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dc.contributor.authorNikulin, A. Y.en
dc.contributor.authorZvereva, E. A.en
dc.contributor.authorNalbandyan, V. B.en
dc.contributor.authorShukaev, I. L.en
dc.contributor.authorKurbakov, A. I.en
dc.contributor.authorKuchugura, M. D.en
dc.contributor.authorRaganyan, G. V.en
dc.contributor.authorPopov, Y. V.en
dc.contributor.authorIvanchenko, V. D.en
dc.contributor.authorVasiliev, A. N.en
dc.date.accessioned2019-07-22T06:43:58Z-
dc.date.available2019-07-22T06:43:58Z-
dc.date.issued2017-
dc.identifier.citationPreparation and characterization of metastable trigonal layered MSb2O6 phases (M = Co, Ni, Cu, Zn, and Mg) and considerations on FeSb2O6 / A. Y. Nikulin, E. A. Zvereva, V. B. Nalbandyan et al. // Dalton Transactions. — 2017. — Vol. 46. — Iss. 18. — P. 6059-6068.en
dc.identifier.issn1477-9226-
dc.identifier.otherhttps://pubs.rsc.org/en/content/articlepdf/2017/dt/c6dt04859epdf
dc.identifier.other1good_DOI
dc.identifier.other437925d0-679a-4aaf-92c0-ad830b8b3157pure_uuid
dc.identifier.otherhttp://www.scopus.com/inward/record.url?partnerID=8YFLogxK&scp=85021774622m
dc.identifier.urihttp://elar.urfu.ru/handle/10995/75113-
dc.description.abstractMSb2O6 compounds (M = Mg, Co, Ni, Cu, Zn) are known in the tetragonal trirutile forms, slightly distorted monoclinically with M = Cu due to the Jahn-Teller effect. In this study, using a low-temperature exchange reaction between ilmenite-type NaSbO3 and molten MSO4-KCl (or MgCl2-KCl) mixtures, these five compositions were prepared for the first time as trigonal layered rosiaite (PbSb2O6)-type phases. Upon heating, they irreversibly transform to the known phases via amorphous intermediates, in contrast to previously studied isostructural MnSb2O6, where the stable phase is structurally related to the metastable phase. The same method was found to be applicable for preparing stable rosiaite-type CdSb2O6. The formula volumes of the new phases show an excellent correlation with the ionic radii (except for M = Cu, for which a Jahn-Teller distortion is suspected) and are 2-3% larger than those for the known forms although all coordination numbers are the same. The crystal structure of CoSb2O6 was refined via the Rietveld method: P31m, a = 5.1318(3) Å, and c = 4.5520(3) Å. Compounds with M = Co and Ni antiferromagnetically order at 11 and 15 K, respectively, whereas the copper compound does not show long-range magnetic order down to 1.5 K. A comparison between the magnetic behavior of the metastable and stable polymorphs was carried out. FeSb2O6 could not be prepared because of the 2Fe2+ + Sb5+ = 2Fe3+ + Sb3+ redox reaction. This electron transfer produces an additional 5s2 shell for Sb and results in a volume increase. A comparison of the formula volume for the stable mixture FeSbO4 + 0.5Sb2O4 with that extrapolated for FeSb2O6 predicted that the trirutile-type FeSb2O6 can be stabilized at high pressures. © 2017 The Royal Society of Chemistry.en
dc.description.sponsorshipThe work was supported by the Russian Foundation for Basic Research under the grant 14-03-01122. A. N. V. acknowledges the support in part from the Ministry of Education and Science of the Russian Federation in the framework of Increase Competitiveness Program of NUST <MISiS> (no. K2-2016-066) and by Act 211 of the Government of Russian Federation, contract no. 02.A03.21.0006.en
dc.format.mimetypeapplication/pdfen
dc.language.isoenen
dc.publisherRoyal Society of Chemistryen
dc.rightsinfo:eu-repo/semantics/openAccessen
dc.sourceDalton Transactionsen
dc.subjectCOBALT COMPOUNDSen
dc.subjectCRYSTAL STRUCTUREen
dc.subjectIRON COMPOUNDSen
dc.subjectJAHN-TELLER EFFECTen
dc.subjectMETASTABLE PHASESen
dc.subjectMIXTURESen
dc.subjectNICKELen
dc.subjectREDOX REACTIONSen
dc.subjectZINCen
dc.subjectCOORDINATION NUMBERen
dc.subjectELECTRON TRANSFERen
dc.subjectEXCHANGE REACTIONen
dc.subjectHIGH PRESSUREen
dc.subjectLONG RANGE MAGNETIC ORDERen
dc.subjectLOW TEMPERATURESen
dc.subjectMAGNETIC BEHAVIORen
dc.subjectMETASTABLE PHASEen
dc.subjectCOPPER COMPOUNDSen
dc.titlePreparation and characterization of metastable trigonal layered MSb2O6 phases (M = Co, Ni, Cu, Zn, and Mg) and considerations on FeSb2O6en
dc.typeArticleen
dc.typeinfo:eu-repo/semantics/articleen
dc.typeinfo:eu-repo/semantics/publishedVersionen
dc.identifier.doi10.1039/c6dt04859e-
dc.identifier.scopus85021774622-
local.affiliationChemistry Faculty, Southern Federal University, 7 ul. Zorge, Rostov-on-Don, 344090, Russian Federationen
local.affiliationFaculty of Physics, Moscow State University, Moscow, 119991, Russian Federationen
local.affiliationPetersburg Nuclear Physics Institute, NRC Kurchatov Institute, Gatchina, 188300, Russian Federationen
local.affiliationFaculty of Physics, St. Petersburg State University, St.-Petersburg, 198504, Russian Federationen
local.affiliationInstitute for Earth Sciences, Southern Federal University, 40 ul. Zorge, Rostov-on-Don, 344090, Russian Federationen
local.affiliationUral Federal University, Ekaterinburg, 620002, Russian Federationen
local.affiliationNational University of Science and Technology MISiS, Moscow, 119049, Russian Federationen
local.contributor.employeeВасильев Александр Николаевичru
local.description.firstpage6059-
local.description.lastpage6068-
local.issue18-
local.volume46-
dc.identifier.wos000400986500035-
local.identifier.pure1811118-
local.identifier.eid2-s2.0-85021774622-
local.identifier.wosWOS:000400986500035-
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