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Absorption  of Nuclear Radiation                127





                                                   I
                                                   Ir
                                                   I
                                                   Y
                                                   i    f
                                                     d

                The  activity  measured  is proportional  to  the particle  flux  ~  reaching  the  detector

                                               R  =  kde t ~                        (6.4)

              where  kde t  =  Sde t ~bde t and

                                              t~  =  ~abs t~0                       (6.5)

               and

                                         r  =  ~bsample  nA/(47rr 2 )                (6.6)

               $0 is the flux of particles (particles m- 2 S- 1) which reach the detector from the source when
               ~kabs -  1,  and  n  is the number of particles  emitted per decay  (n  >  1 only  for y  following
               c~-  and  B-decays).  Thus  if  every  B-decay  yields  2y  (in  cascade)  and  y  is  the  measured
               radiation,  then  n v  =  2,  and #0  =  n~At3/(4r r 2 ) y-quanta m -2  s-1.  In branched  decay n
               will  not  be  an  integer.  Equation  (6.6)  is  the  so  called  1/r 2-law  since  the  measured  flux
               varies  as  the  inverse  of the  square  of the distance  to the  source.
                These  equations  are  valid  as  long  as  the conditions  at  the  source  and  at the  detector,  as
               well  as r,  are kept constant.  When  an absorber  is inserted between  the source and detector
               (Fig.  6.1),  ~kabs depends on the absorber thickness x (m).  For zero absorber thickness,  flabs
               =  1  in  accurate  measurements.  There  is  a  small  absorption  due  to  the  air  between  the
               sample  and  detector  unless  the  measurement  is done  in a  vacuum.
                Absorption  curves  relate  the variation  of either R or  q~ to the  thickness  of the absorbing
               material.  In  Figure  6.3  the relative  transmission  ~/~0  is plotted  as a  function  of absorber
               thickness for different kinds of radiation.  For charged particles,  i.e.  electrons,  protons,  and
               heavier  ions,  #/#Q  reaches  zero  at  a  certain  x-value  (Xmax); this  is  referred  to  as  the
               maximum  range,  R,  of  the  particles.  The  range  can  be  expressed  by  either  the  average
               range (x  =  C 1 for heavy ions and C 3 for electrons) or the maximum (or extrapolated)  range
               (C 2 and  C 4,  respectively,  in Fig.  6.3).  The loss of energy  involves collisions  with  atomic
               electrons,  and  the  energy  loss per  collision  and  the number  or collisions  varies  from  one
               ionizing particle to the next,  resulting in a slight straggling in the range.  The average range
               is  the  meaningful  one.
                Figure 6.4  shows an absorption curve for 32p.  The radioactivity R has been  measured as
               a function of aluminum absorber thickness in linear density, kg m-2 or more commonly mg
               cm -2.  The  low activity  "tail"  (C 4 in Fig.  6.4)  is the background activity R b,  which has to
               be  subtracted  from  the  measured  value R m to obtain  the  true value  for  the  radiation  (e.g.
               32p).  R  =  R m -  R b. The extrapolation of R to a value equal to R b (i.e.  C3) gives the range.
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