Bifurcation sequences in the symmetric 1:1 Hamiltonian resonance
arXiv:1512.00707 · doi:10.1142/S0218127416300111
Abstract
We present a general review of the bifurcation sequences of periodic orbits in general position of a family of resonant Hamiltonian normal forms with nearly equal unperturbed frequencies, invariant under symmetry. The rich structure of these classical systems is investigated with geometric methods and the relation with the singularity theory approach is also highlighted. The geometric approach is the most straightforward way to obtain a general picture of the phase-space dynamics of the family as is defined by a complete subset in the space of control parameters complying with the symmetry constraint. It is shown how to find an energy-momentum map describing the phase space structure of each member of the family, a catastrophe map that captures its global features and formal expressions for action-angle variables. Several examples, mainly taken from astrodynamics, are used as applications.
36 pages, 10 figures, accepted on International Journal of Bifurcation and Chaos. arXiv admin note: substantial text overlap with arXiv:1401.2855
References in corpus (8)
- On the Orbit Structure of the Logarithmic Potential
- Halo orbits around the collinear points of the restricted three-body problem
- An energy-momentum map for the time-reversal symmetric 1:1 resonance with Z_2 X Z_2 symmetry
- Equivariant singularity analysis of the 2:2 resonance
- Stability of axial orbits in galactic potentials
- Qualitative and analytical results of the bifurcation thresholds to halo orbits
- The symmetric 1:2 resonance
- Normal forms for the epicyclic approximations of the perturbed Kepler problem
Cited by in corpus (6)
- A Hopf variables view on the libration points dynamics
- Structure of the center manifold of the L1 and L2 collinear libration points in the restricted three-body problem
- Orbital perturbation coupling of primary oblateness and solar radiation pressure
- The phase-space architecture in extrasolar systems with two planets in orbits of high mutual inclination
- Analytic Methods to Find Beating Transitions of Asymmetric Gaussian Beams in GNLS equations
- Bifurcation sequences in the secular 3D planetary 3-Body problem: a geometric approach