Ab. Alekseyev et al., THEORETICAL-STUDY OF THE ENERGIES AND LIFETIMES OF THE LOW-LYING STATES OF BISMUTH FLUORIDE, Chemical physics, 173(3), 1993, pp. 333-344
A series of CI calculations has been carried out for various low-lying
electronic states of the bismuth fluoride molecule by employing relat
ivistic effective core potentials including spin-orbit effects. It is
found that the lowest 0+ excited state (A0+) of this system contains a
large contribution from the pi --> sigma* 3PI lambda-s state, especi
ally at bond distances which are equal to or greater than the equilibr
ium value for the X(1)0+ ground state. The B0+ state at somewhat highe
r energy is found to contain the largest portion of the b1SIGMA+ chara
cter arising from the pi4pi2 configuration, in disagreement with earl
ier calculations by Balasubramanian who only reports a single excited
state of this (0+) symmetry. Results of the latter study for the X(1)0
+, X(2)1 and a2 states of lower energy are in good agreement with thos
e of the present work, however. The relatively large r(e) value observ
ed for the A0+ state is quite consistent with the present theoretical
description, as well as the correspondingly lower vibrational frequenc
y compared to that of X(1)0+. Radiative lifetimes have also been obtai
ned for a number of excited states and the results are found to be in
reasonably good agreement with recent measured data. An explanation is
also provided for the anomalous mu0/mu1 ratio for the A0+ --> X trans
itions, again based on the large amount of 3PI character in the upper
state. The present data also provide a clear assignment for the A' and
A'' states recently found for this system (OMEGA = 1 and 0-) respecti
vely. The lifetime of the X(2)1 state is computed to be 1.05 ms and a
zero-field splitting of 6937 cm-1 is obtained, both of which results a
re in good agreement with the corresponding measured values of 1.4 ms
and 6768 cm-1. The next-lowest-energy state (a2) is predicted to have
a lifetime which is 80 times larger, a result which is consistent with
the failure to date to observe emission bands initiating from this st
ate.