Divisor function explained

In mathematics, and specifically in number theory, a divisor function is an arithmetic function related to the divisors of an integer. When referred to as the divisor function, it counts the number of divisors of an integer (including 1 and the number itself). It appears in a number of remarkable identities, including relationships on the Riemann zeta function and the Eisenstein series of modular forms. Divisor functions were studied by Ramanujan, who gave a number of important congruences and identities; these are treated separately in the article Ramanujan's sum.

A related function is the divisor summatory function, which, as the name implies, is a sum over the divisor function.

Definition

The sum of positive divisors function σz(n), for a real or complex number z, is defined as the sum of the zth powers of the positive divisors of n. It can be expressed in sigma notation as

\sigmaz(n)=\sumd\middz,

where

{d\midn}

is shorthand for "d divides n".The notations d(n), ν(n) and τ(n) (for the German Teiler = divisors) are also used to denote σ0(n), or the number-of-divisors function . When z is 1, the function is called the sigma function or sum-of-divisors function, and the subscript is often omitted, so σ(n) is the same as σ1(n) .

The aliquot sum s(n) of n is the sum of the proper divisors (that is, the divisors excluding n itself,), and equals σ1(n) - n; the aliquot sequence of n is formed by repeatedly applying the aliquot sum function.

Example

For example, σ0(12) is the number of the divisors of 12:

\begin{align} \sigma0(12)&=10+20+30+40+60+120\\ &=1+1+1+1+1+1=6, \end{align}

while σ1(12) is the sum of all the divisors:

\begin{align} \sigma1(12)&=11+21+31+41+61+121\\ &=1+2+3+4+6+12=28, \end{align}

and the aliquot sum s(12) of proper divisors is:

\begin{align} s(12)&=11+21+31+41+61\\ &=1+2+3+4+6=16. \end{align}

σ-1(n) is sometimes called the abundancy index of n, and we have:

\begin{align} \sigma-1(12)&=1-1+2-1+3-1+4-1+6-1+12-1\\ &=\tfrac11+\tfrac12+\tfrac13+\tfrac14+\tfrac16+\tfrac1{12}\\ &=\tfrac{12}{12}+\tfrac6{12}+\tfrac4{12}+\tfrac3{12}+\tfrac2{12}+\tfrac1{12}\\ &=\tfrac{12+6+4+3+2+1}{12}=\tfrac{28}{12}=\tfrac73=\tfrac{\sigma1(12)}{12} \end{align}

Table of values

The cases x = 2 to 5 are listed in through, x = 6 to 24 are listed in through .

n factorization 0(n)1(n)2(n)3(n)4(n)
1style='text-align:center;'111111
2style='text-align:center;'2235917
3style='text-align:center;'324102882
4style='text-align:center;'22372173273
5style='text-align:center;'52626126626
6style='text-align:center;'2×3412502521394
7style='text-align:center;'728503442402
8style='text-align:center;'23415855854369
9style='text-align:center;'32313917576643
10style='text-align:center;'2×5418130113410642
11style='text-align:center;'11212122133214642
12style='text-align:center;'22×3628210204422386
13style='text-align:center;'13214170219828562
14style='text-align:center;'2×7424250309640834
15style='text-align:center;'3×5424260352851332
16style='text-align:center;'24531341468169905
17style='text-align:center;'17218290491483522
18style='text-align:center;'2×326394556813112931
19style='text-align:center;'192203626860130322
20style='text-align:center;'22×56425469198170898
21style='text-align:center;'3×74325009632196964
22style='text-align:center;'2×1143661011988248914
23style='text-align:center;'2322453012168279842
24style='text-align:center;'23×386085016380358258
25style='text-align:center;'5233165115751391251
26style='text-align:center;'2×1344285019782485554
27style='text-align:center;'3344082020440538084
28style='text-align:center;'22×7656105025112655746
29style='text-align:center;'2923084224390707282
30style='text-align:center;'2×3×5872130031752872644
31style='text-align:center;'3123296229792923522
32style='text-align:center;'256631365374491118481
33style='text-align:center;'3×114481220372961200644
34style='text-align:center;'2×174541450442261419874
35style='text-align:center;'5×74481300433441503652
36style='text-align:center;'22×329911911552611813539
37style='text-align:center;'372381370506541874162
38style='text-align:center;'2×194601810617402215474
39style='text-align:center;'3×134561700615442342084
40style='text-align:center;'23×58902210737102734994
41style='text-align:center;'412421682689222825762
42style='text-align:center;'2×3×78962500866883348388
43style='text-align:center;'432441850795083418802
44style='text-align:center;'22×116842562972363997266
45style='text-align:center;'32×56782366953824158518
46style='text-align:center;'2×2347226501095124757314
47style='text-align:center;'4724822101038244879682
48style='text-align:center;'24×31012434101310685732210
49style='text-align:center;'7235724511179935767203
50style='text-align:center;'2×5269332551417596651267

Properties

Formulas at prime powers

For a prime number p,

\begin{align} \sigma0(p)&=2

n)
\\ \sigma
0(p

&=n+1\\ \sigma1(p)&=p+1 \end{align}

because by definition, the factors of a prime number are 1 and itself. Also, where pn# denotes the primorial,

\sigma0(pn\#)=2n

since n prime factors allow a sequence of binary selection (

pi

or 1) from n terms for each proper divisor formed. However, these are not in general the smallest numbers whose number of divisors is a power of two; instead, the smallest such number may be obtained by multiplying together the first n Fermi–Dirac primes, prime powers whose exponent is a power of two.[1]

Clearly,

1<\sigma0(n)<n

for all

n>2

, and

\sigmax(n)>n

for all

n>1

,

x>0

.

