1 Introduction
The natural inner product on
$3$
-space defines an algebraic variety
There are several ways to analyze its diophantine properties quantitatively. The equation (1) defines the isotropy cone of a senary quadratic form. In this view, one would ask for an asymptotic formula for the number
$P(X)$
of solutions of (1) in integers not exceeding
$X$
in modulus. A prudent yet routine treatment of this classical question, by the circle method or otherwise, leads one to a positive number
$C_{0}$
with
Alternatively, the left-hand side of (1) is a bilinear form in the variables
$\mathbf{x}=(x_{0},x_{1},x_{2})$
and
$\mathbf{y}=(y_{0},y_{1},y_{2})$
. The first question then is to count the integral solutions of (1) inside a box, with
$\mathbf{x}$
and
$\mathbf{y}$
bounded independently. Thus, writing
$|\mathbf{x}|=\max (|x_{0}|,|x_{1}|,|x_{2}|)$
, an asymptotic expansion is desired for the number
$M(X,Y)$
of
$\mathbf{x},\mathbf{y}\in (\mathbb{Z}\backslash \{0\})^{3}$
that satisfy (1) and lie inside the box
$|\mathbf{x}|\leqslant X$
,
$|\mathbf{y}|\leqslant Y$
. The following theorem provides such a result featuring the sums
and the function
Empty sums are to be read as
$0$
and, consequently,
$F(0)=0$
.
Theorem 1. Let
$\frac{3}{2}\leqslant X\leqslant Y$
. Then
Note that the reservoir of variables
$\mathbf{x},\mathbf{y}$
has about
$(4XY)^{3}$
elements, so that the error term in Theorem 1 corresponds to nearly square root cancellation. This seems to be the limit of what can be expected from the circle method in this problem.
The asymptotic expansion of
$M(X,Y)$
is somewhat involved, but this is inevitable when
$X$
is small and one insists on errors not much larger than
$(XY)^{3/2}$
. When
$X$
gets larger, the main term smoothes out. To see this, let
$t>0$
, write
and note that
Then, equipped with the elementary formula
we readily find that
holds whenever
$\frac{3}{2}\leqslant X\leqslant Y$
. This estimate exhibits square root cancellation in the shorter of the two variables, this time relative to the size of the leading term. We also note that
$P(X)-M(X,X)$
is the number of solutions of (1) with at least one variable
$0$
. Aided by Lemma 2 below, we easily find that
and then recover (2) with
$C_{0}=2(33-\unicode[STIX]{x1D70B}^{2})\unicode[STIX]{x1D701}(2)\unicode[STIX]{x1D701}(3)^{-1}.$
Continuing this line of thought, one may consider
$x=(x_{0}:x_{1}:x_{2})$
and
$y=(y_{0}:y_{1}:y_{2})$
as projective coordinates. The equation (1) then defines a variety
$\mathscr{V}$
in biprojective space. Note that all
$(x_{0}:x_{1}:x_{2})\in \mathbb{P}^{2}(\mathbb{Q})$
have exactly two representations by primitive
$\mathbf{x}=(x_{0},x_{1},x_{2})\in \mathbb{Z}^{3}$
and these differ only by sign, so that their norms
$|\mathbf{x}|$
depend only on the projective point. If
$(x,y)\in \mathbb{P}^{2}(\mathbb{Q})\times \mathbb{P}^{2}(\mathbb{Q})$
is represented by primitive
$\mathbf{x},\mathbf{y}\in \mathbb{Z}^{3}$
satisfying (1), one defines an anticanonical height of this point by
$|\mathbf{x}|^{2}|\mathbf{y}|^{2}.$
One is then interested in the number
$N(B)$
of rational points on
$\mathscr{V}$
of height not exceeding
$B$
. Thus,
$4N(B)$
is the number of all primitive
$\mathbf{x},\mathbf{y}\in \mathbb{Z}^{3}$
satisfying (1), with
$|\mathbf{x}|^{2}|\mathbf{y}|^{2}\leqslant B$
.
Theorem 2. There is a real number
$C$
such that one has
We shall prove Theorem 1 by the circle method and deduce Theorem 2 from Theorem 1 by a development of Dirichlet’s hyperbola method. A direct attempt at Theorem 2 by the circle method occurs in work of Spencer [Reference Spencer7]. He considered the Zariski open subset
$\mathscr{U}$
of
$\mathscr{V}$
where no projective coordinate vanishes. For the number
$N_{0}(B)$
of all points in
$\mathscr{U}$
that are counted by
$N(B)$
, he obtained the asymptotic formula
$N_{0}(B)=c_{0}B\log B+O(B),$
with some positive
$c_{0}$
. It is somewhat unnatural to neglect the points on coordinate hyperplanes and, indeed, one has
We shall confirm this in the final section of this paper. In particular, we see that Spencer’s
$c_{0}$
coincides with the leading constant in Theorem 2. The variety
$\mathscr{V}$
is a prototypical example of a flag variety, for which qualitative asymptotic formulae for the number of rational points of bounded height have been obtained in [Reference Franke, Manin and Tschinkel5]. According to a far-reaching conjecture put forward in [Reference Franke, Manin and Tschinkel5], such formulae should hold for large classes of varieties. Our contribution here is the first instance of an explicit power saving in the error term for the variety under consideration.
