Hollow Plasma Acceleration Driven by a Relativistic Reflected Hollow Laser

W. P. Wang, C. Jiang, H. Dong, X. M. Lu, J. F. Li, R. J. Xu, Y. J. Sun, L. H. Yu, Z. Guo, X. Y. Liang, Y. X. Leng, R. X. Li, and Z. Z. Xu
Phys. Rev. Lett. 125, 034801 – Published 17 July 2020

Abstract

In order to address the present difficulty in experimentally generating the relativistic Laguerre-Gaussian laser, primarily due to damage caused to optical modulators, a high-reflectivity phase mirror is applied in the femtosecond petawatt laser system to generate a relativistic hollow laser at the highest intensity of 6.3×1019W/cm2 for the first time. A simple optical model is used to verify that the vortex laser may be generated in this new scheme; using such a relativistic vortex laser, the hollow plasma drill and acceleration are achieved experimentally and proven by particle-in-cell simulations. With the development of the petawatt laser, this scheme opens up possibilities for the convenient production of the relativistic hollow laser at high repetition and possible hollow plasma acceleration, which is important for a wide range of applications such as the generation of radiation sources with orbital angular momentum, fast ignition for inertial confinement fusion, and jet research in the astrophysical environment.

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  • Received 18 October 2019
  • Revised 21 June 2020
  • Accepted 30 June 2020

DOI:https://doi.org/10.1103/PhysRevLett.125.034801

© 2020 American Physical Society

Physics Subject Headings (PhySH)

Accelerators & BeamsPlasma Physics

Authors & Affiliations

W. P. Wang1,*,§, C. Jiang1,2,3,§, H. Dong1,3, X. M. Lu1, J. F. Li1, R. J. Xu1, Y. J. Sun1, L. H. Yu1, Z. Guo1, X. Y. Liang1, Y. X. Leng1, R. X. Li1,2,3,†, and Z. Z. Xu1,‡

  • 1State Key Laboratory of High Field Laser Physics and CAS Center for Excellence in Ultra-intense Laser Science, Shanghai Institute of Optics and Fine Mechanics (SIOM), Chinese Academy of Sciences (CAS), Shanghai 201800, China.
  • 2School of Physical Science and Technology, ShanghaiTech University, Shanghai 201210, China
  • 3University of Chinese Academy of Sciences, Beijing 100049, China

  • *Corresponding authors. wangwenpeng@siom.ac.cn
  • Corresponding authors. ruxinli@siom.ac.cn
  • Corresponding authors. zzxu@mail.shcnc.ac.cn
  • §These authors contributed equally to this work.

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Vol. 125, Iss. 3 — 17 July 2020

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