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

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190 CHAPTER 5<br />

For the case of a point source of S thermal neutrons per second in a spherically<br />

shaped nonmultiplying medium (a medium which contains no fissile material) of<br />

radius R, thermal diffusion length L, and diffusion coefficient D, the flux of neutrons<br />

escaping from the surface is<br />

φ =<br />

S<br />

4π RD × e −R/L . (5.62)<br />

W EXAMPLE 5.15<br />

A Pu–Be neutron source that emits 10 6 neutrons/s is in the center of a spherical<br />

water shield whose diameter is 50 cm. How many thermal neutrons are escaping per<br />

square centimeter per second from the surface of the shield?<br />

Solution<br />

Since the radius of the water shield is much greater than the fast diffusion length<br />

given in Table 5-7, we may assume (for the purpose of this calculation) that essentially<br />

all the fast neutrons are thermalized and that the thermal neutrons are diffusing<br />

outward from the center. Substituting the appropriate numbers in<strong>to</strong> Eq. (5.62), we<br />

have<br />

10<br />

φ =<br />

6 neutrons/s<br />

4π × 25 cm × 0.16 cm e −25 cm/2.88 cm = 3.4 neutrons/s<br />

cm2 .<br />

Absorption<br />

The discussion above shows that fast neutrons are rapidly degraded in energy by<br />

elastic collisions if they interact with low-a<strong>to</strong>mic-numbered substances. As neutrons<br />

reach thermal or near thermal energies, their likelihood of capture by an absorber<br />

nucleus increases. The absorption cross section of many nuclei, as the neutron energy<br />

becomes very small, has been found <strong>to</strong> be inversely proportional <strong>to</strong> the square root<br />

of its kinetic energy and thus <strong>to</strong> vary inversely with its velocity:<br />

σ ∝ 1<br />

√ ∝<br />

E 1<br />

. (5.63)<br />

v<br />

Equation (5.63) is called the one-over-v law for slow neutron absorption. For 10 B,<br />

this relationship is valid for the span of energies from 0.02 <strong>to</strong> 1000 eV, as shown in<br />

Figure 5-25. Thermal neutron cross sections are usually given for neutrons whose<br />

most probable energy is 0.025 eV. If the cross section at energy E0 is σ0, then the

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