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10.6 Phase Portraits  333


                                                                              λt
                                                                                      μt
                                                                    X(t) = c 1 E 1 e + c 2 E 2 e .
                                        Examine trajectories along an arbitrary point P 0 other than the origin.
                                           1. If P 0 is on L 1 , then c 2 = 0 and X(t) moves on part of L 1 away from the origin as t
                                              increases, because e →∞ as t →∞.
                                                              λt
                                                                                                               μt
                                           2. If P 0 is on L 2 , then c 1 =0 and X(t) moves on part of L 2 toward the origin, because e →0
                                              as t →∞. Thus, along these lines, some trajectories move toward the origin, others move
                                              away.
                                           3. Now suppose P 0 is on neither L 1 or L 2 . Then the trajectory through P 0 does not pass
                                              arbitrarily close to the origin for any times but instead moves toward the origin asymptotic
                                              to L 2 and then away from the origin asymptotic to L 1 as t increases. We may think
                                              of L 1 and L 2 as separating the plane into four regions with each trajectory confined to
                                              one region (because a trajectory starting in one of these regions cannot cross another
                                              trajectory along one of L 1 or L 2 to pass into another region). The trajectories move along
                                              L 1 away from the origin and along L 2 toward the origin or in one of the four regions these
                                              lines determine, sweeping toward and then away from the origin asymptotic to these lines.
                                              This is similar to Halley’s comet entering our solar system and moving toward the Sun,
                                              then sweeping along a curve that takes it away from the Sun.
                                           In this case, we call the origin a saddle point.
                                           The behavior we have just described can be seen in the following example.


                                 EXAMPLE 10.21
                                        The system

                                                                            −1   3

                                                                      X =           X
                                                                             2  −2
                                        has general solution

                                                                          −1   −4t     3  t
                                                                 X(t) = c 1   e   + c 2  e .
                                                                           1           2
                                        The eigenvalues of A are −4 and 1, real and of opposite sign. Figure 10.18 shows a phase portrait,
                                        with a saddle point at the origin.

                                        Case 3: A Has Equal Eigenvalues
                                        Suppose A has the eigenvalue λ of multiplicity 2. There are two possibilities.

                                        Case 3(a): A Has Two Linearly Independent Eigenvectors E 1 and E 2
                                        Now the general solution is
                                                                                     λt
                                                                     X = (c 1 E 1 + c 2 E 2 )e .
                                        If

                                                                         a           h
                                                                    E 1 =   and E 2 =   ,
                                                                         b           k
                                        then, in terms of components,
                                                                           λt
                                                                                               kt
                                                           x(t) = (c 1 a + c 2 b)e and y(t) = (c 1 h + c 2 k)e .
                                        Now
                                                                        y(t)
                                                                           = constant.
                                                                        x(t)



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                                   October 14, 2010  20:32  THM/NEIL   Page-333        27410_10_ch10_p295-342
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