The divisor function is multiplicative (since each divisor c of the product mn with

\gcd(m,n)=1

distinctively correspond to a divisor a of m and a divisor b of n), but not completely multiplicative:

\gcd(a,b)=1\Longrightarrow\sigmax(ab)=\sigmax(a)\sigmax(b).

The consequence of this is that, if we write

n=

r
\prod
i=1
ai
p
i

where r = ω(n) is the number of distinct prime factors of n, pi is the ith prime factor, and ai is the maximum power of pi by which n is divisible, then we have:

\sigmax(n)=

r
\prod
i=1
ai
\sum
j=0
jx
p
i

=

r
\prod
i=1

\left(1+

x
p
i

+

2x
p
i

++

aix
p
i

\right).

which, when x ≠ 0, is equivalent to the useful formula:

\sigmax(n)=

r
\prod
i=1
(ai+1)x
p-1
i
x-1
p
i

.

When x = 0,

\sigma0(n)

is:

\sigma0(n)=\prod

r
i=1

(ai+1).

This result can be directly deduced from the fact that all divisors of

n

are uniquely determined by the distinct tuples

(x1,x2,...,xi,...,xr)

of integers with

0\lexi\leai

(i.e.

ai+1

independent choices for each

xi

).

For example, if n is 24, there are two prime factors (p1 is 2; p2 is 3); noting that 24 is the product of 23×31, a1 is 3 and a2 is 1. Thus we can calculate

\sigma0(24)

as so:

\sigma0(24)=

2
\prod
i=1

(ai+1)=(3+1)(1+1)=42=8.

The eight divisors counted by this formula are 1, 2, 4, 8, 3, 6, 12, and 24.

Other properties and identities

Euler proved the remarkable recurrence:[2] [3] [4]

\begin{align} \sigma1(n)&=\sigma1(n-1)+\sigma1(n-2)-\sigma1(n-5)-\sigma1(n-7)+\sigma1(n-12)+\sigma1(n-15)+\\[12mu] &=\sumi\in\N(-1)i+1\left(\sigma1\left(n-

1
2

\left(3i2-i\right)\right)+\sigma1\left(n-

1
2

\left(3i2+i\right)\right)\right), \end{align}

where

\sigma1(0)=n

if it occurs and

\sigma1(x)=0

for

x<0

, and

\tfrac{1}{2}\left(3i2\mpi\right)

are consecutive pairs of generalized pentagonal numbers (starting at offset 1). Indeed, Euler proved this by logarithmic differentiation of the identity in his pentagonal number theorem.

For a non-square integer, n, every divisor, d, of n is paired with divisor n/d of n and

\sigma0(n)

is even; for a square integer, one divisor (namely

\sqrtn

) is not paired with a distinct divisor and

\sigma0(n)

is odd. Similarly, the number

\sigma1(n)

is odd if and only if n is a square or twice a square.

We also note s(n) = σ(n) − n. Here s(n) denotes the sum of the proper divisors of n, that is, the divisors of n excluding n itself. This function is used to recognize perfect numbers, which are the n such that s(n) = n. If s(n) > n, then n is an abundant number, and if s(n) < n, then n is a deficient number.

If is a power of 2,

n=2k

, then

\sigma(n)=22k-1=2n-1

and

s(n)=n-1

, which makes n almost-perfect.

As an example, for two primes

p,q:p<q

, let

n=pq

.

Then

\sigma(n)=(p+1)(q+1)=n+1+(p+q),

\varphi(n)=(p-1)(q-1)=n+1-(p+q),

and

n+1=(\sigma(n)+\varphi(n))/2,

p+q=(\sigma(n)-\varphi(n))/2,

where

\varphi(n)

is Euler's totient function.

Then, the roots of

(x-p)(x-q)=x2-(p+q)x+n=x2-[(\sigma(n)-\varphi(n))/2]x+[(\sigma(n)+\varphi(n))/2-1]=0

express p and q in terms of σ(n) and φ(n) only, requiring no knowledge of n or

p+q

, as

p=(\sigma(n)-\varphi(n))/4-\sqrt{[(\sigma(n)-\varphi(n))/4]2-[(\sigma(n)+\varphi(n))/2-1]},

q=(\sigma(n)-\varphi(n))/4+\sqrt{[(\sigma(n)-\varphi(n))/4]2-[(\sigma(n)+\varphi(n))/2-1]}.

