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

Kenji Tomita | Zendy

AI Assistant Blog Pricing

Home ZAIA Blog

Open Access

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

Author(s) -

Kenji Tomita

Publication year - 1988

Publication title -

progress of theoretical physics

Language(s) - French

Resource type - Journals

eISSN - 1347-4081

pISSN - 0033-068X

DOI - 10.1143/ptp.79.1345

Subject(s) - physics , astrophysics , galaxy , dark matter , redshift , spectral density , galaxy cluster , correlation function (quantum field theory) , quantum mechanics , statistics , mathematics , dielectric

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

The content you want is available to Zendy users.

Already have an account? Click here to sign in.

Having issues? You can contact us here

Accelerating Research