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Binding Energy per Nucleon Curve (HL IB Physics)

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Katie M

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Katie M

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Binding Energy per Nucleon Curve

  • 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

Exam Tip

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:

  • 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)

The Strong Nuclear Force

  • In the nucleus, there are electrostatic forces between the protons due to their electric charge and gravitational forces due to their mass
  • Comparatively, gravity is a very weak force and the electrostatic repulsion between protons is therefore much stronger than their gravitational attraction
  • If these were the only forces, the nucleus wouldn’t hold together
  • Therefore, the force that does hold the nucleus together is called the strong nuclear force
  • The strong nuclear force keeps the nucleus stable since it holds quarks together
  • Since protons and neutrons are made up of quarks, the strong force keeps them bound within a nucleus

2.1.3Electrostatic-vs-Strong-Nuclear

Whilst the electrostatic force is a repulsive force in the nucleus, the strong nuclear force holds the nucleus together

Range of the Strong Nuclear Force

  • The strength of the strong nuclear force between two nucleons varies with the separation between them
  • This can be plotted on a graph which shows how the force changes with separation

2.1.3Strong-Nuclear-Force-Graph

The strong nuclear force is repulsive before a separation of ~ 0.5 fm and attractive up till ~ 3.0 fm

  • The key features of this graph are that the strong nuclear force is:
    • Repulsive closer than around 0.5 fm (femtometres, 10-15 m)
    • Attractive up to around 3.0 fm
    • Reaches a maximum attractive value at around 1.0 fm (the typical nuclear separation)
    • Becomes zero after 3.0 fm
  • In comparison to other fundamental forces, the strong force has a very small range (only up to 3.0 fm)

Exam Tip

  • You may see the strong nuclear force also referred to as the strong interaction
  • Remember to write that after 3 fm, the strong force becomes 'zero' or 'has no effect' rather than it is ‘negligible’.
  • Recall that 1 fm = 1 × 10–15 m

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Katie M

Author: Katie M

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.

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