . (3) 1 2 z w 1 z w 2 Hence we deduce that
2 2 K∞ \ SO(2, 2) 'loc (SO(2) × SO(2)) \ (SL2(R) × SL2(R)) ' H1 × H2, 2 2 2 where H1 ' H ' H2. Note also that the action of at splits into the action of t/2 −t/2 (bt, bt), where bt = diag(e , e ). Put
d∞ = d := max{d 2 , d 2 }. SO(2,2) H1 H2
Lemma 2.1. Let H∞ be one of SO(2, 1), SO(3, 1) or SO(2, 2). Let K∞ be a maximal compact subgroup of H∞. Then there exists a constant C∞ > 0 such that for any t > 0 and for any r ∈ (0, 2t), −1 −2t+r m∞ k ∈ K∞ : d∞(atkat , 1) ≤ r < C∞e , (4) where m∞ is the normalized Haar measure on K∞. ∼ ∼ Proof. Assume that H∞ = SO(3, 1) = SL2(C) and K∞ = SU(2). For each t > 0, 3 K∞ acts transitively on the hyperbolic sphere S2t ⊂ H of radius 2t centered at i. Since d∞ is H∞-invariant, −1 m∞ k ∈ K∞ : d∞(atkat , 1) ≤ r = m∞ ({k ∈ K∞ : d∞(atk, at) ≤ r}) 2t 3 = LebS y ∈ S2t : dH (y, e i) ≤ r .
Here, LebS is the Lebesgue measure such that LebS(S2t) = 1. For the relation with 3 the p-adic case, p < ∞, let us mention that S2t is isomorphic to ∂H . Let x = e2ti and let θ be the angle between two geodesics from i to x and from i to y (Figure 1). By the hyperbolic law of cosines θ cosh(d(x, y)) = 1 + sinh2(2t) · (1 − cos θ) = 1 + 2 sinh2(2t) sin2( ), 2 and since d(x, y) ≤ r, we obtain that θ is bounded by e−2t+r/2. Hence