logo

Solving the Laplace Equation Independent of the Jet Axis in Cylindrical Coordinates Using the Method of Separation of Variables 📂Mathematical Physics

Solving the Laplace Equation Independent of the Jet Axis in Cylindrical Coordinates Using the Method of Separation of Variables

Theorem

The general solution of the Laplace’s equation with cylindrical symmetry in the cylindrical coordinate system is as follows.

V(s,ϕ)=A0lns+B0+k=1(Aksk++Bksk)(Ckcoskϕ+Dksinkϕ) V(s,\phi) = A_{0} \ln s +B_{0} +\sum \limits _{k=1} ^\infty ( A_{k} s^k ++ B_{k} s^{-k} )( C_{k}\cos k\phi + D_{k}\sin k\phi)

Proof

Step 0

When boundary conditions are more easily represented in cylindrical coordinates, one has to solve the Laplace’s equation for cylindrical coordinates. The Laplace’s equation in cylindrical coordinates is as follows. (Reference1, Reference2)

2V=1ss(sVs)+1s22Vϕ2+2Vz2=0 \nabla ^2 V = \dfrac{1}{s} \dfrac{\partial }{ \partial s} \left( s\dfrac{\partial V}{\partial s} \right) + \dfrac{1}{s^2} \dfrac{\partial ^2 V}{\partial \phi^2 } +\dfrac{\partial ^2 V }{\partial z^2 }=0

Let’s say that the potential VV is a function independent of zz. In other words, it’s assumed that the value of VV does not change when only zz varies while other values remain the same. Then, the change in VV due to zz is 00, which means the third term disappears.

1ss(sVs)+1s22Vϕ2=0(1) \dfrac{1}{s} \dfrac{\partial }{ \partial s} \left( s\dfrac{\partial V}{\partial s} \right) + \dfrac{1}{s^2} \dfrac{\partial ^2 V}{\partial \phi^2 } =0 \tag{1}

Suppose that the potential V(s,ϕ)V(s,\phi) is a function possible to separate variables. It means that VV is composed of the product of a function S(s)S(s) solely of ss and a function Φ(ϕ)\Phi (\phi) solely of ϕ\phi. If we insert V(s,ϕ)=S(s)Φ(ϕ)V(s,\phi)=S(s) \Phi (\phi) into (1)(1), it becomes the following.

1sdds(sdSds)Φ+1s2d2Φdϕ2S=0 \dfrac{1}{s} \dfrac{d }{d s} \left( s \dfrac{d S}{d s} \right) \Phi + \dfrac{1}{s^2} \dfrac{d ^2 \Phi }{d \phi ^2 } S=0

Multiplying both sides by s2SΦ\dfrac{s^2}{S \Phi} yields

sSdds(sdSds)+1Φd2Φdϕ2=0 \dfrac{s}{S} \dfrac{d }{d s} \left( s \dfrac{d S}{d s} \right) + \dfrac{1}{\Phi} \dfrac{d ^2 \Phi }{d \phi ^2 } =0

For this equation to hold, both the first and the second terms must be constants. This is because the first term is affected when ss changes, but the second term is unaffected by ss. However, their sum must result in 00, leading to the entire first term being a constant. Similarly, the second term is also a constant.

sSdds(sdSds)=C1 \dfrac{s}{S} \dfrac{d }{d s} \left( s \dfrac{dS}{ds} \right) = C_{1}

1Φd2Φdϕ2=C2 \dfrac{1}{\Phi} \dfrac{ d^2 \Phi} {d \phi ^2} =C_2

(1)(1)’s complex partial differential equation is transformed into two simple ordinary differential equations. Solving each differential equation to find S(s)S(s) and Φ(ϕ)\Phi (\phi) and multiplying them gives us the desired V(s,ϕ)V(s,\phi). Since C1+C2=0C_{1}+C_2=0, the two constants are of the same magnitude but opposite in sign. Here, C2C_2 must be a negative constant. This is because the differential equation’s solution turns out to be in the form of Φ(ϕ)=Aekϕ+Bekϕ\Phi (\phi)=Ae^{k\phi}+Be^{-k\phi} when C2C_2 is positive (Solution Reference). Being a cylindrical coordinate system, Φ(ϕ)=Φ(ϕ+2π)\Phi (\phi) = \Phi (\phi+2\pi) must be satisfied, but the aforementioned equation does not. Therefore, C1C_{1} is a positive constant, and C2C_2 is a negative constant.

sSdds(sdSds)=k2 \dfrac{s}{S} \dfrac{d }{d s} \left( s \dfrac{dS}{ds} \right) =k^2

1Φd2Φdϕ2=k2 \dfrac{1}{\Phi} \dfrac{ d^2 \Phi} {d \phi ^2} =-k^2

Step 1

1Φd2Φdϕ2=k2 \dfrac{1}{\Phi} \dfrac{ d^2 \Phi} {d \phi ^2} =-k^2

The solution to the above differential equation is well-known to be Φ(ϕ)=e±ikϕ\Phi (\phi)=e^{\pm ik \phi}. (Reference) Hence, the general solution is

Φ(ϕ)=Aeikϕ+Beikϕ \Phi (\phi) = A e^{ik\phi} + Be^{-ik\phi}

Using Euler’s formula eiθ=cosθ+isinθe^{i\theta}=\cos \theta + i\sin \theta, it can be represented as follows.

