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138                  Radiochemistry and Nuclear Chemistry




























                      FIG.  6.11.  Bottles containing  highly radioactive  9~  solutions glow  in the  dark  due  to
                      ~erenkov  radiation from daughter 90y (Errmx 2.3 MeV).

               emitted coherently in a cone whose axis is the direction of the moving particle (Fig.  6.8e).
               The angle of the cone 0 is obtained from

                                               sin 0  =  C/Vp                       (6.17)

               This  ~erenkov  radiation  is  the  source of  the bluish  light observed  in highly  radioactive
               solutions (Fig.  6.11) and around reactor fuel dements  submerged in water.  The radiation
               can be used for detecting #-particles and for measuring high particle energies (from 0).  For
               a  fast electron  the energy loss  through  r   radiation  is  _<  0.1%  of the energy  loss
               through other processes.  r   detectors are described in Ch.  8.



               6.4.4.  Positron  annihilation

                Positrons interact with matter through ionization, excitation, emission of bremsstrahlung,
               and ~erenkov  radiation in the same manner as negative electrons.  As the kinetic energy of
               the  positron  decreases  in  the  absorber,  there  is  an  increase  in  probability  of  direct
               interaction between the positron and an electron (Fig.  6.8d) in which both the positron and
               electron  are  annihilated.  The  energy  of  the  two  electron  masses  is  converted  into
               electromagnetic radiation. This process, known as positron annihilation,  is a characteristic
               means of identification of positron emission.  Since an electron mass is equivalent to 0.51
               MeV,  and  the  kinetic energy  of the particles of annihilation is  essentially  zero,  the  total
               energy  for  the  annihilation  process  is  1.02  MeV.  In  order  to  conserve  momentum  the
               photons must be emitted with equal energy and in exactly opposite direction in case of only
               two  photons  (the  dominating case).  These  photons  of 0.51  MeV  each  are  referred  to  as
               annihilation radiation. The presence of'y-rays at 0.51 MeV in the electromagnetic spectrum
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