Written by IGCSEPhysics Content Team · Physics subject adviser: K. S. Tan, 15+ years teaching IGCSE Physics · Checked against the Cambridge IGCSE Physics (0625) 2026 to 2028 syllabus
Topic 5 is one of the shorter topics but is conceptually demanding. Students who understand the particle model and nuclear notation tend to find it straightforward.
What Topic 5 covers
- The nuclear model of the atom (protons, neutrons, electrons, isotopes, Rutherford scattering)
- Radioactivity (alpha, beta, gamma; properties, detection, background radiation)
- Half-life (definition, calculations, graphical determination)
- Nuclear reactions (fission, fusion, nuclear equations)
Priority areas
Must-know facts
- Proton: charge +1, mass 1, in nucleus
- Neutron: charge 0, mass 1, in nucleus
- Electron: charge -1, mass 1/1836, orbiting nucleus
- Atomic (proton) number Z = number of protons
- Mass (nucleon) number A = protons + neutrons
- Isotopes: same Z, different A
Must-know radiation properties
| Property | Alpha | Beta | Gamma |
|---|---|---|---|
| Identity | Helium nucleus (2p + 2n) | High-speed electron | EM wave |
| Charge | +2 | -1 | 0 |
| Mass | 4 | ~0 | 0 |
| Penetration | Stopped by paper | Stopped by aluminium (~5 mm) | Reduced by thick lead or concrete |
| Ionising ability | Strongest | Moderate | Weakest |
| Deflection in fields | Deflected (toward negative plate) | Deflected (toward positive plate) | Not deflected |
Must-know calculations
- Half-life from a decay graph or table
- Remaining activity or mass after n half-lives: N = N0 x (1/2)^n
- Nuclear equations balancing (conserve mass number and atomic number)
Must-know concepts
- Why radioactive decay is random and spontaneous (cannot be predicted or controlled)
- Sources of background radiation (cosmic rays, rocks, medical, food, radon gas)
- Why background count must be subtracted from measured count
- The difference between irradiation and contamination
- Safety precautions for handling radioactive sources
- How fission produces a chain reaction (neutrons released hit more nuclei)
- How fusion requires extremely high temperatures (to overcome electrostatic repulsion)
Revision strategy for Topic 5
2-day intensive plan
- Day 1: Atomic structure (learn nuclear notation, isotopes, Rutherford scattering experiment and its conclusions). Radiation types (learn the table above, practise comparing alpha, beta and gamma). Nuclear equations.
- Day 2: Half-life (definition, graph reading, calculations). Fission and fusion (describe each, compare, explain why fusion is difficult). Safety and applications. Past paper questions.
Common mistakes in Topic 5
- Confusing atomic number with mass number.
- Saying alpha radiation is “absorbed” by paper (it is stopped or blocked, not absorbed in the physics sense).
- Writing unbalanced nuclear equations (always check that mass numbers and atomic numbers balance).
- Confusing fission and fusion (fission splits large nuclei; fusion joins small nuclei).
- Saying half-life means “half the radiation is gone” (it means half the unstable nuclei have decayed, or the activity has halved).
- Not subtracting background radiation when analysing experimental data.
Self-test checklist
After revision, you should be able to:
- State the properties of protons, neutrons and electrons.
- Define isotope and give an example.
- Compare alpha, beta and gamma radiation.
- Read half-life from a graph or table.
- Calculate remaining activity after multiple half-lives.
- Write and balance nuclear equations.
- Describe fission and fusion and their differences.
- State safety precautions for handling radioactive sources.
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