Presentation Speech by Professor E. Hulthén, Chairman of the Nobel Committee for Physics
Your Majesties, Your Royal Highnesses,
Ladies and Gentlemen.
The notion of matter as something built up of very tiny and
indivisible atoms is a heritage from classical times. Since,
however, experimental research in our days has shown that the
atoms in their turn are complicated structures, the notion of
indivisibility has been transferred to the so-called elementary
particles of which the atom is composed, in the hope of therewith
having reached the ultimate limit for the division of
matter.
However, the different kinds of elementary particles showed an
alarming tendency to increase in number - something which is at
variance with the attractive idea that matter is built up of one
or at most two kinds of particles.
Among the most successful and noteworthy uation is Dirac's theory of
particles and attempts to interpret this situation is Dirac's
theory of particles and antiparticles, which may be designated,
almost, as each other's mirror images. Both kinds of particles
are conceived as arising through the formation of pairs and as
reciprocally annihilating each other. The world in which we find
ourselves belongs, by chance, to the one kind of particles, among
which sporadically occurring antiparticles are very quickly
destroyed. On account of the mirror symmetry it would be very
difficult to decide whether a remote star or galaxy belonged to
the one or the other kind of matter.
There were probably very few physicists who at first ascribed to
this side of Dirac's otherwise very valuable theory any real
import until, quite suddenly and unexpectedly, the first
antiparticle, the positive electron, was discovered by Anderson in cosmic
radiation in the year 1931. Continued investigations showed that
the new particle behaved in all respects according to Dirac's
theory: that it was manifested, namely, in connection with some
energetic process, always together with an ordinary electron, and
that it disappeared in the same way and with equal suddenness.
Today nothing is better known and clearly elucidated than this
process of pair formation and annihilation.
Nonetheless it now seemed desirable to test the validity of this
remarkable theory upon the antiparticle to the proton, the
nucleus of the hydrogen atom - a process which required, however,
about 2,000 times as great an amount of energy. Such quantas of
energy do, certainly, occur in cosmic radiation, but in such a
random way that it was finally realized that the only systematic
way of investigating the process was through the controlled
production of the antiproton by means of an accelerator with a
sufficiently high capacity.
It has been said of the Bevatron, the great proton
accelerator at Berkeley University in California, that it was
constructed chiefly with a view to the production of antiprotons.
This is perhaps an exaggeration, but in so far correct as its
peak achievement, 6 milliard electron volts, was set with a view
to the energy required for the pair formation of protons -
antiprotons. That it was constructed in Berkeley was due to the
tradition established there ever since Lawrence built the first
cyclotron and McMillan developed the principle for the
synchronization of relativistic particles.
But even if antiproton research was thus first made possible
through this technologically very impressive machine, the actual
discovery and investigation of the antiproton was chiefly the
merit of Chamberlain and Segrè. With similar methods an
antiparticle to the neutron has subsequently been discovered, a
discovery whose importance lies in the fact that the concept of
the antiparticle was thereby extended to include also the neutral
elementary particles.
Professor Emilio Segrè, Professor Owen
Chamberlain. Your discovery of the antiproton was made possible
through the excellent resources at the Radiation Laboratory in
Berkeley. It is, however, your ingenious methods for the
detection and analysis of the new particle that the Royal Swedish
Academy of Sciences wishes to recognize on this occasion.
I need surely not remind you, Professor Segrè, of the
occasion, twenty-one years ago, when your compatriot Enrico Fermi
received his Nobel Prize in this selfsame place. You and he were
intimate friends and you had been collaborating with great
success. Both of you belonged to that group of distinguished
Italian scientists that was westward bound in those days.
Also you, Professor Chamberlain, must surely have an intimate and
abiding recollection of your years together with Fermi in
Chicago.
Gentlemen, I now ask you to receive your prize from the hands of
His Majesty the King.
From Nobel Lectures,
Copyright © The Nobel Foundation 1959