ZEROS OF REPLICABLE FUNCTIONS BEN TOOMEY Abstract. Following the work of Asai Kaneko and Ninomiya for Faber polynomials associated

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ZEROS OF REPLICABLE FUNCTIONS
BEN TOOMEY
Abstract. Following the work of Asai, Kaneko, and Ninomiya for Faber polynomials associated
to PSL2(Z), and Bannai, Kojima, and Miezaki’s partial proof for the case of Γ
0(2), we show that
the zeros of certain modular functions associated to some low-level genus zero groups are all located
on the boundary of certain natural fundamental domains for Γ. The groups considered are Γ
0(2),
Γ
0(3), Γ0(2 k2), Γ
0(5), Γ0(6)+, Γ
0(7), Γ0(4 k2)+, Γ0(3 k3), and Γ0(10)+.
Contents
1. Introduction 1
2. Motivation and description of method 2
3. Groups 4
3.1. Fractional linear transformations 4
3.2. Groups 8
3.3. Additional groups 11
3.4. Fundamental domains 11
3.5. Replicable groups 15
4. Functions 23
4.1. Modular Surfaces 23
4.2. Modular Functions 25
4.3. Genus Zero Groups, Hauptmoduls 26
4.4. Replicable functions 27
4.5. Monstrous Moonshine 28
5. Faber Polynomials for Replicable Functions 30
5.1. Harmonics and Faber Polynomials 30
5.2. Beginning the approximation 31
5.3. Completing the approximation 34
6. Proofs of Theorem 1 40
6.1. The case Γ = Γ
0(2) 40
6.2. The case Γ = Γ0(6)+ 42
6.3. The case of Γ = Γ0(3 k3) 44
7. Appendix I: Special values of modular functions 46
References 48
1. Introduction
In 1998, Asai, Kaneko, and Ninomiya [2] located the zeros of a certain basis for the space of
weakly holomorphic modular functions for PSL2(Z), using the action of Hecke operators. A decade
later, Bannai, Kojima, and Miezaki [4] suggested that the twisted Hecke operators appearing in
Date: October 10, 2022.
2020 Mathematics Subject Classification. Primary 11F03; Secondary 11F06.
1
arXiv:2210.03668v1 [math.NT] 7 Oct 2022
2 BEN TOOMEY
the Monstrous Moonshine correspondence might be used to locate zeros of weakly holomorphic
modular functions for other groups.
Let
(1.1) S={Γ
0(2),Γ
0(3),Γ
0(5),Γ0(6)+,Γ
0(7),Γ0(4 k2)+,Γ0(3 k3),Γ0(10)+}.
These groups (see §3.2 for a description) have the important property that for each Γ ∈ S, the
associated modular surface Y(Γ) is genus zero, and has only one cusp (see §4.1). As a consequence,
the C-vector space of weakly holomorphic modular functions for Γ has a basis of the form {Fn(τ) =
qn+O(q)|n0}, where each Fn(τ) is uniquely determined. We define a particular fundamental
domain D(Γ) for each Γ ∈ S (see §3.4), and locate the zeros of this basis {Fn(τ)}in the given
fundamental domain D(Γ).
Theorem 1.1. Let Γ∈ S and let nN. Then all nzeros for the unique modular function
Fn(τ) = qn+O(q)for Γare on the lower boundary of the fundamental domain D(Γ), except for
the cases of n= 2 and Γ=Γ
0(5),Γ
0(7), where one zero is on the lower boundary and one zero is
on the side boundary of D(Γ).
We demonstrate the particular cases of Γ
0(2), Γ0(6)+, and Γ0(3 k3) below in Section 6. The
other cases are similar in nature. While there are several other genus zero groups with one cusp,
the groups in Shave the property that the functions Fn(τ) are real-valued on the lower boundary
of D(Γ), allowing us to use the intermediate value theorem to locate zeros.
Bannai, Kojima, and Miezaki [4] obtained a partial proof in the case of Γ
0(2), locating at least
n1 of the nzeros for each function Fn(τ) in the fundamental domain D
0(2)). There are some
minor errors in the write up of their proof, having to do with the bookkeeping involved with twisted
Hecke operators (their formula has the replicate function depending on n, when it instead depends
on a, where a|n). In order to avoid this bookkeeping, and the inevitable errors that would creep
in, we develop a technique to bypass this part of the proof method.
For the particular cases of Γ
0(2) and Γ
0(3), our results are previously known, due to results of
Choi and Im [6] and Hanamoto and Kuga [14], respectively. Their results cover a broader class of
modular forms, but since the methods used are sufficiently dissimilar, we still offer our own proofs
below.
