Le. Bowman et al., INFRARED AND MOLECULAR-DYNAMICS STUDY OF D2O ROTATIONAL RELAXATION INSUPERCRITICAL CO2 AND XE, Journal of physical chemistry, 100(47), 1996, pp. 18327-18334
Supercritical fluid solvents allow continuous tuning of solvent densit
y and therefore continuous control of the number and distance of solve
nt-solute interactions. Such interactions exert torque on molecules in
solution and thereby influence the way in which the rotational orient
ation of a solute molecule varies with time. In this work, we examine
the rotational relaxation of D2O in two supercritical fluid solvents:
Xe and CO2. In the former case, there are no electrostatic interaction
s between the solute and solvent. Since the nonelectrostatic interacti
ons of D2O are very nearly centrosymmetric about the center of mass, X
e is expected to exert tittle torque on the rotating solute until liqu
id densities are reached. For D2O dissolved in CO2, the dipole-quadrup
ole interaction can exert torque on the rotating D2O, thereby hinderin
g its rotation. Molecular dynamics simulations of these systems were u
sed to calculate dipole autocorrelation functions containing only cont
ributions from the solute rotational motion. These were then used to p
redict the rotation wings of the asymmetric stretching band, v(3), of
D2O. Infrared spectra for this band were obtained in both solvents at
110.0 degrees C as a function of density. In Xe, the experimental and
simulated correlation functions indicated that the solute was free to
rotate, even at the highest densities examined. In CO2, however, the r
otation of D2O was increasingly hindered as the solvent density was in
creased from gaslike to liquidlike densities. At low densities the cor
relation functions had negative minima, indicating a partial reversal
in the direction of the average transition dipole moment vector as the
molecules freely rotated. In CO2, at high densities the functions exh
ibited simple, monotonic decay, indicating a persistence in the direct
ion of the vector with time and substantially hindered rotation.