To solve the problem, we need to understand why the binding energy per nucleon varies with the mass number of a nucleus.
- Binding energy per nucleon is the average energy that holds each nucleon (proton or neutron) together in the nucleus.
- It indicates the stability of a nucleus; higher values mean greater stability.
- When plotting binding energy per nucleon against mass number, the graph rises sharply for light nuclei, reaches a peak around iron (mass number ~56), and then gradually decreases for heavier nuclei.
- For small nuclei, adding more nucleons means more strong nuclear force interactions, which increases the binding energy per nucleon.
- The strong nuclear force is a short-range force attracting nucleons tightly together.
- As the nucleus gets larger, the size of the nucleus increases.
- Protons repel each other due to electrostatic (Coulomb) force, which acts over longer distances.
- The repulsive force among protons reduces overall binding energy per nucleon as the nucleus grows larger.
- Also, the strong nuclear force acts effectively only over short distances, so nucleons farther apart feel less attraction.
Binding energy per nucleon initially increases and then decreases with mass number because the size of the nucleus increases with mass number, leading to decreased binding energy per nucleon.
Mass Defect and Energy Released in the Fission of \( ^{235}_{92}\text{U} \)
When a neutron collides with \( ^{235}_{92}\text{U} \), the nucleus gives \( ^{140}_{54}\text{Xe} \) and \( ^{94}_{38}\text{Sr} \) as fission products, and two neutrons are ejected. Calculate the mass defect and the energy released (in MeV) in the process.
Given: