No Infinite Spin for Partial Collisions converging to isolated CC on the plane

Anna Gierzkiewicz, Rodrigo Gonçalves Schaefer, Piotr Zgliczyński
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Abstract

The infinite spin problem is a problem concerning the rotational behavior of total collision orbits in the $n$-body problem. The question makes also sense for partial collision. When a~cluster of bodies tends to a (partial) collision, then its normalized shape curve tends to the set of normalized central configurations, which in the planar case has $SO(2)$ symmetry. This leaves a possibility that the normalized shape curve tends to the circle obtained by rotation of some central configuration instead of a particular point on it. This is the \emph{infinite spin problem}. We show that it is not possible if the limiting circle is isolated from other connected components of set of normalized central configuration. Our approach extends the method from recent work for total collision by Moeckel and Montgomery, which was based on combination of the center manifold theorem with {\L}ojasiewicz inequality. To that we add a shadowing result for pseudo-orbits near normally hyperbolic manifold and careful estimates on the influence of other bodies on the cluster of colliding bodies.
平面上收敛到孤立 CC 的部分碰撞没有无限旋转
无穷自旋问题是一个关于总碰撞轨道在 $n$ 体问题中的旋转行为的问题。这个问题对于部分碰撞也有意义。当一团物体趋向于(部分)碰撞时,它的归一化形状曲线就会趋向于归一化中心配置的集合,在平面情况下,该集合具有$SO(2)$对称性。这就留下了一种可能性,即归一化形状曲线趋向于某个中心构型旋转后得到的圆,而不是圆上的某个点。我们证明,如果极限圆从归一化中心构型集合的其他连通成分中分离出来,那么这是不可能的。我们的方法扩展了莫克尔和蒙哥马利最近研究全碰撞的方法,该方法基于中心流形定理与{\L}ojasiewicz不等式的结合。在此基础上,我们还增加了正常双曲流形附近伪轨道的阴影结果,以及其他天体对碰撞天体群的影响的仔细估计。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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