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A Novel Generalization of the Liouville Function λ(n)\lambda(n) and a Convergence Result for the Associated Dirichlet Series

\fnmSky Pelletier \surWaterpeace 0000-0002-2231-0160 \orgnameRowan University, \orgaddress\cityGlassboro, \stateNJ, \postcode08028, \countryUSA \orgnameSouthern New Hampshire University, \orgaddress\cityManchester, \stateNH, \postcode03106, \countryUSAfootnotetext: Statements and Declarations This research did not receive any specific grant from funding agencies in the public, commercial, or not-for-profit sectors and there are no interests to declare. Affiliation information is for contact purposes only and does not imply any support or affiliation with this work. [email protected] [email protected]
Abstract

We introduce a novel arithmetic function w(n)w(n), a generalization of the Liouville function λ(n)\lambda(n), as the coefficients of a Dirichlet series, and as a special case of a parametrized family of functions wm(n)w_{m}(n). We prove some useful special properties of these arithmetic functions and then focus on convergence of their Dirichlet series. In particular, we show that each function wm(n)w_{m}(n) injectively maps \mathbb{N} into a dense subset of the unit circle in \mathbb{C} and that Fm(s)=nwm(n)nsF_{m}(s)=\sum_{n}\frac{w_{m}(n)}{n^{s}} converges for all ss with (s)(12,1)\Re(s)\in\left(\frac{1}{2},1\right). Finally, we show that the family of functions wm(n)w_{m}(n) converges to λ(n)\lambda(n) and that Fm(s)F_{m}(s) converges uniformly in mm to nλ(n)ns\sum_{n}\frac{\lambda(n)}{n^{s}}, implying convergence of that series in the same region and thereby proving a particularly interesting property about a closely related function.

keywords:
Liouville function, Dirichlet series, Riemann Hypothesis
pacs:
[

MSC Classification]11M26, 11M06

1 Introduction

Definition of F(s)F(s) and w(n)w(n)

We define an arithmetic function w(n)w(n) as the coefficients of the Dirichlet series given by

F(s)=n=1w(n)ns:=p,prime(1eiψ(p)ps+eiψ(p2)p2seiψ(p3)p3s+)F(s)=\sum_{n=1}^{\infty}\frac{w(n)}{n^{s}}:=\prod_{p,\ \mathrm{prime}}\left(1-\frac{e^{i\psi(p)}}{p^{s}}+\frac{e^{i\psi(p^{2})}}{p^{2s}}-\frac{e^{i\psi(p^{3})}}{p^{3s}}+\cdots\right) (1)

where ψ(pk)\psi(p^{k}) is given by

ψ(pk):=πp2G(1(p1p)k)\psi(p^{k}):=\frac{\pi}{p^{2}G}\left(1-\left(\frac{p-1}{p}\right)^{k}\right) (2)

in which we are letting G=pp2G=\sum_{p}p^{-2} be the sum of the reciprocals of the primes squared. We note that F(s)F(s) is a kind of Euler product defining each w(n)w(n) based on the prime factorization of nn.

Lemma 1.

w(n)w(n) has the following properties:

  1. 1.

    w(n)w(n) is multiplicative: w(ab)w(ab) = w(a)w(b)w(a)w(b) for any coprime a,ba,b\in\mathbb{N}

  2. 2.

    w:Cw:\mathbb{N}\to C is injective, where C={z||z|=1}C=\{z\in\mathbb{C}\ \big{|}\ |z|=1\}, the unit circle in \mathbb{C}.

  3. 3.

    arg(w(n))[0,π)\arg(w(n))\in[0,\pi) for λ(n)=1\lambda(n)=1 and arg(w(n))(π,2π)\arg(w(n))\in(\pi,2\pi) for λ(n)=1\lambda(n)=-1, where λ(n)\lambda(n) is the Liouville function.

Proof.

Properties 1 and 2 follow directly from the arithmetic of fractions with coprime denominators. We therefore begin by proving Property 3.

Observe that if the prime factorization of nn is given by n=p1k1p2k2pJkJn=p_{1}^{k_{1}}p_{2}^{k_{2}}\cdots p_{J}^{k_{J}}, then w(n)=eiθ(n)w(n)=e^{i\theta(n)} where

θ(n)=arg(w(n))=π2(1λ(n))+j=1Jψ(pjkj).\theta(n)=\arg(w(n))=\frac{\pi}{2}\left(1-\lambda(n)\right)+\sum_{j=1}^{J}\psi\bigl{(}p_{j}^{k_{j}}\bigr{)}. (3)

From the definition of w(n)w(n) in (1) it is clear how the sum in (3) results from each prime factor pjkjp_{j}^{k_{j}} of nn contributing a factor of exp(iψ(pjkj))\exp\bigl{(}i\psi\bigl{(}p_{j}^{k_{j}}\bigr{)}\bigr{)} to w(n)w(n), and likewise the term π2(1λ(n))\frac{\pi}{2}\left(1-\lambda(n)\right) results from the alternating signs in the series in (1), whereby each prime factor of nn contributes a factor of 1=eiπ-1=e^{i\pi} to w(n)w(n), thereby shifting θ(n)\theta(n) by π\pi. Next, observe that ψ(pk)\psi(p^{k}) is the kthk^{\mathrm{th}} partial sum of the geometric series with a=πp3Ga=\frac{\pi}{p^{3}G} and r=p1pr=\frac{p-1}{p}. Therefore, limkψ(pk)=πp2G\lim_{k\to\infty}\psi(p^{k})=\frac{\pi}{p^{2}G}, and so p(limkψ(pk))=π\sum_{p}\left(\lim_{k\to\infty}\psi(p^{k})\right)=\pi, since we defined GG to be the sum of the reciprocals of the primes squared.

Imagine a hypothetical number nn whose prime factorization contains all prime numbers in infinite multiplicity. Then for all pjkjp_{j}^{k_{j}} in its prime factorization, kjk_{j}\to\infty for each jj\in\mathbb{N}. So the value of j=1ψ(pjkj)\sum_{j=1}^{\infty}\psi\bigl{(}p_{j}^{k_{j}}\bigr{)} in the argument of w(n)w(n) for such a theoretical nn would be π\pi, and for any actual nn\in\mathbb{N} the sum would be less than π\pi. Therefore, if nn has an even number of prime factors, the argument of w(n)w(n) would be in [0,π)[0,\pi) (zero being the argument of w(1)w(1)), and since if nn has an odd number of prime factors we introduce an extra factor 1-1, having the effect of adding π\pi to arg(w(n))\arg(w(n)), in that case arg(w(n))(π,2π)\arg(w(n))\in(\pi,2\pi). This proves Property 3. ∎

Lemma 2 (Density Lemma).

The set of coefficients {w(n)}\{w(n)\} for nn\in\mathbb{N} is dense in CC, the unit circle in \mathbb{C}.

Proof.

We saw above that w(n)=eiθ(n)w(n)=e^{i\theta(n)} where

θ(n)=π2(1λ(n))+p|nπp2G(1(p1p)kp),\theta(n)=\frac{\pi}{2}\left(1-\lambda(n)\right)+\sum_{p|n}\frac{\pi}{p^{2}G}\left(1-\left(\frac{p-1}{p}\right)^{k_{p}}\right), (4)

with G=p1p2G=\sum_{p}\frac{1}{p^{2}} and where kpk_{p} is the multiplicity of the prime factor p|np|n. Thus, to show {w(n)}\{w(n)\} dense in CC, we will show {θ(n)}\{\theta(n)\} dense in (0,2π)(0,2\pi).

