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Preparation and Characterization of Francisite Solid Solutions Cu3Bi(Se1–x Te x O3)2O2Br (x = 0–1): Possibility for Francisites as Starting Materials for Oxide van der Waals Ferromagnets

We synthesized the solid solutions Cu3Bi­(Se1–x Te x O3)2O2Br (x = 0, 0.25, 0.5, 0.75, 1) for the first time and characterized their structures by X-ray diffraction (XRD) measurements and their magnetic properties by electron spin resonance (ESR), magnetic susceptibility, magnetization, and specific...

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Published in:Chemistry of materials 2023-01, Vol.35 (2), p.511-520
Main Authors: Markina, Maria, Vasilchikova, Tatyana, Kuznetsova, Elena, Berdonosov, Peter, Olenev, Andrey, Chung, Seung Hwan, Koo, Hyun-Joo, Whangbo, Myung-Hwan, Vasiliev, Alexander
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container_issue 2
container_start_page 511
container_title Chemistry of materials
container_volume 35
creator Markina, Maria
Vasilchikova, Tatyana
Kuznetsova, Elena
Berdonosov, Peter
Olenev, Andrey
Chung, Seung Hwan
Koo, Hyun-Joo
Whangbo, Myung-Hwan
Vasiliev, Alexander
description We synthesized the solid solutions Cu3Bi­(Se1–x Te x O3)2O2Br (x = 0, 0.25, 0.5, 0.75, 1) for the first time and characterized their structures by X-ray diffraction (XRD) measurements and their magnetic properties by electron spin resonance (ESR), magnetic susceptibility, magnetization, and specific heat measurements as well as by density functional theory (DFT) calculations. The Néel temperature T N and the critical field μ 0 H C needed for the metamagnetic transition increase with x, while the magnetization at a given magnetic field and the Curie–Weiss temperature Θ decrease with x. We show that the tendency for the interlayer antiferromagnetic (AFM) coupling in francisites is not explained by interlayer spin exchange but by the interlayer high-spin orbital interaction that occur across the van der Waals (vdW) gaps, hence indicating that francisites are vdW ferromagnets. This is surprising because, so far, well-established vdW ferromagnets are either layered tellurides or layered iodides. The trends in T N, μ 0 H C, and the magnetization of Cu3Bi­(Se1–x Te x O3)2O2Br as a function of x are well explained by the interlayer AFM interactions, and that in the Θ is explained by the intralayer spin exchanges. We proposed how one might modify francisites to make their interlayer interactions ferromagnetic (FM), hence leading to oxide vdW ferromagnets.
doi_str_mv 10.1021/acs.chemmater.2c02865
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The Néel temperature T N and the critical field μ 0 H C needed for the metamagnetic transition increase with x, while the magnetization at a given magnetic field and the Curie–Weiss temperature Θ decrease with x. We show that the tendency for the interlayer antiferromagnetic (AFM) coupling in francisites is not explained by interlayer spin exchange but by the interlayer high-spin orbital interaction that occur across the van der Waals (vdW) gaps, hence indicating that francisites are vdW ferromagnets. This is surprising because, so far, well-established vdW ferromagnets are either layered tellurides or layered iodides. The trends in T N, μ 0 H C, and the magnetization of Cu3Bi­(Se1–x Te x O3)2O2Br as a function of x are well explained by the interlayer AFM interactions, and that in the Θ is explained by the intralayer spin exchanges. 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We show that the tendency for the interlayer antiferromagnetic (AFM) coupling in francisites is not explained by interlayer spin exchange but by the interlayer high-spin orbital interaction that occur across the van der Waals (vdW) gaps, hence indicating that francisites are vdW ferromagnets. This is surprising because, so far, well-established vdW ferromagnets are either layered tellurides or layered iodides. The trends in T N, μ 0 H C, and the magnetization of Cu3Bi­(Se1–x Te x O3)2O2Br as a function of x are well explained by the interlayer AFM interactions, and that in the Θ is explained by the intralayer spin exchanges. 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title Preparation and Characterization of Francisite Solid Solutions Cu3Bi(Se1–x Te x O3)2O2Br (x = 0–1): Possibility for Francisites as Starting Materials for Oxide van der Waals Ferromagnets
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