Some values of Ramsey numbers for C-4 versus stars

Some values of Ramsey numbers for C-4 versus stars
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C4 与恒星的拉姆齐数的一些值

DOI:
10.1016/j.ffa.2016.11.012
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发表时间:
2017
影响因子:
1
通讯作者:
Cheng T. C. Edwin
Cheng T. C. Edwin
中科院分区:
数学2区
文献类型:
--
作者:
Zhang Xuemei;Chen Yaojun;Cheng T. C. Edwin

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对于给定的两个图G1和G2,Ramsey数R(G1,G2)是最小的整数N,使得对于任意N阶图,要么G包含G1的拷贝,要么它的补图包含G2的拷贝.设Cm是长为m的圈,K1,n是n+ 1阶星星. Parsons(1975)[6]证明了对于所有n≥ 2,R(C4,K1,n)≤ n+<$n− 1 <$+ 2,并且当n是素数幂的平方时等式成立。设q为素数幂。本文首先利用Galois域Fq构造了一个不含C4的q2 - 1个顶点的图Γ q,然后证明了R(C 4,K 1,(q− 1)2+ t)=(q− 1)2+ q+ t,其中q≥ 4为偶数,t= 1,0,− 2,R(C 4,K 1,q(q− 1)− t)= q 2− t,其中q≥ 5为奇数,t= 2,4,.,2004年4月。
For two given graphs G 1 and G 2, the Ramsey number R (G 1, G 2) is the smallest integer N such that for any graph of order N, either G contains a copy of G 1 or its complement contains a copy of G 2. Let C m be a cycle of length m and K 1, n a star of order n+ 1. Parsons (1975)[6] shows that R (C 4, K 1, n)≤ n+⌊ n− 1⌋+ 2 for all n≥ 2 and the equality holds if n is the square of a prime power. Let q be a prime power. In this paper, we first construct a graph Γ q on q 2− 1 vertices without C 4 by using the Galois field F q, and then we prove that R (C 4, K 1,(q− 1) 2+ t)=(q− 1) 2+ q+ t for q≥ 4 is even and t= 1, 0,− 2, and R (C 4, K 1, q (q− 1)− t)= q 2− t for q≥ 5 is odd and t= 2, 4,..., 2⌈ q 4⌉.