Ramanujan's sum explained

Ramanujan's sum should not be confused with Ramanujan summation.

In number theory, Ramanujan's sum, usually denoted cq(n), is a function of two positive integer variables q and n defined by the formula

cq(n)=\sum1e2{q}n},

where (a, q) = 1 means that a only takes on values coprime to q.

Srinivasa Ramanujan mentioned the sums in a 1918 paper.[1] In addition to the expansions discussed in this article, Ramanujan's sums are used in the proof of Vinogradov's theorem that every sufficiently large odd number is the sum of three primes.[2]

Notation

For integers a and b,

a\midb

is read "a divides b" and means that there is an integer c such that
b
a

=c.

Similarly,

a\nmidb

is read "a does not divide b". The summation symbol

\sumd\midmf(d)

means that d goes through all the positive divisors of m, e.g.

\sumd\mid12f(d)=f(1)+f(2)+f(3)+f(4)+f(6)+f(12).

(a,b)

is the greatest common divisor,

\phi(n)

is Euler's totient function,

\mu(n)

is the Möbius function, and

\zeta(s)

is the Riemann zeta function.

Formulas for cq(n)

Trigonometry

eix=\cosx+i\sinx,

and elementary trigonometric identities.

\begin{align} c1(n)&=1\\ c2(n)&=\cosn\pi\\ c3(n)&=2\cos\tfrac23n\pi\\ c4(n)&=2\cos\tfrac12n\pi\\ c5(n)&=2\cos\tfrac25n\pi+2\cos\tfrac45n\pi\\ c6(n)&=2\cos\tfrac13n\pi\\ c7(n)&=2\cos\tfrac27n\pi+2\cos\tfrac47n\pi+2\cos\tfrac67n\pi\\ c8(n)&=2\cos\tfrac14n\pi+2\cos\tfrac34n\pi\\ c9(n)&=2\cos\tfrac29n\pi+2\cos\tfrac49n\pi+2\cos\tfrac89n\pi\\ c10(n)&=2\cos\tfrac15n\pi+2\cos\tfrac35n\pi\\ \end{align}

and so on (..,,...). cq(n) is always an integer.

Kluyver

Let

2\pii
q
\zeta
q=e

.

Then is a root of the equation . Each of its powers,

\zetaq,

2,
\zeta
q

\ldots,

q-1
\zeta
q

,

q
\zeta
q

=

0
\zeta
q

=1

is also a root. Therefore, since there are q of them, they are all of the roots. The numbers

n
\zeta
q
where 1 ≤ nq are called the q-th roots of unity. is called a primitive q-th root of unity because the smallest value of n that makes
n
\zeta
q

=1

is q. The other primitive q-th roots of unity are the numbers
a
\zeta
q
where (a, q) = 1. Therefore, there are φ(q) primitive q-th roots of unity.

Thus, the Ramanujan sum cq(n) is the sum of the n-th powers of the primitive q-th roots of unity.

It is a fact[3] that the powers of are precisely the primitive roots for all the divisors of q.

Example. Let q = 12. Then

\zeta12,

5,
\zeta
12
7,
\zeta
12
and
11
\zeta
12
are the primitive twelfth roots of unity,
2
\zeta
12
and
10
\zeta
12
are the primitive sixth roots of unity,
3
\zeta
12

=i

and
9
\zeta
12

=-i

are the primitive fourth roots of unity,
4
\zeta
12
and
8
\zeta
12
are the primitive third roots of unity,
6
\zeta
12

=-1

is the primitive second root of unity, and
12
\zeta
12

=1

is the primitive first root of unity.

Therefore, if

ηq(n)=

q
\sum
k=1
kn
\zeta
q

is the sum of the n-th powers of all the roots, primitive and imprimitive,

ηq(n)=\sumd\midcd(n),

and by Möbius inversion,

cq(n)=\sumd\mid\mu\left(

q
d\right)η

d(n).

It follows from the identity xq − 1 = (x − 1)(xq−1 + xq−2 + ... + x + 1) that

ηq(n)=\begin{cases}0&q\nmidn\q&q\midn\\end{cases}

and this leads to the formula

cq(n)=\sumd\mid\mu\left(

q
d

\right)d,

published by Kluyver in 1906.[4]

This shows that cq(n) is always an integer. Compare it with the formula

\phi(q)=\sumd\mu\left(

q
d

\right)d.

von Sterneck

It is easily shown from the definition that cq(n) is multiplicative when considered as a function of q for a fixed value of n:[5] i.e.

