A Simplified Model of the Formation of Structures in Dark Matter

Details A Simplified Model of the Formation of Structures in Dark Matter A Simplified Model of the Formation of Structures in Dark Matter

2004-10-24

arxiv.org/abs/astro-ph/0410573v1

Astronomy and Astrophysics

Astrophysics

3 pages, 1 figure, Talk presented at the International Conference "Astrophysics and Cosmology after Gamow - Theory and Observa

Scientific paper

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.

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