Phase Plane Analysis

6 PHASE PLANE

6.0 Introduction

  • This chapter introduces two-dimensional nonlinear systems.
  • General properties are considered.
  • Classification of fixed points is built on knowledge of linear systems (Chapter 5).
  • Examples include biology (competition) and physics (conservative systems, reversible systems, pendulum).
  • The chapter discusses index theory, a topological method for global phase portrait information.
  • Focus is mainly on fixed points; closed orbits and bifurcations are covered in subsequent chapters.

6.1 Phase Portraits

  • General form of a vector field on the phase plane:

    x˙=f(x)\dot{x} = f(x)

    where x=(x<em>1,x</em>2)x = (x<em>1, x</em>2), x˙=(f<em>1(x),f</em>2(x))\dot{x} = (f<em>1(x), f</em>2(x)).

  • xx represents a point in the phase plane, x˙\dot{x} is the velocity vector at that point.

  • A phase point traces out a solution x(t)x(t), corresponding to a trajectory winding through the phase plane.

  • The phase plane is filled with trajectories since each point can be an initial condition.

  • For nonlinear systems, finding trajectories analytically is generally not possible.

  • The goal is to determine qualitative behavior directly from properties of f(x)f(x).

  • Salient features of a phase portrait:

    1. Fixed points (where f(x)=0f(x^*) = 0), corresponding to steady states or equilibria.
    2. Closed orbits, corresponding to periodic solutions where x(t+T)=x(t)x(t + T) = x(t) for all tt, for some T > 0.
    3. Arrangement of trajectories near fixed points and closed orbits.
    4. Stability or instability of fixed points and closed orbits.
  • Numerical computation:

    • Numerical integration of x˙=f(x)\dot{x} = f(x) is used.

    • Runge-Kutta method in vector form:

      x<em>n+1=x</em>n+16(k<em>1+2k</em>2+2k<em>3+k</em>4)x<em>{n+1} = x</em>n + \frac{1}{6}(k<em>1 + 2k</em>2 + 2k<em>3 + k</em>4)

      where

      k<em>1=f(x</em>n)k<em>1 = f(x</em>n),

      k<em>2=f(x</em>n+Δt2k1)k<em>2 = f(x</em>n + \frac{\Delta t}{2}k_1),

      k<em>3=f(x</em>n+Δt2k2)k<em>3 = f(x</em>n + \frac{\Delta t}{2}k_2),

      k<em>4=f(x</em>n+Δtk3)k<em>4 = f(x</em>n + \Delta t k_3).

    • Stepsize Δt=0.1\Delta t = 0.1 usually provides sufficient accuracy.

  • Direction field plots provide a clearer picture of flow direction.

EXAMPLE 6.1.1:
  • System: x˙=1+eyx\dot{x} = 1 + e^{-y} - x, y˙=y\dot{y} = -y.

  • Fixed point: (x<em>,y</em>)=(1,0)(x^<em>, y^</em>) = (1, 0).

  • Stability: Unstable, based on analysis of the equations.

  • Nullclines: Curves where x˙=0\dot{x} = 0 or y˙=0\dot{y} = 0 indicate purely horizontal or vertical flow.

    • y˙=0\dot{y} = 0 occurs on the line y=0y = 0.
    • x˙=0\dot{x} = 0 occurs on the curve x=1+eyx = 1 + e^{-y}.
  • The nullclines partition the plane into regions where x˙\dot{x} and y˙\dot{y} have various signs, giving a sense of the overall flow pattern.

  • The fixed point is a nonlinear version of a saddle point.

6.2 Existence, Uniqueness, and Topological Consequences

  • Existence and Uniqueness Theorem:

    • For the initial value problem x˙=f(x)\dot{x} = f(x), x(0)=x<em>0x(0) = x<em>0, if ff is continuous and its partial derivatives f</em>ix<em>j\frac{\partial f</em>i}{\partial x<em>j}, i,j=1,,ni, j = 1, …, n, are continuous for xx in some open connected set DRnD \subset R^n, then for x</em>0Dx</em>0 \in D, the initial value problem has a unique solution x(t)x(t) on some time interval (τ,τ)(-\tau, \tau) about t=0t = 0.
    • Existence and uniqueness are guaranteed if ff is continuously differentiable.
  • Corollary: Different trajectories never intersect.

  • In two-dimensional phase spaces, these results have strong topological consequences.

  • Poincaré-Bendixson theorem: If a trajectory is confined to a closed, bounded region with no fixed points, it approaches a closed orbit.

6.3 Fixed Points and Linearization

  • Extends linearization technique from one-dimensional systems.

  • Approximates phase portrait near a fixed point using a linear system.

  • Consider the system x˙=f(x,y)\dot{x} = f(x, y), y˙=g(x,y)\dot{y} = g(x, y) with fixed point (x<em>,y</em>)(x^<em>, y^</em>).

  • Let u=xx<em>,v=yy</em>u = x - x^<em>, v = y - y^</em> denote small disturbances from the fixed point.

