At t < 0 a particle with mass m is located in a one-dimensional potential described by
U(x) = ∞, x < 0, x > L,
U(x) = 0, 0 ≤ x ≤
L.
A potential of ΔV(x) = αx is added to 0 ≤
x ≤ L from t = 0 with α
<< 1.
(a) What are the energy eigenvalues and eigenstates for the system at t
< 0?
(b) Calculate the first order correction to the lowest two energy eigenvalues
at t --> ∞ by treating ΔV(x) as a perturbation.
Solution:
In the WKB approximation, find the allowed
energies that a ball of mass m, bouncing due to gravity on a perfectly
reflecting surface, can have.
You can use the fact that for this problem
the WKB approximation gives
∮p dq = (n - ¼)h,
( n = 1, 2, ...), where p(q) is the momentum of the ball at the height q and the integral is over
a full periodic path.
Solution:
H = ε
| 2 | 0 | 0.1 | ||
| 0 | 3 | 0 | ||
| 0.1 | 0 | 2 |
.
Estimate the eigenvalues of this Hamiltonian using perturbation theory. Do you have to use degenerate or non-degenerate perturbation theory?
Solution:
H0 = ε
| 2 | 0 | 0 | ||
| 0 | 3 | 0 | ||
| 0 | 0 | 2 |
.
Let
| 1 | ||
| 0 | ||
| 0 |
,  
| 0 | ||
| 1 | ||
| 0 |
,  
| 0 | ||
| 0 | ||
| 1 |
denote the eigenbasis of H0.
| 0 | ||
| 1 | ||
| 0 |
is an eigenvector of H with eigenvalue 3ε.
To find the other eigenvalues of H using first order perturbation theory we
diagonalize the matrix
| 0 | 0.1 | ||
| 0.1 | 0 |
.
The energy eigenvalues are 2.1 ε with eigenvector 2-½
| 1 | ||
| 0 | ||
| 1 |
,  
and 1.9 ε with eigenvector 2-½
| 1 | ||
| 0 | ||
| -1 |
.