The Finite Square Well

The next most complicated potential is where we drop the walls of the infinite square well down to V0>0. In this case, we will observe bound states (E<V0) and unbound states (E>V0). For now, we focus on bound states, which lead to quantized energy eigenstates. The potential we are given is:

V(x)={V0if x<a0if a<x<aV0if x>a

We can show that the general solutions for energy eigenstates are:

ϕE(x)={Aeqx+Beqxif x<aCsinkx+Dcoskxif a<x<aFeqx+Geqxif x>a

where k=2mE2>0 and q=2m(V0E)2>0.

  1. Question: There are 3 “boundary” conditions on ϕE(x). What are they?
    • Discussion: What is the physical or practical origin of each of these boundary conditions? Why are there not additional conditions on the derivatives of ϕE(x)?
  2. Question: We can apply these boundary conditions (as in McIntyre or my notes), and show that the energy equations we must satisfy are: katan(ka)=qa and kacot(ka)=qa. How do we know these equations are transcendental? That is, how do we recognize that we won’t be able to find an analytical solution?
    • Discussion: What are some ways we can find approximate solutions to these equations? What are the benefits and tradeoffs to each method you come up with?
  3. Question: Using McIntyre’s definitions for z=2MEa22 and z0=2MV0a22, derive the transcendental relationships: ztan(z)=z02z2 and zcot(z)=z02z2.
    • Discussion: For a strongly bound particle, what would your expect for the values of z0 and z? What about for a weakly bound particle?