Halo formation and emittance growth in the transport of spherically symmetric mismatched bunched beam

Detalhes bibliográficos
Autor(a) principal: Silva, Thales Marques Corrêa da
Data de Publicação: 2015
Outros Autores: Pakter, Renato, Rizzato, Felipe Barbedo, Levin, Yan
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UFRGS
Texto Completo: http://hdl.handle.net/10183/142386
Resumo: The effect of an initial envelope mismatch on the transport of bunched spherically symmetric beams is investigated. A particle-core model is used to estimate the maximum radius that halo particles can reach. The theory is used to obtain an empirical formula that provides the halo size as a function of system parameters. Taking into account, the incompressibility property of the Vlasov dynamics and the resulting Landau damping, an explicit form for the final stationary distribution attained by the beam is proposed. The distribution is fully self-consistent, presenting no free fitting parameters. The theory is used to predict the relevant beam transport properties, such as the final particle density distribution, the emittance growth, and the fraction of particles that will be expelled to form halo. The theoretical results are compared to the explicit N-particle dynamics simulations, showing a good agreement.
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spelling Silva, Thales Marques Corrêa daPakter, RenatoRizzato, Felipe BarbedoLevin, Yan2016-06-09T02:08:29Z20151070-664Xhttp://hdl.handle.net/10183/142386000911108The effect of an initial envelope mismatch on the transport of bunched spherically symmetric beams is investigated. A particle-core model is used to estimate the maximum radius that halo particles can reach. The theory is used to obtain an empirical formula that provides the halo size as a function of system parameters. Taking into account, the incompressibility property of the Vlasov dynamics and the resulting Landau damping, an explicit form for the final stationary distribution attained by the beam is proposed. The distribution is fully self-consistent, presenting no free fitting parameters. The theory is used to predict the relevant beam transport properties, such as the final particle density distribution, the emittance growth, and the fraction of particles that will be expelled to form halo. The theoretical results are compared to the explicit N-particle dynamics simulations, showing a good agreement.application/pdfengPhysics of plasmas. Melville. Vol. 22, no. 2 (Feb. 2015), 023102, 8 p.Equacao de vlasovDinâmica de feixes de partículasFormação de aglomerados em feixes de partículasHalo formation and emittance growth in the transport of spherically symmetric mismatched bunched beamEstrangeiroinfo: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:UFRGSORIGINAL000911108.pdf000911108.pdfTexto completo (inglês)application/pdf940922http://www.lume.ufrgs.br/bitstream/10183/142386/1/000911108.pdf24eabb404cbb6b77d1b30149c3ebab6bMD51TEXT000911108.pdf.txt000911108.pdf.txtExtracted Texttext/plain36011http://www.lume.ufrgs.br/bitstream/10183/142386/2/000911108.pdf.txt29c60b0eaf4b8e309c3e9dec65d7bb01MD52THUMBNAIL000911108.pdf.jpg000911108.pdf.jpgGenerated Thumbnailimage/jpeg2140http://www.lume.ufrgs.br/bitstream/10183/142386/3/000911108.pdf.jpg210ebdf573e9f0e9dfe785052d77b9ecMD5310183/1423862023-08-30 03:59:26.90414oai:www.lume.ufrgs.br:10183/142386Repositório de PublicaçõesPUBhttps://lume.ufrgs.br/oai/requestopendoar:2023-08-30T06:59:26Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false
dc.title.pt_BR.fl_str_mv Halo formation and emittance growth in the transport of spherically symmetric mismatched bunched beam
title Halo formation and emittance growth in the transport of spherically symmetric mismatched bunched beam
spellingShingle Halo formation and emittance growth in the transport of spherically symmetric mismatched bunched beam
Silva, Thales Marques Corrêa da
Equacao de vlasov
Dinâmica de feixes de partículas
Formação de aglomerados em feixes de partículas
title_short Halo formation and emittance growth in the transport of spherically symmetric mismatched bunched beam
title_full Halo formation and emittance growth in the transport of spherically symmetric mismatched bunched beam
title_fullStr Halo formation and emittance growth in the transport of spherically symmetric mismatched bunched beam
title_full_unstemmed Halo formation and emittance growth in the transport of spherically symmetric mismatched bunched beam
title_sort Halo formation and emittance growth in the transport of spherically symmetric mismatched bunched beam
author Silva, Thales Marques Corrêa da
author_facet Silva, Thales Marques Corrêa da
Pakter, Renato
Rizzato, Felipe Barbedo
Levin, Yan
author_role author
author2 Pakter, Renato
Rizzato, Felipe Barbedo
Levin, Yan
author2_role author
author
author
dc.contributor.author.fl_str_mv Silva, Thales Marques Corrêa da
Pakter, Renato
Rizzato, Felipe Barbedo
Levin, Yan
dc.subject.por.fl_str_mv Equacao de vlasov
Dinâmica de feixes de partículas
Formação de aglomerados em feixes de partículas
topic Equacao de vlasov
Dinâmica de feixes de partículas
Formação de aglomerados em feixes de partículas
description The effect of an initial envelope mismatch on the transport of bunched spherically symmetric beams is investigated. A particle-core model is used to estimate the maximum radius that halo particles can reach. The theory is used to obtain an empirical formula that provides the halo size as a function of system parameters. Taking into account, the incompressibility property of the Vlasov dynamics and the resulting Landau damping, an explicit form for the final stationary distribution attained by the beam is proposed. The distribution is fully self-consistent, presenting no free fitting parameters. The theory is used to predict the relevant beam transport properties, such as the final particle density distribution, the emittance growth, and the fraction of particles that will be expelled to form halo. The theoretical results are compared to the explicit N-particle dynamics simulations, showing a good agreement.
publishDate 2015
dc.date.issued.fl_str_mv 2015
dc.date.accessioned.fl_str_mv 2016-06-09T02:08:29Z
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dc.identifier.uri.fl_str_mv http://hdl.handle.net/10183/142386
dc.identifier.issn.pt_BR.fl_str_mv 1070-664X
dc.identifier.nrb.pt_BR.fl_str_mv 000911108
identifier_str_mv 1070-664X
000911108
url http://hdl.handle.net/10183/142386
dc.language.iso.fl_str_mv eng
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dc.relation.ispartof.pt_BR.fl_str_mv Physics of plasmas. Melville. Vol. 22, no. 2 (Feb. 2015), 023102, 8 p.
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