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Cosmological neutrino simulations at extreme scale

Emberson, JD, Yu, H-R, Inman, D, Zhang, T-J, Pen, U-L, Harnois-Déraps, J, Yuan, S, Teng, H-Y, Zhu, H-M, Chen, X and Xing, Z-Z (2017) Cosmological neutrino simulations at extreme scale. Research in Astronomy and Astrophysics, 17 (8). ISSN 1674-4527

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Constraining neutrino mass remains an elusive challenge in modern physics. Precision measurements are expected from several upcoming cosmological probes of large-scale structure. Achieving this goal relies on an equal level of precision from theoretical predictions of neutrino clustering. Numerical simulations of the non-linear evolution of cold dark matter and neutrinos play a pivotal role in this process. We incorporate neutrinos into the cosmological N-body code CUBEP3M and discuss the challenges associated with pushing to the extreme scales demanded by the neutrino problem. We highlight code optimizations made to exploit modern high performance computing architectures and present a novel method of data compression that reduces the phase-space particle footprint from 24 bytes in single precision to roughly 9 bytes. We scale the neutrino problem to the Tianhe-2 supercomputer and provide details of our production run, named TianNu, which uses 86% of the machine (13 824 compute nodes). With a total of 2.97 trillion particles, TianNu is currently the world's largest cosmological N-body simulation and improves upon previous neutrino simulations by two orders of magnitude in scale. We finish with a discussion of the unanticipated computational challenges that were encountered during the TianNu runtime.

Item Type: Article
Uncontrolled Keywords: 0201 Astronomical and Space Sciences
Subjects: Q Science > QB Astronomy
Q Science > QC Physics
Divisions: Astrophysics Research Institute
Publisher: IOP Publishing
Date Deposited: 23 Jul 2020 08:54
Last Modified: 04 Sep 2021 06:57
DOI or ID number: 10.1088/1674-4527/17/8/85
URI: https://researchonline.ljmu.ac.uk/id/eprint/13348
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