Quanta: Where the Smooth World Turns Grainy

Shine light on metal and electrons pop out — but only if the colour is right, no matter how bright the beam. Explaining that one stubborn fact broke classical physics.

lesson 2 of 3 in this unit

Builds on: 5.3 Colour & the Spectrum: Most Light Is Invisible2.1 Energy: The Quantity That Only Changes Costume

An experiment that shouldn’t have mattered

Light falling on a metal can kick electrons off its surface — the photoelectric effect. Classically, light is a wave delivering energy continuously, so brighter light should kick harder, and even dim light should manage eventually. The metal disagreed on every count:

  • Below a threshold frequency, nothing — however blinding the beam, however long you wait.
  • Above it, electrons leave instantly, even in the dimmest light.
  • Brighter light: more electrons, but not faster ones. Only bluer light makes faster ones.

Einstein’s uncomfortable answer

In 1905 Einstein took Planck’s bookkeeping trick literally: light arrives in indivisible packets — photons — each carrying an energy set only by frequency:

E = h·fh = 6.63 × 10⁻³⁴ J·s — the granularity of the universe, in one tiny constant

Now the stubborn facts are obvious. An electron is freed by absorbing one photon; if that photon’s E is below the escape cost (the work function), nothing happens — a million weak packets don’t pool. Brightness is just packet count: more electrons, same energy each. Red light is cheap coins, ultraviolet is high-denomination notes, and the metal is a vending machine that takes exact change only. This — not relativity — is what Einstein’s Nobel Prize cites.

Matter is grainy too

The graininess spreads. Atoms hold electrons only on discrete energy rungs — which is why heated elements emit sharp spectral lines (last lesson’s fingerprints): each line is a photon of exactly one rung-to-rung drop. A neon sign’s orange and a sodium lamp’s yellow are quantum leaps you can see from the street. Yet waves refuse to leave the story: streams of single electrons build up interference patterns, and Unit 4’s wave-test says wave while the clicks of detectors say particle. Both, in honesty, are true — the quantum world’s standing offer of humility.

You use this daily

Solar panels are the photoelectric effect monetised — photons promoting electrons into a current. Camera sensors count photons; LEDs run the effect in reverse, each electron dropping a rung and paying out one photon whose colour is the rung height. E = hf is consumer electronics now.

⚗️ Lab — The Photoelectric Bench

A metal plate, a light source with frequency and brightness dials, an electron counter.

  • Start deep in the red and crank the brightness to maximum: nothing. Not one electron.
  • Now slide the frequency up — at the threshold, electrons instantly, even at minimum brightness.
  • Above threshold, compare the dials: brightness moves the count; frequency moves the speed.
5.0 ×10¹⁴ Hz
50%
Electrons
none
Brightness controls
how many — never how fast
Frequency controls
each electron's energy
Because
E = hf, exact change only

Work it by hand — 0 / 1

No multiple choice here: compute the value and type it. Suffixes like 2.5k or 20m are understood; answers within ±3% count.

1. A photon of blue light has f = 6.6 × 10¹⁴ Hz. What is its energy, in joules? (h = 6.63 × 10⁻³⁴; answer like 4.4e-19)

Check your understanding

1. Dim ultraviolet light frees electrons from a metal; blinding red light frees none. Why?

2. Making the (above-threshold) light brighter changes…

3. Why do heated elements emit sharp spectral lines instead of a smooth rainbow?

4. What is the energy of a photon set by?