Introduce the velocity variable . The second-order differential equation becomes the autonomous planar systemA 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 areThe Jacobian matrix isFor 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 integralAt 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 haveAbove 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 energyIndeed . 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 areThe 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 fromEvery 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.
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