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Sandbox Physics

L04 · Gain and feedback

Single-Pass Optical Amplifier

Why does an inverted medium stop giving exponential gain? Because the light it amplifies spends the inversion. Each new photon from stimulated emission moves an atom out of the upper level, and the seed and the spontaneous emission all draw on the same inversion. The more the light grows, the lower the gain, until it saturates. Bright output from a medium with no mirrors is amplified spontaneous emission, not a laser.

Send a seed beam through a pumped medium. Compare its amplified power with a forward ASE channel, follow how the inversion is used up along the medium, and get a bright output with no feedback mirror.

Interactive modelSingle-Pass Optical Amplifier
Input seed power—\text{—}
Output seed-channel power—\text{—}
Selected forward ASE power—\text{—}
Seed power gain—\text{—}
Small-signal reference gain—\text{—}
Saturation power—\text{—}
Exit local gain—\text{—}
Exit inversion fraction remaining—\text{—}
Total forward photon flux—\text{—}

Physics tutorial

Use the inversion once

BackgroundAs the seed travels through the medium, it takes energy from the pumped upper level. The lower laser level empties quickly, so the local upper-level density sets the gain.

Why it mattersA bright amplified beam can appear even when no light is sent back through the medium. It helps to recognize saturation and amplified spontaneous emission (ASE) before adding feedback.

Start with the essentials

Focus question
Does light still come out when the seed is removed, and would that prove the medium is oscillating?
One-sentence intuition
The seed and the collected ASE draw on the same stored inversion, so more power in either one leaves less inversion for both.

Core mathematical model

Frequency-dependent cross section

σ(Δ)=σ01+(Δ/γ)2,g0=σN0\sigma(\Delta)=\frac{\sigma_0}{1+(\Delta/\gamma)^2},\qquad g_0=\sigma N_0

Detuning is measured in gain half-widths. Cross section is per emitter; density is per cubic metre and gain is per metre.

Steady depletion at each point

N(z)=N01+[Ps(z)+Pa(z)]/Psat,Psat=hνAστN(z)=\frac{N_0}{1+[P_s(z)+P_a(z)]/P_{\mathrm{sat}}},\quad P_{\mathrm{sat}}=\frac{h\nu A}{\sigma\tau}

The pump keeps restoring the upper-level density toward its unsaturated value with a fixed recovery time. The lower level stays empty. The mode area is 0.5 square millimetres and the recovery time is 0.5 milliseconds.

Seed and ASE share one inversion

dPsdz=σNPs,dPadz=σNPa+βhνANτ\frac{dP_s}{dz}=\sigma NP_s,\qquad\frac{dP_a}{dz}=\sigma NP_a+\beta\frac{h\nu AN}{\tau}

When the spontaneous channel is on, its collection fraction is 0.0001. That source term and the seed amplification use up the same upper-level energy. No backward wave is included.

An independent check without ASE

ln⁡PoutPin+Pout−PinPsat=g0L(β=0)\ln\frac{P_{\mathrm{out}}}{P_{\mathrm{in}}}+\frac{P_{\mathrm{out}}-P_{\mathrm{in}}}{P_{\mathrm{sat}}}=g_0L\quad(\beta=0)

With ASE switched off, this implicit relation checks the numerical propagation. A weak enough seed gets plain exponential gain, and the optical power added is limited by the pump that replenishes the inversion.

Common difficulties

The ASE readout is one forward channel

Typical misconceptionThe ASE power shown is all the spontaneous light the medium gives off.

Better mental modelOnly one forward channel, with a set range of angles and frequencies, is collected. Backward and uncollected emission are left out, so this readout is not the total fluorescence.

Saturation comes from the populations

Typical misconceptionThe detector or the display is what caps the power.

Better mental modelThe total optical power in the model depletes the computed upper-level density. The power readout is linear and does not depend on how bright the schematic scene looks.

Run the experiment

  1. 01

    Find the weak-seed limit

    Choose Weak seed. Turn off Selected spontaneous channel and lower the logarithmic seed power. Compare the seed gain with the small-signal reference.

    What to observe: At low photon flux, the inversion stays nearly uniform along the medium and the gain approaches the reference value.
  2. 02

    Use up the inversion along the medium

    Choose Saturation and increase the medium length. Compare the signal trace, the inversion at the exit and the local gain.

    What to observe: The upper-level density drops along the beam path, and the signal gain stays below the unsaturated exponential prediction.
  3. 03

    Get output without a seed

    Choose ASE without seed. Turn Selected spontaneous channel off, then on again.

    What to observe: With no seed and no spontaneous source, the output stays dark. Any nonzero source is amplified in a single pass, with no feedback loop at all.
  4. 04

    Tune off the gain line

    Choose Weak seed, then increase the detuning and leave every other setting as it is.

    What to observe: The stimulated cross section and the local saturation power change together, consistent with each other. More intensity cannot make up for missing frequency overlap.
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