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102    CHAPTER 3  The Laplace Transform

                              −t  
  t
                     19. f (t) = e +  f (t − τ)dτ                      Show that
                                  0
                                     
  t                                           ∞
                     20. f (t) =−1 + t − 2  f (t − τ)sin(τ)dτ
                                      0                                 F(s)G(s) =  L[H(t − τ) f (t − τ)](s)g(τ)dτ.
                                
  t
                     21, f (t) = 3 +  f (τ)cos(2(t − τ))dτ                        0
                                 0
                                             2τ
                     22. f (t) = cos(t) + e −2t  
  t  f (τ)e dτ       Use the definitions of the Heaviside function and of
                                       0
                                                                       the transform to obtain
                     23. Solve for the replacement function r(t) if f (t) = A,
                                                                                     ∞   ∞

                        constant, and m(t) = e −kt  with k a positive constant.  F(s)G(s) =  e −st g(τ) f (t − τ)dτ.
                        Graph r(t).                                                  0  τ
                     24. Solve for the replacement function r(t) if f (t) = A +  Reverse the order of integration to obtain
                        Bt and m(t) = e −kt .Graph r(t).
                                                                                     ∞     t  −st

                     25. Solve for the replacement function r(t) if f (t) = A +  F(s)G(s) =  e  g(τ) f (t − τ)dτ dt
                                                                                    0  0
                        Bt + Ct and m(t) = e −kt .Graph r(t).
                              2
                                                                                     ∞

                     26. Prove the convolution theorem. Hint: First write         =   e  −st ( f ∗ g)(t)dt.
                                                                                    0
                                          ∞

                               F(s)G(s) =  F(s)e  −sτ g(τ)dτ.          From this, show that L[ f ∗ g](s) = F(s)G(s).
                                         0
                     3.5         Impulses and the Delta Function
                                   Informally, an impulse is a force of extremely large magnitude applied over an extremely
                                   short period of time (imagine hitting your thumb with a hammer). We can model this idea
                                   as follows. First, for any positive number   consider the pulse δ   defined by
                                                                  1
                                                           δ   (t) = [H(t) − H(t −  )].

                                       This pulse, which is graphed in Figure 3.22, has magnitude (height) of 1/  and dura-
                                   tion of  .The Dirac delta function is thought of as a pulse of infinite magnitude over an
                                   infinitely short duration and is defined to be

                                                                δ(t) = lim δ   (t).
                                                                       →0+





                                                                    δ (t)
                                                                     ε
                                                                      1/ε





                                                                    ε               t










                                                         FIGURE 3.22 δ   (t)



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                                   October 14, 2010  14:14  THM/NEIL    Page-102        27410_03_ch03_p77-120
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