Bloch sphere — where it appears
Named by 2 essays across one field — each of them below, with the objects they name alongside it.
Also named here as quantum projection noise — the same set of essays touches all of them, so they are one junction rather than several.
The wait that sets the precision
To measure an atom's frequency, the obvious method is to drive it and look for the response, and the sharpness of the answer is set by how long the drive lasts. Norman Ramsey found in 1949 that most of the drive is wasted. Two short pulses with a long wait between them do better than one long pulse, because during the wait the atom keeps its own time undisturbed, and any difference from the drive's time piles up as an angle the second pulse can read. Every primary clock in the world runs on that idea, and its precision is set by two numbers: how long the atoms can be left alone, and how many of them there are.
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.
Atomic clockQuantum projection noiseBinomial distributionEntanglementInterferenceLinewidthMeasurementSpin squeezingStandard quantum limitSuperpositionTwo-level systemUncertainty principle