2002
DOI: 10.1088/0953-8984/14/8/333
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A Raman scattering study of the phase transitions in SrTiO3and in the mixed system (Sr1-xCax)TiO3at ambient pressure fromT= 300 K down to 8 K

Abstract: The room-temperature Raman spectra of Sr 1−x Ca x TiO 3 (SCT) for x = 0.06 (SCT06), 0.12 (SCT12) and 0.30 (SCT30) are shown to contain first-order Raman lines corresponding to E g and B 1g modes, which appear below 105 K in pure SrTiO 3 . The E g line shows slight asymmetry, indicating the orthorhombic structure of SCT for x 0.06. The low-temperature Raman spectra of SCT06 and SCT12 contain Raman-active modes of symmetry B 2g and E g , predicted by group theory but not observed in SrTiO 3 or SCT0.7 (x = 0.007)… Show more

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Cited by 63 publications
(61 citation statements)
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“…52 A single low frequency peak positioned at 80 cm −1 of antiferroelectric origin was also observed in the antiferroelectric perovskite Sr 0.70 Ca 0.30 TiO 3 . 55 Consistent with these related compounds, we assign the 60 cm −1 mode in Bi 0.8 La 0.2 FeO 3 to an antiferroelectric displacement of the A site.…”
Section: The La20 Structuresupporting
confidence: 76%
“…52 A single low frequency peak positioned at 80 cm −1 of antiferroelectric origin was also observed in the antiferroelectric perovskite Sr 0.70 Ca 0.30 TiO 3 . 55 Consistent with these related compounds, we assign the 60 cm −1 mode in Bi 0.8 La 0.2 FeO 3 to an antiferroelectric displacement of the A site.…”
Section: The La20 Structuresupporting
confidence: 76%
“…A recently proposed phase diagram is reproduced in Figure 1, after Carpenter et al (2006a). For Ca-rich compositions, the sequence of transitions with falling temperature is Pandey, 1999, 2001a;Ranjan et al, 2000;Mishra et al, 2001;Ouillon et al, 2002;Ranson et al, 2005;Mishra et al, 2005Mishra et al, , 2006a, and there has been a further suggestion of monoclinic symmetry (Woodward et al, 2006). From an earth sciences perspective, the CST solid solution has…”
Section: Introductionmentioning
confidence: 90%
“…3(a), which hardens upon cooling, corresponds to an A 1g phonon mode. [8][9][10][11] This mode disappears above the well-known STO antiferrodistortive (AFD) structural transition temperature 105 K. [12] The second peak (labeled by the blue marker) lying very close to the A 1g peak has very distinct features. This mode softens upon cooling, and saturates in energy at low temperature ( Fig.…”
mentioning
confidence: 98%
“…STO undergoes the cubic-tetragonal AFD transition when cooled below 105 K, which allows the appearance of the A 1g Raman mode. [8,9,11] The AFD is a nonpolar structural distortion which suppresses the competing FE instability. [21] (See illustrations in Fig.…”
mentioning
confidence: 99%