title: Bernoulli number
text: In mathematics, the Bernoulli numbers  are a sequence of rational numbers which occur frequently in analysis. The Bernoulli numbers appear in (and can be defined by) the Taylor series expansions of the tangent and hyperbolic tangent functions, in Faulhaber's formula for the sum of m-th powers of the first n positive integers, in the Euler–Maclaurin formula, and in expressions for certain values of the Riemann zeta function.
  
  The values of the first 20 Bernoulli numbers are given in the adjacent table. Two conventions are used in the literature, denoted here by  and ; they differ only for , where  and . For every odd , . For every even ,  is negative if  is divisible by 4 and positive otherwise. The Bernoulli numbers are special values of the Bernoulli polynomials , with  and .
  
  The Bernoulli numbers were discovered around the same time by the Swiss mathematician Jacob Bernoulli, after whom they are named, and independently by Japanese mathematician Seki Takakazu.  Seki's discovery was posthumously published in 1712 in his work Katsuyō Sanpō; Bernoulli's, also posthumously, in his Ars Conjectandi of 1713.  Ada Lovelace's note G on the Analytical Engine from 1842 describes an algorithm for generating Bernoulli numbers with Babbage's machine. As a result, the Bernoulli numbers have the distinction of being the subject of the first published complex computer program.
  
  Notation
  The superscript  used in this article distinguishes the two sign conventions for Bernoulli numbers. Only the  term is affected: 
    with  ( / ) is the sign convention prescribed by NIST and most modern textbooks.
    with  ( / ) was used in the older literature, and (since 2022) by Donald Knuth following Peter Luschny's "Bernoulli Manifesto".
  
  In the formulas below, one can switch from one sign convention to the other with the relation , or for integer  = 2 or greater, simply ignore it.
  
  Since  for all odd , and many formulas only involve even-index Bernoulli numbers, a few authors write "" instead of . This article does not follow that notation.
  
  History
  
  Early history 
  The Bernoulli numbers are rooted in the early history of the computation of sums of integer powers, which have been of interest to mathematicians since antiquity.
  
  Methods to calculate the sum of the first  positive integers, the sum of the squares and of the cubes of the first  positive integers were known, but there were no real 'formulas', only descriptions given entirely in words. Among the great mathematicians of antiquity to consider this problem were Pythagoras (c. 572–497 BCE, Greece), Archimedes (287–212 BCE, Italy), Aryabhata (b. 476, India), Abu Bakr al-Karaji (d. 1019, Persia) and Abu Ali al-Hasan ibn al-Hasan ibn al-Haytham (965–1039, Iraq).
  
  During the late sixteenth and early seventeenth centuries mathematicians made significant progress.  In the West Thomas Harriot (1560–1621) of England, Johann Faulhaber (1580–1635) of Germany, Pierre de Fermat (1601–1665) and fellow French mathematician Blaise Pascal (1623–1662) all played important roles.
  
  Thomas Harriot seems to have been the first to derive and write formulas for sums of powers using symbolic notation, but even he calculated only up to the sum of the fourth powers.  Johann Faulhaber gave formulas for sums of powers up to the 17th power in his 1631 Academia Algebrae, far higher than anyone before him, but he did not give a general formula.
  
  Blaise Pascal in 1654 proved Pascal's identity relating the sums of the th powers of the first  positive integers for .
  
  The Swiss mathematician Jakob Bernoulli (1654–1705) was the first to realize the existence of a single sequence of constants  which provide a uniform formula for all sums of powers.
  
  The joy Bernoulli experienced when he hit upon the pattern needed to compute quickly and easily the coefficients of his formula for the sum of the th powers for any positive integer  can be seen from his comment. He wrote:
  
  "With the help of this table, it took me less than half of a quarter of an hour to find that the tenth powers of the first 1000 numbers being added together will yield the sum 91,409,924,241,424,243,424,241,924,242,500."
  
  Bernoulli's result was published posthumously in Ars Conjectandi in 1713.  Seki Takakazu independently discovered the Bernoulli numbers and his result was published a year earlier, also posthumously, in 1712. However, Seki did not present his method as a formula based on a sequence of constants.
  
  Bernoulli's formula for sums of powers is the most useful and generalizable formulation to date. The coefficients in Bernoulli's formula are now called Bernoulli numbers, following a suggestion of Abraham de Moivre.
  
