Thickness effect on the easy axis distribution in exchange biased Co/IrMn bilayers

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This work has been partially supported by the Brazilian agencies CNPq and FAPERJ. H. S. T. thanks to the Peruvian Doctoral Scholarship Program of CIENCIACTIVA (CONCYTEC) for financial support under Grand #218-2014-FONDECYT. J. Q-M and C. V. L. are grateful to CIENCIACTIVA (CONCYTEC) for partial fina...

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Detalles Bibliográficos
Autores: Tarazona H.S., Tafur M., Quispe-Marcatoma J., Landauro C.V., Baggio-Saitovitch E., Schmool D.S.
Formato: artículo
Fecha de Publicación:2019
Institución:Consejo Nacional de Ciencia Tecnología e Innovación
Repositorio:CONCYTEC-Institucional
Lenguaje:inglés
OAI Identifier:oai:repositorio.concytec.gob.pe:20.500.12390/806
Enlace del recurso:https://hdl.handle.net/20.500.12390/806
https://doi.org/10.1016/j.physb.2019.05.005
Nivel de acceso:acceso abierto
Materia:Rotatable anisotropy
Antiferromagnetism
Coercive force
Domain walls
Film growth
Free energy
Frequency modulation
Antiferromagnetic grains
Domain wall formation
Easy axis
Exchange bias
Magnetic field direction
Phenomenological modeling
Power law relationship
Magnetic anisotropy
https://purl.org/pe-repo/ocde/ford#1.03.00
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network_acronym_str CONC
network_name_str CONCYTEC-Institucional
repository_id_str 4689
dc.title.none.fl_str_mv Thickness effect on the easy axis distribution in exchange biased Co/IrMn bilayers
title Thickness effect on the easy axis distribution in exchange biased Co/IrMn bilayers
spellingShingle Thickness effect on the easy axis distribution in exchange biased Co/IrMn bilayers
Tarazona H.S.
Rotatable anisotropy
Antiferromagnetism
Coercive force
Coercive force
Domain walls
Film growth
Free energy
Frequency modulation
Antiferromagnetic grains
Antiferromagnetic grains
Domain wall formation
Easy axis
Exchange bias
Magnetic field direction
Magnetic field direction
Phenomenological modeling
Power law relationship
Magnetic anisotropy
https://purl.org/pe-repo/ocde/ford#1.03.00
title_short Thickness effect on the easy axis distribution in exchange biased Co/IrMn bilayers
title_full Thickness effect on the easy axis distribution in exchange biased Co/IrMn bilayers
title_fullStr Thickness effect on the easy axis distribution in exchange biased Co/IrMn bilayers
title_full_unstemmed Thickness effect on the easy axis distribution in exchange biased Co/IrMn bilayers
title_sort Thickness effect on the easy axis distribution in exchange biased Co/IrMn bilayers
author Tarazona H.S.
author_facet Tarazona H.S.
Tafur M.
Quispe-Marcatoma J.
Landauro C.V.
Baggio-Saitovitch E.
Schmool D.S.
author_role author
author2 Tafur M.
Quispe-Marcatoma J.
Landauro C.V.
Baggio-Saitovitch E.
Schmool D.S.
author2_role author
author
author
author
author
dc.contributor.author.fl_str_mv Tarazona H.S.
Tafur M.
Quispe-Marcatoma J.
Landauro C.V.
Baggio-Saitovitch E.
Schmool D.S.
dc.subject.none.fl_str_mv Rotatable anisotropy
topic Rotatable anisotropy
Antiferromagnetism
Coercive force
Coercive force
Domain walls
Film growth
Free energy
Frequency modulation
Antiferromagnetic grains
Antiferromagnetic grains
Domain wall formation
Easy axis
Exchange bias
Magnetic field direction
Magnetic field direction
Phenomenological modeling
Power law relationship
Magnetic anisotropy
https://purl.org/pe-repo/ocde/ford#1.03.00
dc.subject.es_PE.fl_str_mv Antiferromagnetism
Coercive force
Coercive force
Domain walls
Film growth
Free energy
Frequency modulation
Antiferromagnetic grains
Antiferromagnetic grains
Domain wall formation
Easy axis
Exchange bias
Magnetic field direction
Magnetic field direction
Phenomenological modeling
Power law relationship
Magnetic anisotropy
dc.subject.ocde.none.fl_str_mv https://purl.org/pe-repo/ocde/ford#1.03.00
description This work has been partially supported by the Brazilian agencies CNPq and FAPERJ. H. S. T. thanks to the Peruvian Doctoral Scholarship Program of CIENCIACTIVA (CONCYTEC) for financial support under Grand #218-2014-FONDECYT. J. Q-M and C. V. L. are grateful to CIENCIACTIVA (CONCYTEC) for partial financial support through the Excellence Center Programs. J. Q-M is also grateful to the GEMaC Laboratory, for the hospitality during the preparation of this manuscript. In addition, E. B. S. acknowledges support from FAPERJ through several grants including Emeritus Professor fellow and CNPq for BPA and corresponding grants.
