Quantitative single shot and spatially resolved plasma wakefield diagnostics

Muhammad Firmansyah Kasim, James Holloway, Luke Ceurvorst, Matthew C. Levy, Naren Ratan, James Sadler, Robert Bingham, Philip N. Burrows, Raoul Trines, Matthew Wing, Peter Norreys

Research output: Contribution to journalArticle

4 Citations (Scopus)
59 Downloads (Pure)

Abstract

Diagnosing plasma conditions can give great advantages in optimizing plasma wakefield accelerator experiments. One possible method is that of photon acceleration. By propagating a laser probe pulse through a plasma wakefield and extracting the imposed frequency modulation, one can obtain an image of the density modulation of the wakefield. In order to diagnose the wakefield parameters at a chosen point in the plasma, the probe pulse crosses the plasma at oblique angles relative to the wakefield. In this paper, mathematical expressions relating the frequency modulation of the laser pulse and the wakefield density profile of the plasma for oblique crossing angles are derived. Multidimensional particle-in-cell simulation results presented in this paper confirm that the frequency modulation profiles and the density modulation profiles agree to within 10%. Limitations to the accuracy of the measurement are discussed in this paper. This technique opens new possibilities to quantitatively diagnose the plasma wakefield density at known positions within the plasma column.

Original languageEnglish
Article number081302
Number of pages12
JournalPhysical Review Special Topics: Accelerators and Beams
Volume18
Issue number8
DOIs
Publication statusPublished - 6 Aug 2015

Keywords

  • mathematical expressions
  • frequency modulation
  • laser pulse
  • wakefield density profile
  • oblique crossing angles
  • plasma wakefield density

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    Kasim, M. F., Holloway, J., Ceurvorst, L., Levy, M. C., Ratan, N., Sadler, J., ... Norreys, P. (2015). Quantitative single shot and spatially resolved plasma wakefield diagnostics. Physical Review Special Topics: Accelerators and Beams, 18(8), [081302]. https://doi.org/10.1103/PhysRevSTAB.18.081302