Given a graph G and a coloring of its edges, a subgraph of G is called rainbow if its edges have distinct colors. The rainbow girth of an edge coloring of G is the minimum length of a rainbow cycle in G. A generalization of the famous Caccetta-Haggkvist conjecture (CHC), proposed by the first author, is that if G has n vertices, G is n-edge-colored and the size of every color class is k, then the rainbow girth is at most \lceil \frac{n}{k} \rceil. In the only known example showing sharpness of this conjecture, that stems from an example for the sharpness of CHC, the color classes are stars. This suggests that in the antipodal case to stars, namely matchings, the result can be improved. Indeed, we show that the rainbow girth of n matchings of size at least 2 is O(\log n), as compared with the general bound of \lceil \frac{n}{2} \rceil.
翻译:根据图表 G 及其边缘的颜色, G 的子集称为彩虹, 如果它的边缘有不同的颜色。 G 的边缘色的彩虹亮度是 G 中彩虹周期最小长度。 第一作者提出的著名的 Caccetta- Haggkvist 的光学猜想(CHC) 的概括性表示, 如果 G 有 n 的 脊椎, G 是 正对色的, 并且每个彩色等级的大小是 k, 那么彩虹的亮度最多为\ lcel\ frac{n{ { { }\ rce}\ rceil。 在唯一已知显示这种猜想的亮度的例子中, 彩色等级是恒星的亮度。 这意味着, 在恒星的抗波体中, 即匹配, 结果是可以改进的。 事实上, 我们显示, 与\ lceil\ frac2}\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\\