• Nem Talált Eredményt

2.8 Counting subgroups of finite abelian groups

2.8.2 Subgroups of rank three groups

Now we consider the subgroups of the groupZmˆZnˆZr, which has rank three when pm, n, rq ą 1.

Theorem 2.8.5 (Hampejs and T´oth [38, Th. 2.1]). Let m, n, r P N. The subgroups of the group Γ“ZmˆZnˆZr can be represented as follows.

(i) Choose a, b, cPN such that a|m, b|n, c|r.

(ii) Compute A:“gcdpa, n{bq, B :“gcdpb, r{cq, C :“gcdpa, r{cq.

(iii) Compute

X:“ ABC

gcdpapr{cq, ABCq. (iv) Let s :“at{A, where 0ďtďA´1.

(v) Let

v :“ bX

Bgcdpt, Xqw, where 0ďwďBgcdpt, Xq{X´1.

(vi) Find a solution u0 of the linear congruence

pr{cqu”rvs{pbcq (mod a).

(vii) Let u:“u0`az{C, where 0ďz ďC´1.

(viii) Consider

Ua,b,c,t,w,z :“ xpa,0,0q,ps, b,0q,pu, v, cqy

“ tpia`js`ku, jb`kv, kcq: 0ďiďn{a´1,0ďj ďn{b´1,0ďk ďn{c´1u.

Then Ua,b,c,t,w,z is a subgroup of order mnr{pabcq of Γ. Moreover, there is a bijection between the set of6-tuples pa, b, c, t, w, zq satisfying the conditions (i)-(viii) and the set of subgroups of Γ.

Next we give a formula for the number of subgroups of Γ.

Theorem 2.8.6 (Hampejs and T´oth [38, Th. 2.2]). For every m, n, r P N the total number of subgroups of the group ZmˆZnˆZr is given by

spm, n, rq “ ÿ

a|m, b|n, c|r

ABC

X2 PpXq, (2.47)

with the notation of Theorem 2.8.5, where Ppnq is the gcd-sum function.

If one of m, n, r is 1, then formula (2.47) reduces to (2.44).

I remark that in the joint paper with T˘arn˘auceanu [93, Cor. 2.2] we proved, based on formula (2.38), that the total number of subgroups of the rank three p-group Zpλ1 ˆ Zpλ2 ˆZpλ3, withλ1 ěλ2 ěλ3 ě1, is given by the following polynomial:

Fppq pp2´1q2pp´1q,

where

Fppq “pλ3`1qpλ1´λ2`1qpλ23`5`2pλ3`1qpλ23`4

´2pλ3`1qpλ1´λ2qpλ23`3´2pλ3`1qpλ23`2

` pλ3`1qpλ1´λ2´1qpλ23`1´ pλ12´λ3`3qp3`4

´2p3`3` pλ12´λ3 ´1qp3`2

` pλ123`5qp2 `2p´ pλ123`1q.

This formula was also obtained by Oh [72, Cor. 2.2], using different arguments.

The final result of this chapter is an asymptotic formula for the number of subgroups spn, n, nq of Z3n. The values of this function for 1 ď n ď 50, obtained by Theorem 2.8.6 and using the software Mathematica, are given in Table 1.

Table 1. Values ofspnq:“spn, n, nq for 1ďn ď50

n spnq n spnq n spnq n spnq n spnq

1 1 11 268 21 3248 31 1988 41 3448

2 16 12 3612 22 4288 32 22308 42 51968

3 28 13 368 23 1108 33 7504 43 3788

4 129 14 1856 24 22456 34 9856 44 34572

5 64 15 1792 25 2607 35 7424 45 28480

6 448 16 4387 26 5888 36 57405 46 17728

7 116 17 616 27 5776 37 2816 47 4516

8 802 18 7120 28 14964 38 12224 48 122836

9 445 19 764 29 1744 39 10304 49 9009

10 1024 20 8256 30 28672 40 51328 50 41712 Define the multiplicative function h by

spn, n, nq “ÿ

d|n

d2τpdqhpn{dq pnP Nq (2.48) and letHpzq “ř8

n“1hpnqn´z be the Dirichlet series of h.

