Magnetic Gruneisen parameter for model systems
Autor(a) principal: | |
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Data de Publicação: | 2019 |
Outros Autores: | , , , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1103/PhysRevB.100.054446 http://hdl.handle.net/11449/186089 |
Resumo: | The magnetocaloric effect (MCE), which is the refrigeration based on the variation of the magnetic entropy, is of great interest in both technological applications and fundamental research. The MCE is quantified by the magnetic Gruneisen parameter Gamma(mag). We report on an analysis of Gamma(mag) for the classical Brillouin-like paramagnet for a modified Brillouin function taking into account a zero-field splitting originated from the spin-orbit (SO) interaction and for the one-dimensional Ising (1DI) model under a longitudinal field. For the Brillouin-like model with SO interaction and the longitudinal 1DI model, a sign-change in the MCE is observed for vanishing T and B. SO interaction leads to a narrowing of the enhancement of Gamma(mag) for T and B -> 0. Our findings emphasize the relevance of Gamma(mag) for exploring critical points. Also, we show that the Brillouin model with and without SO interaction can be recovered from the 1DI model in the regime of high temperatures and vanishing coupling constant J. |
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Repositório Institucional da UNESP |
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2946 |
spelling |
Magnetic Gruneisen parameter for model systemsThe magnetocaloric effect (MCE), which is the refrigeration based on the variation of the magnetic entropy, is of great interest in both technological applications and fundamental research. The MCE is quantified by the magnetic Gruneisen parameter Gamma(mag). We report on an analysis of Gamma(mag) for the classical Brillouin-like paramagnet for a modified Brillouin function taking into account a zero-field splitting originated from the spin-orbit (SO) interaction and for the one-dimensional Ising (1DI) model under a longitudinal field. For the Brillouin-like model with SO interaction and the longitudinal 1DI model, a sign-change in the MCE is observed for vanishing T and B. SO interaction leads to a narrowing of the enhancement of Gamma(mag) for T and B -> 0. Our findings emphasize the relevance of Gamma(mag) for exploring critical points. Also, we show that the Brillouin model with and without SO interaction can be recovered from the 1DI model in the regime of high temperatures and vanishing coupling constant J.Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)T.U.V.S.O.T.EAustrian Academy of Science OAWAustrian Science Fund (FWF)Sao Paulo State Univ, UNESP, Dept Fis, IGCE, BR-13506900 Rio Claro, SP, BrazilSao Paulo State Univ, UNESP, Fac Engn Ilha Solteira, BR-15385000 Ilha Solteira, SP, BrazilJohannes Kepler Univ Linz, Inst Semicond & Solid State Phys, A-4040 Linz, AustriaUniv Sao Paulo, Dept Astron, BR-05508090 Sao Paulo, BrazilSao Paulo State Univ, UNESP, Dept Fis, IGCE, BR-13506900 Rio Claro, SP, BrazilSao Paulo State Univ, UNESP, Fac Engn Ilha Solteira, BR-15385000 Ilha Solteira, SP, BrazilFAPESP: 2011/22050-4FAPESP: 2017/07845-7CNPq: 302498/20176CNPq: 305668/2018-8Austrian Science Fund (FWF): P26164-N20Amer Physical SocUniversidade Estadual Paulista (Unesp)Johannes Kepler Univ LinzUniversidade de São Paulo (USP)Gomes, Gabriel O. [UNESP]Squillante, Lucas [UNESP]Seridonio, A. C. [UNESP]Ney, AndreasLagos, Roberto E. [UNESP]Souza, Mariano de [UNESP]2019-10-04T12:41:11Z2019-10-04T12:41:11Z2019-08-28info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article10http://dx.doi.org/10.1103/PhysRevB.100.054446Physical Review B. College Pk: Amer Physical Soc, v. 100, n. 5, 10 p., 2019.2469-9950http://hdl.handle.net/11449/18608910.1103/PhysRevB.100.054446WOS:000482940800006Web of Sciencereponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review Binfo:eu-repo/semantics/openAccess2021-10-23T04:23:35Zoai:repositorio.unesp.br:11449/186089Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T21:03:30.579467Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Magnetic Gruneisen parameter for model systems |