If(q,r)=1thencq(n)cr(n)=cqr(n).

From the definition (or Kluyver's formula) it is straightforward to prove that, if p is a prime number,

cp(n)=\begin{cases} -1&ifp\nmidn\\ \phi(p)&ifp\midn\\ \end{cases} ,

and if pk is a prime power where k > 1,

c
pk

(n)=\begin{cases} 0&ifpk-1\nmidn\\ -pk-1&ifpk-1\midnandpk\nmidn\\ \phi(pk)&ifpk\midn\\ \end{cases} .

This result and the multiplicative property can be used to prove

cq(n)=\mu\left(

q\right)
(q,n)
\phi(q)
\phi\left(q\right)
(q,n)

.

This is called von Sterneck's arithmetic function.[6] The equivalence of it and Ramanujan's sum is due to Hölder.[7] [8]

Other properties of cq(n)

For all positive integers q,

\begin{align} c1(q)&=1\\ cq(1)&=\mu(q)\\ cq(q)&=\phi(q)\\ cq(m)&=cq(n)&&form\equivn\pmodq\\ \end{align}

For a fixed value of q the absolute value of the sequence

\{cq(1),cq(2),\ldots\}

is bounded by φ(q), and for a fixed value of n the absolute value of the sequence

\{c1(n),c2(n),\ldots\}

is bounded by n.

If q > 1

a+q-1
\sum
n=a

cq(n)=0.

Let m1, m2 > 0, m = lcm(m1, m2). Then[9] Ramanujan's sums satisfy an orthogonality property:

1
m
m
\sum
k=1
c
m1

(k)

c
m2

(k)=\begin{cases}\phi(m)&m1=m2=m,\ 0&otherwise\end{cases}

Let n, k > 0. Then[10]

\sum\stackrel{d\midn}{\gcd(d,k)=1}d

\mu(\tfrac{n
d

)}{\phi(d)}=

\mu(n)cn(k)
\phi(n)

,

known as the Brauer - Rademacher identity.

If n > 0 and a is any integer, we also have[11]

\sum\stackrel{1\lek\len}{\gcd(k,n)=1}cn(k-a)=\mu(n)cn(a),

due to Cohen.

