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dc.contributor.authorXu, W.en
dc.contributor.authorDong, W.en
dc.contributor.authorLayek, S.en
dc.contributor.authorShulman, M.en
dc.contributor.authorGlazyrin, K.en
dc.contributor.authorBykova, E.en
dc.contributor.authorBykov, M.en
dc.contributor.authorHanfland, M.en
dc.contributor.authorPasternak, M. P.en
dc.contributor.authorLeonov, I.en
dc.contributor.authorGreenberg, E.en
dc.contributor.authorRozenberg, G. K.en
dc.date.accessioned2022-10-19T05:20:24Z-
dc.date.available2022-10-19T05:20:24Z-
dc.date.issued2022-
dc.identifier.citationPressure-induced high-spin/low-spin disproportionated state in the Mott insulator FeBO3 / W. Xu, W. Dong, S. Layek et al. // Scientific Reports. — 2022. — Vol. 12. — Iss. 1. — 9647.en
dc.identifier.issn20452322-
dc.identifier.otherhttps://www.scopus.com/inward/record.uri?eid=2-s2.0-85131788128&doi=10.1038%2fs41598-022-13507-4&partnerID=40&md5=b4731c1201bc6014e4bfac3d223a992dlink
dc.identifier.urihttp://elar.urfu.ru/handle/10995/117917-
dc.description.abstractThe pressure-induced Mott insulator-to-metal transitions are often accompanied by a collapse of magnetic interactions associated with delocalization of 3d electrons and high-spin to low-spin (HS-LS) state transition. Here, we address a long-standing controversy regarding the high-pressure behavior of an archetypal Mott insulator FeBO3 and show the insufficiency of a standard theoretical approach assuming a conventional HS-LS transition for the description of the electronic properties of the Mott insulators at high pressures. Using high-resolution x-ray diffraction measurements supplemented by Mössbauer spectroscopy up to pressures ~ 150 GPa, we document an unusual electronic state characterized by a “mixed” HS/LS state with a stable abundance ratio realized in the R3 ¯ c crystal structure with a single Fe site within a wide pressure range of ~ 50–106 GPa. Our results imply an unconventional cooperative (and probably dynamical) nature of the ordering of the HS/LS Fe sites randomly distributed over the lattice, resulting in frustration of magnetic moments. © 2022, The Author(s).en
dc.description.sponsorshipEAR-1634415; U.S. Department of Energy, USDOE: DE-FG02-94ER14466; Office of Science, SC: DE-AC02-06CH11357; Argonne National Laboratory, ANL; University of Chicago; Israel Science Foundation, ISF: 1189/14, 1552/18, 1748/20; Helmholtz Association; 122021000039-4en
dc.description.sponsorshipThe authors would like to thank Dr. A. Chumakov (ESRF, Grenoble, France, Kurchatov Institute, Moscow, Russia) and Dr. G. Smirnov (Kurchatov Institute, Moscow, Russia) who provided us by high-quality single crystals of FeBO, Prof. L. Dubrovinsky and Prof. D. I. Khomskii for valuable discussions, Dr. V. Prakapenka and Dr. I Kantor for experimental assistance with the facilities of the 13ID-D GSECARS beamline of APS and Dr. S. Clark for experimental assistance with the facilities of the beam line 12.2.2 at ALS, Berkeley. We are grateful also to the team of the ID-27 beamline of the European Synchrotron Radiation Facility, Grenoble, for assisting with the powder XRD measurements. A few Mössbauer spectrum at 115 and 140 GPa were collected at the ID-18 beamline of the European Synchrotron Radiation Facility. We are grateful to Dr. D. G. Merkel, Dr. R. Rüffer and Dr. A. Chumakov for their assistance in using beamline ID-18 and Dr. G. Hearne and Dr. E. Carleschi for assisting with the SMS measurements. This research was supported by Israeli Science Foundation (Grants No. 1189/14, No. 1552/18 and No. 1748/20). I.L. acknowledges support by the state assignment of Minobrnauki of Russia (theme “Electron” No. 122021000039-4). Portions of this work were performed at GeoSoilEnviroCARS (The University of Chicago, Sector 13), Advanced Photon Source (APS), Argonne National Laboratory. GeoSoilEnviroCARS is supported by the National Science Foundation–Earth Sciences (EAR-1634415) and Department of Energy– GeoSciences (DE-FG02-94ER14466). This research also used resources of the Advanced Photon Source, a U.S. Department of Energy (DOE) Office of Science User Facility operated for the DOE Office of Science by Argonne National Laboratory under Contract No. DE-AC02-06CH11357. We acknowledge DESY (Hamburg, Germany), a member of the Helmholtz Association HGF, for the provision of experimental facilities. Parts of this research were carried out at P02.2 station of PETRA-III, DESY. 3en
