aimnova.
DashboardMy LearningPaper MasteryStudy Plan

Stay in the loop

Study tips, product updates, and early access to new features.

aimnova.

AI-powered IB study platform with personalised plans, instant feedback, and examiner-style marking.

IB Subjects
  • All IB Subjects
  • IB Diploma
  • IB ESS
  • IB Economics
  • IB Business Management
  • IB Math AI
  • IB Math AA
  • IB Physics
  • IB Biology
  • IB Chemistry
  • IB History
  • IB History (2028+)
  • IB Global Politics
  • IB Psychology
  • IB Philosophy
  • IB Geography
  • IB Spanish B
  • IB German B
  • IB Italian B
  • IB French B
  • IB English B
  • IB English A Lang & Lit
  • IB Spanish A Lang & Lit
  • IB French A Lang & Lit
Question Banks
  • ESS Question Bank
  • Economics Question Bank
  • Business Management Question Bank
  • Math AI Question Bank
  • Math AA Question Bank
  • Physics Question Bank
  • Biology Question Bank
  • Chemistry Question Bank
  • History Question Bank
  • History (2028+) Question Bank
  • Global Politics Question Bank
  • Psychology Question Bank
  • Philosophy Question Bank
  • Geography Question Bank
  • Spanish B Question Bank
  • German B Question Bank
  • Italian B Question Bank
  • French B Question Bank
  • English B Question Bank
  • English A Lang & Lit Question Bank
  • Spanish A Lang & Lit Question Bank
  • French A Lang & Lit Question Bank
Predicted Topics 2026
  • ESS Predictions 2026
  • Economics Predictions 2026
  • Business Management Predictions 2026
  • Math AI Predictions 2026
  • Math AA Predictions 2026
  • Physics Predictions 2026
  • Geography Predictions 2026
  • Spanish B Predictions 2026
  • German B Predictions 2026
  • Italian B Predictions 2026
  • French B Predictions 2026
  • English B Predictions 2026

Study Resources

  • Free Study Notes
  • Mock Exams
  • Revision Guide
  • Flashcards
  • Exam Skills
  • Command Terms
  • Past Paper Feedback
  • Grade Calculator
  • Exam Timetable 2026

Company

  • Features
  • Pricing
  • About Us
  • Blog
  • Contact
  • Terms
  • Privacy
  • Cookies

© 2026 Aimnova. All rights reserved.

Made with 💜 for IB students worldwide

c059741
NotesPhysics HLTopic 5.3
Unit 5 · Nuclear and quantum physics · Topic 5.3

IB Physics HL — Radioactive decay

Topic 5.3 of IB Physics covers Radioactive decay, which is part of Unit 5: Nuclear and quantum physics. Students explore key concepts including Types of radiation and their properties, Decay equations and conservation laws, Energy released in radioactive decay, and more. A strong understanding of radioactive decay is essential for IB Physics HL exams and builds the foundation for connected topics across the syllabus.

Higher Level students should use this topic hub as a map: start with the shared sub-topics, then follow the HL-only extensions and exam-skill links where this topic asks for deeper analysis.

Exam technique guidePractice questions

Key concepts in Radioactive decay

Key Idea: An unstable nucleus calms down by throwing out radiation — and this topic is the four things the IB asks about that. What the radiation is and how it behaves (α, β⁻, γ); how to balance a decay equation so the new nucleus falls out; how much energy the decay releases through E = mc²; and how fast a source weakens, measured by its half-life. It is examined on both papers. Paper 1A is quick multiple-choice — identify a radiation from how it penetrates or deflects, pick the daughter's A and Z, or halve a count rate over a whole number of half-lives. Paper 2 is longer structured work — a show that the released energy is about 5 MeV from a mass defect, a show that the alpha carries about 98% of it, completing a nuclear equation, or correcting a count rate for background.

📋 Key formulas & rules

Only one equation in this topic carries the data-booklet badge — E = mc². Everything else is a rule you memorise: how A and Z change in each decay, and the halving rule for half-life. The exponential decay law A = A₀e⁻λᵗ is not on the SL booklet, so at SL you only ever halve over whole half-lives.

