A Simplified Model of the Formation of Structures in Dark Matter
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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.
3 pages, 1 figure, Talk presented at the International Conference "Astrophysics and Cosmology after Gamow - Theory and Observations" (Odessa, August 8-14, 2004)
3 pages, 1 figure, Talk presented at the International Conference "Astrophysics and Cosmology after Gamow - Theory and Observations" (Odessa, August 8-14, 2004)