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dc.contributor.authorGómez Ortiz, Fernando 
dc.contributor.authorCarral Sainz, Nayara 
dc.contributor.authorSifuna, James
dc.contributor.authorMonteseguro Padrón, Virginia 
dc.contributor.authorCuadrado, Ramón
dc.contributor.authorGarcía Fernández, Pablo (físico) 
dc.contributor.authorJunquera Quintana, Francisco Javier 
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2024-03-01T18:39:35Z
dc.date.available2024-03-01T18:39:35Z
dc.date.issued2023-05
dc.identifier.issn0010-4655
dc.identifier.otherPGC2018-096955-B-C41es_ES
dc.identifier.otherPID2021-125927NA-C22es_ES
dc.identifier.urihttps://hdl.handle.net/10902/32039
dc.description.abstractWe report the extension of the density-functional theory plus Hubbard U (DFT+U) method to the case of non-collinear magnetism and spin-orbit coupling in a framework of numerical atomic orbitals. Both the Hubbard repulsion term U, and the exchange J parameters are explicitly included and treated separately. The occupation numbers of the localized orbitals belonging to the correlated shell are computed from the projections of the Kohn-Sham eigenfunctions onto a set of non-overlapping, orthogonal, localized projectors. We provide the detailed expressions for the total energy, forces and stresses including the Pulay corrections. Our implementation on the version 5.0 of the SIESTA package has been validated with simulations carried out in isolated atoms and bulk solids including atoms with a strong spin-orbit couplinges_ES
dc.description.sponsorshipF.G.-O., N.C.-S., P.G.-F., and J.J. acknowledge financial support from Grant No. PGC2018-096955-B-C41 funded by MCIN/AEI/10.13039/501100011033 and by ERDF “A way of making Europe” by the European Union. F.G.-O. acknowledges financial support from Grant No. FPU18/04661 funded by MCIN/AEI/10.13039/501100011033. V. M. acknowledges financial support from Grant No. PID2021-125927NA-C22 funded by MCIN/AEI/10.13039/501100011033 and by ERDF “A way of making Europe” by the European Union, and the Beatriz Galindo Fellowship Grant No. BG20/000777. N.C.-S. acknowledges financial support from “Concepción Arenal” Grant No. BDNS:524538 of the University of Cantabria funded by the Government of Cantabria.es_ES
dc.format.extent10 p.es_ES
dc.language.isoenges_ES
dc.publisherElsevieres_ES
dc.rights©2023 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY-NC-ND license (http://creativecommons.org/licenses/by-nc-nd/4.0/).es_ES
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/*
dc.sourceComputer Physics Communications, 2023, 286, 108684es_ES
dc.subject.otherDFT+Ues_ES
dc.subject.otherSpin-orbites_ES
dc.subject.otherNon-collinear magnetismes_ES
dc.subject.otherNumerical atomic orbitalses_ES
dc.subject.otherSIESTAes_ES
dc.titleCompatibility of DFT+U with non-collinear magnetism and spin-orbit coupling within a framework of numerical atomic orbitalses_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.publisherVersionhttps://doi.org/10.1016/j.cpc.2023.108684es_ES
dc.rights.accessRightsopenAccesses_ES
dc.identifier.DOI10.1016/j.cpc.2023.108684
dc.type.versionpublishedVersiones_ES


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©2023 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY-NC-ND license (http://creativecommons.org/licenses/by-nc-nd/4.0/).Excepto si se señala otra cosa, la licencia del ítem se describe como ©2023 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY-NC-ND license (http://creativecommons.org/licenses/by-nc-nd/4.0/).