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book   Mobk070    March 22, 2007  11:7








                     122  ESSENTIALS OF APPLIED MATHEMATICS FOR SCIENTISTS AND ENGINEERS
                                                             2 3
                                                                   4 5
                                             1               s ς   s ς
                            Since the function sinh ς s = ς +   +     + ... the function
                                             s               3!     5!
                                                            1
                                                              sinh ς s
                                                            s
                       is analytic and Y (s ) can be written as the ratio of two analytic functions
                                                                1  sinh ς s
                                                                s
                                                        Y (s ) =
                                                                s cosh s
                       Y (s ) therefore has a simple pole at s = 0 and the residue there is
                                                                            2 3
                                                                           s ς
                                                    lim           lim ς +   3!  + ...
                                       R(s = 0) =       sY (s ) =                   = gς
                                                  s → 0         s → 0     cosh s
                       The remaining poles are the singularities of cosh s . But cosh s = cosh x cos y + i sinh x sin y,
                       so the zeros of this function are at x = 0and cosy = 0.
                            Hence, s n = i(2n − 1)π/2. The residues at these points are

                                          lim     g sinh ς s   s τ  g sinh ς s n s n τ
                            R(s = s n ) =         d           e  =   2        e  (n =±1, ±2, ±3 ...)
                                        s → s n  s  (s cosh s )     s n  sinh s n
                                                  ds
                       Since
                                                   2n − 1               2n − 1

                                             sinh i       (πς) = i sin        (πς)
                                                      2                   2
                       we have
                                                             2n−1
                                                      gi sin    (πς)           2n − 1
                                       R(s = s n ) =          2          exp i       πτ
                                                      2n−1         2n−1
                                                           
 2          
         2
                                                   −      π  i sin    π
                                                       2            2
                       and
                                                         2n − 1

                                                    sin        π = (−1)  n+1
                                                           s
                            The exponential function can be written as
                                            2n − 1           2n − 1             2n − 1

                                      exp i       πτ = cos          πτ + i sin        πτ
                                              2                 2                 2
                            Note that for the poles on the negative imaginary axis (n < 0) this expression can be
                       written as

                                           2m − 1            2m − 1             2m − 1
                                     exp i        πτ = cos          πτ − i sin         πτ
                                              2                 2                  2
                       where m =−n > 0. This corresponds to the conjugate poles.
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