5 research outputs found
Kinetic and Product Study of the Reactions of C(<sup>1</sup>D) with CH<sub>4</sub> and C<sub>2</sub>H<sub>6</sub> at Low Temperature
The reactions of atomic carbon in
its first excited <sup>1</sup>D state with both CH<sub>4</sub> and
C<sub>2</sub>H<sub>6</sub> have been investigated using a continuous
supersonic flow reactor over the 50ā296 K temperature range.
CĀ(<sup>1</sup>D) atoms were generated in situ by the pulsed laser
photolysis of CBr<sub>4</sub> at 266 nm. To follow the reaction kinetics,
product H atoms were detected by vacuum ultraviolet laser-induced
fluorescence at 121.567 nm. Absolute H-atom yields for both reactions
were determined by comparison with the H-atom signal generated by
the reference CĀ(<sup>1</sup>D) + H<sub>2</sub> reaction. Although
the rate constant for the CĀ(<sup>1</sup>D) + CH<sub>4</sub> reaction
is in excellent agreement with earlier work at room temperature, this
process displays a surprising reactivity increase below 100 K. In
contrast, the reactivity of the CĀ(<sup>1</sup>D) + C<sub>2</sub>H<sub>6</sub> system decreases as the temperature falls, obeying a capture-type
rate law. The H-atom product yields of the CĀ(<sup>1</sup>D) + CH<sub>4</sub> reaction agree with the results of earlier crossed-beam experiments
at higher collision energy. Although no previous data is available
on the product channels of the CĀ(<sup>1</sup>D) + C<sub>2</sub>H<sub>6</sub> reaction, comparison with earlier work involving the same
singlet C<sub>3</sub>H<sub>6</sub> potential energy surface allows
us to draw conclusions from the measured H-atom yields
Unusual Low-Temperature Reactivity of Water: The CH + H<sub>2</sub>O Reaction as a Source of Interstellar Formaldehyde?
Water
is an important reservoir species for oxygen in interstellar
space and plays a key role in the physics of star formation through
cooling by far-infrared emission. While water vapor is present at
high abundances in the outflows of protostars, its contribution to
the chemical evolution of these regions is a minor one due to its
limited low temperature reactivity in the gas-phase. Here, we performed
kinetic experiments on the barrierless CH + H<sub>2</sub>O reaction
in a supersonic flow reactor down to 50 K. The measured rate increases
rapidly below room temperature, confirming and extending the predictions
of previous statistical calculations. The open product channels for
this reaction suggest that this process could be an important gas-phase
route for formaldehyde formation in protostellar envelopes
Ring-Polymer Molecular Dynamics for the Prediction of Low-Temperature Rates: An Investigation of the C(<sup>1</sup>D) + H<sub>2</sub> Reaction
Quantum mechanical calculations are
important tools for predicting
the rates of elementary reactions, particularly for those involving
hydrogen and at low temperatures where quantum effects become increasingly
important. These approaches are computationally expensive, however,
particularly when applied to complex polyatomic systems or processes
characterized by deep potential wells. While several approximate techniques
exist, many of these have issues with reliability. The ring-polymer
molecular dynamics method was recently proposed as an accurate and
efficient alternative. Here, we test this technique at low temperatures
(300ā50 K) by analyzing the behavior of the barrierless CĀ(<sup>1</sup>D) + H<sub>2</sub> reaction over the two lowest singlet potential
energy surfaces. To validate the theory, rate coefficients were measured
using a supersonic flow reactor down to 50 K. The experimental and
theoretical rates are in excellent agreement, supporting the future
application of this method for determining the kinetics and dynamics
of a wide range of low-temperature reactions
Quantum Tunneling Enhancement of the C + H<sub>2</sub>O and C + D<sub>2</sub>O Reactions at Low Temperature
Recent
studies of neutral gas-phase reactions characterized by
barriers show that certain complex forming processes involving light
atoms are enhanced by quantum mechanical tunneling at low temperature.
Here, we performed kinetic experiments on the activated CĀ(<sup>3</sup>P) + H<sub>2</sub>O reaction, observing a surprising reactivity increase
below 100 K, an effect that is only partially reproduced when water
is replaced by its deuterated analogue. Product measurements of H-
and D-atom formation allowed us to quantify the contribution of complex
stabilization to the total rate while confirming the lower tunneling
efficiency of deuterium. This result, which is validated through statistical
calculations of the intermediate complexes and transition states has
important consequences for simulated interstellar water abundances
and suggests that tunneling mechanisms could be ubiquitous in cold
dense clouds
Gas-Phase Kinetics of the Hydroxyl Radical Reaction with Allene: Absolute Rate Measurements at Low Temperature, Product Determinations, and Calculations
The gas phase reaction of the hydroxyl radical with allene
has been studied theoretically and experimentally in a continuous
supersonic flow reactor over the range 50 ā¤ <i>T</i>/K ā¤ 224. This reaction has been found to exhibit a negative
temperature dependence over the entire temperature range investigated,
varying between (0.75 and 5.0) Ć 10<sup>ā11</sup> cm<sup>3</sup> molecule<sup>ā1</sup> s<sup>ā1</sup>. Product
formation from the reaction of OH and OD radicals with allene (C<sub>3</sub>H<sub>4</sub>) has been investigated in a fast flow reactor
through time-of-flight mass spectrometry, at pressures between 0.8
and 2.4 Torr. The branching ratios for adduct formation (C<sub>3</sub>H<sub>4</sub>OH) in this pressure range are found to be equal to
34 Ā± 16% and 48 Ā± 16% for the OH and OD + allene reactions,
respectively, the only other channel being the formation of CH<sub>3</sub> or CH<sub>2</sub>D + H<sub>2</sub>CCO (ketene). Moreover,
the rate constant for the OD + C<sub>3</sub>H<sub>4</sub> reaction
is also found to be 1.4 times faster than the rate constant for the
OH + C<sub>3</sub>H<sub>4</sub> reaction at 1.5 Torr and at 298 K.
The experimental results and implications for atmospheric chemistry
have been rationalized by quantum chemical and RRKM calculations