首页> 外文OA文献 >Rotational energy transfer in collisions between CO(X singlet sigma plus, v=2, J=0, 1,4, and 6) and He at temperatures from 294 to 15 K.
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Rotational energy transfer in collisions between CO(X singlet sigma plus, v=2, J=0, 1,4, and 6) and He at temperatures from 294 to 15 K.

机译:在294至15 K的温度下,CO(X单峰sigma加,v = 2,J = 0,1,4,和6)和He之间的碰撞中的旋转能量转移。

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摘要

Infrared-vacuum ultraviolet double resonance experiments have been implemented in the ultracold environment provided by a Cinétique de Réaction en Ecoulement Supersonique Uniforme apparatus. With this technique rate coefficients of two kinds have been measured for rotational energy transfer in collisions between CO and He: (a) those for total removal from the selected rotational states J = 0, 1, 4, and 6 in the vibronic state X 1+, v = 2, and (b) those for transfer between selected initial and specific final states. Using different Laval nozzles, results have been obtained at several different temperatures: 294, 149, 63, 27, and 15 K. The thermally averaged cross sections for total removal by collisions with He show only slight variations both with initial rotational state and with temperature. The variation of state-to-state rate coefficients with J show several general features: (i) a decrease with increasing J; (ii) a propensity to favor odd J over even J; and (iii) at lower temperatures, the distribution of rate coefficients against J becomes narrower, and decreases in J are increasingly favored over increases in J, a preference which is most strongly seen for higher initial values of J. The results are shown to be in remarkably good agreement with those obtained in ab initio scattering calculations by Dalgarno and co-workers [Astrophys. J. 571, 1015 (2002)].
机译:红外真空双共振实验已在CinétiquedeRéactionen Ecoulement Supersonique Uniforme仪器提供的超冷环境中进行。通过这种技术,已经测量了两种速率系数,用于在CO和He之间的碰撞中进行旋转能量传递:(a)在振动状态X 1中用于从选定旋转状态J = 0、1、4和6中完全去除的速率系数。 +,v = 2,以及(b)在选定的初始状态和特定最终状态之间转换的那些。使用不同的拉伐尔喷嘴,在以下几种不同的温度下均获得了结果:294、149、63、27和15K。与He碰撞导致全部去除的热平均横截面在初始旋转状态和温度下仅显示出细微变化。状态对状态速率系数随J的变化表现出几个一般特征:(i)随着J的增加而减小; (ii)倾向于奇J胜于偶J的倾向; (iii)在较低的温度下,针对J的速率系数的分布会变窄,并且J的减小比J的增大受到越来越多的青睐,对于J的较高初始值而言,这种偏好最为明显。结果表明,与Dalgarno及其同事从头算散射计算中获得的结果非常吻合[Astrophys。 J. 571,1015(2002)]。

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