Carty David, Goddard Andrew, Köhler Sven P K, Sims Ian R, Smith Ian W M
School of Chemistry, The University of Birmingham, Edgbaston, Birmingham B15 2TT, U.K.
J Phys Chem A. 2006 Mar 9;110(9):3101-9. doi: 10.1021/jp054429u.
The kinetics of the reaction between O atoms and OH radicals, both in their electronic ground state, have been investigated at temperatures down to ca. 39 K. The experiments employed a CRESU (Cinétique deRéaction en Ecoulement Supersonique Uniforme) apparatus to attain low temperatures. Both reagents were created using pulsed laser photolysis at 157.6 nm of mixtures containing H2O and O2 diluted in N2 carrier gas. OH radicals were formed by both direct photolysis of H2O and the reaction between O(1D) atoms and H2O. O(3P) atoms were formed both as a direct product of O2 photolysis and by the rapid quenching of O(1D) atoms formed in that photolysis by N2 and O2. The rates of removal of OH radicals were observed by laser-induced fluorescence, and concentrations of O atoms were estimated from a knowledge of the absorption cross-section for O2 at 157.6 nm and of the measured fluence from the F2 laser at this wavelength. To obtain a best estimate of the rate constants for the O + OH reaction, we had to correct the raw experimental data for the following: (a) the decrease in the laser fluence along the jet due to the absorption by O2 in the gas mixture, (b) the increase in temperature, and consequent decrease in gas density, as a result of energy released in the photochemical and chemical processes that occurred, and (c) the formation of OH(v = 0) as a result of relaxation, particularly by O2, of OH radicals formed in levels v > 0. Once these corrections were made, the rate constant for reaction between OH and O(3P) atoms showed little variation in the temperature range of 142 to 39 K and had a value of (3.5 +/- 1.0) x 10(-11) cm3 molecule(-1) s(-1). It is recommended that this value is used in future chemical models of dense interstellar clouds.
对处于电子基态的氧原子(O)与氢氧自由基(OH)之间反应的动力学进行了研究,温度低至约39K。实验采用了超声速均匀流反应动力学(CRESU)装置来实现低温。两种反应物均通过在157.6nm波长下用脉冲激光光解含H₂O和O₂且稀释于氮气载气中的混合物来产生。OH自由基通过H₂O的直接光解以及O(¹D)原子与H₂O之间的反应形成。O(³P)原子既作为O₂光解的直接产物形成,也通过在该光解过程中形成的O(¹D)原子被N₂和O₂快速猝灭而形成。通过激光诱导荧光观测OH自由基的去除速率,并根据O₂在157.6nm处的吸收截面以及该波长下F₂激光的测量通量来估算O原子的浓度。为了获得O + OH反应速率常数的最佳估计值,我们必须对原始实验数据进行如下校正:(a) 由于气体混合物中O₂的吸收导致沿射流激光通量的降低;(b) 由于光化学和化学过程中释放的能量导致温度升高以及随之而来的气体密度降低;(c) 由于v > 0能级形成的OH自由基通过弛豫(特别是被O₂弛豫)而形成OH(v = 0)。一旦进行了这些校正,OH与O(³P)原子之间反应的速率常数在142至39K的温度范围内变化很小,其值为(3.5 ± 1.0) × 10⁻¹¹ cm³ molecule⁻¹ s⁻¹。建议在未来致密星际云的化学模型中使用该值。