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A simplified model of the formation of structures in dark matter

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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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Keywords: Dark matter; Large-scale structure of the Universe

Document Type: Research Article

Affiliations: Moscow Engineering Physics Institute, Moscow, Russia

Publication date: 2005-10-01

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