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RADIATIVE CHARGE TRANSFER IN COLLISIONS OF Li WITH H~+

机译:Li与H〜+碰撞中的径向电荷转移

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摘要

We present cross sections for the radiative charge transfer process Li(2s) + H~+ → Li~+(1s~2) + H(1s) + hω for collision energies between 0.1 meV and 10 eV and rate coefficients for temperatures between 10 and 40,000 K. At 300 K, the rate coefficient is 1.3 x 10~(13) cm~3 s~(-1). The results are obtained through a fully quantum-mechanical method using completely ab initio molecular data. Cross sections for the total collision-induced radiative decay, radiative charge transfer plus radiative association, from the entrance Li(2s) + H~+ channel are calculated with the optical potential method. Radiative charge; transfer dominates radiative association for the considered collision energies, but direct charge transfer will become important at higher energies. The emission spectrum, which has a peak at wavelengths near 158 nm, due to radiative charge transfer is given for several collision energies. Implications to the lithium ionization fraction in the postrecombination era of the early universe are discussed.
机译:我们给出了辐射电荷转移过程的截面Li(2s)+ H〜+→Li〜+(1s〜2)+ H(1s)+hω(碰撞能量介于0.1 meV和10 eV之间)和速率系数(温度介于10之间)和40,000K。在300 K时,速率系数为1.3 x 10〜(13)cm〜3 s〜(-1)。通过使用完全从头算的分子数据的完全量子力学方法获得结果。用光势法计算了入射Li(2s)+ H〜+通道的碰撞引起的总辐射衰减,辐射电荷转移和辐射缔合的截面。辐射电荷;对于所考虑的碰撞能量,转移主要支配着辐射缔合,但是在较高能量下,直接电荷转移将变得很重要。对于几种碰撞能量,给出了由于辐射电荷转移而在接近158 nm的波长处具有峰值的发射光谱。讨论了早期宇宙的重组后时代对锂离子化部分的影响。

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