A simplified model of the formation of structures in dark matter

Astronomy and Astrophysics – Astronomy

Scientific paper

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Dark Matter, Large-Scale Structure Of The Universe

Scientific paper

The collapse of a rotating three-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, secular instability and transition from a spheroid to a three-axis ellipsoid are investigated numerically and analytically in this dynamic model.

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