Nuclear Fusion and Nuclear Fission are two types of nuclear reactions:
- Nuclear Fusion is the process in which two light nuclei combine to form a heavier nucleus, releasing a large amount of energy. For example, in stars, hydrogen nuclei fuse to form helium, releasing energy.
- Nuclear Fission is the process in which a heavy nucleus splits into two or more lighter nuclei, accompanied by the release of energy. Fission is commonly used in nuclear reactors.
Energy Released in Nuclear Fusion Reaction:
The energy released in a nuclear reaction is given by the difference in mass between the reactants and products, multiplied by \( c^2 \) (where \( c \) is the speed of light). The mass defect (\( \Delta m \)) is the difference between the total mass of the reactants and the total mass of the products.
Step 1: Calculate the mass defect.
The total mass of the reactants is the sum of the masses of \( ^1\text{H}_2 \) and \( ^1\text{H}_3 \):
\[
m_{\text{reactants}} = m_{^1\text{H}_2} + m_{^1\text{H}_3} = 2.0141 + 3.0160 = 5.0301 \, \text{amu}
\]
The total mass of the products is the sum of the masses of \( ^2\text{He}_4 \) and \( ^1\text{n}^1 \):
\[
m_{\text{products}} = m_{^2\text{He}_4} + m_{^1\text{n}^1} = 4.0026 + 1.0087 = 5.0113 \, \text{amu}
\]
The mass defect \( \Delta m \) is:
\[
\Delta m = m_{\text{reactants}} - m_{\text{products}} = 5.0301 - 5.0113 = 0.0188 \, \text{amu}
\]
Step 2: Convert mass defect to energy.
Using the equivalence of mass and energy (\( E = \Delta m \times c^2 \)), and knowing that \( 1 \, \text{amu} = 931 \, \text{MeV}/c^2 \), the energy released \( Q \) is:
\[
Q = \Delta m \times 931 = 0.0188 \times 931 = 17.5 \, \text{MeV}
\]
Thus, the energy released in this nuclear fusion reaction is \( Q = 17.5 \, \text{MeV} \).