On the complexity of reconstructing H‐free graphs from their Star Systems
On the complexity of reconstructing H‐free graphs from their Star Systems
复制标题
关于从恒星系统重建无 H 图的复杂性
DOI:
10.1002/jgt.20544
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发表时间:
2011
影响因子:
0.9
通讯作者:
J. A. Telle
中科院分区:
文献类型:
--
作者:
F. Fomin;Jan Kratochvíl;D. Lokshtanov;Federico Mancini;J. A. Telle
In the Star System problem we are given a set system and asked whether it is realizable by the multi‐set of closed neighborhoods of some graph, i.e. given subsets S1, S2, …, Sn of an n‐element set V does there exist a graph G = (V, E) with {N[v]: v∈V} = {S1, S2, …, Sn}? For a fixed graph H the H‐free Star System problem is a variant of the Star System problem where it is asked whether a given set system is realizable by closed neighborhoods of a graph containing no H as an induced subgraph. We study the computational complexity of the H‐free Star System problem. We prove that when H is a path or a cycle on at most four vertices the problem is polynomial time solvable. In complement to this result, we show that if H belongs to a certain large class of graphs the H‐free Star System problem is NP‐complete. In particular, the problem is NP‐complete when H is either a cycle or a path on at least five vertices. This yields a complete dichotomy for paths and cycles. Copyright © 2010 John Wiley & Sons, Ltd. 68:113‐124, 2011