Our Nuclear Future: Facts, Dangers and OpportunitiesTeller, Edward
Science
Our Nuclear Future: Facts, Dangers and Opportunities
Teller, Edward
Nuclear energy -- Popular works; Nuclear weapons; Radioactivity -- Physiological effect
Calcium⁴⁰ and argon⁴⁰ are both stable nuclei. The second reaction is
followed immediately by a gamma ray emission from the argon⁴⁰. The one
per cent of argon found in the earth’s atmosphere comes almost entirely
from the second reaction. These radioactivities are also interesting
because appreciable amounts of potassium⁴⁰ are always present in human
tissue.
All nuclei at the heavy end of the periodic system are radioactive alpha
emitters. Uranium, for example, has no stable isotopes; they all undergo
alpha decay. But there is another mode of spontaneous decay of uranium,
which is much less frequent than alpha decay but is of much greater
practical importance. This is the fission process.
The fission process is just like alpha decay in that the nucleus breaks
up into two fragments. The main difference between these processes is in
the relative weights of the fragments. In the alpha decay of U²³⁸, for
instance, one fragment has a weight of four and the other 234. In the
fission process the fragments tend to be more nearly equal in weight.
For example, one may weigh 90 and the other 148.[6] Other weight
combinations are also possible.
The explanation of spontaneous fission is in essence the same as that of
alpha decay. Spontaneous fission, however, is a less probable process
because the two fragments are more strongly bound to each other by the
nuclear forces than they are in alpha decay. More energy must be
borrowed, and it must be borrowed for a longer term in order to
penetrate the energy barrier.
The relative likelihoods of spontaneous fission and alpha decay can be
appreciated from the following fact. In one hour in a gram of U²³⁸ there
occur about 45 million alpha decays but only about 25 spontaneous
fissions.
Once the energy barrier has been overcome, the energy released in alpha
decay or spontaneous fission is proportional to the charges on the two
fragments. For alpha decay, the product of the charges is 2 × 90 = 180;
for spontaneous fission, this product will typically be about 40 × 52 =
2,080. Hence one might expect the fission energy release to be 10 to 15
times greater than the alpha energy release. As a matter of fact the
fission energy release is even greater than this estimate indicates,
being about 30 to 50 times greater than the alpha energy release. That
so large an amount of energy is released, is a very important feature of
the fission process from the point of view of practical utilization of
atomic energy.
Being at the end of the periodic system, uranium requires a large ratio
of neutrons to protons for its greatest stability. The fission
fragments, however, lie in the middle of the system of elements,
requiring a much smaller ratio of neutrons to protons for stability.
This has two consequences.
Public-domain text, read in full here on John Shaqi.
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