Apatite and garnet stability in the Al-Ca-Mg-Si-(Gd/Y/Yb)-O systems and implications for T/EBC: CMAS reactions

This work advances the understanding of the influence of rare earth (RE) ion radius on the stability and extent of the garnet solid solution phase in the (ytterbia/yttria/gadolinia)-calcia-magnesia-alumina-silica systems. Guided by the crystal chemistry and charge neutrality constraints, selected compositions in the notional garnet stability field were synthesized, equilibrated at 1400 degrees C, and characterized to determine the equilibrium phases and their compositions. The results show a significant reduction in the stability of the silicate garnet relative to apatite with increasing RE ion radius. Apatite was not observed for any composition in the Yb-containing system, the Y-containing system formed both garnet and apatite, and there was no evidence of silicate garnets in the Gd-containing system. However, despite the apparent differences in stability relative to apatite, the extent of the garnet solid solution increases only slightly for the Yb- compared to Y-containing systems. The quantitative microchemical analysis suggests that Mg2+ prefers the octahedral site over the dodecahedral site in the garnet structure, and that the solubility of Mg2+ in the dodecahedral site increased in the system containing Yb3+ compared to Y3+. The results are discussed for their relevance to reactions between RE-containing thermal and environmental barrier coatings and CMAS-type silicate deposits.

Automated summary

This study investigates the influence of rare earth ion radius on the stability and extent of the garnet solid solution phase. Results show a reduction in stability of silicate garnet with increasing rare earth ion radius. Different rare earth systems exhibit varied phases formation, but the extent of the garnet solid solution only slightly increases compared to apatite stability.