Table

Ramanujan sum cs(n)
n
123456789101112131415161718192021222324252627282930
s11 1 1 1 1 1 1 1 1 11 1 1 1 1 1 1 1 1 11 1 1 1 1 1 1 1 1 1
2 -1 1 -1 1 -1 1 -1 1 -1 1-1 1 -1 1 -1 1 -1 1 -1 1-1 1 -1 1 -1 1 -1 1 -1 1
3 -1 -1 2 -1 -1 2 -1 -1 2 -1 -1 2 -1 -1 2 -1 -1 2 -1 -1 2 -1 -1 2 -1 -1 2 -1 -1 2
4 0 -2 0 2 0 -2 0 2 0 -2 0 2 0 -2 0 2 0 -2 0 2 0 -2 0 2 0 -2 0 2 0 -2
5 -1 -1 -1 -1 4-1 -1 -1 -1 4-1 -1 -1 -1 4-1 -1 -1 -1 4-1 -1 -1 -1 4-1 -1 -1 -1 4
6 1 -1 -2 -1 1 2 1 -1 -2 -1 1 2 1 -1 -2 -1 1 2 1 -1 -2 -1 1 2 1 -1 -2 -1 1 2
7 -1 -1 -1 -1 -1 -1 6 -1 -1 -1 -1 -1 -1 6 -1 -1 -1 -1 -1 -1 6 -1 -1 -1 -1 -1 -1 6 -1 -1
8 0 0 0 -4 0 0 0 4 0 0 0 -4 0 0 0 40 0 0 -4 0 0 0 40 0 0 -4 0 0
9 0 0 -3 0 0 -3 0 0 60 0 -3 0 0 -3 0 0 60 0 -3 0 0 -3 0 0 60 0 -3
101 -1 1 -1 -4 -1 1 -1 1 4 1 -1 1 -1 -4 -1 1 -1 1 41 -1 1 -1 -4 -1 1 -1 1 4
11-1 -1 -1 -1 -1 -1 -1 -1 -1 -1 10-1 -1 -1 -1 -1 -1 -1 -1 -1 -1 10-1 -1 -1 -1 -1 -1 -1 -1
120 2 0 -2 0 -4 0 -2 0 2 0 40 2 0 -2 0 -4 0 -2 0 2 0 40 2 0 -2 0 -4
13-1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 12-1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 12-1 -1 -1 -1
141 -1 1 -1 1 -1 -6 -1 1 -1 1 -1 1 61 -1 1 -1 1 -1 -6 -1 1 -1 1 -1 1 61 -1
151 1 -2 1 -4 -2 1 1 -2 -4 1 -2 1 1 81 1 -2 1 -4 -2 1 1 -2 -4 1 -2 1 1 8
160 0 0 0 0 0 0 -8 0 0 0 0 0 0 0 80 0 0 0 0 0 0 -8 0 0 0 0 0 0
17-1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 16-1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1
180 0 3 0 0 -3 0 0 -6 0 0 -3 0 0 3 0 0 60 0 3 0 0 -3 0 0 -6 0 0 -3
19-1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 18-1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1
200 2 0 -2 0 2 0 -2 0 -8 0 -2 0 2 0 -2 0 2 0 8 0 2 0 -2 0 2 0 -2 0 -8
211 1 -2 1 1 -2 -6 1 -2 1 1 -2 1 -6 -2 1 1 -2 1 1 121 1 -2 1 1 -2 -6 1 -2
221 -1 1 -1 1 -1 1 -1 1 -1 -10-1 1 -1 1 -1 1 -1 1 -1 1 101 -1 1 -1 1 -1 1 -1
23-1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 22-1 -1 -1 -1 -1 -1 -1
240 0 0 4 0 0 0 -40 0 0 -80 0 0 -40 0 0 40 0 0 80 0 0 4 0 0
250 0 0 0 -50 0 0 0 -50 0 0 0 -50 0 0 0 -50 0 0 0 200 0 0 0 -5
261 -1 1 -1 1 -1 1 -1 1 -1 1 -1 -12-1 1 -1 1 -1 1 -1 1 -1 1 -1 1 121 -1 1 -1
270 0 0 0 0 0 0 0 -90 0 0 0 0 0 0 0 -90 0 0 0 0 0 0 0 180 0 0
280 2 0 -2 0 2 0 -2 0 2 0 -2 0 -120 -2 0 2 0 -2 0 2 0 -2 0 2 0 120 2
29-1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 -1 28-1
30-1 1 2 1 4 -2 -1 1 2 -4 -1 -2 -1 1 -8 1 -1 -2 -1 -4 2 1 -1 -2 4 1 2 1 -1 8

Ramanujan expansions

If f(n) is an arithmetic function (i.e. a complex-valued function of the integers or natural numbers), then a convergent infinite series of the form:

infty
f(n)=\sum
q=1

aqcq(n)

or of the form:

infty
f(q)=\sum
n=1

ancq(n)

where the, is called a Ramanujan expansion[12] of f(n).

Ramanujan found expansions of some of the well-known functions of number theory. All of these results are proved in an "elementary" manner (i.e. only using formal manipulations of series and the simplest results about convergence).[13] [14] [15]

The expansion of the zero function depends on a result from the analytic theory of prime numbers, namely that the series

infty\mu(n)
n
\sum
n=1

converges to 0, and the results for r(n) and r′(n) depend on theorems in an earlier paper.[16]

All the formulas in this section are from Ramanujan's 1918 paper.

Generating functions

The generating functions of the Ramanujan sums are Dirichlet series:

\zeta(s)\sum\delta\midq\mu\left(

q
\delta

\right)\delta1-s=

infty
\sum
n=1
cq(n)
ns

is a generating function for the sequence cq(1), cq(2), ... where q is kept constant, and

\sigmar-1(n)
nr-1\zeta(r)

=

infty
\sum
q=1
cq(n)
qr

is a generating function for the sequence c1(n), c2(n), ... where n is kept constant.

There is also the double Dirichlet series

\zeta(s)\zeta(r+s-1)
\zeta(r)

=

infty
\sum
q=1
infty
\sum
n=1
cq(n)
qrns

.

