Local Pictures of Nonlinear Worlds
A nonlinear system , is understood equilibrium by equilibrium: find all points where , compute the JACOBIAN , and evaluate it at each.
Near the equilibrium the system behaves like , so the linear classification (saddle, node, spiral — by trace and determinant) applies locally. The Hartman–Grobman principle: the linearization tells the truth except in the borderline center case.
Lotka–Volterra , : at the coexistence point the Jacobian is — trace , eigenvalues : closed orbits, populations cycling forever out of phase.
Competing species , : the interior equilibrium has Jacobian determinant — a SADDLE, so coexistence is unstable and one species excludes the other. Ecology, decided by a determinant.
The pendulum has equilibria at (hanging) and (balanced upright).
Step 1 — linearize at : gives , a center: small swings oscillate with period .
Step 2 — linearize at : gives , eigenvalues : a SADDLE — the inverted pendulum falls.
Step 3 — what linearization misses: the true period GROWS with amplitude, and the special orbits into the saddle separate swinging from over-the-top spinning. The phase portrait stitches all of this together.
Linearization explains the local picture, but genuinely nonlinear systems can do what linear ones never can: multiple equilibria, limit cycles (heartbeats are one), and chaos (weather). The Jacobian toolkit of this topic is the entry door; the Lorenz attractor is what lives three doors down.
For , , find the equilibria and classify . Work: equilibria at . Jacobian ; at origin: trace , det , discriminant : a stable SPIRAL — the pendulum rings down, exactly as friction predicts.
Proofs & Why It Matters
Write for a small displacement from the equilibrium . Taylor: , and by definition of equilibrium.
So : to first order the displacement obeys the linear system with matrix , and when 's eigenvalues have nonzero real part the quadratic remainder is too weak to change the picture.
The quantity is conserved: — expanding, .
Trajectories live on level curves of , which are closed loops around — so the center predicted by the linearization is genuine, not an artifact.
Going Deeper: Worked Problems
Classify every equilibrium of , .
Step 1 — equilibria: each equation vanishes on two curves; intersections: , , , and the interior solution of , : .
Step 2 — Jacobian: .
Step 3 — evaluate and classify: at : , both positive — source. At : , eigenvalues — stable node. At : , eigenvalues — stable node. At : , det — saddle.
Step 4 — the story: two stable "one species wins" states, an unstable coexistence saddle whose stable manifold is the knife-edge dividing the winners. Competitive exclusion, read off four small matrices.
The system , has Jacobian at the origin — a center. Is the origin actually stable?
Step 1 — the linearization says "center" (eigenvalues ), the one case Hartman–Grobman does NOT cover.
Step 2 — switch to polar coordinates: with , compute , so .
Step 3 — the radius GROWS: trajectories spiral outward, and the origin is unstable — the cubic terms the linearization discarded decide everything.
Step 4 — the lesson: when the linear part gives a center, look for a conserved quantity (as with Lotka–Volterra) or a radial equation; only nonlinear information can break the tie.