Definition 6.4.1 Permutation.
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A permutation is a function \(f:X \to X\) for some set \(X\) such that \(f\) is onto and one-to-one. In other words, a permutation is a bijection from a set to itself. Equivalently, a permutation is a function whose rule is a pairing of a set with itself. For example, the function \(h: \mathbb{R} \to \mathbb{R}\) defined by \(h(x) = 3x\) is a permutation, as we saw in ExampleΒ 6.3.34.
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We are often interested in a permutation of the set \(\{1,2,\ldots,n\}\) for some positive integer \(n\text{.}\) We can describe such permutations by listing the values, drawing the standard dot diagram, or using 2-line notation\begin{equation*} \alpha = \left(\begin{array}{ccc cc} 1 \amp 2 \amp 3 \amp \ldots \amp n \\ \alpha(1) \amp \alpha(2) \amp \alpha(3) \amp \ldots \amp \alpha(n) \end{array} \right) \end{equation*}For example, if \(\sigma: \{1,2,3,4\} \to \{1,2,3,4\}\) is the permutation defined by \(\sigma(1)=2\text{,}\) \(\sigma(2)=3\text{,}\) \(\sigma(3)=4\text{,}\) and \(\sigma(4)=1\text{,}\) then we write\begin{equation*} \sigma = \left(\begin{array}{ccc c} 1 \amp 2 \amp 3 \amp 4 \\ 2 \amp 3 \amp 4 \amp 1 \end{array} \right)\text{.} \end{equation*}In the 2-line notation, the first line is always \(1 2 3 \ldots n\) and the second line contains each of \(1, 2, 3, \ldots, n\) exactly once.
