© Jean-Michel ALLIMI/INSU/LUTH/CNRS Images
Reference
19910001_0227
"Tranches" bi-dimensionnelles d'un Univers de matière noire simulé par ordinateur (CRAY 2). Le spect
"Tranches" bi-dimensionnelles d'un Univers de matière noire simulé par ordinateur (CRAY 2). Le spectre de fluctuation de densité de matière considéré favorise la formation de grandes structures (longs filaments sur les images). Evolution à 4 temps différents: t 1.
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