In simple terms
A friendly intro before the formal notes — no formulas yet.
A Barcode for Every Element
An atom is a tiny, dense, positive nucleus surrounded by electrons that are only allowed to sit at particular energy levels — like rungs on a ladder, never in between. When an electron drops from a higher rung to a lower one, the atom spits out a single packet of light (a photon) whose energy is exactly the gap between the rungs. Because the rungs are fixed, the colours an element emits are fixed too, giving every element a unique light 'barcode'.
Think of a vending machine that only accepts exact change. The electron ladder has rungs worth fixed amounts of energy, and a photon is a coin of one fixed value. An electron can only jump down between rungs if a photon-coin of exactly the right value comes out; it can only jump up if it swallows a coin of exactly the right value. That is why a hot gas glows in a few sharp colours rather than a smooth rainbow — only certain coins exist for that element.
- 1
Fire alpha particles at gold foil (Geiger–Marsden) and, from the few that bounce back, deduce a tiny dense positive nucleus surrounded by mostly empty space.
- 2
Describe any nucleus with : protons, neutrons; isotopes share but differ in .
- 3
Accept that electrons occupy only discrete energy levels — the sharp lines in a spectrum prove the gaps are fixed.
- 4
Use and to turn the energy of a jump between two levels into the frequency or wavelength of the photon released, converting eV to J first.
Explore the concept
Use the live diagram, PhET or GeoGebra sim, and synced steps — play it, drag controls, or tap a step.
Step 1
Fire alpha particles at gold foil (Geiger–Marsden) and, from the few that bounce back, deduce a tiny dense positive nucleus surrounded by mostly empty space.
Key formulas
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Full topic notes
Formal explanation with the rigour you need for the exam.
Evidence for the nucleus: Geiger–Marsden scattering
Before 1911 the accepted 'plum pudding' model imagined the atom as a diffuse cloud of positive charge with electrons dotted through it. Under Ernest Rutherford's direction, Hans Geiger and Ernest Marsden fired a beam of alpha particles (helium nuclei, ) at a very thin gold foil, surrounded by a zinc-sulphide screen that flashed wherever a particle struck. If the plum-pudding picture were right, the fast, massive alpha particles should have sailed through with only tiny deflections.
Most did pass almost straight through — but a small fraction were deflected through large angles, and about 1 in 8000 bounced almost straight back towards the source. A diffuse charge could never turn a fast alpha particle around; only a concentrated charge could. Rutherford's own words capture the shock: it was 'almost as incredible as if you fired a 15-inch shell at a piece of tissue paper and it came back and hit you.'
Most pass nearly straight through → the atom is mostly empty space.
A few deflect through large angles → there is a concentrated region of positive charge that repels the positive alpha particles.
A tiny fraction rebound → that charge sits in a nucleus that is extremely small, very dense, and carries almost all the atom's mass.
Protons, neutrons, electrons and nuclear notation
The nucleus is built from nucleons — protons and neutrons — and is surrounded by electrons. The proton number fixes which element you have; the number of neutrons can vary. Any specific nucleus (a nuclide) is written in standard notation.
is the chemical symbol, is the proton number (number of protons), and is the nucleon number (total protons + neutrons). The number of neutrons follows from . A neutral atom has as many electrons as protons, so it also has electrons. Isotopes are nuclides of the same element — the same — but with different , and therefore a different number of neutrons; because they share the same electron count they are chemically identical but differ in mass and nuclear stability.
Discrete energy levels and line spectra
The electrons around the nucleus cannot take any energy they please. Each is restricted to a set of allowed energy levels, like rungs on a ladder with nothing permitted in between. The levels are labelled with negative energies because a bound electron has less energy than a free one (the free state at rest is the eV reference); the ground state is the most negative, and higher levels lie closer to eV. The strongest evidence for these discrete rungs comes from the light atoms give out.
Heat a low-density gas until it glows and split its light with a prism or diffraction grating, and you do not get a smooth rainbow. You get a few sharp bright lines at particular wavelengths — an emission line spectrum — with darkness in between. Each line is produced when an electron falls from a higher level to a lower one and the atom releases a single photon carrying exactly the energy gap. Pass white light through the same gas when it is cool and you see the reverse: a continuous spectrum crossed by dark absorption lines at exactly the same wavelengths, where electrons have absorbed photons to jump up. The pattern of lines is unique to each element — a light 'barcode' — and the very existence of sharp lines is only possible if the energy gaps, and hence the levels, are fixed and discrete.
Continuous spectrum: every wavelength present (hot solids, liquids, dense gases). Not evidence for discrete levels.
Emission line spectrum: bright lines on dark — electrons falling DOWN between levels emit photons.
Absorption line spectrum: dark lines on a continuous background — electrons jumping UP absorb matching photons.
