Page 323 - Academic Press Encyclopedia of Physical Science and Technology 3rd Analytical Chemistry
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 Encyclopedia of Physical Science and Technology  EN009N-447  July 19, 2001  23:3






               840                                                                          Microwave Molecular Spectroscopy


               TABLE XXV Relative Second-Order Stark Shifts for Linear  (if present). The contribution of each component has the
               Molecules a                                       form
                                          2
                       Value of ∆[J(J + + 1) − − 3M ]/J(J + + 1)(2J − − 1)(2J + + 3)     (2)    2  2     2
                                     for various M                      E g  Jτ M  = µ   A J,τ + B J,τ M ,  (111)
                                                                                   g
                          0      1       2      3       4        where A and B are called Stark coefficients and depend
                                                                 on J, τ, and the inertial asymmetry κ. Though simple
               J = 0 → 1  0.5333  —      —      —       —        expressions cannot be given for these coefficients, they
               J = 1 → 2  −0.1524  0.1238  —    —       —        may be calculated from second-order perturbation theory
               J = 2 → 3  −0.0254  −0.0071  0.0476  —   —        and knowledge of the direction cosine matrix elements in
               J = 3 → 4  −0.0092  −0.0056  0.0052  0.0288  —    the asymmetric rotor basis. They have been tabulated for
               J = 4 → 5  −0.0044  −0.0033  −0.0001  0.0054  0.0165  low J. Once these quantities are specified, the second-
                                                                 order Stark energy may be calculated from Eq. (111).
                 a  Multiply entry by (0.50344) µ   /2B to obtain the shift of the
                                     2 2 2
               Stark component from the undisplaced line.          With asymmetric rotors, the possibility of degeneracies
                                                                 or near degeneracies exists, and in this case the above
                                                                 second-order expression does not apply. Near degenera-
               The perturbation connects adjacent J states. Evaluation  cies often occur between asymmetry doublets. For J = 2
               of the direction cosine matrix elements in the basis |J, M)  and a near-prolate rotor, for instance, the pair of levels
               and the energy level differences gives            2 1,2 ,2 1,1 or 2 2,1 ,2 2,0 interact via µ a , and this interaction

                    (2)            2                             is very large if the levels are very close together. Ordinary
                 E       = (0.50334)
                      J,M
                                                                 second-order perturbation theory then fails. Thus a transi-
                               2
                              µ   2  "  J(J + 1) − 3M 2  #       tion involving a level that can interact with a nearby level
                           ×                              ,      does not exhibit a typical second-order effect. To a good
                              2B    J(J + 1)(2J − 1)(2J + 3)
                                                                 approximation, these levels may be separated from the
                                                 J  = 0  (109)   other levels, and the problem can be treated by standard
                                                                 methods of quantum mechanics as a two-level system.
               In addition, for J = 0 and M = 0, we have                           0  0
                                                                 Consider two levels ψ , ψ that are eigenfunctions of the
                                                                                      2
                                                                                   1
                                                                                                              0
                                                                                                        0
                        (2)              2  2  2                 unperturbed Hamiltonian   0 with eigenvalues E and E .
                                                                                                        1
                                                                                                             2
                      E    J=0  =−(0.50344) µ   /6B.    (110)    The complete Hamiltonian is   =   0 +     , with     the
               The Stark splitting  ν (2)  depends on the difference of  perturbation. In the basis of   0 , there are no off-diagonal
                                                                 elements from   0 and no diagonal elements for     . The
               the bracket term in Eq. (109) for the two levels involved
                                                                 secular determinant thus has the form
               in the transition. Table XXV gives the difference in the
               bracket term for some J → J + 1, M → M transitions.              E − E
                                                                                0

                                                                                1        µ 12
               It follows from the table that Stark components can oc-                  0       = 0,       (112)
                                                                                 µ 12  E − E

                                                                                        2
               cur on both the high- and low-frequency sides of the un-
               perturbed line. For the J = 2 → 3 transition, two low-  where µ 12   = (1|    |2). The roots are
               frequency Stark lobes and one high-frequency lobe are
                                                                         1     0  0     1      0  0   2  2  2    1/2
               predicted and observed for OCS in Fig. 3. Furthermore,  E 1,2 =  E + E  ±  E + E  + 4  µ     ,
                                                                         2  1    2   2   1    2        12
               the magnitude of the splitting decreases with increasing
                                                                                                           (113)
               J, and the largest high-frequency displacement occurs
               for M = J. As a quantitative example, consider OCS,  with E > E ; the plus sign is used for E 1 and the negative
                                                                       0
                                                                           0
                                                                       1
                                                                           2
               where 2B = 12,162.97, µ = 0.715 D, and a large field  sign for E 2 . When (E − E ) > 4  µ , the above can be
                                                                                              2
                                                                                       0 2
                                                                                  0
                                                                                                2
                                                                                                12
                                                                                       2
                                                                                  1
                 = 2800 V/cm. For the J, M = (2, 2) → (3, 2) transition,  expanded to give a second-order effect:
               we find  ν (2)  = 4 MHz, which is easily observable but
                                                                                         2
               quite small compared with a first-order effect.                      0   µ    2
                                                                                         12
                                                                             E 1 = E +        +· · · ,     (114)
                                                                                   1
                                                                                        0
                                                                                       E − E  0
                                                                                        1    2
               B. Asymmetric-Top Molecules
                                                                                         2
                                                                                       µ    2
                                                                                   0     12
               For an asymmetric rotor, the analysis basically follows       E 2 = E −  0    0  +· · · .   (115)
                                                                                   2
                                                                                       E − E 2
                                                                                        1
               the same procedure; however, the details require more
               space than possible in the scope of this presentation. The  Note, however, that the second-order effect could be rather
               Stark effect is usually second order, and the Stark energy  large if the energy denominator is small. If the perturbation
                                                                                         2
                                                                                      2
                                                                               0 2
                                                                          0
               contains contributions from all three dipole components  is large, (E − E ) < 4µ   , then
                                                                          1    2      12
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