CERN Accelerating science

Article
Report number arXiv:2312.13883
Title Filamentation of a Relativistic Proton Bunch in Plasma
Author(s)

Verra, L. (CERN) ; Amoedo, C. (CERN) ; Torrado, N. (CERN ; Lisbon, IST) ; Clairembaud, A. (CERN ; IJCLab, Orsay) ; Mezger, J. (Munich, Max Planck Inst.) ; Pannell, F. (University Coll. London) ; Pucek, J. (Munich, Max Planck Inst.) ; van Gils, N. (CERN) ; Bergamaschi, M. (Munich, Max Planck Inst.) ; Della Porta, G. Zevi (CERN ; Munich, Max Planck Inst.) ; Lopes, N. (Lisbon, IST) ; Sublet, A. (CERN) ; Turner, M. (CERN) ; Gschwendtner, E. (CERN) ; Muggli, P. (Munich, Max Planck Inst.) ; Agnello, R. (LPHE, Lausanne) ; Ahdida, C.C. (CERN) ; Andrebe, Y. (LPHE, Lausanne) ; Apsimon, O. (Manchester U. ; Cockcroft Inst. Accel. Sci. Tech.) ; Apsimon, R. (Cockcroft Inst. Accel. Sci. Tech. ; Lancaster U.) ; Arnesano, J.M. (CERN) ; Bencini, V. (CERN ; JAI, UK) ; Blanchard, P. (LPHE, Lausanne) ; Burrows, P.N. (JAI, UK) ; Buttenschön, B. (Greifswald, Max Planck Inst.) ; Caldwell, A. (Munich, Max Planck Inst.) ; Chung, M. (UNIST, Ulsan) ; Cooke, D.A. (University Coll. London) ; Davut, C. (Manchester U. ; Cockcroft Inst. Accel. Sci. Tech.) ; Demeter, G. (Wigner RCP, Budapest) ; Dexter, A.C. (Cockcroft Inst. Accel. Sci. Tech. ; Lancaster U.) ; Doebert, S. (CERN) ; Farmer, J. (Munich, Max Planck Inst.) ; Fasoli, A. (LPHE, Lausanne) ; Fonseca, R. (Lisbon, CFTP ; Lisbon, IST) ; Furno, I. (LPHE, Lausanne) ; Granados, E. (CERN) ; Granetzny, M. (Wisconsin U., Madison) ; Graubner, T. (Philipps U. Marburg) ; Grulke, O. (Greifswald, Max Planck Inst. ; Denmark, Tech. U.) ; Guran, E. (CERN) ; Henderson, J. (Cockcroft Inst. Accel. Sci. Tech. ; Daresbury) ; Kedves, M.Á. (Wigner RCP, Budapest) ; Kraus, F. (Philipps U. Marburg) ; Krupa, M. (CERN) ; Lefevre, T. (CERN) ; Liang, L. (Manchester U. ; Cockcroft Inst. Accel. Sci. Tech.) ; Liu, S. (TRIUMF) ; Lotov, K. (Novosibirsk, IYF ; Novosibirsk State U.) ; Calderon, M. Martinez (CERN) ; Mazzoni, S. (CERN) ; Moon, K. (UNIST, Ulsan) ; Guzmán, P.I. Morales (Munich, Max Planck Inst.) ; Moreira, M. (Lisbon, IST) ; Nechaeva, T. (Munich, Max Planck Inst.) ; Okhotnikov, N. (Novosibirsk, IYF ; Novosibirsk State U.) ; Pakuza, C. (JAI, UK) ; Pardons, A. (CERN) ; Pepitone, K. (Uppsala U.) ; Poimendidou, E. (CERN) ; Pukhov, A. (Heinrich Heine U., Dusseldorf) ; Ramjiawan, R.L. (CERN ; JAI, UK) ; Ranc, L. (Munich, Max Planck Inst.) ; Rey, S. (CERN) ; Rossel, R. (CERN) ; Saberi, H. (Manchester U. ; Cockcroft Inst. Accel. Sci. Tech.) ; Schmitz, O. (Wisconsin U., Madison) ; Senes, E. (CERN) ; Silva, F. (Rio de Janeiro, IMPA) ; Silva, L. (Lisbon, IST) ; Spear, B. (JAI, UK) ; Stollberg, C. (LPHE, Lausanne) ; Swain, C. (Cockcroft Inst. Accel. Sci. Tech. ; Liverpool U.) ; Topaloudis, A. (CERN) ; Tuev, P. (Novosibirsk, IYF ; Novosibirsk State U.) ; Velotti, F. (CERN) ; Verzilov, V. (TRIUMF) ; Vieira, J. (Lisbon, IST) ; Walter, E. (U. Edinburgh, Higgs Ctr. Theor. Phys.) ; Welsch, C. (Cockcroft Inst. Accel. Sci. Tech. ; Liverpool U.) ; Wendt, M. (CERN) ; Wing, M. (University Coll. London) ; Wolfenden, J. (Cockcroft Inst. Accel. Sci. Tech. ; Liverpool U.) ; Woolley, B. (CERN) ; Xia, G. (Cockcroft Inst. Accel. Sci. Tech. ; Manchester U.) ; Yarygova, V. (Novosibirsk, IYF ; Novosibirsk State U.) ; Zepp, M. (Wisconsin U., Madison)

Publication 2024-05-07
Imprint 2023-12-21
Number of pages 8
In: Phys. Rev. E 109 (2024) 055203
DOI 10.1103/PhysRevE.109.055203 (publication)
Subject category physics.acc-ph ; Accelerators and Storage Rings ; physics.plasm-ph ; Other Fields of Physics
Accelerator/Facility, Experiment CERN AWAKE
Abstract We show in experiments that a long, underdense, relativistic proton bunch propagating in plasma undergoes the oblique instability, that we observe as filamentation. We determine a threshold value for the ratio between the bunch transverse size and plasma skin depth for the instability to occur. At the threshold, the outcome of the experiment alternates between filamentation and self-modulation instability (evidenced by longitudinal modulation into microbunches). Time-resolved images of the bunch density distribution reveal that filamentation grows to an observable level late along the bunch, confirming the spatio-temporal nature of the instability. We calculate the amplitude of the magnetic field generated in the plasma by the instability and show that the associated magnetic energy increases with plasma density.
Copyright/License publication: © 2024 authors (License: CC BY 4.0)
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 Record created 2023-12-23, last modified 2024-09-06


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