E=mc2E = mc^{2}E=mc2
Mass–energy equivalence (given in the data booklet, Theme E). Here m is the mass defect Δm and E is the energy released. Fast route in MeV: keep Δm in u and multiply by 931.5, since 1 u = 931.5 MeV c⁻².
EEE
energy released in the decay, the disintegration energy Q (J, or MeV)
mmm
mass defect Δm — the mass that disappears in the decay
ccc
speed of light, 3.00 × 10⁸ m s⁻¹ (given constant)
ZAX  ⟶  Z−2A−4Y  +  24α{}^{A}_{Z}X \;\longrightarrow\; {}^{A-4}_{Z-2}Y \;+\; {}^{4}_{2}\alphaZA​X⟶Z−2A−4​Y+24​α
Alpha decay — NOT printed in the booklet; memorise it. The daughter has 4 fewer nucleons and 2 fewer protons. Check: tops (A − 4) + 4 = A; bottoms (Z − 2) + 2 = Z. Balanced.
ZAX{}^{A}_{Z}XZA​X
parent nuclide before decay (A on top = protons + neutrons, Z below = protons)
Z−2A−4Y{}^{A-4}_{Z-2}YZ−2A−4​Y
daughter: nucleon number falls by 4, proton number by 2
24α{}^{4}_{2}\alpha24​α
alpha particle = a helium-4 nucleus (2 protons + 2 neutrons)
ZAX  ⟶  Z+1    AY  +  −1    0e  +  νˉ{}^{A}_{Z}X \;\longrightarrow\; {}^{\;\;A}_{Z+1}Y \;+\; {}^{\;\;0}_{-1}e \;+\; \bar{\nu}ZA​X⟶Z+1A​Y+−10​e+νˉ
Beta-minus decay — NOT in the booklet; memorise it. A neutron becomes a proton, so A is unchanged and Z rises by 1. The electron's −1 charge is what forces Z UP by one to keep the bottoms balanced.
ZAX{}^{A}_{Z}XZA​X
parent nuclide before decay
Z+1    AY{}^{\;\;A}_{Z+1}YZ+1A​Y
daughter: nucleon number unchanged, proton number rises by 1
−1    0e{}^{\;\;0}_{-1}e−10​e
beta-minus particle = an electron (made when a neutron becomes a proton)
νˉ\bar{\nu}νˉ
antineutrino — emitted with the electron (no charge, ≈ no mass)
A=A0(12)nA = A_{0}\left(\tfrac{1}{2}\right)^{n}A=A0​(21​)n
The halving rule for half-life — NOT a booklet equation. After n WHOLE half-lives the activity (or count rate) is the start value halved n times. Work out n = total time ÷ half-life first.
AAA
the activity (or count rate) after the time has passed
A0A_{0}A0​
the starting activity (or count rate)
nnn
the number of WHOLE half-lives that have passed, n = total time ÷ half-life
KEαKEtotal=mdmd+mα\frac{KE_{\alpha}}{KE_{\text{total}}} = \frac{m_{d}}{m_{d} + m_{\alpha}}KEtotal​KEα​​=md​+mα​md​​
Energy-sharing ratio — NOT printed; it comes from the parent being at rest (equal and opposite momentum) and KE = p²/2m. The LIGHT product (the alpha) takes the bigger share, close to but just under 100% for a heavy parent.
KEαKE_{\alpha}KEα​
kinetic energy carried by the alpha (the light product)
KEtotalKE_{\text{total}}KEtotal​
total energy released in the decay
mdm_{d}md​
mass of the daughter (the heavy product)
mαm_{\alpha}mα​
mass of the alpha (the light product)

☢️ The three radiations side by side

PropertyAlpha (α)Beta-minus (β⁻)Gamma (γ)
What it isA helium nucleus (2 p + 2 n), ⁴₂HeA fast electron from the nucleusA high-energy photon
Charge+2−10 (neutral)
PenetrationLowest — paper / a few cm of air / skinMedium — a few mm of aluminiumHighest — thick lead or concrete
Ionising powerStrongestMediumWeakest
Deflected by a field?Yes (small, +)Yes (large, opposite way, −)No (neutral)
Going α → β → γ: penetration goes UP (paper → aluminium → lead) and ionising power goes DOWN (α strongest → γ weakest). The best ioniser travels the shortest distance — α dumps its energy fastest, so it is stopped first. And only γ (neutral) is not bent by a field.

