Modeling ultra-high frequency radiation emission in PIC codes

Bibliographic Details
Main Author: Pardal, M.
Publication Date: 2018
Other Authors: Sainte-Marie, A., Reboul-Salze, A., Vieira, J., Fonseca, R. A.
Language: eng
Source: Repositórios Científicos de Acesso Aberto de Portugal (RCAAP)
Download full: http://hdl.handle.net/10071/22826
Summary: From the mysterious?ray bursts, which can be studied through the spatiotemporal structure of the radiation we receive, to the creation of sources of x-rays capable of probing nanoscale structures, radiation emission by relativistic charges is a key research field in plasma physics.The processes behind radiation emission in plasmas result from strongly non-linear many body interactions which involve relativistic effects, so they are best modeled through Particle-In-Cell (PIC) simulations. However, capturing this radiation directly in PIC simulations is very challenging due to the large disparity between the temporal and spatial scales associated with such phenomena. Current algorithms only describe radiation processes in the Fourier space (e.g.JRAD [1]), missing the spatiotemporal features of the emitted radiation, which is crucial to many fields, such as super-resolution microscopy [2] and astrophysics [3].
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spelling Modeling ultra-high frequency radiation emission in PIC codesFrom the mysterious?ray bursts, which can be studied through the spatiotemporal structure of the radiation we receive, to the creation of sources of x-rays capable of probing nanoscale structures, radiation emission by relativistic charges is a key research field in plasma physics.The processes behind radiation emission in plasmas result from strongly non-linear many body interactions which involve relativistic effects, so they are best modeled through Particle-In-Cell (PIC) simulations. However, capturing this radiation directly in PIC simulations is very challenging due to the large disparity between the temporal and spatial scales associated with such phenomena. Current algorithms only describe radiation processes in the Fourier space (e.g.JRAD [1]), missing the spatiotemporal features of the emitted radiation, which is crucial to many fields, such as super-resolution microscopy [2] and astrophysics [3].European Physical Society2021-06-29T10:17:28Z2018-01-01T00:00:00Z20182021-06-29T11:06:31Zconference objectinfo:eu-repo/semantics/publishedVersionapplication/pdfhttp://hdl.handle.net/10071/22826eng979-10-96389-08-7Pardal, M.Sainte-Marie, A.Reboul-Salze, A.Vieira, J.Fonseca, R. A.info:eu-repo/semantics/openAccessreponame:Repositórios Científicos de Acesso Aberto de Portugal (RCAAP)instname:FCCN, serviços digitais da FCT – Fundação para a Ciência e a Tecnologiainstacron:RCAAP2024-07-07T02:26:05Zoai:repositorio.iscte-iul.pt:10071/22826Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireinfo@rcaap.ptopendoar:https://opendoar.ac.uk/repository/71602025-05-28T17:58:19.316612Repositórios Científicos de Acesso Aberto de Portugal (RCAAP) - FCCN, serviços digitais da FCT – Fundação para a Ciência e a Tecnologiafalse
dc.title.none.fl_str_mv Modeling ultra-high frequency radiation emission in PIC codes
title Modeling ultra-high frequency radiation emission in PIC codes
spellingShingle Modeling ultra-high frequency radiation emission in PIC codes
Pardal, M.
title_short Modeling ultra-high frequency radiation emission in PIC codes
title_full Modeling ultra-high frequency radiation emission in PIC codes
title_fullStr Modeling ultra-high frequency radiation emission in PIC codes
title_full_unstemmed Modeling ultra-high frequency radiation emission in PIC codes
title_sort Modeling ultra-high frequency radiation emission in PIC codes
author Pardal, M.
author_facet Pardal, M.
Sainte-Marie, A.
Reboul-Salze, A.
Vieira, J.
Fonseca, R. A.
author_role author
author2 Sainte-Marie, A.
Reboul-Salze, A.
Vieira, J.
Fonseca, R. A.
author2_role author
author
author
author
dc.contributor.author.fl_str_mv Pardal, M.
Sainte-Marie, A.
Reboul-Salze, A.
Vieira, J.
Fonseca, R. A.
description From the mysterious?ray bursts, which can be studied through the spatiotemporal structure of the radiation we receive, to the creation of sources of x-rays capable of probing nanoscale structures, radiation emission by relativistic charges is a key research field in plasma physics.The processes behind radiation emission in plasmas result from strongly non-linear many body interactions which involve relativistic effects, so they are best modeled through Particle-In-Cell (PIC) simulations. However, capturing this radiation directly in PIC simulations is very challenging due to the large disparity between the temporal and spatial scales associated with such phenomena. Current algorithms only describe radiation processes in the Fourier space (e.g.JRAD [1]), missing the spatiotemporal features of the emitted radiation, which is crucial to many fields, such as super-resolution microscopy [2] and astrophysics [3].
publishDate 2018
dc.date.none.fl_str_mv 2018-01-01T00:00:00Z
2018
2021-06-29T10:17:28Z
2021-06-29T11:06:31Z
dc.type.driver.fl_str_mv conference object
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dc.identifier.uri.fl_str_mv http://hdl.handle.net/10071/22826
url http://hdl.handle.net/10071/22826
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv 979-10-96389-08-7
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dc.publisher.none.fl_str_mv European Physical Society
publisher.none.fl_str_mv European Physical Society
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instname:FCCN, serviços digitais da FCT – Fundação para a Ciência e a Tecnologia
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