The polynomial with Ramanujan sum's as coefficients can be expressed with cyclotomic polynomial[17]
q
\sum
n=1

cq(n)xn-1=(xq-1)

\Phiq'(x)
\Phiq(x)

=\Phiq'(x)\prod\begin{array{c}d\midq\\[-4pt]dq\end{array}}\Phid(x)

.

σk(n)

σk(n) is the divisor function (i.e. the sum of the k-th powers of the divisors of n, including 1 and n). σ0(n), the number of divisors of n, is usually written d(n) and σ1(n), the sum of the divisors of n, is usually written σ(n).

If s > 0,

\begin{align} \sigmas(n)&=ns\zeta(s+1)\left(

c1(n)
1s+1

+

c2(n)
2s+1

+

c3(n)
3s+1

+ … \right)\\ \sigma-s(n)&=\zeta(s+1)\left(

c1(n)+
1s+1
c2(n)+
2s+1
c3(n)
3s+1

+ … \right) \end{align}

Setting s = 1 gives

\sigma(n)=

\pi2
6

n\left(

c1(n)
1

+

c2(n)
4

+

c3(n)
9

+\right).

If the Riemann hypothesis is true, and

-\tfrac12<s<\tfrac12,

\sigmas(n)=\zeta(1-s)\left(

c1(n)
11-s

+

c2(n)
21-s

+

c3(n)
31-s

+\right)=ns\zeta(1+s)\left(

c1(n)
11+s

+

c2(n)
21+s

+

c3(n)
31+s

+\right).

d(n)

d(n) = σ0(n) is the number of divisors of n, including 1 and n itself.

\begin{align} -d(n)&=

log1
1

c1(n)+

log2
2

c2(n)+

log3
3

c3(n)+\\ -d(n)(2\gamma+logn)&=

log21
1

c1(n)+

log22
2

c2(n)+

log23
3

c3(n)+\end{align}

where γ = 0.5772... is the Euler–Mascheroni constant.

φ(n)

Euler's totient function φ(n) is the number of positive integers less than n and coprime to n. Ramanujan defines a generalization of it, if

a1
n=p
1
a2
p
2
a3
p
3

is the prime factorization of n, and s is a complex number, let

-s
\varphi
1
-s
)(1-p
2
-s
)(1-p
3

),

so that φ1(n) = φ(n) is Euler's function.[18]

He proves that

\mu(n)ns
\varphis(n)\zeta(s)

=

infty
\sum
\nu=1
\mu(n\nu)
\nus

and uses this to show that

\varphis(n)\zeta(s+1)=
ns
\mu(1)c1(n)+
\varphis+1(1)
\mu(2)c2(n)+
\varphis+1(2)
\mu(3)c3(n)
\varphis+1(3)

+ … .

Letting s = 1,

\varphi(n)=

6
\pi2

n\left(c1(n)-

c2(n)-
22-1
c3(n)-
32-1
c5(n)+
52-1
c6(n)
(22-1)(32-1)

-

c7(n)+
72-1
c10(n)
(22-1)(52-1)

- … \right).

Note that the constant is the inverse[19] of the one in the formula for σ(n).

Λ(n)

Von Mangoldt's function unless n = pk is a power of a prime number, in which case it is the natural logarithm log p.

(m)=cm(1)+

1
2

cm(2)+

13c
m(3)+ …

Zero

For all n > 0,

0=c1(n)+

12c
2(n)+
13c
3(n)+

.

This is equivalent to the prime number theorem.[20] [21]

r2s(n) (sums of squares)

r2s(n) is the number of way of representing n as the sum of 2s squares, counting different orders and signs as different (e.g., r2(13) = 8, as 13 = (±2)2 + (±3)2 = (±3)2 + (±2)2.)

Ramanujan defines a function δ2s(n) and references a paper[22] in which he proved that r2s(n) = δ2s(n) for s = 1, 2, 3, and 4. For s > 4 he shows that δ2s(n) is a good approximation to r2s(n).

s = 1 has a special formula:

\delta2(n)=\pi\left(

c1(n)
1

-

c3(n)
3

+

c5(n)
5

-\right).

In the following formulas the signs repeat with a period of 4.

\begin{align} \delta2s(n)&=

\pisns-1
(s-1)!

