In simple terms
A friendly intro before the formal notes — no formulas yet.
Radioactive decay
Cambridge 9702 Paper 4 - Radioactive decay (23.2). Senpai Corner diagram-backed pilot with premium structure and live visuals.
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23.2 Radioactive decay.
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Radioactive decay is the spontaneous disintegration of a nucleus to form a more stable nucleus, resulting in the emission of an alpha, beta or gamma particles .
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Evidence for the random nature of radioactive decay can be seen from the fluctuations in the count rate of a Geiger-Muller counter.
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This proves that radioactive decay is both spontaneous and random .
What this topic covers
The official Cambridge syllabus points this lesson works through.
- 23.2.1
Understand that fluctuations in count rate provide evidence for the random nature of radioactive decay
- 23.2.2
Understand that radioactive decay is both spontaneous and random
- 23.2.3
Define activity and decay constant, and recall and use
- 23.2.4
Define half-life
- 23.2.5
Use
- 23.2.6
Understand the exponential nature of radioactive decay, and sketch and use the relationship , where x could represent activity, number of undecayed nuclei or received count rate
Explore the concept
Use the live diagram and synced steps — play it or tap a step card to walk through.
Decay curve N falls exponentially: the more nuclei remain, the faster the count drops.
8 more simulations for this topic — run them in the Simulations section below
Simulations
Every simulation here runs the real model — try the steps on a card, then check what you see against the notes.
8 simulations · 5 to start with
Start herein this order — each one shows a different piece of the topic
- PhETStart here · 1Java · best on a laptop9702 23.2 · IB E.3
Alpha Decay
Watch a polonium-211 nucleus, or a custom one, emit an alpha particle; the timing chart shows when each decay happens.
Why this one: Watch a bucket of nuclei decay at random while the chart shows half of them gone after each half-life.
Try this
- Reset and watch one nucleus — note how long it waits before decaying.
- Reset again — the wait is different each time.
- On the Multiple Nuclei screen, start 100 nuclei and read when half are gone.
Look for Decay is random for one nucleus but the half-life of a large sample is fixed.
Simulation by PhET Interactive Simulations, University of Colorado Boulder · Licensed to MarkScheme (public licence CC BY-NC 4.0 since 2026-03-30)
- PhETStart here · 2Java · best on a laptop9702 23.2
Radioactive Dating Game
Measure how much carbon-14 or uranium-238 is left in rocks, bones and other objects and read off their age from the decay curve.
Why this one: Read how much carbon-14 remains and use the decay curve to find an object's age.
Try this
- On the Half Life screen, start a batch of carbon-14 nuclei and read the time when half remain.
- On the Dating Game screen, probe a bone with the carbon-14 detector — read the percentage left and slide the age until the curve matches.
- Probe a rock with the uranium-238 detector instead — why is carbon-14 useless here?
Look for After n half-lives a fraction (½)ⁿ remains; choose an isotope whose half-life suits the age being measured.
Simulation by PhET Interactive Simulations, University of Colorado Boulder · Licensed to MarkScheme (public licence CC BY-NC 4.0 since 2026-03-30)
- PhETStart here · 3Java · best on a laptop9702 23.2 · 11.1–11.2 · IB E.3
Beta Decay
Watch hydrogen-3 or carbon-14 nuclei undergo beta decay, emitting an electron and an antineutrino, with half-life timing.
Why this one: Watch carbon-14 nuclei decay one by one and compare the timing with the half-life.
Try this
- Watch one hydrogen-3 nucleus decay — count the particles that leave.
- Switch to carbon-14 — it waits much longer on average.
- Start many nuclei and read the time when half have decayed.
Look for In β⁻ decay a neutron becomes a proton plus an electron and an antineutrino; Z rises by one.
Simulation by PhET Interactive Simulations, University of Colorado Boulder · Licensed to MarkScheme (public licence CC BY-NC 4.0 since 2026-03-30)
- 3JCN PhysicsStart here · 49702 23.2 · 9702 11.1 · IB E.3
Alpha Decay
Watch an alpha particle tunnel out of a heavy nucleus
Why this one: See what a single decay looks like: an alpha particle escaping a heavy nucleus.
Try this
- Watch the alpha particle tunnel out of the nucleus.
- Count the change in proton and nucleon numbers.
Look for The nucleus loses two protons and four nucleons.