  • Taylor series expansion:

    u˙=fxu+fyv+O(u2,v2,uv)\dot{u} = \frac{\partial f}{\partial x}u + \frac{\partial f}{\partial y}v + O(u^2, v^2, uv)

    v˙=gxu+gyv+O(u2,v2,uv)\dot{v} = \frac{\partial g}{\partial x}u + \frac{\partial g}{\partial y}v + O(u^2, v^2, uv)

  • Jacobian matrix at the fixed point (x<em>,y</em>)(x^<em>, y^</em>): (fxamp;fy gxamp;gy)\begin{pmatrix} \frac{\partial f}{\partial x} &amp; \frac{\partial f}{\partial y} \ \frac{\partial g}{\partial x} &amp; \frac{\partial g}{\partial y} \end{pmatrix}

  • Linearized system:

    (u˙ v˙)=(fxamp;fy gxamp;gy)(u v)\begin{pmatrix} \dot{u} \ \dot{v} \end{pmatrix} = \begin{pmatrix} \frac{\partial f}{\partial x} &amp; \frac{\partial f}{\partial y} \ \frac{\partial g}{\partial x} &amp; \frac{\partial g}{\partial y} \end{pmatrix} \begin{pmatrix} u \ v \end{pmatrix}

  • The linearized system gives a qualitatively correct picture near (x<em>,y</em>)(x^<em>, y^</em>) if the fixed point is not a borderline case (center, degenerate node, star, non-isolated fixed points).

EXAMPLE 6.3.1:
  • System: x˙=xx3\dot{x} = x - x^3, y˙=2y\dot{y} = -2y.

  • Fixed points: (0,0),(1,0),(1,0)(0, 0), (1, 0), (-1, 0).

  • Jacobian matrix: (13x2amp;0 0amp;2)\begin{pmatrix} 1 - 3x^2 &amp; 0 \ 0 &amp; -2 \end{pmatrix}.

  • Classification:

    • (0,0)(0, 0): Stable node.
    • (1,0),(1,0)(1, 0), (-1, 0): Saddle points.
  • The x and y equations are uncoupled.

  • Phase portrait is symmetric in both x and y axes.

EXAMPLE 6.3.2:
  • System: x˙=y+ax(x2+y2)\dot{x} = -y + ax(x^2 + y^2), y˙=x+ay(x2+y2)\dot{y} = x + ay(x^2 + y^2).

  • Linearized system predicts a center at the origin for all values of aa.

  • In polar coordinates: r˙=ar3\dot{r} = ar^3, θ˙=1\dot{\theta} = 1.

    • If a < 0: Stable spiral.
    • If a=0a = 0: Center.
    • If a > 0: Unstable spiral.
  • Centers are sensitive to small nonlinear terms.

  • Stars and degenerate nodes can be altered by small nonlinearities, but their stability remains unchanged.

  • Robust cases:

    • Repellers (sources): both eigenvalues have a positive real part.
    • Attractors (sinks): both eigenvalues have a negative real part.
    • Saddles: one eigenvalue is positive and one is negative.
  • Marginal cases:

    • Centers: both eigenvalues are pure imaginary.
    • Higher-order and non-isolated fixed points: at least one eigenvalue is zero.
  • Hyperbolic fixed points: all eigenvalues satisfy Re(λ)0Re(\lambda) \neq 0. Their stability type is unaffected by small nonlinear terms.

  • Nonhyperbolic fixed points are fragile.

  • Hartman-Grobman theorem: the local phase portrait near a hyperbolic fixed point is topologically equivalent to the phase portrait of the linearization.

  • Structural stability: a phase portrait is structurally stable if its topology is unchanged by small perturbations.

6.4 Rabbits versus Sheep

  • Lotka-Volterra model of competition between two species (rabbits and sheep).

  • Assumptions:

    1. Each species grows to its carrying capacity in the absence of the other (logistic growth).
    2. Conflicts reduce growth rate, more severely for rabbits.
  • Model: x˙=x(3x2y)\dot{x} = x(3 - x - 2y), y˙=y(2yx)\dot{y} = y(2 - y - x) where x(t)x(t) is the population of rabbits and y(t)y(t) is the population of sheep.

  • Fixed points: (0,0),(0,2),(3,0),(1,1)(0, 0), (0, 2), (3, 0), (1, 1).

  • Jacobian matrix: (32x2yamp;2x yamp;22yx)\begin{pmatrix} 3 - 2x - 2y &amp; -2x \ -y &amp; 2 - 2y - x \end{pmatrix}.

  • Classification:

    • (0,0)(0, 0): Unstable node.
    • (0,2),(3,0)(0, 2), (3, 0): Stable nodes.
    • (1,1)(1, 1): Saddle point.
  • One species generally drives the other to extinction.

  • Principle of competitive exclusion: two species competing for the same limited resource typically cannot coexist.

  • Basin of attraction: the set of initial conditions x0x_0 such that x(t)xx(t) \rightarrow x^* as tt \rightarrow \infty.

  • Separatrices: trajectories that comprise the stable manifold of the saddle; they partition phase space into regions of different long-term behavior.

