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Название: Influence of Rare-earth Ion Radii on the Low-spin to Intermediate-spin State Transition in Lanthanide Cobaltite Perovskites: LaCoO3 Versus HoCoO3
Авторы: Nekrasov, I. A.
Streltsov, S. V.
Korotin, M. A.
Anisimov, V. I.
Дата публикации: 2003
Издатель: American Physical Society (APS)
Библиографическое описание: Influence of Rare-earth Ion Radii on the Low-spin to Intermediate-spin State Transition in Lanthanide Cobaltite Perovskites: LaCoO3 Versus HoCoO3 / I. A. Nekrasov, S. V. Streltsov, M. A. Korotin et al. // Physical Review B - Condensed Matter and Materials Physics. — 2003. — Vol. 68. — Iss. 23. — P. .
Аннотация: We present first-principles (local-density approximation) LDA+U calculations of electronic structure and magnetic state for LaCoO3 and HoCoO3. Low-spin to intermediate-spin state transition was found in our calculations using experimental crystallographic data for both materials with a much higher transition temperature for HoCoO3, which agrees well with the experimental estimations. Low-spin state (Formula presented) (nonmagnetic) to intermediate-spin state (Formula presented) (magnetic) transition of Co3+ ions happens due to the competition between crystal-field t2g − eg splitting and effective exchange interaction between 3d spin orbitals. We show that the difference in crystal structure parameters for HoCoO3 and LaCoO3 due to the smaller ionic radius of Ho ion comparing with La ion results in stronger crystal-field splitting for HoCoO3 (0.09 eV ≈ 1000 K larger than for LaCoO3) and hence tips the balance between the low-spin and intermediate-spin states to the nonmagnetic solution in HoCoO3. © 2003 The American Physical Society.
Ключевые слова: COBALT
HOLMIUM
LANTHANIDE
PEROVSKITE
ARTICLE
CALCULATION
CHEMICAL STRUCTURE
CRYSTAL STRUCTURE
MAGNETISM
MATHEMATICAL ANALYSIS
PHASE TRANSITION
RADIUS
TEMPERATURE DEPENDENCE
URI: http://elar.urfu.ru/handle/10995/111501
Условия доступа: info:eu-repo/semantics/openAccess
Идентификатор SCOPUS: 85039023548
Идентификатор PURE: 8160368
ISSN: 1098-0121
Сведения о поддержке: The work was supported by the INTAS Project No. 01-0278 and the Russian Foundation for Basic Research through Grants Nos. RFFI-01-02-17063 (I.V.A., I.A.N., M.A.K.) and RFFI-03-02-06026, the grant of Ural Branch of the Russian Academy of Sciences for Young Scientists, Grant of the President of Russia for Young Scientists, Grant No. MK-95.2003.02 (I.A.N.).
Располагается в коллекциях:Научные публикации ученых УрФУ, проиндексированные в SCOPUS и WoS CC

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