PKDGRAV3: beyond trillion particle cosmological simulations for the next era of galaxy surveys

Douglas Potter, Joachim Stadel, Romain Teyssier
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引用次数: 149

Abstract

We report on the successful completion of a 2 trillion particle cosmological simulation to \(z=0\) run on the Piz Daint supercomputer (CSCS, Switzerland), using 4000+ GPU nodes for a little less than 80?h of wall-clock time or 350,000 node hours. Using multiple benchmarks and performance measurements on the US Oak Ridge National Laboratory Titan supercomputer, we demonstrate that our code PKDGRAV3, delivers, to our knowledge, the fastest time-to-solution for large-scale cosmological N-body simulations. This was made possible by using the Fast Multipole Method in conjunction with individual and adaptive particle time steps, both deployed efficiently (and for the first time) on supercomputers with GPU-accelerated nodes. The very low memory footprint of PKDGRAV3 allowed us to run the first ever benchmark with 8 trillion particles on Titan, and to achieve perfect scaling up to 18,000 nodes and a peak performance of 10 Pflops.

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PKDGRAV3:超越万亿粒子的宇宙学模拟,为下一个星系调查时代做准备
我们报告成功完成了2万亿粒子宇宙学模拟\(z=0\)运行在Piz Daint超级计算机(CSCS,瑞士)上,使用4000多个GPU节点,略低于80?H为挂钟时间或350,000个节点小时。使用美国橡树岭国家实验室泰坦超级计算机上的多个基准测试和性能测量,我们证明了我们的代码PKDGRAV3,据我们所知,提供了大规模宇宙n体模拟的最快求解时间。这是通过将快速多极方法与个体和自适应粒子时间步骤相结合,在具有gpu加速节点的超级计算机上有效地(也是第一次)部署而实现的。PKDGRAV3非常低的内存占用使我们能够在泰坦上运行第一个具有8万亿粒子的基准测试,并实现完美的扩展到18,000个节点和10 Pflops的峰值性能。
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