Presentation + Paper
29 August 2022 Low thermal expansion at cryogenic temperature in Fe39-xCo49+xCr10Ni2 alloy used for astronomical telescopes
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Abstract
Fe39Co49Cr10Ni2 has exhibited ultra-low thermal expansion with its average coefficient of approximately 0.13 × 10−6/K between 100 K and 300 K from cryogenic to room temperatures. This value is extremely close to that of the fused silica used for cameras and spectrographs mounted on astronomical telescopes. The nature of the low thermal expansion of Fe39−xCo49+xCr10Ni2 has been clarified by the measurements of the magnetic properties and the numerical simulations based on the path-integral effective-classical-potential theory. The saturation magnetization is found to decrease with increasing temperature in the range from 100 K to 350 K. The rate of decrease becomes larger at temperatures over 150 K. The numerical calculation has shown that this magnetic behavior is attributed to the electronic state changes from high spin state to low spin state in the Co atoms, which occurs at temperatures over 150 K. The electronic state changes in Co atoms are found to strongly contribute to the low thermal expansion for the first time in Fe39−xCo49+xCr10Ni2.
Conference Presentation
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Hiromichi T. Fujii, Naoki Sakaguchi, Kotaro Ona, Fumihiro Uraguchi, Yutaka Hayano, and Toshihiko Yokoyama "Low thermal expansion at cryogenic temperature in Fe39-xCo49+xCr10Ni2 alloy used for astronomical telescopes", Proc. SPIE 12188, Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation V, 1218806 (29 August 2022); https://doi.org/10.1117/12.2626196
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KEYWORDS
Iron

Magnetism

Chemical species

Cryogenics

Temperature metrology

Cobalt

Astronomical telescopes

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