Theorem 2.8.7 (Hampejs and T´oth [38, Th. 2.3]). For every ε ą0, ÿ

nďx

spn, n, nq “ x3

3 pHp3qplogx`2γ´1q `H1p3qq `Opx2`θ`εq, (2.49) where θ is the exponent in the Dirichlet divisor problem (1.1).

Chapter 3

Results for multiplicative functions of several variables

3.1 Counting r-tuples of positive integers with k-wise relatively prime components

Let r ě k ě 2 be fixed integers. The positive integers n1, . . . , nr are called k-wise relatively prime if anyk of them are relatively prime, that is pni1, . . . , nikq “1 for every 1ďi1 ă ¨ ¨ ¨ ăik ďr. In particular, in the case k “2 the integers are pairwise relatively prime and fork “r they are mutually relatively prime.

Let Sr,k denote the set of r-tuples of positive integers with k-wise relatively prime components and let %r,k stand for its characteristic function. What is the asymptotic density

dr,k “ lim

xÑ8

1 xr

ÿ

n1,...,nrďx

%r,kpn1, . . . , nrq

of the setSr,k? Heuristically, the probability that a positive integer is divisible by a fixed prime pis 1{p, hence the probability that given r positive integers exactly j of them are divisible by p is

ˆr j

˙1 pj

ˆ 1´ 1

p

˙r´j

and the probability that they are k-wise relatively prime is Pr,k “ź

p k´1

ÿ

j“0

ˆr j

˙1 pj

ˆ 1´ 1

p

˙r´j

. (3.1)

Note that for every rěkě2,

c ź

pąr´1

ˆ

1´pr´1q2 p2

˙

ďPr,2 ďPr,k ďPr,r “ ź

p

ˆ 1´ 1

pr

˙ ,

with some constant c ą 0 (depending on r), hence the infinite product (3.1) converges.

Some approximate values ofPr,k are shown by Table 2.

Table 2. Approximate values of Pr,k for 2ďk ďr ď8 Pr,k k“2 k “3 k “4 k“5 k “6 k “7 k “8 r “2 0.607

r “3 0.286 0.831

r “4 0.114 0.584 0.923

r “5 0.040 0.357 0.768 0.964

r “6 0.013 0.195 0.576 0.873 0.982

r “7 0.004 0.097 0.394 0.734 0.930 0.991

r “8 0.001 0.045 0.247 0.573 0.837 0.962 0.995

If k “ r, then it is well known that dr,r “ Pr,r “ 1{ζprq is the correct value of the corresponding asymptotic density. The casek“2 was treated by the author [95], proving by an inductive approach that

ÿ

n1,...,nrďx

%r,2pn1, . . . , nrq “ dr,2xr`O`

xr´1plogxqr´1˘

, (3.2)

wheredr,2 “Pr,2.

In the case k “ 2, the asymptotic density was also deduced by Cai and Bach [14, Th. 3.3] using probabilistic arguments. J. Hu [43, 44] proved that dr,k “ Pr,k for every rěkě2. In fact, by generalizing the method of [95] it was shown in [43] that

ÿ

n1,...,nrďx

%r,kpn1, . . . , nrq “Pr,kxr`O`

xr´1plogxqδr,k˘

, (3.3)

whereδr,k“max

!`r´1

j

˘: 1ďj ďk´1 )

. Fork “2 the asymptotic formula (3.3) reduces to (3.2).

Referring to our paper [95], de Reyna and Heyman [29] considered modified pair-wise coprimality conditions and by using certain graph representations they obtained asymptotic formulas similar to (3.3). Probabilistic aspects of pairwise coprimality were investigated by Fern´andez and Fern´andez [35].

It is the goal of the present Section to use a method, which differs from all approaches mentioned above and which seems to be the most natural, to establish the asymptotic formula (3.3) with a better error term. More exactly, we take into account that the function%r,kpn1, . . . , nrqis multiplicative, viewed as an arithmetic function ofr variables.

Therefore, its multiple Dirichlet series can be expressed as an Euler product and an explicit formula can be given for it. Then we use the convolution method to obtain the desired asymptotic formula by elementary arguments.

We prove the following results. Let ejpx1, . . . , xrq denote the elementary symmetric polynomials in x1, . . . , xr of degreej (j ě0).

