Halo formation and emittance growth in the transport of spherically symmetric mismatched bunched beam
Autor(a) principal: | |
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Data de Publicação: | 2015 |
Outros Autores: | , , |
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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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 |
dc.type.driver.fl_str_mv |
Estrangeiro info:eu-repo/semantics/article |
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/10183/142386 |
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 |
language |
eng |
dc.relation.ispartof.pt_BR.fl_str_mv |
Physics of plasmas. Melville. Vol. 22, no. 2 (Feb. 2015), 023102, 8 p. |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
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application/pdf |
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