8 research outputs found
Detection of Two Highly Stable Silicon Nitrides: HSiNSi and H<sub>3</sub>SiNSi
The formation mechanisms of silicon
nitride and silicon nitrogen
hydrogen films, both produced by chemical vapor deposition (CVD) techniques
and widely used in electronic device fabrication, are poorly understood.
Identification of gas-phase intermediates formed from starting materials,
typically silane, ammonia, and/or nitrogen, is a critical step in
assessing the interplay between gas and surface processes in film
formation. Two potential intermediates in this process, HSiNSi and
H<sub>3</sub>SiNSi, have now been detected in a molecular beam by
means of rotational spectroscopy. Both molecules were produced in
electrical discharges of CVD-like gas mixtures and are the most readily
observed siliconānitrogen-containing molecules in the 6ā20
GHz frequency range, though neither has been the subject of prior
experimental or theoretical studies. HSiNSi and H<sub>3</sub>SiNSi
are likely formed from reactions involving the silanitrile radical
(SiN, isoelectronic to CN), implying that similar gas-phase reactions
may be involved in film growth
Spectroscopic Detection and Structure of Hydroxidooxidosulfur (HOSO) Radical, An Important Intermediate in the Chemistry of Sulfur-Bearing Compounds
The rotational spectrum of hydroxidooxidosulfur,
HOSO, an intermediate
of particular interest in the combustion of sulfur-rich fuels, has
been determined to high accuracy from gas-phase measurements. Detection
of specific isotopic species using isotopically enriched gases suggests
that HOSO is formed in our discharge nozzle via the reaction H + SO<sub>2</sub> (+M) ā HOSO (+M). A precise experimental <i>r</i><sub>0</sub> geometry has also been derived from the isotopic analysis;
HOSO has a <i>cis</i> configuration, but the subtle structural
question of its planarity remains unresolved. From the derived spectroscopic
constants, <i>in situ</i> and remote sensing for this fundamental
radical can now be undertaken in a variety of environments, including
in combustion reactors, the troposphere of Earth, and Io, the innermost
Galilean moon of Jupiter
Temperature and Pressure Dependences of the Reactions of Fe<sup>+</sup> with Methyl Halides CH<sub>3</sub>X (X = Cl, Br, I): Experiments and Kinetic Modeling Results
The
pressure and temperature dependences of the reactions of Fe<sup>+</sup> with methyl halides CH<sub>3</sub>X (X = Cl, Br, I) in He
were measured in a selected ion flow tube over the ranges 0.4 to 1.2
Torr and 300ā600 K. FeX<sup>+</sup> was observed for all three
halides and FeCH<sub>3</sub><sup>+</sup> was observed for the CH<sub>3</sub>I reaction. FeCH<sub>3</sub>X<sup>+</sup> adducts (for all
X) were detected in all reactions. The results were interpreted assuming
two-state reactivity with spin-inversions between sextet and quartet
potentials. Kinetic modeling allowed for a quantitative representation
of the experiments and for extrapolation to conditions outside the
experimentally accessible range. The modeling required quantum-chemical
calculations of molecular parameters and detailed accounting of angular
momentum effects. The results show that the FeX<sup>+</sup> products
come via an insertion mechanism, while the FeCH<sub>3</sub><sup>+</sup> can be produced from either insertion or S<sub>N</sub>2 mechanisms,
but the latter we conclude is unlikely at thermal energies. A statistical
modeling cannot reproduce the competition between the bimolecular
pathways in the CH<sub>3</sub>I reaction, indicating that some more
direct process must be important
Kinetics of Cations with C<sub>2</sub> Hydrofluorocarbon Radicals
Reactions
of the cations Ar<sup>+</sup>, O<sub>2</sub><sup>+</sup>, CO<sub>2</sub><sup>+</sup>, and CF<sub>3</sub><sup>+</sup> with
the C<sub>2</sub> radicals C<sub>2</sub>H<sub>5</sub>, H<sub>2</sub>C<sub>2</sub>F<sub>3</sub>, C<sub>2</sub>F<sub>3</sub>, and C<sub>2</sub>F<sub>5</sub> were investigated using the variable electron
and neutral density attachment mass spectrometry technique in a flowing
afterglowāLangmuir probe apparatus at room temperature. Rate
coefficients for observed product channels for these 16 reactions
are reported as well as rate coefficients and product branching fractions
for the 16 reactions of the same cations with each of the stable neutrals
used as radical precursors (the species RI, where R is the radical
studied). Reactions with the stable neutrals proceed by charge transfer
at or near the collisional rate coefficient where energetically allowed;
where charge transfer is endothermic, bond-breaking/bond-making chemistry
occurs. While also efficient, reactions with the radicals are more
likely to occur at a smaller fraction of the collisional rate coefficient,
and bond-breaking/bond-making chemistry occurs even in some cases
where charge transfer is exothermic. It is noted that unlike radical
reactions with neutral species, which occur with rate coefficients
that are generally elevated compared to those of stable species, ionāradical
reactivity is generally decreased relative to that of reactions with
stable species. In particular, long-range charge transfer appears
more likely to be frustrated in the ionāradical systems
Analysis of the Pressure and Temperature Dependence of the Complex-Forming Bimolecular Reaction CH<sub>3</sub>OCH<sub>3</sub> + Fe<sup>+</sup>
The
kinetics of the reaction CH<sub>3</sub>OCH<sub>3</sub> + Fe<sup>+</sup> has been studied between 250 and 600 K in the buffer gas
He at pressures between 0.4 and 1.6 Torr. Total rate constants and
branching ratios for the formation of Fe<sup>+</sup>OĀ(CH<sub>3</sub>)<sub>2</sub> adducts and of Fe<sup>+</sup>OCH<sub>2</sub> + CH<sub>4</sub> products were determined. Quantumāchemical calculations
provided the parameters required for an analysis in terms of statistical
unimolecular rate theory. The analysis employed a recently developed
simplified representation of the rates of complex-forming bimolecular
reactions, separating association and chemical activation contributions.
