intermediate · Physics · Time-Dependent Perturbation & Fermi's Golden Rule
Transition Amplitudes
We now derive the single most important formula of the module: the first-order
transition amplitude. It answers the question — if the system starts in ∣i⟩,
how much amplitude has leaked into a different state ∣f⟩ after the perturbation
has acted?
The Dyson series, truncated
In the interaction picture the state obeys
iℏ∂t∂∣ΨI(t)⟩=H^I′(t)∣ΨI(t)⟩.
Integrating both sides from 0 to t turns this into an integral equation:
∣ΨI(t)⟩=∣ΨI(0)⟩−ℏi∫0tH^I′(t′)∣ΨI(t′)⟩dt′.
This is exact but implicit — ∣ΨI⟩ appears on both sides. The perturbative idea
is to iterate it, generating the Dyson series. To first order we approximate the
state inside the integral by its initial value ∣ΨI(0)⟩=∣i⟩:
∣ΨI(t)⟩≈∣i⟩−ℏi∫0tH^I′(t′)∣i⟩dt′.
Projecting onto the final state
The amplitude to be found in a different state ∣f⟩ (with f=i) is its
coefficient cf(t)=⟨f∣ΨI(t)⟩. Projecting the expansion above and using
⟨f∣i⟩=0:
where in the last step we used H^I′(t′)=eiH^0t′/ℏH^′(t′)e−iH^0t′/ℏ
acting on the eigenstates, which produces the phase ei(Ef−Ei)t′/ℏ=eiωfit′.
The object ⟨f∣H^′(t′)∣i⟩≡Hfi′(t′) is the matrix element of the
perturbation between the two states.
Worked example: a constant perturbation
Suppose the perturbation is simply switched on at t=0 and held constant,
H^′(t)=V^ for t>0, so the matrix element Vfi=⟨f∣V^∣i⟩
is time-independent. The integral is elementary:
Taking the magnitude and using ∣eiθ−1∣=2∣sin(θ/2)∣:
cf(1)(t)=ℏ∣Vfi∣∣ωfi∣2sin(ωfit/2).
Why the phase matters
The integrand carries the oscillating phase eiωfit′. For a constant
perturbation this phase oscillates and the integral does not grow without bound — the
amplitude just wiggles. The way to make the integral build up is to give the
perturbation its own oscillation that cancels this phase. That is precisely the harmonic
drive and resonance we study next.
Try it
Compute the magnitude of the first-order amplitude for a constant perturbation with
Vfi=0.5, ωfi=2.0, t=1.0, in units ℏ=1. Use
∣cf(1)∣=(∣Vfi∣/ℏ)2∣sin(ωfit/2)∣/∣ωfi∣ and return the number.
Run your code to see the quantum state.
Sign in on the full site to ask questions and join the discussion.