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dc.contributor.authorLago, J.
dc.contributor.authorZiivkovic, I.
dc.contributor.authorMalkin, B. Z.
dc.contributor.authorRodríguez Fernández, Jesús 
dc.contributor.authorGhigna, P.
dc.contributor.authorDalmas de Réotier, P.
dc.contributor.authorYaouanc, A.
dc.contributor.authorRojo, T.
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2023-04-21T12:21:14Z
dc.date.available2023-04-21T12:21:14Z
dc.date.issued2010-06
dc.identifier.issn0031-9007
dc.identifier.issn1079-7114
dc.identifier.otherMAT2007-66737-C02-01es_ES
dc.identifier.otherMAT2008-06542-C04es_ES
dc.identifier.urihttps://hdl.handle.net/10902/28560
dc.description.abstractHere we present a detailed study of the spinel CdEr2Se4 and show it to be a new instance of spin ice, the first one in an erbium material and the first one in a spinel. Definitive experimental evidence comes from the temperature dependence of the magnetic entropy, which shows an excellent agreement with the predicted behavior for a spin ice state. Crystal field calculations demonstrate that the change in the local environment from that of the titanates completely alters the rare-earth anisotropy giving rise, in the case of Er3+, to the required Ising anisotropy, when Er2Ti2O7 behaves as an XY antiferromagnet. This finding opens up the possibility of new exotic ground states within the CdR2Se4 and CdR2Se4 families.es_ES
dc.description.sponsorshipThe authors would like to acknowledge L. Jaubert for useful discussions as well as H. Luetkens and C. Baines for technical assistance during the SR measurements at PSI. Part of this work was financially supported by the Spanish Ministerio de Educación (projects MAT2007-66737-C02-01 and MAT2008-06542-C04).es_ES
dc.format.extent4 p.es_ES
dc.language.isoenges_ES
dc.publisherAmerican Physical Societyes_ES
dc.rights© 2010 The American Physical Societyes_ES
dc.sourcePhysical Review Letters, 2010, 104(24), 247203es_ES
dc.titleCdEr2Se4: a new erbium spin ice system in a spinel structurees_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.publisherVersionhttps://doi.org/10.1103/PhysRevLett.104.247203es_ES
dc.rights.accessRightsopenAccesses_ES
dc.identifier.DOI10.1103/PhysRevLett.104.247203
dc.type.versionpublishedVersiones_ES


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