Work Function & Stopping Potential
Also known as: Photoelectric equation · Einstein's photoelectric relation
Shine light on a metal and electrons pop out — but only if the light's color is bluer than a threshold, no matter how bright. Einstein explained it: light arrives as packets of energy hf. One packet kicks out one electron, but the electron must first pay an 'exit toll' φ to escape the metal. Whatever energy is left over becomes the electron's kinetic energy. Brightness adds more packets (more electrons) but never more energy per electron — that only comes from higher frequency.
Photons strike a metal; when hf exceeds the work function, electrons are ejected with the leftover energy as speed.
Equivalent forms
A straight line: plot stopping voltage vs frequency and its slope is h/e — Millikan measured Planck's constant this way while trying to prove Einstein wrong.
Where it holds
Dimensional analysis
In his 'miracle year' Einstein proposed that light itself is quantized, not just its emission (as Planck had assumed). The photoelectric paper — not relativity — won him the 1921 Nobel Prize. Robert Millikan spent a decade trying to disprove the light-quantum idea, and instead confirmed the linear law and measured h to 0.5%.
- Photomultiplier tubes and night-vision devices
- Solar-cell surface engineering
- X-ray photoelectron spectroscopy (XPS) for material analysis
- Brighter light does NOT give faster electrons — only more of them
- There is a sharp threshold frequency below which nothing happens
- Emission is essentially instantaneous, contradicting the classical energy-accumulation picture
What if…
No electrons emerge no matter how intense the beam — the classic classical-physics failure.
The threshold frequency drops, so even red light can eject electrons — why cesium is used in photocathodes.
Stopping potential for sodium
- f:
- 8.0e14 Hz
- φ:
- 2.28 eV
- K_\max = 3.31 - 2.28 = 1.03\,\mathrm{eV}
- V_{0} = K_\max /e = 1.03\,\mathrm{V}