Physics – Optics
Scientific paper
Sep 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009cqgra..26q5007v&link_type=abstract
Classical and Quantum Gravity, Volume 26, Issue 17, pp. 175007 (2009).
Physics
Optics
4
Scientific paper
Silicon is under consideration as a substrate material for the mirror masses and quasi-monolithic suspension stages of 'third generation' gravitational wave detectors. Identifying a jointing technique to attach the silicon suspension elements to the optics with repeatable high strength and low mechanical loss is critical. Hydroxide-catalysis bonding is the method of choice for current quasi-monolithic silica suspensions. Here we present measurements of the shear strength of hydroxide-catalysis bonds between silicon samples. Strengths of approximately 3.9 N mm-2 are found, comparable to strengths found for silica to silica bonds. Scanning electron microscope imaging shows that the bonds between two silicon parts with thermally grown SiO2 layers are wedged with bond thicknesses varying from 30 nm to several micrometres. We suggest a possible explanation for this observation.
Bezensek B.
Cunningham W.
Hough James
Martin Ivar
Murray Pat
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