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Extreme UV optical constants of rare-earth metals free from effects of air contamination

机译:不受空气污染影响的稀土金属的极高UV光学常数

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The determination of EUV optical constants in rare-earth metals is much hampered by the high reactivity and easy air contamination of these materials. The most difficult regions are a long wavelengths part of the EUV interval and the vicinity of absorbtion edges. In this study the optical constants of La and Tb are determined in a wide energy interval 14-400 eV. The study is performed by our recent method, which is suitable for reactive materials and for intervals around the absorption edges of elements. The samples are identically protected films with thickness ~10 nm or ~100 nm, which are deposited on silicon photodiodes. Mathematical treatment separates the contributions of a capping layer and a rare-earth metal and provides data which are free from the effects of air contamination. The precision and behavior of optical constants, as well as the parameters of the O_(2,3) and N_(4,5) edges in La and Tb are analyzed.
机译:稀土金属中EUV光学常数的测定由于这些材料的高反应性和易受空气污染而受到很大阻碍。最困难的区域是EUV间隔的长波部分以及吸收边缘附近。在这项研究中,La和Tb的光学常数在14-400 eV的宽能量区间内确定。该研究是通过我们最近的方法进行的,该方法适用于反应性材料以及元素吸收边缘周围的间隔。样品是厚度相同的保护膜,厚度约为10nm或100nm,沉积在硅光电二极管上。数学处理将覆盖层和稀土金属的作用分开,并提供不受空气污染影响的数据。分析了光学常数的精度和行为,以及La和Tb中O_(2,3)和N_(4,5)边的参数。

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