ABSTRACT
Gas-phase emission spectra of the hitherto unknown free radical BiNa have been measured in the NIR range with a Fourier transform spectrometer. The emissions were observed from a fast-flow system in which bismuth vapor in argon carrier gas was passed through a microwave discharge and mixed with sodium vapor in an observation tube. Two systems of blue-degraded bands observed in the ranges 8900-9800 and 7200-7800 cm(-1) were measured at high spectral resolution and vibrational and rotational analyses were performed. To aid in the analysis of the experimental data, a series of relativistic configuration interaction calculations has been carried out to obtain potential curves for the low-lying states of BiNa and also electric dipole transition moments connecting them. As in the isovalent BiH system, the ground state of BiNa is found to be X(3)Sigma(-) with a spin splitting of about 1769 cm(-1). The first excited state is A(3)Pi, and the observed band systems are assigned to the transitions A(3)Pi(A(2)0(+)) --> X(3)Sigma(-)(X(1)0(+), X(2)1). Comparison with earlier work on the isovalent BiH system emphasizes that the relative weakness of the varsigma MO in BiNa is responsible for qualitative differences in the electronic spectra of these two systems. Copyright 2000 Academic Press.
ABSTRACT
The Ã(2)A' --> &Xtilde;(2)A" electronic band system of HO(2) has been simulated in emission using an extended version of the program RENNER (P. Jensen, M. Brumm, W. P. Kraemer, and P. R. Bunker, J. Mol. Spectrosc. 171, 31-57 (1995)). The two electronic states involved in this transition have strongly bent equilibrium geometries but they correlate together to form a (2)Pi state at linearity. As a result the energy level pattern in the states is affected by electronic angular momentum effects (i.e., the Renner effect and spin-orbit coupling). To simulate the spectrum, we have calculated ab initio the potential energy surfaces, electric dipole moment surfaces, magnetic dipole moment surfaces, spin-orbit coupling parameter, and the electronic angular momentum matrix elements. Some of the forbidden DeltaK(a) = 0 transitions occurring in the spectrum are induced by the magnetic dipole transition moment, and the others are electric dipole transitions that gain intensity because of the Renner interaction, spin-orbit coupling, or because of rotation-vibration interaction. All of these effects are allowed for in our calculation. The electric dipole transition moment is very small (0.017 D at the ground state equilibrium geometry) and because of this the magnetic dipole transitions are quite visible; the strongest magnetic dipole transitions are calculated to be about 10 times weaker than the strongest electric dipole transitions. In this way previous experimental assignments (E. H. Fink and D. A. Ramsay, J. Mol. Spectrosc. 185, 304-324 (1997)) are confirmed theoretically. Copyright 1999 Academic Press.
ABSTRACT
Spin-orbit MRD-CI calculations have been carried out for the potential energy surfaces of the seven lowest-lying electronic states of the BiOH molecule by employing relativistic effective core potentials. The HBiO isomer is found to be 4020 cm-1 less stable because of its inability to form multiple Bi-O bands. A bent 3A" BiOH ground state is predicted, which is split into all three of its components by spin-orbit coupling. The calculated X2A"-X1A' splitting is computed to be 5217 cm-1, but the corresponding X3-X2 value is only 29 cm-1. Fink et al. have observed spectral bands which appear with a Te value of 6200 cm-1 which are likely caused by BiOH. Since calculations at the same level for BiF underestimate the observed X2-X1 spin-orbit splitting by 650 cm-1, it appears that the present calculations are consistent with this experimental assignment. A vibrational progression with a 500 cm-1 frequency is also observed and this result fits in well with the computed Bi-O stretch omegae value of 527 cm-1. The calculations also find a relatively large 1Delta splitting (600 cm-1) because of the bent BiOH geometry, with comparatively strong transitions to the X1A' ground state, and it is suggested that the experimental BiOH assignment can be confirmed on this basis. Much stronger transitions to the 1Delta component should also be observed in emission in the 10 000 cm-1 range. Copyright 1997 Academic Press. Copyright 1997Academic Press
