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Investigations of whisper gallery mirrors for extreme ultraviolet (EUV) and soft X-rays

机译:研究耳语走廊镜的极紫外(EUV)和柔和X射线

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The authors have examined optical constants and predicted reflectivities of candidate surface coatings for whisper gallery mirrors (WGMs) in the extreme ultraviolet. The spectral regime near 100-150 AA has been identified in the literature as particularly promising due to the high WGM reflectivities of the noble metals in the vicinity of their Cooper minima in this regime. The authors confirm this basic result using newer EUV optical data, and they have sought candidate surface materials which would extend the range over which WGMs may be used to longer wavelengths. It is found that substantial WGM reflectivities are predicted for a variety of elements in the EUV, and that TE peak reflection is larger than TM peak reflection by on the order of 10%; however, most of the elements which do reflect well have surfaces which are vulnerable to oxygen contamination.
机译:这组作者检查了光学常数,并预测了在极紫外线下耳语画廊镜(WGM)的候选表面涂层的反射率。在文献中已确定100-150 AA附近的光谱制度特别有前景,因为在这种制度下,贵金属在其库珀极值附近具有很高的WGM反射率。作者使用较新的EUV光学数据证实了这一基本结果,他们已经寻求候选表面材料,该材料将扩大WGM可以用于更长波长的范围。已经发现,对于EUV中的各种元素,可以预测出相当大的WGM反射率,并且TE峰反射比TM峰反射大大约10%;但是,大多数能很好反射的元素的表面都容易受到氧气污染。

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