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Research Article | Open Access

In-situ observation and mechanism of calcium–magnesium–alumina–silicate (CMAS) melts-induced degradation of RE2SiO5 (RE = Tb, Dy, Ho, Y, Er, Tm, and Yb) ceramics at 1500 °C

Zhilin TianaKeyu MingaLiya Zhenga( )Zhilin ChenaFan ZhouaPeng LiuaZihao QiuaDonghui WeibBin Lia( )Jingyang Wangc( )
School of Materials, Shenzhen Campus of Sun Yat-sen University, Shenzhen 518107, China
School of Metallurgy, Northeastern University, Shenyang 110819, China
Shenyang National Laboratory for Materials Science, Institute of Metal Research, Chinese Academy of Sciences, Shenyang 110016, China
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Abstract

Rare earth (RE) silicate is one of the most promising environmental barrier coatings for silicon-based ceramics in gas turbine engines. However, calcium–magnesium–alumina–silicate (CMAS) corrosion becomes much more serious and is the critical challenge for RE silicate with the increasing operating temperature. Therefore, it is quite urgent to clarify the mechanism of high-temperature CMAS-induced degradation of RE silicate at relatively high temperatures. Herein, the interaction between RE2SiO5 and CMAS up to 1500 ℃ was investigated by a novel high-temperature in-situ observation method. High temperature promotes the growth of the main reaction product (Ca2RE8(SiO4)6O2) fast along the [001] direction, and the precipitation of short and horizontally distributed Ca2RE8(SiO4)6O2 grains was accelerated during the cooling process. The increased temperature increases the solubility of RE elements, decreases the viscosity of CMAS, and thus elevates the corrosion reaction rate, making RE2SiO5 fast interaction with CMAS and less affected by RE element species.

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Journal of Advanced Ceramics
Pages 2315-2330
Cite this article:
Tian Z, Ming K, Zheng L, et al. In-situ observation and mechanism of calcium–magnesium–alumina–silicate (CMAS) melts-induced degradation of RE2SiO5 (RE = Tb, Dy, Ho, Y, Er, Tm, and Yb) ceramics at 1500 °C. Journal of Advanced Ceramics, 2023, 12(12): 2315-2330. https://doi.org/10.26599/JAC.2023.9220822

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Received: 14 August 2023
Revised: 25 October 2023
Accepted: 26 October 2023
Published: 04 January 2024
© The Author(s) 2023.

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