To begin, let x(0,π)x\in(0,\pi) and choose ϵ>0\epsilon>0. We will show there exists an infinite sequence {nk}\{n_{k}\} such that θ(nk)\theta(n_{k}) is within an ϵ\epsilon-radius of xx for all sufficiently large kk. We will construct {nk}\{n_{k}\} by identifying prime factors to use to build θ(nk)\theta(n_{k}) to be in the proper interval when kk is sufficiently large. We will accomplish this essentially by identifying terms of πGp1p2\frac{\pi}{G}\sum_{p}^{\infty}\frac{1}{p^{2}} which will yield a sum in the ϵ\epsilon-neighborhood of xx.

First, let x0=xx_{0}=x and choose b0b_{0} as large as possible such that

B0=πGj=b01pj2>x0ϵ.B_{0}=\frac{\pi}{G}\sum_{j=b_{0}}^{\infty}\frac{1}{p_{j}^{2}}>x_{0}-\epsilon. (5)

Next, if B0>x0+ϵB_{0}>x_{0}+\epsilon, choose t0t_{0} as large as possible such that

T0=πGj=t0+11pj2>B0(x0+ϵ)T_{0}=\frac{\pi}{G}\sum_{j=t_{0}+1}^{\infty}\frac{1}{p_{j}^{2}}>B_{0}-(x_{0}+\epsilon) (6)

(If we have that B0x0+ϵB_{0}\leq x_{0}+\epsilon, instead choose t0t_{0} sufficiently large so that T0T_{0} is small enough for |x0(B0T0)|<ϵ\left|x_{0}-\left(B_{0}-T_{0}\right)\right|<\epsilon). Clearly t0+1b0t_{0}+1\geq b_{0}, since B0>B0(x0+ϵ)B_{0}>B_{0}-(x_{0}+\epsilon) and t0t_{0} is chosen to be the largest such that (6) holds. If t0+1>b0t_{0}+1>b_{0} then let S0=B0T0=πGj=b0t01pj2S_{0}=B_{0}-T_{0}=\frac{\pi}{G}\sum_{j=b_{0}}^{t_{0}}\frac{1}{p_{j}^{2}}. Otherwise, if t0+1=b0t_{0}+1=b_{0}, then by the choice of t0t_{0} it follows that

πGj=t0+21pj2B0(x0+ϵ)=(πGj=b01pj2)(x0+ϵ),\frac{\pi}{G}\sum_{j=t_{0}+2}^{\infty}\frac{1}{p_{j}^{2}}\leq B_{0}-(x_{0}+\epsilon)=\left(\frac{\pi}{G}\sum_{j=b_{0}}^{\infty}\frac{1}{p_{j}^{2}}\right)-(x_{0}+\epsilon), (7)

and so since t0+1=b0t_{0}+1=b_{0} we have

x0+ϵ+πGj=t0+21pj2πGj=t0+11pj2,x_{0}+\epsilon+\frac{\pi}{G}\sum_{j=t_{0}+2}^{\infty}\frac{1}{p_{j}^{2}}\leq\frac{\pi}{G}\sum_{j=t_{0}+1}^{\infty}\frac{1}{p_{j}^{2}}, (8)

and therefore x0+ϵπG1pj2x_{0}+\epsilon\leq\frac{\pi}{G}\frac{1}{p_{j}^{2}} for j=t0+1=b0j=t_{0}+1=b_{0}. In this case, let p=pjp=p_{j} and choose k0k_{0} the largest such that ψ(pk0)x0\psi(p^{k_{0}})\leq x_{0}, and let S0=ψ(pk0)S_{0}=\psi(p^{k_{0}}). Note that this choice of k0k_{0} is always possible: if KK is the set of all kk\in\mathbb{N} such that ψ(pk)x0\psi(p^{k})\leq x_{0}, then KK is finite, since otherwise limkψ(pk)=πG1pj2x0\lim_{k\to\infty}\psi(p^{k})=\frac{\pi}{G}\frac{1}{p_{j}^{2}}\leq x_{0}, but this is a contradiction since we had that x0+ϵπG1pj2x_{0}+\epsilon\leq\frac{\pi}{G}\frac{1}{p_{j}^{2}}. It remains to be seen that KK is nonempty, so assume to get a contradiction that

x0<ψ(p1)=πp2G(1p1p)=πp3G,x_{0}<\psi(p^{1})=\frac{\pi}{p^{2}G}\left(1-\frac{p-1}{p}\right)=\frac{\pi}{p^{3}G}, (9)

but since b0b_{0} was chosen to be the largest such that πGj=b01pj2>x0ϵ\frac{\pi}{G}\sum_{j=b_{0}}^{\infty}\frac{1}{p_{j}^{2}}>x_{0}-\epsilon, therefore

πGj=b0+11pj2x0ϵ,\frac{\pi}{G}\sum_{j=b_{0}+1}^{\infty}\frac{1}{p_{j}^{2}}\leq x_{0}-\epsilon, (10)

and if we let qq be the next prime after pp, so q=pb0+1q=p_{b_{0}+1}, then we have in particular that πG1q2<x0ϵ\frac{\pi}{G}\frac{1}{q^{2}}<x_{0}-\epsilon. However, for any successive primes p,qp,q, from Bertrand’s Postulate we have that q<2pq<2p, or equivalently, 1p<2q\frac{1}{p}<\frac{2}{q}, and so it follows that

πGqq3=πG1q2<x0ϵ<x0<πG1p3<πG8q3,\frac{\pi}{G}\frac{q}{q^{3}}=\frac{\pi}{G}\frac{1}{q^{2}}<x_{0}-\epsilon<x_{0}<\frac{\pi}{G}\frac{1}{p^{3}}<\frac{\pi}{G}\frac{8}{q^{3}}, (11)

which is a contradiction unless q<8q<8. However, if q<8q<8 then p{2,3,5}p\in\{2,3,5\}, in which case we know numerically that

ψ(p1)=πp3G<πGj=b0+11pj2,\psi(p^{1})=\frac{\pi}{p^{3}G}<\frac{\pi}{G}\sum_{j=b_{0}+1}^{\infty}\frac{1}{p_{j}^{2}}, (12)

and the sum on the right is less than or equal to x0ϵx_{0}-\epsilon by our choice of b0b_{0}. This contradicts our assumption that x0<ψ(p1)x_{0}<\psi(p^{1}). Hence that assumption is false; KK is nonempty, and there exists some maximum k0k_{0} such that ψ(pk0)x0\psi(p^{k_{0}})\leq x_{0}.

We have now that S0=B0T0S_{0}=B_{0}-T_{0} or S0=ψ(pk0)S_{0}=\psi(p^{k_{0}}), and in either case S0S_{0} has been constructed such that S0<x+ϵS_{0}<x+\epsilon. Finally, let ϵ0=|xS0|\epsilon_{0}=\left|x-S_{0}\right|, and if ϵ0<ϵ\epsilon_{0}<\epsilon, then we have obtained a sum which is within an ϵ\epsilon-radius of xx, but if ϵ0ϵ\epsilon_{0}\geq\epsilon, it follows that S0<xϵS_{0}<x-\epsilon. In that case repeat the process above, this time letting x1=ϵ0x_{1}=\epsilon_{0}, choosing the maximum possible b1b_{1} and t1t_{1} to form B1>x1ϵB_{1}>x_{1}-\epsilon and T1>B1(x1+ϵ)T_{1}>B_{1}-(x_{1}+\epsilon) as in (5) and (6), and letting S1=S0+(B1T1)S_{1}=S_{0}+(B_{1}-T_{1}), or if B1=T1B_{1}=T_{1} letting S1=S0+ψ(pk1)S_{1}=S_{0}+\psi(p^{k_{1}}) for p=pb1p=p_{b_{1}} and k1k_{1} maximum such that ψ(pk1)x1\psi(p^{k_{1}})\leq x_{1}. Let ϵ1=|xS1|\epsilon_{1}=\left|x-S_{1}\right|, and note that we have either T1>B1(x1+ϵ)T_{1}>B_{1}-(x_{1}+\epsilon), from which it follows that (B1T1)<x1+ϵ\left(B_{1}-T_{1}\right)<x_{1}+\epsilon, or else we have ψ(pk1)x1\psi(p^{k_{1}})\leq x_{1}, and in either case we have S1<x+ϵS_{1}<x+\epsilon; furthermore, note that ϵ1<ϵ0\epsilon_{1}<\epsilon_{0}.

