The physicsEach photon carries E = hf, and each electron is freed by one photon, so Emax = hf − Φ and eVs = Emax, exact in every readout, taking the collector to have the same work function as the photo-surface. h = 6.626×10−34 J s, e = 1.602×10−19 C, hc = 1240 eV nm.
The modelElectrons leave with kinetic energies spread evenly from zero to Emax. One photon in a hundred frees an electron, at every wavelength; real surfaces vary strongly with wavelength. At 0 V half the electrons head for the collector, and a positive collector draws in the rest. Real tubes round off the foot of the curve.
The apparatusA lamp and a grating monochromator, 200–700 nm, with the mercury lines at 254, 365, 405, 436, 546 and 577 nm marked. Illuminated area 1.0 cm². Work functions: caesium 2.10, sodium 2.36, zinc 4.33, copper 4.65 eV — typical values; a real surface varies by a few tenths of an eV.
The drawingElectrons are slowed tens of millions of times. Each wave packet stands for 2×1010 photons and each dot for 2×108 electrons, except in No waiting, where each stands for one. The measured limit on the delay, under 3 ns, is from Lawrence and Beams (1928).
What it is built onDocumented student difficulties: that brighter light gives faster electrons, that the supply voltage is what pulls electrons out, and that the current–voltage graph is a straight line through the origin. Steinberg, Oberem & McDermott (1996), Am. J. Phys. 64, 1370; Steinberg & Oberem (2000), J. Comput. Math. Sci. Teach. 19, 115; McKagan, Handley, Perkins & Wieman (2009), Am. J. Phys. 77, 87.