The abacus cosmological N-body code

ABSTRACT We present abacus, a fast and accurate cosmological N-body code based on a new method for calculating the gravitational potential from a static multipole mesh. The method analytically separates the near- and far-field forces, reducing the former to direct 1/r2 summation and the latter to a...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2021-11, Vol.508 (1), p.575-596
Hauptverfasser: Garrison, Lehman H, Eisenstein, Daniel J, Ferrer, Douglas, Maksimova, Nina A, Pinto, Philip A
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Sprache:eng
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Zusammenfassung:ABSTRACT We present abacus, a fast and accurate cosmological N-body code based on a new method for calculating the gravitational potential from a static multipole mesh. The method analytically separates the near- and far-field forces, reducing the former to direct 1/r2 summation and the latter to a discrete convolution over multipoles. The method achieves 70 million particle updates per second per node of the Summit supercomputer, while maintaining a median fractional force error of 10−5. We express the simulation time-step as an event-driven ‘pipeline’, incorporating asynchronous events such as completion of co-processor work, input/output, and network communication. abacus has been used to produce the largest suite of N-body simulations to date, the abacussummit suite of 60 trillion particles, incorporating on-the-fly halo finding. abacus enables the production of mock catalogues of the volume and resolution required by the coming generation of cosmological surveys.
ISSN:0035-8711
1365-2966
DOI:10.1093/mnras/stab2482