Atomic & nuclear physics: radioactivity, half-life, fission/fusion
JAMBWAECNECO
What the syllabus asks
JAMB: Atomic and nuclear physics
WAEC: Structure of the atom (models of the atom, nucleus, isotopes); radioactivity (alpha, beta, gamma; properties; detection; decay equations; half-life and decay constant); nuclear reactions (fission, fusion, mass defect, binding energy, E = mc²); uses and hazards of radioactivity
NECO: Structure of the atom (models of the atom, nucleus, isotopes); radioactivity (alpha, beta, gamma; properties; detection; decay equations; half-life and decay constant); nuclear reactions (fission, fusion, mass defect, binding energy, E = mc²); uses and hazards of radioactivity
What you will learn
- Describe the nuclear model of the atom and the evidence for it.
- Use A, Z and N notation and identify isotopes.
- Compare the properties of alpha, beta and gamma radiation.
- Write and balance nuclear decay equations.
- Solve half-life problems from data, tables and graphs.
- Calculate mass defect and binding energy; explain fission, fusion, uses and hazards.
Key points
- Rutherford: atom mostly empty; tiny dense positive nucleus.
- ᴬ_Z X: Z protons, A − Z neutrons; isotopes have equal Z, different A.
- α = ⁴₂He (most ionising, least penetrating); β⁻ = electron; γ = EM wave (most penetrating, uncharged).
- α decay: A − 4, Z − 2; β⁻ decay: Z + 1; γ: no change in A or Z.
- Half-life: N = N₀(½)^(t/T); λ = 0.693/T; activity A = λN; subtract background.
- Mass defect × 931 MeV = binding energy; E = mc².
- Fission: heavy nucleus splits (reactor: fuel, moderator, control rods, coolant); fusion: light nuclei join at very high temperature.
- Uses: radiotherapy, tracers, gauges, carbon dating, smoke detectors; follow safety rules (tongs, lead, distance, short time).
Start here: Models of the atom
Our picture of the atom developed through experiments.
- Dalton (1803): atoms are tiny indivisible spheres.
- Thomson (1897): discovered the electron; proposed the "plum pudding" model, a sphere of positive charge with electrons embedded.
- Rutherford (1911): the alpha-scattering experiment showed that the atom is mostly empty space with a tiny, dense, positive nucleus.
- Bohr (1913): electrons move in fixed orbits (energy levels) and emit or absorb light only when they jump between levels (the lesson “Quantum physics: photoelectric effect & X-rays”).
Rutherford’s gold-foil experiment
Geiger and Marsden fired alpha particles at very thin gold foil. Results and conclusions:
| Observation | Conclusion |
|---|---|
| Most alpha particles passed straight through | The atom is mostly empty space |
| A few were deflected through large angles | There is a concentrated positive charge |
| Very few (about 1 in 8,000) bounced back | The positive charge and most of the mass are in a very tiny nucleus |
The nucleus is about 10⁻¹⁵ m across, while the atom is about 10⁻¹⁰ m: if the atom were the size of a football stadium, the nucleus would be a small bead on the centre spot.
Why could the plum pudding model not explain the alpha particles that bounced back?
- In that model the positive charge is spread thinly, so its field is weak everywhere.
- A weak, spread-out charge cannot turn back a fast, heavy alpha particle. Only a concentrated charge can.
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Practice questions
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Key words
- Nucleus
- The small central part of an atom containing protons and neutrons.
- Nucleon
- A proton or a neutron.
- Atomic number (Z)
- Number of protons in the nucleus.
- Mass number (A)
- Number of nucleons in the nucleus.
- Isotopes
- Atoms of the same element with different numbers of neutrons.
- Nuclide
- A particular nucleus with specified A and Z.
- Radioactivity
- Spontaneous disintegration of unstable nuclei with emission of radiation.
- Activity
- Number of disintegrations per second; unit becquerel (Bq).
- Half-life
- Time taken for half the radioactive nuclei in a sample to decay.
- Decay constant (λ)
- Probability per unit time that a nucleus decays; λ = 0.693/T.
- Ionisation
- Removing electrons from atoms, producing ions.
- Mass defect
- Difference between the total mass of separate nucleons and the mass of the nucleus.
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