Modeling ultra-high frequency radiation emission in PIC codes
| Main Author: | |
|---|---|
| Publication Date: | 2018 |
| Other Authors: | , , , |
| 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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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]. |
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2018 |
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2018-01-01T00:00:00Z 2018 2021-06-29T10:17:28Z 2021-06-29T11:06:31Z |
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conference object |
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info:eu-repo/semantics/publishedVersion |
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publishedVersion |
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http://hdl.handle.net/10071/22826 |
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http://hdl.handle.net/10071/22826 |
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eng |
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eng |
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979-10-96389-08-7 |
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openAccess |
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application/pdf |
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European Physical Society |
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European Physical Society |
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