Abstract
The conversion of Ba–Al2O3 –Si–SiO2, Ba–Al–Al2O3 –SiO2, and Ba–Sr–Al–Al2O3 –SiO2 precursors into monolithic, monoclinic celsian has been examined. The relative amounts of metal and oxide in each type of precursor were adjusted so that the overall stoichiometry and molar volume were similar to those of the desired product, celsian. Metal + oxide mixtures were mechanically alloyed and then uniaxially pressed to yield 84–92% dense precursor disks. The precursors were converted into celsian by exposure to a series of heat treatments from 300–1500 °C in oxygen-bearing gases. Differences and similarities in the phase evolution of the various precursors are discussed. Celsian disks were produced that retained the precursor shape, dimensions, and relative (% theoretical) density.
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JCPDS Cards: #01-1291 for Be; #20-0164 for BeO; #35-0821 for Mg; #45-0946 for MgO; #23-0430 for Ca; 37-1497 for CaO; #03-0865 for CaO2; #15-0306 for Sr; #06-0520 for SrO; #07-0234 for SrO2; #6-0235 for Ba; #22-1056 for BaO; #7-233 for BaO2; #4-0791 for Al; #43-1484 for a–Al2O3; #27-1402 for Si; #39-1425 for SiO2 (cristobalite); #33-1161 for SiO2 (quartz); #06-0696 for Fe; #25-1402 for Fe2O3; #06-0615 for FeO; #04-0836 for Cu; #05-0667 for Cu2O; #05-0682 for Ti; #24-1276 for TiO2 (rutile) #05-0665 for Zr; #36-420 for ZrO2; #08-0056 for Ce; #34-0394 for CeO2; #5-0378 for BaCO3; #26-1403 for Ba2SiO4; #26-1402 for b–BaSiO3; #26-176 for β–BaSi2O5; #17-306 for BaAl2O4; #31-1336 for β–SrAl2O4; #12-725 for orthorhombic (pseudo-hexagonal) BaAl2Si2O8; #28-125 for hexagonal BaAl2Si2O8; #38-1450 for monoclinic BaAl2Si2O8; #38-1452 for monoclinic Ba0.5Sr0.5Al2Si2O8; #22-511 for (Ba, Sr)SiO3; #20-143 for BaSrSi2O6; #39-1256 for Sr2SiO4.
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Allameh, S.M., Sandhage, K.H. The oxidative transformation of solid, barium-metal-bearing precursors into monolithic celsian with a retention of shape, dimensions, and relative density. Journal of Materials Research 13, 1271–1285 (1998). https://doi.org/10.1557/JMR.1998.0182
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DOI: https://doi.org/10.1557/JMR.1998.0182