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has the form of a second order Euler equation for the radial component v(r). Its solutions
                                                           k
                   are obtained by the substitution v(r) = r . We discover that this is a solution if and only
                   if
                                                   2
                                              2
                                            k − n = 0,      and hence k = ±n.
                   Therefore, for n 6= 0, we find two linearly independent solutions
                                                   n
                                          v 1 (r) = r ,  v 2 (r) = r −n , n = 1, 2, . . . .       (10.46)

                   If n = 0, there is an additional logarithmic solution
                                              v 1 (r) = 1,  v 2 (r) = ln r, n = 0.                (10.47)


                   Combining (10.44) and (10.46), (10.47), we produce a complete list of separable polar
                   coordinate solutions to the Laplace equation:

                                                       n
                                                                   n
                                                 1,   r cos nθ,   r sin nθ,                       (10.48)
                                       ln r,  r −n  cos nθ,  r −n  sin nθ  n = 1, 2, . . . .      (10.49)

                   Now, the solutions (10.48) are continuous (in fact analytic) at the origin, whereas the
                   solutions (10.49) have singularities as r = 0. The latter are not relevant since we require
                   the solution u to remain bounded and smooth - even at the center of the disk. Thus, we
                   should only use the former to form a candidate series solution

                                                        ∞
                                                       X
                                                 a 0           n            n
                                        u(r, θ) =   +     (a n r cos nθ + b n r sin nθ)           (10.50)
                                                  2
                                                       n=1
                   to the Dirichlet boundary value problem. The coefficients a n , b n will be prescribed by the
                   boundary conditions (10.40). Substituting r = 1, we find
                                                     ∞
                                                    X
                                               a 0          n
                                     u(1, θ) =    +    (a n r cos nθ + b n sin nθ) = h(θ).
                                               2
                                                    n=1
                   We recognize this as a standard Fourier series for the 2π periodic function h(θ). Therefore,

                                              π                          π
                                             Z                          Z
                                           1                          1
                                     a n =      h(θ) cos nθdθ,  b n =     h(θ) sin nθdθ           (10.51)
                                           π                          π
                                            −π                         −π
                   are precisely its Fourier coefficients.
                   Example 7.1 Consider the Dirichlet boundary value problem on the unit disk with

                                              u(1, θ) = θ  for   − π < θ < π.

                   The boundary data can be interpreted as a wire in the shape of a single turn of a spiral
                   helix sitting over the unit circle, with a jump discontinuity, of magnitude 2π, at (−1; 0).
                   Consider the function h(θ) = θ at (−π; π). Its Fourier coefficients

                                                                    2
                                               a 0 = a n = 0,  b n =  (−1) n+1 .
                                                                   n


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