Coexisting magnetic structures and spin-reorientation in Er0.5_{0.5}Dy0.5_{0.5}FeO3_{3}: Bulk magnetization, neutron scattering, specific heat, and \emph{Ab-initio} studies

preprint2021arXivOpen access

Abstract

The complex magnetic structures, spin-reorientation and associated exchange interactions have been investigate in Er0.5_{0.5}Dy0.5_{0.5}FeO3_3 using bulk magnetization, neutron diffraction, specific heat measurements and density functional theory calculations. The Fe3+^{3+} spins order as G-type antiferromagnet structure depicted by Γ4Γ_{4}(GxG_{x},AyA_{y},FzF_{z}) irreducible representation below 700K, similar to its end compounds. The bulk magnetization data indicate occurrence of the spin-reorientation and rare-earth magnetic ordering below ∼\sim75 K and 10 K, respectively. The neutron diffraction studies confirm an "incomplete" Γ4Γ_{4}→{\rightarrow} Γ2Γ_{2}(FxF_{x},CyC_{y},GzG_{z}) spin-reorientation initiated ≤\leq75 K. Although, the relative volume fraction of the two magnetic structures varies with decreasing temperature, both co-exist even at 1.5 K. At 8 K, Er3+^{3+}/Dy3+^{3+} moments order as cyRc_{y}^R arrangement develop, which gradually increases in intensity with decreasing temperature. At 2 K, magnetic structure associated with czRc_{z}^R arrangement of Er3+^{3+}/Dy3+^{3+} moments also appears. At 1.5 K the magnetic structure of Fe3+^{3+} spins is represented by a combination of Γ2Γ_{2}+Γ4Γ_{4}+Γ1Γ_{1}, while the rare earth moments coexists as cyRc_{y}^R and czRc_{z}^R corresponding to Γ2Γ_{2} and Γ1Γ_{1} representation, respectively. The observed Schottky anomaly at 2.5 K suggests that the "rare-earth ordering" is induced by polarization due to Fe3+^{3+} spins. The Er3+^{3+}-Fe3+^{3+} and Er3+^{3+}-Dy3+^{3+} exchange interactions, obtained from first principle calculations, primarily cause the complicated spin-reorientation and cyRc_{y}^R rare-earth ordering, respectively, while the dipolar interactions between rare-earth moments, result in the czRc_{z}^R type rare-earth ordering at 2 K.

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