Paper
12 June 2018 Minimizing "Tone Reversal" during 19x nm mask inspection
Author Affiliations +
Abstract
19x nm defect inspection is the strongest candidate for initial EUV production until high-throughput E-Beam or Actinic inspection is ready. However, EUV mask inspection on an optical, 19x nm wavelength tool has some difficulties compared to optical masks. The issue of varying base pattern contrast is an example of one such difficulty. This paper explores the defect sensitivity differences among the base pattern sizes, as well as the relationship between base pattern contrast and defect sensitivity. Focus offset and polarization adjustments on programmed defect test masks are used to create new inspection recipes.
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Kazunori Seki, Karen Badger, Masashi Yonetani, Anka Birnstein, Jan Heumann, Takeshi Isogawa, Toshio Konishi, and Yutaka Kodera "Minimizing "Tone Reversal" during 19x nm mask inspection", Proc. SPIE 10807, Photomask Japan 2018: XXV Symposium on Photomask and Next-Generation Lithography Mask Technology, 108070D (12 June 2018); https://doi.org/10.1117/12.2502006
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Cited by 1 scholarly publication.
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KEYWORDS
Inspection

Photomasks

Extreme ultraviolet

Polarization

Opacity

Defect detection

Deep ultraviolet

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