Continue until we have ϵk<ϵ\epsilon_{k}<\epsilon for some kk. This is possible since given a sum SmS_{m} and ϵm=|xSm|\epsilon_{m}=\left|x-S_{m}\right| with ϵmϵ\epsilon_{m}\geq\epsilon, we can always find a tail of πGp1p2\frac{\pi}{G}\sum_{p}\frac{1}{p^{2}} using only primes larger than were used to form SmS_{m} and which when added to SmS_{m} takes us greater than xϵx-\epsilon, and we have already shown a method for cutting off the tail in the event that it takes us greater than x+ϵx+\epsilon; this process reduces ϵm\epsilon_{m} and the process terminates when we have ϵk<ϵ\epsilon_{k}<\epsilon for some kk, yielding SkS_{k}, a sum in the range (xϵ,x+ϵ)\left(x-\epsilon,x+\epsilon\right).

Recall that we are in the process of identifying primes to use to form {nk}\{n_{k}\}, so at each iteration of this process we must necessarily identify primes which have not yet been used. To see that we can always find a sufficiently large tail of the series which does not use any primes already used, assume we have obtained a sum SmS_{m} and ϵm=xSm\epsilon_{m}=x-S_{m} as described above, with ϵmϵ\epsilon_{m}\geq\epsilon, and for notational convenience let n=m+1n=m+1. Let bnb_{n} be maximum such that

Bn=πGj=bn1pj2>xnϵB_{n}=\frac{\pi}{G}\sum_{j=b_{n}}^{\infty}\frac{1}{p_{j}^{2}}>x_{n}-\epsilon (13)

(following the same method as before, having at this stage replaced xx with xn=ϵmx_{n}=\epsilon_{m}, the distance from SmS_{m} to xx). We must consider two cases: the first case in which the last term added to form SmS_{m} was (BmTm)(B_{m}-T_{m}), in which we need to show that bn>tmb_{n}>t_{m}, and the second case in which the last term added was ψ(pkm)\psi(p^{k_{m}}) for p=pbmp=p_{b_{m}} and appropriate choice of kmk_{m}

In the first case, note that if the term containing ptm+1p_{t_{m}+1} were included in BmTmB_{m}-T_{m}, then we would have BmTm>xm+ϵB_{m}-T_{m}>x_{m}+\epsilon, by choice of tmt_{m} as in (6). Therefore, if we let bn=tm+1b_{n}=t_{m}+1, then we would have already Bn>xnϵB_{n}>x_{n}-\epsilon. Hence, since bnb_{n} is the maximum which allows BnB_{n} to fulfill this condition, we have that bn>tmb_{n}>t_{m}.

Now in the second case, in which Sm=Sm1+ψ(pkm)S_{m}=S_{m-1}+\psi(p^{k_{m}}) where p=pbmp=p_{b_{m}}, since kmk_{m} was chosen as the maximum such that ψ(pkm)xm\psi(p^{k_{m}})\leq x_{m} (or equivalently, such that Sm=Sm1+ψ(pkm)xS_{m}=S_{m-1}+\psi(p^{k_{m}})\leq x), and since we must have SmxϵS_{m}\leq x-\epsilon or else we would not need to continue, then the difference ψ(pkm+1)ψ(pkm)>xnϵ\psi(p^{k_{m}+1})-\psi(p^{k_{m}})>x_{n}-\epsilon (since the distance from our current SmS_{m} to xx is exactly ϵm=xn\epsilon_{m}=x_{n}). Hence it suffices to show there exists a BnB_{n} greater than this difference, but note that ψ(pkm+1)ψ(pkm)\psi(p^{k_{m}+1})-\psi(p^{k_{m}}) is the difference between successive partial sums of a convergent geometric series, and so we have that ψ(pkm+1)ψ(pkm)ψ(p2)ψ(p)<ψ(p2)\psi(p^{k_{m}+1})-\psi(p^{k_{m}})\leq\psi(p^{2})-\psi(p)<\psi(p^{2}). Finally, since

ψ(p2)=πp2G(1(p1p)2)=πp2G(2p1p2)<2πp3G,\psi(p^{2})=\frac{\pi}{p^{2}G}\left(1-\left(\frac{p-1}{p}\right)^{2}\right)=\frac{\pi}{p^{2}G}\left(\frac{2}{p}-\frac{1}{p^{2}}\right)<\frac{2\pi}{p^{3}G}, (14)

we see that if we can find a BnB_{n} larger than 2πp3G\frac{2\pi}{p^{3}G} we are done. In fact, if we let qq be the next prime after pp, so q=pbm+1q=p_{b_{m}+1}, then since q<2pq<2p implies 2q2<8p22q^{2}<8p^{2}, which implies

2π8p2G<πq2G,\frac{2\pi}{8p^{2}G}<\frac{\pi}{q^{2}G}, (15)

we have that if p>8p>8 it follows that

2πp3G<2π8p2G<πq2G,\frac{2\pi}{p^{3}G}<\frac{2\pi}{8p^{2}G}<\frac{\pi}{q^{2}G}, (16)

and so ψ(p2)<πq2G<Bn\psi(p^{2})<\frac{\pi}{q^{2}G}<B_{n}, letting

Bn=πGj=bm+11pj2.B_{n}=\frac{\pi}{G}\sum_{j=b_{m}+1}^{\infty}\frac{1}{p_{j}^{2}}. (17)

On the other hand if p<8p<8 it is easily verifiable numerically that ψ(p2)<Bn\psi(p^{2})<B_{n} with BnB_{n} as defined in (17).

We have that, in either case, the algorithm producing a value SmS_{m} with ϵmϵ\epsilon_{m}\geq\epsilon will always continue with a Bn>xnϵB_{n}>x_{n}-\epsilon, with appropriate choice of TnT_{n} or ψ(pkn)\psi(p^{k_{n}}) (with none of the terms of BnB_{n} using primes used to form SmS_{m}), providing Sn<x+ϵS_{n}<x+\epsilon, with Sn>SmS_{n}>S_{m}. Note the SkS_{k} are increasing and bounded above by x+ϵx+\epsilon, and the algorithm continues until we have that ϵk=|xSk|<ϵ\epsilon_{k}=\left|x-S_{k}\right|<\epsilon for some kk.

Suppose however that the algorithm fails to terminate because the above criterion is never met. In that case, suppose to get a contradiction that there exists some δ>0\delta>0 so that ϵkϵ+δ\epsilon_{k}\geq\epsilon+\delta for all kk; that is, the algorithm continues, with each successive SkS_{k} increasing, but never getting closer than δ\delta to the interval (xϵ,x+ϵ)\left(x-\epsilon,x+\epsilon\right). However, note that for any given Sn=Sm+(BnTn)S_{n}=S_{m}+(B_{n}-T_{n}), the term Bn>δB_{n}>\delta by the argument above. Meanwhile, recall that if the term containing ptn+1p_{t_{n}+1} were included in BnTnB_{n}-T_{n}, then we would have BnTn>xn+ϵB_{n}-T_{n}>x_{n}+\epsilon, by choice of tnt_{n} as in (6). Hence, if we let p=ptn+1p=p_{t_{n}+1} we must have that the term πp2G>δ\frac{\pi}{p^{2}G}>\delta, and that inequality must hold at every iteration of the algorithm. This is a contradiction since πp2G<δ\frac{\pi}{p^{2}G}<\delta for sufficiently large pp. A similar argument shows that as the algorithm continues, eventually the first term of BnB_{n} will itself be less than δ\delta, so that the choice of tnt_{n} will no longer require the special case involving ψ(pkn)\psi(p^{k_{n}}). Hence, no such δ\delta exists, and the algorithm will eventually terminate with some Sk(xϵ,x+ϵ)S_{k}\in\left(x-\epsilon,x+\epsilon\right), as desired.