Theorem 3.1.1 (T´oth [111, Th. 2.1]). Let r ě k ě 2 and let si P C (1ď i ď r). If

<si ą1 (1ďiďr), then

8

ÿ

n1,...,nr“1

%r,kpn1, . . . , nrq

ns11¨ ¨ ¨nsrr “ζps1q ¨ ¨ ¨ζpsrqDr,kps1, . . . , srq, where

Dr,kps1, . . . , srq “ ź

p

˜ 1´

r

ÿ

j“k

p´1qj´k

ˆj ´1 k´1

˙

ejpp´s1, . . . , p´srq

¸

is absolutely convergent if <psi1 ` ¨ ¨ ¨ `sijq ą 1 for every 1 ď i1 ă . . . ă ij ď r with kďj ďr.

Theorem 3.1.2 (T´oth [111, Th. 2.2]). If rěkě2, then ÿ

n1,...,nrďx

%r,kpn1, . . . , nrq “Ar,kxr`OpRr,kpxqq, where

Ar,k“ź

p

˜ 1´

r

ÿ

j“k

p´1qj´k ˆr

j

˙ˆj´1 k´1

˙1 pj

¸

(3.4) and

Rr,kpxq “

#xr´1, if rěk ě3,

xr´1plogxqr´1, if rěk “2. (3.5) Fork ě3 the error term Rr,kpxq is better than in (3.3), obtained by J. Hu [43]. Note also that Ar,k “ Pr,k, given by (3.1), which follows by certain properties of the binomial coefficients.

3.2 The average value of the least common multiple of k positive integers

Consider the greatest common divisor pn1, . . . , nkqof n1, . . . , nkP N. It is easy to see that for any arithmetic functionf we have the identity

ÿ

n1,...,nkďx

fppn1, . . . , nkqq “ ÿ

dďx

pµ˚fqpdq Yx

d ]k

, (3.6)

which leads to asymptotic formulas for this sum. For example, if fpnq “ n and k ě 3, then we have

ÿ

n1,...,nkďx

pn1, . . . , nkq “ ζpk´1q

ζpkq xk`OpRkpxqq,

where R3pxq “ x2logx and Rkpxq “ xk´1 for k ě 4. The case fpnq “ n, k “ 2 can be treated separately by writing

ÿ

m,nďx

pm, nq “ 2 ÿ

mďnďx

pm, nq ´ ÿ

nďx

n

“2ÿ

nďx

pµ˚idτqpnq ´ x2

2 `Opxq, giving, by using elementary arguments, the formula

ÿ

m,nďx

pm, nq “ x2 ζp2q

ˆ

logx`2γ´1

2 ´ζp2q

2 ´ ζ1p2q ζp2q

˙

`Opx1`θ`εq, (3.7) valid for everyε ą0, where γ is Euler’s constant andθ is the exponent appearing in the Dirichlet divisor problem (1.1). Here (3.7) is equivalent to formula (2.20), concerning the gcd-sum function.

For the least common multiple of k positive integers there is no formula similar to (3.6). However, in the case k “2, the lcm of the integers m, nP N can be written using their gcd as rm, ns “ mn{pm, nq, which enables to establish the following asymptotic formula, valid for anyr PN:

ÿ

m,nďx

rm, nsr “ ζpr`2q

ζp2q ¨ x2pr`1q

pr`1q2 `Opx2r`1plogxq2{3plog logxq4{3q, which is a consequence of the result (1.4) of Walfisz onř

nďxφpnq.

The above and related results go back to the work of Ces`aro [18], Cohen[22], Diaconis and Erd˝os [31], Tanigawa and Zhai [92], Ikeda and Matsuoka [47], and others.

The result

ÿ

m,n,qďx

rm, n, qsr „cr x3pr`1q

pr`1q3 pxÑ 8q,

valid for r P N, without any error term and with a computable constant cr given in an implicit form, was obtained by J. L. Fern´andez and P. Fern´andez [34, Th. 3(b)].

