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2.7 Particles in three dimensions               57

                        so that T and R become
                                              16E(V 0 ÿ E)  ÿ2a p 
                                                                2m(V 0 ÿE)="
                                          T                e
                                                   V 2
                                                     0
                                                  16E(V 0 ÿ E)  ÿ2a p 
                                                                    2m(V 0 ÿE)="
                                          R   1 ÿ        2     e
                                                       V  0
                        In the limit as a !1,as V 0 !1,as m !1, or any combination, the
                        transmission coef®cient T approaches zero and the re¯ection coef®cient R
                        approaches unity, which are the classical-mechanical values. We also note that
                        in the limit " ! 0, the classical values for T and R are obtained.
                          Examples of tunneling in physical phenomena occur in the spontaneous
                        emission of an alpha particle by a nucleus, oxidation±reduction reactions,
                        electrode reactions, and the umbrella inversion of the ammonia molecule. For
                        these cases, the potential is not as simple as the one used here, but must be
                        selected to approximate as closely as possible the actual potential. However,
                        the basic qualitative results of the treatment here serve to explain the general
                        concept of tunneling.



                                            2.7 Particles in three dimensions

                        Up to this point we have considered particle motion only in the x-direction.
                        The generalization of Schrodinger wave mechanics to three dimensions is
                                                  È
                        straightforward. In this section we summarize the basic ideas and equations of
                        wave mechanics as expressed in their three-dimensional form.
                          The position of any point in three-dimensional cartesian space is denoted by
                        the vector r with components x, y, z, so that
                                                    r ˆ ix ‡ jy ‡ kz                      (2:60)
                        where i, j, k are, respectively, the unit vectors along the x, y, z cartesian
                        coordinate axes. The linear momentum p of a particle of mass m is given by

                                      dr        dx    dy    dz
                                p ˆ m    ˆ m i    ‡ j    ‡ k     ˆ ip x ‡ jp y ‡ k p z    (2:61)
                                      dt        dt    dt    dt
                        The x-component, p x , of the momentum now needs to carry a subscript,
                        whereas before it was denoted simply as p. The scalar or dot product of r and
                        p is
                                               .      .
                                              r p ˆ p r ˆ xp x ‡ yp y ‡ zp z
                        and the magnitude p of the vector p is
                                                                       2 1=2
                                                                  2
                                                  .
                                                             2
                                            p ˆ (p p) 1=2  ˆ ( p ‡ p ‡ p )
                                                             x    y    z
                        The classical Hamiltonian H(p, r) takes the form
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