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book   Mobk070    March 22, 2007  11:7








                     82  ESSENTIALS OF APPLIED MATHEMATICS FOR SCIENTISTS AND ENGINEERS
                       must be zero. The boundary condition at ζ = 1is

                                       Z ζ =−C 1 (γ L/r 1 )sin(γ L/r 1 ) = 0,  or  γ L/r 1 = nπ     (5.39)

                       The boundary condition at η = 1 requires

                                                    C 3 [J (β) + BJ 0 (β)] = 0or

                                                        0
                                                                                                    (5.40)
                                                    BJ 0 (β) = β J 1 (β)
                       which is the transcendental equation for finding β m . Also note that

                                                                2
                                                           2
                                                          λ = γ + β  2 m                            (5.41)
                                                                n
                       By superposition we write the final form of the solution as
                                                     ∞   ∞
                                                                      2
                                                                   2
                                                                −(γ +β )τ
                                        U(τ, η, ς) =       K nm e  n  m  J 0 (β m η)cos(nπς)        (5.42)
                                                     n=0 m=0
                       K nm is found using the orthogonality properties of J 0 (β m η) and cos(nπζ) after using the initial
                       condition.

                             1              1                     1              1

                                                                                      2
                                                                      2
                               rJ 0 (β m η)dη  cos(nπς)dς = K nm   rJ (β m η)dη    cos (nπς)dς      (5.43)
                                                                      0
                           r=0           ς=−1                   r=0           ς=−1
                       Example 5.5 (Heat transfer in a sphere). Consider heat transfer in a solid sphere whose
                       surface temperature is a function of θ, the angle measured downward from the z-axis (see Fig.
                       1.3, Chapter 1). The problem is steady and there is no heat source.

                                                  ∂ 2        1  ∂       ∂u
                                                r   (ru) +          sin θ    = 0
                                                 ∂r 2      sin θ ∂θ     ∂θ
                                                u(r = 1) = f (θ)                                    (5.44)

                                                u is bounded
                       Substituting x = cos θ,

                                                   ∂ 2       ∂          ∂u
                                                                      2
                                                 r   (ru) +     (1 − x )    = 0                     (5.45)
                                                  ∂r 2      ∂x          ∂x
                       We separate variables by assuming u = R(r)X(x). Substitute into the equation, divide by RX
                       and find
                                                                   2
                                                  r         [(1 − x )X ]

                                                                              2
                                                    (r) =−               =±λ                        (5.46)
                                                  R              X
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