The height zeta function of
$\mathscr{V}$
is defined by the series
with summation restricted to primitive
$\mathbf{x},\mathbf{y}\in \mathbb{Z}^{3}$
. By partial summation and Theorem 2, it follows that this series is absolutely convergent in Re
$s>1$
and admits an analytic continuation to the region Re
$s>7/8$
,
$s\neq 1$
, with a double pole at
$s=1$
. Moreover, for any
$\unicode[STIX]{x1D703}>7/8$
, in the region Re
$s\geqslant \unicode[STIX]{x1D703}$
,
$|s-1|\geqslant 1$
, one obtains the growth estimate
$O(|s|)$
as a by-product.
As an aside, we briefly comment on an automorphic approach to the analysis of the variety
$\mathscr{V}$
. The solutions of (1) in primitive vectors
$\mathbf{x},\mathbf{y}$
are in one-to-one correspondence with the cosets of
$\unicode[STIX]{x1D6E4}_{\infty }\backslash \text{SL}_{3}(\mathbb{Z})$
, where
$\unicode[STIX]{x1D6E4}_{\infty }$
is the group of integral upper triangular unipotent matrices. Therefore, a sum over the integral solutions of (1) can be expressed in terms of the minimal parabolic Eisenstein series
$E(g,s_{1},s_{2})$
on
$\text{GL}_{3}$
, as defined in [Reference Bump3, p. 100]. In particular (see [Reference Bump3, (7.2)]), one finds that
where again the sum on the left runs over primitive
$\mathbf{x},\mathbf{y}$
and
$\mathbf{1}$
denotes the
$3\times 3$
identity matrix. The function
$E(\mathbf{1},\frac{2}{3}s,\frac{2}{3}s)$
is meromorphic in the complex plane and in
$\operatorname{Re}s>\frac{1}{2}$
the only poles are at
$s=1$
and
$s=3/4$
[Reference Bump3, Theorem 7.1]. If one is prepared to replace the maximum norm in the notion of height by the euclidean one, a conclusion similar to the one in Theorem 2 is readily recovered. One can express the height zeta function (10) in terms of more general Eisenstein series associated to non-trivial
$\text{SO}_{3}$
-types (cf. [Reference Buttcane and Miller4]), but this leads to delicate convergence issues. It should be noted that the relation to the theory of Eisenstein series plays a similar role, in much broader generality, in the important work of Frankeet al [Reference Franke, Manin and Tschinkel5].
Despite its apparently more limited scope for the problem at hand, our more elementary treatment is of interest because a circle method approach promises success in situations where a suitable group action is not available. In a more general context of multi-homogeneous varieties, this was carried out in our forthcoming article [Reference Blomer and Brüdern1]Footnote 1 . In the present paper, variations of this circle of ideas are developed that provide more control on the error term featured in Theorem 2. We refer to §5, perhaps the most original part of the present communication. Our approach differs substantially from the version of the hyperbola method detailed in [Reference Blomer and Brüdern1].
As a by-product of our analysis, we are led to a curious identity involving the integral sine
that we have not been able to locate in the literature.
Theorem 3. One has
2 The circle method
The circle method argument prominently features the sum
Lemma 1. Let
$\frac{3}{2}\leqslant X\leqslant Y$
. Let
$\unicode[STIX]{x1D6FC}\in \mathbb{R}$
suppose that
$a\in \mathbb{Z}$
and
$q\in \mathbb{N}$
are coprime and satisfy
$|q\unicode[STIX]{x1D6FC}-a|\leqslant q^{-1}$
. Then
Proof. If
$q>XY$
, then the estimate for
$f(\unicode[STIX]{x1D6FC})$
supplied by Lemma 1 is weaker than the “trivial” bound
$f(\unicode[STIX]{x1D6FC})\ll XY$
that is immediate from (12). Thus, we may suppose that
$q\leqslant XY$
. By (12),
where, as usual,
$\Vert \unicode[STIX]{x1D6FD}\Vert$
denotes the distance of the real number
$\unicode[STIX]{x1D6FD}$
to its nearest integer. Lemma 2.1 of Vaughan [Reference Vaughan8] now supplies an estimate for
$f(\unicode[STIX]{x1D6FC})$
, as required.◻
Lemma 2. Let
$\frac{3}{2}\leqslant X\leqslant Y$
. Then
Proof. By orthogonality, the integral in question equals the number of solutions of
$xy=uv$
in integers
$x,y,u,v$
satisfying
By symmetry, it suffices to count solutions with
$1\leqslant u\leqslant x\leqslant X$
. Write
Then
$(x^{\prime };u^{\prime })=1$
and hence
$x^{\prime }\mid v$
,
$u^{\prime }\mid y$
. Consequently, one has
$v=x^{\prime }w$
,
$y=u^{\prime }w$
for some
$w\in \mathbb{Z}$
and it follows that the integral in question does not exceed eight times the number of tuples
$(d,x^{\prime },u^{\prime },w)$
with
Now
$x^{\prime }\leqslant X\leqslant Y$
and, therefore,
This completes the proof of Lemma 2. ◻
Recall that
$M(X,Y)$
denotes the number of
$\mathbf{x},\mathbf{y}\in (\mathbb{Z}\backslash \{0\})^{3}$
with
$|\mathbf{x}|\leqslant X$
,
$|\mathbf{y}|\leqslant Y$
that satisfy (1). Then, by (12) and orthogonality,
We consider separately the contributions to (13) that arise from major and minor arcs. To define the latter, let
The intervals
$\{\unicode[STIX]{x1D6FC}:|q\unicode[STIX]{x1D6FC}-a|\leqslant Q/(XY)\}$
with
$1\leqslant a\leqslant q\leqslant Q$
and
$(a;q)=1$
are disjoint and their union is denoted by
$\mathfrak{M}$
. Let
$\mathfrak{m}=[Q/(XY),1+Q/(XY)]\backslash \mathfrak{M}$
.
