Bifurcations in a non-symmetric cubic potential.

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Galaxy: Kinematics And Dynamics, Stellar Dynamics, Celestial Mechanics

Scientific paper

For a Hamiltonian corresponding to a perturbed couple of harmonic oscillators -but without symmetries- we obtain the evolution phase flow of the reduced Hamiltonian. The loss of symmetry produces a bifurcation that does not appear in the symmetric case, namely, one where a stable point crosses an unstable point yielding a cusp in the level curve. This result may be considered as a warning to some of the conclusions derived in galactic dynamics from too symmetric Hamiltonian.

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