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N-body simulations with two-orders-of-magnitude higher performance using wavelets

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arxiv astro-ph/0302343 v1 pith:BY4TU4N5 submitted 2003-02-18 astro-ph physics.comp-phphysics.plasm-ph

N-body simulations with two-orders-of-magnitude higher performance using wavelets

classification astro-ph physics.comp-phphysics.plasm-ph
keywords simulationsn-bodygalaxiesnoiseperformancewaveletswillavailable
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Noise is a problem of major concern for N-body simulations of structure formation in the early Universe, of galaxies and plasmas. Here for the first time we use wavelets to remove noise from N-body simulations of disc galaxies, and show that they become equivalent to simulations with two orders of magnitude more particles. We expect a comparable improvement in performance for cosmological and plasma simulations. Our wavelet code will be described in a following paper, and will then be available on request.

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