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Sandbox Physics

L06 · Gain and feedback

Laser Noise Startup Workbench

Pump an effective four-level medium inside a lossy cavity. Watch actual random spontaneous mode-seeding events, the turn-on delay, gain clamping and relaxation oscillations.

Interactive modelLaser Noise Startup Workbench
Model time—\text{—}
Elapsed round trips—\text{—}
Upper fraction / inversion—\text{—}
Loss-compensating upper fraction—\text{—}
Mean cavity mode photons—\text{—}
Useful 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{—}
Accepted spontaneous mode events—\text{—}

Physics tutorial

Let a mode grow from one random event

BackgroundPumping stores upper-state excitation while the cavity loses photons. A spontaneously emitted photon can enter the selected cavity mode; once gain beats loss, stimulated emission grows that mode.

Why it mattersNear-zero initial light makes turn-on delay visible. The growing field then drains the same reservoir that supplied the gain.

Start with the essentials

Focus question
Can a pumped above-threshold medium remain exactly dark when spontaneous seeding is disabled?
One-sentence intuition
The threshold compares unsaturated gain with complete cavity loss. Finite spontaneous seeding smooths the transition; above threshold, saturation clamps gain near loss.

Core mathematical model

Coupled reservoir and photon flow

n˙=R(1−n)−nτu−GnScNa,S˙c=(Gn−κ)Sc+βNanτu\dot n=R(1-n)-\frac{n}{\tau_u}-G n\frac{S_c}{N_a},\qquad\dot S_c=(Gn-\kappa)S_c+\beta\frac{N_a n}{\tau_u}

The displayed equations are the mean drift. In the simulation, the selected spontaneous contribution uses Poisson jumps: each accepted event removes one upper emitter and adds one mode photon. The remaining radiation is continuous.

Geometry, spectral overlap and loss

G=2σ0NaATR[1+(Δν/γ)2],κ=−ln⁡[Rb(1−T)(1−ℓ)]TRG=\frac{2\sigma_0N_a}{AT_R[1+(\Delta\nu/\gamma)^2]},\quad\kappa=-\frac{\ln[R_b(1-T)(1-\ell)]}{T_R}

The gain medium is traversed twice per linear-cavity round trip. The active-emitter count is fixed at one billion; changing area therefore changes density and photon overlap. Cavity time is a vacuum-equivalent optical length.

Ideal zero-noise threshold

nth=κ/G,n0=Rτu1+Rτu,Rth=nthτu(1−nth)n_{\mathrm{th}}=\kappa/G,\quad n_0=\frac{R\tau_u}{1+R\tau_u},\quad R_{\mathrm{th}}=\frac{n_{\mathrm{th}}}{\tau_u(1-n_{\mathrm{th}})}

The pump threshold is unreachable when the required fraction is at least one. This is an ideal zero-noise threshold, not a sharp discontinuity in a finite spontaneously seeded trajectory.

Gain clamping and calibrated output

nss≃nth,Sc,ss≃Na[R(1−nth)−nth/τu]κ,Pout=hνκoutScn_{\mathrm{ss}}\simeq n_{\mathrm{th}},\quad S_{c,\mathrm{ss}}\simeq\frac{N_a[R(1-n_{\mathrm{th}})-n_{\mathrm{th}}/\tau_u]}{\kappa},\quad P_{\mathrm{out}}=h\nu\kappa_{\mathrm{out}}S_c

The first two relations neglect the small spontaneous source above threshold. Output loss is the logarithmic attenuation from the output mirror divided by round-trip time; power is an averaged envelope readout.

Common difficulties

The stochastic events are only seeding

Typical misconceptionThe photon-number trace is an exact quantum counting simulation.

Better mental modelSpontaneous cavity events are discrete, but stimulated growth and loss use a positive classical envelope model. It does not calculate photon correlations, phase diffusion or linewidth.

Positive gain is insufficient

Typical misconceptionAny positive inversion guarantees oscillation.

Better mental modelUnsaturated gain must overcome complete feedback loss. Strong output coupling, internal loss or spectral mismatch can make the threshold unreachable.

Run the experiment

  1. 01

    Separate noise from oscillation

    Compare Below threshold and Above threshold using Advance 10 μs. Read the event count and output even in the weak state.

    What to observe: Below threshold, spontaneous photons can leave the cavity but do not sustain a macroscopic mode. Above threshold, the mode grows and depletes stored inversion.
  2. 02

    Test the exact dark state

    Choose Exact dark state and advance 10 μs. Inject one photon, then advance again.

    What to observe: Without a noise source, an exactly zero classical photon population remains zero. A single injected photon supplies the missing seed.
  3. 03

    Observe relaxation

    Choose Relaxation oscillation and advance. Compare the upper fraction with the loss threshold and inspect the linear output trace.

    What to observe: Population storage, photon buildup and depletion produce overshoot and damped exchange; photon decay and upper-state recovery have different timescales.
  4. 04

    Break spectral overlap

    Choose Above threshold, increase mode detuning, then advance again. Turn the pump off to observe decay.

    What to observe: Detuning reduces gain overlap while mirror loss remains. The state is preserved when rates change; each preset and random-seed change starts a new preparation.