intermediate · Physics · Spin-½ Systems & Pauli Algebra
Spin in a Magnetic Field
A spinning charge carries a magnetic moment, so a spin-½ particle in an external magnetic field has
its energy split according to its spin orientation. This is the Zeeman effect, and its dynamics —
Larmor precession — are the foundation of nuclear magnetic resonance, MRI, and qubit control.
The magnetic moment and the Hamiltonian
The magnetic moment of a spin-½ is proportional to its spin,
μ=γS,
where γ is the gyromagnetic ratio. The energy of a moment in a field B is
−μ⋅B, so the Hamiltonian is
H=−μ⋅B=−γS⋅B.
Choosing the field along z, B=Bz^,
H=−γBSz=−2γBℏσz.
Energy eigenstates and the splitting
Since H is proportional to σz, its eigenstates are ∣0⟩ and ∣1⟩ with energies
E↑=−2γBℏ,E↓=+2γBℏ.
(For γ>0 the spin-up state is the lower-energy ground state — the moment prefers to align with
the field.) The gap between them is
ΔE=E↓−E↑=γBℏ=ℏωL,ωL≡γB,
defining the Larmor angular frequencyωL.
Larmor precession
A spin not aligned with the field is a superposition of the two energy eigenstates. Under time evolution
e−iHt/ℏ the relative phase between them winds at rate ωL, which makes the Bloch vector
precess about the field axis at the Larmor frequency:
⟨Sx⟩(t)=⟨Sx⟩(0)cosωLt+⟨Sy⟩(0)sinωLt,
with ⟨Sz⟩ constant. The transverse spin rotates exactly like a classical gyroscope in a
field — one of the cleanest correspondences between quantum and classical mechanics.
Try it
For γ=5 and B=0.4 (with ℏ=1), compute the Larmor angular frequency
ωL=γB. It should equal 2, which is also the energy splitting ΔE=ℏωL.
Run your code to see the quantum state.
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