Standard quantum limit — where it appears
Named by 2 essays across one field — each of them below, with the objects they name alongside it.
The noise pushed below the floor
A perfectly steady laser beam still flickers, by an amount set by the vacuum itself, and for most of the twentieth century that flicker was treated as the floor of any optical measurement. It is a floor only for one shape of noise. Light can be made quieter than the vacuum in one property by being made louder in another — and the price, the fragility and the use of that trade are all visible in how the noise is shaped, which is why the world's gravitational-wave detectors now run on it.
The atoms that measure better together
A clock read with a hundred independent atoms locates its phase no better than the scatter of a hundred coin tosses allows, because each atom answers the final question by itself. Let the atoms interact for a moment before they are read and that scatter can be shaped: the round uncertainty of their combined spin is sheared into a thin ellipse, and a phase error invisible against the coin-toss noise becomes four standard deviations wide. The gain grows with the number of atoms, and it is real only if the detector can count atoms nearly one by one.
Named alongside it
The objects these essays reach for when they reach for this one.
Uncertainty principleAtomic clockBinomial distributionBloch sphereEntanglementGravitational wavesOptical lossQuadratureQuantum projection noiseShot noiseSpin squeezingSqueezed light