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Introduction to Health Physics: Fourth Edition - Ruang Baca FMIPA UB

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96 CHAPTER 4<br />

when an orbital electron is captured. It is thus seen that in all types of radioactive<br />

decay involving either the capture or emission of an electron, a neutrino must be<br />

emitted in order <strong>to</strong> conserve energy. However, in contrast <strong>to</strong> positron and negatron<br />

(ordinary beta) decay, in which the neutrino carries off the difference between the<br />

actual kinetic energy of the particle and the maximum observed kinetic energy and,<br />

therefore, has a continuous energy distribution, the neutrino in orbital electron<br />

capture is necessarily monoenergetic.<br />

Whenever an a<strong>to</strong>m is transformed by orbital electron capture, an X-ray, characteristic<br />

of the daughter element, is emitted as an electron from an outer orbit<br />

falls in<strong>to</strong> the energy level that had been occupied by the captured electron. That<br />

characteristic X-rays of the daughter should be observed follows from the fact that<br />

the X-ray pho<strong>to</strong>n is emitted after the nucleus captures the orbital electron and is<br />

thereby transformed in<strong>to</strong> the daughter. These low-energy characteristic X-rays must<br />

be considered by health physicists when they compute absorbed radiation doses<br />

from internally deposited iso<strong>to</strong>pes that decay by orbital electron capture.<br />

Isomeric Transitions<br />

Gamma Rays<br />

Gamma rays are monochromatic electromagnetic radiations that are emitted from<br />

the nuclei of excited a<strong>to</strong>ms following radioactive transformations; they provide a<br />

mechanism for ridding excited nuclei of their excitation energy without affecting<br />

either the a<strong>to</strong>mic number or the a<strong>to</strong>mic mass number of the a<strong>to</strong>m. Since the health<br />

physicist is concerned with all radiations that come from radioactive substances and<br />

since X-rays are indistinguishable from gamma rays, characteristic X-rays that arise<br />

in the extranuclear structure of many nuclides must be considered by the health<br />

physicist in evaluating radiation hazards. However, because of the low energy of<br />

characteristic X-rays, they are of importance mainly in the case of internally deposited<br />

radionuclides. Annihilation radiation—the gamma rays resulting from the mutual<br />

annihilation of positrons and negatrons—are usually associated, for health physics<br />

purposes, with those radionuclides that emit positrons. In considering the radiation<br />

hazard from 22 Na, for example, two 0.51-MeV pho<strong>to</strong>ns (the energy equivalent of<br />

the two particles that were annihilated) from the annihilation process, which are<br />

not shown on the decay scheme, must be considered <strong>to</strong>gether with the 1.277-MeV<br />

gamma ray, which is shown on the decay scheme. The general rule in health physics,<br />

therefore, is au<strong>to</strong>matically <strong>to</strong> associate positron emission with gamma radiation in<br />

all problems involving shielding, dosimetry, and radiation hazard evaluation.<br />

Internal Conversion<br />

Internal conversion is an alternative isomeric mechanism <strong>to</strong> radiative transition by<br />

which an excited nucleus of a gamma-emitting a<strong>to</strong>m may rid itself of excitation energy.<br />

It is an interaction in which a tightly bound electron interacts with its nucleus,<br />

absorbs the excitation energy from the nucleus, and is ejected from the a<strong>to</strong>m. Internally<br />

converted electrons appear in monoenergetic groups. The kinetic energy<br />

of the converted electron is always found <strong>to</strong> be equal <strong>to</strong> the difference between the<br />

energy of the gamma-ray emitted by the radionuclide and the binding energy of<br />

the converted electron of the daughter element. Since electrons in the L energy

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