The Symmetrical One-dimensional Newtonian Four-body Problem: A Numerical Investigation

Numerical simulations of the one-dimensional Newtonian four-body problem have been conducted for the special case in which the bodies are distributed symmetrically about the centre of mass. Simulations show a great similarity between this problem and the one-dimensional Newtonian three-body problem....

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Veröffentlicht in:Celestial mechanics and dynamical astronomy 2002-02, Vol.82 (2), p.179-201
1. Verfasser: Sweatman, Winston L
Format: Artikel
Sprache:eng
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Zusammenfassung:Numerical simulations of the one-dimensional Newtonian four-body problem have been conducted for the special case in which the bodies are distributed symmetrically about the centre of mass. Simulations show a great similarity between this problem and the one-dimensional Newtonian three-body problem. As in that problem the orbits can be divided into three different categories which form well-defined regions on a Poincare section: there is a region of quasiperiodic orbits about a Schubart-like periodic orbit, there is a region of fast-scattering encounters and in between these two regions there is a chaotic scattering region. The Schubart-like periodic orbit's stability to perturbation is studied. It is apparently stable in one-dimension but is unstable in three-dimensions.
ISSN:0923-2958
1572-9478
DOI:10.1023/A:1014599918133