Is light a stream of bullets, or waves? The photoelectric effect declared: bullets. Electrons are ejected from metal only if the light frequency exceeds a threshold, and the energy depends on the color, not the brightness. Einstein's equation E = hf — W precisely describes how much energy the electron retains after escape.
How it works
Used in solar cells (photons create electron-hole pairs), in light sensors, in photomultipliers for detecting weak light signals. It also explains the red edge of the photoelectric effect — the minimum frequency at which current still flows.
💡 Einstein received the 1921 Nobel Prize for explaining the photoelectric effect, not for the theory of relativity, which initially seemed too bold.
In 1905, Albert Einstein proposed that light consists of quanta (photons) with energy hf. When it hits a metal, the photon disappears, and its energy goes into ejecting an electron. The work function W is the 'entry ticket' for the electron. Analogy: a vending machine that accepts only coins of a certain denomination; if the coin is smaller, the product doesn't come out.
How it works
Used in solar cells (photons create electron-hole pairs), in light sensors, in photomultipliers for detecting weak light signals. It also explains the red edge of the photoelectric effect — the minimum frequency at which current still flows.
💡 Millikan spent 10 years on experiments trying to disprove Einstein's equation, but ended up confirming it with high accuracy and measured Planck's constant.
Einstein's photoelectric equation: the maximum kinetic energy of a photoemitted electron equals the energy of the absorbed photon minus the work function: E_k = hf — W. It embodies the quantum nature of light, where energy is transferred to matter in portions.
Discovery
Albert Einstein, inspired by Max Planck's quantum hypothesis, introduced the concept of the photon and proposed the photoelectric equation in his March 1905 paper. Experimental confirmation was provided by Robert Millikan in 1916 after years of testing. Einstein received the Nobel Prize in Physics in 1921 precisely for this work.
How it works
The equation underlies photoemission spectroscopy, which allows measuring the work function of materials and surface chemical composition. Applicable for ultraviolet and visible radiation on metals; for the X-ray range relativistic corrections are required, and for semiconductors electron affinity is used instead of the work function.
Caveats
At high intensities, multi-photon processes are possible, not described by the simple equation; The equation assumes instantaneous emission, but in reality there is a time delay; Does not take into account the effect of temperature on electron distribution
E_k = h f - W
E_k — maximum kinetic energy of the ejected electron (in joules or eV), h — Planck's constant (h ≈ 6.626×10⁻³⁴ J·s), f — frequency of the incident light, W — work function of the material (energy required for an electron to leave the surface, typically 2 to 5 eV for metals).
E = h f
E — energy of the photon, h — Planck's constant, f — frequency of the radiation.
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