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RADIATION PROTECTION - ILEA

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Historical Prologue 7<br />

P.3A Decay of the carbon-14 nucleus,<br />

6<br />

14<br />

C.<br />

The carbon-14 nucleus, with 6 protons and 8<br />

neutrons, is not stable, because the ratio of<br />

neutrons to protons is too high. The ratio is<br />

changed by the spontaneous transformation of<br />

one of the neutrons into a proton and the emission<br />

of an energetic beta particle (negative)<br />

from the nucleus. The average lifetime of the<br />

nucleus is 8,250 years. After its decay, however,<br />

the resultant nitrogen-14 nucleus (7 protons,<br />

7 neutrons) is stable.<br />

= Proton<br />

= Neutron<br />

{ β {<br />

−<br />

6p<br />

8n<br />

7p<br />

7n<br />

22<br />

P.3B Decay of the sodium-22 nucleus, 11<br />

Na.<br />

The sodium-22 nucleus, with 11 protons and<br />

11 neutrons, is also not stable. The ratio of protons<br />

to neutrons is too high. The ratio is usually<br />

changed by the spontaneous transformation of<br />

one of the protons into a neutron and the emission<br />

of an energetic positron (positive beta<br />

particle) from the nucleus. About 10 percent of<br />

the time, the ratio is changed by the capture<br />

by a proton of an electron from an inner orbit,<br />

which transforms it into a neutron. The average<br />

lifetime of the unstable sodium-22 nucleus is<br />

3.75 years. The resultant neon-22 nucleus (10<br />

protons, 12 neutrons) is stable.<br />

11 10<br />

11 12<br />

3 The Development of a Radiation Technology<br />

After the discovery of the neutron, major developments in nuclear research<br />

came in rapid succession: the discovery of uranium fission in 1939, and the<br />

recognition of the possibility of releasing enormous amounts of energy;<br />

achievement of the first self-sustaining fission reaction in a reactor in 1942;<br />

explosion of nuclear fission devices in 1945; production of thermonuclear<br />

explosions in 1952; commissioning of the first nuclear-powered submarine,<br />

the Nautilus, in 1954; and the development of high-energy accelerators,<br />

with energies over 10 9 electron volts (GeV) in the fifties and exceeding<br />

10 12 electron volts (1 TeV) at the present time. The result of these<br />

developments was the creation of an extensive radiation technology concerned<br />

with the production of energetic radiations for use in research,<br />

medical treatment, and industry.<br />

β +<br />

4 The Need for Radiation Protection<br />

The development of a radiation technology left its occupational casualties—physicists,<br />

radiologists, radiation chemists—researchers who investigated<br />

the properties and uses of these energetic radiations without appreci-

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