2011
DOI: 10.1111/j.1365-2966.2011.18431.x
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The Global Symplectic Integrator: an efficient tool for stability studies of dynamical systems. Application to the Kozai resonance in the restricted three-body problem

Abstract: Following the discovery of extrasolar systems, the study of long‐term evolution and stability of planetary systems is enjoying a renewed interest. While non‐symplectic integrators are very time‐consuming because of the very long time‐scales and the small integration steps required to have a good energy preservation, symplectic integrators are well suited for the study of such orbits on long time‐spans. However, stability studies of dynamical systems generally rely on non‐symplectic integrations of deviation ve… Show more

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Cited by 4 publications
(2 citation statements)
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“…Actually, in Sect. 3 we show that, for negative energies E close to zero, the phase space acquires a structure reminiscent to the one of the non-integrable Lidov-Kozai case of the restricted three-body problem (i.e., non-intersecting trajectories examined in a higher than quadrupolar development of the disturbing function, see Libert et al (2011)). The typical behavior of the trajectories in the Lidov-Kozai regime is to (quasi-)periodically exchange eccentricity with mutual inclination.…”
Section: Introductionmentioning
confidence: 69%
“…Actually, in Sect. 3 we show that, for negative energies E close to zero, the phase space acquires a structure reminiscent to the one of the non-integrable Lidov-Kozai case of the restricted three-body problem (i.e., non-intersecting trajectories examined in a higher than quadrupolar development of the disturbing function, see Libert et al (2011)). The typical behavior of the trajectories in the Lidov-Kozai regime is to (quasi-)periodically exchange eccentricity with mutual inclination.…”
Section: Introductionmentioning
confidence: 69%
“…The method makes it possible for the Lyapunov exponent to be consequently recovered. For these reasons, MEGNO has been largely used in the framework of planetary systems [58,59], satellites and spatial debris [60][61][62] and also generic nonlinear dynamical systems [57]. The method overcomes the above mentioned limitation by performing a sort of time average of the norm of the deviation vector (see Appendix A).…”
Section: Master Stability Function On Hypergraphsmentioning
confidence: 99%