Distortion-Dependent Raman Spectra and Mode Mixing in RMnO3 Perovskites
| dc.creator | Iliev, M. N. | |
| dc.creator | Abrashev, M. V. | |
| dc.creator | Laverdiere, J. | |
| dc.creator | Jandl, S. | |
| dc.creator | Gospodinov, M. M. | |
| dc.creator | Wang, Y. -Q. | |
| dc.creator | Sun, Y. -Y. | |
| dc.date | 2005-10-07 | |
| dc.date.accessioned | 2026-07-07T06:44:11Z | |
| dc.date.available | 2026-07-07T06:44:11Z | |
| dc.description | 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 rR as a whole confirms the commonly accepted Raman line assignments with two noticeable exceptions: (1) with decreasing rR the stretching Ag(1) and bending Ag(3) modes strongly mix for R=Sm to Tb, while for further decrease or rR (R=Dy,Ho,Y) the Ag(3) mode is observed at higher frequency than Ag(1) mode; (2) similar distortion-dependent mode mixing takes place for the rotational Ag(2) and O1(x) [Ag(7)] modes. The mode mixing is particularly strong for the RMnO3 compounds with rR values close to the transition from A-type to incommensurate sinusoidal antiferromagnetic ordering at low temperatures. The frequency of rotational Ag(2) and Ag(4) modes scales to the angles of MnO6 [101] and [010] rotations, respectively, and could be used as a measure of their value. | |
| dc.identifier | https://arxiv.org/abs/cond-mat/0510198 | |
| dc.identifier | http://arxiv.org/abs/cond-mat/0510198 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/102696 | |
| dc.subject | Materials Science | |
| dc.subject | Strongly Correlated Electrons | |
| dc.title | Distortion-Dependent Raman Spectra and Mode Mixing in RMnO3 Perovskites | |
| dc.type | text |