Kustaanheimo-Stiefel transformation with an arbitrary defining vector
Abstract
Kustaanheimo-Stiefel (KS) transformation depends on the choice of some preferred direction in the Cartesian 3D space. This choice, seldom explicitly mentioned, amounts typically to the direction of the first or the third coordinate axis in celestial mechanics and atomic physics, respectively. The present work develops a canonical KS transformation with an arbitrary preferred direction, indicated by what we call a defining vector. Using a mix of vector and quaternion algebra, we formulate the transformation in a reference frame independent manner. The link between the oscillator and Keplerian first integrals is given. As an example of the present formulation, the Keplerian motion in a rotating frame is re-investigated.
Cite
@article{arxiv.1701.02147,
title = {Kustaanheimo-Stiefel transformation with an arbitrary defining vector},
author = {Slawomir Breiter and Krzysztof Langner},
journal= {arXiv preprint arXiv:1701.02147},
year = {2017}
}
Comments
Accepted to Celestial Mechanics and Dynamical Astronomy. In memoriam Andre Deprit