电子能量分布的弛豫对电子雪崩统计的影响

W. Legler
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引用次数: 30

摘要

在高E/p值时,电场在气体中产生的电子雪崩的大小分布受电离后电子能量分布中的弛豫过程的影响。对这种影响的描述需要一个电离系数,它取决于雪崩大小n以及与阴极的距离。缺乏关于这种依赖关系的信息妨碍了对雪崩分布的严格计算。最近,Cookson和Lewis提出了一个解决方案,他们引入了一个只依赖于n的电离系数。目前的工作表明,由于物理原因,这个建议必须被拒绝。作者先前基于“个体”电离系数的概念给出了一个近似解,并与Cookson和Lewis等人讨论的Polya分布进行了比较。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The influence of the relaxation of the electron energy distribution on the statistics of electron avalanches
The distribution of sizes of electron avalanches produced in a gas by an electric field at high values of E/p is influenced by the relaxation processes in the electron energy distribution after an ionization. The description of this influence requires an ionization coefficient which depends on the avalanche size n as well as on the distance from the cathode. Lack of information on this dependence prevents a rigorous calculation of the avalanche distribution. Recently Cookson and Lewis suggested a solution of the problem by the introduction of an ionization coefficient depending on n only. The present work shows that this proposal must be rejected for physical reasons. An approximate solution previously given by the author, which is based on the concept of an `individual' ionization coefficient, is compared with the Polya distribution discussed by Cookson and Lewis and other authors.
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