publishDate 2019
dc.date.accessioned.none.fl_str_mv 2024-05-30T23:13:38Z
dc.date.available.none.fl_str_mv 2024-05-30T23:13:38Z
dc.date.issued.fl_str_mv 2019
dc.type.none.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.uri.none.fl_str_mv https://hdl.handle.net/20.500.12390/806
dc.identifier.doi.none.fl_str_mv https://doi.org/10.1016/j.physb.2019.05.005
dc.identifier.scopus.none.fl_str_mv 2-s2.0-85065698888
url https://hdl.handle.net/20.500.12390/806
https://doi.org/10.1016/j.physb.2019.05.005
identifier_str_mv 2-s2.0-85065698888
dc.language.iso.none.fl_str_mv eng
language eng
dc.relation.ispartof.none.fl_str_mv Physica B: Condensed Matter
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.publisher.none.fl_str_mv Elsevier B.V.
publisher.none.fl_str_mv Elsevier B.V.
dc.source.none.fl_str_mv reponame:CONCYTEC-Institucional
instname:Consejo Nacional de Ciencia Tecnología e Innovación
instacron:CONCYTEC
instname_str Consejo Nacional de Ciencia Tecnología e Innovación
instacron_str CONCYTEC
institution CONCYTEC
reponame_str CONCYTEC-Institucional
collection CONCYTEC-Institucional
repository.name.fl_str_mv Repositorio Institucional CONCYTEC
repository.mail.fl_str_mv repositorio@concytec.gob.pe
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spelling Publicationrp00839500rp02068600rp01110500rp00840500rp01241400rp02069600Tarazona H.S.Tafur M.Quispe-Marcatoma J.Landauro C.V.Baggio-Saitovitch E.Schmool D.S.2024-05-30T23:13:38Z2024-05-30T23:13:38Z2019https://hdl.handle.net/20.500.12390/806https://doi.org/10.1016/j.physb.2019.05.0052-s2.0-85065698888This work has been partially supported by the Brazilian agencies CNPq and FAPERJ. H. S. T. thanks to the Peruvian Doctoral Scholarship Program of CIENCIACTIVA (CONCYTEC) for financial support under Grand #218-2014-FONDECYT. J. Q-M and C. V. L. are grateful to CIENCIACTIVA (CONCYTEC) for partial financial support through the Excellence Center Programs. J. Q-M is also grateful to the GEMaC Laboratory, for the hospitality during the preparation of this manuscript. In addition, E. B. S. acknowledges support from FAPERJ through several grants including Emeritus Professor fellow and CNPq for BPA and corresponding grants.It is commonly assumed that in uncompensated FM/AF interfaces, the easy axes of antiferromagnetic grains are aligned toward the magnetic field direction applied during the film growth. However, due to several intrinsic and extrinsic factors, these easy axes can be aligned away from the unidirectional axis. In this context, the aim of this work is to study the relationship between the easy axes distribution (EAD) and thickness of both the ferromagnetic (FM) and antiferromagnetic (AF) layers in Co/IrMn bilayer systems. A phenomenological model for the free energy of the system that takes into account a domain wall formation in the AF layer and a Gaussian-type distribution of their easy axes is used. Thus, we simulate and fit the magnetization curves and get several magnetic parameters like rotatable anisotropy field, exchange bias field, coercivity and magnetic anisotropy. Our results show that when the AF thickness is increased, the width of the easy-axis distribution also increases following a power-law relationship. However, no correlation is observed when the FM thickness is varied. Furthermore, considering an easy-axis distribution we observe a significant reduction in coercivity as well as a slight decrease of the exchange bias field.Consejo Nacional de Ciencia, Tecnología e Innovación Tecnológica - ConcytecengElsevier B.V.Physica B: Condensed Matterinfo:eu-repo/semantics/openAccessRotatable anisotropyAntiferromagnetism-1Coercive force-1Coercive force-1Domain walls-1Film growth-1Free energy-1Frequency modulation-1Antiferromagnetic grains-1Antiferromagnetic grains-1Domain wall formation-1Easy axis-1Exchange bias-1Magnetic field direction-1Magnetic field direction-1Phenomenological modeling-1Power law relationship-1Magnetic anisotropy-1https://purl.org/pe-repo/ocde/ford#1.03.00-1Thickness effect on the easy axis distribution in