Nonlinear Dynamics, Lorenz Model and Formation of Binary Stars

dc.creatorChang, Yi-Fang
dc.date2008-06-01
dc.date.accessioned2026-07-07T09:42:10Z
dc.date.available2026-07-07T09:42:10Z
dc.descriptionBased on the Lorenz model derived from the equations of hydrodynamics of nebula, we discuss the formation of binary stars by the qualitative analysis theory of nonlinear equation. Here the two wings in the Lorenz model form just the binary stars, whose Roche surface is result of evolution under certain condition. The nonlinear interaction plays a crucial role, and is necessary condition of the formation of binary stars and of multiple stars. While the linear equations form only a single star. Moreover, the Lorenz model may be obtained from synergetics yet, and some dynamical equations of the order parameter can also form the binary star system.
dc.description8 pages
dc.identifierhttps://arxiv.org/abs/0806.0188
dc.identifierhttp://arxiv.org/abs/0806.0188
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/162085
dc.subjectGeneral Physics
dc.titleNonlinear Dynamics, Lorenz Model and Formation of Binary Stars
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