Periodic orbits and their bifurcations in a 3-D system

Mathematics

Scientific paper

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Astronomical Models, Branching (Mathematics), Mathematical Models, Orbit Calculation, Orbits, Stability, Uniqueness, Barred Galaxies, Classical Mechanics, Elliptical Galaxies, Hamiltonian Functions

Scientific paper

We study some simple periodic orbits and their bifurcations in the Hamiltonian (H = 1/2 ((x dot)2 + (y dot)2 + (z dot)2 + Ax2 + By2 + Cz2) - epsilon xz2 - eta yz2. We give the forms of the orbits, the characteristics of the main families, and some existence diagrams and stability diagrams. The existence diagram of the family 1a contains regions that are stable (S), simply unstable (U), doubly unstable (DU) and complex unstable (Delta). In the regions S and U there are lines of equal rotation number m/n. Along these lines we have bifurcations of families of periodic orbits of multiplicity n. When these lines reach the boundary of the complex unstable region, they are tangent to it. Inside the region Delta there are lines m/n, along which the orbits 1a, described n-times, are doubly unstable; however, along these lines there are no bifurcations of n-ple periodic orbits. The families bifurcating from 1a exist only in certain regions of the parameter space (epsilon, eta). The limiting lines of these regions join at particular points representing collisions of bifurcations. These collisions of bifurcations produce a nonuniqueness of the various families of periodic orbits. The complicated structure of the various bifurcations can be understood by constructing appropriate stability diagrams.

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