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
[Illustration: _USAEC—Argonne National Laboratory_
13. Cutaway section of a nuclear reactor. The heart of the reactor
is a small region at the center where the fission energy is
generated. Most of the weight and volume are needed for cooling
apparatus and shielding material to keep in nuclear radiation.]
For the radioactivity to affect areas at a large distance from the point
of the explosion, considerable time must elapse while the atomic cloud
rises and drifts in the horizontal winds. During this time more
disintegrations occur, due mainly to the short-lived nuclei. The rate at
which they occur keeps diminishing as the short-lived nuclei disappear.
Roughly speaking, the rate diminishes simply in proportion to the time.
More precisely, the rate drops somewhat faster, decreasing by a factor
of ten when the time increases by a factor of seven. A minute after the
explosion the activity is less than one per cent of what it is at a
second. After an hour it is less than one per cent of its value at a
minute. This law for the decrease in activity of fission products is, of
course, quite different from the simple law of radioactive decay. The
latter law applies to a single radioactive species. The fission products
consist at any instant of many different radioactive species. Each one
obeys the simple law of radioactive decay, but the totality follows a
different law.
It should be kept in mind that the product nucleus of a radioactive
disintegration may itself be radioactive with a different half-life. For
example, there is strontium⁹⁰. Only a small amount of this isotope is
made directly in the fission process. The fission process yields large
quantities of krypton⁹⁰, which decays with a half-life of one-half
minute into rubidium⁹⁰. The latter has a half-life of three minutes and
decays into strontium⁹⁰. This is how practically all of the strontium⁹⁰
is made in the explosion. Thus both the intensity and the nature of the
radioactivity keep changing with time.
These facts are important because they determine the magnitude and the
character of the danger when the radioactivity finally falls out of the
cloud and is deposited on the surface of the earth. Those radioactive
particles which disintegrate while still in the cloud need not worry us
since this radiation can have no effect on living organisms that may be
underneath. Provided that the cloud is more than a few hundred feet
above the ground, the beta and gamma rays released in these
disintegrations merely dissipate their energy in ionizing the air.
Public-domain text, read in full here on John Shaqi.
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