Environmental-barrier coating ceramics for resistance against attack by molten calcia-magnesia-aluminosilicate (CMAS) glass: Part I, YAlO3 and γ-Y2Si2O7
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作者:
Turcer, Laura R.
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Brown Univ, Sch Engn, Providence, RI 02912 USABrown Univ, Sch Engn, Providence, RI 02912 USA
Turcer, Laura R.
[1
]
Krause, Amanda R.
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Brown Univ, Sch Engn, Providence, RI 02912 USA
Lehigh Univ, Dept Mat Sci & Engn, Bethlehem, PA 18015 USABrown Univ, Sch Engn, Providence, RI 02912 USA
Krause, Amanda R.
[1
,2
]
Garces, Hector F.
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Brown Univ, Sch Engn, Providence, RI 02912 USABrown Univ, Sch Engn, Providence, RI 02912 USA
Garces, Hector F.
[1
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Zhang, Lin
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Brown Univ, Sch Engn, Providence, RI 02912 USABrown Univ, Sch Engn, Providence, RI 02912 USA
Zhang, Lin
[1
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Padture, Nitin P.
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Brown Univ, Sch Engn, Providence, RI 02912 USABrown Univ, Sch Engn, Providence, RI 02912 USA
Padture, Nitin P.
[1
]
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[1] Brown Univ, Sch Engn, Providence, RI 02912 USA
[2] Lehigh Univ, Dept Mat Sci & Engn, Bethlehem, PA 18015 USA
The high-temperature (1500 degrees C) interactions of two promising dense, polycrystalline EEC ceramics, YAIO(3) (YAP) and gamma-Y2Si2O7, with a calcia-magnesia-aluminosilicate (CMAS) glass have been explored as part of a model study. Despite the fact that the optical basicities of both the EBC ceramics and the CMAS are similar, they both react with the CMAS. In the case of the Si-free YAIO(3), the reaction zone is small and it comprises three regions of reaction-crystallization products, including Y-Ca-Si apatite solid -solution (ss) and Y3Al5O12 (YAG)(ss). In contrast, only Y-Ca-Si apatite(ss) forms in the case of Si-containing gamma-Y2Si2O7, and the reaction zone is an order-of magnitude thicker. These CMAS interactions are analyzed in detail, and are found to be strikingly different than those observed in Y-free EBC ceramics (beta-Yb2Si2O7 and beta-Sc2Si2O7) in the accompanying Part II paper. This is attributed to the presence of the Y in the YAIO(3) and gamma-Y2Si2O7 EBC ceramics.
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Ecole Natl Super Phys Grenoble, INPG, CNRS, UMR 5628,Lab Mat & Genie Phys, F-38402 St Martin Dheres, FranceEcole Natl Super Phys Grenoble, INPG, CNRS, UMR 5628,Lab Mat & Genie Phys, F-38402 St Martin Dheres, France
Chaix-Pluchery, O
;
Chenevier, B
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Ecole Natl Super Phys Grenoble, INPG, CNRS, UMR 5628,Lab Mat & Genie Phys, F-38402 St Martin Dheres, FranceEcole Natl Super Phys Grenoble, INPG, CNRS, UMR 5628,Lab Mat & Genie Phys, F-38402 St Martin Dheres, France
Chenevier, B
;
Robles, JJ
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Ecole Natl Super Phys Grenoble, INPG, CNRS, UMR 5628,Lab Mat & Genie Phys, F-38402 St Martin Dheres, FranceEcole Natl Super Phys Grenoble, INPG, CNRS, UMR 5628,Lab Mat & Genie Phys, F-38402 St Martin Dheres, France
机构:
Ecole Natl Super Phys Grenoble, INPG, CNRS, UMR 5628,Lab Mat & Genie Phys, F-38402 St Martin Dheres, FranceEcole Natl Super Phys Grenoble, INPG, CNRS, UMR 5628,Lab Mat & Genie Phys, F-38402 St Martin Dheres, France
Chaix-Pluchery, O
;
Chenevier, B
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Ecole Natl Super Phys Grenoble, INPG, CNRS, UMR 5628,Lab Mat & Genie Phys, F-38402 St Martin Dheres, FranceEcole Natl Super Phys Grenoble, INPG, CNRS, UMR 5628,Lab Mat & Genie Phys, F-38402 St Martin Dheres, France
Chenevier, B
;
Robles, JJ
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Ecole Natl Super Phys Grenoble, INPG, CNRS, UMR 5628,Lab Mat & Genie Phys, F-38402 St Martin Dheres, FranceEcole Natl Super Phys Grenoble, INPG, CNRS, UMR 5628,Lab Mat & Genie Phys, F-38402 St Martin Dheres, France