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664    CHAPTER 18  The Potential Equation


                                 which is a necessary condition for this problem to have a solution. Write the solution
                                                              ∞
                                                      1    1     1     π
                                                                                          2
                                             U(r,θ) = a 0 +       r  n  cos(n(ξ − θ))cos(ξ)sin (ξ)dξ.
                                                      2    π    n    −π
                                                             n=1
                                 Evaluate this integral:
                                                           π
                                                                              2
                                                           cos(n(ξ − θ))cos(ξ)sin (ξ)dξ =
                                                         −π
                                                 ⎧
                                                 ⎪0                       for n = 2,4,5,6,7,···
                                                 ⎨
                                                   π cos(θ)/4             for n = 1
                                                 ⎪
                                                   −π cos (θ) + 3π cos(θ)/4  for n = 3.
                                                 ⎩       2
                                 The solution is
                                                        1    1         1  3     3     3
                                                U(r,θ) = a 0 + r cos(θ) + r  −cos (θ) +  cos(θ)
                                                        2    4         3              4
                                                        1    1         1           1
                                                                                     3
                                                                             3
                                                                          3
                                                      = a 0 + r cos(θ) − r cos (θ) + r cos(θ).
                                                        2    4         3           4
                                                                                                   2
                                                                                           2
                                 To convert this solution to rectangular coordinates, let x =r cos(θ) and r = x + y to obtain
                                                                                               2
                                                               1    1    1    1
                                                                                  2
                                                                                      2
                                                                           3
                                                       u(x, y) = a 0 + x − x + (x + y )
                                                               2    4    3    4
                                 with a 0 as an arbitrary constant.
                                 18.8.3 A Neumann Problem for the Upper Half-Plane
                                 To illustrate a Neumann problem for an unbounded set, consider:
                                                         2
                                                       ∇ u(x, y) = 0for −∞ < x < ∞, y > 0
                                 and
                                                         ∂u
                                                           (x,0) = f (x) for −∞ < x < ∞.
                                                         ∂y
                                    Again, notice that ∂u/∂y is the derivative of u normal to the horizontal axis, which is the
                                 boundary of the upper half-plane.
                                    Assume that
                                                                  ∞

                                                                    f (x)dx = 0
                                                                 −∞
                                 as a necessary condition for a solution to exist.
                                    We can solve this problem by separation of variables. However, there is an elegant device
                                 for reducing this problem to one we have already solved. Let
                                                                       ∂u
                                                                    v =   .
                                                                       ∂y
                                 Then
                                                                                       2
                                                                                 2
                                                      ∂  2     ∂u     ∂  2    ∂u     ∂    ∂ u  ∂ u
                                                 2
                                                ∇ v =          +          =         +     = 0.
                                                      ∂x  2  ∂y  ∂y 2  ∂y   ∂y  ∂x  2  ∂y  2

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                                   October 14, 2010  15:27  THM/NEIL   Page-664        27410_18_ch18_p641-666
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