Φ(ϕ)=Acoskϕ+Bsinkϕ \Phi ( \phi) = A\cos k\phi + B \sin k\phi

Here, AA and BB are complex constants, different from the constants mentioned before. Let’s now check if Φ(ϕ)=Φ(ϕ+2π)\Phi (\phi)=\Phi (\phi+2\pi) is satisfied.

Φ(ϕ+2π)=Acosk(ϕ+2π)+Bsink(ϕ+2π)=Acos(kϕ+2kπ)+Bsin(kϕ+2kπ) \begin{align*} \Phi (\phi+2\pi) &= A\cos k(\phi +2\pi) + B \sin k(\phi+2\pi) \\ &= A\cos (k\phi +2k\pi) + B \sin (k\phi+2k\pi) \end{align*}

If k=0,±1,±2,k= 0, \pm 1, \pm 2, \cdots then

Φ(ϕ)=Acos(kϕ)+Bsin(kϕ)=Φ(ϕ) \begin{align*} \Phi (\phi) &= A\cos (k\phi) + B \sin (k\phi) \\ &= \Phi ( \phi) \end{align*}

Hence, the solution is

Φ(ϕ)=Acoskϕ+Bsinkϕ(k=0,1,2) \Phi ( \phi) = A\cos k\phi + B \sin k\phi\quad (k=0,1,2\cdots)

In the case of negative values, it overlaps with the case of positive values, so only the cases of positive values need to be documented. However, the case of k=0k=0 is actually not included in the solution. This is because, when solving the differential equation with k=0k=0,

d2Φdϕ2=0 \dfrac{ d^2 \Phi} {d \phi^2 } =0

    dΦdϕ=C \implies \dfrac{ d \Phi}{d \phi}=C

    Φ=Cϕ+D \implies \Phi=C\phi +D

we get Φ\Phi, which lacks the periodicity mentioned earlier. Thus, the final solution obtained is

Φ(ϕ)=Acoskϕ+Bsinkϕ,  (k=1,2) \Phi ( \phi) = A\cos k\phi + B \sin k\phi,\ \ (k=1,2\cdots)

Step 2

sSdds(sdSds)=k2 \dfrac{s}{S} \dfrac{d }{d s} \left( s \dfrac{dS}{ds} \right) =k^2

Simplifying the above differential equation yields

s(dSds+sd2Sds2)=k2S s\left( \dfrac{d S}{ds} + s \dfrac{d^2 S}{d s^2} \right) =k^2 S

    s2d2Sds2+sdSdsk2S=0 \implies s^2 \dfrac{d^2 S}{d s^2 } + s\dfrac{d S}{ds} -k^2 S=0

This is Euler’s equation, which can be solved in the manner described here, but in this document, it’s solved more simply. Utilizing that the solution to the differential equation comes in the form of sns^n and substituting S=snS=s^n,

s2(n)(n1)sn2+snsn1k2sn=0 s^2(n)(n-1)s^{n-2} +sns^{n-1}-k^2s^n=0

    n(n1)+nk2=0 \implies n(n-1)+n-k^2=0

    n2k2=0 \implies n^2-k^2=0

n=±k \therefore n=\pm k The two solutions of the differential equation are sks^k and sks^{-k}. The general solution is a linear combination of the two solutions, and adding the condition of kk from Step 1,

S(s)=Csk+Dsk,k=1,2, S(s) = Cs^k+Ds^{-k},\quad k=1,2,\cdots However, it’s important that S(s)S(s) exists for the case of k=0k=0. Solving the differential equation when k=0k=0 yields

sSdds(sdSds)=0 \dfrac{s}{S} \dfrac{d }{d s} \left( s \dfrac{dS}{ds} \right) =0

    dds(sdSds)=0 \implies \dfrac{ d}{ds} \left( s \dfrac{ dS }{ds} \right) =0

    sdSds=C \implies s\dfrac{dS}{ds}=C

    dS=Csds \implies dS=\dfrac{C}{s} ds

    S(s)=Clns+D \implies S(s)=C\ln s +D

Thus, the final expression of the general solution is

S(s)=A0lns+B0+k=1(Aksk+Bksk) S(s)=A_{0} \ln s +B_{0} +\sum \limits _{k=1} ^\infty ( A_{k} s^k + B_{k} s^{-k})

Step 3

Combining the results of Step 1 and Step 2, the potential is as follows.

V(s,ϕ)=A0lns+B0+k=1(Aksk++Bksk)(Ckcoskϕ+Dksinkϕ) V(s,\phi) = A_{0} \ln s +B_{0} +\sum \limits _{k=1} ^\infty ( A_{k} s^k ++ B_{k} s^{-k} )( C_{k}\cos k\phi + D_{k}\sin k\phi)