  Bernoulli's formula is sometimes called Faulhaber's formula after Johann Faulhaber who found remarkable ways to calculate sum of powers but never stated Bernoulli's formula. According to Knuth a rigorous proof of Faulhaber's formula was first published by Carl Jacobi in 1834. Knuth's in-depth study of Faulhaber's formula concludes (the nonstandard notation on the LHS is explained further on):
  
  "Faulhaber never discovered the Bernoulli numbers; i.e., he never realized that a single sequence of constants  ... would provide a uniform
  
  for all sums of powers. He never mentioned, for example, the fact that almost half of the coefficients turned out to be zero after he had converted his formulas for  from polynomials in  to polynomials in ."
  
  In the above Knuth meant ; instead using  the formula avoids subtraction:
  
  Reconstruction of "Summae Potestatum" 
  
  The Bernoulli numbers (n)/(n) were introduced by Jakob Bernoulli in the book Ars Conjectandi published posthumously in 1713 page 97. The main formula can be seen in the second half of the corresponding facsimile. The constant coefficients denoted , ,  and  by Bernoulli are mapped to the notation which is now prevalent as , , , . The expression  means  – the small dots are used as grouping symbols. Using today's terminology these expressions are falling factorial powers . The factorial notation  as a shortcut for  was not introduced until 100 years later. The integral symbol on the left hand side goes back to Gottfried Wilhelm Leibniz in 1675 who used it as a long letter  for "summa" (sum). The letter  on the left hand side is not an index of summation but gives the upper limit of the range of summation which is to be understood as . Putting things together, for positive , today a mathematician is likely to write Bernoulli's formula as:
  
   
  
  This formula suggests setting  when switching from the so-called 'archaic' enumeration which uses only the even indices 2, 4, 6... to the modern form (more on different conventions in the next paragraph). Most striking in this context is the fact that the falling factorial  has for  the value . Thus Bernoulli's formula can be written
   
  
  if , recapturing the value Bernoulli gave to the coefficient at that position.
  
  The formula for  in the first half of the quotation by Bernoulli above contains an error at the last term; it should be  instead of .
  
  Definitions 
  Many characterizations of the Bernoulli numbers have been found in the last 300 years, and each could be used to introduce these numbers.  Here only four of the most useful ones are mentioned:
  
   a recursive equation,
   an explicit formula,
   a generating function,
   an integral expression.
  
  For the proof of the equivalence of the four approaches.
  
  Recursive definition 
  The Bernoulli numbers obey the sum formulas
   
  where  and  denotes the Kronecker delta. Solving for  gives the recursive formulas
  
  Explicit definition 
  In 1893 Louis Saalschütz listed  a total of 38 explicit formulas for the Bernoulli numbers, usually giving some reference in the older literature. One of them is (for ):
  
  Generating function 
  The exponential generating functions are
  
  where the substitution is . If we let  and  then
  
  Then  and for  the m term in the series for  is:
  
  If
  
  then we find that
  
  showing that the values of  obey the recursive formula for the Bernoulli numbers .
  
  The (ordinary) generating function
   
  
  is an asymptotic series. It contains the trigamma function .
  
  Integral Expression 
  From the generating functions above, one can obtain the following integral formula for the even Bernoulli numbers:
  
  Bernoulli numbers and the Riemann zeta function 
  
  The Bernoulli numbers can be expressed in terms of the Riemann zeta function:
  
             for  .
  
  Here the argument of the zeta function is 0 or negative.
  
  By means of the zeta functional equation and the gamma reflection formula the following relation can be obtained:
  
   for  .
  
  Now the argument of the zeta function is positive.
  
  It then follows from  () and Stirling's formula that
    for  .
  
  Efficient computation of Bernoulli numbers 
  
  In some applications it is useful to be able to compute the Bernoulli numbers  through  modulo , where  is a prime; for example to test whether Vandiver's conjecture holds for , or even just to determine whether  is an irregular prime. It is not feasible to carry out such a computation using the above recursive formulae, since at least (a constant multiple of)  arithmetic operations would be required. Fortunately, faster methods have been developed which require only  operations (see big  notation).
  
  David Harvey describes an algorithm for computing Bernoulli numbers by computing  modulo  for many small primes , and then reconstructing  via the Chinese remainder theorem. Harvey writes that the asymptotic time complexity of this algorithm is  and claims that this implementation is significantly faster than implementations based on other methods. Using this implementation Harvey computed  for . Harvey's implementation has been included in SageMath since version 3.1. Prior to that, Bernd Kellner computed  to full precision for  in December 2002 and Oleksandr Pavlyk for  with Mathematica in April 2008.
  
