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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|i\rangle, how much amplitude has leaked into a different state f|f\rangle after the perturbation has acted?

The Dyson series, truncated

In the interaction picture the state obeys

itΨI(t)=H^I(t)ΨI(t).i\hbar\,\frac{\partial}{\partial t}\,|\Psi_I(t)\rangle = \hat H'_I(t)\,|\Psi_I(t)\rangle .

Integrating both sides from 00 to tt turns this into an integral equation:

ΨI(t)=ΨI(0)i0tH^I(t)ΨI(t)dt.|\Psi_I(t)\rangle = |\Psi_I(0)\rangle - \frac{i}{\hbar}\int_0^t \hat H'_I(t')\,|\Psi_I(t')\rangle\,dt' .

This is exact but implicit — ΨI|\Psi_I\rangle 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|\Psi_I(0)\rangle = |i\rangle:

ΨI(t)ii0tH^I(t)idt.|\Psi_I(t)\rangle \approx |i\rangle - \frac{i}{\hbar}\int_0^t \hat H'_I(t')\,|i\rangle\,dt' .

Projecting onto the final state

The amplitude to be found in a different state f|f\rangle (with fif \neq i) is its coefficient cf(t)=fΨI(t)c_f(t) = \langle f|\Psi_I(t)\rangle. Projecting the expansion above and using fi=0\langle f|i\rangle = 0:

cf(1)(t)=i0tfH^I(t)idt=i0tfH^(t)ieiωfitdt\boxed{\,c_f^{(1)}(t) = -\frac{i}{\hbar}\int_0^t \langle f|\hat H'_I(t')|i\rangle\,dt' = -\frac{i}{\hbar}\int_0^t \langle f|\hat H'(t')|i\rangle\, e^{\,i\omega_{fi}t'}\,dt'\, }

where in the last step we used H^I(t)=eiH^0t/H^(t)eiH^0t/\hat H'_I(t') = e^{i\hat H_0 t'/\hbar}\hat H'(t')e^{-i\hat H_0 t'/\hbar} acting on the eigenstates, which produces the phase ei(EfEi)t/=eiωfite^{i(E_f - E_i)t'/\hbar} = e^{i\omega_{fi}t'}. The object fH^(t)iHfi(t)\langle f|\hat H'(t')|i\rangle \equiv H'_{fi}(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=0t=0 and held constant, H^(t)=V^\hat H'(t) = \hat V for t>0t>0, so the matrix element Vfi=fV^iV_{fi} = \langle f|\hat V|i\rangle is time-independent. The integral is elementary:

cf(1)(t)=iVfi0teiωfitdt=iVfieiωfit1iωfi=Vfieiωfit1ωfi.c_f^{(1)}(t) = -\frac{i}{\hbar}\,V_{fi}\int_0^t e^{\,i\omega_{fi}t'}\,dt' = -\frac{i}{\hbar}\,V_{fi}\,\frac{e^{\,i\omega_{fi}t}-1}{i\omega_{fi}} = -\frac{V_{fi}}{\hbar}\,\frac{e^{\,i\omega_{fi}t}-1}{\omega_{fi}} .

Taking the magnitude and using eiθ1=2sin(θ/2)|e^{i\theta}-1| = 2|\sin(\theta/2)|:

cf(1)(t)=Vfi2sin(ωfit/2)ωfi.\big|c_f^{(1)}(t)\big| = \frac{|V_{fi}|}{\hbar}\,\frac{2\,\big|\sin(\omega_{fi}t/2)\big|}{|\omega_{fi}|} .

Why the phase matters

The integrand carries the oscillating phase eiωfite^{i\omega_{fi}t'}. 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=0.5V_{fi}=0.5, ωfi=2.0\omega_{fi}=2.0, t=1.0t=1.0, in units =1\hbar=1. Use cf(1)=(Vfi/)2sin(ωfit/2)/ωfi|c_f^{(1)}| = (|V_{fi}|/\hbar)\,2|\sin(\omega_{fi}t/2)|/|\omega_{fi}| and return the number.

Run your code to see the quantum state.

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