2. Motivation and description of method
We briefly summarize the strategies of the prior work mentioned in Section 1, which motivate
our method. Let
Hn:= a b
0da, b, d Z, ad =n, 0b < d,
which we call the Hecke set of level n(see Def. 3.25). As noted above, Asai, Kaneko, and Ninomiya
[2] proved the result of Theorem 1.1 for the group Γ = PSL2(Z). Let
T1A(τ) = j(τ)744 = q1+ 196884q+ 21493760qq+···
where j(τ) is the classical j-invariant. To locate the zeros of Fn(τ), they first observe that the
classical Hecke operators Tnfor modular forms (see, e.g. [16]) provide the identity1
Fn(τ) = qn+O(q) = n(T1A(τ)|Tn) = X
H∈Hn
T1A(Hτ).
They also observe that when τis ‘near infinity’ — that is, has sufficiently large imaginary part
— then T1A(τ)q1, and in fact, using the non-negativity of the Fourier coefficients of T1A(τ),
they show T1A(τ)e2πiτ <1335 whenever τis in the commonly-used fundamental domain for
1The conflicting notations T1Aand Tnare unfortunately rather standard here.
ZEROS OF REPLICABLE FUNCTIONS 3
PSL2(Z), bounded below by the unit circle and to the left and right by |Re τ| ≤ 1
2. We denote this
fundamental domain by D(PSL2(Z)).
So, for each H∈ Hn, let GHPSL2(Z) be such that GHHτ ∈ D(PSL2(Z)). Then
Fn(τ)X
H∈Hn
e2πiGHHτ X
H∈HnT1A(Hτ )e2πiGHHτ
=X
H∈HnT1A(GHHτ )e2πiGHHτ
(modularity of T1A)
<1335n2,
since there are σ1(n)n2elements in Hn. The problem then becomes one of approximating the
left-hand sum above. By a consideration of cases, and restricting to τon the lower boundary of
D(PSL2(Z) (that is, to the unit circle), they show that for most H∈ Hn, one has e2πiGHHτ
eπnIm τ, but there are three exceptions. By bounding one of these three exceptional terms, the
remaining two serve as an approximation of Fn(τ). After some algebra, this gives a bound (see [2]
for details) Fn(τ)e2πnIm τ2 cos(2πnRe τ)< M n2e2πnIm τ+n2eπnIm τ+ 1 <2,
for n2 and τon the lower boundary of D(PSL2(Z)). Since Fn(τ) is real-valued on the lower
boundary, the approximation by cosine above shows Fn(τ) changes sign n+ 1 times along the unit
circle with real part in the interval [0,1
2], we deduce that Fn(τ) has nzeros on the lower boundary
of D(Γ).
Bannai, Kojima, and Miezaki [4] sought to extend this technique to families of modular func-
tions for groups other than PSL2(Z). Their key observation is that twisted Hecke operators from
Monstrous Moonshine (see §4.5 below) could replace the classical Hecke operators above. Briefly,
with twisted Hecke operators, one has a family of functions {f(a)(τ), a N}, with each f(a)a
normalized Hauptmodul for a genus zero group Γ(a)(analogous to the role of T1A(τ) and PSL2(Z)
above). Letting f(H)=f(a)for H=a b
0d∈ Hn, this family of functions satisfies the twisted Hecke
relations,
Fn(τ) = qn+O(q) = X
H∈Hn
f(H)(Hτ),
where now Fn(τ) is the unique weakly-holomorphic modular function for Γ(1) having a pole of order
nat infinity and holomorphic everywhere else. In particular, letting f(a)=T1Afor all aN, the
twisted Hecke operators include the case of PSL2(Z) above as a special case.
In Bannai, Kojima, and Miezaki [4], they consider the case of Γ(1) = Γ
0(2), where the functions
f(a)may either be T1A(τ) or T2A(τ) = q1+ 4372q+ 96256q2+. . . [8], the unique normalized
Hauptmodul for Γ
0(2), depending on the parity of a. This significantly complicates the bookkeeping,
but a consideration of cases was sufficient for them to locate n1 zeros on the lower boundary.
With some extra care in our bounding procedure, we are able to locate all nzeros.
In order to directly extend [2], we will require that Γ = Γ(1) be a group having only one cusp.
This ensures there exists a fundamental domain D(Γ) which is bounded away from the real line,
similar to D(PSL2(Z)). Somewhat surprisingly, when Γ(1) has only one cusp, then Γ(a)has one cusp
for all aN, and moreover, each normalized Hauptmodul f(a)has non-negative Fourier coefficients
(8). Taken together, this is sufficient to produce a bound
Fn(τ)X
H∈Hn
e2πiGHHτ < M n2,
4 BEN TOOMEY
for some M > 0, analogous to the case of PSL2(Z) above. Unlike for PSL2(Z), however, here
each GHΓ(H), which depends on H, so that a consideration of cases becomes significantly more
error-prone.