By Dirichlet’s theorem on diophantine approximation, for each
$\unicode[STIX]{x1D6FC}\in \mathbb{R}$
there are coprime integers
$a$
,
$q$
with
$1\leqslant q\leqslant 2\sqrt{XY}$
and
$|q\unicode[STIX]{x1D6FC}-a|\leqslant Q/(XY)$
. Hence,
$\unicode[STIX]{x1D6FC}\in \mathfrak{m}$
implies
$q>Q$
here and Lemma 1 yields
By (14) and Lemma 2, we now see that
We now develop an approximation to
$f(\unicode[STIX]{x1D6FC})$
for use on the major arcs. When
$\unicode[STIX]{x1D6FC}\in \mathfrak{M}$
, there is a unique triple
$(q,a,\unicode[STIX]{x1D6FD})\in \mathbb{N}^{2}\times \mathbb{R}$
with
We use this notation throughout the subsequent argument.
We put
$\unicode[STIX]{x1D6FC}=(a/q)+\unicode[STIX]{x1D6FD}$
within (12) and separate terms with
$q\mid x$
from those with
$q\nmid x$
. In the portion where
$q\mid x$
, we restore the term
$y=0$
to infer that
where
Lemma 3. Let
$\unicode[STIX]{x1D6FC}$
be real and
$a\in \mathbb{Z}$
and
$q\in \mathbb{N}$
be coprime with
$|q\unicode[STIX]{x1D6FC}-a|\leqslant Q/(XY)$
. Then
Proof. A very similar estimate occurs as Vaughan [Reference Vaughan9, Lemma 2.12]. We give the simple proof, for completeness. We have
$g_{1}(\unicode[STIX]{x1D6FC})=0$
for all
$\unicode[STIX]{x1D6FC}$
, whence we may suppose that
$q\geqslant 2$
. Summing over
$y$
yields
Now
$\Vert \unicode[STIX]{x1D6FC}x\Vert \geqslant \Vert ax/q\Vert -|\unicode[STIX]{x1D6FD}x|$
. But
$q\nmid x$
and
$(a;q)=1$
imply
$\Vert ax/q\Vert \geqslant 1/q$
, whereas
$|\unicode[STIX]{x1D6FD}x|\leqslant XQ/(qXY)\leqslant 1/(2q)$
by (14). This shows that
$\Vert \unicode[STIX]{x1D6FC}x\Vert \geqslant \frac{1}{2}\Vert ax/q\Vert$
and, so,
$$\begin{eqnarray}g_{q}(\unicode[STIX]{x1D6FC})\ll \mathop{\sum }_{\substack{ 0<|x|\leqslant X \\ q\nmid x}}\biggl\|\frac{ax}{q}\biggr\|^{-1}\ll \biggl(\frac{X}{q}+1\biggr)\mathop{\sum }_{u=1}^{q-1}\biggl\|\frac{au}{q}\biggr\|^{-1}.\end{eqnarray}$$
The conclusion of the lemma is now immediate.