dc.description.sponsorshipThe authors would like to thank Dr. A. Chumakov (ESRF, Grenoble, France, Kurchatov Institute, Moscow, Russia) and Dr. G. Smirnov (Kurchatov Institute, Moscow, Russia) who provided us by high-quality single crystals of FeBO3 , Prof. L. Dubrovinsky and Prof. D. I. Khomskii for valuable discussions, Dr. V. Prakapenka and Dr. I Kantor for experimental assistance with the facilities of the 13ID-D GSECARS beamline of APS and Dr. S. Clark for experimental assistance with the facilities of the beam line 12.2.2 at ALS, Berkeley. We are grateful also to the team of the ID-27 beamline of the European Synchrotron Radiation Facility, Grenoble, for assisting with the powder XRD measurements. A few Mössbauer spectrum at 115 and 140 GPa were collected at the ID-18 beamline of the European Synchrotron Radiation Facility. We are grateful to Dr. D. G. Merkel, Dr. R. Rüffer and Dr. A. Chumakov for their assistance in using beamline ID-18 and Dr. G. Hearne and Dr. E. Carleschi for assisting with the SMS measurements. This research was supported by Israeli Science Foundation (Grants No. 1189/14, No. 1552/18 and No. 1748/20). I.L. acknowledges support by the state assignment of Minobrnauki of Russia (theme “Electron” No. 122021000039-4). Portions of this work were performed at GeoSoilEnviroCARS (The University of Chicago, Sector 13), Advanced Photon Source (APS), Argonne National Laboratory. GeoSoilEnviroCARS is supported by the National Science Foundation–Earth Sciences (EAR-1634415) and Department of Energy– GeoSciences (DE-FG02-94ER14466). This research also used resources of the Advanced Photon Source, a U.S. Department of Energy (DOE) Office of Science User Facility operated for the DOE Office of Science by Argonne National Laboratory under Contract No. DE-AC02-06CH11357. We acknowledge DESY (Hamburg, Germany), a member of the Helmholtz Association HGF, for the provision of experimental facilities. Parts of this research were carried out at P02.2 station of PETRA-III, DESY.en
dc.format.mimetypeapplication/pdfen
dc.language.isoenen
dc.publisherNature Researchen
dc.rightsinfo:eu-repo/semantics/openAccessen
dc.sourceScientific Reportsen
dc.titlePressure-induced high-spin/low-spin disproportionated state in the Mott insulator FeBO3en
dc.typeArticleen
dc.typeinfo:eu-repo/semantics/articleen
dc.typeinfo:eu-repo/semantics/publishedVersionen
dc.identifier.doi10.1038/s41598-022-13507-4-
dc.identifier.scopus85131788128-
local.contributor.employeeXu, W., School of Physics and Astronomy, Tel-Aviv University, Tel-Aviv, 69978, Israelen
local.contributor.employeeDong, W., Deutsches Elektronen Synchrotron (DESY), Notkestr. 85, Hamburg, 22607, Germanyen
local.contributor.employeeLayek, S., School of Physics and Astronomy, Tel-Aviv University, Tel-Aviv, 69978, Israel, Department of Physics, School of Engineering, University of Petroleum and Energy Studies (UPES), Uttarakhand, Dehradun, 248007, Indiaen
local.contributor.employeeShulman, M., School of Physics and Astronomy, Tel-Aviv University, Tel-Aviv, 69978, Israelen
local.contributor.employeeGlazyrin, K., Deutsches Elektronen Synchrotron (DESY), Notkestr. 85, Hamburg, 22607, Germanyen
local.contributor.employeeBykova, E., Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC 20015, United Statesen
local.contributor.employeeBykov, M., Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC 20015, United Statesen
local.contributor.employeeHanfland, M., European Synchrotron Radiation Facility, BP220, Grenoble, 38043, Franceen
local.contributor.employeePasternak, M.P., School of Physics and Astronomy, Tel-Aviv University, Tel-Aviv, 69978, Israelen
local.contributor.employeeLeonov, I., M.N. Miheev Institute of Metal Physics, Russian Academy of Sciences, Yekaterinburg, 620108, Russian Federation, Ural Federal University, Yekaterinburg, 620002, Russian Federationen
local.contributor.employeeGreenberg, E., School of Physics and Astronomy, Tel-Aviv University, Tel-Aviv, 69978, Israel, Applied Physics Division, Soreq NRC, Yavne, 81800, Israelen
local.contributor.employeeRozenberg, G.K., School of Physics and Astronomy, Tel-Aviv University, Tel-Aviv, 69978, Israelen
local.issue1-
local.volume12-
dc.identifier.wos000809441100067-
local.contributor.departmentSchool of Physics and Astronomy, Tel-Aviv University, Tel-Aviv, 69978, Israelen
local.contributor.departmentDeutsches Elektronen Synchrotron (DESY), Notkestr. 85, Hamburg, 22607, Germanyen
local.contributor.departmentDepartment of Physics, School of Engineering, University of Petroleum and Energy Studies (UPES), Uttarakhand, Dehradun, 248007, Indiaen
local.contributor.departmentEarth and Planets Laboratory, Carnegie Institution for Science, Washington, DC 20015, United Statesen
local.contributor.departmentEuropean Synchrotron Radiation Facility, BP220, Grenoble, 38043, Franceen
local.contributor.departmentM.N. Miheev Institute of Metal Physics, Russian Academy of Sciences, Yekaterinburg, 620108, Russian Federationen
local.contributor.departmentUral Federal University, Yekaterinburg, 620002, Russian Federationen
local.contributor.departmentApplied Physics Division, Soreq NRC, Yavne, 81800, Israelen
local.identifier.pure30525510-
local.description.order9647-
local.identifier.eid2-s2.0-85131788128-
local.identifier.wosWOS:000809441100067-
local.identifier.pmid35689001-
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