Identificador persistente para citar o vincular este elemento: http://hdl.handle.net/10553/75659
Campo DC Valoridioma
dc.contributor.authorOrtega, Yanarisen_US
dc.contributor.authorFernández Hevia, Danielen_US
dc.contributor.authorOviedo, J.en_US
dc.contributor.authorSan-Miguel, M. A.en_US
dc.date.accessioned2020-11-18T08:49:08Z-
dc.date.available2020-11-18T08:49:08Z-
dc.date.issued2014en_US
dc.identifier.issn0169-4332en_US
dc.identifier.otherWoS-
dc.identifier.urihttp://hdl.handle.net/10553/75659-
dc.description.abstractHere we report a systematic study on the structural and energetic properties of the stoichiometric and reduced anatase (001) surfaces by using periodic density functional calculations. Structural and energetic properties for different surface models are investigated, as well as their stability as a function of the slab thickness. The calculations indicated that a 3 x 3 x 6 model is adequate to describe the pure and reduced anatase TiO2 (001) surfaces. Our calculations on the reduced system have demonstrated that the outermost oxygen vacancy, in the first atomic layer, is the most stable defect. A comparison between (001) and (101) surfaces reveals that defect creation is easier on the former. Thus, a higher vacancy concentration on that surface is expected. On the other hand, calculations at higher vacancy concentrations show repulsive interactions among defects what might inhibit further vacancy creation. The electronic structure has been examined by means of DFT+U methodology. The Hubbard U parameter influences considerably the location of defect states in the Ti 3d band and is essential to correctly describe the electronic structure. We conclude that the value U = 4.0 eV is a correct choice, which produces mid states in the band gap, a charge density localization and increases geometry deformation because of repulsive interactions, but effects on energetics are limited. (C) 2014 Elsevier B. V. All rights reserved.en_US
dc.languageengen_US
dc.relationINNPACTO (Ministerio de Ciencia e Innovación)en_US
dc.relationCASCADA (Ministerio de Ciencia e Innovación)en_US
dc.relation.ispartofApplied Surface Scienceen_US
dc.sourceApplied Surface Science [ISSN 0169-4332], v. 294, p. 42-48, (Marzo 2014)en_US
dc.subject221128 Superficiesen_US
dc.subject.otherGeneralized Gradient Approximationen_US
dc.subject.otherTotal-Energy Calculationsen_US
dc.subject.otherTitanium-Dioxideen_US
dc.subject.otherOxygen Vacanciesen_US
dc.subject.otherTio2 110en_US
dc.subject.otherAdsorptionen_US
dc.subject.otherTio2(110)en_US
dc.subject.otherOxideen_US
dc.subject.otherDiffractionen_US
dc.subject.otherPrinciplesen_US
dc.subject.otherAnataseen_US
dc.subject.otherDften_US
dc.subject.otherDft Plus Uen_US
dc.subject.otherReduced Surfacesen_US
dc.subject.otherOxygen Vacancy Formation Energiesen_US
dc.subject.otherElectronic Structureen_US
dc.titleA DFT study of the stoichiometric and reduced anatase (001) surfacesen_US
dc.typeinfo:eu-repo/semantics/Articleen_US
dc.typeArticleen_US
dc.identifier.doi10.1016/j.apsusc.2013.12.105en_US
dc.identifier.scopus84894073745-
dc.identifier.isi000331613700008-
dc.contributor.authorscopusid36773667500-
dc.contributor.authorscopusid36793606200-
dc.contributor.authorscopusid7004537269-
dc.contributor.authorscopusid7007180997-
dc.identifier.eissn1873-5584-
dc.description.lastpage48en_US
dc.description.firstpage42en_US
dc.relation.volume294en_US
dc.investigacionCienciasen_US
dc.type2Artículoen_US
dc.contributor.daisngid1386131-
dc.contributor.daisngid3261521-
dc.contributor.daisngid1246832-
dc.contributor.daisngid818123-
dc.description.numberofpages7en_US
dc.utils.revisionen_US
dc.contributor.wosstandardWOS:Ortega, Y-
dc.contributor.wosstandardWOS:Hevia, DF-
dc.contributor.wosstandardWOS:Oviedo, J-
dc.contributor.wosstandardWOS:San-Miguel, MA-
dc.date.coverdateMarzo 2014en_US
dc.identifier.ulpgcen_US
dc.contributor.buulpgcBU-BASen_US
dc.description.sjr0,958
dc.description.jcr2,711
dc.description.sjrqQ1
dc.description.jcrqQ1
dc.description.scieSCIE
item.grantfulltextnone-
item.fulltextSin texto completo-
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