exchange biased Co/IrMn bilayersinfo:eu-repo/semantics/articlereponame:CONCYTEC-Institucionalinstname:Consejo Nacional de Ciencia Tecnología e Innovacióninstacron:CONCYTEC#PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE#20.500.12390/806oai:repositorio.concytec.gob.pe:20.500.12390/8062024-05-30 15:22:59.756http://purl.org/coar/access_right/c_14cbinfo:eu-repo/semantics/closedAccessmetadata only accesshttps://repositorio.concytec.gob.peRepositorio Institucional CONCYTECrepositorio@concytec.gob.pe#PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE#<Publication xmlns="https://www.openaire.eu/cerif-profile/1.1/" id="5d78e5e2-dd33-4155-a6f7-3bd01670f96f"> <Type xmlns="https://www.openaire.eu/cerif-profile/vocab/COAR_Publication_Types">http://purl.org/coar/resource_type/c_1843</Type> <Language>eng</Language> <Title>Thickness effect on the easy axis distribution in exchange biased Co/IrMn bilayers</Title> <PublishedIn> <Publication> <Title>Physica B: Condensed Matter</Title> </Publication> </PublishedIn> <PublicationDate>2019</PublicationDate> <DOI>https://doi.org/10.1016/j.physb.2019.05.005</DOI> <SCP-Number>2-s2.0-85065698888</SCP-Number> <Authors> <Author> <DisplayName>Tarazona H.S.</DisplayName> <Person id="rp00839" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Tafur M.</DisplayName> <Person id="rp02068" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Quispe-Marcatoma J.</DisplayName> <Person id="rp01110" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Landauro C.V.</DisplayName> <Person id="rp00840" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Baggio-Saitovitch E.</DisplayName> <Person id="rp01241" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Schmool D.S.</DisplayName> <Person id="rp02069" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> </Authors> <Editors> </Editors> <Publishers> <Publisher> <DisplayName>Elsevier B.V.</DisplayName> <OrgUnit /> </Publisher> </Publishers> <Keyword>Rotatable anisotropy</Keyword> <Keyword>Antiferromagnetism</Keyword> <Keyword>Coercive force</Keyword> <Keyword>Coercive force</Keyword> <Keyword>Domain walls</Keyword> <Keyword>Film growth</Keyword> <Keyword>Free energy</Keyword> <Keyword>Frequency modulation</Keyword> <Keyword>Antiferromagnetic grains</Keyword> <Keyword>Antiferromagnetic grains</Keyword> <Keyword>Domain wall formation</Keyword> <Keyword>Easy axis</Keyword> <Keyword>Exchange bias</Keyword> <Keyword>Magnetic field direction</Keyword> <Keyword>Magnetic field direction</Keyword> <Keyword>Phenomenological modeling</Keyword> <Keyword>Power law relationship</Keyword> <Keyword>Magnetic anisotropy</Keyword> <Abstract>It is commonly assumed that in uncompensated FM/AF interfaces, the easy axes of antiferromagnetic grains are aligned toward the magnetic field direction applied during the film growth. However, due to several intrinsic and extrinsic factors, these easy axes can be aligned away from the unidirectional axis. In this context, the aim of this work is to study the relationship between the easy axes distribution (EAD) and thickness of both the ferromagnetic (FM) and antiferromagnetic (AF) layers in Co/IrMn bilayer systems. A phenomenological model for the free energy of the system that takes into account a domain wall formation in the AF layer and a Gaussian-type distribution of their easy axes is used. Thus, we simulate and fit the magnetization curves and get several magnetic parameters like rotatable anisotropy field, exchange bias field, coercivity and magnetic anisotropy. Our results show that when the AF thickness is increased, the width of the easy-axis distribution also increases following a power-law relationship. However, no correlation is observed when the FM thickness is varied. Furthermore, considering an easy-axis distribution we observe a significant reduction in coercivity as well as a slight decrease of the exchange bias field.</Abstract> <Access xmlns="http://purl.org/coar/access_right" > </Access> </Publication> -1
score 13.448654
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