intermediate · Physics · Time-Independent Perturbation Theory
Second-Order Energy Corrections
Going to second order
The first-order energy used only the unperturbed states. The second-order correction is the first place
the state correction feeds back into the energy. Return to the order-by-order expansion and collect
the λ2 terms of the eigenvalue equation:
Project onto ⟨n(0)∣. As before the H^(0) term cancels, and with the normalization
choice ⟨n(0)∣n(1)⟩=0 the En(1) term drops too. What survives is
En(2)=⟨n(0)∣H^′∣n(1)⟩.
Now substitute the explicit first-order state from the previous lesson,
∣n(1)⟩=∑m=nEn(0)−Em(0)⟨m(0)∣H^′∣n(0)⟩∣m(0)⟩.
Using ⟨n(0)∣H^′∣m(0)⟩=⟨m(0)∣H^′∣n(0)⟩∗ (Hermiticity),
the numerator becomes a squared modulus:
En(2)=m=n∑En(0)−Em(0)⟨m(0)∣H^′∣n(0)⟩2.
What the formula tells you
Two features are worth memorizing:
The numerator is always non-negative because it is ∣⋅∣2. The sign of each term is
therefore set entirely by the energy denominator.
The ground state always shifts down. For the lowest level, every other state has higher energy,
so E0(0)−Em(0)<0 for all m, making every term negative. Second-order perturbation
theory lowers the ground-state energy — a manifestation of level repulsion: nearby states "push
apart," and the lower one is pushed further down.
The single-term case
For a two-level system there is only one other state, so the sum collapses to one term. With
H^(0)=diag(E0(0),E1(0)) and real coupling
V=⟨1(0)∣H^′∣0(0)⟩, the ground state's second-order shift is
E0(2)=E0(0)−E1(0)∣V∣2.
If E0(0)=1, E1(0)=4, and V=0.6, then
E0(2)=0.36/(1−4)=−0.12 — negative, as expected for a ground state.
Try it
Compute the second-order ground-state shift E0(2) for E0(0)=1, E1(0)=4, and real
coupling V=0.6, and return it as a number.
Run your code to see the quantum state.
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