2003
DOI: 10.1016/s0378-4371(03)00582-x
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Chaotic transfers in three- and four-body systems

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Cited by 11 publications
(8 citation statements)
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“…Regularization of collisions are studied by Álvarez-Ramírez, Delgado, and Vidal in [32]. Chaotic motions were studied numerically by Gidea and Burgos in [33], and by Álvarez-Ramírez and Barrabés in [34]. Perturbative proofs of the existence of chaotic motions are found in the work of She, Cheng and Li [35,36,37], and also in the work of Alvarez-Ramírez, García, Palacián, and Yanguas [38].…”
Section: Introductionmentioning
confidence: 99%
“…Regularization of collisions are studied by Álvarez-Ramírez, Delgado, and Vidal in [32]. Chaotic motions were studied numerically by Gidea and Burgos in [33], and by Álvarez-Ramírez and Barrabés in [34]. Perturbative proofs of the existence of chaotic motions are found in the work of She, Cheng and Li [35,36,37], and also in the work of Alvarez-Ramírez, García, Palacián, and Yanguas [38].…”
Section: Introductionmentioning
confidence: 99%
“…The model under consideration can be used in studying the dynamics of planets orbiting systems of binary stars (see [14,11]), in which case the primaries have Another possible application regards mass transfers in binary stars. Mass transfer commonly occurs in tight binary star systems.…”
Section: Introductionmentioning
confidence: 99%
“…Earlier models for the dynamics of a planet near a binary star system only considered the motion of the planet in a planar orbit either about one of the stars, or well outside of the binary (see [3]). Our models suggest that spatial configurations, with long term chaotic motion, are also possible (see [4]). The methods involved here could also be useful in studying the classical mechanics of spatial three-body configurations (non-zero angular momentum) of two electron atoms (see [5]).…”
Section: Introductionmentioning
confidence: 76%