Computer simulation of the stochastic dynamics of super-paramagnetic particles in ferrofluids
Autor(a) principal: | |
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Data de Publicação: | 2006 |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UFRGS |
Texto Completo: | http://hdl.handle.net/10183/75786 |
Resumo: | Several papers have been written on the complex problem of the stochastic dynamics of the magnetic moments of super-paramagnetic particles, simultaneously with the stochastic rotation of these colloidal particles in a ferrofluid [1–3]. None of these works, however, is sufficiently general and conveniently simple and clear to be used in sumulational works to appropriately describe the experimental super-paramagntetic resonance lines. We have a new proposal for the equations of rotational motion, which is appropriate for simulations. Those equations are stochastic differential equations with multiplicative noise. Therefore, they have to be interpreted as Stratonovich-Langevin equations and the roles of stochastic calculus have to be used in the simulations. For this reason we will briefly present the essence of the numerical algorithms used in the solutions of Stratonovich equations. Finally, the simulational results for the magnetic response functions, and the corresponding dynamic susceptibilities, will be shown and their consequences will be analyzed. |
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Scherer, Claudio2013-07-11T02:22:05Z20060103-9733http://hdl.handle.net/10183/75786000554069Several papers have been written on the complex problem of the stochastic dynamics of the magnetic moments of super-paramagnetic particles, simultaneously with the stochastic rotation of these colloidal particles in a ferrofluid [1–3]. None of these works, however, is sufficiently general and conveniently simple and clear to be used in sumulational works to appropriately describe the experimental super-paramagntetic resonance lines. We have a new proposal for the equations of rotational motion, which is appropriate for simulations. Those equations are stochastic differential equations with multiplicative noise. Therefore, they have to be interpreted as Stratonovich-Langevin equations and the roles of stochastic calculus have to be used in the simulations. For this reason we will briefly present the essence of the numerical algorithms used in the solutions of Stratonovich equations. Finally, the simulational results for the magnetic response functions, and the corresponding dynamic susceptibilities, will be shown and their consequences will be analyzed.application/pdfengBrazilian journal of physics. Vol. 36, n. 3A (Sept. 2006), p. 676-681FísicaFerrofluidMagnetic fluidComputer simulationStochastic dynamicSuper-paramagneticComputer simulation of the stochastic dynamics of super-paramagnetic particles in ferrofluidsinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/otherinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/openAccessreponame:Repositório Institucional da UFRGSinstname:Universidade Federal do Rio Grande do Sul (UFRGS)instacron:UFRGSORIGINAL000554069.pdf000554069.pdfTexto completo (inglês)application/pdf193876http://www.lume.ufrgs.br/bitstream/10183/75786/1/000554069.pdfb8f50b371725be26f6b4c9eb11616a2aMD51TEXT000554069.pdf.txt000554069.pdf.txtExtracted Texttext/plain20772http://www.lume.ufrgs.br/bitstream/10183/75786/2/000554069.pdf.txtecaa78eabc7fd8a18c980cb053db07abMD52THUMBNAIL000554069.pdf.jpg000554069.pdf.jpgGenerated Thumbnailimage/jpeg1808http://www.lume.ufrgs.br/bitstream/10183/75786/3/000554069.pdf.jpgde0f1eaa5d658f426c9b2f7911b65718MD5310183/757862023-07-21 03:31:11.414015oai:www.lume.ufrgs.br:10183/75786Repositório de PublicaçõesPUBhttps://lume.ufrgs.br/oai/requestopendoar:2023-07-21T06:31:11Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false |
dc.title.pt_BR.fl_str_mv |
Computer simulation of the stochastic dynamics of super-paramagnetic particles in ferrofluids |
title |
Computer simulation of the stochastic dynamics of super-paramagnetic particles in ferrofluids |
spellingShingle |
Computer simulation of the stochastic dynamics of super-paramagnetic particles in ferrofluids Scherer, Claudio Física Ferrofluid Magnetic fluid Computer simulation Stochastic dynamic Super-paramagnetic |
title_short |
Computer simulation of the stochastic dynamics of super-paramagnetic particles in ferrofluids |
title_full |
Computer simulation of the stochastic dynamics of super-paramagnetic particles in ferrofluids |
title_fullStr |
Computer simulation of the stochastic dynamics of super-paramagnetic particles in ferrofluids |
title_full_unstemmed |
Computer simulation of the stochastic dynamics of super-paramagnetic particles in ferrofluids |
title_sort |
Computer simulation of the stochastic dynamics of super-paramagnetic particles in ferrofluids |
author |
Scherer, Claudio |
author_facet |
Scherer, Claudio |
author_role |
author |
dc.contributor.author.fl_str_mv |
Scherer, Claudio |
dc.subject.por.fl_str_mv |
Física |
topic |
Física Ferrofluid Magnetic fluid Computer simulation Stochastic dynamic Super-paramagnetic |
dc.subject.eng.fl_str_mv |
Ferrofluid Magnetic fluid Computer simulation Stochastic dynamic Super-paramagnetic |
description |
Several papers have been written on the complex problem of the stochastic dynamics of the magnetic moments of super-paramagnetic particles, simultaneously with the stochastic rotation of these colloidal particles in a ferrofluid [1–3]. None of these works, however, is sufficiently general and conveniently simple and clear to be used in sumulational works to appropriately describe the experimental super-paramagntetic resonance lines. We have a new proposal for the equations of rotational motion, which is appropriate for simulations. Those equations are stochastic differential equations with multiplicative noise. Therefore, they have to be interpreted as Stratonovich-Langevin equations and the roles of stochastic calculus have to be used in the simulations. For this reason we will briefly present the essence of the numerical algorithms used in the solutions of Stratonovich equations. Finally, the simulational results for the magnetic response functions, and the corresponding dynamic susceptibilities, will be shown and their consequences will be analyzed. |
publishDate |
2006 |
dc.date.issued.fl_str_mv |
2006 |
dc.date.accessioned.fl_str_mv |
2013-07-11T02:22:05Z |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/other |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://hdl.handle.net/10183/75786 |
dc.identifier.issn.pt_BR.fl_str_mv |
0103-9733 |
dc.identifier.nrb.pt_BR.fl_str_mv |
000554069 |
identifier_str_mv |
0103-9733 000554069 |
url |
http://hdl.handle.net/10183/75786 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.ispartof.pt_BR.fl_str_mv |
Brazilian journal of physics. Vol. 36, n. 3A (Sept. 2006), p. 676-681 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
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