Page 97 - Essentials of applied mathematics for scientists and engineers
P. 97

book   Mobk070    March 22, 2007  11:7








                                                 SOLUTIONS USING FOURIER SERIES AND INTEGRALS        87
                   Separation of variables as y = T(τ)R(η)S(θ), substituting into the equation and dividing by
                   TRS,
                                             T      1           1 S
                                                                          2
                                                 =     (ηR ) +       =−λ                        (5.79)
                                                                2
                                              T     ηR         η S
                   The negative sign is because we anticipate sine and cosine solutions for T.
                        We also note that
                                                     η           S
                                               2 2                        2
                                              λ η +   (ηR ) =−      =±β                         (5.80)
                                                     R            S
                   To avoid exponential solutions in the θ direction we must choose the positive sign. Thus we
                   have
                                                                      2

                                                             T =−λ T
                                                                      2
                                                              S =−β S                           (5.81)

                                                          2 2
                                                                 2
                                               η(ηR ) + (η λ − β )R = 0

                   The solutions of the first two of these are
                                               T = A 1 cos(λτ) + A 2 sin(λτ)
                                                                                                (5.82)
                                                S = B 1 cos(βθ) + B 2 sin(βθ)

                   The boundary condition on the initial velocity guarantees that A 2 = 0. β must be an integer so
                   that the solution comes around to the same place after θ goes from 0 to 2π.Either B 1 and B 2
                   can be chosen zero because it doesn’t matter where θ begins (we can adjust f (r,θ)).
                                              T(τ)S(θ) = AB cos(λτ)sin(nθ)                      (5.83)

                   The differential equation for R should be recognized from our discussion of Bessel functions.
                   The solution with β = n is the Bessel function of the first kind order n. The Bessel function
                   of the second kind may be omitted because it is unbounded at r = 0. The condition that
                   R(1) = 0 means that λ is the mth root of J n (λ mn ) = 0. The solution can now be completed
                   using superposition and the orthogonality properties.
                                                 ∞   ∞

                                     y(τ, η, θ) =       K nm J n (λ mn η)cos(λ mn τ)sin(nθ)     (5.84)
                                                 n=0 m=1
                   Using the initial condition

                                                     ∞  ∞

                                           f (η, θ) =      K nm J n (λ mn η)sin(nθ)             (5.85)
                                                    n=0 m=1
   92   93   94   95   96   97   98   99   100   101   102