  {| class=wikitable style="text-align:right"
  ! Computer !! Year !! n !! Digits*
  |-
  |align=left| J. Bernoulli || ~1689 || 10 || 1
  |-
  |align=left| L. Euler || 1748 || 30 || 8
  |- 
  |align=left| J. C. Adams || 1878 || 62 || 36
  |- 
  |align=left| D. E. Knuth, T. J. Buckholtz || 1967 ||  || 
  |- 
  |align=left| G. Fee, S. Plouffe || 1996 ||  || 
  |- 
  |align=left| G. Fee, S. Plouffe || 1996 ||  || 
  |- 
  |align=left| B. C. Kellner || 2002 ||  || 
  |- 
  |align=left| O. Pavlyk || 2008 ||  || 
  |- 
  |align=left| D. Harvey || 2008 ||  || 
  |}
  * Digits is to be understood as the exponent of 10 when  is written as a real number in normalized scientific notation.
  
  A possible algorithm for computing Bernoulli numbers in the Julia programming language is given by
  
  b    = Array{Float64}(undef, n+1)
  b[1] = 1
  b[2] = -0.5
  for m=2:n 
      for k=0:m
          for v=0:k
              b[m+1] += (-1)^v * binomial(k,v) * v^(m) / (k+1)
          end
      end
  end
  return b
  
  Applications of the Bernoulli numbers
  
  Asymptotic analysis 
  Arguably the most important application of the Bernoulli numbers in mathematics is their use in the Euler–Maclaurin formula. Assuming that  is a sufficiently often differentiable function the Euler–Maclaurin formula can be written as
  
   
  
  This formulation assumes the convention . Using the convention  the formula becomes
  
   
  
  Here  (i.e. the zeroth-order derivative of  is just ). Moreover, let  denote an antiderivative of . By the fundamental theorem of calculus,
  
   
  
  Thus the last formula can be further simplified to the following succinct form of the Euler–Maclaurin formula
  
   
  
  This form is for example the source for the important Euler–Maclaurin expansion of the zeta function
  
   
  
  Here  denotes the rising factorial power.
  
  Bernoulli numbers are also frequently used in other kinds of asymptotic expansions. The following example is the classical Poincaré-type asymptotic expansion of the digamma function .
  
  Sum of powers 
  
  Bernoulli numbers feature prominently in the closed form expression of the sum of the th powers of the first  positive integers. For  define
  
  This expression can always be rewritten as a polynomial in  of degree . The coefficients of these polynomials are related to the Bernoulli numbers by Bernoulli's formula:
   
  where  denotes the binomial coefficient.
  
  For example, taking  to be 1 gives the triangular numbers  .
  
  Taking  to be 2 gives the square pyramidal numbers  .
  
   
  
  Some authors use the alternate convention for Bernoulli numbers and state Bernoulli's formula in this way:
   
  
  Bernoulli's formula is sometimes called Faulhaber's formula after Johann Faulhaber who also found remarkable ways to calculate sums of powers.
  
  Faulhaber's formula was generalized by V. Guo and J. Zeng to a -analog.
  
  Taylor series
  The Bernoulli numbers appear in the Taylor series expansion of many trigonometric functions and hyperbolic functions.
  
  Tangent
  
   
  Cotangent
   
  
  Hyperbolic tangent
  
  Hyperbolic cotangent
  
  Laurent series
  The Bernoulli numbers appear in the following Laurent series:
  
  Digamma function:
  
  Use in topology 
  The Kervaire–Milnor formula for the order of the cyclic group of diffeomorphism classes of exotic -spheres which bound parallelizable manifolds involves Bernoulli numbers. Let  be the number of such exotic spheres for , then
  
  The Hirzebruch signature theorem for the  genus of a smooth oriented closed manifold of dimension 4n also involves Bernoulli numbers.
  
  Connections with combinatorial numbers 
  The connection of the Bernoulli number to various kinds of combinatorial numbers is based on the classical theory of finite differences and on the combinatorial interpretation of the Bernoulli numbers as an instance of a fundamental combinatorial principle, the inclusion–exclusion principle.
  
  Connection with Worpitzky numbers 
  The definition to proceed with was developed by Julius Worpitzky in 1883. Besides elementary arithmetic only the factorial function  and the power function  is employed. The signless Worpitzky numbers are defined as
  
   
  
  They can also be expressed through the Stirling numbers of the second kind
  
   
  
  A Bernoulli number is then introduced as an inclusion–exclusion sum of Worpitzky numbers weighted by the harmonic sequence 1, , , ...
  
   
  
  This representation has .
  
