Abstract
In the present paper, the magnetic structure and spin reorientation of mixed rare-earth orthoferrite have been investigated. At room temperature, our neutron-diffraction measurements reveal that the magnetic structure of spins in belongs to irreducible representation () as observed in both parent compounds ( and ). The neutron-diffraction study also confirms the presence of a spin-reorientation transition where the magnetic structure of spins changes from to ) representation between 75 and 20 K while maintaining a G-type antiferromagnetic configuration. Such a gradual spin reorientation is unusual since the large single ion anisotropy of ions is expected to cause an abrupt ) rotation of the spins. At 10 K, the magnetic structure is represented by (). Unexpectedly, the structure of spins re-emerges below 10 K, which also coincides with the development of rare-earth () magnetic ordering having configuration. Such re-emergence of a magnetic structure has been a rare phenomenon in orthoferrites. The absence of a second-order phase transition in rare-earth ordering, interpreted from heat capacity data, suggests the prominent role of and exchange interactions. These interactions suppress the independent rare-earth magnetic ordering observed in both parent compounds due to exchange interactions. Our density-functional-theory calculations including Coulomb correlation and spin-orbit interaction effects () reveal that the C-type arrangement of rare-earth ions (), with () configuration for moments, is energetically very close to a phase with the same rare-earth magnetic ordering but () configuration of spins. Further, the and exchange interactions are observed to play significant roles in the complex spin reorientation with the re-emergence of at low temperature. Consistent with the experimental observations, our calculations established the mixed phase ( and ) to be the magnetic ground state of moments.
5 More- Received 29 June 2020
- Revised 9 September 2020
- Accepted 9 September 2020
DOI:https://doi.org/10.1103/PhysRevB.102.144432
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