Also, knowing and either

\sigma(n)

or

\varphi(n)

, or, alternatively,

p+q

and either

\sigma(n)

or

\varphi(n)

allows an easy recovery of p and q.

In 1984, Roger Heath-Brown proved that the equality

\sigma0(n)=\sigma0(n+1)

is true for infinitely many values of, see .

Series relations

Two Dirichlet series involving the divisor function are:

infty
\sum
n=1
\sigmaa(n)
ns

=\zeta(s)\zeta(s-a)fors>1,s>a+1,

where

\zeta

is the Riemann zeta function. The series for d(n) = σ0(n) gives:
infty
\sum
n=1
d(n)
ns

=\zeta2(s)fors>1,

and a Ramanujan identity

infty
\sum
n=1
\sigmaa(n)\sigmab(n)
ns

=

\zeta(s)\zeta(s-a)\zeta(s-b)\zeta(s-a-b)
\zeta(2s-a-b)

,

which is a special case of the Rankin–Selberg convolution.

A Lambert series involving the divisor function is:

infty
\sum
n=1

qn\sigmaa(n)=

infty
\sum
n=1
infty
\sum
j=1

naqjn=

infty
\sum
n=1
naqn
1-qn

for arbitrary complex |q| ≤ 1 and a. This summation also appears as the Fourier series of the Eisenstein series and the invariants of the Weierstrass elliptic functions.

For

k>0

, there is an explicit series representation with Ramanujan sums

cm(n)

as :[5]

\sigmak(n)=

infty
\zeta(k+1)n
m=1
cm(n)
mk+1

.

The computation of the first terms of

cm(n)

shows its oscillations around the "average value"

\zeta(k+1)nk

:

\sigmak(n)=\zeta(k+1)nk\left[1+

(-1)n
2k+1

+

2\cos2\pin
3
3k+1

+

2\cos\pin
2
4k+1

+\right]

Growth rate

In little-o notation, the divisor function satisfies the inequality:

forall\varepsilon>0,d(n)=o(n\varepsilon).

More precisely, Severin Wigert showed that:

\limsupn\toinfty

logd(n)
logn/loglogn

=log2.

On the other hand, since there are infinitely many prime numbers,

\liminfn\toinftyd(n)=2.

In Big-O notation, Peter Gustav Lejeune Dirichlet showed that the average order of the divisor function satisfies the following inequality:

forallx\geq1,\sumn\leqd(n)=xlogx+(2\gamma-1)x+O(\sqrt{x}),

where

\gamma

is Euler's gamma constant. Improving the bound

O(\sqrt{x})

in this formula is known as Dirichlet's divisor problem.

The behaviour of the sigma function is irregular. The asymptotic growth rate of the sigma function can be expressed by:

\limsupn → infty

\sigma(n)
nloglogn

=e\gamma,

where lim sup is the limit superior. This result is Grönwall's theorem, published in 1913 . His proof uses Mertens' third theorem, which says that:

\limn\toinfty

1
logn

\prodp\le

p
p-1

=e\gamma,

where p denotes a prime.

In 1915, Ramanujan proved that under the assumption of the Riemann hypothesis, Robin's inequality

\sigma(n)<e\gammanloglogn

(where γ is the Euler–Mascheroni constant)holds for all sufficiently large n . The largest known value that violates the inequality is n=5040. In 1984, Guy Robin proved that the inequality is true for all n > 5040 if and only if the Riemann hypothesis is true . This is Robin's theorem and the inequality became known after him. Robin furthermore showed that if the Riemann hypothesis is false then there are an infinite number of values of n that violate the inequality, and it is known that the smallest such n > 5040 must be superabundant . It has been shown that the inequality holds for large odd and square-free integers, and that the Riemann hypothesis is equivalent to the inequality just for n divisible by the fifth power of a prime .

Robin also proved, unconditionally, that the inequality:

\sigma(n)<e\gammanloglogn+

0.6483 n
loglogn
holds for all n ≥ 3.

A related bound was given by Jeffrey Lagarias in 2002, who proved that the Riemann hypothesis is equivalent to the statement that:

\sigma(n)<Hn+

Hn
e

log(Hn)

for every natural number n > 1, where

Hn

is the nth harmonic number, .

See also

References

External links

Notes and References

  1. see section 47, pp. 405–406, reproduced in Collected Papers of Srinivasa Ramanujan, Cambridge Univ. Press, 2015, pp. 124–125
  2. math/0411587. Euler. Leonhard. An observation on the sums of divisors. Bell. Jordan. 2004.
  3. https://scholarlycommons.pacific.edu/euler-works/175/, Découverte d'une loi tout extraordinaire des nombres par rapport à la somme de leurs diviseurs
  4. https://scholarlycommons.pacific.edu/euler-works/542/, De mirabilis proprietatibus numerorum pentagonalium
  5. Book: E. Krätzel . Zahlentheorie . VEB Deutscher Verlag der Wissenschaften . Berlin . 1981 . 130. (German)