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44487-B4
Investigating the Molecular Interactions Between Solute and Cosolvent Molecules in Supercritical CO2
Steven G. Mayer, University of Portland
Project Activities
The ACS-PRF grant provided
me with salaries for two students for two summers as well as my salary for
three summers. The equipment funds were
used to acquire a Thermo Scientific 380 FT-IR spectrometer. This spectrometer in combination with a Raman
spectrometer that I purchased with a grant from the National Science Foundation, has been a tremendous asset to my research
program as well as to several of my colleagues at the University
of Portland, Portland State University, and a local
company. The proposed research requires
that a very large number of spectra be collected for the
solute-solvent/cosolvent systems under investigation and we have made excellent
progress toward that goal primarily due to the inherent efficiency of both the
FT-IR and the FT-Raman systems.
Furthermore, I have been able to allow guest researchers to collect
spectra with a relatively small time commitment, thus allowing me to make it
more widely available.
I began the summer 2008 research
with a new group of three undergraduate students. The first two weeks were devoted to training
the students on the equipment and explaining the overall scope of the
project. Given our success with observing
fundamental molecular interactions in solute/cosolvent systems, I decided to
investigate the interaction between CO2 and H2O. I
chose this current project in response to the intense interest, within the
scientific community, in understanding the fundamental molecular interactions
between CO2 and H2O.
Further knowledge of this system may lead to the development of new
technology to capture and sequester CO2. Our ability to observe changes in the
vibrational spectra of a molecule is a very sensitive technique for probing the
local environment. However, CO2
and H2O are essentially opaque in the infrared region of the
electromagnetic spectrum. To solve this
experimental problem, we designed a high-pressure flow cell for infrared
spectroscopy of gases, liquids, and supercritical fluids, specifically those
that have an extremely large absorption cross-section. The design is specific to the Thermo
Scientific Smart Orbit attenuated total reflectance (ATR) module that is part
of the Thermo 380 FT-IR spectrometer.
This cell will withstand pressures up to 35 MPa
(5130 psi); thereby, allowing us to duplicate the
pressures and temperatures of the deep ocean, where it has been proposed to
sequester CO2. The manuscript
reporting this design has been submitted to the marketing department at Thermo
Scientific for inclusion in their technical communication.
We used the high-pressure cell to
collect a series of infrared spectra in addition to the Raman spectra that were
collected simultaneously. The Table 2
lists the conditions at which spectra were collected.
Table 2: Mixtures of CO2 and H2O
for which Raman and infrared spectra have been collected at the specified
temperatures and 1500 p.s.i. pressure.
Concentration of CO2 in H2O | 279 K | 285 K | 295 K | 305 K | 315 K | 335 K |
90% | x | x | x | x | x | x |
80% | x | x | x | x | x | x |
70% | x | x | x | x | x | x |
60% | x | x | x | x | x | x |
50% | x | x | x | x | x | x |
40% | x | x | x | x | x | x |
30% | x | x | x | x | x | x |
20% | x | x | x | x | x | x |
10% | x | x | x | x | x | x |
Each entry in Table 2
consists of 10 separate spectra of 32 scans each at 1 cm-1 resolution. In this way, we can calculate the standard
error such that the peak shifts that we observed will be statistically
meaningful. Furthermore, for the 90% and
10% mixtures, spectra were collected at pressures from 1000 to 3000 p.s.i. in increments of 100 p.s.i.
at all six temperatures listed.
Findings
We were able to reproduce
the Raman spectra obtained by Sum, et al. (J. Phys.
Chem. B 1997, 101, 7371-7377) of CO2 incorporated into clathrate hydrates and then use the identical conditions to
collect infrared absorption spectra of these structures. We found that the enclathrated
CO2 exhibited rotational structure similar to gas phase CO2. Calculation of the rotational constant
suggests that the CO2 freely rotates inside the clathrate. We predicted this phenomenon based on a
suggestion by Consani and Pimentel in their paper on enclathrated C2D2 (J. Phys. Chem.,
1987, 91, 289-293). Furthermore, we
found that the infrared absorption spectra revealed that CO2 exists
in several different environments that are highly dependent upon the
concentration of CO2 in H2O, the temperature, and the mixing
time.
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