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4.2 Quantum treatment                       109
                                        P(y)













                                           21                        y     1
                                Figure 4.1 Classical probability density for an oscillating particle.



                                                4.2 Quantum treatment
                        The classical Hamiltonian H(x, p) for the harmonic oscillator is

                                                    p 2          p 2       2 2
                                                                      1
                                          H(x, p) ˆ    ‡ V(x) ˆ     ‡ mù x                (4:11)
                                                    2m           2m   2
                                                 ^
                        The Hamiltonian operator H(x, ^ p) is obtained by replacing the momentum p
                        in equation (4.11) with the momentum operator ^ p ˆÿi" d=dx
                                                                2
                                             ^ p 2             " d  2
                                        ^         1    2 2              1   2 2
                                        H ˆ     ‡ mù x ˆÿ             ‡ mù x              (4:12)
                                             2m   2            2m dx 2  2
                        The Schrodinger equation is, then
                                È
                                                 2
                                              2
                                             " d ø(x)    1   2 2
                                          ÿ           ‡ mù x ø(x) ˆ Eø(x)                 (4:13)
                                                         2
                                            2m dx  2
                          It is convenient to introduce the dimensionless variable î by the de®nition
                                                               1=2
                                                          mù
                                                    î ˆ           x                       (4:14)
                                                           "
                        so that the Hamiltonian operator becomes

                                                       "ù        d 2
                                                  ^          2
                                                  H ˆ       î ÿ                           (4:15)
                                                        2       dî 2
                        Since the Hamiltonian operator is written in terms of the variable î rather than
                        x, we should express the eigenstates in terms of î as well. Accordingly, we
                        de®ne the functions ö(î) by the relation
                                                               1=4
                                                           "
                                                 ö(î) ˆ          ø(x)                     (4:16)
                                                          mù
                        If the functions ø(x) are normalized with respect to integration over x
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