Star Colouring of Bounded Degree Graphs and Regular Graphs

Abstract

A kk-star colouring of a graph GG is a function f:V(G)β†’{0,1,…,kβˆ’1}f:V(G)\to\{0,1,\dots,k-1\} such that f(u)β‰ f(v)f(u)\neq f(v) for every edge uvuv of GG, and every bicoloured connected subgraph of GG is a star. The star chromatic number of GG, Ο‡s(G)\chi_s(G), is the least integer kk such that GG is kk-star colourable. We prove that Ο‡s(G)β‰₯⌈(d+4)/2βŒ‰\chi_s(G)\geq \lceil (d+4)/2\rceil for every dd-regular graph GG with dβ‰₯3d\geq 3. We reveal the structure and properties of even-degree regular graphs GG that attain this lower bound. The structure of such graphs GG is linked with a certain type of Eulerian orientations of GG. Moreover, this structure can be expressed in the LC-VSP framework of Telle and Proskurowski (SIDMA, 1997), and hence can be tested by an FPT algorithm with the parameter either treewidth, cliquewidth, or rankwidth. We prove that for pβ‰₯2p\geq 2, a 2p2p-regular graph GG is (p+2)(p+2)-star colourable only if n:=∣V(G)∣n:=|V(G)| is divisible by (p+1)(p+2)(p+1)(p+2). For each pβ‰₯2p\geq 2 and nn divisible by (p+1)(p+2)(p+1)(p+2), we construct a 2p2p-regular Hamiltonian graph on nn vertices which is (p+2)(p+2)-star colourable. The problem kk-STAR COLOURABILITY takes a graph GG as input and asks whether GG is kk-star colourable. We prove that 3-STAR COLOURABILITY is NP-complete for planar bipartite graphs of maximum degree three and arbitrarily large girth. Besides, it is coNP-hard to test whether a bipartite graph of maximum degree eight has a unique 3-star colouring up to colour swaps. For kβ‰₯3k\geq 3, kk-STAR COLOURABILITY of bipartite graphs of maximum degree kk is NP-complete, and does not even admit a 2o(n)2^{o(n)}-time algorithm unless ETH fails

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