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dc.contributor.author
dos Santos, G.
dc.contributor.author
Romá, Federico José
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Tranchida, J.
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Castedo, S.
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Cugliandolo, L. F.
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Bringa, Eduardo Marcial
dc.date.available
2024-02-19T15:12:53Z
dc.date.issued
2023-10
dc.identifier.citation
dos Santos, G.; Romá, Federico José; Tranchida, J.; Castedo, S.; Cugliandolo, L. F.; et al.; Feasibility analysis towards the simulation of hysteresis with spin-lattice dynamics; American Physical Society; Physical Review B; 108; 13; 10-2023; 134417-134430
dc.identifier.issn
2469-9950
dc.identifier.uri
http://hdl.handle.net/11336/227483
dc.description.abstract
We use spin-lattice dynamics simulations to study the possibility of modeling the magnetic hysteresis behavior of a ferromagnetic material. The temporal evolution of the magnetic and mechanical degrees of freedom is obtained through a set of two coupled Langevin equations. Hysteresis loops are calculated for different angles between the external field and the magnetocrystalline anisotropy axes. The influence of several relevant parameters is studied, including the field frequency, magnetic damping, magnetic anisotropy (magnitude and type), magnetic exchange, and system size. The role played by a moving lattice is also discussed. For a perfect bulk ferromagnetic system we find that, at low temperatures, the exchange and lattice dynamics barely affect the loops, while the field frequency and magnetic damping have a large effect on it. The influence of the anisotropy magnitude and symmetry are found to follow the expected behavior. We show that a careful choice of simulation parameters allows for an excellent agreement between the spin-lattice dynamics measurements and the paradigmatic Stoner-Wohlfarth model. Furthermore, we extend this analysis to intermediate and high temperatures for the perfect bulk system and for spherical nanoparticles, with and without defects, reaching values close to the Curie temperature. In this temperature range, we find that lattice dynamics has a greater role on the magnetic behavior, especially in the evolution of the defective samples. This study opens the possibility for more accurate inclusion of lattice defects and thermal effects in hysteresis simulations.
dc.format
application/pdf
dc.language.iso
eng
dc.publisher
American Physical Society
dc.rights
info:eu-repo/semantics/openAccess
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.subject
MAGNETISM
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SIMULATIONS
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SPIN-LATTICE-MODELS
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NANOPARTICLES
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Física de los Materiales Condensados
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Ciencias Físicas
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CIENCIAS NATURALES Y EXACTAS
dc.title
Feasibility analysis towards the simulation of hysteresis with spin-lattice dynamics
dc.type
info:eu-repo/semantics/article
dc.type
info:ar-repo/semantics/artículo
dc.type
info:eu-repo/semantics/publishedVersion
dc.date.updated
2024-02-19T10:27:29Z
dc.identifier.eissn
2469-9969
dc.journal.volume
108
dc.journal.number
13
dc.journal.pagination
134417-134430
dc.journal.pais
Estados Unidos
dc.description.fil
Fil: dos Santos, G.. Universidad de Mendoza; Argentina
dc.description.fil
Fil: Romá, Federico José. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Luis. Instituto de Física Aplicada "Dr. Jorge Andrés Zgrablich". Universidad Nacional de San Luis. Facultad de Ciencias Físico Matemáticas y Naturales. Instituto de Física Aplicada "Dr. Jorge Andrés Zgrablich"; Argentina. Universidad Nacional de San Luis. Facultad de Ciencias Físico Matemáticas y Naturales. Departamento de Física; Argentina
dc.description.fil
Fil: Tranchida, J.. No especifíca;
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Fil: Castedo, S.. No especifíca;
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Fil: Cugliandolo, L. F.. Université Pierre et Marie Curie. Laboratoire de Physique Théorique et Hautes Energies; Francia
dc.description.fil
Fil: Bringa, Eduardo Marcial. Universidad de Mendoza; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
dc.journal.title
Physical Review B
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://link.aps.org/doi/10.1103/PhysRevB.108.134417
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1103/PhysRevB.108.134417
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