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Stability and chaos in Kustaanheimo-Stiefel space induced by the Hopf fibration

Stability and chaos in Kustaanheimo-Stiefel space induced by the Hopf fibration
Stability and chaos in Kustaanheimo-Stiefel space induced by the Hopf fibration
The need for the extra dimension in Kustaanheimo–Stiefel (KS) regularization is explained by the topology of the Hopf fibration, which defines the geometry and structure of KS space. A trajectory in Cartesian space is represented by a four-dimensional manifold called the fundamental manifold. Based on geometric and topological aspects classical concepts of stability are translated to KS language. The separation between manifolds of solutions generalizes the concept of Lyapunov stability. The dimension-raising nature of the fibration transforms fixed points, limit cycles, attractive sets, and Poincaré sections to higher dimensional subspaces. From these concepts chaotic systems are studied. In strongly perturbed problems, the numerical error can break the topological structure of KS space: points in a fibre are no longer transformed to the same point in Cartesian space. An observer in three dimensions will see orbits departing from the same initial conditions but diverging in time. This apparent randomness of the integration can only be understood in four dimensions. The concept of topological stability results in a simple method for estimating the time-scale in which numerical simulations can be trusted. Ideally, all trajectories departing from the same fibre should be KS transformed to a unique trajectory in three-dimensional space, because the fundamental manifold that they constitute is unique. By monitoring how trajectories departing from one fibre separate from the fundamental manifold a critical time, equivalent to the Lyapunov time, is estimated. These concepts are tested on N-body examples: the Pythagorean problem, and an example of field stars interacting with a binary
1365-2966
2444-2454
Urrutxua, Hodei
ec73b9d7-654f-4db7-9ff3-68ad05543cfe
Urrutxua, Hodei
ec73b9d7-654f-4db7-9ff3-68ad05543cfe

Urrutxua, Hodei (2016) Stability and chaos in Kustaanheimo-Stiefel space induced by the Hopf fibration. Monthly Notices of the Royal Astronomical Society, 459 (3), 2444-2454. (doi:10.1093/mnras/stw780).

Record type: Article

Abstract

The need for the extra dimension in Kustaanheimo–Stiefel (KS) regularization is explained by the topology of the Hopf fibration, which defines the geometry and structure of KS space. A trajectory in Cartesian space is represented by a four-dimensional manifold called the fundamental manifold. Based on geometric and topological aspects classical concepts of stability are translated to KS language. The separation between manifolds of solutions generalizes the concept of Lyapunov stability. The dimension-raising nature of the fibration transforms fixed points, limit cycles, attractive sets, and Poincaré sections to higher dimensional subspaces. From these concepts chaotic systems are studied. In strongly perturbed problems, the numerical error can break the topological structure of KS space: points in a fibre are no longer transformed to the same point in Cartesian space. An observer in three dimensions will see orbits departing from the same initial conditions but diverging in time. This apparent randomness of the integration can only be understood in four dimensions. The concept of topological stability results in a simple method for estimating the time-scale in which numerical simulations can be trusted. Ideally, all trajectories departing from the same fibre should be KS transformed to a unique trajectory in three-dimensional space, because the fundamental manifold that they constitute is unique. By monitoring how trajectories departing from one fibre separate from the fundamental manifold a critical time, equivalent to the Lyapunov time, is estimated. These concepts are tested on N-body examples: the Pythagorean problem, and an example of field stars interacting with a binary

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Accepted/In Press date: 31 March 2016
e-pub ahead of print date: 6 April 2016
Organisations: Astronautics Group

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Local EPrints ID: 391468
URI: http://eprints.soton.ac.uk/id/eprint/391468
ISSN: 1365-2966
PURE UUID: e0c9ec6d-6459-41b0-984f-52c1064002d9

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Date deposited: 16 Jun 2016 08:14
Last modified: 14 Mar 2024 23:29

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