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84     CHAPTER 3  The Laplace Transform


                                 To solve for the constants, observe that if we added the fractions on the right the numerator would
                                 have to equal the numerator 2s − 1 of the fraction on the left. Therefore,

                                              A(s + 1)(s + 3) + B(s − 1)(s + 3) + C(s − 1)(s + 1) = 2s − 1.
                                 We can solve for A, B, and C by inserting values of s into this equation. Put s = 1 to get 8A = 1,
                                 so A = 1/8. Put s =−1 to get −4B =−3, so B = 3/4. Put s =−3 to get 8C =−7, so C =−7/8.
                                 Then
                                                              1   1    3  1    7  1
                                                        Y(s) =       +       −       .
                                                              8 s − 1  4 s + 1  8 s + 3
                                 Invert this to obtain the solution
                                                                 1    3     7
                                                                        −t
                                                                   t
                                                           y(t) = e + e − e   −3t .
                                                                 8    4     8
                                    Partial fractions decompositions are frequently used with the Laplace transform. The
                                 appendix at the end of this chapter reviews the algebra of this technique.
                                    Notice that the transform method does not first produce the general solution and then solve
                                 for the constants to satisfy the initial conditions. Equations (3.1), (3.2), and (3.3) insert the initial
                                 conditions directly into an algebraic equation for the transform of the unknown function. Still,
                                 we could have solved the problem of Example 3.3 by methods from Chapter 2. The object here
                                 was to illustrate a technique. This technique extends to problems beyond the reach of methods
                                 from Chapter 2, and this is the subject of the next section.



                        SECTION 3.2        PROBLEMS



                                                                               2

                     In each of Problems 1 through 10, use the Laplace trans-  8. y + 9y = t ; y(0) = y (0) = 0

                     form to solve the initial value problem.
                                                                    9. y + 16y = 1 + t; y(0) =−2, y (0) = 1


                      1. y + 4y = 1; y(0) =−3                      10. y − 5y + 6y = e ; y(0) = 0, y (0) = 2

                                                                                   −t




                      2. y − 9y = t; y(0) = 5                      11. Prove Theorem 3.1. Hint: Write
                      3. y + 4y = cos(t); y(0) = 0


                                                                                          ∞
                                −t
                      4. y + 2y = e ; y(0) = 1                                  L[ f ](s) =  e −st  f (t)dt



                                                                                         0
                      5. y − 2y = 1 − t; y(0) = 4

                      6. y + y = 1; y(0) = 6, y (0) = 0                and integrate by parts.





                      7. y − 4y + 4y = cos(t); y(0) = 1, y (0) =−1  12. Derive equation (3.3). Hint: Integrate by parts twice.
                     3.3         Shifting and the Heaviside Function
                                 The shifting theorems of this section will enable us to solve problems involving pulses and other
                                 discontinuous forcing functions.
                                 3.3.1  The First Shifting Theorem
                                                                    at
                                 We will show that the Laplace transform of e f (t) is the transform of f (t), shifted a units to the
                                 right. This shift is achieved by replacing s by s − a in F(s) to obtain F(s − a).
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                                   October 14, 2010  14:14   THM/NEIL   Page-84         27410_03_ch03_p77-120
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