A Simplified Model of the Formation of Structures in Dark Matter
Astrophysics
2007-05-23 v1
Abstract
The collapse of a rotating 3-axis ellipsoid is approximated by a system of ordinary differential equations. Violent relaxation, mass and angular momentum losses are taken into account phenomenologically. The formation of the equilibrium configuration and different types of instability are investigated.
Keywords
Cite
@article{arxiv.astro-ph/0410573,
title = {A Simplified Model of the Formation of Structures in Dark Matter},
author = {O. Yu. Tsupko and G. S. Bisnovatyi-Kogan},
journal= {arXiv preprint arXiv:astro-ph/0410573},
year = {2007}
}
Comments
3 pages, 1 figure, Talk presented at the International Conference "Astrophysics and Cosmology after Gamow - Theory and Observations" (Odessa, August 8-14, 2004)