Now, let II index the primes used in all the sums of the form πGj=bt1pj2\frac{\pi}{G}\sum_{j=b}^{t}\frac{1}{p_{j}^{2}} and JJ index the primes and multiplicities used in the form ψ(pk)\psi(p^{k}). Let n=jIpjn=\prod_{j\in I}p_{j} and let m=jJpjkjm=\prod_{j\in J}p_{j}^{k_{j}}. (If II is empty, instead let II index a sufficiently large prime pp so that πp2G+Sk\frac{\pi}{p^{2}G}+S_{k} is still within ϵ\epsilon of xx, and if JJ is empty, instead let m=1m=1). Now if λ(m)=1\lambda(m)=-1 (\dagger) replace mm by pmpm for some pp indexed by II. Then for all kk\in\mathbb{N}, let nk=mn2kn_{k}=mn^{2k}, noting that λ(nk)=1\lambda(n_{k})=1, and as kk\to\infty the contribution to θ(nk)\theta(n_{k}) by the primes indexed by II will converge on πGjI1pj2\frac{\pi}{G}\sum_{j\in I}\frac{1}{p_{j}^{2}}, and so {θ(nk)}\{\theta(n_{k})\} will have infinitely many terms within the interval (xϵ,x+ϵ)\left(x-\epsilon,x+\epsilon\right), as desired. Hence, {θ(n)}\{\theta(n)\} is dense in (0,π)(0,\pi).

A similar argument, adjusting line ()(\dagger) appropriately, shows there exists an infinite sequence of integers {nk}\{n_{k}\}, with each nkn_{k} having λ(nk)=1\lambda(n_{k})=-1, which sequence {θ(nk)}\{\theta(n_{k})\} converges to any x(π,2π)x\in(\pi,2\pi). Hence we have finally that {w(n)}\{w(n)\}, nn\in\mathbb{N}, is dense in the unit circle in \mathbb{C}, as desired. ∎

Lemma 3.

For any x,y(0,π),x<yx,y\in(0,\pi),x<y, let

A\displaystyle A =\displaystyle= {n|θ(n)(x,y)}\displaystyle\left\{n\in\mathbb{N}\ \big{|}\ \theta(n)\in\left(x,y\right)\right\} (18)
B\displaystyle B =\displaystyle= {n|θ(n)(x+π,y+π)},\displaystyle\left\{n\in\mathbb{N}\ \big{|}\ \theta(n)\in\left(x+\pi,y+\pi\right)\right\}, (19)

and define the natural density of a set SS in \mathbb{N} by

δ(S)=limN|{n<N|nS}|N,\delta(S)=\lim_{N\to\infty}\frac{\left|\left\{n<N\ \big{|}\ n\in S\right\}\right|}{N}, (20)

if that limit exists. Then δ(A)\delta(A) and δ(B)\delta(B) exist and are equal.

Proof.

Let x(0,π)x\in(0,\pi), and define

Ax\displaystyle A_{x} =\displaystyle= {n|θ(n)(x,π)}\displaystyle\left\{n\in\mathbb{N}\ \big{|}\ \theta(n)\in\left(x,\pi\right)\right\} (21)
Bx\displaystyle B_{x} =\displaystyle= {n|θ(n)(π+x,2π)}.\displaystyle\left\{n\in\mathbb{N}\ \big{|}\ \theta(n)\in\left(\pi+x,2\pi\right)\right\}. (22)

Now let X=AxBxX=A_{x}\cup B_{x}. XX is a subset of \mathbb{N}, and since the Density Lemma implies that XX is nonempty, it has a least element; call it d0d_{0}, and let X0=d0={d0n|n}X_{0}=d_{0}\mathbb{N}=\left\{d_{0}n\ \big{|}\ n\in\mathbb{N}\right\}. Note that δ(X0)=1d0\delta(X_{0})=\frac{1}{d_{0}}. The Prime Number Theorem implies that the natural density of nn\in\mathbb{N} for which λ(n)=1\lambda(n)=1 equals the natural density of mm\in\mathbb{N} for which λ(m)=1\lambda(m)=-1, and it follows that δ(X0Ax)=δ(X0Bx)\delta(X_{0}\cap A_{x})=\delta(X_{0}\cap B_{x}).

We have, again from the Density Lemma, that XX0X-X_{0} is not empty, so let d1d_{1} be its smallest element and define X1=d1X_{1}=d_{1}\mathbb{N} similarly to above, and note that PNT again implies δ(X1Ax)=δ(X1Bx)\delta(X_{1}\cap A_{x})=\delta(X_{1}\cap B_{x}). Let m1=lcm(d0,d1)m_{1}=\mathrm{lcm}(d_{0},d_{1}) be the least common multiple, and note that if we similarly define M1=m1M_{1}=m_{1}\mathbb{N} then we have that M1=X0X1M_{1}=X_{0}\cap X_{1} and that δ(M1Ax)=δ(M1Bx)\delta(M_{1}\cap A_{x})=\delta(M_{1}\cap B_{x}). Since natural density is additive, we have that

δ(X0Ax)\displaystyle\delta(X_{0}\cap A_{x}) =\displaystyle= δ(X0AxM1)+δ(X0AxM1c)\displaystyle\delta(X_{0}\cap A_{x}\cap M_{1})+\delta(X_{0}\cap A_{x}\cap M_{1}^{c}) (23)
δ(X1Ax)\displaystyle\delta(X_{1}\cap A_{x}) =\displaystyle= δ(X1AxM1)+δ(X1AxM1c)\displaystyle\delta(X_{1}\cap A_{x}\cap M_{1})+\delta(X_{1}\cap A_{x}\cap M_{1}^{c}) (24)

and likewise if we replace AxA_{x} with BxB_{x}. It follows that

δ((X0X1)Ax)=δ((X0X1)Bx).\delta\left(\left(X_{0}\cup X_{1}\right)\cap A_{x}\right)=\delta\left(\left(X_{0}\cup X_{1}\right)\cap B_{x}\right). (25)

Continue in this way to let d2d_{2} be the least element of X(X0X1)X-(X_{0}\cup X_{1}), letting X2=d2X_{2}=d_{2}\mathbb{N} and m2=lcm(m1,d2)m_{2}=\mathrm{lcm}(m_{1},d_{2}), concluding ultimately that for all kk

δ(kXkAx)=δ(kXkBx),\delta\left(\bigcup_{k}X_{k}\cap A_{x}\right)=\delta\left(\bigcup_{k}X_{k}\cap B_{x}\right), (26)

implying that δ(Ax)=δ(Bx)\delta(A_{x})=\delta(B_{x}). Now let y(0,π)y\in(0,\pi) with x<yx<y and define Ay,By,YA_{y},B_{y},Y similarly to above. Then if we define W=XYW=X-Y, A=AxAyA=A_{x}-A_{y}, and B=BxByB=B_{x}-B_{y}, we have that δ(WA)=δ(WB)\delta\left(W\cap A\right)=\delta\left(W\cap B\right) and so δ(A)=δ(B)\delta(A)=\delta(B) as desired. ∎

We see that the structure of w(n)w(n) as defined in (1) is quite rich. In particular, it is easy to see that w(n)w(n) has fractal structure, with the image of any subset AA of \mathbb{N} infinitely repeated in scaled pseudocopies by multiplying every aAa\in A by other natural numbers, for example by powers of 22. However, rather than investigate this rich structure specifically, we will instead turn to the question of convergence of the associated Dirichlet series.

2 Convergence

We will now demonstrate the following fact about our series F(s)F(s).

