Cratering induced by slow highly charged ions on ultrathin PMMA films
Autor(a) principal: | |
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Data de Publicação: | 2022 |
Outros Autores: | , , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UFRGS |
Texto Completo: | http://hdl.handle.net/10183/257893 |
Resumo: | Highly charged ions are a well-known tool for the nanostructuring of surfaces. We report on the thickness dependence of nanostructures produced by single 260 keV Xe38+ ions on ultrathin poly(methyl methacrylate) (PMMA) films (1 nm to 60 nm) deposited onto Si substrates. The nanostructures induced by slow highly charged ions are rimless craters with a diameter of around 15 nm, which are roughly independent of the thickness of the films down to layers of about 2 nm. The crater depth and thus the overall crater volume are, however, thickness-dependent, decreasing in size in films thinner than ~25 nm. Our findings indicate that although the potential energy of the highly charged ions is the predominant source of deposited energy, the depth of the excited material contributing to crater formation is much larger than the neutralization depth of the ions, which occurs in the first nanometer of the solid at the projectile velocity employed here. This suggests synergism between kinetic and potential-driven processes in nanostructure formation in PMMA. |
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Thomaz, Raquel SilvaErnst, PhilippGrande, Pedro LuisSchleberger, M.Papaleo, Ricardo Meurer2023-05-10T03:27:44Z20222218-2004http://hdl.handle.net/10183/257893001162367Highly charged ions are a well-known tool for the nanostructuring of surfaces. We report on the thickness dependence of nanostructures produced by single 260 keV Xe38+ ions on ultrathin poly(methyl methacrylate) (PMMA) films (1 nm to 60 nm) deposited onto Si substrates. The nanostructures induced by slow highly charged ions are rimless craters with a diameter of around 15 nm, which are roughly independent of the thickness of the films down to layers of about 2 nm. The crater depth and thus the overall crater volume are, however, thickness-dependent, decreasing in size in films thinner than ~25 nm. Our findings indicate that although the potential energy of the highly charged ions is the predominant source of deposited energy, the depth of the excited material contributing to crater formation is much larger than the neutralization depth of the ions, which occurs in the first nanometer of the solid at the projectile velocity employed here. This suggests synergism between kinetic and potential-driven processes in nanostructure formation in PMMA.application/pdfengAtoms. Basel. Vol. 10, no. 4 (Dec. 2022), 96, 7 p.NanoestruturasFilmes finosÍonsPolimetil metacrilatoSlow highly charged ionsNanostructuresRadiation effectsSingle-ion impactsPolymer thin filmsPMMACratering induced by slow highly charged ions on ultrathin PMMA filmsEstrangeiroinfo: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:UFRGSTEXT001162367.pdf.txt001162367.pdf.txtExtracted Texttext/plain27150http://www.lume.ufrgs.br/bitstream/10183/257893/2/001162367.pdf.txtafb42667705406977ee10522b99fb2ccMD52ORIGINAL001162367.pdfTexto completo (inglês)application/pdf10577510http://www.lume.ufrgs.br/bitstream/10183/257893/1/001162367.pdf61ec69e670b8bbf0c89c495d424fae28MD5110183/2578932024-05-24 06:42:03.677868oai:www.lume.ufrgs.br:10183/257893Repositório de PublicaçõesPUBhttps://lume.ufrgs.br/oai/requestopendoar:2024-05-24T09:42:03Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false |
dc.title.pt_BR.fl_str_mv |
Cratering induced by slow highly charged ions on ultrathin PMMA films |
title |
Cratering induced by slow highly charged ions on ultrathin PMMA films |
spellingShingle |
Cratering induced by slow highly charged ions on ultrathin PMMA films Thomaz, Raquel Silva Nanoestruturas Filmes finos Íons Polimetil metacrilato Slow highly charged ions Nanostructures Radiation effects Single-ion impacts Polymer thin films PMMA |
title_short |
Cratering induced by slow highly charged ions on ultrathin PMMA films |
title_full |
Cratering induced by slow highly charged ions on ultrathin PMMA films |
title_fullStr |
Cratering induced by slow highly charged ions on ultrathin PMMA films |
title_full_unstemmed |
Cratering induced by slow highly charged ions on ultrathin PMMA films |
title_sort |
Cratering induced by slow highly charged ions on ultrathin PMMA films |
author |
Thomaz, Raquel Silva |
author_facet |
Thomaz, Raquel Silva Ernst, Philipp Grande, Pedro Luis Schleberger, M. Papaleo, Ricardo Meurer |
author_role |
author |
author2 |
Ernst, Philipp Grande, Pedro Luis Schleberger, M. Papaleo, Ricardo Meurer |
author2_role |
author author author author |
dc.contributor.author.fl_str_mv |
Thomaz, Raquel Silva Ernst, Philipp Grande, Pedro Luis Schleberger, M. Papaleo, Ricardo Meurer |
dc.subject.por.fl_str_mv |
Nanoestruturas Filmes finos Íons Polimetil metacrilato |
topic |
Nanoestruturas Filmes finos Íons Polimetil metacrilato Slow highly charged ions Nanostructures Radiation effects Single-ion impacts Polymer thin films PMMA |
dc.subject.eng.fl_str_mv |
Slow highly charged ions Nanostructures Radiation effects Single-ion impacts Polymer thin films PMMA |
description |
Highly charged ions are a well-known tool for the nanostructuring of surfaces. We report on the thickness dependence of nanostructures produced by single 260 keV Xe38+ ions on ultrathin poly(methyl methacrylate) (PMMA) films (1 nm to 60 nm) deposited onto Si substrates. The nanostructures induced by slow highly charged ions are rimless craters with a diameter of around 15 nm, which are roughly independent of the thickness of the films down to layers of about 2 nm. The crater depth and thus the overall crater volume are, however, thickness-dependent, decreasing in size in films thinner than ~25 nm. Our findings indicate that although the potential energy of the highly charged ions is the predominant source of deposited energy, the depth of the excited material contributing to crater formation is much larger than the neutralization depth of the ions, which occurs in the first nanometer of the solid at the projectile velocity employed here. This suggests synergism between kinetic and potential-driven processes in nanostructure formation in PMMA. |
publishDate |
2022 |
dc.date.issued.fl_str_mv |
2022 |
dc.date.accessioned.fl_str_mv |
2023-05-10T03:27:44Z |
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/10183/257893 |
dc.identifier.issn.pt_BR.fl_str_mv |
2218-2004 |
dc.identifier.nrb.pt_BR.fl_str_mv |
001162367 |
identifier_str_mv |
2218-2004 001162367 |
url |
http://hdl.handle.net/10183/257893 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.ispartof.pt_BR.fl_str_mv |
Atoms. Basel. Vol. 10, no. 4 (Dec. 2022), 96, 7 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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