How Do You Determine the Ground State Energy in a Spherical Infinite Well?

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SUMMARY

The discussion focuses on determining the ground state energy and wave function of a particle constrained between two concentric hard spheres with radii ##r = a## and ##r = b##. The relevant equation is derived from the radial component of the time-independent Schrödinger equation, leading to the effective differential equation $$\frac{d^2 u}{dr^2} = -\frac{2mE}{\hbar^2}u$$. The solution involves boundary conditions where the wave function must vanish at the sphere boundaries, specifically ##R(a) = 0## and ##R(b) = 0##. The challenge lies in quantizing the wave number ##k## from these boundary conditions, which is essential for finding the ground state energy.

PREREQUISITES
  • Understanding of quantum mechanics, specifically the time-independent Schrödinger equation.
  • Familiarity with boundary conditions in quantum systems.
  • Knowledge of spherical coordinates and radial wave functions.
  • Basic concepts of infinite potential wells in quantum mechanics.
NEXT STEPS
  • Study the quantization conditions for infinite square wells in quantum mechanics.
  • Learn about the application of boundary conditions in solving differential equations in quantum systems.
  • Explore the concept of angular momentum in quantum mechanics, particularly the role of the quantum number ##\ell##.
  • Investigate the graphical representation of wave functions in spherical potentials.
USEFUL FOR

Students and professionals in quantum mechanics, particularly those studying or working with spherical potentials and wave functions in confined systems.

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Homework Statement


A particle of mass ##m## is constrained to move between two concentric hard spheres of radii ##r = a## and ##r = b##. There is no potential between the spheres. Find the ground state energy and wave function.

Homework Equations


$$\frac{-\hbar^2}{2m} \frac{d^2 u}{dr^2} + [V(r) + \frac{-\hbar^2}{2m} \frac{\ell (\ell + 1)}{r^2}]u = Eu$$

The Attempt at a Solution


The relevant equation here is the radial equation component of the time independent schroedinger equation for a central potential, where ##u(r) \equiv rR(r)##. Effectively, this is an infinite square well potential such that inside the concentric spheres the potential is ##0## and in the ground state ##\ell = 0## so our effective differential equation becomes
$$\frac{d^2 u}{dr^2} = -\frac{2mE}{\hbar^2}u \equiv -k^2 u$$
with the solution
$$u(r) = rR(r) = A sin(kr) + B cos(kr)$$
We can apply the boundary conditions that ##R(a) = 0## and ##R(b) = 0##. However, my problem comes from the fact that I don't know how to get anything out of these boundary conditions. Most of the time, the problem is that ##a = 0## and that boundary condition gives the quantization of ##k##, but here I don't see how to pull out that quantization. Is there some part of this problem that I'm missing?
 
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however, my problem comes from the fact that I don't know how to get anything out of these boundary conditions.
If you just look at it you can see the shape the solutions have to have. Sketch the first few on your diagram.
 

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