STEP-BY-STEP ANSWER:
Step 1: Assume a solution of the form u(r,θ)= R(r) Θ(θ) and substitute into Laplace’s equation in polar coordinates: u_rr + (1/r) u_r + (1/r^2) u_θθ = 0.
Step 2: Separate the variables by introducing a separation constant λ. This leads to two ODEs: r^2 R''(r) + r R'(r) - λR(r) = 0 and Θ''(θ) + λΘ(θ) = 0.
Step 3: Solve the angular equation. For periodicity, choose λ = n^2 (n = 0, 1, 2, …) so that Θ(θ)= A_n cos nθ + B_n sin nθ.
Step 4: Solve the radial equation which becomes Euler’s equation with solutions R(r)= C_n r^n + D_n r^(-n). Boundedness as r→0 forces D_n = 0.
Step 5: Compose the full solution and match the boundary condition at r=1, expanding f(θ) into its Fourier series to determine coefficients.
Final Answer: u(r,θ)= A_0 + Σ_{n=1}^∞ (A_n cos nθ + B_n sin nθ) r^n, with Fourier coefficients determined by A_0= (1/2π)∫_0^(2π)f(θ)dθ, A_n= (1/π)∫_0^(2π)f(θ) cos nθ dθ, and B_n= (1/π)∫_0^(2π)f(θ) sin nθ dθ.