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P. 68

2.7 Particles in three dimensions               59

                        where the gradient operator = is de®ned as
                                                       @     @      @
                                                 =   i   ‡ j    ‡ k
                                                       @x    @ y    @z
                        Using these relations, we may express the Hamiltonian operator in three
                        dimensions as
                                                       ÿ" 2
                                                   ^         2
                                                  H ˆ      = ‡ V(r)
                                                        2m
                                                    2
                        where the laplacian operator = is de®ned by
                                                           @ 2   @ 2   @ 2
                                               2     .
                                             =   = = ˆ        ‡     ‡
                                                          @x 2  @ y 2  @z 2
                                                 È
                          The time-dependent Schrodinger equation is
                                          @Ø(r, t)
                                                     ^
                                       i"         ˆ HØ(r, t)
                                             @t
                                                     ÿ" 2
                                                          2
                                                  ˆ      = Ø(r, t) ‡ V(r)Ø(r, t)          (2:68)
                                                     2m
                        The stationary-state solutions to this differential equation are
                                                Ø n (r, t) ˆ ø n (r)e ÿiE n t="           (2:69)

                        where the spatial functions ø n (r) are solutions of the time-independent
                            È
                        Schrodinger equation
                                          ÿ" 2
                                                2
                                              = ø n (r) ‡ V(r)ø n (r) ˆ E n ø n (r)       (2:70)
                                           2m
                        The most general solution to equation (2.68) is

                                                       X           ÿiE n t="
                                              Ø(r, t) ˆ    c n ø n (r)e                   (2:71)
                                                         n
                        where c n are arbitrary complex constants.
                          The expectation value of a function f (r, p) of position and momentum is
                        given by

                                                   …
                                                                 "

                                        hf (r, p)iˆ Ø (r, t) f r,  = Ø(r, t)dr            (2:72)
                                                                  i
                        Equivalently, expectation values of three-dimensional dynamical quantities
                        may be evaluated for each dimension and then combined, if appropriate, into
                        vector notation. For example, the two Ehrenfest theorems in three dimensions
                        are
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