The stability of an atomic nucleus depends on its binding energy per nucleon, E. This energy represents the average energy that needs to be supplied to liberate a nucleon from the nucleus. One may visualize this qualitatively by imagining a well of potential energy, the depth of which represents E for a particular nucleus. Nuclei with deeper binding energy wells are more stable and occur at intermediate mass numbers. In the graph of E against mass number shown, 5626Fe has a value of E of 8.8 MeV and is one of the most stable of nuclides. There are three other nuclides, 42He, 126C, and 168O lying significantly above the main curve. Though these are not the most stable of all nuclides, they are considerably more stable than those of other nuclides of adjacent mass numbers. Nuclides of intermediate masses, such as iron, have the greatest values of E. Therefore if the conditions are right, there will be a tendency for nuclides of mass lower than iron to undergo fusion to enhance stability by acquiring a deeper E well. When nuclei heavier than iron undergo fission, energy is released which is equivalent to the difference in E of the parent and daughter nuclei (see also liquid-drop model; Q-value).
Nuclear stability
- radioisotope imaging
- radiolocation
- radiology
- radiolysis
- radiometric dating
- radionuclide
- radiosonde
- radiotherapy
- radiotransparent
- radium
- radius of curvature
- radius of gyration
- radius vector
- radon
- rainbow
- RAM
- Raman effect
- ramjet
- Ramsay, Sir William
- Ramsden eyepiece
- random alloy
- random walk
- Rankine cycle
- Rankine temperature scale
- Raoult's law