We avoid this brute force approach by proving some group theoretic results relating to twisted
Hecke operators in Section §3. In Section §4 we review some needed facts about modular functions
and replication. We then apply these results to approximate the modular functions Fn(τ) for groups
like those in the set Sabove, in Section §5, culminating with Theorem 5.13, which is the analogue
of the approximation produced in [2] for PSL2(Z). Finally, in Section §6, we prove a few cases
to demonstrate the method, beginning with Γ
0(2), the simplest nontrivial case involving twisted
Hecke operators. We also present the case of Γ0(6)+, which demonstrates handling a case where
the lower boundary consists of more than one arc, as well as Γ0(3 k3), where we use additional
results (§5.1) involving ‘harmonics,’ as they were dubbed in [8]. Additional cases may be found in
our upcoming thesis [19].
3. Groups
3.1. Fractional linear transformations. The material here is substantially similar to the expo-
sition given by Duncan and Frenkel [12], with some minor differences in notation.
Definition 3.1. Let
Ω := PGL+
2(Q)
={a b
c d |a, b, c, d Q, ad bc > 0}{tI|tQ r {0}},
where I= ( 1 0
0 1 ) is the identity matrix.
We also define the following notation for elements of Ω. Let x, y Qwith y > 0. Then
Tx:= ( 1x
0 1 ),[y] := y0
0 1 ,and S:= 01
1 0 .
We further define the following subgroups of Ω:
:= {a b
c d |c= 0},
T
:= {a b
0d|a=d}
={Tx|xQ},
and
D
:= a b
0d|b= 0}
={[y]|yQ, y > 0}.
That is, Ω is the group of all rational 2 ×2 matrices with positive determinant, up to scalar
equivalence. For elements of Ω, we generally choose a matrix for coset representative having
integral entries, by simultaneously scaling the entries when necessary. In particular, for p
qQ, we
often write
Tp
q=q p
0q,p
q=p0
0q,
with the latter expression in Ω only for p
q>0.
For any M=a b
c d , we may take as coset representative for M1the matrix d b
ca, having the
same determinant as the coset representative for M. Since an involution WΩ satisfies W1=W
(up to scalar multiplication), from the form of the inverse above we may deduce that involutions
are precisely the elements of the form W=a b
cafor some a, b, c Z. That is, involutions are the
trace zero elements of Ω.
Lemma 3.2. Let s, t, x, y Qwith x, y > 0. Then
ZEROS OF REPLICABLE FUNCTIONS 5
(1) TsTt=Ts+t,
(2) (Ts)t=Tst,
(3) [x] [y]=[xy], and in particular [x]1=x1,
(4) S1=S,
(5) [y]Tt=Tty [y],
(6) [y]S=S[y]1,
(7) ST tS=(It= 0
T1
t1
t2ST 1
tt6= 0.
Proof. In each case, one computes each side as matrices and compares. Note the identity (Ts)t=Tst
involves an appropriate choice of root when tQis not an integer, that is, we are implicitly defining
(Ts)1
n=Ts
nfor any nonzero nZ(one may check that this is the unique nth root of Tsin Ω).
In preparation for Theorem 3.4 below, we introduce some further notation:
Definition 3.3. For any M=a b
c d Ω, we define the following functions from Ω to P1(Q):
π(M) := d
c,
ρ2(M) := ad bc
c2,
σ(M) := (a
dM
1M /
,
θ(M) := (b
dM
a
cM /
.
We further define2ρ: Ω P1(R) by ρ(M) = pρ2(M).
We now define an important decomposition of elements of Ω.
Theorem 3.4 (Involutory Decomposition).Let M=a b
c d . Then
M=(Tθ(M)[σ(M)] M
Tθ(M)ρ2(M)ST π(M)M /.
Moreover, this factorization is unique, in that if M=Tx[y]ST z(resp. M=Tx[y]) then x=θ(M),
y=ρ2(M), and z=π(M)(resp. x=θ(M),y=σ(M)).
Proof. First, suppose M, so
M=a b
0d=1b
d
0 1 a0
0d=Tθ(M)[σ(M)] .
Moreover, if M=Tθ(M)[σ(M)] = Tx[y], then Txθ(M)=σ(M)y1, and since ΩT
D
={I}
we must have Txθ(M)=I=σ(M)y1, so x=θ(M) and y=σ(M), and the given factorization
is unique.
2We note that Duncan and Frenkel define the function %, where %(M) = ρ2(M) (not ρ(M)).
摘要:

ZEROSOFREPLICABLEFUNCTIONSBENTOOMEYAbstract.FollowingtheworkofAsai,Kaneko,andNinomiyaforFaberpolynomialsassociatedtoPSL2(Z),andBannai,Kojima,andMiezaki'spartialproofforthecaseof0(2),weshowthatthezerosofcertainmodularfunctionsassociatedtosomelow-levelgenuszerogroupsarealllocatedontheboundaryofcertai...

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