Emission and absorption lines for one element sit at identical wavelengths, because the same level structure sets both.
The photon, $E = hf$ and the electronvolt
Light is emitted and absorbed in discrete packets called photons. The energy of one photon depends only on its frequency, through Planck's relation.
Here J s is the Planck constant, is the frequency, and the second form uses with m s⁻¹ to bring in the wavelength . A higher frequency (shorter wavelength) always means a more energetic photon: blue-light photons carry more energy than red-light ones. Because atomic energies in joules are awkwardly small, physicists use the electronvolt (eV) — the energy an electron gains crossing a potential difference of one volt: J. Energy levels are usually quoted in eV, but needs SI units, so you must convert any eV value to joules before substituting.
From a transition to a photon wavelength
When an electron drops from a higher level to a lower level , the photon released carries an energy equal to the difference between the levels — never the value of a single level. This is the single most common conceptual error in the topic.
Common mistakes examiners penalise
Using a single level's energy instead of the difference — the photon energy is . Watch the double negative: eV, not or .
Forgetting to convert eV to joules before substituting into or — the equations need SI units. This single slip typically costs the answer mark.
Confusing multiply and divide in the eV↔J conversion — multiply by to reach joules, divide to reach eV.
Calling emission lines a continuous spectrum — sharp separate lines are the evidence for discrete levels; a continuous rainbow is not.
Mixing up emission and absorption — falling electrons EMIT (bright lines); electrons jumping up ABSORB (dark lines). Both appear at the same wavelengths for a given element.
Thinking brighter light means higher-energy photons — brightness sets the NUMBER of photons; shows each photon's energy is fixed by frequency alone.
Mishandling — if given a frequency, find ; do not put a frequency where the equation expects a wavelength.
Over-rounding mid-calculation or dropping units — keep an extra figure through the working and attach m, Hz or J to the final answer.
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 one wrong number early on does not have to cost you the marks that follow. But that protection only exists if the method is written down. Study how each mark below is earned by a specific line.
Where this leads
The discrete-level, photon picture built here underpins the rest of the unit. The same governs the photoelectric effect, where photons eject electrons from a metal, and the same idea of quantised energy carries into the nucleus, where discrete nuclear energy states explain gamma emission. The eV, introduced here as a convenience, becomes the natural energy unit for nuclear reactions and mass–energy calculations. Master the habit — photon energy is the gap between levels, convert to joules, then use — and the quantum physics that follows becomes variations on a method you already own.
Worked examples
See the formulas applied — reveal one step at a time, like the exam.
A nuclide of uranium is written . State the number of (i) protons, (ii) neutrons and (iii) electrons in a neutral atom of this nuclide. [3]
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Use with , .
A photon of green light has a frequency of Hz. Calculate its energy (a) in joules and (b) in electronvolts. (Take J s and J.) [3]
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(a) Use . [M1: correct equation] J. [A1: answer with unit]
Convert (a) an ionisation energy of eV into joules, and (b) a photon energy of J into electronvolts. (Use J.) [2]
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(a) eV → J: multiply by . J. [A1]
In a hydrogen atom an electron falls from the level at eV to the level at eV. Calculate the wavelength of the emitted photon. (Take J s, m s⁻¹, J.) [3]
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Step 1 — energy of the photon = the DIFFERENCE between the levels. eV. [M1: correct difference]
An electron in an atom falls from a level at eV to a level at eV. Calculate the energy of the emitted photon and its wavelength. (Take J s, m s⁻¹, J.) [4]
- 1
Model answer — full working.
How it all connects
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Tap a linked idea to see how it connects back to the main topic — that connection is what examiners reward.
Glossary
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Quick check
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Revision flashcards
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Geiger–Marsden key result
Alpha particles fired at thin gold foil: most pass almost straight through, a few deflect by large angles, about 1 in 8000 bounces back. Conclusion: the atom is mostly empty space with a tiny, dense, positively charged nucleus holding almost all the mass.
Key takeaways
Review these before you close the topic — retrieval beats re-reading.
- ✓
Most pass nearly straight through → the atom is mostly empty space.
- ✓
A few deflect through large angles → there is a concentrated region of positive charge that repels the positive alpha particles.
- ✓
A tiny fraction rebound → that charge sits in a nucleus that is extremely small, very dense, and carries almost all the atom's mass.
Practice — then mark it
The whole point: a real Cambridge question, marked mark-by-mark.
Get a Paper 2 calculation marked: work an energy-level transition to a photon wavelength with full working
Get a Paper 2 calculation marked: work an energy-level transition to a photon wavelength with full working
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Frequently asked
Checkpoint
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Before you move on: do Get a Paper 2 calculation marked: work an energy-level transition to a photon wavelength with full working on paper, snap a photo, and get examiner-style feedback on exactly where you win and lose marks.