  Consider the sequence , . From Worpitzky's numbers ,  applied to  is identical to the Akiyama–Tanigawa transform applied to  (see Connection with Stirling numbers of the first kind). This can be seen via the table:
  
  {| style="text-align:center"
  |+ Identity ofWorpitzky's representation and Akiyama–Tanigawa transform
  |-
  |1|| || || || || ||0||1|| || || || ||0||0||1|| || || ||0||0||0||1|| || ||0||0||0||0||1|| 
  |-
  |1||−1|| || || || ||0||2||−2|| || || ||0||0||3||−3|| || ||0||0||0||4||−4|| || || || || || || 
  |-
  |1||−3||2|| || || ||0||4||−10||6|| || ||0||0||9||−21||12|| || || || || || || || || || || || || 
  |-
  |1||−7||12||−6|| || ||0||8||−38||54||−24|| || || || || || || || || || || || || || || || || || || 
  |-
  |1||−15||50||−60||24|| || || || || || || || || || || || || || || || || || || || || || || || || 
  |-
  |}
  
  The first row represents .
  
  Hence for the second fractional Euler numbers  () /  ():
  
  A second formula representing the Bernoulli numbers by the Worpitzky numbers is for 
  
   
  
  The simplified second Worpitzky's representation of the second Bernoulli numbers is:
  
   () / () =  × () / ()
  
  which links the second Bernoulli numbers to the second fractional Euler numbers. The beginning is:
  
  The numerators of the first parentheses are  (see Connection with Stirling numbers of the first kind).
  
  Connection with Stirling numbers of the second kind 
  
  If one defines the Bernoulli polynomials  as:
  
  where  for  are the Bernoulli numbers.
  
  One also has the following for Bernoulli polynomials,
  
  The coefficient of  in  is .
  
  Comparing the coefficient of  in the two expressions of Bernoulli polynomials, one has:
  
   
  
  (resulting in ) which is an explicit formula for Bernoulli numbers and can be used to prove Von-Staudt Clausen theorem.
  
  Connection with Stirling numbers of the first kind 
  The two main formulas relating the unsigned Stirling numbers of the first kind  to the Bernoulli numbers (with ) are
  
   
  
  and the inversion of this sum (for , )
  
   
  
  Here the number  are the rational Akiyama–Tanigawa numbers, the first few of which are displayed in the following table.
  
  {| class="wikitable" style="text-align=center"
  |+ Akiyama–Tanigawa number
  ! !!0!!1!!2!!3!!4
  |-
  ! 0 
  | 1 ||  ||  ||  || 
  |-
  ! 1 
  |  ||  ||  ||  || ...
  |-
  ! 2 
  |  ||  ||  || ... || ...
  |-
  ! 3 
  | 0 ||  || ... || ... || ...
  |-
  ! 4 
  | − || ... || ... || ... || ...
  |}
  
  The Akiyama–Tanigawa numbers satisfy a simple recurrence relation which can be exploited to iteratively compute the Bernoulli numbers. This leads to the algorithm shown in the section 'algorithmic description' above. See /.
  
  An autosequence is a sequence which has its inverse binomial transform equal to the signed sequence. If the main diagonal is zeroes = , the autosequence is of the first kind. Example: , the Fibonacci numbers. If the main diagonal is the first upper diagonal multiplied by 2, it is of the second kind. Example: /, the second Bernoulli numbers (see ). The Akiyama–Tanigawa transform applied to  = 1/ leads to  (n) /  (n + 1). Hence:
  
  {| class="wikitable" style="text-align:center"
  |+ Akiyama–Tanigawa transform for the second Euler numbers
  |-
  !  !! 0 !! 1 !! 2 !! 3 !! 4
  |-
  ! 0
  | 1 ||  ||  ||  || 
  |-
  ! 1 
  |  ||  ||  ||  || ...
  |-
  ! 2 
  | 0 ||  ||  || ... || ...
  |-
  ! 3 
  | − || − || ... || ... || ...
  |-
  ! 4 
  | 0 || ... || ... || ... || ...
  |}
  
  See  and .  () /  () are the second (fractional) Euler numbers and an autosequence of the second kind.
  
  ( = ) × (  = ) =  = .
  
  Also valuable for  /  (see Connection with Worpitzky numbers).
  
  Connection with Pascal's triangle
  There are formulas connecting Pascal's triangle to Bernoulli numbers
  
  where  is the determinant of a n-by-n Hessenberg matrix part of Pascal's triangle whose elements are: 
  
  Example:
  
  Connection with Eulerian numbers 
  There are formulas connecting Eulerian numbers  to Bernoulli numbers:
  
  Both formulae are valid for  if  is set to . If  is set to − they are valid only for  and  respectively.
  
