Exploring the nature of collisionless shocks under laboratory conditions

Detalhes bibliográficos
Autor(a) principal: Stockem, A.
Data de Publicação: 2014
Outros Autores: Fiuza, F., Bret, A., Fonseca, R. A., Silva, L. O.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)
Texto Completo: http://hdl.handle.net/10071/7495
Resumo: Collisionless shocks are pervasive in astrophysics and they are critical to understand cosmic ray acceleration. Laboratory experiments with intense lasers are now opening the way to explore and characterise the underlying microphysics, which determine the acceleration process of collisionless shocks. We determine the shock character – electrostatic or electromagnetic – based on the stability of electrostatic shocks to transverse electromagnetic fluctuations as a function of the electron temperature and flow velocity of the plasma components, and we compare the analytical model with particle-in-cell simulations. By making the connection with the laser parameters driving the plasma flows, we demonstrate that shocks with different and distinct underlying microphysics can be explored in the laboratory with state-of-the-art laser systems.
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spelling Exploring the nature of collisionless shocks under laboratory conditionsCollisionless shocks are pervasive in astrophysics and they are critical to understand cosmic ray acceleration. Laboratory experiments with intense lasers are now opening the way to explore and characterise the underlying microphysics, which determine the acceleration process of collisionless shocks. We determine the shock character – electrostatic or electromagnetic – based on the stability of electrostatic shocks to transverse electromagnetic fluctuations as a function of the electron temperature and flow velocity of the plasma components, and we compare the analytical model with particle-in-cell simulations. By making the connection with the laser parameters driving the plasma flows, we demonstrate that shocks with different and distinct underlying microphysics can be explored in the laboratory with state-of-the-art laser systems.Nature Publishing Group2014-06-09T14:27:21Z2014-01-01T00:00:00Z20142019-05-20T16:06:41Zinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://hdl.handle.net/10071/7495eng2045-232210.1038/srep03934Stockem, A.Fiuza, F.Bret, A.Fonseca, R. A.Silva, L. O.info:eu-repo/semantics/openAccessreponame:Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)instname:Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informaçãoinstacron:RCAAP2023-11-09T17:46:05Zoai:repositorio.iscte-iul.pt:10071/7495Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireopendoar:71602024-03-19T22:22:06.758755Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) - Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informaçãofalse
dc.title.none.fl_str_mv Exploring the nature of collisionless shocks under laboratory conditions
title Exploring the nature of collisionless shocks under laboratory conditions
spellingShingle Exploring the nature of collisionless shocks under laboratory conditions
Stockem, A.
title_short Exploring the nature of collisionless shocks under laboratory conditions
title_full Exploring the nature of collisionless shocks under laboratory conditions
title_fullStr Exploring the nature of collisionless shocks under laboratory conditions
title_full_unstemmed Exploring the nature of collisionless shocks under laboratory conditions
title_sort Exploring the nature of collisionless shocks under laboratory conditions
author Stockem, A.
author_facet Stockem, A.
Fiuza, F.
Bret, A.
Fonseca, R. A.
Silva, L. O.
author_role author
author2 Fiuza, F.
Bret, A.
Fonseca, R. A.
Silva, L. O.
author2_role author
author
author
author
dc.contributor.author.fl_str_mv Stockem, A.
Fiuza, F.
Bret, A.
Fonseca, R. A.
Silva, L. O.
description Collisionless shocks are pervasive in astrophysics and they are critical to understand cosmic ray acceleration. Laboratory experiments with intense lasers are now opening the way to explore and characterise the underlying microphysics, which determine the acceleration process of collisionless shocks. We determine the shock character – electrostatic or electromagnetic – based on the stability of electrostatic shocks to transverse electromagnetic fluctuations as a function of the electron temperature and flow velocity of the plasma components, and we compare the analytical model with particle-in-cell simulations. By making the connection with the laser parameters driving the plasma flows, we demonstrate that shocks with different and distinct underlying microphysics can be explored in the laboratory with state-of-the-art laser systems.
publishDate 2014
dc.date.none.fl_str_mv 2014-06-09T14:27:21Z
2014-01-01T00:00:00Z
2014
2019-05-20T16:06:41Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
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dc.identifier.uri.fl_str_mv http://hdl.handle.net/10071/7495
url http://hdl.handle.net/10071/7495
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv 2045-2322
10.1038/srep03934
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dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv Nature Publishing Group
publisher.none.fl_str_mv Nature Publishing Group
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