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5.5

Spin precession

In a magnetic field a spin circles the field like a gyroscope, at a rate set by the field strength alone. A hospital MRI machine works by listening to that rate.

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After this section you should be able to

  • Write down the Hamiltonian of a spin in a magnetic field and solve the time evolution completely
  • Compute the Larmor frequency and explain why it is independent of the spin's initial direction
  • Explain resonance and Rabi oscillations qualitatively — how a rotating transverse field flips the spin
  • Walk through the basic NMR/MRI workflow — polarise, flip, listen

The previous section’s SG apparatus answers “which way does the spin point right now”. This section asks the next natural question: between two measurements, what is the spin doing?

This is not mere theoretical fussiness. Every hydrogen nucleus in your body is a spin 12\tfrac12, and a hospital’s magnetic resonance imaging (MRI) machine spends its whole day talking to them — the physics it relies on is precisely the answer to “how does spin evolve between measurements”.

The Hamiltonian: one term is all that survives

Place a particle with magnetic moment μ\vec\mu in a uniform field B=Bz^\vec B=B\hat z. Uniform means no force (last section’s force came from the gradient), so the particle does not move; the position ledger is perfectly quiet, and only the spin ledger evolves. The energy is just the classical orientation energy:

H^=μB=γBS^z(5.5.1)\hat H=-\vec\mu\cdot\vec B=-\gamma B\,\hat S_z\tag{5.5.1}

Here μ=γS^\vec\mu=\gamma\hat{\vec S}, and the proportionality constant γ\gamma is the gyromagnetic ratio — one fixed value per particle species. For the electron γe=geμB/|\gamma_e|=g_e\mu_B/\hbar (with ge2.002g_e\approx2.002); the proton’s is about 660 times smaller (larger mass, smaller moment).

This is arguably the simplest non-trivial Hamiltonian in quantum mechanics: a 2×22\times2 diagonal matrix. The eigenstates are just ,\ket{\uparrow},\ket{\downarrow}, with energies

E=γB2,E=+γB2(5.5.2)E_\uparrow=-\frac{\gamma\hbar B}{2},\qquad E_\downarrow=+\frac{\gamma\hbar B}{2}\tag{5.5.2}

(We narrate with γ\gamma positive; the electron’s γ\gamma is actually negative, which merely reverses the sense of rotation.) The gap between the two levels, ΔE=γB\Delta E=\gamma\hbar B, opens linearly with the field — this is the Zeeman splitting in its simplest two-level form. Converting that gap to a frequency, write

ωΔE=γB(5.5.3)\omega\equiv\frac{\Delta E}{\hbar}=\gamma B\tag{5.5.3}

This frequency is about to become the star of the show.

Solving the evolution: the spin circles the field

Resonance: how to flip a spin

Watching a spin go round in circles is not much use by itself; we also want to control it — say, flip an up spin to down. The level gap is ω\hbar\omega, so intuition says: apply a perturbation at exactly the frequency ω\omega.

Concretely: on top of the large static field B0z^B_0\hat z, add a small field B1B_1 rotating in the xy plane (B1B0B_1\ll B_0) at frequency ωrf\omega_{\text{rf}}. The qualitative results (the full solution uses the rotating-frame trick of section 3.9; here we make the physics clear):

  • Off resonance (ωrf\omega_{\text{rf}} away from ω0=γB0\omega_0=\gamma B_0): the small field rotates “out of step” with the spin; its push helps one moment and hinders the next, averaging to almost nothing.
  • On resonance (ωrf=ω0\omega_{\text{rf}}=\omega_0): view things from a frame rotating along with the spin. The effect of the big field B0B_0 is exactly cancelled by the rotation, leaving only a stationary small field B1B_1 — so the spin turns slowly about B1B_1 at the gentle rate ω1=γB1\omega_1=\gamma B_1, arcing from the north pole down to the south and back. The probability swings back and forth between \ket{\uparrow} and \ket{\downarrow}:
P(t)=sin2ω1t2(on resonance)(5.5.9)P_{\downarrow}(t)=\sin^2\frac{\omega_1 t}{2}\quad(\text{on resonance})\tag{5.5.9}

This swing is the Rabi oscillation. Time the shutdown of the small field precisely and you can park the spin anywhere you like: run for t=π/ω1t=\pi/\omega_1 (a ”π\pi pulse”) and the flip is complete; run half as long (a ”π/2\pi/2 pulse”) and the spin lies flat on the equator — the key move NMR uses below.

NMR and MRI: turning this section into a machine

The workflow of nuclear magnetic resonance (NMR), in the language of this section, takes three sentences:

  1. Polarise. Put the sample in a strong field B0B_0. In thermal equilibrium slightly more spins point up than down (the lower-energy state is a touch more populated — only about ten parts per million at room temperature and 3 T, but with 102310^{23} nuclei in the sample the net magnetisation is plenty), giving the sample a net magnetic moment along z.
  2. Flip. Fire a radio-frequency π/2\pi/2 pulse tuned to ω0=γB0\omega_0=\gamma B_0, laying the net moment flat into the xy plane.
  3. Listen. The flattened moment precesses at the Larmor frequency like a spinning bar magnet, inducing an oscillating voltage at ω0\omega_0 in a pickup coil. Measure that signal’s frequency and decay.

Why is it worth listening to? Because the BB in ω0=γB\omega_0=\gamma B is the actual field at the nucleus, slightly shielded by the surrounding electron cloud — the same nucleus in different chemical environments shifts in frequency by a few parts per million (the “chemical shift”). From one spectrum a chemist reads off molecular structure; that is NMR spectroscopy.

MRI runs the trick in reverse: deliberately make B0B_0 a gradient field that varies with position, so that frequency becomes a barcode for location — receive a signal at 127.68 MHz and you know it came from the slice of tissue where the field matches that frequency. Add the fact that signals decay at different rates in different tissues (water and fat have different relaxation times), and a three-dimensional image of soft tissue can be reconstructed. The hammering noise you hear inside an MRI machine is the gradient coils rapidly switching that “barcode”.

What comes next

Up to now we have been playing with a single spin. But in real systems angular momenta rarely come alone: the electron in hydrogen has both orbital angular momentum L^\hat{\vec L} and spin S^\hat{\vec S}; helium has the spins of two electrons; protons and neutrons assemble into nuclei.

Put two angular momenta side by side — what is the total? The classical answer, “add the vectors”, runs into immediate trouble in quantum mechanics: not even one vector’s three components can be simultaneously sharp, so what exactly would you add? The next section gives the correct addition, and its answer will also explain “singlet” and “triplet” — words that will keep returning in chemical bonds and entangled states.

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