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Les fonctions de correlation et les distributions des vitesses des galaxies et amas de galaxies sont etudiees en utilisant la methode directe de simulation a n corps pour ces objets et la methode de difference simple pour la matiere sombre consistant en produit de desintegration. La matiere sombre empeche l'agencement a petite echelle des galaxies et aide a l'agencement a grande echelle des amas de galaxies

Clustering of Galaxies and Clusters of Galaxies in a Decaying-Particle Cosmological Model with a Massive Decay Product