  A binary tree representation
  The Stirling polynomials  are related to the Bernoulli numbers by . S. C. Woon described an algorithm to compute  as a binary tree:
  
  Woon's recursive algorithm (for ) starts by assigning to the root node . Given a node  of the tree, the left child of the node is  and the right child . A node  is written as  in the initial part of the tree represented above with ± denoting the sign of .
  
  Given a node  the factorial of  is defined as
  
  Restricted to the nodes  of a fixed tree-level  the sum of  is , thus
  
  For example:
  
  Integral representation and continuation
  
  The integral
   
  has as special values  for .
  
  For example,  and . Here,  is the Riemann zeta function, and  is the imaginary unit. Leonhard Euler (Opera Omnia, Ser. 1, Vol. 10, p. 351) considered these numbers and calculated
  
   
  
  Another similar integral representation is
  
  The relation to the Euler numbers and 
  
  The Euler numbers are a sequence of integers intimately connected with the Bernoulli numbers. Comparing the
  asymptotic expansions of the Bernoulli and the Euler numbers shows that the Euler numbers  are in magnitude approximately  times larger than the Bernoulli numbers . In consequence:
  
   
  
  This asymptotic equation reveals that  lies in the common root of both the Bernoulli and the Euler numbers. In fact  could be computed from these rational approximations.
  
  Bernoulli numbers can be expressed through the Euler numbers and vice versa. Since, for odd ,  (with the exception ), it suffices to consider the case when  is even.
  
  These conversion formulas express a connection between the Bernoulli and the Euler numbers. But more important, there is a deep arithmetic root common to both kinds of numbers, which can be expressed through a more fundamental sequence of numbers, also closely tied to . These numbers are defined for  as
  
  The magic of these numbers lies in the fact that they turn out to be rational numbers.  This was first proved by Leonhard Euler in a landmark paper De summis serierum reciprocarum (On the sums of series of reciprocals) and has fascinated mathematicians ever since. The first few of these numbers are
  
    ( / )
  
  These are the coefficients in the expansion of .
  
  The Bernoulli numbers and Euler numbers can be understood as special views of these numbers, selected from the sequence  and scaled for use in special applications.
  
   
  
  The expression [ even] has the value 1 if  is even and 0 otherwise (Iverson bracket).
  
  These identities show that the quotient of Bernoulli and Euler numbers at the beginning of this section is just the special case of  when  is even. The  are rational approximations to  and two successive terms always enclose the true value of . Beginning with  the sequence starts ( / ):
  
   
  
  These rational numbers also appear in the last paragraph of Euler's paper cited above.
  
  Consider the Akiyama–Tanigawa transform for the sequence  () /  ():
  
  {| class="wikitable" style="text-align:right;"
  ! 0 
  |1||||0||−||−||−||0
  |-
  ! 1 
  | || 1|| || 0|| −|| −||
  |-
  ! 2 
  | −|| || || || || ||
  |-
  ! 3 
  | −1|| −|| −|| || || ||
  |-
  ! 4 
  | || −|| −|| || || ||
  |-
  ! 5 
  | 8|| || || || || ||
  |-
  ! 6 
  | −|| || || || || ||
  |}
  
  From the second, the numerators of the first column are the denominators of Euler's formula. The first column is − × .
  
  An algorithmic view: the Seidel triangle
  
  The sequence Sn has another unexpected yet important property: The denominators of Sn+1 divide the factorial . In other words: the numbers , sometimes called Euler zigzag numbers, are integers.
  
    (). See ().
  
  Their exponential generating function is the sum of the secant and tangent functions.
  
   .
  
  Thus the above representations of the Bernoulli and Euler numbers can be rewritten in terms of this sequence as
  
  These identities make it easy to compute the Bernoulli and Euler numbers: the Euler numbers  are given immediately by  and the Bernoulli numbers  are fractions obtained from  by some easy shifting, avoiding rational arithmetic.
  
  What remains is to find a convenient way to compute the numbers . However, already in 1877 Philipp Ludwig von Seidel published an ingenious algorithm, which makes it simple to calculate .
  
  Start by putting 1 in row 0 and let  denote the number of the row currently being filled
  If  is odd, then put the number on the left end of the row  in the first position of the row , and fill the row from the left to the right, with every entry being the sum of the number to the left and the number to the upper
  At the end of the row duplicate the last number.
  If  is even, proceed similar in the other direction.
  
