30年的加速器高强度负离子源

V. Dudnikov
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引用次数: 5

摘要

30年前,1971年7月1日,人们首次观察到铯混合物后气体放电中负离子发射的显著增强。这一观察结果为表面等离子体源(SPS)的发展奠定了基础,SPS通过等离子体粒子与电极的相互作用有效地产生负离子,而在电极上吸附的铯降低了表面功函数。负离子发射电流密度从平面阴极下的j/spl sim/ 10 mA/cm/sup 2/迅速增加到3.7 A/cm/sup 2/,在优化几何聚焦的长脉冲SPS中增加到8 A/cm/sup 2/,在直流SPS中增加到0.3 A/cm/sup 2/,最近增加到0.7 A/cm/sup 2/。电荷交换冷却的发现有助于将负离子温度T降低到1 eV以下,并将亮度提高了许多数量级,达到与最佳质子源相容的水平,B=j/T 1 a /cm/sup 2/ eV。SPS与电荷交换注入的结合改进了大型加速器的操作,并允许光束积累达到空间电荷极限,并多次克服了这一极限。早期用于加速器的SPS已经运行了25年,没有进行任何修改。将描述用于加速器的SPS的高级版本。将考虑负离子束形成、输运、空间电荷中和-过中和和不稳定阻尼的特点。将讨论SPS操作和高亮度光束生产的实际问题。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
30 years of high-intensity negative ion sources for accelerators
Thirty years ago, July 1, 1971, significant enhancement of negative ion emission from a gas discharge following an admixture of cesium was observed for the first time. This observation become the basis for the development of Surface Plasma Sources (SPS) for efficient production of negative ions from the interaction of plasma particles with electrodes on which adsorbed cesium reduced the surface work-function. The emission current density of negative ions increased rapidly from j/spl sim/ 10 mA/cm/sup 2/ to 3.7 A/cm/sup 2/ with a flat cathode and up to 8 A/cm/sup 2/ with an optimized geometrical focusing in the long pulse SPS, and to 0.3 A/cm/sup 2/ for DC SPS, recently increased up to 0.7 A/cm/sup 2/. Discovery of charge-exchange cooling helped decrease the negative ion temperature T below 1 eV, and increase brightness by many orders to a level compatible with the best proton sources, B=j/T> 1 A/cm/sup 2/ eV. The combination of the SPS with charge-exchange injection improved large accelerator operation and has permitted beam accumulation up to the space-charge limit and overcome this limit several times. The early SPS for accelerators have been in operation without modification for /spl sim/25 years. An advanced version of the SPS for accelerators will be described. Features of negative ion beam formation, transportation, space-charge neutralization-overneutralization, and instability damping will be considered. Practical aspects of SPS operation and high brightness beam production will be discussed.
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