The excitation spectra of the 15V 31 344.9 band of the CS2 V B-1(2)<-- X (1
)Sigma(g)(+) transition and the changes in these spectra with the applicati
on of a magnetic field of up to 12 kG have been measured with sub-Doppler r
esolution. The radiative lifetimes of rotationally resolved single lines an
d single Zeeman components were measured under collision-free conditions. A
ll of the fluorescence decays were observed to be of a single exponential.
Large Zeeman splittings were observed for many lines. The only symmetry all
owed spin-orbit interaction is that of the (3)A(2)(B-2) component with the
B-1(2) state. The (3)A(2)(B-2) component has no magnetic moment, but a magn
etic moment is induced when it is mixed with the (3)A(2)(A(1),B-1) componen
ts. The mixing of the (3)A(2)(B-2) and (3)A(2)(A(1),B-1) components is faci
litated by spin-rotation interaction and the Zeeman interaction. From analy
sis of the observed Zeeman splittings of the perturbed levels, the (3)A(2)(
B-2) component was determined to lie 14 cm(-1) below the nearly degenerate
(3)A(2)(A(1)) and (3)A(2)(B-1) components in the energy region where the 15
V band is observed. Irregular energy shifts and splittings of rotational li
nes were observed, and these were attributed to (a) Coriolis interaction be
tween the (VB2)-B-1(v(')(a(1));K=0JM) and V B-1(2)(v(b(2));K=1JM) levels an
d (b) resonant spin-orbit interaction between the rotational levels V B-1(2
)(v(')(a(1));KJM) and R (3)A(2)(v(a(1));KJM). These interactions become app
reciable when two levels lie close in energy. Large Zeeman splittings were
observed in case (b). Many vibrational lines with irregular intensity and s
pacing were observed in each band. These were attributed to (c) Fermi reson
ance between the vibrational levels in the V B-1(2) state and (d) resonant
spin-orbit interaction between vibrational levels in the V B-1(2) and R (3)
A(2) states. In case (d), large Zeeman splittings were observed for a serie
s of rotational lines in a vibrational band. The background lines were iden
tified from observed Zeeman splittings as the transitions to levels of the
R (3)A(2) state, which are induced by resonant spin-orbit interaction with
the levels of the V B-1(2) state. The intensity of the excitation spectrum
of the V B-1(2)<-- X(1)Sigma(g)(+) transition was observed to decrease as t
he magnetic field increases. This was attributed to a mixing of the (3)A(2)
state with the V B-1(2) state and the resulting triplet-triplet emission,
which was not detected in this experiment. It was possible to evaluate the
lifetime of the radiative triplet-triplet emission via deperturbation analy
sis of the perturbed lines. (C) 2000 American Institute of Physics. [S0021-
9606(00)00525-0].