6106 J. Am. Chem. Soc., Vol. 120, No. 24, 1998
Ault
reactants, each diluted in argon, were prepared in separate gas-handling
manifolds. The two deposition lines were then joined with an Ultratorr
tee at a distance from the cryogenic surface, and the flowing gas samples
were permitted to mix and react during passage through the merged
region. The length of this region was variable, from 10 to 300 cm. In
addition, the merged region could be heated to as high as 400 °C, to
induce further reaction. The flowing gas mixture exited the tip of the
deposition line and was sprayed onto the 14 K cold surface for 20-24
h before final infrared spectra were recorded either on a Bruker 113v
or a Perkin-Elmer Spectrum 2000 Fourier transform infrared spectrom-
-
1
eter at 1 cm resolution. Additional experiments were conducted in
the twin jet mode, where the two reactants, each diluted in argon, were
co-deposited on the cold surface from separate nozzles. A number of
these matrixes were subsequently warmed to 33-35 K to permit
annealing and limited diffusion, and then recooled to 14 K and
additional spectra recorded. Also, many of these matrices were
irradiated with the filtered output of a medium-pressure Hg arc after
which additional spectra were recorded.
Chromyl chloride (Aldrich) was introduced into the vacuum system
as the vapor above the room-temperature liquid, after purification in a
glass finger by freeze-pump-thaw cycles. CH
3
OH (Aldrich), CD
OH, CD OD, CH OH, and CH 18OH (all Cambridge Isotope
3
-
1
3
3 3 3
Laboratories, 99% isotopic enrichment) were also introduced as the
vapor above the room-temperature liquid, after repeated freeze-pump-
2
thaw cycles. In several experiments, CH O was employed as a reactant;
this species was produced by sublimation of solid paraformaldehyde
CH O) at approximately 50 °C from a metal finger attached to the
Figure 1. Infrared spectra over selected spectral regions of matrixes
(
2
x
prepared by twin jet deposition of samples of Ar/CrCl
2 2
O ) 100 and
deposition line. In a few experiments, HCl (Matheson) was employed
as a reactant after introduction into the vacuum system from a lecture
bottle and purification by freeze-pump-thaw cycles at 77 K. Argon
was used as the matrix gas in all experiments, and was used without
further purification.
Ar/CH OH ) 250. The upper trace was taken before annealing while
3
the lower trace was taken after annealing to 33 K and recooling to 14
K. Bands denoted by an asterisk are attributable to species A.
addition, blank experiments were conducted in the merged jet
mode with the merged region heated to as high as 380 °C, for
comparison to the merged jet pyrolysis experiments. The
spectra of Ar/CrCl2O2 ) 100 samples after pyrolysis to 380 °C
were unchanged relative to deposition through a room-temper-
ature line. In contrast, there was some evidence of decomposi-
Ab initio calculations were conducted on the likely intermediate
species in this study, using the Gaussian 94 suite of programs.26 Both
restricted Hartree-Fock and density functional calculations employing
the Becke functional B3LYP were conducted to locate stable minima,
determine structures, and calculate vibrational spectra. Final calcula-
tions with full geometry optimization employed the 6-311G* triple-ú
basis set, after initial calculations with smaller basis sets were run to
approximately locate energy minima. Calculations were carried out
on a Silicon Graphics Indigo 2 workstation.
tion of Ar/CH OH samples above 300 °C, leading to the
3
production of CH4, CO, and CO2 in the matrix. There was no
evidence of decomposition of Ar/CH2O samples during high-
temperature pyrolysis.
CrCl2O2 + CH3OH. (a) Twin Jet Experiments. The
reaction chemistry of these two compounds was initially
explored in a twin jet experiment in which a sample of Ar/
CrCl2O2 ) 100 was co-deposited with a sample of Ar/CH3OH
Results
Blank experiments were carried out in the twin jet mode for
each of the reagents alone in argon prior to any co-deposition
experiments. The spectra obtained were in good agreement with
)
250. The resultant spectrum showed intense bands due to
literature spectra.2
7-33
the two parent species, along with a set of very weak new
absorptions at 429, 443, 944, 978, 1010, 1313, 3586, and 3596
Several of these blank experiments were
subsequently annealed to around 34 K, recooled, and scanned.
Some aggregation was noted in spectra of CH3OH samples,
while no distinct changes were noted in spectra of CrCl2O2
samples. A blank experiment of each reagent was also irradiated
with the Pyrex/H2O-filtered output of a medium-pressure Hg
arc lamp. No changes were seen as a result of irradiation. In
-
1
-1
cm , with the 944, cm band appearing as a triplet with
-
1
maxima at 938, 944 and 951 cm . This matrix was then
annealed to 33 K and recooled to 14 K and an additional
spectrum recorded. All of the new, weak bands listed above
(hereafter referred to as set A) grew by an factor of nearly 10,
as shown in Figure 1. In addition, all of these bands grew by
the same amount (i.e. they maintained a constant intensity ratio
with respect to one another). A very slight reduction in parent
monomer intensities was noted, and some growth in bands due
to the parent CH3OH dimer (also seen in annealed blank
experiments). This annealed matrix was then irradiated for 1
h with the output of a medium-pressure Hg arc, using a Pyrex/
H2O filter, and an additional spectrum recorded. The bands of
set A were greatly decreased as a result of irradiation, and new
infrared absorptions appear at 676, 1129, 1150, 1425, and 1445
(
26) Gaussian 94, Revision E.1; Frisch, M. J.; Trucks, G. W.; Schlegel,
H. B.; Gill, P. M. W.; Johnson, B. G.; Robb, M. A.; Cheeseman, J. R.;
Keith, T.; Petersson, G. A.; Montgomery, J. A.; Raghavachari, K.;
Al-Laham, M. A.; Zakrzewski, V. G.; Ortiz, J. V.; Foresman, J. B.;
Cioslowski, J.; Stefanov, B. B.; Nanayakkara, M.; Challacombe, M.; Peng,
C. Y.; Ayala, P. Y.; Chen, W.; Wong, M. W.; Andres, J. L.; Binkley, J. S.;
Defrees, D. J.; Baker, J.; Stewart, J. P.; Head-Gordon, M.; Gonzalez, C.;
Pople, J. A.; Gaussian, Inc.: Pittsburgh, PA, 1995.
(
(
27) Varetti, E. L.; Muller, A. Spectrochim. Acta 1978, 34A, 895.
28) Beattie, I. R.; Marsden, C. J.; Ogden, J. S. J. Chem. Soc., Dalton
Trans. 1980, 535.
(
(
29) Barnes, A. J.; Hallam, H. E. Trans. Faraday Soc. 1970, 66, 1920.
30) Barnes, A. J.; Hallam, H. E.; Scrimshaw, G. F. Trans. Faraday Soc.
-1
cm (hereafter referred to as set B) as well as a group of bands
-
1
1
969, 65, 3150.
31) Maillard, D.; Schriver, A.; Perchard, J. P. J. Chem. Phys. 1979, 71,
05.
at 2704, 2731, 2752, 2764, 2784, and 2800 cm (set C), as
shown in Figure 2. Further irradiation resulted in complete
destruction of bands in set A, and some additional growth of
bands in sets B and C.
(
5
(
(
32) Nelander, B. J. Mol. Struct. 1978, 50, 223.
33) Bach, S. B. H.; Ault, B. S. J. Phys. Chem. 1984, 88, 3600.