Introduce the velocity variable . The second-order differential equation becomes the autonomous planar system
A critical point of a dynamical system is a point where both components of the vector field vanish: here and . It is a stationary solution in the phase plane. The Jacobian matrix at each such point gives the local linear stability of a planar equilibrium. For the equations below, a conserved energy also determines the nonlinear phase portrait; this is important because purely imaginary eigenvalues alone do not generally prove that an equilibrium is a center equilibrium.
Here the autonomous planar system is , . Its equilibrium points are
The Jacobian matrix is
For even , the eigenvalues are , so these points are unstable saddle equilibria. Writing , their local unstable and stable directions are and respectively. For odd , the eigenvalues are .
To classify the latter points nonlinearly, differentiate the first integral
At this energy has a strict local minimum. Its nearby level sets are closed curves, proving that the odd- points are stable center equilibria, with no attraction to the center. The phase portrait consists of closed oscillatory orbits for , heteroclinic orbits at joining consecutive saddle equilibria, and open rotating orbits for . The separating curves have
Above the horizontal axis , so flow is rightward; below it flow is leftward. The closed orbits are clockwise, and these same signs orient every separating and rotating orbit.
For both parameters the autonomous planar system is , . It has the conserved energy
Indeed . At any equilibrium point the eigenvalues satisfy
For , the quadratic is strictly positive, so the only equilibrium point is , with eigenvalues . Since has the sign of , has a unique strict minimum at zero and tends to infinity in both directions. All positive energy levels are closed curves surrounding this stable center equilibrium. They are clockwise: rightward when and leftward when .
For , factor . The three equilibrium points and their classifications are
The two center equilibria are stable but not asymptotically stable; the saddle equilibrium is unstable. At the saddle equilibrium the local unstable and stable directions are and .
The potential values are , , and . Consequently there are closed loops around the left center for , closed loops in both wells for , and a figure-eight pair of homoclinic orbits at . At the right center is a stationary point while the left well still has a closed orbit. For , each closed curve encircles both centers and the saddle.
The two homoclinic orbits satisfy . Their outer turning points can be located exactly from
Every nonstationary energy curve is oriented to the right in the upper half-plane and to the left in the lower half-plane. The sketches show the closed curves, the separating orbits, the stable and unstable saddle directions and the direction of flow.
Figure 1.
Clockwise phase flows, alternating pendulum saddles and centers, and the one-well and two-well quartic potentials
. Details.

Articles by others on the same topic (0)

There are currently no matching articles.