Step 1: The nuclear density \( \rho \) is given by: \[ \rho = \frac{{Mass}}{{Volume}} = \frac{A}{\frac{4}{3} \pi R^3} \] where \( A \) is the mass number, and \( R \) is the radius of the nucleus.
The radius of the nucleus is related to the mass number \( A \) by the empirical relation: \[ R \propto A^{1/3} \]
Step 2: Therefore, the density is given by: \[ \rho \propto \frac{A}{R^3} \propto \frac{A}{(A^{1/3})^3} = \frac{A}{A} = 1 \]
Step 3: Hence, the ratio of the nuclear densities of the two nuclei will be \( 1:1 \).
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: