Computational Investigation on the Formation and Decomposition Reactions of the C(4)H(3)O Compound.

Gas-phase mechanism and kinetics of the formation and decomposition reactions of the C(4)H(3)O compound, a crucial intermediate of the atmospheric and combustion chemistry, were investigated using ab initio molecular orbital theory and the very expensive coupled-cluster CCSD(T)/CBS(T,Q,5)//B3LYP/6-311++G(3df,2p) method together with transition state theory and Rice-Ramsperger-Kassel-Macus kinetic predictions. The potential energy surface established shows that the C(3)H(3) + CO addition reaction has four main entrances in which C(3)H(3) + CO → IS1-cis (CHCCH(2)CO) is the most energetically favorable channel. The calculated results revealed that the bimolecular rate constants are positively dependent on both temperatures (T = 300-2000 K) and pressures (P = 1-76,000 Torr). Of these values, the k (1) rate constant of the C(3)H(3) + CO → IS1-cis addition channel is dominant over the 300-2000 K temperature range, increasing from 1.53 × 10(-20) to 1.04 × 10(-13) cm(3) molecule(-1) s(-1) with the branching ratio reducing from 62% to 44%. The predicted unimolecular rate coefficients in the ranges of T = 300-2000 K and P = 1-76,000 Torr revealed that the intermediate products IS1-cis , IS1-trans , and IS2 are rather unstable and would rapidly decompose back to the reactants (C(3)H(3) + CO), especially at high temperatures (T > 1000 K). The high-pressure limit rate constants for the C(4)H(3)O decomposition leading to products (C(3)H(3) + CO), (CHCCHCO + H), and (CHCO + C(2)H(2)) have been found to be in excellent agreement with the available literature values proposed by Tian et al. (Combust. Flame, 2011, 158, 756-773) without any adjustment from the ab initio calculations. Therefore, the predicted temperature- and pressure-dependent rate constants can be confidently used for modeling CO-related systems under atmospheric and combustion conditions.