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 |
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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. |
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ISSN: | 0923-2958 1572-9478 |
DOI: | 10.1023/A:1014599918133 |