High-temperature induced ferromagnetism on gamma-Fe precipitates in FeCu solid solutions

dc.contributor.authorGorria, Pedro
dc.contributor.authorMartínez Blanco, David
dc.contributor.authorBlanco, Jesús A.
dc.contributor.authorPérez, María José
dc.contributor.authorHernando Grande, Antonio
dc.contributor.authorFernández Barquín, luis
dc.contributor.authorSmith, Ronald I.
dc.date.accessioned2023-06-20T12:39:32Z
dc.date.available2023-06-20T12:39:32Z
dc.date.issued2005-07
dc.description©2005 The American Physical Society. The work was partially supported by the Research Grants MAT2002-04178-C04, AT2002-11621-E, MAT2003- 06942, FICyT-PB02-037, and by EU under IHP program. We also thank the ISIS facility UK for the allocation of neutron beam time. D.M.-B. thanks the Spanish MICyT for additional support.
dc.description.abstractExperimental results of magnetization and neutron diffraction in the temperature range 300-1100 K evidence an anomalous high-temperature irreversible magnetic behavior on metastable FeCu solid solutions. When the temperature is increased above 500 K, a segregation process takes place in the as-milled sample which gives rise to the appearance of Fe (bcc) and Cu (fcc) phases. Further heating shows that the magnetization at 850 K falls down due to the temperature dependence of the bcc-Fe magnetization and the onset of the alpha-gamma martensite transformation. The temperature of this martensite phase transition (1020 K) is more 100 K lower than that of pure alpha-Fe (1183 K). On cooling from high temperatures (1100 K), the magnetization does not appreciably increase its value until the temperature is lowered below 900 K, showing a broad hysteresis between the forward (warming) and the reverse (cooling) transformations. Apart of the above mentioned bcc-Fe and fcc-Cu phases, on cooling, a small amount of isolated gamma-Fe precipitates (approximate to 5%) is detected. Further heating above 600 K show a large magnetization enhancement, reaching a value 50% higher with respect to the value measured at room temperature. During cooling from 1100 K the maximum value of magnetization is not recovered. The origin of this anomalous high temperature magnetic behavior is explained on the basis of strong magnetovolume instabilities in gamma-Fe. Furthermore, the thermal expansion coefficient of the gamma-Fe precipitates (21-23x10(-6) K-1), obtained from the neutron-diffraction patterns, is in excellent agreement with that calculated theoretically (20-24x10(-6) K-1, along the studied temperature range 300-1100 K). This fact is a signature of an anti-Invar behavior in gamma-Fe precipitates that could explain this surprising magnetic response.
dc.description.departmentDepto. de Física de Materiales
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipMEC, Spain
dc.description.sponsorshipFYCIT, Spain
dc.description.sponsorshipEU under IHP program
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/44169
dc.identifier.doi10.1103/PhysRevB.72.014401
dc.identifier.issn1098-0121
dc.identifier.officialurlhttp://dx.doi.org/10.1103/PhysRevB.72.014401
dc.identifier.relatedurlhttps://journals.aps.org
dc.identifier.urihttps://hdl.handle.net/20.500.14352/52096
dc.issue.number1
dc.journal.titlePhysical review B
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.projectIDMAT2002-04178-C04
dc.relation.projectIDAT2002-11621-E
dc.relation.projectIDMAT2003- 06942
dc.relation.projectIDFICyT-PB02-037
dc.rights.accessRightsopen access
dc.subject.cdu538.9
dc.subject.keywordMagnetic-Properties
dc.subject.keywordMossbauer-spectroscopy
dc.subject.keywordImmiscible elements
dc.subject.keywordCu alloys
dc.subject.keywordIron
dc.subject.keywordInvar
dc.subject.keywordDecomposition
dc.subject.keywordStability
dc.subject.keywordOrigin
dc.subject.keywordStates
dc.subject.ucmFísica de materiales
dc.subject.ucmFísica del estado sólido
dc.subject.unesco2211 Física del Estado Sólido
dc.titleHigh-temperature induced ferromagnetism on gamma-Fe precipitates in FeCu solid solutions
dc.typejournal article
dc.volume.number72
dspace.entity.typePublication
relation.isAuthorOfPublication930014e1-7363-41d3-b971-b824e05f84b2
relation.isAuthorOfPublication.latestForDiscovery930014e1-7363-41d3-b971-b824e05f84b2

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