The ABACUS cosmological N-body code

被引:94
作者
Garrison, Lehman H. [1 ]
Eisenstein, Daniel J. [2 ]
Ferrer, Douglas [2 ]
Maksimova, Nina A. [2 ]
Pinto, Philip A. [3 ]
机构
[1] Simons Fdn, Ctr Computat Astrophys, Flatiron Inst, 162 Fifth Ave, New York, NY 10010 USA
[2] Harvard & Smithsonian, Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
[3] Univ Arizona, Steward Observ, 933 N Cherry Ave, Tucson, AZ 85121 USA
关键词
methods: numerical; cosmology: theory; GALAXY CORRELATION-FUNCTION; DARK-MATTER; SIMULATIONS; CATALOGS; DESIGN;
D O I
10.1093/mnras/stab2482
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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/r(2) 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.
引用
收藏
页码:575 / 596
页数:22
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