Bell number

Partitions of sets can be arranged in a partial order, showing that each partition of a set of size n "uses" one of the partitions of a set of size n-1.

The 52 partitions of a set with 5 elements

In general, B_n is the number of partitions of a set of size n. A partition of a set S is defined as a family of nonempty, pairwise disjoint subsets of S whose union is S. For example, B₃ = 5 because the 3-element set {a, b, c} can be partitioned in 5 distinct ways:

{ {a}, {b}, {c} }

{ {a}, {b, c} }

{ {b}, {a, c} }

{ {c}, {a, b} }

{ {a, b, c} }.

As suggested by the set notation above, the ordering of subsets within the family is not considered; ordered partitions are counted by a different sequence of numbers, the ordered Bell numbers. B₀ is 1 because there is exactly one partition of the empty set. This partition is itself the empty set; it can be interpreted as a family of subsets of the empty set, consisting of zero subsets. It is vacuously true that all of the subsets in this family are non-empty subsets of the empty set and that they are pairwise disjoint subsets of the empty set, because there are no subsets to have these unlikely properties.

The partitions of a set correspond one-to-one with its equivalence relations. These are binary relations that are reflexive, symmetric, and transitive. The equivalence relation corresponding to a partition defines two elements as being equivalent when they belong to the same partition subset as each other. Conversely, every equivalence relation corresponds to a partition into equivalence classes.[2] Therefore, the Bell numbers also count the equivalence relations.

If a number N is a squarefree positive integer (meaning that it is the product of some number n of distinct prime numbers), then B_n gives the number of different multiplicative partitions of N. These are factorizations of N into numbers greater than one, treating two factorizations as the same if they have the same factors in a different order.[3] For instance, 30 is the product of the three primes 2, 3, and 5, and has B₃ = 5 factorizations:

${\displaystyle 30=2\times 15=3\times 10=5\times 6=2\times 3\times 5}$

The Bell numbers also count the rhyme schemes of an n-line poem or stanza. A rhyme scheme describes which lines rhyme with each other, and so may be interpreted as a partition of the set of lines into rhyming subsets. Rhyme schemes are usually written as a sequence of Roman letters, one per line, with rhyming lines given the same letter as each other, and with the first lines in each rhyming set labeled in alphabetical order. Thus, the 15 possible four-line rhyme schemes are AAAA, AAAB, AABA, AABB, AABC, ABAA, ABAB, ABAC, ABBA, ABBB, ABBC, ABCA, ABCB, ABCC, and ABCD.[1]

The Bell numbers come up in a card shuffling problem mentioned in the addendum to Gardner (1978). If a deck of n cards is shuffled by repeatedly removing the top card and reinserting it anywhere in the deck (including its original position at the top of the deck), with exactly n repetitions of this operation, then there are nⁿ different shuffles that can be performed. Of these, the number that return the deck to its original sorted order is exactly B_n. Thus, the probability that the deck is in its original order after shuffling it in this way is B_n/nⁿ, which is significantly larger than the 1/n! probability that would describe a uniformly random permutation of the deck.

Related to card shuffling are several other problems of counting special kinds of permutations that are also answered by the Bell numbers. For instance, the nth Bell number equals the number of permutations on n items in which no three values that are in sorted order have the last two of these three consecutive. In a notation for generalized permutation patterns where values that must be consecutive are written adjacent to each other, and values that can appear non-consecutively are separated by a dash, these permutations can be described as the permutations that avoid the pattern 1-23. The permutations that avoid the generalized patterns 12-3, 32-1, 3-21, 1-32, 3-12, 21-3, and 23-1 are also counted by the Bell numbers.[4] The permutations in which every 321 pattern (without restriction on consecutive values) can be extended to a 3241 pattern are also counted by the Bell numbers.[5] However, the Bell numbers grow too quickly to count the permutations that avoid a pattern that has not been generalized in this way: by the (now proven) Stanley–Wilf conjecture, the number of such permutations is singly exponential, and the Bell numbers have a higher asymptotic growth rate than that.

