2017
DOI: 10.1007/s10884-017-9627-x
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Dynamics in the Charged Restricted Circular Three-Body Problem

Abstract: The existence and stability of periodic solutions for different types of perturbations associated to the Charged Restricted Circular Three Body Problem (shortly, CHRCTBP) is tackled using reduction and averaging theories as well as the technique of continuation of Poincaré for the study of symmetric periodic solutions. The determination of KAM 2-tori encasing some of the linearly stable periodic solutions is proved. Finally, we analyze the occurrence of Hamiltonian-Hopf bifurcations associated to some equilibr… Show more

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(5 citation statements)
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“…In celestial mechanics, one of the most well-known integrable model is the Kepler problem. There exist many other problems that are formulated as a perturbation of the Kepler problem in Cartesian coordinates (see [5,6,10,13] and references therein) or in rotating coordinates (see, e.g., [16,21,25,27]). Poincaré [28] considered the investigation of periodic solutions of the restricted three-body problem where, in particular, he classified the periodic orbits of second kind that are generated by the elliptic orbits of the planar Kepler problem (the first kind are generated by the circular orbits of the planar Kepler problem).…”
Section: Introductionmentioning
confidence: 99%
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“…In celestial mechanics, one of the most well-known integrable model is the Kepler problem. There exist many other problems that are formulated as a perturbation of the Kepler problem in Cartesian coordinates (see [5,6,10,13] and references therein) or in rotating coordinates (see, e.g., [16,21,25,27]). Poincaré [28] considered the investigation of periodic solutions of the restricted three-body problem where, in particular, he classified the periodic orbits of second kind that are generated by the elliptic orbits of the planar Kepler problem (the first kind are generated by the circular orbits of the planar Kepler problem).…”
Section: Introductionmentioning
confidence: 99%
“…There are considerable works that have contributed to find the periodic solution for perturbations of an integrable problem (see [1,7]). For a perturbed Kepler problem, some of these works apply the method of average of first kind (see, e.g., [3,4,14,25,27]). The technique of combining discrete symmetries of Hamiltonian and the Poincaré continuation method has been considered in other works for twodegree-of-freedom (2-DOF) and three-degree-of-freedom problems (see, e.g., [5,10,25,[31][32][33][34][35]).…”
Section: Introductionmentioning
confidence: 99%
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