Theorem 1 (Convergence of FN(s)F_{N}(s) for (s)(12,1)\Re(s)\in\left(\frac{1}{2},1\right)).

Define

FN(s):=n=1Nw(n)ns,F_{N}(s):=\sum_{n=1}^{N}\frac{w(n)}{n^{s}}, (27)

where w(n)w(n) is as defined in (1). Then

limNFN(s)=F(s)=n=1w(n)ns\lim_{N\to\infty}F_{N}(s)=F(s)=\sum_{n=1}^{\infty}\frac{w(n)}{n^{s}} (28)

converges for all ss with (s)(12,1)\Re(s)\in\left(\frac{1}{2},1\right).

Proof.

We will take advantage of the following fact:

Proposition 1.7.7, p43 in [1] Let a(n)a(n) be a sequence, and define A(x)=nxa(n)A(x)=\sum_{n\leq x}a(n). If |A(x)|Mxα|A(x)|\leq Mx^{\alpha} for all x1x\geq 1, where α0\alpha\geq 0, then [the Dirichlet series] n=1a(n)ns\sum_{n=1}^{\infty}\frac{a(n)}{n^{s}} is convergent for all s=σ+its=\sigma+it with σ>α\sigma>\alpha.

We will show that there exists an N0N_{0} and MM such that for all N>N0N>N_{0}, |n=1Nw(n)|<MNα\big{|}\sum_{n=1}^{N}w(n)\big{|}<MN^{\alpha} for α(12,1)\alpha\in\left(\frac{1}{2},1\right). With the proposition above, this will demonstrate the convergence desired.

Fix α(12,1)\alpha\in\left(\frac{1}{2},1\right), and for each NN\in\mathbb{N} define J=NαJ=\lfloor N^{\alpha}\rfloor and K=N1αK=\lfloor N^{1-\alpha}\rfloor. Then N=JK+RNN=JK+R_{N}. (If it happens that RNJR_{N}\geq J, we instead define K=N1αK=\lceil N^{1-\alpha}\rceil, so that in either case RN<JR_{N}<J). Let ΘN={arg(w(n))[0,2π),nN}\Theta_{N}=\{\arg(w(n))\in[0,2\pi),n\leq N\} be the set of principal arguments of w(n)w(n) with nNn\leq N, and let ΘN=ΘNΘRN\Theta_{N}^{*}=\Theta_{N}-\Theta_{R_{N}} be the set after removing the arguments of w(n)w(n) for nRNn\leq R_{N}. Order the JKJK elements of ΘN\Theta_{N}^{*} such that

θ1,1<θ1,2<<θ1,K<θ2,1<<θj,k<<θJ,K.\theta_{1,1}<\theta_{1,2}<\cdots<\theta_{1,K}<\theta_{2,1}<\cdots<\theta_{j,k}<\cdots<\theta_{J,K}. (29)

Letting N=|ΘN|=JKN^{*}=\left|\Theta_{N}^{*}\right|=JK, we have

n=RN+1RN+Nw(n)=JKeiθj,k=KJeiθj,k.\sum_{n=R_{N}+1}^{R_{N}+N^{*}}w(n)=\sum^{J}\sum^{K}e^{i\theta_{j,k}}=\sum^{K}\sum^{J}e^{i\theta_{j,k}}. (30)

Therefore,

|n=RN+1RN+Nw(n)||Jeiθj,1|++|Jeiθj,K|Kmaxk|Jeiθj,k|.\begin{split}\Bigg{|}\sum_{n=R_{N}+1}^{R_{N}+N^{*}}w(n)\Bigg{|}&\leq\Bigg{|}\sum^{J}e^{i\theta_{j,1}}\Bigg{|}+\cdots+\Bigg{|}\sum^{J}e^{i\theta_{j,K}}\Bigg{|}\\ &\leq K\cdot\max_{k}\Bigg{|}\sum^{J}e^{i\theta_{j,k}}\Bigg{|}.\end{split} (31)

Let kk be the value which maximizes the expression above, and define θj=θj,k\theta_{j}=\theta_{j,k} so that |Jeiθj|=maxk|Jeiθj,k|\Big{|}\sum^{J}e^{i\theta_{j}}\Big{|}=\max_{k}\Big{|}\sum^{J}e^{i\theta_{j,k}}\Big{|}, and we have

|n=RN+1RN+Nw(n)|K|Jeiθj|=|JeiθjK|.\Bigg{|}\sum_{n=R_{N}+1}^{R_{N}+N^{*}}w(n)\Bigg{|}\leq K\Bigg{|}\sum^{J}e^{i\theta_{j}}\Bigg{|}=\Bigg{|}\sum^{J}e^{i\theta_{j}}K\Bigg{|}. (32)

Therefore,

2πJ|n=RN+1RN+Nw(n)|2πJ|JeiθjK|=|JeiθjK2πJ|.\frac{2\pi}{J}\Bigg{|}\sum_{n=R_{N}+1}^{R_{N}+N^{*}}w(n)\Bigg{|}\leq\frac{2\pi}{J}\Bigg{|}\sum^{J}e^{i\theta_{j}}K\Bigg{|}=\Bigg{|}\sum^{J}e^{i\theta_{j}}\frac{K2\pi}{J}\Bigg{|}. (33)

Consider the partition of [0,2π][0,2\pi] induced by the {θj}\{\theta_{j}\} and extend this partition to cover the interval [0,K2π][0,K2\pi] by replacing each of the θj\theta_{j} with {θj,θj+2π,θj+4π,,θj+(K1)2π}\{\theta_{j},\theta_{j}+2\pi,\theta_{j}+4\pi,\cdots,\theta_{j}+(K-1)2\pi\}. Now choose θ1\theta_{1}^{*} from among the first KK values, θ2\theta_{2}^{*} from among the next KK, and so forth, in such a way that the set {eiθj}={eiθj}\{e^{i\theta_{j}^{*}}\}=\{e^{i\theta_{j}}\}. Then we have that

|JeiθjK2πJ|=|JeiθjK2πJ|.\Bigg{|}\sum^{J}e^{i\theta_{j}}\frac{K2\pi}{J}\Bigg{|}=\Bigg{|}\sum^{J}e^{i\theta_{j}^{*}}\frac{K2\pi}{J}\Bigg{|}. (34)

This last sum is similar to a Riemann sum approximating I=0K2πeiθ𝑑θI=\int_{0}^{K2\pi}e^{i\theta}d\theta (if each θj\theta_{j}^{*} were necessarily in its associated interval of width K2πJ\frac{K2\pi}{J} we would already have a Riemann sum). We will show that the norm of the partition of [0,K2π][0,K2\pi] naturally induced by the set {θj}\{\theta_{j}^{*}\} goes to zero, making the corresponding sum a Riemann sum which converges to the indicated integral, and that in the limit the above sum converges to that Riemann sum. Specifically, we note that

N1αNα=NN2α=1N2α1,\frac{N^{1-\alpha}}{N^{\alpha}}=\frac{N}{N^{2\alpha}}=\frac{1}{N^{2\alpha-1}}, (35)

and 2α1>02\alpha-1>0 since α>12\alpha>\frac{1}{2}. Therefore, as NN\to\infty, N1αNα0\frac{N^{1-\alpha}}{N^{\alpha}}\to 0. Furthermore, since KN1α+1K\leq N^{1-\alpha}+1, K2πNα0\frac{K2\pi}{N^{\alpha}}\to 0. Also, if ΔθJ\Delta\theta_{J} is the norm of the partition naturally induced by {θj}\{\theta_{j}^{*}\} for a given J=NαJ=\lfloor N^{\alpha}\rfloor, then we have from the Density Lemma that as NN\to\infty, ΘN\Theta^{*}_{N} becomes dense, and so ΔθJ0\Delta\theta_{J}\to 0 (observing that the θj\theta_{j}^{*} were each selected from among KK as ordered in (29) above, so that as JJ\to\infty, the density of ΘN\Theta_{N}^{*} ensures that the width of the interval containing each set of KK points in (29) goes to zero. Furthermore, the JJ points θj\theta_{j}^{*} are distributed among KK subintervals of width 2π2\pi, and as NN\to\infty, we have that J/KJ/K\to\infty, so each subinterval ends up with infinitely many points θj\theta_{j}^{*}).