  Seidel's algorithm is in fact much more general (see the exposition of Dominique Dumont ) and was rediscovered several times thereafter.
  
  Similar to Seidel's approach D. E. Knuth and T. J. Buckholtz gave a recurrence equation for the numbers  and recommended this method for computing  and  'on electronic computers using only simple operations on integers'.
  
  V. I. Arnold rediscovered Seidel's algorithm and later Millar, Sloane and Young popularized Seidel's algorithm under the name boustrophedon transform.
  
  Triangular form:
  
  {| style="text-align:right"
  | || || || || || || 1|| || || || || || 
  |-
  | || || || || || 1|| || 1|| || || || || 
  |-
  | || || || || 2|| || 2|| || 1|| || || || 
  |-
  | || || || 2|| || 4|| || 5|| || 5|| || || 
  |-
  | || || 16|| || 16|| || 14|| || 10|| || 5|| || 
  |-
  | || 16|| || 32|| || 46|| || 56|| || 61|| || 61|| 
  |-
  |272|| ||272|| ||256|| ||224|| ||178|| ||122|| || 61
  |}
  
  Only , with one 1, and , with two 1s, are in the OEIS.
  
  Distribution with a supplementary 1 and one 0 in the following rows:
  
  {| style="text-align:right"
  | || || || || || || 1|| || || || || ||   
  |-
  | || || || || || 0|| || 1|| || || || || 
  |-
  | || || || || −1|| || −1|| ||  0|| || || || 
  |-
  | || || || 0|| || −1|| || −2|| || −2|| || || 
  |-
  | || ||  5|| ||  5|| ||  4|| ||  2|| ||  0|| || 
  |-
  | || 0|| || 5|| || 10|| || 14|| || 16|| || 16|| 
  |-
  |−61|| ||−61|| ||−56|| ||−46|| ||−32|| ||−16|| || 0
  |}
  
  This is , a signed version of . The main andiagonal is . The main diagonal is . The central column is . Row sums: 1, 1, −2, −5, 16, 61.... See . See the array beginning with 1, 1, 0, −2, 0, 16, 0 below.
  
  The Akiyama–Tanigawa algorithm applied to  () / () yields:
  
  {| style="text-align:right"
  | 1|| 1|| || 0|| −|| −|| −
  |-
  | 0|| 1|| || 1|| 0|| −
  |-
  | −1|| −1|| || 4|| 
  |-
  | 0|| −5|| −|| 1
  |-
  | 5|| 5|| −
  |-
  | 0|| 61
  |-
  | −61
  |}
  
  1. The first column is . Its binomial transform leads to:
  
  {| style="text-align:right"
  |-
  | 1|| 1|| 0|| −2|| 0|| 16|| 0
  |-
  |0||−1||−2||2||16||−16
  |-
  |−1||−1||4||14||−32
  |-
  |0||5||10||−46
  |-
  |5||5||−56
  |-
  |0||−61
  |-
  |−61
  |}
  
  The first row of this array is . The absolute values of the increasing antidiagonals are . The sum of the antidiagonals is 
  
  2. The second column is . Its binomial transform yields:
  
  {| style="text-align:right"
  |-
  | 1|| 2|| 2|| −4|| −16|| 32|| 272
  |-
  |1||0||−6||−12||48||240
  |-
  |−1||−6||−6||60||192
  |-
  |−5||0||66||32
  |-
  |5||66||66
  |-
  |61||0
  |-
  |−61
  |}
  
  The first row of this array is . The absolute values of the second bisection are the double of the absolute values of the first bisection.
  
  Consider the Akiyama-Tanigawa algorithm applied to  () / ( () = abs( ()) + 1 = .
  
  {| style="text-align:right"
  |1||2||2||||1||||
  |-
  |−1||0||||2||||0
  |-
  |−1||−3||−||3||
  |-
  |2||−3||−||−13
  |-
  |5||21||−
  |-
  |−16||45
  |-
  |−61
  |}
  
  The first column whose the absolute values are  could be the numerator of a trigonometric function.
  
   is an autosequence of the first kind (the main diagonal is ). The corresponding array is:
  
  {| style="text-align:right"
  |0||−1||−1||2||5||−16||−61
  |-
  |−1||0||3||3||−21||−45
  |-
  |1||3||0||−24||−24
  |-
  |2||−3||−24||0
  |-
  |−5||−21||24
  |-
  |−16||45
  |-
  |−61
  |}
  
  The first two upper diagonals are  =  × . The sum of the antidiagonals is  = 2 × (n + 1).
  
