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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 |
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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. We proposed how one might modify francisites to make their interlayer interactions ferromagnetic (FM), hence leading to oxide vdW ferromagnets.</description><identifier>ISSN: 0897-4756</identifier><identifier>EISSN: 1520-5002</identifier><identifier>DOI: 10.1021/acs.chemmater.2c02865</identifier><language>eng</language><publisher>American Chemical Society</publisher><ispartof>Chemistry of materials, 2023-01, Vol.35 (2), p.511-520</ispartof><rights>2022 American Chemical Society</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><orcidid>0000-0003-3558-6761 ; 0000-0002-3385-5801 ; 0000-0001-8642-8371 ; 0000-0002-2220-1124 ; 0000-0001-9232-8289</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,27903,27904</link.rule.ids></links><search><creatorcontrib>Markina, Maria</creatorcontrib><creatorcontrib>Vasilchikova, Tatyana</creatorcontrib><creatorcontrib>Kuznetsova, Elena</creatorcontrib><creatorcontrib>Berdonosov, Peter</creatorcontrib><creatorcontrib>Olenev, Andrey</creatorcontrib><creatorcontrib>Chung, Seung Hwan</creatorcontrib><creatorcontrib>Koo, Hyun-Joo</creatorcontrib><creatorcontrib>Whangbo, Myung-Hwan</creatorcontrib><creatorcontrib>Vasiliev, Alexander</creatorcontrib><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</title><title>Chemistry of materials</title><addtitle>Chem. Mater</addtitle><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.</description><issn>0897-4756</issn><issn>1520-5002</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><sourceid/><recordid>eNpNUc1Kw0AQXkTBWn0EYY7tIXV_kmwieNBgVaik0IrHsNls2i1tIrupRE--g-_jw_gkbmwRL_Pzzcw3zHwInRM8IpiSCyHtSC7VZiMaZUZUYhqFwQHqkYBiL8CYHqIejmLu-TwIj9GJtSuMiRuNeuhratSLMKLRdQWiKiBZukw6Iv2-A-sSxkZUUlvdKJjVa110dtsVLSRbdqMHM0W-Pz5bmCtoIWVDmtIbA4MWrgC7AhlewrS2Vud6rZs3KGvzj9OCsDBrhGl0tYDH7ggt1va3K211oeBVVFAoA8-iw8fKmHojFpVq7Ck6Kh2mzva-j57Gt_Pk3pukdw_J9cQTJOaN58dMySgoeOQzHFDGOS65lCyPOM39EtPQBZiKmJOcyJj4NAgZjQgLA1EUYcz6iOx43a-zVb01lduWEZx1AmQd-CdAtheA_QB9WX8Q</recordid><startdate>20230124</startdate><enddate>20230124</enddate><creator>Markina, Maria</creator><creator>Vasilchikova, Tatyana</creator><creator>Kuznetsova, Elena</creator><creator>Berdonosov, Peter</creator><creator>Olenev, Andrey</creator><creator>Chung, Seung Hwan</creator><creator>Koo, Hyun-Joo</creator><creator>Whangbo, Myung-Hwan</creator><creator>Vasiliev, Alexander</creator><general>American Chemical Society</general><scope/><orcidid>https://orcid.org/0000-0003-3558-6761</orcidid><orcidid>https://orcid.org/0000-0002-3385-5801</orcidid><orcidid>https://orcid.org/0000-0001-8642-8371</orcidid><orcidid>https://orcid.org/0000-0002-2220-1124</orcidid><orcidid>https://orcid.org/0000-0001-9232-8289</orcidid></search><sort><creationdate>20230124</creationdate><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</title><author>Markina, Maria ; Vasilchikova, Tatyana ; Kuznetsova, Elena ; Berdonosov, Peter ; Olenev, Andrey ; Chung, Seung Hwan ; Koo, Hyun-Joo ; Whangbo, Myung-Hwan ; Vasiliev, Alexander</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a197t-493ec85d78430523770f7cc3b872b4f02687202a971b1c9142563281365add693</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Markina, Maria</creatorcontrib><creatorcontrib>Vasilchikova, Tatyana</creatorcontrib><creatorcontrib>Kuznetsova, Elena</creatorcontrib><creatorcontrib>Berdonosov, Peter</creatorcontrib><creatorcontrib>Olenev, Andrey</creatorcontrib><creatorcontrib>Chung, Seung Hwan</creatorcontrib><creatorcontrib>Koo, Hyun-Joo</creatorcontrib><creatorcontrib>Whangbo, Myung-Hwan</creatorcontrib><creatorcontrib>Vasiliev, Alexander</creatorcontrib><jtitle>Chemistry of materials</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Markina, Maria</au><au>Vasilchikova, Tatyana</au><au>Kuznetsova, Elena</au><au>Berdonosov, Peter</au><au>Olenev, Andrey</au><au>Chung, Seung Hwan</au><au>Koo, Hyun-Joo</au><au>Whangbo, Myung-Hwan</au><au>Vasiliev, Alexander</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>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</atitle><jtitle>Chemistry of materials</jtitle><addtitle>Chem. Mater</addtitle><date>2023-01-24</date><risdate>2023</risdate><volume>35</volume><issue>2</issue><spage>511</spage><epage>520</epage><pages>511-520</pages><issn>0897-4756</issn><eissn>1520-5002</eissn><abstract>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.</abstract><pub>American Chemical Society</pub><doi>10.1021/acs.chemmater.2c02865</doi><tpages>10</tpages><orcidid>https://orcid.org/0000-0003-3558-6761</orcidid><orcidid>https://orcid.org/0000-0002-3385-5801</orcidid><orcidid>https://orcid.org/0000-0001-8642-8371</orcidid><orcidid>https://orcid.org/0000-0002-2220-1124</orcidid><orcidid>https://orcid.org/0000-0001-9232-8289</orcidid></addata></record> |
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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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