intermediate · Physics · Time Evolution & the Schrödinger Picture
Expectation Value Dynamics
We have followed states and probabilities through time. Often the most physical question is how an
observable's average moves — the position of a wavepacket, the magnetisation of a spin. This
lesson tracks ⟨A^⟩(t) directly.
Two routes to the same curve
There are two equivalent ways to compute ⟨A^⟩(t):
Evolve the state, then sandwich:
⟨A^⟩(t)=⟨ψ(t)∣A^∣ψ(t)⟩ with
∣ψ(t)⟩=U(t)∣ψ(0)⟩.
Evolve the operator (Heisenberg form):
⟨A^⟩(t)=⟨ψ(0)∣U†A^U∣ψ(0)⟩=⟨ψ(0)∣A^H(t)∣ψ(0)⟩.
For our worked example the operator route is cleanest because Pauli operators rotate into each other.
A precessing spin
Take H^=2ℏωσz and watch the observable σx. A standard
identity for conjugating a Pauli by a Z-rotation gives the Heisenberg-evolved operator
σx(t)=U†σxU=cos(ωt)σx−sin(ωt)σy,
and similarly σy(t)=cos(ωt)σy+sin(ωt)σx, while
σz(t)=σz. Now choose the initial state ∣+⟩, the +1 eigenstate of
σx, for which ⟨σx⟩0=1, ⟨σy⟩0=0,
⟨σz⟩0=0. Taking expectation values:
⟨σx⟩(t)=cos(ωt),⟨σy⟩(t)=sin(ωt),⟨σz⟩(t)=0.
The Bloch picture
These three averages are the components of the Bloch vectorr(t)=(⟨σx⟩,⟨σy⟩,⟨σz⟩). Here
r(t)=(cosωt,sinωt,0),
a unit vector sweeping counterclockwise around the z-axis in the equatorial plane at angular frequency
ω. The expectation values are not abstract — they are literally the coordinates of the spin's
arrow on the Bloch sphere, precessing like a gyroscope.
Consistency with Ehrenfest
You can also get ⟨σx⟩(t)=cosωt from Ehrenfest's theorem:
dtd⟨σx⟩=ℏi⟨[H^,σx]⟩. Since
[σz,σx]=2iσy, this gives ⟨σx⟩˙=−ω⟨σy⟩,
and likewise ⟨σy⟩˙=ω⟨σx⟩. Solving this coupled pair
with the given initial conditions reproduces ⟨σx⟩(t)=cosωt and
⟨σy⟩(t)=+sinωt — consistent with the operator route above — and the next
lesson formalises this Ehrenfest route.
Try it
This is a numerical exercise — your code should return a number. Compute
⟨σx⟩(t)=cos(ωt) at ωt=π/3.
Run your code to see the quantum state.
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