1965
DOI: 10.1103/physrev.138.a1537
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Dielectric Dispersion of Some Perovskite Zirconates

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Cited by 133 publications
(46 citation statements)
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“…The asymmetrical shape of the line extending from 210 to 290 cm −1 should be related with the high phonon density of states which prevails in this frequency region [7]. However, an additional feature at 119 cm −1 comes out in the rhombohedral phase of BTZ05 on cooling down to 15 K. This line was never reported before in BT, but previously detected from IR measurements in barium zirconate [8]. According to the mass ratio Zr/Ti (= 1.9), which is not very far from the square of the frequency ratio 180/119 (= 2.3), it could be associated with a normal mode involving Zr ions motion against the oxygen octahedra.…”
Section: Raman Scatteringmentioning
confidence: 71%
“…The asymmetrical shape of the line extending from 210 to 290 cm −1 should be related with the high phonon density of states which prevails in this frequency region [7]. However, an additional feature at 119 cm −1 comes out in the rhombohedral phase of BTZ05 on cooling down to 15 K. This line was never reported before in BT, but previously detected from IR measurements in barium zirconate [8]. According to the mass ratio Zr/Ti (= 1.9), which is not very far from the square of the frequency ratio 180/119 (= 2.3), it could be associated with a normal mode involving Zr ions motion against the oxygen octahedra.…”
Section: Raman Scatteringmentioning
confidence: 71%
“…[15,27] This feature had never been reported before in BT, but was previously detected in the infrared spectrum of BaZrO 3 . [34] On the basis of this observation, Farhi et al [27] have proposed that the feature arose from a normal mode involving Zr ions, which implies that nanometer-sized Zr (or Zr rich) zones exist, because otherwise the phonon lifetime would have been too short to result in a defined, separated Raman feature. On the other hand, on the basis of high-pressure Raman studies Kreisel et al [33] had excluded local pure BaZrO 3 zones and rather proposed Zr-rich domains, because of the fact that BaZrO 3 shows (for p > 12 Gpa) a well-defined Raman signature with sharp and intense bands at ∼400 and ∼620 cm −1 , which were not observed in the high-pressure Raman spectra.…”
Section: Resultsmentioning
confidence: 99%
“…The infrared-reflectivity spectra of SrTiO 3 and CaTiO 3 are shown, for comparison; the spectra of each end member are comparable to the literature (15,19 , which are assigned to the O-Ti-O bend and Figure 5a shows the Raman spectra of Sr 1Ϫx Ca x TiO 3 (x ϭ 0-1) in the frequency range 150-850 cm Ϫ1 . The Racation-TiO 3 lattice vibration, it seems hard to comment on their x dependence.…”
mentioning
confidence: 98%