Nuclear fusion is the process where two nuclei with a lower binding energy per nucleon merge to create a nucleus with a higher binding energy per nucleon.
During nuclear fusion, two light atomic nuclei, such as hydrogen isotopes like deuterium and tritium, combine to form a heavier nucleus, for example, helium. This process is characterized by the resulting nucleus possessing a greater binding energy per nucleon than the original nuclei, indicating increased nuclear stability post-fusion.
For elements lighter than iron, which have comparatively lower binding energies per nucleon, fusion occurs because the resulting heavier nucleus achieves a higher binding energy per nucleon. This energy release makes the fusion process energetically favorable.
The nuclear reaction involving the formation of a nucleus with greater binding energy per nucleon from two nuclei with lower binding energy per nucleon is termed nuclear fusion.
Assuming the experimental mass of \( {}^{12}_{6}\text{C} \) as 12 u, the mass defect of \( {}^{12}_{6}\text{C} \) atom is____MeV/\( c^2 \).
(Mass of proton = 1.00727 u, mass of neutron = 1.00866 u, 1 u = 931.5 MeV/\( c^2 \))
The binding energy per nucleon of \(^{209} \text{Bi}\) is _______ MeV. \[ \text{Take } m(^{209} \text{Bi}) = 208.98038 \, \text{u}, \, m_p = 1.007825 \, \text{u}, \, m_n = 1.008665 \, \text{u}, \, 1 \, \text{u} = 931 \, \text{MeV}/c^2. \]