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A COUPLED MCSCF-PERTURBATION TREATMENT OF ELECTRONIC SPECTRA           49

                        4.3.   RESULTS AND DISCUSSION
                         The analysis of the variational wavefunctions clearly shows  admixtures of valence and
                         Rydberg characters in many states, either at the orbital level or at the CI level. We will not
                         discuss this point here, but will focuse on transition energies.
                        The transition energies  from the ground  state to the  lowest 60 vertical  excited states
                        considered in this study are reported in Table 2 (30 singlets) and in Table 3 (30 triplets)
                         where they  are compared to the  avalaible  experimental results and to some  previous
                         theoretical calculations [45,60,65,68].
                         It is  immediately  seen  that the  agreement of our  computed  values  with  experimental
                         transitions is excellent for both valence and Rydberg states. The discrepancies vary from
                        0.00 eV to 0.40 eV for the largest of them. An exact value of the deviation is however
                        difficult to obtain due to both the experimental band widths and the fact that many observed
                         transitions are not  necessary vertical  so  that structural  effects  and  vibrational shifts are
                         involved. However, the calculated root-mean-square deviation of the computed values from
                         their experimental assignment is found to be, for the whole spectrum, about   . To
                         our knowledge, there has been no report, whatever might have been the theoretical method
                         used, of such a small deviation between theory and experiment when dealing with so many
                        excited states together.

                         Within a few exceptions, all singlet states can be correlated to an observed experimental
                         feature. Especially, the high density of states around 11.8 and  12.7 eV is compatible with
                         the observation of unresolved broad peaks in the  11.6-11.9 eV and  12.5-12.8 eV spectral
                         intervals [60]. Unfortunately, the lack of spectroscopic resolution makes any unambiguous
                         one-to-one assignment impossible in these regions.
                        The situation is more favorable at lower energies: up to about 11 eV, each calculated singlet
                         state correlates unambiguously to a well-resolved experimental line, and the deviation from
                        the experiment does  not  exceed  0.35 eV which  is the  largest discrepancy  observed.
                        Compared to the calculations by Harding and Goddard [60], the agreement between both
                         methods is excellent. Each state reported by these authors is found in our calculations. In
                         addition, we report some new singlet states of Rydberg character whose description has
                        been made  possible essentially because of the  larger  flexibility of both our  MCSCF
                        calculation and one-particle space (basis set including semi-diffuse orbitals that were not in
                        reference [60]). Our calculations provide a clear-cut assignment for the
                                                          states which were not reported previously. It is
                         important to notice that most of these new states correlate to the recent experimental results
                        obtained in the study by Brint and Sommer [62] which is devoted to the Rydberg series. It
                         is worth to emphasize that all their lower terms of the ns (3 states), np (6 states) and nd (4
                        terms) series can be related to a calculated state. Getting a correct description of the higher
                        terms of these series would however require the inclusion of a Rydberg orbital progression
                         in the basis set, so as the consideration of f functions as suggested in reference [62].
                        The same comments apply to the triplet states, although comparison to experiments is more
                        difficult due to the  lack of experimental determinations, even  in the  low energy  region.
                         However, as seen in Table 3, the agreement with avalaible data is excellent, and shows the
                         same quality  as for singlet states.  So  is  the correlation with the  results by  Harding and
                        Goddard [60].  In the triplet manifold, as  in the singlet one, the  largest flexibility of the
                        present method allows for more states to be found: as an example, we tentatively assign the
                             or the    state, missing in reference [60], to a peak reported at 9.59 eV [69].
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