Bernoulli number



         



In mathematics, the Bernoulli numbers Bn were first discovered in connection with the closed forms of the sums

<math>\sum_{k=0}^{m-1} k^n = 0^n + 1^n + 2^n + \cdots + {(m-1)}^n <math>

for various fixed values of n. The closed forms are always polynomials in m of degree n+1 and are called Bernoulli polynomials. The coefficients of the Bernoulli polynomials are closely related to the Bernoulli numbers, as follows:

<math>\sum_{k=0}^{m-1} k^n = {1\over{n+1}}\sum_{k=0}^n{n+1\choose{k}} B_k m^{n+1-k}<math>

For example, taking n to be 1, we have 0 + 1 + 2 + ... + (m−1) = 1/2 (B0 m2 + 2 B1 m1) = 1/2 (m2m).

The Bernoulli numbers were first studied by Jakob Bernoulli, after whom they were named by Abraham de Moivre.

Bernoulli numbers may be calculated by using the following recursive formula:

<math>\sum_{j=0}^m{m+1\choose{j}}B_j = 0<math>

plus the initial condition that B0 = 1.

The Bernoulli numbers may also be defined using the technique of generating functions. Their exponential generating function is x/(ex − 1), so that:

<math>

\frac{x}{e^x-1} = \sum_{n=0}^{\infin} B_n \frac{x^n}{n!} <math> for all values of x of absolute value less than 2π (the radius of convergence of this power series).

Sometimes the lower-case bn is used in order to distinguish these from the Bell numbers.

The first few Bernoulli numbers (sequences and in OEIS) are listed below.

nBn
01
1−1/2
21/6
30
4−1/30
50
61/42
70
8−1/30
90
105/66
110
12−691/2730
130
147/6

It can be shown that Bn = 0 for all odd n other than 1. The appearance of the peculiar value B12 = −691/2730 appears to rule out the possibility of a simple closed form for Bernoulli numbers.

The Bernoulli numbers also appear in the Taylor series expansion of the tangent and hyperbolic tangent functions, in the Euler-Maclaurin formula, and in expressions of certain values of the Riemann zeta function.

In note G of Ada Byron's notes on the analytical engine from 1842 an algorithm for computer generated Bernoulli numbers was described for the first time.

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