Their proof is by an ingenious method based on the identityrm, n, qspm, nqpm, qqpn, qq “ mnqpm, n, qq (m, n, q P N) and using the dominated convergence theorem. As far as we know, there are no other asymptotic results in the literature for the sum

ÿ

n1,...,nkďx

fprn1, . . . , nksq, (3.8)

in the casek ě3, wheref is an arithmetic function. It seems that the method of [34] can not be extended for k ě3, even in the case fpnq “nr. Also, it is not possible to reduce the estimation of the sum (3.8) to sums of a single variable, like in (3.6).

In this Section we deduce an asymptotic formula with remainder term for the sum (3.8), wherek ě2 andf belongs to a large class of multiplicative arithmetic functions.

LetrPRbe a fixed number. LetAr denote the class of complex valued multiplicative arithmetic functions satisfying the following properties: there exist real constants C1, C2 such that

|fppq ´pr| ďC1pr´1{2 for every prime p, (i)

and

|fppνq| ďC2pνr for every prime power pν with νě2. (ii) Note that conditions (i) and (ii) imply that

|fppνq| ďC3pνr for every prime power pν with νě1, (iii) whereC3 “maxpC1`1, C2q.

For example, the following functions belong to the classAr: fpnq “nr, σpnqr, φpnqr, σpeqpnqr (r P R), fpnq “ σrpnq “ ř

d|ndr (r P R with r ě 1{2). Furthermore, if f is a bounded multiplicative function such thatfppq “1 for every prime p, then f PA0. In particular, µ2 PA0.

Theorem 3.2.1 (Hilberdink and T´oth [42, Th. 2.1]). Let k ě 2 be a fixed integer and let f PAr be a function, where r ą ´1 is real. Then for every εą0,

ÿ

n1,...,nkďx

fprn1, . . . , nksq “Cf,k xkpr`1q pr`1qk `O

´

xkpr`1q´12minpr`1,1q`ε¯

, (3.9)

and

ÿ

n1,...,nkďx

fprn1, . . . , nksq

pn1¨ ¨ ¨nkqr “Cf,kxk`O

´

x12minpr`1,1q`ε¯

, (3.10)

where

Cf,k “ź

p

ˆ 1´ 1

p

˙k 8

ÿ

ν1,...,νk“0

fppmaxpν1,...,νkqq ppr`1qpν1`¨¨¨`νkq.

Formula (3.9) shows that the average order offprn1, . . . , nksqisCf,kpn1¨ ¨ ¨nkqr, in the sense that

ÿ

n1,...,nkďx

fprn1, . . . , nksq „ ÿ

n1,...,nkďx

Cf,kpn1¨ ¨ ¨nkqr pxÑ 8q. From (3.10) we deduce that

xÑ8lim 1 xk

ÿ

n1,...,nkďx

fprn1, . . . , nksq

pn1¨ ¨ ¨nkqr “Cf,k,

representing the mean value of the functionfprn1, . . . , nksq{pn1¨ ¨ ¨nkqr.

Theorem 3.2.2 (Hilberdink and T´oth [42, Th. 2.2]). Let k ě 2 be a fixed integer Note that our method does not work in the case r “ ´1, that is for the sum

Skpxq:“ ÿ

n1,...,nkďx

1 rn1, . . . , nks.

By using different arguments, we proved (unpublished) that Skpxq — plogxq2k´1 for every kě2, this sum being related to ř

nďxτpnqk{n. However, we are not able to obtain an asymptotic formula for Skpxq.

Among other special cases of the above results we consider here only the function σPA1.

Corollary 3.2.4 (Hilberdink and T´oth [42, Cor. 3]). Let k ě 2. Then for every εą0,

ÿ

n1,...,nkďx

σprn1, . . . , nksq “Cσ,kx2k 2k `O`

x2k´1{2`ε˘ , and

ÿ

n1,...,nkďx

σprn1, . . . , nksq

n1¨ ¨ ¨nk “Cσ,kxk`O`

xk´1{2`ε˘ , where

Cσ,k “ź

p

ˆ 1´ 1

p

˙k 8

ÿ

ν1,...,νk“0

σppmaxpν1,...,νkqq p2pν1`¨¨¨`νkq . In particular,

Cσ,2 “ζp3qζp4qź

p

ˆ 1` 1

p2 ´ 2 p3 ´ 2

p5 ` 2 p6

˙ .