CERN Accelerating science

Article
Report number arXiv:2011.04398
Title Generating ultra-dense pair beams using 400 GeV/c protons
Author(s) Arrowsmith, C.D. (Oxford U.) ; Shukla, N. (CINECA) ; Charitonidis, N. (CERN) ; Boni, R. (Rochester U.) ; Chen, H. (LLNL, Livermore) ; Davenne, T. (Rutherford) ; Dyson, A. (Oxford U.) ; Froula, D.H. (Rochester U.) ; Gudmundsson, J.T. (Iceland U. ; Royal Inst. Tech., Stockholm) ; Huffman, B.T. (Oxford U.) ; Kadi, Y. (CERN) ; Reville, B. (Heidelberg, Max Planck Inst.) ; Richardson, S. (AWRE, Aldermaston) ; Sarkar, S. (Oxford U.) ; Shaw, J.L. (Rochester U.) ; Silva, L.O. (Lisbon, CFP) ; Simon, P. (CERN) ; Trines, R.M.G.M. (Rutherford) ; Bingham, R. (Rutherford ; Strathclyde U.) ; Gregori, G. (Oxford U.)
Publication 2021-05-11
Imprint 2020-11-09
Number of pages 9
In: Phys. Rev. Res. 3, 2 (2021) pp.023103
DOI 10.1103/physrevresearch.3.023103 (publication)
10.1103/PhysRevResearch.3.023103
10.1103/PhysRevResearch.3.023103 (publication)
Subject category hep-ph ; Particle Physics - Phenomenology ; astro-ph.HE ; Astrophysics and Astronomy ; physics.plasm-ph ; Other Fields of Physics
Abstract A previously unexplored experimental scheme is presented for generating low-divergence, ultra-dense, relativistic, electron-positron beams using 400 GeV/c protons available at facilities such as HiRadMat and AWAKE at CERN. Preliminary Monte-Carlo and Particle-in-cell simulations demonstrate the possibility of generating beams containing $10^{13}-10^{14}$ electron-positron pairs at sufficiently high densities to drive collisionless beam-plasma instabilities, which are expected to play an important role in magnetic field generation and the related radiation signatures of relativistic astrophysical phenomena. The pair beams are quasi-neutral, with size exceeding several skin-depths in all dimensions, allowing for the first time the examination of the effect of competition between transverse and longitudinal instability modes on the growth of magnetic fields. Furthermore, the presented scheme allows for the possibility of controlling the relative density of hadrons to electron-positron pairs in the beam, making it possible to explore the parameter spaces for different astrophysical environments.
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publication: © 2021-2025 authors (License: CC-BY-4.0)



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