General Solution to the Laplace Equation in Spherical Coordinates
📂Partial Differential EquationsGeneral Solution to the Laplace Equation in Spherical Coordinates
Theorem
In spherical coordinates, the Laplace equation is as follows:
∇2f=r21∂r∂(r2∂r∂f)+r2sinθ1∂θ∂(sinθ∂θ∂f)+r2sin2θ1∂2ϕ∂2f=0
Explanation
Assuming that f can be separated into variables as f(r,θ,ϕ)=R(r)Θ(θ)Φ(ϕ), the general solution for the radial component can be derived by solving the Euler differential equation as follows:
R(r)=l=0∑∞Rl(r)=l=0∑∞(Alrl+rl+1Bl)
The solutions for the polar angle θ and the azimuthal angle ϕ are specifically called spherical harmonics, as follows:
Ylm(θ,ϕ)=eimϕPlm(cosθ)
Here, Plm is the associated Legendre polynomial. Where l is a non-negative integer, and m is an integer that satisfies −l≤m≤l. Therefore, the general solution for θ and ϕ components is as follows:
Θ(θ)Φ(ϕ)=l=0∑∞m=−l∑leimϕPlm(cosθ)
Combining the two results above, the general solution of the Laplace equation in spherical coordinates can be obtained as follows:
f(r,θ,ϕ)=R(r)Θ(θ)Φ(ϕ)=l=0∑∞m=−l∑l(Alrl+rl+1Bl)eimϕPlm(cosθ)
If the radial component has symmetry, the solution to the Laplace equation is a spherical harmonic. In the case of symmetry regarding the azimuthal angle ϕ, the solution is as follows:
f(r,θ)=l=0∑∞(Alrl+rl+1Bl)Pl(cosθ)
Here, Pl(x) is the Legendre polynomial.