The relations are given as a (finite) binary relation R on Σ∗. To form the quotient monoid, these relations are extended to monoid congruences as follows:
First, one takes the symmetric closure R ∪ R−1 of R. This is then extended to a symmetric relation E ⊂ Σ∗ × Σ∗ by defining x ~E y if and only if x = sut and y = svt for some strings u, v, s, t ∈ Σ∗ with (u,v) ∈ R ∪ R−1. Finally, one takes the reflexive and transitive closure of E, which then is a monoid congruence.
In the typical situation, the relation R is simply given as a set of equations, so that R = { u 1 = v 1 , … , u n = v n } {\displaystyle R=\{u_{1}=v_{1},\ldots ,u_{n}=v_{n}\}} . Thus, for example,
is the equational presentation for the bicyclic monoid, and
is the plactic monoid of degree 2 (it has infinite order). Elements of this plactic monoid may be written as a i b j ( b a ) k {\displaystyle a^{i}b^{j}(ba)^{k}} for integers i, j, k, as the relations show that ba commutes with both a and b.
Presentations of inverse monoids and semigroups can be defined in a similar way using a pair
where
is the free monoid with involution on X {\displaystyle X} , and
is a binary relation between words. We denote by T e {\displaystyle T^{\mathrm {e} }} (respectively T c {\displaystyle T^{\mathrm {c} }} ) the equivalence relation (respectively, the congruence) generated by T.
We use this pair of objects to define an inverse monoid
Let ρ X {\displaystyle \rho _{X}} be the Wagner congruence on X {\displaystyle X} , we define the inverse monoid
presented by ( X ; T ) {\displaystyle (X;T)} as
In the previous discussion, if we replace everywhere ( X ∪ X − 1 ) ∗ {\displaystyle ({X\cup X^{-1}})^{*}} with ( X ∪ X − 1 ) + {\displaystyle ({X\cup X^{-1}})^{+}} we obtain a presentation (for an inverse semigroup) ( X ; T ) {\displaystyle (X;T)} and an inverse semigroup I n v ⟨ X | T ⟩ {\displaystyle \mathrm {Inv} \langle X|T\rangle } presented by ( X ; T ) {\displaystyle (X;T)} .
A trivial but important example is the free inverse monoid (or free inverse semigroup) on X {\displaystyle X} , that is usually denoted by F I M ( X ) {\displaystyle \mathrm {FIM} (X)} (respectively F I S ( X ) {\displaystyle \mathrm {FIS} (X)} ) and is defined by
or
Book and Otto, Theorem 7.1.7, p. 149 ↩