Skip to main content
Sandbox Physics

IN34 · Read the spin rhythm

Optically Pumped Magnetometer

How can light read atomic precession without mistaking brightness drift for a magnetic field? A magnetic field sets the atomic precession frequency. A weak probe turns that motion into a changing polarization; two optical channels and an independent brightness monitor separate common probe drift. Pump drift changes the spins themselves and needs a separate check.

Drive polarized cesium spins with an RF field and sweep through resonance. Compare two counted optical channels, probe drift and the separate static weak-field response.

Interactive modelOptically Pumped Magnetometer

Signed response from simulated photon gates

Cosine channel XXNegative-sine channel YY

f/Hzf/\mathrm{Hz} · φ/mrad\varphi/\mathrm{mrad}

Retained detector counts at the strongest response

Collector ACollector B

t/mst/\mathrm{ms} · photons per gate

Standards, blanks and inference conditions

CSV retains every time gate, two detectors, probe and pump monitors, signed references, frequency or coil readback, dark observations and three known analyzer angles. The fit reads these observations only. Mx fits a common centre and absorptive width with nuisance amplitudes and phases. Static inference assumes independently known pumping and relaxation and stays inside the monotonic branch.

First eight raw gates of the selected record
Gatet0/st_0/\mathrm{s}ABProbe monitorPump monitor
Separate synthetic ideal reference

The ideal reference is generating context stored separately in JSON. It is excluded from the raw CSV and from every inference.

Physics tutorial

Read a spin rhythm with light

BackgroundCircular pump light orients cesium spins. A transverse RF field drives their precession, and a weak probe reads the resulting optical rotation.

Why it mattersThe detectors count photons. A field interpretation needs to distinguish atomic motion from changes in the light source.

Start with the essentials

Focus question
How can light read atomic precession without mistaking brightness drift for a magnetic field?
One-sentence intuition
A normalized detector pair cancels common probe brightness; pumping changes spin orientation and relaxation and needs its own monitor.

Core mathematical model

Spin orientation dynamics

P˙=P×γFB−Γ0P+R(kp−P)\dot{\mathbf P}=\mathbf P\times\gamma_F\mathbf B-\Gamma_0\mathbf P+R(\mathbf k_p-\mathbf P)

Torque sets precession, relaxation removes orientation, and the pump replenishes it along the optical axis. Pumping also increases the total relaxation rate. Rates and optical gain are declared teaching assumptions.

A cesium frequency scale at low field

fL=γF2π∣B∣,γF2π=3.4986 Hz/nTf_L=\frac{\gamma_F}{2\pi}|\mathbf B|,\qquad\frac{\gamma_F}{2\pi}=3.4986\,\mathrm{Hz/nT}

One ground-state hyperfine manifold is selected. A resolved resonance centre becomes a field magnitude through the known gyromagnetic ratio.

Signed quadratures follow IN13

X=2⟨φcos⁡ψ⟩,Y=−2⟨φsin⁡ψ⟩X=\sqrt2\langle\varphi\cos\psi\rangle,\qquad Y=-\sqrt2\langle\varphi\sin\psi\rangle

Dark observations and independent rotation standards convert the detector counts to rotation. The saved cosine and negative-sine references then give RMS-scaled signed channels. A cosine signal leading the reference gives positive quadrature.

A separate static low-field branch

Px=−RγFBy(Γ0+R)2+(γFBy)2P_x=-\frac{R\gamma_F B_y}{(\Gamma_0+R)^2+(\gamma_F B_y)^2}

RF is off, the pump points along the positive longitudinal axis and the field is transverse. Rotation is approximately linear near zero and eventually turns over. Inference uses only the declared monotonic interval.

Common difficulties

What normalization removes

Typical misconceptionNormalization removes every laser-power change.

Better mental modelCommon probe brightness multiplies both outputs and can cancel. Pump power changes the spins and linewidth, so it needs a separate check.

Zero field and rotating waves

Typical misconceptionSetting the resonance frequency to zero makes a zero-field magnetometer.

Better mental modelThe rotating-wave approximation needs sufficiently fast precession. The static branch solves the RF-off equation directly; collision physics for SERF is absent.

Run the experiment

  1. 01

    Drag the field dial

    Hold the gold bias dial and drag horizontally.

    What to observe: The resonance centre moves with the field; the spin arrow and newly acquired counts update during the drag.
  2. 02

    Compare two drifts

    Choose Probe brightness drifts, then Pump power drifts.

    What to observe: Normalization preserves the resonance under common probe drift. The independent pump monitor detects pump drift and withholds a stationary inference.
  3. 03

    Find a directional dead zone

    Choose Look along the field, then return to Driven precession.

    What to observe: A probe along the static field cannot see transverse precession. Photon counts remain available, but the magnetic conclusion is withheld.
  4. 04

    Try the static branch

    Choose Static weak field and slowly change the bias field.

    What to observe: With RF off, rotation changes across the calibrated coil sweep. Leaving the monotonic branch withholds a unique field.
  5. 05

    Keep and replay

    Keep a sweep, change pumping, select the earlier record and export CSV.

    What to observe: Its time gates, standards and counts stay fixed. The CSV contains no generating field and can still reproduce the inference.

Related experiments and articles

Continue exploring

From spin preparation to magnetic readout

How does prepared atomic orientation become an optical magnetic-field measurement?

  1. LabOptical Pumping and RelaxationPrepare atomic populations and compare pumping with relaxation.
  2. LabHanle Lifetime SpectrometerRead how an optical Hanle line depends on the excited-state lifetime; keep that lifetime distinct from ground-state relaxation.
  3. LabLock-In AmplifierCompare signed cosine and negative-sine channels with a retained reference.
  4. You are hereOptically Pumped MagnetometerInfer a resonance from counted probe light and compare probe drift with pump drift.

How physics instruments measure · Reading path

How physics instruments measure

Articles on this path that use this experiment, followed by the other experiments they suggest.

  1. ArticleReading a magnetic field in the rhythm of atoms
FeedbackSomething broken, confusing, or missing on this page?Tell us
What kind of feedback?

Sent with this page’s address, its Lab ID, the site language and your device type. Please leave out personal details. Feedback is kept for up to 12 months.Privacy policy