In simple terms
A friendly intro before the formal notes — no formulas yet.
Light that Behaves Like Bullets
Shine light on a metal and, under the right conditions, electrons are ejected. Classical physics — light as a continuous wave — predicts the wrong behaviour completely. The results only make sense if light arrives in discrete packets of energy called photons, each delivering its energy to a single electron all at once. The same duality runs backwards too: electrons, which we think of as particles, can diffract like waves.
Imagine trying to knock a coconut off a shelf. A classical 'wave' is like a gentle, continuous breeze — blow long enough and hard enough and surely the coconut must eventually fall. But the photoelectric effect says otherwise: it is like throwing balls. One ball below a certain size will NEVER dislodge the coconut, no matter how many you throw per second. Only a single ball above the critical size does the job — and any extra size becomes the coconut's leftover speed. Each photon is one such ball, and it must act alone.
- 1
Treat light as a stream of photons, each carrying energy set only by the frequency, not the brightness.
- 2
For a photon to eject an electron, its energy must at least equal the work function — the minimum energy binding the electron to the metal.
- 3
Any energy the photon carries above becomes the electron's maximum kinetic energy: .
- 4
Turn the argument around: since waves carry momentum, a particle with momentum has a wavelength , and firing electrons at a crystal produces a diffraction pattern that proves it.
Explore the concept
Use the live diagram, PhET or GeoGebra sim, and synced steps — play it, drag controls, or tap a step.
Step 1
Treat light as a stream of photons, each carrying energy set only by the frequency, not the brightness.
Key formulas
Tap any symbol to reveal exactly what it means and its units.
Full topic notes
Formal explanation with the rigour you need for the exam.
The photoelectric effect: evidence for the photon
Shine ultraviolet light on a clean metal plate and electrons are ejected from its surface. These ejected electrons are called photoelectrons, and the phenomenon is the photoelectric effect. What made it revolutionary was not that electrons come off, but the precise WAY they come off — a way the wave model of light gets completely wrong.
Einstein resolved every one of these puzzles with a single bold idea: light itself is quantised into packets — photons — each carrying an energy fixed by the frequency. A photon is absorbed by one electron in an all-or-nothing event. This is why a below-threshold photon can never free an electron even in a bright beam: each electron only ever meets one photon at a time, and if that single photon is too weak, nothing happens.
Existence of a threshold frequency. Below a certain frequency , no electrons are emitted at all — no matter how intense the light or how long it shines. The wave model predicts that any frequency should work if the light is bright enough.
Instantaneous emission. Above , electrons appear the instant the light arrives, with no time delay for energy to 'build up'. The wave model predicts a measurable lag.
Maximum kinetic energy depends on frequency, not intensity. Increasing the frequency increases the electrons' maximum kinetic energy; increasing the intensity does not. The wave model predicts brighter light should give more energetic electrons.
Intensity controls the number, not the energy. Brighter light of the same frequency simply ejects more electrons per second.
Photon energy, the work function and Einstein's equation
The energy of a single photon depends only on the frequency of the light (or equivalently its wavelength , since ).
To escape the metal, an electron must be supplied with at least a minimum amount of energy called the work function, — a property of the metal alone. The lowest-frequency photon that can just supply this energy defines the threshold frequency, through . When a photon of higher frequency arrives, it spends freeing the electron and hands the leftover energy to the electron as kinetic energy. The most weakly bound electrons keep the most, so the maximum kinetic energy of the photoelectrons is Einstein's photoelectric equation:
is the energy delivered by one photon.
is the work function — the 'entry fee' to leave the metal.
is the maximum kinetic energy of the emitted photoelectrons. If , then would be negative, which is impossible — so no emission occurs.
A graph of against is a straight line of gradient , with -intercept and -intercept .
The electronvolt and the stopping potential
At the quantum scale, the joule is an awkwardly large unit, so we use the electronvolt (eV): the energy an electron gains when accelerated through a potential difference of 1 volt. Since energy transferred is charge times voltage, J. To convert an energy from joules to electronvolts, divide by ; to go the other way, multiply.
