Page 52 - Radiochemistry and nuclear chemistry
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CHAPTER  3



                                Nuclear Mass and Stability




                                                Contents

                              3.1.   Patterns of nuclear stability       41
                              3.2.   Neutron to proton ratio             43
                              3.3.   Mass defect                         45
                              3.4.   Binding energy                      47
                              3.5.   Nuclear radius                      48
                              3.6.   Semiempirical mass equation         50
                              3.7.   Valley of/3-stability               51
                              3.8.   The missing elements: 43Tc and ePm   53
                                     3.8.1.   Promethium                 53
                                     3.8.2.   Technetium                 54
                              3.9.   Other modes of instability          56
                             3.10.   Exercises                           56
                             3.11.   Literature                          57


                                      3. I.  Patterns  of nuclear stability


                There are approximately 275 different nuclei which have shown no evidence of radioactive
               decay and, hence,  are said to be stable with respect to radioactive decay. When these nuclei
               are compared for their constituent nucleons, we find that approximately 60 % of them have
               both  an even number of protons and an even number of neutrons (even-even nuclei).  The
               remaining  40%  are  about  equally  divided  between  those  that  have  an  even  number  of
               protons and  an odd number of neutrons (even-odd nuclei) and  those with  an odd number
               of protons and an even number of neutrons (odd-even nuclei). There are only 5 stable nuclei
               known which have both  an odd number of protons and odd number of neutrons  (odd-odd
                                         50
               nuclei); 2H, 6Li,  I~   I~N, and 23 V.  It is significant that the first stable odd-odd nuclei are
               abundant in the very light elements (the low abundance of 12H has a special explanation,  see
               Ch.  17).  The  last nuclide  is  found  in  low  isotopic  abundance  (0.25 %)  and  we  cannot  be
               certain  that  this nuclide  is not unstable  to radioactive decay with extremely long half-life.
                Considering  this  pattern  for  the  stable  nuclei,  we  can  conclude  that  nuclear  stability  is
               favored  by  even  numbers  of protons  and  neutrons.  The  validity  of this  statement  can  be
               confirmed further by considering for any particular element the number and types of stable
               isotopes;  see  Figure  3.1.  Elements  of even atomic number  (i.e.  even number of protons)
               are  characterized  by  having  a  relatively  sizable  number  of  stable  isotopes,  usually  3  or
               more.  For  example,  the  element  tin,  atomic  number  50,  has  10  stable  isotopes  while


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