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Macro-star networks: efficient low-degree alternatives to star graphs

机译:巨星网络:星图的有效低度替代

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We propose a new class of interconnection networks, called macro-star networks, which belong to the class of Cayley graphs and use the star graph as a basic building module. A macro-star network can have node degree that is considerably smaller than that of a star graph of the same size, and diameter that is sublogarithmic and asymptotically within a factor of 1.25 from a universal lower bound (given its node degree). We show that algorithms developed for star graphs can be emulated on suitably constructed macro-stars with asymptotically optimal slowdown. This enables us to obtain through emulation a variety of efficient algorithms for the macro-star network, thus proving its versatility. Basic communication tasks, such as the multimode broadcast and the total exchange, can be executed in macro-star networks in asymptotically optimal time under both the single-port and the all-port communication models. Moreover, no interconnection network with similar node degree can perform these communication tasks in time that is better by more than a constant factor than that required in a macro-star network. We show that macro-star networks can embed trees, meshes, hypercubes, as well as star, bubble-sort, and complete transposition graphs with constant dilation. We introduce several variants of the macro-star network that provide more flexibility in scaling up the number of nodes. We also discuss implementation issues and compare the new topology with the star graph and other popular topologies.
机译:我们提出了一种称为宏星网络的新型互连网络,该网络属于Cayley图类,并使用星图作为基本的构建模块。宏星形网络的节点度可以大大小于相同大小的星形图的节点度,并且其直径在从对数下限(给定其节点度)的1.25倍之内是对数次渐近的。我们表明,为星图开发的算法可以在渐近最优减慢的适当构造的宏观星上进行仿真。这使我们能够通过仿真获得多种适用于宏星网络的有效算法,从而证明其多功能性。在单端口和全端口通信模型下,基本通信任务(例如多模式广播和总交换)都可以在渐近最优时间在宏星网络中执行。而且,没有一个具有相似节点度的互连网络可以及时执行这些通信任务,而这些通信任务要比宏星网络所要求的时间要好一个常数。我们表明,巨星网络可以嵌入树,网格,超立方体以及恒星,气泡排序和具有恒定膨胀的完整换位图。我们介绍了巨星网络的几种变体,它们在扩展节点数量方面提供了更大的灵活性。我们还将讨论实现问题,并将新拓扑与星形图和其他流行拓扑进行比较。

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