In number theory, a branch of mathematics, Ramanujan's sum, usually denoted cq(n), is a function of two positive integer variables q and n defined by the formula
Contents
- Notation
- Trigonometry
- Kluyver
- von Sterneck
- Other properties of cqn
- Table
- Ramanujan expansions
- Generating functions
- kn
- dn
- n
- Zero
- r2sn sums of squares
- r2sn sums of triangles
- Sums
- References
where (a, q) = 1 means that a only takes on values coprime to q.
Srinivasa Ramanujan introduced the sums in a 1918 paper. 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.
Notation
For integers a and b,
means that d goes through all the positive divisors of m, e.g.
Trigonometry
These formulas come from the definition, Euler's formula
and so on ( A000012, A033999, A099837, A176742,.., A100051,...) They show that cq(n) is always real.
Kluyver
Let
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 that the powers of ζq are precisely the primitive roots for all the divisors of q.
Example. Let q = 12. Then
ζ12, ζ125, ζ127, and ζ1211 are the primitive twelfth roots of unity,ζ122 and ζ1210 are the primitive sixth roots of unity,ζ123 = i and ζ129 = −i are the primitive fourth roots of unity,ζ124 and ζ128 are the primitive third roots of unity,ζ126 = −1 is the primitive second root of unity, andζ1212 = 1 is the primitive first root of unity.Therefore, if
is the sum of the n-th powers of all the roots, primitive and imprimitive,
and by Möbius inversion,
It follows from the identity xq − 1 = (x − 1)(xq−1 + xq−2 + ... + x + 1) that
and this leads to the formula
published by Kluyver in 1906.
This shows that cq(n) is always an integer. Compare it with the formula
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: i.e.
From the definition (or Kluyver's formula) it is straightforward to prove that, if p is a prime number,
and if pk is a prime power where k > 1,
This result and the multiplicative property can be used to prove
This is called von Sterneck's arithmetic function. The equivalence of it and Ramanujan's sum is due to Hölder.
Other properties of cq(n)
For all positive integers q,
For a fixed value of q the absolute value of the sequence
cq(1), cq(2), ... is bounded by φ(q), andfor a fixed value of n the absolute value of the sequence
c1(n), c2(n), ... is bounded by n.If q > 1
Let m1, m2 > 0, m = lcm(m1, m2). Then Ramanujan's sums satisfy an orthogonality property:
Let n, k > 0. Then
known as the Brauer - Rademacher identity.
If n > 0 and a is any integer, we also have
due to Cohen.
Table
1+1+1+1+1 1+1+1+1+1 1+1+1+1+1 1+1+1 +(1×0)
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
or of the form
where the ak ∈ C, is called a Ramanujan expansion 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).
The expansion of the zero function depends on a result from the analytic theory of prime numbers, namely that the series
converges to 0, and the results for r(n) and r′(n) depend on theorems in an earlier paper.
All the formulas in this section are from Ramanujan's 1918 paper.
Generating functions
The generating functions of the Ramanujan sums are Dirichlet series:
is a generating function for the sequence cq(1), cq(2), ... where q is kept constant, and
is a generating function for the sequence c1(n), c2(n), ... where n is kept constant.
There is also the double Dirichlet series
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,
and
Setting s = 1 gives
If the Riemann hypothesis is true, and
d(n)
d(n) = σ0(n) is the number of divisors of n, including 1 and n itself.
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
is the prime factorization of n, and s is a complex number, let
so that φ1(n) = φ(n) is Euler's function.
He proves that
and uses this to show that
Letting s = 1,
Note that the constant is the inverse of the one in the formula for σ(n).
Λ(n)
Von Mangoldt's function Λ(n) = 0 unless n = pk is a power of a prime number, in which case it is the natural logarithm log p.
Zero
For all n > 0,
This is equivalent to the prime number theorem.
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 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:
In the following formulas the signs repeat with a period of 4.
If s ≡ 0 (mod 4),
If s ≡ 2 (mod 4),
If s ≡ 1 (mod 4) and s > 1,
If s ≡ 3 (mod 4),
and therefore,
r′2s(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 δ′2s(n) such that r′2s(n) = δ′2s(n) for s = 1, 2, 3, and 4, and that for s > 4, δ′2s(n) is a good approximation to r′2s(n).
Again, s = 1 requires a special formula:
If s is a multiple of 4,
If s is twice an odd number,
If s is an odd number and s > 1,
Therefore,
Sums
Let
Then for s > 1,