TY - JOUR
T1 - Spatiotemporal dynamics of ultrarelativistic beam-plasma instabilities
AU - San Miguel Claveria, P.
AU - Davoine, X.
AU - Peterson, J. R.
AU - Gilljohann, M.
AU - Andriyash, I.
AU - Ariniello, R.
AU - Clarke, C.
AU - Ekerfelt, H.
AU - Emma, C.
AU - Faure, J.
AU - Gessner, S.
AU - Hogan, M. J.
AU - Joshi, C.
AU - Keitel, C. H.
AU - Knetsch, A.
AU - Kononenko, O.
AU - Litos, M.
AU - Mankovska, Y.
AU - Marsh, K.
AU - Matheron, A.
AU - Nie, Z.
AU - O'Shea, B.
AU - Storey, D.
AU - Vafaei-Najafabadi, N.
AU - Wu, Y.
AU - Xu, X.
AU - Yan, J.
AU - Zhang, C.
AU - Tamburini, M.
AU - Fiuza, F.
AU - Gremillet, L.
AU - Corde, S.
N1 - Publisher Copyright:
© 2022 authors. Published by the American Physical Society. Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI.
PY - 2022/6/1
Y1 - 2022/6/1
N2 - An electron or electron-positron beam streaming through a plasma is notoriously prone to microinstabilities. For a dilute ultrarelativistic infinite beam, the dominant instability is a mixed mode between longitudinal two-stream and transverse filamentation modes, with a phase velocity oblique to the beam velocity. A spatiotemporal theory describing the linear growth of this oblique mixed instability is proposed which predicts that spatiotemporal effects generally prevail for finite-length beams, leading to a significantly slower instability evolution than in the usually assumed purely temporal regime. These results are accurately supported by particle-in-cell (PIC) simulations. Furthermore, we show that the self-focusing dynamics caused by the plasma wakefields driven by finite-width beams can compete with the oblique instability. Analyzed through PIC simulations, the interplay of these two processes in realistic systems bears important implications for upcoming accelerator experiments on ultrarelativistic beam-plasma interactions.
AB - An electron or electron-positron beam streaming through a plasma is notoriously prone to microinstabilities. For a dilute ultrarelativistic infinite beam, the dominant instability is a mixed mode between longitudinal two-stream and transverse filamentation modes, with a phase velocity oblique to the beam velocity. A spatiotemporal theory describing the linear growth of this oblique mixed instability is proposed which predicts that spatiotemporal effects generally prevail for finite-length beams, leading to a significantly slower instability evolution than in the usually assumed purely temporal regime. These results are accurately supported by particle-in-cell (PIC) simulations. Furthermore, we show that the self-focusing dynamics caused by the plasma wakefields driven by finite-width beams can compete with the oblique instability. Analyzed through PIC simulations, the interplay of these two processes in realistic systems bears important implications for upcoming accelerator experiments on ultrarelativistic beam-plasma interactions.
U2 - 10.1103/PhysRevResearch.4.023085
DO - 10.1103/PhysRevResearch.4.023085
M3 - Article
AN - SCOPUS:85130588960
SN - 2643-1564
VL - 4
JO - Physical Review Research
JF - Physical Review Research
IS - 2
M1 - 023085
ER -