PDES: SEPARATION OF VARIABLES AND OTHER METHODS
Thus, writingu(ρ, φ)=P(ρ)Φ(φ) and using the expression (21.23), Laplace’s
equation (21.26) becomes
Φ
ρ
∂
∂ρ
(
ρ
∂P
∂ρ
)
+
P
ρ^2
∂^2 Φ
∂φ^2
=0.
Now, employing the same device as previously, that of dividing through by
u=PΦ and multiplying through byρ^2 , results in the separated equation
ρ
P
∂
∂ρ
(
ρ
∂P
∂ρ
)
+
1
Φ
∂^2 Φ
∂φ^2
=0.
Following our earlier argument, since the first term on the RHS is a function of
ρonly, whilst the second term depends only onφ, we obtain the twoordinary
equations
ρ
P
d
dρ
(
ρ
dP
dρ
)
=n^2 , (21.27)
1
Φ
d^2 Φ
dφ^2
=−n^2 , (21.28)
where we have taken the separation constant to have the formn^2 for later
convenience; for the present,nis a general (complex) number.
Let us first consider the case in whichn= 0. The second equation, (21.28), then
has the general solution
Φ(φ)=Aexp(inφ)+Bexp(−inφ). (21.29)
Equation (21.27), on the other hand, is the homogeneous equation
ρ^2 P′′+ρP′−n^2 P=0,
which must be solved either by trying a power solution inρor by making the
substitutionρ=exptas described in subsection 15.2.1 and so reducing it to an
equation with constant coefficients. Carrying out this procedure we find
P(ρ)=Cρn+Dρ−n. (21.30)
Returning to the solution (21.29) of the azimuthal equation (21.28), we can
see that if Φ, and henceu, is to be single-valued and so not change whenφ
increases by 2πthennmust be an integer. Mathematically, other values ofnare
permissible, but for the description of real physical situations it is clear that this
limitation must be imposed. Having thus restricted the possible values ofnin
one part of the solution, the same limitations must be carried over into the radial
part, (21.30). Thus we may write a particular solution of the two-dimensional
Laplace equation as
u(ρ, φ)=(Acosnφ+Bsinnφ)(Cρn+Dρ−n),