Consider a linear 2nd-order ODE system, \[ \dot{\mathbf{y}} = B \mathbf{y} \] It may have one or a line of critical points, because unless \( B = 0 \), \( B \text{y} =0 \) has a unique solution or solutions forming a one-dimensional linear space. We assume \( \det(B) \ne 0 \) in the following discussion.
If \( B \) has real (nonzero) eigenvalues \( \lambda, \mu \), for example \( B = \begin{pmatrix} \lambda & 0 \\ 0 & \mu \end{pmatrix}\) , then \(\begin{cases} y_1 = y_1(0) e^{\lambda t} \\ y_2 = y_2(0) e^{\mu t} \end{cases}\).
If \( B \) has a pair of complex conjugate eigenvalues \( a \pm ib \), for example \( B = \begin{pmatrix} a & b \\ -b & a \end{pmatrix} \) , then \(\begin{cases} y_1 = A e^{at} \sin(bt+\phi) \\ y_2 = A e^{at} \cos(bt+\phi) \end{cases}\)
For linear systems, closed orbits exist around a center and have the same period. For a nonlinear system, a center found in its linearized form may not be an actual center; but symmetry of the original system about \(y\)-axis suffice to preserve this property.
For a nonlinear 2nd-order ODE system: \[ \frac{\text{d}}{\text{d}t} \begin{pmatrix} x \\ y \end{pmatrix} = \begin{pmatrix} f(x,y) \\ g(x,y) \end{pmatrix} \]
To get the phase plane near a critical point, we just need a coordinate transformation, which does not change the eigenvalues of \(A\) and the type of the critical point.
If \( \mathbf{v} \) is an eigenvector corresponding to eigenvalue \( \lambda \) of the linearized system, along the line of the eigenvector we have \( \dot{x} = \lambda x \). This means along the eigenvectors at the critical point, trajectories go directly into or away from the critical point, approximately in a straight line.
Trajectories in the Duffing equation
A form of Duffing equation is
\[ u'' + u - u^3 = 0 \]
Or, in the form of ODE systems,
\[ \begin{cases} u' = v \\ v' = -u+u^3 \end{cases} \]
We find three critical points: \( (0,0) \) and \( (\pm 1,0) \). Furthermore, the first one is a center, and the other two are saddles.
Homoclinic orbits
A trajectory may connect two critical points, or forms a loop from and toward the same critical point. The former one is called a heteroclinic orbit, and the latter a homoclinic orbit.
We've already seen heteroclinic orbits in duffing equation, now we illustrate a homoclinic oribt by the following system.
\[ \begin{cases} x' = y + y(1-x^2)[y^2-x^2(1-\frac{x^2}{2})] \\ y' = x(1-x^2) - y[y^2-x^2(1-\frac{x^2}{2})] \end{cases} \]
There are also three critical points: \( (0,0) \) and \( (\pm 1,0) \). The origin is a saddle, while the other two are unstable focus (foci).
Note: Period of homoclinic or heteroclinic orbit
Van der Pol equation has an attracting limit cycle.
The Poincare-Bendixon theorem and limit cycle
A limit cycle is a closed orbit that each trajectory nearby either goes towards it, or leaves away. It is another important type of closed orbits.
Certain theorems guarantee the existence of a limit cycle.
Poincare-Bendixon Theorem:
Hierarchy of local stabilities in nonlinear dynamical systems:
Notice that Lyapunov stability is distinct from local attractiveness.
An equilibrium is globally asymptotically stable if it is Lyapunov stable and globally attractive, that is, all trajectories converge to it.
A Lyapunov function \( V(\mathbf{x}) \) for an autonomous dynamical system \( \dot{\mathbf{x}} = \mathbf{g}(\mathbf{x}) \) with an equilibrium point at the origin is a locally positive-definite and continuously differentiable function such that its time derivative is locally negative-semidefinite:
An equilibrium is Lyapunov stable if and only if the dynamical system has a Lyapunov function. An equilibrium is locally asymptotically stable if and only if the dynamical system has a Lyapunov function whose time derivative is locally negative-definite. An equilibrium is globally asymptotically stable if the dynamical system has a radially unbounded global Lyapunov function whose time derivative is globally negative-definite.
Lyapunov function is analogous to the energy of a dissipative physical system, while not unique and thus easier to find.
A subset of the phase space is an attractor if it is the smallest subset of itself that is forward invariant and has a basin of attraction: \( \Phi(A, t) \subseteq A, \forall t > 0 \); and \( \exists B \in \tau(X), B \supseteq A\), \( \forall b \in B, \forall \varepsilon > 0, \exists T > 0: \Phi(b, t) \in N_\varepsilon(A), \forall t > T \).
Types of attractors:
The ω-limit set of a trajectory \( \Phi(x, t) \) of a dynamical system is the set of limit points of all convergent subsequences of the forward trajectory: \( \Omega_x = \{ \omega \mid \exists \{t_k\}, \lim_{k \to \infty} t_k = +\infty, \lim_{k \to \infty} \Phi(x, t_k) = \omega \} \).