Page 109 - Radiochemistry and nuclear chemistry
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98                   Radiochemistry  and Nuclear  Chemistry


                                 TABLE 5.2.  Primordial  radionuclides for Z  <  82  (Pb)

                        Nuclide    Isotopic abundance   Decay mode and   Half-life (years)
                                         %           particle energy MeV
                        4~              0.0117        ~-  EC  1.31         1.26 x 109
                        "~V             0.250         B-  EC  (0.601)      >  1.4 x 1017
                        S7Rb           27.83          B-  0.273            4.88 x 101~
                         llSIn         95.72          fl-  1.0             4.4 x 1014
                         lZ'~re         0.905         EC  (0.052)          1.3 x 1013
                         13SLa          0.092         3-  EC               1.06 x 1011
                         144Nd         23.80          o~                   2.1 x 1015
                        147Sm           15.0          et 2.23              1.06 X l0 II
                        14SSm           11.3          tx 1.96              7 X 1015
                        1761m           2.59          /J- (1.188)          3.8 x 101~
                         174Hf          0.162         ct                   2x1015
                         lSTRe         62.60          B-  0.0025           4.2x 101~
                         19~            0.012         ot                   6.5x10 II
                        Values within parenthesis  refer to decay energies.
                       ,         ,   ,,   ,,   ,   ,   ,   .  .  .  .  .  .  ,   ,   ,   ,,   ,
                Because of the long half-lives of these nuclides they must have been formed at the time
               of (or possibly even before) the formation of the solar system and of the earth.  When  the
               earth's  crust  solidified,  these  radionuclides  became  trapped  in  rocks.  As  they  decayed,
               decay products accumulated  in the closed rock environment.  By measuring the amount of
               parent  and  daughter  nuclides,  it  is  possible  with  the half-life  to  calculate  how  long  this
               environment (e.g.  a rock formation) has existed.  This is the bases for nuclear dating (also
               called  "radioactive clocks'), and almost all of the nuclides in Table 5.2 can be used for this
               purpose.  In  w 5.8  we discuss dating methods  for the K-Ar  and Rb-Sr  systems.
                A  careful  look  at these naturally  occurring  long-lived nuclei  reveals  that  some of them
               appea:r in short decay series,  e.g.  152Gd ~  148Sm ~  144Nd --*  140Ce  and  19~  ~  186Os  --~
               182W. The heavy element  series beginning  with U  and Th isotopes  are therefore referred
               to as long decay series.


               5.2.2.  Elements in the natural radioactive decay series

                In Chapter  1 we briefly discussed the existence of four long series of genetically  related
               radioactive nuclides beginning with Th,  U or Np and ending with Pb or Bi.  In Figure 5.1
               we  present  all  known  isotopes  of  elements  81TI to  92 U.  Some  of  these  nuclides  occur
               naturally  in  the  long  decay  series  shown  in  Figure  2.11.  Others  are  produced  through
               nuclear  reactions  according  to  the schemes in  Figure 4.8  and principles  described  in  Ch.
               12-15.  The first series in Figure  1.2 is known as the thorium decay series,  and consists of
               a group  of radionuclides  related through decay in which all the mass numbers  are evenly
               divisible by four (the 4n series).  It has its natural origin in 232Th which occurs with  100 %
               isotopic  abundance.  Natural  thorium  has  a  specific  activity  S  of  4.06  MBq/kg,  as  its


               1 The  student can easily trace the decay series in Fig. 5.1  with a transparent marker.
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