Ultra-thin-film characterization with vacuum ultraviolet spectroscopic reflectometry (VUV-SR)

I. Burki, C. Rivas
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引用次数: 1

Abstract

Vacuum ultraviolet spectroscopic reflectometry (VUV SR) is a non-destructive, thin film measurement technique extending traditional reflectance spectroscopy to complex, multi band-gap, films stacks. The VUV SR system is a high throughput, production worthy metrology tool, able to resolve ultra-thin, multi-layer films in a single, broad band (800nm down to 120nm) spectral measurement. The dispersion in the films at the smaller VUV wavelengths allows high resolution of disparate thickness, optical properties and composition within thin film systems, not possible with existing UV optical methods. Optical systems such as spectroscopic ellipsometers (SE) are unable to resolve wide band gap films such as the SiO2-like interface layer between a Hf-based high-k layer and a Si substrate due to intrinsic hardware limitations of the low wavelength range (typically below 150nm). Absorption in the films begins to dominate at incident wavelengths below 190nm, resulting in enhanced reflectance resolution. The resolution of multiple band-gap films being used in sub-45nm semiconductor device manufacturing technology, includes individual films with absorption peaks in the broadband, and less than 190nm (190-150nm, 150-130nm and 130-120nm) wavelength ranges. Applying fitting models and optical properties to the reflectance data, the thicknesses of individual films and their composition can be determined.
真空紫外光谱反射法(VUV-SR)表征超薄膜
真空紫外光谱反射法(VUV SR)是一种非破坏性的薄膜测量技术,将传统的反射光谱技术扩展到复杂的、多带隙的薄膜层。VUV SR系统是一种高通量,具有生产价值的计量工具,能够在单个宽带(800nm至120nm)光谱测量中解决超薄多层薄膜。在较小的紫外波长下,薄膜中的色散可以在薄膜系统中实现不同厚度、光学性质和成分的高分辨率,这是现有紫外光学方法无法实现的。由于低波长范围(通常低于150nm)固有的硬件限制,诸如光谱椭偏仪(SE)之类的光学系统无法分辨宽带隙薄膜,例如基于hf的高k层和Si衬底之间的类似sio2的界面层。在入射波长低于190nm时,薄膜中的吸收开始占主导地位,从而提高了反射分辨率。用于sub-45nm半导体器件制造技术的多带隙薄膜的分辨率,包括具有宽带吸收峰的单个薄膜,以及小于190nm (190-150nm, 150-130nm和130-120nm)波长范围。通过对反射率数据的拟合模型和光学性质,可以确定单个薄膜的厚度及其组成。
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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