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10.2 Nuclear motion in diatomic molecules           277
                                                                           3
                                                               2
                                                                                        4
                            E (1)  ˆhnjV9jniˆ b 1 hnjqjni‡ b 2 hnjq jni‡ b 3 hnjq jni‡ b 4 hnjq jni
                             nJ
                                                                                         (10:46)
                                                 k
                        The matrix elements hnjq jni are evaluated in Section 4.4. According to
                        equations (4.45c) and (4.50e), the ®rst and third terms on the right-hand side of
                        (10.46) vanish. The matrix elements in the second and fourth terms are given
                        by equations (4.48b) and (4.51c), respectively. Thus, the ®rst-order correction
                        in equation (10.46) is
                                                            2
                             (1)     " ÿ     1     3   "      2       1
                           E nJ  ˆ b 2  ìù  n ‡  2  ‡ b 4  2 ìù  n ‡ n ‡  2

                                    2                            2      h           i
                                  6B ÿ     1           1    "     (4)   ÿ    1  2  1
                                    e
                               ˆ       n ‡   J(J ‡ 1) ‡          U (0) n ‡       ‡       (10:47)
                                  "ù       2            16 ìù                 2    4
                        where equations (10.40), (10.45b), and (10.45d) have been substituted.
                                                                           3
                          Since the perturbation corrections due to b 1 q and b 3 q vanish in ®rst order,
                        we must evaluate the second-order corrections E (2)  in order to ®nd the
                                                                        nJ
                        in¯uence of these perturbation terms on the nuclear energy levels. According
                        to equation (9.34), this second-order correction is
                                                 3   2
                                 X   hkjb 1 q ‡ b 3 q jni
                         (2)
                        E   ˆÿ
                         nJ               (0)   (0)
                                k(6ˆn)  E k  ÿ E n
                                               2                        3                 3   2
                                   X    hkjqjni          X   hkjqjnihkjq jni    2  X  hkjq jni
                                 2
                            ˆÿb                  ÿ 2b 1 b 3                 ÿ b
                                 1     (k ÿ n)"ù                (k ÿ n)"ù       3     (k ÿ n)"ù
                                  k(6ˆn)                 k(6ˆn)                  k(6ˆn)
                                                                                         (10:48)
                        where the unperturbed energy levels are given by equation (4.30). The matrix
                                                                                             (2)
                        elements in equation (10.48) are given by (4.45) and (4.50), so that E nJ
                        becomes
                                 b 2    (n ‡ 1)"  n"
                         (2)      1
                        E nJ  ˆÿ  "ù  2ìù    ÿ 2ìù
                                      "                                                   #
                                                   1=2           3=2         1=2        3=2
                                2b 1 b 3  (n ‡ 1)"      (n ‡ 1)"        n"         n"
                              ÿ                      3              ÿ          3
                                 "ù        2ìù           2ìù           2ìù        2ìù
                                           3
                                 b 2     "      (n ‡ 1)(n ‡ 2)(n ‡ 3)
                              ÿ   3                              ‡ 9(n ‡ 1) 3
                                "ù 2ìù                3

                                                                                n(n ÿ 1)(n ÿ 2)
                                                                            3
                                                                        ÿ9n ÿ
                                                                                      3
                        This equation simpli®es to
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