论文标题
部分可观测时空混沌系统的无模型预测
On the possible implications of Dark Matter in the rings of Saturn: a conjecture
论文作者
论文摘要
在本文中，我们讨论了弗里茨·兹维奇（Fritz Zwicky）[1]众所周知的命题的一些后果，该命题在190年代发表，《暗物质》“模仿”常规物质的惯性惯性行为。特别是，我们考虑了一些特殊的动力区域，例如行星系统边缘的气态巨头环系统的环境。本文是较早的论文[2]的延续，其中表明重力相互作用的颗粒可能会在Lagrange点L4和L5附近保留数千年。这为暗物质（如果存在）提供了足够的时间来与通常的物质互动。我们还讨论了与数学意义上可能被认为是单数的地方有关的许多问题。
In this article we discuss some consequences of the well-known proposition of Fritz Zwicky [1], published in the nineteen thirties, that Dark Matter `mimics' the inertia-gravitational behaviour of usual matter. In particular, we consider some special dynamical regions such as those of the Ring Systems of the gaseous giants at the edge of the Planetary System. This article is a continuation of an earlier paper [2], where it was shown that gravitationally interacting particles may remain near the Lagrange Points L4 and L5 for many thousands of years. This provides enough time for the Dark Matter, if present there, to interact with the usual matter. We discuss also a number of questions related to places which might be considered singular in the mathematical sense.