Taking into account Lemma 3, we have finally that

limN2πNα|n=RN+1n=RN+Nw(n)|limN|JeiθjK2πNα|limN|JeiθjK2πJ|=limN|JeiθjΔθj|=limK|0K2πeiθ𝑑θ|=0.\begin{split}\lim_{N\to\infty}\frac{2\pi}{N^{\alpha}}\Bigg{|}\sum_{n=R_{N}+1}^{n=R_{N}+N^{*}}w(n)\Bigg{|}&\leq\lim_{N\to\infty}\Bigg{|}\sum^{J}e^{i\theta_{j}^{*}}\frac{K2\pi}{N^{\alpha}}\Bigg{|}\\ &\leq\lim_{N\to\infty}\Bigg{|}\sum^{J}e^{i\theta_{j}^{*}}\frac{K2\pi}{J}\Bigg{|}\\ &=\lim_{N\to\infty}\Bigg{|}\sum^{J}e^{i\theta_{j}^{*}}\Delta\theta_{j}\Bigg{|}\\ &=\lim_{K\to\infty}\left|\int_{0}^{K2\pi}e^{i\theta}d\theta\right|\\ &=0.\end{split} (36)

The equality between lines 2 and 3 of (36) can be obtained by partitioning the interval (0,π)(0,\pi), repeating the partition for (0+kπ,π+kπ)(0+k\pi,\pi+k\pi) for kk in {0,,2K1}\{0,\ldots,2K-1\}, and breaking the sum in line 2 into a series of sums over each part, where each part is an interval on diametrically opposite sides of the unit circle. Specifically, if (x,y)(0,π)(x,y)\subset(0,\pi) is a given part, and if we let

A\displaystyle A =\displaystyle= {θ(x,y)|θθj(mod2π)}\displaystyle\left\{\theta\in(x,y)\ \big{|}\ \theta\equiv\theta_{j}^{*}\pmod{2\pi}\right\} (37)
B\displaystyle B =\displaystyle= {θ(x+π,y+π)|θθj(mod2π)},\displaystyle\left\{\theta\in(x+\pi,y+\pi)\ \big{|}\ \theta\equiv\theta_{j}^{*}\pmod{2\pi}\right\}, (38)

then by Lemma 3, the natural density of each such set of parts A,BA,B is identical; that is, δ(A)=δ(B)\delta(A)=\delta(B), so the restriction of the sum in line 2 to those θj\theta_{j}^{*} congruent to the elements of ABA\cup B converges to its respective Riemann sum, and the sum of all such restricted sums for each part (x,y)(x,y) yields line 3.

We have shown that if we remove the first RNR_{N} points from consideration, then the magnitude of the sum of the remaining NN^{*} points is O(Nα)O(N^{\alpha}) (We actually showed a stronger condition but it suffices that the sum is O(Nα)O(N^{\alpha})). We will next show that the magnitude of the sum of the first RNR_{N} points is also O(Nα)O(N^{\alpha}), in which case, by the Proposition mentioned above, the Dirichlet series F(s)F(s) converges for (s)(12,1)\Re(s)\in\left(\frac{1}{2},1\right). In fact, since RN<JNαR_{N}<J\leq N^{\alpha} for all NN, it follows that

|n=1RNw(n)|n=1RN|w(n)|=RN<Nα.\left|\sum_{n=1}^{R_{N}}w(n)\right|\leq\sum_{n=1}^{R_{N}}\left|w(n)\right|=R_{N}<N^{\alpha}. (39)

It follows that the magnitude of the sum of the first RNR_{N} points is indeed O(Nα)O(N^{\alpha}), and so with the previous result, we have that for all α(12,1)\alpha\in\left(\frac{1}{2},1\right) there exist M,N0M,N_{0} such that for all N>N0N>N_{0}

|n=1Nw(n)|M2πNα.\Bigg{|}\sum_{n=1}^{N}w(n)\Bigg{|}\leq\frac{M}{2\pi}N^{\alpha}. (40)

Therefore, by Proposition 1.1.7 from [1], referenced previously, we have thus shown the convergence of FN(s)F_{N}(s) to F(s)F(s) for all ss with (s)(12,1)\Re(s)\in\left(\frac{1}{2},1\right). This completes the proof of Theorem 1. ∎

3 Generalization of FNF_{N} to Fm,NF_{m,N}

Let us now extend our definition of FF to a parametrized family of Dirichlet series Fm,N(s)F_{m,N}(s) with coefficients wm(n)w_{m}(n) as follows:

Fm,N(s):=n=1Nwm(n)ns,F_{m,N}(s):=\sum_{n=1}^{N}\frac{w_{m}(n)}{n^{s}}, (41)

where wm(n)=eiθm(n)w_{m}(n)=e^{i\theta_{m}(n)}, and

θm(n)=π2(1λ(n))+j=1Jψm(pjkj),\theta_{m}(n)=\frac{\pi}{2}\left(1-\lambda(n)\right)+\sum_{j=1}^{J}\psi_{m}(p_{j}^{k_{j}}), (42)

where we define ψm(pk)\psi_{m}(p^{k}) to be

ψm(pk)=1mψ(pk)=πmp2G(1(p1p)k),\psi_{m}(p^{k})=\frac{1}{m}\psi(p^{k})=\frac{\pi}{mp^{2}G}\left(1-\left(\frac{p-1}{p}\right)^{k}\right), (43)

again letting n=p1k1p2k2pJkJn=p_{1}^{k_{1}}p_{2}^{k_{2}}\cdots p_{J}^{k_{J}} be the prime factorization of nn. (We note that F(s),w(n)F(s),w(n) defined earlier are thus the special cases F1(s),w1(n)F_{1}(s),w_{1}(n).)

We state first an important corollary to Lemma 2, omitting the proof, which is substantially similar to the proof of Lemma 2.

Lemma 4 (Density Lemma Redux).

Given mm\in\mathbb{N}, the arguments A={θ|θ=arg(wm(n)),n}A=\{\theta\ \big{|}\ \theta=\arg(w_{m}(n)),n\in\mathbb{N}\} for wm(n)w_{m}(n) as defined above are dense in the set Am=[0,πm)(π,π+πm)A_{m}=\left[0,\frac{\pi}{m}\right)\cup\left(\pi,\pi+\frac{\pi}{m}\right).

We now demonstrate a crucial fact about Fm,N(s)F_{m,N}(s).

Theorem 2 (Fm,N(s)F_{m,N}(s) converges uniformly in mm).

For fixed ss\in\mathbb{C} with (s)(12,1)\Re(s)\in\left(\frac{1}{2},1\right),

Fm(s):=limNFm,N(s)=limNn=1Nwm(n)ns=n=1wm(n)nsF_{m}(s):=\lim_{N\to\infty}F_{m,N}(s)=\lim_{N\to\infty}\sum_{n=1}^{N}\frac{w_{m}(n)}{n^{s}}=\sum_{n=1}^{\infty}\frac{w_{m}(n)}{n^{s}} (44)

converges uniformly in mm\in\mathbb{N}.

Proof.

