This vector field is the negative of the one in part (a). For the same positive-definite quadratic form,
The ellipse is invariant and has no stationary point. The angular variable increases around it, with a finite return time . It therefore explicitly supplies a periodic solution. Alternatively, the Poincare-Bendixson theorem applies to any compact invariant annulus with , because its boundaries point inward and there is no equilibrium in the annulus.
If a periodic orbit had a point with , then would strictly increase along it and could not return; a point with would make it strictly decrease. A periodic orbit meeting remains on that ellipse by uniqueness of solutions. Consequently the ellipse is the unique periodic orbit, up to time translation. It is attracting, and all nonzero trajectories approach it.
Figure 1.
The invariant quadratic ellipse separates attraction from finite-time escape in the first system and is the unique attracting periodic orbit in the reversed system; inner and outer circles show the optimal attraction and escape radii
.

Articles by others on the same topic (0)

There are currently no matching articles.