\left(

c1(n)
1s

+

c4(n)
2s

+

c3(n)+
3s
c8(n)
4s

+

c5(n)
5s

+

c12(n)
6s

+

c7(n)
7s

+

c16(n)
8s

+\right)&&s\equiv0\pmod4\\[6pt] \delta2s(n)&=

\pisns-1
(s-1)!

\left(

c1(n)
1s

-

c4(n)
2s

+

c3(n)
3s

-

c8(n)
4s

+

c5(n)
5s

-

c12(n)
6s

+

c7(n)
7s

-

c16(n)
8s

+\right)&&s\equiv2\pmod4\\[6pt] \delta2s(n)&=

\pisns-1
(s-1)!

\left(

c1(n)
1s

+

c4(n)
2s

-

c3(n)
3s

+

c8(n)
4s

+

c5(n)
5s

+

c12(n)
6s

-

c7(n)
7s

+

c16(n)
8s

+\right)&&s\equiv1\pmod4ands>1\\[6pt] \delta2s(n)&=

\pisns-1\left(
(s-1)!
c1(n)
1s

-

c4(n)
2s

-

c3(n)
3s

-

c8(n)
4s

+

c5(n)-
5s
c12(n)-
6s
c7(n)-
7s
c16(n)
8s

+\right)&&s\equiv3\pmod4\\ \end{align}

and therefore,

\begin{align} r2(n)&=\pi\left(

c1(n)
1

-

c3(n)
3

+

c5(n)
5

-

c7(n)
7

+

c11(n)-
11
c13(n)
13

+

c15(n)
15

-

c17(n)
17

+\right)\\[6pt] r4(n)&=\pi2n\left(

c1(n)
1

-

c4(n)
4

+

c3(n)
9

-

c8(n)
16

+

c5(n)
25

-

c12(n)
36

+

c7(n)
49

-

c16(n)
64

+\right)\\[6pt] r6(n)&=

\pi3n2
2

\left(

c1(n)
1

-

c4(n)
8

-

c3(n)
27

-

c8(n)
64

+

c5(n)
125

-

c12(n)
216

-

c7(n)
343

-

c16(n)
512

+\right)\\[6pt] r8(n)&=

\pi4n3\left(
6
c1(n)
1

+

c4(n)
16

+

c3(n)
81

+

c8(n)
256

+

c5(n)
625

+

c12(n)
1296

+

c7(n)
2401

+

c16(n)
4096

+\right) \end{align}

r2s(n) (sums of triangles)

r'2s(n)

is the number of ways n can be represented as the sum of 2s triangular numbers (i.e. the numbers 1, 3 = 1 + 2, 6 = 1 + 2 + 3, 10 = 1 + 2 + 3 + 4, 15, ...; the n-th triangular number is given by the formula n(n + 1)/2.)

The analysis here is similar to that for squares. Ramanujan refers to the same paper as he did for the squares, where he showed that there is a function

\delta'2s(n)

such that

r'2s(n)=\delta'2s(n)

for s = 1, 2, 3, and 4, and that for s > 4,

\delta'2s(n)

is a good approximation to

r'2s(n).

Again, s = 1 requires a special formula:

\delta'2(n)=

\pi\left(
4
c1(4n+1)-
1
c3(4n+1)
3

+

c5(4n+1)
5

-

c7(4n+1)
7

+\right).

If s is a multiple of 4,

\begin{align} \delta'2s(n)&=

(\pi)s
2
\left(n+
(s-1)!
s
4\right)

s-1\left(

c
1(n+s
4)
1s

+

c
3(n+s
4)
3s

+

c
5(n+s
4)
5s

+\right)&&s\equiv0\pmod4\\[6pt] \delta'2s(n)&=

(\pi)s
2
\left(n+
(s-1)!
s
4\right)

s-1\left(

c
1(2n+s
2)
1s

+

c
3(2n+s
2)
3s

+

c
5(2n+s
2)
5s

+\right)&&s\equiv2\pmod4\\[6pt] \delta'2s(n)&=

(\pi)s
2
\left(n+
(s-1)!
s
4\right)

