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As discussed previously,
American scientists' concerns about the uses Adolf Hitler might make
of the German discovery of fission in December 1939 led to
investigations of nuclear energy production in the United States.
Fission, in which a slow neutron splits a heavy atom into two atoms of
approximately half the weight of the original, released tremendous
amounts of energy that might be used in a power-producing pile (a
reactor) or a bomb
By the time the United States entered World War II
in December 1941, several projects were under way to investigate the
separation of fissionable uranium 235 from uranium 238, the
manufacture of plutonium, and the feasibility of nuclear piles and
explosions.
Physicist and Nobel laureate Arthur Holly Compton
organized the Metallurgical Laboratory at the University of Chicago in
early 1942 to study plutonium and fission piles. Compton asked
theoretical physicist J. Robert Oppenheimer of the University of
California to study the feasibility of a nuclear weapon.
In the spring of 1942, Oppenheimer and his former
postdoctoral student, Robert Serber of the University of Illinois,
worked with Oppenheimer's students Eldred Nelson and Stan Frankel on
the problems of neutron diffusion (how neutrons moved in the chain
reaction) and hydrodynamics (how the explosion produced by the chain
reaction might behave).
To review this work and the general theory of
fission reactions, Oppenheimer convened a summer study at the
University of California-Berkeley in June 1942. Theorists Hans Bethe,
John Van Vleck, Edward Teller, Felix Bloch, Richard Tolman and Emil
Konopinski concluded that a fission bomb was feasible.
The chief uncertainties lay in the experimental
values for neutron cross-sections -the probabilities that neutrons
would strike a fissionable atom and either cause it to fission, be
absorbed or be scattered -and neutron multiplication -the numbers of
neutrons that would be produced in fission and cause other atoms to
fission in a rapid chain reaction.
The scientists suggested that such a reaction could
be initiated by assembling a critical mass -an amount of nuclear
explosive adequate to sustain it - either by firing two subcritical
masses of plutonium or uranium 235 together or by imploding (crushing)
a hollow sphere made of these materials with a blanket of high
explosives. Until the numbers were better known, this was all that
could be done. "Everyone seemed to be saying, well, that's all
settled, let's talk about something interesting," Serber recalled.
Teller saw another possibility: By surrounding a
fission bomb with deuterium and tritium, a much more powerful "superbomb"
might be constructed. This concept was based on studies made by Bethe
before the war of energy production in stars. When the detonation wave
from the fission bomb moved through the mixture of deuterium and
tritium nuclei, they would fuse together to produce much more energy
than fission, just as elements fused in the sun produce light and
heat.
Bethe was skeptical, and as Teller proposed scheme
after scheme for a "superbomb," Bethe refuted each one. When Teller
raised the possibility that an atomic bomb might ignite the
atmosphere, however, he kindled a worry that was not entirely
extinguished until the Trinity test, even though Bethe showed,
theoretically, that it couldn't happen.
The summer conferences, the results of which were
later summarized by Serber in "The Los Alamos Primer" (LA-1), provided
the theoretical basis for the design of the atomic bomb, which was to
become the principal task at Los Alamos during the war, and the idea
of the H-bomb, which was to haunt the Laboratory in the postwar era.
Seldom has a physics summer school been as portentous for the future
of mankind.
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