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首页> 外文期刊>Journal of nanoscience and nanotechnology >Recent Progress on RE_2O_3-Mo/W Emission Materials
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Recent Progress on RE_2O_3-Mo/W Emission Materials

机译:RE_2O_3-Mo / W排放材料的最新进展

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摘要

RE_2O_3-Mo/W cathodes were prepared by powder metallurgy method. La_2O_3-Y_2O_3-Mo cermet cathodes prepared by traditional sintering method and spark plasma sintering (SPS) exhibit different secondary emission properties. The La_2O_3-Y_2O_3-Mo cermet cathode prepared by SPS method has smaller grain size and exhibits better secondary emission performance. Monte carlo calculation results indicate that the secondary electron emission way of the cathode correlates with the grain size. Decreasing the grain size can decrease the positive charging effect of RE_2O_3 and thus is favorable for the escaping of secondary electrons to vacuum. The Scandia doped tungsten matrix dispenser cathode with a sub-micrometer microstructure of matrix with uniformly distributed nanometer-particles of Scandia has good thermionic emission property. Over 100 A/cm~2 full space charge limited current density can be obtained at 950C_b. The cathode surface is covered by a Ba-Sc-O active surface layer with nano-particles distributing mainly on growth steps of W grains, leads to the conspicuous emission property of the cathode.
机译:采用粉末冶金法制备了RE_2O_3-Mo / W阴极。通过传统的烧结方法和火花等离子体烧结(SPS)制备的La_2O_3-Y_2O_3-Mo金属陶瓷阴极表现出不同的二次发射性能。采用SPS法制备的La_2O_3-Y_2O_3-Mo金属陶瓷阴极晶粒尺寸较小,二次发射性能更好。蒙特卡洛计算结果表明,阴极的二次电子发射方式与晶粒尺寸有关。减小晶粒尺寸可以降低RE_2O_3的正电荷效应,因此有利于二次电子逃逸至真空。具有亚微米微观结构的基质和具有均匀分布的Scandia纳米颗粒的Scandia掺杂钨基体分配器阴极具有良好的热电子发射性能。在950C_b时可获得超过100 A / cm〜2的全空间电荷限制电流密度。阴极表面被Ba-Sc-O活性表面层覆盖,纳米颗粒主要分布在W晶粒的生长步骤上,从而导致阴极显着的发射特性。

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