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book   Mobk070    March 22, 2007  11:7








                                                                  STURM–LIOUVILLE TRANSFORMS        143
                   and this is simply


                                                       ∞
                                                           sin(λ n x)

                                              u(x, t) =          # U(λ n , t)
                                                          #       2
                                                           sin(λ n ) #
                                                      n=1
                                                          #
                   with λ n given by the transcendental equation above. The final solution is therefore
                                                  ∞
                                                      2(1 − cos λ n )
                                                                              2
                                                                            −λ t
                                         u(x, t) =        1         sin(λ n x)e  n
                                                     λ n − sin(2λ n )
                                                  n=1     2
                   9.2    GENERALIZATION: THE STURM–LIOUVILLE TRANSFORM:
                          THEORY
                   Consider the differential operator D



                                    D[ f (x)] = A(x) f + B(x) f + C(x) f   a ≤ x ≤ b             (9.1)
                   with boundary conditions of the form



                                           N α [ f (x)] x=a = f (a)cos α + f (a)sin α
                                                                                                 (9.2)

                                           N β [ f (x)] x=b = f (b)cos β + f (b)sin β
                   where the symbols N α and N β are differential operators that define the boundary conditions.
                   For example the differential operator might be


                                                      D[ f (x)] = f xx

                   and the boundary conditions might be defined by the operators

                                                 N α [ f (x)] x=a = f (a) = 0

                   and


                                             N β [ f (x)] x=b = f (b) + Hf (b) = 0

                        We define an integral transformation

                                                       b

                                           T[ f (x)] =   f (x)K(x,λ)dx = F(λ)                    (9.3)
                                                      a
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