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UNIT 2
               MODULE 3: ATOMIC AND NUCLEAR PHYSICS (cont’d)


                SPECIFIC OBJECTIVES                  EXPLANATORY NOTES          SUGGESTED  PRACTICAL
                                                                                ACTIVITIES

                3.       Atomic Mass

                Students should be able to:

                3.1.     define  ‘mass  defect’  and  Nuclear  Stability  should  be
                         ‘binding energy’;          mentioned.     Refer   to
                                                    Specific Objective 4.1.

                3.2.     calculate  mass  defect  and  Explanation   of   the
                         binding  energy  in  eV  or  relevance of binding energy
                         joules;                    per nucleon to nuclear
                                                    fusion  and  to  nuclear
                                                    fission.

                3.3.     use    the     relationship  Include   calculation   of
                         between energy and mass in  energy  release  in  fission,
                         nuclear reactions          fusion or nuclear decay.
                                       2
                          ΔE  =  Δm  c   to  solve
                         problems;                  Sketch a labelled diagram to
                                                    illustrate a chain reaction.

                3.4.     use  the  atomic  mass  unit   Brief  account  of  early
                         (u) as a unit  of energy;   theories    of    atomic
                                                    structure, including those of
                                                    Thomson,     Bohr     and
                                                    Rutherford,        should
                                                    introduce this section.

                3.5.     represent     graphically     the     Mention   “Island   of
                         relationship     between  instability”.
                         binding  energy  per  nucleon
                         and nucleon number;

                3.6.     compare  the  values  of  Nuclear  fusion  is  the
                         binding  energy  per  nucleon  process  by  which  stars
                         when  undergoing  nuclear  release    energy     and
                         fission or fusion;         elements  are  made,  for
                                                    example, H -> He.













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