6.5 Conservative Systems

  • Newton’s law F=maF = ma.
  • Particle of mass mm moving along the x-axis, subject to a nonlinear force F(x)F(x).
  • Equation of motion: mx¨=F(x)m\ddot{x} = F(x).
  • Potential energy: F(x)=dVdxF(x) = -\frac{dV}{dx}.
  • Energy conservation: E=12mx˙2+V(x)E = \frac{1}{2}m\dot{x}^2 + V(x) is constant.
  • Conserved quantity: a real-valued continuous function E(x)E(x) that is constant on trajectories, i.e., dEdt=0\frac{dE}{dt} = 0.
  • Conservative systems cannot have any attracting fixed points.
EXAMPLE 6.5.2:
  • Particle of mass m=1m = 1 moving in a double-well potential V(x)=12x2+14x4V(x) = -\frac{1}{2}x^2 + \frac{1}{4}x^4.

  • Equation of motion: x¨=xx3\ddot{x} = x - x^3 or the vector field x˙=y\dot{x} = y, y˙=x+x3\dot{y} = -x + x^3.

  • Equilibrium points: (0,0),(±1,0)(0, 0), (\pm 1, 0).

  • Jacobian matrix: (0amp;1 1+3x2amp;0)\begin{pmatrix} 0 &amp; 1 \ -1 + 3x^2 &amp; 0 \end{pmatrix}.

  • Classification:

    • (0,0)(0, 0): Saddle point.
    • (±1,0)(\pm 1, 0): Centers.
  • Homoclinic orbits: trajectories that start and end at the same fixed point.

  • Nonlinear Centers Theorem: For the system x˙=f(x)\dot{x} = f(x), where x=(x,y)R2x = (x, y) \in R^2, if there exists a conserved quantity E(x)E(x) and x<em>x^<em> is an isolated fixed point which is a local minimum of EE, then all trajectories sufficiently close to x</em>x^</em> are closed.

6.6 Reversible Systems

  • Many mechanical systems have time-reversal symmetry.
  • System of the form mx¨=F(x)m\ddot{x} = F(x) is symmetric under time reversal.
  • Reversible system: invariant under ttt \rightarrow -t and yyy \rightarrow -y.
  • Examples: systems of the form x˙=f(x,y)\dot{x} = f(x, y), y˙=g(x,y)\dot{y} = g(x, y), where ff is odd in yy and gg is even in yy.
  • Nonlinear Centers Theorem for Reversible Systems: If the origin x=0x^* = 0 is a linear center for the continuously differentiable system x˙=f(x,y)\dot{x} = f(x, y), and the system is reversible, then sufficiently close to the origin, all trajectories are closed curves.
  • Heteroclinic trajectories or saddle connections: connect different saddle points.
  • General definition of reversibility: a mapping R(x)R(x) satisfies R2(x)=xR^2(x) = x.
EXAMPLE 6.6.3:
  • System: x˙=xycos(y)\dot{x} = -x - y - cos(y), y˙=yxcos(x)\dot{y} = y - x - cos(x).
  • Reversible, but not conservative.

6.7 Pendulum

  • Equation of motion: θ¨+gLsin(θ)=0\ddot{\theta} + \frac{g}{L}sin(\theta) = 0.
  • Nondimensionalized equation: θ¨+sin(θ)=0\ddot{\theta} + sin(\theta) = 0.
  • Corresponding system in the phase plane: θ˙=v\dot{\theta} = v, v˙=sin(θ)\dot{v} = -sin(\theta).
  • Fixed points: (θ<em>,v</em>)=(kπ,0)(\theta^<em>, v^</em>) = (k\pi, 0), where kk is any integer.
  • Nonlinear Center Theorem implies the origin is a nonlinear center.
  • Energy function: E=12v2cos(θ)E = \frac{1}{2}v^2 - cos(\theta).
  • Cylindrical Phase Space: incorporating the geometric difference between linear velocity and the angle, it is more illuminating to look at the phase portrait on a cylinder.
  • Damping: θ¨+bθ˙+sin(θ)=0\ddot{\theta} + b\dot{\theta} + sin(\theta) = 0, where b > 0 is the damping strength.

6.8 Index Theory

  • Provides global information about the phase portrait.

  • Index of a Closed Curve: an integer that measures the winding of the vector field on C.

    I<em>C=12π[ϕ]</em>CI<em>C = \frac{1}{2\pi} [\phi]</em>C

  • Where ϕ\phi is a smooth vector field in phase plane and C is closed curve.

  • Index of a Point: I=IC\begin{aligned} I = I_C\end{aligned}

  • Properties: A closed curve C surrounds n isolated fixed points x<em><em>1,,x</em></em>nx^<em><em>1 , … , x^</em></em>n:

    I<em>C=I</em>1+I<em>2++I</em>n\begin{aligned} I<em>C = I</em>1 + I<em>2 + … + I</em>n \end{aligned}

    Where I<em>kI<em>k is the index of x</em>kx^*</em>k, for k=1,,nk = 1, …, n.

  • Theorem 6.8.2: Any closed orbit in the phase plane must enclose fixed points whose indices sum to +1. Has many practical consequences in determining systems dynamics.
    Example 6.8.1-6, discuss Index theory and its applications. Integral formula for the index of a curve.