84 Chapter Two
0 5 10 15 20LeadTotal
Pair production
Compton
scatteringPhotoelectric effect251.6
1.4
1.2
1.0
0.8
0.6
0.4
0.2
Linear attenuation coefficient, cm^0-^1
Photon energy, MeVFigure 2.29Linear attentuation coefficients for photons in lead.Pair production becomes increasingly likely the more the photon energy exceeds
the threshold of 1.02 MeV. The greater the atomic number of the absorber, the lower
the energy at which pair production takes over as the principal mechanism of energy
loss by gamma rays. In the heaviest elements, the crossover energy is about 4 MeV, but
it is over 10 MeV for the lighter ones. Thus gamma rays in the energy range typical of
radioactive decay interact with matter largely through Compton scattering.
The intensity Iof an x- or gamma-ray beam is equal to the rate at which it trans-
ports energy per unit cross-sectional area of the beam. The fractional energy dIIlost
by the beam in passing through a thickness dxof a certain absorber is found to be pro-
portional to dx: dx (2.24)The proportionality constant is called the linear attenuation coefficientand its
value depends on the energy of the photons and on the nature of the absorbing material.
Integrating Eq. (2.24) givesRadiation intensity II 0 ex (2.25)The intensity of the radiation decreases exponentially with absorber thickness x.
Figure 2.29 is a graph of the linear attenuation coefficient for photons in lead as a func-
tion of photon energy. The contribution to of the photoelectric effect, Compton scat-
tering, and pair production are shown.
We can use Eq. (2.25) to relate the thickness xof absorber needed to reduce the
intensity of an x- or gamma-ray beam by a given amount to the attenuation coefficient
. If the ratio of the final and initial intensities is II 0 ,ex ex ln xAbsorber thickness x (2.26)ln (I 0 I)
I 0
II 0
II
I 0dI
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