  − is an autosequence of the second kind, like for instance  / . Hence the array:
  
  {| style="text-align:right"
  |-
  |2||1||−1||−2||5||16||−61
  |-
  |−1||−2||−1||7||11||−77
  |-
  |−1||1||8||4||−88
  |-
  |2||7||−4||−92
  |-
  |5||−11||−88
  |-
  |−16||−77
  |-
  |−61
  |}
  
  The main diagonal, here , is the double of the first upper one, here . The sum of the antidiagonals is  = 2 × (1).  −  = 2 × .
  
  A combinatorial view: alternating permutations
  
  Around 1880, three years after the publication of Seidel's algorithm, Désiré André proved a now classic result of combinatorial analysis. Looking at the first terms of the Taylor expansion of the trigonometric functions
   and  André made a startling discovery.
  
  The coefficients are the Euler numbers of odd and even index, respectively. In consequence the ordinary expansion of  has as coefficients the rational numbers .
  
   
  
  André then succeeded by means of a recurrence argument to show that the alternating permutations of odd size are enumerated by the Euler numbers of odd index (also called tangent numbers) and the alternating permutations of even size by the Euler numbers of even index (also called secant numbers).
  
  Related sequences
  The arithmetic mean of the first and the second Bernoulli numbers are the associate Bernoulli numbers: 
  , , , , ,  / . Via the second row of its inverse Akiyama–Tanigawa transform , they lead to Balmer series  / .
  
  The Akiyama–Tanigawa algorithm applied to  () /  () leads to the Bernoulli numbers  / ,  / , or   without , named intrinsic Bernoulli numbers .
  
  {| style="text-align:center; padding-left; padding-right: 2em;"
  |-
  |1||||||||
  |-
  |||||||||
  |-
  |0||||||||
  |-
  |−||−||−||−||0
  |-
  |0||−||−||−||−
  |}
  
  Hence another link between the intrinsic Bernoulli numbers and the Balmer series via  ().
  
   () = 0, 2, 1, 6,... is a permutation of the non-negative numbers.
  
  The terms of the first row are f(n) = . 2, f(n) is an autosequence of the second kind. 3/2, f(n) leads by its inverse binomial transform to 3/2 −1/2 1/3 −1/4 1/5 ... = 1/2 + log 2.
  
  Consider g(n) = 1/2 – 1 / (n+2) = 0, 1/6, 1/4, 3/10, 1/3. The Akiyama-Tanagiwa transforms gives:
  
  {| style="text-align:center; padding-left; padding-right:2em;"
  |-
  |0||||||||||||...
  |-
  |−||−||−||−||−||−||...
  |-
  |0||−||−||−||−||−||...
  |-
  |||||||||0||−||...
  |}
  
  0, g(n), is an autosequence of the second kind.
  
  Euler  () /  () without the second term () are the fractional intrinsic Euler numbers  The corresponding Akiyama transform is:
  
  {| style="text-align:center; padding-left; padding-right: 2em;"
  |-
  |1||1||||||
  |-
  |0||||||||
  |-
  |−||−||0||||
  |-
  |0||−||−||−||−
  |-
  |||||−||−||−
  |}
  
  The first line is .  preceded by a zero is an autosequence of the first kind. It is linked to the Oresme numbers. The numerators of the second line are  preceded by 0. The difference table is:
  
  {| style="text-align:center; padding-left; padding-right: 2em;"
  |-
  |0||1||1||||||||
  |-
  |1||0||−||−||−||−||−
  |-
  |−1||−||0||||||||
  |}
  
  Arithmetical properties of the Bernoulli numbers
  
  The Bernoulli numbers can be expressed in terms of the Riemann zeta function as  for integers  provided for  the expression  is understood as the limiting value and the convention  is used. This intimately relates them to the values of the zeta function at negative integers. As such, they could be expected to have and do have deep arithmetical properties. For example, the Agoh–Giuga conjecture postulates that  is a prime number if and only if  is congruent to −1 modulo . Divisibility properties of the Bernoulli numbers are related to the ideal class groups of cyclotomic fields by a theorem of Kummer and its strengthening in the Herbrand-Ribet theorem, and to class numbers of real quadratic fields by Ankeny–Artin–Chowla.
  
  The Kummer theorems 
  The Bernoulli numbers are related to Fermat's Last Theorem (FLT) by Kummer's theorem, which says:
  
  If the odd prime  does not divide any of the numerators of the Bernoulli numbers  then  has no solutions in nonzero integers.
  
