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dc.contributor.authorKvashnin, Y. O.en
dc.contributor.authorCardias, R.en
dc.contributor.authorSzilva, A.en
dc.contributor.authorDi, Marco, I.en
dc.contributor.authorKatsnelson, M. I.en
dc.contributor.authorLichtenstein, A. I.en
dc.contributor.authorNordström, L.en
dc.contributor.authorKlautau, A. B.en
dc.contributor.authorEriksson, O.en
dc.date.accessioned2021-08-31T15:02:47Z-
dc.date.available2021-08-31T15:02:47Z-
dc.date.issued2016-
dc.identifier.citationMicroscopic Origin of Heisenberg and Non-Heisenberg Exchange Interactions in Ferromagnetic bcc Fe / Y. O. Kvashnin, R. Cardias, A. Szilva, et al. — DOI 10.1103/PhysRevLett.116.217202 // Physical Review Letters. — 2016. — Vol. 116. — Iss. 21. — 217202.en
dc.identifier.issn319007-
dc.identifier.otherFinal2
dc.identifier.otherAll Open Access, Green3
dc.identifier.otherhttps://www.scopus.com/inward/record.uri?eid=2-s2.0-84971254480&doi=10.1103%2fPhysRevLett.116.217202&partnerID=40&md5=df0385825bb34d723ec70668f7331b87
dc.identifier.otherhttp://arxiv.org/pdf/1510.01872m
dc.identifier.urihttp://elar.urfu.ru/handle/10995/102252-
dc.description.abstractBy means of first principles calculations, we investigate the nature of exchange coupling in ferromagnetic bcc Fe on a microscopic level. Analyzing the basic electronic structure reveals a drastic difference between the 3d orbitals of Eg and T2g symmetries. The latter ones define the shape of the Fermi surface, while the former ones form weakly interacting impurity levels. We demonstrate that, as a result of this, in Fe the T2g orbitals participate in exchange interactions, which are only weakly dependent on the configuration of the spin moments and thus can be classified as Heisenberg-like. These couplings are shown to be driven by Fermi surface nesting. In contrast, for the Eg states, the Heisenberg picture breaks down since the corresponding contribution to the exchange interactions is shown to strongly depend on the reference state they are extracted from. Our analysis of the nearest-neighbor coupling indicates that the interactions among Eg states are mainly proportional to the corresponding hopping integral and thus can be attributed to be of double-exchange origin. By making a comparison to other magnetic transition metals, we put the results of bcc Fe into context and argue that iron has a unique behavior when it comes to magnetic exchange interactions. © 2016 American Physical Society.en
dc.format.mimetypeapplication/pdfen
dc.language.isoenen
dc.publisherAmerican Physical Societyen
dc.rightsinfo:eu-repo/semantics/openAccessen
dc.sourcePhys Rev Lett2
dc.sourcePhysical Review Lettersen
dc.subjectCALCULATIONSen
dc.subjectELECTRONIC STRUCTUREen
dc.subjectFERMI SURFACEen
dc.subjectFERROMAGNETIC MATERIALSen
dc.subjectFERROMAGNETISMen
dc.subjectTRANSITION METALSen
dc.subjectFERMI SURFACE NESTINGen
dc.subjectFIRST-PRINCIPLES CALCULATIONen
dc.subjectHEISENBERG PICTURESen
dc.subjectMAGNETIC EXCHANGE INTERACTIONSen
dc.subjectMAGNETIC TRANSITIONSen
dc.subjectMICROSCOPIC LEVELSen
dc.subjectNEAREST-NEIGHBOR COUPLINGen
dc.subjectNON-HEISENBERG EXCHANGE INTERACTIONSen
dc.subjectEXCHANGE INTERACTIONSen
dc.titleMicroscopic Origin of Heisenberg and Non-Heisenberg Exchange Interactions in Ferromagnetic bcc Feen
dc.typeArticleen
dc.typeinfo:eu-repo/semantics/articleen
dc.typeinfo:eu-repo/semantics/publishedVersionen
dc.identifier.doi10.1103/PhysRevLett.116.217202-
dc.identifier.scopus84971254480-
local.contributor.employeeKvashnin, Y.O., Department of Physics and Astronomy, Division of Materials Theory, Uppsala University, Box 516, Uppsala, SE-75120, Sweden
local.contributor.employeeCardias, R., Faculdade de Fisica, Universidade Federal Do Para, Belem, Pará, 66075-110, Brazil
local.contributor.employeeSzilva, A., Department of Physics and Astronomy, Division of Materials Theory, Uppsala University, Box 516, Uppsala, SE-75120, Sweden
local.contributor.employeeDi Marco, I., Department of Physics and Astronomy, Division of Materials Theory, Uppsala University, Box 516, Uppsala, SE-75120, Sweden
local.contributor.employeeKatsnelson, M.I., Radboud University of Nijmegen, Institute for Molecules and Materials, Heijendaalseweg 135, Nijmegen, 6525 AJ, Netherlands, Theoretical Physics and Applied Mathematics Department, Ural Federal University, Mira Street 19, Ekaterinburg, 620002, Russian Federation
local.contributor.employeeLichtenstein, A.I., Theoretical Physics and Applied Mathematics Department, Ural Federal University, Mira Street 19, Ekaterinburg, 620002, Russian Federation, Institute of Theoretical Physics, University of Hamburg, Jungiusstrasse 9, Hamburg, 20355, Germany
local.contributor.employeeNordström, L., Department of Physics and Astronomy, Division of Materials Theory, Uppsala University, Box 516, Uppsala, SE-75120, Sweden
local.contributor.employeeKlautau, A.B., Faculdade de Fisica, Universidade Federal Do Para, Belem, Pará, 66075-110, Brazil
local.contributor.employeeEriksson, O., Department of Physics and Astronomy, Division of Materials Theory, Uppsala University, Box 516, Uppsala, SE-75120, Sweden
local.issue21-
local.volume116-
local.contributor.departmentDepartment of Physics and Astronomy, Division of Materials Theory, Uppsala University, Box 516, Uppsala, SE-75120, Sweden
local.contributor.departmentFaculdade de Fisica, Universidade Federal Do Para, Belem, Pará, 66075-110, Brazil
local.contributor.departmentRadboud University of Nijmegen, Institute for Molecules and Materials, Heijendaalseweg 135, Nijmegen, 6525 AJ, Netherlands
local.contributor.departmentTheoretical Physics and Applied Mathematics Department, Ural Federal University, Mira Street 19, Ekaterinburg, 620002, Russian Federation
local.contributor.departmentInstitute of Theoretical Physics, University of Hamburg, Jungiusstrasse 9, Hamburg, 20355, Germany
local.identifier.pure866151-
local.identifier.pure6fb89ac2-1a53-4c7b-bf8f-e664e28b45dduuid
local.description.order217202-
local.identifier.eid2-s2.0-84971254480-
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