⚖️ How A and Z change in each decay

DecayWhat leaves the nucleusNucleon number AProton number Z
Alpha (α)a helium-4 nucleus (2 p + 2 n)falls by 4 (A → A − 4)falls by 2 (Z → Z − 2)
Beta-minus (β⁻)an electron + an antineutrinounchanged (A → A)rises by 1 (Z → Z + 1)
The top numbers add up the same on both sides (nucleon number A conserved), and the bottom numbers add up the same (proton number Z conserved). That single check finds the daughter every time. For a chain of two decays, apply the changes one at a time and keep a running tally; use N = A − Z if asked for neutrons.

📉 Half-life vs energy — the two calculations

Half-life / activityEnergy released
What it answersHow weak is the source after some time?How much energy does one decay give out?
Key relationshipA = A₀ × (½)ⁿ, with n = time ÷ half-lifeE = mc²; in MeV, Δm(u) × 931.5
First stepSubtract the background count rateFind the mass defect Δm = parent − total products
UnitsActivity in becquerel (Bq) = decays per secondEnergy in J or MeV (1 u = 931.5 MeV c⁻²)
Watch out forHALVE each half-life — don't subtract a fixed amountKeep ALL decimal places — Δm is a tiny number

✏️ Worked exam-style questions

IB-style questionState[3 marks]

An unknown radiation passes straight through a sheet of paper but is stopped by a 3 mm aluminium plate. When it crosses a magnetic field it is deflected. State which type of radiation it is, giving a reason from each observation.

🔒 Model answer plan

See the mark-by-mark plan — for / against / judgement, with marking guidance — in study mode.

Unlock free for 7 days →
IB-style questionDetermine[3 marks]

Radium-226 (A = 226, Z = 88) emits an alpha particle, and the nucleus it forms then emits a beta-minus particle. Find the nucleon number, proton number AND neutron number of the FINAL nuclide.

🔒 Model answer plan

See the mark-by-mark plan — for / against / judgement, with marking guidance — in study mode.

Unlock free for 7 days →
IB-style questionShow that[4 marks]

A nucleus at rest decays by alpha emission. The masses are: parent = 230.033130 u, daughter = 226.025410 u, alpha = 4.002600 u. (a) Show that the energy released is about 5 MeV. (b) The daughter has mass 226 u and the alpha 4 u — show that the alpha carries about 98% of that energy. (1 u = 931.5 MeV c⁻².)

🔒 Model answer plan

See the mark-by-mark plan — for / against / judgement, with marking guidance — in study mode.

Unlock free for 7 days →
IB-style questionDetermine[3 marks]

A detector near a fresh source reads 124 counts per second. With the source removed the background reads 4 counts per second. The source has a half-life of 15 minutes. Find the count rate the SAME detector reads after 30 minutes.

🔒 Model answer plan

See the mark-by-mark plan — for / against / judgement, with marking guidance — in study mode.

Unlock free for 7 days →

🧠 Quick self-check

Tap each card to reveal the answer.

Which radiation penetrates the FURTHEST, and which ionises the STRONGEST? Gamma (γ) penetrates furthest (needs thick lead); alpha (α) ionises the strongest (but is stopped by paper). Penetration and ionising power run in opposite orders.

In ALPHA decay, how do A and Z change? In BETA-MINUS? Alpha: A falls by 4, Z falls by 2. Beta-minus: A is unchanged, Z rises by 1 (a neutron becomes a proton, emitting an electron).

Why does the proton number RISE in beta-minus, not fall? The emitted electron has a bottom number of −1, so to keep the bottoms balanced the daughter's Z must be one MORE than the parent's. A neutron has turned into a proton.

