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Shine light on a metal surface and electrons can be knocked clean off it — but only if the light’s colour is right. Brightness turns out to be irrelevant to whether this happens at all, a fact that stumped physicists until Einstein proposed treating light as a stream of particles rather than a continuous wave.
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When electromagnetic radiation above a certain frequency strikes a metal surface, electrons — — are emitted. Three key observations define the effect: emission is (effectively) instantaneous; below a , no electrons are emitted at all, however intense the light; and above the threshold, increasing intensity increases the NUMBER of photoelectrons per second, but never their maximum kinetic energy.
A wave model of light cannot explain this: it predicts energy should accumulate continuously regardless of frequency, so a dim light of any frequency should eventually free an electron given enough time. Experimentally, below the threshold frequency, no amount of waiting or brightening ever produces emission.
Tip — Learn the three key observations as a set — instant emission, a sharp threshold frequency, and intensity affecting only the RATE (never the maximum energy) of emission.
Einstein explained the effect by treating light as photons, each carrying energy . A photoelectron is emitted when a single photon transfers its entire energy to a single electron at once — explaining the instantaneous emission. Freeing an electron costs a minimum energy, the , , unique to each metal; a photon below this energy can never free an electron, no matter how many arrive, which defines the threshold frequency.
Any surplus photon energy beyond the work function becomes kinetic energy of the emitted electron. The MAXIMUM kinetic energy corresponds to the least tightly bound electrons at the surface.
Tip — If the calculated hf comes out less than φ, no photoelectrons are emitted at all — don’t report a negative kinetic energy; report zero emission.
Equation recap
Common mistakes to avoid
Key takeaways
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