The Bernoulli numbers are a sequence of signed rational numbers that can be defined by the identity
(1) |
These numbers arise in the series expansions of trigonometric functions, and are extremely important in number theory and analysis.
There are actually two definitions for the Bernoulli numbers. To distinguish them, the Bernoulli numbers as defined in modern usage (National Bureau of Standards convention) are written
Bernoulli numbers defined by the modern definition are denoted and sometimes called "even-index" Bernoulli numbers. These are the Bernoulli numbers returned, by example, by the Mathematica function BernoulliB[n].
The Bernoulli number can be defined by the contour integral
(2) |
where the contour encloses the origin, has radius less than (to avoid the poles at ), and is traversed in a counterclockwise direction (Arfken 1985, p. 413).
The first few Bernoulli numbers are
(3) | |||
(4) | |||
(5) | |||
(6) | |||
(7) | |||
(8) | |||
(9) | |||
(10) | |||
(11) | |||
(12) | |||
(13) | |||
(14) | |||
(15) |
(Sloane's A000367 and A002445), with
(16) |
for n = 1, 2, ....
The numbers of digits in the numerator of for the n = 2, 4, ... are 1, 1, 1, 1, 1, 3, 1, 4, 5, 6, 6, 9, 7, 11, ... (Sloane's A068399), while the numbers of digits in the corresponding denominators are 1, 2, 2, 2, 2, 4, 1, 3, 3, 3, 3, 4, 1, 3, 5, 3, ... (Sloane's A092904). Both are plotted above.
The running maxima of denominators are 1, 6, 30, 42, 66, 2730, 14322, 1919190, ... (Sloane's A100194), which occur for n = 2, 4, 6, 8, 12, 14, 32, 38, ... (Sloane's A100195).
The number of digits in the numerator to for n = 0, 1, ... are 1, 1, 83, 1779, 27691, ... (Sloane's A103233).
for 1806, but for no other n (Kellner 2005).
The only known Bernoulli numbers having prime numerators occur for n = 10, 12, 14, 16, 18, 36, and 42 (Sloane's A092132), corresponding to 5, -691, 7, -3617, 43867, -26315271553053477373, and 1520097643918070802691 (Sloane's A092133), with no other primes for (E. W. Weisstein, Apr. 17, 2005).
The following table summarizes record computations of the nth Bernoulli number
n | digits in numerator | date | reference |
Fee and Plouffe | |||
2002 | Plouffe (2002) | ||
Dec. 16, 2002 | Kellner | ||
Feb. 10, 2003 | Kellner |
The denominator of (mod 1) is given by the von Staudt-Clausen theorem, which also implies that the denominator of is squarefree (Hardy and Wright 1979). Another curious property is that the fraction part of in decimal has a decimal period which divides n, and there is a single digit before that period (Conway 1996).
Consider the generating function
(17) |
which converges uniformly for and all x (Castellanos 1988). Taking the partial derivative gives
(18) |
The solution to this differential equation can be found using separation of variables as
(19) |
so integrating gives
(20) |
But integrating (20) explicitly gives
(21) |
so
(22) |
Solving for T(t) and plugging back into (19) then gives
(23) |
(Castellanos 1988). Setting x = 0 and adding to both sides then gives
(24) |
Letting then gives
(25) |
for
The Bernoulli numbers may also be calculated from
(26) |
The Bernoulli numbers are given by the double sum
(27) |
where is a binomial coefficient. They also satisfy the sum
(28) |
as well as the interesting sums
(29) | |||
(30) |
(Lehmer 1935, Carlitz 1968), as well as the nice sum identity
(31) |
(Gosper).
An asymptotic expansion for the even Bernoulli numbers is
(32) |
Bernoulli numbers appear in expressions of the form
An analytic solution exists for even orders,
(33) |
for n = 1, 2, ..., where is the Riemann zeta function. Another intimate connection with the Riemann zeta function is provided by the identity
(34) |
An integral in terms of the Euler polynomial is given by
(35) |
where is an Euler polynomial (J. Crepps, pers. comm., Apr. 2002).
Bernoulli first used the Bernoulli numbers while computing
(36) |
along with a form for which he derived inductively to compute the sums up to n = 10 (Boyer 1968, p. 85). For
(37) |
where the notation means the quantity in question is raised to the appropriate power k, and all terms of the form are replaced with the corresponding Bernoulli numbers
Written explicitly in terms of a sum of powers,
(38) | |||
(39) | |||
(40) |
where
(41) |
It is also true that the coefficients of the terms sum to 1,
(42) |
which Bernoulli stated without proof.
Ramanujan gave a number of curious infinite sum identities involving Bernoulli numbers (Berndt 1994).
The older definition of the Bernoulli numbers, no longer in widespread use, defines using the equations
(43) |
for
(44) |
for (Whittaker and Watson 1990, p. 125). The Bernoulli numbers may be calculated from the integral
(45) |
and analytically from
(46) |
for n = 1, 2, ..., where is the Riemann zeta function.
The Bernoulli numbers are a superset of the archaic ones since
(47) |
The first few Bernoulli numbers are
(48) | |||
(49) | |||
(50) | |||
(51) | |||
(52) | |||
(53) | |||
(54) | |||
(55) | |||
(56) | |||
(57) | |||
(58) |
Agoh's Conjecture, Bernoulli Function, Bernoulli Number of the Second Kind, Bernoulli Polynomial, Debye Functions, Euler-Maclaurin Integration Formulas, Euler Number, Figurate Number Triangle, Genocchi Number, Integer Sequence Primes, Irregular Prime, Modified Bernoulli Number, Pascal's Triangle, Riemann Zeta Function, von Staudt-Clausen Theorem
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