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
If the purpose of the nuclear accelerating machines were to produce
cheap energy, they would not be of much value. A nuclear reaction may
typically release five to 20 million electron-volts of energy. But to
obtain this reaction, a million particles had to be accelerated to
energies of several million electron-volts. The recoverable and useable
energy will be only a minute fraction of the total invested.
On the other hand, as a tool for scientific discovery, the atom-smashers
have been of great importance. That one event in a million has given us
much of our knowledge of nuclear physics.
The achievement of nuclear reactions by particle bombardment did not
actually wait on the invention of man-made accelerating machines.
Energetic alpha particles are available from the radioactive decay of
heavy elements. In 1919 Ernest Rutherford used such radioactive elements
as a source of alpha particles. The alpha particles were made to bombard
ordinary nitrogen, causing the reaction:
He⁴ + N¹⁴ → O¹⁷ + proton
(2 protons) (7 protons) (8 protons)
(2 neutrons) (7 neutrons) (9 neutrons)
That is, an alpha particle plus a nitrogen¹⁴ nucleus react to produce a
nucleus of (stable) oxygen¹⁷ plus a proton. Oxygen¹⁷ is a nucleus with 8
protons and 9 neutrons. The ordinary abundant form of oxygen has 8
protons and 8 neutrons. Natural oxygen contains a small amount of
oxygen¹⁷.
Later, in 1934, Irene Curie Joliot (the daughter of the discoverer of
radium, Madame Curie) and her husband, Frederic Joliot, used naturally
available alpha particles to make artificial radioactive nuclei for the
first time. The reaction was:
He⁴ + aluminum²⁷ → phosphorus³⁰ + neutron
(2 protons) (13 protons) (15 protons)
(2 neutrons) (14 neutrons) (15 neutrons)
Phosphorus³⁰ is an unstable nucleus and emits a beta ray (a positron) to
become silicon³⁰ (which is stable). The half-life for this decay is
about 2.5 minutes. The Joliots’ reaction was the first instance in which
man had produced radioactivity and known it. Actually cyclotrons had
been producing radioactivity in good abundance for the preceding two
years—but physicists had been unaware of this fact.
It is amusing that nature has also provided us with an atom-smashing
machine and indeed one that produces far greater energies than any
apparatus yet devised by man. This machine operates on the principle of
fluctuating, turbulent magnetic fields in interstellar space. Cosmic
particles—mainly protons, but also some alpha particles and even heavier
nuclei—are accelerated by these changing magnetic fields and hurled
occasionally into the earth’s atmosphere. The energies of these cosmic
particles are enormous, ranging from billions of electron-volts to
values a million times higher.
Public-domain text, read in full here on John Shaqi.
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