Edexcel A-Level Physics 9PH0
Working as a Physicist
Mechanics
Electric Circuits
Materials
Waves and Particle Nature of Light
Further Mechanics
Electric and Magnetic Fields
Nuclear and Particle Physics
Thermodynamics
Space
Nuclear Radiation
Gravitational Fields
Oscillations
Nuclear Radiation
- 7 subtopics
- 11 things to know
- Papers 2 and 3
What Nuclear Radiation covers
Paper 2 content covering binding energy and the curve that explains both fission and fusion, the three types of nuclear radiation and how they are absorbed, nuclear equations, and the random, spontaneous nature of radioactive decay.
Where it is assessed
Papers 2 and 3
Advanced Physics II, then the general and practical principles paper.
Check the Pearson Edexcel specification ↗The 7 subtopics
Each one has its own page.
- Mass deficit, binding energy and the atomic mass unitRecall questions on binding energy and mass deficit, why a nucleus is lighter than its nucleons, ΔE = c²Δm, and the atomic mass unit in SI units, joules and MeV.Open →
- Binding energy per nucleon, fission and fusionRecall questions on why binding energy per nucleon measures stability, the shape of the curve and the nuclide at its peak, and why fusion needs high temperature and density.Open →
- Background radiation and the three types of nuclear radiationRecall questions on the sources of background radiation, correcting a count rate for it, and what alpha, beta-minus and gamma radiation are.Open →
- Ionising power, penetration and changes in the nucleusRecall questions on ranges and absorbers, the ranking for ionising ability and the link with penetration, deflection in an electric field, and how each decay changes the nucleus.Open →
- Nuclear equations and investigating gamma absorptionRecall questions on which quantities balance, writing alpha and beta-minus equations, the lead absorption experiment and its graph, and half-value thickness.Open →
- Activity, the decay constant and half-lifeRecall questions on decay being spontaneous and random, the definitions and units of activity and decay constant, and how λ = ln 2 / t½ follows.Open →
- Decay graphs and half-life calculationsRecall questions on the exponential equations and their logarithmic form, which graph gives the decay constant, reading a half-life from a curve, and why heating changes nothing.Open →
What you need to know
Answer each one before you reveal it.
What is the atomic mass unit in SI units, and how is binding energy per nucleon calculated for helium-4?
What is binding energy per nucleon, which nuclide sits at the peak of the curve, and what does fusion require and release?
What are an alpha particle and a beta-minus particle, and why is the background count measured over a long time?
Which quantities balance in a nuclear equation, how does gamma emission change a nucleus, and what is the equation for the alpha decay of uranium-238?
For carbon-14's beta-minus decay, give the nuclear equation, name what is emitted besides the electron, and say why the source–detector distance must stay constant.
How do the nucleon and proton numbers change in alpha decay, and how do alpha, beta and gamma rank for ionising ability?
What are the activity of a source and the decay constant, and what are their units?
What equation links activity to the decay constant and the number of undecayed nuclei, and what gives the activity after a time t?
What is the logarithmic form of the decay equation, and why is a mean of several half-life readings better than one?
What fraction of the original nuclei remains after 1.5 half-lives, and what happens to the half-life if the sample is heated strongly?
Take Nuclear Radiation further
The same content, four other ways.
Commonly confused
Pairs that lose marks when they are blurred together.
Activity vs Count rate
Activity: decays occurring per unit time. Count rate: detected events occurring per unit time.
Half-life vs Decay constant
Half-life: time for activity or undecayed nuclei to halve. Decay constant: probability of decay per nucleus per unit time.
Questions from this topic
Each one with the model answer underneath.
- 1
What is meant by the binding energy of a nucleus?
Model answer
It is the energy that must be supplied to separate a nucleus completely into its individual protons and neutrons.
- 2
What is the mass deficit of a nucleus?
Model answer
It is the difference between the total mass of the separate nucleons and the mass of the assembled nucleus.
- 3
Why is a nucleus always less massive than the nucleons it is made from?
Model answer
Energy is released when the nucleons bind together, and that release of energy corresponds to a loss of mass through ΔE = c²Δm.
- 4
State the equation linking a change in energy to the associated change in mass:
Model answer
ΔE = c²Δm, where c is the speed of light in a vacuum.
- 5
What value of the speed of light should be used in mass–energy calculations?
Model answer
The speed of light in a vacuum is 3.00 × 10⁸ m s⁻¹.
- 6
How is the atomic mass unit defined?
Model answer
One atomic mass unit is one twelfth of the mass of a neutral atom of carbon-12.
What is inside Levo
Six ways to work the same material.
Nuclear Radiation revision questions
- What does Nuclear Radiation cover in Edexcel A-Level Physics?
- 7 subtopics: mass deficit, binding energy and the atomic mass unit, binding energy per nucleon, fission and fusion, background radiation and the three types of nuclear radiation, ionising power, penetration and changes in the nucleus, nuclear equations and investigating gamma absorption, activity, the decay constant and half-life and decay graphs and half-life calculations. Each one has its own page with questions and model answers.
- How is Nuclear Radiation organised?
- By the Edexcel 9PH0 specification, subtopic by subtopic, so it matches the order you are taught it in.
Every question in Nuclear Radiation, on a schedule.
Attempt a question from memory, write the correct version, then attempt it again. Levo records the jump between your first attempt and your last, and brings each question back on the day you are due to forget it.
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