Nuclear Binding Energy & Mass Deficit (Edexcel A Level Physics): Revision Note

Exam code: 9PH0

Katie M

Written by: Katie M

Reviewed by: Caroline Carroll

Updated on

Nuclear Binding Energy

  • Experiments into nuclear structure have found that the total mass of a nucleus is less than the sum of the masses of its constituent nucleons

    • This difference in mass is known as the mass defect or mass deficit

    • Mass defect is defined as:

      The difference between the measured mass of a nucleus and the sum total of the masses of its constituents

  • The mass defect Δm of a nucleus can be calculated using:

Δm = Zmp + (A  Z)mn  mtotal

  • Where:

    • Z = proton number

    • A = nucleon number

    • mp = mass of a proton (kg)

    • mn = mass of a neutron (kg)

    • mtotal = measured mass of the nucleus (kg)

Binding Energy, downloadable AS & A Level Physics revision notes

A system of separated nucleons has a greater mass than a system of bound nucleons

  • Due to mass-energy equivalence, this decrease in mass implies that energy is released

  • Energy and mass are proportional, so, the total energy of a nucleus is less than the sum of the energies of its constituent nucleons

  • Binding energy is defined as:

    The energy required to break a nucleus into its constituent protons and neutrons

  • The formation of a nucleus from a system of isolated protons and neutrons therefore releases energy, making it an exothermic reaction

    • This can be calculated using the equation:

ΔE = Δmc2

Mass-Energy Equivalence

  • Einstein showed in his Theory of Relativity that matter can be considered a form of energy and hence, he proposed:

    • Mass can be converted into energy

    • Energy can be converted into mass

  • This is known as mass-energy equivalence, and can be summarised by the equation:

ΔE = Δmc2

  • Where:

    • E = energy (J)

    • m = mass (kg)

    • c = the speed of light (m s-1)

  • Some examples of mass-energy equivalence are:

    • The fusion of hydrogen into helium in the centre of the sun

    • The fission of uranium in nuclear power plants

    • Nuclear weapons

    • High-energy particle collisions in particle accelerators

Worked Example

The binding energy per nucleon is 7.98 MeV for an atom of Oxygen-16 (16O).

Determine an approximate value for the energy required, in MeV, to completely separate the nucleons of this atom.

Answer:

Step 1: List the known quantities

  • Binding energy per nucleon, E = 7.98 MeV

Step 2: State the number of nucleons

  • The number of nucleons is 8 protons and 8 neutrons, therefore 16 nucleons in total

Step 3: Find the total binding energy

  • The binding energy for oxygen-16 is:

7.98 × 16 = 127.7 MeV

Step 4: State the final answer

  • The approximate total energy needed to completely separate this nucleus is 127.7 MeV

Examiner Tips and Tricks

Binding energy is named in a confusing way, so be careful!

Avoid describing the binding energy as the energy stored in the nucleus – this is not correct – it is energy that must be put into the nucleus to pull it apart.

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Katie M

Author: Katie M

Expertise: Curriculum Expert

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.

Caroline Carroll

Reviewer: Caroline Carroll

Expertise: Head of Content Delivery

Caroline graduated from the University of Nottingham with a degree in Chemistry and Molecular Physics. She spent several years working as an Industrial Chemist in the automotive industry before retraining to teach. Caroline has over 12 years of experience teaching GCSE and A-level chemistry and physics. She is passionate about delivering high-quality resources to help students achieve their full potential.