3JCN Physics Simulation by Thomas Nguyen · CC BY 4.0
- SimuPhysicsStart here · 59702 23.2 · IB E.3
Probability Simulator
Run coin tosses in bulk and watch the experimental fraction close in on the theoretical value
Why this one: Toss many coins and watch the fraction settle — random events, predictable in bulk.
Try this
- Run 10 tosses and read the fraction.
- Run 1000 and compare.
- Run again and compare the two runs.
Look for The experimental fraction approaches the theoretical value as the number of trials grows.
Open on SimuPhysicsRuns on their siteSimuPhysics by Mohamed Abdelsalam · Licensed to MarkScheme (site publishes no licence; served with frame-ancestors self)
More simulations3 more on this topic — core ones first
- 3JCN PhysicsCore9702 23.2 · 9702 11.1 · IB E.3
Beta Decay
Watch a neutron become a proton with beta and antineutrino emission
Try this
- Watch the neutron become a proton.
- Identify the beta particle and the antineutrino.
Look for Nucleon number stays the same while proton number rises by one, with charge conserved.
3JCN Physics Simulation by Thomas Nguyen · CC BY 4.0
- 3JCN PhysicsCore9702 23.2 · 9702 11.1 · IB E.3
Gamma Decay
See an excited nucleus de-excite by emitting a gamma photon
Try this
- Watch the excited nucleus emit the gamma photon.
- Compare the nucleus before and after.
Look for Gamma emission changes neither proton nor nucleon number, only the energy of the nucleus.
3JCN Physics Simulation by Thomas Nguyen · CC BY 4.0
- PhET9702 11.1 · 23.2 · IB E.4
Build a Nucleus
Add protons and neutrons to a nucleus and watch which decays it undergoes.
Try this
- Build carbon-14 (6p, 8n) — the sim shows β⁻ decay; what does it become?
- Build a heavy nucleus like uranium-238 — watch the α decay and the new Z and A.
- On the “Chart”, trace a decay chain across the valley of stability.
Look for α: Z−2, A−4. β⁻: Z+1, A same. Too many neutrons → β⁻; too heavy → α.
Simulation by PhET Interactive Simulations, University of Colorado Boulder · Licensed to MarkScheme (public licence CC BY-NC 4.0 since 2026-03-30)
Key formulas
Tap any symbol to reveal exactly what it means and its units.
Tap a symbol — great for exam definitions
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Full topic notes
Formal explanation with the rigour you need for the exam.
The Nature of Radioactive Decay
Radioactive decay isn't something we can control or predict for a single nucleus. It possesses two crucial characteristics: it's spontaneous and random. This means it occurs without any external influence, such as changes in temperature or pressure, and we can't tell when a specific nucleus will decay. Evidence for this randomness comes from observing the count rate of a radioactive source with a Geiger-Muller tube; the readings fluctuate unpredictably around an average value, confirming that the decays are individual, random events.
23.2 Radioactive decay.
Radioactive decay is the spontaneous disintegration of a nucleus to form a more stable nucleus, resulting in the emission of an alpha, beta or gamma particles .
Evidence for the random nature of radioactive decay can be seen from the fluctuations in the count rate of a Geiger-Muller counter.
This proves that radioactive decay is both spontaneous and random .
The average decay rate (A) is the average number of nuclei which are expected to decay per unit overtime .
The decay constant is the probability that the nucleus will decay per unit time.
The Decay Constant (\lambda)
While individual decays are random, for a large sample, the overall rate of decay can be statistically predicted. The decay constant (symbol \lambda, pronounced 'lambda') helps us quantify this. It represents the probability that any single nucleus will decay per unit of time. A larger \lambda means a higher probability of decay and thus a less stable nucleus, leading to a shorter half-life. Conversely, a very small decay constant indicates a very stable isotope that decays slowly over a long period.
Definition: Probability of a single nucleus decaying per unit time.
Unit: Typically s^{-1} (per second) or year^{-1} (per year).
Higher \lambda means a shorter lifetime for the isotope.
Activity (A)
The activity of a radioactive sample measures how many nuclei are decaying per second. It's essentially the 'strength' of the radiation from a source. Since it's directly related to the decay constant and the number of undecayed nuclei, activity also decreases as the sample decays. While the SI unit is the Becquerel (Bq), an older, non-SI unit, the Curie (Ci), is sometimes encountered, where 1 Ci = 3.7 x 10¹⁰ Bq.
Activity, Where: = activity (Bq) = decay constant (s^{-1}) = number of undecayed nuclei
Definition: The rate at which nuclei decay in a radioactive sample.