Recalling the relation between
$\unicode[STIX]{x1D6FC}\in \mathfrak{M}$
and
$a,q,\unicode[STIX]{x1D6FD}$
, a function
$f^{\ast }:\mathfrak{M}\rightarrow \mathbb{C}$
is defined via
$f^{\ast }(\unicode[STIX]{x1D6FC})=f_{q}^{\ast }(\unicode[STIX]{x1D6FD})$
. By (16) and Lemma 3, we then have
and, hence, by binomial expansion,
◻
Lemma 4. For
$\frac{3}{2}\leqslant X\leqslant Y$
, one has
Equipped with this lemma, we infer from (17) and Lemma 2 that
The next tasks ahead of us are a proof of Lemma 4 and the evaluation of the integral on the right-hand side of (18). There are parallels in the treatment of the two problems. We begin with the obvious identity
and apply it within (16) to bring in the sum
through the relation
$f^{\ast }(\unicode[STIX]{x1D6FC})=w_{q}(q\unicode[STIX]{x1D6FD})$
. Hence, on considering the contributions from the individual intervals comprising the major arcs separately, we find via the substitution
$\unicode[STIX]{x1D6FE}=q\unicode[STIX]{x1D6FD}$
that
and
Next, we compare
$w_{q}(\unicode[STIX]{x1D6FE})$
with the cognate sum
With this in view, note that for
$|t|\leqslant \unicode[STIX]{x1D70B}/2$
, one has
Hence, for
$|\unicode[STIX]{x1D6FE}|\leqslant (2X)^{-1}$
, we may take
$t=\unicode[STIX]{x1D70B}\unicode[STIX]{x1D6FE}x$
and sum over
$0<|x|\leqslant X/q$
. By (19) and (22), we infer that
holds uniformly in
$q\in \mathbb{N}$
. This implies the bound
and, from (20) and a routine estimation, we deduce that
The trivial upper bounds
are valid for
$q\in \mathbb{N}$
,
$\unicode[STIX]{x1D6FE}\in \mathbb{R}$
and are easily inferred from (22). It follows that
$v_{q}\in L^{2}(\mathbb{R})$
, whence
$v_{q}$
has an
$L^{2}$
Fourier transform
$\hat{v}_{q}$
, defined as the
$L^{2}$
limit of the sequence of functions
as
$n\rightarrow \infty$
. However, as is familiar, the limit
exists for all
$\unicode[STIX]{x1D6FC}\in \mathbb{R}$
and equals the function
$h:\mathbb{R}\rightarrow [0,1]$
with
$h(\unicode[STIX]{x1D6FC})=1$
for
$|\unicode[STIX]{x1D6FC}|<\frac{1}{2}$
and
$h(\unicode[STIX]{x1D6FC})=0$
for
$|\unicode[STIX]{x1D6FC}|>\frac{1}{2}$
. Hence, the Fourier transforms of the individual summands in (22) can be computed by rescaling (26) and we find that
We apply Plancherel’s theorem, asserting that
to confirm the estimate
$$\begin{eqnarray}\displaystyle \int _{-\infty }^{\infty }|v_{q}(\unicode[STIX]{x1D6FE})|^{2}\,d\unicode[STIX]{x1D6FE} & = & \displaystyle \mathop{\sum }_{1\leqslant x,y\leqslant X/q}\frac{4}{xy}\int _{-\infty }^{\infty }h\biggl(\frac{\unicode[STIX]{x1D6FC}}{(2[Y]+1)x}\biggr)h\biggl(\frac{\unicode[STIX]{x1D6FC}}{(2[Y]+1)y}\biggr)\,d\unicode[STIX]{x1D6FC}\nonumber\\ \displaystyle & {\leqslant} & \displaystyle 8(2[Y]+1)\mathop{\sum }_{1\leqslant x\leqslant y\leqslant X/q}\frac{1}{y}\ll \frac{XY}{q}.\end{eqnarray}$$
Note that
$v_{q}$
is an empty sum unless
$q\leqslant X$
. Hence, we may sum the above over
$q\leqslant X$
and inject the result into (24). This establishes Lemma 4.
For a similar treatment of (21), we write
$w_{q}=v_{q}+(w_{q}-v_{q})$
and then use binomial expansion in conjunction with (23) to see that
holds for
$|\unicode[STIX]{x1D6FE}|\leqslant (2X)^{-1}$
and hence in particular when
$|\unicode[STIX]{x1D6FE}|\leqslant Q/(XY)$
. By (27), integration over the latter range yields
We now use the second part of (25) together with (27) to control the error introduced by completing the integral on the right to
and then infer that
We combine this with (18) and (21) to deduce that
We wish to complete the sum over
$q$
as well. By (25), (27) and (28), one finds that
$J(q)\ll (XY)^{2}q^{-2}$
and, hence,
We may add this to (29) and then add back in the contribution from the minor arcs. By (15) and (13), we then conclude as follows.
Lemma 5. Let
$\frac{3}{2}\leqslant X\leqslant Y$
. Then
3 The singular integral
In this section, we compute the singular integral (28). Progress depends on the following identity that is reported in Gradshteyn and Ryzhik [Reference Gradshteyn and Ryzhik6, 3.763, nos 1 and 4]. A straightforward proof is readily given via Cauchy’s integral formulae.
Lemma 6. For a real number
$\unicode[STIX]{x1D708}$
, let
$\Box (\unicode[STIX]{x1D708})=\unicode[STIX]{x1D708}|\unicode[STIX]{x1D708}|$
. Then, for positive real numbers
$\unicode[STIX]{x1D714}_{1},\unicode[STIX]{x1D714}_{2},\unicode[STIX]{x1D714}_{3}$
, one has
$$\begin{eqnarray}\displaystyle & & \displaystyle \int _{-\infty }^{\infty }\frac{\sin \unicode[STIX]{x1D714}_{1}t\sin \unicode[STIX]{x1D714}_{2}t\sin \unicode[STIX]{x1D714}_{3}t}{t^{3}}\,dt\nonumber\\ \displaystyle & & \displaystyle \qquad =\frac{\unicode[STIX]{x1D70B}}{8} (\,(\unicode[STIX]{x1D714}_{1}+\unicode[STIX]{x1D714}_{2}+\unicode[STIX]{x1D714}_{3})^{2}+\Box (\unicode[STIX]{x1D714}_{1}-\unicode[STIX]{x1D714}_{2}-\unicode[STIX]{x1D714}_{3})+\Box (\unicode[STIX]{x1D714}_{2}-\unicode[STIX]{x1D714}_{3}-\unicode[STIX]{x1D714}_{1})\nonumber\\ \displaystyle & & \displaystyle \qquad \quad +\,\Box (\unicode[STIX]{x1D714}_{3}-\unicode[STIX]{x1D714}_{1}-\unicode[STIX]{x1D714}_{2})).\nonumber\end{eqnarray}$$
We apply this result to (28), recalling (22). Then, using symmetry in
$x_{1},x_{2},x_{3}$
, one finds that
where
$$\begin{eqnarray}S(n)=\mathop{\sum }_{\substack{ 1\leqslant x_{i}\leqslant n \\ i=1,2,3}}\frac{(x_{1}+x_{2}+x_{3})^{2}+3\Box (x_{1}-x_{2}-x_{3})}{x_{1}x_{2}x_{3}}.\end{eqnarray}$$
Recall the function
$F$
as defined in (4).
