2015
DOI: 10.1103/physrevb.92.035414
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Polar catastrophe and the structure ofKTa1xNbxO3surfaces: Resu

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Cited by 3 publications
(8 citation statements)
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“…4 For the KTN targets, the data for the phonons below the Einstein mode appear to be dispersive, but the data are quite noisy, and surface phonon modes could be identified only over less than a half of the SBZ. [5][6][7] We believe that the existence of the Einstein mode for all these materials is consistent with the picture of the surface noted above, composed of potassium and oxygen ions. 7 However, the DS data for the 30% Nb targets suggest a more complex picture.…”
Section: Introductionsupporting
confidence: 88%
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“…4 For the KTN targets, the data for the phonons below the Einstein mode appear to be dispersive, but the data are quite noisy, and surface phonon modes could be identified only over less than a half of the SBZ. [5][6][7] We believe that the existence of the Einstein mode for all these materials is consistent with the picture of the surface noted above, composed of potassium and oxygen ions. 7 However, the DS data for the 30% Nb targets suggest a more complex picture.…”
Section: Introductionsupporting
confidence: 88%
“…This mode is essentially the same for all (001) surfaces studied in both the h10i and h11i azimuths. 7 For the pure KTaO 3 surface, a second lower energy dispersionless branch was measured in the h10i azimuth at 80 K and in the h11i azimuth at 140 K. However, at higher temperatures in both h10i and h11i, these lower energy phonon modes are found to be dispersive, but the curves extend over less than half the SBZ. 4 For the KTN targets, the data for the phonons below the Einstein mode appear to be dispersive, but the data are quite noisy, and surface phonon modes could be identified only over less than a half of the SBZ.…”
Section: Introductionmentioning
confidence: 87%
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