Cold-cavity comb
The optical length of the cavity sets the mode spacing. The offset slides the whole comb relative to the atomic line, and each mode keeps its relative order number while you tune.
L09 · Modes and cavity design
Which cavity modes survive after they saturate the gain? If all modes draw on the same gain, usually only the one with the lowest threshold survives; it pulls the gain below what the others need. Hole burning breaks that sharing. When modes feed on different groups of atoms in the spectrum, or on different spots along the cavity, several can lase at once. A filter that adds loss at the rivals' frequencies raises their thresholds and leaves one.
Slide the cavity's mode comb across a gain line and see which modes survive. Compare shared homogeneous gain, separate spectral classes of atoms, standing-wave hole burning and a frequency-selective loss, then record a mode hop.
Physics tutorial
BackgroundA cavity allows only a set of discrete frequencies. The gain line and any frequency-dependent loss decide which of these modes can grow from a weak start. Once the gain saturates, the outcome can change.
Why it mattersSeveral modes can start above threshold, yet the steady state need not keep them all. What happens depends on whether the modes draw on the same atoms, on groups of atoms with different transition frequencies, or on different regions of a standing wave.
Start with the essentials
The optical length of the cavity sets the mode spacing. The offset slides the whole comb relative to the atomic line, and each mode keeps its relative order number while you tune.
A single class of atoms gives a homogeneous Lorentzian line. A Gaussian spread of classes gives a Voigt profile. The normalization makes the unsaturated gain at line center equal to the pump setting.
With intensities normalized to a mean of one, a standing wave overlaps more with itself than with the standing wave of a different axial order. This assumes gain spread evenly through the whole cavity; a short crystal needs a different overlap integral.
The overlaps are exact for the chosen numerical integration and geometry. The saturation formula extends the first-order expansion of local saturation in a form that stays positive; it is not a full spatial Maxwell–Bloch solution.
The mode with the smallest ratio of loss to gain profile has the lowest unsaturated threshold. A tiny classical floor lets suppressed modes grow back after tuning. A mode with more than one percent of the total intensity counts as active.
This linear estimate for a single line at threshold pulls the lasing frequency toward the atomic resonance. The cold-cavity linewidth comes from a base logarithmic round-trip power loss of 0.08. The competition spectrum stays at the cold-cavity frequencies, and the estimate is switched off when its assumptions do not hold.
Typical misconceptionEvery mode whose unsaturated gain exceeds its loss shows up in the final spectrum.
Better mental modelThreshold is checked before the gain saturates. The final gain has to be worked out with all the competing modes present.
Typical misconceptionSeveral surviving lines automatically form short pulses.
Better mental modelThis model tracks no mode phases, so it cannot predict beating, phase locking, pulse formation or linewidth. Later Labs cover those.
Typical misconceptionA homogeneously broadened standing-wave laser must have one mode.
Better mental modelDifferent standing-wave patterns can use up the gain in different places. The travelling-wave reference removes this spatial effect, and even then modes with exactly equal thresholds can share the output.
Choose Homogeneous competition and note how many modes are threshold candidates. Advance three times, then compare that number with the active modes and the side-mode suppression.
What to observe: Several modes initially qualify, but the mode with the smallest threshold depletes the shared gain and suppresses its neighbors.Compare Spectral hole burning and Standing-wave hole burning at the same pump and cavity length. Advance each three times.
What to observe: In spectral hole burning, the modes draw on different classes of atoms, so they saturate each other less. In standing-wave hole burning, each mode overlaps most with itself, which leaves gain for neighboring orders. The two mechanisms are different.Load Filtered inhomogeneous gain, then move the filter center. Inspect both loss and saturated gain before and after advancing.
What to observe: Modes near the filter center see less loss. A wide gain line need not give broad output once the competing thresholds are raised.Load Near a mode hop and advance, then use Tune right and evolve twice. Watch the dominant mode order and the cold-cavity offset.
What to observe: The winning mode changes when the comb moves past half a mode spacing. Tuning keeps the existing intensities, so the takeover can take time.