Nuclear Physics Part 2 Flashcards
What is mass defect or mass difference?
The difference in mass between a nucleus and the mass of its constituent nucleons.
What is binding energy?
The energy needed to separate all of the nucleons in a nucleus.
How do you work out the average binding energy per nucleon?
Binding energy divided by nucleon number.
Describe the graph of Average Binding Energy Per Nucleon against Nucleon Number.
- Steep gradient starting at about 1 MeV/2 nucleons and peaking at 8.8 MeV/56 nucleon number
- Steady decrease after peak down to about 7.2 MeV/250 nucleons
What is the most stable nucleus?
Iron.
What is Fission?
When large nuclei are unstable and split into two smaller nuclei.
Why is energy released in Fission?
Because the new, smaller nuclei have a higher average binding energy per nucleon.
How can Fission be induced?
By making a neutron enter a Uranium-235 nucleus, causing it to become very unstable.
What is a low energy neutron called?
A thermal neutron.
What is Fusion?
When two light nuclei combine to create a larger nucleus.
Why is a lot of energy released in Fusion?
Because the new, heavier nuclei have a much higher average binding energy per nucleon.
Why is it so hard to fuse nuclei together and about how much kinetic energy is needed?
- Because all nuclei are positively charged therefore there will be an electrostatic force of repulsion between them
- About 1 MeV of kinetic energy needed to fuse nuclei together
How can you tell if it is energetically favourable for an element to undergo fission or fusion?
- By looking at the graph of average binding energy per nucleon against nucleon number
- Elements to the right of Iron can release energy through nuclear fission, and elements to the left of Iron can release energy through nuclear fusion
How can you work out the energy released through fusion or fission?
The change in binding energy gives the energy released.
What is another way of finding the energy released during fission or fusion other than using the graph?
Using E = Δmc ^ 2, where Δm is the total difference in mass between the initial and final nuclei (including neutrons).