Several alpha-radioactive nuclides whose atomic numbers are less than 82 are found
in nature, though they are not very abundant.
The intermediate members of each decay series have much shorter half-lives than
their parent nuclide. As a result, if we start with a sample of NAnuclei of a parent
nuclide A, after a period of time an equilibrium situation will come about in which
each successive daughter B,C,... decays at the same rate as it is formed. Thus the
activities RA,RB,RC,... are all equal at equilibrium, and since R Nwe have
NAANBBNCC... (12.9)
Each number of atoms NA,NB,NC,... decreases exponentially with the decay con-
stant Aof the parent nuclide, but Eq. (12.9) remains valid at any time. Equation (12.9)
can be used to establish the decay constant (or half-life) of any member of the series
if the decay constant of another member and their relative proportions in a sample are
known.
Example 12.6
The atomic ratio between the uranium isotopes^238 U and^234 U in a mineral sample is found to
be 1.8 104. The half-life of^234 U is T 1 2 (234) 2.5 105 y. Find the half-life of^238 U.
Solution
Since T 1 2 0.693, from Eq. (12.9) we have
T 1 2 (238) T 1 2 (234)
(1.8 104 )(2.5 105 y)4.5 109 y
This method is convenient for finding the half-lives of very long-lived and very short-lived
radionuclides that are in equilibrium with other radionuclides whose half-lives are easier to measure.
12.4 ALPHA DECAY
Impossible in classical physics, it nevertheless occurs
Because the attractive forces between nucleons are of short range, the total binding
energy in a nucleus is approximately proportional to its mass number A, the number
of nucleons it contains. The repulsive electric forces between protons, however, are of
unlimited range, and the total disruptive energy in a nucleus is approximately
proportional to Z^2 [Eq. (11.12)]. Nuclei which contain 210 or more nucleons are so
large that the short-range nuclear forces that hold them together are barely able to
counterbalance the mutual repulsion of their protons. Alpha decay occurs in such nuclei
as a means of increasing their stability by reducing their size.
Why are alpha particles emitted rather than, say, individual protons or^32 He nuclei?
The answer follows from the high binding energy of the alpha particle. To escape from
a nucleus, a particle must have kinetic energy, and only the alpha-particle mass is
sufficiently smaller than that of its constituent nucleons for such energy to be available.
N(238)
N(234)
Radioactive
equilibrium
432 Chapter Twelve
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