Basel problem explained
The Basel problem is a problem in mathematical analysis with relevance to number theory, concerning an infinite sum of inverse squares. It was first posed by Pietro Mengoli in 1650 and solved by Leonhard Euler in 1734, and read on 5 December 1735 in The Saint Petersburg Academy of Sciences.[1] Since the problem had withstood the attacks of the leading mathematicians of the day, Euler's solution brought him immediate fame when he was twenty-eight. Euler generalised the problem considerably, and his ideas were taken up more than a century later by Bernhard Riemann in his seminal 1859 paper "On the Number of Primes Less Than a Given Magnitude", in which he defined his zeta function and proved its basic properties. The problem is named after Basel, hometown of Euler as well as of the Bernoulli family who unsuccessfully attacked the problem.
The Basel problem asks for the precise summation of the reciprocals of the squares of the natural numbers, i.e. the precise sum of the infinite series:
The sum of the series is approximately equal to 1.644934.[2] The Basel problem asks for the exact sum of this series (in closed form), as well as a proof that this sum is correct. Euler found the exact sum to be
and announced this discovery in 1735. His arguments were based on manipulations that were not justified at the time, although he was later proven correct. He produced an accepted proof in 1741.
The solution to this problem can be used to estimate the probability that two large random numbers are coprime. Two random integers in the range from 1 to
, in the limit as
goes to infinity, are relatively prime with a probability that approaches
, the reciprocal of the solution to the Basel problem.
Euler's approach
Euler's original derivation of the value
essentially extended observations about finite
polynomials and assumed that these same properties hold true for infinite series.
Of course, Euler's original reasoning requires justification (100 years later, Karl Weierstrass proved that Euler's representation of the sine function as an infinite product is valid, by the Weierstrass factorization theorem), but even without justification, by simply obtaining the correct value, he was able to verify it numerically against partial sums of the series. The agreement he observed gave him sufficient confidence to announce his result to the mathematical community.
To follow Euler's argument, recall the Taylor series expansion of the sine functionDividing through by
gives
The Weierstrass factorization theorem shows that the right-hand side is the product of linear factors given by its roots, just as for finite polynomials. Euler assumed this as a heuristic for expanding an infinite degree polynomial in terms of its roots, but in fact it is not always true for general
.
[3] This factorization expands the equation into:
If we formally multiply out this product and collect all the terms (we are allowed to do so because of Newton's identities), we see by induction that the coefficient of is [4]
But from the original infinite series expansion of, the coefficient of is . These two coefficients must be equal; thus,
Multiplying both sides of this equation by −2 gives the sum of the reciprocals of the positive square integers.
This method of calculating
is detailed in expository fashion most notably in Havil's
Gamma book which details many
zeta function and
logarithm-related series and integrals, as well as a historical perspective, related to the
Euler gamma constant.
Generalizations of Euler's method using elementary symmetric polynomials
Using formulae obtained from elementary symmetric polynomials,[5] this same approach can be used to enumerate formulae for the even-indexed even zeta constants which have the following known formula expanded by the Bernoulli numbers:
For example, let the partial product for
expanded as above be defined by
. Then using known formulas for elementary symmetric polynomials (a.k.a., Newton's formulas expanded in terms of
power sum identities), we can see (for example) that
and so on for subsequent coefficients of
. There are other forms of Newton's identities expressing the (finite) power sums
in terms of the
elementary symmetric polynomials,
ei\equiv
,-
,-
,-
,\ldots\right),
but we can go a more direct route to expressing non-recursive formulas for
using the method of
elementary symmetric polynomials. Namely, we have a recurrence relation between the elementary symmetric polynomials and the
power sum polynomials given as on this page by
which in our situation equates to the limiting recurrence relation (or generating function convolution, or product) expanded as
Then by differentiation and rearrangement of the terms in the previous equation, we obtain that
Consequences of Euler's proof
By the above results, we can conclude that
is
always a
rational multiple of
. In particular, since
and integer powers of it are
transcendental, we can conclude at this point that
is
irrational, and more precisely,
transcendental for all
. By contrast, the properties of the odd-indexed
zeta constants, including
Apéry's constant
, are almost completely unknown.
The Riemann zeta function
The Riemann zeta function is one of the most significant functions in mathematics because of its relationship to the distribution of the prime numbers. The zeta function is defined for any complex number with real part greater than 1 by the following formula:
Taking, we see that is equal to the sum of the reciprocals of the squares of all positive integers:
Convergence can be proven by the integral test, or by the following inequality:
This gives us the upper bound 2, and because the infinite sum contains no negative terms, it must converge to a value strictly between 0 and 2. It can be shown that has a simple expression in terms of the Bernoulli numbers whenever is a positive even integer. With :
A proof using Euler's formula and L'Hôpital's rule
has a
Weierstrass factorization representation as an infinite product:
The infinite product is analytic, so taking the natural logarithm of both sides and differentiating yields
(by uniform convergence, the interchange of the derivative and infinite series is permissible). After dividing the equation by
and regrouping one gets
We make a change of variables (
):
Euler's formula can be used to deduce thator using the corresponding hyperbolic function:
Then
Now we take the limit as
approaches zero and use
L'Hôpital's rule thrice. By
Tannery's theorem applied to
, we can
interchange the limit and infinite series so that
and by L'Hôpital's rule
A proof using Fourier series
Use Parseval's identity (applied to the function) to obtainwhere
for, and . Thus,
and
Therefore,as required.
Another proof using Parseval's identity
Given a complete orthonormal basis in the space
}(0, 1) of L2
periodic functions over
(i.e., the subspace of
square-integrable functions which are also
periodic), denoted by
,
Parseval's identity tells us that
where
\|x\|:=\sqrt{\langlex,x\rangle}
is defined in terms of the
inner product on this
Hilbert space given by
We can consider the orthonormal basis on this space defined by
ek\equivek(\vartheta):=\exp(2\pi\imathk\vartheta)
such that
\langleek,ej\rangle=
e2\pi\imathd\vartheta=\deltak,j
. Then if we take
, we can compute both that