Bernoulli Number — Definition, Formula & Examples
Bernoulli numbers are a specific sequence of rational numbers that appear naturally in formulas for sums of integer powers, in the Taylor series of certain functions, and throughout number theory.
The Bernoulli numbers are the sequence of rational numbers defined by the exponential generating function , or equivalently by the recursion for , with .
Key Formula
Where:
- = The $n$th Bernoulli number
- = Initial value, equal to 1
- = Binomial coefficient
How It Works
You can compute Bernoulli numbers one at a time using the recursion. Start with , then for each , solve for . This gives . All odd-indexed Bernoulli numbers beyond are zero, so in practice you only need to track even indices.
Worked Example
Problem: Compute the Bernoulli numbers B₀, B₁, and B₂ using the recursive formula.
B₀: By definition, the first Bernoulli number is
B₁: For n = 1, solve the equation involving the sum with k = 0 to 1:
B₂: For n = 2, sum over k = 0 and k = 1:
Answer: , , . The sequence continues , , and so on.
Why It Matters
Bernoulli numbers give closed-form expressions for power sums like via Faulhaber's formulas. They also appear in the Euler–Maclaurin summation formula and connect to the Riemann zeta function at negative integers, making them central to analytic number theory.
Common Mistakes
Mistake: Confusing the two sign conventions for B₁. Some textbooks define B₁ = +1/2 instead of −1/2.
Correction: Check which convention your course uses. The generating function gives , while the alternative shifts to . Both are standard.
