By Fatskills Exam Guides Team — the exam nerds behind 28,500+ quizzes and 2.1M practice questions across 500+ global exams.
Complete Guide for GCSE/A-Level Students & Teachers
"Mastering binding energy, fusion/fission, and exponential decay doesn’t just explain how stars shine or how nuclear power works—it’s worth up to 15% of your GCSE/A-Level Physics exam and appears in every major paper (AQA, Edexcel, OCR). One wrong unit or misread graph, and you lose 3-4 marks instantly. This guide gives you the exact steps to solve any question—fast and error-free."
Before diving in, ensure you understand:1. Atomic structure – Protons, neutrons, nucleons, and mass number (A) vs. atomic number (Z).2. Energy-mass equivalence – Einstein’s E = mc² (energy = mass × speed of light²).3. Graph interpretation – Reading binding energy per nucleon curves and decay graphs.
(If any of these are shaky, pause and review them first—this topic builds on them!)
Formula: BE = Δm × c² - BE = Binding energy (J) - Δm = Mass defect (kg) = (Mass of nucleons) – (Mass of nucleus) - c = Speed of light (3 × 10⁸ m/s) → MEMORISE THIS
Alternative (for MeV): BE (MeV) = Δm (u) × 931.5 MeV/u - 1 atomic mass unit (u) = 1.66 × 10⁻²⁷ kg → MEMORISE THIS - 931.5 MeV/u → Given on exam sheet
Formula: N = N₀ e⁻ᶫᵗ - N = Number of undecayed nuclei at time t - N₀ = Initial number of nuclei - λ = Decay constant (s⁻¹) - t = Time (s) - e = Euler’s number (~2.718) → Given on exam sheet
Alternative (for half-life): λ = ln(2) / t₁/₂ - ln(2) ≈ 0.693 → MEMORISE THIS
Activity (A): A = λN - A = Activity (Bq) - λ = Decay constant (s⁻¹) - N = Number of undecayed nuclei
Formula: Energy released = BE of products – BE of reactants (If positive, energy is released; if negative, energy is absorbed.)
Step 1: Identify the nucleus and its nucleons. - Write down the mass number (A) and atomic number (Z). - Calculate total nucleons: A = protons + neutrons.
Step 2: Find the mass defect (Δm). - Look up the actual mass of the nucleus (given in the question or data sheet). - Calculate the total mass of individual nucleons: - Mass of protons = Z × mass of proton (1.00728 u) - Mass of neutrons = (A – Z) × mass of neutron (1.00867 u) - Δm = (Mass of nucleons) – (Mass of nucleus)
Step 3: Convert mass defect to energy. - If Δm is in kg, use BE = Δm × c². - If Δm is in u, use BE (MeV) = Δm × 931.5.
Step 4: Calculate binding energy per nucleon (if asked). - BE per nucleon = BE / A
Step 1: Write the nuclear equation. - Balance mass numbers (A) and atomic numbers (Z) on both sides.
Step 2: Find the binding energy of reactants and products. - Use the binding energy per nucleon curve (given in exams) or calculate from mass defect.
Step 3: Calculate energy released. - Energy released = BE of products – BE of reactants - If positive, energy is released (exothermic). - If negative, energy is absorbed (endothermic).
Step 4: Check units. - If BE is in MeV, answer in MeV. - If BE is in J, answer in J.
Step 1: Identify what’s given and what’s asked. - Given: N₀, t, λ, t₁/₂, or A - Asked: N, A, t, or λ
Step 2: Choose the right formula. - If half-life (t₁/₂) is given, use λ = ln(2) / t₁/₂. - If decay constant (λ) is given, use N = N₀ e⁻ᶫᵗ. - If activity (A) is asked, use A = λN.
Step 3: Plug in the numbers. - Use base-10 logs if e is not on your calculator (some exams allow 2⁻ᵗ/ᵗ¹/² instead). - For N = N₀ e⁻ᶫᵗ, take the natural log (ln) of both sides if solving for t or λ.
Step 4: Check units. - λ must be in s⁻¹ (if time is in seconds). - t must match the units of λ (e.g., if λ is in years⁻¹, t must be in years).
Question: Calculate the binding energy of a helium-4 nucleus (²⁴He) in MeV. Given: - Mass of helium-4 nucleus = 4.00150 u - Mass of proton = 1.00728 u - Mass of neutron = 1.00867 u
Step 1: Identify nucleons. - A = 4, Z = 2 - Protons = 2, Neutrons = 2
Step 2: Calculate mass defect (Δm). - Mass of nucleons = (2 × 1.00728) + (2 × 1.00867) = 4.03190 u - Δm = 4.03190 u – 4.00150 u = 0.03040 u
Step 3: Convert to energy. - BE = 0.03040 u × 931.5 MeV/u = 28.3 MeV
Step 4: Binding energy per nucleon. - BE per nucleon = 28.3 MeV / 4 = 7.08 MeV/nucleon
What we did and why: We found the mass defect (difference between nucleon mass and nucleus mass), then converted it to energy using E = mc² (via 931.5 MeV/u). This tells us how much energy holds the nucleus together.
Question: Calculate the energy released when two deuterium nuclei (²¹H) fuse to form helium-3 (³²He) and a neutron. Given: - Mass of deuterium (²¹H) = 2.01355 u - Mass of helium-3 (³²He) = 3.01493 u - Mass of neutron = 1.00867 u
Step 1: Write the nuclear equation. ²¹H + ²¹H → ³²He + ¹⁰n
Step 2: Calculate mass defect (Δm). - Mass of reactants = 2 × 2.01355 u = 4.02710 u - Mass of products = 3.01493 u + 1.00867 u = 4.02360 u - Δm = 4.02710 u – 4.02360 u = 0.00350 u
Step 3: Convert to energy. - Energy released = 0.00350 u × 931.5 MeV/u = 3.26 MeV
What we did and why: We compared the total mass before and after fusion. The mass lost (Δm) was converted to energy using E = mc². This is how stars (like the Sun) release energy!
Question: A sample of iodine-131 has an initial activity of 800 Bq. Its half-life is 8 days. a) Calculate the decay constant (λ). b) What will the activity be after 24 days?
Part a) Step 1: Use half-life to find λ. - λ = ln(2) / t₁/₂ - λ = 0.693 / (8 × 24 × 3600 s) = 1.00 × 10⁻⁶ s⁻¹
Part b) Step 1: Use exponential decay formula. - A = A₀ e⁻ᶫᵗ - t = 24 days = 24 × 24 × 3600 s = 2,073,600 s - A = 800 e⁻(1.00×10⁻⁶ × 2,073,600) - A = 800 e⁻².⁰⁷³⁶ ≈ 800 × 0.126 ≈ 101 Bq
Alternative (using half-lives): - 24 days = 3 half-lives (24 / 8 = 3) - A = A₀ × (1/2)³ = 800 × 1/8 = 100 Bq (slight rounding difference)
What we did and why: We used half-life to find λ, then applied the exponential decay formula to find activity after a given time. The alternative method (using half-lives directly) is faster in exams—always check if time is a multiple of half-life!
"Listen up—this is your last-minute nuclear physics cheat sheet.
Now go crush that exam—you’ve got this!"
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