Lemma 7. Let
$n$
be a natural number. Then
$S(n)=F(n)$
.
Proof. In (31), we isolate terms where
$\Box$
is non-negative. Then
where
$$\begin{eqnarray}\displaystyle S_{1}(n) & = & \displaystyle \displaystyle \mathop{\sum }_{\substack{ 1\leqslant x_{i}\leqslant n \\ i=1,2,3}}\frac{(x_{1}+x_{2}+x_{3})^{2}}{x_{1}x_{2}x_{3}},\nonumber\\ \displaystyle S_{2}(n) & = & \displaystyle \displaystyle \mathop{\sum }_{x_{2}+x_{3}\leqslant x_{1}\leqslant n}\frac{(x_{1}-x_{2}-x_{3})^{2}}{x_{1}x_{2}x_{3}},\nonumber\\ \displaystyle S_{3}(n) & = & \displaystyle \displaystyle \mathop{\sum }_{\substack{ 1\leqslant x_{i}\leqslant n \\ i=1,2,3}}\frac{(x_{1}-x_{2}-x_{3})^{2}}{x_{1}x_{2}x_{3}}.\nonumber\end{eqnarray}$$
The goal is now to express these sums in terms of
$A(n)$
and
$B(n)$
, as defined in (3). By symmetry in
$x_{1},x_{2},x_{3}$
, one readily confirms that
$$\begin{eqnarray}S_{1}(n)=\mathop{\sum }_{\substack{ 1\leqslant x_{i}\leqslant n \\ i=1,2,3}}\biggl(\frac{3x_{1}}{x_{2}x_{3}}+\frac{6}{x_{3}}\biggr)=\frac{3}{2}n(n+1)A(n)^{2}+6n^{2}A(n).\end{eqnarray}$$
Similarly,
$$\begin{eqnarray}S_{3}(n)=\mathop{\sum }_{\substack{ 1\leqslant x_{i}\leqslant n \\ i=1,2,3}}\biggl(\frac{3x_{1}}{x_{2}x_{3}}-\frac{2}{x_{3}}\biggr)=\frac{3}{2}n(n+1)A(n)^{2}-2n^{2}A(n).\end{eqnarray}$$
The sum
$S_{2}$
is symmetric only in
$x_{2},x_{3}$
. Hence, we only find that
We treat the four summands separately. The rightmost term is
Similarly, the penultimate term contributes
$$\begin{eqnarray}\displaystyle \mathop{\sum }_{x_{2}+x_{3}\leqslant x_{1}\leqslant n}\frac{4}{x_{3}} & = & \displaystyle \mathop{\sum }_{x_{3}\leqslant n}\frac{4}{x_{3}}\mathop{\sum }_{x_{1}=x_{3}}^{n}(x_{1}-x_{3})\nonumber\\ \displaystyle & = & \displaystyle \mathop{\sum }_{x_{3}\leqslant n}\frac{2}{x_{3}}(n-x_{3})(n-x_{3}+1)=2n(n+1)A(n)-3n^{2}-n.\nonumber\\ \displaystyle & & \displaystyle\end{eqnarray}$$
Next, one finds that
where
To evaluate
$T_{2}(n)$
, note that terms with
$x_{1}=x_{2}$
do not contribute and that the summands are invariant under
$x_{1}\leftrightarrow x_{2}$
. This shows that
$$\begin{eqnarray}T_{2}(n)=\frac{1}{2}\mathop{\sum }_{\substack{ x_{1}\leqslant n \\ x_{2}\leqslant n}}\frac{(x_{1}-x_{2})^{2}}{x_{1}x_{2}}=\mathop{\sum }_{\substack{ x_{1}\leqslant n \\ x_{2}\leqslant n}}\frac{x_{1}}{x_{2}}-n^{2}=\frac{1}{2}n(n+1)A(n)-n^{2}.\end{eqnarray}$$
One also has
$$\begin{eqnarray}\displaystyle T_{1}(n) & = & \displaystyle \mathop{\sum }_{x_{2}\leqslant x_{1}\leqslant n}\frac{1}{x_{2}}-\mathop{\sum }_{x_{2}\leqslant x_{1}\leqslant n}\frac{1}{x_{1}}\nonumber\\ \displaystyle & = & \displaystyle \mathop{\sum }_{x_{2}\leqslant n}\frac{n-x_{2}+1}{x_{2}}-n=(n+1)A(n)-2n.\nonumber\end{eqnarray}$$
It follows that
For the first summand in (35), we first sum over
$x_{1}$
to infer that
