Fa. Gianturco et al., COMPUTED DISTRIBUTIONS OF ROTOVIBRATIONAL TRANSITIONS IN LIH(X(1)SIGMA(+)) AND LIH+(X(2)SIGMA(+)), Astronomy & Astrophysics. Supplement series, 117(2), 1996, pp. 377-392
Accurate potential energy curves for the ground electronic states of L
iH and LiH+ are employed to generate vibrational and rotational levels
over a broad range of J values for both systems. The corresponding di
pole functions are computed and used to obtain the frequency and inten
sity distributions of all relevant transitions between bound states fo
r pure vibrational excitations, pure rotational excitations and for di
pole allowed rovibrational processes. This extensive set of absorption
data for both molecules is employed to locate the most likely region
in the infrared spectrum where characteristic lines could be observed.
Such data should be useful in experimental attempts to search for LiH
and LiH+ lines at high redshifts. We found that transitions between i
onic levels will be markedly less intense than those for the neutral s
ystem and that transitions between rotationally 'hot' levels will be m
arkedly more intense than those between low-J levels.