Slowdown of interpenetration of two counterpropagating plasma slabs due to collective effects

Detalhes bibliográficos
Autor(a) principal: Shulka, N
Data de Publicação: 2022
Outros Autores: Schoeffler, K. M., Vieira, J., Fonseca, R. A., Boella, E, 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/10071/25580
Resumo: The nonlinear evolution of electromagnetic instabilities driven by the interpenetration of two e-,e+ plasma clouds is explored using ab initio kinetic plasma simulations. We show that the plasma clouds slow down due to both oblique and Weibel generated electromagnetic fields, which deflect the particle trajectories, transferring bulk forward momentum into transverse momentum and thermal velocity spread. This process causes the flow velocity vinst to decrease approximately by a factor of 1/3 in a time interval ?t?B?p∼c/(vfl?B), where ?B is the magnetic equipartition parameter determined by the nonlinear saturation of the instabilities, vfl is the initial flow speed, and ?p is the plasma frequency. For the ?B measured in our simulations, ?t?B is close to 10 times the instability growth time. We show that as long as the plasma slab length L>vfl?t?B, the plasma flow is expected to slow down by a factor close to 1/3.
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spelling Slowdown of interpenetration of two counterpropagating plasma slabs due to collective effectsThe nonlinear evolution of electromagnetic instabilities driven by the interpenetration of two e-,e+ plasma clouds is explored using ab initio kinetic plasma simulations. We show that the plasma clouds slow down due to both oblique and Weibel generated electromagnetic fields, which deflect the particle trajectories, transferring bulk forward momentum into transverse momentum and thermal velocity spread. This process causes the flow velocity vinst to decrease approximately by a factor of 1/3 in a time interval ?t?B?p∼c/(vfl?B), where ?B is the magnetic equipartition parameter determined by the nonlinear saturation of the instabilities, vfl is the initial flow speed, and ?p is the plasma frequency. For the ?B measured in our simulations, ?t?B is close to 10 times the instability growth time. We show that as long as the plasma slab length L>vfl?t?B, the plasma flow is expected to slow down by a factor close to 1/3.American Physical Society2022-05-31T13:05:59Z2022-01-01T00:00:00Z20222022-05-31T14:05:31Zinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://hdl.handle.net/10071/25580eng1539-375510.1103/PhysRevE.105.035204Shulka, NSchoeffler, K. M.Vieira, J.Fonseca, R. A.Boella, ESilva, 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:RCAAP2023-11-09T17:56:12Zoai:repositorio.iscte-iul.pt:10071/25580Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireopendoar:71602024-03-19T22:28:46.630610Repositório 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 Slowdown of interpenetration of two counterpropagating plasma slabs due to collective effects
title Slowdown of interpenetration of two counterpropagating plasma slabs due to collective effects
spellingShingle Slowdown of interpenetration of two counterpropagating plasma slabs due to collective effects
Shulka, N
title_short Slowdown of interpenetration of two counterpropagating plasma slabs due to collective effects
title_full Slowdown of interpenetration of two counterpropagating plasma slabs due to collective effects
title_fullStr Slowdown of interpenetration of two counterpropagating plasma slabs due to collective effects
title_full_unstemmed Slowdown of interpenetration of two counterpropagating plasma slabs due to collective effects
title_sort Slowdown of interpenetration of two counterpropagating plasma slabs due to collective effects
author Shulka, N
author_facet Shulka, N
Schoeffler, K. M.
Vieira, J.
Fonseca, R. A.
Boella, E
Silva, L. O.
author_role author
author2 Schoeffler, K. M.
Vieira, J.
Fonseca, R. A.
Boella, E
Silva, L. O.
author2_role author
author
author
author
author
dc.contributor.author.fl_str_mv Shulka, N
Schoeffler, K. M.
Vieira, J.
Fonseca, R. A.
Boella, E
Silva, L. O.
description The nonlinear evolution of electromagnetic instabilities driven by the interpenetration of two e-,e+ plasma clouds is explored using ab initio kinetic plasma simulations. We show that the plasma clouds slow down due to both oblique and Weibel generated electromagnetic fields, which deflect the particle trajectories, transferring bulk forward momentum into transverse momentum and thermal velocity spread. This process causes the flow velocity vinst to decrease approximately by a factor of 1/3 in a time interval ?t?B?p∼c/(vfl?B), where ?B is the magnetic equipartition parameter determined by the nonlinear saturation of the instabilities, vfl is the initial flow speed, and ?p is the plasma frequency. For the ?B measured in our simulations, ?t?B is close to 10 times the instability growth time. We show that as long as the plasma slab length L>vfl?t?B, the plasma flow is expected to slow down by a factor close to 1/3.
publishDate 2022
dc.date.none.fl_str_mv 2022-05-31T13:05:59Z
2022-01-01T00:00:00Z
2022
2022-05-31T14:05:31Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://hdl.handle.net/10071/25580
url http://hdl.handle.net/10071/25580
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv 1539-3755
10.1103/PhysRevE.105.035204
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv American Physical Society
publisher.none.fl_str_mv American Physical Society
dc.source.none.fl_str_mv reponame:Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)
instname:Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informação
instacron:RCAAP
instname_str Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informação
instacron_str RCAAP
institution RCAAP
reponame_str Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)
collection Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)
repository.name.fl_str_mv Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) - Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informação
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