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Authordc.contributor.authorRoldán Molina, A. 
Authordc.contributor.authorNúñez Vásquez, Álvaro 
Authordc.contributor.authorDuine, R. A. 
Admission datedc.date.accessioned2018-12-20T14:15:22Z
Available datedc.date.available2018-12-20T14:15:22Z
Publication datedc.date.issued2017
Cita de ítemdc.identifier.citationPhysical Review Letters, Volumen 118, Issue 6, 2018,
Identifierdc.identifier.issn10797114
Identifierdc.identifier.issn00319007
Identifierdc.identifier.other10.1103/PhysRevLett.118.061301
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/155282
Abstractdc.description.abstract© 2017 American Physical Society.We show that the interaction between the spin-polarized current and the magnetization dynamics can be used to implement black-hole and white-hole horizons for magnons - the quanta of oscillations in the magnetization direction in magnets. We consider three different systems: easy-plane ferromagnetic metals, isotropic antiferromagnetic metals, and easy-plane magnetic insulators. Based on available experimental data, we estimate that the Hawking temperature can be as large as 1 K. We comment on the implications of magnonic horizons for spin-wave scattering and transport experiments, and for magnon entanglement.
Lenguagedc.language.isoen
Publisherdc.publisherAmerican Physical Society
Type of licensedc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
Sourcedc.sourcePhysical Review Letters
Keywordsdc.subjectPhysics and Astronomy (all)
Títulodc.titleMagnonic Black Holes
Document typedc.typeArtículo de revista
dcterms.accessRightsdcterms.accessRightsAcceso Abierto
Catalogueruchile.catalogadorSCOPUS
Indexationuchile.indexArtículo de publicación SCOPUS
uchile.cosechauchile.cosechaSI


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Except where otherwise noted, this item's license is described as Attribution-NonCommercial-NoDerivs 3.0 Chile