Using gpu for modelling of self-gravitating systems
Abstract
We analyse the performance of graphic processor units in N-body simulations of self-gravitating systems. We find that it is possible to model dwarf galaxies on a one-to-one scale using available hardware. Refs 10. Figs 6.
Keywords:
dynamics of galaxies, GPU, N-body simulation
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Articles of "Vestnik of Saint Petersburg University. Mathematics. Mechanics. Astronomy" are open access distributed under the terms of the License Agreement with Saint Petersburg State University, which permits to the authors unrestricted distribution and self-archiving free of charge.