Page 62 - Radiochemistry and nuclear chemistry
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Nuclear  Mass  and  Stability                 51

              forces  gives  rise  to  the  effect  of  surface  tension.  Consequently,  the  negative  term  in  the
              mass  equation  reflecting  this  unsaturation  effect  should  be  similar  to  a  surface  tension
              expression.  (e)  Finally,  we  have  seen  that  nuclei  with  an  even  number  of  protons  and
              neutrons are more stable than nuclei with an odd number of either type of nucleon and that
              the  least  stable  nuclei  are  those  for  odd  numbers  of  both  neutrons  and  protons.  This
              odd-even effect  must also be included  in a  mass equation.
                Taking  into account  these various  factors,  we can write a semiempirical  mass equation.
              However,  it  is  often  more  useful  to  write  the  analogous  equation  for  the  mass  defect  or
              binding energy of the nucleus,  recalling (3.5).  Such an equation,  first derived by C.  F. von
              Weizs,~cker in  1935,  would have the  form:

                      EB(MeV)  =  avA  -  a a (N-   Z)2[A  -  a c Z  2[All3  -  as A2/3  •  asia 3/4   (3.8)

              The  first  term  in  this  equation  takes into  account the proportionality of the energy  to the
              total number  of nucleons  (the volume energy);  the second term,  the variations  in neutron
              and proton ratios (the asymmetry energy); the third term,  the Coulomb forces of repulsion
              for  protons  (the  Coulomb  energy);  the  fourth,  the  surface  tension  effect  (the  surface
              energy).  In  the  fifth term,  which accounts  for the odd-even effect,  a positive sign is used
              for even proton-even neutron nuclei and a negative sign for odd proton-odd neutron nuclei.
              For nuclei  of odd A (even-odd  or odd-even)  this  term has  the value  of zero.  Comparison
              of this equation with  actual  binding  energies of nuclei  yields a  set of coefficients;  e.g.

                            a v  =  15.5,  a a  =  23,  a c  =  0.72,  a s  =  16.8,  a~  =  34

              With  these coefficients the binding energy equations (3.2) and (3.5) give agreement within
              a  few percent  of the measured values  for most nuclei  of mass number greater than 40.
                When  the calculated  binding  energy is compared with  the experimental  binding energy,
              it is seen that for certain values of neutron and proton numbers,  the disagreement is more
              serious.  These  numbers  are  related  to  the  so-called  "magic  numbers",  which  we  have
              indicated  in  Figure  3.1,  whose  recognition  led  to  the  development  of  the  nuclear  shell
              model  described  in a  later chapter.



                                         3.7.  Valley of O-stability
                If the semiempirical  mass equation  is written as a function of Z,  remembering  that N  =
              A  -  Z,  it  reduces  to a quadratic  equation of the form

                                      E B  =  a Z  2  +  b Z  +  c  +  d/A 3/4      (3.9)

              where the terms a,  b and c also contain A.  This quadratic equation describes a parabola for
              constant values  of A.  Consequently,  we would expect  that  for any  family  of isobars  (i.e.
              constant A) the masses should fall upon a parabolic curve.  Such a curve is shown in Figure
              3.5.  In returning to Figure 3.1, the isobar line with constant A but varying Z cuts diagonally
              through  the  line  of  stable  nuclei.  We  can  picture  this  as  a  valley,  where  the  most  stable
              nuclei  lie at the bottom of it (cf.  Figs.  3.1  and 3.5),  while unstable nuclei lie up the valley
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