$$\begin{eqnarray}\displaystyle \mathop{\sum }_{x_{3}+x_{2}\leqslant x_{1}\leqslant n}\frac{x_{1}}{x_{2}x_{3}} & = & \displaystyle \frac{1}{2}\mathop{\sum }_{x_{2}+x_{3}\leqslant n}\frac{n(n+1)-(x_{2}+x_{3}-1)(x_{2}+x_{3})}{x_{2}x_{3}}\nonumber\\ \displaystyle & = & \displaystyle \frac{1}{2}(n(n+1)U_{0}(n)+U_{1}(n)-U_{2}(n)),\nonumber\end{eqnarray}$$
where
By symmetry,
and
$$\begin{eqnarray}\displaystyle U_{2}(n) & = & \displaystyle 2\mathop{\sum }_{x+y\leqslant n}\frac{x}{y}+n(n-1)=\mathop{\sum }_{y\leqslant n}\frac{(n-y)(n-y+1)}{y}+n(n-1)\nonumber\\ \displaystyle & = & \displaystyle n(n+1)A(n)-(2n+1)n+\frac{1}{2}n(n+1)+n(n-1)\nonumber\\ \displaystyle & = & \displaystyle n(n+1)A(n)-\frac{1}{2}n^{2}-\frac{3}{2}n.\nonumber\end{eqnarray}$$
To compute
$U_{0}(n)$
, we substitute
$z=x+y$
for
$y$
. This yields
and, by symmetry, it follows that
$$\begin{eqnarray}U_{0}(n)=\mathop{\sum }_{\substack{ x\leqslant n,z\leqslant n \\ x\neq z}}\frac{1}{xz}=A(n)^{2}-B(n).\end{eqnarray}$$
The last four identities combine to
The lemma now follows from (32), (33), (34), and (40), on recalling (4).
We are ready to deduce Theorem 1. By (30), Lemmas 7, and 5, one finds that
Note that
$(2[Y]+1)^{2}=4Y^{2}+O(Y)$
. Since
$F(n)\ll n^{2}$
holds for all
$n$
, we may indeed replace the first factor by
$4Y^{2}$
, with an error bounded by
$O(X^{2}Y)$
, and Theorem 1 follows.◻
4 A curious identity
Theorem 3 is also readily available. In the work of §§2 and 3, we temporarily take
$X=Y\in \mathbb{N}$
. Then, by (30), Lemma 7, equations (5) and (6),
Next, we derive an alternative expression for
$J(1)$
. Still restricted to the case
$X=Y\in \mathbb{N}$
, we observe symmetry in the sum (22) to infer that
with the obvious interpretation that the function
$(\sin t)/t$
takes the value
$1$
at
$t=0$
. We now apply Euler’s summation formula. When
$|\unicode[STIX]{x1D6FE}|\leqslant X^{-3/2}$
, this gives
$$\begin{eqnarray}\displaystyle v_{1}(\unicode[STIX]{x1D6FE}) & = & \displaystyle 2\int _{0}^{X}\frac{\sin \unicode[STIX]{x1D70B}(2X+1)\unicode[STIX]{x1D6FE}t}{\unicode[STIX]{x1D70B}\unicode[STIX]{x1D6FE}t}\,dt+O(X^{3/2})\nonumber\\ \displaystyle & = & \displaystyle \frac{2}{\unicode[STIX]{x1D70B}\unicode[STIX]{x1D6FE}}\operatorname{Si}(\unicode[STIX]{x1D70B}(2X+1)X\unicode[STIX]{x1D6FE})+O(X^{3/2}).\nonumber\end{eqnarray}$$
and we then insert the expansion of
$v_{1}(\unicode[STIX]{x1D6FE})$
to deduce that
$$\begin{eqnarray}\displaystyle J(1) & = & \displaystyle \frac{8}{\unicode[STIX]{x1D70B}^{3}}\int _{-X^{-3/2}}^{X^{-3/2}}(\operatorname{Si}(\unicode[STIX]{x1D70B}(2X+1)X\unicode[STIX]{x1D6FE}))^{3}\,\frac{\text{d}\unicode[STIX]{x1D6FE}}{\unicode[STIX]{x1D6FE}^{3}}+O(X^{7/2})\nonumber\\ \displaystyle & = & \displaystyle \frac{32}{\unicode[STIX]{x1D70B}}X^{4}\int _{-\infty }^{\infty }\frac{(\operatorname{Si}\unicode[STIX]{x1D6FE})^{3}}{\unicode[STIX]{x1D6FE}^{3}}\,d\unicode[STIX]{x1D6FE}+O(X^{7/2}).\end{eqnarray}$$
Since
$(\operatorname{Si}\unicode[STIX]{x1D6FE})^{3}\unicode[STIX]{x1D6FE}^{-3}$
is even, the identity (11) follows from comparing (41) with (42).
