Laboratoire Interdisciplinaire Carnot de Bourgogne, UMR CNRS 5209, Université de Bourgogne, 21078 Dijon Cedex, France.
Phys Chem Chem Phys. 2011 Nov 14;13(42):19089-100. doi: 10.1039/c1cp21232j. Epub 2011 Sep 30.
Ortho-para H(2) conversion reactions mediated by the exchange of a H(+) proton have been investigated at very low energy for the first time by means of a time independent quantum mechanical (TIQM) approach. State-to-state probabilities and cross sections for H(+) + H(2) (v = 0, j = 0,1) processes have been calculated for a collision energy, E(c), ranging between 10(-6) eV and 0.1 eV. Differential cross sections (DCSs) for H(+) + H(2) (v = 0, j = 1) → H(+) + H(2) (v' = 0, j' = 0) for very low energies only start to develop a proper global minimum around the sideways scattering direction (θ≈ 90°) at E(c) = 10(-3) eV. Rate coefficients, a crucial information required for astrophysical models, are provided between 10 K and 100 K. The relaxation ortho-para process j = 1 → j' = 0 is found to be more efficient than the j = 0 → j' = 1 conversion at low temperatures, in line with the extremely small ratio between the ortho and para species of molecular hydrogen predicted at the temperature of interstellar cold molecular clouds. The results obtained by means of a statistical quantum mechanical (SQM) model, which has previously proved to provide an adequate description of the dynamics of the title reactions at a higher collision energy regime, have been compared with the TIQM results. A reasonable good agreement has been found with the only exception of the DCSs for the H(+) + H(2) (v = 0, j = 1) → H(+) + H(2) (v' = 0, j' = 0) process at very low energy. SQM cross sections are also slightly below the quantum results. Estimates for the rate coefficients, in good accord with the TIQM values, are a clear improvement with respect to pioneering statistical studies on the reaction.
首次通过非时变量子力学(TIQM)方法研究了在极低能量下通过质子交换进行的 ortho-para H(2) 转换反应。对于碰撞能量 E(c) 在 10(-6) eV 至 0.1 eV 之间的 H(+) + H(2) (v = 0, j = 0,1) 过程,计算了 H(+) + H(2) (v = 0, j = 1) 过程的态态概率和截面。对于极低能量,仅在 E(c) = 10(-3) eV 时,H(+) + H(2) (v = 0, j = 1) → H(+) + H(2) (v' = 0, j' = 0) 的微分截面 (DCS) 才开始在侧向散射方向 (θ≈90°) 附近形成合适的全局最小值。在 10 K 至 100 K 之间提供了天体物理模型所需的关键信息,即速率系数。在低温下,发现 ortho-para 弛豫过程 j = 1 → j' = 0 比 j = 0 → j' = 1 转换更有效,这与星际冷分子云温度下预测的分子氢的 ortho 和 para 物种之间的极小比例一致。与先前在更高碰撞能量范围内证明能够对标题反应动力学进行适当描述的统计量子力学 (SQM) 模型的结果进行了比较。仅在极低能量下 H(+) + H(2) (v = 0, j = 1) → H(+) + H(2) (v' = 0, j' = 0) 过程的 DCS 除外,发现了很好的一致性。SQM 截面也略低于量子结果。与反应的开创性统计研究相比,对于速率系数的估计,与 TIQM 值非常吻合,是一个明显的改进。