Page 57 - Electrical Properties of Materials
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40                            The electron

                                   and this is nothing else but our good old wave solution, at least as a function
                                   of time, if we equate

                                                              E =  ω.                       (3.12)
                                   This is actually something we have suggested before [eqn (2.27)] by recourse
                                   to Planck’s formula. So we may call E the energy of the electron. However,
                                   before making such an important decision let us investigate eqn (3.10) which
                                   also contains E. We could rewrite eqn (3.10) in the form:
                                                            2
                                                               2
                                                         –   ∇ + V ψ = Eψ.                  (3.13)
                                                          2m
                                     The second term in the bracket is potential energy, so we are at least in
                                                                    2
                                   good company. The first term contains ∇ , the differential operator you will
                                   have met many times in electrodynamics. Writing it symbolically in the form:

                                                            2  2  1      2
                                                         –  ∇ =     (–i ∇) ,                (3.14)
                                                          2m     2m
                                   we can immediately see that by introducing the new notation,

                                                              p =–i ∇,                      (3.15)
                                   and calling it the ‘momentum operator’ we may arrive at an old familiar
                                   relationship:
                                                          p 2
                                                             = kinetic energy.              (3.16)
                                                         2m
                                   Thus, on the left-hand side of eqn (3.13) we have the sum of kinetic and
                                   potential energies in operator form and on the right-hand side we have a con-
                                   stant E having the dimensions of energy. Hence, we may, with good conscience,
                                   interpret E as the total energy of the electron.
                                     You might be a little bewildered by these definitions and interpretations, but
                                   you must be patient. You cannot expect to unravel the mysteries of quantum
                                   mechanics at the first attempt. The fundamental difficulty is that first steps in
                                   quantum mechanics are not guided by intuition. You cannot have any intuitive
                                   feelings because the laws of quantum mechanics are not directly experienced
                                   in everyday life. The most satisfactory way, at least for the few who are math-
                                   ematically inclined, is to plunge into the full mathematical treatment and leave
                                   the physical interpretation to a later stage. Unfortunately, this method is lengthy
                                   and far too abstract for an engineer. So the best we can do is to digest alternately
                                   a little physics and a little mathematics and hope that the two will meet.

                                   3.4  The electron as a wave
                                   Let us look at the simplest case when V = 0 and the electron can move only
                                   in one dimension. Then eqn (3.13), which is often called the time-independent
                                   Schrödinger equation, reduces to
                                                              2
                                                            2
                                                            ∂ ψ
                                                                 + Eψ = 0.                  (3.17)
                                                          2m ∂z 2
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