Steiner Shallow-Light Trees are Exponentially Lighter than Spanning Ones

Michael Elkin, Shay Solomon
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引用次数: 23

Abstract

For a pair of parameters $\alpha,\beta \ge 1$, a spanning tree $T$ of a weighted undirected $n$-vertex graph $G = (V,E,w)$ is called an \emph{$(\alpha,\beta)$-shallow-light tree} (shortly, $(\alpha,\beta)$-SLT)of $G$ with respect to a designated vertex $rt \in V$ if (1) it approximates all distances from $rt$ to the other vertices up to a factor of $\alpha$, and(2) its weight is at most $\beta$ times the weight of the minimum spanning tree $MST(G)$ of $G$. The parameter $\alpha$ (respectively, $\beta$) is called the \emph{root-distortion}(resp., \emph{lightness}) of the tree $T$. Shallow-light trees (SLTs) constitute a fundamental graph structure, with numerous theoretical and practical applications. In particular, they were used for constructing spanners, in network design, for VLSI-circuit design, for various data gathering and dissemination tasks in wireless and sensor networks, in overlay networks, and in the message-passing model of distributed computing. Tight tradeoffs between the parameters of SLTs were established by Awer buch et al.\ \cite{ABP90, ABP91} and Khuller et al.\ \cite{KRY93}. They showed that for any $\epsilon >, 0$there always exist $(1+\epsilon, O(\frac{1}{\epsilon}))$-SLTs, and that the upper bound $\beta = O(\frac{1}{\epsilon})$on the lightness of SLTs cannot be improved. In this paper we show that using Steiner points one can build SLTs with \emph{logarithmic lightness}, i.e., $\beta = O(\log \frac{1}{\epsilon})$. This establishes an \emph{exponential separation} between spanning SLTs and Steiner ones. One particularly remarkable point on our tradeoff curve is $\epsilon =0$. In this regime our construction provides a \emph{shortest-path tree} with weight at most $O(\log n) \cdot w(MST(G))$. Moreover, we prove matching lower bounds that show that all our results are tight up to constant factors. Finally, on our way to these results we settle (up to constant factors) a number of open questions that were raised by Khuller et al.\ \cite{KRY93} in SODA'93.
斯坦纳浅光树比生成树更轻
对于一对参数$\alpha,\beta \ge 1$,一个加权无向$n$ -顶点图$G = (V,E,w)$的生成树$T$被称为\emph{$(\alpha,\beta)$-浅光树}(简称$(\alpha,\beta)$ -SLT)的$G$相对于一个指定顶点$rt \in V$,如果(1)它将$rt$到其他顶点的所有距离近似为$\alpha$的一个因子,(2)其权值不超过$\beta$乘以$G$的最小生成树$MST(G)$的权值。参数$\alpha$(分别为$\beta$)称为\emph{根部变形}。, \emph{亮度})的树$T$。浅光树(SLTs)是一种基本的图结构,具有广泛的理论和实际应用。特别是,它们被用于构建扳手、网络设计、vlsi电路设计、无线和传感器网络中的各种数据收集和传播任务、覆盖网络以及分布式计算的消息传递模型。Awer buch等人\cite{ABP90, ABP91}和Khuller等人\cite{KRY93}建立了slt参数之间的紧密权衡。结果表明,对于任何$\epsilon >, 0$都存在$(1+\epsilon, O(\frac{1}{\epsilon}))$ - slt,并且slt的亮度上界$\beta = O(\frac{1}{\epsilon})$无法提高。在本文中,我们证明了使用斯坦纳点可以用\emph{对数亮度},即$\beta = O(\log \frac{1}{\epsilon})$来构建slt。这在跨越slt和Steiner之间建立了\emph{指数分离}。在我们的权衡曲线上,一个特别值得注意的点是$\epsilon =0$。在这种情况下,我们的结构提供了一个重量最多为$O(\log n) \cdot w(MST(G))$的\emph{最短路径树}。此外,我们证明了匹配下界,表明我们所有的结果都紧绷于常数因子。最后,在我们得出这些结果的过程中,我们解决了(直到常数因素)Khuller等人在SODA'93中提出的一些悬而未决的问题\cite{KRY93}。
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