A Simplified Model of the Formation of Structures in Dark Matter

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dc.creatorTsupko, O. Yu.
dc.creatorBisnovatyi-Kogan, G. S.
dc.date2004-10-24
dc.date.accessioned2026-07-07T02:15:28Z
dc.date.available2026-07-07T02:15:28Z
dc.descriptionThe 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.
dc.description3 pages, 1 figure, Talk presented at the International Conference "Astrophysics and Cosmology after Gamow - Theory and Observations" (Odessa, August 8-14, 2004)
dc.identifierhttps://arxiv.org/abs/astro-ph/0410573
dc.identifierhttp://arxiv.org/abs/astro-ph/0410573
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8418
dc.subjectAstrophysics
dc.titleA Simplified Model of the Formation of Structures in Dark Matter
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