The binding energy of a nucleus is defined as the energy required to disassemble the nucleus into its constituent protons and neutrons. In simpler terms, it is the energy released when a nucleus is formed from its individual nucleons.
To calculate the energy released during the nuclear reaction, we use the mass-energy equivalence formula:
\[
E = \Delta m . c^2
\]
Where:
- \( \Delta m \) is the mass defect (the difference between the mass of the reactants and products),
- \( c \) is the speed of light (\( c = 3 \times 10^8 \, \text{m/s} \)).
Step 1: Calculate the mass defect (\(\Delta m\))
The mass defect is the difference between the total mass of the reactants and the total mass of the products:
\[
\Delta m = \left( \text{Mass of reactants} \right) - \left( \text{Mass of products} \right)
\]
For the reaction \( \ ^3Li^6 + \ ^0n^1 \longrightarrow \ ^2He^4 + \ ^1H^3 \), the mass defect is:
\[
\Delta m = \left( 6.015126 + 1.008665 \right) - \left( 4.002604 + 3.016049 \right)
\]
\[
\Delta m = 7.023791 - 7.018653 = 0.005138~\text{u}
\]
Step 2: Convert the mass defect into energy
To convert the mass defect into energy, we use the formula \( E = \Delta m . c^2 \). First, we need to convert the mass defect into kilograms:
\[
1~\text{u} = 1.660539 \times 10^{-27}~\text{kg}
\]
\[
\Delta m = 0.005138~\text{u} \times 1.660539 \times 10^{-27}~\text{kg/u}
\]
\[
\Delta m = 8.526 \times 10^{-30}~\text{kg}
\]
Now, applying Einstein's equation:
\[
E = \Delta m . c^2 = 8.526 \times 10^{-30} . (3 \times 10^8)^2
\]
\[
E = 8.526 \times 10^{-30} . 9 \times 10^{16} = 7.673 \times 10^{-13}~\text{J}
\]
So, the energy released in the reaction is:
\[
E = 7.673 \times 10^{-13}~\text{J}
\]