A Lyapunov function near an equilibrium is a continuously differentiable positive-definite function , vanishing there, whose derivative along trajectories is nonpositive. The strict Second Lyapunov theorem says a negative-definite derivative implies local asymptotic stability.
For sharper bounds than the circular test , put , and
A direct multiplication gives . Its eigenvalues are . Since the nonlinear vector field is ,
For , the derivative is strictly negative. The Lyapunov theorem proves asymptotic stability. In fact gives and
so the solution stays bounded, exists for all positive time and converges exponentially to zero.
The ellipse is invariant. In polar coordinates, , so it is a nonconstant periodic orbit, not part of the basin. For , use to obtain . This implies finite-time blow-up by comparison with the scalar equation. Thus the exact basin is and every point outside its closure escapes to unbounded norm within its maximal existence interval.
The largest open disc centred at zero lying in this exact basin has radius
The smallest radius such that every point strictly outside its circle escapes is the largest radius on the invariant ellipse:
These are optimal: a larger attraction disc contains a periodic-orbit point, and a smaller escape threshold leaves a periodic-orbit point in its exterior. This is an exact quadratic basin boundary.
The simpler radial derivative is . It only certifies attraction for and strictly increasing norm for . Those are optimal thresholds for a sign test on that radial derivative, not for the actual attraction and escape regions. If “increases without bound” is read as requiring monotonic increase from the initial instant, the smallest such uniform radius is : at direction , any smaller threshold permits an initially decreasing norm. The sharper above concerns eventual unbounded escape, which need not be monotone at every instant.
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
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