N-body simulations with two-orders-of-magnitude higher performance using wavelets
Artikel i vetenskaplig tidskrift, 2003

Noise is a problem of major concern for N-body simulations of structure formation in the early Universe, and 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.


Alessandro Romeo

Chalmers, Institutionen för radio- och rymdvetenskap

Cathy Horellou

Chalmers, Institutionen för radio- och rymdvetenskap

Jöran Bergh

Göteborgs universitet

Chalmers, Institutionen för matematik

Monthly Notices of the Royal Astronomical Society

0035-8711 (ISSN) 1365-2966 (eISSN)

Vol. 342 2 337-344


Astronomi, astrofysik och kosmologi


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