A method of symplectic integrations with adaptive time-steps for individual Hamiltonians in the planetary N-body problem
A new algorithm is developed for long-term integrations of the N-body problem. The method uses symplectic integrations of the Hamiltonian equations of motion for each body. This allows one to employ individual adaptive time-steps in computations. The efficiency of this technique is demonstrated by s...
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Veröffentlicht in: | Celestial mechanics and dynamical astronomy 2007-07, Vol.98 (3), p.191-202 |
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Format: | Artikel |
Sprache: | eng |
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Online-Zugang: | Volltext |
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Zusammenfassung: | A new algorithm is developed for long-term integrations of the N-body problem. The method uses symplectic integrations of the Hamiltonian equations of motion for each body. This allows one to employ individual adaptive time-steps in computations. The efficiency of this technique is demonstrated by several tests performed for typical problems of Solar System dynamics.[PUBLICATION ABSTRACT] |
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ISSN: | 0923-2958 1572-9478 |
DOI: | 10.1007/s10569-007-9077-6 |