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130                 Radiochemistry and Nuclear Chemistry


                Whereas  it  is  possible  to  specify  maximum  ranges  for  charged  particles,  this  is  not
              possible for neutral particles such as neutrons and v-quanta.  If the absorber is not too thick,
              these particles undergo only one collision,  or at the most a few,  before they are absorbed.
              As a  result  the absorption  curve has an exponential  form.

                                              r  =  ~b 0 e- zx                      (6.7)

              where  tt is  the total attenuation  coefficient. Thus  for n  and ~ we have


                                             ~bab s  (x)  =  e -px                  (6.8)
                The  reduction  in  intensity  of a  beam  can  occur  by  two  mechanisms.  One  involves  the
              deflection or scattering of the particles from the direct line of path between the source and
              the detector and is described by the scattering coefficient tts. The second mode of reduction
              is the complete transfer of the projectile energy to the absorbing material (the particles  are
               "captured"  )  and  is  designated  by  the  (energy) absorption  coefficient  #a"  The  (total)
              attenuation  coefficient  in (6.7)  is the sum of both  these modes.

                                              #  =  #s  +  #a                       (6.9)

              Both  tts  and  tt a can  be  measured  independently.  The  (total)  attenuation  coefficient  is  of
              primary interest in radiation shielding, while the (energy) absorption coefficient is important
              in  considering  radiation  effects on matter.



                                6.3.  Absorption  of  protons  and  heavier  ions
                The  mode  of interaction  of protons  and heavier charged particles  with  the atoms  of the
              absorbing material can be illustrated by considering the absorption of a-particles.  With rare
              exception,  a-particles emitted by radioactive nuclides have energies between 4 and 9 MeV.
              Since  the  a-particles  are  so  much  heavier  than  electrons,  they are deflected  very  slightly
              when their Coulomb  fields interact with atoms or molecules to form ion pairs.  As a result,
              c~-particles  travel in a straight line as they pass through matter,  which explains the straight
              paths observed for a-particles in cloud chamber photographs (Fig.  6.5).  This is in contrast
              to the very curved or irregular paths of the secondary electrons emitted in the formation of
              the ion pair.  For a 5 MeV a-particle the maximum energy of the secondary electrons is 2.7
              keV.  However  only a small  fraction of the  secondary electrons  actually receive this much
              energy;  the average energy  of the secondary electrons  is closer  to  100 eV.  The  ionization
              caused by more energetic secondary  electrons  is usually referred  to as 6-tracks (cf.  {}7.2).
                In solids  and liquids  the total path  length for a-particles  from radioactive decay  is quite
              short.  However,  in  gases  at  standard  temperature  and  pressure  the  paths  are  several
              centimeters long (Table 6.2).  The range in air for c~-particles with an initial energy Ec~ MeV
              can  be calculated  by  the empirical  equation  (Pair =  1.293  kg m-3):

                               J~air =  0.31Ea 3/2 (cm)  =  0.40 Ea 3/2 (nag cm -2)   (6.10)

              The  range/~z  in  other materials  can  be approximated  roughly by
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