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dc.contributor.authorKáňa, Tomáš
dc.contributor.authorHüger, Erwin
dc.contributor.authorLegut, Dominik
dc.contributor.authorČák, Miroslav
dc.contributor.authorŠob, Mojmír
dc.date.accessioned2016-06-15T12:26:03Z
dc.date.available2016-06-15T12:26:03Z
dc.date.issued2016
dc.identifier.citationPhysical Review B. 2016, vol. 93, issue 13, art. no. 134422.cs
dc.identifier.issn2469-9950
dc.identifier.issn2469-9969
dc.identifier.urihttp://hdl.handle.net/10084/111662
dc.description.abstractBy means of ab initio calculations, we investigated structural and magnetic properties of Pd and Rh thin films, determining their lattice parameters and epitaxial stresses when they are grown on various substrates, and provided a comparison with available experimental data. Further, we studied in detail the magnetic properties of Pd in the higher-energy hcp structure and of Rh in the higher-energy bcc structure. The results predict that the hcp(112¯0) Pd films [grown by epitaxy on the Nb(001) substrate] should not be ferromagnetically ordered. Concerning the hcp Pd, we mainly investigated the influence of the hcp c/a ratio on the hcp film stability and on the ferromagnetic order. It turns out that the c/a ratio has to be below 1.622 to induce the ferromagnetic order in hcp Pd. We proposed a technological route for obtaining ferromagnetic hcp(112¯0) Pd films and explained the experimentally observed ferromagnetism in twinned Pd nanoparticles induced by strain. We also found that bcc Rh is ferromagnetically ordered, but it cannot be stabilized in the form of thin films. Therefore, we investigated the dependence of ferromagnetic order in bct Rh on the tetragonal c/a ratio and compared our results with experiments performed on Rh/Fe(001) multilayers.cs
dc.language.isoencs
dc.publisherAmerican Physical Societycs
dc.relation.ispartofseriesPhysical Review Bcs
dc.relation.urihttp://dx.doi.org/10.1103/PhysRevB.93.134422cs
dc.rights©2016 American Physical Societycs
dc.titleMagnetism and deformation of epitaxial Pd and Rh thin filmscs
dc.typearticlecs
dc.identifier.doi10.1103/PhysRevB.93.134422
dc.type.statusPeer-reviewedcs
dc.description.sourceWeb of Sciencecs
dc.description.issue13cs
dc.description.firstpageart. no. 134422cs
dc.identifier.wos000374528700003


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