The convergence of Fm,N(s)F_{m,N}(s) with m>1m>1 follows a similar argument to Theorem 1. We note first that the difference between F1,NF_{1,N} and Fm,NF_{m,N} is exactly that the coefficients w1(n)w_{1}(n) are scaled to be wm(n)w_{m}(n) with arguments in the interval [0,πm)\left[0,\frac{\pi}{m}\right) when λ(n)=1\lambda(n)=1 or (π,π+πm)\left(\pi,\pi+\frac{\pi}{m}\right) when λ(n)=1\lambda(n)=-1. Thus, proof of convergence is accomplished by replacing the integral 0K2πeiθ𝑑θ\int_{0}^{K2\pi}e^{i\theta}d\theta in (36) with 0K2πδ(θ)eiθ𝑑θ\int_{0}^{K2\pi}\delta(\theta)e^{i\theta}d\theta, where δ(θ)\delta(\theta) is an indicator function defined to be 1 when θAm\theta\in A_{m} and 0 otherwise, here letting

Am=a=0[0+2πa,πm+2πa)(π+2πa,π+πm+2πa),A_{m}=\bigcup_{a=0}^{\infty}\left[0+2\pi a,\frac{\pi}{m}+2\pi a\right)\cup\Big{(}\pi+2\pi a,\pi+\frac{\pi}{m}+2\pi a\Big{)}, (45)

so that the integrand is nonzero only on the intervals where the arguments of the wm(n)w_{m}(n) may exist. The convergence of each Fm,N(s)F_{m,N}(s) to Fm(s)F_{m}(s) for (s)(12,1)\Re(s)\in\left(\frac{1}{2},1\right) then follows from the argument set forth in Theorem 1.

It remains to be seen that this convergence is uniform in mm\in\mathbb{N}. Defining JJ and KK as in the proof of Theorem 1, we had from (36) that

limN2πNα|nΘNw1(n)|limN|j=1JeiθjK2πNα|,\lim_{N\to\infty}\frac{2\pi}{N^{\alpha}}\Bigg{|}\sum_{n\in\Theta^{*}_{N}}w_{1}(n)\Bigg{|}\leq\lim_{N\to\infty}\Bigg{|}\sum_{j=1}^{J}e^{i\theta_{j}^{*}}\frac{K2\pi}{N^{\alpha}}\Bigg{|}, (46)

and we established that the sum on the right in (46) converges to a Riemann sum which itself converges to zero. Hence, for any ϵ>0\epsilon>0, there exists N0(ϵ)N_{0}(\epsilon) such that for all N>N0(ϵ)N>N_{0}(\epsilon),

|j=1JeiθjK2πNα|<ϵ.\Bigg{|}\sum_{j=1}^{J}e^{i\theta_{j}^{*}}\frac{K2\pi}{N^{\alpha}}\Bigg{|}<\epsilon. (47)

Let N>N0N>N_{0} and consider the set ΘN\Theta_{N}^{*} of arguments of w1(n)w_{1}(n) for RN<nNR_{N}<n\leq N as before. (We note that the proof of the corresponding result for Fm,NF_{m,N} regarding the first RNR_{N} points from the latter part of the proof of Theorem 1 follows the same argument as in that proof, and so we will consider here only the convergence to zero of the magnitude of the sum of the JKJK-many points in ΘN\Theta_{N}^{*}.) For any mm\in\mathbb{N}, m>1m>1, let Ψm,N=ΘNAm\Psi_{m,N}=\Theta_{N}^{*}\cap A_{m} for AmA_{m} as defined in (45). Then if we restrict the sum in (47) to include only those θjΨm,N\theta_{j}^{*}\in\Psi_{m,N}, we have now

|θjΨm,NeiθjK2πNα|<ϵ,\Bigg{|}\sum_{\theta_{j}^{*}\in\Psi_{m,N}}e^{i\theta_{j}^{*}}\frac{K2\pi}{N^{\alpha}}\Bigg{|}<\epsilon, (48)

since this last sum, by the same argument as previously, is also a Riemann sum, which in this case converges to

0K2πδ(θ)eiθ𝑑θ=0,\int_{0}^{K2\pi}\delta(\theta)e^{i\theta}d\theta=0, (49)

with δ(θ)\delta(\theta) as defined above. That the sum in (48) will be less than ϵ\epsilon for all NN greater than the same N0(ϵ)N_{0}(\epsilon) is due to the fact that the intervals of the integral zeroed out by the indicator function δ(θ)\delta(\theta), namely where θAm\theta\notin A_{m}, would otherwise exactly cancel each other in the integral. Removing the points θjΨm,N\theta^{*}_{j}\notin\Psi_{m,N} has the effect of being a perfectly convergent Riemann sum for these intervals, so that if the total error of a given Riemann sum were ϵ=ϵm+ϵ0\epsilon=\epsilon_{m}+\epsilon_{0}, with ϵ0\epsilon_{0} being the error from the θjΨm,N\theta_{j}^{*}\notin\Psi_{m,N}, then the sum in (48) would effectively have ϵ0=0\epsilon_{0}=0 and the result follows.

Now, let the norm of the partition of Am[0,(K1)2π)A_{m}\cap\left[0,(K-1)2\pi\right) induced by θjΨm,N\theta_{j}^{*}\in\Psi_{m,N} in (48) be Δ1,N\Delta_{1,N}, and let Δm,N\Delta_{m,N} be the norm of the partition induced by the θj\theta_{j}^{*} from Fm,NF_{m,N}, noting that these are the arguments θ1(n)\theta_{1}(n) of the JJ points w1(n)w_{1}(n) from the proof of Theorem 1, scaled to be θm(n)Am\theta_{m}(n)\in A_{m}. Call this set of points Θm,N\Theta_{m,N}, and observe that Δm,N<Δ1,N\Delta_{m,N}<\Delta_{1,N}. Therefore, the partition induced by Θm,N\Theta_{m,N} is finer than the partition induced by Ψm,N\Psi_{m,N}, and since both converge to 0K2πδ(θ)eiθ𝑑θ=0\int_{0}^{K2\pi}\delta(\theta)e^{i\theta}d\theta=0, we must have that

|θjΘm,NeiθjK2πNα||θjΨm,NeiθjK2πNα|<ϵ.\Bigg{|}\sum_{\theta_{j}^{*}\in\Theta_{m,N}}e^{i\theta_{j}^{*}}\frac{K2\pi}{N^{\alpha}}\Bigg{|}\leq\Bigg{|}\sum_{\theta_{j}^{*}\in\Psi_{m,N}}e^{i\theta_{j}^{*}}\frac{K2\pi}{N^{\alpha}}\Bigg{|}<\epsilon. (50)

Note that our choice of m>1m>1 was arbitrary and that (50) holds for all N>N0N>N_{0}, where N0(ϵ)N_{0}(\epsilon) depends only on ϵ\epsilon and not on our choice of mm. Hence,

limNFm,N(s)=Fm(s)\lim_{N\to\infty}F_{m,N}(s)=F_{m}(s) (51)

converges uniformly in mm, as desired. ∎

It remains to be seen that Fm(s)F_{m}(s) converges as mm\to\infty, for which we need the following result.

Theorem 3.

Fm(s)F_{m}(s) is Cauchy.

Proof.

Fix ss\in\mathbb{C} such that (s)(12,1)\Re(s)\in\left(\frac{1}{2},1\right) and let ϵ>0\epsilon>0. We will show that there exists MM\in\mathbb{N} such that for all m,q>Mm,q>M, |Fm(s)Fq(s)|<ϵ\big{|}F_{m}(s)-F_{q}(s)\big{|}<\epsilon.

