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1      ν
                                                          x
                                              J ν (x) →       ,
                                                      ν! 2
                                                                   ν

                                                        (ν − 1)!  2
                                              N ν (x) →−             .
                                                           π     x
                        Because J ν (x) and N ν (x) oscillate for large argument, they can represent standing waves
                        along the radial direction. However, N ν (x) is unbounded for small x and is inappropriate
                        for regions containing the origin. The Hankel functions become complex exponentials for
                        large argument, hence represent traveling waves. Finally, K ν (x) is unbounded for small x
                        and cannot be used for regions containing the origin, while I ν (x) increases exponentially
                        for large x and cannot be used for unbounded regions.


                        Examples.   Consider the boundary value problem for Laplace’s equation
                                                         2
                                                        ∇ V (ρ, φ) = 0                        (A.126)
                        in the region

                                           0 ≤ ρ ≤∞,    0 ≤ φ ≤ φ 0 ,  −∞ < z < ∞,
                        where the boundary conditions are

                                                 V (ρ, 0) = 0,  V (ρ, φ 0 ) = V 0 .

                        Since there is no z-dependence we let k z = 0 in (A.120) and choose a z = 0. Then
                                  2
                              2
                         2
                        k = k − k = 0 since k = 0. There are two possible solutions, depending on whether
                                  z
                         c
                        k φ is zero. First let us try k φ  = 0. Using (A.123) and (A.125) we have
                                      V (ρ, φ) = [A φ sin(k φ φ) + B φ cos(k φ φ)][a ρ ρ −k φ  + b ρ ρ ].  (A.127)
                                                                                   k φ
                        Assuming k φ > 0 we must have b ρ = 0 to keep the solution finite. The condition
                        V (ρ, 0) = 0 requires B φ = 0.Thus
                                                   V (ρ, φ) = A φ sin(k φ φ)ρ  −k φ .

                        Our final boundary condition requires
                                               V (ρ, φ 0 ) = V 0 = A φ sin(k φ φ 0 )ρ −k φ .

                        Because this cannot hold for all ρ, we must resort to k φ = 0 and

                                               V (ρ, φ) = (a φ φ + b φ )(a ρ ln ρ + b ρ ).    (A.128)
                        Proper behavior as ρ →∞ dictates that a ρ = 0. V (ρ, 0) = 0 requires b φ = 0.Thus
                        V (ρ, φ) = V (φ) = b φ φ. The constant b φ is found from the remaining boundary condition:
                        V (φ 0 ) = V 0 = b φ φ 0 so that b φ = V 0 /φ 0 . The final solution is

                                                       V (φ) = V 0 φ/φ 0 .

                        It is worthwhile to specialize this to φ 0 = π/2 and compare with the solution to the same
                        problem found earlier using rectangular coordinates. With a = 0 in (A.116) we have

                                                         2     ∞  −k y x  sin k y y
                                                V (x, y) =     e         dk y .
                                                         π  0        k y



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