The Bell numbers satisfy a recurrence relation involving binomial coefficients:[7]

${\displaystyle B_{n+1}=\sum _{k=0}^{n}{\binom {n}{k}}B_{k}.}$

It can be explained by observing that, from an arbitrary partition of n + 1 items, removing the set containing the first item leaves a partition of a smaller set of k items for some number k that may range from 0 to n. There are ${\displaystyle {\tbinom {n}{k}}}$ choices for the k items that remain after one set is removed, and B_k choices of how to partition them.

A different summation formula represents each Bell number as a sum of Stirling numbers of the second kind

${\displaystyle B_{n}=\sum _{k=0}^{n}\left\{{n \atop k}\right\}.}$

The Stirling number ${\displaystyle \left\{{n \atop k}\right\}}$ is the number of ways to partition a set of cardinality n into exactly k nonempty subsets. Thus, in the equation relating the Bell numbers to the Stirling numbers, each partition counted on the left hand side of the equation is counted in exactly one of the terms of the sum on the right hand side, the one for which k is the number of sets in the partition.[8]

Spivey (2008) has given a formula that combines both of these summations:

${\displaystyle B_{n+m}=\sum _{k=0}^{n}\sum _{j=0}^{m}\left\{{m \atop j}\right\}{n \choose k}j^{n-k}B_{k}.}$

The exponential generating function of the Bell numbers is

${\displaystyle B(x)=\sum _{n=0}^{\infty }{\frac {B_{n}}{n!}}x^{n}=e^{e^{x}-1}.}$

In this formula, the summation in the middle is the general form used to define the exponential generating function for any sequence of numbers, and the formula on the right is the result of performing the summation in the specific case of the Bell numbers.

One way to derive this result uses analytic combinatorics, a style of mathematical reasoning in which sets of mathematical objects are described by formulas explaining their construction from simpler objects, and then those formulas are manipulated to derive the combinatorial properties of the objects. In the language of analytic combinatorics, a set partition may be described as a set of nonempty urns into which elements labelled from 1 to n have been distributed, and the combinatorial class of all partitions (for all n) may be expressed by the notation

${\displaystyle \mathrm {S\scriptstyle ET} (\mathrm {S\scriptstyle ET} _{\geq 1}({\mathcal {Z}})).}$

Here, ${\displaystyle {\mathcal {Z}}}$ is a combinatorial class with only a single member of size one, an element that can be placed into an urn. The inner ${\displaystyle \mathrm {S\scriptstyle ET} _{\geq 1}}$ operator describes a set or urn that contains one or more labelled elements, and the outer ${\displaystyle \mathrm {S\scriptstyle ET} }$ describes the overall partition as a set of these urns. The exponential generating function may then be read off from this notation by translating the ${\displaystyle \mathrm {S\scriptstyle ET} }$ operator into the exponential function and the nonemptiness constraint ≥1 into subtraction by one.[9]

An alternative method for deriving the same generating function uses the recurrence relation for the Bell numbers in terms of binomial coefficients to show that the exponential generating function satisfies the differential equation ${\displaystyle B'(x)=e^{x}B(x)}$. The function itself can be found by solving this equation.[10][11][12]

The Bell numbers satisfy Dobinski's formula[13][10][12]

${\displaystyle B_{n}={\frac {1}{e}}\sum _{k=0}^{\infty }{\frac {k^{n}}{k!}}.}$

This formula can be derived by expanding the exponential generating function using the Taylor series for the exponential function, and then collecting terms with the same exponent.[9] It allows B_n to be interpreted as the nth moment of a Poisson distribution with expected value 1.

The nth Bell number is also the sum of the coefficients in the nth complete Bell polynomial, which expresses the nth moment of any probability distribution as a function of the first n cumulants.