title |
Magnetic Gruneisen parameter for model systems |
spellingShingle |
Magnetic Gruneisen parameter for model systems Gomes, Gabriel O. [UNESP] |
title_short |
Magnetic Gruneisen parameter for model systems |
title_full |
Magnetic Gruneisen parameter for model systems |
title_fullStr |
Magnetic Gruneisen parameter for model systems |
title_full_unstemmed |
Magnetic Gruneisen parameter for model systems |
title_sort |
Magnetic Gruneisen parameter for model systems |
author |
Gomes, Gabriel O. [UNESP] |
author_facet |
Gomes, Gabriel O. [UNESP] Squillante, Lucas [UNESP] Seridonio, A. C. [UNESP] Ney, Andreas Lagos, Roberto E. [UNESP] Souza, Mariano de [UNESP] |
author_role |
author |
author2 |
Squillante, Lucas [UNESP] Seridonio, A. C. [UNESP] Ney, Andreas Lagos, Roberto E. [UNESP] Souza, Mariano de [UNESP] |
author2_role |
author author author author author |
dc.contributor.none.fl_str_mv |
Universidade Estadual Paulista (Unesp) Johannes Kepler Univ Linz Universidade de São Paulo (USP) |
dc.contributor.author.fl_str_mv |
Gomes, Gabriel O. [UNESP] Squillante, Lucas [UNESP] Seridonio, A. C. [UNESP] Ney, Andreas Lagos, Roberto E. [UNESP] Souza, Mariano de [UNESP] |
description |
The magnetocaloric effect (MCE), which is the refrigeration based on the variation of the magnetic entropy, is of great interest in both technological applications and fundamental research. The MCE is quantified by the magnetic Gruneisen parameter Gamma(mag). We report on an analysis of Gamma(mag) for the classical Brillouin-like paramagnet for a modified Brillouin function taking into account a zero-field splitting originated from the spin-orbit (SO) interaction and for the one-dimensional Ising (1DI) model under a longitudinal field. For the Brillouin-like model with SO interaction and the longitudinal 1DI model, a sign-change in the MCE is observed for vanishing T and B. SO interaction leads to a narrowing of the enhancement of Gamma(mag) for T and B -> 0. Our findings emphasize the relevance of Gamma(mag) for exploring critical points. Also, we show that the Brillouin model with and without SO interaction can be recovered from the 1DI model in the regime of high temperatures and vanishing coupling constant J. |
publishDate |
2019 |
dc.date.none.fl_str_mv |
2019-10-04T12:41:11Z 2019-10-04T12:41:11Z 2019-08-28 |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://dx.doi.org/10.1103/PhysRevB.100.054446 Physical Review B. College Pk: Amer Physical Soc, v. 100, n. 5, 10 p., 2019. 2469-9950 http://hdl.handle.net/11449/186089 10.1103/PhysRevB.100.054446 WOS:000482940800006 |
url |
http://dx.doi.org/10.1103/PhysRevB.100.054446 http://hdl.handle.net/11449/186089 |
identifier_str_mv |
Physical Review B. College Pk: Amer Physical Soc, v. 100, n. 5, 10 p., 2019. 2469-9950 10.1103/PhysRevB.100.054446 WOS:000482940800006 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Physical Review B |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
10 |
dc.publisher.none.fl_str_mv |
Amer Physical Soc |
publisher.none.fl_str_mv |
Amer Physical Soc |
dc.source.none.fl_str_mv |
Web of Science reponame:Repositório Institucional da UNESP instname:Universidade Estadual Paulista (UNESP) instacron:UNESP |
instname_str |
Universidade Estadual Paulista (UNESP) |
instacron_str |
UNESP |
institution |
UNESP |
reponame_str |
Repositório Institucional da UNESP |
collection |
Repositório Institucional da UNESP |
repository.name.fl_str_mv |
Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP) |
repository.mail.fl_str_mv |
|
_version_ |
1808129279354994688 |