Satisfactory agreement between experimental results and kinetic modeling
was obtained that allows for an extrapolation of the data over wide
ranges of conditions. Possible reaction pathways with or without spin-inversion
are discussed in relation to the kinetic modeling results
Determining Rate Constants and Mechanisms for Sequential Reactions of Fe<sup>+</sup> with Ozone at 500 K
We present rate constants
and product branching ratios for the
reactions of FeO<sub><i>x</i></sub><sup>+</sup> (<i>x</i> = 0ā4) with ozone at 500 K. Fe<sup>+</sup> is observed
to react with ozone at the collision rate to produce FeO<sup>+</sup> + O<sub>2</sub>. The FeO<sup>+</sup> in turn reacts with ozone at
the collision rate to yield both Fe<sup>+</sup> and FeO<sub>2</sub><sup>+</sup> product channels. Ions up to FeO<sub>4</sub><sup>+</sup> display similar reactivity patterns. Three-body clustering reactions
with O<sub>2</sub> prevent us from measuring accurate rate constants
at 300 K although the data do suggest that the efficiency is also
high. Therefore, it is probable that little to no temperature dependence
exists over this range. Implications of our measurements to the regulation
of atmospheric iron and ozone are discussed. Density functional calculations
on the reaction of Fe<sup>+</sup> with ozone show no substantial kinetic
barriers to make the FeO<sup>+</sup> + O<sub>2</sub> product channel,
which is consistent with the reactionās efficiency. While a
pathway to make FeO<sub>2</sub><sup>+</sup> + O is also found to be
barrierless, our experiments indicate no primary FeO<sub>2</sub><sup>+</sup> formation for this reaction
The Simplest Criegee Intermediate (H<sub>2</sub>Cī»OāO): Isotopic Spectroscopy, Equilibrium Structure, and Possible Formation from Atmospheric Lightning
A number of research groups have
recently succeeded in producing the simple carbonyl oxides H<sub>2</sub>COO and CH<sub>3</sub>CHOO in sufficient quantity to observe them
spectroscopically and to probe the kinetics of their reactions with
NO<sub>2</sub> and SO<sub>2</sub>. These latter studies provide evidence
that the carbonyl oxides play an important role in the atmosphere,
likely contributing to pollutant removal, aerosol formation, and planetary
cooling. In this work, Fourier transform microwave and double-resonance
spectroscopy are combined with theory to study five isotopic species
of H<sub>2</sub>Cī»OāO, and a precise equilibrium structure
is reported for this ephemeral yet crucial reactive intermediate.
In contrast to the other investigations, which have exclusively produced
H<sub>2</sub>Cī»OāO by halogen chemistry, passing a mixture
of methane and excess molecular oxygen through an electrical discharge
generates this isomer of H<sub>2</sub>CO<sub>2</sub> with high selectivity,
thereby suggesting that the molecule is produced in the direct vicinity
of atmospheric lightning
Further Insight into the Reaction FeO<sup>+</sup> + H<sub>2</sub> ā Fe<sup>+</sup> + H<sub>2</sub>O: Temperature Dependent Kinetics, Isotope Effects, and Statistical Modeling
The reactions of FeO<sup>+</sup> with
H<sub>2</sub>, D<sub>2</sub>, and HD were studied in detail from 170
to 670 K by employing a
variable temperature selected ion flow tube apparatus. High level
electronic structure calculations were performed and compared to previous
theoretical treatments. Statistical modeling of the temperature and
isotope dependent rate constants was found to reproduce all data,
suggesting the reaction could be well explained by efficient crossing
from the sextet to quartet surface, with a rigid near thermoneutral
barrier accounting for both the inefficiency and strong negative temperature
dependence of the reactions over the measured range of thermal energies.
The modeling equally well reproduced earlier guided ion beam results
up to translational temperatures of about 4000 K