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dc.contributor.author양인상-
dc.date.accessioned2016-08-28T12:08:20Z-
dc.date.available2016-08-28T12:08:20Z-
dc.date.issued2011-
dc.identifier.issn0377-0486-
dc.identifier.otherOAK-8045-
dc.identifier.urihttps://dspace.ewha.ac.kr/handle/2015.oak/222007-
dc.description.abstractWe have studied the rare-earth (R) dependence of the phonon and magnon scattering in hexagonal RMnO3 (R = Tb, Dy, Ho, Er) thin films using Raman scattering spectroscopy. We found, as the ionic radius of R decreases from Tb to Er, the phonons shift to higher energies. Our results indicate that both the lattice constants a and c of hexagonal RMnO3 would decrease when the ionic radius of R decreases, and the lattice constant c would have a weaker R dependence. The magnons also shift to higher energies when the radius of the R ion decreases, and they show faster upshift than the phonons. In addition, the Néel temperature also shows a systematic increasing behavior when the radius of the R ion decreases. The dependence of the rare-earth R on the magnons and the Néel temperature can be explained by the rapid increase of the spin-exchange integral when the Mn-Mn distance decreases. © 2011 John Wiley & Sons, Ltd.-
dc.languageEnglish-
dc.titleRaman scattering studies of hexagonal rare-earth RMnO3 (R = Tb, Dy, Ho, Er) thin films-
dc.typeArticle-
dc.relation.issue9-
dc.relation.volume42-
dc.relation.indexSCI-
dc.relation.indexSCIE-
dc.relation.indexSCOPUS-
dc.relation.startpage1774-
dc.relation.lastpage1779-
dc.relation.journaltitleJournal of Raman Spectroscopy-
dc.identifier.doi10.1002/jrs.2925-
dc.identifier.wosidWOS:000295806900010-
dc.identifier.scopusid2-s2.0-80052967686-
dc.author.googleHien N.T.M.-
dc.author.googleOh S.-Y.-
dc.author.googleChen X.-B.-
dc.author.googleLee D.-
dc.author.googleJang S.-Y.-
dc.author.googleNoh T.W.-
dc.author.googleYang I.-S.-
dc.contributor.scopusid양인상(7101797839)-
dc.date.modifydate20230210140835-
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