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Detection and Measurement  Techniques             231

              premixed  with  acid  and  scintillator  solution  before  counting;  the  use  of  that  system  is
              described  in  w



                                     8.9.  Absolute  disintegration  rates

               The  determination  of absolute  disintegration  rates  is of great  importance  in  all  areas  of
              nuclear  chemistry,  tracer  work,  age  calculation,  etc.  Numerous  methods  have  been
              employed,  many  using  techniques  described  above,  as track counting,  liquid  scintillation
              measurements,  47r proportional counters,  etc.  If the nuclei decay through/~-7 emission,  the
              absolute rate may be obtained by two detectors placed close to each  side of a thin sample,
              one  detector/~-sensitive  and  the other "y-sensitive.
               When only a single detector in  a conventional counting set-up is available (e.g.  detector
              arrangement in Fig.  8.4),  absolute counting rates can be obtained for unknown samples by
              comparison  with  known  standards.
               When standards are not available it is possible to obtain an approximate estimation of the
              absolute  disintegration  rate  from  a  knowledge  of  the  various  factors  that  influence  the
              counting efficiency.  The detection efficiency ff is defined as a ratio between the count rate
              and the absolute disintegration rate (4.45).  This detection efficiency,  which was discussed
              briefly in  w   is the product of all the factors which influence the measured count rate and
              may be expressed  as

                                                                                  (8.16)
                                        =  ~det~res~'geom~back~self~abs
              where   •det   =  counting  efficiency  of detector,
                             =  resolving  time correction  (see  w
                      !~geom   =  geometry  factor (see  w
                             =  backscattering  factor,
                      ~back
                      ~self   =  self-absorption  factor  (~bsample =  ~bbackl~self ),  and
                             =  absorption  factor  (see  w

                The efficiency  of the detector is a measure of the number of counts registered compared
              to  the number  of particles  that enter  the  sensitive volume of the detector.  This  efficiency
              is  approximately  100%  for  a-  and  high-energy/3-particles  in  most  detectors,  but  often
              substantially  lower  for -y-rays.  Inasmuch as it  is quite  difficult  to apply  simple  geometric
              considerations  to  the  solid  angle  subtended  by  a  detector  for  a  source  which  is  not
              concentrated  at  a point,  usually  the  factors  ~det  and  l~geo m are  determined  experimentally
              by using a very  thin standard source of approximately the same area as the unknown.  The
              factor  ~bgeo m can  be calculated  for circular  samples and  detector windows,  see  w
                It was noted  in  w   that/~-rays undergo  large angle deflections.  As a result,/~-particles
              from  the  sample  which  may  start  in  a  direction  away  from  detector  can  be  deflected  by
              several  scattering events back into the detector.  Such backscattering  is dependent  upon the
              atomic  number  of the  material  upon which  the sample  is supported  (cf.  Fig.  6.14).  ffback
              increases  with  backing  material  thickness up  to a  saturation  thickness  beyond  which  it  is
              constant.  Counting  is usually done with either  an essentially weightless backing  (~kback =
              1)  or  with  a  backing  sufficiently  thick  as  to  have  saturation.  The  saturation  thickness
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