Understandings:
Nuclear fusion
- Light nuclei can undergo fusion reactions as this increases the binding energy per nucleon.
- Fusion reactions are a promising energy source as the fuel is inexpensive and abundant, and no radioactive waste is produced.
- Absorption spectra are used to analyse the composition of stars.
Nuclear fission
- Heavy nuclei can undergo fission reactions as this increases the binding energy per nucleon.
- 235U undergoes a fission chain reaction:
neutrons.
- The critical mass is the mass of fuel needed for the reaction to be self- sustaining.
- 239Pu, used as a fuel in “breeder reactors”, is produced from 238U by neutron capture.
- Radioactive waste may contain isotopes with long and short half-lives.
- Half-life is the time it takes for half the number of atoms to decay.
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International-mindedness:
- The use of nuclear energy is monitored internationally by the International Atomic Energy Agency.
- High-energy particle physics research involves international collaboration. There are accelerator facilities at CERN, DESY, SLAC, Fermi lab and Brookhaven. Results are disseminated and shared by scientists in many countries.
- The ITER project is a collaboration between many countries and aims to demonstrate that fusion is an energy source of the future.
Theory of knowledge:
- The use of nuclear energy carries risks as well as benefits. Who should ultimately be responsible for assessing these? How do we know what is best for society and the individual?
Utilization:
Syllabus and cross-curricular links:
Topic 2.1—isotopes
Topic 2.2—the emission spectrum of hydrogen
Physics topic 7.2—nuclear fusion
Aims:
- Aim 7: Computer animations and simulations of radioactive decay, and nuclear fusion and fission reactions.
- Aim 8: Consideration of the environmental impact of nuclear energy illustrating the implications of using science and technology.
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