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Orbital-motion-limited theory of dust charging and plasma response

机译:轨道运动限制的尘埃充电和等离子体响应理论

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摘要

The foundational theory for dusty plasmas is the dust charging theory thatprovides the dust potential and charge arising from the dust interaction with aplasma. The most widely used dust charging theory for negatively charged dustparticles is the so-called orbital motion limited (OML) theory, which predictsthe dust potential and heat collection accurately for a variety ofapplications, but was previously found to be incapable of evaluating the dustcharge and plasma response in any situation. Here we report a revised OMLformulation that is able to predict the plasma response and hence the dustcharge. Numerical solutions of the new OML model show that the widely-usedWhipple approximation of dust charge-potential relationship agrees with OMLtheory in the limit of small dust radius compared with plasma Debye length, butincurs large (order-unity) deviation from the OML prediction when the dust sizebecomes comparable with or larger than plasma Debye length. This latter case isexpected for the important application of dust particles in a tokamak plasma.
机译:尘埃等离子体的基础理论是尘埃带电理论,该理论提供了尘埃电势和尘埃与等离子体的相互作用所产生的电荷。带负电的尘埃粒子使用最广泛的尘埃带电理论是所谓的轨道运动限制(OML)理论,该理论可以准确预测各种应用的尘埃势能和热量收集,但是以前发现它无法评估尘埃带电和等离子体在任何情况下都应作出回应。在这里,我们报告了一种经过修订的OML公式,该公式能够预测等离子体响应并因此预测粉尘电荷。新的OML模型的数值解表明,与等离子体Debye长度相比,广泛使用的Whipple逼近尘埃电势关系与OML理论在小尘埃半径的限制内是一致的,但是当OML预测与OML预测相比出现较大的(有序性)偏差时。尘埃尺寸变得等于或大于等离子德拜长度。后一种情况可预期用于托卡马克等离子体中灰尘颗粒的重要应用。

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