Paper
9 May 2013 Slumping of Si wafers at high temperature
M. Mika, O. Jankovsky, P. Simek, O. Lutyakov, R. Havlikova, Z. Sofer, R. Hudec, L. Pina, A. Inneman, L. Sveda, V. Marsikova
Author Affiliations +
Abstract
Space X-ray imaging telescopes have delivered unique observations that have been significantly contributing to many important discoveries of current astrophysics. For future telescopes with a larger collecting area and a better angular resolution, the limiting factor is their X-ray reflecting mirror array. Therefore, for a successful construction of future lightweight and highly reflecting X-ray mirrors, new cost-effective technologies and progressive materials are needed. Currently, the very promising materials are silicon foils which are commercially produced on a large scale. We focused on the plastic deformation of thin monocrystalline silicon foils, which was necessary for the precise thermal forming of the foils to 3D shapes. To achieve the plastic deformation, we applied forced slumping at temperatures from 1200 to 1400°C. The final shapes and the surface quality of the foils were measured using a Taylor Hobson contact profilometer and examined with an Atomic Forced Microscopy. We studied the effects of temperature, applied slumping force, heattreatment time, crystal orientation, and furnace atmosphere on the shape and surface quality of the formed foils.
© (2013) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
M. Mika, O. Jankovsky, P. Simek, O. Lutyakov, R. Havlikova, Z. Sofer, R. Hudec, L. Pina, A. Inneman, L. Sveda, and V. Marsikova "Slumping of Si wafers at high temperature", Proc. SPIE 8777, Damage to VUV, EUV, and X-ray Optics IV; and EUV and X-ray Optics: Synergy between Laboratory and Space III, 87770Z (9 May 2013); https://doi.org/10.1117/12.2021586
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KEYWORDS
Silicon

Semiconducting wafers

Space telescopes

X-ray telescopes

Mirrors

Crystals

X-rays

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