  Prime numbers with this property are called regular primes. Another classical result of Kummer are the following congruences.
  
  Let  be an odd prime and  an even number such that  does not divide . Then for any non-negative integer 
   
  
  A generalization of these congruences goes by the name of -adic continuity.
  
  -adic continuity
  
  If ,  and  are positive integers such that  and  are not divisible by  and , then
  
  Since , this can also be written
  
  where  and , so that  and  are nonpositive and not congruent to 1 modulo . This tells us that the Riemann zeta function, with  taken out of the Euler product formula, is continuous in the -adic numbers on odd negative integers congruent modulo  to a particular , and so can be extended to a continuous function  for all -adic integers  the -adic zeta function.
  
  Ramanujan's congruences 
  
  The following relations, due to Ramanujan, provide a method for calculating Bernoulli numbers that is more efficient than the one given by their original recursive definition:
  
  Von Staudt–Clausen theorem 
  
  The von Staudt–Clausen theorem was given by Karl Georg Christian von Staudt and Thomas Clausen independently in 1840. The theorem states that for every ,
   
  is an integer. The sum extends over all primes  for which  divides .
  
  A consequence of this is that the denominator of  is given by the product of all primes  for which  divides . In particular, these denominators are square-free and divisible by 6.
  
  Why do the odd Bernoulli numbers vanish? 
  The sum
  
  can be evaluated for negative values of the index . Doing so will show that it is an odd function for even values of , which implies that the  sum has only terms of odd index. This and the formula for the Bernoulli sum imply that  is 0 for  even and ; and that the term for  is cancelled by the subtraction.  The von Staudt–Clausen theorem combined with Worpitzky's representation also gives a combinatorial answer to this question (valid for n > 1).
  
  From the von Staudt–Clausen theorem it is known that for odd  the number  is an integer. This seems trivial if one knows beforehand that the integer in question is zero. However, by applying Worpitzky's representation one gets
  
   
  
  as a sum of integers, which is not trivial. Here a combinatorial fact comes to surface which explains the vanishing of the Bernoulli numbers at odd index. Let  be the number of surjective maps from } to }, then . The last equation can only hold if
  
   
  
  This equation can be proved by induction. The first two examples of this equation are
  
  ,
  .
  
  Thus the Bernoulli numbers vanish at odd index because some non-obvious combinatorial identities are embodied in the Bernoulli numbers.
  
  A restatement of the Riemann hypothesis 
  The connection between the Bernoulli numbers and the Riemann zeta function is strong enough to provide an alternate formulation of the Riemann hypothesis (RH) which uses only the Bernoulli numbers. In fact Marcel Riesz proved that the RH is equivalent to the following assertion:
  
  For every  there exists a constant  (depending on ) such that  as .
  
  Here  is the Riesz function
  
   
  
   denotes the rising factorial power in the notation of D. E. Knuth. The numbers  occur frequently in the study of the zeta function and are significant  because  is a -integer for primes  where  does not divide .  The  are called divided Bernoulli numbers.
  
  Generalized Bernoulli numbers
  The generalized Bernoulli numbers are certain algebraic numbers, defined similarly to the Bernoulli numbers, that are related to special values of Dirichlet -functions in the same way that Bernoulli numbers are related to special values of the Riemann zeta function.
  
  Let  be a Dirichlet character modulo . The generalized Bernoulli numbers attached to  are defined by
  
   
  
  Apart from the exceptional , we have, for any Dirichlet character , that  if .
  
  Generalizing the relation between Bernoulli numbers and values of the Riemann zeta function at non-positive integers, one has the for all integers :
  
   
  
  where  is the Dirichlet -function of .
  
  Eisenstein–Kronecker number
  
  Eisenstein–Kronecker numbers are an analogue of the generalized Bernoulli numbers for imaginary quadratic fields. They are related to critical L-values of Hecke characters.
  
  Appendix
  
  Assorted identities
  
  See also 
   Bernoulli polynomial
   Bernoulli polynomials of the second kind
   Bell number
   Euler number
   Genocchi number
   Kummer's congruences
   Poly-Bernoulli number
   Hurwitz zeta function
   Euler summation
   Stirling polynomial
   Sums of powers
  
  Notes
  
  References 
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  Footnotes
  
  External links
   
   The first 498 Bernoulli Numbers from Project Gutenberg
   A multimodular algorithm for computing Bernoulli numbers
   The Bernoulli Number Page
   Bernoulli number programs at LiteratePrograms
   
   
   
   
   
   
  
  Number theory
  Topology
  Integer sequences