Cosmological Simulations in Exascale Era
December 01, 2017 ยท Declared Dead ยท ๐ arXiv.org
"No code URL or promise found in abstract"
Evidence collected by the PWNC Scanner
Authors
D. Goz, L. Tornatore, G. Taffoni, G. Murante
arXiv ID
1712.00252
Category
astro-ph.IM
Cross-listed
astro-ph.GA,
cs.DC,
cs.SE
Citations
3
Venue
arXiv.org
Last Checked
1 month ago
Abstract
The architecture of Exascale computing facilities, which involves millions of heterogeneous processing units, will deeply impact on scientific applications. Future astrophysical HPC applications must be designed to make such computing systems exploitable. The ExaNeSt H2020 EU-funded project aims to design and develop an exascale ready prototype based on low-energy-consumption ARM64 cores and FPGA accelerators. We participate to the design of the platform and to the validation of the prototype with cosmological N-body and hydrodynamical codes suited to perform large-scale, high-resolution numerical simulations of cosmic structures formation and evolution. We discuss our activities on astrophysical applications to take advantage of the underlying architecture.
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