Our Nuclear Future: Facts, Dangers and Opportunities — John Shaqi
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
Living organisms breathe in carbon (in the form of carbon dioxide) from
the air. Most of this carbon is ordinary stable carbon¹²; a tiny
fraction is radioactive carbon¹⁴. The organism is unable to distinguish
between the two isotopes, and takes in carbon¹⁴ in the same ratio to
carbon¹² as exists in the atmosphere. This ratio persists throughout the
organism’s lifetime, but when the organism dies and no more carbon is
assimilated, the ratio begins to decrease as the carbon¹⁴ nuclei
gradually disintegrate. By observing the ratio of carbon¹⁴ to carbon¹²
in fossil remains and other archeological objects, the date at which
death occurred can be calculated. In this way the age of ancient
Egyptian mummies has been found, and it has been shown that some sequoia
wood is more than 1,500 years old. By measuring the carbon¹⁴ in trees
that were killed by the last advance of glaciation, and looking into
other remains of life from the last ice age, it has been possible to
show that this last ice age occurred only 10,000 years ago—instead of
20,000 years, as had been previously believed. Carbon¹⁴-dating has
therefore thoroughly revised our ideas about the rapidity with which the
empires known to history have emerged from the most primitive
conditions. A crucial part of the argument is that isotopes of the same
element are chemically indistinguishable.
An alternative reaction which may occur when neutrons strike nitrogen,
is
N¹⁴ + neutron → carbon¹² + H³
(7 protons) (6 protons) (1 proton)
(7 neutrons) (6 neutrons) (2 neutrons)
H³, triton, is also radioactive, undergoing a beta decay to become He³
(2 protons and 1 neutron) with a half-life of 12.25 years. Tritons too
can be used for dating old objects—for example, old wine. The water in
the wine cannot be replenished with cosmic-ray tritons after the wine
has been bottled. Thus fifty per cent of the tritons disappear every
12.25 years.
We have here two examples of nuclear reactions induced by neutron
bombardment. Recalling the disadvantages of charged particles as nuclear
projectiles for alchemists, it must surely seem that neutrons would be
ideal for this purpose. Being chargeless, they are neither electrically
repelled by the nuclei nor constantly slowed down by energy-losing
collisions with the electrons. The fate of almost every neutron moving
in a large piece of matter is eventual collision with a nucleus.[7]
Neutrons are ideal nuclear projectiles, except for one thing: they are
hard to get.
Protons and alpha particles are found abundantly in nature as the nuclei
of hydrogen and helium atoms. Neutrons, however, are not found in
nature, and in the past have been made in nuclear reactions that were
themselves initiated by charged particles. For example,
He⁴ + beryllium⁹ → C¹² + neutron
(2 protons) (4 protons) (6 protons)
(2 neutrons) (5 neutrons) (6 neutrons)
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