Origin of the multiferroic spiral spin-order in the RMnO3 perovskites
| dc.creator | Dong, Shuai | |
| dc.creator | Yu, Rong | |
| dc.creator | Yunoki, Seiji | |
| dc.creator | Liu, J. -M. | |
| dc.creator | Dagotto, Elbio | |
| dc.date | 2008-07-15 | |
| dc.date | 2008-10-21 | |
| dc.date.accessioned | 2026-07-07T10:11:56Z | |
| dc.date.available | 2026-07-07T10:11:56Z | |
| dc.description | The origin of the spiral spin-order in perovskite multiferroic manganites $R$MnO$_{3}$ ($RE=$ Tb or Dy) is here investigated using a two $e_{\rm g}$-orbitals double-exchange model. Our main result is that the experimentally observed spiral phase can be stabilized by introducing a relatively weak next-nearest-neighbor superexchange coupling ($\sim10%$ of the nearest-neighbor superexchange). Moreover, the Jahn-Teller lattice distortion is also shown to be essential to obtain a realistic spiral period. Supporting our conclusions, the generic phase diagram of undoped perovskite manganites is obtained using Monte Carlo simulations, showing phase transitions from the A-type antiferromagnet, to the spiral phase, and finally to the E-type antiferromagnet, with decreasing size of the $R$ ions. These results are qualitatively explained by the enhanced relative intensity of the superexchanges. | |
| dc.description | 6 pages, 4 figures | |
| dc.identifier | https://arxiv.org/abs/0807.2395 | |
| dc.identifier | http://arxiv.org/abs/0807.2395 | |
| dc.identifier | Phys. Rev. B 78, 155121 (2008) | |
| dc.identifier | doi:10.1103/PhysRevB.78.155121 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/172021 | |
| dc.subject | Strongly Correlated Electrons | |
| dc.subject | Materials Science | |
| dc.title | Origin of the multiferroic spiral spin-order in the RMnO3 perovskites | |
| dc.type | text |