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Absorption  of Nuclear Radiation                141


               scattering.  This  process  is  known  as  backscattering,  since  the  backing  (or  support)  for
               radioactive  samples  may  cause  scattering  of a  certain  fraction  of the  particles  through  as
               much  as  180 ~  The  fraction  of back-scattered/3-radiation  depends  on the geometry  of the
               measuring  system,  the energy of the/~-particles,  and the thickness and electron density of
               the backing material.  In Figure 6.14 the percent backscattering as a function of the atomic
               number of the backing material is shown for four/~-energies (Emax); the radioactive sample
               is considered  infinitely  thin (i.e.  no self-absorption).  From the curve  for 32p on platinum
               (Z =  78) we see that about 40 % of the measured radiation is due to back-scattered radiation
               (0.8/(1.0  +  0.8)  =  0.4).  Backscattering increases with the thickness of the backing material
               up  to a  saturation  value which is reached when the thickness of the backing  is about one-
               fifth of the extrapolated  range of the/3-particles  in  that material.


                                       6.5.  Absorption  of v-radiation

                The  absence  of  charge  and  rest  mass  for  7-rays  results  in  little  interaction  with  the
               absorbing  atoms  and  in  long  ranges.  The  number  of ion  pairs  produeexl  in  a  given  path
               length  by  7-rays  is only  1-10%  of that produced  by ~-particles  of the same  energy  (Fig.
               6.5);  e.g.  a  1 MeV  7-ray  produces  only  about  one  ion  pair  per  centimeter  of  air.  As  a
               consequence  of this  low specific  ionization of 7-rays,  the ionization is almost completely
               secondary  in nature  resulting  from the action of a  few high energy primary  ion pairs.



               6.5.1.  Attenuation  coefficient

                Unlike  heavy  particles  and  electrons  which  lose  their  energy  as  a  result  of  many
               collisions,  7-rays  are  completely  stopped  in  one or,  at most,  a  few interactions.  For  thin
               absorbers the attenuation of 7-rays follows relation (6.7), where ~ is the number of photons
               m -2  s-1.  The proportionality factor #  is called the (total) attenuation coefficient.  When it
               has the dimension of m- 1 and the thickness x is expressed in meters,  #  is referred  to as the
               linear attenuation coefficient.  The attenuation coefficient can be expressed  in other ways:

                                    Pm  =  P/P  =  era NA/M  =  a e ZN A/M          (6.19)


               where p  is the density,  M  the average atomic weight,  and Z  the average atomic number of
               the  absorber.  NAp/M  can  be  replaced  by  N v,  by  which  we  can  define  a  macroscopic
               absorption cross-section F, (cf.  w 14.1).  E- 1 is the mean free path or relaxation length of the
               radiation  in  the absorbing  material.  #m (in cm 2 g-1  when x is in centimeters)  is the mass
               attenuation  coefficient;  o a is  the probability  of reaction  between  a  7-ray  and  the  electron
               cloud of the absorber atom (atomic reaction cross-section, m 2 atom- 1); oe is the probability
               of  the  reaction  of  a  -y-ray  with  a  single  electron  of  the  absorber  (electron  reaction
               cross-section,  m 2 electron- 1). oa and o e are analogous to the nuclear reaction cross-sections
               discussed later.  In Table 6.1  only the equivalent nuclear and atomic reaction cross-sections
               are  given.
                Since a  7-ray  may be removed from the beam in the  first  few Angstr6ms of its entrance
               into  the  absorber  or  may  travel  several  centimeters  with  no  interaction  at  all  and  then be
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