Binding Energy (AQA A Level Physics)

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Katie M

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Katie M

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Binding Energy per Nucleon Graph

  • In order to compare nuclear stability, it is useful to look at the binding energy per nucleon

  • The binding energy per nucleon is defined as:

    The binding energy of a nucleus divided by the number of nucleons in the nucleus

  • A higher binding energy per nucleon indicates a higher stability

  • In other words, more energy is required to separate the nucleons contained within a nucleus

By plotting a graph of binding energy per nucleon against nucleon number, the stability of elements can be inferred

Key Features of the Graph

  • At low values of A:

    • Nuclei have lower binding energies per nucleon than at large values of A, but they tend to be stable when N = Z

    • This means light nuclei have weaker electrostatic forces and will undergo fusion

    • The gradient is much steeper compared to the gradient at large values of A

    • This means that fusion reactions release a greater binding energy than fission reactions

  • At high values of A:

    • Nuclei have generally higher binding energies per nucleon, but this gradually decreases with A

    • This means the heaviest elements are the most unstable and will undergo fission

    • The gradient is less steep compared to the gradient at low values of A

    • This means that fission reactions release less binding energy than fission reactions

  • Iron (A = 56) has the highest binding energy per nucleon, which makes it the most stable of all the elements

  • Helium (4He), carbon (12C) and oxygen (16O) do not fit the trend

    • Helium-4 is a particularly stable nucleus hence it has a high binding energy per nucleon

    • Carbon-12 and oxygen-16 can be considered to be three and four helium nuclei, respectively, bound together

Comparing Fusion & Fission

Similarities

  • In both fusion and fission, the total mass of the products is slightly less than the total mass of the reactants

  • The mass defect is equivalent to the binding energy that is released

  • As a result, both fusion and fission reactions release energy

Differences

  • In fusion, two smaller nuclei combine into a larger nucleus

  • In fission, an unstable nucleus splits into two smaller nuclei

  • Fusion occurs between light nuclei (A < 56)

  • Fission occurs in heavy nuclei (A > 56)

  • In light nuclei, attractive nuclear forces dominate over repulsive electrostatic forces between protons, and this contributes to nuclear stability 

  • In heavy nuclei, repulsive electrostatic forces between protons begin to dominate over attractive nuclear forces, and this contributes to nuclear instability

  • Fusion releases much more energy per kg than fission

  • Fusion requires a greater initial input of energy than fission

Worked Example

The equation below represents one possible decay of the induced fission of a nucleus of uranium-235.

U presubscript 92 presuperscript 235 plus n presubscript 0 presuperscript 1 rightwards arrow S presubscript 38 presuperscript 91 r plus scriptbase X e end scriptbase presubscript 54 presuperscript 142 plus 3 n presubscript 0 presuperscript 1

The graph shows the binding energy per nucleon plotted against nucleon number A.

Worked Example - Binding Energy Graph, downloadable AS & A Level Physics revision notes

Calculate the energy released:

(a) By the fission process represented by the equation

(b) When 1.0 kg of uranium, containing 3% by mass of U-235, undergoes fission

Answer:

Part (a)

Step 1: Use the graph to identify each isotope’s binding energy per nucleon

8-4-4-worked-example---binding-energy-graph-ans-new
  • Binding energy per nucleon (U-235) = 7.5 MeV

  • Binding energy per nucleon (Sr-91) = 8.2 MeV

  • Binding energy per nucleon (Xe-142) = 8.7 MeV

Step 2: Determine the binding energy of each isotope

Binding energy = Binding Energy per Nucleon × Mass Number

  • Binding energy of U-235 nucleus = (235 × 7.5) = 1763 MeV

  • Binding energy of Sr-91 = (91 × 8.2) = 746 MeV

  • Binding energy of Xe-142 = (142 × 8.7) = 1235 MeV

Step 3: Calculate the energy released

Energy released = Binding energy after (Sr + Xe) – Binding energy before (U)

Energy released = (1235 + 746) – 1763 = 218 MeV

Part (b)

Step 1: Calculate the energy released by 1 mol of uranium-235

  • There are NA (Avogadro’s number) atoms in 1 mol of U-235, which is equal to a mass of 235 g

  • Energy released by 235 g of U-235 = (6 × 1023) × 218 MeV 

Step 2: Convert the energy released from MeV to J

  • 1 MeV = 1.6 × 10–13 J

  • Energy released = (6 × 1023) × 218 × (1.6 × 10–13) = 2.09 × 1013 J

Step 3: Work out the proportion of uranium-235 in the sample

  • 1 kg of uranium which is 3% U-235 contains 0.03 kg or 30 g of U-235

Step 4: Calculate the energy released by the sample

Energy released from 1 kg of Uranium = left parenthesis 2.09 space cross times space 10 to the power of 13 right parenthesis space cross times space 30 over 235 space equals space 2.67 space cross times space 10 to the power of 12 space straight J

Examiner Tips and Tricks

Checklist on what to include (and what not to include) in an exam question asking you to draw a graph of binding energy per nucleon against nucleon number:

  • You will be expected to draw the best fit curve AND a cross to show the anomaly that is helium

  • Do not begin your curve at A = 0, this is not a nucleus!

  • Make sure to correctly label both axes AND units for binding energy per nucleon

  • You will be expected to include numbers on the axes, mainly at the peak to show the position of iron (56Fe)

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Katie M

Author: Katie M

Expertise: Physics

Katie has always been passionate about the sciences, and completed a degree in Astrophysics at Sheffield University. She decided that she wanted to inspire other young people, so moved to Bristol to complete a PGCE in Secondary Science. She particularly loves creating fun and absorbing materials to help students achieve their exam potential.