s-1\left(

c1(4n+s)
1s

-

c3(4n+s)+
3s
c5(4n+s)
5s

-\right)&&s\equiv1\pmod2ands>1 \end{align}

Therefore,

\begin{align} r'2(n)&=

\pi\left(
4
c1(4n+1)
1

-

c3(4n+1)
3

+

c5(4n+1)
5

-

c7(4n+1)
7

+\right)\\[6pt] r'4(n)&=\left(

\pi
2
2\left(n+12\right)
\left(c1(2n+1)
1
\right)+
c3(2n+1)
9

+

c5(2n+1)
25

+\right)\\[6pt] r'6(n)&=

(\pi)3
2
\left(n+
2
34\right)\left(
2
c1(4n+3)-
1
c3(4n+3)
27

+

c5(4n+3)
125

- … \right)\\[6pt] r'8(n)&=

(\pi)4
2
6

(n+1)3\left(

c1(n+1)
1

+

c3(n+1)
81

+

c5(n+1)
625

+\right)\end{align}

Sums

Let

\begin{align} Tq(n)&=cq(1)+cq(2)++cq(n)\\ Uq(n)&=Tq(n)+\tfrac12\phi(q) \end{align}

Then for,

\begin{align} \sigma-s(1)++\sigma-s(n)&=\zeta(s+1)\left(n+

T2(n)
2s+1

+

T3(n)+
3s+1
T4(n)
4s+1

+ … \right)\\ &=\zeta(s+1)\left(n+\tfrac12+

U2(n)
2s+1

+

U3(n)
3s+1

+

U4(n)
4s+1

+ … \right)-\tfrac12\zeta(s)\\ d(1)+ … +d(n)&=-

T2(n)log2
2

-

T3(n)log3
3

-

T4(n)log4
4

-\\ d(1)log1++d(n)logn&=-

22)
T
2(n)(2\gammalog2-log
-
2
23)
T
3(n)(2\gammalog3-log
-
3
24)
T
4(n)(2\gammalog4-log
4

- … \\ r2(1)+ … +r2(n)&=\pi\left(n-

T3(n)+
3
T5(n)-
5
T7(n)
7

+ … \right) \end{align}

See also

References

External links

Notes and References

  1. Ramanujan, On Certain Trigonometric Sums ...
    These sums are obviously of great interest, and a few of their properties have been discussed already. But, so far as I know, they have never been considered from the point of view which I adopt in this paper; and I believe that all the results which it contains are new.
    (Papers, p. 179). In a footnote cites pp. 360 - 370 of the Dirichlet–Dedekind German: Vorlesungen über Zahlentheorie, 4th ed.
  2. Nathanson, ch. 8.
  3. Hardy & Wright, Thms 65, 66
  4. G. H. Hardy, P. V. Seshu Aiyar, & B. M. Wilson, notes to On certain trigonometrical sums ..., Ramanujan, Papers, p. 343
  5. Schwarz & Spilken (1994) p.16
  6. B. Berndt, commentary to On certain trigonometrical sums..., Ramanujan, Papers, p. 371
  7. Knopfmacher, p. 196
  8. Hardy & Wright, p. 243
  9. Tóth, external links, eq. 6
  10. Tóth, external links, eq. 17.
  11. Tóth, external links, eq. 8.
  12. B. Berndt, commentary to On certain trigonometrical sums..., Ramanujan, Papers, pp. 369 - 371
  13. Ramanujan, On certain trigonometrical sums...
    The majority of my formulae are "elementary" in the technical sense of the word - they can (that is to say) be proved by a combination of processes involving only finite algebra and simple general theorems concerning infinite series
    (Papers, p. 179)
  14. The theory of formal Dirichlet series is discussed in Hardy & Wright, § 17.6 and in Knopfmacher.
  15. Knopfmacher, ch. 7, discusses Ramanujan expansions as a type of Fourier expansion in an inner product space which has the cq as an orthogonal basis.
  16. Ramanujan, On Certain Arithmetical Functions
  17. Nicol, p. 1
  18. This is Jordan's totient function, Js(n).
  19. Cf. Hardy & Wright, Thm. 329, which states that
    6<
    \pi2
    \sigma(n)\phi(n)
    n2

    <1.

  20. Hardy, Ramanujan, p. 141
  21. B. Berndt, commentary to On certain trigonometrical sums..., Ramanujan, Papers, p. 371
  22. Ramanujan, On Certain Arithmetical Functions