Binding Energy Per Nucleon And Nuclear Stability
Key idea: Interpret the binding energy per nucleon curve, identify stable nuclei near iron, and relate the curve to energy release in fusion and fission (A Level Physics).
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The core idea
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Learning objectives
- Relate binding energy per nucleon to fission, fusion, applications and hazards.
1. Definitions (Must Know)
A. Binding energy per nucleon
The binding energy per nucleon is: E_b/A where E_b is the total binding energy and A is the nucleon number.
It is a useful measure of stability: larger E_b/A generally means nucleons are more tightly bound.
2. Key Ideas (What Earns Marks)
- The curve of E_b/A vs A peaks around iron/nickel (A ≈ 56): these nuclei are among the most stable.
- Light nuclei (A small) can release energy by fusion (moving up the curve).
- Very heavy nuclei (A large) can release energy by fission (moving down towards the peak).
3. Detailed Explanations
A. How to read the curve
- If a reaction moves nuclei to a higher E_b/A, the products are more tightly bound.
- The difference in total binding energy appears as released energy (mainly kinetic energy and radiation).
B. Why fusion releases energy for light nuclei
For small A, the curve rises steeply. Combining two light nuclei to form a heavier nucleus closer to the peak increases E_b/A, so energy can be released.
C. Why fission releases energy for heavy nuclei
For very large A, splitting a heavy nucleus into two medium-mass nuclei moves the products closer to the peak (higher E_b/A), so energy can be released.
“Energy is released when the products have a higher binding energy per nucleon than the reactants.”
4. Common Mistakes
- Saying “fusion always releases energy” (it releases energy mainly when light nuclei fuse towards the peak).
- Confusing “binding energy per nucleon” with “binding energy” (total).
- Reading the curve backwards (remember: higher E_b/A means more stable).
5. Exam Tips
- If asked which process releases energy, compare where the nuclei sit on the E_b/A curve.
- Use “move towards the peak near iron” as the key reasoning.
- State what energy becomes: mainly kinetic energy of products and gamma radiation.
6. Worked Examples
Modelled example 1
Binding energy per nucleon calculation
Problem
Study the worked solution
Normalise the total
Method
Divide the whole-nucleus binding energy by its nucleon number.Reason
E_b/A is the average binding energy associated with each nucleon.Working
E_b/A = (1.20 × 10⁻¹⁰)/16Evaluate
Method
E_b/A = 7.50 × 10⁻¹² J per nucleon.Reason
The answer is an average energy, not the total binding energy.Working
E_b/A = 7.50 × 10⁻¹² J nucleon⁻¹
Guided practice 2
Fusion vs fission reasoning
Problem
Try this before viewing the solution
Hints
Hint 1: track the vertical movement
Hint 2: connect binding to release
View solution step by step
Read the light-nucleus region
Method
For small A, E_b/A rises steeply as nucleon number increases.Reason
The fused product lies closer to the curve’s peak.Working
light reactants → product with higher E_b/AInterpret the product
Method
The product’s nucleons are more tightly bound and its total binding energy is greater.Reason
Higher binding energy per nucleon across the same conserved nucleon total means greater total binding.Working
Δ E_b > 0State the energy outcome
Method
The increase in binding energy is released, mainly as kinetic energy and radiation.Reason
The more tightly bound products have lower total mass-energy.Working
lower product mass-energy → energy released
Common misconception 3
Which process releases energy? (given E_b/A)
Learner claim
Try this before viewing the solution
View solution step by step
Interpret higher binding
Method
The products are more tightly bound.Reason
Their binding energy per nucleon is higher by about 0.9 MeV.Working
8.5 > 7.6Correct the energy picture
Method
More tightly bound products have lower total mass-energy, not extra stored energy waiting to be supplied.Reason
Binding energy is the energy required to separate the bound system.Working
higher binding → lower bound-system mass-energyState the outcome
Method
Fission releases the mass-energy difference, mainly as fragment kinetic energy and radiation.Reason
The products move toward the iron-region peak.Working
reactants → more tightly bound products + released energy
Examiner practice 4
Energy release estimate from change in E_b/A
Examination question
Try this before viewing the solution
View solution step by step
Convert average increase to total
1 markMethod
Multiply the per-nucleon increase by the conserved nucleon total.Reason
All 240 nucleons contribute to the change in total binding energy.Working
Δ E ≈ A Δ(E_b/A)Evaluate
1 markMethod
Δ E ≈ 216 MeV.Reason
The increase in total binding energy appears as released energy.Working
Δ E ≈ 240(0.9) = 216 MeV
Self-mark with the mark scheme
Compare your response with each mark point. Select a point only when your response contains that evidence.
Self-mark the total-binding relation and energy estimate.
Challenge 5
Comparing stability (qualitative)
Independent transfer
Try this before viewing the solution
Hints
Hint 1: interpret the larger average
View solution step by step
Compare the values
Method
Nucleus X is more stable by binding energy per nucleon.Reason
8.7 MeV per nucleon exceeds 7.9 MeV per nucleon.Working
8.7 > 7.9Interpret physically
Method
On average, more energy per nucleon must be supplied to separate X completely.Reason
Its nucleons are more tightly bound.Working
higher E_b/A → greater average separation energy
7. Mind Stretchers
Mind stretcher 1: Why are very heavy nuclei less stable?Extension
Show Answer
For very large A, E_b/A is lower than near the peak, meaning nucleons are (on average) less tightly bound. That makes heavy nuclei more likely to release energy by splitting into more stable mid-mass nuclei.
Mind stretcher 2: Why doesn’t E_b/A keep increasing forever?Extension
The strong nuclear force is attractive, so why does binding energy per nucleon stop increasing and start decreasing for very heavy nuclei?
Show Answer
The strong nuclear force is short-range: each nucleon strongly binds only to nearby nucleons, so the “extra binding” gained by adding more nucleons eventually saturates.
However, electric repulsion between protons is long-range and increases as more protons are added. For very heavy nuclei, increasing Coulomb repulsion reduces stability, so E_b/A decreases.
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Course and syllabus information
- Course
- GCE A-Level H2 Physics
- Edition
- GCE A-Level H2 Physics 2027