The ExaNeSt and EuroExa H2020 EU-funded projects aim to design and develop an exascale ready computing platform prototype based on low-energy-consumption ARM64 cores and FPGA accelerators. We participate in the application-driven design of the hardware solutions and prototype validation. To carry on this work we are using, among others, Hy-Nbody, a state-of-the-art direct N-body code. Core algorithms of Hy-Nbody have been improved in such a way to increasingly fit them to the exascale target platform. Waiting for the ExaNest prototype release, we are performing tests and code tuning operations on an ARM64 SoC facility: a SLURM managed HPC cluster based on 64-bit ARMv8 Cortex-A72/Cortex-A53 core design and powered by a Mali-T864 embedded GPU. In parallel, we are porting a kernel of Hy-Nbody on FPGA aiming to test and compare the performance-per-watt of our algorithms on different platforms. In this paper we describe how we re-engineered the application and we show first results on ARM SoC.
Cite
@article{arxiv.1812.00367,
title = {Astrophysical code migration into Exascale Era},
author = {David Goz and Sara Bertocco and Luca Tornatore and Giuliano Taffoni},
journal= {arXiv preprint arXiv:1812.00367},
year = {2018}
}
Comments
4 pages, 1 figure, 1 table; proceedings of ADASS XXVIII, accepted by ASP Conference Series