Page 58 - Radiochemistry and nuclear chemistry
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Nuclear Mass and Stability                    47


               nuclear reaction formulas and energies refer to single atoms (or molecules), while chemical
               reactions  and equations  refer  to number of moles;  we have:

                      1 eV/molecule  =   1.6022  •  10-19  x  6.0221  •  1023 =  96.48  kJ mole- 1  =
                                       3.8268  •  10 -2o  •  6.0221  •  1023 =  23.045  kcal  mole -1

               Thus,  the  formation of deuterium  from a neutron and a hydrogen atom would  lead  to  the
               liberation of 214.6  •  106 kJ (51.3  •  106 kcal) for each mole of deuterium atoms formed.
               By  comparison,  then,  the  nuclear  reaction  leading  to  the  formation  of  deuterium  is
               approximately  half a  million  times  more  energetic  than  the  chemical  reaction  leading  to
               formation of CO 2.
                It is  not  common practice  to use mole quantities  in considering  nuclear  reactions  as  the
               number  of  individual  reactions  under  laboratory  conditions  is  well  below  6.02  •  1023.
               Therefore,  in nuclear science one uses the energy and mass changes involved in the reaction
               of individual  particles  and nuclei.



                                           3.4.  Binding energy

                The energy  liberated m  the formation of CO 2 from the elements,  the heat of formation,
               is a measure of the stability of the CO 2 molecule.  The larger the heat of formation the more
               stable  the  molecule  since the  more energy  is required  to decompose  the molecule  into  its
               component  atoms.  Similarly,  the  energy  liberated  in  the  formation  of a  nucleus  from  its
               component nucleons is a measure of the stability of that nucleus.  This energy is known as
               the  binding energy (En)  and  has  the  same  significance  in  nuclear  science  as  the  heat  of
               formation  has  in  chemical  thermodynamics.  We  have  seen  that  the  binding  energy  of
               deuterium  is  2.22  MeV.  The  ~He nucleus  is composed of 2 neutrons  and  2  protons.  The
               measured  mass of the 4He atom is 4.002  603  u.  The  mass defect  is:

              AM'He =  MHe  -- 2 M H -  2 M n =  4.002603-2 •  1.007825-2 •  1.008665  =  -0.030377  u

                The binding  energy between  the nucleons  in a nucleus  follows the simple relation

                                       E B (MeV)  =  -931.5 AM A (u)                 (3.5)

               which is just another form of eqn.  (3.3).  Thus the binding energy for 4He is 28.3  MeV.  It
               is quite unlikely that 2 neutrons  and 2 protons would ever collide simultaneously to  form
               a 4He nucleus;  nevertheless,  this calculation is useful because it indicates that to break 4He
               into  its basic  component nucleons would  require at least 28.3  MeV.
                A better indication of the relative stability of nuclei  is obtained when the binding energy
               is divided by  the total number of nucleons  to give the binding energy per nucleon, EB/A.
               For 4He  the  value of EB/A is 28.3/4  or 7.1  MeV,   whereas  for  H  it  is  1.11  for the bond
                                                                   2
               between  the  two  nucleons.  Clearly,  the  4He nucleus  is  considerably  more  stable  than  the
               2H  nucleus.  For  most  nuclei  the  values  of EB/A vary  in  the  rather  narrow  range  5  -  8
               MeV.  To a first approximation,  therefore, EB/A is relatively constant which means that the
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