Rotational state-to-state transition rate coefficients for H2O + H2O collisions at nonequilibrium conditions

Bikramaditya Mandal, M. Żółtowski, Martin Cordiner, Francois Lique, D. Babikov
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Abstract

The goal is to develop a database of rate coefficients for rotational state-to-state transitions in H$_ $O + H$_ $O collisions that is suitable for the modeling of energy transfer in nonequilibrium conditions, in which the distribution of rotational states of H$_ $O deviates from local thermodynamic equilibrium. A two-temperature model was employed that assumed that although there is no equilibrium between all possible degrees of freedom in the system, the translational and rotational degrees of freedom can be expected to achieve their own equilibria independently, and that they can be approximately characterized by Boltzmann distributions at two different temperatures, $T_ kin $ and $T_ rot Upon introducing our new parameterization of the collisional rates, taking into account their dependence on both $T_ kin $ and $T_ rot $, we find a change of up to 20 in the H$_ $O rotational level populations for both ortho and para-H$_ $O for the part of the cometary coma where the nonequilibrium regime occurs.
非平衡条件下 H2O + H2O 碰撞的旋转态-态转换速率系数
目的是建立一个 H$_ $O + H$_ $O 碰撞中旋转状态到状态转变的速率系数数据库,该数据库适用于非平衡条件下的能量转移建模,在非平衡条件下,H$_ $O 的旋转状态分布偏离局部热力学平衡。所采用的双温模型假定,虽然系统中所有可能的自由度之间不存在平衡,但平移和旋转自由度可望独立地达到各自的平衡,而且它们可以近似地用两个不同温度下的玻尔兹曼分布来表征、在引入碰撞速率的新参数化之后,考虑到它们对 $T_ kin $ 和 $T_ rot $ 的依赖性,我们发现在发生非平衡态的彗星彗尾部分,正 H$_ $O 和副 H$_ $O 旋转水平种群的变化高达 20。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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