Abstract
AbstractKinetics and mechanisms for the reactions of HNO with CH3 and C6H5 have been investigated by ab initio molecular orbital (MO) and transition‐state theory (TST) and/or Rice‐Ramsperger‐Kassel‐Marcus/Master Equation (RRKM/ME) calculations. The G2M(RCC, MP2)//B3LYP/6‐31G(d) method was employed to evaluate the energetics for construction of their potential energy surfaces and prediction of reaction rate constants. The reactions R + HNO (R = CH3 and C6H5) were found to proceed by two key product channels giving (1) RH + NO and (2) RNO + H, primarily by direct abstraction and indirect association/decomposition mechanisms, respectively. As both reactions initially occur barrierlessly, their rate constants were evaluated with a canonical variational approach in our TST and RRKM/ME calculations. For practical applications, the rate constants evaluated for the atmospheric‐pressure condition are represented by modified Arrhenius equations in units of cm3 mol−1 s−1 for the temperature range 298–2500 K: κ1A = 1.47 × 1011T0.76 exp[−175/T], κ2A = 8.06 × 103T2.40 exp[−3100/T], κ1B = 3.78 × 105T2.28 exp[230/T], and κ2B = 3.79 × 109T1.19 exp[−4800/T], where A and B represent CH3 and C6H5 reactions, respectively. Based on the predicted rate constant at 1 atm pressure for R + HNO → RNO + H, we estimated their reverse rate constants for R + HNO production from H + RNO in units of cm3 mol−1 s−1: κ−2A′ = 7.01 × 1010 T0.84 exp[120/T] and κ−2B′ = 2.22 × 1019 T−1.01 exp[−9700/T]. The heats of formation at 0 K for CH3NO, CH3N(H)O, CH3NOH, C6H5N(H)O, and C6H5NOH have been estimated to be 18.6, 18.1, 22.5, 47.2, and 50.7 kcal mol−1 with an estimated ±1 kcal mol−1 error. © 2005 Wiley Periodicals, Inc. Int J Chem Kinet 37: 261–274, 2005
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