The Quantum Choir: Why an Extra Soloist Doesn't Boost Volume express

Original: "Scaling theory of decoherence in Dicke superradiance"
arXiv:2607.28034v1 · 2026-07-30 · CC BY 4.0 · 1 min
When each atom is disrupted by random noise, their collective glow can fade to ordinary levels.

A choir where every singer hits the notes precisely sounds louder than you'd expect from a simple sum of voices. A hundred singers aren't just a hundred times louder than one: they're ten thousand times louder. In the world of atoms, something similar happens. In collective behavior discovered by Robert H. Dicke, synchronously emitted photons amplify each other. The brightness grows with the square of the number of atoms.

But a choir is easily ruined. Slight stochastic modeling in rhythm or off-key notes blur the overall harmony. To understand exactly how noise destroys collective emission, physicists included two effects in their model: local loss of synchronization (decoherence) and spontaneous emission by individual atoms. It turned out that depending on their strength, the system can be in three regimes: fully collective, partially collective, and independent loners.

The brightness of N synchronized atoms grows as N² — for example, 100 atoms shine 10 000 times brighter than one!

What proved far more interesting was the boundary between these regimes. The transition from full collectivity to partial resembles the moment a choir loses its conductor: a second ago the singers held the line, and now each is singing on their own. If noise is strong, adding more atoms does not boost the light — the system works as a sum of loners. entropy imposes hard limits. Even increasing the number of atoms won't bring back the collective power.

The boundary between collective and independent emission is sharp: a slight increase in noise pushes atoms from choir mode to scattered soloists.

Collective emission was first observed in the 1970s in sodium vapors. It required temperatures just millionths of a degree above absolute zero — otherwise thermal noise destroyed the synchrony.

I \propto N^2
The intensity of superradiance is proportional to the square of the number of emitters (N²).
Scientists
David DeutschErwin SchrödingerJohn Stewart BellLouis de BroglieLov GroverPaul Benioff
Concepts
Shelford's law of tolerance gravitational decoherence complex system dynamics Cope's rule scalable scale invariance Gause's competitive exclusion principle quantum decoherence open quantum system scaling dephasing spatial coherence decadal variability energy cascade decay Hill equation Schrödinger equation superradiance Stokes' theorem Dynamical Systems