The energy released in a nuclear reaction can be calculated using the mass defect. The mass defect is the difference in mass between the combined mass of the deuterons and the mass of the resulting helium nucleus. The energy corresponding to this mass defect is given by Einstein's equation:
\[
E = \Delta m \cdot c^2
\]
Where \( \Delta m \) is the mass defect, and \( c \) is the speed of light. First, calculate the mass defect:
\[
\Delta m = (2 \times \text{mass of deuteron}) - \text{mass of helium nucleus}
\]
\[
\Delta m = 2 \times 2.01355 \, \text{amu} - 4.0028 \, \text{amu} = 4.0271 \, \text{amu} - 4.0028 \, \text{amu} = 0.0243 \, \text{amu}
\]
Next, convert the mass defect to energy. 1 amu is equivalent to 931.5 MeV, so the energy released is:
\[
E = 0.0243 \, \text{amu} \times 931.5 \, \text{MeV/amu} = 22.62 \, \text{MeV}
\]
Thus, the energy released in the reaction is 22.62 MeV.