Journal article
Magneto-orbital ordering in the divalent A-site quadruple perovskite manganites AMn7O12(A=Sr, Cd, and Pb)
- Abstract:
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Through analysis of variable temperature neutron powder diffraction data, we present solutions for the magnetic structures of SrMn7O12, CdMn7O12, and PbMn7O12 in all long-range ordered phases. The three compounds were found to have magnetic structures analogous to that reported for CaMn7O12. They all feature a higher temperature lock-in phase with commensurate magneto-orbital coupling, and a delocked, multi-k magnetic ground state where incommensurate magneto-orbital coupling gives rise to a constant-moment magnetic helix with modulated spin helicity. CdMn7O12 represents a special case in which the orbital modulation is commensurate with the crystal lattice and involves stacking of fully and partially polarized orbital states. Our results provide a robust confirmation of the phenomenological model for magneto-orbital coupling previously presented for CaMn7O12. Furthermore, we show that the model is universal to the A quadruple perovskite manganites synthesised to date, and that it is tunable by selection of the A-site ionic radius.
- Publication status:
- Published
- Peer review status:
- Peer reviewed
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- Files:
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(Preview, Accepted manuscript, pdf, 3.7MB, Terms of use)
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- Publisher copy:
- 10.1103/PhysRevB.96.054448
Authors
- Publisher:
- American Physical Society
- Journal:
- Physical Review B More from this journal
- Volume:
- 96
- Issue:
- 5
- Pages:
- 054448
- Publication date:
- 2017-08-17
- Acceptance date:
- 2017-08-18
- DOI:
- EISSN:
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2469-9969
- ISSN:
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2469-9950
- Keywords:
- Pubs id:
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pubs:708360
- UUID:
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uuid:c1f7c8c0-08d2-4928-89b9-81498abc830a
- Local pid:
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pubs:708360
- Source identifiers:
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708360
- Deposit date:
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2017-09-12
Terms of use
- Copyright holder:
- American Physical Society
- Copyright date:
- 2017
- Notes:
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This is the author accepted manuscript following peer review version of the article. The final version is
available online from American Physical Society at: https://doi.org/10.1103/PhysRevB.96.054448
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