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A nucleus is specified by its number of protons Z, number of neutrons N, and the mass number A = Z+N. The nucleons (protons and neutrons) in a nucleus are bound together -- their total energy is less than the total energy of the separated particles. The binding energy is the amount of energy given up when the nucleus is formed. Plotting the binding energy per nucleon versus the mass number A (Figure 14-01) shows that starting from Hydrogen, nuclei become more stable as there are more protons and neutrons, until Iron. After that, the trend reverses. |
Figure 14-01 Nuclear Binding Energy [view large image] |
Figure 14-02 Proton/Neutron & Decay [view large image] |
Note : binding energy = - potential energy (see "Energy of A Particle") |
c, where the fine structure constant
= 1/137. Thus, the number of protons Z in the nucleus cannot excess 137 or the velocity would be greater than the speed of light in violation of special relativity. Under the more sophisticated Dirac equation, the limit of Z is 173 imposed by the rising of binding energy up to pairs creation, which renders the atom unstable. The heaviest nucleus to have been identified experimentally has Z = 118.