Several common elementary methods of computing molecular properties, p
rerequisite to molecular dynamics studies, are tested for their validi
ty for CS2+. Judged sufficiently accurate, these methods are then used
to aid in investigating the collisionally activated dissociation of C
S2+ upon impact with xenon. Rice-Ramsperger-Kassel-Marcus (RRKM) unimo
lecular decay rate calculations are presented and compared to experime
ntal studies employing collisional activation. RRKM theory is shown to
reproduce the experimental results for collision energies near thresh
old. When corrected for vibrational anharmonicity, the RRKM calculatio
n shows agreement with the experimental results over a slightly wider
range of energies. A discussion is given on the applicability of the '
'adiabatic criteria'' to describing electronic excitations in the coll
isional activation process. This model is shown to provide a better de
scription of the activation process than direct vertical excitation.