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dc.contributor.authorCristopher Moore
dc.contributor.authorMichael Nauenberg
dc.date.accessioned2017-05-09T00:19:04Z
dc.date.available2017-05-09T00:19:04Z
dc.date.copyrightOctober, 2006
dc.date.issued2006
dc.identifier.issn1555-1415
dc.identifier.otherJCNDDM-25552#307_1.pdf
dc.identifier.urihttp://yetl.yabesh.ir/yetl/handle/yetl/133255
dc.description.abstractSince the discovery of the figure-eight orbit for the three-body problem [, 1993, Phys. Rev. Lett., 70, pp. 3675–3679] a large number of periodic orbits of the n-body problem with equal masses and beautiful symmetries have been discovered. However, most of those that have appeared in the literature are either planar or are obtained from perturbations of planar orbits. Here we exhibit a number of new three-dimensional periodic n-body orbits with equal masses and cubic symmetry, including some whose moment of inertia tensor is a scalar. We found these orbits numerically, by minimizing the action as a function of the trajectories’ Fourier coefficients. We also give numerical evidence that a planar three-body orbit first found in [, 1976, Celest. Mech., 13, pp. 267–285], rediscovered by [Moore, 1993], and found to exist for different masses by [, 2001, Phys. Lett., 292, pp. 93–99], is dynamically stable.
dc.publisherThe American Society of Mechanical Engineers (ASME)
dc.titleNew Periodic Orbits for the n-Body Problem
dc.typeJournal Paper
dc.journal.volume1
dc.journal.issue4
dc.journal.titleJournal of Computational and Nonlinear Dynamics
dc.identifier.doi10.1115/1.2338323
dc.journal.fristpage307
dc.journal.lastpage311
dc.identifier.eissn1555-1423
dc.keywordsScalars
dc.keywordsInertia (Mechanics)
dc.keywordsForce
dc.keywordsN-body problem (Celestial mechanics)
dc.keywordsDimensions
dc.keywordsBraid (Textile)
dc.keywordsAngular momentum
dc.keywordsCollisions (Physics)
dc.keywordsTrajectories (Physics)
dc.keywordsTensors
dc.keywordsGradients AND Intersections
dc.treeJournal of Computational and Nonlinear Dynamics:;2006:;volume( 001 ):;issue: 004
dc.contenttypeFulltext


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