Distortion-dependent Raman spectra and mode mixing in RMnO3 perovskites (R=La,Pr,Nd,Sm,Eu,Gd,Tb,Dy,Ho,Y)

被引:237
作者
Iliev, MN [1 ]
Abrashev, MV
Laverdière, J
Jandl, S
Gospodinov, MM
Wang, YQ
Sun, YY
机构
[1] Univ Houston, Texas Ctr Superconduct, Houston, TX 77204 USA
[2] Univ Houston, Dept Phys, Houston, TX 77204 USA
[3] Univ Sofia, Fac Phys, Sofia 1164, Bulgaria
[4] Univ Sherbrooke, Dept Phys, Sherbrooke, PQ J1K 2R1, Canada
[5] Bulgarian Acad Sci, Inst Solid State Phys, BU-1184 Sofia, Bulgaria
来源
PHYSICAL REVIEW B | 2006年 / 73卷 / 06期
关键词
D O I
10.1103/PhysRevB.73.064302
中图分类号
T [工业技术];
学科分类号
08 ;
摘要
The polarized Raman spectra of orthorhombic RMnO3 series (R=La,Pr,Nd,Sm,Eu,Gd,Tb,Dy,Ho,Y) were studied at room temperature. The variation of phonon frequencies with R ionic radius r(R) as a whole confirms the commonly accepted Raman line assignments with two noticeable exceptions: (1) with decreasing r(R) the stretching A(g)(1) and bending A(g)(3) modes strongly mix for R=Sm to Tb, while for further decrease or r(R) (R=Dy,Ho,Y) the A(g)(3) mode is observed at higher frequency than A(g)(1) mode; (2) similar distortion-dependent mode mixing takes place for the rotational A(g)(2) and O1(x) [A(g)(7)] modes. The mode mixing is particularly strong for the RMnO3 compounds with r(R) values close to the transition from A type to incommensurate sinusoidal antiferromagnetic ordering at low temperatures. The frequency of rotational A(g)(2) and A(g)(4) modes scales to the angles of MnO6 [101] and [010] rotations, respectively, and could be used as a measure of their value.
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页数:6
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