All the atoms of a particular radioactive species have the same probability of disintegrating in a given time, so that an appreciable sample of radioactive material, containing many millions of atoms, always changes or disintegrates at the same rate. This rate at which the material changes is expressed in terms of the half-life, the time required for one half the atoms initially present to disintegrate, which is constant for any particular isotope.
Half-lives of radioactive materials range from fractions of a second for the most unstable to billions of years for those which are only slightly unstable. Decay is said to occur in the parent nucleus and produce a daughter nucleus. Decay from a parent to a daughter nucleus may produce alpha, beta particles, and neutrinos. Gamma radiation may be produced as the nucleus is de-excited but this is only after the alpha or beta decay has taken place. Radioactive decay results in a mass loss, which is converted to energy (the disintegration energy) according to the formula E = mc2. Often, the daughter nucleus is also radioactive, and so on down the line for several successive generations of nuclei until a stable one is finally reached. The three such naturally occurring series are shown in the following table:
Series | Starting Isotope | Half-Life (years) | Stable End Product |
---|---|---|---|
Radium | U-238 | 4.47x109 | Pb-206 |
Actinium | U-235 | 7.04x108 | Pb-207 |
Thorium | Th-232 | 1.41x1010 | Pb-208 |
Note: there are naturally occurring radioactive isotopes (such as C-14) but they are not part of a series.
Half life is also important in calculating populations, although it is only applicable where the resources available to the population remain surplus to the needs. In these situations the population and its demands increase rapidly, so in reality the resources are always a limiting factor.
See also: radioactive decay, nuclear fission, radiometric dating
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