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Microstructure formation in radially counterstreaming electron flows
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dc.contributor.author | Iñigo Gamiz, Lucas I | |
dc.contributor.author | Ersfeld, Bernhard | |
dc.contributor.author | Brunetti, Enrico | |
dc.contributor.author | Yoffe, Samuel R | |
dc.contributor.author | Cairns, R Alan | |
dc.contributor.author | Noble, Adam | |
dc.contributor.author | Holt, George K | |
dc.contributor.author | Jaroszynski, Dino A | |
dc.date.accessioned | 2021-04-08T11:30:23Z | |
dc.date.available | 2021-04-08T11:30:23Z | |
dc.date.issued | 2021-04-07 | |
dc.identifier | 273717374 | |
dc.identifier | ca662798-3043-46c0-8633-54a87e506e01 | |
dc.identifier | 000637835900001 | |
dc.identifier | 85104568268 | |
dc.identifier.citation | Iñigo Gamiz , L I , Ersfeld , B , Brunetti , E , Yoffe , S R , Cairns , R A , Noble , A , Holt , G K & Jaroszynski , D A 2021 , ' Microstructure formation in radially counterstreaming electron flows ' , New Journal of Physics , vol. 23 , no. 4 , 043017 . https://doi.org/10.1088/1367-2630/abe8f6 | en |
dc.identifier.issn | 1367-2630 | |
dc.identifier.other | Jisc: 017796f27cef4b1e96925cfdc3008c04 | |
dc.identifier.other | publisher-id: njpabe8f6 | |
dc.identifier.other | manuscript: abe8f6 | |
dc.identifier.other | other: njp-112543.r2 | |
dc.identifier.uri | https://hdl.handle.net/10023/22986 | |
dc.description | We acknowledge the support of the UK EPSRC, Grant Number EP/N028694/1, and the EC's Laserlab-Europe H2020 EC-GA Nos. 654148 and 871124. | en |
dc.description.abstract | A theoretical model is developed to describe the formation of microstructures due to plasma streaming instabilities in radially convergent geometries. Microstructures in the form of radial spokes are found experimentally in laser wakefield accelerators. The eigenvalues of a set of coupled linear ordinary differential equations are obtained and the complex wavenumbers calculated to give the local growth rates. The predictions are confirmed using particle-in-cell (PIC) simulations carried out for two counter-propagating converging/diverging plasma annuli. The simulations consistently demonstrate unstable growth for interactions between two counterpropagating annuli with different number densities. The growth rates obtained from the PIC simulations agree well with the growth rates from the semi-analytical model. The theory presented in this paper can provide powerful insight into converging plasma beams found in space and laboratory scale plasma. | |
dc.format.extent | 8 | |
dc.format.extent | 2357039 | |
dc.language.iso | eng | |
dc.relation.ispartof | New Journal of Physics | en |
dc.subject | Paper | en |
dc.subject | Plasma microstructures | en |
dc.subject | Plasma instabilities | en |
dc.subject | Streaming instabilities | en |
dc.subject | Wakefield accelerator | en |
dc.subject | QC Physics | en |
dc.subject | TK Electrical engineering. Electronics Nuclear engineering | en |
dc.subject | DAS | en |
dc.subject.lcc | QC | en |
dc.subject.lcc | TK | en |
dc.title | Microstructure formation in radially counterstreaming electron flows | en |
dc.type | Journal article | en |
dc.contributor.sponsor | EPSRC | en |
dc.contributor.institution | University of St Andrews. Statistics | en |
dc.contributor.institution | University of St Andrews. Applied Mathematics | en |
dc.identifier.doi | https://doi.org/10.1088/1367-2630/abe8f6 | |
dc.description.status | Peer reviewed | en |
dc.identifier.grantnumber | EP/N028694/1 | en |
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