The key concept behind the release of energy in fusion (and fission) reactions is binding energy. Binding energy is the energy that is lost when a nucleus is created from protons and neutrons. If you added up the total mass of the nucleons (protons and neutrons) that compose an atom, you would notice that this sum is less than the actual mass of the atom. This missing mass, called the mass defect, is a measure of the atom’s binding energy. It is released during the formation of a nucleus from the composing nucleons. This energy would have to be put back into the nucleus in order to decompose it into its individual nucleons. The greater the binding energy per nucleon in the atom, the greater the atom’s stability. To calculate the binding energy of a nucleus, all you have to do is sum the mass of the individual nucleons, and then subtract the mass of the atom itself. The mass leftover is then converted into its energy equivalent. The relation between mass and energy is shown in Einstein’s famous equation E = mc2. However, we will just multiply the mass by a conversion factor to have the units of energy in millions of electron volts (MeV), a standard unit of energy in nuclear physics. Therefore, the equation for binding energy that you can use later is: Eb = (Z × mH + N × mn – misotope) × 931.5 MeV/amu Eb = binding energy, in MeV Z = number of protons mH = mass of a hydrogen atom (1.007825 atomic mass units, or amu) N = number of neutrons mn = mass of a neutron (1.008664904 amu) misotope = actual mass of the isotope 931.5 Mev/amu = the conversion factor to convert mass into energy, in units of MeV....
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