Development of extreme ultraviolet interferometry for laser plasma source operation

A. Ray-Chaudhuri, K. Krenz, R. Nissen, S. Haney, C. H. Fields, W. Sweatt, A. MacDowell
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引用次数: 1

Abstract

When characterizing an extreme ultraviolet (EUV) lithographic optical system, visible light interferometry is limited to measuring wavefront aberration caused by surface figure error while failing to measure wavefront errors induced by the multilayer coatings. This fact has generated interest in developing interferometry at an EUV camera's operational wavelength (at-wavelength testing), which is typically around 13 nm. While a laser plasma source (LPS) is being developed as a lithography production source, it has generally been considered that only an undulator located at a synchrotron facility can provide the necessary laser-like point source for EUV interferometry. Although an undulator-based approach has been successfully demonstrated, it would be advantageous to test a camera in its operational configuration. We are developing the latter approach by utilizing extended source size schemes to provide usable flux throughput. A slit or a grating mounted at the source plane can provide the necessary spatial coherence for lateral shearing interferometry. The usable source size is limited only by the well-corrected field of view of the camera under test. The development of this interferometer will be presented.
激光等离子体源操作极紫外干涉测量技术的发展
在对极紫外光刻光学系统进行表征时,可见光干涉测量仅限于测量由表面图形误差引起的波前像差,而无法测量由多层涂层引起的波前误差。这一事实引起了人们对在EUV相机的工作波长(at-波长测试)上开发干涉测量法的兴趣,该波长通常在13 nm左右。虽然激光等离子体源(LPS)正在作为光刻生产源进行开发,但通常认为只有位于同步加速器设施中的波动器才能为EUV干涉测量提供必要的类激光点源。虽然基于波动器的方法已经成功地证明了,但在其操作配置中测试相机将是有利的。我们正在开发后一种方法,利用扩展源大小方案来提供可用的通量吞吐量。在源平面上安装狭缝或光栅可以为横向剪切干涉测量提供必要的空间相干性。可用的光源尺寸仅受被测相机的良好校正视场的限制。本文将介绍该干涉仪的研制。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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