Phase Space Dynamics of a Plasma Wakefield Dechirper for Energy Spread Reduction

Y. P. Wu, J. F. Hua, Z. Zhou, J. Zhang, S. Liu, B. Peng, Y. Fang, Z. Nie, X. N. Ning, C.-H. Pai, Y. C. Du, W. Lu, C. J. Zhang, W. B. Mori, and C. Joshi
Phys. Rev. Lett. 122, 204804 – Published 24 May 2019

Abstract

Plasma-based accelerators have made impressive progress in recent years. However, the beam energy spread obtained in these accelerators is still at the 1% level, nearly one order of magnitude larger than what is needed for challenging applications like coherent light sources or colliders. In plasma accelerators, the beam energy spread is mainly dominated by its energy chirp (longitudinally correlated energy spread). Here we demonstrate that when an initially chirped electron beam from a linac with a proper current profile is sent through a low-density plasma structure, the self-wake of the beam can significantly reduce its energy chirp and the overall energy spread. The resolution-limited energy spectrum measurements show at least a threefold reduction of the beam energy spread from 1.28% to 0.41% FWHM with a dechirping strength of 1(MV/m)/(mmpC). Refined time-resolved phase space measurements, combined with high-fidelity three-dimensional particle-in-cell simulations, further indicate the real energy spread after the dechirper is only about 0.13% (FWHM), a factor of 10 reduction of the initial energy spread.

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  • Received 20 January 2019
  • Revised 19 April 2019

DOI:https://doi.org/10.1103/PhysRevLett.122.204804

© 2019 American Physical Society

Physics Subject Headings (PhySH)

Accelerators & BeamsPlasma Physics

Authors & Affiliations

Y. P. Wu1, J. F. Hua1,*, Z. Zhou1, J. Zhang1, S. Liu1, B. Peng1, Y. Fang1, Z. Nie1, X. N. Ning1, C.-H. Pai1, Y. C. Du1, W. Lu1,†, C. J. Zhang2, W. B. Mori2, and C. Joshi2

  • 1Department of Engineering Physics, Tsinghua University, Beijing 100084, China
  • 2University of Los Angeles, Los Angeles, California 90095, USA

  • *jfhua@tsinghua.edu.cn
  • weilu@tsinghua.edu.cn

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Vol. 122, Iss. 20 — 24 May 2019

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