The Photoelectric Effect
Why a dim blue light can eject electrons that a blinding red light never touches.
A Puzzle Classical Physics Couldn't Solve
In the late 1800s, physicists shone light on metal surfaces and watched electrons pop out — the photoelectric effect. It seemed easy to explain if light is a wave: brighter light carries more energy, so brighter light should knock electrons out with more energy. But that's not what happened.
Turn up the intensity of dim red light as much as you like, and nothing comes out. Switch to a faint blue light, and electrons fly out immediately. The color (frequency) of the light mattered — not how bright it was. Something was deeply wrong with treating light as a smooth, continuous wave.
In 1905, Einstein proposed that light isn't continuous when it interacts with matter — it arrives in discrete packets of energy called photons. Each photon carries a fixed amount of energy that depends only on the light's frequency, never its intensity. A single photon either has enough energy to knock an electron free, or it doesn't. Turning up the intensity just sends more photons per second; it doesn't make any one photon more energetic.
Reading the Stopping Voltage
Experimentally, physicists measure \(KE_{max}\) by applying a reverse voltage just strong enough to stop the fastest electrons from reaching a collector — the stopping potential \(V_0\), where \(eV_0 = KE_{max}\). Plot \(KE_{max}\) against frequency for a given metal and you get a straight line. Its slope is exactly \(h\) — the same constant no matter which metal you test — and its x-intercept is the threshold frequency \(f_0\). That graph, built from real data, is some of the cleanest evidence we have that light is quantized.
- Find the photon energy using \(E = hf = \dfrac{hc}{\lambda}\). Using \(hc = 1240\,\text{eV·nm}\): \(E = \dfrac{1240}{400} = 3.10\,\text{eV}\).
- Apply Einstein's equation: \(KE_{max} = hf - W = 3.10\,\text{eV} - 2.28\,\text{eV}\).
- \(KE_{max} = 0.82\,\text{eV}\).
- Relate work function to threshold wavelength: \(W = \dfrac{hc}{\lambda_0}\). Using \(hc = 1240\,\text{eV·nm}\): \(W = \dfrac{1240}{580} \approx 2.14\,\text{eV}\).
- Convert to joules: \(W = 2.14\,\text{eV} \times 1.60\times10^{-19}\,\text{J/eV} \approx 3.43\times10^{-19}\,\text{J}\).
- Find the threshold frequency from \(f_0 = W/h\): \(f_0 = \dfrac{3.43\times10^{-19}}{6.63\times10^{-34}} \approx 5.17\times10^{14}\,\text{Hz}\).
It's tempting to think brighter light means faster electrons. It doesn't. Intensity controls how many photons arrive per second, so it changes the number of electrons ejected (the photocurrent) — not their maximum speed. Only a higher frequency (bluer light) increases \(KE_{max}\), because that's what increases the energy of each individual photon. Keep intensity and frequency firmly separated in your mind, and this topic gets much less confusing.
Check your understanding
- Light delivers energy in discrete packets called photons, each carrying E = hf — determined by frequency alone, never by intensity.
- Every metal has a work function W: the minimum energy needed to free an electron from its surface.
- Only light above the threshold frequency f0 = W/h (or below the threshold wavelength λ0 = hc/W) can eject electrons, no matter how bright it is.
- Einstein's equation KEmax = hf − W predicts the maximum kinetic energy of ejected electrons; intensity only changes how many electrons are ejected, not how fast.