How do we actually measure ? By making the electrons pay it back. In the experiment, a reverse potential difference is applied that pushes emitted electrons back toward the metal. As this voltage is increased, fewer electrons have enough energy to cross, until at the stopping potential even the fastest electron is just turned back and the current falls to zero. The work done against the field, , then equals the maximum kinetic energy:
E_{max} = eV_s
The stopping potential depends only on the frequency of the light and the metal — never on the intensity. If an exam question doubles the brightness and asks what happens to the stopping potential, the answer is 'no change'. More intensity means more electrons per second, but each of the fastest ones has exactly the same maximum kinetic energy.
Wave–particle duality and the de Broglie wavelength
The photoelectric effect shows light behaving as particles, yet interference and diffraction show it behaving as a wave. Light is neither purely one nor the other — it has a dual nature, and which face it shows depends on the experiment. In 1924 Louis de Broglie made the daring proposal that this duality is symmetric: if waves can act like particles, then particles should act like waves. He assigned every particle of momentum a wavelength:
The larger a particle's momentum, the shorter its de Broglie wavelength.
Everyday objects have enormous momentum compared with , so their wavelengths are unimaginably small and no wave behaviour is ever observed.
For an electron, which has a tiny mass, the wavelength can be comparable to atomic spacings — small enough to be seen in diffraction.
An electron accelerated through a potential difference gains kinetic energy , from which its momentum, and hence , can be found.
Electron diffraction: evidence for matter waves
De Broglie's idea would have stayed a curiosity without proof — and the proof is electron diffraction. When a beam of electrons is fired through a thin layer of graphite or a crystal, it does not simply make a single bright spot as particles would. Instead it produces concentric rings on a screen, exactly the diffraction pattern a wave makes when it passes through a regularly spaced lattice. Diffraction is a purely wave phenomenon, so the pattern is direct evidence that the electrons travel as waves with a definite wavelength. Measuring the ring spacing gives a wavelength that agrees precisely with , confirming de Broglie's relation.
In 'evidence for' questions, name the phenomenon AND the property it demonstrates. Say that electron DIFFRACTION (or the ring pattern) is the evidence, and that diffraction is a WAVE behaviour, so it shows electrons — normally treated as particles — have a wavelength. A bare 'electrons diffract' without linking diffraction to wave behaviour rarely earns full marks.
The Heisenberg uncertainty principle (qualitative)
If a particle is also a wave, it cannot be pinned to a single exact point — a wave is spread out. This intuition is captured by Werner Heisenberg's uncertainty principle: it is impossible to know both the position and the momentum of a particle with perfect precision at the same instant. The more precisely you fix one, the less precisely the other can be known. Written qualitatively, the product of the uncertainty in position and the uncertainty in momentum has a lower bound:
This is a fundamental feature of nature, not a shortcoming of measuring instruments — even a perfect instrument cannot beat it.
Confine a particle to a very small region (small ) and its momentum becomes correspondingly uncertain (large ), and vice versa.
There is a matching uncertainty relation between energy and time, .
The effect is negligible for large objects because is so small, but it dominates behaviour at the atomic scale.
Common mistakes examiners penalise
Thinking intensity changes the electrons' energy — brighter light of the same frequency ejects MORE electrons per second, but the maximum kinetic energy and the stopping potential are unchanged. Only frequency changes .
Believing below-threshold light works if it is bright or shines long enough — it never does. One electron meets one photon, and a below-threshold photon simply lacks the energy ; electrons cannot pool energy from several photons.
Mixing joules and electronvolts inside — convert everything to the same unit before subtracting. Subtracting a work function in eV from a photon energy left in joules is a classic mark-losing slip.
Confusing the work function with the threshold frequency — they are linked by but is an energy and is a frequency. Do not equate their numerical values.
Inverting the de Broglie relation — it is , so LARGER momentum gives a SHORTER wavelength. Writing or is wrong.
Saying 'electrons diffract' without linking diffraction to wave behaviour — the evidence argument needs the step that diffraction is a wave property, so the electrons must have a wavelength.
Treating the uncertainty principle as an instrument limitation — it is a fundamental limit; the particle does not simultaneously possess an exact position and an exact momentum.
