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RADIATION PROTECTION - ILEA

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6 | Beta Particles 27<br />

2.3 Decrease of counting rate of an indium-<br />

116 source after an arbitrary starting time.<br />

Measurements were made with a G-M counter.<br />

Each count was taken for one minute, starting<br />

30 seconds before the time recorded for the<br />

count. When plotted on semilogarithmic paper,<br />

the results of the measurements fall close to a<br />

straight line drawn as a best fit, with a half-life<br />

of 54 minutes. They do not fall exactly on the<br />

line because of statistical variations in the<br />

number of disintegrations in a fixed counting<br />

interval (see Part Four, section 6).<br />

Counts in 1 minute<br />

10,000<br />

9000<br />

8000<br />

7000<br />

6000<br />

5000<br />

4000<br />

3000<br />

2000<br />

1000<br />

20 40 60 80 100<br />

Decoy time (min)<br />

mately 79 percent of the 238 U and 99 percent of the 40 K have been lost by<br />

decay since creation because of their radioactivity.<br />

6.1.2 Maximum and Average Energies of Beta Particles<br />

The energies of the beta particles given off in radioactive decay of the<br />

various radionuclides listed in Table 2.1 are expressed in terms of both a<br />

maximum energy and an average energy. The maximum energies range<br />

from 0.018 million electron volts (MeV) for tritium to 2.24 MeV for<br />

strontium-90 (from the yttrium-90 decay product). The tritium betas are<br />

very weak, the maximum energy of 0.018 MeV, or 18,000 eV, being less<br />

than the energies of electrons hitting the screens of most TV tubes. Average<br />

energies are given for the beta sources because, as stated earlier, the nature<br />

of beta decay is such that any individual beta particle can have any energy<br />

up to the maximum (E max ). However, only a very small fraction of the<br />

emitted beta particles have energies near the maximum. The frequency<br />

with which energies below the maximum are carried by the beta particles is<br />

given by energy spectrum curves, which have characteristic shapes. Energy<br />

spectra for tritium and carbon-14, low-energy beta emitters, and for phosphorous-32,<br />

a high-energy beta emitter, are shown in Figure 2.4. Energy

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