Abstract

A mathematical model of the early stage of the formation of interstellar clouds resulting from the interaction of oppositely directed cosmic particle flows and evolution of the clouds into planetary systems is proposed. An important role in the evolution is played by mechanical energy dissipation caused mainly by particle collisions. The simulation is based on the classical n-body problem and the Newtonian theory of instantaneous collisions of rigid bodies with a relative velocity recovery factor smaller than unity. The performed computations suggest that this model is applicable in cosmogonic theories of planetary system formation.

中文翻译：

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相反方向的粒子流相互作用的模拟

摘要

提出了由相反方向的宇宙粒子流的相互作用和云团演化成行星系统而导致的星际云团形成早期的数学模型。在演化过程中的重要作用是主要由粒子碰撞引起的机械能耗散。该模拟基于经典n体问题和相对速度恢复因子小于1的刚体瞬时碰撞的牛顿理论。进行的计算表明，该模型适用于行星系统形成的世界理论。