Slowdown of interpenetration of two counterpropagating plasma slabs due to collective effects
Autor(a) principal: | |
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Data de Publicação: | 2022 |
Outros Autores: | , , , , |
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 |
repository.mail.fl_str_mv |
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1799134850438922240 |