The Bell numbers obey Touchard's congruence: If p is any prime number then[14]

${\displaystyle B_{p+n}\equiv B_{n}+B_{n+1}{\pmod {p}}}$

or, generalizing[15]

${\displaystyle B_{p^{m}+n}\equiv mB_{n}+B_{n+1}{\pmod {p}}.}$

Because of Touchard's congruence, the Bell numbers are periodic modulo p, for every prime number p; for instance, for p = 2, the Bell numbers repeat the pattern odd-odd-even with period three. The period of this repetition, for an arbitrary prime number p, must be a divisor of

${\displaystyle {\frac {p^{p}-1}{p-1}}}$

and for all prime p ≤ 101 and p = 113, 163, 167, or 173 it is exactly this number (sequence A001039 in the OEIS).[16][17]

The period of the Bell numbers to modulo n are

1, 3, 13, 12, 781, 39, 137257, 24, 39, 2343, 28531167061, 156, 25239592216021, 411771, 10153, 48, 51702516367896047761, 39, 109912203092239643840221, 9372, 1784341, 85593501183, 949112181811268728834319677753, 312, 3905, 75718776648063, 117, 1647084, 91703076898614683377208150526107718802981, 30459, 568972471024107865287021434301977158534824481, 96, 370905171793, 155107549103688143283, 107197717, 156, ... (sequence A054767 in the OEIS)

An application of Cauchy's integral formula to the exponential generating function yields the complex integral representation

${\displaystyle B_{n}={\frac {n!}{2\pi ie}}\int _{\gamma }{\frac {e^{e^{z}}}{z^{n+1}}}\,dz.}$

Some asymptotic representations can then be derived by a standard application of the method of steepest descent.[18]

The Bell numbers form a logarithmically convex sequence. Dividing them by the factorials, B_n/n!, gives a logarithmically concave sequence.[19][20][21]

Several asymptotic formulas for the Bell numbers are known. In Berend & Tassa (2010) the following bounds were established:

${\displaystyle B_{n}<\left({\frac {0.792n}{\ln(n+1)}}\right)^{n}}$ for all positive integers ${\displaystyle n}$;

moreover, if ${\displaystyle \varepsilon >0}$ then for all ${\displaystyle n>n_{0}(\varepsilon )}$,

${\displaystyle B_{n}<\left({\frac {e^{-0.6+\varepsilon }n}{\ln(n+1)}}\right)^{n}}$

where ${\displaystyle ~n_{0}(\varepsilon )=\max \left\{e^{4},d^{-1}(\varepsilon )\right\}~}$ and ${\displaystyle ~d(x):=\ln \ln(x+1)-\ln \ln x+{\frac {1+e^{-1}}{\ln x}}\,.}$ The Bell numbers can also be approximated using the Lambert W function, a function with the same growth rate as the logarithm, as [22]

${\displaystyle B_{n}\sim {\frac {1}{\sqrt {n}}}\left({\frac {n}{W(n)}}\right)^{n+{\frac {1}{2}}}\exp \left({\frac {n}{W(n)}}-n-1\right).}$

Moser & Wyman (1955) established the expansion

${\displaystyle B_{n+h}={\frac {(n+h)!}{W(n)^{n+h}}}\times {\frac {\exp(e^{W(n)}-1)}{(2\pi B)^{1/2}}}\times \left(1+{\frac {P_{0}+hP_{1}+h^{2}P_{2}}{e^{W(n)}}}+{\frac {Q_{0}+hQ_{1}+h^{2}Q_{2}+h^{3}Q_{3}+h^{4}Q_{4}}{e^{2W(n)}}}+O(e^{-3W(n)})\right)}$

uniformly for ${\displaystyle h=O(\ln(n))}$ as ${\displaystyle n\rightarrow \infty }$, where ${\displaystyle B}$ and each ${\displaystyle P_{i}}$ and ${\displaystyle Q_{i}}$ are known expressions in ${\displaystyle W(n)}$.[23]

The asymptotic expression

${\displaystyle {\begin{aligned}{\frac {\ln B_{n}}{n}}&=\ln n-\ln \ln n-1+{\frac {\ln \ln n}{\ln n}}+{\frac {1}{\ln n}}+{\frac {1}{2}}\left({\frac {\ln \ln n}{\ln n}}\right)^{2}+O\left({\frac {\ln \ln n}{(\ln n)^{2}}}\right)\\&{}\qquad {\text{as }}n\to \infty \end{aligned}}}$

was established by de Bruijn (1981).