Abstract
The Kepler problem for planetary motion is a two-body dynamic model with an attractive force obeying the inverse square law, and has a direct analogue in any dimension. While the magnetized Kepler problems were discovered in the late 1960s, it is not clear until recently that their higher dimensional analogues can exist at all. Here we present a possible route leading to the discovery of these high dimensional magnetized models.
Information
Published: 1 January 2014
First available in Project Euclid: 13 July 2015
zbMATH: 1311.70022
MathSciNet: MR3287758
Digital Object Identifier: 10.7546/giq-15-2015-196-203
Rights: Copyright © 2014 Institute of Biophysics and Biomedical Engineering, Bulgarian Academy of Sciences
