Planck constant — where it appears
Named by 4 essays across 2 fields — each of them below, with the objects they name alongside it.
The curve that would not come down
Classical physics predicted that a warm object radiates infinite power at short wavelengths. Every step of the derivation was correct, the prediction was absurd, and closing the gap required assuming that energy comes in lumps.
Light arrives in lumps, and brightness only changes how many
Shine dim blue light on a metal and electrons come out. Shine intense red light and none do, however long the wait. The frequency decides whether anything happens; the intensity decides only how much.
Everything has a wavelength, and almost nothing shows it
If light with a momentum can behave like a particle, a particle with a momentum can behave like a wave. The wavelength is Planck's constant over the momentum, which for anything larger than a molecule is a number too small to have consequences.
The test of mass and energy that needs a ruler
The most direct test of E = mc² weighed two silicon atoms and measured a gamma ray. A silicon-28 nucleus that captures a slow neutron becomes silicon-29 and loses three ten-thousandths of its mass as gamma rays; weigh both atoms in a trap where they circle a magnetic field, measure the gamma rays by the angle at which a silicon crystal diffracts them, and the two sides agree to four parts in ten million. What the comparison needed is the interesting part: the recoil of the atom, a correction four hundred times larger than the precision, computed from the momentum relativity gives to light; angles of a few hundred picoradians; and a chain of constants tying a frequency and a ruler to the same number.
Named alongside it
The objects these essays reach for when they reach for this one.
BlackbodyQuantisationSpectrumWavelengthAtomic mass unitBinding energyBragg diffractionCrossover scaleDecoherenceDiffractionEnergy conservationEquipartition