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L31 · Feedback without mirrors

Random Laser

Can scattering hold light long enough to lase? It can. Light that scatters many times wanders through the pumped medium along a long, tangled path and picks up gain the whole way. With enough gain it grows past threshold without any mirrors. That diffuse growth is one effect; sharp random resonances selected by interference are a different one.

Let multiple scattering do the job of mirrors. Change the sample size, the gain and the pumped core, and record how the light grows, saturates and diffuses out of the sample.

Interactive modelRandom Laser
Resolved optical threshold candidates—\text{—}
Selected coherent wavelength—\text{—}
Selected outgoing-mode threshold—\text{—}
Selected mode participation fraction—\text{—}
Outgoing boundary residual—\text{—}
Candidates above unsaturated gain threshold—\text{—}
Elapsed model time—\text{—}
Optical thickness—\text{—}
Diffusion coefficient—\text{—}
Full-inversion gain threshold—\text{—}
Initial principal growth rate—\text{—}
Second diffusion growth rate—\text{—}
Third diffusion growth rate—\text{—}
Mean normalized energy—\text{—}
Total normalized escape flux—\text{—}
Current net energy growth rate—\text{—}
Central excited fraction—\text{—}
Captured time samples—\text{—}
Initial gain regime—\text{—}
Diffusion approximation—\text{—}

Physics tutorial

Scattering creates a long residence time

BackgroundA disordered gain medium can get feedback without the usual pair of mirrors.

Why it mattersHere multiple scattering does the job of the mirrors. Change the sample size, the gain and the pumped core to see how the light grows, saturates and diffuses out.

Start with the essentials

Focus question
Can scattering hold light long enough to lase?
One-sentence intuition
Diffusion explains how trapped light grows overall, but sharp random resonances come from interference, which diffusion cannot predict.

Core mathematical model

Light energy diffuses and grows

∂tW=D∇2W+v(g0n−α)W+snD=vℓt/3\begin{aligned}\partial_t W&=D\nabla^2W+v(g_0n-\alpha)W+s n\\D&=v\ell_t/3\end{aligned}

More scattering lowers the diffusion coefficient, so light takes longer to escape.

The inversion saturates

n˙=p(r)(1−n)−n(1+W)τnp(r)=p0(r<a)\begin{aligned}\dot n&=\frac{p(r)(1-n)-n(1+W)}{\tau_n}\\p(r)&=p_0\quad(r<a)\end{aligned}

This normalized rate law, chosen for the Lab, limits the gain. It is not a quantum model of any particular material.

Threshold for a uniformly pumped sphere

W(R)=0λ1=v(g−α)−Dπ2R2gth=α+π2ℓt3R2\begin{aligned}W(R)&=0\\\lambda_1&=v(g-\alpha)\\&\quad-\frac{D\pi^2}{R^2}\\g_{\rm th}&=\alpha+\frac{\pi^2\ell_t}{3R^2}\end{aligned}

The boundary here absorbs perfectly and ignores the extrapolation length. This formula uses the effective unsaturated gain. The full-inversion gain threshold readout also accounts for the initial excited fraction and the pumped core, using a numerical eigenvalue.

Spatial modes of the intensity

L=D∇2+v(g−α)LΦj=λjΦjΦj(r)∝sin⁡(jπr/R)/r\begin{aligned}\mathcal L&=D\nabla^2+v(g-\alpha)\\\mathcal L\Phi_j&=\lambda_j\Phi_j\\\Phi_j(r)&\propto\sin(j\pi r/R)/r\end{aligned}

The radial sine form applies to uniform unsaturated gain; a pumped core uses numerical eigenvectors. Higher-order basis functions change sign, but the physical intensity remains nonnegative.

Energy balance and escape through the surface

Uˉ=3R3∫0RWr2 drUˉ˙=Gˉ+Sˉ−Aˉ−FˉFˉ=−3DR∂rW∣R\begin{aligned}\bar U&=\frac{3}{R^3}\int_0^R Wr^2\,dr\\\dot{\bar U}&=\bar G+\bar S-\bar A-\bar F\\\bar F&=-\frac{3D}{R}\left.\partial_rW\right|_R\end{aligned}

The page divides energy and total surface escape by the sphere volume. Fluxes between neighbouring cells cancel; the remaining outer flux per volume is the reported output.

When diffusion is valid

R/ℓt≫1max⁡(g0,α)ℓt≪1\begin{aligned}R/\ell_t&\gg1\\\max(g_0,\alpha)\ell_t&\ll1\end{aligned}

With weak scattering the diffusion picture breaks down, and the model does not add coherent resonances to make up for it.

A separate layered sample with interference

Ej(z)=Ajeiknjz+Bje−iknjznj=nj,r−igj/(2k)(ARBR)=M(k,g)(ALBL)\begin{aligned}E_j(z)&=A_je^{ikn_jz}\\&\quad+B_je^{-ikn_jz}\\n_j&=n_{j,r}-ig_j/(2k)\\\binom{A_R}{B_R}&=M(k,g)\binom{A_L}{B_L}\end{aligned}

The refractive indices and widths of the seeded layers set the reflection at each interface and the phase of the light. This sample is not an optical reconstruction of the diffusing sphere.

Threshold modes with light only leaving

AL=BR=0M22(k,gth)=0P=(∫∣E∣2dz)2L∫∣E∣4dz\begin{aligned}A_L&=B_R=0\\M_{22}(k,g_{\rm th})&=0\\\mathcal P&=\frac{(\int |E|^2dz)^2}{L\int |E|^4dz}\end{aligned}

The solver looks for a real frequency and a positive gain that satisfy both outgoing-boundary conditions. The participation ratio measures how concentrated a mode is in space. The modes found are candidates: the list is not complete, and saturation is not included.

Common difficulties

Random lasing must show speckle

Typical misconceptionThe smooth diffusion map should show narrow, random spectral spikes.

Better mental modelThe sphere shows how the ensemble-averaged intensity diffuses. To find threshold modes selected by interference, switch to the separate coherent layer sample; those modes are not derived from the sphere data.

A positive growth rate means endless growth

Typical misconceptionAbove the linear threshold, the output keeps growing without limit.

Better mental modelStimulated emission uses up the local inversion, so the gain drops and the output saturates.

Run the experiment

  1. 01

    Cross the threshold

    Compare Diffuse feedback and Below threshold. Each preset automatically records twenty nanoseconds; the replay illustrates surface escape.

    What to observe: When the initial growth rate is positive, the light grows at first and then levels off at a finite, saturated output.
  2. 02

    Change how long light stays

    Keep the gain fixed and shrink the sample or weaken the scattering.

    What to observe: Light escapes faster, and the threshold goes up.
  3. 03

    Change the pump region

    Compare the Small pump core and Whole-volume pump presets.

    What to observe: When the outer shell is not pumped, the leading spatial mode needs more gain to keep going.
  4. 04

    Look at coherent modes

    Open Advanced controls and choose Show coherent layers. Pick a mode, then change the layer seed or the pumped fraction; the separate optical calculation updates automatically.

    What to observe: Each mode has its own wavelength, threshold and participation. Compare these, and the outgoing-boundary residual, with the layer stack shown in the apparatus.
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