Clique-width

In graph theory, the clique-width of a graph G is the minimum number of labels needed to construct G by means of the following 4 operations :

  1. Creation of a new vertex v with label i ( noted i(v) )
  2. Disjoint union of two labeled graphs G and H ( denoted G \oplus H )
  3. Joining by an edge every vertex labeled i to every vertex labeled j (denoted η(i,j)), where i \neq j
  4. Renaming label i to label j ( denoted ρ(i,j) )

Cographs are exactly the graphs with clique-width at most 2;[1] every distance-hereditary graph has clique-width at most 3 while the clique-width of unit interval graphs is unbounded (based on their grid structure).[2] Similarly, the clique-width of bipartite permutation graphs is unbounded (based on similar grid structure).[3] Based on the characterization of cographs as the graphs without induced subgraph isomorphic to a chordless path with four vertices, the clique-width of many graph classes defined by forbidden induced subgraphs is classified.,[4][5] Many optimization problems that are NP-hard for more general classes of graphs may be solved efficiently by dynamic programming on graphs of bounded clique-width.[6][7] In particular, every graph property that can be expressed in MSO1 monadic second-order logic (a form of logic allowing quantification over sets of vertices) has a linear-time algorithm for graphs of bounded clique-width, by a form of Courcelle's theorem.[7]

The theory of graphs of bounded clique-width resembles that for graphs of bounded treewidth, but unlike treewidth allows for dense graphs. If a family of graphs has bounded clique-width, then either it has bounded treewidth or every complete bipartite graph is a subgraph of a graph in the family.[8] Treewidth and clique-width are also connected through the theory of line graphs: a family of graphs has bounded treewidth if and only if their line graphs have bounded clique-width.[9]

See also

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References

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