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Derivation of Bessel's Equation 📂Mathematical Physics

Derivation of Bessel's Equation

Definition

The differential equation below is called the ν\nuth order Bessel’s equation.

x2y+xy+(x2ν2)y= 0x(xy)+(x2ν2)y= 0y+1xy+(1ν2x2)y= 0 \begin{align*} x^2 y^{\prime \prime} +xy^{\prime} +(x^2-\nu^2)y =&\ 0 \\ x(xy^{\prime})^{\prime} + (x^2- \nu ^2) y =&\ 0 \\ y^{\prime \prime}+\frac{1}{x} y^{\prime} + \left( 1-\frac{\nu^{2}}{x^{2}} \right)y =&\ 0 \end{align*}

Description

The solution to the Bessel’s equation is called the Bessel function.

Bessel functions are often seen in physics, engineering, and more, especially in problems involving cylindrical symmetry. For this reason, Bessel functions are also known as cylinder functions, though this term is less commonly used.

Derivation

In two-dimensional polar coordinates, the wave equation is given as follows.

2ut2=c2(2ur2+1rur+1r22uθ2) \begin{equation} \dfrac{\partial ^2 u}{\partial t^2} = c^2 \left( \dfrac{\partial ^2 u}{\partial r^2}+\frac{1}{r}\dfrac{\partial u}{\partial r}+\frac{1}{r^2} \dfrac{\partial ^2 u}{\partial \theta ^2}\right) \end{equation}

cc is a constant. Let’s assume that the solution uu to the above equation is a function that can be separated into variables.

u(t,r,θ)=T(t)R(r)Θ(θ) u(t, r, \theta)=T(t)R(r)\Theta (\theta)

Substituting (1)(1) gives

TRΘ=c2(TRΘ+1rTRΘ+1r2TRΘ) T^{\prime \prime}R\Theta=c^2\left( TR^{\prime \prime}\Theta + \dfrac{1}{r}TR^{\prime}\Theta + \frac{1}{r^2}TR\Theta^{\prime \prime} \right)

Dividing both sides by c2TRΘc^2TR\Theta gives

Tc2T=RR+RrR+Θr2Θ \dfrac{T^{\prime \prime}}{c^2T}=\dfrac{R^{\prime \prime}}{R}+\dfrac{R^{\prime}}{rR}+\dfrac{\Theta^{\prime \prime}}{r^2\Theta}

The left-hand side is a function solely of tt, and the right-hand side is a function of rr and θ\theta, thus both sides of the equation must be constant. If the left-hand side were not constant with respect to tt, changing the value of tt would change the left-hand side without altering the right, breaking the equality. Therefore, for all tt, rr, and θ\theta, both sides must be constant. Let’s call this constant μ2-\mu ^2. Then,

Tc2T=RR+RrR+Θr2Θ=μ2 \begin{equation} \dfrac{T^{\prime \prime}}{c^2T}=\dfrac{R^{\prime \prime}}{R}+\dfrac{R^{\prime}}{rR}+\dfrac{\Theta^{\prime \prime}}{r^2\Theta}=-\mu^2 \end{equation}

First, let’s examine the equation for rr and θ\theta.

RR+RrR+Θr2Θ=μ2 \dfrac{R^{\prime \prime}}{R}+\dfrac{R^{\prime}}{rR}+\dfrac{\Theta^{\prime \prime}}{r^2\Theta}=-\mu^2

Multiply both sides by r2r^2 and separate the equation into terms for rr and θ\theta,

r2RR+rRR+r2μ2=ΘΘ \dfrac{r^2R^{\prime \prime}}{R}+\dfrac{rR^{\prime}}{R}+r^2\mu^2=-\dfrac{\Theta^{\prime \prime}}{\Theta}

Both sides of the equation, for reasons mentioned earlier, must also be constant. Let’s call this constant ν2\nu^2. Then, we get the following equation.

ΘΘ=ν2    Θ=ν2Θ \begin{equation} -\dfrac{\Theta^{\prime \prime}}{\Theta}=\nu^2 \quad \implies \quad \Theta^{\prime \prime} =-\nu^2 \Theta \quad \end{equation}

Returning to (2)(2) and organizing the equation for tt yields

T=c2μ2T \begin{equation} T^{\prime \prime}=-c^2\mu^2T \end{equation}

Substituting (3)(3) and (4)(4) into (2)(2) and organizing appropriately gives the following.

c2μ2Tc2T=RR+RrR+ν2Θr2Θ    1RR+1rRR+(μ2ν2r2)=0    r2R(r)+rR(r)+(μ2r2ν2)R(r)=0 \begin{align*} &&\dfrac{-c^2 \mu^2 T}{c^2T}=\dfrac{R^{\prime \prime}}{R}+\frac{R^{\prime}}{rR}+\dfrac{-\nu^2\Theta}{r^2\Theta} \\ \implies &&\frac{1}{R}R^{\prime \prime}+\dfrac{1}{rR}R^{\prime}+\left(\mu^2-\frac{\nu^2}{r^2}\right) =0 \\ \implies && r^2R^{\prime \prime}(r)+rR^{\prime}(r)+(\mu^2r^2-\nu^2)R(r)=0 \end{align*}

Now, let’s introduce a substitution μr=x\mu r=x. And then let it be as follows.

R(r)=f(μr)=f(x),R(r)=μf(μr)=μf(x),R(r)=μ2f(μr)=μ2f(x) R(r)=f(\mu r)=f(x),\quad R^{\prime}(r)=\mu f^{\prime}(\mu r)=\mu f^{\prime}(x),\quad R^{\prime \prime}(r)=\mu^2 f^{\prime \prime}(\mu r)=\mu^2 f^{\prime \prime}(x)

Substituting these equations into the ones we obtained earlier gives

x2μ2μ2f(x)+xμμf(x)+(x2ν2)f(x)=0    x2f(x)+xf(x)+(x2ν2)f(x)=0 \begin{align*} && \frac{x^2}{\mu^2}\mu^2f^{\prime \prime}(x) + \dfrac{x}{\mu}\mu f(x)+(x^2-\nu^2)f(x)&= 0 \\ \implies && x^2f^{\prime \prime}(x) + x f(x)+(x^2-\nu^2)f(x)&= 0 \end{align*}

The above equation is known as the ν\nuth order Bessel’s equation. It is commonly found in the following form.

x2y+xy+(x2ν2)y=0x(xy)+(x2ν2)y=0 \begin{align*} x^2 y^{\prime \prime} +xy^{\prime} +(x^2-\nu^2)y&= 0 \\ x(xy^{\prime})^{\prime}+(x^2 \nu ^2) y&= 0 \end{align*}

The first solution to this equation is as follows, and it is called the first kind Bessel function.

Jν(x)=n=0(1)nΓ(n+1)Γ(n+ν+1)(x2)2n+ν J_{\nu}(x)=\sum \limits_{n=0}^{\infty}\frac{(-1)^{n}}{\Gamma (n+1)\Gamma (n+\nu+1)} \left( \frac{x}{2} \right)^{2n+\nu}

The second solution is as follows, and it is called the second kind Bessel function.​​​

Nν(x)=Yν(x)=cos(νπ)Jν(x)Jν(x)sin(νπ) N_{\nu}(x)=Y_{\nu}(x)=\frac{\cos (\nu \pi)J_{\nu}(x)-J_{-\nu}(x)}{\sin (\nu\pi)}

Therefore, the general solution to the Bessel’s equation is as follows.

y(x)=AJν(x)+BNν(x) y(x)=AJ_{\nu}(x)+BN_{\nu}(x)

In this case, AA and BB are constants.