TL;DR
This paper presents a detailed calculation of high-energy neutron flux at exascale supercomputing sites using Monte Carlo techniques, enabling better prediction and mitigation of radiation-induced errors in future supercomputers.
Contribution
It introduces a novel method to calculate neutron flux above 50 MeV considering atmospheric profiles, seasonal variations, and site-specific coefficients for improved error risk assessment.
Findings
Neutron flux varies seasonally and with atmospheric pressure.
Barometric coefficients for each site enable risk prediction.
Potential for improved error mitigation strategies in exascale computing.
Abstract
The age of exascale computing has arrived and the risks associated with neutron and other atmospheric radiation are becoming more critical as the computing power increases, hence, the expected Mean Time Between Failures will be reduced because of this radiation. In this work, a new and detailed calculation of the neutron flux for energies above 50 MeV is presented. This has been done by using state-of-the-art Monte Carlo astroparticle techniques and including real atmospheric profiles at each one of the next 23 exascale supercomputing facilities. Atmospheric impact in the flux and seasonal variations were observed and characterised, and the barometric coefficient for high-energy neutrons at each site was obtained. With these coefficients, potential risks of errors associated with the increase in the flux of energetic neutrons, such as the occurrence of single event upsets or transients,…
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