2009
DOI: 10.1016/j.jallcom.2008.09.034
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Influence of the modifier on the short and long range disorder of stannate perovskites

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Cited by 40 publications
(15 citation statements)
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References 16 publications
(29 reference statements)
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“…According to the ICDD 76-0606, the peak at 27º indicated the presence of CaCO 3 as a secondary phase. The presence of CaCO 3 in CaSnO 3 and Ca 1-x Sr x SnO 3 samples was also confirmed in [26,27]. Fig.…”
Section: Characterization Of the Materialssupporting
confidence: 54%
See 1 more Smart Citation
“…According to the ICDD 76-0606, the peak at 27º indicated the presence of CaCO 3 as a secondary phase. The presence of CaCO 3 in CaSnO 3 and Ca 1-x Sr x SnO 3 samples was also confirmed in [26,27]. Fig.…”
Section: Characterization Of the Materialssupporting
confidence: 54%
“…The bands located at 870, 1051, and 1454 cm -1 were assigned to carbonate vibrations [31], and the band at 1643 cm -1 was associated with water angular deformation. The vibrations assigned to stannates (SnO 3 2-) generally produce highintensity bands in the infrared region at 300-400 cm -1 and 600-700 cm -1 with a band broadening typical of orthorhombic perovskite structures [27,32]. The mid-IR spectrum of CaSnO 3 showed a band at 641 cm -1 assigned to the stretching mode of Sn-O [33,34].…”
Section: Characterization Of the Materialsmentioning
confidence: 99%
“…In case of the SSSrSnO 3 powder, the Raman spectrum is in agreement with Zhang's previously reported result [11] in terms of the active modes of SrSnO 3 located at 119, 150, 168, 220, 257, 305, 403, 511, 596, 713 and 890 cm À1 . On the other hand, the Raman spectrum of SrSnO 3 nanoparticles is very different from that of SS-SrSnO 3 and bears more resemblance to Alves's result [20,21] where bands appear at 93, 108, 119, 152, 186, 227, 250, 261, 406, 577, 703 and 986 cm À1 . This difference has relevance to the incorporation of carbonate anions into the SrSnO 3 structure.…”
Section: Resultsmentioning
confidence: 76%
“…Stannates such as CaSnO 3 , SrSnO 3 and BaSnO 3 have been reported in the literature as compounds with the classic perovskite structure, with stoichiometry ABO 3 [1,2].…”
Section: Introductionmentioning
confidence: 99%