Since Fm,N(s)F_{m,N}(s) converges to Fm(s)F_{m}(s) uniformly in mm, there exists N0N_{0} such that for all N>N0N>N_{0} we have that |Fm,N(s)Fm(s)|<ϵ4\big{|}F_{m,N}(s)-F_{m}(s)\big{|}<\frac{\epsilon}{4} for all mm. In particular, for any such NN and for any m,qm,q\in\mathbb{N}, we have that

|Fm(s)Fq(s)|=|Fm(s)Fm,N(s)+Fm,N(s)Fq,N(s)+Fq,N(s)Fq(s)||Fm(s)Fm,N(s)|+|Fm,N(s)Fq,N(s)|+|Fq,N(s)Fq(s)|<ϵ4+|Fm,N(s)Fq,N(s)|+ϵ4.\begin{split}\big{|}F_{m}(s)-F_{q}(s)\big{|}&=\big{|}F_{m}(s)-F_{m,N}(s)+F_{m,N}(s)-F_{q,N}(s)+F_{q,N}(s)-F_{q}(s)\big{|}\\ &\leq\big{|}F_{m}(s)-F_{m,N}(s)\big{|}+\big{|}F_{m,N}(s)-F_{q,N}(s)\big{|}+\big{|}F_{q,N}(s)-F_{q}(s)\big{|}\\ &<\frac{\epsilon}{4}+\big{|}F_{m,N}(s)-F_{q,N}(s)\big{|}+\frac{\epsilon}{4}.\end{split} (52)

We thus seek MM\in\mathbb{N} such that for all m,q>Mm,q>M, |Fm,N(s)Fq,N(s)|<ϵ2{\big{|}F_{m,N}(s)-F_{q,N}(s)\big{|}}<\frac{\epsilon}{2}. Now, Fm,N(s):=n=1Nwm(n)nsF_{m,N}(s):=\sum_{n=1}^{N}\frac{w_{m}(n)}{n^{s}}, and likewise for Fq,N(s)F_{q,N}(s), so

|Fm,N(s)Fq,N(s)|=|n=1Nwm(n)nsn=1Nwq(n)ns|=|n=1N(wm(n)wq(n)ns)|n=1N|wm(n)wq(n)ns|.\begin{split}\big{|}F_{m,N}(s)-F_{q,N}(s)\big{|}&=\Bigg{|}\sum_{n=1}^{N}\frac{w_{m}(n)}{n^{s}}-\sum_{n=1}^{N}\frac{w_{q}(n)}{n^{s}}\Bigg{|}\\ &=\Bigg{|}\sum_{n=1}^{N}\left(\frac{w_{m}(n)-w_{q}(n)}{n^{s}}\right)\Bigg{|}\\ &\leq\sum_{n=1}^{N}\Bigg{|}\frac{w_{m}(n)-w_{q}(n)}{n^{s}}\Bigg{|}.\end{split} (53)

However, for each n1,,Nn\in 1,\ldots,N

|wm(n)wq(n)ns|=|eiθm(n)eiθq(n)ns||θm(n)θq(n)|,\Bigg{|}\frac{w_{m}(n)-w_{q}(n)}{n^{s}}\Bigg{|}=\Bigg{|}\frac{e^{i\theta_{m}(n)}-e^{i\theta_{q}(n)}}{n^{s}}\Bigg{|}\leq\big{|}\theta_{m}(n)-\theta_{q}(n)\big{|}, (54)

if we consider the principal arguments. Note that if λ(n)=1\lambda(n)=1, θm(n)[0,πm)\theta_{m}(n)\in\left[0,\frac{\pi}{m}\right), and if λ(n)=1\lambda(n)=-1, θm(n)(π,π+πm)\theta_{m}(n)\in\left(\pi,\pi+\frac{\pi}{m}\right), for all mm, and likewise for θq(n)\theta_{q}(n) for all qq. Hence, choose MM sufficiently large such that πM<ϵ2N\frac{\pi}{M}<\frac{\epsilon}{2N}. Then for all m,q>Mm,q>M and each nn, |θm(n)θq(n)|<πM<ϵ2N\big{|}\theta_{m}(n)-\theta_{q}(n)\big{|}<\frac{\pi}{M}<\frac{\epsilon}{2N}, and therefore

n=1N|wm(n)wq(n)ns|<ϵ2,\sum_{n=1}^{N}\Bigg{|}\frac{w_{m}(n)-w_{q}(n)}{n^{s}}\Bigg{|}<\frac{\epsilon}{2}, (55)

as desired. Therefore, Fm(s)F_{m}(s) is Cauchy. ∎

We are nearly complete, and for our final result we will use the following theorem.

Theorem 4 (Theorem 2.15 in [2]).

If s(n,m)s(n,m) is a double sequence such that

  1. (i)

    the iterated limit limm(limns(n,m))=a\lim_{m\to\infty}(\lim_{n\to\infty}s(n,m))=a, and

  2. (ii)

    the limit limns(n,m)\lim_{n\to\infty}s(n,m) exists uniformly in mm\in\mathbb{N}

then the double limit limn,ms(n,m)=a\lim_{n,m\to\infty}s(n,m)=a.

It follows from Theorems 2, 3, and 4 that Fm(s)F_{m}(s) converges to some function W(s)W(s). Since each wm(n)w_{m}(n) clearly converges to λ(n)\lambda(n), we have that

W(s):=limmFm(s)=limmn=1wm(n)ns=n=1(limmwm(n)ns)=n=1λ(n)ns,\begin{split}W(s):=\lim_{m\to\infty}F_{m}(s)&=\lim_{m\to\infty}\sum_{n=1}^{\infty}\frac{w_{m}(n)}{n^{s}}\\ &=\sum_{n=1}^{\infty}\left(\lim_{m\to\infty}\frac{w_{m}(n)}{n^{s}}\right)\\ &=\sum_{n=1}^{\infty}\frac{\lambda(n)}{n^{s}},\end{split} (56)

where passing the limit inside the infinite sum is justified by the uniform convergence in mm of the sums, and it follows that Fm(s)F_{m}(s) converges uniformly in mm to W(s)=n=1λ(n)nsW(s)=\sum_{n=1}^{\infty}\frac{\lambda(n)}{n^{s}}. Therefore, W(s)W(s) converges for all ss with (s)(12,1)\Re(s)\in\left(\frac{1}{2},1\right), and we have our final result:

Theorem 5 (Riemann).

Define ζ(s)\zeta(s) as the analytic continuation of the function given by

ζ(s)=n1ns\zeta(s)=\sum_{n}\frac{1}{n^{s}} (57)

for ss\in\mathbb{C} with (s)>1\Re(s)>1. Then ζ(s)0\zeta(s)\neq 0 for all ss with (s)(0,12)(12,1)\Re(s)\in\left(0,\frac{1}{2}\right)\cup\left(\frac{1}{2},1\right).

Proof.

We have from above that W(s)=n=1λ(n)nsW(s)=\sum_{n=1}^{\infty}\frac{\lambda(n)}{n^{s}}, and therefore, this series being well-known, that W(s)=ζ(2s)ζ(s)W(s)=\frac{\zeta(2s)}{\zeta(s)}. Furthermore, W(s)W(s) converges for all ss with (s)(12,1)\Re(s)\in\left(\frac{1}{2},1\right) Since ζ(2s)\zeta(2s) is known to be absolutely convergent and nonzero in this region, we see that 1ζ(s)\frac{1}{\zeta(s)} converges everywhere in the same region, and therefore we have that ζ(s)0\zeta(s)\neq 0 when (s)(12,1)\Re(s)\in\left(\frac{1}{2},1\right). The symmetry of ζ(s)\zeta(s) about the line (s)=12\Re(s)=\frac{1}{2} for ss with (s)(0,1)\Re(s)\in\left(0,1\right) being well known, the result follows. ∎

4 Acknowledgements

The author would like to thank Dr. Abdul Hassen and to especially thank Dr. Marcus Wright, both of Rowan University, for their invaluable guidance and help checking and proofreading this paper. The author thanks Drs. Barry Mazur and William Stein for their excellent expository book Prime Numbers and the Riemann Hypothesis, which inspired the present work. The author gratefully acknowledges Kevin Hughes for his insightful and clarifying questions and suggestions and for his enduring friendship. The author dedicates this work to his dear friend, the late Dr. Tom Osler.

References

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