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9.3 Non-degenerate perturbation theory            239

                          Equation (9.12) has the form
                                            N
                                           X
                                               a ki x i ˆ 0,  k ˆ 1, 2, ... , N           (9:13)
                                            iˆ1
                        for which a trivial solution is x i ˆ 0 for all i. A non-trivial solution exists if,
                        and only if, the determinant of the coef®cients a ki vanishes


                                                a 11  a 12      a 1N


                                                a 21  a 22      a 2N
                                                                       ˆ 0




                                               a N1  a N2       a NN
                        This determinant or its equivalent algebraic expansion is known as the secular
                        equation. In equation (9.12) the parameters c i correspond to the unknown
                        quantities x i in equation (9.13) and the terms (H ki ÿ E S ki ) correspond to the
                        coef®cients a ki . Thus, a non-trivial solution for the N parameters c i exists only
                        if the determinant with elements (H ki ÿ E S ki ) vanishes

                                 H 11 ÿ E S 11  H 12 ÿ E S 12       H 1N ÿ E S 1N


                                H 21 ÿ E S 21  H 22 ÿ E S 22      H 2N ÿ E S 2N
                                                                                 ˆ 0      (9:14)




                               H N1 ÿ E S N1  H N2 ÿ E S N2      H NN ÿ E S NN
                          The secular equation (9.14) is satis®ed only for certain values of E . Since
                        this equation is of degree N in E , there are N real roots
                                             E 0 < E 1 < E 2 <     < E Nÿ1
                        According to the variation theorem, the lowest root E 0 is an upper bound to the
                                                                                   1
                        ground-state energy E 0 : E 0 < E 0 . The other roots may be shown to be upper
                        bounds for the excited-state energy levels
                                         E 1 < E 1 , E 2 < E 2 , ... , E Nÿ1 < E Nÿ1




                                        9.3 Non-degenerate perturbation theory

                        Perturbation theory provides a procedure for ®nding approximate solutions to
                               È
                        the Schrodinger equation for a system which differs only slightly from a system
                                                                                ^
                        for which the solutions are known. The Hamiltonian operator H for the system
                        of interest is given by
                                                   N
                                                " 2 X  1
                                         ^                2
                                         H ˆÿ            = ‡ V(r 1 , r 2 , ... , r N )
                                                          i
                                                2     m i
                                                   iˆ1
                        1  J. K. L. MacDonald (1933) Phys. Rev. 43, 830.
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