Nuclear Fusion (Edexcel IAL Physics)
Spec point —
135
Nuclear Fusion
- Fusion is defined as:
Small nuclides that combine together to make larger nuclei, releasing energy
- Low mass nuclei, such as hydrogen and helium, can undergo fusion and release energy
- On Earth, research is focused on achieving the deuterium-tritium (D-T) reaction
- This involves fusing a deuterium nucleus and a tritium nucleus together to produce a helium nucleus and a neutron
H _ 1 ^ 2 + H _ 1 ^ 3 -> He _ 2 ^ 4 + n _ 0 ^ 1
Deuterium-tritium fusion

The fusion of deuterium and tritium nuclei to form a helium nucleus and a neutron, with the release of energy
Conditions for nuclear fusion
-
For two nuclei to fuse, both nuclei must have high kinetic energy
-
This is because nuclei must be able to get close enough to fuse
-
However, two forces acting within the nuclei make this difficult to achieve
-
Electrostatic repulsion
- Protons inside the nuclei are positively charged, which means that they electrostatically repel one another
-
Strong nuclear force
- The strong nuclear force, which binds nucleons together, acts at very short distances within nuclei
- Therefore, nuclei must get very close together for the strong nuclear force to take effect
-
-
It takes a great deal of energy to overcome the electrostatic force, hence, fusion can only be achieved in an extremely hot, dense environment, such as the core of a star
Fusion products
-
When two hydrogen nuclei (protons) fuse, a deuterium nucleus is produced
- A positron and an electron neutrino are also produced as one of the protons converts into a neutron through beta-plus decay
H _ 1 ^ 1 + H _ 1 ^ 1 -> H _ 1 ^ 2 + e ^ + + nu _ e
-
In the centres of stars, four hydrogen nuclei
( H _ 1 ^ 1 )fuse to produce a helium nucleus , plus the release of energy- This provides fuel for the star to continue burning
The proton-proton chain

The proton-proton chain involves a series of nuclear reactions which produces a helium nucleus from the fusion of four protons
Exam Hint In the fusion process, the mass of the new, heavier nucleus is less than the mass of the constituent parts of the nuclei fused together, as some mass is converted into energy.
Not all of this energy is used as binding energy for the new, larger nucleus, so energy will be released from this reaction. The binding energy per nucleon afterwards is higher than at the start.
Was this revision note helpful?
Build on this topic