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arXiv 2103.10902physics.plasm-phphysics.app-ph
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高功率脉冲磁控溅射放电中电子能量分布函数

On the electron energy distribution function in the high power impulse magnetron sputtering discharge

Martin Rudolph, A. Revel, D. Lundin, H. Hajihoseini, N. Brenning, M. A. Raadu, A. Anders, T. M. Minea, J. T. Gudmundsson

摘要:

本文应用电离区模型和电子的Orsay Boltzmann方程耦合电离和激发态动力学模型研究了高功率脉冲磁控溅射(HiPIMS)放电的电子动力学。在OBELIX中,假定大体积(冷)电子呈现麦克斯韦能量分布,并且在离子轰击时从靶表面发射的二次(热)电子被视为高能量尾部,而在OBELIX中,使用各向同性玻尔兹曼方程自洽地计算电子能量分布。这两个模型在某种意义上是合并的,即从EQUIPMENT的输出被用作OBELIX的输入。粒子密度的时间演化被发现同意非常好的两个模型之间。此外,一个非常好的协议之间的双麦克斯韦电子能量分布的假设的ESTA和OBELIX模型计算的电子能量分布证明。因此,可以得出结论,假设双麦克斯韦电子能量分布,构成一个冷的散装电子组和一个热的次级电子组,是一个很好的近似模型的HiPIMS放电。

英文摘要:

We apply the Ionization Region Model (IRM) and the Orsay Boltzmann equation for ELectrons coupled with Ionization and eXcited states kinetics (OBELIX) model to study the electron kinetics of a high power impulse magnetron sputtering (HiPIMS) discharge. In the IRM the bulk (cold) electrons are assumed to exhibit a Maxwellian energy distribution and the secondary (hot) electrons, emitted from the target surface upon ion bombardment, are treated as a high energy tail, while in the OBELIX the electron energy distribution is calculated self-consistently using an isotropic Boltzmann equation. The two models are merged in the sense that the output from the IRM is used as an input for OBELIX. The temporal evolutions of the particle densities are found to agree very well between the two models. Furthermore, a very good agreement is demonstrated between the bi-Maxwellian electron energy distribution assumed by the IRM and the electron energy distribution calculated by the OBELIX model. It can therefore be concluded that assuming a bi-Maxwellian electron energy distribution, constituting a cold bulk electron group and a hot secondary electron group, is a good approximation for modeling the HiPIMS discharge.

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