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Hysteresis shift in Fe-filled carbon nanotubes due to γ-Fe

dc.contributor.authorPrados, C.
dc.contributor.authorCrespo del Arco, Patricia
dc.contributor.authorGonzález, J. M.
dc.contributor.authorHernando Grande, Antonio
dc.contributor.authorMarcos, J. F.
dc.contributor.authorGancedo, R.
dc.contributor.authorGrobert, N.
dc.contributor.authorTerrones, M.
dc.contributor.authorWalton, R. M.
dc.contributor.authorKroto, H. W.
dc.date.accessioned2023-06-20T20:20:28Z
dc.date.available2023-06-20T20:20:28Z
dc.date.issued2002-03-15
dc.description©2002 The American Physical Society
dc.description.abstractThe phase distribution of high aspect ratio, Fe-filled carbon nanotubes prepared by pyrolyzing a mixture of powered ferrocene and C_(60) has been determined by means of Mössbauer spectroscopy. Our results for that characterization are closely related to the observation, after field cooling processes, of a hysteresis loop shift and clearly suggest a spatial phase distribution which includes the presence of a g-Fe/α-Fe interface. The temperature ependence of the hysteresis loop shift is discussed in terms of localized regions at that interface exhibiting uncompensated antiferromagnetism within reduced dimensions.
dc.description.departmentDepto. de Física de Materiales
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/42230
dc.identifier.doi10.1103/PhysRevB.65.113405
dc.identifier.issn1098-0121
dc.identifier.officialurlhttp://dx.doi.org/10.1103/PhysRevB.65.113405
dc.identifier.relatedurlhttps://journals.aps.org
dc.identifier.urihttps://hdl.handle.net/20.500.14352/60113
dc.issue.number11
dc.journal.titlePhysical review B
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.rights.accessRightsopen access
dc.subject.cdu538.9
dc.subject.keywordPhysics
dc.subject.keywordCondensed matter
dc.subject.ucmFísica de materiales
dc.subject.ucmFísica del estado sólido
dc.subject.unesco2211 Física del Estado Sólido
dc.titleHysteresis shift in Fe-filled carbon nanotubes due to γ-Fe
dc.typejournal article
dc.volume.number65
dspace.entity.typePublication
relation.isAuthorOfPublication930014e1-7363-41d3-b971-b824e05f84b2
relation.isAuthorOfPublication.latestForDiscovery930014e1-7363-41d3-b971-b824e05f84b2

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