5 The hyperbola method
The transition from an asymptotic formula for
$M(X,Y)$
to one for
$N(B)$
is the theme of this and the following section. Let
$M^{\prime }(B)$
denote the number of
$\mathbf{x},\mathbf{y}\in (\mathbb{Z}\backslash \{0\})^{3}$
satisfying
$(1)$
and
$|\mathbf{x}|^{2}|\mathbf{y}|^{2}\leqslant B.$
An asymptotic formula for
$M^{\prime }(B)$
is given in (50) below. One may apply Dirichlet’s hyperbola method in its classical form to the natural numbers
$|\mathbf{x}|$
and
$|\mathbf{y}|$
. This yields
Unfortunately, in this form the method is not particularly useful, because each of the differenced terms within the sum over
$l$
will import an error of size
$B^{3/4}(\log B)^{2}$
from Theorem 1, summing up to
$B(\log B)^{2}$
, far too big for a successful estimation. To surmount this difficulty, one works with fewer terms. In [Reference Blomer and Brüdern1], we proposed a combination of linear and geometric progressions as sample points, while here we employ a quadratic sequence. Define
$L\in \mathbb{N}$
by
$(L-1)^{2}<B^{1/4}\leqslant L^{2}$
, so that
Then, one readily confirms the lower bound
where
Likewise, one finds the corresponding upper bound
We now evaluate the right-hand sides of (44) and (45) with the aid of Theorem 1. It will be convenient to write
so that we conclude from (8) and (43) that
and the same asymptotic formula holds for
$M(B^{1/4},B^{1/4})$
. Similarly, one has
By (5), the main term on the right-hand side may now be written in the form
In the first summand here, we apply (7) and then use Euler’s summation formula to find a real number
$c_{1}$
with
Hence, the first summand in (48) equals
$2\unicode[STIX]{x1D701}(2)\unicode[STIX]{x1D701}(3)^{-1}cB\log B^{1/4}+c^{\prime }B+O(B^{7/8})$
for some suitable
$c^{\prime }\in \mathbb{R}$
. In the second summand in (48), we sum over all
$l$
to remove dependence on
$L$
. By (6), this introduces an error not exceeding
Collecting together, we now deduce from (47) that
holds with some suitable real number
$c^{\prime \prime }$
and then we obtain the lower bound
with some
$c^{\prime \prime \prime }\in \mathbb{R}$
. One may apply the same argument to the right-hand side of (45) and, with hardly any change in the preceding computation, this leads to an upper bound for
$M^{\prime }(B)$
in which the leading term coincides with the one in (49). Thus, we have established the asymptotic formula
6 Proof of Theorem 2
Recall that
$N_{0}(B)$
is the number of rational points of height not exceeding
$B$
on the Zariski open subset
$\mathscr{U}$
of
$\mathscr{V}$
where no projective coordinate vanishes. According to a comment preceding the statement of Theorem 2, one observes that
$4N_{0}(B)$
is the number of primitive vectors
$\mathbf{x},\mathbf{y}\in \mathbb{Z}^{3}$
counted by
$M^{\prime }(B)$
. We remove the conditions
$(x_{0};x_{1};x_{2})=(y_{0};y_{1};y_{2})=1$
by Möbius inversion to arrive at
By (50) and straightforward estimates, it follows that there is a number
$C^{\prime }$
with
By (46) and (9), the conclusion of Theorem 2 is now available.
It remains to establish (9). As above, we see that
$4(N(B)-N_{0}(B))$
equals the number of primitive vectors
$\mathbf{x},\mathbf{y}\in \mathbb{Z}^{3}$
with
$|\mathbf{x}|^{2}|\mathbf{y}|^{2}\leqslant B$
satisfying (1) and
$x_{0}x_{1}x_{2}y_{0}y_{1}y_{2}=0$
. Let
$W_{j}$
denote the number of pairs
$\mathbf{x},\mathbf{y}$
counted here, with exactly
$j$
of the integers
$x_{0},x_{1},x_{2},y_{0},y_{1},y_{2}$
zero. Since a primitive
$\mathbf{x}\in \mathbb{Z}^{3}$
is non-zero, at most two of
$x_{0},x_{1},x_{2}$
are zero. Further, if (say)
$x_{0}=x_{1}=0$
, then
$\mathbf{x}$
is primitive if and only if
$x_{2}=\pm 1$
. Thus,
$W_{4}\ll 1$
and
$W_{j}=0$
for
$j\geqslant 5$
and, hence,
For the rest of this section we put
$Z=B^{1/2}$
in the interest of readability. For a solution counted by
$W_{3}$
, one of
$\mathbf{x},\mathbf{y}$
must have two of its coordinates zero. Hence, we may suppose temporarily that
$x_{0}=x_{1}=0$
. Then, as just observed,
$x_{2}=\pm 1$
and (1) implies
$y_{2}=0$
. Because there are two choices for
$x_{2}$
and six symmetric choices for the particular role attributed to
$x_{0},x_{1},y_{2}$
, it follows that
$$\begin{eqnarray}W_{3}=12\mathop{\sum }_{\substack{ 0<|y_{0}|,|y_{1}|\leqslant Z \\ (y_{0};y_{1})=1}}1=\frac{48}{\unicode[STIX]{x1D701}(2)}Z^{2}+O(Z\log Z).\end{eqnarray}$$
Here we have used Satz 1.3.4 and the discussion following that result in Brüdern [Reference Brüdern2].
