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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