• Open Access

Flexible x-ray source with tunable polarization and orbital angular momentum from Hermite-Gaussian laser modes driven plasma channel wakefield

B. Lei, T. Teter, J. W. Wang, V. Yu. Kharin, C. B. Schroeder, M. Zepf, and S. G. Rykovanov
Phys. Rev. Accel. Beams 22, 071302 – Published 29 July 2019
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Abstract

A plasma channel undulator/wiggler may be created through the plasma wakefield excited by the beating of several Hermite-Gaussian laser modes propagating in a parabolic plasma channel. Control over both the betatron and undulator forces is conveniently achieved by tuning the amplitude ratios, colors, and order numbers of the modes. A special structure of the undulator/wiggler field without the focusing force near the propagation axis is generated inside the plasma wakefield by matching the strengths of the fundamental and first-order Hermite-Gaussian modes. The electron beam only experiences forced undulator oscillations in such a field, which significantly improves the quality of the emitted radiation. Since the value of the undulator strength parameter could be in a wide range, less or larger than unity, it is capable of generating narrow bandwidth x-ray, as well as the synchrotronlike high-energy x/γ-ray, radiation by harmonics. Additionally, controlling the relative phases between the laser modes allows for polarization control of the plasma undulator. High-order harmonics produced from a circularly polarized plasma undulator clearly show the vortex nature and carry well-defined orbital angular momentum.

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  • Received 14 January 2019

DOI:https://doi.org/10.1103/PhysRevAccelBeams.22.071302

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.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Accelerators & Beams

Authors & Affiliations

B. Lei1,2,*, T. Teter1,2, J. W. Wang3, V. Yu. Kharin1, C. B. Schroeder4, M. Zepf1,2, and S. G. Rykovanov1,5,†

  • 1Helmholtz Institute Jena, Fröbelstieg 3, 07743 Jena, Germany
  • 2Faculty of Physics and Astronomy, Friedrich-Schiller-Universität Jena, 07743 Jena, Germany
  • 3Shanghai Institute of Optics and Fine Mechanics, Chinese Academy of Sciences, 201800 Shanghai, China
  • 4Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA
  • 5Center for Computational and Data-Intensive Science and Engineering, Skolkovo Institute of Science and Technology, Moscow 121205, Russia

  • *B.Lei@gsi.de
  • S.Rykovanov@gsi.de

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Vol. 22, Iss. 7 — July 2019

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