Abstract

We developed an extreme ultraviolet (EUV) scatterometer equipped with a table-top EUV source for the characterization of nanoscale grating lines. Appropriate orders of high-harmonic generation at wavelengths ranging from 25 to 35 nm are selected as the coherent light source for high-resolution spatial performance. It is shown that the grating surface profile significantly affects the scattered diffraction intensities and can be retrieved by the structure reconstruction algorithms using inverse modeling by rigorous coupled wave analysis.

Highlights

  • Scatterometry is an optical metrology technique designed for analyzing the changes of light intensity in a device

  • The scatterometers used in the semiconductor industry are typically specular spectroscopic systems, which work at a fixed angle of incidence but in broadband wavelengths range in the visible or UV, and measure only the zeroth-order diffraction

  • The diffraction angles were calculated from arctangent of jxi − x0j∕R, where jxi − x0j is the distance between the diffraction peaks (m 1⁄4 Æ1) and the CCD center

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Summary

Introduction

Scatterometry is an optical metrology technique designed for analyzing the changes of light intensity in a device. The scatterometers used in the semiconductor industry are typically specular spectroscopic systems, which work at a fixed angle of incidence but in broadband wavelengths range in the visible or UV, and measure only the zeroth-order diffraction. In contrast to variableangle and specular spectroscopic scatterometries, the proposed extreme ultraviolet (EUV) scatterometer is designed to measure the intensity of nonzeroth-order diffraction at a fixed incident angle and at multiple laser-like wavelengths. A microscopic translation stage, for mounting the CCD, was designed to adjust the distance between the grating target and the CCD detector in a range of 25.0 to 40.5 mm This allows both the m 1⁄4 þ1 and −1 diffracted beams to be directly and simultaneously collected by the CCD camera with maximal spatial resolution. The comparison with CD measurements using a cross-sectional scanning electron microscope (SEM) showed a good correlation of the results

Sample Details
Grating Equation for HHG Wavelengths Calibration
Theoretical Model of Grating-Diffraction Response of HHG
Diffraction Intensities Correction
Library Match Process
HHG Wavelengths Determination
Library Generation and Matching Process
Summary
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