Worlds Within Worlds: The Story of Nuclear Energy, Volume 3 (of 3): Nuclear Fission; Nuclear Fusion; Beyond FusionAsimov, Isaac
History
Worlds Within Worlds: The Story of Nuclear Energy, Volume 3 (of 3): Nuclear Fission; Nuclear Fusion; Beyond Fusion
Asimov, Isaac
Nuclear energy -- Popular works
The antiproton was as unlikely to last as long as the positron was. It
was surrounded by myriads of proton-containing nuclei and in a tiny
fraction of a second it would encounter one. The antiproton and the
proton also underwent mutual annihilation, but having 1836 times the
mass, they produced 1836 times the energy that was produced in the case
of an electron and a positron.
There was even an “antineutron”, a particle reported in 1956 by the
Italian-American physicist Oreste Piccioni (1915- ) and his
co-workers. Since the neutron has no charge, the antineutron has no
charge either, and one might wonder how the antineutron would differ
from the neutron then. Actually, both have a small magnetic field. In
the neutron the magnetic field is pointed in one direction with
reference to the neutron’s spin; in the antineutron it is pointed in the
other.
[Illustration: _Bubble chamber photograph of an antiproton
annihilation._]
In 1965 the American physicist Leon Max Lederman (1922- ) and his
co-workers produced a combination of an antiproton and an antineutron
that together formed an “antideuteron”, which is the nucleus of
antihydrogen-2.
This is good enough to demonstrate that if antiparticles existed by
themselves without the interfering presence of ordinary particles, they
could form “antimatter”, which would be precisely identical with
ordinary matter in every way except for the fact that electric charges
and magnetic fields would be turned around.
If antimatter were available to us, and if we could control the manner
in which it united with matter, we would have a source of energy much
greater and, perhaps, simpler to produce than would be involved in
hydrogen fusion.
To be sure, there is no antimatter on earth, except for the
submicroscopic amounts that are formed by the input of tremendous
energies. Nor does anyone know of any conceivable way of forming
antimatter at less energy than that produced by mutual annihilation, so
that we might say that mankind can never make an energy profit out of
it—except that with the memory of Rutherford’s prediction that nuclear
energy of any kind could never be tapped, one hesitates to be
pessimistic about anything.
The Unknown
Physical theory makes it seem that particles and antiparticles ought to
exist in the universe in equal quantities. Yet on earth (and, we can be
quite certain, in the rest of the solar system and even, very likely, in
the rest of the galaxy) protons, neutrons, and electrons are common,
while antiprotons, antineutrons, and positrons are exceedingly rare.
Could it be that when the universe was first formed there were indeed
equal quantities of particles and antiparticles but that they were
somehow segregated, perhaps into galaxies and “antigalaxies”? If so,
there might occasionally be collisions of a galaxy and an antigalaxy
with the evolution of vast quantities of energy as mutual annihilation
on a cosmic scale takes place.
Public-domain text, read in full here on John Shaqi.
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