论文标题
最后的旅程。 I. Mira超级计算机上的极端尺度模拟
The Last Journey. I. An Extreme-Scale Simulation on the Mira Supercomputer
论文作者
论文摘要
最后的旅程是一个仅重力,宇宙学的N体模拟,在周期盒中演变出超过1.24万亿个颗粒,其侧面长度为5.025GPC。它是使用BG/Q系统MIRA上的HACC仿真和分析框架实现的。选择宇宙参数与普朗克卫星的结果一致。一系列分析工具已经在原位运行,以实现各种各样的科学项目,同时可以使产生的数据量可管理。从红移Z〜10开始生成分析输出,以允许在后处理中使用半分析建模方法来构建合成星系目录。作为我们原位分析管道的一部分,我们采用了一种新方法来跟踪光晕子结构,从而引入了Subhalo内核的概念。多波长合成天空图的产生通过原位产生颗粒灯杆的促进,也从Z〜10开始。我们提供了模拟设置和生成的数据产品的概述;提出了第一组分析结果。数据的一个子集已公开可用。
The Last Journey is a large-volume, gravity-only, cosmological N-body simulation evolving more than 1.24 trillion particles in a periodic box with a side-length of 5.025Gpc. It was implemented using the HACC simulation and analysis framework on the BG/Q system, Mira. The cosmological parameters are chosen to be consistent with the results from the Planck satellite. A range of analysis tools have been run in situ to enable a diverse set of science projects, and at the same time, to keep the resulting data amount manageable. Analysis outputs have been generated starting at redshift z~10 to allow for construction of synthetic galaxy catalogs using a semi-analytic modeling approach in post-processing. As part of our in situ analysis pipeline we employ a new method for tracking halo sub-structures, introducing the concept of subhalo cores. The production of multi-wavelength synthetic sky maps is facilitated by generating particle lightcones in situ, also beginning at z~10. We provide an overview of the simulation set-up and the generated data products; a first set of analysis results is presented. A subset of the data is publicly available.