In mathematics, the Bernoulli polynomials occur in the study of many special functions and in particular the Riemann zeta function and the Hurwitz zeta function. This is in large part because they are an Appell sequence, i.e. a Sheffer sequence for the ordinary derivative operator. Unlike orthogonal polynomials, the Bernoulli polynomials are remarkable in that the number of crossings of the x-axis in the unit interval does not go up as the degree of the polynomials goes up. In the limit of large degree, the Bernoulli polynomials, appropriately scaled, approach the sine and cosine functions.
The Bernoulli polynomials Bn admit a variety of different representations. Which among them should be taken to be the definition may depend on one's purposes.
for n ≥ 0, where bk are the Bernoulli numbers.
The generating function for the Bernoulli polynomials is
The generating function for the Euler polynomials is
The Bernoulli polynomials are also given by
where D = d/dx is differentiation with respect to x and the fraction is expanded as a formal power series.
The Bernoulli polynomials are the unique polynomials determined by
The integral operator
on polynomials f, is the same as
An explicit formula for the Bernoulli polynomials is given by
Note the remarkable similarity to the globally convergent series expression for the Hurwitz zeta function. Indeed, one has
where ζ(s, q) is the Hurwitz zeta; thus, in a certain sense, the Hurwitz zeta generalizes the Bernoulli polynomials to non-integer values of n.
The inner sum may be understood to be the nth forward difference of xm; that is,
where Δ is the forward difference operator. Thus, one may write
This formula may be derived from an identity appearing above as follows: since the forward difference operator Δ is equal to
where D is differentiation with respect to x, we have
As long as this operates on an mth-degree polynomial such as xm, one may let n go from 0 only up to m.
An integral representation for the Bernoulli polynomials is given by the Nörlund–Rice integral, which follows from the expression as a finite difference.
An explicit formula for the Euler polynomials is given by
This may also be written in terms of the Euler numbers Ek as
We have
See Faulhaber's formula for more on this.
The Bernoulli numbers are given by An alternate convention defines the Bernoulli numbers as . This definition gives Bn = −nζ(1 − n) where for n = 0 and n = 1 the expression −nζ(1 − n) is to be understood as limx → n −xζ(1 − x). The two conventions differ only for n = 1 since B1(1) = 1/2 = −B1(0).
The Euler numbers are given by
The first few Bernoulli polynomials are:
The first few Euler polynomials are
At higher n, the amount of variation in Bn(x) between x = 0 and x = 1 gets large. For instance,
which shows that the value at x = 0 (and at x = 1) is −3617/510 ≈ −7.09, while at x = 1/2, the value is 118518239/3342336 ≈ +7.09. D.H. Lehmer[1] showed that the maximum value of Bn(x) between 0 and 1 obeys
unless n is 2 modulo 4, in which case
(where is the Riemann zeta function), while the minimum obeys
unless n is 0 modulo 4, in which case
These limits are quite close to the actual maximum and minimum, and Lehmer gives more accurate limits as well.
The Bernoulli and Euler polynomials obey many relations from umbral calculus:
(Δ is the forward difference operator).
These polynomial sequences are Appell sequences:
These identities are also equivalent to saying that these polynomial sequences are Appell sequences. (Hermite polynomials are another example.)
Zhi-Wei Sun and Hao Pan [2] established the following surprising symmetric relation: If r + s + t = n and x + y + z = 1, then
where
The Fourier series of the Bernoulli polynomials is also a Dirichlet series, given by the expansion
This is a special case of the analogous form for the Hurwitz zeta function
This expansion is valid only for 0 ≤ x ≤ 1 when n ≥ 2 and is valid for 0 < x < 1 when n = 1.
The Fourier series of the Euler polynomials may also be calculated. Defining the functions
and
for , the Euler polynomial has the Fourier series
and
Note that the and are odd and even, respectively:
and
They are related to the Legendre chi function as
and
The Bernoulli and Euler polynomials may be inverted to express the monomial in terms of the polynomials. Specifically, one has
and
The Bernoulli polynomials may be expanded in terms of the falling factorial as
where and
denotes the Stirling number of the second kind. The above may be inverted to express the falling factorial in terms of the Bernoulli polynomials:
where
denotes the Stirling number of the first kind.
The multiplication theorems were given by Joseph Ludwig Raabe in 1851:
Indefinite integrals
Definite integrals
A periodic Bernoulli polynomial Pn(x) is a Bernoulli polynomial evaluated at the fractional part of the argument x. These functions are used to provide the remainder term in the Euler–Maclaurin formula relating sums to integrals. The first polynomial is a sawtooth function.