SI Unit: The Becquerel (Bq), where 1 Bq = 1 decay per second (s^{-1}).
Activity is directly proportional to the number of undecayed nuclei present.
Exponential Decay and Decay Curves
The number of undecayed nuclei, and consequently the activity, in a radioactive sample decreases exponentially over time. This means that in equal time intervals, the same fraction of remaining nuclei will decay, not the same absolute number. When plotted on a graph of N or A against time, this relationship produces a characteristic exponential decay curve that starts at N₀ (or A₀) and asymptotically approaches zero but never quite reaches it. These exponential relationships are critical for calculations.
Number of undecayed nuclei: Activity: Where: = initial number of nuclei = initial activity = number of nuclei at time = activity at time = Euler's number (approx. 2.718)
Half-Life ($t_{1/2}$)
The half-life is a unique characteristic for each radioactive isotope. It's the time it takes for exactly half of the radioactive nuclei in a sample to decay. After one half-life, 50% of the original sample remains. After two half-lives, 25% (half of 50%) remains, and so on. Importantly, the half-life remains constant, regardless of the initial amount of the substance or its physical conditions.
Half-life and decay constant: Where: = half-life (s, min, hr, etc.) = decay constant (s^{-1}, min^{-1}, hr^{-1}, etc.)
Definition: Time for half of the nuclei in a sample to decay.
Constant: Unique for each isotope, independent of initial quantity.
After 'n' half-lives, the remaining fraction of nuclei (or activity) is .
Derivation of the Half-Life Formula
The relationship between half-life and the decay constant can be derived directly from the exponential decay equation. By definition, at the moment the time elapsed equals one half-life (), the number of remaining nuclei () will be exactly half of the initial number (). By substituting these conditions into the decay equation, we can isolate and solve for .
Start with the decay equation: Substitute and : Divide by : Take the natural logarithm (ln) of both sides: Using logarithm rules, and : Finally, rearrange for :
Worked examples
See the formulas applied — reveal one step at a time, like the exam.
A radioactive isotope has a decay constant of $2.5 \times 10^{-3}$ s^{-1}. Calculate its half-life in seconds. Then, if a sample initially has an activity of 480 Bq, what will its activity be after 5.0 minutes?
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Calculate the half-life ():
An ancient wooden artifact is found to have a carbon-14 activity of 0.180 Bq per gram of carbon. A modern, living sample of wood has an activity of 0.250 Bq per gram of carbon. Given that the half-life of carbon-14 is 5730 years, calculate the age of the artifact.
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Calculate the decay constant (\lambda):
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
Key terms for this topic — skim now; the Check step will test them.
- spontaneous
It possesses two crucial characteristics: it's spontaneous and random. This means it occurs without any external influence, such as changes in temperature or pressure, and we can't tell when a specific nucleus will decay.
- decay constant
The decay constant (symbol \lambda, pronounced 'lambda') helps us quantify this.
- activity
The activity of a radioactive sample measures how many nuclei are decaying per second. It's essentially the 'strength' of the radiation from a source.
- half-life
The half-life is a unique characteristic for each radioactive isotope.
Quick check
Write your answer first, then compare it with the model one — the gap is what you would have lost.
Teach it back
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Teach it back
Explain this topic as if teaching a friend. We name the gaps an examiner would still dock.
Revision flashcards
Guess first, then flip — retrieval beats re-reading.
Key takeaways
Review these before you close the topic — retrieval beats re-reading.
23.2 Radioactive decay.
Radioactive decay is the spontaneous disintegration of a nucleus to form a more stable nucleus, resulting in the emission of an alpha, beta or gamma particles .
Evidence for the random nature of radioactive decay can be seen from the fluctuations in the count rate of a Geiger-Muller counter.
This proves that radioactive decay is both spontaneous and random .
The average decay rate (A) is the average number of nuclei which are expected to decay per unit overtime .
The decay constant is the probability that the nucleus will decay per unit time.
Practice — then mark it
The whole point: a real Cambridge question, marked mark-by-mark.
State the names of the particles emitted as Q decays to form R.
This isotope of samarium is radioactive and decays by emitting particles. Gamma-radiation is not emitted. The energy spectrum of the emitted particles is shown in Fig. 6.1. Explain how Fig. 6.1 shows that this isotope of samarium emits α-particles and does not emit β-particles.
Extra simulations & links
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Frequently asked
Checkpoint
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Before you move on: do 9702/22 · Q6(b)(ii) on paper, snap a photo, and get examiner-style feedback on exactly where you win and lose marks.
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