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dc.creatorUnzueta, Iraultzaes_ES
dc.creatorSánchez-Alarcos Gómez, Vicentees_ES
dc.creatorRecarte Callado, Vicentees_ES
dc.creatorPérez de Landazábal Berganzo, José Ignacioes_ES
dc.creatorZabala, Nereaes_ES
dc.creatorGarcía, José Ángeles_ES
dc.creatorPlazaola, Fernandoes_ES
dc.date.accessioned2019-11-07T10:56:28Z
dc.date.available2019-11-07T10:56:28Z
dc.date.issued2019
dc.identifier.citationI. Unzueta, V. Sánchez-Alarcos, V. Recarte, J. I. Pérez-Landazábal, N. Zabala, J. A. García, and F. Plazaola: Identification of a Ni-vacancy defect in Ni-Mn-Z (Z=Ga, Sn, In): An experimental and DFT positron-annihilation study. Phys. Rev. B 99, 064108. https://doi.org/10.1103/PhysRevB.99.064108en
dc.identifier.issn2469-9969 (Electronic)
dc.identifier.urihttps://hdl.handle.net/2454/35317
dc.description.abstractBy means of experimental positron-annihilation-lifetime measurements and theoretical density functional theory (DFT) positron-lifetime calculations, vacancy-type defects in Ni50Mn50−xSnx (x = 25, 20, 15, 13, 10) and Ni50Mn50−xInx (x = 25, 20, 16, 13) systems are systematically studied. The study is extended to Ni-Mn-Ga systems as well. Experimental results are complemented with electron-positron DFT calculations carried out within the local density approximation and generalized gradient approximation, where five different parametrizations accounting for the γ (r) enhancement factor are analyzed. Theoretical results indicate that the Boronski-Nieminen parametrization of γ (r) is the one that best predicts the experimental results, which ultimately enables us to identify VNi as the vacancy present in the studied samples. The characteristic positron lifetime related to VNi ranges between 181 and 191 ps in Ni-Mn-Sn/In systems. Positron-annihilation-lifetime spectroscopy results in these two systems delimit the lower bound of the achievable vacancy concentration, which is much larger compared with the reported values in Ni-Mn-Ga systems. The present work, along with setting the basis for positron simulations in Ni-Mn based Heusler alloys, delimits the effect that the variation of vacancies has in the martensitic transformation in Ni-Mn-Sn systems.en
dc.description.sponsorshipThis work is supported by Eusko Jaurlaritza under Grants No. IT-1005-16 and No. IT-756-13 and by Spanish Ministry of Economy and Competitiveness under Grant No. MAT2015- 65165-C2-R (MINECO/FEDER). I. Unzueta also wants to acknowledge Eusko Jaurlaritza for Grant No. PRE-2014-214.en
dc.format.extent12 p.
dc.format.mimetypeapplication/pdfen
dc.language.isoengen
dc.publisherAmerican Physical Societyen
dc.relation.ispartofPhysical Review B 99, 064108 (2019)en
dc.rights© 2019 American Physical Societyen
dc.subjectDefectsen
dc.subjectFirst order phase transitionsen
dc.subjectVacanciesen
dc.subjectHeusler alloysen
dc.subjectDensity functional theoryen
dc.subjectElectron correlation calculationsen
dc.subjectPositron annihilation spectroscopyen
dc.titleIdentification of a Ni-vacancy defect in Ni-Mn-Z (Z = Ga, Sn, In): an experimental and DFT positron-annihilation studyen
dc.typeArtículo / Artikuluaes
dc.typeinfo:eu-repo/semantics/articleen
dc.contributor.departmentCienciases_ES
dc.contributor.departmentZientziakeu
dc.contributor.departmentInstitute for Advanced Materials and Mathematics - INAMAT2es_ES
dc.rights.accessRightsAcceso abierto / Sarbide irekiaes
dc.rights.accessRightsinfo:eu-repo/semantics/openAccessen
dc.identifier.doi10.1103/PhysRevB.99.064108
dc.relation.projectIDinfo:eu-repo/grantAgreement/MINECO//MAT2015-65165-C2-1-R/ES/en
dc.relation.publisherversionhttps://doi.org/10.1103/PhysRevB.99.064108
dc.type.versionVersión publicada / Argitaratu den bertsioaes
dc.type.versioninfo:eu-repo/semantics/publishedVersionen


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