You have requested a machine translation of selected content from our databases. This functionality is provided solely for your convenience and is in no way intended to replace human translation. Neither SPIE nor the owners and publishers of the content make, and they explicitly disclaim, any express or implied representations or warranties of any kind, including, without limitation, representations and warranties as to the functionality of the translation feature or the accuracy or completeness of the translations.
Translations are not retained in our system. Your use of this feature and the translations is subject to all use restrictions contained in the Terms and Conditions of Use of the SPIE website.
20 September 2013Extreme ultraviolet mask defect observation using an extreme ultraviolet microscope
To predict the effect of a phase defect position relative to the absorber pattern on a wafer printed image, a programmed
phase defect mask was fabricated, and was observed using an extreme ultraviolet (EUV) microscope employing EUV
light from a beam line BL3 of the New SUBARU at the University of Hyogo. The mask prepared for this work contains
programmed phase defects along with half-pitch (hp) 64 nm lines-and-spaces (L/S) absorber patterns. The phase defects
were located at different locations in reference to the absorber lines. A lithography simulator predicted that when the
distance between the line center and defect center range from 26 to 102 nm, the prepared 1.8 nm-high and 57.4 nm-wide
phase defects would cause errors of more than 10 % in wafer printed critical dimension (CD). The EUV microscope
could identify these phase defects with the EUV light intensity losses of more than 17 % in comparison to the space
pattern image intensity in the absence of the phase defect. The EUV microscope can predict the existence of the phase
defect, and its impact on a wafer printed CD even where the EUV microscope does not completely emulate the image of
the EUV scanner.