3.1: Time-Independent Degenerate Perturbation Theory
( \newcommand{\kernel}{\mathrm{null}\,}\)
We have seen how we can find approximate solutions for a system whose Hamiltonian is of the form
ˆH=ˆH0+ˆV
When we assumed that ˆH and ˆH0 possess discrete, non-degenerate eigenvalues only. This led to a mixing of states where
|ϕ0⟩=|n0⟩+∑k≠0Vk0(E0−Ek)|nk⟩
Clearly, if E0=Ek this diverges. As do the higher order energy shifts (see 2.4). Thus for the degenerate case we cannot associate a particular perturbed state |ϕ0⟩ with a particular unperturbed state |n0⟩: we need to take a different approach. In fact, the approximation we make is completely different: we assume that the small perturbation only mixes those states which are degenerate. We then solve the problem exactly for that subset of states.
Assume that ˆH0 possesses N degenerate eigenstates |m⟩ with eigenvalue Edeg. It may also possesses non-degenerate eigenstates, which can be treated separately by non-degenerate perturbation theory. We write a perturbed eigenstate |ϕj⟩ as an linear expansion in the unperturbed degenerate eigenstates only:
|ϕj⟩=∑i|mi⟩⟨mi|ϕj⟩=∑icji|mi⟩
Where i here runs over degenerate states only. The TISE now becomes:
[ˆH0+ˆV]|ϕj⟩=[ˆH0+ˆV]∑icji|mi⟩=Ej∑icji|mi⟩
but we know that for all degenerate eigenstates ˆH0|mi⟩=Edeg|mi⟩. So we obtain:
∑icjiˆV|mi⟩=(Ej−Edeg)∑icji|mi⟩
premultiplying by some unperturbed state ⟨mk| gives
∑icji[⟨mk|ˆV|mi⟩−δik(Ej−Edeg)]=0
We can get a similar equation from each unperturbed state |mk⟩. We thus have an eigenvalue problem: the eigenvector has elements cji and the eigenvalues are ΔEj=Ej−Edeg. Writing the matrix elements between the ith and kth unperturbed degenerate states as Vik≡⟨mi|ˆV|mk⟩ we recover the determinantal equation:
|V11−ΔEjV12...V1NV21V22−ΔEj...V2N............VN1VN2...VNN−ΔEj|=0
The N eigenvalues obtained by solving this equation give the shifts in energy due to the perturbation, and the eigenvectors give the perturbed states |ϕ⟩ in the unperturbed, degenerate basis set |m⟩.