Uphill acceleration in a spatially modulated electrostatic field particle accelerator

Detalhes bibliográficos
Autor(a) principal: Almansa, Ivanessa da Silveira
Data de Publicação: 2018
Outros Autores: Burton, David A., Cairns, R.A., Marini, Samuel, Peter, Eduardo Alcides, Rizzato, Felipe Barbedo, Russman, Felipe Boff
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UFRGS
Texto Completo: http://hdl.handle.net/10183/204117
Resumo: Spatially modulated electrostatic fields can be designed to efficiently accelerate particles by exploring the relationships between the amplitude, the phase velocity, the shape of the potential, and the initial velocity of the particle. The acceleration process occurs when the value of the velocity excursions of the particle surpasses the phase velocity of the carrier, as a resonant mechanism. The ponderomotive approximation based on the Lagrangian average is usually applied in this kind of system in non-accelerating regimes. The mean dynamics of the particle is well described by this approximation far from resonance. However, the approximation fails to predict some interesting features of the model near resonance, such as the uphill acceleration phenomenon. A canonical perturbation theory is more accurate in these conditions. In this work, we compare the results from the Lagrangian average and from a canonical perturbation theory, focusing in regions where the results of these two approaches differ from each other.
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spelling Almansa, Ivanessa da SilveiraBurton, David A.Cairns, R.A.Marini, SamuelPeter, Eduardo AlcidesRizzato, Felipe BarbedoRussman, Felipe Boff2020-01-14T04:15:28Z20181070-664Xhttp://hdl.handle.net/10183/204117001109683Spatially modulated electrostatic fields can be designed to efficiently accelerate particles by exploring the relationships between the amplitude, the phase velocity, the shape of the potential, and the initial velocity of the particle. The acceleration process occurs when the value of the velocity excursions of the particle surpasses the phase velocity of the carrier, as a resonant mechanism. The ponderomotive approximation based on the Lagrangian average is usually applied in this kind of system in non-accelerating regimes. The mean dynamics of the particle is well described by this approximation far from resonance. However, the approximation fails to predict some interesting features of the model near resonance, such as the uphill acceleration phenomenon. A canonical perturbation theory is more accurate in these conditions. In this work, we compare the results from the Lagrangian average and from a canonical perturbation theory, focusing in regions where the results of these two approaches differ from each other.application/pdfengPhysics of plasmas. Melville. Vol. 25, no. 11 (Nov. 2018), 113107, 6 p.Aceleradores de partículasSimulação numéricaOndas eletrostáticasUphill acceleration in a spatially modulated electrostatic field particle acceleratorEstrangeiroinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/openAccessreponame:Repositório Institucional da UFRGSinstname:Universidade Federal do Rio Grande do Sul (UFRGS)instacron:UFRGSTEXT001109683.pdf.txt001109683.pdf.txtExtracted Texttext/plain28274http://www.lume.ufrgs.br/bitstream/10183/204117/2/001109683.pdf.txtca1de2abd86709e3f5e9332dbe0e33d2MD52ORIGINAL001109683.pdfTexto completo (inglês)application/pdf1110892http://www.lume.ufrgs.br/bitstream/10183/204117/1/001109683.pdf8ebafd617537ef2f5a3f446b3bb93b5bMD5110183/2041172023-08-25 03:32:08.219937oai:www.lume.ufrgs.br:10183/204117Repositório de PublicaçõesPUBhttps://lume.ufrgs.br/oai/requestopendoar:2023-08-25T06:32:08Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false
dc.title.pt_BR.fl_str_mv Uphill acceleration in a spatially modulated electrostatic field particle accelerator
title Uphill acceleration in a spatially modulated electrostatic field particle accelerator
spellingShingle Uphill acceleration in a spatially modulated electrostatic field particle accelerator
Almansa, Ivanessa da Silveira
Aceleradores de partículas
Simulação numérica
Ondas eletrostáticas
title_short Uphill acceleration in a spatially modulated electrostatic field particle accelerator
title_full Uphill acceleration in a spatially modulated electrostatic field particle accelerator
title_fullStr Uphill acceleration in a spatially modulated electrostatic field particle accelerator
title_full_unstemmed Uphill acceleration in a spatially modulated electrostatic field particle accelerator
title_sort Uphill acceleration in a spatially modulated electrostatic field particle accelerator
author Almansa, Ivanessa da Silveira
author_facet Almansa, Ivanessa da Silveira
Burton, David A.
Cairns, R.A.
Marini, Samuel
Peter, Eduardo Alcides
Rizzato, Felipe Barbedo
Russman, Felipe Boff
author_role author
author2 Burton, David A.
Cairns, R.A.
Marini, Samuel
Peter, Eduardo Alcides
Rizzato, Felipe Barbedo
Russman, Felipe Boff
author2_role author
author
author
author
author
author
dc.contributor.author.fl_str_mv Almansa, Ivanessa da Silveira
Burton, David A.
Cairns, R.A.
Marini, Samuel
Peter, Eduardo Alcides
Rizzato, Felipe Barbedo
Russman, Felipe Boff
dc.subject.por.fl_str_mv Aceleradores de partículas
Simulação numérica
Ondas eletrostáticas
topic Aceleradores de partículas
Simulação numérica
Ondas eletrostáticas
description Spatially modulated electrostatic fields can be designed to efficiently accelerate particles by exploring the relationships between the amplitude, the phase velocity, the shape of the potential, and the initial velocity of the particle. The acceleration process occurs when the value of the velocity excursions of the particle surpasses the phase velocity of the carrier, as a resonant mechanism. The ponderomotive approximation based on the Lagrangian average is usually applied in this kind of system in non-accelerating regimes. The mean dynamics of the particle is well described by this approximation far from resonance. However, the approximation fails to predict some interesting features of the model near resonance, such as the uphill acceleration phenomenon. A canonical perturbation theory is more accurate in these conditions. In this work, we compare the results from the Lagrangian average and from a canonical perturbation theory, focusing in regions where the results of these two approaches differ from each other.
publishDate 2018
dc.date.issued.fl_str_mv 2018
dc.date.accessioned.fl_str_mv 2020-01-14T04:15:28Z
dc.type.driver.fl_str_mv Estrangeiro
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dc.identifier.uri.fl_str_mv http://hdl.handle.net/10183/204117
dc.identifier.issn.pt_BR.fl_str_mv 1070-664X
dc.identifier.nrb.pt_BR.fl_str_mv 001109683
identifier_str_mv 1070-664X
001109683
url http://hdl.handle.net/10183/204117
dc.language.iso.fl_str_mv eng
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dc.relation.ispartof.pt_BR.fl_str_mv Physics of plasmas. Melville. Vol. 25, no. 11 (Nov. 2018), 113107, 6 p.
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