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Non-Degenerate Perturbation Theory
Let us now generalize our perturbation analysis to deal
with systems possessing more than two energy eigenstates.
Consider a system in which the energy
eigenstates of the unperturbed Hamiltonian, , are denoted
|
(894) |
where runs from 1 to . The eigenstates are assumed to
be orthonormal, so that
|
(895) |
and to form a complete set. Let us now try to
solve the energy eigenvalue problem for the perturbed Hamiltonian:
|
(896) |
If follows that
|
(897) |
where can take any value from 1 to . Now, we can express
as a linear superposition of the unperturbed energy eigenstates:
|
(898) |
where runs from 1 to . We can combine the above
equations to give
|
(899) |
where
|
(900) |
Let us now develop our perturbation expansion. We assume that
|
(901) |
for all , where is our expansion parameter.
We also assume that
|
(902) |
for all . Let us search for a modified version of the th unperturbed
energy eigenstate for which
|
(903) |
and
for . Suppose that we write out Eq. (899) for ,
neglecting terms which are
according to our expansion
scheme. We find that
|
(906) |
giving
|
(907) |
Substituting the above expression into Eq. (899),
evaluated for , and neglecting
terms, we obtain
|
(908) |
Thus, the modified th energy eigenstate possesses an eigenvalue
|
(909) |
and a wavefunction
|
(910) |
Incidentally, it is easily demonstrated that the modified eigenstates remain orthonormal
to
.
Next: Quadratic Stark Effect
Up: Time-Independent Perturbation Theory
Previous: Two-State System
Richard Fitzpatrick
2010-07-20