Dropping units or over-rounding mid-calculation — carry extra figures through the working and round only the final answer; always attach the correct unit (J, eV, m, or Hz).
Model answer — marked the way our engine marks it
In Paper 2 the marks are analytic: each is tied to a specific line of working — a method mark (M) or an answer mark (A) — and error-carried-forward (ECF) means a wrong number early on does not have to cost you the marks that follow. But that protection only exists if your method is written down. The photoelectric worked example above shows this in full: earns M1, the photon energy converted to eV earns A1, applying earns a second M1, and the final eV earns the last A1 — with ECF shielding the answer marks if an earlier number slips. Study how each mark is earned by a specific line, and write your own solutions the same way.
Where this leads
The photon and the matter wave are the doorway to the rest of quantum physics. Photon energy reappears in atomic spectra and the emission and absorption of light by energy levels; the de Broglie wavelength underpins why atoms have quantised orbits and why electrons behave as standing waves; and the uncertainty principle sets the ground rules for the full quantum-mechanical description of confined particles. Master the habit here — identify whether the wave or the particle picture applies, keep your energy units consistent, show every line — and the quantum topics that follow become variations on a method you already own.
Worked examples
See the formulas applied — reveal one step at a time, like the exam.
Light of frequency 8.0×10¹⁴ Hz strikes a metal of work function 2.0 eV. Calculate the maximum kinetic energy of the emitted photoelectrons in eV. (h = 6.63×10⁻³⁴ J s; 1 eV = 1.6×10⁻¹⁹ J) [4]
- 1
Model answer — full working.
A metal has a threshold frequency of 5.5×10¹⁴ Hz. (a) Calculate the work function of the metal in joules. (b) Light of wavelength 4.0×10⁻⁷ m is shone on the metal. Determine the maximum kinetic energy of the emitted photoelectrons in joules. (h = 6.63×10⁻³⁴ J s; c = 3.0×10⁸ m s⁻¹.) [4]
- 1
Model answer — full working.
An electron travels at 2.0×10⁶ m s⁻¹. Calculate its de Broglie wavelength. (Mass of electron m = 9.11×10⁻³¹ kg; h = 6.63×10⁻³⁴ J s.) [3]
- 1
Model answer — full working.
How it all connects
The big idea sits in the middle — tap a linked idea to explore the link.
Tap a linked idea to see how it connects back to the main topic — that connection is what examiners reward.
Glossary
Try to recall each definition before you reveal it.
Quick check
Answer in your head first — then tap to check. No pressure.
Revision flashcards
Flip the card. Test yourself before the exam.
The photoelectric effect
The emission of electrons (photoelectrons) from a metal surface when electromagnetic radiation of high enough frequency is shone on it. Its features cannot be explained by the classical wave model of light.
Key takeaways
Review these before you close the topic — retrieval beats re-reading.
- ✓
Existence of a threshold frequency. Below a certain frequency , no electrons are emitted at all — no matter how intense the light or how long it shines. The wave model predicts that any frequency should work if the light is bright enough.
- ✓
Instantaneous emission. Above , electrons appear the instant the light arrives, with no time delay for energy to 'build up'. The wave model predicts a measurable lag.
- ✓
Maximum kinetic energy depends on frequency, not intensity. Increasing the frequency increases the electrons' maximum kinetic energy; increasing the intensity does not. The wave model predicts brighter light should give more energetic electrons.
- ✓
Intensity controls the number, not the energy. Brighter light of the same frequency simply ejects more electrons per second.
Practice — then mark it
The whole point: a real Cambridge question, marked mark-by-mark.
Get a Paper 2 calculation marked: solve a photoelectric problem with full working
Get a Paper 2 calculation marked: solve a photoelectric problem with full working
Extra simulations & links
PhET, GeoGebra and other curated tools — open in a new tab.
Frequently asked
Checkpoint
One marked question is worth ten re-reads — close the loop before you move on.
Reading it isn’t knowing it — prove it.
Before you move on: do Get a Paper 2 calculation marked: solve a photoelectric problem with full working on paper, snap a photo, and get examiner-style feedback on exactly where you win and lose marks.