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r, s, t-COLORINGS OF STARS

机译:r,s,t-星星的色彩

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摘要

Given non-negative integers r, s, and t, an [r, s, t]-coloring of a graph G with vertex set V(G) and edge set E (G) is a mapping c from V(G)UE(G) to the color set {0,1,... ,k- 1} such that |c(v_i)-c(v_i)| ≥ r every two adjacent vertices v_i,v_j, |c(e_i) - c(e_j)| ≥ s for any two adjacent edges e_i,e_j, and |c(v_i) - c(e_j)| ≥ t for all pairs of incident vertices and edges, respectively. The [r, s, t]-chromatic number χr,s,t{G) of G is defined to be the minimum k such that G admits an [r, s, t]-coloring. This is an obvious generalization of all classical graph colorings since c is a vertex coloring if r = 1, s = t = 0, an edge coloring if s = 1,r = i = 0, and a total coloring if r = s = t = l, respectively. In this paper, we completely determine the [r, s, t]-chromatic numbers for stars. Thus we obtain a lower bound for χr,s,t(G) for an arbitrary graph G that only depends on r, s, t and the maximum degree Δ(G).
机译:给定非负整数r,s和t,具有顶点集V(G)和边集E(G)的图G的[r,s,t]着色是来自V(G)UE的映射c (G)设置为颜色集{0,1,...,k-1},使得| c(v_i)-c(v_i)| ≥r每两个相邻的顶点v_i,v_j,| c(e_i)-c(e_j)|对于任意两个相邻边e_i,e_j和| c(v_i)-c(e_j)|≥s对于所有成对的入射顶点和边缘,≥t。 G的[r,s,t]色数χr,s,t {G)被定义为最小值k,使得G允许[r,s,t]色。这是所有经典图形着色的明显概括,因为如果r = 1,s = t = 0,则c是顶点着色;如果s = 1,r = i = 0,则是边缘着色;如果r = s = 0,则是总着色。 t = 1。在本文中,我们完全确定了恒星的[r,s,t]色数。因此,对于仅依赖于r,s,t和最大度数Δ(G)的任意图G,我们获得了χr,s,t(G)的下界。

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