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First teaching 2023

First exams 2025

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Calculating Energy Released in Nuclear Reactions (CIE A Level Physics)

Revision Note

Leander

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Leander

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Calculating energy released in nuclear reactions

  • The binding energy is equal to the amount of energy released in forming the nucleus, and can be calculated using:

E = (Δm)c2

  • Where:
    • E = Binding energy released (J)
    • Δm = mass defect (kg)
    • c = speed of light (m s-1)
  • The daughter nuclei produced as a result of both fission and fusion have a higher binding energy per nucleon than the parent nuclei
  • Therefore, energy is released as a result of the mass difference between the parent nuclei and the daughter nuclei

Worked example

When uranium-235 nuclei undergo fission by absorbing slow-moving neutrons, two reactions are possible:

Reaction space 1 colon space straight U presubscript 92 presuperscript 235 space plus space straight n presubscript 0 presuperscript 1 space rightwards arrow space Xe presubscript 54 presuperscript 139 space plus space Sr presubscript 38 presuperscript 95 space plus space 2 straight n presubscript 0 presuperscript 1 space plus space energy

Reaction space 2 colon space straight U presubscript 92 presuperscript 235 space plus space straight n presubscript 0 presuperscript 1 space rightwards arrow space 2 Pd presubscript 46 presuperscript 116 space plus space x straight c space plus space energy

(a)
For reaction 2, identify the particle c, and state the number, x, of such particles produced in the reaction.
(b)
The binding energy per nucleon, E, for a number of nuclides is given by the table below. Use the table to show that the energy  produced in reaction 1 is about 210 MeV.
(c)
The energy produced in reaction 2 is 163 MeV. Suggest, with supporting reason, which one of the two reactions is more likely to happen.

nuclide E / MeV
Sr presubscript 38 presuperscript 95 8.74
Xe presubscript 54 presuperscript 139 8.39
straight U presubscript 92 presuperscript 235 7.60

Answer:

Part (a)

Step 1:  Balance the number of protons on each side (bottom number)

92 = (2 × 46) + xnp (where np is the number of protons in c)

xnp = 92 – 92 = 0

Therefore, c must be a neutron

Step 2: Balance the number of nucleons on each side

235 + 1 = (2 × 116) + x

x = 235 + 1 – 232 = 4

  • Therefore, 4 neutrons are generated in the reaction

Part (b)

Step 1: Find the binding energy of each nucleus

Total binding energy of each nucleus = Binding energy per nucleon × Mass number

Binding energy of 95Sr = 8.74 × 95 = 830.3 MeV

Binding energy of 139Xe = 8.39 × 139 = 1166.21 MeV

Binding energy of 235U = 7.60 × 235 = 1786 MeV

Step 2: Calculate the difference in energy between the products and reactants

Energy released in reaction 1 = ESr + EXe – EU

Energy released in reaction 1 = 830.3 + 1166.21 – 1786

Energy released in reaction 1 = 210.5 MeV

Part (c)

  • Since reaction 1 releases more energy than reaction 2, its end products will have a higher binding energy per nucleon
    • Hence they will be more stable
  • This is because the more energy is released, the further it moves up the graph of binding energy per nucleon against nucleon number (A)
    • Since at high values of A, the binding energy per nucleon gradually decreases with A
  • Nuclear reactions will tend to favour the more stable route, therefore, reaction 1 is more likely to happen

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Leander

Author: Leander

Expertise: Physics

Leander graduated with First-class honours in Science and Education from Sheffield Hallam University. She won the prestigious Lord Robert Winston Solomon Lipson Prize in recognition of her dedication to science and teaching excellence. After teaching and tutoring both science and maths students, Leander now brings this passion for helping young people reach their potential to her work at SME.