Solving Schrödinger's Equation for Cylindrical Boundaries

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Homework Statement


I must get the first eigenvalues of the time independent Schrödinger's equation for a particle of mass m inside a cylinder of height h and radius a where ##h \sim a##.
The boundary conditions are that psi is worth 0 everywhere on the surface of the cylinder.

Homework Equations


##-\frac{\hbar ^2}{2m} \triangle \psi =E \psi##.
Laplacian in cylindrical coordinates.

The Attempt at a Solution


I've used separation of variables on the PDE, seeking for the solutions of the form ##\psi (\rho, \theta , z)=R(\rho) \Theta (\theta ) Z(z)##.
I reached that ##\frac{Z''}{Z}=\text{constant}=-\lambda ^2##. Assuming that the Z function is periodic and worth 0 at the top and bottom of the cylinder, I reached that ##Z(z)=B \sin \left ( \frac{n\pi n}{h} \right )## where n=1,2, 3, etc.
Then I reached that ##\frac{\Theta''}{\Theta} = -m^2## where m=0, 1, 2, etc (because it must be periodic with period 2 pi). So that ##\Theta (\theta )=C \cos (m \theta ) +D \sin (m \theta)##.
Then the last ODE remaining to solve is ##\rho ^2 R''+\rho R'+R \{ \rho ^2 \left [ \frac{2mE}{\hbar ^2} - \left ( \frac{n\pi}{h} \right )^2 \right ] -m^2 \}=0##. This is where I'm stuck.
It's very similar to a Bessel equation and Cauchy-Euler equation but I don't think it is either. So I don't really know how to tackle that ODE. Any idea? Wolfram alpha does not seem to solve it either: http://www.wolframalpha.com/input/?i=x^2y%27%27%2Bxy%27%2By%28x^2*k-n^2%29%3D0.
 
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TSny said:
Look's like Bessel's equation. See http://www.efunda.com/math/bessel/bessel.cfm
Hmm ok.
Of course, you'll need to rescale ##\rho## to simplify the expression inside your { }.
Hmm what do you mean exactly? I have an equation of the form ##\rho ^2 R''+\rho R' +R(\rho ^2 p^2 -m^2)## where p is a constant for a given n.
Rescaling rho means to get ##p^2=1##?
 


Yes. Define a new independent variable (##x##, say) in terms of ##\rho## such that you get the standard form of Bessel's equation.
 


TSny said:
Yes. Define a new independent variable (##x##, say) in terms of ##\rho## such that you get the standard form of Bessel's equation.

I try ##x=\rho p## so ##\rho =x/p## but then the ODE changes to ##\frac{x^2R''}{p^2}+\frac{xR'}{p}+R(x^2-m^2)=0##. I could multiply by ##p^2## but I would not get the standard form of the Bessel equation. I don't see how I could rescale the factor in front of rho ^2 without rescaling the coefficients in front of R'' and R.
 


You need to take care of the rescaling in the derivatives, too. For example, ##dR/d\rho = \left(dR/dx\right)\left(dx/d\rho\right)##
 


TSny said:
You need to take care of the rescaling in the derivatives, too. For example, ##dR/d\rho = \left(dR/dx\right)\left(dx/d\rho\right)##

Oh right, I totally missed this!
So indeed now I recognize a Bessel equation!
Therefore I get that the solutions of the form ##\psi =R ( \rho ) \Theta (\theta ) Z(z)=B_n \sin \left ( \frac{n\pi z}{h} \right ) [C_m \cos (m\theta ) + D_m \sin (m \theta )]J_m \left ( \rho \sqrt {\frac{2mE}{\hbar ^2} - \frac{n^2 \pi ^2}{h^2}} \right )##.
So the solution that satisfies the boundary condition is a linear combination of those.
I'm not 100% sure about what they mean by "eigenvalues". Eigenfrequencies? Lowest energies possible? (They only want the first 3 eigenvalues).
I'm pretty sure this will concern the cases (1) n=1 and m=0 and m=1. (2) n=2, m=0. But I'm not sure what they are asking me.
 


I think they want the three lowest energies. They are called eigenvalues because they are eigenvalues of the time independent Schrodinger equation ##H|\psi> = E|\psi>##
 


You don't seem to have used the boundary condition at ρ=a.
 
  • #10


TSny said:
I think they want the three lowest energies. They are called eigenvalues because they are eigenvalues of the time independent Schrodinger equation ##H|\psi> = E|\psi>##

Ok thanks!
Hmm I don't know how to get that information.
I have a feeling I should add a subscript "n" under "E" in ##\psi =R ( \rho ) \Theta (\theta ) Z(z)=B_n \sin \left ( \frac{n\pi z}{h} \right ) [C_m \cos (m\theta ) + D_m \sin (m \theta )]J_m \left ( \rho \sqrt {\frac{2mE}{\hbar ^2} - \frac{n^2 \pi ^2}{h^2}} \right )## and then isolate ##E_n## but not sure to what I should equate the equation.
 
  • #11


Follow haruspex's lead.
 
  • #12


Oh right guys sorry. And thanks for helping. I did not see haruspex's post.
So if ##x_p## is the p'th zero of the Bessel function then ##E_n= \left ( \frac{\hbar ^2}{2m} \right ) \left [ \left ( \frac{x_p}{a} \right ) ^2 +\left ( \frac{n^2 \pi ^2}{h^2} \right ) \right ]##. I guess I'll have to check if I can replace "p" by "n". It's not obvious to me at a first glance.
 
  • #13


Ok I've thought a bit on this. The first 3 lowest energy values are when ##x_p=x_0##. So ##E_1= \frac{\hbar ^2}{2m} \left [ \left ( \frac{x_0}{a} \right ) ^2 + \frac{\pi ^2}{h^2} \right ]##, ##E_2= \frac{\hbar ^2}{2m} \left [ \left ( \frac{x_0}{a} \right ) ^2 + \frac{4\pi ^2}{h^2} \right ]## and ##E_3= \frac{\hbar ^2}{2m} \left [ \left ( \frac{x_0}{a} \right ) ^2 + \frac{9\pi ^2}{h^2} \right ]##.
I'm not very confident because I don't know if ##\frac{\hbar ^2 }{2m} \left [ \left ( \frac{x_1}{a} \right ) ^2 + \frac{\pi ^2}{h^2} \right ] <\frac{\hbar ^2}{2m} \left [ \left ( \frac{x_0}{a} \right ) ^2 + \frac{9\pi ^2}{h^2} \right ]## for example.
 
  • #14


You'll need to consult a Table of Roots

The problem states that the height of the cylinder is approx. equal to the radius: h\approx a, which should help figure out the lowest three energies.
 
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  • #15


TSny said:
You'll need to consult a Table of Roots

The problem states that the height of the cylinder is approx. equal to the radius: h\approx a, which should help figure out the lowest three energies.

Great and thank you once more.
I get from lower to upper: ##E_{1,0}##, ##E_{1,1}## and ##E_{2,0}## where the subscript are ##E_{n,p}##.
 
  • #16


I think that might be correct.
 
  • #17


:approve:
TSny said:
I think that might be correct.
Thanks for all.
 
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