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
The alpha particle needs some extra energy to escape. According to the
laws of older physics there is no possibility for it to obtain this
extra energy and therefore escape is impossible. But the more newly
discovered laws governing the motion of neutrons and protons (the laws
of quantum mechanics) are not so stringent; they permit the alpha
particle to use “borrowed” energy to overcome the energy barrier. Of
course the alpha particle must always repay the loan—which it can easily
do out of the large fund of electric energy that is released when it
gets out of the repulsive range of the residual nucleus. There is no
interest on the loan.
Such energy loans are not automatically granted in nature. There are two
factors which make the loan improbable: if the amount is big or if the
term is long. These restrictions effectively limit the particles which
may apply for an energy loan. Objects of great size and weight are
unable to qualify, but the small particles of the atomic world often do.
The more energy carried off by the alpha particle after the alpha decay,
the less energy must be borrowed in order to overcome the barrier, and
the more rapidly the decay may be expected to occur. So sensitive is the
decay to the energy of the alpha particle, that an alpha particle
carrying twice the energy is emitted a hundred trillion times fester.
Half-lives for alpha decay vary from a fraction of a second to billions
of years. But even the shortest half-life for alpha decay is remarkably
long compared to the time required for the alpha particle to cross the
nucleus. This means that the alpha particle makes a tremendous number of
attempts to escape from the nucleus before it actually succeeds.
According to the older classical theory the alpha process should never
occur, and in fact it occurs with a very small probability.
A single alpha decay is not usually a sufficient process to bring about
stability of the daughter nucleus. A whole chain of radioactive decays
is usually required before stability is achieved. Most nuclei which emit
alpha particles belong to one of these radioactive decay chains.
The heavy nuclei for which alpha decay occurs all contain a large excess
of neutrons. Since the alpha particle carries off exactly two neutrons
and two protons, the ratio of the number of neutrons to the number of
protons is increased in the daughter nucleus. This has an unstabilizing
influence. (Actually, in lighter nuclei stability requires that the
ratio of neutrons to protons be closer to unity.) The daughter nucleus
is thus apt to be beta-active, converting a neutron into a proton (plus
an electron and a neutrino) in order to decrease its ratio of neutrons
to protons. In this way a chain of radioactive decays may occur, more or
less alternating between alpha and beta emissions, with gamma rays being
occasionally emitted also.
Public-domain text, read in full here on John Shaqi.
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