Fast way to get the energy released in MeV from a mass defect? Find Δm in u (parent − total products), then multiply by 931.5 (since 1 u = 931.5 MeV c⁻²). The c² in E = mc² is already built into the 931.5.

Which decay product carries most of the energy, and why? The lighter one (the alpha). The parent is at rest, so the two products fly off with equal and opposite momentum; with KE = p²/2m, the smaller mass gets the bigger kinetic energy.

What must you do BEFORE halving a count rate over a half-life? Subtract the background count rate (true source rate = measured − background). Then halve the source rate once per half-life, and add the background back if the question wants the measured value.


🎯 Exam tips

Exam Tips

  • α → β → γ: penetration goes UP (paper → aluminium → lead) and ionising power goes DOWN (α strongest → γ weakest). Only γ (neutral) is not deflected by a field. To identify a radiation, use penetration to narrow it down, then deflection to confirm whether it is charged.
  • Most penetrating ≠ most dangerous. From OUTSIDE the body alpha is safe (the skin stops it) but gamma is the bigger hazard; INSIDE the body (breathed in/swallowed) alpha is the most dangerous because of its strong ionising power.
  • Every decay equation: the TOP numbers balance (nucleon number A conserved) and the BOTTOM numbers balance (proton number Z conserved). Alpha: A − 4, Z − 2. Beta-minus: A unchanged, Z + 1 — the electron's −1 charge forces Z UP, so never drop it.
  • For a decay CHAIN, apply each emission one at a time and keep a running tally of A and Z. Use N = A − Z if asked for the neutron number.
  • Energy released: find the mass defect FIRST (parent − total products), then E = mc². In MeV, just multiply Δm(in u) by 931.5. Keep every decimal place when subtracting masses — Δm is a tiny number and early rounding ruins it.
  • Energy sharing: the parent is at rest, so the products have equal and opposite momentum; with KE = p²/2m the LIGHT product (alpha) carries most of the energy. Its share = mdₐᵤgₕₜₑᵣ ÷ (mdₐᵤgₕₜₑᵣ + mₐₗₚₕₐ), close to but just under 100% for a heavy parent.
  • Half-life: ALWAYS subtract the background count rate before halving, then add it back if the question wants the measured value. Work out n = time ÷ half-life and multiply by (½)ⁿ — halve once per half-life, never subtract a fixed amount. Activity is in becquerel (Bq) = decays per second.
  • Two samples with the SAME half-life keep the same RATIO of activities over time, because both fall by the same factor (½)ⁿ.

What you'll learn in Topic 5.3

  • 5.3.1 Types of radiation and their properties
  • 5.3.2 Decay equations and conservation laws
  • 5.3.3 Energy released in radioactive decay
  • 5.3.4 Half-life, activity and background radiation
  • 5.3.5 Quantitative analysis of decay (HL)
Suggested study order: Read the notes for each sub-topic below → test yourself with flashcards → attempt practice questions → review exam technique.

Study resources — 5.3 Radioactive decay

5.3.1

Types of radiation and their properties

Notes
5.3.2

Decay equations and conservation laws

Notes
5.3.3

Energy released in radioactive decay

Notes
5.3.4

Half-life, activity and background radiation

Notes
5.3.5

Quantitative analysis of decay (HL)

Notes

Ready to study Radioactive decay?

Get expert practice questions with instant AI feedback, and a study planner tailored to your IB Physics HL exam date.

Start studying free

Topic 5.3 Radioactive decay forms a core part of Unit 5: Nuclear and quantum physics in IB Physics HL. Mastering these concepts will strengthen your understanding of connected topics across the syllabus and prepare you for exam questions that require analysis, evaluation, and real-world application.

Previous topic
5.2 Quantum physics (HL)
Next topic
5.4 Fission
All Physics HL topics
Exam technique

Ready to practice?

Get AI-graded practice questions, mock exams, flashcards, and a personalised study plan — all aligned to your IB syllabus.

Start Studying Free

No credit card required · Cancel anytime