Next, consider a solution counted by
$W_{2}$
. Suppose that
$x_{0}=0$
, say. If it were the case that
$x_{1}y_{1}=0$
, then by (1) one would have
$x_{2}y_{2}=0$
and such a solution is not counted by
$W_{2}$
. We conclude that
$x_{0}=y_{0}=0$
and (1) reduces to
$x_{1}y_{1}+x_{2}y_{2}=0$
. But
$\mathbf{x},\mathbf{y}$
are primitive and we conclude that
$(x_{1},x_{2})=\pm (y_{2},-y_{1})$
. The size constraint
$|\mathbf{x}||\mathbf{y}|\leqslant Z$
implies
$x_{1}^{2}\leqslant Z$
and
$x_{2}^{2}\leqslant Z$
and, observing symmetry, it follows that
$W_{2}\ll Z$
.
This leaves us with the estimation of
$W_{1}$
. By symmetry,
$W_{1}=6W_{1}^{\prime }$
, where
$W_{1}^{\prime }$
is the number of solutions counted by
$W_{1}$
with
$x_{0}=0$
. Hence,
$W_{1}^{\prime }$
is the number of integers
$x_{1},x_{2},y_{0},y_{1},y_{2}$
, all non-zero, with
$x_{1}y_{1}+x_{2}y_{2}=0$
and
For any tuple counted here, we have
$x_{1}\mid y_{2}$
and
$x_{2}\mid y_{1}$
. Hence, we may write
$y_{2}=ux_{1}$
and
$y_{1}=-ux_{2}$
, with some non-zero integer
$u$
, and it follows that
$W_{1}^{\prime }$
is the number of non-zero integers
$x_{1},x_{2},u$
and
$y=y_{0}$
with
Thus,
$W_{1}^{\prime }=16W_{1}^{\prime \prime }$
, where
$W_{1}^{\prime \prime }$
is number of positive
$x_{1},x_{2},u,y$
counted by
$W_{1}^{\prime }$
.
Note that
$(x_{1};x_{2})=1$
and
$x_{1}=x_{2}>0$
imply that
$x_{1}=x_{2}=1$
. Let
$W_{1}^{+}$
denote the number of tuples counted by
$W_{1}^{\prime \prime }$
, where
$x_{1}<x_{2}$
, and let
$W_{1}^{0}$
denote the number of such tuples with
$x_{1}=x_{2}=1$
. Then, by symmetry in
$x_{1}$
and
$x_{2}$
, we have
$W_{1}^{\prime \prime }=W_{1}^{0}+2W_{1}^{+}$
. Moreover, as in the treatment of
$W_{3}$
, we see that
$$\begin{eqnarray}W_{1}^{0}=\mathop{\sum }_{\substack{ 1\leqslant u,y\leqslant Z \\ (u;y)=1}}1=\frac{1}{\unicode[STIX]{x1D701}(2)}Z^{2}+O(Z\log Z).\end{eqnarray}$$
For the evaluation of
$W_{1}^{+}$
, note that for a given
$x=x_{2}$
, there are
$\unicode[STIX]{x1D711}(x)$
choices for
$x_{1}$
. Further, the conditions on the natural number
$y$
read
$y\leqslant Z/x$
and
$(y;u)=1$
. As is well known, there are
$(Z/x)(\unicode[STIX]{x1D711}(u)/u)+O(d(u))$
such
$y$
; here
$d(u)$
is the number of divisors of
$u$
. We now see that
$W_{1}^{+}$
equals
$$\begin{eqnarray}\displaystyle & & \displaystyle \mathop{\sum }_{\substack{ ux^{2}\leqslant Z \\ x\geqslant 2}}\unicode[STIX]{x1D711}(x)\biggl(\frac{Z\unicode[STIX]{x1D711}(u)}{xu}+O(d(u))\biggr)\nonumber\\ \displaystyle & & \displaystyle \quad =Z\mathop{\sum }_{2\leqslant x\leqslant \sqrt{Z}}\frac{\unicode[STIX]{x1D711}(x)}{x}\mathop{\sum }_{u\leqslant Z/x^{2}}\frac{\unicode[STIX]{x1D711}(u)}{u}+O(Z(\log Z)^{2}).\nonumber\end{eqnarray}$$
The remaining sums are routinely computed via [Reference Brüdern2, Satz 1.3.4] and partial summation and one then has
$$\begin{eqnarray}\displaystyle W_{1}^{+} & = & \displaystyle \frac{Z^{2}}{\unicode[STIX]{x1D701}(2)}\mathop{\sum }_{x=2}^{\infty }\frac{\unicode[STIX]{x1D711}(x)}{x^{3}}+O(Z^{3/2}(\log Z)^{2})\nonumber\\ \displaystyle & = & \displaystyle Z^{2}\biggl(\frac{1}{\unicode[STIX]{x1D701}(3)}-\frac{1}{\unicode[STIX]{x1D701}(2)}\biggr)+O(Z^{3/2}(\log Z)^{2}).\nonumber\end{eqnarray}$$
Collecting together, we first find that
and then insert our findings on
$W_{j}$
in (51) to confirm (9).