Page 59 - 4811
P. 59

Complex inversion formula


                  Consequently, (4.11) yields


                        ∫                            ∫   π                                      π
                                                2M       2   2Rtφ        2M         π      2Rtφ  2
                                  ts                          −                             −
                               e F(s)ds ≤                  e    π  dφ =         ·        e    π    =

                                               R p−1                     R p−1   −2Rt
                           BCD                           0                                        0
                                               Mπ
                                            =       (1 − e −Rt ) → 0 as R → ∞.                             2
                                                 p
                                               R t
                                                 ts
                  Over the arc AB, we have |e | ≤ e       tx  = c for fixed t > 0, and the length of AB,
                  l(AB), remains bounded as R → ∞, so that

                                           ∫
                                                                cMl(AB)
                                                   ts

                                                 e F(s)ds ≤                   → 0
                                                                    R p
                                              AB
                  as R → ∞. Here we have taken x to be the value through which the Bromwich line
                  passes, as in Figure 4.1.
                  Likewise,
                                            ∫
                                                   ts

                                                  e F(s)ds → 0 as R → ∞.

                                               DE
                  As a consequence, we have our desired conclusion:
                                                       ∫
                                                              ts
                                                  lim       e F(s)ds = 0.
                                                 R→∞
                                                         C R
               . . . .




                   Remark 4.1E Some considerations:
                     1. We could have replaced the growth condition (4.8) with

                                                            |F(s)| ≤ ε R ,

                        where ε R → 0 as R → ∞, uniformly for s on C R . For example,

                                                                    log s
                                                            F(s) =
                                                                      s

                        does satisfy this latter condition but not (4.8).
                     2. If c R is any subarc of C R , say given by π/2 ≤ θ ≤ θθ ≤ 3π/2, then
                                                                                 ′
                                                                          ′
                                                                          1
                                                                                 2
                                                   ∫  θ ′ 2         ∫  3π
                                                                       2
                                                        e Rt cos θ dθ ≤  e Rt cos θ dθ
                                                     θ ′ 1           π 2
                        as the integrand is positive. Since the right-hand integral features in (4.10)
                        and is ultimately bounded above by a quantity that tends to zero as R → 0,
                        we deduce that
                                                            ∫
                                                                 ts
                                                       lim      e F(s)ds = 0.
                                                       R→∞
                                                             C R
                     3. Sometimes it is advantageous to use parabolas or other contours instead of
                        semicircles.
               . . . . .


                                                              58
   54   55   56   57   58   59   60   61   62   63   64