In combinatorial mathematics, a partial permutation, or sequence without repetition, on a finite set Sis a bijection between two specified subsets of S. That is, it is defined by two subsets U and V of equal size, and a one-to-one mapping from U to V. Equivalently, it is a partial function on S that can be extended to a permutation.[1] [2]
It is common to consider the case when the set S is simply the set of the first n integers. In this case, a partial permutation may be represented by a string of n symbols, some of which are distinct numbers in the range from 1 to
n
◊◊, ◊1, ◊2, 1◊, 2◊, 12, 21.
The number of partial permutations on n items, for n = 0, 1, 2, ..., is given by the integer sequence
1, 2, 7, 34, 209, 1546, 13327, 130922, 1441729, 17572114, 234662231, ... where the nth item in the sequence is given by the summation formula
n | |
\sum | |
i=0 |
i!\binom{n}{i}2
P(n)=2nP(n-1)-(n-1)2P(n-2).
P(n-1)
P(n-1)
(n-1)P(n-1)
(n-1)P(n-1)
-(n-1)2P(n-2)
Some authors restrict partial permutations so that either the domain[4] or the range[3] of the bijection is forced to consist of the first k items in the set of n items being permuted, for some k. In the former case, a partial permutation of length k from an n-set is just a sequence of k terms from the n-set without repetition. (In elementary combinatorics, these objects are sometimes confusingly called "k-permutations" of the n-set.)