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Infrared and Molecular Dynamics Study of D2O
Rotational Relaxation in Supercritical CO2
and Xe
LE Bowman,
BJ Palmer, BC Garrett, JL Fulton, CR Yonker, DM Pfund, and SL
Wallen. J. Phys. Chem. 100(47):18327-18334 (1996).
Abstract: Supercritical fluid solvents allow continuous
turning of solvent density and therefore continuous control of the
number and distance of solvent-solute interactions. Such interactions
exert torque on molecules in solution and thereby influence the
way in which the rotational orientation 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 interactions between the solute
and solvent. Since the nonelectrostatic interactions of D2O
are very nearly centrosymmetric about the center of mass, Xe is
expected to exert little torque on the rotating solute until liquid
densities are reached. For D2O
dissolved in CO2, the dipole-quadrupole
interaction can exert torque on the rotating D2O,
thereby hindering its rotation. Molecular dynamics simulations of
these systems were used to calculate dipole autocorrelation functions
containing only contributions from the solute rotational motion.
These were then used to predict the rotation wings of the asymmetric
stretching band, v3, of D2O. Infrared
spectra for this band were obtained in both solvents at 110.0°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 rotation of D2O was
increasingly hindered as the solvent density was increased from
gas-like to liquid-like densities. At low densities the correlation
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 exhibited simple, monotonic decay,
indicating a persistence in the direction of the vector with time
and substantially hindered rotation.
For information about supercritical fluid capabilities at PNNL, please contact Clement Yonker, at (509) 372-4748, clem.yonker@pnl.gov.
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