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L06 · Gain and feedback

Laser Noise Startup Workbench

Where does the first photon in a laser cavity come from? In an unseeded cavity, spontaneous emission can put the first photon into the selected mode. If gain exceeds all cavity losses, stimulated emission amplifies that seed; depletion then limits its growth. An injected photon can provide a seed too.

Watch a recorded laser startup from random mode seeding. Move the output mirror, compare gain with loss, and seed an exact dark state with one photon.

Interactive modelLaser Noise Startup Workbench
Integrated record duration—\text{—}
Elapsed round trips—\text{—}
Recorded end upper fraction—\text{—}
Loss-compensating upper fraction—\text{—}
Recorded end mean mode photons—\text{—}
Recorded end output power—\text{—}
Current stimulated gain rate—\text{—}
Total cavity loss rate—\text{—}
Round-trip net logarithmic gain—\text{—}
Ideal zero-noise pump threshold—\text{—}
Cumulative spontaneous mode events—\text{—}

Physics tutorial

Let a mode grow from one random event

BackgroundThe pump stores energy in the upper laser level while the cavity keeps losing photons. A spontaneously emitted photon can land in the cavity mode; once gain beats loss, stimulated emission makes that mode grow.

Why it mattersBecause the cavity starts with almost no light, you can see how long the laser takes to turn on. Once the field grows, it drains the same stored excitation that supplied its gain.

Start with the essentials

Focus question
If spontaneous emission into the mode is switched off, can a medium pumped above threshold stay exactly dark?
One-sentence intuition
Gain above loss lets a seed grow; if the model omits seeding, an exactly zero photon population stays zero.

Core mathematical model

Rate equations for stored excitation and cavity photons

n˙=R(1−n)−nτu−GnScNaS˙c=(Gn−κ)Sc+βNanτu\begin{aligned}\dot n&=R(1-n)\\&\quad-\frac{n}{\tau_u}-\frac{GnS_c}{N_a}\\\dot S_c&=(Gn-\kappa)S_c\\&\quad+\frac{\beta N_a n}{\tau_u}\end{aligned}

The first equation evolves the upper-state fraction; the second evolves the cavity photon population. There are one billion active emitters. Spontaneous mode seeds arrive as accepted Poisson events: each removes one excited emitter and adds one photon. Stimulated growth and losses are continuous averages.

Geometry, spectral overlap and loss

G=2σ0NaATR×11+(Δν/γ)2κ=−ln⁡RbTR−ln⁡(1−T)TR−ln⁡(1−ℓ)TR\begin{aligned}G&=\frac{2\sigma_0N_a}{AT_R}\\&\quad\times\frac{1}{1+(\Delta\nu/\gamma)^2}\\\kappa&=-\frac{\ln R_b}{T_R}\\&\quad-\frac{\ln(1-T)}{T_R}\\&\quad-\frac{\ln(1-\ell)}{T_R}\end{aligned}

In a linear cavity, light crosses the gain medium twice per round trip. The number of active emitters is fixed at one billion, so changing the mode area changes their density and their overlap with the photons. The round-trip time uses a vacuum-equivalent optical length.

Ideal zero-noise threshold

nth=κ/Gn0=Rτu1+RτuRth=nthτu(1−nth)\begin{aligned}n_{\mathrm{th}}&=\kappa/G\\n_0&=\frac{R\tau_u}{1+R\tau_u}\\R_{\mathrm{th}}&=\frac{n_{\mathrm{th}}}{\tau_u(1-n_{\mathrm{th}})}\end{aligned}

If the required upper-level fraction is one or more, no finite pump rate reaches threshold. This is a zero-source steady-state reference. Finite seeding leaves a weak background below it; a single trajectory still contains discrete one-photon spontaneous jumps.

Gain clamping and envelope output

nss≃nthκSc,ssNa≃R(1−nth)−nthτuPout=hνκoutSc\begin{aligned}n_{\mathrm{ss}}&\simeq n_{\mathrm{th}}\\\frac{\kappa S_{c,\mathrm{ss}}}{N_a}&\simeq R(1-n_{\mathrm{th}})\\&\quad-\frac{n_{\mathrm{th}}}{\tau_u}\\P_{\mathrm{out}}&=h\nu\kappa_{\mathrm{out}}S_c\end{aligned}

The first two relations ignore the small spontaneous source above threshold. The output loss rate is the logarithmic attenuation at the output mirror divided by the round-trip time, and the displayed power is an average taken from the envelope.

Common difficulties

Only the seeding is random

Typical misconceptionThe photon-number trace is an exact quantum simulation that counts every photon.

Better mental modelThe spontaneous events in the mode are discrete, but stimulated growth and loss follow a classical envelope that stays positive. The model does not compute photon correlations, phase diffusion or linewidth.

Positive gain is not enough

Typical misconceptionAny positive inversion is enough to make the laser oscillate.

Better mental modelThe unsaturated gain has to beat all the losses in one trip around the cavity. Strong output coupling, internal loss or a mode far from the gain line can put threshold out of reach.

Run the experiment

  1. 01

    Tell noise from lasing

    Compare Below threshold and Above threshold. Each selection automatically acquires ten microseconds. Read the event count and the output, even when the light is weak.

    What to observe: Below threshold, spontaneous photons leak out of the cavity, but they never build a macroscopic population in the mode. Above threshold, the mode grows and uses up the stored inversion.
  2. 02

    Start from exact darkness

    Choose Exact dark state, then use Inject one photon and evolve. The one-photon intermediate sample is retained before ten more microseconds are integrated.

    What to observe: With no noise source, a classical photon population of exactly zero stays at zero. One injected photon provides the missing seed.
  3. 03

    Watch relaxation oscillations

    Choose Relaxation oscillation. Compare the acquired upper fraction with the loss threshold; Logarithmic photon trace in Advanced controls changes only the display scale.

    What to observe: Stored population, photon buildup and depletion produce an overshoot, followed by a damped exchange of energy between the atoms and the photons. Photon decay and upper-level recovery happen on different timescales.
  4. 04

    Move the mode off the gain line

    Choose Above threshold and increase the mode offset. Return to Above threshold, switch Pump on off, and inspect the continued record.

    What to observe: Detuning reduces gain without changing mirror loss. Numerical parameters prepare a new run. Switching pumping or seeding keeps the stored state and integrates ten more microseconds, so the subsequent decay remains in the same record.

Related experiments and articles

Continue exploring

From a seed to laser light

Does a smooth startup curve describe what happens in every individual run?

  1. LabLaser Startup from NoiseFollow the mean start-up of many modes and see one win.
  2. You are hereLaser Noise Startup WorkbenchRepeat stochastic seeding and inspect the recorded photon history.

Probes and measurement · Reading path

Controlled light and precision measurement

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

  1. ArticleHow an ammonia beam became a microwave oscillator
  2. LabAbsorption, Spontaneous & Stimulated EmissionWatch a probe beam grow, then fade, in a prepared gas
  3. LabPumping & Population InversionPump three gases with one lamp and see which one amplifies
  4. LabPassive Optical ResonatorCompare stored light with self-sustained oscillation
  5. LabStable Resonator & Transverse ModesCurve two mirrors and size an iris until one beam shape is left
  6. LabBuild & Debug Your First LaserTest gain against cavity loss
  7. LabLaser Startup from NoiseWatch many cavity frequencies compete for one gain
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